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componentset.xml
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componentset.xml
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<?xml version="1.0"?>
<!-- DTD in buildsupport/starconf/componentinfo.dtd -->
<componentset>
<component id="astrom" support="S">
<version>3.8</version>
<path>applications/astrom</path>
<description>Basic astrometry package</description>
<abstract><p>ASTROM performs ``plate reductions''. You supply star
positions from a catalogue and the (x,y) ccoordinates of the
corresponding star images. ASTROM uses this information to
establish the relationship between (x,y) and (ra,dec) enabling the
coordinates of ``unknown stars'' to be determined.</p></abstract>
<dependencies >
<build>sla</build><build>cfitsio</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>P T Wallace</name>
<uname>ptw</uname>
<email>P.T.Wallace@rl.ac.uk</email>
</person>
<person>
<name>Norman Gray</name>
<uname>nxg</uname>
<email>norman@astro.gla.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun5</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="atools" support="S">
<version>1.9-14</version>
<path>applications/atools</path>
<description>ATOOLS - AST applications</description>
<abstract><p>
ATOOLS is a package of applications which manipulate descriptions
of coordinate frames, mappings, etc, in the form of AST Objects (see
SUN/210). Each application within the ATOOLS package corresponds closely
to one of the functions within the AST library. ATOOLS thus provides a
high-level interface to the AST library.
</p></abstract>
<dependencies >
<build>pcs</build><build>ast</build><build>cnf</build><build>hds</build><build>fio</build><build>grp</build><build>ifd</build><build>ndf</build><build>par</build><build>sae</build><build option='link'>kaplibs</build><build option='link'>atl</build><build option='link'>ast</build><build option='link'>shl</build><sourceset>sst</sourceset>
</dependencies>
<developers>
<person>
<name>David S. Berry</name>
<uname>dsb</uname>
<email>dsb@ast.man.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation></documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="ccdpack" support="S">
<version>4.1-1</version>
<path>applications/ccdpack</path>
<description>CCD data reduction package</description>
<abstract>
<p>CCDPACK is a package of programs for reducing CCD-like data. They
allow you to debias, remove dark current, flatfield, register,
resample and normalize data from single- or multiple-CCD instruments.
</p>
<p>CCDPACK is designed to help you to reduce your data easily.
The basic reduction stages can be set up using an X based GUI that
controls an automated reduction system.
The GUI is designed to allow you to start working without any
detailed knowledge of the package (or indeed of CCD reduction).
Registration is performed using graphical, script based or automated
techniques that help reduce the amount of work to a minimum.
</p>
<p>This document is intended for all users of CCDPACK.
It provides instruction in how to use CCDPACK, describes CCD reduction
in general and contains complete descriptions of the individual
programs.
</p>
</abstract>
<dependencies >
<build>pcs</build><sourceset>messgen</sourceset><build>ard</build><build>ast</build><build>blt</build><build>chr</build><build>cnf</build><build>fio</build><build>generic</build><build>grp</build><build>hds</build><build>idi</build><build>ifd</build><build>itcl</build><build>ndf</build><build>ndg</build><build>one</build><build>par</build><build>pcs</build><build>pgplot</build><build>prm</build><build>psx</build><build>tcl</build><build>tk</build><build>trn</build><build option='link'>agi</build><build option='link'>blt</build><build option='link'>graphpar</build><build option='link'>img</build><build option='link'>pda</build><build option='link'>ref</build><build option='link'>shl</build><build option='link'>sla</build><build option='link'>startcl</build><configure>itcl</configure><configure>tcl</configure><configure>tk</configure><configure>blt</configure><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>Peter Draper</name>
<uname>pwd</uname>
</person>
</developers>
<bugreports>ccdpack@starlink.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
<notes>
<p>Except for contents of obsolete dir</p>
</notes>
</copyright>
</component>
<component id="coco" support="S">
<version>2.2-8</version>
<path>applications/coco</path>
<description>Conversion of Celestial Coordinates</description>
<abstract><p>
The COCO program converts star coordinates from one system to
another. Both the improved IAU system, post-1976, and the old pre-1976
system are supported.
