$\xi$ distributions for different jet $p_T$ bins.

$\xi$ distributions for different jet $p_T$ bins.

The $j_T/p_{T}^{\rm jet}$ distributions for different jet $p_T$ bins.

The $j_T/p_{T}^{\rm jet}$ distributions for different jet $p_T$ bins.

$r$ distributions for different jet $p_T$ bins.

Distribution of $E_{\text{T}}^{\text{miss}}$ in SROS-on-b-$e\mu\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. The hatched band includes all statistical and systematic uncertainties.

Distribution of $m_{\text{T}}^{\text{min}}$ in SROS-on-b-$e\mu\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. The hatched band includes all statistical and systematic uncertainties.

Distribution of $E_{\text{T}}^{\text{miss}}$ in SRSS-$2\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. The hatched band includes all statistical and systematic uncertainties.

Observed ($N_{\text{obs}}$) and expected ($N_{\text{exp}}$) yields after the background-only fit for the flavor-merged inclusive SRs. The third and fourth columns list the 95\% CL upper limits on the visible cross-section ($\sigma_{\text{vis}}^{95}$) and on the number of signal events ($S_\text{obs}^{95}$). The fifth column ($S_\text{exp}^{95}$) shows the 95\% CL upper limit on the number of signal events, given the expected number of background events and its $\pm 1\sigma$ variations. The last two columns indicate the CL$_{\text{b}}$ value, i.e. the confidence level observed for the background-only hypothesis, and the discovery $p$-value ($p(s = 0)$) with its associated statistical significance $Z$. If the observed yield is below the expected yield, the $p$-value is capped at 0.5.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{e}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Observed and expected exclusion limits on the SBH model where only $\tilde{\mu}_{\text{L}}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100~GeV.

Distribution of $E_{\text{T}}^{\text{miss}}$ in SROS-off-b-$e\mu\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. Ratio values outside the graph range are indicated by brown arrows. The hatched band includes all statistical and systematic uncertainties.

Distribution of $m_{\text{T}}^{\text{min}}$ in SROS-off-b-$e\mu\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. Ratio values outside the graph range are indicated by brown arrows. The hatched band includes all statistical and systematic uncertainties.

Distribution of $E_{\text{T}}^{\text{miss}}$ in SRSS-$eee$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. Ratio values outside the graph range are indicated by brown arrows. The hatched band includes all statistical and systematic uncertainties.

Distribution of $E_{\text{T}}^{\text{miss}}$ in SRSS-$ee\mu$. The SR selections are applied for each distribution, except for the variable shown, for which the selection is indicated by a black arrow. The last bin includes the overflow. The `Others' category contains the production of Higgs boson, 3-top, 4-top, and single-top processes. Distributions for SBH signals are overlaid. The bottom panels show the ratio of the observed data to the predicted total background yields. Ratio values outside the graph range are indicated by brown arrows. The hatched band includes all statistical and systematic uncertainties.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ is considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $m(\tilde{\ell}_{\text{L}}^{\pm})$ vs $m(\tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 150 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

Observed and expected exclusion limits on the SBH model where mass-degenerate $\tilde{e}_{\text{L}}$, $\tilde{\mu}_{\text{L}}$ and $\tilde{\nu}$ are considered. The expected 95% CL exclusion limit is shown as a dashed black line, with the yellow band indicating $\pm1\sigma_{\text{exp}}$ including all uncertainties except for the signal cross-section uncertainty. The observed 95% CL exclusion limit is shown as a red solid line, with the dotted red lines indicating $\pm1\sigma_{\text{theory}}$ due to the signal cross-section uncertainty. The limits are shown projected onto the $\Delta m(\tilde{\chi}^0_3, \tilde{\chi}^0_1)$ vs $\Delta m(\tilde{\ell}_{\text{L}}, \tilde{\chi}^0_3)$ plane, with $m(\tilde{\chi}^0_1)$ assumed to be 100 GeV.

