PointingModelOffsets » History » Version 11
Pointing Model Offsets¶
In order to study the effects the pointing model may have on the offsets, new offsets were calculated with possible corrections from the effects of the hexapod trim values.
The following histograms show the distribution of the offsets before trim corrections, and with a trim correction of both addition and subtraction.
RA offset with: No correction, addition of a scaled (.0176 arcsec/micron) trim_dy value, subtraction of the scaled trim_dy value
Dec offset with: No correction, addition of a scaled (.0176 arcsec/micron) trim_dx value, subtraction of the scaled trim_dx value
The effect of the corrections are arguably more visible on a 3D plot. The following show the tweak values and exposure ID values (essentially time, in order to better show the exposure groups)
versus the offsets.
Blue = Original offsets
Green = Original offsets + (.0176 * trim)
Red = Original offsets - (.0176 * trim)
Declination offsets vs trim_dy (vs expid):
By applying trim corrections, the offsets should no longer include the part of the offset due to hexapod corrections.
As can be seen, adding the correction (green) makes each set of four data points taken in the same position much more horizontal, removing correlation with trim values.
Subtracting the correction makes each set of four data point correlate much more strongly with trim values.
After applying the correction, the offsets can then be reexamined for correlations with the telescopes position. The plots below illustrate the relations. Each set of graphs
has the correction applied in both directions.
The following two plots show the Declination offsets plotted against the declination of the telescope. The color scale shows the HA of the telescope.Correction added and correction subtracted, respectively
The following two plots show the RA offsets plotted against the declination of the telescope. The color scale shows the HA of the telescope.Correction added and correction subtracted, respectively