Image Details

Choose export citation format:

Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

  • Authors: Arghajit Jana, Claudio Ricci, Franz E. Bauer, Kriti Kamal Gupta, Benny Trakhtenbrot, Alessia Tortosa, Ruancun Li, Luis C. Ho, Richard Mushotzky, Hsiang-Kuang Chang, Yaherlyn Diaz, Georgios Dimopoulos, Kristína Kallová, Michael J. Koss, Stéphane Paltani, Matthew J. Temple

Arghajit Jana et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

Left panel: variation of X-ray bolometric correction (κ2−10) as a function of αOX. The blue circles, green diamonds, purple down-triangles, red up-triangles, and orange squares represent the data points from NGC 1566, NGC 2617, Mrk 590, Mrk 1018, and IRAS 23226–3843, respectively. The yellow stars represent the binned data point. The black line represents the best fits (Equation (4)) of the data. The green dashed line represents the κ2−10αOX relation for unobscured BASS AGNs (K. K. Gupta et al. 2024). Right panel: same as right panel but with binned data. The shaded regions represent the 1-σ scatter.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse