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Deep Inelastic Scattering 11
Dijet Production 11
Electron production 11
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Jet Production 11
Neutral Current 11
Single Differential Cross Section 9
Transverse Momentum Dependence 3
Azimuthal Angular Dependence 2
Double Differential Cross Section 2

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E+ P --> E+ JET JET X 11
E- P --> E- JET JET X 6
E+ P --> E+ JET JET JET X 2
E+ P --> E+ JET X 2
E- P --> E- JET JET JET X 2
GAMMA P --> JET JET X 2
E+ P --> 2JET E+ X 1
E+ P --> E+ CHARGED X 1
E+ P --> E+ K0 X 1
E+ P --> E+ N JET JET X 1

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DSIG/DET 7
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0.0 ≤ √s < 1.0
1.0 ≤ √s < 2.0
2.0 ≤ √s < 5.0
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10.0 ≤ √s < 100.0
100.0 ≤ √s < 1000.0
1000.0 ≤ √s < 7000.0
7000.0 ≤ √s < 8000.0
8000.0 ≤ √s < 13000.0
√s ≥ 13000.0

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Abramowicz, H. 11
Adamczyk, L. 11
Adamus, M. 11
Antonioli, P. 11
Arneodo, M. 11
Bamberger, A. 11
Bari, G. 11
Barreiro, F. 11
Basile, M. 11
Behrens, U. 11

rivet Analysis
Dijet cross-sections in photoproduction at HERA

The ZEUS collaboration Breitweg, J. ; Derrick, M. ; Krakauer, D. ; et al.

Eur.Phys.J.C 1 (1998) 109-122, 1998.

https://inspirehep.net/literature/450085 Inspire Record 450085 DOI 10.17182/hepdata.44384 https://doi.org/10.17182/hepdata.44384

Dijet cross sections are presented using photoproduction data obtained with the ZEUS detector during 1994. These measurements represent an extension of previous results, as the higher statistics allow cross sections to be measured at higher jet transverse energy (ETJ). Jets are identified in the hadronic final state using three different algorithms, and the cross sections compared to complete next-to-leading order QCD calculations. Agreement with these calculations is seen for the pseudorapidity dependence of the direct photon events with ETJ > 6 GeV and of the resolved photon events with ETJ > 11 GeV. Calculated cross sections for resolved photon processes with 6 GeV < ETJ < 11 GeV lie below the data.

28 data tables

Table 1

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.0 TO 1.0. The second DSYS errors are the correlated uncertainties.

Table 2

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.0 TO 1.0. The second DSYS errors are the correlated uncertainties.

Table 3

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.0 TO 1.0. The second DSYS errors are the correlated uncertainties.

Table 4

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.0 TO 1.0. The second DSYS errors are the correlated uncertainties.

Table 5

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 6

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 7

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 8

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 9

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 10

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 11

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 12

Dijet cross section using the PUCELL jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 13

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 14

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 15

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 16

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 17

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 18

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 19

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 20

Dijet cross section using the EUCELL jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 21

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 22

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 23

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 24

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be > 0.75. The second DSYS errors are the correlated uncertainties.

Table 25

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 6 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 26

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 8 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 27

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 11 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

Table 28

Dijet cross section using the KTCLUS jet alogrithm with a minimum ET for each jet of 15 GeV and a requirement on X(NAME=GAMMA_OBS) to be 0.30 TO 0.75. The second DSYS errors are the correlated uncertainties.

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rivet Analysis Dijet cross-sections in photoproduction at HERA

rivet Analysis
Dijet cross-sections in photoproduction at HERA