ISCS J1432.4+3250 , the SIMBAD biblio

ISCS J1432.4+3250 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST05:46:09


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Title First 3 Authors
2011ApJ...732...33B 985   K A D S   X C       25 31 55 X-ray emission from two infrared-selected galaxy clusters at z > 1.4 in the IRAC shallow cluster survey. BRODWIN M., STERN D., VIKHLININ A., et al.
2012ApJ...756..114S 588       D     X C       15 17 46 Assembly of the red sequence in infrared-selected galaxy clusters from the IRAC shallow cluster survey. SNYDER G.F., BRODWIN M., MANCONE C.M., et al.
2013ApJ...768....1M 208       D     X         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.
2013A&A...554A..79A 384     A D S   X C       9 8 15 Observational evidence that massive cluster galaxies were forming stars at z ∼ 2.5 and did not grow in mass at later times. ANDREON S.
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 55       D     X         2 48 179 The era of star formation in galaxy clusters. BRODWIN M., STANFORD S.A., GONZALEZ A.H., et al.
2014A&A...564A..17N 15       D               1 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.
2014ApJ...797..109R 118           X C       2 4 22 Candidate clusters of galaxies at z > 1.3 identified in the Spitzer South Pole telescope deep field survey. RETTURA A., MARTINEZ-MANSO J., STERN D., et al.
2015ApJ...800..107W 55       D     X         2 15 9 Star formation in high-redshift cluster ellipticals. WAGNER C.R., BRODWIN M., SNYDER G.F., 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.
2017ApJ...834...53W 135       D     X         4 36 13 The evolution of star formation activity in cluster galaxies over 0.15 < z < 1.5. WAGNER C.R., COURTEAU S., BRODWIN M., et al.
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.
2021A&A...649A..42C viz 17       D               2 141 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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