Table A.5
Photometric data used in this study for σ Lib.
| σ Lib | |||
| λ | λ F λ | error λFλ | ref. |
| [μm] | [Wm-2] | [Wm-2] | |
|
|
|||
| 3.46 × 10-1 | 1.62 × 10-11 | 5.96 × 10-13 | 4 |
| 3.60 × 10-1 | 2.82 × 10-11 | − | 6 |
| 3.60 × 10-1 | 2.62 × 10-11 | − | 1 |
| 4.01 × 10-1 | 9.69 × 10-11 | 3.57 × 10-12 | 4 |
| 4.23 × 10-1 | 1.98 × 10-10 | 6.70 × 10-12 | 4 |
| 4.40 × 10-1 | 3.08 × 10-10 | − | 1 |
| 4.40 × 10-1 | 3.28 × 10-10 | − | 6 |
| 4.48 × 10-1 | 3.24 × 10-10 | 1.19 × 10-11 | 4 |
| 5.39 × 10-1 | 9.09 × 10-10 | 3.35 × 10-11 | 4 |
| 5.49 × 10-1 | 9.77 × 10-10 | 2.97 × 10-11 | 4 |
| 5.50 × 10-1 | 1.02 × 10-9 | − | 1 |
| 5.50 × 10-1 | 1.08 × 10-9 | − | 6 |
| 5.81 × 10-1 | 1.16 × 10-9 | 4.26 × 10-11 | 4 |
| 7.00 × 10-1 | 2.60 × 10-9 | − | 1 |
| 7.00 × 10-1 | 2.96 × 10-9 | − | 6 |
| 9.00 × 10-1 | 5.35 × 10-9 | − | 1 |
| 9.00 × 10-1 | 5.98 × 10-9 | − | 6 |
| 1.24 | 5.19 × 10-9 | 7.84 × 10-10 | 12 |
| 1.25 | 5.65 × 10-9 | − | 6 |
| 1.25 | 5.20 × 10-9 | 1.40 × 10-10 | 7 |
| 1.66 | 5.70 × 10-9 | 9.13 × 10-10 | 12 |
| 2.16 | 3.35 × 10-9 | 6.12 × 10-10 | 12 |
| 2.20 | 3.21 × 10-9 | 4.88 × 10-11 | 6 |
| 2.20 | 3.09 × 10-9 | 4.88 × 10-11 | 7 |
| 3.40 | 1.18 × 10-9 | − | 1 |
| 3.50 | 1.00 × 10-9 | 2.52 × 10-11 | 7 |
| 3.50 | 9.46 × 10-10 | 2.52 × 10-11 | 7 |
| 5.00 | 3.23 × 10-10 | − | 1 |
| 5.00 | 3.60 × 10-10 | − | 6 |
| 1.02 × 101 | 3.51 × 10-11 | − | 1 |
| 1.02 × 101 | 4.42 × 10-11 | − | 6 |
| 1.20 × 101 | 3.55 × 10-11 | 7.10 × 10-12 | 3 |
| 2.50 × 101 | 3.69 × 10-12 | 7.39 × 10-13 | 3 |
| 6.00 × 101 | 3.00 × 10-13 | 6.00 × 10-14 | 3 |
| 1.00 × 102 | 6.84 × 10-14 | 1.37 × 10-14 | 3 |
| 1.20 × 103 | 3.02 × 10-17 | 6.75 × 10-18 | 10 |
| 3.57 × 104 | <4.54 × 10-19 | − | 5 |
| 6.14 × 104 | <1.03 × 10-20 | − | 5 |
References. (1) UBVRIJKLMNH Photoelectric Catalogue (Morel & Magnenat 1978). (2) Selby et al. (1988). (3) IRAS catalogue of Point Sources, Version 2.0. (4) Observations in the Geneva Photometric System 4 (Rufener 1989). (5) Radio continuum emission from stars (Wendker 1995). (6) Stellar Photometry in Johnson’s 11-color system (Ducati 2002). (7) Color corrected data from COBE DIRBE Point Source Catalog (Smith et al. 2004). (8) Cohen et al. (2005). (9) Dehaes et al. (2007). (10) IRAM observations (this article). (11) VLA observations (this article). (12) 2MASS All-Sky Catalog of Point Sources (Skrutskie et al. 2006). (13) CSO observations (this article). (14) Ground-based and KAO data from M. Cohen et al. for the ISO CWW absolute calibration programme.
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