OGLE-2018-BLG-0506L Overview

OGLE-2018-BLG-0506L

OGLE-2018-BLG-0506L b

Overview Parameters Nearby Data Bibliography 1 Legend Expand All

OGLE-2018-BLG-0506L Architecture & Discovery Information

Name	Orbital Separation	Planet Size	Method	Year	Reference	Disposition
OGLE-2018-BLG-0506L
OGLE-2018-BLG-0506L b	3 au	16.3 M_⨁	Microlensing	2022	Hwang et al. 2022	Confirmed Planet

OGLE-2018-BLG-0506L Stellar Parameters (6 Solutions)

RA: 17h50m31.16s

Dec: -31d55m26.6s

Distance: 5600+1400-1600
pc

Parallax: ---

Ecliptic Latitude: -8.50151 deg

Ecliptic Longitude: 267.96226 deg

Galactic Latitude: -2.44687 deg

Galactic Longitude: 357.98566 deg

Total Proper Motion: ---

Proper Motion (RA): ---

Proper Motion (Dec): ---

Photometry

Tools: Planetary Systems; IRSA Finding Chart; Stellar Hosts

Source	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022
M_✶ (M_⦿)	0.63+0.37-0.32	0.63+0.37-0.32	0.63+0.37-0.32	0.63+0.37-0.32	0.63+0.37-0.32	0.63+0.37-0.32

OGLE-2018-BLG-0506L b Planetary Parameters (6 Solutions)

Status: Confirmed Planet

Detected By: Microlensing

Tools: Planetary Systems; Microlensing

Source	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022	Hwang et al. 2022
M_p (M_⨁)	16.3+12.0-8.5	16.3+12.0-8.5	16.3+12.0-8.5	16.3+12.0-8.5	16.3+12.0-8.5	16.3+12.0-8.5
M_p (M_Jup)	0.0513+0.0378-0.0267	0.0513+0.0378-0.0267	0.0513+0.0378-0.0267	0.0513+0.0378-0.0267	0.0513+0.0378-0.0267	0.0513+0.0378-0.0267
a (au)	3.0+0.7-0.8	3.0+0.7-0.8	3.0+0.7-0.8	3.0+0.7-0.8	3.0+0.7-0.8	3.0+0.7-0.8

Nearby Data (within 30 arcseconds) Browse Nearby Data

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Known Objects: 1 Confirmed Planets; 21 2MASS Point Source Catalog

Data Files: 1 Associated Literature Data

Bibliography (1 Reference)

Systematic KMTNet Planetary Anomaly Search. II. Six New q < 2 × 10^-4 Mass-ratio Planets
Hwang et al. 2022 Reference Overview

System
Star
Confirmed
Candidate
False Positive Planet
Controversial
False Positive

Aliases
Data Access
Transit Prediction Service
Time Series
Kepler | K2

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