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Medium-resolution 0.97–5.3 μm Spectra of Very Young Benchmark Brown Dwarfs with NIRSpec on Board the James Webb Space Telescope

  • Authors: Elena Manjavacas, Pascal Tremblin, Stephan Birkmann, Jeff Valenti, Catarina Alves de Oliveira, Tracy L. Beck, G. Giardino, N. Lützgendorf, B. J. Rauscher, M. Sirianni

Elena Manjavacas et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 14.

Markov Chain Monte Carlo (MCMC) corner plot with the best-fit parameters (effective temperature, T eff; surface gravity, log g; radius, R; parallax, ω; and mass, M) derived with the best fit using the BT-Settl CIFIST models for TWA 28. The vertical lines show the 1σ uncertainties of each parameter as derived by the MCMC fitting.

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