other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2004A&A...427..397H - Astronomy and Astrophysics, volume 427, 397-413 (2004/11-4)
Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS). Redshifts, velocity dispersions and substructure for 5 clusters.
HALLIDAY C., MILVANG-JENSEN B., POIRIER S., POGGIANTI B.M., JABLONKA P., ARAGON-SALAMANCA A., SAGLIA R.P., DE LUCIA G., PELLO R., SIMARD L., CLOWE D.I., RUDNICK G., DALCANTON J.J., WHITE S.D.M. and ZARITSKY D.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): galaxies: clusters: general - galaxies: distances and redshifts - galaxies: evolution
VizieR on-line data: <Available at CDS (J/A+A/427/397): cl1040.dat cl105411.dat cl105412.dat cl1216.dat cl1232.dat>
Nomenclature: Catalogues: EDCS JHHMMSSs+DDMMSSsA N=158+128+131+136+119.
CDS comments: Membership probability in Simbad comes from the membership flag given in tables: flag "1", for cluster members within 3 sigma cluster of the cluster redshift, has been interpreted into 100%; flag "2", for galaxies at 3 to 4 sigma cluster from the cluster redshift, has been interpreted into 80%; flag "3", for galaxies at 4 to 10 sigma cluster from the cluster redshift, has been interpreted into 50%; flag "0", for fore- or background galaxies, has been interpreted into O%.
Simbad objects: 661