Table 1
Parameters for Planck ERCSC-IIFSCz galaxies with SED fits.
| RA | Dec | FSS | dist | zspect | log(L) | log(L) | log(L) | log(L) | log(L) | log(L) | type | AV | log(M∗) | log(Mdust) |
| cirr | cirr | cirr | SB | Arp220 | Opt | M⊙ | M⊙ | |||||||
| ψ = 5 | ψ = 1 | ψ = 0.1 | ||||||||||||
|
|
||||||||||||||
| Template | ||||||||||||||
|
|
||||||||||||||
| 202.46930 | 47.19290 | F13277+4727 | 0.1 | 0.001544 | 10.05 | 9.49 | 9.60 | 10.35 | Sbc | 0.0 | 10.75 | 7.54 | ||
| M51 | ||||||||||||||
| 185.72728 | 15.82777 | F12203+1605 | 0.4 | 0.005240 | 10.53 | 10.19 | 9.98 | 11.22 | Sbc | 0.0 | 11.62 | 8.15 | ||
| M100 | ||||||||||||||
| 148.97540 | 69.68221 | F09517+6954 | 0.2 | 0.000677 | 9.19 | 10.41 | 9.95 | E | 0.0 | 10.54 | 7.18 | |||
| M82 | ||||||||||||||
| 233.74080 | 23.49795 | F15327+2340 | 0.4 | 0.01813 | 12.15 | 10.58 | E | 0.0 | 11.17 | 8.15 | ||||
| Arp220 | ||||||||||||||
|
|
||||||||||||||
| 16-band, z < 0.01 | ||||||||||||||
|
|
||||||||||||||
| 175.24310 | 11.47154 | F11383+1144 | 0.1 | 0.003312 | 9.70 | 9.69 | 9.24 | 10.00 | Sab | 0.0 | 10.57 | 7.58 | ||
| NGC 3810 | ||||||||||||||
| 143.03957 | 21.50516 | F09293+2143 | 0.2 | 0.001855 | 9.70 | 9.49 | 9.38 | 10.41 | Scd | 0.2 | 10.79 | 7.43 | ||
| NGC 2903 | ||||||||||||||
| 213.89354 | 36.22261 | F14134+3627 | 0.3 | 0.009591 | 10.19 | 9.60 | 10.70 | Sab | 0.65 | 11.27 | 8.44 | |||
| NGC 5529 | ||||||||||||||
| 181.50023 | 47.47356 | F12034+4745 | 0.3 | 0.001888 | 8.90 | 9.09 | 8.60 | 9.65 | Sab | 0.6 | 10.22 | 6.95 | ||
| NGC 4096 | ||||||||||||||
| 206.59677 | 43.86664 | F13443+4407 | 0.5 | 0.008036 | 9.90 | 9.99 | 10.60 | Scd | 0.4 | 11.04 | 7.86 | |||
| NGC 5297 | ||||||||||||||
| 184.95674 | 29.61180 | F12173+2953 | 0.7 | 0.003102 | 9.64 | 10.40 | Scd | 0.0 | 10.94 | 7.45 | ||||
| NGC 4274 | ||||||||||||||
| 218.18851 | 49.45234 | F14310+4940 | 0.4 | 0.007052 | 10.60 | 10.70 | Sab | 0.4 | 11.27 | 7.71 | ||||
| NGC 5676 | ||||||||||||||
| 178.20813 | 44.12143 | F11502+4423 | 0.5 | 0.002699 | 9.59 | 9.10 | 9.90 | Scd | 0.5 | 10.34 | 7.40 | |||
| NGC 3938 | ||||||||||||||
|
|
||||||||||||||
| Cold log(S857/S545) < 0.4 | ||||||||||||||
|
|
||||||||||||||
| 159.78535 | 41.69160 | F10361+4155 | 2.0 | 0.002228 | 8.52 | 8.10 | 7.50 | sb | 0.2 | 7.52 | 7.33 | |||
| 179.31494 | 49.28748 | F11547+4933 | 0.4 | 0.002592 | 8.79 | 8.70 | sb | 0.0 | 8.72 | 6.60 | ||||
