Catalogue of the Rozhen Observatory Schmidt Telescope

1994 ◽  
pp. 377-379
Author(s):  
A. Mutafov ◽  
P. Ilcheva ◽  
M. Kusheva ◽  
M. Michailov ◽  
Z. Borisov ◽  
...  
Keyword(s):  
1966 ◽  
Vol 24 ◽  
pp. 337
Author(s):  
W. Iwanowska

A new 24-inch/36-inch//3 Schmidt telescope, made by C. Zeiss, Jena, has been installed since 30 August 1962, at the N. Copernicus University Observatory in Toruń. It is equipped with two objective prisms, used separately, one of crown the other of flint glass, each of 5° refracting angle, giving dispersions of 560Å/mm and 250Å/ mm respectively.


1998 ◽  
Vol 7 (4) ◽  
Author(s):  
A. Alksnis ◽  
A. Balklavs ◽  
I. Eglītis ◽  
O. Paupers
Keyword(s):  

1976 ◽  
Vol 31 ◽  
pp. 124-129
Author(s):  
S. Röser

In recent years satellite observations of the region of the Earth-Moon libration points L4 and L5 became available, which showed different results. Roach (1975) has measured perturbations of the Zodiacal Light intensity near the libration points L4 and L5 with a photometer on board the OSO-6 satellite. He interpreted the results as counterglow of a cloud of particles, having an angular diameter of 6 degrees and an average brightness of 20 S10v, whereas observations by Burnett et al. (1974) set an upper limit of 10 S10 blue. Earth bound observations made by Bruman (1969) with the 48-inch Palomar Schmidt telescope gave no indication for discrete objects nor for clouds.


Supernovae ◽  
1991 ◽  
pp. 724-726
Author(s):  
Christian Pollas
Keyword(s):  

1992 ◽  
Vol 258 (3) ◽  
pp. 521-526 ◽  
Author(s):  
D. E. Holmgren ◽  
R. J. H. McCausland ◽  
P. L. Dufton ◽  
F. P. Keenan ◽  
D. Kilkenny

1988 ◽  
pp. 234-238 ◽  
Author(s):  
C. M. Humphries ◽  
D. H. Morgan
Keyword(s):  

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