source: trunk/docs/future.tex

Last change on this file was 1028, checked in by MatthewWhiting, 12 years ago

A large bunch of additions & improvements to the Guide

File size: 2.7 KB
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[303]1% -----------------------------------------------------------------------
2% future.tex: Future possible developments for Duchamp.
3% -----------------------------------------------------------------------
4% Copyright (C) 2006, Matthew Whiting, ATNF
5%
6% This program is free software; you can redistribute it and/or modify it
7% under the terms of the GNU General Public License as published by the
8% Free Software Foundation; either version 2 of the License, or (at your
9% option) any later version.
10%
11% Duchamp is distributed in the hope that it will be useful, but WITHOUT
12% ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
13% FITNESS FOR A PARTICULAR PURPOSE.  See the GNU General Public License
14% for more details.
15%
16% You should have received a copy of the GNU General Public License
17% along with Duchamp; if not, write to the Free Software Foundation,
18% Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307, USA
19%
20% Correspondence concerning Duchamp may be directed to:
21%    Internet email: Matthew.Whiting [at] atnf.csiro.au
22%    Postal address: Dr. Matthew Whiting
23%                    Australia Telescope National Facility, CSIRO
24%                    PO Box 76
25%                    Epping NSW 1710
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27% -----------------------------------------------------------------------
[158]28\secA{Future developments}
29
[162]30Here are lists of planned improvements and a wish-list of
[158]31features that would be nice to include (but are not planned in the
[162]32immediate future). Let me know if there are items not on these lists,
33or items on the list you would like prioritised.
[158]34
[162]35Planned developments:
[158]36\begin{itemize}
[162]37\item Parallelisation of the code, to improve speed particularly on
38multi-core machines.
[158]39
40\item Better determination of the noise characteristics of
41  spectral-line cubes, including understanding how the noise is
[162]42  generated and developing a model for it.
[158]43 
44\item Include more source analysis. Examples could be: shape
45  information; measurements of HI mass; more variety of measurements
[162]46  of velocity width and profile.
[158]47
48\item Improved ability to reject interference, possibly on the
[162]49  spectral shape of features.
[158]50
51\item Ability to separate (de-blend) distinct sources that have been
[162]52  merged.
53\end{itemize}
[158]54
[162]55Wish-list:
56\begin{itemize}
57\item Incorporation of Swinburne's S2PLOT
58\footnote{\href{http://astronomy.swin.edu.au/s2plot/}
59{http://astronomy.swin.edu.au/s2plot/}} code for improved
60visualisation.
[158]61\item Link to lists of possible counterparts (\eg via NED/SIMBAD/other
[162]62  VO tools?).
[158]63
64\item On-line web service interface, so a user can upload a cube and
[162]65  get back a source-list.
[158]66
[258]67\item Embed \duchamp in a GUI, to move away from the text-based
[162]68  interaction.
[158]69\end{itemize}
70
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