The X-CLASS−redMaPPer galaxy cluster comparison
T. SadibekovaService d’astrophysique, IRFU, CEA Saclay, FranceM. PierrreService d’astrophysique, IRFU, CEA Saclay, FranceNicolas ClercMax Planck Institut für Extraterrestische Physik, Postfach 1312, 85741 Garching bei München, GermanyL. FaccioliService d’astrophysique, IRFU, CEA Saclay, FranceR. GastaudService d’électronique, des détecteurs et d’informatique, IRFU, CEA Saclay, FranceJ. P. Le FèvreService d’électronique, des détecteurs et d’informatique, IRFU, CEA Saclay, FranceEduardo RozoKIPAC, SLAC National Accelerator Laboratory, Menlo Park CA 94025, USAE. S. RykoffKIPAC, SLAC National Accelerator Laboratory, Menlo Park CA 94025, USA
2014en
ABI
Annotatsiya
Context. This paper is the first in a series undertaking a comprehensive correlation analysis between optically selected and X-ray-selected cluster catalogues. The rationale of the project is to develop a holistic picture of galaxy clusters utilising optical and X-ray-cluster-selected catalogues with well-understood selection functions.
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