ClG J1103-1246 , the SIMBAD biblio

ClG J1103-1246 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST11:30:51


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Title First 3 Authors
2005A&A...444..365W viz 50 127 EDisCS - the ESO distant cluster survey. Sample definition and optical photometry. WHITE S.D.M., CLOWE D.I., SIMARD L., et al.
2007MNRAS.374..809D 4 22 198 The build-up of the colour-magnitude relation in galaxy clusters since z ∼ 0.8. DE LUCIA G., POGGIANTI B.M., ARAGON-SALAMANCA A., et al.
2008A&A...482..419M viz 1341 75 Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields. MILVANG-JENSEN B., NOLL S., HALLIDAY C., et al.
2008MNRAS.387.1253W 15       D               1 91 99 The evolution of the brightest cluster galaxies since z ∼ 1 from the ESO Distant Cluster Survey (EDisCS). WHILEY I.M., ARAGON-SALAMANCA A., DE LUCIA G., et al.
2009ApJ...693..112P 93       D     X         3 28 134 The environments of starburst and post-starburst galaxies at z = 0.4-0.8. POGGIANTI B.M., ARAGON-SALAMANCA A., ZARITSKY D., et al.
2009A&A...497..713B 15       D               1 20 26 Frequency and properties of bars in cluster and field galaxies at intermediate redshifts. BARAZZA F.D., JABLONKA P., DESAI V., et al.
2009A&A...499...47S viz 76               F     1 241 72 Evolution of red-sequence cluster galaxies from redshift 0.8 to 0.4: ages, metallicities, and morphologies. SANCHEZ-BLAZQUEZ P., JABLONKA P., NOLL S., et al.
2009Msngr.136...54P 76             C       1 4 3 The ESO Distant Cluster sample: galaxy evolution and environment out to z = 1. POGGIANTI B., ARAGON-SALAMANCA A., BAMFORD S., et al.
2010A&A...523A..21G 15       D               1 15 20 The DAFT/FADA survey. I. Photometric redshifts along lines of sight to clusters in the z=[0.4,0.9] interval. GUENNOU L., ADAMI C., ULMER M.P., et al.
2010A&A...524A...6S viz 15       D               1 314 67 The fundamental plane of EDisCS galaxies. The effect of size evolution. SAGLIA R.P., SANCHEZ-BLAZQUEZ P., BENDER R., et al.
2011MNRAS.410..280J 15       D               2 52 23 The colour–magnitude relation of elliptical and lenticular galaxies in the ESO distant cluster survey. JAFFE Y.L., ARAGON-SALAMANCA A., DE LUCIA G., et al.
2012A&A...537A..64G 1 13 26 Intracluster light in clusters of galaxies at redshifts 0.4 < z< 0.8. GUENNOU L., ADAMI C., DA ROCHA C., et al.
2013A&A...550A..58V 17       D               1 21 44 The galaxy stellar mass function and its evolution with time show no dependence on global environment. VULCANI B., POGGIANTI B.M., OEMLER A.Jr, et al.
2014A&A...561A.112G 39           X         1 138 18 Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range. GUENNOU L., ADAMI C., DURRET F., et al.
2015MNRAS.450.1246K 16       D               1 16 13 Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey. KELKAR K., ARAGON-SALAMANCA A., GRAY M.E., et al.
2016A&A...595A..73B 16       D               1 38 5 Velocity segregation effects in galaxy clusters at 0.4 ≤ z ≤ 1.5. BARSANTI S., GIRARDI M., BIVIANO A., et al.
2017MNRAS.469.4551K 16       D               1 14 7 The effect of the environment on the structure, morphology and star formation history of intermediate-redshift galaxies. KELKAR K., GRAY M.E., ARAGON-SALAMANCA A., et al.
2018ApJ...869....6D 16       D               1 17 1 Tidal interactions and mergers in intermediate-redshift EDisCS clusters. DEGER S., RUDNICK G., KELKAR K., et al.
2019MNRAS.486..868K 17       D               1 13 2 The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase-space view of EDisCS. KELKAR K., GRAY M.E., ARAGON-SALAMANCA A., et al.
2019ApJ...885....6J 17       D               3 27 ~ Preprocessing among the infalling galaxy population of EDisCS clusters. JUST D.W., KIRBY M., ZARITSKY D., et al.
2021A&A...649A..42C viz 17       D               1 141 14 Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data. CHU A., DURRET F. and MARQUEZ I.

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