Table 1.
Key properties of the PHANGS–MUSE sample of galaxies used in this work.
| Galaxy | D | log(M⋆) | log(SFR) | i | Copt. PSF | θbm | NH II | Notes |
|---|---|---|---|---|---|---|---|---|
| [Mpc] | [M⊙] | [M⊙ yr−1] | [deg] | [arcsec] | [pc] | |||
| IC 5332 | 9.0 | 9.67 | −0.39 | 26.9 | 0.87 | 38 | 545 | |
| NGC 0628 | 9.8 | 10.34 | 0.24 | 8.9 | 0.92 | 44 | 1712 | Grand-design spiral |
| NGC 1087 | 15.9 | 9.93 | 0.12 | 42.9 | 0.92 | 71 | 912 | |
| NGC 1300 | 19.0 | 10.62 | 0.07 | 31.8 | 0.89 | 82 | 944 | Nuclear ring |
| NGC 1365 | 19.6 | 10.99 | 1.23 | 55.4 | 1.16 | 109 | 550 | AGN, nuclear ring |
| NGC 1385 | 17.2 | 9.98 | 0.32 | 44.0 | 0.77 | 64 | 913 | |
| NGC 1433 | 18.6 | 10.87 | 0.05 | 28.6 | 0.91 | 82 | 851 | Nuclear ring |
| NGC 1512 | 18.8 | 10.71 | 0.11 | 42.5 | 1.25 | 114 | 477 | Nuclear ring |
| NGC 1566 | 17.7 | 10.78 | 0.66 | 29.5 | 0.80 | 69 | 1561 | AGN |
| NGC 1672 | 19.4 | 10.73 | 0.88 | 42.6 | 0.96 | 90 | 934 | AGN, nuclear ring |
| NGC 2835 | 12.2 | 10.00 | 0.09 | 41.3 | 1.15 | 68 | 732 | |
| NGC 3351 | 10.0 | 10.36 | 0.12 | 45.1 | 1.05 | 51 | 690 | Nuclear ring |
| NGC 3627 | 11.3 | 10.83 | 0.58 | 57.3 | 1.05 | 58 | 970 | AGN |
| NGC 4254 | 13.1 | 10.42 | 0.49 | 34.4 | 0.89 | 57 | 2022 | |
| NGC 4303 | 17.0 | 10.52 | 0.73 | 23.5 | 0.78 | 64 | 2043 | AGN, nuclear ring, NIRCam covers half |
| NGC 4321 | 15.2 | 10.75 | 0.55 | 38.5 | 1.16 | 86 | 1239 | Nuclear ring, NIRCam covers half |
| NGC 4535 | 15.8 | 10.53 | 0.33 | 44.7 | 0.71⋆ | 54 | 1097 | AGN |
| NGC 5068 | 5.2 | 9.40 | −0.56 | 35.7 | 1.04 | 26 | 1174 | |
| NGC 7496 | 18.7 | 10.00 | 0.35 | 35.9 | 0.89 | 81 | 535 | AGN |
Notes.
Distances are taken from the compilation of Anand et al. (2021), stellar mass and SFR are from Leroy et al. (2021b), inclinations from Lang et al. (2020) where available, otherwise from Leroy et al. (2021b), and PSF FWHM of the copt MUSE data are from Emsellem et al. (2022) (⋆ for this galaxy the copt FWHM is smaller than the F2100W PSF, so we used an ‘aggressive’ kernel to convolve the JWST data to a Gaussian PSF). θbm gives the size of the common resolution element with no inclination correction. NH II gives the number of H II regions from Groves et al. (2023) overlapping with the MIRI footprint, detected in F2100W, and meeting our other selection criteria (see text). The notes include information on which galaxies have partial coverage with NIRCam.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.