ISCS J1432.3+3253 , the SIMBAD biblio

ISCS J1432.3+3253 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:06:05


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Title First 3 Authors
2013ApJ...768....1M 16       D               6 52 126 The cluster and field galaxy active galactic nucleus fraction at z = 1-1.5: evidence for a reversal of the local anticorrelation between environment and AGN fraction. MARTINI P., MILLER E.D., BRODWIN M., et al.
2013ApJ...779..137Z viz 15       D               2 480 30 Hα star formation rates of z > 1 galaxy clusters in the IRAC Shallow Cluster Survey. ZEIMANN G.R., STANFORD S.A., BRODWIN M., et al.
2013ApJ...779..138B 93       D       C       2 48 179 The era of star formation in galaxy clusters. BRODWIN M., STANFORD S.A., GONZALEZ A.H., et al.
2016ApJ...825...72A viz 94       D       C       2 142 72 Star formation and AGN activity in galaxy clusters from z=1-2: a multi-wavelength analysis featuring Herschel/PACS. ALBERTS S., POPE A., BRODWIN M., et al.
2016A&A...593A...2A viz 157           X C       3 174 14 Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr. ANDREON S., DONG H. and RAICHOOR A.
2018MNRAS.479.3563F viz 177       D       C F     6 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.
2020ApJ...899...85S 308       D S   X         7 5 16 The morphology-density relationship in 1 < z < 2 clusters. SAZONOVA E., ALATALO K., LOTZ J., 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               7 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.
2025A&A...697A.150S 19       D               1 37 ~ Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon. SAMANSO N., NANTAIS J.B., ALBERTS S., et al.

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