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We present the RASS-MCMF catalog of 8,465 X-ray selected galaxy clusters over 25,000 deg$^2$ of extragalactic sky. The accumulation of deep, multiband optical imaging data, the development of the Multi-Component Matched Filter cluster…

Cosmology and Nongalactic Astrophysics · Physics 2023-08-30 Matthias Klein , Daniel Hernández-Lang , Joseph J Mohr , Sebastian Bocquet , Aditya Singh

The eROSITA Final Equatorial-Depth Survey (eFEDS), covering ~140 square degrees, was performed as part of the performance verification phase of the eROSITA telescope on board of the Russian-German satellite Spectrum-Roentgen-Gamma (SRG). In…

Context. Clusters of galaxies are important for cosmology and astrophysics. They may be discovered through either the summed optical/IR radiation originating from their member galaxies or via X-ray emission originating from the hot…

Cosmology and Nongalactic Astrophysics · Physics 2016-12-21 Alexey Mints , Axel Schwope , Simon Rosen , François-Xavier Pineau , Francisco Carrera

We discuss an algorithm whereby the massive galaxy clusters detected in the SRG/eROSITA all-sky survey are identified and their photometric redshifts are estimated. For this purpose, we use photometric redshift estimates for galaxies and…

We investigate, using simulated galaxy catalogues, the completeness of searches for massive clusters of galaxies in redshift surveys or imaging surveys with photometric redshift estimates, i.e. what fraction of clusters (M>10^14/h Msun) are…

Astrophysics · Physics 2008-11-26 Martin White , C. S. Kochanek

We select galaxy cluster candidates from the high-redshift (BEST_Z > 0.9) end of the first SRG/eROSITA All-Sky Survey (eRASS1) galaxy cluster catalogue, for which we obtain moderately deep J-band imaging data with the OMEGA2000 camera at…

We describe updates to the \redmapper{} algorithm, a photometric red-sequence cluster finder specifically designed for large photometric surveys. The updated algorithm is applied to $150\,\mathrm{deg}^2$ of Science Verification (SV) data…

We present an extension to a Sunyaev-Zel'dovich Effect (SZE) selected cluster catalog based on observations from the South Pole Telescope (SPT); this catalog extends to lower signal-to-noise than the previous SPT-SZ catalog and therefore…

Cosmology and Nongalactic Astrophysics · Physics 2023-10-05 M. Klein , J. J. Mohr , S. Bocquet , M. Aguena , S. W. Allen , O. Alves , B. Ansarinejad , M. L. N. Ashby , D. Bacon , M. Bayliss , B. A. Benson , L. E. Bleem , M. Brodwin , D. Brooks , E. Bulbul , D. L. Burke , R. E. A. Canning , J. E. Carlstrom , A. Carnero Rosell , J. Carretero , C. L. Chang , C. Conselice , M. Costanzi , A. T. Crites , L. N. da Costa , M. E. S. Pereira , T. M. Davis , J. De Vicente , S. Desai , T. de Haan , M. A. Dobbs , P. Doel , I. Ferrero , A. M. Flores , J. Frieman , E. M. George , G. Giannini , M. D. Gladders , A. H. Gonzalez , S. Grandis , D. Gruen , R. A. Gruendl , G. Gutierrez , N. W. Halverson , S. R. Hinton , G. P. Holder , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. D. Hrubes , N. Huang , D. J. James , G. Khullar , K. Kim , L. Knox , R. Kraft , F. Kéruzoré , A. T. Lee , D. Luong-Van , G. Mahler , A. Mantz , D. P. Marrone , J. L. Marshall , M. McDonald , J. J. McMahon , J. Mena-Fernández , F. Menanteau , S. S. Meyer , R. Miquel , J. Myles , S. Padin , A. Pieres , A. A. Plazas Malagón , C. Pryke , C. L. Reichardt , K. Reil , J. Roberson , A. K. Romer , C. Romero , J. E. Ruhl , B. R. Saliwanchik , L. Salvati , E. Sanchez , A. Saro , K. K. Schaffer , T. Schrabback , M. Schubnell , I. Sevilla-Noarbe , K. Sharon , E. Shirokoff , M. Smith , T. Somboonpanyakul , B. Stalder , S. A. Stanford , A. A. Stark , V. Strazzullo , E. Suchyta , M. E. C. Swanson , G. Tarle , C. To , K. Vanderlinde , J. D. Vieira , A. von der Linden , N. Weaverdyck , R. Williamson , P. Wiseman , M. Young

