Detectability of Habitable Planets around Very Low-Mass Stars

Martioli E.; Martín E. L.; Cabrera J.; Solano E.; Tata R.

Vol. 44 No. 1 (2014), Contributions

Vol. 44 No. 1 (2014)

Contributions

Detectability of Habitable Planets around Very Low-Mass Stars

Martioli E.⁺⁻
Martín E. L.⁺⁻
Cabrera J.⁺⁻
Solano E.⁺⁻
Tata R.⁺⁻

Martioli E.

Laboratório Nacional de Astrofísica (LNA/MCTI), Rua Estados Unidos, 154 Itajubá - MG, Brazil.

Martín E. L.

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Cabrera J.

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Solano E.

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Tata R.

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Keywords

Astrobiology
Techniques: spectroscopic
Techniques: photometric
Stars: late-type
Stars: flare

How to Cite

Detectability of Habitable Planets around Very Low-Mass Stars. (2014). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 44(1), 8-8. https://astronomia.unam.mx/journals/rmxac/article/view/2014rmxac..44....8m

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Abstract

We present observations of 18 very low-mass stars with Kepler light curves available in the public archive, where we performed a search for transits and characterized the photometric variability to estimate the effects of stellar activity in the detectability of habitable planets around stars at the cool end of the stellar mass distribution.

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Detectability of Habitable Planets around Very Low-Mass Stars

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