Plot ? |
Symb ? |
Source * |
OPS? ** |
Average ? |
Thresholds ? |
N_ data |
QC1 parameter |
Data downloads |
Remarks |
| method |
value |
unit |
method |
value |
| 1 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm J+Block filter |
| 2 |
| QC1DB |
no |
MEDIAN |
-9.65999 |
MAG/AS2 |
none | |
55 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, H filter |
| 3 |
| QC1DB |
no |
MEDIAN |
-10.4479 |
MAG/AS2 |
none | |
74 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, Ks filter |
| 4 |
| QC1DB |
no |
MEDIAN |
0.0 |
MAG/AS2 |
none | |
284 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, L filter |
| 5 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_3.21 filter chopping=True |
| 5 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_3.21 filter chopping=False |
| 6 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_3.28 filter chopping=True |
| 6 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_3.28 filter chopping=False |
| 7 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_3.80 filter |
| 8 |
| QC1DB |
no |
MEDIAN |
|
MAG/AS2 |
none | |
0 |
qc_sky_mag |
all (full time range)
| Sky brightness for LW-arm, NB_4.07 filter |
| |
|
*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 QC parameters derived from
science imaging pipeline products. The sky brightness is measured:
Dark subtracted and flatfielded raw science imaging frames are used for
the sky extraction subroutine, that determines the sky level in ADU for
each raw frame. The median sky level of the stack is taken. The counts
are converted in instrumental magnitudes per square arc second. No
extinction correction is applied, no photometric zeropoint is applied.
These plots describe:
Fig. 1.sky brightness, for LW J+Block.
Fig. 2.sky brightness, for LW H.
Fig. 3.sky brightness, for LW Ks.
Fig. 4.sky brightness, for LW L.
Fig. 5.sky brightness, for LW NB_3.21 chopping and jitter observations
are plot with different symbols.
Fig. 6.sky brightness, for LW NB_3.28 chopping and jitter observations
are plot with different symbols.
Fig. 7.sky brightness, for LW NB_3.80.
Fig. 8.sky brightness, for LW NB_4.07.
Find more information about ISAAC science imaging products
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
|