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KRONOS I: The 1–2.8 μm JWST Transmission Spectrum of the 23 Myr V1298 Tau c

  • Authors: Matthew M. Murphy, Matthew C. Nixon, Adina D. Feinstein, Luis Welbanks, Girish M. Duvvuri, Saugata Barat, Benjamin V. Rackham, Darryl Z. Seligman, Michael Radica, Ian J. M. Crossfield, Kevin France, John H. Livingston, Jonathan Lunine, Rafael Luque, Catriona Murray, Sagnick Mukherjee, Biruk Nardos, Sydney Petz, Hinna Shivkumar

Matthew M. Murphy et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

Detrended light curves and best-fit models of the NIRISS/SOSS order-1 broadband light curve. Gray points are at the native time cadence of ∼13 s, and black points are binned to ∼5 minute cadence. Each panel shows the result of the four methods we implemented to account for heterogeneous stellar surface features in the light curve: (1) masking the features, (2) modeling them as Gaussians, (3) modeling them with fleck, and (4) modeling them with a GP. ✎

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