Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming clouds complexes
PI: P. André
PACS Maps
SPIRE Maps
Uncertainty Maps
250 microns | 350 microns | 500 microns |
---|---|---|
37 arcsec | ||
Gouldbelt_250_SIGMA_final_1_16384_partial.fits | Gouldbelt_350_SIGMA_final_1_16384_partial.fits | Gouldbelt_500_SIGMA_final_1_16384_partial.fits |
HiPS
Enter the following URLs in Aladin (“Files” then “Use directly a URL”):
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_250
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_350
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_500
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_250_SIGMA
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_350_SIGMA
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/Gouldbelt_500_SIGMA
OR
unzip the directory and put it directly in an Aladin window to display the map
Maps:
250 microns | 350 microns | 500 microns |
---|---|---|
Gouldbelt_250.zip | Gouldbelt_350.zip | Gouldbelt_500.zip |
Uncertainty maps:
250 microns | 350 microns | 500 microns |
---|---|---|
Gouldbelt_250_SIGMA.zip | Gouldbelt_350_SIGMA.zip | Gouldbelt_500_SIGMA.zip |