ࡱ> jlghi5@݁bjbj22 ?:XXdyx       2 824f2 GNCFEFEFEFCF(JM$/PRRM xxxM  N|||x  CF|xCF|| .F   @ q5= r18?BN0GN 9 S|S@2 2     @S @LN߉\|;YMM2 2 FR$/f2 2 R Annual Report 1/12/2002 30/11/2003 for Research Infrastructure RTD Project ASTRO-WISE HPRI-CT-2001-50029 Groningen, 31 Januari 2004 NOVA/ OmegaCEN Kapteyn Instituut Rijksuniversiteit Groningen This document can be found on the INTERNET at the following address: http://www.astro-wise.org/doc_nova2.html The Annual Report covers the second year of the project. IHP-ARI RESEARCH INFRASTRUCTURE RTD PROJECT Annual Report 1/12/2002 30/11/2003 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 - ESOProf. A. RenziniLSF-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 second year the project plan as outlined in the contract has been continued. Following the plan for Phase II of the project, a prototype of the AstroWise system has been implemented. An evaluation took place of the proto-type underlying pipeline, as delivered by WP1. At an AstroWise workshop in November at Groningen this prototype was reviewed and a set of modification of class definitions was settled. Hardware for WP3 (disk storage) and WP4 (computers) have been implemented at various nodes. The central database systems have been put into operation (WP3) and a new preliminary version of the visualization tool has been delivered (WP2). 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 second year of the project. The programme entered Phase II: evaluate and prepare for mass production, highlights include: A prototype image pipeline (WP1), written in the Astro-Wise paradigm, was implemented and disseminated over partners, using the Astro-Wise dissemination concepts A proof of concept of the innovative AstroWise system, integrating parallel computes, off-sided- Terabyte disk storage, pipeline processing in an archival environment was achieved in April 2003. The NOVA/OmegaCEN group celebrated FIRST VIRTUAL LIGHT, a major achievement and milestone of the project The AstroWise Architectural Design document describing the Astro-Wise system in detail was approved and released, in July 2003. The organization of the project, as outlined in the contract, was maintained: Two PI meeting were held, one in July 2003 in Leiden, one on 19 November 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 telecons between local contacts were continued The Architectural design has been completed. The design document details for each of the work packages (1-5) 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) ADD Version 1.0 will form the basis for the actual implementations, and constitutes the blueprint of the project. Further highlights during the reporting period include: The main design of ASTRO-WISE system has been presented at the JENAM (Joint European-National Astronomy) conference in Budapest in August 2003. A workshop on photometric pipelines organized by ASTRO-WISE was attended by 15 persons of the consortium (Groningen 17-21 November 2003) The AstroWise project was presented at a meeting of the EU RTN SISCO project (5 September 2003 in Napoli). an overview of the technical progress made (on a task by task basis) and of the main results, highlighting any innovations 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 next to the design work: WP1: A prototype Image pipeline has been further developed and reviewed, capable to convert 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. The proto-type demonstrated the feasibility of this key-idea. See also WP3. Proof of concept was celebrated in April 2003. WP1: Various meetings and work visits (OAC- Napoli May 7-9) on Quality control were held (Munich Jan 23-24) WP1 OAC Detailed review of the calibration pipeline (pre-reduction phase): all the recipes concerning master BIAS, dome and twilight Flat Field, master Flat Field and Fringing Pattern creation have been tested and improved. In particular, for what concerns the fringing, a new method to calculate the scaling factor was added. WP1 OAC: Implementation and integration on the pipeline of Quality Control tools for the calibration pipeline. The following tools have been submitted: SignTest (BIAS frames), QC DomeFlat, QC TwilightFlat and QC Outlayers. WP1: The USM has done extensive testing of each step in the reduction pipeline using ESO wide-field imager (WFI) and CTIO big-throughput camera (BTC) data sets. A local data-base was implemented, populated and integrated this with the Astro-wise pipeline operation. A software routine was written to remove cosmic-ray features from imaging data. A wrapper script was written in python to integrate this programme to the Astro-Wise pipeline environment. The advantage of this program over other existing cosmic-ray programs is that it