Measurements of the Dust Properties in z ≃ 1–3 Submillimeter Galaxies with ALMA-Reference-Cited by-同舟云学术

Measurements of the Dust Properties in z ≃ 1–3 Submillimeter Galaxies with ALMA

Published:2021-09-01 Issue:1 Volume:919 Page:30
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

da Cunha E.^ORCID,Hodge J. A.^ORCID,Casey C. M.^ORCID,Algera H. S. B.^ORCID,Kaasinen M.^ORCID,Smail I.^ORCID,Walter F.^ORCID,Brandt W. N.^ORCID,Dannerbauer H.^ORCID,Decarli R.^ORCID,Groves B. A.^ORCID,Knudsen K. K.^ORCID,Swinbank A. M.^ORCID,Weiss A.,van der Werf P.,Zavala J. A.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac0ae0/pdf

Reference110 articles.

1. Laboratory Results on Millimeter-Wave Absorption in Silicate Grain Materials at Cryogenic Temperatures

2. 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

3. AzTEC millimetre survey of the COSMOS field - III. Source catalogue over 0.72 deg2 and plausible boosting by large-scale structure

4. Dust formation history of galaxies: A critical role of metallicity dust mass growth by accreting materials in the interstellar medium

5. Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift

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