mirror sites: PL (internal link) HQ     [?]

Quality Control and
Data Processing


CAL | HC | refs | QC
QUALITY CONTROL
    HOME
SPHERE QC
Trending & QC1
   IFS background
Pipeline
QC links:
SPHERE: IFS Background
IFS background rate | IFS persistence

 
HC PLOTS
background rate for IFS
persistence
QC1 database (advanced users): browse | plot

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.

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)

IFS raw background frame with DIT=30 sec and YJH-band (INS4.OPTI13.NAME = DIC_H, INS2.MODE = NIROBS).


IFS background rate
IFS background rate | IFS persistence

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/secHC [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
IFS background rate | 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.


Send comments to <qc_sphere@eso.org> powered by QC [webCMS v1.0.1]