Wisconsin PCA-based Stellar Masses and Velocity Dispersions

DR9
DR10
DR11
DR12
BOSS
CAS (click, then search in Schema Browser)
stellarMassPCAWiscBC03
CAS (click, then search in Schema Browser)
stellarMassPCAWiscM11
GALAXY
Yan-Mei Chen, Guinevere Kauffmann, Christy A. Tremonti, Simon White, Timothy M. Heckman, Katarina Kovač, Kevin Bundy, John Chisholm, Claudia Maraston, Donald P. Schneider, Adam S. Bolton, Benjamin A. Weaver, Jon Brinkmann
Type:
Scientific Analysis Catalog
Location on SAS:
https://data.sdss.org/sas/dr12/boss/spectro/redux/galaxy/v1_1/
DATAMODEL:
https://data.sdss.org/datamodel/files/BOSS_GALAXY_REDUX/GALAXY_VERSION
This VAC is described in full at www.sdss.org/dr17/spectro/galaxy_wisconsin/

Wisconsin stellar masses and velocity dispersions are derived from the optical rest-frame spectral region (3700-5500 Ångstroms) using a principal component analysis (PCA) method (Chen et al. 2012). The estimation is based on a library of model spectra generated using the single stellar population models of Bruzal & Charlot (2003) and Maraston & Strömbäck (2011), and with a broad range of star-formation histories, metallicities, dust extinctions, and stellar velocity dispersions.

  1. SDSS
  2. Value Added Catalogs
  3. Wisconsin PCA-based Stellar Masses and Velocity Dispersions