The XMM Cluster Archive Super Survey (X-CLASS) is a serendipitously-detected X-ray-selected sample of 845 galaxy clusters based on 2774 XMM archival observations and covering approximately 90 deg$^2$ spread across the high-Galactic latitude…

Cosmology and Nongalactic Astrophysics · Physics 2017-04-12 J. Ridl , N. Clerc , T. Sadibekova , L. Faccioli , F. Pacaud , J. Greiner , T. Krühler , A. Rau , M. Salvato , M. -L. Menzel , H. Steinle , P. Wiseman , K. Nandra , J. Sanders

The first SRG/eROSITA All-Sky Survey (eRASS1) provides the largest intracluster medium-selected galaxy cluster and group catalog covering the western galactic hemisphere. Compared to samples selected purely on X-ray extent, the sample…

In November 2019, eROSITA on board of SRG observatory started to map the entire sky in X-rays. After the 4-year survey program, it will reach flux limits about 25 times deeper than ROSAT. During the SRG Performance Verification phase,…

We present and analyze the optical and X-ray catalogs of moderate-redshift cluster candidates from the ROSAT Optical X-ray Survey, or ROXS. The survey covers 4.8 square degrees (23 ROSAT PSPC pointings). The cross-correlated cluster…

We describe an automated method for detecting clusters of galaxies in imaging and redshift galaxy surveys. The Adaptive Matched Filter (AMF) method utilizes galaxy positions, magnitudes, and---when available---photometric or spectroscopic…

Astrophysics · Physics 2010-11-04 Jeremy Kepner , Xiaohui Fan , Neta Bahcall , James Gunn , Robert Lupton , Guohong Xu

We present an optimised galaxy cluster finder, 3D-Matched-Filter (3D-MF), which utilises galaxy cluster radial profiles, luminosity functions and redshift information to detect galaxy clusters in optical surveys. This method is an…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-07 M. Milkeraitis , L. Van Waerbeke , C. Heymans , H. Hildebrandt , J. P. Dietrich , T. Erben

Galaxy clusters are useful cosmological probes and interesting astrophysical laboratories. With growing cluster samples, a deeper understanding of the sample characteristics and improved control of systematics becomes more crucial. In this…

Cosmology and Nongalactic Astrophysics · Physics 2024-10-23 Matthias Klein , Joseph J. Mohr , Christopher T. Davies

We present a new catalog of high-redshift candidate \textit{Herschel} sources. Our sample is obtained after applying a multifrequency filtering method ("matched multifilter"), which is designed to improve the signal-to-noise ratio (S/N) of…

Astrophysics of Galaxies · Physics 2019-02-06 A. Manjón-García , D. Herranz , J. M. Diego , L. Bonavera , J. González-Nuevo

We present first results on the use of a colour space filter for detecting galaxy clusters at cosmological redshifts in the XMM Large Scale Structure Survey. All clusters studied, but one, are successfully colour--detected in spite of their…

Astrophysics · Physics 2007-05-23 S. Andreon , J. Willis , H. Quintana , I. Valtchanov , M. Pierre , F. Pacaud

Groups and clusters of galaxies are a current focus of astronomical research owing to their role in determining the environmental effects on galaxies and the constraints they provide to cosmology. The eROSITA X-ray telescope on board the…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-02 A. Finoguenov , A. Merloni , J. Comparat , K. Nandra , M. Salvato , E. Tempel , A. Raichoor , J. Richard , J. -P. Kneib , A. Pillepich , M. Sahlén , P. Popesso , P. Norberg , R. McMahon

We present MMT spectroscopic observations of two massive galaxy cluster candidates at redshift $z\sim0.07$ that show extended and diffuse X-ray emission in the ROSAT All Sky Survey (RASS) images. The targets were selected from a previous…

Cosmology and Nongalactic Astrophysics · Physics 2022-11-30 Kaiyuan Chen , Weiwei Xu , Linhua Jiang

The first SRG/eROSITA all-sky X-ray survey, eRASS1, resulted in a catalogue of over twelve thousand optically-confirmed galaxy groups and clusters in the western Galactic hemisphere. Using the eROSITA images of these objects, we measure and…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-19 J. S. Sanders , Y. E. Bahar , E. Bulbul , V. Ghirardini , A. Liu , N. Clerc , M. E. Ramos-Ceja , T. H. Reiprich , F. Balzer , J. Comparat , M. Kluge , F. Pacaud , X. Zhang
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