Optical follow-up identifications of hard X-ray/soft γ-ray sources discovered by the "SIGMA" telescope.

Details Optical follow-up identifications of hard X-ray/soft γ-ray sources discovered by the "SIGMA" telescope. Optical follow-up identifications of hard X-ray/soft γ-ray sources discovered by the "SIGMA" telescope.

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990msngr..60...16b&link_type=abstract

The Messenger, vol. 60, p. 16-18

Physics

3

X-Ray Sources: Optical Identifications, Gamma-Ray Sources: Optical Identifications

Scientific paper

The aim of this programme is to search for the optical counterparts of hard X-raylsoft y-ray sources (including y-ray bursts and transient events) discovered by the SIGMA telescope (successfully launched on December 1, 1989), also exploiting the soft X-ray data of the all sky survey to be performed by the ROSAT satellite (launched on May 31, 1990).

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