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The H star formation main sequence in cluster and field galaxies at
Julie Nantais, Gillian Wilson, Adam Muzzin +16
We calculate H-based star formation rates and determine the star formation rate-stellar mass relation for members of three SpARCS clusters at and serendipitously id…
Carnegie Supernova Project II: The slowest rising Type Ia supernova LSQ14fmg and clues to the origin of super-Chandrasekhar/03fg-like events
E. Y. Hsiao, P. Hoeflich, C. Ashall +34
The Type Ia supernova (SN Ia) LSQ14fmg exhibits exaggerated properties which may help to reveal the origin of the "super-Chandrasekhar" (or 03fg-like) group. The optical spectrum i…
The Morphology-Density relationship in 1<z<2 clusters
Elizaveta Sazonova, Katherine Alatalo, Jennifer Lotz +8
The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which…
Evaluating the Calibration of SN Ia Anchor Datasets with a Bayesian Hierarchical Model
Miles Currie, David Rubin, Greg Aldering +3
Inter-survey calibration remains an important systematic uncertainty in cosmological studies using type Ia supernova (SNe Ia). Ideally, each survey would measure its system through…
The SNEMO and SUGAR Companion Datasets
G. Aldering, P. Antilogus, C. Aragon +41
The Nearby Supernova Factory has made spectrophotometric observations of Type Ia supernovae since . This work presents an interim version of the data produced, including $210…
Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
Kyle Finner, M. James Jee, Tracy Webb +4
In the hierarchical structure formation model of the universe, galaxy clusters are assembled through a series of mergers. Accordingly, it is expected that galaxy clusters in the ea…