Spectroscopic target selection for the Sloan Digital Sky Survey: the luminous red galaxy sample

Show full item record

Redirect: RIT Scholars content from RIT Digital Media Library has moved from http://ritdml.rit.edu/handle/1850/1953 to RIT Scholar Works http://scholarworks.rit.edu/article/1152, please update your feeds & links!
Title: Spectroscopic target selection for the Sloan Digital Sky Survey: the luminous red galaxy sample
Author: Eisenstein, Daniel; Annis, James; Gunn, James; Szalay, Alexander; Connolly, Andrew; Nichol, Robert; Bahcall, Neta; Bernardi, Mariangela; Burles, Scott; Castander, Francisco; Fukugita, Masataka; Hogg, David; Ivezic, Zeljko; Knapp, Gillian; Lupton, Robert; Narayanan, Vijay; Postman, Marc; Riechart, Dan; Richmond, Michael; Schneider, Donald; Schlegel, David; Strauss, Michael; SubbaRao, Mark; Tucker, Douglas; Vanden Berk, Daniel; Vogeley, Michael; Weinberg, David; Yanny, Brian
Abstract: We describe the target selection and resulting properties of a spectroscopic sample of luminous, red galaxies (LRG) from the imaging data of the Sloan Digital Sky Survey (SDSS). These galaxies are selected on the basis of color and magnitude to yield a sample of luminous, intrinsically red galaxies that extends fainter and further than the main flux-limited portion of the SDSS galaxy spectroscopic sample. The sample is designed to impose a passively-evolving luminosity and rest- frame color cut to a redshift of 0.38. Additional, yet more luminous, red galaxies are included to a redshift of 0.5. Approximately 12 of these galaxies per square degree are targeted for spectroscopy, so the sample will number over 100,000 with the full survey. SDSS commissioning data indicate that the algorithm efficiently selects luminous (Mg −21.4), red galaxies, that the spectroscopic success rate is very high, and that the resulting set of galaxies is approximately volume-limited out to z = 0.38. When the SDSS is complete, the LRG spectroscopic sample will fill over 1h−3 Gpc3 with an approximately homogeneous population of galaxies and will therefore be well suited to studies of large-scale structure and clusters out to z = 0.5. (Refer to PDF file for exact formulas).
Description: Also archived in: arXiv:astro-ph/0108153 v1 9 Aug 2001
Record URI: http://hdl.handle.net/1850/1953
Date: 2001-11

Files in this item

Files Size Format View
MRichmondArticle11-2001.pdf 748.3Kb PDF View/Open

The following license files are associated with this item:

This item appears in the following Collection(s)

Show full item record

Search RIT DML

Advanced Search