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CAIRNS: The Cluster And Infall Region Nearby Survey
The CAIRNS (Cluster and Infall Region Nearby Survey) project is a spectroscopic survey of the infall regions surrounding eight nearby, rich, X-ray?luminous clusters of galaxies. We have collected
RVSAO 2.0: Digital Redshifts and Radial Velocities
RVSAO is a set of programs to obtain redshifts and radial velocities from digital spectra. RVSAO operates in the IRAF environment. The heart of the system is xcsao, which implements the
The Updated Zwicky Catalog (UZC)
ABSTRACT The Zwicky Catalog of galaxies (ZC), with \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont}
THE CHEMICAL EVOLUTION OF STAR-FORMING GALAXIES OVER THE LAST 11 BILLION YEARS
We calculate the stellar mass-metallicity relation at five epochs ranging to z {approx} 2.3. We quantify evolution in the shape of the mass-metallicity relation as a function of redshift; the
The Southern Sky Redshift Survey
We report redshifts, magnitudes, and morphological classifications for 5369 galaxies with mB ≤ 15.5 and for 57 galaxies fainter than this limit, in two regions covering a total of 1.70 sr in the
Discovery of an Unbound Hypervelocity Star in the Milky Way Halo
We have discovered a star, SDSS J090745.0+024507, leaving the Galaxy with a heliocentric radial velocity of 853 ± 12 km s-1, the largest velocity ever observed in the Milky Way halo. The star is
MEASURING THE ULTIMATE HALO MASS OF GALAXY CLUSTERS: REDSHIFTS AND MASS PROFILES FROM THE HECTOSPEC CLUSTER SURVEY (HECS)
The infall regions of galaxy clusters represent the largest gravitationally bound structures in a ΛCDM universe. Measuring cluster mass profiles into the infall regions provides an estimate of the
Hypervelocity Stars III. The Space Density and Ejection History of Main Sequence Stars from the Galactic Center
We report the discovery of three new unbound hypervelocity stars (HVSs), stars traveling with such extreme velocities that dynamical ejection from a massive black hole (MBH) is their only suggested
CAIRNS: The Cluster and Infall Region Nearby Survey. II. Environmental Dependence of Infrared Mass-to-Light Ratios
CAIRNS (Cluster and Infall Region Nearby Survey) is a spectroscopic survey of the infall regions surrounding nine nearby rich clusters of galaxies. In our previous paper, we used redshifts within ~10
V - AND R-BAND GALAXY LUMINOSITY FUNCTIONS AND LOW SURFACE BRIGHTNESS GALAXIES IN THE CENTURY SURVEY
We use 64 deg2 of deep V and R CCD images to measure the local V- and R-band luminosity functions of galaxies. The V0 < 16.7 and R0 < 16.2 redshift samples contain 1255 and 1251 galaxies and are
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