Figure 4 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 4.

Light curves. Top: integrated flux of the Swift/XRT X-ray band, 0.3–10 keV. Middle: UV integrated flux, from the M2 band (~2246 Å) of Swift/UVOT. Bottom: integrated Hα broad-line flux. The largest average variation was observed for the Hα profile, of 20%, followed by the X-rays, which varied by 13%, while the UV did not show significant variation.

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