ClG J1037-1243 , the SIMBAD biblio

ClG J1037-1243 , the SIMBAD biblio (40 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.30CEST15:45:51


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Title First 3 Authors
2001ApJS..137..117G viz 1185 111 The Las Campanas distant cluster survey: the catalog. GONZALEZ A.H., ZARITSKY D., DALCANTON J.J., et al.
2002ApJ...579..577G 40 12 Tests of the Las Campanas distant cluster survey from confirmation observations for the ESO distant cluster survey. GONZALEZ A.H., ZARITSKY D., SIMARD L., et al.
2003Msngr.112...19R 10 4 Studying high redshift galaxy clusters with the ESO Distant Cluster Survey. RUDNICK G., WHITE S., ARAGON-SALAMANCA A., et al.
2004A&A...427..397H viz 661 84 Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS). Redshifts, velocity dispersions and substructure for 5 clusters. HALLIDAY C., MILVANG-JENSEN B., POIRIER S., et al.
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.
2006A&A...451..395C 1 20 71 Weak lensing mass reconstructions of the ESO Distant Cluster Survey. CLOWE D., SCHNEIDER P., ARAGON-SALAMANCA A., et al.
2006ApJ...642..188P 2 65 263 The evolution of the star formation activity in galaxies and its dependence on environment. POGGIANTI B.M., VON DER LINDEN A., DE LUCIA G., 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.
2007ApJ...660.1151D viz 2 25 138 The morphological content of 10 EDisCS clusters at 0.5 < z < 0.8. DESAI V., DALCANTON J.J., 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 17       D               2 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.
2009ApJ...700.1559R 130       D     X   F     3 27 90 The rest-frame optical luminosity function of cluster galaxies at z < 0.8 and the assembly of the cluster red sequence. RUDNICK G., VON DER LINDEN A., PELLO R., et al.
2009A&A...501..419B 15       D               1 77 21 The orbital velocity anisotropy of cluster galaxies: evolution. BIVIANO A. and POGGIANTI B.M.
2009A&A...508.1141S 15       D               3 22 32 Evolution of the early-type galaxy fraction in clusters since z = 0.8. SIMARD L., CLOWE D., DESAI V., et al.
2009A&A...508.1173P 205       D     X         6 21 39 Photometric redshifts and cluster tomography in the ESO distant cluster survey. PELLO R., RUDNICK G., DE LUCIA G., et al.
2010ApJ...711..192J 130       D     X   F     3 34 46 The environmental dependence of the evolving S0 fraction. JUST D.W., ZARITSKY D., SAND D.J., et al.
2010MNRAS.405..995P 15       D               1 18 28 The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts. POGGIANTI B.M., DE LUCIA G., VARELA J., et al.
2010ApJ...720...87F 16       D               1 19 43 Dust-obscured star formation in intermediate redshift galaxy clusters. FINN R.A., DESAI V., RUDNICK G., 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.412..246V 39           X         1 31 77 Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0. VULCANI B., POGGIANTI B.M., ARAGON-SALAMANCA A., et al.
2011MNRAS.413..921V 38           X         1 87 18 The evolution of early-type galaxies in clusters from z∼ 0.8 to z ∼ 0: the ellipticity distribution and the morphological mix. VULCANI B., POGGIANTI B.M., DRESSLER A., et al.
2012A&A...537A..64G 365       D     X C F     8 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 173       D     X C       4 138 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.
2015MNRAS.450.3665S viz 16       D               1 430 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
2016A&A...589A..82C 16       D               1 37 6 Disc colours in field and cluster spiral galaxies at 0.5 ≲ z ≲ 0.8. CANTALE N., JABLONKA P., COURBIN F., et al.
2016A&A...595A..73B 16       D               4 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.
2017ApJ...850..181R viz 16       D               1 491 6 Determining the halo mass scale where galaxies lose their gas. RUDNICK G., JABLONKA P., MOUSTAKAS J., 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.
2019A&A...622A..78D 309       D     X C F     6 39 3 Link between brightest cluster galaxy properties and large scale extensions of 38 DAFT/FADA and CLASH clusters in the redshift range 0.2 < z < 0.9. DURRET F., TARRICQ Y., MARQUEZ I., 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...880..119C 17       D               1 25 ~ The rest-frame H-band luminosity function of red-sequence galaxies in clusters at 1.0 < z < 1.3. CHAN J.C.C., WILSON G., RUDNICK G., et al.
2019ApJ...885....6J 268       D     X         7 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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