(Q28855412)

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

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

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

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

unconfirmed exoplanet

2 references

SIMBAD

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

catalog code

Kepler-369c

catalog

Kepler Confirmed Names

3 references

SIMBAD

Kepler object of interest

KOI-2179.01

catalog

3 references

SIMBAD

Kepler object of interest

KOI-2179c

catalog

2 references

imported from Wikimedia project

TIC 26961231c

1 reference

discoverer or inventor

Kepler

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

Cygnus

1 reference

based on heuristic

parent astronomical body

4 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-369

object stated in reference as

Kepler-369

orbital period

14.871 day

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

The occurrence rate of small planets around small stars

14.87153514±0.00005078 day

1 reference

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

14.87151592±0.00000433 day

1 reference

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

14.8714615618±0.0000446923 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

14.87155876±0.000054 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

14.871572±0.000083 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

0.094 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

3.8414±0.5763 milliarcsecond

2 references

13.784±1.072 milliarcsecond per year

2 references

right ascension component of proper motion

19.447±1.09 milliarcsecond per year

2 references

1.23±0.18 Earth radius

1 reference

The occurrence rate of small planets around small stars

1.427±0.487 Earth radius

1 reference

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

1.52±0.43 Earth radius

1 reference

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

1.27±0.2 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

0.126±0.005 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

18,200±6,210 kilometre

1 reference

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

3 references