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