We present long slit spectra for a magnitude limited sample of 35 E and S0
galaxies of the Coma cluster. The high quality of the data allowed us to de
rive spatially resolved spectra for a substantial sample of Coma galaxies f
ar the first time. From these spectra we obtained rotation curves: the velo
city dispersion profiles and the H-3 and H-4 coefficients of the Hermite de
composition of the line of sight velocity distribution. Moreover, we derive
the radial line index profiles of Mg, Fe and H beta line indices out to R
approximate to 1r(e) - 3r(e) with high signal-to-noise ratio. We describe t
he galaxy sample, the observations and data reduction, and present the spec
troscopic database. Groundbased photometry for a subsample of 8 galaxies is
also presented.
The Coma cluster is one of the richest known clusters of galaxies, spanning
about 4 decades in density. Hence it is the ideal place to study the struc
ture of galaxies as a function of environmental density in order to constra
in the theories of galaxy formation and evolution. Based on the spectroscop
ic database: presented, we will discuss these issues in a series of future
papers.