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@nobodyinperson@fosstodon.org
2026-08-19 14:31:17

Holy cow, remember to clean your #uv cache from time to time, folks 😅
UPDATE: Seems to contain some links, deleting the cache only freed like 9GiB, but still...
#Python

/home/yann/.cache/uv/
27,6 GiB
505.110 Dateien (15 %)
@heiseonline@social.heise.de
2026-08-13 14:33:03

heise | UV-Messgeräte im Test: Was sie tatsächlich leisten und wo sie schwächeln
Zu viel Sonne und UV-Licht sind für die Haut gefährlich. Gadgets können die Belastung messen und warnen, wenn sie zu hoch wird. Wir stellen ein paar davon vor.

@publicvoit@graz.social
2026-07-28 15:51:06

#Python #uv users on #Debian: I've been using this setup:
apt install extrepo
extrepo enable uv
apt install uv
That worked perfectly for all local users using standard Debian package management …

@hynek@mastodon.social
2026-07-25 11:45:12

Based on the linked research by Charlie Marsh, here's setup-cached-uv 2.6.0 that doesn't run `uv cache prune --ci` by default anymore: github.com/hynek/setup-cached-

@Dragofix@veganism.social
2026-09-17 01:15:01

Microplastics fall across rural Switzerland, adding over 200 tons yearly to land and water phys.org/news/2026-09-micropla

@primonatura@mstdn.social
2026-09-16 12:00:17

"Microplastics fall across rural Switzerland, adding over 200 tons yearly to land and water"
#Switzerland #Plastic #Plastics

@michabbb@social.vivaldi.net
2026-08-16 20:30:03

🧠 Routing strategies: LLM-as-classifier, signal-driven stage router, escalation router (weak tier first, a judge decides whether to escalate), random split for A/B tests, or a custom algorithm you write yourself
🚀 Launcher path: uv tool install "nemo-switchyard[cli]", then switchyard launch claude --model switchyard to point #ClaudeCode, Codex CLI or OpenClaw at an open-sou…

@arXiv_astrophGA_bot@mastoxiv.page
2026-07-21 09:39:22

Replaced article(s) found for astro-ph.GA. arxiv.org/list/astro-ph.GA/new
[2/3]:
- Hunting Wandering 3<z<8 Black Holes: Spatial Offsets in Ionization Ratio and Continuum Emission
Urvi Thakurdesai, et al.
arxiv.org/abs/2606.30715 mastoxiv.page/@arXiv_astrophGA
- Spectral Energy Distributions of Globular Clusters in VV191a
Ashton Cardona, et al.
arxiv.org/abs/2607.10352 mastoxiv.page/@arXiv_astrophGA
- The different methods to calculate cluster membership probabilities
Tahereh Ramezani, Prapti Mondal, Katerina Neumannova, Ernst Paunzen, Johana Supikova, Gabriel Szasz
arxiv.org/abs/2607.13711 mastoxiv.page/@arXiv_astrophGA
- On the current status of tidal tails of Galactic open clusters
Tahereh Ramezani, Prapti Mondal, Katerina Neumannova, Ernst Paunzen, Johana Supikova, Gabriel Szasz
arxiv.org/abs/2607.13747 mastoxiv.page/@arXiv_astrophGA
- The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stri...
Bethany Ludwig, Maria R. Drout, Ylva Gotberg, Dustin Lang, Alexander Laroche
arxiv.org/abs/2505.18632 mastoxiv.page/@arXiv_astrophSR
- Observable signature of magnetic tidal coupling in hierarchical triple systems
Marta Cocco, Gianluca Grignani, Troels Harmark, Marta Orselli, Davide Panella, Daniele Pica
arxiv.org/abs/2510.24897 mastoxiv.page/@arXiv_grqc_bot/
- Periodic Gravitational Lensing with Oscillating Boson Stars
Xing-Yu Yang, Tan Chen, Rong-Gen Cai
arxiv.org/abs/2511.19606 mastoxiv.page/@arXiv_grqc_bot/
- Search for Dark Matter Annihilation and Decay with H$\alpha$ Line Emission
Rebecca K. Leane
arxiv.org/abs/2512.09019 mastoxiv.page/@arXiv_hepph_bot
- Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors
Anton Chudaykin, Mikhail M. Ivanov, Oliver H. E. Philcox
arxiv.org/abs/2602.18554 mastoxiv.page/@arXiv_astrophCO
- Can wormholes have vanishing Love numbers?
Shauvik Biswas
arxiv.org/abs/2605.03025 mastoxiv.page/@arXiv_grqc_bot/
toXiv_bot_toot

