ࡱ> QSNOP5@Lbjbj22 ?&XXTxD D D N Z Z Z n SSS8*TTn /- VjWWWW[X[X[XA(Dl$D,$;/R1,Z c[X[Xcc,Z Z WW,qqqcxZ WZ Wqcqtqr&  Z Z mWV 0_0 Sj],0/-A,)2o)2mn n Z Z Z Z )2Z m\[XU[ qu])_][X[X[X,,n n GSp(n n S Annual Report 1/12/2003 30/11/2004 for Research Infrastructure RTD Project ASTRO-WISE HPRI-CT-2001-50029 Groningen, 1 Februari 2005 NOVA/ OmegaCEN Kapteyn Instituut Rijksuniversiteit Groningen This document can be found on the INTERNET at the following address: http://www.astro-wise.org/Public/annual-2004.doc The Annual Report covers the third year of the project. IHP-ARI RESEARCH INFRASTRUCTURE RTD PROJECT Annual Report 1/12/2003 30/11/2004 Contract N HPRI-CT-2001-50029Project TitleAstronomical Wide-Field imaging system for Europe ASTRO-WISEStart date of contract1/12/2001End date of contract1/12/2005Contract value (EURO)1.500.000 EuroInternet homepage HYPERLINK "http://www.astro-wise.org" http://www.astro-wise.orgContract Manager/Co-ordinatorDr E.A. ValentijnTelephone N+31-50-3634011 +31-6-48276416 mobileFax N+31 50-3636100E-Mail address HYPERLINK "mailto:valentyn@astro.rug.nl" valentyn@astro.rug.nl Partnership Summary Participant number (Co-ordinating partner as participant N1) Name of Participating Organisation  Name of Responsible PersonRole in Project*001Nederlandse Onderzoekschool voor Astronomie NOVADr E. A. Valentijn LSF-IHP002European Southern Observatory - ESODr P. QuinnLSF-IHP003Osservatorio Astronomico di Capodimonte OACProf. M. CapaccioliLSF-IHP004Centre National de la Recherche Scientifique- TERAPIXDr Y. MellierLSF-IHP005Ludwig-Maximilians-Universitat - USMProf. R. BenderLSF-IHP * LSF-IHP: a research infrastructure funded for access under the IHP programme LSF-TMR: a research infrastructure funded for access under the TMR programme LSF-OTH: a research infrastructure outside the IHP or TMR programmes IND: an industrial or commercial enterprise OTHER: other types of participant 1. EXECUTIVE SUMMARY This summary should be as comprehensive and clear as possible. It should contain, in about 200 words a description: of the main objectives and characteristics of the RTD project, emphasising its innovative aspects and its potential impact on the quality and quantity of access provided by Europes research infrastructures, and of the work performed and achievements. ---------------------------------------------------------------------------------------------------------------------- Objectives The ASTRO-WISE programme co-ordinates the development work to deal with and access astronomical wide field imaging data. It provides an operational environment for researchers to analyse and access the huge data volumes of observational data produced by a new generation of Europes wide field imaging telescopes. The programme pools the expertise of a number of European groups with experience or commitment to optical wide-field survey work. All partner sites will function as (linked) national data centres. The code and expertise to run additional satellite centres is a deliverable of the project. ASTRO-WISE develops and disseminates in the community software tools needed to access the wide-field image data, to perform individual research programmes. The huge data volumes require an innovative dynamical approach, in which results can be re-derived, customized to the users specific needs. To this end, the various calibration data and other input files are distributed over a network, which connects the data centres. The geographical distribution of the key information (both methods and data) is provided by the system, allowing the various National Data centres to work cooperatively in an efficient manner and optimally profit from the work done at each of the centres. This enhancement, consolidation and dissemination through National data centres, is going to build up the Astronomical Wide-field Imaging System for Europe. Results In this third year the project plan as outlined in the contract has been continued. Following the plan for Phase II of the project, the prototype of the AstroWise system has been evaluated and prepared for mass production. Following the recommendations set at the AstroWise workshop at the end of the previous year (November 2003) the prototype has been further developed and made ready for mass production. To test this, 10 Terabyte of data of a smaller imaging camera ( HYPERLINK "mailto:WFI@2.2m" WFI@2.2m) has been ingested into the system. This in itself, was a first test