</p></abstract>
<dependencies >
<build>sla</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Patrick Wallace</name>
<uname>ptw</uname>
</person>
</developers>
<documentation> sun56</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="convert" support="S">
<version>1.8</version>
<path>applications/convert</path>
<description>CONVERT -- format-conversion package</description>
<abstract><p>
The CONVERT package contains utilities for converting data files between
Starlink's Extensible n-dimensional Data Format (NDF), which is used by most
Starlink applications, and a number of other common data formats.
</p></abstract>
<dependencies >
<build>pcs</build><build>ast</build><build>chr</build><build>cnf</build><build>cvg</build><build>cfitsio</build><build>figaro</build><build>fio</build><build>grp</build><build>hds</build><build>kaplibs</build><build>mers</build><build>ndf</build><build>ndg</build><build>par</build><build>pcs</build><build>prm</build><build>psx</build><build>sae</build><build>shl</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Malcolm J. Currie</name>
<uname>mjc</uname>
<email>mjc@star.rl.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>G.J.Privett</name>
</person>
<person>
<name>A.J.Chipperfield</name>
</person>
<person>
<name>D.S.Berry</name>
<uname>dsb</uname>
</person>
<person>
<name>A.C.Davenhall</name>
<uname>acd</uname>
</person>
</developers>
<documentation> sun55</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="cupid" support="S">
<version>2.1</version>
<path>applications/cupid</path>
<description>CUPID - AST applications</description>
<abstract><p>
CUPID is a package of applications which identify and analyse clumps of
emission within 2- or 3- dimensional data arrays.
</p></abstract>
<dependencies >
<build>pcs</build><sourceset>messgen</sourceset><build>mers</build><build>atl</build><build>cnf</build><build>cvg</build><build>ifd</build><build>irq</build><build>ndf</build><build>sae</build><build>pda</build><build>thr</build><build option='link'>atl</build><build option='link'>kaplibs</build><build option='link'>ast</build><build option='link'>shl</build><build option='link'>thr</build><sourceset>sst</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>David S. Berry</name>
<uname>dsb</uname>
<email>dsb@ast.man.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun255</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year>2005</year>
<name>Joint Astronomy Centre Hawaii</name>
</copyright>
</component>
<component id="cursa" support="S">
<version>6.5</version>
<path>applications/cursa</path>
<description>CURSA - Catalogue and Table Manipulation Applications</description>
<abstract><p>
CURSA is a package of Starlink applications for manipulating astronomical
catalogues and similar tabular datasets. It provides facilities for:
browsing or examining catalogues, selecting subsets from a catalogue,
sorting catalogues, copying catalogues, pairing two catalogues, converting
catalogue coordinates between some celestial coordinate systems, plotting
finding charts and photometric calibration. Also, subsets can be extracted
from a catalogue in a format suitable for plotting using other Starlink
packages, such as PONGO. CURSA can access catalogues held in the popular
FITS table format, the Tab-Separated Table (TST) format or the Small Text
List (STL) format. Catalogues in the STL and TST formats are simple ASCII
text files. CURSA also includes some facilities for accessing remote
on-line catalogues via the Internet.
</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>sae</build><build option='link'>cat</build><build option='link'>fio</build><build option='link'>par</build><build option='link'>pda</build><build option='link'>ndf</build><build option='link'>pgplot</build><build option='link'>startcl</build><build>graphpar</build><sourceset>star2html</sourceset><configure>perl</configure><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Clive Davenhall</name>
<uname>acd</uname>
</person>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun190 ssn76</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="daophot" support="U">
<version>1.3-6</version>
<path>applications/daophot</path>
<description>Stellar Photometry Package</description>
<abstract>
<p>DAOPHOT is a stellar photometry package designed by Peter Stetson
at DAO to deal with crowded fields. The package performs various
tasks including finding objects, aperture photometry, obtaining the
point-spread function, and profile-fitting photometry.
