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] “Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations” Patricio E. Cubillos — «Gen TSO is a noise calculator specifically tailored to simulate James Webb Space Telescope (JWST) time-series observations of exoplanets. Gen TSO enables the estimation of signal-to-noise ratios (S/N) for transit or eclipse depths through an interactive graphical interface, similar to the JWST Exposure Time Calculator…»
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[arXiv] “Time-Domain And MultiMessenger Astrophysics Communications Science Analysis Group Report” Jamie A. Kennea, Judith L. Racusin, Eric Burns et al. — «The Time-Domain And MultiMessenger (TDAMM) Communications Science Analysis Group (TDAMMCommSAG) was formulated to describe the unique technical challenges of communicating rapidly to and from NASA astrophysics missions studying the most variable, transient, and extreme…»
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[arXiv] “Energy calibration of GTM on ground” Chien-You Huang, Hsiang-Kuang Chang, Chih-Hsun Lin et al. — «The Gamma-ray Transients Monitor (GTM) on board the Formosat-8B (FS-8B) satellite is designed to detect and localize Gamma-Ray Bursts (GRBs). By utilizing 2+2 CITIROC chips to manipulate 4+4 detectors, which are composed of GAGG(Ce) scintillators coupled with Silicon Photomultipliers (SiPMs) and oriented in various…»
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[arXiv] “Multi-Observatory Research of Young Stellar Energetic Flares (MORYSEF): X-ray Flare Related Phenomena and Multi-epoch Behavior” Konstantin V. Getman, Eric D. Feigelson, Abygail R. Waggoner et al. — «The most powerful stellar flares driven by magnetic energy occur during the early pre-main sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares…»
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[arXiv] “Upgrading SPHERE with the second stage AO system SAXO+: frequency-based data-driven controller for adaptive optics” Isaac Dinis, François Wildi, Damien Ségransan et al. — «This study introduces a novel frequency-based data-driven controller for adaptive optics, using power spectral density for optimization while ensuring stability criteria. It addresses disturbance rejection, command amplitude constraints and system…»
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[arXiv] “Gas phase Elemental abundances in Molecular cloudS (GEMS). X. Observational effects of turbulence on the chemistry of molecular clouds” L. Beitia-Antero, A. Fuente, D. Navarro-Almaida et al. — «(Abridged) We explore the chemistry of the most abundant C, O, S, and N bearing species in molecular clouds, in the context of the IRAM 30 m Large Programme Gas phase Elemental abundances in Molecular Clouds (GEMS). In this…»
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[arXiv] “Breaking degeneracies in exoplanetary parameters through self-consistent atmosphere-interior modelling” Christian Wilkinson, Benjamin Charnay, Stéphane Mazevet et al. — «Context: A new generation of instruments (e.g., JWST, ELTs, PLATO, Ariel) is providing atmospheric spectra and mass/radius measurements for large exoplanet populations, challenging planetary models used to interpret these findings. Aims: We develop a…»