Here are observations of thermal SiO in W75N, as well as 43 GHz
continuum of the same source. Fast switching is applied.
This is the resulting observe file. Parts of the file are
marked in color, with explanations below. These are things you need
to look for in your observe file, to make sure the schedule is
correct.
| 21 20 00.0000 |
For a tipping scan this is the azimuth (in degrees) at which the tip should be performed. The important thing here is to avoid shadowing in the compact C and D configurations. |
| +20 00 00.000 |
The Dec determines whether the tip is done from low to high elevation, or from high to low elevation. Close to 23 degrees means from low to high elevations, while nearer to 55 degrees means the pass goes from high to low elevations. |
| TE |
This defines a tipping scan (set by specifying "Tipping scan" in the OBSERVE Source Page). |
| XX |
XX defines the observing frequency. Since this is a pointing scan, it should be in X-band. |
| IA |
This defines a referenced pointing scan with IF A (set by specifying "Det. ref. point." in the OBSERVE Source Page). |
| 10 |
The integration time in seconds. Make sure this is 10 for your pointing scan. |
| T |
This T shows that you are applying the pointing corrections to the observing scan (set by specifying "Referenced Pointing" in the OBSERVE Source Page). |
| 2222 |
Defines the bandwidth code for the 4 IFs, here 12.5 MHz |
| 1A |
Defines the correlator mode; 1A means single IF spectral processing on IF A. |
| //OF NOD SKY |
Fast switching is determined by this 'off-set' card in 'NOD SKY' mode |
| 20 38 36.5000 +42 37 33.500 |
RA and Dec of the first source in the fast switching cycle (here the target source). Note that in spectral line mode you want to have the first source in the cycle to be your target, since OBSERVE will Doppler track on the first source in this card. |
| 20 12 05.6373 +46 28 55.787 |
RA and Dec of the second source in the fast switching cycle (here the calibrator) |
| 85 55 |
The amount of time spent on the first and second source in the fast switching cycle (85 sec and 55 sec respectively). Move time is included. |
| VTL |
Important for spectral line: the //FI card defines the Fluke synthesizer frequencies. V stands for velocities according to the radio convention and that you define a rest frequency in addition to velocity of the source; T stands for center frequency reference and finally L for an LSR rest frame. If you are observing extragalactic targets you probably want to have "ZTB" instead of "VTL", where Z stands for optical velocity convention (and that you define a rest frequency in addition to velocity of the source), T as above and B for a barycentric rest frame. |
| 10.000 |
Fluke A and B velocities in km/s - the velocity of your target. |
| 43423.760000 43423.760000 |
Fluke A and B line rest frequencies in MHz - the line rest frequencies. |