| discov_num |
notes |
refcode |
| KOI2754 |
This system hosts a 0.7 Rearth planet candidate with a 1.3 day period |
|
|
(Burke et al. 2014). Our ARIES observations revealed a companion 2.11 |
KOI2014a |
|
J mags and 1.65 Ks mags fainter than KOI2754 at a 0".763 separation. |
|
|
The predicted Kp mag of the companion star is Kp = 15.3 (dKp = 3.0) |
|
|
if the star is a dwarf and Kp = 15.2 (dKp = 2.9) if the star is a |
|
|
giant. The companion star was also detected in the WIYN speckle |
|
|
imaging acquired with DSSI. The companion is 3.12 mag. fainter than |
|
|
KOI2754 at 692 nm and 2.56 mags fainter at 880 nm. Assuming that the |
|
|
planet orbits the target star and that all of the light from the |
|
|
companion is captured in the Kepler aperture, then the planet radius |
|
|
should be increased by 3% to account for dilution. KOI2754 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 |
