discov_num |
notes |
refcode |
KOI 266 |
This system contains a 1.6 Rearth planet candidate with a 25.3 day |
|
|
period and a second 1.8 Rearth planet candidate with a 47.7 day period |
|
|
(Burke et al. 2014). It was classified by Slawson et al. (2011) as a |
KOI2014a |
|
detached eclipsing binary with a period of 25.3 days, suggesting that |
KOI2011a |
|
the 1.6 Rearth planet candidate with the same period might not |
|
|
actually be a planet. Instead, the observed decrease in flux every |
|
|
25.3 days might be an eclipsing binary diluted by the light of a |
|
|
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 |
KOI2011a |
not - |
Slawson, R.W., Prsa, A., Welsh, W.F., et al. |
2011AJ....142..160S |
KOI2011a |
|
AJ 142, 160, 2011 (see Dressing et al. 2014) |
2014AJ....148...78D |
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 |