SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line Diagnostics

We use the Herschel /PACS spectrometer to study the global and spatially resolved far-infrared (FIR) fine-structure line emission in a sample of 52 galaxies that constitute the SHINING survey. These galaxies include star-forming, active-galactic nuclei (AGNs), and luminous infrared galaxies (LIRGs). We find an increasing number of galaxies (and kiloparsec-size regions within galaxies) with low line-to-FIR continuum ratios as a function of increasing FIR luminosity ( L FIR ), dust infrared color, L FIR to molecular gas mass ratio ( L FIR / M mol ), and FIR surface brightness (Σ FIR ). The correlations between the [C ii ]/FIR or [O i ]/FIR ratios with Σ FIR are remarkably tight (∼0.3 dex scatter over almost four orders of magnitude in Σ FIR ). We observe that galaxies with and Σ FIR ≳ 10 11 L ⊙ kpc −2 tend to have weak fine-structure line-to-FIR continuum ratios, and that LIRGs with infrared sizes ≳1 kpc have line-to-FIR ratios comparable to those observed in typical star-forming galaxies. We analyze the physical mechanisms driving these trends in Paper II. The combined analysis of the [C ii ], [N ii ] 122 μ m, and [O iii ] 88 μ m lines reveals that the fraction of the [C ii ] line emission that arises from neutral gas increases from 60% to 90% in the most active star-forming regions and that the emission originating in the ionized gas is associated with low-ionization, diffuse gas rather than with dense gas in H ii regions. Finally, we report the global and spatially resolved line fluxes of the SHINING galaxies to enable the comparison and planning of future local and high- z studies.