We have obtained deep, long-slit spectroscopy along the major axis of NGC 6166, the cD
galaxy in the cluster A2199, in order to measure the kinematics of intracluster stars at large …

… parameters with the accuracy needed for the fundamental plane (Kelson et al. 2000a). …
As is discussed in more detail in Kelson et al. (2000a), the R-band selected sample contains …

We present new results on the fundamental plane of galaxies in two rich clusters, Cl 1358+
62 at z= 0.33 and MS 2053-04 at z= 0.58, based on Keck and Hubble Space Telescope …

… The spectroscopy and surface photometry are discussed by Kelson et al. (2000a, 2000b).
Using these data, we now analyze the fundamental plane in the cluster, with the goal of …

In this paper we analyze previously published spectra with high signal-to-noise ratios of E/S0s
in the rich cluster CL 1358+ 62 at z= 0.33. Introducing techniques for fitting stellar …

… , University of California at Santa Cruz, Santa Cruz, CA … remain elusive (Pahre 1998; although
consult Kelson 1998), the … vector (within DD Kelson, in preparation). In other words, large …

… Another source of error arises from uncertainties in the Extragalactic Distance Scale Key
Projectœs correction to the zero point (see, eg, Stetson 1998); we estimate that it introduces an …

We present new results from a systematic study of absorption-line strengths of galaxies in
clusters approaching redshifts of unity. In this Letter, we specifically compare the strengths of …

We have obtained deep, long-slit spectroscopy along the major axis of NGC 6166, the cD
galaxy in the cluster Abell 2199, in order to measure the kinematics of intracluster starlight at …

We select E+ A candidates from a spectroscopic data set of~ 800 field galaxies and measure
the E+ A fraction at 0.3< z< 1 to be 2.7%�1.1%, a value lower than that in galaxy clusters at …