Plot
? |
Symb
? |
Source
* |
Average ? |
Thresholds ? |
N_
data |
QC1
parameter |
Data
downloads |
Remarks |
| method |
value |
unit |
method |
value |
| 1 |
o | QC1DB |
MEDIAN |
23.17766 |
ADU |
VAL | 5.0,300.0 |
50 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture in the J-band at all camera scales (ADU)
(this FULL data set is scored) |
| 1 |
• | QC1DB |
none |
|
ADU |
none | |
46 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: J-band/250 mas scale |
| 1 |
• | QC1DB |
none |
|
ADU |
none | |
1 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: J-band/100 mas scale |
| 1 |
• | QC1DB |
none |
|
ADU |
none | |
3 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: J-band/25 mas scale |
|
| 2 |
o | QC1DB |
MEDIAN |
17.62373 |
ADU |
VAL | 5.0,300.0 |
51 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture in the H-band at all camera scales (ADU)
(this FULL data set is scored) |
| 2 |
• | QC1DB |
none |
|
ADU |
none | |
38 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H-band/250 mas scale |
| 2 |
• | QC1DB |
none |
|
ADU |
none | |
12 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H-band/100 mas scale |
| 2 |
• | QC1DB |
none |
|
ADU |
none | |
1 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H-band/25 mas scale |
|
| 3 |
o | QC1DB |
MEDIAN |
10.9559 |
ADU |
VAL | 5.0,300.0 |
194 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture in the K-band at all camera scales (ADU)
(this FULL data set is scored) |
| 3 |
• | QC1DB |
none |
|
ADU |
none | |
91 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: K-band/250 mas scale |
| 3 |
• | QC1DB |
none |
|
ADU |
none | |
95 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: K-band/100 mas scale |
| 3 |
• | QC1DB |
none |
|
ADU |
none | |
8 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: K-band/25 mas scale |
|
| 4 |
o | QC1DB |
MEDIAN |
10.79047 |
ADU |
VAL | 5.0,300.0 |
152 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture in the H+K-band at all camera scales (ADU)
(this FULL data set is scored) |
| 4 |
• | QC1DB |
none |
|
ADU |
none | |
98 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H+K-band/250 mas scale |
| 4 |
• | QC1DB |
none |
|
ADU |
none | |
34 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H+K-band/100 mas scale |
| 4 |
• | QC1DB |
none |
|
ADU |
none | |
20 |
qc_net_flux |
this |
last_yr |
all
|
mean flux per pixel within a 3 sigma aperture: H+K-band/25 mas scale |
|
| |
|
*Data sources: QC1DB: QC1 database; LOCAL: local text file
|
| Plot 1 | | data source: | sinfoni_std
(QC1 database) |
parameter | dataset:
(numbers applicable to o ) | qc_net_flux | o |
| median: | 23.17766 | ADU |
| fixed thresholds: | 5.0...300.0 | ADU |
| N_data: | 50 |
| [click on plot for closeup] |
| Plot 2 | | data source: | sinfoni_std
(QC1 database) |
parameter | dataset:
(numbers applicable to o ) | qc_net_flux | o |
| median: | 17.62373 | ADU |
| fixed thresholds: | 5.0...300.0 | ADU |
| N_data: | 51 |
| [click on plot for closeup] |
| Plot 3 | | data source: | sinfoni_std
(QC1 database) |
parameter | dataset:
(numbers applicable to o ) | qc_net_flux | o |
| median: | 10.9559 | ADU |
| fixed thresholds: | 5.0...300.0 | ADU |
| N_data: | 194 |
| [click on plot for closeup] |
| Plot 4 | | data source: | sinfoni_std
(QC1 database) |
parameter | dataset:
(numbers applicable to o ) | qc_net_flux | o |
| median: | 10.79047 | ADU |
| fixed thresholds: | 5.0...300.0 | ADU |
| N_data: | 152 |
| [click on plot for closeup] |
These are the trending plots for the SINFONI QC parameters derived
from the telluric STD stars.
Telluric standard star monitoring has been implemented beginning 2009-05-01.
The intent is to monitor the MINIMUM flux of the STD star to insure that it has an adequate S/N.
Flux levels should be above 5 ADU/pixel within a 3 sigma aperture.
Find more information about SINFONI STD calibration data
here.
Other QC parameters are also trended
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
|
