The Morphological Content of 10 EDisCS Clusters at 0.5 <z< 0.8
Author(s) -
Vandana Desai,
Julianne J. Dalcanton,
Alfonso AragónSalamanca,
P. Jablonka,
Bianca M. Poggianti,
Stephanie M. Gogarten,
L. Simard,
B. MilvangJensen,
Gregory Rudnick,
Dennis Zaritsky,
Douglas Clowe,
C. Halliday,
R. Pelló,
R. P. Saglia,
S. V. White
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/513310
Subject(s) - physics , astrophysics , redshift , context (archaeology) , galaxy , velocity dispersion , galaxy cluster , cluster (spacecraft) , astronomy , content (measure theory) , star formation , geography , mathematical analysis , mathematics , archaeology , computer science , programming language
18 pages, 7 figures; To be published in ApJ; minor changes made to table labelsInternational audienceWe describe Hubble Space Telescope (HST) imaging of 10 of the 20 ESO Distant Cluster Survey (EDisCS) fields. Each ~40 arcmin2 field was imaged in the F814W filter with the Advanced Camera for Surveys Wide Field Camera. Based on these data, we present visual morphological classifications for the ~920 sources per field that are brighter than Iauto=23 mag. We use these classifications to quantify the morphological content of 10 intermediate-redshift (0.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom