Source directory | /data/lofarschool/data/Exercise-PSR-02 |
---|---|
Contact person | Jason Hessels |
This exercise simultaneously illustrates two fundamental steps in pulsar data reduction: dedispersion and folding.
Little prerequisite knowledge required, except perhaps knowing what a pulsar is, which you should know already!
In this exercise, the user takes a number of subbands and both folds and dedisperses these with respect to each other in order to bring a pulsar signal out of the noise. This is done in a number of steps, which illustrate how one can optimize the detected signal, starting from a rough estimate of the spin ephemeris. This exercise uses the PRESTO routine “prepfold”, which produces a detailed diagnostic plot with signal properties. Such plots are the cornerstone of pulsar searches, in which one must separate potential astronomical signals for a background of RFI signals, some of which are particularly good at masquerading as pulsars. There are _many_ options one can use with prepfold, so feel free to try these out!
DATA:
The “raw” data is a set of LOFAR subbands:
B0809+74_081220_4tiles.sub(000,283-327)
with corresponding meta-data:
B0809+74_081220_4tiles.sub.inf
Using a python script, these subbands were extracted to PRESTO format from a beam-formed HDF5 file, which in turn was created with the DAL routine “bf2h5”. When running bf2h5 on the truly raw, station data, the time resolution is downsampled by a factor of 128.
OTHER FILES:
B0809+74.par: This ascii file contains the rotational ephemeris of the pulsar, necessary for predicting the required folding period at the observation epoch.
COMMANDS.txt: The commands that the user should run (in order).
PULSAR_ENV: Required environment variables for running PRESTO (bash shell assumed).
prepfold -timing B0809+74.par B0809+74_081220_4tiles.sub[0-9]*
prepfold -start 0.02 -timing B0809+74.par B0809+74_081220_4tiles.sub[0-9]*
prepfold -o BEST_FOLD -start 0.02 -topo -par B0809+74.par -fine B0809+74_081220_4tiles.sub[0-9]*