works in crowded stellar fields, and when the image point spread function is under-sampled. WP1: Terapix developed a quality control suite for their wide field imaging pipeline: QFITS. It was provided to AstroWise to review whether it could be of use for the AstroWise system. WP1: Terapix developed improvement on the interpolation scheme of SWARP (image resampling-combination programme) and increased its speed by a factor 3-4. An important gain since this is the most time consuming step in the image pipeline. WP2: Further development has been done in NOVA/OmegaCEN with fast computer algorithms to associate on the basis of positional coordinates two very large tables, with at least 100.000 entries (associate tool). Progress is good, but this took much more time than anticipated. Own build solutions had to be made as both industrial solutions and that of the US Sloan digital sky survey were not satisfactory. A prototype of the new visualisation tool has been delivered. It was not using OpenGL yet and this will be made in the beginning of the third year. WP2: USM have begun 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. All of the core Fortran programs for the SED fitting package have been completed. WP2: Terapix delivered a preliminary version of the visualization tool Panorapix. WP3: A meeting/workshop was organized in May 2003 at NOVA/OmegaCEN to share knowledge with local data base administrators on operating Oracle/db. The meeting was attended by NOVA/OmegaCEN, USM and OAC, WP3: The federated database operated by 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 implemented at NOVA/OmegaCEN and successfully attached to the pipeline and storage environment. To this end a new fileserver was developed as well as a Python interface to Oracle-db. 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: OAC: Released an updated version of the ASTRO-BENCH software (more details at http://www.na.astro.it/beowulf/). ASTRO-BENCH has been used on many different hardware systems. Benchmark results can be seen on the web site:http://www.astro-wise.org/astro-bench_result.htm WP4 - 5 OAC: A new powerful Beowulf system has been delivered to OAC in November 2003. The new system consists of 17 nodes Opteron based (16 slaves + 1 master) with gigabit connection. Each node is equipped with 2 CPUs Opteron 244, and 2 GB RAM (6 GB for the master). More details at http://www.na.astro.it/beowulf/. Preliminary results show that for WFI images processed on half cluster (eight nodes) the processing speed is 3.7 Mpixel/s. WP4 - 5 USM: The USM will act as the data center for all of the German partners in the OmegaCam/Astro-wise consortium. For this purpose USM purchased, implemented, and optimized a 16 CPU (8 nodes) Beowulf PC cluster with 6GB of RAM per node, a 1.3 GB/sec Myrinet optical fibre connection, and 2 TB of raid level 5 storage. In order to allow current and future users of the Astro-wise pipeline to independently reduce their OmegaCam data, we also purchased and integrated four PC workstations, each having a raid level 5 storage capacity of 815 GB. WP4 - 5: NOVA/OmegaCEN: A fileserver, hosting Astro-Wises central CVS repositories, Oracle Enterprise manager and servers with 5 Tbyte of disk space were installed. Both servers are equipped with 12 200 GB IDE disks (parallel ATA for the first server, serial ATA for the second) and a 3ware RAID controller and are connected via a 24-port GB ethernet switch, which was also bought, to the parallel cluster of the University computing centre. WP4-5: Terapix: Several data storage configurations have been installed and tested. We have been impressed by the reliability of disks that were installed on the Terapix network: only two over 100 crashed in one year. Terapix chose to store data on each computing node, rather than to use a central data server, minimizing access time. For reliability and speed access, Terapix (as well as other partners) are using hardware RAID5, with 3ware cards. File system : XFS, most efficient for very large (>1GB) files (compared to ext3, Reiserfs, JFS) XFS is developed by SGI, and is a patch on the Linux kernel. Its stability being now demonstrated, it is included in the vanilla 2.6 version of the kernel. The following nodes are connected to a gigabit switch, and are all accessible from any node on the cluster via NFS cross-mounting. OS: Linux Mandrake CLIC - kernel 2.4.21-0.13mdkenterprise 1 3ware Escalade 7850: 8 disk 123GB Maxtor arrived January 2002 4 3ware Escalade 7850: 8 disk 100GB Western Digital arrived January 2002 4 3ware Escalade 7500-12: 12 disks 250GB Maxtor arrived March 2003 Performance of 3Ware Escalade 7500-12, 9x250GB disks (2TB effective) and XFS file system: Read: 112 MB/s Write: 57 MB/s Cf. http://terapix.iap.fr/cplt/oldSite/hard/cluster/raid_config.html for testing details. OS: Linux Mandrake 9.2 Opteron 2 3ware Escalade 8506-8: 16 disks 250GB Maxtor arrived July 2003. 