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Reanalyzing Jupiter ISO/SWS Data through a More Recent Atmospheric Model
Published 2023-11-01“…To help in this endeavour, we used Infrared Space Observatory Short Wavelength Spectrometer (ISO/SWS) Jupiter observations in the 793–1500 cm<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msup><mrow></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup></semantics></math></inline-formula> region together with the Nonlinear Optimal Estimator for MultivariatE Spectral analySIS (NEMESIS) radiative transfer suite to retrieve the temperature–pressure profile and the chemical abundances for various chemical species. …”
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A Candidate for the Least-massive Black Hole in the First 1.1 Billion Years of the Universe
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Dust and Cold Gas Properties of Starburst HyLIRG Quasars at z ∼ 2.5
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Constraints on the Persistent Radio Source Associated with FRB 20190520B Using the European VLBI Network
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From Atmospheric Evolution to the Search of Species of Astrobiological Interest in the Solar System—Case Studies Using the Planetary Spectrum Generator
Published 2022-03-01“…For Jupiter, the detection of ammonia, phosphine, deuterated methane and methane was studied, by comparing the simulations with IR observations by the Infrared Space Observatory (ISO) at approximately 7–12 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">μ</mi></semantics></math></inline-formula>m. …”
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A Centiparsec-scale Compact Radio Core in the Nearby Galaxy M60
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Big Three Dragons: Molecular Gas in a Bright Lyman-break Galaxy at z = 7.15
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An SiO Toroid and Wide-angle Outflow Associated with the Massive Protostar W75N(B)-VLA2
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AMUSE-Antlia. I. Nuclear X-Ray Properties of Early-type Galaxies in a Dynamically Young Galaxy Cluster
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Discovery of Hydrogen Radio Recombination Lines at z = 0.89 toward PKS 1830-211
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Resolved CO(1–0) Emission and Gas Properties in Luminous Dusty Star-forming Galaxies at z = 2–4
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A Simultaneous Dual-site Technosignature Search Using International LOFAR Stations
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