Profile fitting in crowded regions is performed iteratively,
which improves the accuracy of the photometry.</p>
</abstract>
<dependencies >
<build>pcs</build><build option='link'>sae</build><build option='link'>mers</build><build option='link'>pcs</build><build option='link'>ndf</build><build option='link'>psx</build><build option='link'>chr</build><build option='link'>agi</build><build option='link'>gks</build><build option='link'>cnf</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person><name>Peter Stetson</name><role>Original author</role></person>
<person><name>Nicholas Eaton</name></person>
<person><name>Grant Privett</name></person>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun42</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Peter Stetson/DAO</name>
</copyright>
</component>
<component id="datacube" support="S">
<version>1.3</version>
<path>applications/datacube</path>
<description>DATACUBE - An IFS datacube manipulation package</description>
<abstract><p>DATACUBE is a package which includes the IFU Data Product Co
okbook (SC/16), a small number of applications used for AXIS and WCS
manipulation, and a collection of example shell and IDL scripts for IFS data
cube manipulation. </p></abstract>
<dependencies >
<build>pcs</build><build option='link'>shl</build><build option='link'>pcs</build><use>kappa</use><use>figaro</use><use>convert</use><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Alasdair Allan</name>
<uname>aa</uname>
<email>aa@astro.ex.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun237 sc16</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="dipso" support="S">
<version>3.6-5</version>
<path>applications/dipso</path>
<description>DIPSO -- A friendly spectrum analysis program</description>
<abstract><p>
</p></abstract>
<dependencies >
<build option='link'>ast</build><build option='link'>cat</build><build option='link'>kaplibs</build><build option='link'>snx</build><build option='link'>pda</build><build option='link'>ndf</build><build option='link'>sae</build><sourceset>star2html</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>David S. Berry</name>
<uname>dsb</uname>
<email>dsb@ast.man.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun50</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="docfind" support="S">
<version>1.3-2</version>
<path>applications/docfind</path>
<description>Starlink document index searching</description>
<abstract><p>
Simplify searching of Starlink documents. See also findme/showme.
</p></abstract>
<dependencies >
<build>info</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Peter Allan</name>
</person>
<person>
<name>Martin Bly</name>
</person>
</developers>
<documentation> sun38</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="echomop" support="S">
<version>3.3-7</version>
<path>applications/echomop</path>
<description>Echelle Data Reduction Package</description>
<abstract>
<p>ECHOMOP provides facilities for the extraction of
spectra from 2-D data frames. These data can be single-order
spectra, or multi-order echelle spectra.</p>
<p>A substantial degree of automation is provided, particularly in
the traditionally manual functions for cosmic-ray detection and
wavelength calibration; manual overrides are available.</p>
<p>Features include; robust and flexible order tracing, optimal
extraction, support for variance arrays, and 2-D distortion
fitting and extraction.</p>
</abstract>
<dependencies >
<build>pcs</build><build>cnf</build><build>fio</build><build>hds</build><build>hlp</build><build>mers</build><build>ndf</build><build>par</build><build>pda</build><build>pgp</build><build>prm</build><build>sae</build><build>sla</build><build>shl</build><build>mers</build><build option='link'>kaplibs</build><sourceset>htx</sourceset>
</dependencies>
<developers>
<person>
<name>Dave Mills</name>
</person>
<person>
<name>John Webb</name>
</person>
<person>
<name>Martin Clayton</name>
</person>
<person>
<name>Norman Gray</name>
<uname>nxg</uname>
<email>norman@astro.gla.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun152</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
<copyright>
<year></year>
<name>Others...</name>
<notes>
<p>Various small contributions, mostly from UCL</p>
</notes>
</copyright>
</component>
<component id="echwind" support="S">
<version>3.1-4</version>
<path>applications/echwind</path>
<description>UCL Echelle Spectrograph Observation Planning</description>
<abstract><p>
ECHWIND is used to assist in the planning of observations with either the
Utrecht Echelle Spectrograph (UES) or the UCL coude echelle spectrograph
(UCLES). It can be run at your home institution, when preparing an observing
proposal, or before or during an observing run.
