(Q87706366)

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

Kepler object of interest

catalog code

Gaia DR2 2131737340118958336

1 reference

KIC 11014932

1 reference

2MASS J18524967+4834498

1 reference

KOI-1432

2 references

Kepler-299

catalog

Kepler Confirmed Names

2 references

Spectroscopic Properties of Cool Stars

Gaia DR3 2131737340118958336

1 reference

TIC 48304460

1 reference

SPOCS 4171

1 reference

1 reference

inferred from equatorial coordinates

child astronomical body

Kepler-299c

c

0 references

Kepler-299e

e

0 references

Kepler-299b

b

0 references

Kepler-299d

reason for deprecated rank

d

0 references

distance from Earth

1,084.83±27.54 parsec

item/value with less precision and/or accuracy

1 reference

1,109.385±23.2609 parsec

1 reference

1,084.83±27.5386 parsec

1 reference

1,084.89±27.55 parsec

1 reference

stellar rotational velocity

1.9±1 kilometre per second

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

2.1±0.6 kilometre per second

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

parallax

0.9218±0.0234 milliarcsecond

1 reference

0.9014±0.0189 milliarcsecond

1 reference

declination component of proper motion

5.58±0.055 milliarcsecond per year

1 reference

5.521±0.027 milliarcsecond per year

1 reference

right ascension component of proper motion

8.226±0.042 milliarcsecond per year

1 reference

8.294±0.021 milliarcsecond per year

1 reference

radial velocity

10.4 kilometre per second

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

type of variable star

rotating variable star

2 references

Photometric amplitude distribution of stellar rotation of KOIs--Indication for spin-orbit alignment of cool stars and high obliquity for hot stars

Inferring probabilistic stellar rotation periods using Gaussian processes

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.875±0.028

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.51±0.027

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.44±0.04

1 reference

14.998343±0.002768

1 reference

luminosity

0.89158636±0.05867517 solar luminosity

1 reference

metallicity

0.120

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

0.07

2 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

−0.02

1 reference

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

−0.052

1 reference

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

0.02

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

radius

1.0563953±0.0252217 solar radius

1 reference

1.03±0.21 solar radius

1 reference

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

diameter

1,410,000 kilometre

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

2 references

283.20696159271 degree

1 reference

declination

48.58049845404 degree

1 reference

effective temperature

5,678 kelvin

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

5,885 kelvin

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

5,525 kelvin

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

reason for deprecated rank

5,617 kelvin

item/value with less precision and/or accuracy

1 reference

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

5,675 kelvin

2 references

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap

5,457±65.4805 kelvin

1 reference

5,645 kelvin

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

5,526 kelvin

1 reference

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

5,617±112 kelvin

1 reference

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

surface gravity

22,600 centimetre per square second

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

33,900 centimetre per square second

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

22,400 centimetre per square second

2 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

24,800 centimetre per square second

1 reference

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

45,000 centimetre per square second

1 reference

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

31,000 centimetre per square second

1 reference

A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap

25,000 centimetre per square second

1 reference