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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