This is an old revision of the document!
Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming clouds complexes
PI: P. André
Maps
250 microns | 350 microns | 500 microns |
---|---|---|
Gouldbelt_250_1_16384_partial.fits | Gouldbelt_350_1_16384_partial.fits | Gouldbelt_500_1_16384_partial.fits |
Uncertainty Maps
250 microns | 350 microns | 500 microns |
---|---|---|
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
(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 |