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herschel [2018/09/28 10:02]
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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 __**Following are the Herschel Key Programs with SPIRE photometric observations. Healpix and HiPS maps can be downloaded on each page:**__ __**Following are the Herschel Key Programs with SPIRE photometric observations. Healpix and HiPS maps can be downloaded on each page:**__
-^Key Programs ​                                ​^  ​Maps                                        ^ +^Key Programs ​                                ​^ ​  
-Galactic Cold Cores //(PI: M. Juvela & I. Ristorcelli)// ​ | **[[Herschel ​Galactic Cold Cores|Here]]**|\\ ​                                  |DEBRIS- Disc Emission via a Bias-free Reconnaissance in the Infrared/​Sub-millimetre ​//(PI : B. Matthews)// |**[[Herschel DEBRIS|Here]]**|\\ +|[[Herschel ​DEBRIS|DEBRIS- Disc Emission via a Bias-free Reconnaissance in the Infrared/​Sub-millimetre (PI : B. Matthews)]]|\\ 
- +|[[Herschel Dunes|DUNES- Cold Disks around Nearby Stars. A search for Edgeworth-Kuiper Belt analogues (PI: C. Eiroa)]]|\\ 
-| DUNES- Cold Disks around Nearby Stars. A search for Edgeworth-Kuiper Belt analogues ​//(PI: C. Eiroa)//|** [[Herschel Dunes|Here]]**|\\ +|[[Herschel EPoS|EPoS- The earliest phases of star formation: From low- to high-mass objects (PI: O. Krause)]]|\\ 
-  ​* ​EPoS- The earliest phases of star formation: From low- to high-mass objects ​//(PI: O. Krause)// **[[Herschel ​EPoS|Here]]**\\ +|[[Herschel ​Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\  
-  ​* ​GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel ​//(PI: D. Elbaz)// **[[Herschel ​GOODS|Here]]**  \\ +|[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]|  \\ 
-  ​* ​H-ATLAS- The Herschel Thousand Degree Survey ​//(PI: S. Eales)// **[[Herschel H-atlas|Here]]**\\ +|[[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 Lensing Survey ​//(PI: E. Egami)// **[[Herschel Lensing Survey|Here]]**\\ +|[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ 
-  ​* ​HELGA- The Herschel Exploitation of the Local Galaxy Andromeda ​//(PI: J. Fritz)// **[[Herschel HELGA|Here]]**\\ +|[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ 
-  ​* ​Heritage- HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds ​//(PI: M. Meixner)// **[[Herschel Heritage|Here]]**\\ +|[[Herschel HELGA|HELGA- The Herschel Exploitation of the Local Galaxy Andromeda (PI: J. Fritz)]]|\\ 
-  ​* ​HerMES- The Herschel Multi-tiered Extragalactic Survey: Measuring the Infrared Galaxy Formation History of the universe ​ //(PI: S. Oliver)// **[[Herschel Hermes|Here]]**\\ +|[[Herschel Heritage|Heritage- HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds (PI: M. Meixner)]]|\\ 
-  ​* ​HerM33es- Herschel M33 Extended Survey ​//(PI: C. Kramer)// **[[Herschel HerM33es|Here]]**\\ +|[[Herschel Hermes|HerMES- The Herschel Multi-tiered Extragalactic Survey: Measuring the Infrared Galaxy Formation History of the universe (PI: S. Oliver)]]|\\ 
-  ​* ​HeViCS- Herschel Virgo Cluster Survey ​//(PI: J. Davies)// **[[Herschel HeViCS|Here]]**\\ +|[[Herschel HerM33es|HerM33es- Herschel M33 Extended Survey (PI: C. Kramer)]]|\\ 
-  ​* ​Hi-GAL- The Herschel infrared Galactic Plane Survey ​//(S. Molinari)// **[[Herschel Hi-GAL|Here]]**\\ +|[[Herschel HeViCS|HeViCS- Herschel Virgo Cluster Survey (PI: J. Davies)]]|\\ 
-  ​* ​Hobys- The Herschel imaging survey of OB Young Stellar objects ​//(PI: F. Motte)// **[[Herschel ​Hobys|Here]]**\\ +|[[Herschel Hi-GAL|Hi-GAL- The Herschel infrared Galactic Plane Survey (S. Molinari)]]|\\ 
-  ​* ​Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel ​//(R. Kennicutt)// **[[Herschel Kingfish|Here]]**\\ +|[[Herschel Hobys|Hobys- The Herschel imaging survey of OB Young Stellar objects (PI: F. Motte)]]|\\ 
-  ​* ​The ISM in Low Metallicity Environments:​ Bridging the Gap Between Local Universe and Primordial Galaxies ​//(PI: S. Madden)// **[[Herschel Madden|Here]]**\\ +|[[Herschel ​HRS|HRS- The Herschel Reference Survey (PI: S. Eales)]]|\\ 
-  ​* ​The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>​2 ​//(PI: K. Meisenheimer)// **[[Herschel Meisenheimer|Here]]**\\ +|[[Herschel Kingfish|Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (R. Kennicutt)]]|\\ 
-  ​* ​SAG-4- Evolution of interstellar dust //(PI: A. Abergel)// **[[Herschel SAG-4|Here]]**\\ +|[[Herschel Madden|The ISM in Low Metallicity Environments:​ Bridging the Gap Between Local Universe and Primordial Galaxies (PI: S. Madden)]]|\\ 
-  ​* ​VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies ​//(PI: C. Wlison)// **[[Herschel VNGS|Here]]** \\+|[[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 VNGS|VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies (PI: C. Wilson)]]|\\
  
 === Original WCS Data === === Original WCS Data ===