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Direct Spectroscopic Confirmation of the Young Embedded Protoplanet WISPIT 2c

  • Authors: Chloe Lawlor, Richelle F. van Capelleveen, Guillaume Bourdarot, Christian Ginski, Matthew A. Kenworthy, Tomas Stolker, Laird Close, Alexander J. Bohn, Frank Eisenhauer, Paulo Garcia, Sebastian F. Hönig, Jens Kammerer, Laura Kreidberg, Sylvestre Lacour, Jean-Baptiste Le Bouquin, Eric Mamajek, Mathias Nowak, Thibaut Paumard, Christian Straubmeier, Nienke van der Marel

Chloe Lawlor et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 3.

Drift-Phoenix spectral model overlaid with the K-band spectrum obtained with VLTI/GRAVITY, H-band VLT/SPHERE, ﹩z^{\prime} ﹩-band MagAO-X, and L-band LBTI/LMIRCam photometry of WISPIT 2 c. The modeled spectrum is based on the max likelihood fitting of temperature and radius. The figure also contains a zoomed-in region of 2.2–2.4 μm to highlight the CO absorption band heads, marked by the pink box.

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