Tootfinder

Vuoden huiputus -kilpailun ylivoimaiseksi voittajaksi Atrian ja Arman Alizadin lihantuotantoa markkinoiva sarja “Oodi suomalaiselle ruoalle”. https://www.greenpeace.org/finland/blogit/

Vuoden huiputus -kilpailun ylivoimaiseksi voittajaksi Atrian ja Arman Alizadin lihantuotantoa markkinoiva sarja “Oodi suomalaiselle ruoalle”. - Greenpeace Suomi
Vuoden törkeimmästä viherpesuteosta jaettavan Vuoden Huiputus -palkinnon voittaja on Atrian ja tv-kasvo Arman Alizadin sarja “Oodi suomalaiselle ruoalle”. Voittaja julkistettiin lauantaina 6.6. Greenpeacen Nousu-festivaalien yhteydessä Helsingin Tekstin talolla. Greenpeacen järjestämässä…

„Guild Wars 3“ angekündigt: MMORPG-Reihe kommt erstmals auf Konsole
ArenaNet hat „Guild Wars 3“ angekündigt. Das Spiel erscheint für PC und bringt die MMORPG-Reihe erstmals auch auf eine Heimkonsole.
https…

„Guild Wars 3“ angekündigt: MMORPG-Reihe kommt erstmals auf Konsole
ArenaNet hat „Guild Wars 3“ angekündigt. Das Spiel erscheint für PC und bringt die MMORPG-Reihe erstmals auch auf eine Heimkonsole.

Claude Opus 4.8 and Sonnet 5 seem worse at tool calls than older models, likely due to post-training that assumes Claude Code-like harnesses as targets (Armin Ronacher/Armin Ronacher's Thoughts and Writings)
https://lucumr.pocoo.org/2026/7/4/better-models-worse-tools/…

Better Models: Worse Tools
About an aggravating tool-calling regression in newer Claude models.

🇺🇦 #NowPlaying on BBCRadio3's #ThroughTheNight
Unico Wilhelm van Wassenaer, Combattimento & Jan Willem de Vriend:
🎵 Concerto armonico No 6 in E flat major (from Sei Concerti Armonici, 1740)
#UnicoWilhelmvanWassenaer
https://open.spotify.com/track/5O7QyV8tAoxMtewlVJmaWr

Wirbel vor ORF-Wahl - Armin Wolf: „Rassistische Fake-News-Schleuder“ #News #Nachrichten

Stumm grüßte ich den Nachbarn, der am Dach eines der Zwillingsbabies in seinen Armen in den Schlaf schaukelte.

vandaag terug uit Duitsland met de trein. Heb ik nét tickets gekocht en alles geregeld verschijn ineens in beeld dat de trein niet naar Arnhem rijdt. Gelukkig nog wel een (veel duurder) sneller alternatief over Hengelo gevonden. Het zšl een keertje vlekkeloos gaan met DB.
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Fietsen meenemen in de regionale treinen is eigenlijk wel heel makkelijk

Singapore-based Multiplier, which acquires accounting firms to boost their growth with AI tools, raised a $35M Series B led by TheGP at a $300M valuation (Maria Armental/Wall Street Journal)
https://www.

Is Dark Matter Really Matter?
Jun-Qian Jiang, Arman Shafieloo
https://arxiv.org/abs/2608.04763 https://arxiv.org/pdf/2608.04763 https://arxiv.org/html/2608.04763
arXiv:2608.04763v1 Announce Type: new
Abstract: In the standard model of cosmology, it is assumed that dark matter is pressureless with equation of state $w=0$ and dark energy has $w=-1$. We test these assumptions jointly using DESI DR2 distance measurements, including the recent Lyman-$\alpha$ full-shape Alcock-Paczynski (AP) information, DES supernovae, and two complementary CMB treatment. When constant $w_{dm}$ and $w_{de}$ are varied together, we find $w_{dm}=0.000968^{ 0.000501}_{-0.000496}$ and $w_{de}=-0.9380^{ 0.0259}_{-0.0262}$ (68%). With an alternative CMB treatment that marginalizes over the lensing spectrum, the corresponding constraints are $w_{dm}=0.000870^{ 0.000408}_{-0.000410}$ and $w_{de}=-0.9353^{ 0.0258}_{-0.0254}$. Both standard $\Lambda$CDM values are disfavored at approximately $2\sigma$ in the joint extension. Neither parameter departs significantly from its standard value when only that parameter is varied. This behavior arises because late-time distances favor $w_{de}>-1$, while maintaining the early-Universe physical matter density requires a compensating positive $w_{dm}$, which changes the mapping to the matter density today. Allowing dynamical dark energy clarify further on complexity of the situation: phantom crossing for dark energy makes $w_{dm}=0$ consistent with the data, whereas a positive $w_{dm}$ preference persists when crossing is forbidden. Interestingly, the Pad'e-$w$ parameterization that provides a flexible description of a class of quintessence models (with no phantom crossing), along with $w_{dm}$ free, is even mildly favored over the phantom-crossing $w_0w_a$ model according to both the best-fit $\chi^2$ and the DIC under both CMB treatments. One can conclude that the apparent preference for phantom crossing may instead reflect deviations in the dark-matter sector rather than dark-energy dynamics alone. [abridged]
toXiv_bot_toot

🇺🇦 #NowPlaying on BBCRadio3's #ThisClassicalLife
Antonio Vivaldi, Simon Standage, Micaela Comberti, Jaap ter Linden, The English Concert & Trevor Pinnock:
🎵 Concerto for 2 violins and cello in G minor, RV 578 from L'estro armonico
https://open.spotify.com/track/5eiysiGVYiQcXZUbaZQ4pI