of ingestion of large amounts of raw data. With these test data the system has been further qualified and optimized. At the very end of the reporting period an AstroWise workshop was held at which the work plan for the remaining part of the work was defined. The consortium had to face the late delivery of one of the most important infrastructure facilities the project is supporting: ESOs VLT-Survey Telescope and OmegaCAM. Details of the work packages have been specified for the remaining development work of the project: i) the introduction of context/privelages, ii) the design for distributed processing , iii) distributed archiving and iv) Quality control. Hardware for WP5 (disk storage) and WP4 (computers) have been upgraded at various nodes. The central database systems have been upgraded (WP3), migrated to Oracle 10g and the fileserver has been updated. Project Manager contact information- Valentijn see previous page 2. Comparison with the Project Programme Scientific and Technical Performance This section should be an overview covering all the aspects of the work undertaken by the partners to date. 2.1 Summary of the specific project objectives The programme will establish a number of data centres where the voluminous wide-field imaging data can be processed to the specifications of the user, who can select on the basis of atmospheric conditions, quality of calibration data, etc which data to process and how. The linking of the data centres means that the user will always have access to the most up-to-date data. highlights, if any, of important research results from the project (please, attach abstract of corresponding publication to Annex 1); 2.2.1 Highlights The official starting date of the project is 1/12/2001; so this report describes the third year of the project. The programme executed last part of Phase II: evaluate and prepare for mass production, highlights include: The system was stress tested on a very large dataset of 10 Terabyte of Wide field imaging data ( HYPERLINK "mailto:WFI@2.2m" WFI@2.2m telescope) which was: ingested software-wise into the AstroWise database system (archive WP3), was physically stored on AstroWise hardware (provided by WP4), was partly processed on a parallel cluster (provided by WP5) by pipeline software delivered by WP1, was viewed by users by AstroWise provided user interfaces (WP2) connected to the database The prototype image pipeline (WP1), written in the Astro-Wise paradigm, was extensively tested and improved using these test data and also that of other wide filed imaging instruments (La Palma WFC, MDM). Quality control tools have been added to the system (WP1- WP2) A first extensive draft version of the AstroWise Manual describing operations and user manual the Astro-Wise system was prepared and is available on www.astro-wise.org. The organization of the project, as outlined in the contract, was maintained: A PI meeting was held, on 2 Dec 2004 in Groningen (minutes are listed on www.astro-wise.org). The project web site  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org was maintained listing descriptions of the WPs, documentation pages, tutorials, agenda, minutes etc, etc. The project website is essentially for internal usage, though some outreach pages have been included. A project news group has been implemented  HYPERLINK "mailto:news@astro-wise.org" news@astro-wise.org and is frequently used by all partners. Two-weekly teleconferences between local contacts were continued work packages (1-5) describe the contents of the project: WP1: design, data model and development rules for the data reduction pipeline to be build. WP2: Description of visualization tools and particularly in the case of the new to be developed visualization tool detailed design specifications are included. Description of database access tools. WP3: Design of Federated Database to distribute administrative and calibration data as well as documentation and software over the participating sites in support of WP1 and WP2. In addition the database will deliver or point to data items such as raw and processed image data and will contain source lists. WP3 provides the glue for the whole project. WP4-5 Lists the hardware currently operated or expected in the future by the partners. Pooling expertise for the setting up of the edge of technology hardware configurations (parallel processors WP4 and dozens of Terabyte disk storage - WP5). The Architectural