| RAdeg DEdeg deg deg | Nx --- | Ny --- | size Kibyte | FileName --- | Title --- |
|---|---|---|---|---|---|
| 272.30450 -19.41283 | 113 | 120 | 112 | Field011-BETA_pacs.fits | HiGal-11 dust extinction of the Planck model for PACS FoV |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-BETA_spire.fits | HiGal-11 dust extinction of the Planck model for SPIRE FoV |
| 272.30450 -19.41283 | 113 | 120 | 112 | Field011-TAU353_pacs.fits | HiGal-11 dust optical depth at 353GHz of the Planck model for PACS FoV |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-TAU353_spire.fits | HiGal-11 dust optical depth at 353GHz of the Planck model for SPIRE FoV |
| 272.30450 -19.41283 | 113 | 120 | 112 | Field011-TEMP_pacs.fits | HiGae-11 temperature of the Planck dust model for PACS FoV |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-TEMP_spire.fits | HiGal-11 temperature of the Planck dust model for PACS FoV |
| 272.28635 -19.41885 | 3904 | 3933 | 119967 | Field011-pacs160_JyPasec.fits | HiGal-11 Herschel/PACS 160um image |
| 272.30450 -19.41283 | 113 | 120 | 112 | Field011-planck160_JyPasec.fits | HiGal-11 flux as Planck would observed at 160um having similar instruments to Herschel |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-planck250_JyPasec.fits | HiGal-11 flux as Planck would observed at 250um having similar instruments to Herschel |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-planck350_JyPasec.fits | HiGal-11 flux as Planck would observed at 350um having similar instruments to Herschel |
| 272.64733 -19.41519 | 115 | 123 | 118 | Field011-planck500_JyPasec.fits | HiGal-11 flux as Planck would observed at 500um having similar instruments to Herschel |
| 272.27746 -19.41256 | 2132 | 2160 | 35986 | Field011-spire250_JyPasec.fits | HiGal-11 Herschel/SPIRE 250um image |
| 272.27912 -19.41256 | 1280 | 1300 | 13011 | Field011-spire350_JyPasec.fits | HiGal-11 Herschel/SPIRE 350um image |
| 272.27746 -19.41283 | 914 | 929 | 6643 | Field011-spire500_JyPasec.fits | HiGal-11 Herschel/SPIRE 500um image |
| 272.29424 -19.42288 | 2668 | 2831 | 59015 | Field011_feathered_160.fits | HiGal-11 result of combining Planck and Herschel at 160um |
| 272.63696 -19.42557 | 1450 | 1541 | 17463 | Field011_feathered_250.fits | HiGal-11 result of combining Planck and Herschel at 250um |
| 272.63752 -19.42446 | 870 | 925 | 6294 | Field011_feathered_350.fits | HiGal-11 result of combining Planck and Herschel at 350um |
| 272.63724 -19.42529 | 621 | 660 | 3209 | Field011_feathered_500.fits | HiGal-11 result of combining Planck and Herschel at 500um |
| 272.27746 -19.41283 | 914 | 929 | 3327 | Field011_feathered_nh.fits | HiGal-11 column density as obtained from our combined images |
| 272.27746 -19.41283 | 914 | 929 | 3327 | Field011_feathered_temp.fits | HiGal-11 temperature as obtained from our combined images |
| 052.59865 +30.93826 | 121 | 140 | 141 | Perseus_04_nom-BETA_pacs.fits | Perseus 04 dust extinction of the Planck model for PACS FoV |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-BETA_spire.fits | Perseus 04 dust extinction of the Planck model for SPIRE FoV |
| 052.59865 +30.93826 | 121 | 140 | 141 | Perseus_04_nom-TAU353_pacs.fits | Perseus 04 dust optical depth at 353GHz of the Planck model for PACS FoV |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-TAU353_spire.fits | Perseus 04 dust optical depth at 353GHz of the Planck model for SPIRE FoV |
| 052.59865 +30.93826 | 121 | 140 | 141 | Perseus_04_nom-TEMP_pacs.fits | Perseus 04 temperature of the Planck dust model for PACS FoV |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-TEMP_spire.fits | Perseus 04 temperature of the Planck dust model for SPIRE FoV |
| 052.58919 +30.93215 | 4387 | 4535 | 155441 | Perseus_04_nom-pacs160_JyPasec.fits | Perseus 04 Herschel/PACS 160um image |
| 052.59865 +30.93826 | 121 | 140 | 141 | Perseus_04_nom-planck160_JyPasec.fits | Perseus 04 flux as Planck would observed at 160um having similar instruments to Herschel |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-planck250_JyPasec.fits | Perseus 04 flux as Planck would observed at 250um having similar instruments to Herschel |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-planck350_JyPasec.fits | Perseus 04 flux as Planck would observed at 350um having similar instruments to Herschel |
| 052.23969 +30.86813 | 122 | 147 | 146 | Perseus_04_nom-planck500_JyPasec.fits | Perseus 04 flux as Planck would observed at 500um having similar instruments to Herschel |
| 052.56246 +30.86490 | 2387 | 2492 | 46482 | Perseus_04_nom-spire250_JyPasec.fits | Perseus 04 Herschel/SPIRE 250um image |
| 052.56301 +30.86518 | 1433 | 1499 | 16791 | Perseus_04_nom-spire350_JyPasec.fits | Perseus 04 Herschel/SPIRE 350um image |
| 052.55996 +30.86518 | 1024 | 1071 | 8578 | Perseus_04_nom-spire500_JyPasec.fits | Perseus 04 Herschel/SPIRE 500um image |
| 052.58853 +30.92808 | 2838 | 3300 | 73173 | Perseus_04_nom_feathered_160.fits | Perseus 04 result of combining Planck and Herschel at 160um |
| 052.22979 +30.85817 | 1536 | 1849 | 22196 | Perseus_04_nom_feathered_250.fits | Perseus 04 result of combining Planck and Herschel at 250um |
| 052.22951 +30.85817 | 921 | 1109 | 7988 | Perseus_04_nom_feathered_350.fits | Perseus 04 result of combining Planck and Herschel at 350um |
| 052.23035 +30.85845 | 658 | 792 | 4078 | Perseus_04_nom_feathered_500.fits | Perseus 04 result of combining Planck and Herschel at 500um |
| 052.55996 +30.86518 | 1024 | 1071 | 4295 | Perseus_04_nom_feathered_nh.fits | Perseus 04 column density as obtained from our combined images |
| 052.55996 +30.86518 | 1024 | 1071 | 4295 | Perseus_04_nom_feathered_temp.fits | Perseus 04 temperature as obtained from our combined images |