Recent Astronomical Research Utilizing a High Gain Image Intensifier Tube††Contribution of the Kitt Peak National Observatory, No. 135.

Author(s):  
W.C. Livingston ◽  
C.R. Lynds ◽  
L.A. Doe
1998 ◽  
Vol 162 ◽  
pp. 267-272
Author(s):  
K. Leather ◽  
F. Andrews ◽  
R. Hall ◽  
W. Orchiston

Carter Observatory is the National Observatory of New Zealand and was opened in 1941. For more than ten years the Observatory has maintained an active education program for visiting school groups (see Andrews, 1991), and education now forms one of its four functions. The others relate to astronomical research; public astronomy; and the preservation of New Zealands astronomical heritage (see Orchiston and Dodd, 1995).Since the acquisition of a small Zeiss planetarium and associated visitor centre in 1992, the public astronomy and education programs at the Carter Observatory have witnessed a major expansion (see Orchiston, 1995; Orchiston and Dodd, 1996). A significant contributing factor was the introduction by the government of a new science curriculum into New Zealand schools in 1995 (Science in the New Zealand Curriculum, 1995). “Making Sense of Planet Earth and Beyond” comprises one quarter of this curriculum, and the “Beyond” component is astronomy.


1980 ◽  
Vol 51 (1) ◽  
pp. 616-618
Author(s):  
G. N. Chapman ◽  
J. C. Ramage ◽  
A. J. Walton
Keyword(s):  

Author(s):  
Kenneth H. Downing ◽  
Ming-Hsiu Ho ◽  
Robert M. Glaeser

We have investigated the possibility of using a charge coupled device (CCD) as a direct, electron-sensitive readout device for a CTEM. Two-dimensional imaging CCD's, developed as normal television camera elements, are semiconductor devices in which an image is formed on an array of photo-sensitive sites, causing the accumulation of an electric charge proportional to the incident flux. The video signal is generated by sequentially transferring the charges for each element of a line, in bucket-brigade fashion, to the input of the video amplifier. Sensitivity of the CCD to electrons has been demonstrated by the successful application in photocathode tubes, where the photoelectrons are accelerated to an energy up to 15 keV onto the image sensing area of the CCD. The application of the device in a 100 keV transmission electron microscope (Ferrier and Chapman, private communication), with the device in vacuo at the image plane, seems to have promising possibilities for image intensifier, electron counting, and computer input devices. A CCD readout system should have several advantages over previously designed video readout systems, including elimination of the phosphor, fiber optic or lens coupling, and intermediate image intensifier stages. The high gain and low noise of the device should allow detection of single electrons with a detective quantum efficiency near unity.


1969 ◽  
Vol 15 (8) ◽  
pp. 258-260 ◽  
Author(s):  
A. R. Lang ◽  
K. Reifsnider

1998 ◽  
Vol 162 ◽  
pp. 214-219
Author(s):  
W. Orchiston ◽  
B. Carter ◽  
R. Dodd ◽  
R. Hall

Carter Observatory is the gazetted National Observatory of New Zealand, and opened in 1941 December. From the start, the main function of the Observatory was to provide for the astronomical needs of the citizens of, and visitors to, the Wellington region, and today this remains one of its four recognised functions (Orchiston and Dodd, 1995). The other three are to conduct astronomical research of international significance; provide a national astronomy education service for school students, teachers, and trainee teachers; and assist in the preservation of New Zealand's astronomical heritage.


Nature ◽  
1980 ◽  
Vol 284 (5751) ◽  
pp. 42-44 ◽  
Author(s):  
Alan J. Walton ◽  
N. C. Debenham

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