Stellar Rotation in Kepler Data

Amy McQuillan     Tsevi Mazeh     Suzanne Aigrain

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ASCII Tables:

M Dwarf Sample
The tables below are the full versions of Table 2-5 from McQuillan, Aigrain & Mazeh, accepted MNRAS 2013, arXiv:1303.6787, please consult this paper for full details and caveats before using any of the results below.

Table 2. M dwarfs with rotation periods: Table 2: Periodic.txt

Table 3. Objects identified as likely giants: Table 3: Giants.txt

Table 4. Objects with two distinct periods in their light curves: Table 4: Multi-Period.txt

Table 5. No rotation period detected in Q1-4: Table 5: Non-Period.txt

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