source: tags/release-1.1.7/docs/future.tex @ 1455

Last change on this file since 1455 was 303, checked in by Matthew Whiting, 17 years ago
  • Update the Outputs chapter to mention the use of F_tot.
  • Fixed comments in pgplot_related.c
  • Added distribution text to tex files.
File size: 3.2 KB
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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
26%                    AUSTRALIA
27% -----------------------------------------------------------------------
28\secA{Future developments}
29
30Here are lists of planned improvements and a wish-list of
31features that would be nice to include (but are not planned in the
32immediate future). Let me know if there are items not on these lists,
33or items on the list you would like prioritised.
34
35Planned developments:
36\begin{itemize}
37\item Parallelisation of the code, to improve speed particularly on
38multi-core machines.
39
40\item Better determination of the noise characteristics of
41  spectral-line cubes, including understanding how the noise is
42  generated and developing a model for it.
43 
44\item Include more source analysis. Examples could be: shape
45  information; measurements of HI mass; more variety of measurements
46  of velocity width and profile.
47
48\item Improved ability to reject interference, possibly on the
49  spectral shape of features.
50
51\item Ability to separate (de-blend) distinct sources that have been
52  merged.
53\end{itemize}
54
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.
61\item Link to lists of possible counterparts (\eg via NED/SIMBAD/other
62  VO tools?).
63
64\item On-line web service interface, so a user can upload a cube and
65  get back a source-list.
66
67\item Embed \duchamp in a GUI, to move away from the text-based
68  interaction.
69\end{itemize}
70
71\secA{Why ``\duchamp''?}
72
73Well, it's important for a program to have a name, and the initial
74working title of \emph{cubefind} was somewhat uninspiring. I wanted to
75avoid the classic astronomical approach of designing a cute acronym,
76and since it is designed to work on cubes, I looked at naming it after
77a cubist. \emph{Picasso}, sadly, was already taken \citep{minchin99},
78so I settled on naming it after Marcel Duchamp, another cubist, but
79also one of the first artists to work with ``found objects''.
80
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