activity
19982007
most citedAutomated selection and characterization of emission-line sources in ACS WFC grism data

9 citations · 9 across the 2 of their papers we have counts for

collaborators
Showing astro-phShow all

10 papers · 1 filter

astro-ph20079 cited

Automated selection and characterization of emission-line sources in ACS WFC grism data

Gerhardt R. Meurer, Z. I. Tsvetanov, C. Gronwall +10

We present complimentary techniques to find emission-line targets and measure their properties in a semi-automated fashion from grism observations obtained with the Advanced Camera…

astro-ph2004

HST/ACS Coronagraphic Imaging of the AU Microscopii Debris Disk

John E. Krist, D. R. Ardila, D. A. Golimowski +5

We present {\it Hubble Space Telescope} Advanced Camera for Surveys multicolor coronagraphic images of the recently discovered edge-on debris disk around the nearby ( pc) M…

astro-ph2001

Cluster Galaxy Populations from z=0.33 - 0.83: Characterizing Evolution with CL1358+62

Kim-Vy Tran, Garth Illingworth, Marijn Franx

We combine HST WFPC mosaics of clusters at multiple redshifts with Keck LRIS spectroscopy to characterize different galaxy populations and how they evolve. By combining quantitativ…

astro-ph2000

Evolution of Cluster Early-Type Galaxies

P. G. van Dokkum, M. Franx, D. D. Kelson +2

The slow evolution of the M/L ratios, colors, and line strengths of cluster early-type galaxies to z=1 suggests that their stars were formed at very high redshift. At the same time…

astro-ph2000

Type Ia Supernovae and the Value of the Hubble Constant

Brad K. Gibson, Chris B. Brook

The methodology involved in deriving the Hubble Constant via the calibration of the corrected peak luminosities of Type Ia supernovae (SNe) is reviewed. We first present a re-analy…

astro-ph1999

Luminous red mergers in the z=0.83 cluster MS1054-03: Direct evidence for hierarchical formation of massive early-type galaxies

P. G. van Dokkum, M. Franx, D. Fabricant +2

We present results from a morphological study of the distant X-ray cluster MS1054-03 at z=0.83. We have obtained a large, two color HST WFPC2 mosaic of this cluster, and measured r…