(Q86844246)

catalog code

Gaia DR2 2080452613110460928

1 reference

2MASS J19413907+4615592

1 reference

KIC 9597345

1 reference

Kepler-218

Kepler Confirmed Names

2 references

Kepler object of interest

KOI-711

catalog

2 references

Fourth USNO CCD Astrograph Catalog

UCAC4 682-070731

catalog

1 reference

Spectroscopic Properties of Cool Stars

Gaia DR3 2080452613110460928

1 reference

TIC 271662623

1 reference

SPOCS 3964

1 reference

1 reference

inferred from equatorial coordinates

child astronomical body

Kepler-218b

series ordinal

b

0 references

Kepler-218 c

series ordinal

c

0 references

Kepler-218d

series ordinal

d

0 references

distance from Earth

669.031±6.535 parsec

1 reference

669.031±6.5349 parsec

1 reference

669.703±5.3371 parsec

1 reference

669.703±5.3372 parsec

1 reference

669.02±6.55 parsec

1 reference

stellar rotational velocity

1.4±1 kilometre per second

1 reference

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

9.42 kilometre per second

1 reference

3.139 kilometre per second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

2.1±0.5 kilometre per second

1 reference

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

parallax

1.4947±0.0146 milliarcsecond

1 reference

1.4932±0.0119 milliarcsecond

1 reference

declination component of proper motion

20.872±0.026 milliarcsecond per year

1 reference

20.888±0.015 milliarcsecond per year

1 reference

right ascension component of proper motion

8.118±0.028 milliarcsecond per year

1 reference

8.129±0.015 milliarcsecond per year

1 reference

radial velocity

−49.6±18.2 kilometre per second

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

−54.925301±0.01283 kilometre per second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

−60.05±4.93 kilometre per second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

−67.1±5.66 kilometre per second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

−55.32±2.83 kilometre per second

1 reference

Gaia Data Release 3

−56.7 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

spectral class

G8IV

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

G7

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

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

12.732±0.025

1 reference

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

12.386±0.019

1 reference

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

12.311±0.022

1 reference

13.894723±0.002761

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

14.076±0.01

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

14.981±0.01

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

13.943±0.1

1 reference

luminosity

0.9407797±0.02782185 solar luminosity

1 reference

metallicity

0.371

1 reference

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

0.11

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

0.30

3 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

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

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

0.37

1 reference

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

0.194

1 reference

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

0.315

1 reference

0.25

1 reference

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

0.339

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

0.249

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

radius

1.1004195±0.23951415 solar radius

1 reference

1.06±0.08 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

1,460,000 kilometre

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

2 references

295.41282781292995 degree

1 reference

declination

46.26649020197 degree

1 reference

effective temperature

5,593 kelvin

1 reference

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

5,276 kelvin

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

5,502 kelvin

3 references

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

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

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

5,501 kelvin

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

5,488 kelvin

1 reference

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

5,419±707.615 kelvin

1 reference

5,499 kelvin

1 reference

5,348 kelvin

2 references

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

5,446 kelvin

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

5,427 kelvin

1 reference

5,590 kelvin

1 reference

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

5,500 kelvin

1 reference

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

5,502±74 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

20,700 centimetre per square second

1 reference

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

8,300 centimetre per square second

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

24,900 centimetre per square second

1 reference

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

24,500 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

24,600 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

28,000 centimetre per square second

1 reference

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

22,440 centimetre per square second

1 reference

22,340 centimetre per square second

1 reference

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

14,860 centimetre per square second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

21,000 centimetre per square second

1 reference

17,460 centimetre per square second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

33,000 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

20,000 centimetre per square second

1 reference