The Oxford SWIFT spectrograph: First commissioning and on-sky results
The Oxford SWIFT spectrograph, an I and z band (6500-10500 A) integral field spectrograph, is designed to operate as a facility instrument at the 200 inch Hale Telescope on Palomar Mountain, in conjunction with the Palomar laser guide star adaptive optics system PALAO (and its upgrade to PALM3000)....
Asıl Yazarlar: | Thatte, N, Tecza, M, Clarke, F, Goodsall, T, Fogarty, L, Houghton, R, Salter, G, Scott, N, Davies, R, Bouchez, A, Dekany, R |
---|---|
Materyal Türü: | Journal article |
Dil: | English |
Baskı/Yayın Bilgisi: |
2010
|
Benzer Materyaller
-
The Oxford SWIFT integral field spectrograph - art. no. 62693L
Yazar:: Thatte, N, ve diğerleri
Baskı/Yayın Bilgisi: (2006) -
Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z=0.77
Yazar:: Kassin, SA, ve diğerleri
Baskı/Yayın Bilgisi: (2011) -
Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z= 0.77
Yazar:: Kassin, SA, ve diğerleri
Baskı/Yayın Bilgisi: (2011) -
SWIFT: An adaptive optics assisted I/z band integral field spectrograph
Yazar:: Tecza, M, ve diğerleri
Baskı/Yayın Bilgisi: (2006) -
SWIFT Observations of the Arp 147 Ring galaxy system
Yazar:: Fogarty, L, ve diğerleri
Baskı/Yayın Bilgisi: (2011)