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JWST COMPASS: NIRSpec/G395H Transmission Observations of the Sub-Neptune HD 15337 c

  • Authors: Nicole L. Wallack, Peter Gao, Michael Greklek-McKeon, Annabella Meech, Artyom Aguichine, Munazza K. Alam, Lili Alderson, Natasha E. Batalha, Natalie M. Batalha, Anna Gagnebin, Tyler A. Gordon, James Kirk, Mercedes López-Morales, Sarah E. Moran, Jea Iyanla Redai, Nicholas Scarsdale, Johanna Teske, Hannah R. Wakeford, Nicholas F. Wogan, Angie Wolfgang

Nicole L. Wallack et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

Spectra for both visits for each of the Eureka! (left) and Tiberius (right) reductions. We show the differences between the two visits within a reduction pipeline on the bottom panels in units of σ (black) and ppm (blue). While there are some differences between the visits, the points generally agree, with median differences of <1σ. Only two points in the Eureka! spectra and one point in the Tiberius spectra deviate by more than 3σ between visits.

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