Redshifts in the Southern Abell Redshift Survey Clusters. I. The Data | Zendy

M. J. Way | Zendy; H. Quintana | Zendy; L. Infante | Zendy; D. G. Lambas | Zendy; H. Muriel | Zendy

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Redshifts in the Southern Abell Redshift Survey Clusters. I. The Data

Author(s) -

M. J. Way,

H. Quintana,

L. Infante,

D. G. Lambas,

H. Muriel

Publication year - 2005

Publication title -

the astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.61

H-Index - 271

eISSN - 1538-3881

pISSN - 0004-6256

DOI - 10.1086/462418

Subject(s) - physics , astrophysics , redshift , galaxy , galaxy cluster , redshift survey , astronomy , telescope , cluster (spacecraft) , galaxy groups and clusters , abell 2744 , brightest cluster galaxy , computer science , programming language

The Southern Abell Redshift Survey contains 39 clusters of galaxies withredshifts in the range 0.0 < z < 0.31 and a median redshift depth of z =0.0845. SARS covers the region 0 < decl < -65 deg, R.A. < 5h, R.A. > 21h (whileavoiding the LMC and SMC) with b > 40. Cluster locations were chosen from theAbell and Abell-Corwin-Olowin catalogs while galaxy positions were selectedfrom the Automatic Plate Measuring Facility galaxy catalog withextinction-corrected magnitudes in the range 15 <= b_j < 19. SARS utilized theLas Campanas 2.5 m duPont telescope, observing either 65 or 128 objectsconcurrently over a 1.5 sq deg field. New redshifts for 3440 galaxies arereported in the fields of these 39 clusters of galaxies.

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