GASKAP-the galactic ASKAP survey
- Dickey, John M.
- McClure-Griffiths, Naomi
- Gibson, Steven J.
- G\uf3mez, Jos\ue9 F.
- Imai, Hiroshi
- Jones, Paul
- Stanimirovi\u107, Sne\u17eana
- Van Loon, Jacco Th.
- Walsh, Andrew
- Alberdi, A.
- Anglada, G.
- Uscanga, L.
- Arce, H.
- Bailey, M.
- Begum, A.
- Wakker, B.
- Bekhti, N. Ben
- Kalberla, P.
- Winkel, B.
- Bekki, K.
- For, B.-Q.
- Staveley-Smith, L.
- Westmeier, T.
- Burton, M.
- Cunningham, M.
- Dawson, J.
- Ellingsen, S.
- Diamond, P.
- Green, J. A.
- Hill, A. S.
- Koribalski, B.
- McConnell, D.
- Rathborne, J.
- Voronkov, M.
- Douglas, K. A.
- English, J.
- Ford, H. Alyson
- Lockman, F. J.
- Foster, T.
- Gomez, Y.
- Green, A.
- Bland-Hawthorn, J.
- Gulyaev, S.
- Hoare, M.
- Joncas, G.
- Kang, J.-H.
- Kerton, C. R.
- Koo, B.-C.
- Leahy, D.
- Lo, N.
- Migenes, V.
- Nakashima, J.
- Zhang, Y.
- Nidever, D.
- Peek, J. E. G.
- Tafoya, D.
- Tian, W.
- Wu, D.
DOIAbstract
A survey of the Milky Way disk and the Magellanic System at the wavelengths of the 21-cm atomic hydrogen (H i) line and three 18-cm lines of the OH molecule will be carried out with the Australian Square Kilometre Array Pathfinder telescope. The survey will study the distribution of H i emission and absorption with unprecedented angular and velocity resolution, as well as molecular line thermal emission, absorption, and maser lines. The area to be covered includes the Galactic plane (|b| < 10\ub0) at all declinations south of \u3b4 = +40\ub0, spanning longitudes 167\ub0 through 360\ub0to 79 at b = 0\ub0, plus the entire area of the Magellanic Stream and Clouds, a total of 13 020 deg2. The brightness temperature sensitivity will be very good...
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