We present a comprehensive study of phase curves and secondary eclipses in the Kepler data set using all data from 16 quarters that were available in 2013-2014 .
Our sample consists of 20 confirmed planets with R _ { p } > 4 R _ { e } , P < 10 d , V _ { mag } < 15 .
Here we derive their temperatures and albedos , with an eye towards constraining models for the formation and evolution of such planets .
Where there was overlap our results confirm parameters derived by previous studies , whereas we present new results for Kepler 1b-8b , 12b-15b , 17b , 40b , 41b , 43b , 44b , 76b , 77b , and 412b derived in a consistent manner .
We also present lightcurve analyses for Kepler 91b and Kepler 74b , which both show extra dimmings at times other than from the expected primary and secondary eclipses .
Corrected for thermal emission we find most of the massive planets from our sample to be low in albedo ( < 0.1 ) with a few having higher albedo ( > 0.1 ) .