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Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N

  • Authors: Caleb I. Cañas, Chad F. Bender, Suvrath Mahadevan, Dmitry Bizyaev, Nathan De Lee, Scott W. Fleming, Fred Hearty, Steven R. Majewski, Christian Nitschelm, Donald P. Schneider, Javier Serna, Keivan G. Stassun, Guđmundur Stefánsson, Guy S. Stringfellow, John C. Wilson

Caleb I. Cañas et al 2023 The Astrophysical Journal Supplement Series 265 .

  • Provider: AAS Journals

Caption: Figure 1.

A plot of the KOIs listed in Table 1 and observed by our program overlaid on the Kepler footprint from Mullally et al. (2016a). The APOGEE-KOI field is listed above the CCD modules from the Kepler field observed as part of our program between 2013 and 2020. The 1.°49 APOGEE-N FOV is plotted as a dotted circle. The marker reflects the DR25 disposition from the NASA Exoplanet Archive. The APOGEE-KOI program observed 714 confirmed planets (blue circles), 441 planetary candidates (red squares), and 446 false positives (green diamonds) for a median of 19 visits. For reference, KOIs not observed as part of this program but observed multiple times with APOGEE-N are shown as black triangles.

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