ISCS J1429.3+3437 , the SIMBAD biblio

ISCS J1429.3+3437 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:52:44


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Title First 3 Authors
2008ApJ...684..905E viz 15       D               1 123 230 Clusters of galaxies in the first half of the universe from the IRAC Shallow Survey. EISENHARDT P.R.M., BRODWIN M., GONZALEZ A.H., et al.
2009AJ....138.1271D 15       D               1 71 55 An intensive Hubble space telescope survey for z>1 type Ia supernovae by targeting galaxy clusters. DAWSON K.S., ALDERING G., AMANULLAH R., et al.
2011ApJ...737...59J 281       D S   X C       6 35 92 Scaling relations and overabundance of massive clusters at z ≳ 1 from weak-lensing studies with the Hubble space telescope. JEE M.J., DAWSON K.S., HOEKSTRA H., et al.
2012ApJ...745...32B 15       D               1 75 42 The Hubble space telescope cluster supernova survey. II. The type Ia supernova rate in high-redshift galaxy clusters. BARBARY K., ALDERING G., AMANULLAH R., et al.
2012ApJ...750....1M 15       D               1 76 36 The Hubble space telescope cluster supernova survey. III. Correlated properties of type Ia supernovae and their hosts at 0.9 < z < 1.46. MEYERS J., ALDERING G., BARBARY K., et al.
2012ApJ...756..114S 93       D       C       12 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.
2012ApJ...761..141M 16       D               1 14 29 The faint end of the cluster-galaxy luminosity function at high redshift. MANCONE C.L., BAKER T., GONZALEZ A.H., et al.
2013ApJ...768....1M 16       D               3 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.
2013MNRAS.434..878S 15       D               2 32 23 The mass-concentration relation in massive galaxy clusters at redshift ∼ 1. SERENO M. and COVONE G.
2013ApJ...779..137Z viz 92       D     X         3 480 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 16       D               1 48 179 The era of star formation in galaxy clusters. BRODWIN M., STANFORD S.A., GONZALEZ A.H., et al.
2015ApJ...800..107W 16       D               1 15 9 Star formation in high-redshift cluster ellipticals. WAGNER C.R., BRODWIN M., SNYDER G.F., et al.
2015MNRAS.449.2024S 16       D               1 106 30 The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects. SERENO M., GIOCOLI C., ETTORI S., et al.
2015MNRAS.450.3665S viz 16       D               1 430 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
2016MNRAS.455..892G viz 16       D               1 353 14 The galaxy cluster concentration-mass scaling relation. GROENER A.M., GOLDBERG D.M. and SERENO M.
2016MNRAS.456.1681M 16       D               1 18 10 The abundance and colours of galaxies in high-redshift clusters in the cold dark matter cosmology. MERSON A.I., BAUGH C.M., GONZALEZ-PEREZ V., 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 95       D     X         3 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.
2021ApJ...911...82C viz 167           X C       3 388 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.
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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