The expected upper limits on the cross-section for each signal point. The gray numbers represent the values. The expected (dashed) and observed (solid) 95% CL exclusion limits are overlaid. An asymptotic approximation is employed in the CL$_{\text{s}}$ calculation instead of the full calculation using pseudo-experiments.

The observed upper limits on the cross-section for each signal point. The gray numbers represent the values. The expected (dashed) and observed (solid) 95% CL exclusion limits are overlaid. An asymptotic approximation is employed in the CL$_{\text{s}}$ calculation instead of the full calculation using pseudo-experiments.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Acceptance for signals with $m(\tilde{\chi}^0_1)=100$ GeV in flavored-merged SRs. The acceptance is given by the ratio of weighted selected events in the SR to the weighted total number of generated events. The selection is based on generator-level particle information.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Efficiencies for signals with $m(\tilde{\chi}^0_1)=100$ GeV in the $m_{3\ell}$ merged SRSFOS and SRSS. The efficiency is defined by the number of events of reconstructed-level signal simulation divided by the number of events obtained at generator level. Efficiencies below 0.002% are rounded to 0. The efficiency values are affected by statistical fluctuations due to the limited number of events.

Summary of the number of events passing each selection for the $m(\tilde{\ell}_{\text{L}}^{\pm},\tilde{\chi}^0_3,\tilde{\chi}^0_1)=(300, 200, 100)$, $(550, 300, 100)$, $(450, 180, 100)$ GeV signal points, including all production processes. After the initial selections, the table is split into row blocks per inclusive region, and then further for each SR channel. Flavor-binned SRs are shown for SROS-on-b for reference. The generator level selections require to have two or more leptons.

Summary of the number of events passing each selection for the $m(\tilde{\ell}_{\text{L}}^{\pm},\tilde{\chi}^0_3,\tilde{\chi}^0_1)=(300, 200, 100)$, $(550, 300, 100)$, $(450, 180, 100)$ GeV signal points, including all production processes. After the initial selections, the table is split into row blocks per inclusive region, and then further for each SR channel. Flavor-binned SRs are shown for SROS-off-b for reference. The generator level selections require to have two or more leptons.

Summary of the number of events passing each selection for the $m(\tilde{\ell}_{\text{L}}^{\pm},\tilde{\chi}^0_3,\tilde{\chi}^0_1)=(300, 200, 100)$, $(550, 300, 100)$, $(450, 180, 100)$ GeV signal points, including all production processes. After the initial selections, the table is split into row blocks per inclusive region, and then further for each SR channel. Flavor-binned SRs are shown. The generator level selections require to have two or more leptons.

The Charged-hadron yields as a function of pT in different y selections in p+Pb collisions.

The K^{0}_{S} yields as a function of pT in different y selections in Pb+Pb photo-nuclear collisions.

The #Lambda yields as a function of pT in different y selections in Pb+Pb photo-nuclear collisions.

The #Xi^{-} yields as a function of pT in different y selections in Pb+Pb photo-nuclear collisions.

The K^{0}_{S} yields as a function of pT in different y selections in p+Pb collisions.

The #Lambda yields as a function of pT in different y selections in p+Pb collisions.

The #Xi^{-} yields as a function of pT in different y selections in p+Pb collisions.

The Charged-hadron and identified-hadron yields as a function of y in Pb+Pb photo-nuclear collisions.

The Charged-hadron and identified-hadron yields as a function of y in Pb+Pb photo-nuclear collisions.

The Charged-hadron and identified-hadron yields as a function of y in p+Pb collisions.

The Charged-hadron and identified-hadron yields as a function of y in p+Pb collisions.

The meanpT of charged hadrons and identified hadrons as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The meanpT of charged hadrons and identified hadrons as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The meanpT of charged hadrons and identified hadrons as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The meanpT of charged hadrons and identified hadrons as a function of Nchrec in p+Pb collisions.

The meanpT of charged hadrons and identified hadrons as a function of Nchrec in p+Pb collisions.

