Select the P40 ERD file and read it into the PIA buffer. The P40
ERD files have PSER prefix (both PHT-SS and SL measurements are
together in one file).
[ ] (Top Window) Files ->
Files Manager
[ ] Select File Type: ERD and Detectors:
SS/SL
using the two filter windows.
[ ] The P40 ERD file name(s) should appear
in the "Files" subwindow. If not,
you can click
on one of the subdirectory names shown in the
"Subdirectories"
subwindow to see if you can navigate to the desired file.
Once you have
located the correct file in the "Files" subwindow, click on
the file name.
[ ] Click on "Read File" button to read
the selected file into the PIA buffer.
[ ] Option: Click on "Show Header" button
to view or to print the ERD FITS
header.
Select an ERD measurement for processing.
[ ] (Top Window) Buffers ->
Buffers Manager
[ ] Select Data Type: ERD and Detectors:
SL/SS.
All the measurements in the
selected category
should show up in the "measurement" window. Usually,
there are 2 measurements:
the first one is a "pseudo" dark measurement
and the 2nd one
is the real observation. Hence, click on the 2nd
measurement.
[ ] Click on the "Plot & Reduce Data"
button to bring up the PIA ERD window.
[ ] Option: Click on the "Show..." button
in the Buffers Manager window to
view FITS header,
Compact Status or even the data values themselves.
In the case of a chopped observation:
[ ] (SCP Window) Process ->
Background Subtraction (within measurement)
This brings up
two windows: PIA Background Subtraction Menu and a graphic
window displaying
the "grand average signal" per chopper step.
[ ] Usually, one needs only to click on
the "OK" button in the Menu window.
[ ] Click on the "Subtracted meas -> buffer"
button to write the
sky-subtracted
spectrum to the SCP buffer.
[ ] Now let's display the sky-subtracted
spectrum. Exit out of all the Data
Display windows,
then go to the Buffer Control Panel and select SCP and
SL/SS for
the Data Type and Detectors respectively. Select the
background subtracted
data and click on the "Plot & Reduce Data" button
to bring up the
PIA SCP window.
Caution:
avoid using the Load button to display the subtracted data
because this makes
the appropriate Process option (Chopped SPRF)
unavailable.
[ ] (SCP Window) Process -> Power Calibration
--> Chopped SPRF (only for SL)
This will bring
up the AAP window.
[ ] Option: you can save the SCP result
of sky-subtracted spectrum by clicking
in the SCP window
"Data --> Save --> To a PIA Internal File."
In the case of a staring observation:
[ ] (SCP Window) Process -> Power Calibration
--> Default Responses (orbital
dep.) --> Perform
it. This will bring up the AAP window.
[ ] Option: you can save the SCP result
of sky-subtracted spectrum by clicking
in the SCP window
"Data --> Save --> To a PIA Internal File."
Hint: if you have a sky measurement from another
observation, you can do a
sky subtraction from the spectrum of the
current staring observation at
the AAP level by click there "Process -->
Background Subtraction --> another
measurement." Make sure that you loaded the
AAP result of the sky measurement.
Note: This data reduction of SCP to AAP actually produces the intermediate SPD result which is not displayed automatically. You can however display the SPD result using the buffer manager in the conventional way.
[ ] Option: If you have not save the SPD
result, you may want to save the
AAP result now.
To do so, click "Data --> Save --> PIA Internal File"
in each of the
AAP windows displayed.
[ ] (Top Window) Buffers ->
Astrophysical Work
An Astrophysical
Applications Menu window appears on your screen.
[ ] Select the "Spectro-Photometry" function.
This brings up
a window called PIA Spectro-photometry.
[ ] (Spectro-photometry window) Click
on the "File" button and then
"Select measurement."
Choose the measurement to be loaded.
[ ] (Spectro-photometry window) Click
on the "Plot" button to plot the
spectrum in a
number of different ways. Use the "new" option for
the spectrum plot.
Hint: To display the SS and SL parts of the
spectrum together, first plot
one as described above and leave the plot
on. Then read the other part into
Astrophysical Work, but choose "Overplot
--> Synchronized" (instead of "New")
to display the two parts together.