JWST-TST High Contrast: First Direct Spectroscopy of GJ 504 b reveals Clouds and Possible Metal Enrichment
arXiv:2606.19228 · doi:10.3847/1538-3881/ae6919
Abstract
Characterizing the coldest directly imaged companions through direct spectroscopy has only recently become possible with the James Webb Space Telescope. We present moderate-resolution (R 2,700) spectroscopic observations of the directly imaged planetary-mass companion (PMC), GJ 504 b, using the /NIRSpec. As the coldest imaged PMC of the pre-JWST era GJ 504 b is too faint for ground-based spectroscopy, with only photometric observations possible. Leveraging advanced post-processing techniques with a forward modeling framework, we detect the companion at high signal-to-noise (S/N300). We also present the first successful PSF subtraction with angular differential imaging (ADI) in the NIRSpec point cloud, detecting GJ 504 b at S/N and reaching contrast limits . The extracted 2.9--5.3 spectra show strong signatures of several molecular species, including HO, CO, CH, CO, NH, HS, CO, and CO. Atmospheric modeling of the spectra using \texttt{petitRADTRANS}, yields an effective temperature = 5644 K, surface gravity = 4.87, metallicity [M/H] = 0.67, C/O ratio = 0.64, interstellar C/C and O/O isotopologue ratios, and strong evidence of disequilibrium chemistry and salt clouds. The retrieved parameters indicate a mass 25.2 , which is in agreement with the mass range (19--27 ) obtained from ATMO evolutionary models, implying an age of 2.5--4.0 Gyr. Lastly, we compare the abundances of GJ 504 b to its primary, obtaining a stellar abundance of sulfur (S), super-stellar carbon (C), and possibly, oxygen (O). The observed metal enrichment tentatively supports planet-like formation, but does not entirely exclude stellar abundances for GJ 504 b.
35 pages, 20 figures, 6 tables