The Herschel Infrared Galactic plane survey (Hi-GAL) is an unbiased photometric survey covering |b| <= 1.0°, 68 > l > -70° in five passbands between 70 and 500 μm. The nominal beam sizes range from 5-35". Its key science goals include understanding the distribution of the ISM temperature, the formation of molecular clouds, the timeline of high-mass star formation, and the link between local and global star formation properties. The link to the homepage of the Hi-GAL survey can be found here.
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Hi-GAL Extended Observations: Continuum (2D)
Hi-GAL Extended Observations: Continuum (2D)
Sep 5, 2016
Sergio Molinari, 2016, "Hi-GAL Extended Observations: Continuum (2D)", https://doi.org/10.7910/DVN/AGXXHR, Harvard Dataverse, V1
This dataset consists of photometric maps at five wavelengths: 70, 160, 250, 350 and 500μm, which combined cover the peak of the SED for dust temperatures between 8 ≤ T ≤ 50K. The first suite of Hi-GAL data was released in Spring 2016, covering 68°≥ l ≥ -70° and |b| ≤ 1°, with more data to come in future. The public Hi-GAL DR1 data can be retrieved...
HIGAL_Continuum_Data_Access.pdf
HIGAL_Continuum_Data_Access.pdf
Sep 5, 2016 - Hi-GAL Extended Observations: Continuum (2D)
Adobe PDF - 28.6 KB - MD5: d1c0adaa38e46b39b1ca0acce58e49f6
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