Darren Croton
Affiliations: | Swinburne University of Technology, Hawthorn, Victoria, Australia |
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"Darren Croton"Children
Sign in to add trainee| George Vernardos | grad student | 2015 | Swinburne University of Technology |
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Publications
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| Triani D, Croton D, Sinha M. (2019) Mentari: A pipeline to model the galaxy SED using semi analytic models Arxiv: Astrophysics of Galaxies. 15: 119-123 |
| Liu FS, Jia M, Yesuf HM, et al. (2018) On the Transition of the Galaxy Quenching Mode at 0.5 < z < 1 in CANDELS The Astrophysical Journal. 860: 60 |
| Donley JL, Kartaltepe J, Kocevski D, et al. (2018) Evidence for Merger-driven Growth in Luminous, High-z, Obscured AGNs in the CANDELS/COSMOS Field The Astrophysical Journal. 853: 63 |
| Wojtak R, Old L, Mamon GA, et al. (2018) Galaxy Cluster Mass Reconstruction Project – IV. Understanding the effects of imperfect membership on cluster mass estimation Monthly Notices of the Royal Astronomical Society. 481: 324-340 |
| Old L, Wojtak R, Pearce FR, et al. (2018) Galaxy Cluster Mass Reconstruction Project – III. The impact of dynamical substructure on cluster mass estimates Monthly Notices of the Royal Astronomical Society. 475: 853-866 |
| Behroozi PS, Zhu G, Ferguson HC, et al. (2015) Using galaxy pairs to probe star formation during major halo mergers Monthly Notices of the Royal Astronomical Society. 450: 1546-1564 |
| Old L, Wojtak R, Mamon GA, et al. (2015) Galaxy Cluster Mass Reconstruction Project - II. Quantifying scatter and bias using contrasting mock catalogues Monthly Notices of the Royal Astronomical Society. 449: 1897-1920 |
| Bryant JJ, Owers MS, Robotham ASG, et al. (2015) The SAMI Galaxy Survey: Instrument specification and target selection Monthly Notices of the Royal Astronomical Society. 447: 2857-2879 |
| Kartaltepe JS, Mozena M, Kocevski D, et al. (2015) Candels visual classifications: Scheme, data release, and first results Astrophysical Journal, Supplement Series. 221 |
| Rosario DJ, McIntosh DH, Van Der Wel A, et al. (2015) The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS Astronomy and Astrophysics. 573 |