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A Comprehensive Investigation of Gamma-Ray Burst Afterglows Detected by TESS

  • Authors: Hugh Roxburgh, Ryan Ridden-Harper, Zachary G. Lane, Armin Rest, Lancia Hubley, Rebekah Hounsell, Qinan Wang, Sebastian Gomez, Justin Pierel, Muryel Guolo, Sofia Rest, Sophie von Coelln

Hugh Roxburgh et al 2024 The Astrophysical Journal 963 .

  • Provider: AAS Journals

Caption: Figure 2.

Detection pipeline as performed on GRB180807A. Left: events detected by the pipeline on Camera 2 Chip 3 coincident with the time of GRB180807A. The green curve displays the boundary of the 2σ error distance from the estimated location of the GRB as reported by the GCN, which is represented by the green plus in the top left. The colored boxes display the regions of the cutouts we generate and operate upon individually. Each black point represents an “event” detected by the pipeline; these are the signals of asteroids (e.g., top right, each light curve corresponds to a single pixel) or random noise (e.g., middle right). The red star displays the location of the candidate GRB signal (bottom right). Note that the dashed line in each of the light curves on the right represents the reported detection time of GRB180807A.

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