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DustPedia: A Definitive Study of Cosmic Dust in the Local Universe Overview |
 DustPedia Overview |
 DustPedia Primary Data Access |
Overview
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The DustPedia project capitalises on the legacy of the Herschel Space Observatory, using cutting-edge modelling techniques
to study dust in the 875 DustPedia galaxies - representing the vast majority of extended galaxies within 3000 km/s that were observed
by Herschel. This work requires a database of multiwavelength imagery and photometry that greatly exceeds the scope (in terms of
wavelength coverage and number of galaxies) of any previous local-Universe survey.
If you use DustPedia data, please cite the journal articles Clark et al. (2018), as well as the dataset Digital Object Identifier (DOI): 10.26131/IRSA660. |
Data Set Characteristics
| Data Product | Description | Data Access |
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| Images | Herschel PACS: 70, 100, 160 microns Herschel SPIRE: 250, 350, 500 microns Spitzer IRAC: 3.6, 4.5, 5.8, 8 microns Spitzer MIPS: 24, 70, 160 microns WISE: 3.4, 4.6, 12, 22 microns 2MASS: J, H, Ks band SDSS: u, g, r, i, z band GALEX: FUV, NUV Planck: 30, 44, 70, 100, 143, 217, 353, 545, 857 GHz DSS: B, R band |
DustPedia Documentation
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Documentation DustPedia Home Page |