Tootfinder

2025 NFL playoff picture: What Cowboys-Lions means for NFC seeding, wild-card chaos and teams on the bubble

https://www.cbssports.com/nfl/news/nfl-playoff-picture-standings-2025/

Can anyone recommend a tool for basically mass unfollowing Fediverse/Mastodon accounts or otherwise managing your followings?
I'm following almost 2000 accounts and while my feed is very much alive and buzzing, it feels like it doesn't really match my interests. It's too generic.
I need to weed out what I actually care about. Is there anything that can help with that?
#Mastodon

Our brains are shrinking

@… I totally ignored Facebook for three years or so.
I'm not sure why I revisited this year, it was probably to tell whether someone is still alive, after one of my 'death-of-friends-and-family' nightmares.
I found only two acquaintances dead, and one in a wheelchair following a stroke … not too bad, given our ages and the length of time th…

Work Function Mapping Across a-In2Se3 to {\alpha}-In2Se3 to {\gamma}-InSe in RF-Sputtered Thin Films
Marius O. Eji, Md. Sakauat Hasan Sakib, Joseph P. Corbett
https://arxiv.org/abs/2510.08767

Work Function Mapping Across a-In2Se3 to α-In2Se3 to γ-InSe in RF-Sputtered Thin Films
Indium selenide is a phase-change chalcogenide whose polymorphism enables a variety of physical properties to be tuned. Here we directly quantify the evolution of the surface work function across the amorphous-to-crystalline transition in RF-sputtered In2Se3 thin films grown on c-plane Al2O3 (001). By varying deposition temperature (100-500 °C) and film thickness, we establish processing windows for a- In2Se3, α-In2Se3, and γ-InSe, and correlate structure with electronic and morphological pr…

Direct observation of the X-ray counterpart of the H{\alpha} filaments and of the sloshing spiral in the Perseus galaxy cluster
Adrien Picquenot, Fabio Acero, Valeria Olivares, Michela Negro, Gabriel W. Pratt
https://arxiv.org/abs/2510.09559

Direct observation of the X-ray counterpart of the Hα filaments and of the sloshing spiral in the Perseus galaxy cluster
Deep Chandra observations of the Perseus galaxy cluster have allowed for the discovery of X-ray counterparts to the Hα filamentary structures and of a sloshing spiral. However, both components are extremely faint, and their study is largely hindered by the volume-filling hot intracluster medium (ICM). Using the Poisson General Morphological Component Analysis (pGMCA) algorithm, a blind source separation method adapted for Poissonian statistics, we were able to extract detailed, clean morpholog…