Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
- Submitting institution
-
The University of Bath
- Unit of assessment
- 9 - Physics
- Output identifier
- 146441475
- Type
- D - Journal article
- DOI
-
10.1088/0004-637X/788/1/11
- Title of journal
- Astrophysical Journal
- Article number
- 11
- First page
- 1
- 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...11L
- 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
-
22
- Research group(s)
-
A - Astrophysics
- Citation count
- 178
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- As second of 23 authors and direct supervisor of lead author and PhD student Philipp Lang, Stijn Wuyts was the key driver behind this paper. SW conceived the idea of the paper and extended it to the development of the technical tools employed to reconstruct the stellar mass maps from multi-band Hubble Space Telescope imaging and to model the intrinsic stellar mass profiles accounting for finite resolution and neighbouring sources. SW helped with the observational analysis and the comparison to the semi-analytical model. SW wrote about 1/3 of the text and heavily edited the remaining 2/3 of the manuscript.
- Non-English
- No
- English abstract
- -
