discov_num | notes | refcode |
KOI2790 | This system hosts a 0.9 Rearth planet candidate with a 14.0 day period | |
(Burke et al. 2014). The approximate increase to the planet radius is | KOI2014a | |
17% assuming that all of the light from the companion is captured in | ||
the Kepler aperture and that the planet orbits the target star. | ||
KOI2790 does not exhibit a significant source offset during transit. | Dre2014 |
refcode | metd | author | reference |
Dre2014 | A j | Dressing, C.D., Adams, E.R., Dupree, A.K., Kulesa, C., & McCarthy, D. | 2014AJ....148...78D |
Dre2014 | AJ 148, 78, 2014 (additional info from Furlan et al. 2017) | 2017AJ....153...71F | |
KOI2014a | not - | Burke, C.J., Bryson, S.T., Mullally, F., et al. | 2014ApJS..210...19B |
KOI2014a | ApJS 210, 19, 2014 (see Dressing et al. 2014) | 2014AJ....148...78D |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
19586+4051 | KOI2790 | AE | 2012 | 1 | 63 | 8.4 | 13.38 | 20.20 | N R | 195838.30+405037.8 | |
19586+4051 | KOI2790 | AE | 2013 | 1 | 63 | 8.4 | 13.38 | 20.20 | R | 195838.30+405037.8 |