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The Perkins INfrared Exosatellite Survey (PINES) I. Survey Overview, Reduction Pipeline, and Early Results

  • Authors: Patrick Tamburo, Philip S. Muirhead, Allison M. McCarthy, Murdock Hart, David Gracia, Johanna M. Vos, Daniella C. Bardalez Gagliuffi, Jacqueline Faherty, Christopher Theissen, Eric Agol, Julie N. Skinner, Sheila Sagear

Patrick Tamburo et al 2022 The Astronomical Journal 163 .

  • Provider: AAS Journals

Caption: Figure 11.

Transit recovery of WASP-2 b on UT 2021 July 28. The rows show different stages of PAT, going from raw flux to a final light curve. The left column shows the full night of data, while the right column shows a zoom-in on the four blocks that cover the transit event. Top: raw flux measured for WASP-2 and four reference stars. Middle: the normalized flux of WASP-2 and the ALC constructed from the weighted mean of the four reference stars. Bottom: the normalized flux for WASP-2 corrected by the ALC and a linear baseline, along with a transit model of WASP-2 b.

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