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> !u 亖
<galois> 亖: U+4E96 v1.1 (Lo) CJK UNIFIED IDEOGRAPH-4E96
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<raptop> astronomers naming things: https://arxiv.org/abs/2412.09705
<galois> [arXiv] “The Multiband Imaging Survey for High-Alpha PlanetS (MISHAPS) I: Preliminary Constraints on the Occurrence Rate of Hot Jupiters in 47 Tucanae” Alison L. Crisp, Jonas Klüter, Marz L. Newman et al. — «The first generation of transiting planet searches in globular clusters yielded no detections, and in hindsight, only placed occurrence rate limits slightly higher than the measured occurrence rate in the…»
<galois> [arXiv] “Using Felis to Represent the Semantics and Metadata of Astronomical Data Catalogs” Jeremy McCormick, Gregory P. Dubois-Felsmann, Andrei Salnikov et al. — «The Data Management team of the Vera C. Rubin Observatory has developed a data description language and toolset, Felis, for defining the semantics and metadata of its public-facing data catalogs. Felis uses a rich Pydantic data model for describing and validating…»
<galois> [arXiv] “Africanus II. QuartiCal: calibrating radio interferometer data at scale using Numba and Dask” Jonathan S. Kenyon, Simon J. Perkins, Hertzog L. Bester et al. — «Calibration of radio interferometer data ought to be a solved problem; it has been an integral part of data reduction for some time. However, as larger, more sensitive radio interferometers are conceived and built, the calibration problem grows in both size and…»
<raptop> kitty! also, astronomers naming things: https://arxiv.org/abs/2412.09783
<galois> [arXiv] “oMEGACat V: Helium Enrichment in $ω$ Centauri as a Function of Metallicity” C. Clontz, A. C. Seth, Z. Wang et al. — «Constraining the helium enhancement in stars is critical for understanding the formation mechanisms of multiple populations in star clusters. However, measuring helium variations for many stars within a cluster remains observationally challenging. We use Hubble Space Telescope photometry combined with…»