“…The data were compiled using exoplanets.org (Wright et al 2011) and the following publications: HAT-P-2: Bakos et al (2007), van Leeuwen (2007), Pál et al (2010), P rot from v sin i, T eq varies due to eccentricity ( (Salz et al 2015b); HAT-P-20: Bakos et al (2011), P rot from (Salz et al 2015b); WASP-8: Queloz et al (2010), Cubillos et al (2012), P rot from (Salz et al 2015b); WASP-80: Triaud et al (2013), P rot from v sin i; WASP-43: Hellier et al (2011);WASP-18: Hellier et al (2009), Pillitteri et al (2014, P rot from v sin i; HD 209458: Charbonneau et al (2000), Henry et al (2000), Torres et al (2008), Silva-Valio (2008), dayside brightness temperature from Spitzer observation (Crossfield et al 2012);HD 189733: Bouchy et al (2005), Henry & Winn (2008), Southworth (2010), dayside brightness temperature from Spitzer observation (Knutson et al 2007);GJ 1214), Berta et al (2011), Narita et al (2013; GJ 3470: Bonfils et al (2012), Biddle et al (2014);GJ 436: Butler et al (2004), Knutson et al (2011);55 Cnc: Butler et al (1997), McArthur et al (2004, Gray et al (2003), Fischer et al (2008); HAT-P-11: Bakos et al (2010);HD 149026: Sato et al (2005), P rot from v sin i, dayside brightness temperature from Spitzer observation (Knutson et al 2009);HD 97658: Howard et al (2011…”