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| run_amber_processQC.sh | run_amber_bpos_qcDocu.sh | run_amber_p2vm_qcDocu.sh | run_amber_calib_fringe_qcDocu.sh |
. ~/Isabelle/SCRIPTS/MeasureQuality/run_amber_processQC.sh.averaged $RAW_TYPE $DATE $PF
amber_bpos,amber_p2vm,amber_calibrators_K (JH),amber_cutoff, amber_science_fringe (KJH)
>trend_report_BPOS_shiftK_noBCD_HC.html
| >trend_report_P2VM_LJHK_HC.html
| >trend_report_WINDOW_SM_HC.html
| >trend_report_SNR_HC.html
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trend_report_BPOS_shiftK_noBCD_HC.png
trend_report_P2VM_LJHK_HC.png
trend_report_WINDOW_SM_HC.png
trend_report_SNR_HC.png
product_name.fits.gif
QC1db names: amber_bpos | amber_p2vm | amber_cutoff | amber_calibrators_K(JH) | amber_science_fringe (KHJ)
FITS key names for BPOS: QC.REFPIX.A/B/C.K/H/J.SHX/SHY | QC.REFPIX.A/B/C.K/H/J.X/Y | QC.REFPIX.A/B/C.K/H/J.FLUX/PEAKFLUX/SIZX/SIZY/ANGLE
FITS key names for P2VM: QC.P1/2/3.OFFSETX/Y | QC.P2VM.K/H/J.VIS12/VIS23/VIS31 | QC.P2VM.K/H/J.ERRVIS12/ERRVIS23/ERRVIS31
FITS key names for cutoff: CHANMAX/MIN | LAMBDAMAX/MIN |
FITS key names for SNR (amber_calibrators_K/H/J and amber_science_fringeKHJ): QC.FRAMES.SELECTED.SNRGT2 | QC.FRAMES.SELECTED.PERCENT
QC1 params created by pipeline: all (except cutoff)
QC1 params created by this procedure: CHANMAX/MIN | LAMBDAMAX/MIN
BPOS: HC calibration: under Position Ref. measure the XY position of the beam for the 3 beams ABC and the JHK bands. The shift between these different settings and the amber reference (coldstop) is calculated.
BPOS: HC calibration: under Flux Angle Ref. measure the flux, the flux on the peak, the position angle and the size in X and Y of the beam for the 3 beams ABC and the JHK bands.
BPOS: HC calibration: under LAMP. monitoring of the LAMP in (XY, FLUX and SIZZE) for beam A/B/C in J/H/K
Description of algorithms:
P2VM: Calculate the internal instrumental Visibility for the different instrumental settings (Low, Medium and High resolution) and for the 3 baselines (12, 23, 31). The Spectral Configuration is given by OCS.OBS.SPECCONF or INS.MODE, teh observing band by QC.BAND. When observing in Low Resolution JHK or Medium Resolution the offsets between the different photometric channels is also measured
Description of algorithms:
Cutoff: When fringes are obtained in Low Resolution, we monitor the cutoff of the K spectruum, this has been an issue with AMBER and needs to be monitor to insure that the full K spectruum is present in the raw data.
Description of algorithms:
SNR: When fringes are obtained, teh number of frames with a SNR >= 2 is calculated.
(guidelines for acceptance/rejection): for the fringe files, check the Vis2=f(SNR), the shape of the spectruum and the shape of the dispersed fringes (!! still fringes for MR and HR)
To see the individual qcDocu comments, please check the individual documentations