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 11:55] Déborah Paradis |
herschel [2018/10/09 15:10] 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)]]|\\ | |[[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)]]|\\ | |[[Herschel Dunes|DUNES- Cold Disks around Nearby Stars. A search for Edgeworth-Kuiper Belt analogues (PI: C. Eiroa)]]|\\ | ||
| |[[Herschel EPoS|EPoS- The earliest phases of star formation: From low- to high-mass objects (PI: O. Krause)]]|\\ | |[[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)]]|\\ | ||
| |[[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 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)]]|\\ | ||
| Line 34: | Line 34: | ||
| |[[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)]]|\\ | ||