Design Document (ADD) Version 1.0 forms the basis for the actual implementations, and constitutes the blueprint of the project. The implementation of the system proceeded in the third year according the specifications in the ADD. Further highlights during the reporting period include: A web service to view the AstroWise system content has been implemented A workshop Running Surveys in the AstroWise system organized by ASTRO-WISE was attended by 15 persons of the consortium (Groningen 29 November 2004- 3 December 2004) Meetings of complementary programmes were attended (SISCO, AVO Science Working group) for coordination (WP6) an overview of the technical progress made (on a task by task basis) and of the main results, highlighting any 2.2.2 Technical Progress on a task by task basis The main progress for each of the tasks WP1-5 is the implementation of the design as worded in the ADD. Here, we list progress on the implementation and qualification of the system. WP1: A prototype Image pipeline has been stress tested with large amounts of data. The pipeline converts raw image data from the telescope into astrometrically and photometrically calibrated images. The database keeps track of all operations done to the data and eventually facilitates on-the-fly- re-processing of the data, user customized. NOVA/OmegaCEN extensively tested and upgraded the prototype pipelines in on operational environment using test data from the  HYPERLINK "mailto:WFI@2.2m" WFI@2.2m instrument. WP1 OAC: Installation, testing and maintenance of the Astro-Wise pipeline on the new 17 nodes Opteron based Beowulf system. WP1 OAC: Validation of the AW pipeline: a detailed test was done using the WFI data of the OAC Deep Field in order to compare the astrometric and photometric results of the AW pipeline with those obtained with other software (IRAF MSCRED, EIS pipeline, ASTROMETRIX). The results of this test were shown in a AW internal report. WP1 OAC: Quality Control tools for the calibration pipeline has been implemented. These tools were implemented in the "compare" and "verify" methods and are based on the subwindstat class. The implementation is done for BiasFrame, DomeFlatFrame, TwilightFlatFrame and MasterFlat. WP1 OAC: FITSIO compression: some tests with different algorithms (gzip, plio, rice)were done in order to compare the efficiency (lossless data, compression factor). WP1 Terapix: A new version of QualityFITS (Qfits V.1.11) has been released and used on 9000 Megacam input images and on 500 Megacam output (stacked) images. It ran automatically on these images during three full weeks and failed only once due to a bug in Qfits. The bug is now fixed. The Qfits V.1.11 contain new items: automated PSF anisotropy mapping, automated completeness limit calculation. WP1 Terapix: New version of SWARP Weightwatcher have been released that computes more accurately the weighted pixel value and the frontiers of each CCDs. It then handles a better way lower noise areas. Both SWARP and Weightwatcher have been modified to follow more carefully FITS keyword conventions: tests on 10000 Megacam images showed some failures in FITSVERY due to non-standard expressions of Exp. values. All exponent then write with E instead of e (e.g. E+6 instead of e+6). Both SWARP and Weightwatcher have then been publicly released .All software (WSARP+Weightwatcher) have been modify in order to run on 64-bits processors. WP1 Terapix: Terapix developed a new automated software that handles both astrometric and photometric field to field rescaling and calibration. Scamp provides a global astrometric solution based on a complete matrix inversion, instead of an iterative process, as in Astrometrix. The gain is fantastic: the complete astrometric and photometric solutions are provided 100 times much faster than Astrometrix. The drawback is the matrix inversion that demands to handle memory with great care. Terapix spend a huge amount of resources in developing and testing this software. This is a major achievement done mainly by E. Bertin during the past 2 years. It was tested during 8 months on several types of images and in particular on more than 10,000 Megacam images. Scamp public release with complete documentation is expected by Feb. 15, 2005. WP1: The USM maintained the distributed version of the pipeline, running a number of tests using in-house WFI data. A further goal/result was to acquaint future users with the AW system.. WP1: