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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[arXiv] “TOPCAT/STILTS Integration” Mark Taylor — «TOPCAT and STILTS are related packages for desktop analysis of tabular data, presenting GUI and command-line interfaces respectively to much of the same functionality. This paper presents features in TOPCAT that facilitate use of STILTS.»
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[arXiv] “Using the STIX background detector as a proxy for GOES” Muriel Zoë Stiefel, Matej Kuhar, Olivier Limousin et al. — «Context. The Spectrometer/Telescope for Imaging X-Rays (STIX) onboard Solar Orbiter was designed to observe solar flares in the X-ray range of 4-150 keV, providing spectral, temporal and spatial information. Besides 30 imaging detectors, STIX has two additional detectors, the coarse flare locator (CFL) and…»
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[arXiv] “Demonstration of Ultra-Sensitive KIDs for Future THz Space Borne Polarimeters” Stephen J. C. Yates, Alejandro Pascual Laguna, Willem Jellema et al. — «We present measurements and simulations of the polarization purity of leaky lens-antenna coupled microwave Kinetic Inductance Detectors (KIDs) at 1.5 THz. We find the integrated cross-polarization level to be at -21.5 dB for 1 f\#$\lambda$ spatial sampling. The…»
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[arXiv] “Assessing the Impact of Binary Systems on Microlensing Using SPISEA and PopSyCLE Population Simulations” Natasha S. Abrams, Jessica R. Lu, Casey Y. Lam et al. — «Gravitational microlensing provides a unique opportunity to probe the mass distribution of stars, black holes, and other objects in the Milky Way. Population simulations are necessary to interpret results from microlensing surveys. The contribution from binary…»
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[arXiv] “High Resolution {\it BOES} Spectroscopy of Raman-scattered He~II$λ$6545 in Young Planetary Nebulae” Jin Lim, Seok-Jun Chang, Jaejin Shin et al. — «Young planetary nebulae (PNe) are characterized by their hot central stars and the presence of abundant neutral and molecular components, which result from significant mass loss during the asymptotic giant branch (AGB) phase of stellar evolution. Far-UV…»
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[arXiv] “Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES” Juliana Ehrhardt, Luis Thomas, Hanna Kellermann et al. — «We report the confirmation and characterization of four hot Jupiter-type exoplanets initially detected by TESS: TOI-1295 b, TOI-2580 b, TOI-6016 b, and TOI-6130 b. Using observations with the high-resolution echelle spectrograph…»
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[arXiv] “Detecting Exomoons in Free-Floating-Planet Events from Space-based Microlensing Surveys” Hao-Zhu Fu, Subo Dong — «When a planet is ejected from its star-planet system due to dynamical interactions, its satellite may remain gravitationally bound to the planet. The Chinese Space Station Telescope (CSST) will be capable of detecting a large number of low-mass free-floating planet events (FFPs) from a bulge microlensing…»