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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<galois> [arXiv] “BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration history” James Kirk, Eva-Maria Ahrer, Anna B. T. Penzlin et al. — «A primary objective of exoplanet atmosphere characterisation is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether differences in atmospheric…»
<raptop> astronomers naming things: https://arxiv.org/abs/2407.02979
<galois> [arXiv] “Progress on FORS-Up: the first instrument using ELT technologies” H. M. J. Boffin, V. Baldini, S. Bertocco et al. — «ESO is in the process of upgrading one of the two FORS (FOcal Reducer/low dispersion Spectrograph) instruments - a multi-mode (imaging, polarimetry, long-slit, and multi-object spectroscopy) optical instrument mounted on the Cassegrain focus of Unit Telescope 1 of ESO's Very Large Telescope. FORS1 was…»
<raptop> astronomers naming things: https://arxiv.org/abs/2407.03137
<galois> [arXiv] “X-Shooting ULLYSES: Massive Stars at low metallicity -- IV. Spectral analysis methods and exemplary results for O stars” A. A. C. Sander, J. -C. Bouret, M. Bernini-Peron et al. — «CONTEXT: The spectral analysis of hot, massive stars is a fundamental astrophysical method to obtain their intrinsic properties and their feedback. Quantitative spectroscopy for hot, massive stars requires detailed numerical modeling of the…»