RASSCALS NRGs027 , the SIMBAD biblio

RASSCALS NRGs027 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST20:20:02


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Title First 3 Authors
2000ApJ...534..114M viz 289 82 The RASSCALS: an X-ray and optical study of 260 galaxy groups. MAHDAVI A., BOHRINGER H., GELLER M.J., et al.
2000ApJS..129..435B viz 638 455 The northern ROSAT all-sky (NORAS) galaxy cluster survey. I. X-ray properties of clusters detected as extended X-ray sources. BOHRINGER H., VOGES W., HUCHRA J.P., et al.
2001ApJ...554L.129M viz 364 78 The LX-σ relation for galaxies and clusters of galaxies. MAHDAVI A. and GELLER M.J.
2003A&A...406..535Z viz 10290 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
2004AJ....128.2022R 70 28 K-band properties of well-sampled groups of galaxies. RAMELLA M., BOSCHIN W., GELLER M.J., et al.
2004ApJ...607..202M viz 2459 39 A redshift survey of nearby galaxy groups: the shape of the mass density profile. MAHDAVI A. and GELLER M.J.
2009ApJS..184..138H viz 15       D               1 20666 68 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
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.
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.
2016ApJ...824..110O 17       D               2 28 40 The HI content of galaxies in groups and clusters as measured by ALFALFA. ODEKON M.C., KOOPMANN R.A., HAYNES M.P., 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.

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