41 to 48 of 48 Results
Cormac Purcell, 2016, "HOPS Catalogs: Spectral Line", https://doi.org/10.7910/DVN/LTZFAX, Harvard Dataverse, V1
This dataset consists of three catalogs derived from mining the HOPS extended spectral line observations with the ATNF DUCHAMP source finding algorithm. The three catalogs cover the same spectral lines as the extended observations (NH3 (1,1), NH3 (2,2), and H2O masers) and consist of 669 dense molecular clouds. It is 100% complete at the 5σ detecti... |
Sep 5, 2016
The H2O Southern Galactic Plane Survey (HOPS) has mapped a 100 degree strip of the Galactic plane (-70° > l > 30°, | b | < 0.5°) at 12 mm wavelengths. Thermal lines of interest include the NH3 J,K = (1,1) and (2,2) transitions, which probe molecular cloud densities on the order of n > 104 cm-3. The spatial resolution of the survey is 2’, and the ve... |
Melvin Hoare, 2016, "CORNISH Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/EUKSQE, Harvard Dataverse, V1
This dataset includes extended radio continuum observations at 5 GHz towards the first Galactic quadrant of the Milky Way. The region is broken up into 20x20 arcminute tiles, all of which are available for download at here. Alternatively, one can use the image cutout service found here. |
Cormac Purcell, 2016, "CORNISH Catalogs: Source-Based Lists", https://doi.org/10.7910/DVN/ZUQ6C7, Harvard Dataverse, V1
This dataset consists of 3000+ radio emission sources detected in the CORNISH images. The CORNISH team applied an automated source finding procedure to identify a new, uniform catalog of compact radio emission (from HII regions, planetary nebulae, and radio galaxies) with a peak intensity above 7σ. To access the data, you can search for sources wit... |
Sep 5, 2016
The Coordinated Radio and Infrared Survey for High-Mass Star Formation (CORNISH) is an arcsecond-resolution radio continuum survey covering 10°< l < 65° and |b| < 1° at 5 GHz. With an overlapping footprint, it is intended to be the radio counterpart to mid-IR GLIMPSE/MIPSGAL surveys and the near-IR UKIDSS survey of the Galactic plane. One of its ma... |
Sep 5, 2016 - Radio Ammonia Midplane Survey (RAMPS) Dataverse
James Jackson, 2016, "RAMPS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/NMDU7W, Harvard Dataverse, V1
This dataset consists of extended spectral line observations taken with the K-band Focal Plane Array on the Green Bank Telescope (GBT). Lines of study include NH3 (1,1); (2,2); (3,3); (4,4); (5,5), H2O masers, and CH3OH masers. This is a blind survey covering 10° < l < 40° and b < |0.5°|. As of summer 2016, no data has been released; however, once... |
Sep 5, 2016
The Radio Ammonia Midplane Survey (RAMPS) is a program to survey 60 sq. deg. of the Galactic Plane at 1.3 cm using the Green Bank Telescope. Currently in pilot mode (March 2016), the program will map from l=10° - 40° and b= -0.5° - 0.5°. The RAMPS survey is a successor to the HOPS survey and will cover multiple ammonia transitions at higher resolut... |
Sep 5, 2016
The THOR survey is a galactic plane survey covering 15° < l < 67° and b < |1°|. It consists of HI 21 cm observations, 20 recombination lines and 1-2 GHz continuum data at a 20" spatial resolution. One of its main science goals is understanding the dynamics of the interstellar medium and how clouds transition from the atomic to the molecular phase.... |
