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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)

Notes. Given the adopted reference frame for the radial velocity the priors for c are set as .

(†)

In these cases the value for ecosω was derived from the phase shift determined by the authors and the inclination value from exoplanet.org.

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