A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy
Burke-Spolaor, Sarah; ; Postman, Marc; et al.
The Astrophysical Journal, Volume 849, Issue 1, article id. 59, 12 pp. (2017).
apjaa9064f2_hr
Normalized object spectra (black lines) and the 68% confidence intervals on the observed spectrum fluxes (gray shaded areas) shown for A2261 knots 1, 2, and 3 from top to bottom, respectively. The best fits obtained for each knot are shown as red lines. The arrow indicates the rest-frame wavelength of the Mgb spectral feature.
rupke_etal_2017_fig_14
Fig 14 from Rupke et al. (2017). Shows a positive correlation between log outflow mass and log black hole mass.
Turkey Trot 2017
Turkey Trot 2017
The above is one way to do it.
-
- Normalized object spectra (black lines) and the 68% confidence intervals on the observed spectrum fluxes (gray shaded areas) shown for A2261 knots 1, 2, and 3 from top to bottom, respectively. The best fits obtained for each knot are shown as red lines. The arrow indicates the rest-frame wavelength of the Mgb spectral feature.
-
- Fig 14 from Rupke et al. (2017). Shows a positive correlation between log outflow mass and log black hole mass.
This is the radio relic paper.
import antigravity
for i in [1 2 3]:
print i