Notes. Systems are sorted by increasing KIC number (first column). Second and third columns are the effective temperatures, and Kepler magnitudes from the KIC. The “Type” column indicates the type of binary systems: D for detached, SD for semi-detached, OC for over-contact, and ELL for ellipsoidal. The “Ecl” column indicates the number of eclipses that are visible per orbital period (0 for ELL systems, 1 or 2 for the others). Column 6 displays the orbital period P_orb expressed in days rounded at two digits. Columns 7–10 indicate the eclipse depth of the deepest eclipse (primary) expressed in percent, the orbital phase separation “sep” in between the secondary and the primary eclipse, the eclipse duration ratio W₂/W₁, and the sum of eclipse duration relative to orbital period (W₂ + W₁)/P_orb. The pulsator type “Puls type” is either δ-Sct for δ Scuti, γ Dor for γ Doradus, “Rossby”, “RG” for RG solar-like oscillator, “tidal”, SPB for slowly pulsating B-type stars, “WD” for white dwarf, or sdB for subdwarf B. The type “rot” stands for surface stellar “rotation” that may mimic stellar pulsations. The literature references are compacted (see below). “New PB” indicates a target identified both as a pulsator and a binary. Systems identified for the first time are marked with a “Y”. Notes are random relevant specific information regarding each system. “HB” stands for heartbeat, FP for false positive, KOI for Kepler object of interest, P_orb for orbital period, “Ecl.” for eclipse, “harm.” for harmonics, T₁ and T₂ for star 1 star 2 effective temperatures, T_eff refers to the published KIC effective temperature, “SB1” and “SB2” for single or double-lined spectroscopic binary. The label “P_orb = P_orb/2” means that the actual orbital period is half of what Villanova database reported.

References. AS14: Kahraman Aliçavuş et al. (2014), Ali17: Aliçavuş & Soydugan (2017), Arm14: Armstrong et al. (2014), Blj15: Balaji et al. (2015), Bal11: Balona et al. (2011), Bal13: Balona et al. (2013), Bal14: Balona (2014), Bal15: Balona (2015), Bal15b: Balona et al. (2015), Bck14: Beck et al. (2014), Bed11: Bedding et al. (2011), Bel19: Bell et al. (2019), Bog15: Bognár et al. (2015), Bow16: Bowman et al. (2016), Bie17: Biersteker & Schlichting (2017), Bor11: Borucki et al. (2011), Brk14: Borkovits et al. (2014), Brk16: Borkovits et al. (2016), Bra15: Bradley et al. (2015), Bro18: Brogaard et al. (2018), Cei17: Ceillier et al. (2017), Con14: Conroy et al. (2014), Cou11: Coughlin et al. (2011), Deb11: Debosscher et al. (2011), Deb13: Debosscher et al. (2013), Dem15: Demircan & Bulut (2015), Dim17: Dimitrov et al. (2017), DR12: Dodson-Robinson (2012), Don13: Dong et al. (2013), Fra13: Frandsen et al. (2013), Gau13: Gaulme et al. (2013), Gau14: Gaulme et al. (2014), Gau16: Gaulme et al. (2016), GG14: Gaulme & Guzik (2014), Gie15: Gies et al. (2015), Guo16: Guo et al. (2016), Guo17: Guo et al. (2017a), Guo17b: Guo et al. (2017b), Fai15: Faigler et al. (2015), Geo18: George et al. (2018), Hek10: Hekker et al. (2010), Ham13: Hambleton et al. (2013), Ham16: Hambleton et al. (2016), Ham18: Hambleton et al. (2018), Hel16: Hełminiak et al. (2016), Hel17: Hełminiak et al. (2017b), Hel17b: Hełminiak et al. (2017a), KN18: Katsova & Nizamov (2018), Kju16: Kjurkchieva et al. (2016), Kju16b: Kjurkchieva & Atanasova (2016), Kou18: Kouzuma (2018), Kur15: Kurtz et al. (2015b), Kus19: Kuszlewicz et al. (2019) Lee14: Lee et al. (2014), Lee15: Lee et al. (2015), Lee16a: Lee et al. (2016a), Lee16b: Lee et al. (2016b), Lee17: Lee et al. (2017), Leh13: Lehmann et al. (2013), LiB14: Lillo-Box et al. (2014), Lur17: Lurie et al. (2017), Lia17: Liakos (2017), Lia18: Liakos (2018), LN17: Liakos & Niarchos (2017), Mac14: Maceroni et al. (2014), MH18: Manuel & Hambleton (2018), Mas17: Masuda (2017), Mat17: Matson et al. (2017), McN12: McNamara et al. (2012), Moy17: Moya et al. (2017), Mur15: Murphy et al. (2015), Mur18: Murphy et al. (2018), Nie15: Niemczura et al. (2015), Nie17: Niemczura et al. (2017), Ozd17: Özdarcan & Dal (2017), Oro15: Orosz (2015), Pab12: Pablo et al. (2012), Ram14: Ramsay et al. (2014), Rap13: Rappaport et al. (2013), Rap15: Rappaport et al. (2015), Raw16: Rawls et al. (2016), Row10: Rowe et al. (2010), Row15: Rowe et al. (2015), Sow17: Sowicka et al. (2017), Sai18: Saio et al. (2018), Snd16: Sandquist et al. (2016), San16: Santerne et al. (2016), Shp16: Shporer et al. (2016), Smu15: Smullen & Kobulnicky (2015), Sou11: Southworth et al. (2011), Sou15: Southworth (2015), The18: Themeßl et al. (2018), Tho12: Thompson et al. (2012), TM16: Turner & Maynard (2016), Tur15: Turner & Holaday (2015), Tur19: Turner (2019), Uyt11: Uytterhoeven et al. (2011), Wel11: Welsh et al. (2011), Yak15: Yakut (2015), Zha17: Zhang et al. (2017a), Zha17b: Zhang et al. (2017b), ZXB17: Zhang et al. (2017c), Zho10: Zhou (2010), Zim17: Zimmerman et al. (2017)