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] “DarkNESS: developing a skipper-CCD instrument to search for Dark Matter from Low Earth Orbit” Phoenix Alpine, Samriddhi Bhatia, Fernando Chierchie et al. — «The DarkNESS (Dark Matter Nano-satellite Equipped with Skipper Sensors) mission aims to deploy a skipper-CCD CubeSat Observatory to search for dark matter (DM) from Low Earth Orbit. This mission will employ novel skipper-CCDs to investigate O(keV) X-rays from…»
<galois>
[arXiv] “MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators” N. Jannsen, A. Tkachenko, P. Royer et al. — «With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's potential for observing pulsating stars across the Hertzsprung-Russell diagram as part of the PLATO Complimentary…»
<galois>
[arXiv] “Testing the asteroseismic estimates of stellar radii with surface brightness-colour relations and {\it Gaia} DR3 parallaxes. II. Red giants and red clump stars from the {\it Kepler} catalogue” G. Valle, M. Dell'Omodarme, P. G. Prada Moroni et al. — «A recent investigation highlighted peculiar trends between the radii derived from surface brightness-colour relations (SBCRs) combined with Gaia DR3 parallaxes with…»
<galois>
[arXiv] “The Eclipsing Binaries via Artificial Intelligence. II. Need for Speed in PHOEBE Forward Models” Marcin Wrona, Andrej Prša — «In modern astronomy, the quantity of data collected has vastly exceeded the capacity for manual analysis, necessitating the use of advanced artificial intelligence (AI) techniques to assist scientists with the most labor-intensive tasks. AI can optimize simulation codes where computational…»
_whitelogger has joined #kspacademia
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<e_14159>
The KSP-popcorn-discussion is amazing, @egg
<egg|matrix|egg>
hah
<egg|matrix|egg>
I didn’t know you were there
<e_14159>
Only very lurk-y (and in this case with a drive-by message)
<e_14159>
I haven't played KSP in a long time. Every time I feel the urge, I obviously want to automate the missions, so I start reading into kRPC and planning a reusable software architecture. Then I abandon the plan to start playing again.
<galois>
[mastodon] @Eigenraum: [attachment] «Kennt ihr das #TexLaTex Paket RealHats ? Damit kann man Hüte auf Symbole machen. Also richtige Hüte. Und zufällige Hüte. https://ctan.org/pkg/realhats»
<galois>
[arXiv] “MINDS. JWST-MIRI reveals a peculiar CO$_2$-rich chemistry in the drift-dominated disk CX Tau” Marissa Vlasblom, Milou Temmink, Sierra L. Grant et al. — «Radial drift of icy pebbles can have a large impact on the chemistry of the inner regions of protoplanetary disks. Compact dust disks ($\lesssim$50 au) are suggested to have a higher (cold) H$_2$O flux than more extended disks, likely due to efficient radial drift…»
<raptop>
SR1, maybe. SR2/JNO feels like KSP1.5 in some places
<galois>
[arXiv] “New Python-based Architecture for the Keck Observatory Archive” R. Moseley, G. Bruce Berriman, Christopher R. Gelino et al. — «We describe the development of the Keck Observatory Archive (KOA) Data Discovery Service, a web-based dashboard that returns metadata for wide-area queries of the entire archive in seconds. Currently in beta, this dashboard will support exploration, visualization, and data access across multiple…»
<galois>
[arXiv] “Virtual Realities: Is there only one advanced image display that astronomers need?” Christopher J. Fluke, Hugo K. Walsh, Lewis de Zoete Grundy et al. — «Data visualisation is an essential ingredient of scientific analysis, discovery, and communication. Along with a human (to do the looking) and the data (something to look at), an image display device is a key component of any data visualisation workflow. For the…»
<galois>
[arXiv] “Adding TESS to CRÉME. Light curves and masses of 300+ eclipsing binaries” Krzysztof G. Hełminiak, Ayush Moharana, Tilak B. Pawar et al. — «The Comprehensive Research with Echelles on the Most interesting Eclipsing binaries (CR\'EME) projects was aimed to collect high-resolutions spectra of about 380 detached eclipsing binaries (DEBs), which mostly do not have literature RV data. From this vast observational material…»
<galois>
[arXiv] “The April 1, 2471 b.C. eclipse and the end of 4th Egyptian dynasty” Giulio Magli — «On April 1, 2471 bC an impressive, unpredictable phenomenon occurred over the Delta of the Nile: a total solar eclipse, with totality band almost centered on the sacred city of Buto, and with the capital Memphis very close (>95%) to totality. This date is compatible with existing chronologies for the reign of Pharaoh Shepseskaf, who…»
<galois>
[arXiv] “The Hottest Neptunes Orbit Metal-Rich Stars” Shreyas Vissapragada, Aida Behmard — «The Neptune desert is no longer empty. A handful of close-in planets with masses between those of Neptune and Saturn have now been discovered, and their puzzling properties have inspired a number of interesting theories on the formation and evolution of desert-dwellers. While some studies suggest that Neptune desert planets form and evolve…»
<galois>
[arXiv] “Container-Based Pre-Pipeline Data Processing on HPC for XRISM” Satoshi Eguchi, Makoto Tashiro, Yukikatsu Terada et al. — «The X-Ray Imaging and Spectroscopy Mission (XRISM) is the 7th Japanese X-ray observatory, whose development and operation are in collaboration with universities and research institutes in Japan, U.S., and Europe, including JAXA, NASA, and ESA. The telemetry data downlinked from the satellite are…»
<galois>
[arXiv] “GHOST Reduced Data Products for the Gemini Observatory Community and Beyond” Vinicius M. Placco, David Herrera, Brian M. Merino et al. — «The Gemini High-resolution Optical SpecTrograph (GHOST) at Gemini South started regular queue operations in early 2024, bringing a long-sought open-access capability to the astronomy community. This research note briefly describes an effort to provide easy-to-access reduced spectra…»
<galois>
[arXiv] “The clus model in SPEX: projection and resonant scattering effects on the iron abundance and temperature profiles of galaxy clusters” Lýdia Štofanová, Aurora Simionescu, Jelle S. Kaastra — «In this paper we introduce the clus model, which has been newly implemented in the X-ray spectral fitting software package SPEX. Based on the 3D radial profiles of the gas density, temperature, metal abundance, turbulent, and…»
<galois>
[arXiv] “AutoKnots: Adaptive Knot Allocation for Spline Interpolation” Sandro D. P. Vitenti, Fernando de Simoni, Mariana Penna-Lima et al. — «In astrophysical and cosmological analyses, the increasing quality and volume of astronomical data demand efficient and precise computational tools. This work introduces a novel adaptive algorithm for automatic knots (AutoKnots) allocation in spline interpolation, designed to meet…»
<galois>
[arXiv] “The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction” C. Martínez-Sebastián, S. Simón-Díaz, H. Jin et al. — «There is increasing evidence that single-star evolutionary models are inadequate to reproduce all observational properties of massive stars. Binary interaction has emerged as a key factor in the evolution of a significant fraction of massive stars. In this study,…»
<galois>
[arXiv] “A New Method to Derive an Empirical Lower Limit on the Mass Density of a UFO” Abraham Loeb — «I derive a lower limit on the mass of an Unidentified Flying Object (UFO) based on measurements of its speed and acceleration, as well as the infrared luminosity of the airglow around it. If the object's radial velocity can be neglected, the mass limit is independent of distance. Measuring the distance and angular size of the…»