Physical properties and environments of nearby galaxies
MR Blanton, J Moustakas - Annual Review of Astronomy and …, 2009 - annualreviews.org
We review the physical properties of nearby, relatively luminous galaxies, using results from
newly available massive data sets together with more detailed observations. First, we …
newly available massive data sets together with more detailed observations. First, we …
The SDSS-IV extended baryon oscillation spectroscopic survey: overview and early data
…, F Beutler, D Bizyaev, MR Blanton… - The Astronomical …, 2016 - iopscience.iop.org
In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic
Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph …
Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph …
The Luminosity function of galaxies in SDSS commissioning data
MR Blanton, J Dalcanton, D Eisenstein… - The Astronomical …, 2001 - iopscience.iop.org
In the course of its commissioning observations, the Sloan Digital Sky Survey (SDSS) has
produced one of the largest redshift samples of galaxies selected from CCD images. Using …
produced one of the largest redshift samples of galaxies selected from CCD images. Using …
The galaxy luminosity function and luminosity density at redshift z= 0.1
MR Blanton, DW Hogg, NA Bahcall… - The Astrophysical …, 2003 - iopscience.iop.org
… The method is described in detail by MR Blanton (2003, in preparation), and we outline it
briefly here. It is akin to the stepwise maximum likelihood (SWML) method of Efstathiou, Ellis, & …
briefly here. It is akin to the stepwise maximum likelihood (SWML) method of Efstathiou, Ellis, & …
New York University Value-Added Galaxy Catalog: a galaxy catalog based on new public surveys
MR Blanton, DJ Schlegel, MA Strauss… - The Astronomical …, 2005 - iopscience.iop.org
Here we present the New York University Value-Added Galaxy Catalog (NYU-VAGC), a
catalog of local galaxies (mostly below z≈ 0.3) based on a set of publicly released surveys …
catalog of local galaxies (mostly below z≈ 0.3) based on a set of publicly released surveys …
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, …
Estimating fixed-frame galaxy magnitudes in the Sloan Digital Sky Survey
MR Blanton, J Brinkmann, I Csabai, M Doi… - The Astronomical …, 2003 - iopscience.iop.org
… In these analyses a function K(z) is added to the standard cosmological bolometric distance
modulus DM(z) to obtain the relationship between the apparent magnitude mR of band R …
modulus DM(z) to obtain the relationship between the apparent magnitude mR of band R …
Sloan digital sky survey IV: Mapping the Milky Way, nearby galaxies, and the distant universe
MR Blanton, MA Bershady, B Abolfathi… - The Astronomical …, 2017 - iopscience.iop.org
The Sloan Digital Sky Survey (SDSS; York et al. 2000) started observations in 1998 and has
completed three different phases. The data collected includes optical imaging of most of the …
completed three different phases. The data collected includes optical imaging of most of the …
K-corrections and filter transformations in the ultraviolet, optical, and near-infrared
MR Blanton, S Roweis - The Astronomical Journal, 2007 - iopscience.iop.org
Template fits to observed galaxy fluxes allow calculation of K-corrections and conversions
among observations of galaxies at various wavelengths. We present a method for creating …
among observations of galaxies at various wavelengths. We present a method for creating …
Improved background subtraction for the sloan digital sky survey images
MR Blanton, E Kazin, D Muna, BA Weaver… - The Astronomical …, 2011 - iopscience.iop.org
… To do so, we insert fake galaxies into the raw data, using the same tools developed by
Blanton et al. (2005a) and used by several other investigators since (Blanton et al. 2005b; …
Blanton et al. (2005a) and used by several other investigators since (Blanton et al. 2005b; …