Darren Croton

Affiliations: 
Swinburne University of Technology, Hawthorn, Victoria, Australia 
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"Darren Croton"
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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
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