Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
Artikel i vetenskaplig tidskrift, 2022
The 2 mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high-redshift (z greater than or similar to 4), massive, dusty star-forming galaxies (DSFGs). Here we present two likely high-redshift sources, identified in the survey, whose physical characteristics are consistent with a class of optical/near-infrared (OIR)-invisible DSFGs found elsewhere in the literature. We first perform a rigorous analysis of all available photometric data to fit spectral energy distributions and estimate redshifts before deriving physical properties based on our findings. Our results suggest the two galaxies, called MORA-5 and MORA-9, represent two extremes of the "OIR-dark" class of DSFGs. MORA-5 (z(phot) = 4.3(-1.3)(+1.5)) is a significantly more active starburst with a star formation rate (SFR) of 830(-190)(+340) M-circle dot yr(-1) compared to MORA-9 (z(phot) = 4.3(-1.0)(+1.3)), whose SFR is a modest 200(-60)(+250) M-circle dot yr(-1). Based on the stellar masses (M-star approximate to 10(10-11) M-circle dot), space density (n similar to (5 +/- 2) x 10(-6) Mpc(-3), which incorporates two other spectroscopically confirmed OIR-dark DSFGs in the MORA sample at z = 4.6 and z = 5.9), and gas depletion timescales (<1 Gyr) of these sources, we find evidence supporting the theory that OIR-dark DSFGs are the progenitors of recently discovered 3 < z < 4 massive quiescent galaxies.
Författare
Sinclaire M. Manning
University of Massachusetts
The University of Texas at Austin
Caitlin M. Casey
The University of Texas at Austin
Jorge A. Zavala
National Astronomical Observatory of Japan
The University of Texas at Austin
Georgios E. Magdis
Köpenhamns universitet
Danmarks Tekniske Universitet (DTU)
Patrick M. Drew
The University of Texas at Austin
Jaclyn B. Champagne
The University of Texas at Austin
Manuel Aravena
Universidad Diego Portales
Matthieu Bethermin
Aix-Marseille Université
David L. Clements
Imperial College London
Steven L. Finkelstein
The University of Texas at Austin
Seiji Fujimoto
Köpenhamns universitet
Christopher C. Hayward
Flatiron Institute
Jacqueline A. Hodge
Universiteit Leiden
Olivier Ilbert
Aix-Marseille Université
Jeyhan S. Kartaltepe
Rochester Institute of Technology
Kirsten Kraiberg Knudsen
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Anton M. Koekemoer
Space Telescope Science Institute (STScI)
Allison W. S. Man
University of British Columbia (UBC)
Dunlap Institute for Astronomy and Astrophysics
David B. Sanders
University of Hawaii
Kartik Sheth
National Aeronautics and Space Administration (NASA)
Justin S. Spilker
The University of Texas at Austin
Johannes Staguhn
Johns Hopkins University
NASA Goddard Space Flight Center
Margherita Talia
Universita di Bologna
Istituto nazionale di astrofisica (INAF)
Ezequiel Treister
Pontificia Universidad Catolica de Chile
Min S. Yun
University of Massachusetts
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 925 1 23Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
Sannolikhetsteori och statistik
DOI
10.3847/1538-4357/ac366a