This paper is available on arxiv under CC 4.0 license.
Authors:
(1) Andrew Ridden-Harper, Department of Astronomy and Carl Sagan Institute, Cornell University & Las Cumbres Observatory;
(2) Stevanus K. Nugroho, Astrobiology Center & Japan & National Astronomical Observatory of Japan;
(3) Laura Flagg, Department of Astronomy and Carl Sagan Institute, Cornell University;
(4) Ray Jayawardhana, Department of Astronomy, Cornell University;
(5) Jake D. Turner, Department of Astronomy and Carl Sagan Institute, Cornell University & NHFP Sagan Fellow;
(6) Ernst de Mooij, Astrophysics Research Centre, School of Mathematics and Physics & Queen’s University Belfast;
(7) Ryan MacDonald, Department of Astronomy and Carl Sagan Institute;
(8) Emily Deibert, David A. Dunlap Department of Astronomy & Astrophysics, University of Toronto & Gemini Observatory, NSF’s NOIRLab;
(9) Motohide Tamura, Dunlap Institute for Astronomy & Astrophysics, University of Toronto
(10) Takayuki Kotani, Department of Astronomy, Graduate School of Science, The University of Tokyo, Astrobiology Center & National Astronomical Observatory of Japan;
(11) Teruyuki Hirano, Astrobiology Center, National Astronomical Observatory of Japan & Department of Astronomical Science, The Graduate University for Advanced Studies;
(12) Masayuki Kuzuhara, Las Cumbres Observatory & Astrobiology Center;
(13) Masashi Omiya, Las Cumbres Observatory & Astrobiology Center;
(14) Nobuhiko Kusakabe, Las Cumbres Observatory & Astrobiology Center.
Here, we explicitly define the wavelength regions that were excluded from our analysis for having severe telluric contamination or insufficient signal-to-noise ratios (especially at the edges of the spectral orders). The excluded regions for the IGRINS data are shown in Table 3.
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