Tootfinder

The Serial Port’s new video on IRC is good.
I’d been on IRC of some sort, nearly constantly from ~1992 to 2024, and I learned some things from this documentary.
For example, I knew EFNet was Eris-Free net, but I didn’t know that Eris was a rogue server at Berkeley. Makes sense in hindsight. Always thought it was free as in freedom, not free as in exclusive.
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Thermal-orbital evolution of Eris
Ryunosuke Akiba, Francis Nimmo
https://arxiv.org/abs/2508.16532 https://arxiv.org/pdf/2508.16532

Thermal-orbital evolution of Eris
The large Kuiper Belt object (KBO) Eris is nearly as big as Pluto and has a small moon, Dysnomia. Constraints on the system's spin and orbit characteristics were recently used to argue for a dissipative Eris, requiring a differentiated structure but not necessarily a subsurface ocean. Here, we model the thermal history of Eris coupled to its spin-orbital evolution, finding a subsurface ocean is preferred in order for Eris to be sufficiently dissipative. Spinning down Eris without an ocean is di…

Unveiling a protoplanet candidate embedded in the HD 135344B disk with VLT/ERIS / VLT/ERIS Observations of the V960 Mon System - a Dust-embedded Substellar Object Formed by Gravitational Instability? #planet sculpting the dust around it: https://www.eso.org/public/news/eso2513/

VLT/ERIS observations of the V960 Mon system: a dust-embedded substellar object formed by gravitational instability?
Anuroop Dasgupta, Alice Zurlo, Philipp Weber, Francesco Maio, Lucas A. Cieza, Davide Fedele, Antonio Garufi, James Miley, Prashant Pathak, Sebasti\'an P\'erez, Veronica Roccatagliata
https://arxiv.org/abs/…

VLT/ERIS observations of the V960 Mon system: a dust-embedded substellar object formed by gravitational instability?
V960~Mon is an FU Orionis object that shows strong evidence of a gravitationally unstable spiral arm that is fragmenting into several dust clumps. We report the discovery of a new substellar companion candidate around this young star, identified in high-contrast $L'$-band imaging with VLT/ERIS. The object is detected at a projected separation of $0.898 \pm 0.01$ arcseconds with a contrast of $(8.39 \pm 0.07) \times 10^{-3}$. The candidate lies close to the clumps previously detected in the sub-…

Revolutionizing Validation and Verification: Explainable Testing Methodologies for Intelligent Automotive Decision-Making Systems
Halit Eris, Stefan Wagner
https://arxiv.org/abs/2506.16876

Revolutionizing Validation and Verification: Explainable Testing Methodologies for Intelligent Automotive Decision-Making Systems
Autonomous Driving Systems (ADS) use complex decision-making (DM) models with multimodal sensory inputs, making rigorous validation and verification (V&V) essential for safety and reliability. These models pose challenges in diagnosing failures, tracing anomalies, and maintaining transparency, with current manual testing methods being inefficient and labor-intensive. This vision paper presents a methodology that integrates explainability, transparency, and interpretability into V&V processes. W…

Eris tossing an apple of discord into the FOSS conference that reads "for the most functional" (last word scratched off), then mysteriously disappearing

Block Tensor Decomposition: A dual grid scheme with formal O(N3) for THC decomposition of molecular systems
Yueyang Zhang, Xuewei Xiong, Wei Wu, Peifeng Su
https://arxiv.org/abs/2506.19392

Block Tensor Decomposition: A dual grid scheme with formal O(N3) for THC decomposition of molecular systems
Accurate and fast treatment of electron-electron interactions remains a central challenge in electronic structure theory because post-Hartree-Fock methods often suffered from the computational cost for 4-index electron repulsion integrals (ERIs). Low-rank approaches such as tensor hyper-contraction (THC) and interpolative separable density fitting (ISDF) have been proposed for Hartree-Fock exchange and correlation's calculations. Their application to molecular systems remains inefficient due to…

A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
S. de Wet, G. Leloudas, D. Buckley, N. Erasmus, P. J. Groot, E. Zimmerman
https://arxiv.org/abs/2507.11131

A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
Type IIb supernovae (SNe) are a transitional subclass of stripped-envelope SNe showing hydrogen lines in their spectra that gradually weaken and give way to helium lines reminiscent of SNe Ib, which is indicative of stripping through stellar winds or binary interaction. SN 2024abfo is the seventh SN IIb with a direct progenitor detection. We find that the position of the supernova in our ERIS adaptive optics imaging agrees with the progenitor position in archival HST imaging to within 19 mas. T…

Replaced article(s) found for q-bio.GN. https://arxiv.org/list/q-bio.GN/new
[1/1]:
- Rawsamble: Overlapping and Assembling Raw Nanopore Signals using a Hash-based Seeding Mechanism
Firtina, Mordig, Mustafa, Goswami, Ghiasi, Mercogliano, Eris, Lindegger, Kahles, Mutlu