SETI public: Pulsars as beacons for SETI

From: William Edmondson (W.H.Edmondson_at_cs.bham.ac.uk)
Date: Thu Dec 29 2005 - 13:03:00 PST

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    Hi folks

    You may recall many months back I posted a URL for a paper I'd had
    published on a new search strategy. http://www.cs.bham.ac.uk/~whe/
    SETIPaper.pdf

    In February his year I visited Arecibo to gather some data, having
    being awarded some time (see http://www.cs.bham.ac.uk/~whe/
    AOproposal.pdf). We eventually had ~30 hours of dedicated 'scope
    time. Pretty impressive. I even got to drive the machine from my
    office back in UK for one observation session!

    It's been a bit of a slog to get the data storage and processing
    hardware organized (I don't work in a physics/astronomy department at
    the Uni in Birmingham - and yes, although I DO work in a Computer
    Science department we are the last people to need lots of storage
    etc....; it's a pretty theoretical department and many of my
    colleagues work with pencil and paper!).

    Shortly before Christmas the last two disks arrived from Arecibo and
    I now have 3TB of data connected to a dual G5 Mac dedicated to SETI
    work.

    So now the hard work begins. I am, essentially, using some well-known
    techniques from the world of pulsar search astronomy. I can
    recommend the following (but it is expensive):

    Handbook of Pulsar Astronomy, by Duncan Lorimer and Michael Kramer.
    Cambridge University Press. 2005.

    Duncan has been helpful with advice (my physics is a little rusty,
    having completed my degree several decades ago and then moving on to
    other fields).

    I am focussing at the moment on folding techniques, with some
    dispersion correction as well (although the target stars are not that
    far away one might envisage a small mark to space ratio in a pulsed
    transmission, which implies the need for de-dispersion to preserve
    pulse shape....). I am doing this because we have a target
    periodicity to search for, and folding can significantly enhance S/N
    ratio. I'll probably try some FFT as well, just in case there is a
    pulsar waiting to be discovered!

    I'll probably provide another update in a year's time.

    Happy searching in 2006.

    William Edmondson


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