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19982008
most citedThe Red Sequence Luminosity Function in Massive Intermediate Redshift Galaxy Clusters

52 citations · 52 across the 1 of their papers we have counts for

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astro-ph200852 cited

The Red Sequence Luminosity Function in Massive Intermediate Redshift Galaxy Clusters

S. M. Crawford, M. A Bershady, J. G. Hoessel

We measure the rest-frame B-band luminosity function of red-sequence galaxies (RSLF) of five intermediate-redshift (0.5 < z < 0.9), high-mass (sigma > 950 km/s) clusters. Cluster g…

astro-ph2005

Luminous Compact Blue Galaxies in Intermediate Redshift Galaxy Clusters: A Significant But Extreme Butcher-Oemler Population

S. M. Crawford, M. A. Bershady, A. D. Glenn +1

We identify a population of Luminous Compact Blue Galaxies (LCBGs) in two galaxy clusters: MS0451.6-0305 (z=0.54) and Cl1604+4304 (z=0.9). LCBGs are identified via photometric char…

astro-ph2004

Cepheids and Long Period Variables in NGC 4395

F. Thim, J. G. Hoessel, A. Saha +3

Repeated imaging observations of NGC 4395 were made with the WIYN 3.5 m and the KPNO 2.1 m telescopes. From the photometry of the resolved brighter stars in this galaxy eleven Ceph…

astro-ph2003

Short-Period Variable Stars in the M31 Halo

A. E. Dolphin, A. Saha, E. W. Olszewski +4

We report the findings of a new search for RR Lyraes in an M31 halo field located 40 arcminutes from the nucleus of the galaxy along the minor axis. We detected 37 variable stars,…

astro-ph2003

Deep HST Imaging of Sextans A. III. The Star Formation History

Andrew E. Dolphin, A. Saha, Evan D. Skillman +6

We present a measurement of the star formation history of Sextans A, based on WFPC2 photometry that is 50% complete to V=27.5 (M_V ~+ 1.9) and I=27.0. The star formation history an…

astro-ph2002

Deep HST Imaging of Sextans A. II. Cepheids and Distance

Andrew E. Dolphin, A. Saha, Evan D. Skillman +6

We have identified 82 short-period variable stars in Sextans A from deep WFPC2 observations. All of the periodic variables appear to be short-period Cepheids, with periods as small…