SpARCS J003550-431224 , the SIMBAD biblio

SpARCS J003550-431224 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.12.02CET14:24:53


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2009ApJ...697..436H 38           X         1 74 54 The XMM cluster survey: galaxy morphologies and the color-magnitude relation in XMMXCS J2215.9-1738 at z = 1.46. HILTON M., STANFORD S.A., STOTT J.P., et al.
2009ApJ...698.1943W 901     A S   X C       22 26 61 Spectroscopic confirmation of a massive red-sequence-selected galaxy cluster at z = 1.34 in the SpARCS-south Cluster Survey. WILSON G., MUZZIN A., YEE H.K.C., et al.
2010ApJ...711.1185D 131       D     X         4 90 45 Spectroscopic confirmation of three red-sequence selected galaxy clusters at z = 0.87, 1.16, and 1.21 from the SpARCS survey. DEMARCO R., WILSON G., MUZZIN A., et al.
2012ApJ...746..188M 180       D     X         5 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.
2012ApJ...749..169G 39           X         1 80 56 The mid-infrared environments of high-redshift radio galaxies. GALAMETZ A., STERN D., DE BREUCK C., et al.
2012MNRAS.427..550L 250       D     X   F     6 148 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.
2013ApJ...767...39M 41           X         1 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 174       D     X         5 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.
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...564A..17N 95       D       C       2 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.
2015ApJ...812..138F 96       D       C       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.
2016MNRAS.457.2209C 82           X         2 15 18 The accelerated build-up of the red sequence in high-redshift galaxy clusters. CERULO P., COUCH W.J., LIDMAN C., et al.
2017MNRAS.470.4168B 428       D     X C F     9 23 7 Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description. BALOGH M.L., GILBANK D.G., MUZZIN A., et al.
2018MNRAS.479.3563F viz 184       D       C F     7 42 3 The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75. FRIEDMANN M. and MAOZ D.
2019MNRAS.484..595M 145       D     X         4 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.
2020MNRAS.493.5987O 17       D               1 12 ~ The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5. OLD L.J., BALOGH M.L., VAN DER BURG R.F.J., et al.
2020MNRAS.495.3859W 148       D     X         4 51 ~ See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies. WILLIAMS S.C., HOOK I.M., HAYDEN B., et al.
2020A&A...638A.112V 17       D               1 12 ~ The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching. VAN DER BURG R.F.J., RUDNICK G., BALOGH M.L., et al.
2020MNRAS.498.5317W 17       D               1 12 ~ The GOGREEN survey: post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1. WEBB K., BALOGH M.L., LEJA J., 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.
2021MNRAS.502.5882F 18       D               3 67 ~ The delay time distribution of Type-Ia supernovae in galaxy clusters: the impact of extended star-formation histories. FREUNDLICH J. and MAOZ D.
2021ApJ...912...87H 18       D               1 70 ~ The HST See Change program. I. Survey design, pipeline, and supernova discoveries. HAYDEN B., RUBIN D., BOONE K., et al.
2021A&A...649A..42C viz 18       D               3 23 ~ Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data. CHU A., DURRET F. and MARQUEZ I.
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.
2021MNRAS.508..157M 18       D               1 12 ~ The GOGREEN survey: transition galaxies and the evolution of environmental quenching. McNAB K., BALOGH M.L., VAN DER BURG R.F.J., et al.
2021ApJ...920...32C 18       D               1 15 ~ The GOGREEN survey: evidence of an excess of quiescent disks in clusters at 1.0 < z < 1.4. CHAN J.C.C., WILSON G., BALOGH M., et al.
2021ApJ...923..222M 152       D     X         4 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 19       D               1 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.

goto View the references in ADS


2022.12.02-14:24:53

© Université de Strasbourg/CNRS

    • Contact