Identification of GX3+1 from Lunar Occultations

Details Identification of GX3+1 from Lunar Occultations Identification of GX3+1 from Lunar Occultations

Jan 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.235..152j&link_type=abstract

Nature, Volume 235, Issue 5334, pp. 152-155 (1972).

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THE position of GX3+1 has previously been reported by Schnopper et al.1 with sufficient accuracy to allow the times of lunar occultations to be predicted to within about +/-3 min2. This uncertainty in the predicted time can be covered by the relatively brief observation period of the flight of a sounding rocket. Two of the present cycle of lunar occultations were predicted for the rocket range at Woomera, Australia, and were successfully observed: the first on September 27, 1971, by the Leicester X-ray Astronomy Group, and the second on October 24, 1971, by the Mullard Space Science Laboratory, UCL.

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