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No Time for Dead Time: Timing Analysis of Bright Black Hole Binaries with NuSTAR

  • Authors: Matteo Bachetti, Fiona A. Harrison, Rick Cook, John Tomsick, Christian Schmid, Brian W. Grefenstette, Didier Barret, Steven E. Boggs, Finn E. Christensen, William W. Craig, Andrew C. Fabian, Felix Fürst, Poshak Gandhi, Charles J. Hailey, Erin Kara, Thomas J. Maccarone, Jon M. Miller, Katja Pottschmidt, Daniel Stern, Phil Uttley, Dominic J. Walton, Jörn Wilms, and William W. Zhang

Bachetti et al. 2015 The Astrophysical Journal 800 109.

  • Provider: AAS Journals

Caption: Figure 8.

GRS 1915+105: Left: cospectrum before (black) and after (red) clean up of the nth harmonics of the housekeeping operations (at 1 and 0.125 Hz)." Right: evolution of the 1.5 Hz QPO (and a faint first harmonic) in the dynamical cospectrum during the observations. Each time segment represents 64 s of gap-free data. Colors and sizes of the points are both a proxy of power, in arbitrary units.

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