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2nd Annual Report OPTICON Optical Infrared Co-ordination ...

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WP2: Network for UV Astronomy (NUVA)<br />

The objectives for the Network for UltraViolet Astronomy are:<br />

- Formulate and operate a UV astronomy Network<br />

- Plan and execute a road mapping activity<br />

- Carry out exploratory analysis to define scientific requirements for the future and critical<br />

assessment of the publicly available information in various archives.<br />

WP1: An instrumentation meeting was held in Madrid, 17-18 November, to discuss/summarize<br />

the characteristics of the instrumentation required from the science case articles. Two aspects<br />

were analyzed in detail:<br />

1. The target spectral features. This is required to tune the instruments sensitivity to them and<br />

guarantee the optimal detection conditions for them. Also a first set of target lines for narrow<br />

band imaging were identified.<br />

2. Time resolution - requirements to track flares and outburst.<br />

The major conclusion is that the most needed UV capability is high resolution spectroscopy<br />

(Δ/Δ λ = 50,000) in the 950-3200 Angstrom range.<br />

The article summarizing the results of the meeting is being prepared under the co<strong>ordination</strong> of<br />

Norbert Kappelmann (IAAT, Tuebingen) and will be included in the White book of UV<br />

astronomy. Attendees: Norbert Kappelmann, Martin Bartsow, Isabella Pagano, Noah Brosch,<br />

Francisco Najarro, Rosa Gonzalez and Ana I Gomez de Castro<br />

WP2: The UV science case book is, in press. The book will be entitled: “Fundamental problems<br />

in astrophysics: Guideline for future UV observatories” and be published by Astrophysics &<br />

Space Science/Kluwer-Springer (Vol 302). This book represents the draft of the “White book”<br />

for UV astronomy.<br />

WP3 D2: NUVA web site has been established (www.ucm.es/info/nuva) . The web is handled by<br />

a contents manager so it works as an instrument for publication/interaction among the disperse<br />

UV community.<br />

WP3: High Time Resolution Astrophysics (HTRA)<br />

No expenses have been reported in 2005, since most of the communication related to WP3 has<br />

taken place by e-mail and direct contacts in conjunction with activities in JRA3.<br />

The HTRA working group met at NUI Galway in October 2005. The plans for the HTRA<br />

network activities were presented at this meeting. The main activity was a discussion for the<br />

preparation of a 'white book' on HTRA in June 2006. This has provisionally been titled<br />

'Astrophysics in the 4th dimension', with a proposed selection of about 20 reviews, prepared<br />

in the course of a meeting of invited experts. Different subject and topic headings were<br />

discussed at the meeting, along with suggestions for invited speakers.<br />

WP4: Astrophysical Virtual Observatory (AVO)<br />

This was the final year of the Astrophysical Virtual Observatory (AVO) project. The third and<br />

last AVO demonstration was held on January 25 - 26, 2005, at the European Space<br />

Astronomy Centre (ESAC; previously known as VILSPA), near Madrid, concurrent with a<br />

22 <strong>Co</strong>ntract [RII3-CT-2004-001566]<br />

<strong>Annual</strong> <strong>Report</strong>

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