Our observations include photometric and spectral-line observations from both the PACS and SPIRE instruments onboard Herschel, obtained as part of the large KINGFISH (Key Insights on Nearby Galaxies: a Far- Infrared Survey with Herschel, Kennicutt+ 2011PASP..123.1347K) and BtP (B
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Our observations include photometric and spectral-line observations from both the PACS and SPIRE instruments onboard Herschel, obtained as part of the large KINGFISH (Key Insights on Nearby Galaxies: a Far- Infrared Survey with Herschel, Kennicutt+ 2011PASP..123.1347K) and BtP (Beyond the Peak; OT1_jsmith1; P.I. J.D. Smith) projects.
[NII]205um BtP observations were performed with SPIRE-FTS intermediate mapping, which is a 4-point dither. E. Pellegrini et al. (2017, in preparation) will contain a full description of the observations and reductions.
[CII]158um and [NII]122um emission lines, and 70 and 160um continuum maps have been observed as part the Herschel Open Time Key Program KINGFISH. The data and the associated reduction are described in Kennicutt+ (2011PASP..123.1347K) and Croxall+ (2013ApJ...777...96C).
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