Fluxes

Data sample:

1. pp 510 GeV, pythia, geometry 2013 (published as Yuri Fisyak et al., "Thermal neutron flux measurements in the STAR experimental hall", Nucl.Instrum.Meth. A756 (2014) 68-72, DOI: 10.1016/j.nima.2014.04.035).
2. pp 510 GeV, pythia, geometry 2014.
3. AuAu 200 GeV, hijing, geometry 2014.
4. He3Au 200 GeV, hijing, geometry 2014.
5. pAu 200 GeV, hijing, geometry 2013_1x.
6. pAu 200 GeV, hijing, geometry 2014.
7. pp 200 GeV, pythia, geometry 2013_1x.
8. pp 200 GeV, pythia, geometry 2014.

Legend

• The plots are normalized on 1 MHz minimum biased collision rate.
• All plots have an associated root files with canvas and can be downloaded by clicking on picture. The canvas can be redrawn in root and any number can be obtained from the canvas via Options → Status Bar.
• Fig.1 - Fig.4 show neutron fluxes for all ( Fig.1), with E_kin > 100 MeV ( Fig.2), with with E_kin < 250 meV ( Fig.3), and neutron production vertices ( Fig.4).
• Fig.5 - Fig.7 show fluxes for charged hadrons.
• Fig.8 - Fig.11 show fluxes for electrons.
• Fig.12 - Fig.14 show fluxes for γs.
• Fig.15 - Fig.16 show fluxes for γs.
• Fig.17 show deposited energy from charged hadrons, Fig.18 - electrons, Fig.19 - γs.

2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.1
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.2
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.3
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.4
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.5
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.6
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.7
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.8
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.9
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.11
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.12
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.13
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.14
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.15
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.16
2013 pp510, charged hadrons	2014 pp510, charged hadrons	2014 AuAu200, charged hadrons	2014 He3Au200, charged hadrons	2013 pAu200, charged hadrons	2014 pAu200, charged hadrons	2013 pp200, charged hadrons	2014 pp200, charged hadrons
Fig.17
2013 pp510, e±	2014 pp510, e±	2014 AuAu200, e±	2014 He3Au200, e±	2013 pAu200, e±	2014 pAu200, e±	2013 pp200, e±	2014 pp200, e±
Fig.18
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.19
2013 pp510	2014 pp510	2014 AuAu200	2014 He3Au200	2013 pAu200	2014 pAu200	2013 pp200	2014 pp200
Fig.21 hadrons
Fig.22 electrons
Fig.23 gammas