BAX 205.7046+40.4697 , the SIMBAD biblio

BAX 205.7046+40.4697 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST12:48:43


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Title First 3 Authors
1998ApJ...502..558V viz 223 354 A catalog of 200 galaxy clusters serendipitously detected in the ROSAT PSPC pointed observations. VIKHLININ A., McNAMARA B.R., FORMAN W., et al.
2003ApJ...594..154M viz 235 95 The 160 square degree ROSAT survey: the revised catalog of 201 clusters with spectroscopic redshifts. MULLIS C.R., McNAMARA B.R., QUINTANA H., et al.
2004A&A...424.1097S viz 15       D               1 1674 24 Introducing BAX: A database for X-ray clusters and groups of galaxies. SADAT R., BLANCHARD A., KNEIB J.-P., et al.
2005ApJ...633..781K 2 10 63 XMM-Newton observations of evolution of cluster X-ray scaling relations at z=0.4-0.7. KOTOV O. and VIKHLININ A.
2008ApJS..176..374H viz 15       D               129 24 The WARPS survey. VII. The WARPS-II cluster catalog. HORNER D.J., PERLMAN E.S., EBELING H., et al.
2009ApJ...698..317A 15       D               2 29 19 Redshift evolution in the iron abundance of the intracluster medium. ANDERSON M.E., BREGMAN J.N., BUTLER S.C., et al.
2010MNRAS.401.1587V viz 38           X         1 43 2 A far-infrared survey at the North Galactic Pole - I. Nearby star-forming galaxies and effect of confused sources on source counts. VAISANEN P., KOTILAINEN J.K., JUVELA M., et al.
2011ApJ...731...31S 15       D               2 85 25 Evidence for rapid redshift evolution of strong cluster cooling flows. SAMUELE R., McNAMARA B.R., VIKHLININ A., et al.
2011A&A...534A.109P viz 15       D               1 1770 422 The MCXC: a meta-catalogue of X-ray detected clusters of galaxies. PIFFARETTI R., ARNAUD M., PRATT G.W., et al.
2011A&A...535A...4R viz 15       D               1 225 108 Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ∼ 1.5. REICHERT A., BOEHRINGER H., FASSBENDER R., et al.
2012A&A...537A.142B 15       D               2 40 32 An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters. BALDI A., ETTORI S., MOLENDI S., et al.
2012MNRAS.423.3561C viz 15       D               1 424 44 The cosmological analysis of X-ray cluster surveys – II. Application of the CR–HR method to the XMM archive. CLERC N., SADIBEKOVA T., PIERRE M., et al.
2012MNRAS.425..477N viz 15       D               1 1763 27 γ-rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis. NEZRI E., WHITE R., COMBET C., et al.
2012A&A...546A...6A viz 15       D               1 131 18 The enrichment history of the intracluster medium: a Bayesian approach. ANDREON S.
2014MNRAS.437.2607N viz 291       D     X         8 8 6 Low X-ray luminosity galaxy clusters - II. Optical properties and morphological content at 0.18 < z < 0.70. NILO CASTELLON J.L., ALONSO M.V., LAMBAS D.G., et al.
2015A&A...578A..46E viz 16       D               2 83 27 The evolution of the spatially resolved metal abundance in galaxy clusters up to z = 1.4. ETTORI S., BALDI A., BALESTRA I., et al.
2015MNRAS.452.2225G 95       D     X         3 8 10 Low X-ray luminosity galaxy clusters - III. Weak lensing mass determination at 0.18 < z < 0.70. GONZALEZ E.J., FOEX G., NILO CASTELLON J.L., et al.
2016AJ....151..151N 337       D     X C       8 20 ~ Low X-ray luminosity galaxy clusters: main goals, sample selection, photometric and spectroscopic observations. NILO CASTELLON J.L., ALONSO M.V., LAMBAS D.G., et al.
2016MNRAS.463.1929M viz 16       D               1 174 3 The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters. MEHRTENS N., ROMER A.K., NICHOL R.C., et al.
2017MNRAS.468.3322S viz 16       D               1 28168 37 CoMaLit - V. Mass forecasting with proxies: method and application to weak lensing calibrated samples. SERENO M. and ETTORI S.
2021A&A...652A..12K viz 17       D               1 1564 14 The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5. KOULOURIDIS E., CLERC N., SADIBEKOVA T., et al.

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