The SLUGGS survey: a comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to ∼4 effective radii

Author:

Bellstedt Sabine12ORCID,Forbes Duncan A1,Romanowsky Aaron J34,Remus Rhea-Silvia56,Stevens Adam R H7,Brodie Jean P3,Poci Adriano8ORCID,McDermid Richard28,Alabi Adebusola13,Chevalier Leonie1,Adams Caitlin1,Ferré-Mateu Anna1,Wasserman Asher3,Pandya Viraj3ORCID

Affiliation:

1. Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia

2. Australian Astronomical Observatory, PO Box 915, Sydney, NSW 1670, Australia

3. University of California Observatories, 1156 High Street, Santa Cruz, CA 95064, USA

4. Department of Physics and Astronomy, San José State University, One Washington Square, San Jose, CA 95192, USA

5. Universitäts-Sternwarte München, Fakultät für Physik, LMU Munich, Scheinerstr. 1, D-81679 München, Germany

6. Canadian Institute for Theoretical Astrophysics, 60 St. George Street, University of Toronto, Toronto, ON M5S 3H8, Canada

7. International Centre for Radio Astronomy Research, University of Western Australia, Crawley, WA 6009, Australia

8. Department of Physics and Astronomy, Macquarie University, North Ryde, NSW 2109, Australia

Funder

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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