Jets at Intermediate Redshifts: Shedding Light on Emission Mechanisms and Physics

Details Jets at Intermediate Redshifts: Shedding Light on Emission Mechanisms and Physics Jets at Intermediate Redshifts: Shedding Light on Emission Mechanisms and Physics

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2628s&link_type=abstract

Chandra proposal ID #10700299

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We propose observations of a small sample of intermediate-redshift radio jets (2=3-4) tend to confirm the IC/CMB origin of the X-ray emission, the limited morphological information available due to the faintness of the radio emission prevents more detailed studies. Observations at intermediate z will bridge the gap, allowing us to study the role of both the increase of the CMB energy and intergalactic matter densities on the X-ray emission properties and physics of jets.

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