Tootfinder

This https://arxiv.org/abs/2301.04280 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

Non-thermal radiation from dual jet interactions in supermassive black hole binaries
Supermassive black hole binaries (SMBHBs) are natural by-products of galaxy mergers and are expected to be powerful multi-messenger sources. They can be powered by the accretion of matter and then radiate across the electromagnetic spectrum, much like normal active galactic nuclei (AGNs). Current electromagnetic observatories have a good chance of detecting and identifying these systems in the near future. However, precise observational indicators are needed to distinguish individual AGNs from …

Hey everybody, five minutes until #ListeningClub, everybody! https://www.youtube.com/watch?v=0sINb7e7FiM

Air raids last 16 hours per day on average in Kharkiv Oblast obstructing business operations, governor says: https://benborges.xyz/2024/06/17/air-raids-last.html

Russian attacks on Kharkiv, Kherson oblasts kill 1, injure 3, including 102-year-old woman: https://benborges.xyz/2024/06/10/russian-attacks-on.html

Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
Polina Petrov, Stephen R. Taylor, Maria Charisi, Chung-Pei Ma
https://arxiv.org/abs/2406.04409

Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
Supermassive black hole binaries (SMBHBs) present us with exciting opportunities for multi-messenger science. These systems are thought to form naturally in galaxy mergers and therefore have the potential to produce electromagnetic (EM) radiation as well as gravitational waves (GWs) detectable with pulsar timing arrays (PTAs). Once GWs from individually resolved SMBHBs are detected, the identification of the host galaxy will be a major challenge due to the ambiguity in possible EM signatures an…

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