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Hectospec
Reduction Software
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[Definitions] [Preparation] [Observation] [Reduction (Pipeline) (Software) [Distribution] [Archiving]
You can reduce Hectospec data using IRAF tools, but we have written a number of tasks which make it easier. To follow the process described on our Reduction page, you will need the following external IRAF packages:
Here is the modification history of this package.
The package can be downloaded via FTP from
ftp://cfa-ftp.harvard.edu/pub/iraf/hectospec-3.5.8.tar.gz
or via HTTP from
http://tdc-www.harvard.edu/instruments/hectospec/hectospec-3.5.8.tar.gz
Precompiled Redhat Linux and Solaris binaries for IRAF 2.12.2a through 2.14.1 are at
ftp://cfa-ftp.harvard.edu/pub/iraf/hectospec-3.5.8-bin.redhat.tar.gz
or, via HTTP,
http://tdc-www.harvard.edu/instruments/hectospec/hectospec-3.5.8-bin.redhat.tar.gz
and
ftp://cfa-ftp.harvard.edu/pub/iraf/hectospec-3.5.4-bin.ssun.tar.gz
or, via HTTP,
http://tdc-www.harvard.edu/instruments/hectospec/hectospec-3.5.4-bin.ssun.tar.gz
If you are using the Unix ksh pipeline, grab kfunc.tar.gz and mktime.tar.gz, and make them in your search path.
Check http://iraf.noao.edu/iraf/ftp/iraf/extern-v212/ for the latest release. The needed files are usually found in the mscred/ subdirectory.
To process Hectospec data, you need our mscdb entries. Here is the latest mscdb, with both ours and NOAO's entries via ftp:
ftp://cfa-ftp.harvard.edu/pub/iraf/mscdb-4.3.tar.gz
and via http:
http://tdc-www.harvard.edu/instruments/hectospec/mscdb-4.3.tar.gz
Here is the modification history of this package.
You can download the package via anonymous FTP from
ftp://cfa-ftp.harvard.edu/pub/iraf/rvsao-2.7.5.tar.gz
or via HTTP from
http://tdc-www.harvard.edu/iraf/rvsao/rvsao-2.7.5.tar.gz
Precompiled Redhat Linux and Solaris binaries for IRAF 2.12.2a are at
ftp://cfa-ftp.harvard.edu/pub/iraf/rvsao-2.7.5-bin.redhat.tar.gz
or, via HTTP
http://tdc-www.harvard.edu/iraf/rvsao/rvsao-2.7.5-bin.redhat.tar.gz
and
ftp://cfa-ftp.harvard.edu/pub/iraf/rvsao-2.7.5-bin.ssun.tar.gz
or, via HTTP
http://tdc-www.harvard.edu/iraf/rvsao/rvsao-2.7.5-bin.ssun.tar.gz
The templates we use for XCSAO are in rvsao$Templates/
Here is the modification history of this package.
Source code in the IRAF package directory structure is at
ftp://cfa-ftp.harvard.edu/pub/gsc/WCSTools/wcstools-3.7.5.iraf.tar.gz
or, via HTTP
http://tdc-www.harvard.edu/software/wcstools/wcstools-3.7.5.iraf.tar.gz
Here is the modification history of this package.
IRAF SPP source code for the latest version is available at
ftp://cfa-ftp.harvard.edu/pub/iraf/svdfit-1.9.2.tar.gz
or, via HTTP
http://tdc-www.harvard.edu/iraf/svdfit/svdfit-1.9.2.tar.gz
Our singular value decomposition sky subtraction technique, which is not exactly what we use now, is described in a paper published in the April 20, 2000 issue of The Astropysical Journal Letters, which is available through the ADS at
http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000ApJ...533L.183K
Precompiled Redhat Linux and Solaris binaries for IRAF 2.12.2a are at
ftp://cfa-ftp.harvard.edu/pub/iraf/svdfit-1.9.2-bin.redhat.tar.gz
and
ftp://cfa-ftp.harvard.edu/pub/iraf/svdfit-1.9.2-bin.ssun.tar.gz
or, via HTTP
http://tdc-www.harvard.edu/iraf/svdfit/svdfit-1.9.2-bin.redhat.tar.gz
and
http://tdc-www.harvard.edu/iraf/svdfit/svdfit-1.9.2-bin.ssun.tar.gz
You only need it if you are using the Unix-level ksh pipeline programs, especially the sky subtraction task, skyproc.
Source code and binaries for several operating systems are available at http://www.cfa.harvard.edu/~john/starbase/Download.html.