Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Next revision Both sides next revision
herschel [2018/09/28 10:03]
Déborah Paradis
herschel [2018/10/09 15:30]
Déborah Paradis
Line 19: Line 19:
  
 __**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]]**|\\  +|[[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)]]|\\ 
-|DEBRIS- Disc Emission via a Bias-free Reconnaissance in the Infrared/​Sub-millimetre ​//(PI : B. Matthews)// |**[[Herschel DEBRIS|Here]]**|\\ +|[[Herschel EPoS|EPoS- The earliest phases of star formation: From low- to high-mass objects (PI: O. Krause)]]|\\ 
- +|[[Herschel ​Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\  
-| DUNES- Cold Disks around Nearby Stars. A search for Edgeworth-Kuiper Belt analogues ​//(PI: C. Eiroa)//|** [[Herschel Dunes|Here]]**|\\ +|[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]|  \\ 
-  ​* ​EPoS- The earliest phases of star formation: From low- to high-mass objects ​//(PI: O. Krause)// **[[Herschel ​EPoS|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)]] \\ 
-  ​* ​GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel ​//(PI: D. Elbaz)// **[[Herschel ​GOODS|Here]]**  \\ +|[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ 
-  ​* ​H-ATLAS- The Herschel Thousand Degree Survey ​//(PI: S. Eales)// **[[Herschel H-atlas|Here]]**\\ +|[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ 
-  ​* ​Herschel Lensing Survey ​//(PI: E. Egami)// **[[Herschel Lensing Survey|Here]]**\\ +|[[Herschel HELGA|HELGA- The Herschel Exploitation of the Local Galaxy Andromeda (PI: J. Fritz)]]|\\ 
-  ​* ​HELGA- The Herschel Exploitation of the Local Galaxy Andromeda ​//(PI: J. Fritz)// **[[Herschel HELGA|Here]]**\\ +|[[Herschel Heritage|Heritage- HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds (PI: M. Meixner)]]|\\ 
-  ​* ​Heritage- HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds ​//(PI: M. Meixner)// **[[Herschel Heritage|Here]]**\\ +|[[Herschel Hermes|HerMES- The Herschel Multi-tiered Extragalactic Survey: Measuring the Infrared Galaxy Formation History of the universe (PI: S. Oliver)]]|\\ 
-  ​* ​HerMES- The Herschel Multi-tiered Extragalactic Survey: Measuring the Infrared Galaxy Formation History of the universe ​ //(PI: S. Oliver)// **[[Herschel Hermes|Here]]**\\ +|[[Herschel HerM33es|HerM33es- Herschel M33 Extended Survey (PI: C. Kramer)]]|\\ 
-  ​* ​HerM33es- Herschel M33 Extended Survey ​//(PI: C. Kramer)// **[[Herschel HerM33es|Here]]**\\ +|[[Herschel HeViCS|HeViCS- Herschel Virgo Cluster Survey (PI: J. Davies)]]|\\ 
-  ​* ​HeViCS- Herschel Virgo Cluster Survey ​//(PI: J. Davies)// **[[Herschel HeViCS|Here]]**\\ +|[[Herschel Hi-GAL|Hi-GAL- The Herschel infrared Galactic Plane Survey (S. Molinari)]]|\\ 
-  ​* ​Hi-GAL- The Herschel infrared Galactic Plane Survey ​//(S. Molinari)// **[[Herschel Hi-GAL|Here]]**\\ +|[[Herschel Hobys|Hobys- The Herschel imaging survey of OB Young Stellar objects (PI: F. Motte)]]|\\ 
-  ​* ​Hobys- The Herschel imaging survey of OB Young Stellar objects ​//(PI: F. Motte)// **[[Herschel ​Hobys|Here]]**\\ +|[[Herschel ​HRS|HRS- The Herschel Reference Survey (PI: S. Eales)]]|\\ 
-  ​* ​Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel ​//(R. Kennicutt)// **[[Herschel Kingfish|Here]]**\\ +|[[Herschel Kingfish|Kingfish- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (R. Kennicutt)]]|\\ 
-  ​* ​The ISM in Low Metallicity Environments:​ Bridging the Gap Between Local Universe and Primordial Galaxies ​//(PI: S. Madden)// **[[Herschel Madden|Here]]**\\ +|[[Herschel Madden|The ISM in Low Metallicity Environments:​ Bridging the Gap Between Local Universe and Primordial Galaxies (PI: S. Madden)]]|\\ 
-  ​* ​The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>​2 ​//(PI: K. Meisenheimer)// **[[Herschel Meisenheimer|Here]]**\\ +|[[Herschel Meisenheimer|The Dusty Young Universe: Photometry and Spectroscopy of Quasars at z>2 (PI: K. Meisenheimer)]]|\\ 
-  ​* ​SAG-4- Evolution of interstellar dust //(PI: A. Abergel)// **[[Herschel SAG-4|Here]]**\\ +|[[Herschel SAG-4|SAG-4- Evolution of interstellar dust (PI: A. Abergel)]]|\\ 
-  ​* ​VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies ​//(PI: C. Wlison)// **[[Herschel VNGS|Here]]** \\+|[[Herschel VNGS|VNGS- Physical Processes in the Interstellar Medium of Very Nearby Galaxies (PI: C. Wlison)]]|\\
  
 === Original WCS Data === === Original WCS Data ===