Plot ? |
Symb ? |
Source * |
OPS? ** |
Average ? |
Thresholds ? |
N_ data |
QC1 parameter |
Data downloads |
Remarks |
| method |
value |
unit |
method |
value |
| 1 |
[19] | QC1DB |
|
none |
|
ADU |
none | |
17 |
diff_fpn_UL |
this |
last_yr |
all
|
Ks-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 1 |
♦ | QC1DB |
|
none |
|
ADU |
none | |
8 |
diff_fpn_UL |
this |
last_yr |
all
|
H-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 1 |
o | QC1DB |
|
none |
|
ADU |
none | |
11 |
diff_fpn_UL |
this |
last_yr |
all
|
J-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 1 |
| QC1DB |
|
none |
|
ADU |
none | |
15 |
diff_fpn_UL |
this |
last_yr |
all
|
Js-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 2 |
[19] | QC1DB |
|
none |
|
ADU |
none | |
16 |
diff_fpn_UR |
this |
last_yr |
all
|
Ks-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 2 |
♦ | QC1DB |
|
none |
|
ADU |
none | |
8 |
diff_fpn_UR |
this |
last_yr |
all
|
H-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 2 |
o | QC1DB |
|
none |
|
ADU |
none | |
11 |
diff_fpn_UR |
this |
last_yr |
all
|
J-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 2 |
| QC1DB |
|
none |
|
ADU |
none | |
15 |
diff_fpn_UR |
this |
last_yr |
all
|
Js-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 3 |
[19] | QC1DB |
|
none |
|
ADU |
none | |
17 |
diff_fpn_LL |
this |
last_yr |
all
|
Ks-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 3 |
♦ | QC1DB |
|
none |
|
ADU |
none | |
8 |
diff_fpn_LL |
this |
last_yr |
all
|
H-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 3 |
o | QC1DB |
|
none |
|
ADU |
none | |
11 |
diff_fpn_LL |
this |
last_yr |
all
|
J-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 3 |
| QC1DB |
|
none |
|
ADU |
none | |
15 |
diff_fpn_LL |
this |
last_yr |
all
|
Js-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 4 |
[19] | QC1DB |
|
none |
|
ADU |
none | |
17 |
diff_fpn_LR |
this |
last_yr |
all
|
Ks-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 4 |
♦ | QC1DB |
|
none |
|
ADU |
none | |
8 |
diff_fpn_LR |
this |
last_yr |
all
|
H-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 4 |
o | QC1DB |
|
none |
|
ADU |
none | |
11 |
diff_fpn_LR |
this |
last_yr |
all
|
J-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| 4 |
| QC1DB |
|
none |
|
ADU |
none | |
15 |
diff_fpn_LR |
this |
last_yr |
all
|
Js-band FPN from MASTER_IMG_FLAT divided by reference FLAT |
| |
|
*Data sources: QC1DB: QC1 database; LOCAL: local text file | **OPS: to indicate that OPSLOG data are included
|
This plot
This is the trending plot for the ISAAC twilight flat QC parameters of the SW-arm
These plots describe:
The master flat has been divided by a reference master flat to get rid of the
high structural noise (fixed pattern noise). On this differential frame,
a histogram is generated and is fit by a Gaussian to retrieve a robust pixel statistics
and the width is retrieved. This width is a robust estimate of
variationsin the structural noise. Renewal of the reference
flats are indicated.
QC parameters have not been calculated by the pipeline but by
post-pipeline QC scripts, hence there are no values from Paranal to be
included.
Fig.1. upper left quadrant of the detector.
Fig.2. upper right quadrant of the detector.
Fig.3. lower left quadrant of the detector.
Fig.4. lower right quadrant of the detector.
The color coding is : green for H, blue for J and Js, red for K.
This QC1 parameter is sensitive to changes in the structural noise,
which can be due to changes in the fringe pattern, instrumental internal
reflections and the structural noise of the detector itself.
Find more information about ISAAC QC parameters derived from twilight flats
here.
General information
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,
- statistical averages are indicated by a solid line, and thresholds by broken lines
- outliers are marked by a red asterisk. They are defined as data points outside the
threshold lines
- "aliens" (= data points outside the plot Y limits) are marked by a red arrow (↑ or ↓)
- you can download the data for each parameter set if the 'Data downloads' link shows up
|