@nobodyinperson@fosstodon.org
2026-07-16 08:22:34

> nix shell nixpkgs#uv
copying "/nix/store/0lgkd7b0s5ykklkijr9g62r832qdvgvx-nixos-25.05.20250622.c7ab752/nixos" to the store
Why does it take 30 seconds to (uselessly) copy something from the nix store to the nix store?
#nix #nixos

@michabbb@social.vivaldi.net
2026-09-13 00:59:34

🐍 Python 3.11 , MIT licensed, installs via uv or pipx. Runs natively on Windows with optional DPAPI master-key wrapping
#credentials

@tinoeberl@mastodon.online
2026-09-01 08:10:09

#China testet mit Jilin-2 eine schwimmende #Photovoltaik-Anlage auf einer Plattform aus Holz-Bambus-Verbundmaterial.
Die 100-Kilowatt-Anlage soll zeigen, wie widerstandsfähig das Material gegen Wellen, Wind, Salz und UV-Strahlung ist.
Ob der Verbundstoff tatsächlich umweltfreundlicher…

@arXiv_hepth_bot@mastoxiv.page
2026-08-07 08:21:17

Three-Loop Five-Point CK-Dual Amplitudes and UV Structure in N=4 SYM and N=8 SUGRA
Zhiming Cai, Zeyu Li, Gang Yang, Guorui Zhu
arxiv.org/abs/2608.05973 arxiv.org/pdf/2608.05973 arxiv.org/html/2608.05973
arXiv:2608.05973v1 Announce Type: new
Abstract: We construct the complete full-color three-loop five-point integrand of N=4 super-Yang--Mills theory in a representation that manifestly satisfies color--kinematics duality. Its double copy gives the corresponding N=8 supergravity integrand. For four-dimensional external states, we evaluate the ultraviolet poles of both amplitudes in the critical dimension, Dc=6. Extending the external-state dependence to D dimensions is subtle. We consider a candidate replacement of the four-dimensional prefactors by expressions built from D-dimensional tree amplitudes. It reproduces the open-string prediction for the SYM pole with generic D-dimensional external states, whereas the corresponding gravity expression differs from the string-inspired one by an evanescent term.
toXiv_bot_toot

@veit@mastodon.social
2026-06-25 05:49:24

#TIL that there is also a pre-commit check for uv audit: python4data.science/en/latest/

@thomasfuchs@hachyderm.io
2026-07-17 14:08:48

⚠️ PSA: Even when smoke (e.g. from wildfires) filters light, looking directly into the sun is harmful to you—the smoke particles do not filter all wavelengths evenly and the UV light from the sun still gets focused by your eye lens and will injure your eyes.

@primonatura@mstdn.social
2026-08-05 18:00:58

"The biodegradable, self-cleaning fabric made from living caterpillar fungus"
#Textiles #Fabric

@@arXiv_physicsatomph_bot@mastoxiv.page@mastoxiv.page
2026-07-08 08:02:53

Ionization-free femtosecond UV pulse filamentation resulting from non-perturbative Kerr effect saturation due to transient photoexcitation of molecules
V. V. Strelkov, A. V. Shutov, V. D. Zvorykin
arxiv.org/abs/2607.06325

