source: trunk/docs/app-param.tex @ 373

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2% app-param.tex: Section listing all the possible input parameters and
3%                their defaults.
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29\secA{Available parameters}
30\label{app-param}
31
32The full list of parameters that can be listed in the input file are
33given here. If not listed, they take the default value given in
34parentheses. Since the order of the parameters in the input file does
35not matter, they are grouped here in logical sections.
36
37\secB*{Input related}
38\begin{Lentry}
39\item[{ImageFile [no default]}] The filename of the
40  data cube to be analysed.
41\item[{flagSubsection [false]}] A flag to indicate whether one
42  wants a subsection of the requested image.
43\item[{Subsection [ [*,*,*] ]}] The requested subsection
44 -- see \S\ref{sec-input} for details on the subsection format.  If
45 the full range of a dimension is required, use a \texttt{*} (thus the
46 default is the full cube).
47\item[{flagReconExists [false]}] A flag to indicate whether the
48  reconstructed array has been saved by a previous run of \duchamp. If
49  set true, the reconstructed array will be read from the file given
50  by \texttt{reconFile}, rather than calculated directly.
51\item[{reconFile [no default]}] The FITS file that contains the
52  reconstructed array. If \texttt{flagReconExists} is true and this
53  parameter is not defined, the default file that is looked for will
54  be determined by the \atrous parameters (see \S\ref{sec-recon}).
55\item[{flagSmoothExists [false]}] A flag to indicate whether the
56  Hanning-smoothed array has been saved by a previous run of \duchamp. If
57  set true, the smoothed array will be read from the file given
58  by \texttt{smoothFile}, rather than calculated directly.
59\item[{smoothFile [no default]}] The FITS file that has
60  a previously smoothed array. If \texttt{flagSmoothExists}
61  is true and this parameter is not defined, the default file that is
62  looked for will be determined by the smoothing parameters (see
63  \S\ref{sec-smoothing}).
64\end{Lentry}
65
66\secB*{Output related}
67\begin{Lentry}
68\item[{OutFile [duchamp-\\Results.txt]}] The file containing the
69  final list of detections. This also records the list of input
70  parameters.
71\item[{flagSeparateHeader [false]}] A flag to indicate that the header
72  information that would normally be printed at the start of the
73  results file (containing information on the parameters, image
74  statistics and number of detections) should instead be written to a
75  separate file.
76\item[{HeaderFile [duchamp-\\Results.hdr]}] The file to which the
77  header information should be written when
78  \texttt{flagSeparateHeader=true}.
79\item[{SpectraFile [duchamp-\\Spectra.ps]}] The postscript file
80  containing the resulting integrated spectra and images of the
81  detections. 
82\item[{flagLog [false]}] A flag to indicate whether the
83  details of intermediate detections should be logged.
84\item[{LogFile [duchamp-\\Logfile.txt]}] The file in which
85  intermediate detections are logged. These are detections that have
86  not been merged. This is primarily for use in debugging and
87  diagnostic purposes: normal use of the program will probably not
88  require it.
89\item[{flagOutputRecon [false]}] A flag to say whether or not
90  to save the reconstructed cube as a FITS file. The filename will be
91  derived according to the naming scheme detailed in
92  Section~\ref{sec-reconIO}.
93\item[{flagOutputResid [false]}] As for
94  \texttt{flagOutputRecon}, but for the residual array -- the
95  difference between the original cube and the reconstructed cube. The
96  filename will be derived according to the naming scheme detailed in
97  Section~\ref{sec-reconIO}.
98\item[{flagOutputSmooth [false]}] A flag to say whether or not
99  to save the smoothed cube as a FITS file. The filename will be
100  derived according to the naming scheme detailed in
101  Section~\ref{sec-smoothing}.
102\item[{flagVOT [false]}] A flag to say whether to create a
103  VOTable file with the detection information. This will be an XML
104  file in the Virtual Observatory VOTable format.
105\item[{votFile [duchamp-\\Results.xml]}] The VOTable file with
106  the list of final detections. Some input parameters are also
107  recorded.
108\item[{flagKarma [false]}] A flag to say whether to create a
109  Karma annotation file corresponding to the information in
110  \texttt{outfile}. This can be used as an overlay in Karma
111  programs such as \texttt{kvis}.
112\item[{karmaFile [duchamp-\\Results.ann]}] The Karma annotation
113  file showing the list of final detections. 
