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Proceedings Paper

Utilisation Astrononique De La "Camera Electronique Grand Champ" Astronomical Use Of The "Large Field Electronographic Camera".
Author(s): G Wlerick; G Lelievre; B Servan; V Cayatte; D Michet; L Renard; D Horville
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Paper Abstract

The large field Lallemand electronographic camera is an ideal receptor for bidimensional photometry with large instruments. With the C.F.H. 3,6 m Telescope, the angular field is 10' at the Cassegrain F/8 focus ; in such a field, there is enough stars in the range 14 c V , 16 to start a decent electrographic sequence ; this sequence extends up to V = 21 and permits to measure stars up to V - 24 - 25.

Paper Details

Date Published: 9 January 1984
PDF: 8 pages
Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); doi: 10.1117/12.966140
Show Author Affiliations
G Wlerick, Observatoire de Paris (France)
G Lelievre, Observatoire de Paris (France)
B Servan, Observatoire de Paris (France)
V Cayatte, Observatoire de Paris (France)
D Michet, Observatoire de Paris (France)
L Renard, Observatoire de Paris (France)
D Horville, Observatoire de Paris (France)


Published in SPIE Proceedings Vol. 0445:
Instrumentation in Astronomy V
Alec Boksenberg; David L. Crawford, Editor(s)

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