To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3 < z < 6 in the Ultra-deep JADES MIRI F770W Parallel
To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3 < z < 6 in the Ultra-deep JADES MIRI F770W Parallel
Oct 25, 2024·,,,,,,,,,,,,,,,,,,,,,,,,,,
Stacey Alberts
Christina C. Williams
Jakob M. Helton
Katherine A. Suess
Zhiyuan Ji
Irene Shivaei
Jianwei Lyu
George Rieke
William M. Baker
Nina Bonaventura
Andrew J. Bunker
Stefano Carniani
Stephane Charlot
Emma Curtis-Lake
Francesco D'Eugenio
Daniel J. Eisenstein
Anna De Graaff
Kevin N. Hainline
Ryan Hausen
Benjamin D. Johnson
Roberto Maiolino
Eleonora Parlanti
Marcia J. Rieke
Brant E. Robertson
Yang Sun
Sandro Tacchella
Christopher N. A. Willmer
Chris J. Willott
Abstract
We present the robust selection of high-redshift quiescent galaxies (QG) and poststarburst (PSB) galaxies using ultra-deep NIRCam and MIRI imaging from the JWST Advanced Deep Extragalactic Survey (JADES). At $3 < z < 6$
, MIRI $7.7\ \mu\mathrm{m}$
imaging provides rest-frame $J$
band, which is commonly used to break the degeneracy between old stellar populations and dust attenuation at lower redshifts. We identify $23$
passively evolving galaxies in UVJ color space in a mass-limited ($\mathrm{log}_{10}(M_{\ast}/M_{\odot}) \geq 8.5$
) sample over $8.8\ \mathrm{arcmin}^{2}$
. An evaluation of the contribution of the $7.7\ \mu\mathrm{m}$
shows that JADES-like NIRCam coverage ($9+$
photometric bands) can compensate for lacking the $J$
band at these redshifts; however, more limited three-band selections perform better with MIRI. Our sample is characterized by rapid quenching timescales ($\sim 100-600\ \mathrm{Myr}$
) with formation redshifts $z_{\mathrm{form}} \leq 9$
and includes a potential record-holding massive QG at and two QGs with evidence for significant residual dust content ($A_{V} \sim 1-2$
). In addition, we present a large sample of $12$
$\mathrm{log}_{10}(M_{\ast}/M_{\odot}) = 8.5-9.5$
PSBs, demonstrating that UVJ selection can be extended to low mass. An analysis of the environment of our sample reveals that the group known as the Cosmic Rose contains a massive QG and a dust-obscured star-forming galaxy (a so-called Jekyll and Hyde pair) plus three additional QGs within $\sim 20\ \mathrm{kpc}$
. Moreover, the Cosmic Rose is part of a larger overdensity at $z \sim 3.7$
, which contains $7/12$
of our low-mass PSBs. Another four low-mass PSBs are members of an overdensity at $z \sim 3.4$
; this result strongly indicates low-mass PSBs are preferentially associated with overdense environments at $z > 3$
.
Type
Publication
The Astrophysical Journal, Volume 975, Issue 1, id.85, 25 pages
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