MARD-Y3 catalog : J/MNRAS/488/739


Authors : Klein M. orcid , Grandis S., Mohr J.J. (hide) , Grandis S., Mohr J.J. et..al

Bibcode : 2019MNRAS.488..739K (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Clusters, galaxy; X-ray sources; Redshifts
UAT : Galaxy clusters, X-ray sources, Redshifted

Observation (OC)

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Inserted into VizieR : 31-Jul-2019
Last modification : 15-May-2025

A new RASS galaxy cluster catalogue with low contamination extending to z~1 in the DES overlap region. (2019)

Keywords : galaxies clusters: general - galaxies: clusters: intracluster medium - galaxies: distances and redshifts

Abstract:We present the MARD-Y3 catalogue of between 1086 and 2171 galaxy clusters (52 per cent and 65 per cent new) produced using multicomponent matched filter (MCMF) follow-up in 5000 deg^2^ of DES-Y3 optical data of the ~20000 overlapping ROSAT All-Sky Survey source catalogue (2RXS) X-ray sources. Optical counterparts are identified as peaks in galaxy richness as a function of redshift along the line of sight towards each 2RXS source within a search region informed by an X-ray prior. All peaks are assigned a probability fcont of being a random superposition. The clusters lie at 0.02<z<1.1 with more than 100 clusters at z>0.5. Residual contamination is 2.6 per cent and 9.6 per cent for the cuts adopted here. For each cluster we ...(more)
Abstract: (hide)
This is the MARD-Y3 catalog. X-ray selected, optically confirmed cluster catalog (see abstract and paper). The intput X-ray catalog is the RASS based 2RXS catalog (Boller+16). Entries from RA_DEG to EXI_ML are taken from 2RXS. Names are based on 2RXS but the first 3 letters are replaced by MARD (Multi-component mAtch filter confirmed RASS sources using DES data. MCMF keeps up to three counterparts P1..P3) per X-ray candidate. entries ending with _P1.._P3 correspond to the different peaks. Entries ending in _LFCR show the counter part with the lowest f_cont, therefore most likely counterpart. F_cont provides a measure of the contamination fraction caused by random superpositions. A catalog is expected to have a contamination fraction of X when clusters are selected as f_cont<=X. he full catalog provided here is cut at f_cont_LFCR<=0.2 and therefore allows for 20% residual contamination by chance super positions between 2RXS source and optical counter part. The X-ray source detection tends to detect large extended sources as multiple sources. We therefore suggest to exclude multiple detections by selection MULTIPLE_FLAG=0, the most likely counter part will remain in the sample but sourrounding multiples will be excluding. Remaining contamination can be reduced by selecting D_SIG_LFCR<2 (sigma), which excludes candidates with a reasonable WISE counterpart in NWAY and differs more than 2 sigma high (too high luminosity given richness) from the mean luminosity richness relation. DFC_LFCR provides the difference between lowest and second lowest f_cont of the X-ray source. This allows to identify cases with multiple counter parts at different redshifts.
Matthias Klein, matthias.klein(at)physik.lmu.de

                
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