CalFUSE v3.2.3 Is Now Available
The final version of the FUSE calibration pipeline, CalFUSE v3.2.3, is now available for general use. This version includes software changes implemented for the final reprocessing of the FUSE archive, which was completed in December of 2008. For details, please see the Introduction to CalFUSE v3.2.
Downloading CalFUSE
You may download the files directly from our web site using your browser or transfer them via FTP.
> ftp fuse.pha.jhu.edu
login: anonymous
password: your_email_address
ftp> cd fuseftp/calfuse
ftp> binary
ftp> get INSTALLING_CalFUSEv3.2.3
ftp> get INTRO_TO_CalFUSEv3.2.3
ftp> get cfv3.2.3.sw.tar.gz
ftp> get cfv3.2.3.cala.tar.gz
ftp> get cfv3.2.3.calg.tar.gz
ftp> get cfv3.2.3.calz.tar.gz
ftp> quit
Follow the installation instructions in the file INSTALLING_CalFUSEv3.2.3.
Documentation
-
"CalFUSE Version 3: A Data-Reduction Pipeline for the
Far Ultraviolet Spectroscopic Explorer"
(Dixon et al. 2007) is the definitive description
of the CalFUSE data-reduction pipeline. Please cite this work in any
scientific papers that refer to CalFUSE.
-
The CalFUSE Pipeline Reference Guide provides instructions
for running the CalFUSE pipeline and detailed descriptions of its
calibration files.
-
Questions about CalFUSE? Look for answers on the
CalFUSE Frequently-Asked Questions page.
-
Data-analysis tools distributed with the CalFUSE pipeline are reviewed
in the document
FUSE Tools in C. A subset of these programs, designed
specifically for the manipulation of IDF files, is described in the
IDF Cookbook, available in both PDF
and HTML formats.
- The worm is a distinctive feature of the FUSE detector. A detailed explanation of the effect is presented by David Sahnow in his memo, The Worm Explained. Jean Dupuis' white paper All About the Worm catalogs the worms present in all spectral segments and apertures.
Bug Reports
Please report any anomalies to
fuse_support@pha.jhu.edu.
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