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FP line scan

In this example we consider a Fabry Perot line scan of a resolved line at 145.5 m. The continuum flux of the source is 1500 Jy at this wavelength, the integrated line flux is W/m. The velocity dispersion of the source is 100 km/s, giving a linewidth of 0.049 m. The line should be observed with 4 times oversampling, and with 5 resolution elements on either side of the line. The requested S/N on the line is 20.

  1. Calculate the required total S/N on line plus continuum (). First the equivalent continuum flux at the line center of the resolved line has to be calculated. This is done using equation 6.14 from the LWS Observers Manual (page 28):

    The total S/N can then be calculated (see equation 6.13 in the LWS Observers Manual, page 28):

  2. Calculate the S/N per ramp using equation 5

  3. Calculate the number of required ramps using equation 8:

    The number of required ramps is thus 26.

  4. Calculate the integration time per spectral point using equation 9. This gives in this case sec.
  5. Calculate the number of points in the scan using equation 11. This gives .
  6. Calculate the total integration time for the observation using equation 12: sec.
  7. Finally estimate the total time for the observation, taking the overheads into account (including the 180 seconds slewing overhead), using equation 13 and section 6.2. The overheads for this observation are: 180 sec for the slew to the target, 18 sec for the instrument setup, 38 sec for the setup of the FPL, 20 sec for the instrument switch off and 252 sec for the illuminator flashes. The total time for the AOT thus is: sec.
The LWS estimator gives 2152 seconds for this observation, excluding the slew overheads. The PGA software gives 2381 seconds. This proves that estimating the times for an observation using this cookery book may give results that differ significantly from the results given by the PGA software. The reason for this are the exact technical details of how the observation is performed. The observer is again reminded that the most reliable way of estimating observing times is by using the LWS Time Estimator (LTE), version 3.7, or the PGA software.



next up previous contents
Up: Worked examples Previous: Grating line scan



N.R. Trams, P.E. Clegg and B.M. Swinyard
Wed Aug 7 11:47:53 MET DST 1996