Table 1
Photometric fluxes for SED.
| Photometric band | λeff (μm) | Fν (Jy) | Reference |
|
|
|||
| JOHNSON U | 0.36 | 0.050 ± 0.005 | 1 |
| TYCHO2 BT | 0.42 | 0.063 ± 0.005 | 2, 3 |
| JOHNSON B | 0.44 | 0.082 ± 0.005 | 1, 4, 5 |
| HIPPARCOS HP | 0.52 | 0.140 ± 0.005 | 2 |
| TYCHO2 VT | 0.53 | 0.116 ± 0.008 | 2, 3 |
| JOHNSON V | 0.55 | 0.155 ± 0.009 | 1, 4, 5 |
| DENIS I | 0.79 | 0.428 ± 0.008 | 6 |
| DENIS J | 1.23 | 0.87 ± 0.04 | 6 |
| 2MASS J | 1.24 | 0.81 ± 0.02 | 7 |
| 2MASS H | 1.65 | 0.99 ± 0.04 | 7 |
| DENIS KS | 2.16 | 0.87 ± 0.06 | 6 |
| 2MASS KS | 2.16 | 0.81 ± 0.02 | 7 |
| WISE W1 | 3.35 | 0.44 ± 0.01 | 8 |
| IRAC 3.6 | 3.54 | 0.39 ± 0.01 | 9 |
| CASPIR L | 3.58 | 0.39 ± 0.02 | 10 |
| IRAC 4.5 | 4.48 | 0.267 ± 0.004 | 9 |
| WISE W2 | 4.60 | 0.283 ± 0.005 | 8 |
| IRAC 5.8 | 5.70 | 0.197 ± 0.004 | 9 |
| IRAC 8.0 | 7.78 | 0.256 ± 0.002 | 9 |
| AKARI S9W | 8.85 | 0.451 ± 0.009 | 11 |
| IRAS F12 | 11.04 | 0.70 ± 0.06 | 12 |
| WISE W3 | 11.55 | 0.445 ± 0.006 | 8 |
| KECK 11.7 | 11.70 | 0.72 ± 0.04 | 13 |
| KECK 17.9 | 17.90 | 1.45 ± 0.08 | 13 |
| AKARI L18W | 18.92 | 1.45 ± 0.04 | 11 |
| WISE W4 | 22.08 | 2.05 ± 0.03 | 8 |
| IRAS F25 | 23.07 | 2.4 ± 0.2 | 12 |
| MIPS 24 | 24.37 | 2.3 ± 0.2 | 14 |
| IRAS F60 | 58.19 | 3.9 ± 0.4 | 12 |
| MIPS 70 | 69.99 | 3.6 ± 0.7 | 14 |
| PACS B | 70.39 | 3.9 ± 0.2 | 15 |
| IRAS F100 | 99.52 | 5.0 ± 0.5 | 12 |
| PACS R | 160.2 | 7.4 ± 0.7 | 15 |
| MIPS 160 | 161.6 | 6.6 ± 1.3 | 14 |
| SHARC II | 350.0 | 6.1 ± 0.7 | 16 |
| SCUBA 450WB | 456.4 | 4.3 ± 0.9 | 15 |
| JCMT UKT14 | 800.0 | 1.45 ± 0.03 | 17 |
| SCUBA 850WB | 858.9 | 1.4 ± 0.1 | 15 |
| SMA CO3-2 | 867.0 | 1.46 ± 0.04 | 18 |
| JCMT UKT14 | 1100 | 0.87 ± 0.05 | 17 |
| SMA CO2-1 | 1300 | 0.57 ± 0.02 | 18 |
| ATCA 3.4 | 3400 | 0.041 ± 0.009 | 19 |
| VLA 7 | 7000 | 0.008 ± 0.001 | 20 |
Reference. (1) Mermilliod (2006); (2) Perryman & ESA (1997); (3) Høg et al. (2000); (4) Kharchenko (2001); (5) Anderson & Francis (2012); (6) DENIS Consortium (2005); (7) Cutri et al. (2003); (8) Cutri et al. (2012); (9) Hartmann et al. (2005); (10) Calvet et al. (2002); (11) Ishihara et al. (2010); (12) Helou & Walker (1988); (13) Weinberger et al. (2002); (14) Low et al. (2005); (15) Thi et al. (2010); (16) Andrews et al. (2012); (17) Weintraub et al. (1989); (18) Qi et al. (2004); (19) Wilner et al. (2003); (20) Wilner et al. (2000).
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