VizieR Online Data Catalog: The SFRS: 3-33GHz VLA obs. of star-forming regions (Linden+, 2020)

The Star Formation in Radio Survey (SFRS) sample includes targeted observations from 56 nearby galaxies (d_L<30Mpc) in the Spitzer Infrared Nearby Galaxies Survey (SINGS; Kennicutt+ 2003PASP..115..928K) and Key Insights on Nearby Galaxies: a Far-Infrared Survey (KINGFISH; Kennicutt+ 2011PASP..123.1347K) legacy programs (Table 1).

The full sample over the entire sky consists of 118 star-forming complexes (56 nuclei and 62 extranuclear regions), 112 of which (50 nuclei and 62 extranuclear regions; see Tables 2 and 3, respectively) are observable with the VLA (i.e., having δ>-35°).

The observational setup and reduction procedure for the Ka-band (29-37GHz) data (11B-032,13A-129) is described in detail in M18a (Murphy+, 2018, J/ApJS/234/24). Observations in the S band (2-4GHz) were taken during the 2013 VLA B-configuration cycle (13B-215) and utilized the 8-bit sampler. Observations in the Ku band (12-18GHz) were taken in 2014 November in the C configuration (13B-215) using the 3-bit samplers. Both sets of observations utilized the full available bandwidth of the respective receivers.

(7 data files).