aglc - Examples | ||||||||||||
|
The following two demonstration scripts will perform a number of operations and echo the principle aglc functions to the terminal along with commentary. The scripts must be run in ISIS.
Vela X-1 hardness selected spectraThis demo script reads the Vela X-1 events, forms light curves in several bands, plotting as it goes. It then forms a color-color plot, and selects based on the hardness ratio, bins spectra from the selections, and finally re-plots the light curve and marks the bins based on the hardness selection.This example demonstrates the use of reverse indices and dynamic binning of grating spectra. VX1_demo_1.ps.gz is the summary graphic produced. isis.log is an isis log. 44 Boo phased light curve and flare filteringThis demo script reads the 44 Boo - a short period coronally active binary - and bins light curves in two wide bandpasses. From the hardness ratio, it identifies 3 flares, filters the data on the non-flare times, and bins a phased light curve. Using various time manipulation functions, it shows the light curves in unfolded phase, phase, and unbinned phase (i.e., each time's phase bins vs. phase, but not summed).LC_Demo_44_Boo.ps.gz is the summary graphic produced by the script. isis.log is an isis log. Data Files for the ExamplesThe example event files, scripts, logs, and plots may all be downloaded here: Examples.tgz (14MB). Event files have been truncated to the minimum columns required, and are compressed. (They may be used in compressed form if you have cfitsio and/or ciao installed with the gzip option enabled.) |
This page was last updated Apr 15, 2009 by David P. Huenemoerder. To comment on it or the material presented here, send email to dph@space.mit.edu.
![]()