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19962005
most citedAn Automatic Image Reduction Pipeline for the Advanced Camera for Surveys

3 citations · 3 across the 5 of their papers we have counts for

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11 papers · 1 filter

astro-ph2005

Cluster Evolution Since z~1

R. Demarco, J. P. Blakeslee, H. C. Ford +8

We have used the Advanced Camera for Surveys (ACS) on the HST to obtain optical imaging of a sample of 8 galaxy clusters in the redshift range 0.8 < z < 1.3. The ACS data provides…

astro-ph2005

The ACS Virgo Cluster Survey V: SBF Calibration for Giant and Dwarf Early-type Galaxies

Simona Mei, John P. Blakeslee, John L. Tonry +7

As part of the Advanced Camera for Survey (ACS) Virgo Cluster Survey, we have measured Surface Brightness Fluctuations (SBF) in a sample of 100 early-type Virgo galaxies. Distances…

astro-ph2003

The Extragalactic Distance Scale

Joseph B. Jensen, John L. Tonry, John P. Blakeslee

Significant progress has been made during the last 10 years toward resolving the debate over the expansion rate of the Universe. The current value of the Hubble parameter, Ho, is n…

astro-ph20023 cited

An Automatic Image Reduction Pipeline for the Advanced Camera for Surveys

J. P. Blakeslee, K. R. Anderson, G. R. Meurer +2

We have written an automatic image processing pipeline for the Advanced Camera for Surveys (ACS) Guaranteed Time Observation (GTO) program. The pipeline, known as Apsis, supports t…

astro-ph2002

Calibration of Geometric Distortion in the ACS Detectors

G. R. Meurer, D. Lindler, J. P. Blakeslee +9

The off-axis location of the Advanced Camera for Surveys (ACS) is the chief (but not sole) cause of strong geometric distortion in all detectors: the Wide Field Camera (WFC), High…

astro-ph2001

Testing the Supernova, Cepheid, and Early-type Galaxy Distance Scales

John P. Blakeslee

I summarize recent work comparing relative distances measured to individual galaxies with independent methods. The comparisons include: ground-based surface brightness fluctuation…