ESO-EIS prepared and delivered dataproducts from the  HYPERLINK "mailto:WFI@2.2m" WFI@2.2m using the MVM library software. WP2: The development at NOVA/OmegaCEN of fast computer algorithms to associate on the basis of positional coordinates two very large tables, with at least 100.000 entries (associate tool) leaded to a first full implementation. Own build solutions were developed as both industrial solutions and that of the US Sloan digital sky survey were not satisfactory. This is a cutting edge ICT development. Contact with other University ICT groups (e.g Amsterdam CWI ) was arranged in several brainstorm meetings. WP2: USM has completed the Pythonization of the spectral energy distribution (SED) fitting and photometric redshift routines. This included defining class definitions for objects unique to the photometric redshift input and output, as well as creating prototype interfaces for input source lists, filter response curves, SED lists, and output photometric redshift plots. An extensive simulation of the effects of photometric errors, the use of differing combinations of OmegaCAM filters, and variations in survey depths, on the accuracy of photometric redshifts have been done using real and artificial data. This resulted in a fine-tuning of the algorithms. A function that matches a master source catalogue to a series of other filter catalogues (the input for the photometric redshift routines) is still required from the SAssociate code. The integration of the USM photo-z routines into the AW pipeline is pending on this. WP2: Terapix delivered an upgraded but still preliminary version of the visualization tool Panorapix. A new work plan has been agreed at the PI meeting for the development of the tool in the coming period. WP2: NOVA/OmegaCEN made a full Viewer (Graphical User Interface) to view the contents of the database via the internet. This webservice will eventually become a deliverable of the project allowing users to access the database throughout Europe (and beyond) without requiring software licenses. WP2 OAC: Variability tool. Two available programs to search for photometrically variable objects both based on image subtraction with spatially varying kernel were imported, installed and tested on the same data set. The results obtained by the two software were very similar; it was decided to adopt DIA as it was better documented. A number of modifications were defined in order to improve the efficiency of the software (parallelization), add new functionalities (masking in input frames, use of WCS coordinates, selection of the objects to derive the kernel solution, automatic Fourier Transform analysis, phase diagrams) and integrate within the AstroWise environment. Most of these items were implemented and tested using different data sets (FORS1 images on a GC, WFI images on a spherical dwarf galaxy, WFI images on the OACDF "empty field"). WP3: The federated database for documents and source code, CVS, has been successfully used at the various partner institutes, providing the basic computer network infrastructure. The database has been populated with source code, documentation and also internet web site data. This system successfully provides the backbone for a common partner wide development network. WP3: The Oracle database server has been maintained and upgraded to version 10g at NOVA/OmegaCEN. The fileserver was maintained. WP3: Throughout the year, the USM acted as a "test-case" for a federated data-base with Groningen/OmegaCEN. This involved the experimental implementation of streaming technology that allows the sharing of data-base objects across the institutes in the Astro-Wise network. WP4-5: OAC: WP4 and WP5: A new Beowulf system (17 nodes Opteron based) is up and running. The aggregate storage capacity presently amounts to 2.1 TByte. A big effort was undertaken to solve interoperability problems between 3ware raid controller and TYAN motherboard. Release of an updated version of the ASTRO-BENCH software, which now also functions on clusters without limitations on the number of nodes. The new release is much lighter. More details on WP4 developments can be found at http://www.na.astro.it/beowulf. WP4 - 5 USM: The USM will act as the data center for all of the German partners in the OmegaCam/Astro-wise consortium. In particular, it has played a significant role in the joining and organization of the German satellite nodes Bonn and Heidelberg. The