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SpARCS J003550-431224 , the SIMBAD biblio (31 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST05:34:21 |
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 | 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 | 896 | 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 | 130 | 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 | 183 | 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 | 39 | 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 | 248 | 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 | 41 | 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 | 173 | 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 | 20 | 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 | 18 | 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 | 94 | 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 | 95 | 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 | 81 | 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 | 423 | 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 | 181 | 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 | 145 | 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 | 19 | 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 | 145 | 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 | 21 | 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 | 19 | 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 | 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 | 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 | 149 | 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 | 18 | 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 | 18 | 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 | 233 | 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. |