(Q60538324)

The Revised TESS Input Catalog and Candidate Target List

Kepler object of interest

catalog code

KOI-2029

catalog

2 references

kepler_352_b--1960

2MASS J19593516+4603071

1 reference

KIC 9489524

1 reference

Gaia DR2 2085281530744134272

1 reference

Gaia DR3 2085281530744134272

1 reference

TIC 269271535

1 reference

Kepler-352

Kepler Confirmed Names

2 references

Spectroscopic Properties of Cool Stars

kepler_352_b--1960

SPOCS 3942

catalog

1 reference

1 reference

inferred from equatorial coordinates

child astronomical body

Kepler-352b

series ordinal

b

0 references

Kepler-352c

series ordinal

c

0 references

distance from Earth

254.582±1.4 parsec

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

250.545±0.8537 parsec

1 reference

254.582±1.3999 parsec

1 reference

252.733±1.399 parsec

1 reference

stellar rotational velocity

3±1 kilometre per second

1 reference

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

3.2±0.5 kilometre per second

1 reference

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

parallax

3.928±0.0216 milliarcsecond

1 reference

3.9913±0.0136 milliarcsecond

1 reference

declination component of proper motion

−20.254±0.037 milliarcsecond per year

1 reference

−20.29±0.016 milliarcsecond per year

1 reference

right ascension component of proper motion

13.852±0.038 milliarcsecond per year

1 reference

13.875±0.015 milliarcsecond per year

1 reference

radial velocity

−5.87±2.4 kilometre per second

1 reference

−9.8 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

5 references

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

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

Rotation and differential rotation of active Kepler stars

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

Inferring probabilistic stellar rotation periods using Gaussian processes

spectral class

K0

0 references

G8V

1 reference

11.6

0 references

11.61±0.023

astronomical filter

J band

1 reference

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

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

11.18±0.03

1 reference

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

11.132±0.022

1 reference

12.950232±0.002816

1 reference

luminosity

0.34152493±0.00415418 solar luminosity

1 reference

absolute magnitude

25

0 references

metallicity

−0.112

1 reference

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

−0.14

1 reference

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

−0.16

1 reference

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

−0.18

1 reference

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

0.07±0.115

1 reference

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

http://exoplanet.eu/catalog/kepler-352_b/

radius

0.78 solar radius

1 reference

reference URL

0.7413924±0.0615136 solar radius

1 reference

0.7314±0.0458 solar radius

1 reference

The Revised TESS Input Catalog and Candidate Target List

3 references

right ascension

299.89653761026 degree

1 reference

declination

46.05198958741 degree

1 reference

effective temperature

5,223 kelvin

1 reference

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

5,227 kelvin

1 reference

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

5,212 kelvin

1 reference

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

kepler_352_b--1960

5,124.575±226.81 kelvin

1 reference

5,278 kelvin

1 reference

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

5,156 kelvin

1 reference

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

5,219 kelvin

1 reference

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

5,262±180.607 kelvin

1 reference

The Revised TESS Input Catalog and Candidate Target List

surface gravity

36,800 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

42,700 centimetre per square second

1 reference

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

50,900 centimetre per square second

1 reference

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

47,000 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

35,500 centimetre per square second

1 reference

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

44,000 centimetre per square second

1 reference

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

age estimated by a dating method

3.47±3.02 gigaannum

1 reference

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