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/2504.04955
<galois> [arXiv] “The Short-spacing Interferometer Array for Global 21-cm Signal Detection (SIGMA): Design of the Antennas and Layout” Feiyu Zhao, Quan Guo, Qian Zheng et al. — «Numerous experiments have been designed to investigate the Cosmic Dawn (CD) and Epoch of Reionization (EoR) by examining redshifted 21-cm emissions from neutral hydrogen. Detecting the global spectrum of redshifted 21-cm signals is typically achieved through…»
<raptop> astronomers naming things: https://arxiv.org/abs/2504.05001
<galois> [arXiv] “SILVIA: Ultra-precision formation flying demonstration for space-based interferometry” Takahiro Ito, Kiwamu Izumi, Isao Kawano et al. — «We propose SILVIA (Space Interferometer Laboratory Voyaging towards Innovative Applications), a mission concept designed to demonstrate ultra-precision formation flying between three spacecraft separated by 100 m. SILVIA aims to achieve sub-micrometer precision in relative distance…»
<raptop> astronomers naming things: https://arxiv.org/abs/2504.04913
<galois> [arXiv] “The GRINTA hard X-ray mission: an Explorer of the Transient Sky” James Rodi, Lorenzo Natalucci — «The era of time domain multi-messenger (MM) astrophysics requires sensitive, large field-of-view (FoV) observatories that are able to quickly react in order to respond to alerts from gravitational wave (GW) triggers, neutrino detections, and transient sources from all parts of the electromagnetic (EM) spectrum. This is…»
<raptop> astronomers naming things: https://arxiv.org/abs/2504.05286
<galois> [arXiv] “UK APAP R-matrix electron-impact excitation cross-sections for modelling laboratory and astrophysical plasma” G. Del Zanna, G. Liang, J. Mao et al. — «Systematic R-matrix calculations of electron-impact excitation for ions of astrophysical interest have been performed since 2007 for many iso-electronic sequences as part of the UK Atomic Process for Astrophysical Plasma (APAP) network. Rate coefficients for Maxwellian…»
<raptop> astronomers naming things: https://arxiv.org/abs/2504.05401
<galois> [arXiv] “Disentangling the Light Curve of a VIM: A Case Study Using NEOWISE Data” Bringfried Stecklum — «The data collected by the Wide-field Infrared Survey Explorer (WISE, Wright et al. 2010) and its follow-up Near Earth Object (NEO) mission (NEOWISE, Mainzer et al. 2011) represent a treasure trove for variability studies. However, the angular resolution imposed by the primary mirror implies that close double stars are often…»
<raptop> astronomers naming things: https://arxiv.org/abs/2504.05446
<galois> [arXiv] “The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Director's Discretionary Program with Hubble. I. Goals, Design, and Initial Results” Julia Roman-Duval, William J. Fischer, Alexander W. Fullerton et al. — «Specifically selected to leverage the unique ultraviolet capabilities of the Hubble Space Telescope, the Hubble Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES)…»