(untitled)
Adam C. Carnall(Royal Observatory), Charlie Conroy(Center for Astrophysics Harvard & Smithsonian), Benjamin D. Johnson(Center for Astrophysics Harvard & Smithsonian), J. S. Dunlop(Royal Observatory), Joel Leja(Yale University), R. J. McLure(University of Edinburgh)
Edinburgh Research Explorer (University of Edinburgh)
January 1, 2000
Cited by 211
Related Papers
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
|The Astrophysical Journal|2016|2.8k
THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM<i>z</i>= 0-8
|The Astrophysical Journal|2013|2.1k
THE PROPAGATION OF UNCERTAINTIES IN STELLAR POPULATION SYNTHESIS MODELING. I. THE RELEVANCE OF UNCERTAIN ASPECTS OF STELLAR EVOLUTION AND THE INITIAL MASS FUNCTION TO THE DERIVED PHYSICAL PROPERTIES OF GALAXIES
|The Astrophysical Journal|2009|1.9k
CALIFA, the Calar Alto Legacy Integral Field Area survey
|Astronomy and Astrophysics|2011|1.3k
UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
|Monthly Notices of the Royal Astronomical Society|2019|1.2k