3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since z = 3
- Submitting institution
-
The University of Bath
- Unit of assessment
- 9 - Physics
- Output identifier
- 200624627
- Type
- D - Journal article
- DOI
-
10.1088/0004-637X/788/1/28
- Title of journal
- Astrophysical Journal
- Article number
- -
- First page
- 28
- Volume
- 788
- Issue
- 1
- ISSN
- 0004-637X
- Open access status
- Out of scope for open access requirements
- Month of publication
- May
- Year of publication
- 2014
- URL
-
-
- Supplementary information
-
http://adsabs.harvard.edu/abs/2014ApJ...788...28V
- 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
-
29
- Research group(s)
-
A - Astrophysics
- Citation count
- 577
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- The lead author and Stijn Wuyts are the only members of the author list that were actively engaged in both the CANDELS and 3D-HST teams. It is the synergy between the two surveys that enabled this work. SW’s contributions to CANDELS date back to the early proposal writing phases. In this paper specifically, they concentrate on the rest-frame photometry used to separate star-forming and quiescent galaxies, on accounting for colour gradients within galaxies (a necessity demonstrated by Wuyts et al. 2012), and on the interpretation and discussion of results on the size growth of quiescent galaxies (Section 5.2).
- Non-English
- No
- English abstract
- -
