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Table A.1.
References of the data shown in Fig. 1.
| Panel in Fig. 1 | λ, L | Instrument | Res. | Survey, Reference |
|---|---|---|---|---|
| (a, b) | optical | HST, Subaru | NASA, ESA, STScI, R. Gendler and the Subaru Telescope (NAOJ) | |
| (c) | 115 GHz | PdBI | 1.4″ | Schinnerer et al. (2006) |
| (d) | 230 GHz | PdBI | 0.4″ | Schinnerer et al. (2006) |
| (e) | 3 GHz | VLA | 2.0″ | SFRS, Murphy et al. (2018), Linden et al. (2020) |
| (f) | 15 GHz | VLA | 2.1″ | SFRS, Murphy et al. (2018), Linden et al. (2020) |
| (g) | 33 GHz | VLA | 2.1″ | SFRS, Murphy et al. (2018), Linden et al. (2020) |
| (h) | 70 μm | Herschel/PACS | 5.5″ | KINGFISH, Kennicutt et al. (2011) |
| (i) | 24 μm | Spitzer/MIPS | 5.7″ | SINGS, Kennicutt et al. (2003) |
| (j) | 8 μm | Spitzer/IRAC | 2.0″ | SINGS, Kennicutt et al. (2003) |
| (k) | Paβ | HST | 2.0″ | Kessler et al. (2020) |
| (l) | Hα | 3.5-m WIYN telescope | 2.0″ | Long et al. (2019), Kessler et al. (2020) |
| (m) | X-ray | Chandra | ObsIDs 1054 and 13435, Holt et al. (2003) |
Notes: To overlay the contours of CO data on the optical images, we used http://nova.astrometry.net/
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