Table D.1.
(Available in full online) Mid-infrared photometry (flux densities in mJy) for the HRS sample.
| HRS | Desig- | Morph. | VCC | log10 | integrated | central | integrated | central | class | DHI | WHAN | ||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ID | nation | ID | M* | W1 | W1 | W2 | W2 | W3 | W3 | W4 | W4 | W1 | W1 | W2 | W2 | W3 | W3 | W4 | W4 | class | |||||
| (M⊙) | ± | ± | ± | ± | ± | ± | ± | ± | |||||||||||||||||
| 1 | CGCG123-035 | Pec | ⋯ | 8.72 | 8.66 | 2.20 | 5.06 | 1.31 | 20.25 | 5.40 | 20.14 | 6.92 | 8.73 | 2.10 | 5.22 | 1.26 | 20.46 | 5.12 | 22.40 | 6.11 | 1379 | 65 | SFG | ⋯ | HII |
| 2 | UGC05588 | S | ⋯ | 8.77 | 21.79 | 1.12 | 13.87 | 0.68 | 68.25 | 4.26 | 89.77 | 7.44 | 21.41 | 0.98 | 13.56 | 0.64 | 67.39 | 6.66 | 91.82 | 9.41 | 1429 | 68 | SFG | 0.07 | HII |
| 3 | NGC3226 | E2 | ⋯ | 10.21 | 197.61 | 22.36 | 108.59 | 13.65 | 66.39 | 17.47 | 86.12 | 35.48 | 180.09 | 11.31 | 98.08 | 6.71 | 58.68 | 11.62 | 61.05 | 26.54 | 3374 | 151 | Retired | 0.38 | wAGN |
| 4 | NGC3227 | SAB | ⋯ | 10.26 | 371.39 | 39.82 | 273.44 | 24.74 | 829.77 | 66.92 | 1961.59 | 116.55 | 304.65 | 48.34 | 232.62 | 30.54 | 776.36 | 107.38 | 1891.72 | 156.38 | 7745 | 355 | Sy2 | 0.57 | sAGN |
| 5 | IC0610 | Sc | ⋯ | 9.62 | 48.37 | 8.62 | 31.25 | 3.05 | 82.53 | 12.58 | 117.55 | 17.06 | 47.42 | 11.57 | 28.89 | 7.07 | 81.79 | 19.60 | 118.27 | 27.19 | 3086 | 144 | LINER | 0.66 | HII |
| 6 | NGC3245A | SBb | ⋯ | 8.94 | 10.24 | 1.80 | 5.95 | 1.07 | 8.31 | 1.55 | 10.87 | 4.80 | 9.91 | 1.93 | 5.69 | 1.14 | 8.48 | 1.58 | 9.69 | 5.04 | 3306 | 154 | Retired | 0.62 | HII |
| 7 | NGC3245 | SA0 | ⋯ | 10.29 | 247.16 | 21.92 | 136.24 | 11.90 | 78.25 | 4.65 | 195.09 | 14.76 | 235.28 | 35.40 | 128.66 | 19.28 | 77.51 | 6.42 | 205.24 | 13.17 | 14463 | 700 | Retired | 1.02 | wAGN |
| 8 | NGC3254 | SAbc | ⋯ | 9.88 | 97.42 | 17.95 | 57.8 | 10.54 | 100.10 | 24.33 | 102.8 | 28.28 | 94.63 | 16.93 | 54.42 | 10.15 | 97.86 | 26.32 | 101.74 | 30.74 | 14656 | 694 | Retired | 0.07 | wAGN |
| 9 | NGC3277 | SAab | ⋯ | 10.08 | 111.14 | 9.95 | 60.67 | 5.17 | 69.88 | 4.56 | 57.97 | 12.60 | 106.42 | 10.71 | 57.74 | 5.39 | 68.54 | 6.22 | 69.48 | 15.46 | 17245 | 860 | Retired | 0.49 | wAGN |
| 10 | UGC05738 | S | ⋯ | 8.71 | 10.18 | 2.48 | 6.21 | 1.52 | 29.34 | 7.34 | 43.85 | 10.04 | 10.12 | 2.48 | 6.31 | 1.52 | 29.22 | 7.30 | 45.42 | 9.92 | 2103 | 101 | SFG | 0.12 | HII |
Notes. This photometry is obtained from the WISE All-Sky Atlas Image Inventory Table (W1-W4 bands) using the procedures detailed in Section 3.1. Uncertainties (±) represent the standard deviation within each galaxy dataset. The ’integrated’ and ’central’ columns refer to integrated and central aperture fluxes, respectively (see Section 3.1.4), and number of image pixels considered. Central apertures typically comprise < 5 % of the pixel integrated apertures. Excitation classes (’class’) are based on central aperture mIRdds (Section 4.1). Stellar masses (M*) are obtained as described in Section 2.3.2, while morphological types (’Morph.’) are taken from (1). Virgo cluster members (VCMs) are identified via VCC IDs (Section 2.1). H I deficiency parameters (DHI) are taken from (2), and WHAN excitation classes from (3) (including passive = PAS and post-starburst = PSB types, see Appendix C).
Reference. (1) Boselli et al. (2010); (2) Boselli et al. (2014a); (3) Gavazzi et al. (2018).
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