Redshifts in the Southern Abell Redshift Survey clusters. I. The data

被引:14
|
作者
Way, MJ
Quintana, H
Infante, L
Lambas, DG
Muriel, H
机构
[1] NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
[2] Pontificia Univ Catolica Chile, Dept Astron & Astrophys, Santiago 22, Chile
[3] Astron Observ, Grp Invest Astron Teor & Expt, RA-5000 Cordoba, Argentina
[4] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina
关键词
galaxies : clusters : general; galaxies : distances and redshifts;
D O I
10.1086/462418
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Southern Abell Redshift Survey (SARS) contains 39 clusters of galaxies with redshifts in the range 0.0 < z < 0.31 and a median redshift depth of (z) over bar = 0.0845. SARS covers the region 0 degrees < delta < - 65 degrees, alpha < 5(h), alpha > 21(h) ( while avoiding the LMC and SMC), with \b\ > 40 degrees. Cluster locations were chosen from the Abell and Abell-Corwin-Olowin catalogs, while galaxy positions were selected from the Automatic Plate Measuring Facility galaxy catalog with extinction-corrected magnitudes in the range 15 <= b(J) < 19. SARS used the Las Campanas 2.5 m du Pont telescope, observing either 65 or 128 objects concurrently over a 1.5 deg(2) field. New redshifts for 3440 galaxies are reported in the fields of these 39 clusters of galaxies.
引用
收藏
页码:2012 / 2018
页数:7
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