VSOP and Chandra Observations of 0836+710

Details VSOP and Chandra Observations of 0836+710 VSOP and Chandra Observations of 0836+710

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..219m&link_type=abstract

Astrophysical Phenomena Revealed by Space VLBI, Proceedings of the VSOP Symposium, held at the Institute of Space and astronauti

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we describe the radio observations that form part of co-ordinated Chandra, HALCA+VLBA, and VLBA-only observations of the gamma-ray loud quasar 0836+710. The radio observations were at 6 frequencies (1.6, 5, 8, 15, 22, and 43 GHz) with the two lower frequency observations being undertaken with HALCA co-observing with the VLBA. The aim of the radio observations is to determine the peak brightness temperature of each of the VLBI components and hence provide better constraints on predicted X-ray emission than has previously been possible.

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