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Table A.3
Adopted ecosω values to set the priors on the c parameter for the 20 planets with detected secondary eclipse.
Planet | ecosω | Reference |
|
||
corot-1b | 0.0020 ± 0.0029 | Gillon et al. (2009) |
<0.002 | Deming et al. (2011) | |
<0.014 | Alonso et al. (2009) | |
–0.0025 ± 0.0010 | † Parviainen et al. (2013) | |
corot-15b | –0.00249 ± 0.0005 | † Parviainen et al. (2013) |
corot-18b | –0.0154 ± 0.001 | † Parviainen et al. (2013) |
corot-2b | 0.0005 ± 0.0010 | † Parviainen et al. (2013) |
–0.0030 ± 0.0004 | Deming et al. (2011) | |
–0.00291 ± 0.00063 | Gillon et al. (2010) | |
–0.0025 ± 0.0015 | Snellen et al. (2010) | |
hat-p-23b | –0.0011 ± 0.0065 | O’Rourke et al. (2014) |
ogle-tr-56b | –0.00147 ± 0.0049 | Sing & López-Morales (2009) |
tres-3b | <0.0019 | Fressin et al. (2010) |
0.0029 ± 0.0022 | Croll et al. (2010) | |
–0.0066 ± 0.0021 | de Mooij & Snellen (2009) | |
wasp-10b | –0.0552 ± 0.0007 | Kammer et al. (2015) |
–0.0044 ± 0.0004 | Cruz et al. (2015) | |
wasp-12b | 0.000097 ± 0.000401 | † Croll et al. (2010) |
0.0005 ± 0.0010 | † Föhring et al. (2013) | |
0.0014 ± 0.0007 | Campo et al. (2011) | |
0.0050 ± 0.0037 | † López-Morales et al. (2010) | |
wasp-18b | 0.012 ± 0.008 | Zhou et al. (2015) |
–0.0003 ± 0.0002 | Nymeyer et al. (2011) | |
wasp-19b | –0.0056 ± 0.0070 | Zhou et al. (2014) |
–0.0049 ± 0.0023 | Burton et al. (2012) | |
wasp-2b | –0.001 ± 0.001 | Zhou et al. (2015) |
–0.0013 ± 0.0009 | Wheatley et al. (2010) | |
wasp-36b | 0.004 ± 0.006 | Zhou et al. (2015) |
wasp-4b | 0.00030 ± 0.00086 | Beerer et al. (2011) |
-0.001 ± 0.003 | Zhou et al. (2015) | |
wasp-43b | -0.0062 ± 0.0024 | Zhou et al. (2014) |
wasp-46b | 0.004 ± 0.002 | Zhou et al. (2015) |
wasp-5b | 0.008 ± 0.002 | Zhou et al. (2015) |
0.0025 ± 0.0012 | Baskin et al. (2013) | |
kepler-17b | 0.0 < 0.011 | Desert et al. (2011) |
qatar-1b | –0.0123 ± 0.0252 | Cruz et al. (2016) |
hat-p-20b | 0.0132 ± 0.0006 | Deming et al. (2015) |
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