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Relation between \ensuremath{t_\ensuremath{\mathrm{onoff}}} and \ensuremath{\ensuremath{t_\ensuremath{\mathrm{sig}}}^\ensuremath{\mathrm{beam}}}

By construction

Both \ensuremath{\ensuremath{t_\ensuremath{\mathrm{sig}}}^\ensuremath{\mathrm{beam}}} and \ensuremath{t_\ensuremath{\mathrm{onoff}}} are proportional to $\ensuremath{n_\ensuremath{\mathrm{cover}}}\,\ensuremath{t_\ensuremath{\mathrm{submap}}}$ (cf. Eqs. [*] and [*]). It is thus easy to derive that
\begin{displaymath}
\ensuremath{t_\ensuremath{\mathrm{onoff}}}= \ensuremath{\en...
...sqrt{\ensuremath{n_\ensuremath{\mathrm{on/off}}}} \right) }^2.
\end{displaymath} (34)

Using Eq. [*], we can replace \ensuremath{n_\ensuremath{\mathrm{on/off}}} and obtain
\begin{displaymath}
\ensuremath{t_\ensuremath{\mathrm{onoff}}}= \ensuremath{\en...
...sqrt{\ensuremath{n_\ensuremath{\mathrm{beam}}}} \right) }^2.
\end{displaymath} (35)

Using Eqs. [*], [*] and [*], we obtain
\begin{displaymath}
\ensuremath{\sigma_\ensuremath{\mathrm{psw}}} =
\frac{\ens...
...th{\mathrm{tel}}}\,\ensuremath{t_\ensuremath{\mathrm{tel}}}}}.
\end{displaymath} (36)

The last equation in theory enables us to find the rms noise as a function of the elasped telescope time (sensitivity estimation) and vice-versa (time estimation). However, it is not fully straightforward because we must enforce that \ensuremath{n_\ensuremath{\mathrm{cover}}} and \ensuremath{n_\ensuremath{\mathrm{submap}}} have an integer value.


next up previous contents
Next: Time/Sensitivity estimation Up: Position switched Previous: Two key points: 1)   Contents
Gildas manager 2014-07-01