Table 2
Orbital/physical parameters of WASP-3b estimated from individual data (sub-)sets.
| Reference paper | Nt | Telescope | ID | Band | Σr | kr | i | u1 | u1,th |
|
|
|||||||||
| Gibson et al. (2008) | 1 | LT-2.0 m | G1 | (R + V) |
|
|
|
|
0.28 |
| Tripathi et al. (2010) | 2 | FLWO-1.2 m | T5-6 | Sloan g |
|
|
|
|
0.42 |
| Tripathi et al. (2010) | 2 | FLWO-1.2 m | T1,T3 | Sloan i |
|
|
|
|
0.18 |
| Tripathi et al. (2010) | 1 | UH-2.2 m | T4 | Sloan z |
|
|
|
|
0.14 |
| Maciejewski et al. (2010) | 3 | Rohzen-0.6 m | M1-3 | R |
|
|
|
|
0.24 |
| Maciejewski et al. (2010) | 3 | Jena-0.9 m | M4-6 | R |
|
|
|
|
0.24 |
| Christiansen et al. (2011) | 6 | HRI-EPOXI | C1-4,C7-8 | clear |
|
|
|
|
0.28 |
| Littlefield (2011) | 3 | SC-11” | L1-3 | clear |
|
|
|
|
0.28 |
| this work | 4 | IAC80 | N1-2,N4-5 | R |
|
|
|
|
0.24 |
| ⟨ weighted mean ⟩ 1 | – | – | – | – |
|
|
|
– | – |
| ⟨ weighted mean ⟩ 2 | – | – | – | – |
|
|
|
– | – |
Notes. The columns give the reference paper, the number of light curves fitted, the telescope, the ID code of the transits, the filter employed, the fitted sum of the fractional radii (Σr = Rp/a + R ⋆ /a), the fitted ratio of the fractional radii (kr = Rp/R ⋆ ), the fitted inclination i, the fitted linear limb darkening (LD) coefficient u1, and the theoretical linear LD coefficient u1, th interpolated from the Claret (2000, 2004) tables. The quoted error bars are derived from the JKTEBOP RP algorithm. The last two rows show the weighted means of all previous individual estimates before and after discarding the data points T1,T3 (see text for details).
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