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Table 1
Observed fluxes used for the SED fits for NGC 4370.
| Band | Flux (mJy) | Source |
|
|
||
| FUV | 0.0463 ± 0.0063 | a |
| NUV | 0.2166 ± 0.0059 | a |
| u | 6.1 ± 1.1 | b |
| g | 22.9 ± 1.8 | b |
| i | 62.3 ± 2.5 | b |
| z | 80.9 ± 3.2 | b |
| J | 107 ± 21 | c |
| H | 138 ± 21 | c |
| K | 121 ± 24 | c |
| WISE 1 | 73.8 ± 1.9 | d |
| WISE 2 | 39.8 ± 1.3 | d |
| WISE 3 | 64.8 ± 3.1 | d |
| WISE 4 | 56.4 ± 4.7 | d |
| MIPS 24 μm | 48.3 ± 2.1 | e |
| MIPS 70 μm | 1284 ± 132 | e |
| PACS 70 μm | 1348 ± 73 | f |
| PACS 100 μm | 3027 ± 172 | f |
| PACS 160 μm | 3647 ± 231 | f |
| MIPS 160 μm | 2880 ± 350 | e |
| SPIRE 250 μm | 1947 ± 53 | f |
| SPIRE 350 μm | 772 ± 38 | f |
| SPIRE 500 μm | 251 ± 19 | f |
Reference. (a) Cortese et al. (2012a); (b) NGVS, this work; (c) GoldMine (Gavazzi et al. 2003); (d) Agius et al. (2015); (e) Bendo et al. (2012); (f) HeViCS, this work.
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