(Q86843994)

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

catalog code

Gaia DR2 2127179245948119424

1 reference

2MASS J19142016+4444016

1 reference

KIC 8616637

1 reference

Kepler-190

Kepler Confirmed Names

2 references

Kepler object of interest

KOI-579

catalog

2 references

Spectroscopic Properties of Cool Stars

Gaia DR3 2127179245948119424

1 reference

TIC 158789380

1 reference

SPOCS 3831

1 reference

1 reference

inferred from equatorial coordinates

child astronomical body

Kepler-190b

series ordinal

b

0 references

Kepler-190c

series ordinal

c

0 references

distance from Earth

438.885±2.793 parsec

1 reference

435.635±2.3722 parsec

1 reference

438.885±2.7929 parsec

1 reference

stellar rotational velocity

1.7±1 kilometre per second

1 reference

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

1.6±0.5 kilometre per second

1 reference

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

parallax

2.2785±0.0145 milliarcsecond

1 reference

2.2955±0.0125 milliarcsecond

1 reference

declination component of proper motion

−4.431±0.032 milliarcsecond per year

1 reference

−4.433±0.017 milliarcsecond per year

1 reference

right ascension component of proper motion

−8.87±0.028 milliarcsecond per year

1 reference

−8.869±0.014 milliarcsecond per year

1 reference

radial velocity

−43 kilometre per second

1 reference

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

−40.76±10.44 kilometre per second

1 reference

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

type of variable star

rotating variable star

5 references

Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars

Rotation and differential rotation of active Kepler stars

Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators

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

G8

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)

12.728±0.022

1 reference

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

12.279±0.019

1 reference

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

12.231±0.016

1 reference

14.10601±0.002762

1 reference

luminosity

0.3539591±0.0066007 solar luminosity

1 reference

metallicity

0.058

1 reference

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

0.03

1 reference

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

0.009

1 reference

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

0.05

1 reference

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

reason for deprecated rank

0

item/value with less precision and/or accuracy

1 reference

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

radius

0.7803427±0.0214449 solar radius

1 reference

2 references

288.5840298626 degree

1 reference

declination

44.73378921088 degree

1 reference

effective temperature

5,138 kelvin

1 reference

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

5,194 kelvin

1 reference

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

5,106 kelvin

1 reference

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

5,074 kelvin

1 reference

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

5,039.9±67.8565 kelvin

1 reference

5,155 kelvin

1 reference

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

5,083 kelvin

1 reference

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

4,562 kelvin

1 reference

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

surface gravity

43,600 centimetre per square second

1 reference

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

40,700 centimetre per square second

1 reference

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

36,400 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

35,000 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

40,000 centimetre per square second

1 reference

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

38,000 centimetre per square second

1 reference

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

100 centimetre per square second

1 reference