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ASTROSAT/LAXPC REVEALS THE HIGH-ENERGY VARIABILITY OF GRS 1915+105 IN THE χ CLASS

  • Authors: J S Yadav, Ranjeev Misra, Jai Verdhan Chauhan, P C Agrawal, H M Antia, Mayukh Pahari, Dhiraj Dedhia, Tilak Katoch, P. Madhwani, R K Manchanda, B Paul, Parag Shah, and C H Ishwara-Chandra

2016 The Astrophysical Journal 833 27.

  • Provider: AAS Journals

Caption: Figure 9.

In each row, 3.0–80.0 keV fitted power density spectrum in the frequency range of 0.1–10.0 Hz along with its residual (first column), time-lag spectra at the corresponding fundamental QPO frequencies (second column) and fractional rms spectra at the same QPO frequencies (third column) are shown. PDS, time-lag, and rms spectra are calculated at ∼2.55 Hz (top rows), ∼4.53 Hz (middle rows), and ∼6.55 Hz (bottom rows) respectively. In all lag spectra, the 3.0–4.0 keV band is considered to be the reference band.

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