Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xmm.vilspa.esa.es/sas/6.5.0/doc/rgsspecplot.ps.gz Дата изменения: Tue Aug 16 05:54:50 2005 Дата индексирования: Tue Oct 2 09:10:40 2012 Кодировка: Поисковые слова: reflection nebula

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rgsspecplot
August 16, 2005
Abstract
Produces annotated display of RGS spectra
1 Instruments/Modes
RGS Spectroscopy
2 Use
pipeline processing yes
interactive analysis yes
3 Description
This task plots the rst and second order spectra (BETA CHANNEL vs. Counts) for an RGS source,
overlaying the source dependent energy and wavelength scales. The data can be represented in original
format, or rebinned, to contain a minimum number of counts (specied by the user) per bin. In this
case, the counts/channel for each bin are plotted verses the centre of that bin, as a histogram. The error
values are plotted in gray and are always the square root of the counts. Details of the observation and
source are also plotted. Any valid PGPLOT graphics device may be specied for the output.
3.1 Examples
To create a postscript plot, called plot.ps, which contains the rst and second order spectra for source 1,
where the spectra have been rebinned to contain at least 10 counts per bin, a command such as,
rgsspecplot spectrumsets="SPECTRUM0101.FIT SPECTRUM0102.FIT" sourcelistset=rgssources.ds
sourceid=1 plotfile=plot.ps device=/VCPS rebin=yes mincounts=10
can be used.
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4 Parameters
This section documents the parameters recognized by this task (if any).
Parameter Mand Type Default Constraints
spectrumsets yes string
Input spectrum les list to be plotted. These are output from evselect List: rst order.ts sec-
ond order.ts (until DSS procedures are implemented).
sourcelistset yes string
Input RGS source list le (required until DSS procedures are implemented).
sourceid no integer 1 constraints
source number in sourcelist to be used for wavelength/energy scales (until DSS procedures are imple-
mented).
group no Boolean False constraints
Should the spectrum be grouped according to the existing grouping column?
device no string /XW
A valid PGPLOT graphics device for the output (e.g /XSERVE, /VCPS)
plotle no string
Name of hardcopy plot lename
rebin no Boolean False constraints
Rebin the data to contain mincounts/bin?
mincounts no integer constraints
Minimum number of counts per bin
5 Errors
This section documents warnings and errors generated by this task (if any). Note that warnings and
errors can also be generated in the SAS infrastructure libraries, in which case they would not be docu-
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mented here. Refer to the index of all errors and warnings available in the HTML version of the SAS
documentation.
badDevice (error)
Unrecognized PGPLOT device
Incorrect number of spectrum sets given (error)
Has to be either 1 or 2
No plot le supplied (error)
Hard copy device selected
Plot le already exists (error)
SAS-CLOBBER set
Surplus lename (warning)
plotle parameter value ignored
corrective action: -
Rebin requested to be less than 1 (warning)
No rebinning will take place
corrective action: -
Rebinning results in less than 5 bins (warning)
Replacing minimum counts per bin by a smaller number
corrective action: -
Keyword HDUCLAS2 missing (warning)
corrective action: -
Average counts per bin less than 1 (warning)
Replacing minimum counts per bin by (counts specied)
corrective action: -
6 Input Files
1. RGS order/source specic spectrum les (output of evselect)
1. RGS source list le (output of rgsregion)
7 Output Files
1. Hardcopy plot (optional)
8 Algorithm
subroutine rgsspecplot
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For each spectrum
Get observation details from KEYWORDS
Get source details from KEYWORDS
Get a handle on CHANNELS, COUNTS/RATE and GROUPING columns
if (group) then group CHANNELS
if (rebin) then rebin to a minimum counts/bin, specified by the user
Plot spectrum
Plot chip boundaries
Plot source dependent energy and wavelength scales using RGSLIB call lambda2beta:
betaCor = lambda2Beta(wavelength, order, offaxis(1))
end loop
end subroutine rgsspecplot
9 Comments
Error checking for le consistency also required until DSS implemented.
10 Future developments
Once the DataSubSpace has been implemented the code should access the following source-dependent
data from the extraction region le stored in the DSS of the spectrum le. The required keywords will
be/are added by rgsregion.
1. o-axis angle
2. sourceID
3. orderID
The sourcelist and sourceid command line parameters will become defunct.
References
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Figure 1: Examples of rgsspecplot PPS product: Plot showing both spectra plots.
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