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VISIR:
calibration data

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VISIR CALIBRATION DATA: GENERAL

Calibration data for VISIR are taken for two purposes:

  • assess the instrumental status
  • calibrate SCIENCE data.

VISIR calibration data are taken at night (e.g. standard star observations) and as daytime calibrations. On request of the user, also nighttime calibrations can be obtained as part of the Observing Block which generates the SCIENCE data ("attached calibrations"). Since the beginning of operations all the daytime calibrations have only been used to monitor health of the instrument.

All calibration data taken in VISIR are processed by QC Garching to obtain calibration solutions. These solutions come as

  • calibration product fits file frames (e.g. standard star imaging frames)
  • calibration product fits tables (e.g. spectrum extracted in a form of a table)
TYPES OF RAW CALIBRATION DATA

The VISIR data format is described here.

The following calibration data are taken as part of the VISIR calibration plan and/or upon request by the user. Data types are identified by DPR keywords in FITS headers.

mode DPR.CATG DPR.TYPE DPR.TECH purpose typical number taken
per night and setting
dark CALIB DARK IMAGE
SPECTRUM
dark current 3
flat CALIB FLAT IMAGE,DIRECT gain pixel-to-pixel variations, bad pixel map 4-7
photometric standard star
CALIB STD IMAGE,CHOPNOD sensitivity, conversion factor, mean background 2
spectroscopic standard CALIB STD SPECTRUM,CHOPNOD
ECHELLE
sensitivities, flux calibration, telluric features 2
2

 

CALIBRATION PRODUCTS

Complete overview of calibration files and recipes

Raw frame(s) recipe description product(s) [PRO.CATG header keywords]
dark [visir_dark_img.png 3K] visir_img_dark creates a master dark from a set of input raw frames of the imaging detector IMG_DARK_AVG
dark [visir_dark_spc.png 3K] visir_img_dark creates a master dark from a set of input raw frames of the spectroscopic detector SPEC_DARK_AVG
flat field [visir_flat_img.png, 2K] visir_img_ff creates a master flatfield for the imaging detector from a set of 7 input raw frames taken at different temp. of the WarmCalibrationUnit IMG_FF
IMG_BPM
IMG std [visir_std_img.png, 2K]

visir_img_phot

determines sensitivity, background, conversion factor, instrumental response, observing conditions, etc. IMG_PHOT_COMBINED
IMG_PHOT_CONTRIB_MAP
SPEC LR/MR/HR-slit std [visir_std_spec.png, 2K]

visir_spc_phot

determines sensitivity, background and conversion factor as a function of wavelength, instrumental response, observing conditions, sky spectrum, etc. SPC_PHOT_COMBINED
SPC_PHOT_TAB
SPC_PHOT_WEIGHT
SPEC ECHELLE std [visir_std_ech.png, 2K]

visir_spc_phot_ech

determines sensitivity, background and conversion factor as a function of wavelength, instrumental response, observing conditions, sky spectrum, etc. SPC_PHOT_HRG_COMBINED
SPC_PHOT_HRG_TAB
SPC_PHOT_HRG_WEIGHT

Naming scheme

After production and certification, the calibration products are renamed with a more user-friendly scheme which includes type, creation date and relevant setting parameters.

Description of naming scheme

CALIBRATION CASCADE

At present, all sets of VISIR calibration frames are reduced independently, i.e. there is no calibration cascade. In the future the flatfield correction may be included. It's still under investigation.

PROBLEMS AND ISSUES

VISIR pipeline limitations/problems are documented on the Data Package page.

STATIC CALIBRATION FILES

Static calibrations include:

  • catalog of imaging standard stars (PRO.CATG=IMG_STD_CATALOG)
  • catalog of spectroscopic standard stars (PRO.CATG=SPEC_STD_CATALOG)
  • reference arc line table (PRO.CATG=SPEC_CAL_LINES)
  • quantum efficiency map (PRO.CATG=SPEC_CAL_QEFF)


 
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