The 13CO/C18O (J = 3 → 2) Heterodyne Inner Milky Way Plane Survey (CHIMPS) is a high-resolution spectral survey covering |b| ≤ 0.5° and 28° ≲ l ≲ 46°. It has an angular resolution of 15” and consists of 0.5 km/s velocity channels. Because of its rarer isotopologues the survey probes a higher critical density of CO (>10^4 cm^-3) at temperatures less than 20 K. It acts as a good complement to the JCMT and Hi-GAL surveys of the Galactic plane due to similar spatial resolution.
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CHIMPS_Spectral_Data_Access.pdf
CHIMPS_Spectral_Data_Access.pdf
Sep 5, 2016 - CHIMPS Extended Observations: Spectral Line (3D)
Adobe PDF - 32.6 KB - MD5: 1944a328e77a34875fa0e54c913c1086
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