Figure 7 from Short-timescale Monitoring of the X-Ray, UV, and Broad Double-peak Emission Line of the Nucleus of NGC 1097

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Short-timescale Monitoring of the X-Ray, UV, and Broad Double-peak Emission Line of the Nucleus of NGC 1097

Authors: Jaderson S. Schimoia, Thaisa Storchi-Bergmann, Dirk Grupe, Michael Eracleous, Bradley M. Peterson, Jack A. Baldwin, Rodrigo S. Nemmen, and Cláudia Winge

Schimoia et al. 2015 The Astrophysical Journal 800 63.

Provider: AAS Journals

Caption: Figure 7.

Correlation between X-ray and optical data, where black points represent the fluxes of the X-ray band and the broad profile for the same MJD (after interpolation of the optical light curve to match the epochs of Swift observations). The red dashed line is the best linear correlation between the data. The median value of the correlation coefficient is which corresponds to a level of significance of 56.8%–98.4%.

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