[ ESO ] FORS1 Pipeline
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INTRODUCTION

The reduction of FORS1 data at QC1 Garching is done in a semi-automatic manner where raw data are inserted into an automatic reduction machine. This machine is the FORS1 reduction pipeline.
The main functionalities of the FORS1 pipeline are:

  • to produce master calibration data
  • to compute QC1 parameters
for supported modes. FORS1 SCIENCE data have been processed by the pipeline with the best available calibration data. Please note that ESO is not assuming any responsibility in respect to the usefulness of the reduced data. The adopted reduction strategy may not be suitable for the scientific purpose of the observations.

The spectroscopic FORS pipeline is publicly available.

Since April 1, 2008, the new imaging pipeline has been in operation. Information on the imaging pipeline used before can be found here.

OPERATIONS

There are two instances of the FORS1 reduction pipeline:

  • the automatic mode, running on Paranal,
  • the optimized mode, running at HQ Garching and operated by Quality Control.
The automatic mode is used for quick look purposes and for on-site quality control. It processes all raw data sequentially, i.e. as they arrive from the instrument. It produces calibration products and reduced science data, but will usually fail to obtain the best results.

The optimized mode is the mode, which only becomes possible when all data of a night have been collected. Then the calibration data are sorted and assessed independently of their timestamp. The best possible master calibration data are created. Their quality is checked. They are finally applied to the science data of a night. This is the way all calibration data are reduced by QC Garching, as are all science data from Service Mode programmes.

FUNCTIONALITIES

The FORS1 pipeline is run by QC Garching for all the supported modes and produces:

  • master calibration data
    These are produced for both Visitor Mode and Service Mode nights. The raw calibration data are stored in the ESO Archive and are publicly accessible.
  • QC1 parameters
    These are computed for all the master calibration data. These are used to assess the quality of the master calibration data and to trend the instrument evolution. The QC1 parameters are availble through the QC1 web pages.
  • reduced science data.
    These are produced for Service Mode nights. These data are produced using the best available QC-assessed master calibration data.

FILE FORMAT

During the FORS1 detector upgrade on March 28, 2007, the old CCD has been replaced by a mosaic of two blue/UV-optimized CCDs. The upper CCD is referenced as Chip1 (also called master), while the lower CCD is referenced as Chip2 (also called slave). Each FORS2 exposure is split into two files, one for each CCD.
The CCD mosaic is mounted off-axis so that the target falls by default on Chip1 and gap between the two CCDs falls between two MOS slits.

The raw FORS1 files in the standard CCD format (2x2 binning, no windowing) have 2048x1034 pixels. The field of view is limited by the MOS unit, therefore the field of Chip1 is larger than that of Chip2. Two pre/overscan regions are present in the CCD. For the standard CCD format (2x2 binning), these regions are 5 pixels wide (i.e. rows 1...5 for the prescan and 1030...1034 for the overscan). For a graphical description of the detector sections, have a look here (pre-view) or here (ps file). Note that for presentation reason, the pre-scan regions have been artificially enlarged.

Old CCD

Until March 25, 2007 FORS1 was equipped with one CCD. The raw FORS1 files in the standard CCD format (1x1 binning, no windowing) had 2080x2048 pixels. Two readout modes were used: single port (left) and 4 port (right).

Two pre/overscan regions were present in the CCD. For the standard CCD format (1x1 binning), these regions were 16 pixels wide (i.e. columns 1...16 for the prescan and 2065...2080 for the overscan). For a graphical description of the detector sections, have a look  here  (pre-view) or  here  (ps file). Note that for presentation reason, the pre-scan regions have been artificially enlarged.

SUPPORTED MODES AND SETTINGS

The FORS1 pipeline installed in Garching and on Paranal presently supports only the following instrument modes and settings. Non-standard settings are not supported by the pipeline.
 
Supported ModesSupported Settings
Imaging  (IMG)
Binning: 1x1, 2x2
Gain: high/low
Collimator:SR/HR
Windowing: no
Filters: all
Long Slit Spectroscopy (LSS)
Binning: 1x1, 2x2
Gain: high
Collimator:SR/HR
Windowing: no
Grisms:all
Multi Object Spectroscopy (MOS)
Binning: 1x1, 2x2
Gain: high
Collimator:SR/HR
Windowing: no
Grisms:all

The other modes (IPOL, PMOS) are presently not supported by the pipeline. For these modes, only raw calibration data are delivered for Service Mode programmes.


 
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