Minimum and Maximum Acceptable Integration Times for VLA Observing

Ken Sowinski (original November 26, 1996)
Gustaaf van Moorsel (update March 13, 2007)
Gustaaf van Moorsel (update November 21, 2007)

A word of caution

As we are finding out details of the constraints posed by the new Modcomp independent system, the numbers given below are subject to change. Though we will attempt to keep this table up-to-date, this should be taken as a warning that in the future it may not always be accurate. When in doubt, please consult Ken Sowinski or Gustaaf van Moorsel.

Minimum Integration Time - Continuum

For continuum observing we routinely support an integration interval of 1-2/3 seconds. It is possible to specify integration intervals as short as 5/12 seconds if needed, but this places a noticable strain on the system and is discouraged.

Minimum Integration Time - Spectral Line

In the case of spectral line observations, the greater amount of data and processing make a short integration interval impossible, and the limits cannot be expressed as succinctly. The table below shows the minimum achievable integration time (in seconds) as a function of the total number of channels per baseline, and the number of IFs, for a single 27 antenna subarray. Note that the total number of antennas per baseline is the total number of channels multiplied by the total number of IFs.

A few notes: