The Infrared Astronomical Satellite (IRAS) scanned the celestial sphere during 1983 through bandpasses centered at wavelengths of 12, 25, 60 and 100 microns. In addition to sources fixed on the sky, many moving objects were observed. This data set is the largest and least biased survey of asteroids and comets ever conducted. Included are main belt asteroids, Mars-crossers, earth-approachers, and Trojans. Measurements for the known asteroids have been reduced and organized into a number of data products which are available to researchers. The data for 'new' asteroids are being processed.


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    Titel :

    IRAS survey of asteroids


    Beteiligte:
    Matson, D. L. (Autor:in) / Veeder, G. J. (Autor:in) / Tedesco, E. F. (Autor:in) / Lebofsky, L. A. (Autor:in) / Walker, R. G. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1986-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    IRAS survey of asteroids

    Matson, D.L. / Veeder, G.J. / Tedesco, E.F. et al. | Elsevier | 1987


    The IRAS faint source survey

    Moshir, Mehrdad | NTRS | 1991


    IRAS galaxies in the ROSAT survey

    Boller, T. | British Library Online Contents | 1992



    Cosmological studies with the IRAS 60 μm survey

    Rowan-Robinson, Michael | Elsevier | 1991