FORS - FOcal Reducer and low dispersion Spectrograph
Summary
FORS is the visual and near UV FOcal Reducer and low
dispersion Spectrograph for the Very Large
Telescope (VLT) of the European Southern
Observatory (ESO).
Two versions of FORS have been built, upgraded and moved to the
Cassegrain foci of different telescopes in the past years.
FORS is designed as an all-dioptric instrument for the wavelength
range from 330 nm to 1100 nm and provides an image scale of
0".25/pixel (or 0".125/pixel with the high resolution
collimator) in the standard readout mode (2x2 binning).
FORS1 is mounted on UT2 (Kueyen) and equipped with a new mosaic
of two 2k x 4k E2V CCDs (with 15 μm pixels) optimised for the
blue range (<600 nm) while FORS2 is installed on UT1 (Antu)
and optimised for the red with a very low level of fringes thanks
to a mosaic of two 2k x 4k MIT CCDs (with 15 μm pixels).
The geometries of both FORS1 and FORS2 detector systems are very
similar: in both cases the detectors are flat and the bottom
detector is rotated by 0.08 degrees and shifted by about 30 μm
with respect to the upper "master" detector. The gaps
between the two detectors are about 480 μm.
FORS1 has a polarimetric capability while FORS2 allows multi-object
spectroscopy with exchangable masks (MXU) and has a high time
resolution mode (HIT mode).
Publications based on data obtained with the FORS instruments
should quote the following reference paper:
Appenzeller,
I. et al. 1998, The Messenger 94, 1.
Important
- The arrival of X-Shooter in P82 will have an impact on the availability of FORS1, please see the Call for Proposals and the FORS news page for more details.
-
We have successfully completed the blue upgrade of FORS1 on
April 6, 2007. The upgrade included the installation of a new
CCD mosaic (similar to that of FORS2, but optimized for blue
rather than red) and of a new and more efficient set of broad
band filters.
For more information, have a look: here
Contact Information
- Questions related to service mode observations and proposal preparation should be addressed to the User Support Group.
- Questions related to visitor mode observations should be addressed to the Paranal Science Operations team.
Content of these pages
The following items are available on all the FORS pages, using the bar on the left.
- Overview: a short description of the instrument
- News: list of changes affecting the instrument and/or its pages.
- Instrument Description: all the important parameters of the instrument.
- Manuals: links to all the documents related to FORS.
- Tools: a collection of useful tools and informations for preparing and analyzing the FORS observations.
- Instrument Operations Team
- Visitor Instructions: Instrument specific instructions for Visiting Astronomers

