OSO-8 Software: Example 2 - Extract a spectrum from a raw PHA file
To extract a spectrum from the raw PHA data use the tasks osofindfast
(step 1) and osopha (step 2).
Osofindfast, for a given sky position determines times when that position was
viewed by the A, B or C detector. Osopha extracts a 63 channel PHA
spectrum from the raw PHA data, and lightcurves in different energy bands with
40.96 sec time resolution.
Obtaining the “good
observing days” PHA data for input to osopha
The PHA filenaming convention is Npha_XXXX_YYYY.fits where N is the
detector (A, B, or C), XXXX and YYYY are the mission elapsed day
number of the start and stop of this file (from 176 to 1369). The
start and stop days are not all separated by the same amount. There is
not a direct way to find the appropriate PHA file for a given position
or time, however osofindfast can be used to determine the "good
observing days". These day numbers are embedded in the raw rates
filenames listed by osofindfast for the appropriate detector. After
determining the "good days", the appropriate PHA files to input in the
osopha are located in the OSO8 FTP area.
Using osopha
Run the routine OSOPHA. This task will produce both a collimator-corrected
light-curve AND a 1-63 channel PHA spectrum (NON-background subtracted ;
integration time of each data bin is 40.96 seconds).
Before running this tool it is necessary to create an ASCII file containing
a list of raw PHA files which correspond to the "good observing
days".
% cat a0620_list
cpha_176_375.fits
% osopha
Equinox (d/f 1950)[1950.0]
RA in hh mm ss.s or degrees[95.046]
DEC in dd mm ss.s or degrees[-0.32]
Rootname for generated spectral (+rates) output[a0620]
Desired detector [1=B,2=C]:[2]
Input listfile containing raw PHA files[a0620_list]
Contaminating srces in FOV check?(d/f no)[no]
Start PHA channel for broad-band light-curve (d/f 1)[1]
End PHA channel for broad-band light-curve (d/f 63)[63]
No. raw data integ. records (d/f=1 BC=40.96s)[1]
Low c/s threshold for lightcurve (d/f -10000)[-10000.]
High c/s threshold for lightcurve (d/f 10000)[10000.]
Start PHA for soft-band lightcurve [1-63] (d/f 5)[5]
End PHA for soft-band lightcurve [1-63] (d/f 14)[14]
Start PHA for hard-band lightcurve[1-63] (d/f 15)[15]
End PHA for hard-band lightcurve[1-63] (d/f 63)[63]
Input observation start date (dd/mm/yy)[29/09/75]
Input observation start time (hh:mm:ss)[00:00:00]
Input observation end date (dd/mm/yy)[03/10/75]
Input observation end time (hh:mm:ss)[00:00:00]
OSOPHA 1.0.0 start PHA + rates..
OBJECT NAME a0620
SOURCE RA and DEC (1950) 95.046 -0.320
DETECTOR 2
RAW DATA FILE LIST a0620_list
PHASE RESTRICTION ? F
FOV check for CONTAMINATING SOURCES ? F
START and END channels for LC creation 1 63
Integration time (no. raw data records to integrate) 1
INTENSITY CUT (cnts/sec) -10000.000 10000.000
CHANNEL BOUNDARIES 5 14 15 63
Mean BROAD band BKGD level (c/s) 0.000
Mean SOFT band BKGD level (c/s) 0.000
Mean HARD band BKGD level (c/s) 0.000
OBSERVATION START and STOP TIMES :
START day (of 1975) and MILLISECS of that day :
272 0
END day (of 1975) and MILLISECS of that day :
276 0
Creating a0620.lc
Creating a0620.spec
MEAN RATE (+error) for PHA data (c/s/detarea) :
8.083 0.002
HARDNESS RATIO for PHA data : 0.021
PHA ACCUMULATION TIME (secs) : 26202.357
NET AREA of detector (sq. cm) : 61.67
INTEGRATED RATE for PHA data (c/s) : 498.4867
**** OSOPHA 1.0.0 **** finished
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Page authors: Lorella Angelini Jesse Allen
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Last modified: Tuesday, 21-Apr-2020 15:45:23 EDT
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