Table 1
Photometrie points for HD 121617.
| Filter | Flux | Flux corr. | Error | λeff | Ref. |
|---|---|---|---|---|---|
| – | (mJy) | (mJy) | (mJy) | (μm) | – |
| Tycho Β | 4372.0 | 5166.1 | 64.79 | 0.428 | 1 |
| Gaia Gbp | 3993.0 | 4577.1 | 37.59 | 0.504 | 2 |
| Tycho V | 4499.0 | 5111.1 | 48.14 | 0.534 | 1 |
| Gaia G | 3957.0 | 4440.2 | 36.39 | 0.586 | 2 |
| Gaia Grp | 3236.0 | 3506.8 | 30.53 | 0.769 | 2 |
| 2MASS J | 2067.0 | 2143.2 | 58.18 | 1.235 | 3 |
| 2MASS H | 1400.0 | 1431.8 | 60.48 | 1.662 | 3 |
| 2MASS K s | 883.0 | 896.1 | 15.97 | 2.159 | 3 |
| WISE W1 | 409.0 | 411.8 | 14.73 | 3.35 | 4 |
| WISE W2 | 240.0 | 241.0 | 7.56 | 4.60 | 4 |
| WISE W3 | 72.2 | 72.3 | 3.14 | 11.56 | 4 |
| WISE W4 | 567.0 | 567.2 | 31.28 | 22.09 | 4 |
| PACS 100 | 961.8 | 961.8 | 24.25 | 97.90 | 5 |
| PACS 160 | 415.4 | 415.4 | 17.17 | 153.95 | 5 |
| ALMA | 1.86 | 1.86 | 0.29 | 1330.0 | 6 |
Notes. The effective wavelengths were taken from the Spanish Virtual Observatory Filter Profile Service (http://svo2.cab.inta-csic.es/theory/fps/) (Rodrigo et al. 2012; Rodrigo & Solano 2020). The “Flux corr.” column corresponds to the flux corrected to the extinction described in Sect. 3.2.
References. (1) Høg et al. (2000), (2) Gaia Collaboration (2018), (3) Cutri et al. (2003), (4) Wright et al. (2010), (5) this work, and (6) Moór et al. (2017).
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