[MNH2008] cl J1227.9-1138a , the SIMBAD biblio

[MNH2008] cl J1227.9-1138a , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST10:36:43


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Title First 3 Authors
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.
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 91       D       C       3 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.
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.
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.
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.
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.

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