On the SEDs of Jets at Redshifts between 0.01 and 3.8

Details On the SEDs of Jets at Redshifts between 0.01 and 3.8 On the SEDs of Jets at Redshifts between 0.01 and 3.8

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..380..257a&link_type=abstract

At the Edge of the Universe: Latest Results from the Deepest Astronomical Surveys ASP Conference Series, Vol. 380, proceedings o

Astronomy and Astrophysics

Astronomy

Scientific paper

We have been studying the spectral energy distributions (SEDs) of radio selected objects: the core-jet flat-spectrum low-luminosity objects from the 200-mJy sample (0.01 < z < 0.28) and the relativistic-jet flat-spectrum objects from the Caltech-Jodrell Bank (CJF) sample (0.01 < z < 3.8). We compare the radio luminosity range and peak frequency distribution of different samples, and we do not find evidence for the ``blazar sequence'', a model that proposes an anti-correlation between synchrotron peaks and radio power. We conclude that the luminosity is not the main parameter that controls the jet SED's colour.

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