Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision | |||
|
amigps [2021/07/21 12:06] Déborah Paradis |
amigps [2023/04/11 15:17] (current) Déborah Paradis |
||
|---|---|---|---|
| Line 3: | Line 3: | ||
| This 15.7 GHz survey has been carried out using the Arcminute Microkelvin Imager Small Array , which is operated by the Cavendish Astrophysics Group at Lord's Bridge, Cambridgeshire. It is a radio synthesis telescope comprising ten 3.7-m diameter dishes. | This 15.7 GHz survey has been carried out using the Arcminute Microkelvin Imager Small Array , which is operated by the Cavendish Astrophysics Group at Lord's Bridge, Cambridgeshire. It is a radio synthesis telescope comprising ten 3.7-m diameter dishes. | ||
| The AMI Galactic Plane Survey is a large survey of the Galactic Plane, covering the area 76°<l<170° between latitudes of ıbı<5°. The angular resolution is approximately 3'. | The AMI Galactic Plane Survey is a large survey of the Galactic Plane, covering the area 76°<l<170° between latitudes of ıbı<5°. The angular resolution is approximately 3'. | ||
| - | The units of the HEALPix maps are ''Jy/Beam''. | + | The units of the HEALPix maps are ''Jy/Beam''. \\ |
| + | |||
| + | Healpix maps made by D. Paradis. | ||
| ===Reference=== | ===Reference=== | ||