Extended Data Figure 2: Background-subtracted Suzaku XIS03 light curve in the E = 4−10 keV band.
From: Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
The data are binned to the Suzaku orbital period of 5,760 s. The vertical line indicates the time at which the observation is split into two parts for the time-resolved spectral analysis. The effective on-source exposure time is 250 ks. The gaps in the light curve indicate periods in which the satellite could not point to the source. Therefore, the total temporal coverage of the observation is longer, about 500 ks. Errors are at the 1σ level.
