The H2O southern Galactic Plane Survey (HOPS)

The HOPS survey was a survey of selected molecular line transitions in the 12mm window with the Mopra radio-telescope. The HOPS survey covers a longitude range l = (-70°,+30°) and a latitude range of |b| < 0.5°. The total survey area is 100 square degrees.

The key spectral targets of HOPS were H2O masers, the ammonia transitions NH3(1,1), NH3(2,2), NH3(3,3) and NH3(6,6), HC3N (3-2) and the RRL H69α.

The intrinsic angular resolution of the HOPS survey data is ~2 arcminutes, and the velocity resolution is 0.43 km/s. The typical rms sensitivity per 0.43 km/s channel of the HOPS data cubes is σ(T) ~ 0.1K.

CADE delivers H2O maser, RRL H69α, NH3(1,1), NH3(2,2), NH3(3,3), NH3(6,6) and HC3N (3-2) integrated intensity maps of the full HOPS region using the survey's public data release.

Healpix maps made by D. Paradis.

H2O NH3(1,1) HC3N(3,2)

References

Maps

H2O Masers : HOPS_H2O_MOM0_1_4096_partial.fits

RRL H69α : HOPS_H69a_MOM0_1_4096_partial.fits

NH3(1,1) Integrated Intensity : HOPS_NH311_MOM0_1_4096_partial.fits

NH3(2,2) Integrated Intensity : HOPS_NH322_MOM0_1_4096_partial.fits

NH3(3,3) Integrated Intensity : HOPS_NH333_MOM0_1_4096_partial.fits

NH3(6,6) Integrated Intensity : HOPS_NH366_MOM0_1_4096_partial.fits

HC3N (3-2) Integrated Intensity : HOPS_HC3N_MOM0_1_4096_partial.fits

HiPS

Original WCS Data

Project Website