ALMA OBSERVATION OF 158 μm [C II] LINE AND DUST CONTINUUM OF AZ= 7 NORMALLY STAR-FORMING GALAXY IN THE EPOCH OF REIONIZATION-Reference-Cited by-同舟云学术

ALMA OBSERVATION OF 158 μm [C II] LINE AND DUST CONTINUUM OF AZ= 7 NORMALLY STAR-FORMING GALAXY IN THE EPOCH OF REIONIZATION

Published:2014-08-12 Issue:1 Volume:792 Page:34
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Ota Kazuaki^ORCID,Walter Fabian,Ohta Kouji,Hatsukade Bunyo,Carilli Chris L.,da Cunha Elisabete,González-López Jorge,Decarli Roberto,Hodge Jacqueline A.,Nagai Hiroshi,Egami Eiichi,Jiang Linhua^ORCID,Iye Masanori,Kashikawa Nobunari,Riechers Dominik A.,Bertoldi Frank,Cox Pierre,Neri Roberto,Weiss Axel

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/792/i=1/a=34/pdf

Reference97 articles.

1. 350 μm Dust Emission from High‐Redshift Quasars

2. Millimeter observations of HCM 6A, a gravitationally lensed Lyα emitting galaxy at z = 6.56

3. [CII] at 158μm as a star formation tracer in late-type galaxies

4. LOWER-LUMINOSITY GALAXIES COULD REIONIZE THE UNIVERSE: VERY STEEP FAINT-END SLOPES TO THE UV LUMINOSITY FUNCTIONS AT z ⩾ 5-8 FROM THE HUDF09 WFC3/IR OBSERVATIONS

5. A NEW POPULATION OF HIGH-z, DUSTY Lyα EMITTERS AND BLOBS DISCOVERED BYWISE: FEEDBACK CAUGHT IN THE ACT?

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