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| SpARCS J021943-053129 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST18:27:46 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017MNRAS.470.4168B | 95 | D | F | 6 | 23 | 41 | Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description. | BALOGH M.L., GILBANK D.G., MUZZIN A., 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. | ||
| 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 |
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.506.3364R | 42 | X | 1 | 28 | 15 | The GOGREEN survey: dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching. | REEVES A.M.M., BALOGH M.L., VAN DER BURG R.F.J., 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. | ||
| 2022MNRAS.510..674W | 60 | D | X | 2 | 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. | |
| 2024MNRAS.52710680G | 18 | D | 1 | 18 | ~ | Spitzer-selected z > 1.3 protocluster candidates in the LSST Deep Drilling Fields. | GULLY H., HATCH N., BAHE Y., et al. | ||
| 2025MNRAS.541..409H | 205 | D | X C | 4 | 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. |