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Self-calibration

       

The most reliable method for removing atmospheric fluctuations from the data is self-calibration, if the target is strong enough. Self-calibration should be used if the signal-to-noise on the target is high enough to determine the gains in the typical coherence time tex2html_wrap_inline2543 of the atmospheric phase screen, using baselines involving all antennas. For an array of N elements, the r.m.s. noise in the determination of an individual antenna phase gain by self-calibration on a point source of flux density tex2html_wrap_inline2671 Jy will be

(4)  displaymath2688

where tex2html_wrap_inline2573 is the sensitivity in Jy per second per MHz of bandwidth, and tex2html_wrap_inline2675 is the averaging time used for the gain solutions. Unless tex2html_wrap_inline2677 when tex2html_wrap_inline2679 , self-calibration will not improve the data.

There are several reasons why external calibration is useful even if you know you will be able to self-calibrate your final images.

Fortunately, the class of source for which images of high dynamic range are most important is also the class for which self-calibration is most likely to work well--namely, those with weak extended structures around bright small-diameter components. There is however a range of flux densities and structural complexities over which self-calibration cannot be guaranteed to work in typical atmospheric coherence times tex2html_wrap_inline2543 , and for which external calibration therefore remains essential.


next up previous contents index external
Next: Position calibration Up: Atmospheric calibration Previous: External calibration

abridle@nrao.edu
Thu Jul 11 16:26:53 EDT 1996