Has the Kepler data been examined for light curves due to phase changes of non-transitting hot Jupiters and other? I found this article http://www.epj-conferences.org/articles/epjconf/pdf/2011/01/epjconf_ohp2010_03005.pdf from 2011 announcing that two dozen secondary eclipses of "hot Jupters" have been seen in Kepler data. I even think I have seen a light curve showing phase changes of a transiting planet. This makes me think that there should be evidence in the Kepler data for non-transiting planets since the amplitude of the light curve due to planetary phase changes shouldn't be much different from that of a secondary eclipse as long as there is a fairly high inclination (say over 60 degrees).

Is anybody aware of such an examination of the data?
Here's an example paper looking for phase curves of non-transiting planets in the Kepler data: Millholland &amp; Laughlin (2017) "Supervised Learning Detection of Sixty Non-transiting Hot Jupiter Candidates".

The candidates themselves can be found on this webpage.

Unfortunately I'm not aware of any RV followup on them to determine which of these candidates are actually planets.