2 Fiber Channel bay Brownie BR-1200 FC. 12 disks 250GB Maxtor arrived Oct 2003. Accessed via a Gigabit Fiber channel switch, and QLogic QLA 2100 or QLogic QLA 2200 Fiber channel cards on the PCI bus. Test: ICT-Vortex RAID card: much improvement in data writing (200MB/s), same as 3ware for reading. Total: 144 disks, 30.2 TB of disk, 25.5 TB of RAID5 data storage WP6: From January 23 to 24, 2003, the USM hosted and organized a consortium meeting, "Astro-Wise Quality Control and Graphical User Interface Workshop" in Munich. A primary goal of this meeting was to define the tests that are necessary at each stage of the Astro-Wise pipeline processing, in order to determine whether or not the quality of the data is adequate. Further goals included the first definitions of an attribute list associated with each object, and discussions of the interface between the user and the Astro-Wise pipeline. WP6: 2 PI meetings were organized and the regular 2 weekly telecons were held. WP6: The Astro-Wise consortium also started a collaboration with 2 satellite nodes, University of Bonn and the Universite de Liege. 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 Mile- Months Description of milestones, actions and deliverables Stone after kick-offPhase II: evaluate and prepare for mass production 7 15 milestone: WP2 Evaluation - given experience with operational WP1 8 21 milestone:WP1/WP3 1 year operations and population of database review deliverable: set of tools to users and populated calibration database deliverable: export Beta version to satellite sites 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 regime As can be deduced from the reports in the previous sections, which details the progress of the various work packages, the current status of the programme matches well the original outline of the schedule. Beta versions were delivered to partner and satellite institutes. The WP2 evaluation and the WP1/WP3 review was held at the workshop In NOVA/OmegaCEN Groningen in November. Action items following this review are listed on the Astro-Wise web pages. However, during the reporting period, it was announced that ESO will delay its commissioning of the VST telescope and its camera (OmegaCAM). Both do not form part of the present contract, but they do form part of the infrastructure to be supported by AstroWise. The later availability of observational data from this facility might cause a delay in the final qualification of the AstroWise deliverable. 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. NOVA/OmegaCEN plans to attach to the Astro-Wise system a new large Linux cluster of the University and to expand its disk storage capacity, USM will invest a further 120,000 Euro toward upgrading their Beowulf PC cluster. The intent is to increase the total storage capacity of this system to at least 10 TB, and to either add to the number of nodes within the existing cluster (an increase to 16 nodes with 32 CPU's), or to invest in a new 8 node system with new 64-bit CPU's. 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 also deliver the SED fitting and photometric redshift routine, fully integrated into the Astro-Wise pipeline. This will entail completing the Python scripts that call the Fortran programs of the SED fitting software. Terapix will deliver an OpenGL base version of their visualisation tool, following the specification in ADD WP2. OAC will continue their participation in pipeline Quality control and develop a tool for detecting variable sources (WP2). NOVA/OmegaCEN will further qualify and develop the pipelines and distributed archive system. 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 0.9- November 2003 CVS distributed project documentation CVS distributed source code Prototype image 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 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. The prototype reviews and first virtual light event have supported our views on the feasibility of the project and provide proof of concept. 