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@arXiv_astrophHE_bot@mastoxiv.page
2025-07-04 08:30:01

Multi-messenger observations of binary neutron star mergers: synergies between the next generation gravitational wave interferometers and wide-field, high-multiplex spectroscopic facilities
S. Bisero, S. D. Vergani, E. Loffredo, M. Branchesi, N. Hazra, U. Dupletsa, R. I. Anderson
arxiv.org/abs/2507.02055

@jensilber@mastodon.social
2025-05-30 23:59:00

Geniuses, all of them. apnews.com/video/fort-bragg-ba

In a laboratory setting, humans have accelerated particles — protons, antiprotons, electrons, and positrons — to incredibly high energies: up to the TeV (trillions of electron-volts) scale.

But cosmic rays, also including protons, electrons, and other atomic nuclei, are produced up to far greater energies, at the PeV (quadrillions of electron-volts) scale and beyond.

These very high energy cosmic rays are produced somewhere in our own galaxy:
in natural, astrophysical…

@arXiv_astrophSR_bot@mastoxiv.page
2025-06-09 08:40:52

The TESS Ten Thousand Catalog: 10,001 uniformly-vetted and -validated Eclipsing Binary Stars detected in Full-Frame Image data by machine learning and analyzed by citizen scientists
Veselin B. Kostov, Brian P. Powell, Aline U. Fornear, Marco Z. Di Fraia, Robert Gagliano, Thomas L. Jacobs, Julien S. de Lambilly, Hugo A. Durantini Luca, Steven R. Majewski, Mark Omohundro, Jerome Orosz, Saul A. Rappaport, Ryan Salik, Donald Short, William Welsh, Svetoslav Alexandrov, Cledison Marcos da Si…