Stellar and Planetary Parameters for K2's Late-type Dwarf Systems from C1 to C5

Stellar and Planetary Parameters for K2's Late-type Dwarf Systems from C1 to C5

The NASA K2 mission uses photometry to find planets transiting stars of various types. M dwarfs are of high interest since they host more short-period planets than any other type of main-sequence star and transiting planets around M dwarfs have deeper transits compared to other main-sequence stars....

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Bibliographic Details
Main Authors: Martinez, Arturo O., Crossfield, Ian J. M., Schlieder, Joshua E., Dressing, Courtney D., Obermeier, Christian, Livingston, John, Ciceri, Simona, Peacock, Sarah, Beichman, Charles A., Lépine, Sébastien, Aller, Kimberly M., Chance, Quadry A., Petigura, Erik A., Howard, Andrew W., Werner, Michael W.
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
methods: data analysis
planetary systems
stars: fundamental parameters
stars: late-type
techniques: spectroscopic
Online Access:http://hdl.handle.net/10150/623204
http://arizona.openrepository.com/arizona/handle/10150/623204

Internet

http://hdl.handle.net/10150/623204
http://arizona.openrepository.com/arizona/handle/10150/623204

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