egg changed the topic of #kspacademia to: https://git.io/JqLs2 | Dogs are cats. Spiders are cat interferometers. | Document well, for tomorrow you may get mauled by a ネコバス. | <UmbralRaptor> egg|nomz|egg: generally if your eyes are dewing over, that's not the weather. | <ferram4> I shall beat my problems to death with an engineer. | We can haz pdf | Logs: https://esper.irclog.whitequark.org/kspacademia
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<raptop> astronomers naming things: https://arxiv.org/abs/2406.09641
<galois> [arXiv] “Phase-resolving the absorption signatures of water and carbon monoxide in the atmosphere of the ultra-hot Jupiter WASP-121b with GEMINI-S/IGRINS” Joost P. Wardenier, Vivien Parmentier, Michael R. Line et al. — «Ultra-hot Jupiters are among the best targets for atmospheric characterization at high spectral resolution. Resolving their transmission spectra as a function of orbital phase offers a unique window into the 3D…»
<raptop> Though honestly, that's a cool study. Those differences in gas concentrations across the planet are another step towards understanding exoplanet weather
<raptop> astronomers naming things: https://arxiv.org/abs/2406.10032
<galois> [arXiv] “GASTLI: An open-source coupled interior-atmosphere model to unveil gas giant composition” Lorena Acuña, Laura Kreidberg, Meng Zhai et al. — «The metal mass fractions of gas giants are a powerful tool to constrain their formation mechanisms and evolution. The metal content is inferred by comparing mass and radius measurements with interior structure and evolution models. In the midst of the JWST, CHEOPS, TESS, and the…»
<raptop> astronomers naming things: https://arxiv.org/abs/2406.10217
<galois> [arXiv] “MINDS. A multi-instrument investigation into the molecule-rich JWST-MIRI spectrum of the DF Tau binary system” Sierra L. Grant, Nicolas T. Kurtovic, Ewine F. van Dishoeck et al. — «Most stars form in multiple systems whose properties can significantly impact circumstellar disk evolution. We investigate the physical and chemical properties of the equal-mass, small separation (~66 mas, ~9 au) DF Tau binary system.…»
<raptop> It's in the abstract, but astronomers naming things: https://arxiv.org/abs/2406.09516
<galois> [arXiv] “The Japanese Vision for the Black Hole Explorer Mission” Kazunori Akiyama, Kotaro Niinuma, Kazuhiro Hada et al. — «The Black Hole Explorer (BHEX) is a next-generation space very long baseline interferometry (VLBI) mission concept that will extend the ground-based millimeter/submillimeter arrays into space. The mission, closely aligned with the science priorities of the Japanese VLBI community, involves an active…»
<raptop> It's in the abstract, but astronomers naming things: https://arxiv.org/abs/2406.09813
<galois> [arXiv] “Diffuse X-ray Explorer: a high-resolution X-ray spectroscopic sky surveyor on the China Space Station” Hai Jin, Junjie Mao, Liubiao Chen et al. — «DIffuse X-ray Explorer (DIXE) is a proposed high-resolution X-ray spectroscopic sky surveyor on the China Space Station (CSS). DIXE will focus on studying hot baryons in the Milky Way. Galactic hot baryons like the X-ray emitting Milky Way halo and eROSITA bubbles are best…»
<raptop> astronomers naming things: https://arxiv.org/abs/2406.09337
<galois> [arXiv] “Different Planetary Eccentricity-Period (PEP) Distributions of Small- and Giant-Planets” Dolev Bashi, Tsevi Mazeh, Simchon Faigler — «We used the database of $1040$ short-period ($1 \leq P < 200$ days) exoplanets radial-velocity (RV) orbits to study the planetary eccentricity-period (PEP) distribution. We first divided the sample into low- and high-mass exoplanet sub-samples based on the distribution of the (minimum)…»
<raptop> hungry astronomers naming things: https://arxiv.org/abs/2406.09275
<galois> [arXiv] “The CUISINES Framework for Conducting Exoplanet Model Intercomparison Projects, Version 1.0” Linda E. Sohl, Thomas J. Fauchez, Shawn Domagal-Goldman et al. — «As JWST begins to return observations, it is more important than ever that exoplanet climate models can consistently and correctly predict the observability of exoplanets, retrieval of their data, and interpretation of planetary environments from that data. Model…»