SpARCS J033056-284300 , the SIMBAD biblio

SpARCS J033056-284300 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:19:37


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Title First 3 Authors
2012MNRAS.427..550L 282       D     X   F     7 150 160 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.
2016A&A...592A.161N 376       D     X C       9 5 69 Stellar mass function of cluster galaxies at z ∼ 1.5: evidence for reduced quenching efficiency at high redshift. NANTAIS J.B., VAN DER BURG R.F.J., LIDMAN C., et al.
2017ApJ...842L..21N 129           X         3 3 60 ALMA observations of gas-rich galaxies in z ∼ 1.6 galaxy clusters: evidence for higher gas fractions in high-density environments. NOBLE A.G., McDONALD M., MUZZIN A., et al.
2017ApJ...843..126D 334       D     X C       8 6 7 Galaxy merger candidates in high-redshift cluster environments. DELAHAYE A.G., WEBB T.M.A., NANTAIS J., 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.
2018ApJ...866..136F 107       D     X         3 5 57 The evolution of environmental quenching timescales to z ∼ 1.6: evidence for dynamically driven quenching of the cluster galaxy population. FOLTZ R., WILSON G., MUZZIN A., et al.
2020MNRAS.491.3751D 99       D     X         3 42 38 The growth of brightest cluster galaxies and intracluster light over the past 10 billion years. DEMAIO T., GONZALEZ A.H., ZABLUDOFF A., et al.
2020A&A...635A..32C 16       D               1 127 ~ Molecular gas in distant brightest cluster galaxies. CASTIGNANI G., COMBES F., SALOME P., 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.
2020MNRAS.499.3061N 881       D     X C F     20 5 ~ The H α star formation main sequence in cluster and field galaxies at z ∼ 1.6. NANTAIS J., WILSON G., 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               1 141 14 Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data. CHU A., DURRET F. and MARQUEZ I.
2023ApJ...944..213C 367       D     X         9 4 4 A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry. CRAMER W.J., NOBLE A.G., MASSINGILL K., 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.
2024ApJ...975..144C 269           X         6 4 ~ Resolved UV and Optical Color Gradients Reveal Environmental Influence on Galaxy Evolution at Redshift z ∼ 1.6. CRAMER W.J., NOBLE A.G., RUDNICK G., et al.
2025ApJ...985..194P 373           X         8 6 ~ Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies. PIGARELLI A., NOBLE A., RUDNICK G., et al.
2025A&A...698A.204H 93             C       1 21 ~ An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters. HILL R., DEL CARMEN POLLETTA M., BETHERMIN M., et al.

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