Tootfinder

Replaced article(s) found for physics.ins-det. https://arxiv.org/list/physics.ins-det/new
[1/1]:
- A tunable photonic band gap resonator for axion dark matter searches
Lewis, Goulart, Barbosa, Jois, Leder, Sindhwad, Urdinaran, van Bibber
https://arxiv.org/abs/2408.03861 https://mastoxiv.page/@arXiv_physicsinsdet_bot/112925197817813337
- Optimization of Cryogenic Detector Test Station by Rejecting Electromagnetic Interference
Sangbaek Lee, Whitney Armstrong, Maximo DiPreta, Jacob Dulya, Valentine Novosad, Tomas Polakovic
https://arxiv.org/abs/2601.03158 https://mastoxiv.page/@arXiv_physicsinsdet_bot/115852984138241851
- Valley-peak modulation in phase space: a law-invariant VPM and its theta-function structure
Aaron J. Hendrickson, David P. Haefner
https://arxiv.org/abs/2603.01199 https://mastoxiv.page/@arXiv_physicsinsdet_bot/116164317738741185
- Pushing the Limits of Pulse Shape Discrimination in a Large Liquid Xenon Detector
D. S. Akerib, et al.
https://arxiv.org/abs/2603.26877 https://mastoxiv.page/@arXiv_physicsinsdet_bot/116322766877175621
- Cherenkov and scintillation light separation in BGO and BSO crystals coupled to SiPMs for dual-re...
M. Alviggi, et al.
https://arxiv.org/abs/2604.09918 https://mastoxiv.page/@arXiv_physicsinsdet_bot/116402026414652810
- Small but Tubby: A Magnetic Loop Antenna Made from 100 mm Copper Tubing
Peter M\"arki, Markus Niese
https://arxiv.org/abs/2607.10828 https://mastoxiv.page/@arXiv_physicsinsdet_bot/116917273903663314
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https://www.space.com/astronomy/mars/significant-areas-of-mars-may-have-once-been-covered-by-water-scientists-find-hidden-clue-in-spirit-rover-data

Ocular speech tracking persists in blindness, but its dynamics and oculo-cerebral connectivity depend on visual status https://www.eneuro.org/content/early/2026/06/23/ENEURO.0041-26.2026 "ocular speech tracking seems to respond selectively to acoustic features o…

Ocular speech tracking persists in blindness, but its dynamics and oculo-cerebral connectivity depend on visual status
While eye movements have been shown to track the speech envelope, it is unknown whether this reflects a hard-wired mechanism or one shaped by (lifetime) audiovisual experience. Further, questions remain about whether ocular tracking is modulated by speech intelligibility and which brain regions drive these synchronized eye movements. Here, we investigate ocular speech tracking in 47 (20 male), blindfolded early blind, late blind, and sighted individuals using magnetoencephalography (MEG) and so…

headed to the post office to mail a couple mix tapes to ypsilanti and rockingham (va)

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

Let's play a game:
Post the oldest image of your "battle station" / computer setup that you have.
Ideally, post some specs of the system if you can remember.
I'll start:
- photo from 2003
- Pentium II, 350MHz
- 3DFX Voodoo Banshee
- 1024x768 17" Eizo CRT
- Iomega Zip drive, 100MB via Parallel port (*click!*)
- SCSI Scanner hidden away in the background
I think the Mac was a Power Macintosh 6300, but I'm not 100…

so I used to sell themed magnetic poetry sets I made on my etsy but my shops been closed for a while, anyway I made a very basic internet version of my Glitch in the Matrix set that's live now.
doesn't work on mobile sry but ye
https://iantheonline.neocities.org/magnet…

Sea level rise is speeding up and scientists now know exactly why #environment

Sea level rise is speeding up and scientists now know exactly why
The world’s oceans are rising at an accelerating pace, and scientists now say they can fully explain what’s driving it. Warming seawater is the biggest factor, while melting glaciers and polar ice sheets are increasingly pouring more water into the oceans each year. Researchers also solved a puzzling mismatch in sea level measurements that had lingered for years.

Crosslisted article(s) found for astro-ph.GA. https://arxiv.org/list/astro-ph.GA/new
[1/2]:
- From Triadic Interactions to Kolmogorov Scaling: A Deterministic, Scale-Resolved Formulation of E...
Erik Bertram
https://arxiv.org/abs/2607.16381 https://mastoxiv.page/@arXiv_physicsfludyn_bot/116956890026314972
- Dynamical friction in stratified stellar envelopes
Damien Gagnier
https://arxiv.org/abs/2607.16422 https://mastoxiv.page/@arXiv_astrophSR_bot/116956909457047933
- Simultaneous radio, optical and X-ray monitoring of hard X-ray selected AGN: a variability study
L. Hern\'andez-Garc\'ia, F. Panessa, D. Williams-Baldwin, P. Ar\'evalo, A. M. Mu\~noz Arancibia
https://arxiv.org/abs/2607.16423 https://mastoxiv.page/@arXiv_astrophHE_bot/116956887664818723
- Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster
Muhammed K{\i}yami Erdim
https://arxiv.org/abs/2607.16496 https://mastoxiv.page/@arXiv_astrophCO_bot/116956868365097623
- Determination of [Fe/H] in Fundamental mode Classical Cepheids from Gaia DR3 light curve Fourier ...
Roberto Molinaro, et al.
https://arxiv.org/abs/2607.16775 https://mastoxiv.page/@arXiv_astrophSR_bot/116956927940159880
- Escaped White Dwarf Candidates from Open Clusters
Huahui Yan, David R. Miller, Jingkun Zhao, Jincheng Guo, Chengyuan Li
https://arxiv.org/abs/2607.16815 https://mastoxiv.page/@arXiv_astrophSR_bot/116956930692481290
- Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity...
M. Fern\'andez-L\'opez, et al.
https://arxiv.org/abs/2607.17160 https://mastoxiv.page/@arXiv_astrophSR_bot/116956996786764707
- Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
Jun-Rong Liu, Hua Feng, Luis C. Ho
https://arxiv.org/abs/2607.17448 https://mastoxiv.page/@arXiv_astrophHE_bot/116956954089426787
- Binary White Dwarfs as Gravitational Wave Sources for LISA
Sreeta Roy, Surajit Kalita, Tomasz Bulik, Dorota Gondek-Rosi\'nska
https://arxiv.org/abs/2607.17787 https://mastoxiv.page/@arXiv_astrophSR_bot/116957044926341801
- Intracluster light and dark matter halo shapes reflect common assembly, not mutual coupling: shap...
Martin, Hatch, Cui, Fernandez, Bah\'e, Fischer, Montes, Pearce, Sabiu, Yepes, Yoo
https://arxiv.org/abs/2607.17792 https://mastoxiv.page/@arXiv_astrophCO_bot/116956974931041178
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i'm finna mail out some mix tapes this weekend so heads up michigan (ann arbor, ann arbor, and birmingham) and california (LA, oakland, SF).
hey, check out the splatter!