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> tidal quality factors being impossible to get through physical models and needing stuff like this remains darkly amusing: https://arxiv.org/abs/2404.16499
<galois> [arXiv] “Host star properties of hot, warm and cold Jupiters in the solar neighborhood from \textit{Gaia} DR3: clues to formation pathways” Bihan Banerjee, Mayank Narang, P. Manoj et al. — «Giant planets exhibit diverse orbital properties, hinting at their distinct formation and dynamic histories. In this paper, using $\textit{Gaia}$ DR3, we investigate if and how the orbital properties of Jupiters are linked to their host star…»
<raptop> It's in the abstract, but astronomers naming things: https://arxiv.org/abs/2404.16606
<galois> [arXiv] “A general polarimetric model for transiting and non-transiting ringed exoplanets” Allard K. Veenstra, Jorge I. Zuluaga, Jaime A. Alvarado-Montes et al. — «We explore the potential of polarimetry as a tool for detecting and characterizing exorings. For that purpose, we have improved the publicly available photometric code Pryngles by adding the results of radiative transfer calculations that fully include polarization…»
<raptop> (Pryngals)
<raptop> astronomers naming things: https://arxiv.org/abs/2404.16732
<galois> [arXiv] “The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres. No evidence of enhanced evaporation in young planets” J. Orell-Miquel, F. Murgas, E. Pallé et al. — «During the first Gyr of their life, exoplanet atmospheres suffer from different atmospheric escape phenomena that can strongly affect the shape and morphology of the exoplanet itself. These processes can be studied with Ly$\alpha$,…»
<raptop> In the abstract, but astronomers naming things: https://arxiv.org/abs/2404.16089
<galois> [arXiv] “Observational parameters of Blue Large-Amplitude Pulsators” P. Pietrukowicz, M. Latour, I. Soszynski et al. — «Blue Large-Amplitude Pulsators (BLAPs) are a recently discovered class of short-period pulsating variable stars. In this work, we present new information on these stars based on photometric and spectroscopic data obtained for known and new objects detected by the OGLE survey. BLAPs are evolved objects with…»
<raptop> (Also, BLAP sounds lewd)
<SnoopJ> !or BLAP or BRRRAP
<galois> SnoopJ: BLAP
<raptop> *BLAP BLAP BLAP*
<raptop> astronomers naming things: https://arxiv.org/abs/2404.16567
<galois> [arXiv] “J-PLUS: Bayesian object classification with a strum of BANNJOS” A. del Pino, C. López-Sanjuan, A. Hernán-Caballero et al. — «With its 12 optical filters, the Javalambre-Photometric Local Universe Survey (J-PLUS) provides an unprecedented multicolor view of the local Universe. The third data release (DR3) covers 3,192 deg$^2$ and contains 47.4 million objects. However, the classification algorithms currently implemented…»
<raptop> astronomers naming things: https://arxiv.org/abs/2404.16570
<galois> [arXiv] “STELLA lightcurves of energetic pair instability supernovae in the context of SN2018ibb” Chris Nagele, Hideyuki Umeda, Keiichi Maeda — «SN2018ibb is a recently observed hydrogen poor super-luminous supernova which appears to be powered by the decay of $30\;\rm{M_\odot}$ of radioactive nickel. This supernova has been suggested to show hybrid signatures of a pair instability supernova and an interacting supernova. In a…»