Table 4.
Multi-band integrated photometry of M 99 computed with HIP.
| Instrument | Luminosity | Flux | RMS |
|---|---|---|---|
| [107 L⊙] | [Jy] | [mJy] | |
| IRAC 3.6 μm | 370 | 0.68 ± 0.07 | 2 |
| IRAC 4.5 μm | 200 | 0.47 ± 0.05 | 1.4 |
| IRAC 5.2 μm | 435 | 1.3 ± 0.1 | 4 |
| IRAC 8 μm | 950 | 3.9 ± 0.4 | 3 |
| MIPS 24 μm | 340 | 4.2 ± 0.2 | 6 |
| PACS 70 μm | 1625 | 59 ± 3 | 140 |
| PACS 100 μm | 2160 | 112 ± 6 | 150 |
| PACS 160 μm | 1530 | 126 ± 7 | 220 |
| SPIRE 250 μm | 475 | 61 ± 4 | 204 |
| SPIRE 350 μm | 137 | 25 ± 2 | 100 |
| SPIRE 500 μm | 32 | 8.3 ± 0.5 | 55 |
| NIKA2 1.15 mm | 0.99 | 0.59 ± 0.05 | 30 |
| HFI4 1.38 mm | 0.49 | 0.35 ± 0.07 | 68 |
| NIKA2 2 mm | 0.089 | 0.09 ± 0.01 | 9 |
| X-VLA+Eff. 3 cm | 0.0056 | 0.087 ± 0.004 | 0.04 |
| C-VLA+Eff. 6 cm | 0.0048 | 0.148 ± 0.007 | 0.3 |
| L-VLA 20 cm | 0.004 | 0.41 ± 0.01 | 0.02 |
Notes. NIKA2 1.15 and Planck/HFI4 integrated fluxes are CO-subtracted (see Appendix C.6). The NIKA2 RMS includes the scatter driven by large-scale filtering (see Appendix A). Prior to aperture photometry, the sky emission was subtracted from all images. Monochromatic luminosities (i.e. ν Lν) listed in the second column were computed at d = 14.4 Mpc (Table 1).
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