activity
19992003
most citedA wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius

359 citations · 760 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph2003★ 20 cited

New Quasars Detected via Variability in the QUEST1 Survey

A. W. Rengstorf, S. L. Mufson, C. Abad +31

By observing the high galactic latitude equatorial sky in drift scan mode with the QUEST (QUasar Equatorial Survey Team) Phase 1 camera, multi-bandpass photometry on a large strip…

astro-ph2003★ 359 cited

A wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius

T. Treu, R. S. Ellis, J. -P. Kneib +5

We describe a new wide field Hubble Space Telescope survey of the galaxy cluster Cl0024+16 (z~0.4) consisting of a sparse-sampled mosaic of 39 Wide Field and Planetary Camera 2 ima…

astro-ph2002★ 24 cited

Reddening-Independent Quasar Selection from a Wide-Field Optical and Near-IR Imaging Survey

R. G. Sharp, C. N. Sabbey, A. K. Vivas +4

We combine deep, wide-field near-IR and optical imaging to demonstrate a reddening-independent quasar selection technique based on identifying outliers in the (g-z) / (z-H) colour…

astro-ph2002★ 28 cited

A Large Area CCD Camera for the Schmidt Telescope at the Venezuelan National Astronomical Observatory

C. Baltay, J. A. Snyder, P. Andrews +25

We have designed, constructed and put into operation a large area CCD camera that covers a large fraction of the image plane of the 1 meter Schmidt telescope at Llano del Hato in V…

astro-ph2001★ 108 cited

The Las Campanas IR Survey: Early Type Galaxy Progenitors Beyond Redshift One

P. J. McCarthy, R. G. Carlberg, H. -W. Chen +16

(Abridged) We have identified a population of faint red galaxies from a 0.62 square degree region of the Las Campanas Infrared Survey whose properties are consistent with their bei…

astro-ph2001★ 105 cited

The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution

A. E. Firth, R. S. Somerville, R. G. McMahon +15

The LCIR Survey, using the Cambridge IR Survey Instrument (CIRSI), reaches H \~ 20-21 over ~1 deg^2. We present results for 744 arcmin^2 in which public UBVRI data exist. We compar…