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*Date on this monitor changes at 21:00 UT | |||||||||||||||||||||||||||||||||||||||||||
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QC1 plotter
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| Plot [info] |
Symbol [info] |
Source* | Average [info] | Thresholds [info] | N_data | Data downloads | Remarks | ||||
| method | value | unit | method | value | |||||||
| 1 | • | QC1DB | MEDIAN | 516.01758 | PIXEL | none | 375 | this | last_yr | all | X-position of the slit image | ||
| 2 | • | QC1DB | MEDIAN | 499.50000 | PIXEL | none | 375 | this | last_yr | all | Y-position of the slit image | ||
| 3 | • | QC1DB | MEDIAN | -89.51372 | DEGREE | none | 375 | this | last_yr | all | Tilt angle of the slit image | ||
| 4 | • | QC1DB | MEDIAN | 8931412.00000 | ADU | none | 375 | this | last_yr | all | integrated flux of the slit image | ||
| *Data sources: QC1DB: QC1 database; LOCAL: local text file | |||||||||||
This is the trending plot of the through slit images taken as part of the acquisition template for spectroscopy.
This plot describes:
1. The x-position of the slit image.
2. The y-position of the slit image.
3. The tilt angle of the slit image.
4. The flux of the slit image.
The ISAAC acquisition template used for spectroscopy (science observations as well as standard stars use to calibrate telluric lines) generates an acquisition image, or a difference image with TPL.EXPNO=1, followed by an unpredicted number of through slit images taken in an interactive way by the night time astronomer to align the optics. Only the first in the sequence of the through slit images with TPL.EXPNO=2 is investigated here to check how far the camera has been moved after the last alignment. Find more information about ISAAC slit frames here.
Click on any of the plots to see a close-up version.
The latest date is indicated on top of the plot, data points belonging to that date are specially marked. If configured,
General information