"Transparenz ist damit nicht das Ziel, sondern das Ermöglichungsmedium für die Autonomie der Lernenden." @…
https://
Packed house at the @… Summit in Berlin. @… was definitely involved way ahead of the hype. 😎 #SCSSUMMIT2026
Memo: the Army CIO reinstates limits on Army members' AI token usage; docs show the DOD's Ask Sage tool can access 100M tokens via an annual "enterprise pack" (Vittoria Elliott/Wired)
https://www.wired.com/story/the-army-is-burning-through-its-ai-toke…
Buddhist Ways of Being Human in the Age of AI
https://ift.tt/6imDOHM
Journal of Italian Cinema & Media Studies 8.1 is now available Intellect is happy to…
via Input 4 RELCFP https://
Klint Kubiak Presser - 5.20.26 https://www.youtube.com/watch?v=9bddxs4CDW0
Buddhist Ways of Being Human in the Age of AI
https://ift.tt/Hr6BG3D
Journal of Italian Cinema & Media Studies 8.1 is now available Intellect is happy to…
via Input 4 RELCFP https://
HOLY FRIJOLES. Remasters, multiple Fallout releases, completely new games & even new TV shows...
I'll bet $1000 Asha pointed a gun at anyone at Xbox not working on CoD, WoW or Candy Crush.
▶️ Bethesda's MASSIVE Fallout Announcements...
https://youtube.com/watch?v=1DS_we0lo2
🇺🇦 #NowPlaying on BBCRadio3's #EssentialClassics
Isaías Sšvio & Miloš Karadaglić:
🎵 Batacuda
#IsaíasSávio #MilošKaradaglić
https://open.spotify.com/track/4w6ZBjPWvjXENSk1VlPjCb
The Large Magellanic Cloud through the lens of the James Webb Space Telescope: Binaries and the mass function in the galaxy's outskirts
M. V. Legnardi, F. Muratore, A. P. Milone, G. Cordoni, E. Dondoglio, L. N. Gorza, A. Bellini, F. Calura, S. Jang, H. Jerjen, A. Karakas, E. P. Lagioia, C. Li, A. Mastrobuono-Battisti, M. Tailo, E. Vesperini, E. Bortolan, A. F. Marino, S. Di Stefano
https://arxiv.org/abs/2607.19260 https://arxiv.org/pdf/2607.19260 https://arxiv.org/html/2607.19260
arXiv:2607.19260v1 Announce Type: new
Abstract: Nearby galaxies such as the Large Magellanic Cloud (LMC) offer an ideal laboratory to test the initial mass function under different physical conditions, but previous works have been limited by photometric depth and have therefore poorly constrained the low-mass regime. Here, we analyze ultra-deep James Webb Space Telescope observations of a field in the LMC outskirts, near the intermediate-age and massive star cluster NGC 1846. Using the $m_{\rm F322W2}$ versus $m_{\rm F115W}-m_{\rm F322W2}$ color-magnitude diagram, we derive the mass function (MF) down to unprecedentedly low masses ($M=0.17 M_{\odot}$), explicitly accounting for the contribution of unresolved binaries, whose fraction is constrained directly from the data. For systems with mass ratios $q>0.6$, we measure a binary fraction of $f_{\rm bin}^{q>0.6}=0.15\pm0.01$, implying a total binary fraction of $f_{\rm bin}^{\rm TOT}=0.34\pm0.02$ for a flat mass-ratio distribution. This is consistent with values in the Small Magellanic Cloud (SMC) and in the Milky Way field, suggesting similar binary formation efficiency across low-density environments. We also derive the MF over the mass interval 0.17-0.82 $M_{\odot}$ and fit it with a power law, obtaining a slope of $\alpha = -1.49 \pm 0.16$. This slope is shallower than the canonical Salpeter value ($\alpha=-2.35$) and slightly shallower than that measured in the SMC field, while remaining consistent with determinations for Galactic open clusters and for several clusters in the Magellanic Clouds and the Milky Way. Together, these results support a scenario in which both binary formation efficiency and the shape of the low-mass MF depend only weakly on the environment.
toXiv_bot_toot