Paris : les papys dealers renouent avec leurs vielles habitudes et retournent en prison - Le Parisien
https://www.leparisien.fr/paris-75/paris-les-papys-dealers-renoue…
Fuzzing BusyBox: Leveraging LLM and Crash Reuse for Embedded Bug Unearthing
Asmita, Yaroslav Oliinyk, Michael Scott, Ryan Tsang, Chongzhou Fang, Houman Homayoun
https://arxiv.org/abs/2403.03897
Some direct and inverse problems for the Restricted Signed sumset in set of integers
Mohan, Raj Kumar Mistri, Ram Krishna Pandey
https://arxiv.org/abs/2403.03625
Ça semble être beaucoup de milliards pour des infrastructures routières quand on sait que le #REM va bientôt arriver. C’est comme si on savait que ça sera pas assez utilisé.
Aéroport Montréal-Trudeau | Décollage d’un plan « ambitieux » pour la fluidité
It’s not wrong. But it’s not right, either.
“Creating Fluid Typography with the CSS clamp() Function”
https://www.sitepoint.com/fluid-typography-css-clamp-function/#:~…
Hey friends! We just came back from a great hike near #garmischpartenkirchen. We wanted to do this mountain recently but the snow in the upper part was too risky for us.
Today we went there again. Beautiful ascent, nice views. Some spray rain and a slippery, dirty descent. But at the end we even had some sun!
Now we feel tired and a bit sore 😉
Characterizing the 3D Structure of Molecular Cloud Envelopes in the "Cloud Factory" Simulations
Elijah Mullens, Catherine Zucker, Claire E. Murray, Rowan Smith
https://arxiv.org/abs/2403.03112 https://arxiv.org/pdf/2403.03112
arXiv:2403.03112v1 Announce Type: new
Abstract: We leverage recent numerical simulations of highly resolved star-forming regions in a Milky Way-like Galaxy to explore the nature of extended gaseous envelopes around molecular clouds. We extract a sample of two dozen star-forming clouds from the feedback-dominated suite of the "Cloud Factory'' simulations. With the goal of exploring the 3D thermal and chemical structure of the gas, we measure and fit the clouds' radial profiles in multiple tracers, including $n_{H_I}$, $n_{H_2}$, $n_{H_{tot}}$, $n_{CO}$, and gas temperature. We find that while solar neighborhood clouds recently detected via 3D dust mapping have radially symmetric, low-density envelopes that extend $\sim$ 10-15 pc, the simulated cloud envelopes are primarily radially asymmetric with low-density envelopes that extend only $\sim$ 2-3 pc. One potential explanation for the absence of extended envelopes in the simulated clouds may be the lack of magnetic fields, while a stronger local feedback prescription compared to solar neighborhood conditions may drive the radially asymmetric cloud morphologies. We make the pipeline to extract and characterize the radial profile of clouds publicly available, which can be used in complementary and future simulations to shed additional light on the key physics shaping the formation and evolution of star-forming structures in the Milky Way.
XAI-Based Detection of Adversarial Attacks on Deepfake Detectors
Ben Pinhasov, Raz Lapid, Rony Ohayon, Moshe Sipper, Yehudit Aperstein
https://arxiv.org/abs/2403.02955
Risk-Sensitive Mean Field Games with Common Noise: A Theoretical Study with Applications to Interbank Markets
Xin Yue Ren, Dena Firoozi
https://arxiv.org/abs/2403.03915
CoRMF: Criticality-Ordered Recurrent Mean Field Ising Solver
Zhenyu Pan, Ammar Gilani, En-Jui Kuo, Zhuo Liu
https://arxiv.org/abs/2403.03391 https://