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Changes between Version 6 and Version 7 of GPC1_BrightStarAstrometry_SW_LH_scan


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Timestamp:
Apr 26, 2011, 5:06:07 PM (15 years ago)
Author:
watersc1
Comment:

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  • GPC1_BrightStarAstrometry_SW_LH_scan

    v6 v7  
    11= Second Microtest Set =
     2[[wiki:GPC1_BrightStarAstrometry_MT2_Noise]]
    23
    34This data set consisted of two exposures taken with the default voltages, one with the microtest 05 voltages (SW_L = default - 1.0 V, SW_H = default - 1.0 V), and six others that vary only SW_L or SW_H (with the other set to the default value).  To study the impact of these changes, I reduced the data as before, and found the best fit lines in the dx and dy offsets as a function of instrumental magnitudes.  The data were binned using 0.1 magnitude bins, and the fit performed between -14 and -12 (other fits were performed using ranges (-16:-14) and (-12:-10), but are not shown here).