31 to 40 of 48 Results
Erik Rosolowsky, 2016, "BGPS Catalogs: Source-Based Lists", https://doi.org/10.7910/DVN/TQHAJI, Harvard Dataverse, V1
This dataset consists of 8000+ compact sources extracted from the BGPS extended continuum 1.1 mm observations. The sources were obtained using a custom extraction algorithm called "Bolocat", which is tailored to the BGPS maps. According to Rosolowsky et al. 2010, these sources are best characterized as dense molecular clumps. Catalog information ca... |
Yancy Shirley, 2016, "BGPS Catalogs: Spectral Line", https://doi.org/10.7910/DVN/VNDTFT, Harvard Dataverse, V1
This dataset consists of spectroscopic follow-up observations towards dense BGPS molecular clumps derived from the 1.1 mm dust continuum survey. Observations were obtained using the Heinrich Hertz Telescope simultaneously in HCO+ (J = 3-2) and N2H+ (J = 3-2). In total, over 6000 clumps have spectral line observations, with the results published in... |
Sep 5, 2016
The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm survey of dust emission covering -10° <= l <= 90° and |b|<= 0.5°. Version 2 also includes additional coverage of 20 deg^2 in the 3rd and 4th quadrants. The effective angular resolution of the survey is 33”. Additional spectral line follow-up observations towards dense clouds in the survey were al... |
Peter Barnes; Erik Muller, 2016, "ThrUMMS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/CCCKQB, Harvard Dataverse, V1
This dataset consists of extended spectral line observations in the fourth Galactic quadrant of the Milky Way. Targeted lines include 12CO,13CO,C18O,and CN. Individual spectral cubes can be downloaded at the ThrUMMS data release bank here. |
Sep 5, 2016
The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) maps the fourth Galactic quadrant (|b|<1.0°) with the J=1→0 lines of 12CO, 13CO, C18O, and CN near 112 GHz. It has a spatial resolution of ~1’ and a velocity resolution of 0.3 km/s. Its main science goals include understandings the neutral/molecular ISM connection, the physical state of Giant M... |
James Jackson, 2016, "MALT90 Pointed Surveys: Spectral Line", https://doi.org/10.7910/DVN/OLPYKN, Harvard Dataverse, V1
The dataset consists of targeted spectral line observations towards 2000+ high-mass dense cores. For each dense core, (l,b,v) cubes and moment maps in sixteen emission lines are available. All cubes are available for download at the Australia Telescope Online Archive, but an account must be created to access the data. To get an overview of all the... |
Sep 5, 2016
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) Survey is a program targeting sixteen molecular line transitions which typically trace critical densities on the order of 10^5 cm^-3. Particular lines of interest include N2H+, HCO+, HCN, and HNC, along with isotopologues like H13CO+. The velocity resolution of the survey is ~0.11 km/s, while the... |
James Jackson, 2016, "GRS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/OBOBUL, Harvard Dataverse, V1
The GRS dataset consists of extended 13CO (1-0) spectral line mapping in the first Galactic quadrant of the Milky Way. Users can retrieve individual l,b,v cube cutouts in a specified velocity range at the GRS data site here. |
Sep 5, 2016
The Galactic Ring Survey maps the 13CO J=1-0 transition in the first Galactic quadrant (18° <= l <= 55.7° and -1° <= b <= +1°). It has an angular resolution of 46” and a velocity resolution of 0.21 km/s, with almost 2 million spectra. Its main science goal is understanding the kinematics, structure, and astrochemistry of the 5 kpc ring. The link to... |
Andrew Walsh, 2016, "HOPS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/HUHMJV, Harvard Dataverse, V1
This dataset consists of extended spectral line mapping of NH3 (1,1), NH3 (2,2), and H2O masers. The 100 sq. deg. survey region is broken up into eleven strips, and all cubes are available for download at the HOPS data product page here. |
