Figure 3
10.17182/hepdata.144480.v2/t1
Event plane resolutions for calculating $v_3\{\Psi_1\}$ as a function of centrality from $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR.
10.17182/hepdata.144480.v2/t1
Event plane resolutions for calculating $v_3\{\Psi_1\}$ as a function of centrality from $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR.
10.17182/hepdata.144480.v2/t2
$v_3\{\Psi_1\}$ vs. centrality for $\pi^+$, $\pi^-$, and protons using the event plane method in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR.
10.17182/hepdata.144480.v2/t3
$v_3\{\Psi_1\}$ vs. centrality for $K^+$, and $K^-$ using the event plane method in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR.
10.17182/hepdata.144480.v2/t4
$v_3\{\Psi_1\}$ vs. rapidity for protons in three large centrality bins from a symmetric acceptance across midrapidity in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au...
10.17182/hepdata.144480.v2/t5
$v_3\{\Psi_1\}$ vs. rapidity for protons in three large centrality bins from only the backward region in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions...
10.17182/hepdata.144480.v2/t6
$v_3\{\Psi_1\}$ vs. $p_{\mathrm{T}}$ for protons in three large centrality bins in $\sqrt{s_{\textrm{NN}}}=3$ GeV Au+Au collisions at STAR. $v_3\{\Psi_1\}$ becomes increasingly...
Loading Data...
Please try again later, or email info@hepdata.net if this error persists.
This table is too large to load automatically.
The table size is MB, which is greater than our threshold of MB.
Loading Data...
Please try again later, or email info@hepdata.net if this error persists.
Your question will be emailed to those involved with the submission. Please mention the relevant table.
Please log in to HEPData to send a question.