Anita Richards and members of MERLIN, RadioNet and AstroGrid teams. ● 'Old' radio archive access ● Source lists, fixed images or visibility data ● Most.

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Presentation transcript:

Anita Richards and members of MERLIN, RadioNet and AstroGrid teams. ● 'Old' radio archive access ● Source lists, fixed images or visibility data ● Most maps only inner few arcsec, fixed resol n ● MERLIN archive on-demand imaging ● via AstroGrid, using ParselTongue ● Next-generation interferometry ● Archive development strategies ● VO requirements ● Enable all astronomers to use multi-l data Radio data access: on-demand interferometry imaging

Interferometry data  GB – TB raw data per experiment (mins - weeks)  Visibility data Cal sources. antennas etc.  Domain-specific software  No unique product  Resolution v. sensitivity tradeoff by baseline weighting  3D/polarisation cubes, spectra, time series...  Field of view e.g. 8', image pixels 10 mas  Map out regions of interest, usually not all 10 9 pixels  Most PI results too varied to archive  Pipeline data for VOs  Quick Look static images  Flexible products to order  Raw data option rarely wanted if alternatives!

Interferometry visibility amplitude v. baseline length Calibrated, binned visibility amplitudes Quick-look image Data cube First Moment Data examples

IR from warm dust in remnant AGB shell (IRAS, ISO, 2MASS) Non-thermal nebular radiocontinuum (various - Vollmer catalogue) Hot stellar emission FUSE, IUE  Non-expert access pre  Ready-made FITS images Aladin  Catalogues: SpecFind

VLBI data – then and now VLBI data – then and now C20: Search list by experiment code C21: Friendly search Pipeline products VO links

MERLIN 2005 Web forms: static images Calibrated visibility data  Visibilities live on disc, calibrated  Sample products  User version of pipeline  Still need AIPS

What's wrong with that?  Dedicated web site fine for PIs of major projects Able to use domain-specific projects For simple observations, even PIs use pipeline images!  Not really friendly for non-experts  Not convenient for multi-wavelength  Can't be used easily in workflows  Need VO access  Databases of observations and metadata  Static quick-look products  Flexible data products  ATCA/CSIRO prototype imager using VO interferometry data model

2006 AstroGrid Workbench MERLINImager Simple inputs Name/ Pos (Size Resln Freq Date)

User AstroGrid Workbench Task Launcher MERLINImager Position, size, n, resol n, date Registry CEA JBO server Python (perl/dbi) ParselTongue Select AIPS data Image best 5 (calibration, fov) FITS images, logs, to public HTML area SIAP VOTable2006 AstroGrid Task RadioNet package MERLINImager MySpace Aladin, TopCat Download

Interoperability (Plastic)  Matching resolution  Spectral index image 18 cm 6 cm Steep spectrum – SE not AGN

Hunt-the-AGN in Markarian 273 MERLIN 6 cm 18 cm HST 110, 160, 220 N N N SE SE? SW SW?  Compare: old static fixed resolution images

Coming soon: M+VLA HDF(N) cutouts 1” 10 mJy contours + X-ray selected AGN2 1 < z < AGN Starburst with AGN core Starburst

Next Generation Interferometers  e-MERLIN, eVBLI, EVLA ATCA/LBA, LOFAR, GMRT, ALMA, SKA etc  Committed to VO access  Software development RadioNet – ParselTongue (Python over e.g. AIPS) NRAO – CASA (aips++ based, Python scripting). ESO – XML binary and metadata storage  'B2E' obs-to-archive integrated data path  Metadata retrieval  Flexible remote processing of products  VO components in archive management?  Cornish, GMRT, MMB and other surveys

Char DM Markarian 18 cm

Development  Expand/apply VO standards  Spatial frequencies, polarization...  Tools for radio data (Jy/beam, 3+D cubes...)  Authentication  Expand data products/services available  Robustness  Visibility data, spectra, time series  Single-dish data  Image cutouts for Deep Fields  Solve queuing/overload and other problems  Impliment at other sites/other radio datasets

AstroGrid/RadioNet workshop