</p></abstract>
<dependencies >
<build>pgplot</build><build>starx</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Marion Fisher</name>
</person>
<person>
<name>William Lupton</name>
</person>
<person>
<name>Anne Charles</name>
</person>
</developers>
<documentation> sun53</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="esp" support="S">
<version>0.11-4</version>
<path>applications/esp</path>
<description>Extended Surface Photometry</description>
<abstract><p>ESP (Extended Surface Photometry) is a package of
application programs developed to allow you to determine the
photometric properties of galaxies and other extended objects.</p>
<p>It has applications that: detect flatfielding faults, remove
cosmic rays, median filter images, determine image statistics,
determine local background values, perform galaxy profiling, fit 2-D
Gaussian profiles to galaxies, generate pie slice cross-sections
of galaxies and display profiling results.</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>agi</build><build option='link'>ast</build><build option='link'>ard</build><build option='link'>cat</build><build option='link'>chr</build><build option='link'>fio</build><build option='link'>grp</build><build option='link'>hds</build><build option='link'>ndf</build><build option='link'>mers</build><build option='link'>par</build><build option='link'>pcs</build><build option='link'>pda</build><build option='link'>prm</build><build option='link'>psx</build><build option='link'>sae</build><build option='link'>shl</build><build option='link'>sgs</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Norman Gray</name>
<uname>nxg</uname>
<email>norman@astro.gla.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
</person>
<person>
<name>Grant Privett</name>
</person>
</developers>
<documentation> sun180</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year>1996-1999, 2004</year>
<name>Council for the Central Laboratory of the Research Councils</name>
<notes>
<p>Includes some public domain code</p>
</notes>
</copyright>
</component>
<component id="extractor" support="S">
<version>2.5-1</version>
<path>applications/extractor</path>
<description>EXTRACTOR - An Astronomical Source Detection Program</description>
<abstract><p>
EXTRACTOR will detect sources in an astronomical image and build a catalogue
listing them. It is based on the popular SExtractor program, has very
flexible configuration facilities and can handle images and catalogues in a
variety of formats.
</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>ast</build><build option='link'>ndg</build><build option='link'>sae</build><sourceset>star2html</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Peter W. Draper</name>
<uname>pwd</uname>
<email>p.w.draper@durham.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun226</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="extreme" support="U">
<version>0.1-1</version>
<path>applications/extreme</path>
<description>Handling Extreme Data Sets</description>
<abstract>
<p>This package provides some utilities, background documentation,
and associated files for adapting the Starlink Software Collection,
and software which uses it, to handle very large data sets.
The principal focus of this is to move to use of 64 bits of address
space on 64-bit operating systems.</p>
<p>This document (SSN/73) is squarely aimed at the problem of adapting the
Starlink Software Collection, and consequently focuses on
the three operating systems (Solaris, Linux and Tru64) supported by Starlink,
the compiled languages Fortran 77 and ANSI C,
and Starlink's somewhat idiosyncratic build mechanisms.
However, some of the discussion here may be of interest or use to
people who are considering the change from 32 to 64 bits for
software in other contexts.
</p>
</abstract>
<dependencies >
<sourceset>sst</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person>
</developers>
<tests status="yes"/>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="figaro" support="S">
<version>5.6-6</version>
<path>applications/figaro</path>
<description>FIGARO general data-reduction system</description>
<abstract><p>
Figaro is a general-purpose data reduction package.
The programs it contains can be used to process a
wide range of images and spectra.
</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>pda</build><build option='link'>agi</build><build option='link'>grp</build><build option='link'>ndf</build><build option='link'>fio</build><build option='link'>idi</build><build option='link'>shl</build><build option='link'>sla</build><build option='link'>psx</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Keith Shortridge</name>
</person>
<person>
<name>Horst Meyerdierks</name>
</person>
<person>
<name>Martin Clayton</name>
</person>
<person>
<name>Jon Lockley</name>
</person>
<person>
<name>Anne Charles</name>
</person>
<person>
<name>Clive Davenhall</name>
</person>
<person>
<name>Malcolm J Currie</name>
<uname>mjc</uname>
<email>mjc@star.rl.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>Mark Taylor</name>
</person>
<person>
<name>Tim Ash</name>
</person>
<person>
<name>Tim Wilkins</name>
</person>
<person>
<name>Dave Axon</name>
</person>
<person>
<name>John Palmer</name>
</person>
<person>
<name>Anthony Holloway</name>
</person>
<person>
<name>Vito Graffagnino</name>
</person>
</developers>
<documentation> sun86</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="findcoords" support="U">
<version>1.0-2</version>
<path>applications/findcoords</path>
<description>Find the coordinates of a named object</description>
<abstract><p>
findcoords is a utility for finding the equatorial coordinates of
a named astronomical object. You simply enter the name of the object
and its coordinates are displayed.
