Completing a Flux-limited Survey for X-ray Emission from Radio Jets

Details Completing a Flux-limited Survey for X-ray Emission from Radio Jets Completing a Flux-limited Survey for X-ray Emission from Radio Jets

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11838m&link_type=abstract

HST Proposal ID #11838. Cycle 17

Physics

Scientific paper

We will measure the changing flow speeds, magnetic fields, and energy fluxes in well-resolved quasar jets found in our short-exposure Chandra survey by combining new, deep Chandra data with radio and optical imaging. We will image each jet with sufficient sensitivity to estimate beaming factors and magnetic fields in several distinct regions, and so map the variations in these parameters down the jets. HST observations will help diagnose the role of synchrotron emission in the overall SED, and may reveal condensations on scales less than 0.1 arcsec.;

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