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19952001
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astro-ph2001

X-ray temperature and morphology of z>0.8 clusters of galaxies

B. Holden, S. A. Stanford, P. Rosati +4

We discuss our current progress in studying a sample of z>0.8 clusters of galaxies from the ROSAT Distant Cluster Survey. To date, we have Chandra observations for four of the ten…

astro-ph2000

The CFH Optical PDCS survey (COP) I: The Data

C. Adami, B. Holden, F. J. Castander +5

This paper presents and gives the COP (COP: CFHT Optical PDCS; CFHT: Canada-France-Hawaii Telescope; PDCS: Palomar Distant Cluster Survey) survey data. We describe our photometric…

astro-ph1999

Simulations Applied to the Bright SHARC XCLF: Results and Implications

M. P. Ulmer, C. Adami, R. Pildis +3

We have performed simulations of the effectiveness of the Serendipitous High-redshift Archival ROSAT Cluster (SHARC) survey for various model universes. We find, in agreement with…

astro-ph1999

A Turn-over in the Galaxy Luminosity Function of the Coma Cluster Core?

C. Adami, M. P. Ulmer, F. Durret +5

Our previous study of the faint end (R21.5) of the galaxy luminosity function (GLF) was based on spectroscopic data in a small region near the Coma cluster center. In this pr…

astro-ph1997

The Southern SHARC Survey: the z = 0.3 - 0.7 Cluster XLF

D. J. Burke, C. A. Collins, R. M. Sharples +3

We present the z = 0.3 - 0.7 cluster X-ray luminosity function (XLF) determined from the Southern SHARC (Serendipitous High-redshift Archival ROSAT Cluster) survey. Over the lumino…

astro-ph1997

A Search For Large-Scale Structure at High Redshift

A. J. Connolly, A. S. Szalay, A. K. Romer +4

We present new and exciting results on our search for large-scale structure at high redshift. Specifically, we have just completed a detailed analysis of the area surrounding the c…