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herschel [2018/09/30 19:54] Déborah Paradis |
herschel [2023/04/11 15:25] (current) Déborah Paradis |
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| The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec. | The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec. | ||
| - | CADE currently only serves SPIRE photometric data for each Key-Programs. Healpix maps at 250 microns and 350 microns have been smoothed to 37 arcsec. | + | CADE serves SPIRE and PACS photometric data for each Key-Programs. Healpix maps have all been smoothed to 37 arcsec. We also provide Healpix maps of the SPIRE data at 1 and 4 arcmin angular resolutions.\\ |
| - | The units of the Healpix maps are MJy/sr. | + | Concerning the PACS data, CADE serves Healpix maps of the Users Provided Data Products (UPDP) when available, or Highly Processed Data Products (HPDP). When none of these data were available, we produced healpix maps using data processed by the Herschel Pipeline (level 2.5 when possible) using:\\ |
| + | - the High-Pass Filter (HPF) method denoted as HPFMAP \\ | ||
| + | - the JScanam map maker denoted as JSMAP\\ | ||
| + | - the Unimap map maker denoted as UNIMAP\\ | ||
| + | |||
| + | The units of the Healpix maps are MJy/sr.\\ | ||
| + | |||
| + | Healpix maps made by D. Paradis. | ||
| === References === | === References === | ||
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| |[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ | |[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ | ||
| |[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| \\ | |[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| \\ | ||
| + | |[[Herschel Gould Belt|Gould Belt- Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming cloud complexes (PI: P. André)]]| \\ | ||
| |[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ | |[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ | ||
| |[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ | |[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ | ||
| Line 34: | Line 42: | ||
| |[[Herschel Hi-GAL|Hi-GAL- The Herschel infrared Galactic Plane Survey (S. Molinari)]]|\\ | |[[Herschel Hi-GAL|Hi-GAL- The Herschel infrared Galactic Plane Survey (S. Molinari)]]|\\ | ||
| |[[Herschel Hobys|Hobys- The Herschel imaging survey of OB Young Stellar objects (PI: F. Motte)]]|\\ | |[[Herschel Hobys|Hobys- The Herschel imaging survey of OB Young Stellar objects (PI: F. Motte)]]|\\ | ||
| + | |[[Herschel HRS|HRS- The Herschel Reference Survey (PI: S. Eales)]]|\\ | ||
| |[[Herschel Kingfish|Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (R. Kennicutt)]]|\\ | |[[Herschel Kingfish|Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (R. Kennicutt)]]|\\ | ||
| |[[Herschel Madden|The ISM in Low Metallicity Environments: Bridging the Gap Between Local Universe and Primordial Galaxies (PI: S. Madden)]]|\\ | |[[Herschel Madden|The ISM in Low Metallicity Environments: Bridging the Gap Between Local Universe and Primordial Galaxies (PI: S. Madden)]]|\\ | ||
| |[[Herschel Meisenheimer|The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>2 (PI: K. Meisenheimer)]]|\\ | |[[Herschel Meisenheimer|The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>2 (PI: K. Meisenheimer)]]|\\ | ||
| |[[Herschel SAG-4|SAG-4- Evolution of interstellar dust (PI: A. Abergel)]]|\\ | |[[Herschel SAG-4|SAG-4- Evolution of interstellar dust (PI: A. Abergel)]]|\\ | ||
| - | |[[Herschel VNGS|VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies (PI: C. Wlison)]]|\\ | + | |[[Herschel VNGS|VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies (PI: C. Wilson)]]|\\ |
| === Original WCS Data === | === Original WCS Data === | ||