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SINFONI
SCIENCE DATA: GENERAL | Science data
for SINFONI are taken for scientific reasons. In addition they are used for the
following purpose: - assess the instrument status
Science
raw data are contaminated by well known instrumental signatures and by the terristrical
atmosphere. Both effects are eliminated from science raw data by using master
calibrations. The day-time calibrations like DARK, FLAT, WAVE are to extract the
instrumental signatures while the night time calibrations using standard stars
are to monitor the point spread function and the telluric absorption lines, both
effects are due to the terrestrial atmosphere and are changing more frequently
than the instrumental signatures.On special request by the user, day-time calibrations
can be scheduled during night time, on charge of the allocated science observing
time. nighttime (so-called attached calibrations). Day-time calibrations and the
observation of telluric standard stars come for free. See the User's manual for
details. From P75 (April 2005) on four science templates are supported,
they differ only by the pointing offset sequence (the jitter strategy). Science
frames come as IFS stacks. Some or all raw frames of a raw stack (on observation
block) show DPR.TYPE == OBJECT, the others (or none of the stack) show DPR.TYPE
== SKY. If no SKY frames are part of the science stack, sky emission lines cannot
be reduced. This is different to ISAAC long-slit spectroscopy, where the ABBA
nodding sequence is used to get rid of the spectrally resolved night sky. As for
ISAAC and NACO imaging , the SINFONI GenericOffset template allows for telescope
offsets, exceeding a so-called jitter box. The correlation star retrieved from
the first raw frame and used for the rest of the stack could get lost by being
jittered out of the jitter box. For this reason, the rarely used science case
of mosaicing is not supported by the pipeline. |
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| FITS headers |
| frame |
.txt |
| OBJECT
IFS,NODDING |
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| SKY
IFS,NODDING |
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The following types of raw science data exist for the SINFONI
| mode | DPR
TYPE | template |
comment |
| IFS,NODDING | OBJECT SKY | SINFONI_ifs_obs_AutoJitterOffset
SINFONI_ifs_obs_FixedSkyOffset SINFONI_IFS_obs_GenericOffset | | | IFS,JITTER | OBJECT | SINFONI_ifs_obs_AutoJitter | |
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Recipes and products
The
following SINFONI science products are created from raw science files (click here
for a complete overview of calibration files and recipes):
DPR.TECH
| recipe
| description |
product, PRO.CATG |
| IFS,NODDING |
sinfo_rec_jitter | final
IFS cube | | | | | bad
pixel mask | MASK_COADD_OBJ | | | | first
IFS cube | OBS_OBJ | | | | | OBJECT_NODDING_STACKED |
| Association rules
For the reduction of science data calibration products are required. The selection
of appropriate calibration products follow the association
rules. Naming scheme After production
and certification, the science products are renamed after a scheme
which includes type, creation data and relevant SINFONI setting.
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SINFONI calibration
cascade (9K) |
SINFONI science frames require a cascading scheme where the mutual dependencies
of products and raw frames have to be respected. Some products (master darks,
linearity bad pixel map, distortion table) 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 frame, but that
specific frame is chosen which at the moment of processing is closest in time.
All products created by QC Garching follow the science reduction cascade.
![[ISAAC calibration scheme]](../img/scheme_sinfoni_icon.gif)
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