1994
DOI: 10.1016/0370-2693(94)91121-5
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Observation of direct processes in photoproduction at HERA

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Cited by 69 publications
(25 citation statements)
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“…Photoproduction events were selected by requiring that no scattered electron with energy of greater than 5 GeV be identified in the CAL [39]. The photon-proton centreof-mass energy, W , was reconstructed using the Jacquet-Blondel [40] estimator of W , W JB = 2E p i E i (1 − cos θ i ).…”
Section: Jhep09(2013)058mentioning
confidence: 99%
See 2 more Smart Citations
“…Photoproduction events were selected by requiring that no scattered electron with energy of greater than 5 GeV be identified in the CAL [39]. The photon-proton centreof-mass energy, W , was reconstructed using the Jacquet-Blondel [40] estimator of W , W JB = 2E p i E i (1 − cos θ i ).…”
Section: Jhep09(2013)058mentioning
confidence: 99%
“…Here E i and θ i denote the energy and polar angle of the i th energy-flow object (EFO) [41], respectively, and the sum i runs over all final-state energyflow objects built from CTD-MVD tracks and energy clusters measured in the CAL. After correcting for detector effects, the most important of which were energy losses in inactive material in front of the CAL and particle interactions in the beam pipe [39,42], events were selected in the interval 130 < W JB < 300 GeV. The lower limit was set by the trigger requirements, while the upper limit was imposed to suppress remaining DIS events with an unidentified low-energy scattered electron in the CAL [39].…”
Section: Jhep09(2013)058mentioning
confidence: 99%
See 1 more Smart Citation
“…The upper cut rejects possible background from DIS events in which the scattered positron had not been recognised. A systematic shift in the reconstructed values of W JB with respect to the true W of the event, due to energy losses in inactive material in front of the calorimeter and particles lost in the beam pipe, was corrected [12,19], using the MC simulation of the detector described in section 4. The centre of mass energy range covered by the photoproduction sample is then 130 < W < 280 GeV, corresponding to 0.19 < y < 0.87.…”
Section: Offline Data Selectionmentioning
confidence: 99%
“…In such events, the fraction x OBS γ of the photon momentum which participates in the dijet production can be measured [3]. This quantity is sensitive to the relative contributions of resolved and direct processes [12]. In LO QCD direct photon events at the parton level have x OBS γ =1, while resolved photon events populate low values of x OBS γ .…”
Section: Introductionmentioning
confidence: 99%