Abstract Coded mask telescope ART-P onboard internatio n al a s trophysical observatory “GRANAT” is capable to reconstruct images of 1.8 × 1.8 (FWHM) fields of sky and to obtain spectra of sources in 4–30 keV energy range. Telescope is operation in “photon by photon” mode with time resolution ∼4 ms, which makes this telescope appropriate for X-ray pulsar observations. First results of some well known pulsar observations in 1990 February–August are presented below.


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    Title :

    First results of X-ray pulsar observations with the ART-P telescope onboard “GRANAT” observatory


    Contributors:

    Published in:

    Publication date :

    1991-01-01


    Size :

    6 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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