Table 3
Optical and infrared photometry of HIP 17439.
| λ | F obs | F pred | Inst./ | Ref. |
| [μm] | [mJy] | [mJy] | source | |
|
|
||||
| 0.349 | 682.9 ± 12.6 | ... | a | 1 |
| 0.411 | 2119.3 ± 39.0 | ... | a | 1 |
| 0.440 | 3057.8 ± 56.3 | ... | b | 2 |
| 0.466 | 4278.0 ± 78.8 | ... | a | 1 |
| 0.546 | 5924.3 ± 109.1 | ... | a | 1 |
| 0.550 | 5822.4 ± 107.3 | ... | b | 2 |
| 0.790 | 9430.6 ± 173.7 | ... | b | 2 |
| 1.235 | 10 416.0 ± 182.3 | ... | c | 3 |
| 1.662 | 9442.8 ± 139.2 | ... | c | 3 |
| 2.159 | 7085.9 ± 104.4 | ... | c | 3 |
| 3.4 | 3372.0 ± 242.5 | ... | d | 4 |
| 9.0 | 501.4 ± 7.9 | 503.1 | e | 5 |
| 11.5 | 314.4 ± 5.2 | 309.5 | d | 4 |
| 12.0 | 299.2 ± 17.9 | 287.8 | f | 6 |
| 17.0 | 154.7 ± 9.3 | 145.2 | g | 7 |
| 22.1 | 90.4 ± 2.0 | 86.4 | d | 4 |
| 24.0 | 67.8 ± 1.3 | 73.3 | g | 7 |
| 25.0 | 84.3 ± 13.5 | 67.6 | f | 6 |
| 32.0 | 53.1 ± 3.2 | 41.3 | g | 7 |
| 60.0 | 103.0 ± 24.7 | 11.7 | f | 6 |
| 70.0 | 99.1 ± 8.4 | 8.6 | g | 7 |
| 70.0 | 74.5 ± 3.8 | 8.6 | h | 7 |
| 100.0 | 91.3 ± 4.7 | 4.2 | h | 7 |
| 160.0 | 91.9 ± 4.9 | 1.6 | h | 7 |
| 250.0 | 56.3 ± 10.5 | 0.7 | i | 7 |
| 350.0 | 33.9 ± 8.9 | 0.3 | i | 7 |
| 500.0 | (13.5 ± 7.2) | 0.2 | i | 7 |
Notes. Instruments/sources are: (a) Stromgren ubvy; (b) from the Hipparcos catalog: Johnson B, V, and Cousins I; (c) 2MASS JHKs; (d) WISE; (e) AKARI; (f) IRAS; (g) Spitzer; (h) Herschel/PACS, (i) Herschel/SPIRE. Uncertainties are 1-σ and include contributions from both calibration and rms sky noise. Uncertainties on the predicted stellar photospheric fluxes are 1.5%. The SPIRE flux at 500 μm can be considered an upper limit of 21.6 mJy (3σ), while for the modeling we included it as the actual measurement on the marginal detection of the source and 1σ uncertainties for consistency with the other data.
Reference. (1) Hauck & Mermilliod (1998); (2) Perryman et al. (1997); (3) Skrutskie et al. (2006); (4) Cutri & et al. (2012); (5) Ishihara et al. (2010); (6) Moshir & et al. (1990); (7) This work.
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