SSGSS: The Spitzer-SDSS-GALEX Spectroscopic Survey
Matthew J. O'Dowd, David Schiminovich, Benjamin D. Johnson, Marie A., Treyer, Christopher D. Martin, Ted K. Wyder, St\'ephane Charlot, Timothy M., Heckman, Lucimara P. Martins, Mark Seibert, J. M. van der Hulst

TL;DR
The SSGSS provides a comprehensive multi-wavelength spectroscopic dataset of 101 local star-forming galaxies, enabling detailed analysis of their dust, star formation, and AGN properties to improve galaxy evolution models.
Contribution
This paper introduces the SSGSS dataset, combining new mid- to far-infrared spectroscopy with existing multi-wavelength data for a representative galaxy sample.
Findings
Comparison of thermal continuum and silicate absorption with starburst galaxies.
Calibration of PAH luminosity for spectral energy distribution models.
Link between dust mass, star formation history, and AGN activity.
Abstract
The Spitzer-SDSS-GALEX Spectroscopic Survey (SSGSS) provides a new sample of 101 star-forming galaxies at z < 0.2 with unprecedented multi-wavelength coverage. New mid- to far-infrared spectroscopy from the Spitzer Space Telescope is added to a rich suite of previous imaging and spectroscopy, including ROSAT, Galaxy Evolution Explorer, Sloan Digital Sky Survey, Two Micron All Sky Survey, and Spitzer/SWIRE. Sample selection ensures an even coverage of the full range of normal galaxy properties, spanning two orders of magnitude in stellar mass, color, and dust attenuation. In this paper we present the SSGSS data set, describe the science drivers, and detail the sample selection, observations, data reduction, and quality assessment. Also in this paper, we compare the shape of the thermal continuum and the degree of silicate absorption of these typical, star-forming galaxies to those of…
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