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Stellar HostProfile

OGLE-2012-BLG-0950L

M V โ€ข 3300 pc

Records

12

literature rows

Planets

1

system count

References

2

distinct source labels

Approximate color

from effective temperature

Canonical Summary

Adopted host values from all rows

Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.

Mass

0.52 Msun

0.31 to 0.63

12 values โ€ข 9 distinct

Distance

3300 pc

2400 to 4200

12 values โ€ข 7 distinct

Spectral Type

M V

Consistent across records

M V (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

โ—Œ

Discovery

2016

Period

โ€”

Radius

โ€”

Mass

41 MโŠ•

Eq. Temp

โ€”

Provenance

Underlying measurements and references

Download JSONDownload CSV

Evidence Summary

Rows

12

Stellar refs

1

System refs

1

Distancedisputed

12 values โ€ข 7 distinct

Massdisputed

12 values โ€ข 9 distinct

Spectral Typestable

1 values โ€ข 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
โ€”0.55โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.57โ€”โ€”โ€”M V2600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.63โ€”โ€”โ€”โ€”3200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.55โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.63โ€”โ€”โ€”โ€”3200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.33โ€”โ€”โ€”โ€”3600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.38โ€”โ€”โ€”โ€”4200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.31โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.47โ€”โ€”โ€”โ€”2600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.54โ€”โ€”โ€”โ€”2400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.38โ€”โ€”โ€”โ€”4200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.50โ€”โ€”โ€”โ€”2900Koshimoto et al. 2017Koshimoto et al. 2017