| discov_num |
notes |
refcode |
| KOI2879 |
This system was reported to have a 1.4 Rearth planet with a 0.3 day |
|
|
period (Burke et al. 2014), but this signal has been found to be a |
KOI2014a |
|
false positive. Our ARIES observations revealed a companion 0.37 J |
|
|
mags and 0.27 Ks mags fainter than KOI 2879 at a distance of 0".423. |
|
|
Using the J-Ks to Kp-Ks color-color conversion from Howell et al. |
|
|
(2012), we predict that the Kp mag of the companion is Kp = 13.8 |
KOI2012a |
|
(dKp = 1.1) if the star is a dwarf or Kp = 13.9 (dKp = 1.2) if the |
|
|
star is a giant. If any additional planet candidates are detected |
|
|
around KOI2879, their radii will need to be increased by roughly 17% |
|
|
to account for the additional light in the aperture. |
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 |
| KOI2012a |
not - |
Howell, S.B., Rowe, J.F., Bryson, S.T., et al. |
2012ApJ...746..123H |
| KOI2012a |
|
ApJ 746, 123, 2012 (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 |
