SPHERE: IRDIS Flat Field
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HC PLOTS |
counts in brightest CI flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
counts in brightest DBI flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
counts in brightest DPI flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
counts in brightest LSS flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
room mean square of CI master flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
room mean square of DBI master flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
room mean square of DPI master flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
room mean square of LSS master flat |
![](/observing/dfo/quality/ALL/img/sq1.png) |
fixed pattern noise in CI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
fixed pattern noise in DBI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
fixed pattern noise in DPI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
fixed pattern noise in LSS mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
number of bad pixel in CI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
number of bad pixel in DBI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
number of bad pixel in DPI mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
number of bad pixel in LSS mode |
![](/observing/dfo/quality/ALL/img/sq1.png) |
QC1 database (advanced users):
browse |
plot
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The IRDIS arm is operated in four modes:
- CI: classical imaging, the dual beam filter ( INS1.OPTI2.NAME ) is CLEAR
- DBI: dual beam imaging, the dual beam filter ( INS1.OPTI2.NAME ) is one of D_Y23, D_J23, D_H23 or D_K12.
- DPI: differential polarimetric imaging, the dual beam filter ( INS1.OPTI2.NAME ) is one of P0-90, P45-135
- LSS: long slit spectroscopy is flatfielded with imaging flats with dual beam filter=CLEAR and common beam filter being one of W_YJH and W_YHJKs
IRDIS lamp flats are acquired during daytime. The template generates five raw frames with increasing countrate
![](/qc/SPHERE/img/IRDIS_CLI_FLAT.png) |
IRDIS CI master flat using common filter wheel B_H filter and no filter in the dual beam filter wheel
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![](/qc/SPHERE/img/IRDIS_DBI_FLAT_RAW.png) |
IRDIS DBI raw flat (last in the sequence with highest flux), using common filter wheel B_Ks filter and dual beam filter D_K12.
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![](/qc/SPHERE/img/IRDIS_DBI_FLAT.png) |
IRDIS DBI master flat, using common filter wheel B_Ks filter and dual beam filter D_K12.
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IRDIS Flat counts
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[derived from QC procedure] | sphere_irdis_flat..qc_adu_left_4 | counts in the fifth exposure | HC | | [docuSys coming] |
[derived from QC procedure] | sphere_irdis_flat..qc_adu_right_4 | counts in the fifth exposure | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The counts in the brightest flat (the fifth raw flat) is monitored. More
precisely, the QC script takes the last raw frame generated by the
template (which is the brighest frame with the longest DIT) and the first
plane of NAXIS3 = 40 = NDIT planes. Of this plane the median counts in
a central 80x80 pixel large window is taken, for the left and the right
channel center individually. For all four modes (CLI, DBI, DPI and LSS)
in the same way.
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for mode CI for the four broad band filters
B_Y, B_J, B_H and B_Ks.
- for mode DBI for dual band filters
D_H23 and D_K12 for the left and the right optical path separately.
- for mode >DPI for the four broad band filters and the
0-90 optical setup the left and the right optical path separately.
- for the rarely used mode LSS for the
W_YJH and W_YJHKs the right and the left channe;l
separately
Scoring&thresholds IRDIS Flat counts
All counts are scored. Relaxed thresholds are used.
The plot shows the counts in one plane of the raw frame
cube corresponding to NDIT=1. For NDIT=40, the total counts
in the brightest raw flat is 40 times the counts of one
plane of the raw frame cube. To achieve a S/N-ratio = 200
in the brightest raw flat, about 1000 ADU
must be achieved in a single plane. The S/N ratio in the
final master flat (derived from the illuminated regions alone) is not provided by the pipeline.
History
Date |
event |
2018-06 | lamp counts begin to decrease |
2018-07-29T16:28 | LAMP_QL1 is used instead of LAMP_QL2 |
Algorithm IRDIS Flat counts
COUNTS_LEFT is the median counts of the last raw frame of the sequence in the region
[440 490 520 570].
COUNTS_RIGHT is the median counts of the last raw frame of the sequence in the region
[1440 490 1520 570].
IRDIS RMS of master flat
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[derived from QC procedure] | sphere_irdis_flat..qc_rms_left | left channel rms | HC | | [docuSys coming] |
[derived from QC procedure] | sphere_irdis_flat..qc_rms_right | right channel rms | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The RMS of the master flat is monitored for CI, DPI and LSS
to check for cosmetics and potential vignetting.
Scoring&thresholds IRDIS RMS of master flat
The master flat RMS is scored for CI, DPI and LSS modes. Relaxed thresholds are used.
History
No remarks.
Algorithm IRDIS RMS of master flat
It is the RMS of the master flat
IRDIS Fixed-pattern noise of master flat
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[derived from QC procedure] | sphere_irdis_flat..qc_fpn_left | left channel fpn | HC | | [docuSys coming] |
[derived from QC procedure] | sphere_irdis_flat..qc_fpn_right | right channel fpn | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The fixed pattern noise of the master flat is monitored for CI, DPI and LSS.
Scoring&thresholds IRDIS Fixed-pattern noise of master flat
The master flat RMS is scored for CI, DPI and LSS modes. Relaxed thresholds are used.
History
No remarks.
Algorithm IRDIS Fixed-pattern noise of master flat
The value is the fixed-pattern noise (the pixel-to-pixel response ratios) of the detector derived from the master flat.
IRDIS Bad pixel number
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC NUM BADPIXELS | sphere_irdis_flat..qc_num_badpix | number of bad pixel | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The number of bad pixel is monitored for CI, DBI and LSS. This parameter is for both channels (left and right) together.
Scoring&thresholds IRDIS Bad pixel number
The scoring thresholds are based on statistical grounds.
History
No remarks.
Algorithm IRDIS Bad pixel number
The number of bad pixel is composed of the number of static bad pixel derived from the submitted static bad pixel map plus
the dynamic bad pixel, which are those pixel deviating a configurable fraction from the mean linearity.
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