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Blindly Detecting Orbital Modulations of Jets from Merging Supermassive Black Holes

  • Authors: R. O'Shaughnessy, D. L. Kaplan, A. Sesana, and A. Kamble

O'Shaughnessy et al. 2011 The Astrophysical Journal 743 136.

  • Provider: AAS Journals

Caption: Figure 2.

Sources with precession modulation: total number: assuming all binaries have significant spin–orbit misalignment, the number of sources with precession periods P min = 1 minute and P max = 1 year (blue) or 1 month (green) over the entire sky, with flux above F/ epsilon. To guide the eye to scales comparable to future radio surveys like VAST (T. Murphy et al. 2011, in preparation), a horizontal dashed line corresponds to 1/10 4 deg 2 and a vertical dashed line corresponds to 1 mJy.

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