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/2501.14470
<galois> [arXiv] “MINCE III. Detailed chemical analysis of the UVES sample” F. Lucertini, L. Sbordone, E. Caffau et al. — «Context. The MINCE (Measuring at Intermediate Metallicity Neutron-Capture Elements) project aims to provide high quality neutron-capture abundances measurements in several hundred stars at intermediate metallicity,-2.5 < [Fe/H] < -1.5. This project will shed light on the origin of the neutron-capture elements and the…»
<raptop> astronomers naming things: https://arxiv.org/abs/2501.14355
<galois> [arXiv] “The NCORES Program: Precise planetary masses, null results, and insight into the planet mass distribution near the radius gap” David J. Armstrong, Ares Osborn, Remo Burn et al. — «NCORES was a large observing program on the ESO HARPS spectrograph, dedicated to measuring the masses of Neptune-like and smaller transiting planets discovered by the TESS satellite using the radial velocity technique. This paper presents an…»
<raptop> astronomers naming things: https://arxiv.org/abs/2501.14596
<galois> [arXiv] “JWST COMPASS: NIRSpec/G395H Transmission Observations of the Super-Earth TOI-776b” Lili Alderson, Sarah E. Moran, Nicole L. Wallack et al. — «We present two transit observations of the $\sim$520K, 1.85R$_\oplus$, 4.0M$_\oplus$ super-Earth TOI-776b with JWST NIRSpec/G395H, resulting in a 2.8-5.2$\mu$m transmission spectrum. Producing reductions using the ExoTiC-JEDI and Eureka! pipelines, we obtain a median transit…»
<raptop> astronomers naming things: https://arxiv.org/abs/2501.14478
<galois> [arXiv] “Alignment and optical verification of DESHIMA 2.0 at ASTE” A. Moerman, K. Karatsu, J. J. A. Baselmans et al. — «We developed, characterised, and verified an alignment method for the DESHIMA 2.0 instrument, an ultra wide-band spectrometer operating between 200-400 GHz, at the ASTE telescope. Due to the ultra-wide bandwidth of DESHIMA 2.0, we require the alignment to work across the entire spectral range. Moreover,…»
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