The multi-frequency radio light curve of the sub-pc SMBH binary candidate PG 1302-102

arXiv:2608.29682 · astro-ph.GA, astro-ph.HE · Submitted 2026-08-30 · Read on arXiv

astro-ph.GA, astro-ph.HE

Submitted: 2026-08-30

Updated: 2026-08-30

Terminology

• AGN — 5× in this paper · explained in 1 episode
• Calibration — 3× in this paper · explained in 7 episodes
• Red-noise False Alarm Probability — 2× in this paper
• pulsar timing arrays — 2× in this paper · explained in 2 episodes
• Accretion Flows — 1× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Australian Telescope Compact Array — 1× in this paper
• Computational Biology — 1× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes
• Gravitational Wave Emission — 1× in this paper · explained in 2 episodes
• National Research Foundation — 1× in this paper

Sources

• Observational Signatures of Supermassive Black Hole Binaries
• A retrospective view of Miriad

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