The baryon to meson ratio as a function of pT in Pb+Pb photo-nuclear collisions.

The baryon to meson ratio as a function of pT in Pb+Pb photo-nuclear collisions.

The baryon to meson ratio as a function of pT in p+Pb collisions.

The baryon to meson ratio as a function of pT in p+Pb collisions.

The ratios of identified-strange-hadron yield to charged-hadron yields as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The ratios of identified-strange-hadron yield to charged-hadron yields as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The ratios of identified-strange-hadron yield to charged-hadron yields as a function of Nchrec in Pb+Pb photo-nuclear collisions.

The ratios of identified-strange-hadron yield to charged-hadron yields as a function of Nchrec in p+Pb collisions.

The ratios of identified-strange-hadron yield to charged-hadron yields as a function of Nchrec in p+Pb collisions.

The observed EFT limits at 95% CL, shown for the linear+quadratic electron, muon, and combined fits.

The expected EFT limits at 95% CL, shown for the linear-only electron, muon, and combined fits. The PDF eigenvectors in the theoretical uncertainty are used at 68% CL.

The expected EFT limits at 95% CL, shown for the linear+quadratic electron, muon, and combined fits. The PDF eigenvectors in the theoretical uncertainty are used at 68% CL.

The observed EFT limits at 95% CL, shown for the linear-only electron, muon, and combined fits. The PDF eigenvectors in the theoretical uncertainty are used at 68% CL.

The observed EFT limits at 95% CL, shown for the linear+quadratic electron, muon, and combined fits. The PDF eigenvectors in the theoretical uncertainty are used at 68% CL.

Born-level single-differential cross section $\frac{d\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level single-differential cross section $\frac{d\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level single-differential cross section $\frac{d\sigma (W\to e\nu) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^+\to e^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W^-\to e^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W\to e\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W\to e\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W\to e\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W\to e\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross section $\frac{d^2\sigma (W\to e\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level single-differential cross-section $\frac{d\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level single-differential cross-section $\frac{d\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level single-differential cross-section $\frac{d\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} } $ including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^+\to\mu^+\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W^-\to\mu^-\bar{\nu}) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [200-300] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [300-425] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [425-600] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [600-900] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Born-level double-differential cross-section $\frac{d^2\sigma (W\to\mu\nu) }{d m_{\text{T}}^{W} d |\eta| } $ for $m_T^W$ = [900-2000] GeV including the absolute statistical and systematic uncertainties. Symmetric uncertainties are denoted by $\pm$ or $\mp$, where the upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^+$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^-$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^+$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^-$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level single-differential cross-section including the absolute statistical and systematic uncertainties in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Physical sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The systematic uncertainties are related to the unfolding procedure (``unf.''), the jet energy scale/resolution (``JER/JES''), the \met scale and resolution, the electron and muon scale, resolution and efficiency (``Eff.''), the multijet and $t\bar{t}$ (where $t\bar{t}$ RW refers to a reweighting to NNLO) background estimates and normalization of small background processes (``Norm.''). The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[200,300]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[300,425]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[425,600]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[600,900]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Combined Born-level double-differential cross-section including the absolute statistical and systematic uncertainties for $m_T^W=[900,2000]\,\mathrm{GeV}$ in the $\ell^\pm$-channel. Orthogonal sources of systematic uncertainties are shown. The upper sign corresponds to the one standard deviation upward shift of the uncertainty source. The luminosity uncertainty of $0.83\%$ is not included.

Ratio of the $e^\pm$- and $\mu^\pm$-channel single-differential cross sections including the absolute data statistical, $e$-$\mu$-uncorrelated (including signal and background statistical) and $e$-$\mu$-correlated systematic uncertainties and the total uncertainty.

Ratio of the $e^\pm$- and $\mu^\pm$-channel double-differential cross sections including the absolute data statistical, $e$-$\mu$-uncorrelated (including signal and background statistical) and $e$-$\mu$-correlated systematic uncertainties and the total uncertainty.

