ALMA Lensing Cluster Survey: Physical Characterization of Near-infrared-dark Intrinsically Faint ALMA Sources at z = 2-4
Artikel i vetenskaplig tidskrift, 2025
We present results from Atacama Large Millimeter/submillimeter Array (ALMA) spectral line-scan observations at 3 mm and 2 mm bands of three near-infrared-dark (NIR-dark) galaxies behind two massive lensing clusters MACS J0417.5-1154 and RXC J0032.1+1808. Each of these three sources is a (sub)millimeter faint (delensed S1.2 mm < 1 mJy) triply lensed system originally discovered in the ALMA Lensing Cluster Survey. We have successfully detected CO and [C i] emission lines and confirmed that their spectroscopic redshifts are z = 3.652, 2.391, and 2.985. By utilizing a rich multiwavelength data set, we find that the NIR-dark galaxies are located on the star formation main sequence in the intrinsic stellar mass range of log (M*/M⊙) = 9.8-10.4, which is about 1 order of magnitude lower than that of typical submillimeter galaxies (SMGs). These NIR-dark galaxies show a variety in gas depletion times and spatial extent of dust emission. One of the three is a normal star-forming galaxy with gas depletion time consistent with a scaling relation, and its infrared surface brightness is an order of magnitude smaller than that of typical SMGs. Since this galaxy has an elongated axis ratio of ∼0.17, we argue that normal star-forming galaxies in an edge-on configuration can be heavily dust-obscured. This implies that existing deep WFC3/F160W surveys may miss a fraction of typical star-forming main-sequence galaxies due to their edge-on orientation.
Författare
Akiyoshi Tsujita
University of Tokyo
Kotaro Kohno
Research Center for the Early Universe
University of Tokyo
Shuo Huang
Nagoya University
National Astronomical Observatory of Japan
M. Oguri
Chiba University
Ken Ichi Tadaki
Hokkai Gakuen University
I. Smail
Durham University
H. Umehata
Nagoya University
California Institute of Technology (Caltech)
Zhen Kai Gao
National Central University
Academia Sinica
Wei Hao Wang
Academia Sinica
Fengwu Sun
University of Arizona
Harvard-Smithsonian Center for Astrophysics
S. Fujimoto
Cosmic Dawn Center (DAWN)
University of Texas
Niels Bohr Institute
T. Wang
Nanjing University
Ryosuke Uematsu
Kyoto University
D. Espada
Universidad de Granada
F. Valentino
Cosmic Dawn Center (DAWN)
European Southern Observatory (ESO)
Y. Ao
University of Science and Technology of China
Chinese Academy of Sciences
F. E. Bauer
Pontificia Universidad Catolica de Chile
Instituto Milenio de Astrofísica
B. Hatsukade
National Astronomical Observatory of Japan
University of Tokyo
The Graduate University for Advanced Studies (SOKENDAI)
Fumi Egusa
University of Tokyo
Y. Nishimura
University of Tokyo
Anton M. Koekemoer
Space Telescope Science Institute (STScI)
D. Schaerer
Université de Genève
Institut de Recherche en Astrophysique et Planétologie (IRAP)
C. D. P. Lagos
University of Western Australia
Cosmic Dawn Center (DAWN)
ARC Centre of Excellence for All-sky Astrophysics
M. Dessauges-Zavadsky
Université de Genève
G. Brammer
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
Karina I. Caputi
Rijksuniversiteit Groningen
Cosmic Dawn Center (DAWN)
Eiichi Egami
University of Arizona
J. González-López
Universidad Diego Portales
Las Campanas Observatory
Jean Baptiste Jolly
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Max-Planck-Gesellschaft
Kirsten Knudsen
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
V. Kokorev
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
Rijksuniversiteit Groningen
Georgios E. Magdis
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
Danmarks Tekniske Universitet (DTU)
Masami Ouchi
University of Tokyo
National Astronomical Observatory of Japan
Sune Toft
Cosmic Dawn Center (DAWN)
Niels Bohr Institute
John F. Wu
Space Telescope Science Institute (STScI)
Johns Hopkins University
A. Zitrin
Ben-Gurion University of the Negev
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 989 1 115Ämneskategorier (SSIF 2025)
Atom- och molekylfysik och optik
Annan fysik
Astronomi, astrofysik och kosmologi
DOI
10.3847/1538-4357/adb41d