AW group at the USM submitted a BAR (Beratender Ausschuss fr EDV-Anlagen) proposal to the Max-Planck-Gesellschaft for a further 180 kEuros in order to purchase a new 16 + 4 node 64-bit AW cluster with 24 TB of storage. The proposal has been accepted and the cluster will be installed early in 2005. WP4 - 5: NOVA/OmegaCEN: Astro-Wises central CVS repositories, Oracle db and servers with ~10 Tbyte of disk space were maintained (Oracle upgrade to 10g). The AstroWise servers are connected via a 24-port GB ethernet switch to the parallel cluster of the University computing centre. The parallel cluster was frequently used to bench mark and qualify the AstroWise system. WP4-5: Terapix: Terapix decided to start a long testing process of 64-bits processors computing systems. We faced on many problems to optimize BIOS parameters in order to handle these processors in the Terapix 32-/64- bits heterogeneous Network and we did spend two months before getting a stable configuration. All informations regarding these stable configuration have been put on public web pages. WP6: 1 PI meeting was organized and the regular 2 weekly telecons were held. WP6: The Astro-Wise consortium continued its collaboration with the satellite node Sternwarte University of Bonn. A representative visited the Nov 2004 workshop. WP6: Meetings with EU-RTD AVO-Science working group, EU-EURO-VO and EU-RTN-SISCO were attended for coordination with the virtual observatory projects and the Survey design network. 2.3 Comparison The contract reads: The programme is split into three phases, each ending with a deliverable and milestone. Phase I is characterised by design reviews and creating class definitions as soon as possible to receive wide-field imaging data, in order to avoid possible later backwards compatibility problems. During Phase II the system will be developed to prepare for mass production, while during Phase III the system will be fully qualified, populated, and delivered. Phase I: be ready to receive first data without later re-definitions or re-shuffling Table 4.1 Milestones and deliverables - extract for PHASE II - III Mile- Months Description of milestones, actions and deliverables stone after kick-offPhase II: evaluate and prepare for mass production 9 27 action: upgrade of mass storage WP4- ready for bulk operations 10 30 milestone: system full mass production proof (i.e. 100 Tbyte data volume) deliverable: operational pipeline, tools, data, results in Tbyte regimePhase III: qualify, operate and populate the mass production system 11 33 milestone: review and set goals and schedule for final system 12 48 milestone: end of implementation/development work of the project deliverable: key objective of the project - a qualified survey system to be used for the derivation of survey and research results; including pipeline, software tools and databases.  Also during the third year the programme followed the plan as outlined in Annex II - see table above. However, during the reporting period it became very clear that ESO will delay its commissioning of the VST telescope and its camera (OmegaCAM) to the end of 2005. Since this is one of the most important infrastructures the AstroWise system will support this implies that the foreseen qualification, operation and mass production will have to be delayed to the period December 2005 November 2006. Accordingly the PIs decided to re-schedule the last part of Phase II and the Phase III in Programme that can be completed in November 2006, without requiring additional funding. The contract officer will be approached for approval for this changed implementation plan. Details of the workplan and packages are given in the minutes of the AstroWise Survey Workshop held in Nov 2004 in Groningen and are posted at the project website. 