ClG J1054-1245 , the SIMBAD biblio

ClG J1054-1245 , the SIMBAD biblio (55 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST03:02:18

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		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.
2004ApJ...610L..77D 10 5 154 The buildup of the red sequence in galaxy clusters since z ∼ 0.8. DE LUCIA G., POGGIANTI B.M., ARAGON-SALAMANCA A., 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.
2005ApJ...630..206F viz 267 138 Hα-derived star formation rates for three z≃0.75 EDisCS galaxy clusters. FINN R.A., ZARITSKY D., McCARTHY D.W.Jr, 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.
2008ApJ...679..279F 230           X         6 3 26 Mass and redshift dependence of star formation in relaxed galaxy clusters. FINN R.A., BALOGH M.L., ZARITSKY D., 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.
2008ApJ...684..888P 2 24 131 The relation between star formation, morphology, and local density in high-redshift clusters and groups. POGGIANTI B.M., DESAI V., FINN R., et al.
2009ApJ...693..112P 131       D     X         4 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.
2009ApJ...693..617H viz 53       D     X         2 91 30 The ellipticities of cluster early-type galaxies from z ∼ 1 to z ∼ 0: no evolution in the overall distribution of bulge-to-disk ratios. HOLDEN B.P., FRANX M., ILLINGWORTH G.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 168       D       C 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 53       D     X         2 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 92       D         F     1 34 46 The environmental dependence of the evolving S0 fraction. JUST D.W., ZARITSKY D., SAND D.J., et al.
2010MNRAS.401L..39V 15       D               2 10 7 Quantitative measure of evolution of bright cluster galaxies at moderate redshifts. VIKRAM V., WADADEKAR Y., KEMBHAVI A.K., et al.
2010MNRAS.403.1611K 231           X   F     5 16 79 Panoramic Hα and mid-infrared mapping of star formation in a z = 0.8 cluster. KOYAMA Y., KODAMA T., SHIMASAKU K., 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.
2010MNRAS.407L..94S 39           X         1 3 11 Constraining the thermal dust content of Lyman break galaxies in an overdense field at z ~ 5. STANWAY E.R., BREMER M.N., DAVIES L.J.M., et al.
2010ApJ...721L..19V 79             C       1 9 64 Superdense massive galaxies in the ESO distant cluster survey (EDisCS). VALENTINUZZI T., POGGIANTI B.M., SAGLIA R.P., et al.
2010A&A...523A..21G 53       D     X         2 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 53       D     X         2 314 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.
2011MNRAS.412..246V 16       D               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 54       D     X         2 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 94       D         F     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.
2012MNRAS.420.1481V 15       D               1 35 35 The importance of the local density in shaping the galaxy stellar mass functions. VULCANI B., POGGIANTI B.M., FASANO G., et al.
2012A&A...544A.104V viz 93       D     X         3 222 3 Cl 1103.7-1245 at z = 0.96: the highest redshift galaxy cluster in the EDisCS survey. VULCANI B., ARAGON-SALAMANCA A., POGGIANTI B.M., 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 212       D     X C       5 138 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.
2015A&A...575A.116M 33 13 The evolution of the cluster optical galaxy luminosity function between z = 0.4 and 0.9 in the DAFT/FADA survey. MARTINET N., DURRET F., GUENNOU L., 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               2 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.
2017MNRAS.472..254C 81           X         2 18 8 The morphological transformation of red sequence galaxies in clusters since z ∼ 1. CERULO P., COUCH W.J., LIDMAN C., et al.
2018MNRAS.475..523L 263       D     X C F     5 18 4 Star-formation rates of cluster galaxies: nature versus nurture. LAGANA T.F. and ULMER M.P.
2018A&A...618A.128C 41           X         1 35 1 Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ∼ 1.4. CASASOLA V., MAGRINI L., COMBES F., et al.
2018ApJ...869....6D 99       D     X         3 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 17       D               5 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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