Volume 387, Number 1, May III 2002
|Page(s)||26 - 39|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 May 2002|
The scaling relations of early–type galaxies in clusters*
I. Surface photometry in seven nearby clusters
Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, Italy e-mail: firstname.lastname@example.org
2 Dipartimento di Astronomia dell'Università di Padova, Vicolo Osservatorio 2, 35122 Padova, Italy e-mail: email@example.com
3 Copenhagen University Observatory. The Niels Bohr Institute for Astronomy, Physics and Geophysics Juliane Maries Vej 30, 2100 Copenhagen, Denmark e-mail: firstname.lastname@example.org
4 Instituto de Matemáticas y Física Fundamental, CSIC, C/ Serrano 113B, 28006 Madrid, Spain e-mail: email@example.com
Corresponding author: G. Fasano, firstname.lastname@example.org
Accepted: 25 February 2002
This is the first paper of a series investigating the scaling relations of early–type galaxies in clusters. Here we illustrate the multi–band imagery and the image reduction and calibration procedures relative to the whole sample of 22 clusters at . We also present detailed surface photometry of 312 early–type galaxies in 7 clusters in the first redshift bin, –0.075. We give for each galaxy the complete set of luminosity and geometrical profiles, and a number of global, photometric and morphological parameters. They have been evaluated taking into account the effects of seeing. Internal consistency checks and comparisons with data in the literature confirm the quality of our analysis. These data, together with the spectroscopic ones presented in the second paper of the series, will provide the local calibration of the scaling relations.
Key words: galaxies: elliplical and lenticular, cD / galaxies: clusters: general
Tables 6, 7a–7g, the colour prints of Figs. 12a–12g and Figs. 13a–13g are only available in electronic form at http://www.edpsciences.com. The complete set of profiles is available upon request from the authors. Tables 7a–7g are also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (220.127.116.11) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/387/26
© ESO, 2002
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