315 citations · 927 across the 13 of their papers we have counts for
13 papers
The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters
A. Trudeau, Anthony H. Gonzalez, K. Thongkham +8
The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge. Furthermore, stu…
The Massive and Distant Clusters of WISE Survey IX: High Radio Activity in a Merging Cluster
Emily Moravec, Anthony Gonzalez, Simon Dicker +18
We present a multi-wavelength investigation of the radio galaxy population in the galaxy cluster MOO J1506+5137 at =1.090.03, which in previous work we identified as having…
Star-Forming Brightest Cluster Galaxies at 0.25 < z < 1.25: A Transitioning Fuel Supply
M. McDonald, B. Stalder, M. Bayliss +23
We present a multi-wavelength study of 90 brightest cluster galaxies (BCGs) in a sample of galaxy clusters selected via the Sunyaev Zel'dovich effect by the South Pole Telescope, u…
The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years
Stacey Alberts, Alexandra Pope, Mark Brodwin +14
We compare the star formation (SF) activity in cluster galaxies to the field from z=0.3-1.5 using SPIRE 250m imaging. We utilize 274 clusters from the IRAC Shallow Cl…
Optical followup of galaxy clusters detected by the South Pole Telescope
S. Desai, R. Armstrong, M. L. N. Ashby +21
The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's mai…
Low Resolution Spectral Templates for AGNs and Galaxies
R. J. Assef, C. S. Kochanek, The AGES Collaboration
We present a set of low resolution empirical SED templates for AGNs and galaxies in the wavelength range from 0.03 to 30 microns. These templates form a non-negative basis of the c…
Mid-Infrared Variability from the Spitzer Deep, Wide-Field Survey
Szymon Kozlowski, Christopher S. Kochanek, Daniel Stern +30
We use the multi-epoch, mid-infrared Spitzer Deep, Wide-Field Survey to investigate the variability of 474,179 objects in 8.1 deg^2 of the NDWFS Bootes field. We perform a Differen…
The Mid-IR and X-ray Selected QSO Luminosity Function
R. J. Assef, C. S. Kochanek, M. L. N. Ashby +12
We present the J-band luminosity function of 1838 mid-infrared and X-ray selected AGNs in the redshift range 0<z<5.85. These luminosity functions are constructed by combining the d…
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~…
Low Resolution Spectral Templates For AGNs and Galaxies From 0.03 -- 30 microns
R. J. Assef, C. S. Kochanek, M. Brodwin +9
We present a set of low resolution empirical SED templates for AGNs and galaxies in the wavelength range from 0.03 to 30 microns based on the multi-wavelength photometric observati…
Mid-Infrared Galaxy Luminosity Functions from the AGN and Galaxy Evolution Survey
X. Dai, R. J. Assef, C. S. Kochanek +12
We present galaxy luminosity functions at 3.6, 4.5, 5.8, and 8.0 micron measured by combining photometry from the IRAC Shallow Survey with redshifts from the AGN and Galaxy Evoluti…
The Fundamental Manifold of Spheroids
Dennis Zaritsky, Anthony H. Gonzalez, Ann I. Zabludoff
We present a unifying empirical description of the structural and kinematic properties of all spheroids embedded in dark matter halos. We find that the stellar spheroidal component…
The Las Campanas Distant Cluster Survey -- The Correlation Function
Anthony H. Gonzalez, Dennis Zaritsky, Risa H. Wechsler
We present the first non-local (z>0.2) measurement of the cluster-cluster spatial correlation length, using data from the Las Campanas Distant Cluster Survey (LCDCS). We measure th…