</p></abstract>
<dependencies >
<build>cursa</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Clive Davenhall</name>
<uname>acd</uname>
</person>
</developers>
<documentation> sun240</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="fluxes">
<version>1.4-1</version>
<path>applications/fluxes</path>
<description>FLUXES - JCMT Postion and Flux Density Calibration</description>
<abstract><p>
FLUXES calculates accurate topocentric positions of the planets and also
integrated flux densities of five of them at several wavelengths.
These provide calibration information at the effective frequencies and
beam-sizes employed by the UKT14 and SCUBA receivers on the
JCMT telescope based on Mauna Kea, Hawaii.
</p></abstract>
<dependencies >
<build>pcs</build><build>sae</build><build>mers</build><build>fio</build><build>par</build><build>sla</build><link>fio</link><link>sla</link><link>mers</link><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Tim Jenness</name>
<uname>timj</uname>
</person>
<person>
<name>Grant Privett</name>
<uname>gjp</uname>
</person>
<person>
<name>Henry Matthews</name>
<uname>hem</uname>
</person>
<person>
<name>Graeme Watt</name>
<uname>gdw</uname>
</person>
<person>
<name>Catherine Hohenkerk</name>
</person>
</developers>
<documentation> sun213</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="gaia" support="S">
<version>4.4-5</version>
<path>applications/gaia</path>
<description>GAIA - Graphical Astronomy and Image Analysis</description>
<abstract><p>
GAIA is an image display and analysis tool for astronomy. It provides the
usual facilities of image display tools, plus more astronomically useful ones
such as aperture & optimal photometry, contouring, source detection, surface
photometry, arbitrary region analysis, celestial coordinate readout,
calibration and modification, grid overlays, blink comparison, defect patching
and the ability to query on-line (WWW) catalogues.
</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>ard</build><build option='link'>atl</build><build option='link'>ast</build><build option='link'>blt</build><build option='link'>cat</build><build option='link'>cfitsio</build><build option='link'>generic</build><build option='link'>fio</build><build option='link'>gsl</build><build option='link'>img</build><build option='link'>itcl</build><build option='link'>pcs</build><build option='link'>pda</build><build option='link'>sae</build><build option='link'>skycat</build><build option='link'>startcl</build><build option='link'>sla</build><build option='link'>tcl</build><build option='link'>tclx</build><build option='link'>tk</build><build option='link'>tcllibs</build><build option='link'>vtk</build><build option='link'>xerces-c</build><build option='link'>tdom</build><sourceset>star2html</sourceset><configure>tcl</configure><configure>tk</configure><configure>blt</configure><configure>itcl</configure><use>convert</use><use>esp</use><use>extractor</use><use>kappa</use><use>photom</use><use>polpack</use><use>startcl</use><use>tcl</use><use>tk</use><use>blt</use><use>tclx</use><use>tcllibs</use><use>skycat</use><use>tkimg</use><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Peter W. Draper</name>
<uname>pwd</uname>
<email>p.w.draper@durham.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun214</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="generic" support="S">
<version>1.3</version>
<path>applications/generic</path>
<description>A Utility for Compiling Generic Fortran Subroutines</description>
<abstract><p>GENERIC is a utility which preprocesses a generic
Fortran subroutine into its different types and concatenates these
routines into a file. The file can then be compiled with the
Fortran compiler to produce an object module.</p></abstract>
<dependencies >
<sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>S M Beard</name>
</person>
<person>
<name>P M Allan</name>
</person>
</developers>
<documentation> sun7</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="hdstools" support="S">
<version>1.0-2</version>
<path>applications/hdstools</path>
<description>HDSTOOLS - Tools To Display and Edit HDS Objects</description>
<abstract><p>
The HDSTOOLS package contains a number of tools
to edit and display HDS objects. The tools originated in the ASTERIX
package but have now been modified to run as normal Starlink tasks.
