We finish with two examples, the first being for selfcal.
SELFCAL | |
vis=vela.uv.cal | Visibility data-set to be corrected, |
Generally I,Q,U,V visibilities. | |
model=vela.icmp | CLEAN component image |
select | Data to select. |
interval=5 | Self-cal solution interval. |
options=phase | Phase self-calibration, or |
options=amp | Amplitude self-calibration, or |
options=phase,mfs | Phase-selfcal, MFS model, or |
options=amp,mfs | Amplitude self-cal, MFS model |
line | You need to specify this for MFS selfcal, |
can generally default otherwise. |
GPSCAL | |
vis=vela.uv.cal | Visibility data-set to be corrected, |
Should be XX,YY,XY,YX visibilities. | |
model=vela.icmp,vela.qcmp,vela.ucmp | CLEAN component images |
select | Data to select. |
interval=5 | Self-cal solution interval. |
options=phase | Phase self-calibration, or |
options=amp,xyvary | Amplitude self-calibration, or |
options=phase,mfs | Phase-selfcal, MFS model, or |
options=amp,mfs,xyvary | Amplitude self-cal, MFS model |
line | You need to specify this for MFS selfcal, |
can generally default otherwise. |
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