The Spitzer SDSS Statistical Spectroscopic Survey (S5) is a Cycle-5 Spitzer
Legacy program to acquire 5 to 40 micron mid-infrared spectroscopy of a
representative sample of galaxies from SDSS, selected for having prior
photometric coverage in the UV and Halpha fluxes greater than 3x10-15
erg/s/cm2. The S5 project is an extension of the SSGSS over a larger set of SDSS
sources (292) and narrower redshift range. In addition, the S5 sample was
selected without mid-IR prior.
These data represent the first public data release of the full S5 sample. The
dataset includes short-low, long-low, and short-high IRS spectroscopy for the
full sample. Sources have been selected in 48 patches of at least 5 sources
spatially separated by less than 30' in order to take advantage of the cluster
observing mode of Spitzer.
If you use S5 data, please cite the dataset Digital Object Identifier (DOI): 10.26131/IRSA503.
Jump to documentation.
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S5 Overview
S5 Primary Data Access
S5 Galaxy Summaries