Asymmetry of the $\ell^+$- and $\ell^-$-channel single-differential cross-sections including the absolute total statistical and $\ell^+$-$\ell^-$-correlated systematic uncertainties and the total uncertainty.

Asymmetry of the $\ell^+$- and $\ell^-$-channel double-differential cross sections including the absolute total statistical and $\ell^+$-$\ell^-$-correlated systematic uncertainties and the total uncertainty.

p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Spectral temperature parameter for $\Delta^{++}$(1232) from p-$\pi^{+}$ + antip-$\pi^{-}$ correlations in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Width of the $\Delta^{++}$(1232) from p-$\pi^{+}$ + antip-$\pi^{-}$ correlations in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Core source size of p-$\pi^{+}$ + antip-$\pi^{-}$ pairs in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [0.54, 0.75)$ GeV/$c^2$

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [0.75, 0.95)$ GeV/$c^2$

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [0.95, 1.20)$ GeV/$c^2$

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

p-$\pi^{-}$ + p-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Spectral temperature parameter for $\Delta^{0}$(1232) from p-$\pi^{-}$ + p-$\pi^{+}$ correlations in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Width of the $\Delta^{0}$(1232) from p-$\pi^{-}$ + p-$\pi^{+}$ correlations in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Core source size of p-$\pi^{-}$ + p-$\pi^{+}$ pairs in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-p)-$\pi^{+}$ + (antip-antip)-$\pi^{-}$ lower-order correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-p)-$\pi^{-}$ + (antip-antip)-$\pi^{+}$ lower-order correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-$\pi^{+}$)-p + (antip-$\pi^{-}$)-antip lower-order correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-$\pi^{-}$)-p + (antip-$\pi^{+}$)-antip lower-order correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-p-$\pi^{+}$) + (antip-antip-$\pi^{-}$) triplet correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Total lower-order contribution of p-p-$\pi^{+}$ + antip-antip-$\pi^{-}$ in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

(p-p-$\pi^{-}$) + (antip-antip-$\pi^{+}$) triplet correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Total lower-order contribution of p-p-$\pi^{-}$ + antip-antip-$\pi^{+}$ in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Cumulant of p-p-$\pi^{+}$ + antip-antip-$\pi^{-}$ in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Cumulant of p-p-$\pi^{-}$ + antip-antip-$\pi^{+}$ in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.54, 0.75)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.54, 0.75)$ GeV/$c^2$

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.75, 0.95)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.75, 0.95)$ GeV/$c^2$

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.95, 1.20)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.95, 1.20)$ GeV/$c^2$

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

Common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Non-common ancestor p-$\pi^{+}$ + antip-$\pi^{-}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.54, 0.75)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.54, 0.75)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.75, 0.95)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.75, 0.95)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.95, 1.20)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [0.95, 1.20)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.20, 1.50)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [1.50, 2.00)$ GeV/$c^2$

Common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Non-common ancestor p-$\pi^{-}$ + antip-$\pi^{+}$ correlation function in high-multiplicity (0-0.17%) pp collisions at $\sqrt{s}=13$ TeV with PYTHIA 8.2 (Monash 13 Tune) for $m_\text{T} \in [2.00, 2.50)$ GeV/$c^2$

Suppl. Fig. 7. The reconstructed shower angle for all single photon events. The individual signal and background event type categories added together form the unconstrained prediction.

Suppl. Fig. 7. The constrained covariance matrix for the reconstructed shower angle for all single-photon events. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Suppl. Fig. 7. The unconstrained covariance matrix for reconstructed shower angle for all single-photon events. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Fig. 3. The reconstructed number of protons, with a proton KE energy threshold of 35 MeV, for all single-photon events. The individual signal and background event type categories added together form the unconstrained prediction.

Fig. 4, Suppl. Fig. 8. The reconstructed shower energy for zero proton events binned from 0 to 600 MeV. The individual signal and background event type categories added together form the unconstrained prediction.

