Image Details
Caption: Figure 1.
Comparison of 183 GHz spectra (in black) with their 22 GHz counterparts (in red, vertically offset). The 183 GHz spectra have been boxcar smoothed across 10 channels, corresponding to a ∼2 km s−1 post-averaging spectral resolution. Note that the pairs of spectra in each panel were not observed concurrently; in most cases, the 22 GHz spectrum predates the 183 GHz spectrum by multiple years.
© 2023. The Author(s). Published by the American Astronomical Society.