Figure B1 from Disk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-timing Analysis

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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 B1.

(Upper) The effective area of NICER, with the fitted characteristic energies of phenomenological calibration models in Wang et al. (2020a) and this work. (Lower) The residuals for NICER data in Epoch 3 from simultaneous fits with or without the phenomenological calibration models. The ﹩{\chi }^{2}﹩ values quoted are for the simultaneous fit of the 5 epochs.

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