A collection of data that describe the 3D content of our Milky Way Galaxy. In 2022, the URL milkyway3d.org. will point not directly to this Dataverse, but instead to an interactive tool showing survey coverage in a 3D Milky Way. Please stay tuned!
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41 to 45 of 45 Results
CORNISH_Continuum_Data_Access.pdf
CORNISH_Continuum_Data_Access.pdf
Sep 5, 2016 - CORNISH Extended Observations: Continuum (2D)
Adobe PDF - 32.0 KB - MD5: 04f6c7c778e990ea2d6998b50d637d6f
CORNISH_Catalog_Data_Access.pdf
CORNISH_Catalog_Data_Access.pdf
Sep 5, 2016 - CORNISH Catalogs: Source-Based Lists
Adobe PDF - 27.6 KB - MD5: 37731b60d7e6161b44ba78f3d1b4fb9e
Coordinated Radio and Infrared Survey for High-Mass Star Formation (CORNISH) Dataverse(Harvard-Smithsonian Center for Astrophysics)
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...
Radio Ammonia Midplane Survey (RAMPS) Dataverse(Harvard-Smithsonian Center for Astrophysics)
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...
The HI, OH, Recombination Line Survey of the Milky Way (THOR) Survey Dataverse(Harvard-Smithsonian Center for Astrophysics)
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....
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