erass1cl_cosmology_v1.1.fits
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Name | Type | Unit | Description |
---|---|---|---|
DETUID | char[32] | None | Unique source ID |
NAME | char[23] | None | Source name 1eRASS JHHMMSS.s+DDMMSS |
RA | float64 | deg | Right ascension (J2000) |
DEC | float64 | deg | Declination (J2000) |
Z_LAMBDA | float32 | None | Photometric redshift |
Z_LAMBDA_E | float32 | None | 1 sigma error on Z_LAMBDA |
KT | float64 | keV | Temperature measured by MBProj2D |
KT_L | float64 | keV | 1sigma lower limit of KT |
KT_H | float64 | keV | 1sigma upper limit of KT |
L500 | float64 | 10**42 erg s-1 | 0.2-2.3keV luminosity within R500 |
L500_L | float64 | 10**42 erg s-1 | 1sigma lower limit of L500 |
L500_H | float64 | 10**42 erg s-1 | 1sigma upper limit of L500 |
CR500 | float64 | s-1 | Count rate within R500 (CR500) |
CR500_L | float64 | s-1 | 1sigma lower limit of CR500 |
CR500_H | float64 | s-1 | 1sigma upper limit of CR500 |
CR500_NH0 | float64 | s-1 | Unabsorbed count rate within R500 |
CR500_L_NH0 | float64 | s-1 | 1sigma lower limit of CR500_NH0 |
CR500_H_NH0 | float64 | s-1 | 1sigma upper limit of CR500_NH0 |
MGAS500 | float64 | 10**11 solMass | Gas Mass within R500 |
MGAS500_L | float64 | 10**11 solMass | 1sigma lower limit of MGAS500 |
MGAS500_H | float64 | 10**11 solMass | 1sigma upper limit of MGAS500 |
YX500 | float64 | 10**11 keV solMass | The mass proxy Yx within R500 |
YX500_L | float64 | 10**11 keV solMass | 1sigma lower limit of YX500 |
YX500_H | float64 | 10**11 keV solMass | 1sigma upper limit of YX500 |
This work is based on data from eROSITA, the soft X-ray instrument aboard SRG, a joint Russian-German science mission supported by the Russian Space Agency (Roskosmos), in the interests of the Russian Academy of Sciences represented by its Space Research Institute (IKI), and the Deutsches Zentrum für Luft- und Raumfahrt (DLR). The SRG spacecraft was built by Lavochkin Association (NPOL) and its subcontractors and is operated by NPOL with support from the Max Planck Institute for Extraterrestrial Physics (MPE). The development and construction of the eROSITA X-ray instrument was led by MPE, with contributions from the Dr. Karl Remeis Observatory Bamberg \& ECAP (FAU Erlangen-Nuernberg), the University of Hamburg Observatory, the Leibniz Institute for Astrophysics Potsdam (AIP), and the Institute for Astronomy and Astrophysics of the University of Tübingen, with the support of DLR and the Max Planck Society. The Argelander Institute for Astronomy of the University of Bonn and the Ludwig Maximilians Universität Munich also participated in the science preparation for eROSITA. The eROSITA data shown here were processed using the eSASS/NRTA software system developed by the German eROSITA consortium.