ACT-CL J1142.7+1527 , the SIMBAD biblio

ACT-CL J1142.7+1527 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST09:46:38

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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
2015ApJ...812L..40G 898 T K A S   X C       20 21 15 The massive and distant clusters of WISE survey:
MOO
J1142+1527, a 1015 M☉ galaxy cluster at z = 1.19. 		GONZALEZ A.H., DECKER B., BRODWIN M., et al.
2016ATel.9125....1B 120 T         X         2 2 1 SCP16L01: discovery of an unusual transient in MOO-
J1142. 		BOONE K., ALDERING G., AMANULLAH R., et al.
2018MNRAS.479.3563F viz 181       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.
2019ApJS..240...33G viz 268       D     X C       6 2855 54 The Massive and Distant Clusters of WISE Survey. I. Survey overview and a catalog of >2000 galaxy clusters at z ≃ 1. GONZALEZ A.H., GETTINGS D.P., BRODWIN M., et al.
2019ApJ...878...72D 142       D     X         4 16 ~ The Massive and Distant Clusters of WISE Survey. VI. Stellar mass fractions of a sample of high-redshift infrared-selected clusters. DECKER B., BRODWIN M., ABDULLA Z., et al.
2020ApJ...893...74R 2367     A S   X C       54 1 ~ Unveiling the merger dynamics of the most Massive MaDCoWS cluster at z = 1.2 from a multiwavelength mapping of its Intracluster Medium properties. RUPPIN F., McDONALD M., BRODWIN M., et al.
2020ApJ...899...85S 1808       D S   X         42 5 16 The morphology-density relationship in 1 < z < 2 clusters. SAZONOVA E., ALATALO K., LOTZ J., et al.
2020ApJ...902..144D 485       D     X C       11 16 13 The Massive and Distant Clusters of WISE Survey. X. Initial results from a Sunyaev-Zeldovich effect study of Massive galaxy clusters at z > 1 using MUSTANG2 on the GBT. DICKER S.R., ROMERO C.E., DI MASCOLO L., 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.
2021ApJS..253....3H viz 17       D               1 4198 128 The Atacama Cosmology Telescope: a catalog of >4000 Sunyaev-Zel'dovich galaxy clusters. HILTON M., SIFON C., NAESS S., et al.
2021ApJ...912...87H 17       D               2 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.
2021A&A...650A.153D 131           X C       2 14 5 Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z ≃ 1.13. DI MASCOLO L., MROCZKOWSKI T., PERROTT Y., et al.
2021A&A...653A.135O viz 148       D     X         4 94 8 Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey. Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT. ORLOWSKI-SCHERER J., DI MASCOLO L., BHANDARKAR T., et al.
2021MNRAS.508.2600D 104       D       C       3 30 3 Observations of compact sources in galaxy clusters using MUSTANG2. DICKER S.R., BATTISTELLI E.S., BHANDARKAR T., et al.
2022ApJ...936...71D 242       D     X C       5 13 1 The Massive and Distant Clusters of WISE Survey. XI. Stellar Mass Fractions and Luminosity Functions of MaDCoWS Clusters at z ∼ 1. DECKER B., BRODWIN M., SAHA R., et al.
2023Natur.613...37J 19       D               1 10 3 Intracluster light is already abundant at redshift beyond unity. JOO H. and JEE M.J.
2023MNRAS.523.1228L 140           X         3 3 ~ THE THREE HUNDRED Project: the evolution of physical baryon profiles. LI Q., CUI W., YANG X., et al.
2023A&A...678A.197M 47           X         1 7 ~ Joint measurement of the galaxy cluster pressure profile with Planck and SPT-SZ. MELIN J.-B. and PRATT G.W.

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