NAME XMMU J1229.4+0151 , the SIMBAD biblio

NAME XMMU J1229.4+0151 , the SIMBAD biblio (27 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST23:17:57


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Title First 3 Authors
2009A&A...501...49S 379   K A D     X C       10 32 31 Multiwavelength observations of a rich galaxy cluster at z ∼ 1. The HST/ACS colour-magnitude diagram. SANTOS J.S., ROSATI P., GOBAT R., et al.
2009AJ....138.1271D 91       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.
2010MNRAS.404.1603P 40           X         1 2 9 Signature of cool core in Sunyaev-Zeldovich clusters: a multiwavelength approach. PIPINO A. and PIERPAOLI E.
2011MNRAS.411.2667L 207       D     X         6 45 27 The massive galaxy cluster XMMU J1230.3+1339 at z ∼ 1: colour–magnitude relation, Butcher–Oemler effect, X-ray and weak lensing mass estimates. LERCHSTER M., SEITZ S., BRIMIOULLE F., et al.
2011A&A...527A..78F 77           X         2 25 25 A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z = 0.975. Observing the assembly of a massive system. FASSBENDER R., BOEHRINGER H., SANTOS J.S., et al.
2011ApJ...737...59J 285       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.
2011A&A...532L...6N 39           X         1 10 21 Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 at z = 1.49. Indications of a young system with a brightest galaxy in formation. NASTASI A., FASSBENDER R., BOEHRINGER 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...746...85S viz 59           X         1 35 1409 The Hubble Space Telescope Cluster Supernova Survey. V. Improving the dark-energy constraints above z > 1 and building an early-type-hosted supernova sample. SUZUKI N., RUBIN D., LIDMAN C., et al.
2012ApJ...750....1M 15       D               1 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.
2012A&A...540A..45P 39           X         1 24 12 First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND. The galaxy population of XMMU J0338.7+0030 at z = 1.1. PIERINI D., SUHADA R., FASSBENDER R., et al.
2013MNRAS.433..825L 251       D     X         7 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 16       D               2 32 23 The mass-concentration relation in massive galaxy clusters at redshift ∼ 1. SERENO M. and COVONE G.
2014MNRAS.439.2790C 4721 T K A D     X C F     118 65 7 The morphological transformation of red sequence galaxies in the distant cluster
XMMU J1229+0151.
CERULO P., COUCH W.J., LIDMAN C., et al.
2014A&A...564A..17N 16       D               1 26 6 Kinematic analysis of a sample of X-ray luminous distant galaxy clusters. The LX - σv relation in the z > 0.6 universe. NASTASI A., BOEHRINGER H., FASSBENDER R., et al.
2014MNRAS.441..203D viz 726       D     X C F     17 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.450.1268D 199           X   F     4 13 13 Morphological evolution in situ: disc-dominated cluster red sequences at z ∼ 1.25. DE PROPRIS R., BREMER M.N. and PHILLIPPS S.
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 1261       D     X C F     30 15 25 The accelerated build-up of the red sequence in high-redshift galaxy clusters. CERULO P., COUCH W.J., LIDMAN C., et al.
2016MNRAS.461.4517D 56       D     X         2 32 6 Morphological evolution of cluster red sequence galaxies in the past 9 Gyr. DE PROPRIS R., BREMER M.N. and PHILLIPPS S.
2017MNRAS.472..254C 707       D S   X   F     16 18 8 The morphological transformation of red sequence galaxies in clusters since z ∼ 1. CERULO P., COUCH W.J., LIDMAN C., et al.
2021ApJ...911...82C viz 174           X C       3 388 ~ 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.
2021A&A...652A..12K viz 17       D               1 1564 14 The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5. KOULOURIDIS E., CLERC N., SADIBEKOVA T., et al.
2023Natur.613...37J 19       D               1 10 3 Intracluster light is already abundant at redshift beyond unity. JOO H. and JEE M.J.

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