2.4 Planned activities in the next period Partners plan to contribute to the work programme as outlined in the project plan and undertake the necessary steps to prepare the Astro-Wise system for mass production. Partners will operate services (Beta versions) to be used by the local science communities qualifying and testing the system. Large data sets from wide field imaging instruments ( HYPERLINK "mailto:WFI@2.2m" WFI@2.2m, La Palma WFC, US-MDM) will be warehoused and provided to the users. Web services and end-user Graphical interfaced will be further developed. USM will continue to refine the cosmic-ray reduction routine in order to reduce the amount of time required to process an image. USM will test the SED fitting and photometric redshift routine, fully integrated into the Astro-Wise pipeline, using the recently installed associate tools. Terapix will catch up with the delay of the implementation of their visualisation tool, following the specification in ADD WP2. Terapix will build new software to achieve Point spread function homogenization, ie produce images with similar image quality characteristics while taken under different atmospheric conditions. OAC will continue the qualification of the in pipeline Quality control and finish the development of a tool for detecting variable sources (WP2). NOVA/OmegaCEN will further qualify and develop the pipelines and distributed archive system, will build new features in the system which allow to run and identify individual projects (context), will develop graphical user interfaces, finalise the Object Viewer. NOVA/OmegaCEN plans to design and install a distributed processing protocol that allows all kind of satellite sites to enter or link to the system for a wide variety of hardware configurations at the satellite sites. The minutes of the PI meeting 2 Dec 2004, posted at the web site provide details on the work plan of partners. Some work has been shifted to NOVA/OmegaCEN. 3 Deliverables This section should contain the list of contractual deliverables (reports, software codes, experimenta l results, prototype products, etc.) of any tasks completed to date and a comparison with Annex 1 to the contract. The following deliverables were achieved and maintained during the reporting period: Architectural Design Document version 1.0 July 2003 AstroWise Environment: User and developer manual- Draft 2.2- November 2004 (87 pages) CVS distributed project documentation CVS distributed source code Prototype image pipeline Prototype Calibration Pipeline Hardware, parallel computers installed at NOVA/OmegaCEN, OAC, USM and Terapix Hardware, central fileserver and database installed at NOVA/OmegaCEN ASTRO-WISE web site with internal reports on various WP evaluations Test benches for database scalability- WP3 Benchmarks Beowulf clusters WP4 Hard disk towers for Terabyte storage WP5 10 Tbyte of Wide field imaging data ingested into the AstroWise system . State whether the research objectives, as set down in Annex I to the contract, are still relevant and achievable. If not explain, why. Has the methodological approach changed from that described in the contract. If so, how? Any significant deviations from the planned schedule as described in Annex I to the contract should be clearly highlighted and discussed, stating the recommended actions to correct such deviations. The programme is implemented closely to what has been outlined in the Contract Annex I. 4.0 Exploitation and Dissemination of Results This section should describe all project aspects that are pertinent to exploitation and dissemination of results, such as: publications and conference presentations resulting from the project; patentable results, including a list of patents applied for; contacts with potential users and an indication of customer requirements. List in Annex 1 the most significant publications/conference presentations/patents. See Annex 1 and  HYPERLINK "http://www.astro-wise.org" http://www.astro-wise.org 5 Management and Coordination 5.0 Meetings Meetings attended by AstroWise Staff: AstroWise-VISTA coordination meeting 3-4 December Groningen (NL) (E.A.Valentijn, R.Rengelink, E.Deul, D. Boxhoorn, N. Hamby (UK) M.Irwin (UK- Cambridge), Bond and Sutorious(UK)) ((G)A)VO coordination meeting 6-7 May Groningen (NL) W.Voges (GAVO-PI), H-M Adorf (D), G.Lemson (D), G. Tissier (Terapix) E.A.Valentijn, D. Boxhoorn, K.Begeman, E.Helmich, M.Tempelaar, F. Getman (I), T. Linde (UK-Astrogrid), M.Neeser , Vermaas (Lofar), Holties (lofar), IAU Collogium 195 Outskirts in Galaxies, Torino 12-16 March 2004 (E.A. Valentijn, G. Sikkema) 7th Reunion des utilisateurs du CFHT Campbell River Canada, 11-27 May 2004 (Tissier) Note: prior approval for travel outside EU given (dd 4 March 2004) AVO-Science Working group meeting (Euro-VO) Strassbourg (F) 10 11 June 2004 (E.A. Valentijn) Osservatorio di Capodimonte Napoli (I), workvisit 21-23 June 2004 (E.A.Valentijn) 3d Potsdam Think Shop on Robotic Astronomy Potsdam (D) July 2004 (A.Grado) Summer School Data Analysis in Cosmology, Valencia, 6-10 Sept 2004- (T.S. Schneider) Astonomy