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

70 microns 160 microns
37 arcsec
Gouldbelt_70_HPDP_1_16384_partial.fitsGouldbelt_160_HPDP_1_16384_partial.fits
1 arcmin
Gouldbelt_70_HPDP_1arcm_1_8192_partial.fitsGouldbelt_160_HPDP_1arcm_1_8192_partial.fits
4 arcmin
Gouldbelt_70_HPDP_4arcm_1_2048_partial.fitsGouldbelt_160_HPDP_4arcm_1_2048_partial.fits

SPIRE Maps

250 microns 350 microns 500 microns
37 arcsec
Gouldbelt_250_1_16384_partial.fitsGouldbelt_350_1_16384_partial.fitsGouldbelt_500_1_16384_partial.fits
1 arcmin
Gouldbelt_250_1arcm_1_8192_partial.fitsGouldbelt_350_1arcm_1_8192_partial.fitsGouldbelt_500_1arcm_1_8192_partial.fits
4 arcmin
Gouldbelt_250_4arcm_1_2048_partial.fitsGouldbelt_350_4arcm_1_2048_partial.fitsGouldbelt_500_4arcm_1_2048_partial.fits

Uncertainty Maps

250 microns 350 microns 500 microns
37 arcsec
Gouldbelt_250_SIGMA_final_1_16384_partial.fitsGouldbelt_350_SIGMA_final_1_16384_partial.fitsGouldbelt_500_SIGMA_final_1_16384_partial.fits

HiPS

Enter the following URLs in Aladin (“Files” then “Use directly a URL”):
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_250
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_350
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_500
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_250_SIG
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_350_SIG
https://cade.ovgso.fr/documents/Ancillary/4Aladin/Gouldbelt_500_SIG

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