(Q20827539)

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

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

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

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

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

unconfirmed exoplanet

2 references

SIMBAD

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

catalog code

Kepler-52d

catalog

Kepler Confirmed Names

3 references

Kepler object of interest

KOI-775.03

catalog

3 references

Kepler object of interest

KOI-775d

catalog

2 references

imported from Wikimedia project

TIC 399825554d

1 reference

discoverer or inventor

Kepler Space Telescope

1 reference

Portuguese 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

Draco

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-52

object stated in reference as

2MASS J19065712+4958327

orbital period

36.44530957±0.0000042 day

1 reference

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

36.4454819511±0.0001317076 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

36.44516433±0.000291 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

36.4451982±0.0001284 day

1 reference

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

36.445171±0.000253 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

0.182 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

3.0813±0.0231 milliarcsecond

2 references

1.378±0.048 milliarcsecond per year

2 references

right ascension component of proper motion

−3.975±0.05 milliarcsecond per year

2 references

1.96±0.29 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

2.14±0.09 Earth radius

1 reference

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

2.224±0.118 Earth radius

1 reference

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

2.012±0.13 Earth radius

1 reference

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

0.174±0.019 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

28,400±1,500 kilometre

1 reference

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

3 references