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Opticon Porto 1 High Time Resolution Astrophysics Network Andy Shearer Centre for Astronomy School of Physics, NUI, Galway Ireland
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Opticon Porto2 special thanks to Don Phelan, NUI, Galway taking over network administration coordinating the two workshops editing the two volumes of proceedings annual meetings
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Opticon Porto3 Background - rationale for the network Are there special HTRA requirements? detectors high quantum efficiency photon counting low (zero?) read-out noise APDs, EMCCD, PNCCDs, Transition Edge Sensors, superconducting tunnel diodes wide wavelength range UV-IR instruments spectroscopy : Ultraspec photometry : Ultracam, Optima, S-CAM polarimetry : Optima, GASP very short time scales (t < 10 -7 s): Quanteye, GASP
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Opticon Porto4 Key Deliverables & Objectives in FP6 Key Objective “…will bring together the expertise of different teams which have so far developed HTRA independently..” Key Deliverables Report on the state-of-the-art in HTRA International Conference
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Opticon Porto5 Activity Workshop held in June, 2006 at NUI, Galway, Ireland 20 invited experts Over 45 attendees 13 Countries represented Topics Science, Instrumentation, Detectors, Software, Future Plans
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Opticon Porto6 Report on the state-of-the-art in HTRA High Time Resolution Astrophysics Springer-Verlag : Astrophysics & Space Science Library (ASSL) ISBN 978-1-4020-6517-0 & 978-1- 4020-6518-7 Published August 2007 More info on the HTRA website at http://astro.nuigalway.ie/htra http://astro.nuigalway.ie/htra
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Opticon Porto7 International Conference held in Edinburgh in September 2007 “High Time Resolution Astrophysics: The Universe at sub-second timescales” Royal Observatory Edinburgh over 3 days International Scientific Organising Committee Participants from 12 countries 39 papers presented Industrial sponsorship and endorsement of HTRA
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9 Network Deliverables Proceedings Published 2008 ISBN 978-0-7354-0503-5 Network Communication Regular updates and discussions through mailing lists annual network meetings joint observing programmes and instrument development
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Opticon Porto10 Summary All Key Objectives and Deliverables completed in 2008 Real integration and restructuring of the HTRA community International profile resulting from conferences and book publications
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Opticon Porto11 Summary 2 - Science Main science targets Binary systems CVs X-ray binary system Neutron stars Gamma ray Bursts AGN Transits Transients Flaring 2nd order correlations
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Opticon Porto13 adapted from Ryan & Redfern, HTRA, ASSL, 351, 229 see also Dhillon, same volume
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Opticon Porto14 Future plans under FP7 Continuation of the network building upon our work under FP6 .... with the aim of formulating a comprehensive scientific overview of HTRA into the extremely large telescopes [ELT] era...... primarily looking at HTRA science and instrument requirements
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Opticon Porto15 adapted from Ryan & Redfern, HTRA, ASSL, 351, 229 ELT stochastic limits
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Opticon Porto16 Pulsars - limit for HTRA - faint and fast
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Opticon Porto17 * CTA 1 pulsar - Fermi Abdo et al, 2008, science.1165572
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Opticon Porto18 New radio quiet pulsars from Fermi results will need ELT follow-up
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Opticon Porto19 Future plans under FP7 Continuation of the network building upon our work under FP6 .... with the aim of formulating a comprehensive scientific overview of HTRA into the extremely large telescopes [ELT] era...... first network meeting mid-February 2009, Padova also looking other funding EU - Marie Curie and COST ERC funding industrial
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