Plot ? |
Symb ? |
Source * |
Average ? |
Thresholds ? |
N_ data |
QC1 parameter |
Data downloads |
Remarks |
method |
value |
unit |
method |
value |
1 |
o | QC1DB |
MEDIAN |
3.58327 |
ADU |
VAL | 2.0,300.0 |
13 |
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 | |
13 |
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 | |
0 |
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 | |
0 |
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 |
3.06473 |
ADU |
VAL | 2.0,300.0 |
24 |
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 | |
22 |
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 | |
2 |
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 | |
0 |
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 |
3.46857 |
ADU |
VAL | 2.0,300.0 |
112 |
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 | |
14 |
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 | |
94 |
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 | |
4 |
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 |
3.25004 |
ADU |
VAL | 2.0,300.0 |
8 |
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 | |
6 |
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 | |
2 |
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 | |
0 |
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_psf (QC1 database) |
parameter | dataset: (numbers applicable to o ) | qc_net_flux | o |
median: | 3.58327 | ADU |
fixed thresholds: | 2.0...300.0 | ADU |
N_data: | 13 |
[click on plot for closeup] |
Plot 2 | data source: | sinfoni_psf (QC1 database) |
parameter | dataset: (numbers applicable to o ) | qc_net_flux | o |
median: | 3.06473 | ADU |
fixed thresholds: | 2.0...300.0 | ADU |
N_data: | 24 |
[click on plot for closeup] |
Plot 3 | data source: | sinfoni_psf (QC1 database) |
parameter | dataset: (numbers applicable to o ) | qc_net_flux | o |
median: | 3.46857 | ADU |
fixed thresholds: | 2.0...300.0 | ADU |
N_data: | 112 |
[click on plot for closeup] |
Plot 4 | data source: | sinfoni_psf (QC1 database) |
parameter | dataset: (numbers applicable to o ) | qc_net_flux | o |
median: | 3.25004 | ADU |
fixed thresholds: | 2.0...300.0 | ADU |
N_data: | 8 |
[click on plot for closeup] |
This plot
These are the trending plots for the SINFONI QC parameters derived from the PSF calibration frames.
PSF standard star monitoring has been implemented beginning 2009-05-01.
The intent is to monitor the MINIMUM flux of the PSF star to insure that it has an adequate S/N.
Flux levels should be above 3 ADU/pixel within a 3 sigma aperture for the K and H+K-band.
In the case of the J and H-band PSF stars, the minimum allowed flux level is 2 ADU/pixel within a 3 sigma aperture.
The PSF standard star is often used to test the centering of science
exposures. Therefore, we monitor the radial offset from the nominal field
center: R = sqrt[ (x-x0)^2 + (y-y0)^2 ].
Find more information about SINFONI PSF 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
|