ACT-CL J0215.3-0343 , the SIMBAD biblio

ACT-CL J0215.3-0343 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.12.02CET14:59:00


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Title First 3 Authors
2012ApJ...746..188M 24       D               1 10 163 The Gemini cluster astrophysics spectroscopic survey (GCLASS): the role of environment and self-regulation in galaxy evolution at z ∼ 1. MUZZIN A., WILSON G., YEE H.K.C., et al.
2012MNRAS.423.3561C viz 16       D               1 424 41 The cosmological analysis of X-ray cluster surveys – II. Application of the CR–HR method to the XMM archive. CLERC N., SADIBEKOVA T., PIERRE M., et al.
2012MNRAS.427..550L 94       D         F     5 148 96 Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years. LIDMAN C., SUHERLI J., MUZZIN A., et al.
2013MNRAS.430..134W 16       D               1 73 26 Distant galaxy clusters in the XMM Large Scale Structure survey. WILLIS J.P., CLERC N., BREMER M.N., et al.
2013ApJ...767...39M 120           X C       2 13 64 Discovery of a rich cluster at z = 1.63 using the rest-frame 1.6 µm "stellar bump sequence" method. MUZZIN A., WILSON G., DEMARCO R., et al.
2013MNRAS.433..825L 17       D               3 20 63 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.
2013A&A...557A..15V 18       D               3 11 57 The environmental dependence of the stellar mass function at z ∼ 1. Comparing cluster and field between the GCLASS and UltraVISTA surveys. VAN DER BURG R.F.J., MUZZIN A., HOEKSTRA H., et al.
2013A&A...557A..81M viz 16       D               1 4209 16 Classification and environmental properties of X-ray selected point-like sources in the XMM-LSS field. MELNYK O., PLIONIS M., ELYIV A., et al.
2014A&A...561A..79V 17       D               3 10 32 A census of stellar mass in ten massive haloes at z ∼ 1 from the GCLASS Survey. VAN DER BURG R.F.J., MUZZIN A., HOEKSTRA H., et al.
2014A&A...567A..83K 16       D               1 34 13 X-ray AGN in the XMM-LSS galaxy clusters: no evidence of AGN suppression. KOULOURIDIS E., PLIONIS M., MELNYK O., et al.
2014MNRAS.444.2723C 16       D               1 54 29 The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg^2 and its spatial distribution. CLERC N., ADAMI C., LIEU M., et al.
2015ApJ...812..138F 16       D               3 16 15 Evidence for the universality of properties of red-sequence galaxies in x-ray- and red-sequence-selected clusters at z ∼ 1. FOLTZ R., RETTURA A., WILSON G., et al.
2015MNRAS.452.1171W viz 16       D               1 120 43 The XMM Cluster Survey: testing chameleon gravity using the profiles of clusters. WILCOX H., BACON D., NICHOL R.C., et al.
2016A&A...592A...1P viz 16       D               1 5977 113 The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme. PIERRE M., PACAUD F., ADAMI C., et al.
2016A&A...592A...2P viz 16       D               2 118 67 The XXL Survey. II. The bright cluster sample: catalogue and luminosity function. PACAUD F., CLERC N., GILES P.A., et al.
2016A&A...592A...3G 16       D               2 108 33 The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample. GILES P.A., MAUGHAN B.J., PACAUD F., et al.
2016A&A...592A..12E 16       D               1 106 28 The XXL Survey. XIII. Baryon content of the bright cluster sample. ECKERT D., ETTORI S., COUPON J., et al.
2016A&A...593A...2A viz 268     A     X C       6 174 12 Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr. ANDREON S., DONG H. and RAICHOOR A.
2016MNRAS.462.4141L viz 16       D               2 170 5 The XXL survey XV: evidence for dry merger driven BCG growth in XXL-100-GC X-ray clusters. LAVOIE S., WILLIS J.P., DEMOCLES J., et al.
2018MNRAS.477.5517W 17       D               1 19 ~ X-ray versus infrared selection of distant galaxy clusters: a case study using the XMM-LSS and SpARCS cluster samples. WILLIS J.P., RAMOS-CEJA M.E., MUZZIN A., et al.
2018A&A...620A...5A 17       D               1 307 ~ The XXL Survey. XX. The 365 cluster catalogue. ADAMI C., GILES P., KOULOURIDIS E., et al.
2018A&A...620A..18L viz 226       D     X         6 9 ~ The XXL Survey. XXXIII. Chandra constraints on the AGN contamination of z > 1 XXL galaxy clusters. LOGAN C.H.A., MAUGHAN B.J., BREMER M.N., et al.
2018PASJ...70S..20O viz 17       D               1 1922 ~ An optically-selected cluster catalog at redshift 0.1 < z < 1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data. OGURI M., LIN Y.-T., LIN S.-C., et al.
2019MNRAS.484..595M 17       D               1 11 ~ HST/WFC3 grism observations of z ∼ 1 clusters: the cluster versus field stellar mass-size relation and evidence for size growth of quiescent galaxies from minor mergers. MATHARU J., MUZZIN A., BRAMMER G.B., et al.
2019ApJ...875...63M 145       D     X C       3 8 ~ Weak-lensing mass calibration of ACTPol Sunyaev-Zel'dovich clusters with the Hyper Suprime-Cam Survey. MIYATAKE H., BATTAGLIA N., HILTON M., et al.
2020ApJ...890..148U viz 17       D               1 92 ~ Weak-lensing analysis of X-ray-selected XXL galaxy groups and clusters with Subaru HSC data. UMETSU K., SERENO M., LIEU M., et al.
2021MNRAS.500..358B 18       D               1 18 ~ The GOGREEN and GCLASS surveys: first data release. BALOGH M.L., VAN DER BURG R.F.J., MUZZIN A., et al.
2021ApJ...911...82C 18       D               2 387 ~ 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...650A.105B 18       D               1 14 ~ The GOGREEN survey: Internal dynamics of clusters of galaxies at redshift 0.9-1.4. BIVIANO A., VAN DER BURG R.F.J., BALOGH M.L., et al.
2021ApJ...923..222M 63       D     X         2 11 ~ HST/WFC3 grism observations of z ∼ 1 clusters: evidence for rapid outside-in environmental quenching from spatially resolved Hα maps. MATHARU J., MUZZIN A., BRAMMER G.B., et al.
2022MNRAS.510..674W 159       D     X C       3 16 ~ Satellite quenching was not important for z ∼ 1 clusters: most quenching occurred during infall. WERNER S.V., HATCH N.A., MUZZIN A., et al.

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2022.12.02-14:59:00

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