This table lists the measured image shifts induced by the filters as
measured from calibration observations of standard stars. Since no
observations of a standard star can be taken with just the CLEAR
filters, all the positions have been measured relative to the F120M
image position to an accuracy of +/- 1 pixel. The offsets are listed
such that:
Offset = Filter position - F120M position
| Filter | Offset(X) | Offset(Y) |
|---|---|---|
| F120M | =0 | =0 |
| F130M | 0 | 0 |
| F140M | 0 | 0 |
| F140W | -1 | 2 |
| F152M | 0 | 0 |
| F170M | 0 | 0 |
| F165W | 1 | 1 |
| F175W | -1 | 1 |
| F190M | 1 | 0 |
| F210M | 1 | 0 |
| F220W | -1 | 2 |
| F231M | 1 | -3 |
| F253M | -1 | 3 |
| F275W | -1 | 2 |
| F278M | -2 | 4 |
| F307M | -2 | 5 |
| F320W | -73 | 46 |
| F342W | -1 | -2 |
| F346M | -5 | 6 |
| F372M | -4 | 6 |
| F410M | -12 | 17 |
| F430W | 1 | 8 |
| F370LP | 0 | 2 |
| F480LP | -1 | 1 |
| F486N | -6 | 16 |
| F501N | 11 | 0 |
| F502M | -1 | -7 |
| F600M | 24 | 11 |
| F550M | -1 | -5 |
| F1ND | 0 | 0 |
| F2ND | 1 | 0 |
| F4ND | 0 | -1 |
| F6ND | 0 | 0 |