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If the PI wants to reach the same rms noise (
) on
sources
(they must share the same calibrator sources), during a given elapsed
telescope time (
), we have
|
(2) |
where
is the time required to acquire the calibration information
and
the number of such calibration suits.
The calibration time can be written as
|
(3) |
where
,
,
and
are
respectively the typical times needed to perform a pointing, focus and
skydip measurement and an OnOff measurement on a calibrator.
is a multiplicative factor which takes into account
the time to slew to the pointing and/or focus source as well as the
possible need to do such calibrations twice in a row. The number of such
calibrations is dictated by the fact that the maximum duration between two
such calibration suits must be
. This gives
|
(4) |
The time spent per source (
) is linked to the integration time
(
) through the succession of
subscans, each subscan
having an on-source integration time of
and an overhead time of
. The
subscans are grouped into scans, with
an additional overhead time of
per scan. If one scan can
contain at most
subscans, the number of scans (
) and
the residual number of subcans (
) are computed through
We note that the actual number of scan is
when
and
when
. The time spent per source is thus given by
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Gildas manager
2014-07-01