Radio Studies of Objects in the Large Bright Quasar Survey

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

More than one third of the Large Bright Quasar Survey (LBQS) has been observed at 8.4 GHz with the VLA. There is no correlation between radio luminosity and absolute blue magnitude for -28 < MB < -24, and the radio-loud (8.4 GHz luminosity > 10(25) W Hz(-1) ) fraction (10%) does not depend on absolute blue magnitude. There is some evidence for a substantially increased radio-loud fraction (36%) among objects with MB < -28. The frequency of powerful radio emitters appears to decrease smoothly with decreasing optical luminosity for MB > -24, a result which is probably not a selection effect (98% confidence) and represents a physical change in the radio properties of quasars. This was determined by applying the quantitative LBQS selection criteria to a test spectrum simulating a quasar embedded in a red elliptical host galaxy, in which the quasar and host galaxy have equal MB. The radio-loud fraction among all objects in the radio sample with MB > -24 is 3%. The radio-loud fraction remains constant at ~ 10 % from z = 0.5 to z > 3.5, and there is some evidence that this holds for z < 0.5. The distribution of log R (ratio of radio to optical luminosity) appears to be bimodal, with a gap at log R ~ 1 for all redshifts and absolute magnitudes.

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