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20032009
most citedHST/ACS Multiband Coronagraphic Imaging of the Debris Disk around Beta Pictoris

203 citations · 203 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2009

Investigations of the Formation and Evolution of Planetary Systems

Alwyn Wootten, Bryan Butler, Antonio Hales +3

Stars and planets are the fundamental objects of the Universe. Their formation processes, though related, may differ in important ways. Stars almost certainly form from gravitation…

astro-ph2006203 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

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

Feedback and Brightest Cluster Galaxy Formation: ACS Observations of the Radio Galaxy TN J1338--1942 at z=4.1

Andrew W. Zirm, R. A. Overzier, G. K. Miley +12

We present deep optical imaging of the z=4.1 radio galaxy TN J1338--1942 obtained using the ACS on-board HST. The radio galaxy is known to reside within a large galaxy overdensity…

astro-ph2005

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

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…