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 (and subsistence provided): Workshop "OmegaCam's First Surveys", Astro-Wise support June 30 - July 2, 2003, at the Lorentz Center, Leiden University, The Netherlands. Attended by Silvotti, Valentijn PI meeting at Lorentz Center Leiden 2 July 2003 minuted at  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org Attended by Valentijn, Silvotti, Neeser, Saglia, Mellier Astro-Wise workshop Photometry at NOVA/OmegaCEN Groningen 17 -21 November minuted at www.astro-wise.org Particpants: Silvotti, Volpicelli, Paddu, Neeser, Gossl, Snigula, Valentijn, Neeser, Kuijken, Valentijn, Boxhoorn, Vermey, Tempelaar, Rengelink, Deul, Heraudeau, Helmich, Begeman, McCracken, Magnard PI meeting at Astro-Wise Photometry workshop NOVA/OmegaCEN Groningen 19 Nov 2003 minuted at  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org , Valentijn, Kuijken, Silvotti, Neeser, Mellier JENAM (Joint European National Astronomy Meeting) Budapest; AstroWise invited speaker- no subsistence/travel. Valentijn Universite de Liege- Lecture and AstroWise work visit coordinator Valentijn AstroWise Quality control meeting Munich Jan 23-24 minuted at astro-wise.org A. Grado, M. Pavlov, M. Neeser, L. Da Costa, R. Rengelink, R. Saglia Workvisit/ pipeline Quality control- Napoli May 7-9- minuted at astro-wise.org. Rengelink Amersfoort 21 March and 3 Feb coordination with Lofar project - Valentijn ADASS meeting Strassbourg 11 16 Oktober 2003- various AstroWise presentations and poster Malapert, Domisse, Magnard, Bertin Astro-Wise DBA meeting, Groningen, May 12-16. Participants J.Snigula, M. Pavlov, F. Getman, K. Begeman, D. Boxhoorn 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: 1 scientific programmer and 1 scientific programmer (0.4 manyear) Terapix: 1 scientific programmer NOVA: 1 scientific programmer + 0.5 junior programmer NOVA coord: 1 database administrator USM: 1 scientific programmer ESO: 2 scientific programmers (0.75 and 0.9 manyear) 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 2 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 2 /year 2 in year2 [month] [month] [hours]NOVA 41 74 52 16 9 28 220 60/12 160/47 2490 AC NOVA/co-or 12 12 24 24/12 0/4 1560 AC VISTA 22 22 6/0 16 /2 0 ESO 30 72 18 6 6 8 140 36/4 104/22 2895 FC OAC 33 34 18 7 14 12 118 30/7 88/27 2220 AC TERAPIX 10 28 27 14 79 48/12 31/8 2770 FF USM 20 24 3 7 6 8 68 18/9 50/8 1771 AC Total 134 232 130 36 35 104 671 222/56 449/118 13.706 The subcontractor VISTA attended all meetings and a two-day work visit to NOVA-OmegaCEN was arranged for december 2003. The details of the sub-contract with VISTA are not settled yet, which is related to the relatively important recent changes of the status of VISTA since the entrance of the UK in ESO. 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 first 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. 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-ph/0401403 Mass and Light in the Supercluster of galaxies : Ms0302+17 submitted to A and A, R.Gavazzi et al Research Infrastructure RTD Project  PAGE 14 Research Infrastructure RTD Project ASTRO-WISE HPRI-CT-2001-50029 ,-Ze& @ H I O W Z ̳̑rdYJ;JrhH%5CJOJQJmH sH h)5CJOJQJmH sH h)5CJOJQJh)CJOJQJmH sH h)@OJQJmH sH !h)5@CJ$OJQJmHsH!hP5@CJ$OJQJmHsH!hH%5@CJ$OJQJmH sH !h`5@CJ$OJQJmH sH h)hH%!h)5@CJ$OJQJmH sH $h)56@CJ$OJQJmH sH h)5@OJQJmH sH -.23WXYZex `07*$@&$ `07*$a$$ `07*$@&a$$ `0h*$a$$ `0h*$@&a$ `0h*$@&gddY,d܁xyz{$ `07*$a$ `07*$@&gdP `07*$@&gdH%$ `07*$@&a$% & O P Q R S T U V W X Y Z [ \ ] $ `0;*$@&^`;a$$ `0h*$a$$ `07*$a$$ 0\x]\^a$ $\]\^a$ $\]\^a$Z [ \ ] b g k }n[H[H9h)6@OJQJmH sH $hH%56@CJOJQJmH sH $h)56@CJOJQJmH sH h)5CJOJQJmH sH h)5@OJQJmH sH $hH%56@CJOJQJmH sH $h)56@CJOJQJmH sH h)5CJOJQJmH sH h)CJOJQJmH sH !h)5@CJ$OJQJmH sH h)@OJQJmH sH !h)5@CJOJQJmH sH ] ^ _ ` a b c d e f g $ `0;*$@&^`;a$ `077*$^7` 7*$ $ *$a$\]\$a$$a$   , ^ j ]MM$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT `0$*$If$ `0$*$Ifa$$ `0;*$^`;a$ , j   ( ) * I [ \ i ޳ʡiʡ[h)@OJQJmH sH -j%h)@CJOJQJUmH sH !h)5@CJOJQJmHsHh)@CJOJQJmHsH"h)0J"@CJOJQJmH sH -jh)@CJOJQJUmH sH 'jh)@CJOJQJUmH sH h)@CJOJQJmH sH !h)5@CJOJQJmH sH !j k ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd,$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT * ~q `0$*$If$ `0$*$Ifa$pkdX$$IfTl0m ;% 04 laT* + I [ ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT[ \ i ~q `0$*$If$ `0$*$Ifa$pkdc$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT ~q `0$*$If$ `0$*$Ifa$pkd$$IfTl0m ;% 04 laT   % < Q R v zezUUUUU$ `0$*$Ifa$$ `0;*$@&^`;a$$ `0;*$^`;a$pkd$$IfTl0m ;% 04 laT   P Q IJ+W`z|}~ദҦҦ~zjYF%h)5@CJOJQJ^JmH sH !h)5@CJOJQJmH sH h)@CJOJQJmH sH h)h)56CJ\]h)@CJOJQJmH sH h)OJQJmH sH h)@OJQJmH sH h)CJOJQJmH sH h)@CJOJQJmHsHh)@OJQJmH sH h)@CJOJQJmH sH h)5@OJQJmH sH v w UC$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT$ `0$*$Ifa$ 1 9 Skd^$$IfTl\V\\!%. t04 laT$ `0$*$Ifa$9 : > l cSSSS$ `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*+,-./cSSSS$ `0$*$Ifa$kd $$IfTl\V\\!%. t04 laT/01234cSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT456789cSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laT9:;<=>cSSSS$ `0$*$Ifa$kdV$$IfTl\V\\!%. t04 laT>?@ABCcSSSS$ `0$*$Ifa$kd"$$IfTl\V\\!%. t04 laTCDEFGHcSSSS$ `0$*$Ifa$kd$$IfTl\V\\!%. t04 laTHIJcR6 S? 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