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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    Titel :

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


    Beteiligte:
    Gilfanov, M.R. (Autor:in) / Sunyaev, R.A. (Autor:in) / Churazov, E.M. (Autor:in) / Babalyan, G. (Autor:in) / Pavlinsky, M. (Autor:in) / Yamburenko, N.S. (Autor:in) / Khavenson, N. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1991-01-01


    Format / Umfang :

    6 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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