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
<galois>
[arXiv] “Progress report on the BEBOP search for circumbinary planets with radial velocities” Thomas A. Baycroft, Amaury H. M. J. Triaud, Dong Lai — «The BEBOP (Binaries Escorted By Orbiting Planets) survey is a search for circumbinary planets using the radial velocity spectrographs HARPS and SOPHIE, currently focusing on single-lined binaries with a mass ratio $<0.3$. Circumbinary systems are an important testing ground for…»
<galois>
[arXiv] “CLOWN: The PASO cloud detection for optimization of automatic optical surveys” Luís Gonçalves, Bruno Coelho, Domingos Barbosa et al. — «Orbiting space objects have become in the last decade a major nuisance impacting ground astronomy and orbiting space assets, from observatories to satellites and space stations. In particular with the rise of the satellite population in Low Earth Orbits (LEOs), space objects are…»
<galois>
[arXiv] “Characterizing the performance of two C-RED ONE cameras for implementation in RISTRETTO and SAXO+ projects” Muskan Shinde, Jana Anouk Baron, Nicolas Blind et al. — «In the near-infrared wavelength regime, atmospheric turbulence fluctuates at a scale of a few milliseconds, and its precise control requires the use of extreme adaptive optics (XAO) systems equipped with fast and sensitive detectors operating at kHz speeds.…»
<galois>
[arXiv] “STAR NRE: Solving supernova selection effects with set-based truncated auto-regressive neural ratio estimation” Konstantin Karchev, Roberto Trotta — «Accounting for selection effects in supernova type Ia (SN Ia) cosmology is crucial for unbiased cosmological parameter inference -- even more so for the next generation of large, mostly photometric-only surveys. The conventional "bias correction" procedure has a built-in…»
<galois>
[arXiv] “Searching for Tidal Orbital Decay in Hot Jupiters” Efrain Alvarado III, Kate B. Bostow, Kishore C. Patra et al. — «We study transits of several ``hot Jupiter'' systems - including WASP-12 b, WASP-43 b, WASP-103 b, HAT-P-23 b, KELT-16 b, WD 1856+534 b, and WTS-2 b - with the goal of detecting tidal orbital decay and extending the baselines of transit times. We find no evidence of orbital decay in any of the observed…»
<galois>
[arXiv] “Optical turbulence forecast for the European Solar Telescope (EST): the challenge of the day-time regime” Elena Masciadri, Alessio Turchi, Luca Fini — «In this contribution we present preliminary results of a study applied to the Observatories of Roque de Los Muchachos (La Palma) and Teide (Tenerife) in Canary Islands aiming to investigate the possibility to implement an automatic system for the optical turbulence…»
<galois>
[arXiv] “FATE -- an operational automatic system for optical turbulence forecasting at the Very Large Telescope” Elena Masciadri, Alessio Turchi, Luca Fini et al. — «In this contribution we report the on-going progresses of the project FATE, an operational automatic forecast system conceived to deliver forecasts of a set of astroclimatic and atmospheric parameters having the aim to support the science operations (i.e. the…»
<galois>
[arXiv] “Roadmap of GHOST@Gemini's Precision Radial Velocity Mode” Venu M. Kalari, Andreas Seifahrt, Ruben Diaz — «GHOST is a newly operational optical fiber-fed high-resolution spectrograph at the Gemini South 8.1m telescope. It currently offers the choice of two resolution modes captured by one (or two) input IFUs with a FOV of 1.2'' and a spectral resolving power of 56,000 and 76,000 for the unbinned CCDs. At the…»
<galois>
[arXiv] “ESCAPE project. CAPyBARA: a Roman Coronagraph simulator for post-processing methods development” Lisa Altinier, Élodie Choquet, Arthur Vigan et al. — «The Roman Coronagraph Instrument will be the first space facility equipped with deformable mirrors (DMs). These will lead to reach a contrast of $10^{-8}$ or better in a dark hole between $3-9 \lambda/D$. Post-processing techniques play an important role in increasing…»