====== 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. /*Please contact us [[mailto:cade@irap.omp.eu|cade@irap.omp.eu]] if you are interested in HEALPix maps of the other transitions surveyed by HOPS, or if you require maps at a different angular resolution for your science.*/ Healpix maps made by D. Paradis. ^ __**H2O **__ ^ __**NH3(1,1) **__ ^ __**HC3N(3,2) **__ ^ |
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| === References === * 'The H2O southern Galactic Plane Survey (HOPS): I. Techniques and H2O maser data', Walsh et al. 2011, MNRAS 416, 1764 https://ui.adsabs.harvard.edu/abs/2011MNRAS.416.1764W * 'The H2O southern Galactic Plane Survey (HOPS): NH3 (1,1) and (2,2) catalogues', Purcell et al. 2012, MNRAS, 426, 1972 https://ui.adsabs.harvard.edu/abs/2012MNRAS.426.1972P * 'The H2O southern Galactic Plane Survey (HOPS): Paper III - Properties of Dense Molecular Gas across the Inner Milky Way', Longmore et al, 2017, MNRAS, 470, 1462 https://ui.adsabs.harvard.edu/abs/2017MNRAS.470.1462L === Maps === H2O Masers : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_H2O_MOM0_1_4096_partial.fits|HOPS_H2O_MOM0_1_4096_partial.fits]] RRL H69α : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_H69a_MOM0_1_4096_partial.fits|HOPS_H69a_MOM0_1_4096_partial.fits]] NH3(1,1) Integrated Intensity : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_NH311_MOM0_1_4096_partial.fits|HOPS_NH311_MOM0_1_4096_partial.fits]] NH3(2,2) Integrated Intensity : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_NH322_MOM0_1_4096_partial.fits|HOPS_NH322_MOM0_1_4096_partial.fits]] NH3(3,3) Integrated Intensity : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_NH333_MOM0_1_4096_partial.fits|HOPS_NH333_MOM0_1_4096_partial.fits]] NH3(6,6) Integrated Intensity : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_NH366_MOM0_1_4096_partial.fits|HOPS_NH366_MOM0_1_4096_partial.fits]] HC3N (3-2) Integrated Intensity : [[http://cade.irap.omp.eu/documents/Ancillary/HOPS/HOPS_HC3N_MOM0_1_4096_partial.fits|HOPS_HC3N_MOM0_1_4096_partial.fits]] ===HiPS === Enter the following URLs in Aladin ("Files" then "Use directly a URL"): http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_H2O_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_H69a_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_NH311_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_NH322_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_NH333_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_NH366_MOM0 \\ http://cade.irap.omp.eu/documents/Ancillary/4Aladin/HOPS_HC3N_MOM0 \\ === Original WCS Data === https://research.science.mq.edu.au/hops/public/data_cubes.php === Project Website === https://research.science.mq.edu.au/hops/public/index.php