and Databases 10 Sept 2004 OmegaCEN Groningen with CWI Amsterdam SISCO meeting and AstroWise workvisit 20-25 Sept 2004 Groningen, Ms A. Mercurio, E.A. Valentijn, K Kuijken AstroWise Workshop running Surveys at NOVA/OmegaCEN minuted at  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org , E.A.Valentijn, K.Kuijken, R.Silvotti, M.Neeser (D) , Y. Mellier, A. Volpicelli, R.Saglia, J.Snigula (D), O-M. Cordes, E.Deul, K. Begeman, D.Boxhoorn, W-J Vriend, E.Helmich, R.Vermeij, Ph. Heraudeau, M. Tempelaar, T.Schneider, G.Sikkema, F.Getman (I) and A. Volpicelli (I), Gossl (I) PI meeting 2 dec 2004 at OmegCEN/Groningen minuted at  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org , Valentijn, Kuijken, Silvotti, Neeser, Mellier 5.1 Coordination activities The contract reads: The PM team meets at least two times a year, and is in monthly contact with the local contacts. The project management organisation includes the following ingredients to support the communication between partners spread over different sites: - weekly teleconferencing on fixed days and times between local contact persons and other team members - two-monthly meetings reviewing work-packages progress and setting priorities for the next quarter - 6-monthly project review with PM team and external scientists There will be an extensive infrastructure channelling, procedurising and defining fixed formats (classes) of all digital information exchanged between partners. Most of this is handled by work-package 3, which also provides an important management tool. To sum up, the exchange of digital information is supported by the following infrastructure: - project internet web-site, with pages for all official documentation, manuals, arrangements, names of associated persons. pass word protected informal pages for intra consortium communications - federated database for text files, such as source code, manuals etc (eg. CVS) - federated database for all relevant wide-field imaging data, like calibration files We have been operating closely along the lines set out in the contract. 5.2 Tasks per partner Detailed up-to-date tables of persons actually working on the various work packages are posted on our webpages. Partners have contributed to the various workpackages in agreement to what was outlined in the contract. ESO spends less than originally planned. ASTRO-WISE funded personnel include: OAC: 2 scientific programmers Terapix: 1 scientific programmer NOVA: 1 scientific programmer + 1.0 junior programmer+ 0.7 junior qualification scientist USM: 0.2 scientific programmer ESO: 1 scientific programmers (0.25 manyear) and 1 scientist (FC model). The coordinator maintains detailed sheets (Excel) recording the actual spend human resources for each of the work packages for the various partners, both for EU funded staff and matching staff (eligible costs). Table 4.2 presents a copy of this Table from the Contract, in which we added in the last three columns, after the /, the totals of the actually spend human resources of each partner during the reporting period. Due to the three different cost models operated by the various partners any tabulated column has the potential to give a false impression. To avoid misunderstandings we have added in the last column the cost model employed by the particular partner. The last three columns of Table 4.2 are defined as follows: Two but last column: Number of man month funded by the project for the whole contract period, as copied from the Contract. After the / we have indicated how much approximately of these contract units have been spend by the partners during the contract period. One but last column: Number of manmonth contributing to the eligible costs (matching costs, having different definitions in the various costmodels) as copied from table 4.2 from the contract, with after the / the total amount of manmonth during the reporting period assigned by partners to the project, but for which no direct EU funding is given, but which are accounted in the Full cost models. Last column: In the last column we list the actual human resources funded by the project expressed in person hours. Note that in AC models these are the additional costs, while in the full cost models these are the total costs to be multiplied by the fractional EU contribution for deriving the actual EU funding. The last column is the only column which really matters in the actual financial transactions, while