- ... telescope
- Appendices A and B are only available in electronic form at http://www.edpsciences.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... INTEGRAL
- INTErnational
Gamma-Ray Astrophysics Laboratory.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
WEBT
- Whole Earth Blazar Telescope.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... calibrators
- In Sect. 3.1
we show that this assumption was true for all the observed
extragalactic calibrators but 1642+690.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... "chopper-wheel
- Note that the "chopper-wheel''
calibration procedure (which at the 30 m telescope does not
use a chopper wheel) is totally unrelated to the
"beam-switching'' mode (which uses the chopper wheel).
This paradoxical nomenclature has been maintained
for historical reasons.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... source
- We assumed a negligible degree of circular polarization (
),
which is null for the observed Galactic sources and typically
<1% at cm and mm wavelengths for extragalactic AGN
(Clemens Thum private communication; Homan & Lister 2006
and references therein). In particular, at 86 GHz the measured
of 0716+714 is <0.4% (Clemens Thum,
private communication).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.