Share Email Print

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
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

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)

© SPIE. Terms of Use
Back to Top