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Can Minor Merging Account for the Size Growth of Quiescent Galaxies? New Results from the CANDELS Survey
Andrew B. Newman, Richard S. Ellis, Kevin Bundy +1
The presence of extremely compact galaxies at z~2 and their subsequent growth in physical size has been the cause of much puzzlement. We revisit the question using deep infrared Wi…
Galaxies in X-ray Groups I: Robust Membership Assignment and the Impact of Group Environments on Quenching
Matthew R. George, Alexie Leauthaud, Kevin Bundy +19
Understanding the mechanisms that lead dense environments to host galaxies with redder colors, more spheroidal morphologies, and lower star formation rates than field populations r…
The integrated stellar content of dark matter halos
Alexie Leauthaud, Matthew R. George, Peter S. Behroozi +6
Measurements of the total amount of stars locked up in galaxies as a function of host halo mass contain key clues about the efficiency of processes that regulate star formation. We…
Evolution of the Most Massive Galaxies to z=0.6: I. A New Method for Physical Parameter Estimation
Yan-Mei Chen, Guinevere Kauffmann, Christy A. Tremonti +10
We use principal component analysis (PCA) to estimate stellar masses, mean stellar ages, star formation histories (SFHs), dust extinctions and stellar velocity dispersions for ~290…
Oxford SWIFT IFS and multi-wavelength observations of the Eagle galaxy at z=0.77
Susan A. Kassin, L. Fogarty, T. Goodsall +17
The `Eagle' galaxy at a redshift of 0.77 is studied with the Oxford Short Wavelength Integral Field Spectrograph (SWIFT) and multi-wavelength data from the All-wavelength Extended…
The Morphology of Galaxies in the Baryon Oscillation Spectroscopic Survey
Karen L. Masters, Claudia Maraston, Robert C. Nichol +17
We study the morphology of luminous and massive galaxies at 0.3<z<0.7 targeted in the Baryon Oscillation Spectroscopic Survey (BOSS) using publicly available Hubble Space Telescope…