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SINFONI
CALIBRATION DATA: GENERAL | Calibration
data for SINFONI are taken for two purposes: - assess the
instrument status
- reduce science data, take out the instrumental signatures
in science frames
Generally SINFONI calibration data are taken as
daytime calibrations. Telluric standard stars and Point Spread Function Calibration
stars (PSF-stars) are generally observed during the night, as described by the
calibration plan (See User Manual for details). On request of the user, also nighttime
calibrations can be obtained as part of the Observing Block which generates the
SCIENCE data ("attached calibrations"). All calibration data taken
in SINFONI are processed by QC Garching to obtain calibration solutions. These
solutions come as - calibration product fits file frames (e.g. dark
or lampflat frames)
- calibration product fits tables (e.g. slitlet position
tables)
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TYPES OF RAW CALIBRATION
DATA | |
| FITS header examples |
| frame |
.txt |
| DARK |
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| LAMP
FLAT |
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| WAVE
FLAT | |
| LINEARITY |  |
| DISTORTION |  |
| STD |  |
| PSF |  |
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The following types of raw calibration data exist for the SINFONI IFU
mode
| frame | DPR
TYPE | Purpose |
typical number taken per night and setting |
| DARK | DARK | detector
status, dark level, RON, hot (high dark current) pixels |
3 |
| LAMP FLAT | FLAT,LAMP | fixed
pattern noise, vignetting, bad pixel | 10 |
| WAVE | WAVE,LAMP | wavelength
calibration, position of slitlets | 2 |
| DISTORTION | DISTORTION,FIBRE,NS
DISTORTION,WAVE,TECH DISTORTION,FLAT,TECH | optical
distortion, distances of slitlets | | | LINEARITY | LAMP,LINEARITY | Linearity,
bad (non-linear) pixels, fixed pattern noise | 10 | | STANDARD
STAR | STD or SKY,STD | standard
stars for telluric features | 2 | | PSF | PSF-CALIBRATOR
or SKY,PSF-CALIBRATOR | PSF,
Strehl ratio | 2 |
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![[top]](../img/arr1red-up.gif) | CALIBRATION
PRODUCTS | |
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Recipes and products
The
following SINFONI calibration products are created from raw calibration files
(click here for a complete overview of calibration
files and recipes): Naming
scheme After production and certification, the calibration products
are renamed after a scheme which includes type,
creation data and relevant SINFONI setting. . |
![[top]](../img/arr1red-up.gif) | CALIBRATION
CASCADE |
![[ISAAC calibration scheme]](../img/scheme_sinfoni_icon.gif)
SINFONI
calibration cascade
(9K) |
The calibration of SINFONI science frames requires a cascading
scheme where the mutual dependencies of products and raw frames have to be respected.
Some products (dark, distortion) can be produced from raw files only, but most
products require the prior generation of other calibration products. The proper
sequence of all these production steps is called the calibration cascade.
Within that cascade, all products are checked with respect to their quality
and their relationship in time. This means e.g. that a master flat is not only
generated using an arbitrary quality-checked order table, but that specific table
is chosen which at the moment of processing is closest in time. All products
created by QC Garching follow the calibration cascade.
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![[top]](../img/arr1red-up.gif) | OTHER
CALIBRATION TABLES | |
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Static calibrations include a reference arc line table and a static bad pixel
map (for the engineering array only)
| ![[top]](../img/arr1red-up.gif) | ACTUAL
PROBLEMS AND ISSUES | | |
SINFONI Pipeline problems are documented under on the ServiceMode
page. |
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