THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: IMPLICATIONS FOR SPECTRAL LINE INTENSITY MAPPING AT MILLIMETER WAVELENGTHS AND CMB SPECTRAL DISTORTIONS-Reference-Cited by-同舟云学术

THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: IMPLICATIONS FOR SPECTRAL LINE INTENSITY MAPPING AT MILLIMETER WAVELENGTHS AND CMB SPECTRAL DISTORTIONS

Published:2016-12-08 Issue:1 Volume:833 Page:73
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Carilli C. L.^ORCID,Chluba J.,Decarli R.^ORCID,Walter F.^ORCID,Aravena M.^ORCID,Wagg J.,Popping G.,Cortes P.^ORCID,Hodge J.,Weiss A.,Bertoldi F.^ORCID,Riechers D.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/833/i=1/a=73/pdf

Reference57 articles.

1. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND, AND PROPERTIES OF THE FAINTEST DUSTY STAR-FORMING GALAXIES

2. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: SEARCH FOR [${\rm{C}}\,{\rm{II}}$] LINE AND DUST EMISSION IN 6

3. INTENSITY MAPPING OF MOLECULAR GAS DURING COSMIC REIONIZATION

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