Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision Next revision Both sides next revision | ||
herschel [2018/09/28 11:45] Déborah Paradis |
herschel [2018/10/09 15:30] Déborah Paradis |
||
---|---|---|---|
Line 20: | Line 20: | ||
__**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 ^ | ^Key Programs ^ | ||
- | |**[[Herschel Galactic Cold Cores|Galactic Cold Cores //(PI: M. Juvela & I. Ristorcelli)]]**|\\ | + | |[[Herschel DEBRIS|DEBRIS- Disc Emission via a Bias-free Reconnaissance in the Infrared/Sub-millimetre (PI : B. Matthews)]]|\\ |
- | |DEBRIS- Disc Emission via a Bias-free Reconnaissance in the Infrared/Sub-millimetre //(PI : B. Matthews)//|**[[Herschel DEBRIS|Here]]**|\\ | + | |[[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. Wlison)]]|\\ | ||
=== Original WCS Data === | === Original WCS Data === |