A multicomponent matched filter cluster confirmation tool for eROSITA: initial application to the RASS and DES-SV data sets
- Ludwig-Maximilians-Univ. Munich (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
- Ludwig-Maximilians-Univ. Munich (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany); Excellence Cluster Universe, Garching (Germany)
- IIT Hyderabad, Telangana (India)
- Ludwig-Maximilians-Univ. Munich (Germany)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Institut d'Astrophysique de Paris, Paris (France); Univ. College London, London (United Kingdom); UPMC Univ. Paris, Paris (France)
- Univ. College London, London (United Kingdom)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Observatorio Nacional, Rio de Janeiro (Brazil)
- Univ. of Illinois, Urbana, IL (United States); National Center for Supercomputing Applications, Urbana, IL (United States)
- Stanford Univ.,Stanford, CA (United States)
- Ludwig-Maximilians-Univ. Munich (Germany); Excellence Cluster Universe, Garching (Germany)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
- Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- The Ohio State Univ., Columbus, OH (United States)
- Univ. of Washington, Seattle, WA (United States); National Optical Astronomy Observatory, La Serena (Chile)
- Australian Astronomical Observatory, North Ryde, NSW (Australia)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Univ. de Sao Paulo, Sao Paulo (Brazil)
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Princeton Univ., Princeton, NJ (United States)
- Institucio Catalana de Recerca i Estudis Avancats, Barcelona (Spain); The Barcelona Institute of Science and Technology, Bellaterra (Barcelona) (Spain)
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Univ. of Sussex, Brighton (United Kingdom)
- Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), Madrid (Spain)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Instituto de Fisica, Porto Alegre (Brazil)
- Univ. of Southampton, Southampton (United Kingdom)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Univ. Federal do ABC, Santo Andre (Brazil)
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
- National Center for Supercomputing Applications, Urbana, IL (United States)
We describe a multi-component matched filter cluster confirmation tool (MCMF) designed for the study of large X-ray source catalogs produced by the upcoming X-ray all-sky survey mission eROSITA. We apply the method to confirm a sample of 88 clusters with redshifts $0.05<0.8$ in the recently published 2RXS catalog from the ROSAT all-sky survey (RASS) over the 208 deg$^2$ region overlapped by the Dark Energy Survey (DES) science verification (DES-SV) dataset. In our pilot study, we examine all X-ray sources, regardless of their extent. Our method employs a multi-color red sequence (RS) algorithm that incorporates the X-ray count rate and peak position in determining the region of interest for followup and extracts the positionally and color weighted optical richness $$\lambda_{\mathrm{MCMF}}$$ as a function of redshift for each source. Peaks in the $$\lambda_{\mathrm{MCMF}}$$-redshift distribution are identified and used to extract photometric redshifts, richness and uncertainties. The significances of all optical counterparts are characterized using the distribution of richnesses defined along random lines of sight. These significances are used to extract cluster catalogs and to estimate the contamination by random superpositions of unassociated optical systems. The delivered photometric redshift accuracy is $$\delta z / (1+z)=0.010$$. We find a well defined X-ray luminosity-$$\lambda_{\mathrm{MCMF}}$$ relation with an intrinsic scatter of $$\delta \ln(\lambda_\mathrm{MCMF}| L_\mathrm{x})=0.21$$. Matching our catalog with the DES-SV redMaPPer catalog yields good agreement in redshift and richness estimates; comparing our catalog with the South Pole Telescope (SPT) selected clusters shows no inconsistencies. SPT clusters in our dataset are consistent with the high mass extension of the RASS based $$\lambda_{\mathrm{MCMF}}$$-mass relation
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
- Contributing Organization:
- The DES Collaboration
- Grant/Contract Number:
- AC02-76SF00515; AC05-00OR22725; AC02-07CH11359
- OSTI ID:
- 1423126
- Alternate ID(s):
- OSTI ID: 1408217; OSTI ID: 1422381
- Report Number(s):
- arXiv:1706.06577; FERMILAB-PUB-17-025-AE; TRN: US1801710
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Vol. 474, Issue 3; ISSN 0035-8711
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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