RCS J1107-0523 , the SIMBAD biblio

RCS J1107-0523 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:57:36


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Title First 3 Authors
2007AJ....134..282G 12 26 Spectroscopy of moderately high redshift RCS-1 clusters. GILBANK D.G., YEE H.K.C., ELLINGSON E., et al.
2008A&A...483...35S 54       D     X         2 38 177 Searching for cool core clusters at high redshift. SANTOS J.S., ROSATI P., TOZZI P., et al.
2008ApJ...680.1022H 16       D               7 13 44 Chandra X-ray observations of the 0.6 < z < 1.1 red-sequence cluster survey sample. HICKS A.K., ELLINGSON E., BAUTZ M., et al.
2008A&A...489..967B 387       D     X C       10 12 11 Intra cluster medium properties and AGN distribution in high-z RCS clusters. BIGNAMINI A., TOZZI P., BORGANI S., 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.
2014ARep...58..587B viz 15       D               1 137 42 Chandra X-ray galaxy clusters at z < 1.4: Constraints on the inner slope of the density profiles. BABYK Y.V., DEL POPOLO A. and VAVILOVA I.B.
2015MNRAS.447.3723P 16       D               1 91 8 The Chandra Deep Group Survey - cool core evolution in groups and clusters of galaxies. PASCUT A. and PONMAN T.J.
2016MNRAS.455..892G viz 16       D               1 353 14 The galaxy cluster concentration-mass scaling relation. GROENER A.M., GOLDBERG D.M. and SERENO M.
2018ApJ...859...65Y 16       D               1 23 15 X-ray properties of AGN in brightest cluster galaxies. I. A systematic study of the Chandra archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 redshift range. YANG L., TOZZI P., YU H., et al.
2020MNRAS.497.5485Y viz 16       D               1 871 15 Dynamical state for 964 galaxy clusters from Chandra X-ray images. YUAN Z.S. and HAN J.L.
2022MNRAS.513.3013Y viz 17       D               1 1644 7 Dynamical state of galaxy clusters evaluated from X-ray images. YUAN Z.S., HAN J.L. and WEN Z.L.

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