2.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Center for Astrophysics Harvard & SmithsonianUS71 papers
- Space Telescope Science InstituteUS70 papers
- University of MichiganUS65 papers
- University of California, DavisUS55 papers
- University of ArizonaUS53 papers
- Max Planck Institute for Extraterrestrial PhysicsDE52 papers
- University of FloridaUS51 papers
- California Institute of TechnologyUS49 papers
- Jet Propulsion LaboratoryUS49 papers
- University of ChicagoUS46 papers
- Massachusetts Institute of TechnologyUS44 papers
- University of California, Santa CruzUS42 papers
11 papers · 2 filters
CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies
G. Barro, S. M. Faber, P. G. Perez-Gonzalez +32
We analyze the star-forming and structural properties of 45 massive (log(M/Msun)>10) compact star-forming galaxies (SFGs) at 2<z<3 to explore whether they are progenitors of compac…
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…
H Star Formation Rates of > 1 Galaxy Clusters in the IRAC Shallow Cluster Survey
Gregory Zeimann, S. A. Stanford, Mark Brodwin +7
We present Hubble Space Telescope near-IR spectroscopy for 18 galaxy clusters at 1.0 < < 1.5 in the IRAC Shallow Cluster Survey. We use Wide Field Camera 3 grism data to spectr…
Spectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration
J. Newman, A. Abate, F. Abdalla +58
Large sets of objects with spectroscopic redshift measurements will be needed for imaging dark energy experiments to achieve their full potential, serving two goals:_training_, i.e…
The Spitzer-South Pole Telescope Deep Field: Survey Design and IRAC Catalogs
M. L. N. Ashby, S. A. Stanford, M. Brodwin +18
The Spitzer-South Pole Telescope Deep Field (SSDF) is a wide-area survey using Spitzer's Infrared Array Camera (IRAC) to cover 94 square degrees of extragalactic sky, making it the…
A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing
J. E. Geach, R. C. Hickox, L. E. Bleem +52
We measure the cross-power spectrum of the projected mass density as traced by the convergence of the cosmic microwave background lensing field from the South Pole Telescope (SPT)…
Large gas reservoirs and free-free emission in two lensed star-forming galaxies at z=2.7
M. Aravena, E. J. Murphy, J. E. Aguirre +26
We report the detection of CO(1-0) line emission in the bright, lensed star-forming galaxies SPT-S 233227-5358.5 (z=2.73) and SPT-S 053816-5030.8 (z=2.78), using the Australia Tele…
CANDELS Observations of the Environmental Dependence of the Color-Mass-Morphology Relation at z = 1.6
Robert Bassett, Casey Papovich, Jennifer M. Lotz +16
We study the environmental dependence of color, stellar mass, and morphology by comparing galaxies in a forming cluster to those in the field at z = 1:6 with Hubble Space Telescope…
Aperture corrections for disk galaxy properties derived from the CALIFA survey. Balmer emission lines in spiral galaxies
J. Iglesias-Páramo, J. M. Vílchez, L. Galbany +37
This work investigates the effect of the aperture size on derived galaxy properties for which we have spatially-resolved optical spectra. We focus on some indicators of star format…
A CMB lensing mass map and its correlation with the cosmic infrared background
G. P. Holder, M. P. Viero, O. Zahn +54
We use a temperature map of the cosmic microwave background (CMB) obtained using the South Pole Telescope at 150 GHz to construct a map of the gravitational convergence to z ~ 1100…
Constraining The Assembly Of Normal And Compact Passively Evolving Galaxies From Redshift z=3 To The Present With CANDELS
P. Cassata, M. Giavalisco, C. C. Williams +16
We study the evolution of the number density, as a function of the size, of passive early-type galaxies with a wide range of stellar masses 10^10<M*/Msun<10^11.5) from z~3 to z~1,…