Figure 2 from Forty-four New and Known M-dwarf Multiples in the SDSS-III/APOGEE M-dwarf Ancillary Science Sample

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Forty-four New and Known M-dwarf Multiples in the SDSS-III/APOGEE M-dwarf Ancillary Science Sample

Authors: Jacob Skinner, Kevin R. Covey, Chad F. Bender, Noah Rivera, Nathan De Lee, Diogo Souto, Drew Chojnowski, Nicholas Troup, Carles Badenes, Dmitry Bizyaev, Cullen H. Blake, Adam Burgasser, Caleb Cañas, Joleen Carlberg, Yilen Gómez Maqueo Chew, Rohit Deshpande, Scott W. Fleming, J. G. Fernández-Trincado, D. A. García-Hernández, Fred Hearty, Marina Kounkel, Penélope Longa-Peñe, Suvrath Mahadevan, Steven R. Majewski, Dante Minniti, David Nidever, Audrey Oravetz, Kaike Pan, Keivan Stassun, Ryan Terrien, and Olga Zamora

2018 The Astronomical Journal 156 45.

Provider: AAS Journals

Caption: Figure 2.

Histograms of the number of visits observed for different classes of APOGEE DR13 targets. The APOGEE M-dwarf sample exhibits the same overall distribution of visits as the rest of the survey targets; the M-dwarf SB2 candidates are modestly biased toward a larger number of visits, with ∼one more visit per system in both the median and the mean than the broader DR13 sample.

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