(Q28503991)

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

unconfirmed exoplanet

2 references

SIMBAD

Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)

catalog code

Kepler-303c

catalog

Kepler Confirmed Names

3 references

Kepler object of interest

KOI-1515.02

catalog

3 references

Kepler object of interest

KOI-1515c

catalog

2 references

imported from Wikimedia project

TIC 164460208c

1 reference

discoverer or inventor

Kepler Space Telescope

1 reference

Spanish Wikipedia

time of discovery or invention

March 2014

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

2 references

inferred from equatorial coordinates

constellation

Lyra

1 reference

based on heuristic

parent astronomical body

3 references

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

object stated in reference as

Kepler-303

object stated in reference as

2MASS J18523251+4339253

orbital period

7.06117359±0.00001286 day

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

7.06118403±0.00000237 day

1 reference

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

7.0611731694±0.0000120718 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

7.06117534±0.0000138 day

1 reference

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

7.061149±0.000019 day

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

semi-major axis of an orbit

0.057 astronomical unit

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

declination component of proper motion

parallax

4.739±0.0211 milliarcsecond

2 references

−76.789±0.044 milliarcsecond per year

2 references

right ascension component of proper motion

2.436±0.044 milliarcsecond per year

2 references

1.16±0.06 Earth radius

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

1.16±0.17 Earth radius

1 reference

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

1.489±0.176 Earth radius

1 reference

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

1.645±0.151 Earth radius

1 reference

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

0.102±0.008 Jupiter radius

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

diameter

21,000±1,930 kilometre

1 reference

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

3 references