Probing X-Ray Jet Emission Mechanisms in a Complete Blazar Sample

Details Probing X-Ray Jet Emission Mechanisms in a Complete Blazar Sample Probing X-Ray Jet Emission Mechanisms in a Complete Blazar Sample

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11831k&link_type=abstract

HST Proposal ID #11831. Cycle 17

Computer Science

Scientific paper

We propose deep {70 ksec} followup Chandra X-ray observations and new HST ACS/WFC/F475W observations of two quasars, viz., 0106+013 and 1641+399, belonging to the complete flux-limited MOJAVE Chandra blazar sample. These two quasars have HST WFPC2/F702W data available in the archive. Combining the existing optical and radio data with the new Chandra and HST data at an additional optical band we aim to construct a significantly more accurate multi-waveband {four frequency} spectral energy distributions for distinct knots in the jets. This will serve as a first step towards resolving longstanding ambiguities surrounding the primary X-ray emission mechanisms in a well-defined sample of powerful FR-II class jets.;

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