SIMP J013656.5+093347.3 Archives

Top panel: Final flux-calibrated NIRSpec/Prism (blue) and MIRI/LRS (red) spectra of SIMP 0136+0933, compared to the spectrum presented in Vos et al. (2023) (black) and error (shaded in grey). For the NIRSpec and MIRI spectra, each spectrum is plotted individually. Notable absorption features are indicated by horizontal black lines and their labels. For each instrument, we plot each spectrum individually, so the observed spread is a result of both noise and intrinsic variability. Bottom panel: Minimum spectrum subtracted from the maximum spectrum. The maximum and minimum spectra were identified using the 4.5 − 5.1 µm light curve (Figure 4). -- astro-ph.EP

Astronomy & Telescopes, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Exoplanets, -moons, -comets, Gas Giants, Habitable Zones, Icy Worlds, Imaging & Spectroscopy, Status Report

The JWST Weather Report From the Isolated Exoplanet Analog SIMP 0136+0933: Pressure-Dependent Variability Driven by Multiple Mechanisms

by Keith CowingNovember 26, 2024November 26, 2024

Isolated planetary-mass objects share their mass range with planets but do not orbit a star. They lack the necessary mass to support fusion in their cores and thermally radiate their […]

SIMP J013656.5+093347.3

The JWST Weather Report From the Isolated Exoplanet Analog SIMP 0136+0933: Pressure-Dependent Variability Driven by Multiple Mechanisms

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