The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) maps 400 sq. deg. of the inner galaxy (|l| < 60º, |b| < 1.5º) at 870 μm with a uniform sensitivity of a few solar masses at a distance of 1 kpc. It has a spatial resolution of 19”. Its main sciences goals are to understand the early stages of high mass star formation, through a comprehensive analysis of pre/proto-stellar cores and young stellar objects. Compact source catalogs have also been produced from the continuum survey using the clump finding algorithms SExtractor and Gaussclumps. The link to the homepage of the ATLASGAL survey can be found here.
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ATLASGAL Extended Observations: Continuum (2D)
ATLASGAL Extended Observations: Continuum (2D)
Sep 5, 2016
Frédéric Schuller, 2016, "ATLASGAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/GF23ME, Harvard Dataverse, V1
This dataset consists of photometric maps covering 400 sq. deg. of the Galactic plane at 870 microns. All reduced and calibrated emission maps are available in 3x3 degree tiles at the ATLASGAL data bank here.
ATLASGAL Catalogs: Source-Based Lists
ATLASGAL Catalogs: Source-Based Lists
Sep 5, 2016
Timea Csengeri; Yanett Contreras, 2016, "ATLASGAL Catalogs: Source-Based Lists", https://doi.org/10.7910/DVN/OFCYSM, Harvard Dataverse, V1
This dataset consists of compact source catalogs produced from the 870 micron continuum survey using the clump finding algorithms SExtractor and Gaussclumps. The SExtractor derived catalog is outlined in Contreras et al. 2013 and consists of 6639 compact sources. The Gaussclumps derived catalog is outlined in Csengeri et al. 2014 and consists of 10...
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