the previous two columns serve to trace the actual costs of the last column to the tables in the contract and partners agreement (Annex II 4.3). Table 4.2 Human resources by participant and work package with totals for year 3 Human resource breakdown (person-month) WP1 WP2 WP3 WP4 WP5 WP6 Total Funded Not funded Funded Proc tools db Beo sto coor by project by project by project . /year 3 /year 3 in year3 [month] [month] [hours]NOVA 41 74 52 16 9 28 220 60/19 160/49 4030 AC NOVA/co-or 12 12 24 24/0 0/4 0 AC VISTA 22 22 6/0 16/2 0 sub ESO 30 72 18 6 6 8 140 36/3 104/15 1924 FC OAC 33 34 18 7 14 12 118 30/11 88/22 3420 AC TERAPIX 10 28 27 14 79 48/12 31/8 2770 FF USM 20 24 3 7 6 8 68 18/1 50/12 320 AC Total 134 232 130 36 35 104 671 222/46 449/112 12.464 The subcontractor VISTA attended some meetings and a two-day work visit to NOVA-OmegaCEN was arranged for December 2003. The entrance of the UK into ESO involved an in-kind contribution of the VISTA telescope to ESO. Coordination with VISTA is maintained, some of the foreseen sub-contracting work was done by the NOVA. 5.3 Budget An integrated cost statement has been submitted in the Cost Statements in Form E2, which summarizes for each partner the costs for the various budget posts. The consumed money for the third year matches well to the budget, which can be seen directly by comparing the global numbers on form E2 with that of form A4 Yearly costs summary for the first year on the contract. Partners have saved some resources in order to be able to deal with the later delivery of VST/OmegaCAM by ESO. Cost-Statement form E3 lists the transferred sums from Coordinator to partners. 6. SUPPLEMENTARY INFORMATION Annex 1 List of Publications/Patents (1) ASTRO-WISE: Architectural Design Document Version 1.0 Internal Report 78 pages (2) ASTRO-WISE:Users and Programmers Manual 84 pages  Including AstroWise workshop plus PI meeting during the week 29-11-04 3-12-04 Research Infrastructure RTD Project  PAGE 12 Research Infrastructure RTD Project ASTRO-WISE HPRI-CT-2001-50029 ,-.[f|' A W X Ⱦ̳}l^SD5h95CJOJQJmH sH h!n-5CJOJQJmH sH h95CJOJQJh9CJOJQJmH sH  h|Dh9@OJQJmHsH!h95@CJ$OJQJmHsH!hr5@CJ$OJQJmHsH'h|Dh95@CJ$OJQJmHsHh|Dh9mHsHjh90JUh9!h95@CJ$OJQJmH sH $h956@CJ$OJQJmH sH h95@OJQJmH sH ./34XYZ[fyz `07*$@&$ `07*$a$$ `07*$@&a$$ `0h*$a$$ `0h*$@&a$ `0h*$@&ӍKz{|& ' $\]\^a$ $\]\^a$$ `07*$a$ `07*$@&$ `07*$@&a$' X Y Z [ \ ] ^ _ ` a b c d e f g h i $a$$a$$ `0;*$@&^`;a$$ `0h*$a$$ `07*$a$$ 0\x]\^a$X ` c d e f k p    4 r ³o`O?O?O?O?Oh9@CJOJQJmH sH !h95@CJOJQJmH sH h96@OJQJmH sH $h956@CJOJQJmH sH h95CJOJQJmH sH h95@OJQJmH sH $h956@CJOJQJmH sH h95CJOJQJmH sH h9CJOJQJmH sH !h95@CJOJQJmH sH !h95@CJ$OJQJmH sH h9@OJQJmH sH i j k l m n o p    $ `0;*$^`;a$$ `0;*$@&^`;a$ `077*$^7` 7*$ $ *$a$$a$\]\  % & 4 f r qaa$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT `0$*$If$ `0$*$Ifa$r s ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd,$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT 2 ~q `0$*$If$ `0$*$Ifa$pkdX$$IfTl0m ;% 04 laT    0 1 2 Q c d q        Y Z ۡۡۡiۡ[L[[h95@OJQJmH sH h9@OJQJmH sH -j%h9@CJOJQJUmH sH !h95@CJOJQJmHsHh9@CJOJQJmHsH!h95@CJOJQJmH sH "h90J"@CJOJQJmH sH -jh9@CJOJQJUmH sH h9@CJOJQJmH sH 'jh9@CJOJQJUmH sH 2 3 Q c ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laTc d q ~q `0$*$If$ `0$*$Ifa$pkdc$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT  ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT     - E Z [  zezUUUUU$ `0$*$Ifa$$ `0;*$@&^`;a$$ `0;*$^`;a$pkd$$IfTl0m ;% 04 laT  UC$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT$ `0$*$Ifa$  MN/[d~ 3;  ĶĶĪ}l]OOOheCJOJQJmH sH h95CJOJQJmH sH !h95@CJOJQJmH sH h9@CJOJQJmH sH h9h956CJh9@CJOJQJmH sH h9OJQJmH sH h9@OJQJmH sH h9@OJQJmH sH h9CJOJQJmH sH h9@CJOJQJmHsHh9@CJOJQJmH sH    ) 5 = Skd^$$IfTl\V\\!%. t04 laT$ `0$*$Ifa$= > B p cSSSS$ `0$*$Ifa$kd* $$IfTl\V\\!%. t04 laT cSSSS$ `0$*$Ifa$kd $$IfTl\V\\!%. t04 laT cSSSS$ `0$*$Ifa$kd $$IfTl\V\\!%. t04 laT !"#$cSSSS$ `0$*$Ifa$kd $$IfTl\V\\!%. t04 laT$%&'()cSSSS$ `0$*$Ifa$kdZ $$IfTl\V\\!%. t04 laT)*+,-.cSSSS$ `0$*$Ifa$kd& $$IfTl\V\\!%. t04 laT./0123cSSSS$ `0$*$Ifa$kd $$IfTl\V\\!%. t04 laT345678cSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT89:;<=cSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT=>?@ABcSSSS$ `0$*$Ifa$kdV$$IfTl\V\\!%. t04 laTBCDEFGcSSSS$ `0$*$Ifa$kd"$$IfTl\V\\!%. t04 laTGHIJKLcSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laTLMNcR6 S? 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