🇺🇦 #NowPlaying on KEXP's #EasternEchoes
Mei Semones:
🎵 Animaru
#MeiSemones
https://meisemones.bandcamp.com/track/animaru
https://open.spotify.com/track/1SkY6npvIxrTAU1cP4XMIg
The Constraint of Crewed Mars Missions Based on Current Radiation Dose Measurements: #Mars: https://www.esa.int/Science_Exploration/Human_and_Robotic_Exploration/The_radiation_paradox_why_solar_maximum_is_the_safest_time_to_travel_to_Mars
🇺🇦 Auf radioeins läuft...
Moscoman & Tom Sanders:
🎵 In Stereo
#NowPlaying #Moscoman #TomSanders
https://moscoman.bandcamp.com/track/in-stereo-feat-tom-sanders
https://open.spotify.com/track/6VBbmDuYFGj4xAxLM79JB7
Google will wissen, WER hinter einem Text steht – nicht nur WAS drinsteht. 🔍E-E-A-T ist kein Score, den du irgendwo abliest. Aber es bestimmt, ob dein Content in sensiblen Themenbereichen überhaupt eine Chance hat. Autorenprofile, Über-uns-Seiten, Knowledge-Panel-Einträge – das sind Entity-Signale, die Vertrauen aufbauen. Maschinen und Menschen gleichermaßen.
Digitalisierung klingt einfach. Ist sie aber nicht.
In unserem Podcast #9vor9 diskutieren wir mit Holger Klötzner, Stadtrat für Digitalisierung, und Dennis Schwalbach aus dem IT-Maschinenraum der Stadt Darmstadt über Formulare, Fachverfahren – und die Umlaufmappe 📁.
Was bedeutet digitale Verwaltung wirklich?
Wo hakt es noch?
Reinhören unter
L'homme de cro magnon
Fast Makespan Minimization via Short ILPs
Danny Hermelin, Dvir Shabtay
https://arxiv.org/abs/2602.06514 https://arxiv.org/pdf/2602.06514 https://arxiv.org/html/2602.06514
arXiv:2602.06514v1 Announce Type: new
Abstract: Short integer linear programs are programs with a relatively small number of constraints. We show how recent improvements on the running-times of solvers for such programs can be used to obtain fast pseudo-polynomial time algorithms for makespan minimization on a fixed number of parallel machines, and other related variants. The running times of our algorithms are all of the form $\widetilde{O}(p^{O(1)}_{\max} n)$ or $\widetilde{O}(p^{O(1)}_{\max} \cdot n)$, where $p_{\max}$ is the maximum processing time in the input. These improve upon the time complexity of previously known algorithms for moderate values of $p_{\max}$.
toXiv_bot_toot
🇺🇦 #NowPlaying on KEXP's #DriveTime
Pinkshinyultrablast:
🎵 Holy Forest
#Pinkshinyultrablast
https://mahoganyinthecity.bandcamp.com/track/pinkshinyultrablast-holy-forest-waldeinsamkeit-remix
https://open.spotify.com/track/5740WNrWQZEiXK6yoPp2q4
So the new #Kreutz #comet #MAPS is *still* following the constant rapid rise in brightness it has shown since discovery: a dumb extrapolation - https://cobs.si/analysis/?comet=2688&from_date=2026-01-15 00:00&to_date=2026-04-30 00:00&observation_type=V&observation_type=C&plot_x_value=1&plot_y_value=1&fit_option=1&exclude_faint=on&exclude_issue=on&observer=&association=&country=&compare_values=compare - has it get 10,000-times brighter than the Sun at its extremely close perihelion which makes so sense at all, of course, physically.
"It must therefore be assumed that this increase in activity will level off significantly in the near future," writes https://fg-kometen.vdsastro.de/koj_2026/c2026a1/26a1eaus.htm: "More likely are parameters m m0=12.0 mag / n=4 (or even lower), which would still result in a (very short-term) maximum brightness of about –9 mag (but this would probably still be significantly too bright) – always assuming that the comet survives its perihelion passage unscathed."
For other views see http://www.cbat.eps.harvard.edu/iau/cbet/005600/CBET005663.txt and https://arxiv.org/abs/2602.17626 and https://www.facebook.com/photo?fbid=10236580364221799 and https://cometografia.es/cometa-kreutz-2026-a1-maps-analisis/ - and the actual brightness is tracked at https://cobs.si/obs_list?id=2688 where it has reached ~11.5 mag. now.