2026ApJ...997..103H


Query : 2026ApJ...997..103H

2026ApJ...997..103H - Astrophys. J., 997, 103 (2026/January-3)

The Distribution of Quenched Galaxies in the Massive z = 0.87 Galaxy Cluster El Gordo.

HONOR R., COHEN S.H., CARLETON T., WILLNER S.P., POLLETTA M.D.C., WINDHORST R.A., COE D., CONSELICE C.J., DIEGO J.M., DRIVER S.P., D'SILVA J.C.J., FOO N., FRYE B.L., GROGIN N.A., HATHI N.P., JANSEN R.A., KAMIENESKI P.S., KOEKEMOER A.M., LEIMBACH R., MARSHALL M.A., ORTIZ III R., PIRZKAL N., RICOTTI M., ROBOTHAM A.S.G., RUTKOWSKI M.J., RYAN R.E.Jr, SAIKIA P., SUMMERS J., WILLMER C.N.A. and YAN H.

Abstract (from CDS):

El Gordo (ACT-CL J0102-4915) is a massive galaxy cluster with two major mass components at redshift z = 0.87. Using spectral energy distribution fitting results from JWST/NIRCam photometry, the fraction of quenched galaxies in this cluster was measured in two bins of stellar mass: $9\lt {\mathrm{log}}({M}_{* }/{M}_{\odot })\lt 10$ and $10\leqslant \,{\mathrm{log}}({M}_{* }/{M}_{\odot })\lt 12$. While there is no correlation between the quenched fraction and angular separation from the cluster's overall center of mass, there is a correlation between the quenched fraction and angular separation from the center of the nearest of the two mass components for the less-massive galaxies. This suggests that environmental quenching processes are in place at z ∼ 1, and that dwarf galaxies are more affected by those processes than massive galaxies.

Abstract Copyright: © 2026. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxy quenching - Galaxy clusters - Galaxy evolution - Star formation - Galaxies

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ACT-CL J0102-4915 ClG 01 02 52.50 -49 14 58.0           ~ 296 0

Query : 2026ApJ...997..103H

Basic data :
ACT-CL J0102-4915 -- Cluster of Galaxies
Other object types:
otypes_help
ClG (2014ApJ,ACT,...), gLe (2013ApJ), C?G (2014A&A), X (2019MNRAS,2RXS)
ICRS coord. (ep=J2000) :
01 02 52.50 -49 14 58.0 (Optical) [ ] E 2010ApJ...723.1523M
FK4 coord. (ep=B1950 eq=1950) :
01 00 39.49 -49 31 04.4 [ ]
Gal coord. (ep=J2000) :
297.99465 -67.76902 [ ]
Radial velocity / Redshift / cz :
V(km/s) 166460 [~] / z(spectroscopic) 0.870 [~] / cz 260819 [~]
   (Opt) D 2013ApJ...772...25S
Angular size (arcmin):
1.0 1.0 ~ (Rad) D 2015ApJ...813...77Y
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 133
: 28 Display criteria :

Identifiers (10) :
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ACT-CL J0102.9-4916 NAME El Gordo PSZRX G298.02-67.76 SPT-CL J0102-4915
ACT-CL J0102-4915 PSZ1 G297.94-67.76 PSZSPT J0102-4915
MARD J010256.2-491616 PSZ2 G297.97-67.74 2RXS J010256.2-491616

References (296 between 1850 and 2026) (Total 296)
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