| 218.19263 | 9.88910 | F14302+1006 | 0.6 | 0.004574 | 9.40 | 8.92 | 9.60 | Scd | 0.2 | 10.04 | 7.76 | |||
| 208.22507 | –1.12087 | F13503-0052 | 0.4 | 0.004623 | 9.64 | 9.70 | Scd | 0.5 | 10.14 | 7.45 | ||||
| 148.79717 | 9.27136 | F09521+0930 | 0.0 | 0.004854 | 8.92 | 9.40 | 9.60 | Scd | 0.0 | 10.04 | 7.73 | |||
| 219.79150 | 5.25526 | F14366+0534 | 0.4 | 0.005020 | 9.09 | 8.62 | 8.70 | 10.35 | Scd | 0.2 | 10.79 | 7.54 | ||
| 158.12950 | 65.03790 | F10290+6517 | 0.4 | 0.005624 | 9.40 | 8.62 | 9.80 | Scd | 0.2 | 10.24 | 7.48 | |||
| 210.53130 | 55.79348 | F14004+5603 | 1.4 | 0.006014 | 9.05 | 8.67 | 10.25 | Scd | 0.7 | 10.69 | 7.50 | |||
| 208.72266 | 41.30995 | F13527+4133 | 0.0 | 0.007255 | 9.51 | 8.40 | 9.96 | Scd | 0.2 | 10.40 | 6.76 | |||
| 205.57553 | 60.77630 | F13405+6101 | 0.3 | 0.007322 | 9.20 | 8.63 | 9.61 | Sbc | 0.5 | 10.01 | 7.58 | |||
| 228.37207 | 58.49204 | F15122+5841 | 1.0 | 0.008474 | 9.26 | 8.95 | 9.51 | Scd | 0.15 | 9.95 | 7.77 | |||
| 231.67357 | 40.55709 | F15248+4044 | 0.4 | 0.008743 | 9.70 | 9.43 | 9.41 | 10.16 | Scd | 0.7 | 10.60 | 8.31 | ||
| 226.95305 | 54.74415 | F15064+5456 | 0.7 | 0.01043 | 10.00 | 10.16 | Scd | 0.4 | 10.60 | 7.81 | ||||
| 126.57545 | 22.88144 | F08233+2303 | 1.3 | 0.01794 | 10.20 | 10.13 | 9.81 | Scd | 0.3 | 10.25 | 8.99 | |||
| 231.43570 | 52.44624 | F15243+5237 | 0.3 | 0.01948 | 10.19 | 9.81 | 10.44 | Sab | 0.2 | 11.01 | 8.64 | |||
| 237.68201 | 55.60954 | F15495+5545 | 0.2 | 0.03974 | 10.55 | 10.52 | 10.20 | 10.70 | Sab | 0.0 | 11.27 | 9.34 | ||
| 66.76954 | –49.12881 | F04257-4913 | 0.8 | 0.05828 | 10.62 | 11.55 | 10.85 | Sab | 0.0 | 11.42 | 9.43 | |||
Notes. Table columns are: ERCSC RA and Dec, IRAS FSC name, separation between ERCSC and IIFSCz position, spectroscopic redshift, luminosity in cirrus φ = 5, φ = 1 and φ = 0.1 components, luminosity in M82 and Arp220 starburst components, optical luminosity, optical SED type, extinction (additional to that inherent to the individual templates), stellar mass and dust mass. Total far-IR luminosity can be obtained by summing the various different components. Stellar mass and dust mass are calculated as in Rowan-Robinson et al. (2008), where the methods and uncertainties in the derived quantities are discussed in detail. Where the sources have a well known name this is given beneath the IRAS name. All luminosities are measured in solar luminosities.
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