activity
19932020
most citedThe Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set

1.7k citations · 3.9k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.IM2020★ 74 cited

Properties and characteristics of the WFIRST H4RG-10 detectors

Gregory Mosby, Bernard J. Rauscher, Chris Bennett +16

The Wide-Field Infrared Survey Telescope (WFIRST) will answer fundamental questions about the evolution of dark energy over time and expand the catalog of known exoplanets into new…

astro-ph2006★ 203 cited

HST/ACS Multiband Coronagraphic Imaging of the Debris Disk around Beta Pictoris

D. A. Golimowski, D. R. Ardila, J. E. Krist +40

(Abridged.) We present F435W (B), F606W (Broad V), and F814W (Broad I) coronagraphic images of the debris disk around Beta Pictoris obtained with HST's Advanced Camera for Surveys.…

astro-ph2006★ 80 cited

Evolution of the Color-Magnitude Relation in High-Redshift Clusters: Blue Early-Type Galaxies and Red Pairs in RDCS J0910+5422

S. Mei, J. P. Blakeslee, S. A. Stanford +17

The color-magnitude relation has been determined for the RDCS J0910+5422 cluster of galaxies at redshift z = 1.106. Cluster members were selected from HST ACS images, combined with…

astro-ph2005★ 41 cited

A Dynamical Simulation of the Debris Disk Around HD 141569A

D. R. Ardila, S. H. Lubow, D. A. Golimowski +36

We study the dynamical origin of the structures observed in the scattered-light images of the resolved debris disk around HD 141569A. We explore the roles of radiation pressure fro…

astro-ph2005★ 43 cited

Evolution in the Cluster Early-type Galaxy Size-Surface Brightness Relation at z =~ 1

B. P. Holden, J. P. Blakeslee, M. Postman +7

We investigate the evolution in the distribution of surface brightness, as a function of size, for elliptical and S0 galaxies in the two clusters RDCS J1252.9-2927, z=1.237 and RX…

astro-ph2005★ 398 cited

The Morphology - Density Relation in z ~ 1 Clusters

M. Postman, M. Franx, N. Cross +10

We measure the morphology--density relation (MDR) and morphology-radius relation (MRR) for galaxies in seven z ~ 1 clusters that have been observed with the Advanced Camera for Sur…