TY - JOUR
T1 - Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST
AU - Akins, Hollis B.
AU - Casey, Caitlin M.
AU - Allen, Natalie
AU - Bagley, Micaela B.
AU - Dickinson, Mark
AU - Finkelstein, Steven L.
AU - Franco, Maximilien
AU - Harish, Santosh
AU - Haro, Pablo Arrabal
AU - Ilbert, Olivier
AU - Kartaltepe, Jeyhan S.
AU - Koekemoer, Anton M.
AU - Liu, Daizhong
AU - Long, Arianna S.
AU - McCracken, Henry Joy
AU - Paquereau, Louise
AU - Papovich, Casey
AU - Pirzkal, Nor
AU - Rhodes, Jason
AU - Robertson, Brant E.
AU - Shuntov, Marko
AU - Toft, Sune
AU - Yang, Guang
AU - Barro, Guillermo
AU - Bisigello, Laura
AU - Buat, Véronique
AU - Champagne, Jaclyn B.
AU - Cooper, Olivia
AU - Costantin, Luca
AU - Vega, Alexander de la
AU - Drakos, Nicole E.
AU - Faisst, Andreas
AU - Fontana, Adriano
AU - Fujimoto, Seiji
AU - Gillman, Steven
AU - Gómez-Guijarro, Carlos
AU - Gozaliasl, Ghassem
AU - Hathi, Nimish P.
AU - Hayward, Christopher C.
AU - Hirschmann, Michaela
AU - Holwerda, Benne W.
AU - Jin, Shuowen
AU - Kocevski, Dale D.
AU - Kokorev, Vasily
AU - Lambrides, Erini
AU - Lucas, Ray A.
AU - Magdis, Georgios E.
AU - Magnelli, Benjamin
AU - McKinney, Jed
AU - Mobasher, Bahram
PY - 2023
Y1 - 2023
N2 - We present a search for extremely red, dust-obscured, z > 7 galaxies with JWST/NIRCam+MIRI imaging over the first 20 arcmin2
of publicly available Cycle 1 data from the COSMOS-Web, CEERS, and
PRIMER surveys. Based on their red color in F277W−F444W (∼2.5 mag) and
detection in MIRI/F770W (∼25 mag), we identify two galaxies, COS-z8M1
and CEERS-z7M1, that have best-fit photometric redshifts of Z= 8.4 +03 -04 and 7.6 +01 -0.1 respectively. We perform spectral energy distribution fitting with a variety of codes (including bagpipes, prospector, beagle, and cigale) and find a >95% probability that these indeed lie at z > 7. Both sources are compact (Reff ≲ 200 pc) and highly obscured (AV ∼ 1.5–2.5) and, at our best-fit redshift estimates, likely have strong [O iii]+Hβ emission contributing to their 4.4 μm photometry. We estimate stellar masses of ∼1010M⊙ for both sources; by virtue of detection in MIRI at 7.7 μm,
these measurements are robust to the inclusion of bright emission
lines, for example, from an active galactic nucleus. We identify a
marginal (2.9σ) Atacama Large Millimeter/submillimeter Array detection at 2 mm within 05 of COS-z8M1, which, if real, would suggest a remarkably high IR luminosity of ∼1012L⊙. These two galaxies, if confirmed at z
∼ 8, would be extreme in their stellar and dust masses and may be
representative of a substantial population of highly dust-obscured
galaxies at cosmic dawn.
AB - We present a search for extremely red, dust-obscured, z > 7 galaxies with JWST/NIRCam+MIRI imaging over the first 20 arcmin2
of publicly available Cycle 1 data from the COSMOS-Web, CEERS, and
PRIMER surveys. Based on their red color in F277W−F444W (∼2.5 mag) and
detection in MIRI/F770W (∼25 mag), we identify two galaxies, COS-z8M1
and CEERS-z7M1, that have best-fit photometric redshifts of Z= 8.4 +03 -04 and 7.6 +01 -0.1 respectively. We perform spectral energy distribution fitting with a variety of codes (including bagpipes, prospector, beagle, and cigale) and find a >95% probability that these indeed lie at z > 7. Both sources are compact (Reff ≲ 200 pc) and highly obscured (AV ∼ 1.5–2.5) and, at our best-fit redshift estimates, likely have strong [O iii]+Hβ emission contributing to their 4.4 μm photometry. We estimate stellar masses of ∼1010M⊙ for both sources; by virtue of detection in MIRI at 7.7 μm,
these measurements are robust to the inclusion of bright emission
lines, for example, from an active galactic nucleus. We identify a
marginal (2.9σ) Atacama Large Millimeter/submillimeter Array detection at 2 mm within 05 of COS-z8M1, which, if real, would suggest a remarkably high IR luminosity of ∼1012L⊙. These two galaxies, if confirmed at z
∼ 8, would be extreme in their stellar and dust masses and may be
representative of a substantial population of highly dust-obscured
galaxies at cosmic dawn.
U2 - 10.3847/1538-4357/acef21
DO - 10.3847/1538-4357/acef21
M3 - Journal article
VL - 956
JO - The Astrophysical Journal
JF - The Astrophysical Journal
IS - 1
M1 - 61
ER -