Tootfinder

#CabooseDay
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Season 5 Episode 7 "Someone To Baywatch Over You"
#Baywatch

Liberal Entity Matching as a Compound AI Toolchain
Silvery D. Fu, David Wang, Wen Zhang, Kathleen Ge
https://arxiv.org/abs/2406.11255 https://

Dredge Word, Social Media, and Webgraph Networks for Unreliable Website Classification and Identification
Evan M. Williams, Peter Carragher, Kathleen M. Carley
https://arxiv.org/abs/2406.11423

Dredge Word, Social Media, and Webgraph Networks for Unreliable Website Classification and Identification
In an attempt to mimic the complex paths through which unreliable content spreads between search engines and social media, we explore the impact of incorporating both webgraph and large-scale social media contexts into website credibility classification and discovery systems. We further explore the usage of what we define as \textit{dredge words} on social media -- terms or phrases for which unreliable domains rank highly. Through comprehensive graph neural network ablations, we demonstrate tha…

Simons Observatory: Observatory Scheduler and Automated Data Processing
Yilun Guan, Kathleen Harrington, Jack Lashner, Sanah Bhimani, Kevin T. Crowley, Nicholas Galitzki, Ken Ganga, Matthew Hasselfield, Adam D. Hincks, Brian Keating, Brian J. Koopman, Laura Newburgh, David V. Nguyen, Max Silva-Feaver
https://arxiv.org/abs/2406.1…

Simons Observatory: Observatory Scheduler and Automated Data Processing
The Simons Observatory (SO) is a next-generation ground-based telescope located in the Atacama Desert in Chile, designed to map the cosmic microwave background (CMB) with unprecedented precision. The observatory consists of three small aperture telescopes (SATs) and one large aperture telescope (LAT), each optimized for distinct but complementary scientific goals. To achieve these goals, optimized scan strategies have been defined for both the SATs and LAT. This paper describes a software syste…

On the stability of the $m=1$ rigid ballooning mode in a mirror trap with high-beta sloshing ions
Igor Kotelnikov
https://arxiv.org/abs/2406.10488 https://…

On the stability of the $m=1$ rigid ballooning mode in a mirror trap with high-beta sloshing ions
Stability of the ``rigid'' $m = 1$ ballooning mode in a mirror axisymmetric trap is studied for the case of oblique neutral beam injection (NBI), which creates an anisotropic population of fast sloshing ions. Since small-scale modes with azimuthal numbers $m>1$ in long thin (paraxial) mirror traps are easily stabilized by finite Larmor radius (FLR) effects, suppression of the rigid ballooning and flute modes would mean stabilization of all MHD modes, with the exception of mirror and fire-hose d…

Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
Olivier Mousis, Antoine Schneeberger, Thibault Cavali\'e, Kathleen E. Mandt, Artyom Aguichine, Jonathan I. Lunine, Tom Benest Couzinou, Vincent Hue, Rapha\"el Moreno
https://arxiv.org/abs/2406.11530

Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
Olivier Mousis, Antoine Schneeberger, Thibault Cavali\'e, Kathleen E. Mandt, Artyom Aguichine, Jonathan I. Lunine, Tom Benest Couzinou, Vincent Hue, Rapha\"el Moreno
https://arxiv.org/abs/2406.11530

Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
This study, placed in the context of the preparation for the Uranus Orbiter Probe mission, aims to predict the bulk volatile compositions of Uranus and Neptune. Using a protoplanetary disk model, it examines the evolution of trace species through vapor and solid transport as dust and pebbles. Due to the high carbon abundance found in their envelopes, the two planets are postulated to have formed at the carbon monoxide iceline within the protosolar nebula. The time evolution of the abundances of…

Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
Olivier Mousis, Antoine Schneeberger, Thibault Cavali\'e, Kathleen E. Mandt, Artyom Aguichine, Jonathan I. Lunine, Tom Benest Couzinou, Vincent Hue, Rapha\"el Moreno
https://arxiv.org/abs/2406.11530

Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
This study, placed in the context of the preparation for the Uranus Orbiter Probe mission, aims to predict the bulk volatile compositions of Uranus and Neptune. Using a protoplanetary disk model, it examines the evolution of trace species through vapor and solid transport as dust and pebbles. Due to the high carbon abundance found in their envelopes, the two planets are postulated to have formed at the carbon monoxide iceline within the protosolar nebula. The time evolution of the abundances of…