Streaming motions of galaxy clusters within 12 000 km s(-1) - II. New photometric data for the Fundamental Plane

Citation
Rj. Smith et al., Streaming motions of galaxy clusters within 12 000 km s(-1) - II. New photometric data for the Fundamental Plane, M NOT R AST, 327(1), 2001, pp. 249-264
Citations number
35
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
327
Issue
1
Year of publication
2001
Pages
249 - 264
Database
ISI
SICI code
0035-8711(20011011)327:1<249:SMOGCW>2.0.ZU;2-P
Abstract
We present new R-band photometric data for 447 galaxies, gathered for the ' Streaming Motions of Abell Clusters' (SMAC) project. The data comprise 629 individual measurements of the Fundamental Plane (FP) parameters effective radius (R-e) and surface brightness derived from r(1/4)-law profile fitting . More than a third of the galaxies were observed more than once. The photo metric precision is similar to0.02 mag as judged from comparisons of apertu re photometry between repeat observations of galaxies. The combination X-fp = log R-e - 0.33[mu](e), e, which enters into the Fundamental Plane relati on, has internal uncertainties of similar to0.008, corresponding to < 2 per cent in estimated distance. Taken individually, the (correlated) internal errors in R-e and [<mu>](e) are similar to8 per cent and similar to0.12 mag respectively. Comparisons with literature data constrain the external rand om errors to less than or similar to5 per cent in distance (per observation ), which is small in comparison to the similar to 20 per cent scatter in th e FR The data will form part of a merged catalogue of FP parameters, presen ted in a companion paper.