</p></abstract>
<dependencies >
<build>pcs</build><build>hds</build><build>fio</build><build>grp</build><build>mers</build><build>par</build><build>prm</build><build>sae</build><build>shl</build><build>ifd</build><build>psx</build><sourceset>sst</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>A. J. Chipperfield</name>
<uname>ajc</uname>
<email>starlink@jiscmail.ac.uk</email>
</person>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person> </developers>
<documentation> sun245</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
<copyright>
<year></year>
<name>University of Birmingham</name>
</copyright>
</component>
<component id="hdstrace" support="S">
<version>1.2-3</version>
<path>applications/hdstrace</path>
<description>HDSTRACE - Trace an HDS file</description>
<abstract><p>
Traces an HDS file
</p></abstract>
<dependencies >
<build>pcs</build><build option='link'>fio</build><build option='link'>generic</build><build option='link'>prm</build><build option='link'>par</build><build option='link'>sae</build><build option='link'>hds</build><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Malcolm J Currie</name>
<uname>mjc</uname>
<email>mjc@star.rl.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun102</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="htx" support="S">
<version>1.3-2</version>
<path>applications/htx</path>
<description>Hypertext Cross-reference Utilities</description>
<abstract>
<p>This document describes a set of ``Hypertext Cross-Reference
Utilities'' (HTX) which are designed to help maintain large
documentation sets whose constituent documents are written using the
Hypertext Markup Language (HTML).
</p>
<p>The central part of HTX is a hypertext linker, hlink. This allows
hyper-links (or cross-references) to be established between related
documents in such a way that it is easy to maintain their integrity as
individual documents are updated. Information produced by this linking
process is also used by other HTX utilities to provide document search
facilities and the ability to randomly access any part of a documentation
set. This latter capability forms a basis for constructing hypertext
help systems for use by other software.
</p>
<p>The expected readership of this document includes those who read hypertext
documentation, those who write it, and those who maintain it, especially
those who write and maintain Starlink documentation. Software developers
may also be interested in the possibilities for hypertext help that
HTX provides.
</p>
</abstract>
<dependencies >
<sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>Mark Taylor</name>
<uname>mbt</uname>
<email>m.b.taylor@bristol.ac.uk</email>
<role>owner</role>
</person>
</developers>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
<copyright>
<year></year>
<name>Council for the Central Laboratory of the Research Councils</name>
</copyright>
</component>
<component id="icl" support="S">
<version>3.1-11</version>
<path>applications/icl</path>
<description>Interactive Command Language</description>
<abstract><p>ICL shell.
</p></abstract>
<dependencies >
<sourceset>star2html</sourceset><sourceset>messgen</sourceset><build option='link'>pcs</build><build option='link'>cnf</build><build option='link'>sae</build><build option='link'>nbs</build><link>pcs</link><link>cnf</link><link>hlp</link><link>nbs</link><link>hds</link>
</dependencies>
<developers>
<person>
<name>S K Robinson</name>
</person>
<person>
<name>I R Jenkins</name>
</person>
<person>
<name>B K McIlwrath</name>
</person>
</developers>
<documentation> sg5</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="ifd" support="S">
<version>1.2-8</version>
<path>applications/ifd</path>
<description>Interface Definition Files</description>
<abstract>
<p>Interface Definition Files (IFDs) provide a generic method of
defining the interface between Starlink (ADAM) applications and
various software environments. Software is described which enables
developers to create IFDs and use them to create files required
by the Starlink or IRAF environments.</p>
</abstract>
<dependencies >
<sourceset>star2html</sourceset><build>tcl</build><configure>tcl</configure>
</dependencies>
<developers>
<person>
<name>Alasdair Allan</name>
<uname>aa</uname>
<email>aa@astro.ex.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>Alan Chipperfield</name>
</person>
</developers>
<documentation> ssn68</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="kappa" support="S">
<version>2.1-12</version>
<path>applications/kappa</path>
<description>KAPPA - Kernel Application Package</description>
<abstract><p>
KAPPA is an applications package comprising about 200
general-purpose commands for image processing, data visualisation, and
manipulation of the standard Starlink data format---the NDF. It is
intended to work in conjunction with Starlink's various specialised
packages.
