Nearly 5000 distant early-type galaxies in COMBO-17: a red sequence and its evolution since z~ 1
We present the rest-frame colors and luminosities of~ 25,000 m R≲ 24 galaxies in the
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
Differential galaxy evolution in cluster and field galaxies at z≈ 0.3
We measure spectral indexes for 1823 galaxies in the Canadian Network for Observational
Cosmology 1 (CNOC1) sample of 15 X-ray luminous clusters at 0.18< z< 0.55 to investigate …
Cosmology 1 (CNOC1) sample of 15 X-ray luminous clusters at 0.18< z< 0.55 to investigate …
Galaxy luminosity functions to z~ 1 from DEEP2 and COMBO-17: implications for red galaxy formation
The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …
The origin of star formation gradients in rich galaxy clusters
We examine the origin of clustercentric gradients in the star formation rates and colors of rich
cluster galaxies within the context of a simple model where clusters are built through the …
cluster galaxies within the context of a simple model where clusters are built through the …
Galaxy stellar mass assembly between 0.2< z< 2 from the S-COSMOS survey
GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 < z < 2 FROM THE S-COSMOS
SURVEY - IOPscience Skip to content IOP Science home Accessibility Help Search Journals …
SURVEY - IOPscience Skip to content IOP Science home Accessibility Help Search Journals …
The galaxy luminosity function and luminosity density at redshift z= 0.1
MR Blanton, DW Hogg, NA Bahcall… - The Astrophysical …, 2003 - iopscience.iop.org
Using a catalog of 147,986 galaxy redshifts and fluxes from the Sloan Digital Sky Survey
(SDSS), we measure the galaxy luminosity density at z= 0.1 in five optical bandpasses …
(SDSS), we measure the galaxy luminosity density at z= 0.1 in five optical bandpasses …
Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G3Cv1)
ASG Robotham, P Norberg, SP Driver… - Monthly Notices of …, 2011 - academic.oup.com
Using the complete Galaxy and Mass Assembly I (GAMA-I) survey covering∼ 142 deg2 to r
AB= 19.4, of which∼ 47 deg2 is to r AB= 19.8, we create the GAMA-I galaxy group …
AB= 19.4, of which∼ 47 deg2 is to r AB= 19.8, we create the GAMA-I galaxy group …
The broadband optical properties of galaxies with redshifts 0.02< Z< 0.22
MR Blanton, DW Hogg, NA Bahcall… - The Astrophysical …, 2003 - iopscience.iop.org
Using photometry and spectroscopy of 183,487 galaxies from the Sloan Digital Sky Survey,
we present bivariate distributions of pairs of seven galaxy properties: four optical colors …
we present bivariate distributions of pairs of seven galaxy properties: four optical colors …
A new method for galaxy cluster detection. I. The algorithm
MD Gladders, HKC Yee - The Astronomical Journal, 2000 - iopscience.iop.org
Numerous methods for finding clusters at moderate to high redshifts have been proposed in
recent years, at wavelengths ranging from radio to X-rays. In this paper we describe a new …
recent years, at wavelengths ranging from radio to X-rays. In this paper we describe a new …
[O ii] as a star formation rate indicator
We investigate the [O II] emission line as a star formation rate (SFR) indicator using
integrated spectra of 97 galaxies from the Nearby Field Galaxies Survey (NFGS). The …
integrated spectra of 97 galaxies from the Nearby Field Galaxies Survey (NFGS). The …