discov_num | notes | refcode |
KOI1677 | KOI1677 hosts a 2.2 Rearth planet candidate with a 52.1 day orbit and | |
a 0.8 Rearth candidate with a 8.5 day orbit (Batalha et al. 2013). | KOI2013a | |
Assuming that all of the flux from the target star and the companion | ||
is captured in the Kepler aperture and that the planet orbits the | ||
target star, the planet radius estimate should be increased by roughly | ||
2% to account for the contamination from the nearby star. | 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 | |
KOI2013a | not - | Batalha, N.M., Rowe, J.F., Bryson, S.T., et al. | 2013ApJS..204...24B |
KOI2013a | ApJS 204, 24, 2013 (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 |
19187+4042 | KOI1677 | AB | 2012 | 2 | 161 | 0.6 | 14.28 | 17.60 | N R | 191843.04+404201.6 | |
19187+4042 | KOI1677 | AB | 2013 | 1 | 161 | 0.6 | 14.28 | 17.60 | R | 191843.04+404201.6 |