Image Details

Choose export citation format:

SUBMILLIMETER H2O MEGAMASERS IN NGC 4945 AND THE CIRCINUS GALAXY

  • Authors: D. W. Pesce, J. A. Braatz, and C. M. V. Impellizzeri

2016 The Astrophysical Journal 827 68.

  • Provider: AAS Journals

Caption: Figure 2.

H2O megamaser spectra of Circinus. Top: a reproduction of the 22 GHz spectrum taken with the 64 m Parkes telescope in 1998 August from Braatz et al. (2003). Because we restricted the vertical axis range to more easily show the weaker features, the strongest feature (peaking at ∼18 Jy) was cut off. Middle: 321 GHz spectrum extracted from the continuum-subtracted data cube. The channel width is 0.5 km s−1. The atmospheric transmission curve, corresponding to a precipitable water vapor level matching that present during the observation, is overplotted in light gray. Atmospheric transmission curves were taken from the Atacama Pathfinder Experiment (APEX) transmission calculator (http://www.apex-telescope.org/sites/chajnantor/atmosphere/). The recession velocity of the galaxy is marked by a vertical red line. Bottom: phase plot for the calibrated 321 GHz spectrum.

Other Images in This Article
Copyright and Terms & Conditions