Table 3
Measured secondary eclipse depths and brightness temperatures from Eq. (4) as a function of wavelength for WASP-19b.
| Wvl. range (μm) | Depth (ppm) | Tbright (K) | References |
|
|
|||
| 0.42–0.95 | 390 ± 190 |
|
1 |
| 0.81–1.01a | 880 ± 190 |
|
2 |
| 1.525–1.775 | 2760 ± 440 |
|
3 |
| 1.965–2.215 | 3660 ± 670 |
|
4, 5 |
| 3.225–3.975 | 4830 ± 250 |
|
5 |
| 4.0–5.0 | 5720 ± 300 |
|
5 |
| 5.1–6.5 | 6500 ± 1100 |
|
5 |
| 6.55–9.45 | 7300 ± 1200 |
|
5 |
Notes.
Recent results by Lendl et al. (2013) indicate a lower value of the depth of the secondary eclipse than measured by Burton et al. (2012). This lower value is consistent with the ASTEP measurement and theoretical spectra.
Reference. (1) This work (see Fig. 1); (2) Burton et al. (2012); (3) Anderson et al. (2010); (4) Gibson et al. (2010); (5) Anderson et al. (2011).
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