SpARCS J003550-431224 , the SIMBAD biblio

SpARCS J003550-431224 , the SIMBAD biblio (35 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:37:34

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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
2009ApJ...697..436H 37           X         1 74 75 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 886     A S   X C       22 26 142 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 128       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 181       D     X         5 10 271 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 38           X         1 80 60 The mid-infrared environments of high-redshift radio galaxies. GALAMETZ A., STERN D., DE BREUCK C., et al.
2012MNRAS.427..550L 244       D     X   F     6 150 160 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 40           X         1 13 70 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 170       D     X         5 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.
2013A&A...557A..15V 19       D               3 11 103 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 40 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 93       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 94       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 79           X         2 15 25 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 413       D     X C F     9 23 41 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 177       D       C F     7 42 8 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 141       D     X         4 11 41 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 18       D               1 14 39 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 140       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 20       D               1 12 50 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 18       D               1 12 34 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 viz 18       D               1 19 21 The GOGREEN and GCLASS surveys: first data release. BALOGH M.L., VAN DER BURG R.F.J., MUZZIN A., et al.
2021MNRAS.502.5882F 17       D               3 67 16 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 17       D               1 70 7 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 17       D               4 141 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...650A.105B 17       D               1 14 9 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 13 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 17       D               1 15 5 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 viz 143       D     X         4 11 12 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 17       D               1 16 13 Satellite quenching was not important for z ∼ 1 clusters: most quenching occurred during infall. WERNER S.V., HATCH N.A., MUZZIN A., et al.
2022MNRAS.515.5479B 17       D               1 14 3 The GOGREEN survey: constraining the satellite quenching time-scale in massive clusters at z ≳ 1. BAXTER D.C., COOPER M.C., BALOGH M.L., et al.
2023MNRAS.519.4171O 218           X C F     3 3 ~ CALSAGOS: Clustering algorithms applied to galaxies in overdense systems. OLAVE-ROJAS D.E., CERULO P., ARAYA-ARAYA P., et al.
2024MNRAS.52710680G 152       D     X         4 18 ~ Spitzer-selected z > 1.3 protocluster candidates in the LSST Deep Drilling Fields. GULLY H., HATCH N., BAHE Y., et al.
2025MNRAS.539.3058G 1185       D     X C F     24 5 ~ Insights into environmental quenching at z ∼ 1: an enhancement of faint, low-mass passive galaxies in clusters. GULLY H., HATCH N., AHAD S.L., et al.
2025MNRAS.541..409H 19       D               1 17 ~ Distinct origins of environmentally quenched galaxies in the core and outer virialized regions of massive clusters at 0.8 < z < 1.5. HEWITT G., SARRON F., BALOGH M.L., et al.
2025ApJ...994..205A 19       D               2 14 ~ Dynamical Properties and Velocity Dispersion-Mass Relation of z ∼ 1 Galaxy Clusters from the GOGREEN and GCLASS Surveys. ABDULSHAFY S., ABDULLAH M.H., WILSON G., et al.

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