335 citations · 1.3k across the 20 of their papers we have counts for
20 papers
The IMACS Cluster Building Survey. I. Description of the Survey and Analysis Methods
Augustus Oemler, Alan Dressler, Michael G. Gladders +8
The IMACS Cluster Building Survey uses the wide field spectroscopic capabilities of the IMACS spectrograph on the 6.5m Baade Telescope to survey the large-scale environment surroun…
The Suppression of Star Formation and the Effect of Galaxy Environment in Low-Redshift Galaxy Groups
Jesper Rasmussen, John S. Mulchaey, Lei Bai +3
Understanding the interaction between galaxies and their surroundings is central to building a coherent picture of galaxy evolution. Here we use GALEX imaging of a statistically re…
The Nature of Star Formation at 24 microns in the Group Environment at 0.3 < z < 0.55
K. Tyler, G. H. Rieke, D. J. Wilman +7
Galaxy star formation rates (SFRs) are sensitive to the local environment; for example, the high-density regions at the cores of dense clusters are known to suppress star formation…
Witnessing the Formation of a Brightest Cluster Galaxy in a Nearby X-ray Cluster
Jesper Rasmussen, John S. Mulchaey, Lei Bai +3
The central dominant galaxies in galaxy clusters constitute the most massive and luminous galaxies in the Universe. Despite this, the formation of these brightest cluster galaxies…
The First Mid-IR View of the Star-forming Properties of Nearby Galaxy Groups
Lei Bai, Jesper Rasmussen, John S. Mulchaey +3
We present the first mid-IR study of galaxy groups in the nearby Universe based on Spitzer MIPS observations of a sample of nine redshift-selected groups from the XMM-IMACS (XI) pr…
A Spectroscopically Confirmed Excess of 24 micron Sources in a Super Galaxy Group at z=0.37: Enhanced Dusty Star Formation Relative to the Cluster and Field Environment
Kim-Vy H. Tran, Amelie Saintonge, John Moustakas +5
To trace how dust-obscured star formation varies with environment, we compare the fraction of 24 micron sources in a super galaxy group to the field and a rich galaxy cluster at z~…