RCS J2345.4-3632 , the SIMBAD biblio

RCS J2345.4-3632 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST18:26:43

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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
2009AJ....138.1271D 90       D     X         3 71 55 An intensive Hubble space telescope survey for z>1 type Ia supernovae by targeting galaxy clusters. DAWSON K.S., ALDERING G., AMANULLAH R., et al.
2011ApJ...737...59J 281       D S   X C       6 35 92 Scaling relations and overabundance of massive clusters at z ≳ 1 from weak-lensing studies with the Hubble space telescope. JEE M.J., DAWSON K.S., HOEKSTRA H., et al.
2012ApJ...745...32B 15       D               1 75 42 The Hubble space telescope cluster supernova survey. II. The type Ia supernova rate in high-redshift galaxy clusters. BARBARY K., ALDERING G., AMANULLAH R., et al.
2012ApJ...750....1M 53       D     X         2 76 36 The Hubble space telescope cluster supernova survey. III. Correlated properties of type Ia supernovae and their hosts at 0.9 < z < 1.46. MEYERS J., ALDERING G., BARBARY K., et al.
2013MNRAS.433..825L 362       D     X         10 20 74 The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z = 1. LIDMAN C., IACOBUTA G., BAUER A.E., et al.
2013MNRAS.434..878S 15       D               2 32 23 The mass-concentration relation in massive galaxy clusters at redshift ∼ 1. SERENO M. and COVONE G.
2014MNRAS.441..203D viz 482       D     X   F     12 14 58 Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5. DELAYE L., HUERTAS-COMPANY M., MEI S., et al.
2015MNRAS.449.2024S 16       D               1 106 30 The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects. SERENO M., GIOCOLI C., ETTORI S., et al.
2015MNRAS.450.3665S viz 16       D               1 430 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
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.
2016MNRAS.457.2209C 999       D     X C F     24 15 25 The accelerated build-up of the red sequence in high-redshift galaxy clusters. CERULO P., COUCH W.J., LIDMAN C., et al.
2017ApJ...846..120B 238           X C       5 43 17 The KMOS Cluster Survey (KCS). I. The fundamental plane and the formation ages of cluster galaxies at redshift 1.4 < z < 1.6. BEIFIORI A., MENDEL J.T., CHAN J.C.C., et al.
2017MNRAS.472..254C 254       D     X   F     6 18 8 The morphological transformation of red sequence galaxies in clusters since z ∼ 1. CERULO P., COUCH W.J., LIDMAN C., et al.
2018MNRAS.476.1991G 16       D               2 47 1 Spectroscopic characterization of galaxy clusters in RCS-1: spectroscopic confirmation, redshift accuracy, and dynamical mass-richness relation. GILBANK D.G., BARRIENTOS L.F., ELLINGSON E., et al.
2021ApJ...911...82C viz 17       D               1 388 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.
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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