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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 4.

The 0.8–2.8 μm spectrum of V1298 Tau. Top: comparing the observed spectrum to the best-fit three-component model, and the individual components scaled by their respective covering fractions. Bottom: the corresponding data – model residuals. NIRISS/SOSS is flux calibrated to the ∼1% level according to the JWST User Documentation, which is on the order of the magnitude of our residuals relative to the spectrum (≲5%). ✎

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