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Hubble Space Telescope Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS 0745-191

  • Authors: Julie Hlavacek-Larrondo, Hyunseop Choi, 섭 최현, Minghao Guo, 浩 明, Annabelle Richard-Laferrière, Carter Rhea, Marine Prunier, Helen Russell, Andy Fabian, Jonelle L. Walsh, Marie-Joëlle Gingras, Brian McNamara, Steve Allen, André-Nicolas Chené, Alastair Edge, Marie-Lou Gendron-Marsolais, Michael McDonald, Priyamvada Natarajan, Jeremy Sanders, James F. Steiner, Benjamin Vigneron, Anja von der Linden

Julie Hlavacek-Larrondo et al 2025 The Astrophysical Journal 980 .

  • Provider: AAS Journals

Caption: Figure 5.

Best-fitting models for the continuum-subtracted spectra extracted from the pixels with emission-line detection at three slit locations (Positions 2, 1, and 3 from the leftmost column). The full model that contains Hα, [N II], and [S II] emission lines is plotted in red, and each emission-line components are plotted in blue, green, and orange, respectively (longer wavelength transitions in the doublets are shown with dashed lines). The continuum-subtracted spectra and the uncertainties are plotted in black and gray, respectively. We note that the pixels far from the center were binned together. The cyan shade represents a 95% confidence region extracted from the MCMC posterior sampling calculated using emcee package. The fit results are tabulated in Table 1.

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