Sub-millimetre source identifications and the microjansky source population at 8.4 GHz in the William Herschel Deep Field-Reference-Cited by-同舟云学术

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Sub-millimetre source identifications and the microjansky source population at 8.4 GHz in the William Herschel Deep Field

Published:2012-11-01 Issue:2 Volume:428 Page:935-951
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Heywood I.,Bielby R. M.,Hill M. D.,Metcalfe N.,Rawlings S.,Shanks T.,Smirnov O. M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/428/2/935/3186603/sts046.pdf

Reference65 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. Unified Models for Active Galactic Nuclei and Quasars

3. Can the faint submillimetre galaxies be explained in the Λ cold dark matter model?

4. Correcting direction-dependent gains in the deconvolution of radio interferometric images

5. Submillimetre observations of X-ray active galactic nuclei in the William Herschel Deep Field

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1. The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms;Monthly Notices of the Royal Astronomical Society;2022-01-13

2. The nature of sub-millimetre galaxies I: a comparison of AGN and star-forming galaxy SED fits;Monthly Notices of the Royal Astronomical Society;2021-05-06

3. The MAVERIC Survey: Radio Catalogs and Source Counts from Deep Very Large Array Imaging of 25 Galactic Globular Clusters;The Astrophysical Journal;2020-11-03

4. VLA imaging of the XMM-LSS/VIDEO deep field at 1–2 GHz;Monthly Notices of the Royal Astronomical Society;2020-06-20

5. The ATLAS 9.0 GHz survey of the extended Chandra Deep Field South: the faint 9.0 GHz radio population;Monthly Notices of the Royal Astronomical Society;2019-11-19

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