Fig. 4. The constrained covariance matrix for the reconstructed shower energy for zero proton events binned from 0 to 600 MeV. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Fig. 4. The unconstrained covariance matrix for reconstructed shower energy for zero proton events binned from 0 to 600 MeV. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Fig. 6. The reconstructed shower energy for zero proton events binned from 150 to 1250 MeV, with LEE prediction. The individual signal and background event type categories added together form the unconstrained prediction. The "LEE" category is the unfolded MiniBooNE LEE model prediction scaled under the neutrino-target nucleon interaction assumption.

Fig. 6. The constrained covariance matrix for the reconstructed shower energy for zero proton events binned from 150 to 1250 MeV. Both with and without the LEE model added. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Fig. 6. The unconstrained covariance matrix for reconstructed shower energy for zero proton events binned from 150 to 1250 MeV. Both with and without the LEE model added. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Suppl. Fig. 10. The reconstructed shower backwards projected distance for zero proton events. The individual signal and background event type categories added together form the unconstrained prediction.

Suppl. Fig. 9. The reconstructed shower angle for zero proton events. Includes LEE model prediction. The individual signal and background event type categories added together form the unconstrained prediction. The "LEE" category is the unfolded MiniBooNE LEE model prediction scaled under the neutrino-target nucleon interaction assumption.

Suppl. Fig. 9. The constrained covariance matrix for the reconstructed shower angle for zero proton events. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

Suppl. Fig. 9. The unconstrained covariance matrix for reconstructed shower angle for zero proton events. The matrix shows uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Data statistical uncertainties are not included. An example of how to add Pearson data statistical uncertainties can be found in the example code repository.

1$\gamma$Xp shower energy and angle selection efficiencies for true 1$\gamma$Xp events. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. Energy and Angle values represent bin lower edges.

1$\gamma$0p shower energy and angle selection efficiencies for true single-photon events with no other true particles of any energy. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. Energy and Angle values represent bin lower edges.

Covariance matrix showing uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Pearson data statistical uncertainties have been included, and include small correlations due to events which can be selected by both WC and Pandora. The first four bins are the WC $1\gamma Np$, WC $1\gamma 0p$, Pandora $1\gamma 1p$, and Pandora $1\gamma 0p$ channels, and the next four sets of 16 bins are the NC $\pi^0 Np$, NC $\pi^0 0p$, $\nu_\mu$CC $Np$, and $\nu_\mu$CC $0p$ channels. This corresponds to Fig. 1 of the paper and Fig. 6 of the Supplemental Material.

Constrained WC $1\gamma Np$ energy distribution. There are 6 bins from 0 to 600 MeV of reconstructed shower energy, with an additional overflow bin. Constrained systematic uncertainties on the predictions are illustrated, and a more detailed covariance matrix is included in the Constrained Energy Distributions Covariance Matrix tab. This corresponds to Fig. 2 of the paper.

Constrained WC $1\gamma 0p$ energy distribution. There are 14 bins from 0 to 700 MeV of reconstructed shower energy, with an additional overflow bin. Constrained systematic uncertainties on the predictions are illustrated, and a more detailed covariance matrix is included in the Constrained Energy Distributions Covariance Matrix tab. This corresponds to Fig. 2 of the paper.

Constrained Pandora $1\gamma 1p$ energy distribution. There are 6 bins from 0 to 600 MeV of reconstructed shower energy, with an additional overflow bin. Constrained systematic uncertainties on the predictions are illustrated, and a more detailed covariance matrix is included in the Constrained Energy Distributions Covariance Matrix tab. This corresponds to Fig. 2 of the paper.

Constrained Pandora $1\gamma 0p$ energy distribution. There are 14 bins from 0 to 700 MeV of reconstructed shower energy, with an additional overflow bin. Constrained systematic uncertainties on the predictions are illustrated, and a more detailed covariance matrix is included in the Constrained Energy Distributions Covariance Matrix tab. This corresponds to Fig. 2 of the paper.

