An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling.
- Submitting institution
-
University of Durham
- Unit of assessment
- 9 - Physics
- Output identifier
- 101269
- Type
- D - Journal article
- DOI
-
10.1088/0004-637X/806/1/110
- Title of journal
- The Astrophysical Journal
- Article number
- -
- First page
- 110
- Volume
- 806
- Issue
- 1
- ISSN
- 0004637X
- Open access status
- Out of scope for open access requirements
- Month of publication
- -
- Year of publication
- 2015
- URL
-
https://doi.org/10.1088/0004-637X/806/1/110
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
17
- Research group(s)
-
D - Centre for Extragalactic Astronomy
- Citation count
- 205
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- I instigated and was the PI of the Cycle 0 ALMA survey which discovered the sources used in this publication. I worked closely with the lead author on the analysis and writing of this novel paper, through several iterations, most notably contributing to the interpretation of the physical properties of the population in Section 5.
- Non-English
- No
- English abstract
- -
