Tootfinder

bruh I tried migrating my bsky account to my own PDS but for some reason bsky app won't load my profile no matter what even tho querying the profile record directly using goat indicates that my profile still exists in my PDS, why is it not resolving correctly in the endpoint that bsky app view uses??? it's so baffling to me
in any case this is my current account for now https://bsky.app/profile/minot.dev since twatter decided to go straight to hell just when I wanted to be more active again

I’m excited to see the return of Steam Machine.
With my experiments of using the Linux Desktop mode with the Steamdeck … this absolutely puts a full Linux server in a lot of homes.
A good spot for a PDS, Tailscale, and a bunch of other things.
https://bsky.app/profile/jaypeters.net

Jay Peters (@jaypeters.net)
If you want some video of the new Steam Controller and Steam Machine (a Valve-made PC for the living room!), check out this that @seanhollister.bsky.social and I made together!

On The Orbital Evolution of Multiple Wide Super-Jupiters: How Disk Migration and Dispersal Shape the Stability of The PDS 70 System
Clarissa R. Do \'O, Jaehan Bae, Quinn M. Konopacky, Jayke S. Nguyen, Patrick Diamond, Krzysztof Go\'zdziewski, Dawid Jankowski
https://arxiv.org/abs/2510.11021…

On The Orbital Evolution of Multiple Wide Super-Jupiters: How Disk Migration and Dispersal Shape the Stability of The PDS 70 System
Direct imaging has revealed exoplanet systems hosting multiple wide-orbit Super-Jupiters, where planet-planet interactions can shape their long-term dynamical evolution. These strong perturbations may lead to orbital instability, raising questions about the long-term survival of such systems. Shortly after formation, planet-disk interactions can shepherd planets into mean-motion resonances, which may promote long-term stability as seen in HR 8799. However, early-stage processes such as disk pho…

Hunt for the mHz variability in the TESS and XMM-Newton observations of nova-like cataclysmic variables
Andrej Dobrotka, Jozef Magdolen, Martin Melicher\v{c}\'ik
https://arxiv.org/abs/2510.02834

Hunt for the mHz variability in the TESS and XMM-Newton observations of nova-like cataclysmic variables
We analysed the flickering of selected nova-like cataclysmic variables observed by the TESS satellite and XMM-Newton. We searched for break frequencies ($f_{\rm b}$) in the corresponding power density spectra (PDS), and for any long-term evolution. We found a new optical $f_{\rm b}$ in three nova-like systems and confirmed that the value of this frequency is clustered around 1 mHz. V504 Cen and V751 Cyg show possible X-ray counterparts of $f_{\rm b}$ that had previously only been seen in MV Lyr…

exaPD: A highly parallelizable workflow for multi-element phase diagram (PD) construction
Feng Zhang, Zhuo Ye, Maxim Moraru, Ying Wai Li, Weiyi Xia, Yongxin Yao, Ryan Richard, Cai-Zhuang Wang
https://arxiv.org/abs/2510.01400

exaPD: A highly parallelizable workflow for multi-element phase diagram (PD) construction
Phase diagrams (PDs) illustrate the relative stability of competing phases under varying conditions, serving as critical tools for synthesizing complex materials. Reliable phase diagrams rely on precise free energy calculations, which are computationally intensive. We introduce exaPD, a user-friendly workflow that enables simultaneous sampling of multiple phases across a fine mesh of temperature and composition for free energy calculations. The package employs standard molecular dynamics (MD) a…