@arXiv_hepth_bot@mastoxiv.page
2026-08-07 08:21:17

Three-Loop Five-Point CK-Dual Amplitudes and UV Structure in N=4 SYM and N=8 SUGRA
Zhiming Cai, Zeyu Li, Gang Yang, Guorui Zhu
arxiv.org/abs/2608.05973

@michabbb@social.vivaldi.net
2026-08-23 21:03:25

💻 ft shell for chatting locally, attach mode needs no GPU and can drive a server on another machine, and ft launch wires up agents like claude, codex or opencode
🖥️ Install from source with uv, or download the Windows/Linux build at flashml.ai

@arXiv_astrophGA_bot@mastoxiv.page
2026-07-22 08:11:07

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity
Elie Cueto, Anne Hutter
arxiv.org/abs/2607.18868 arxiv.org/pdf/2607.18868 arxiv.org/html/2607.18868
arXiv:2607.18868v1 Announce Type: new
Abstract: To investigate the origins of the high abundance of UV-bright galaxies at z > 10, we present a new semi-analytic model that bridges the gap between small-scale star formation physics and large-scale galaxy evolution by explicitly tracking discrete star-forming clouds within smoothly evolving dark matter potentials. Unlike conventional semi-analytic models, our approach naturally captures the stochasticity of star formation, allowing us to isolate how cloud properties, star formation efficiencies (SFEs), and stellar initial mass functions (IMFs) shape the star-formation burstiness of early galaxies. Clouds are drawn sequentially from a cloud mass distribution, assigned an SFE and IMF depending on cloud mass, metallicity, and redshift, and evolve under the influence of short-timescale stellar feedback. We identify three distinct star formation regimes arising from the interplay between cloud masses, densities, and feedback timescales: a stochastic, feedback-limited regime in low-mass halos with long quiescent phases; a bursty regime regulated by the cloud mass distribution; and a smooth, continuous regime in massive halos. Our fiducial model adopts a dynamic IMF, an SFE linked to cloud properties and the IMF, and massive, moderately dense clouds. Varying assumptions reveals that top-heavy IMFs and enhanced SFEs in massive clouds amplify burstiness, while altering the upper cloud mass or density normalisation is secondary. Among model ingredients, the IMF most strongly impacts the UV luminosity function (LF), while switching to a constant SFE boosts the faint end, and reducing the maximum cloud mass decreases the bright end. These results demonstrate that cloud-scale physics critically shape early galaxy UV luminosity distributions.
toXiv_bot_toot

@arXiv_csGR_bot@mastoxiv.page
2026-07-22 08:35:12

Crosslisted article(s) found for cs.GR. arxiv.org/list/cs.GR/new
[1/1]:
- Vakonomic Fluids
Ritoban Roy-Chowdhury, Mohammad Sina Nabizadeh, Oliver Gross, Anthony Gruber, Albert Chern
arxiv.org/abs/2607.18312 mastoxiv.page/@arXiv_mathph_bo
- ECoNGS: Efficient Compressive Neural Gaussian Splats for Volume Visualization
Kaiyuan Tang, Chaoli Wang
arxiv.org/abs/2607.18466 mastoxiv.page/@arXiv_csCV_bot/
- UVFaceFusion: Fast Multi-view Topologically Consistent Face Reconstruction in the Wild via UV-spa...
Xin Ming, Yuxuan Han, Junhai Yong, Feng Xu
arxiv.org/abs/2607.18798 mastoxiv.page/@arXiv_csCV_bot/
- Appearance Pointers -- Multimodal Region Control of Diffusion Transformers
Rahul Sajnani, Yulia Gryaditskaya, Radom\'ir M\v{e}ch, Srinath Sridhar, Matheus Gadelha
arxiv.org/abs/2607.19344 mastoxiv.page/@arXiv_csCV_bot/
toXiv_bot_toot

@primonatura@mstdn.social
2026-06-23 11:00:30

"Summer solstice heatwave grips much of Europe as France restricts alcohol consumption"
#Europe #France #Heatwave #Climate