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Disk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-timing Analysis

  • Authors: Jingyi Wang, Guglielmo Mastroserio, Erin Kara, Javier A. García, Adam Ingram, Riley Connors, Michiel van der Klis, Thomas Dauser, James F. Steiner, Douglas J. K. Buisson, Jeroen Homan, Matteo Lucchini, Andrew C. Fabian, Joe Bright, Rob Fender, Edward M. Cackett, and Ron A. Remillard

2021 The Astrophysical Journal Letters 910 L3.

  • Provider: AAS Journals

Caption: Figure 4.

Time-lag fit result in Epoch 1. (a) The power spectral density, (b) the lag-frequency spectrum where the dashed lines represent the frequency ranges to extract and fit the lag-energy spectra (c1–c4); the shaded regions are the QPO frequencies (central frequency±HWHM) that we do not include in the time-lag fits. The points in (b) are connected with a Bezier join to guide the eye.

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