Co-ordinated VSOP and Chandra observations of 0836+710

Details Co-ordinated VSOP and Chandra observations of 0836+710 Co-ordinated VSOP and Chandra observations of 0836+710

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205..126m&link_type=abstract

Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at

Computer Science

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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 high redshift (z=2.17) superluminal 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 the VLBA co-observing with the HALCA spacecraft (which is the space element of the Japanese VSOP mission). The aim of the radio observations is to determine the peak brightness temperature for each of the VLBI radio components and hence provide better constraints on predicted X-ray emission than has previously been possible from radio data. Combining the radio data with the X-ray data enables the nature of this gamma-ray loud AGN to be further elucidated.

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