</p></abstract>
<dependencies >
<build>pcs</build><build>agi</build><build>ast</build><build>chr</build><build>cnf</build><build>fio</build><build>grp</build><build>hds</build><build>ifd</build><build>kaplibs</build><build>mers</build><build>ndf</build><build>one</build><build>par</build><build>pcs</build><build>prm</build><build>psx</build><build>sae</build><build>shl</build><build>tcl</build><build>tk</build><build>trn</build><build option='link'>ard</build><build option='link'>atl</build><build option='link'>kaplibs</build><build option='link'>irq</build><build option='link'>one</build><build option='link'>shl</build><sourceset>sst</sourceset><sourceset>star2html</sourceset><sourceset>messgen</sourceset>
</dependencies>
<developers>
<person>
<name>David Berry</name>
<uname>dsb</uname>
<email>d.berry@jach.hawaii.edu</email>
<role>owner</role>
</person>
<person>
<name>Malcolm J. Currie</name>
<uname>mjc</uname>
<email>mjc@star.rl.ac.uk</email>
<role>owner</role>
</person>
</developers>
<documentation> sun95</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="kaprh" support="U">
<version>2.0</version>
<path>applications/kaprh</path>
<description>KAPRH - A home for retired KAPPA applications</description>
<abstract><p>
KAPRH is an applications package containing commands
which have been ``retired'' from the KAPPA package (see SUN/95). They
are retained within KAPRH to satisfy any occasional need there may be for
them.
</p></abstract>
<dependencies >
<build>pcs</build><build>ast</build><build>fio</build><build>gks</build><build>gns</build><build>hds</build><build>idi</build><build>kaplibs</build><build>mers</build><build>ndf</build><build>par</build><build>pcs</build><build>prm</build><build>sae</build><build>trn</build><build>ifd</build><build>generic</build><build option='link'>agi</build><build option='link'>ard</build><build option='link'>cat</build><build option='link'>fio</build><build option='link'>gks</build><build option='link'>gns</build><build option='link'>grp</build><build option='link'>gwm</build><build option='link'>idi</build><build option='link'>kaplibs</build><build option='link'>ncar</build><build option='link'>ndf</build><build option='link'>ndg</build><build option='link'>pda</build><build option='link'>prm</build><build option='link'>psx</build><build option='link'>ref</build><build option='link'>sgs</build><build option='link'>shl</build><build option='link'>sla</build><build option='link'>snx</build><build option='link'>trn</build><sourceset>sst</sourceset><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>David Berry</name>
<uname>dsb</uname>
<email>dsb@ast.man.ac.uk</email>
<role>owner</role>
</person>
<person>
<name>Malcolm Currie</name>
<uname>dsb</uname>
</person>
</developers>
<documentation> sun239</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="messgen" support="S">
<version>1.2</version>
<path>applications/messgen</path>
<description>Starlink Facility Error Message Generation</description>
<abstract>
<p>The MESSGEN program creates files
required for proper operation of the system for associating messages with
Starlink facility status values on UNIX platforms.
The utility program CREMSG can be used to produce
source files for MESSGEN.</p>
</abstract>
<dependencies >
<sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>A J Chipperfield</name>
<uname>ajc</uname>
<email>A.J.Chipperfield@rl.ac.uk</email>
</person>
<person>
<name>B K McIlwrath</name>
<uname>bkm</uname>
<email>B.K.McIlwrath@rl.ac.uk</email>
</person>
<person>
<name>Norman Gray</name>
<uname>nxg</uname>
<email>norman@astro.gla.ac.uk</email>
<role>owner</role>
</person>
</developers>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="news" support="S">
<version>2.1-2</version>
<path>applications/news</path>
<description>Starlink online information system</description>
<abstract><p>Simple interactive tool for reading release notes.
</p></abstract>
<dependencies >
<configure>perl</configure><sourceset>star2html</sourceset>
</dependencies>
<developers>
<person>
<name>G R Mellor</name>
<uname>grm</uname>
</person>
<person>
<name>Martin Dunstan</name>
<uname>mnd</uname>
</person>
<person>
<name>Martin J Bly</name>
<uname>bly</uname>
</person>
</developers>
<documentation> sun195</documentation>
<bugreports>starlink@jiscmail.ac.uk</bugreports>
</component>
<component id="observe" support="U">
<version>2.3-2</version>
<path>applications/observe</path>
<description>OBSERVE --- Check Star Observability</description>
<abstract><p>
OBSERVE is designed to allow you to get a quick overview of the
observability of a star through the year from the geographical
location selected. You will be prompted for the RA and Dec of
the star, the telescope (you can also specify arbitrary