The Astrophysical Journal (Jan 2025)

ALMA Lensing Cluster Survey: Physical Characterization of Near-infrared-dark Intrinsically Faint ALMA Sources at z = 2–4

  • Akiyoshi Tsujita,
  • Kotaro Kohno,
  • Shuo Huang,
  • Masamune Oguri,
  • Ken-ichi Tadaki,
  • Ian Smail,
  • Hideki Umehata,
  • Zhen-Kai Gao,
  • Wei-Hao Wang,
  • Fengwu Sun,
  • Seiji Fujimoto,
  • Tao Wang,
  • Ryosuke Uematsu,
  • Daniel Espada,
  • Francesco Valentino,
  • Yiping Ao,
  • Franz E. Bauer,
  • Bunyo Hatsukade,
  • Fumi Egusa,
  • Yuri Nishimura,
  • Anton M. Koekemoer,
  • Daniel Schaerer,
  • Claudia Lagos,
  • Miroslava Dessauges-Zavadsky,
  • Gabriel Brammer,
  • Karina Caputi,
  • Eiichi Egami,
  • Jorge González-López,
  • Jean-Baptiste Jolly,
  • Kirsten K. Knudsen,
  • Vasily Kokorev,
  • Georgios E. Magdis,
  • Masami Ouchi,
  • Sune Toft,
  • John F. Wu,
  • Adi Zitrin

DOI
https://doi.org/10.3847/1538-4357/adb41d
Journal volume & issue
Vol. 989, no. 1
p. 115

Abstract

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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 S _1.2 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.

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