activity
19942005
most citedExtragalactic Thick Disks: Implications for Early Galaxy Evolution

1 citations · 1 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph20051 cited

Extragalactic Thick Disks: Implications for Early Galaxy Evolution

Julianne J. Dalcanton, Anil Seth, Peter Yoachim

I briefly review the growing evidence that thick stellar disks surround most edge-on disk galaxies. Recent studies show that these extragalactic thick disks have old ages, low meta…

astro-ph2005

The Vertical Structure of Stars in Edge-on Galaxies

Anil Seth, Julianne Dalcanton, Roelof de Jong

We present a summary of our recent work on the vertical distribution of the resolved stellar populations in six low mass, edge-on, spiral galaxies observed with the Hubble Space Te…

astro-ph2001

Tracing Cosmic Evolution with the Las Campanas Distant Cluster Survey

Anthony H. Gonzalez, Julianne J. Dalcanton, Amy E. Nelson +3

The Las Campanas Distant Cluster Survey (LCDCS), which contains over 1000 cluster candidates at z>0.3, is a unique sample with which to probe the evolution of both cluster galaxies…

astro-ph2001

Brightest Cluster Galaxies and the Las Campanas Distant Cluster Survey

Dennis Zaritsky, Amy E. Nelson, Luc Simard +2

We present our study of the evolution of brightest cluster galaxies based on data from the Las Campanas Distant Cluster Survey (Gonzalez et al. 2001) and HST optical and IR imaging…

astro-ph2001

An Overview of the Las Campanas Distant Cluster Survey

Dennis Zaritsky, Anthony H. Gonzalez, Amy E. Nelson +1

We present the Las Campanas Distant Cluster Survey, which has produced over a thousand galaxy cluster candidates at 0.35 < z < 1.1 (see Gonzalez et al. 2001 for the full catalog).…

astro-ph1998

Integrated Stellar Populations of Bulges: First Results

S. C. Trager, J. J. Dalcanton, B. J. Weiner

We present first results from an on-going survey of the stellar populations of the bulges and inner disks of spirals at various points along the Hubble sequence. In particular, we…