| 34 | | At present atlod applies the XYPhase during filling. Nothing else (except maybe atxy) uses them. |
| 35 | | So we can compute the corrections, apply them and drop the XYPhase information, during ATLOD? |
| 36 | | May need to order the RPFITS data stream so that autocorrelations come before cross-correlations |
| 37 | | (and after SYSCAL records), so that the corrections for the cross-correlation can be computed |
| 38 | | before reaching the cross-correlations. |
| 39 | | We will need to carry Tsys info along but may be able to do it more compactly than storing the autocorrelations themselves. |
| 40 | | |
| 41 | | Research required: The phase values computed on a per channel basis will be noisy, and applying them will just introduce noise. |
| 42 | | We need to understand how much smoothing across frequency will be needed. |
| 43 | | Need to do some experiments to understand the sequence of events in reading in a file. |
| | 34 | At present atlod applies the XYPhase during filling. Nothing else (except maybe atxy) uses them. |
| | 35 | So we can compute the corrections, apply them and drop the XYPhase information, during ATLOD? |
| | 36 | May need to order the RPFITS data stream so that autocorrelations come before cross-correlations |
| | 37 | (and after SYSCAL records), so that the corrections for the cross-correlation can be computed |
| | 38 | before reaching the cross-correlations. |
| | 39 | We will need to carry Tsys info along but may be able to do it more compactly than storing the autocorrelations themselves. |
| | 40 | [BR] |
| | 41 | Research required: The phase values computed on a per channel basis will be noisy, and applying them will just introduce noise. |
| | 42 | We need to understand how much smoothing across frequency will be needed. |
| | 43 | Need to do some experiments to understand the sequence of events in reading in a file. |
