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Astronomical Image Time Series Segmentation for Faint, Fast Object Detection

  • Authors: Dan Caselden, J. Davy Kirkpatrick, Lindsey Lack, Andrew White, Federico Marocco, Aaron M. Meisner, Guillaume Colin, Bruce Baller, Kareem Ammar, Thomas P. Bickle, Hunter Brooks, S. L. Casewell, Peter R. M. Eisenhardt, Charles A. Elachi, Jacqueline K. Faherty, John W. Fowler, Daniella C. Bardalez Gagliuffi, Jonathan Gagné, Christopher R. Gelino, Jake Grigorian, Les Hamlet, Hiro Higashimura, 村滉 東, Justin Hong, Issam Ibnouhsein, Tarun Kota, Marc J. Kuchner, Ken A. Marsh, Matteo Paz, Yadukrishna Raghu, Adam C. Schneider, Sajesh Singh, Asa Trek, Kieran Wall, Andrew Washburn, Edward L. Wright, David Zurek

Dan Caselden et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

Density of 176″ × 176″ sky regions that scored ≥0.50 in our full-sky processing of real unWISE images (Section 4). The axes are in equatorial coordinates: R.A. (degrees) and ﹩\sin (\,\rm{declination}\,)﹩. Six key areas are visible: the Galactic plane centered at ∼265° R.A., the north and south ecliptic poles at 270° and 90° R.A., the north and south celestial poles, and an area in the northern sky surrounding the Cassiopeia A supernova remnant at ∼350° R.A.

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