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
15 papers · 1 filter
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 new population of recently quenched elliptical galaxies in the SDSS
Daniel H. McIntosh, Cory Wagner, Andrew Cooper +8
We use the Sloan Digital Sky Survey to investigate the properties of massive elliptical galaxies in the local Universe (z\leq0.08) that have unusually blue optical colors. Through…
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)…
An efficient group authentication for group communications
Lein Harn, Changlu Lin
Group communication implies a many-to-many communication and it goes beyond both one-to-one communication (i.e., unicast) and one-to-many communication (i.e., multicast). Unlike mo…
Crystal Structure and Elastic Properties of Hypothesized MAX Phase-like Compound (Cr2Hf)2Al3C3
Yuxiang Mo, Sitaram Aryal, Paul Rulis +1
The term "MAX phase" refers to a very interesting and important class of layered ternary transition-metal carbides and nitrides with a novel combination of both metal and ceramic-l…
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…
Termination dependent topological surface states of the natural superlattice phase BiSe
Q. D. Gibson, L. M. Schoop, A. P. Weber +9
We describe the topological surface states of BiSe, a compound in the infinitely adaptive Bi-BiSe natural superlattice phase series, determined by a combination…
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,…