Published March 24, 2025 | Version v1
Figure Open

The properties of the obscuring material of an AGNs sample from mid-IR and X-ray simultaneous fitting

Authors/Creators

  • 1. ROR icon Instituto de Astrofísica de Canarias
  • 2. Universidad Nacional Autónoma de México Centro de Radioastronomia y Astrofisica
  • 3. Universidad Nacional Autonóma de México Instituto de Astronomía
  • 4. ROR icon Consejo Superior de Investigaciones Científicas
  • 5. ROR icon Centro de Astrobiología
  • 6. ROR icon Instituto de Astrofísica de Andalucía

Contributors

  • 1. ROR icon Instituto de Astrofísica de Canarias
  • 2. Universidad Nacional Autónoma de México Centro de Radioastronomia y Astrofisica

Description

Comparison of confidence contours for free parameters before and after assuming that the dust and gas emission have the same origin structure.

Two-dimensional ∆χ2 contours for the resulting free parameters of the baseline model before (dotted lines) and after (solid lines) linking the half-opening angle and torus angular width to fit the spectra of each source. The red, green, and blue (dotted and solid) contours mark the 1σ, 2σ, and 3σ errors, respectively. The black circles and blue stars are the resulting values for each parameter before and after linking the half-opening angle and torus angular width, respectively.

Files

AppendixC.pdf

Files (3.0 MB)

Name Size Download all
md5:721069a01e55301c9ff79984e0faaf52
3.0 MB Preview Download