SPHERE: IFS Background
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HC PLOTS |
background rate for IFS |
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persistence |
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QC1 database (advanced users):
browse |
plot
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IFS background calibration frames are acquired with the DIT and NDIT
of the dark frames. No prism is in the optical for background frames,
however the background has a very small dependency on the CPI dichroic
INS4.OPTI13.NAME=DIC_H or DIC_K. The pipeline does not (yet) subtract
the dark of the same DIT.
From the technical point of view the difference between an IFS dark frame
and an IFS background frame is, that in dark the key INS.COMB.ICOR =
N_NS_OPAQUE, which means that all three coronograhic elements are
OPEN and the OCS1.INS.OPTI1.NAME = CLOSED, while in a background
frame INS.COMB.ICOR = N_NS_CLEAR, which means that again all three
coronopgraphic elements are OPEN and the INS.COMB.ICOR = OPEN as well.
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IFS raw background frame with DIT=30 sec and YJ-bands (INS4.OPTI13.NAME = DIC_K, INS2.MODE = IFS-H). (image with cuts = 200,300 ADU)
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IFS raw background frame with DIT=30 sec and YJH-band (INS4.OPTI13.NAME = DIC_H, INS2.MODE = NIROBS).
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IFS background rate
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
QC.BACKGROUND.MEDIAN | sphere_ifs_background..qc_median | median of background | HC | | [docuSys coming] |
[QC procedure] | sphere_ifs_background..qc_backrate | median backgr. in ADU/sec | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Trending
The instrumental background depends on the dichroic in the common path interface (CPI).
INS4.OPTI3.NAME=DIC_K means the YJH-bands are switched to IFS (and IRDIS receives the K-band alone).
INS4.OPI13.NAME=DIC_H means the YJ-bands are switched to IFS and H and K is switched to IRDIS.
Scoring&thresholds IFS background rate
The background rates are scored for both dicroic and three values of DIT.
History
The background frames consist of the dominating detector dark current
(monitored by the IFS dark level plot) and a small component originating
from the instrument. The reported QC parameters cover the instrumental
background radiation plus the dark level of the detector. The
background has a minor dependenece on the CPI dichroic which can be
INS4.OPTI13.NAME=DIC_H or DIC_K and a major dependence on the IFS bench
temperature.
The background is stable within the known ambient temperature fluctuations since begin of operations.
Algorithm IFS background rate
qc_median: counts in the background frame (dark is not subtracted)
qc_backrate: counts in the background frame (dark is not subtracted) divided by exposure time
IFS persistence
QC1_parameters
FITS key |
QC1 database: table, name |
definition |
class* |
HC_plot** |
more docu |
[QC procedure] | sphere_ifs_background..qc_persistence | Counts(PinHolePos minus PinHoleGap) | HC | | [docuSys coming] |
*Class: KPI - instrument performance; HC - instrument health; CAL - calibration quality; ENG - engineering parameter
**There might be more than one. |
Two types of peristence have been observed so far.
- An IFS wavelength calibration frame has been acquired in advance of the IFS dark or IFS background frame and
leaves a pattern covering nearly the whole detector. This effect is described
there.
- An IFS optical distortion calibration frame has been acquired in advance of the IFS dark or IFS background frame and
leaves a pattern of the sliced pinholes. This effect is described here.
IFS_DARK master frames are not used to calibrate observations, only the
ancillary IFS_DARK product IFS_STATIC_BADPIXEL is used, and persistence
does not bias the static bad pixel map. But the IFS_BACK master
calibrations are used to calibrate science observations. The sliced
pinhole pattern is monitored since 2020 in IFS background and IFS dark
frames, but the effect is only monitored in the IFS background frames.
SPHERE IFS day-time calibrations are generated in an order to avoid persistence.
Persistence can show up only in situations, when the sequence is aborted and continued again due
to operational reasons.
Trending
The trending started in 2020. Historic data have been reprocessed back to 2017.
Scoring&thresholds IFS persistence
The values are not scored.
History
Algorithm IFS persistence
The QC parameter is simply: the median counts in the
pipeline product in a window P = [770, 130 --- 850, 1440]
minus the median counts in window B = [640, 1470 --- 720,
1570]. Window P (pinhole) is the area where the pinhole
slice pattern can show up and window B (background) is the
area off the pinhole slice pattern areas on the detector.
This QC parameter is sensitive to pinhole persistence only.
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