Constrained covariance matrix showing constrained uncertainties and correlations between bins due to flux uncertainties, cross-section uncertainties, hadron reinteraction uncertainties, detector systematic uncertainties, Monte-Carlo statistical uncertainties, and dirt (outside cryostat) uncertainties. Pearson data statistical uncertainties have been included, and include small correlations due to events which can be selected by both WC and Pandora. The first seven bins are the WC $1\gamma Np$ reconstructed shower energy from 0-600 MeV with an overflow bin, the next 15 bins are the WC $1\gamma 0p$ reconstructed shower energy from 0-700 MeV with an overflow bin, the next seven bins are the Pandora $1\gamma 1p$ reconstructed shower energy from 0-600 MeV with an overflow bin, and the last 15 bins are the Pandora $1\gamma 0p$ reconstructed shower energy from 0-700 MeV with an overflow bin. This corresponds to Fig. 2 of the paper.

2D efficiency matrix showing the efficiency of the WC $1\gamma Np$ selection with respect to all true NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 15 bins from 0 to 1500 MeV in true photon energy. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. This corresponds to Fig. 9 of the Supplemental Material.

2D efficiency matrix showing the efficiency of the WC $1\gamma 0p$ selection with respect to all true NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 30 bins from 0 to 1500 MeV in true photon energy. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. This corresponds to Fig. 9 of the Supplemental Material.

2D efficiency matrix showing the efficiency of the Pandora $1\gamma 1p$ selection with respect to all true NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 15 bins from 0 to 1500 MeV in true photon energy, with lower bin edges indicated in the table. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. This corresponds to Fig. 9 of the Supplemental Material.

2D efficiency matrix showing the efficiency of the Pandora $1\gamma 0p$ selection with respect to all true NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 30 bins from 0 to 1500 MeV in true photon energy, with lower bin edges indicated in the table. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied. This corresponds to Fig. 9 of the Supplemental Material.

2D efficiency matrix showing the efficiency of the WC $1\gamma 0p$ selection with respect to all true zero-primary-final-state-proton NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 30 bins from 0 to 1500 MeV in true photon energy, with lower bin edges indicated in the table. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied.

2D efficiency matrix showing the efficiency of the Pandora $1\gamma 0p$ selection with respect to all true zero-primary-final-state-proton NC Delta Radiative Decay events which interact in the fiducial volume. The efficiency is shown as a function of true photon energy and angle. There are 10 bins from -1 to 1 in true photon $\cos \theta$ and 30 bins from 0 to 1500 MeV in true photon energy, with lower bin edges indicated in the table. NaN values indicate a "divide by zero" case where zero events were present in the bin before any selection was applied.

$a_2(1320)$ differential cross section in the m=-2 projection split into different reflectivity components, $\frac{d\sigma^+_{-2}}{dt}$ and $\frac{d\sigma^-_{-2}}{dt}$, in bins of four-momentum transfer. The first uncertainty is statistical, the second systematic.

$a_2(1320)$ differential cross section in the m=0 projection split into different reflectivity components, $\frac{d\sigma^+_{0}}{dt}$ and $\frac{d\sigma^-_{0}}{dt}$, in bins of four-momentum transfer. The first uncertainty is statistical, the second systematic.

$a_2(1320)$ differential cross section in the m=+1 projection split into different reflectivity components, $\frac{d\sigma^+_{+1}}{dt}$ and $\frac{d\sigma^-_{+1}}{dt}$, in bins of four-momentum transfer. The first uncertainty is statistical, the second systematic.

$a_2(1320)$ differential cross section in the m=+2 projection split into different reflectivity components, $\frac{d\sigma^+_{+2}}{dt}$ and $\frac{d\sigma^-_{+2}}{dt}$, in bins of four-momentum transfer. The first uncertainty is statistical, the second systematic.