Changes between Version 74 and Version 75 of HetProcedures/HighSpeedBib
- Timestamp:
- Oct 31, 2019 12:28:32 AM (5 years ago)
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HetProcedures/HighSpeedBib
v74 v75 140 140 [astronomer@mcs Bib]$ biblook 20191029_0910_1017.bmp N 141 141 }}} 142 Note that the image basename (20191029_0910_9) and file format (bmp) are specified as two distinct command line arguments. This was done in case the user wished to record other image formats (like tiff). The user places a circle marker around the star and enters a return . At that point the user is shown a single line of values. The last uotputline of the run should show what you need to know:142 The last output line of the run should show what you need to know: 143 143 {{{ 144 144 The final measured peak in the BIB star = 82.66 145 145 }}} 146 You can answer "N" to the next couple questions about cleaning files. It is the usual case that we delete all of the ASCII files made in this process since we are usually just measuring test images in preparation for taking the real data. In the above example we see that the peak level measured in our star image was 204 adu. This would be a safe level for taking high speed BIB images. 147 146 You can answer "N" to the questions about cleaning files. It is the usual case that we delete all of the ASCII files made in this process since we are usually just measuring test images in preparation for taking the real data. In the above example we see that the peak level measured in our star image was 82 adu. This would be a safe level for taking high speed BIB images. 148 147 149 148