GALFA Software Group GALFA-HI –Narrow-band spectral line data cubes of HI emission GALFA-RRL –Narrow-bad spectral line data cubes of recombination lines.

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Presentation transcript:

GALFA Software Group GALFA-HI –Narrow-band spectral line data cubes of HI emission GALFA-RRL –Narrow-bad spectral line data cubes of recombination lines (multiple frequencies within the band) GALFA-CON –Wide-band, spectro-polarimetry (multi-channel) data cubes In process of forming… GALFA image products

Software Stages Phase I - Data Acquisition –Sample multi-beam data streams from the spectrometer –Format and store along with calibration data and positions tags Phase II - Image formation –Apply calibration –Correct for instrumental effects Spectral baselines Non-Gaussian beam Sidelobes –Rasterize/basket weave Phase III – Scientific processing/visualisation –Source catalogues, Rotation measure images, HISA detection, Faraday tomography Data/image Archiving

Status resources GALFA-CON: Phase I: Desh –separate the Cal ONs and OFFs for each of the beams, and averaging data over a desired integration time (e.g. 1 sec). –detect RFI and exclude the affected correlation sets from the average. –van-Vlack correcting the correlations of signals quantized to limited bits. –compute (auto/cross) power spectra corresponding to the average auto/cross correlations, with optional smoothing/windowing etc. –output to ASCII file the average spectral Stokes parameter data for every integration interval with associated sky position information. Phase II : Christy Bredeson, Jo-Anne Brown –Begin work this fall Phase III: –Jo-Anne Brown (rotation measure images) –Desh (Faraday Tomography)

GALFACTS Pilot Study GALFA Continuum Transit Survey Fast scans along meridian Full polarimetry with L-wide & WAPP 4x256 lag correlations “winking” CAL 25 Hz Bonn Image resolution 10′ I Q U

Status resources GALFA-HI(RRL): Phase I: –Output to “Big Dish” FITS file using current software. Phase II: John Goldsten –Development underway using IDL Phase II: –Richard Gooch (visualisation using karma) –?

Issues Role of consortium in phase I and II –Model for software development? Individual efforts or coordinate development? –Common code base (IDL) Identify common features Share algorithms and code –Quality control and oversight? –data products to consortium or software delivered to consortium? –Time line Phase III responsibility of science teams? Data achiving –Who? –Where?

GALFACTS (GALFA Continuum Transit Survey) Covers all sky visible from Arecibo several year project ( )