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.
Featured Dataverses

In order to use this feature you must have at least one published or linked dataverse.

Publish Dataverse

Are you sure you want to publish your dataverse? Once you do so it must remain published.

Publish Dataverse

This dataverse cannot be published because the dataverse it is in has not been published.

Delete Dataverse

Are you sure you want to delete your dataverse? You cannot undelete this dataverse.

Advanced Search

1 to 1 of 1 Result
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...
Add Data

Sign up or log in to create a dataverse or add a dataset.

Sign Up Log In
Share Dataverse

Share this dataverse on your favorite social media networks.

Link Dataverse
Reset Modifications

Are you sure you want to reset the selected metadata fields? If you do this, any customizations (hidden, required, optional) you have done will no longer appear.