first e- evn science and future astronomy projects via expres
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First e- EVN Science and Future Astronomy projects via EXPReS. Michael Garrett Joint Institute for VLBI in Europe. e-VLBI Workshop, Sydney, 13 July 2005. Telescope last mile. e-VLBI Milestones. 2006. 2003. 2004. 2005. e -EVN: Current Status (Astronomer’s Perspective). - PowerPoint PPT PresentationTRANSCRIPT
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First e-EVN Science and Future Astronomy projects via EXPReS
Michael Garrett
Joint Institute for VLBI in Europe
e-VLBI Workshop, Sydney, 13 July 2005.
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20062003 2004 2005
Telescope last mile
e-VLBI Milestones
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e-EVN: Current Status (Astronomer’s Perspective)
• 6 telescopes “on-line”– WSRT, NL (14 x 25m), – Torun, PL (32-m), – Onsala, SE (26 & 25-m), – Jodrell Bank, UK (76-m, 25-m), – Cambridge, UK (or other
MERLIN antennas) – Arecibo, USA (at 155 Mbps)
Medicina May 2005
• Medicina, IT (32-m) connection under construction.
• Robust fringes demonstrated at 128 Mbps (see Arpad Szomoru, JIVE).
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GÉANT-2
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e-VLBI – European Approach
• Get the European and National networking people interested: – SURFnet (6 x 1 Gbps connectivity to EVN Correlator at JIVE)
– GÉANT-2 (DANTE) – Pan-European Research Network
– Most networks under-utilised…
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GÉANT-2
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e-VLBI – European Approach
• Get the European and National networking people interested: – SURFnet (6 x 1 Gbps connectivity to EVN Correlator at JIVE)– GÉANT-2 (DANTE) – Pan-European Research Network– Most networks under-utilised…
• Focus on:
– e-VLBI using existing telescope data acquisition system - Mk5
– Protocol replacement to achieve (> 500 Mbps)
– Last mile connections to EVN telescopes (network problems will solve themselves… eventually)
– Funding future e-VLBI developments (EXPReS)
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Why e-VLBI ?
• Reliability – real-time feedback to the telescopes
• Sensitivity – sustained high data rates possible
• Logistics – No media management
• Rapid science results:– Geodesy – Precision spacecraft navigation
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Why e-VLBI (cont) ?
• Target of Opportunity (ToO) capability:
– Dominated by VLBA currently
– Reliability & Logistics e-VLBI
– Sensitivity e-VLBI
– Rapid science e-VLBI
– Optimal observing strategy (obs. freq., calibrators, telescope array)
– SWIFT, LOFAR Transients etc. ToOs may become much more common e-VLBI
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First e-VLBI Science – Spectral-line (32 Mbps)
PI:Richards et al.September 2004.
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A team of radio astronomers led by JIVE (Gurvits et al.) detected andTracked the Huygens probe using VLBI and e-VLBI techniques (see Tasso Tzimious talk).
e-VLBI Science – ESA Huygens
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VLBI determination of the Huygens descent trajectory
“Doppler interferometry”: ~25 km
A priori accuracy: ~100 km
Full VLBI accuracy: ~ 1 km
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e-VLBI Science – ESA Huygens
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Huygens radial velocity measurements
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• First continuum real-time e-VLBI science:
– March 11 2005 – WSRT, Onsala 25-m, Lovell 76-m, Cambridge 32-m , Arecibo,– Sustained 64 Mbps operations.
– Jodrell & Cambridge “winded-off”
– First part of expt (long scans on calibrators went well)
– Second part employed phase-refererencing (rapid telescope switching) correlator chocked on…
– About 1 hr of good data from 3 hr expt…
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• Target source – SN2001em (in UGC11794):
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Paragi et al. 2005 (astro-ph)Garrett et al. in prep.
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• “First Science” plans:
– Continue technical tests (1 day per 6 weeks)
– Use part of the technical test time to do real science @ 128 Mbps
– Open call for proposals in Autumn 2005
– Move towards sustained science @ 256 Mbps in 2006.
– Develop e-EVN Target of Opportunity policy within EVN
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Future e-VLBI Funding - EXPReS!
• Recently submitted a I3 proposal to the EC (DG-INFSO)
EXPReS = EXpress Production Real-time e-VLBI Service
• EXPReS launched by European Commissioner for Sci & Res:
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EXPReS – major aims • Proposed goals:
– Making e-VLBI an operational astronomical instrument 16 telescopes connected to JIVE at 1 Gbps Transparent inclusion of e-MERLIN antennas within e-EVN Target of Opportunity Capability
– Arpad Szomoru, JIVE.
– Networking Activities (not what you think!) – Expanding the network of telescopes that are on-line – - Paco Colomer, OAN.
– Future developments in e-VLBI > 1 Gbps data rates, distributed correlation, extended LOFAR etc.
– Huib Jan van Langevelde & Arpad Szomoru, JIVE.
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EXPReS – Financing & Partners • Funding:
– EXPReS rated No. 1 out of 43 proposals– EC award – 3.9 Million Euro – Total Cost of EXPReS – 16 Million Euro
• Partners (19 in total):
– The usual suspects – EVN institutes, incl. NAIC (Arecibo), HRAO (South Africa) & ShAO (China)
– Other telescopes: VIRAC (Latvian 32-m RT) + TIGO (6-m telescope, Concepcione Chile) – CSIRO – National Research Networks (SURFnet, AARNET, PNSC) – DANTE (operators of the pan-European network, GÉANT)– Coordinator : JIVE
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EXPReS - Australia
• e-VLBI data transfers (e.g. Huygens) • Remote observing (ATNF – Europe)
– SKA – must seem as though it is on astronomer’s door-step.
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Expanding the e-VLBI Network
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1 Gbps
1 Gbps (2006/7)
1 Gbps (200?)