114\item[{flagMaps [true]}] A flag to say whether to save
115  postscript files showing the 0th moment map of the whole cube
116  (parameter \texttt{momentMap}) and the detection image
117  (\texttt{detectionMap}).
118\item[{momentMap [duchamp-\\MomentMap.ps]}] A postscript file
119  containing a map of the 0th moment of the detected sources, as well
120  as pixel and WCS coordinates.
121\item[{detectionMap [duchamp-\\DetectionMap.ps]}] A postscript
122  file with a map showing each of the detected objects, coloured in
123  greyscale by the number of detected channels in each spatial
124  pixel. Also shows pixel and WCS coordinates.
125\item[{flagXOutput [true]}] A flag to say whether to display a
126  0th moment map in a PGPlot X-window. This will be in addition to any
127  that are saved to a file. This parameter can be overridden by the
128  use of the \texttt{-x} command-line option, which disables the
129  X-windows output.
130\end{Lentry}
131
132\secB*{Modifying the cube}
133\begin{Lentry}
134\item[{flagTrim [false]}] A flag to say whether to trim
135  BLANK pixels from the edges of the cube -- these are typically
136  pixels set to some particular value because they fall outside the
137  imaged area, and trimming them can help speed up the execution.
138\item[{flagMW [false]}] A flag to say whether to ignore
139  channels contaminated by Milky Way (or other) emission -- the
140  searching algorithms will not look at these channels.
141\item[{maxMW [112]}] The maximum channel number that contains
142  ``Milky Way'' emission.
143\item[{minMW [75]}] The minimum channel number that contains
144  ``Milky Way'' emission. Note that the range specified by
145  \texttt{maxMW} and \texttt{minMW} is inclusive.
146\item[{flagBaseline [false]}] A flag to say whether to remove
147  the baseline from each spectrum in the cube for the purposes of
148  reconstruction and detection.
149\end{Lentry}
150
151\secB*{Detection related}
152
153\secC*{General detection}
154\begin{Lentry}
155\item[{flagStatSec [false]}] A flag indicating whether the
156  statistics should be calculated on a subsection of the cube, rather
157  than the full cube. Note that this only applies to the statistics
158  used to determine the threshold, and not for other statistical
159  calculations (such as those in the reconstruction phase).
160\item[{StatSec [ [*,*,*] ]}] The subsection of the cube used
161  for calculating statistics -- see \S\ref{sec-input} for details on
162 the subsection format. Only used if \texttt{flagStatSec=true}.
163\item[{flagNegative [false]}] A flag indicating that the
164  features of interest are negative. The cube is inverted prior to
165  searching.
166\item[{snrCut [3.]}] The threshold, in multiples of $\sigma$ above
167  the mean.
168\item[{threshold [no default]}] The actual value of the
169  threshold. Normally the threshold is calculated from the cube's
170  statistics, but the user can manually specify a value to be used
171  that overrides the calculated value. If this is not specified, the
172  calculated value is used. Also, when the FDR method is requested
173  (see below), the value of the \texttt{threshold} parameter is
174  ignored.
175\item[{flagGrowth [false]}] A flag indicating whether or not to
176  grow the detected objects to a smaller threshold.
177\item[{growthCut [2.]}] The smaller threshold using in growing
178  detections. In units of $\sigma$ above the mean.
179\item[{beamSize [10.]}] The size of the beam in pixels. If the
180  header keywords BMAJ and BMIN are present, then these will be used
181  to calculate the beam size, and this parameter will be ignored.
182\end{Lentry}
183
184\secC*{\Atrous reconstruction}
185\begin{Lentry}
186\item[{flagATrous [false]}] A flag indicating whether or not to
187  reconstruct the cube using the \atrous wavelet
188  reconstruction. See \S\ref{sec-recon} for details.
189\item[{reconDim [1]}] The number of dimensions to use in the
190  reconstruction. 1 means reconstruct each spectrum separately, 2
191  means each channel map is done separately, and 3 means do the whole
192  cube in one go.
193\item[{scaleMin [1]}] The minimum wavelet scale to be used in the
194  reconstruction. A value of 1 means ``use all scales''.
195\item[{scaleMax [0]}] The maximum wavelet scale to be used in the
196  reconstruction. If the value is $\le0$ then the maximum scale is
197  calculated from the size of the input array. Similarly, if the value
198  given is larger than this calculated value, the calculated value is
199  used instead.
200\item[{snrRecon [4]}] The thresholding cutoff used in the
201  reconstruction -- only wavelet coefficients this many $\sigma$ above
202  the mean (or greater) are included in the reconstruction.
