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Submillimeter Galaxies

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arxiv astro-ph/0202228 v2 pith:5AI6YF4K submitted 2002-02-12 astro-ph

Andrew W. Blain (Caltech) , Ian Smail (Durham) , R.J. Ivison (Edinburgh) , J.-P. Kneib (Toulouse) , David T. Frayer (SIRTF Science Center) This is my paper · ORCID
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keywords galaxiessubmmverydiscusshigh-redshiftsignificantsurveysuniverse
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A cosmologically significant population of very luminous high-redshift galaxies has recently been discovered at submm wavelengths. Advances in submm detector technologies have opened this new window on the distant Universe. Here we discuss the properties of the high-redshift submm galaxies, their significance for our understanding of the process of galaxy formation, and the selection effects that apply to deep submm surveys. The submm galaxies generate a significant fraction of the energy output of all galaxies in the early Universe. We emphasize the importance of studying a complete sample of submm galaxies, and stress that because they are typically very faint in other wavebands, these follow-up observations are very challenging. Finally, we discuss the surveys that will be made using the next generation of submm-wave instruments under development.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    The Big Three Dragons galaxy pair at z=7.15 has hot dust (T_d ≈ 78 K) and is almost fully obscured (f_obs ≈ 0.94), implying that UV-bright galaxies can host major hidden starbursts in the early universe.

  2. Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    The CO-to-H2 conversion factor in high-z dusty star-forming galaxies is not required to be 0.8; intermediate to near-Galactic values (median ~4-5) remain dynamically viable.

  3. Tracing luminous infrared galaxy populations through cluster evolution in a cosmological mock redshift survey

    astro-ph.GA 2026-08 conditional novelty 5.0 of 10

    GARDENS-Wide, a 100 square degree mock redshift survey of dusty star-forming galaxies, predicts proto-cluster contraction, a z about 2 peak in star-forming fraction, and TolTEC LSS detection yields.

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