Molecular gas and dust in the highly magnifiedz ~ 2.8 galaxy behind the Bullet Cluster-Reference-Cited by-同舟云学术

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Molecular gas and dust in the highly magnifiedz ~ 2.8 galaxy behind the Bullet Cluster

Published:2012-06-27 Issue: Volume:543 Page:A62
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Johansson D.,Horellou C.,Lopez-Cruz O.,Muller S.,Birkinshaw M.,Black J. H.,Bremer M. N.,Wall W. F.,Bertoldi F.,Castillo E.,Ibarra-Medel H. J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201117918/pdf

Reference65 articles.

1. Dust and molecular content of the lensed quasar, MG0751+2716, atz = 3.2

2. Submillimeter galaxies

3. Strong and Weak Lensing United. III. Measuring the Mass Distribution of the Merging Galaxy Cluster 1ES 0657−558

4. CO emission at Z = 2.2867 in the galaxy IRAS F10214 + 4724

5. The Nature of the Bright Submillimeter Galaxy Population: A Radio-preselected Sample with [ITAL]I[/ITAL] ] ∼25

Cited by 10 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. First Constraints on the Interstellar Medium Conditions of a Low-mass, Highly Obscured z = 4.27 Main-sequence Galaxy;The Astrophysical Journal;2024-07-01

2. The “Cosmic Seagull”: A Highly Magnified Disk-like Galaxy at z ≃ 2.8 behind the Bullet Cluster;The Astrophysical Journal;2018-08-14

3. An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution;Astronomy & Astrophysics;2017-11-29

4. Molecular gas properties of a lensed star-forming galaxy at z ~ 3.6: a case study;Astronomy & Astrophysics;2017-09

5. 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;The Astrophysical Journal;2016-12-08

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