203\item[{filterCode [1]}] The code number of the filter to use in
204  the reconstruction. The options are:
205  \begin{itemize}
206  \item \textbf{1:} B$_3$-spline filter: coefficients =
207    $(\frac{1}{16}, \frac{1}{4}, \frac{3}{8}, \frac{1}{4}, \frac{1}{16})$
208  \item \textbf{2:} Triangle filter: coefficients =
209    $(\frac{1}{4}, \frac{1}{2}, \frac{1}{4})$
210  \item \textbf{3:} Haar wavelet: coefficients =
211    $(0, \frac{1}{2}, \frac{1}{2})$
212  \end{itemize}
213\end{Lentry}
214
215\secC*{Smoothing the cube}
216\begin{Lentry}
217\item[{flagSmooth [false]}] A flag indicating whether to
218  smooth the cube. See \S\ref{sec-smoothing} for details.
219\item[{smoothType [spectral]}] The smoothing method used: either
220  ``spectral'' (with a 1D Hanning filter) or ``spatial'' (with a 2D
221  Gaussian filter). 
222\item[{hanningWidth [5]}] The width of the Hanning smoothing
223  kernel.
224\item[{kernMaj [3]}] The full-width-half-maximum (FWHM) of the
225  2D Gaussian smoothing kernel's major axis.
226\item[{kernMin [3]}] The FWHM of the 2D Gaussian smoothing kernel's
227  minor axis.
228\item[{kernPA [0]}] The position angle, in degrees,
229  anticlockwise from vertical (\ie usually East of North).
230\end{Lentry}
231
232\secC*{FDR method}
233\begin{Lentry}
234\item[{flagFDR [false]}] A flag indicating whether or not to use
235  the False Discovery Rate method in thresholding the pixels.
236\item[{alphaFDR [0.01]}] The $\alpha$ parameter used in the FDR
237  analysis. The average number of false detections, as a fraction of
238  the total number, will be less than $\alpha$ (see
239  \S\ref{sec-detection}).
240\end{Lentry}
241
242\secC*{Merging detections}
243\begin{Lentry}
244\item[{minPix [2]}] The minimum number of spatial pixels for a
245  single detection to be counted.
246\item[{minChannels [3]}] At least one contiguous set of this many
247  channels must be present in the detection for it to be accepted.
248\item[{flagAdjacent [true]}] A flag indicating whether to use
249  the ``adjacent pixel'' criterion to decide whether to merge
250  objects. If not, the next two parameters are used to determine
251  whether objects are within the necessary thresholds.
252\item[{threshSpatial [3.]}] The maximum allowed minimum spatial
253  separation (in pixels) between two detections for them to be merged
254  into one. Only used if \texttt{flagAdjacent = false}.
255\item[{threshVelocity [7.]}] The maximum allowed minimum channel
256  separation between two detections for them to be merged into
257  one.
258\end{Lentry}
259
260\secC*{Other parameters}
261\begin{Lentry}
262\item[{spectralMethod [peak]}] This indicates which method is used
263  to plot the output spectra: \texttt{peak} means plot the spectrum
264  containing the detection's peak pixel; \texttt{sum} means sum the
265  spectra of each detected spatial pixel, and correct for the beam
266  size. Any other choice defaults to \texttt{peak}.
267\item[{spectralUnits [km/s]}] The user can specify the units of
268  the spectral axis. Assuming the WCS of the FITS file is valid, the
269  spectral axis is transformed into velocity, and put into these units
270  for all output and for calculations such as the integrated flux of a
271  detection.
272\item[{pixelCentre [centroid]}] Which of the three ways of
273  expressing the ``centre'' of a detection (see \S\ref{sec-results}
274  for a description of the options) to use for the X, Y, \& Z
275  columns in the output list. Alternatives are: \texttt{centroid, peak,
276  average}.
277\item[{drawBorders [true]}] A flag indicating whether to draw
278  borders around the detected objects in the moment maps included in
279  the output (see for example Fig.~\ref{fig-spect}).
280\item[{drawBlankEdges [true]}] A flag indicating whether to
281  draw the dividing line between BLANK and non-BLANK pixels on the
282  2D images (see for example Fig.~\ref{fig-moment}).
283\item[{verbose [true]}] A flag indicating whether to print the
284  progress of any computationally intensive algorithms (\eg
285  reconstruction, searching or merging algorithms) to the screen.
286\end{Lentry}
287
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