inous galaxy clusters are used to produce morphological measurements for galaxies in their field. | |
in source: | 1E 0015.9+1609 = ClG 0016+1609 |
in source: | 1E 1054.4-0321 = ClG 1054-0321 |
in source: | 1E 1358.4+6245 = ClG 1358+6245 |
in source: | 1E 1621.5+2640 = ClG 1621+2640 |
Ref: | =2005ApJS..157..228S |
by | SAINTONGE A. , SCHADE D., ELLINGSON E., YEE H.K.C., CARLBERG R.G. |
Astrophys. J., Suppl. Ser., 157, 228-250 (2005) | |
Catalog of galaxy morphology in four rich clusters: luminosity evolution of disk galaxies at 0.33 < z < 0.83. | |
o | Tables 2 to 5: <[SSE2005] A-N-XXXX-YYYY> N=331+381+672+258. |
=E= | Catalogue in electronic form as J/ApJS/157/228 |
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