ࡱ> 5@~bjbj22 ?XXux       2 LLL8.MM|2 :OpOOOOP#Q,OQ 7F$R? @ZPP@Z@Z  OODcDcDc@Z. O O Dc@Z DcDcdf V  O.O uܞLn]A0Dha2 2      LgQ6SDc1UDuVgQgQgQ2 2 @L"c"2 2 L Annual Report 1/12/2001 30/11/2002 for Research Infrastructure RTD Project ASTRO-WISE HPRI-CT-2001-50029 Groningen, 28 Januari 2003 Revised 26 Sept 2003 NOVA, Kapteyn Instituut, Rijksuniversiteit Groningen This document can be found on the INTERNET at the following address: http://www.astro-wise.org/doc_nova.html The Annual Report covers the entire project period performed so far. IHP-ARI RESEARCH INFRASTRUCTURE RTD PROJECT Annual Report 1/12/2001 30/11/2002 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 first year the project plan as outlined in the contract has been implemented: i.e. groups of persons associated to work packages are defined, meetings and communication schemes have been initiated. A conceptual design paper of the system has been produced, a preliminary proto-type pipeline has been disseminated over partners, a key-contract with Oracle has been placed and a training course for ASTRO-WISE staff has been organized. A new generation of computer clusters is installed at four sites . With the design and most, but not yet all, of the personnel in place the second year of the project can focus on implementation work, as planned. 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 first year of the project. The programme started with the activation of WP6 coordination: A pre-kick-off meeting was organized in November 2001 in Leiden, at which a first list of names of persons committed to the work packages was made. Local contact persons and WP leaders were identified The project web site  HYPERLINK "http://www.astro-wise.org" www.astro-wise.org was opened, listing the names of these persons, next to descriptions of the WPs, documentation pages, tutorials, agenda etc, etc. The project website is essentially for internal usage, though some outreach pages have been included. A formal inauguration with officials and Na tional press was held at the 13 March 2002 at the University Groningen, see  HYPERLINK "http://www.astro-wise.org/ceremony/Persbericht.html" http://www.astro-wise.org/ceremony/Persbericht.html (press-release, tv coverage etc). At the inauguration super-wide-field images were projected on the wall, by means of 6- real time parallel computers and 6 beamers, employing wide field imaging computing technology. The show was run by own staff and triggered publicity and created important spin-off. The project kick-off meeting was held on the 14th March in Groningen. Tasks and persons contributing to the Architectural design were identified. Two-weekly telecons between local contacts were initiated A first common system for documentation and computer code has been set up (CVS as a federated database - part of WP3) The work programme focussed on the Architectural design. The project has settled a second version of an overall Architectural design (ADD Architectural Design Document) of the Astro-Wise system - see Annex 1-(1). This 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) The ADD was composed by all partners and at a consortium meeting in Paris in May Draft version 0.1 was discussed. The basic set-up was agreed and the comments at and after the meeting led to the current Draft version 0.2. On the basis of this approval, an important contract with Oracle Inc has been placed. The Oracle database will provide the main workhorse for WP3, which in turn supports the implementation of WP1 and WP2. The contract encompasses the licenses for all ASTRO-WISE partners (as foreseen in the present EU-contract), but also identifies ASTRO-WISE as innovative and leading providing high discounts and free high level consultancy for at least the first two years of the contract. ADD Version 1.0, basis for the actual implementations, and the formal blueprint of our project is planned during the second year of the project. Further highlights during the reporting period include: The main design of ASTRO-WISE system has been presented at a conference in Garching on Toward an International Virtual Observatory see Annex 1- (2). The paper is now available. New EU funded personnel started at various partner sites. A training-course organized by ASTRO-WISE was attended by 30 persons related to the consortium 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 fulfilment of the design as worded in the ADD- see above. Here, we list progress next to the design level: WP1: A prototype Image pipeline has been made, capable to convert raw image data from the telescope into astrometrically and photometrically calibrated images. The prototype has been distributed over 3 partner sites (NOVA, USM and OAC). The prototype matches the requirements of the design and is innovative and unique in the sense of the integration of the operating software modules and the surrounding local database. 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. WP2: Experiments have been done with fast computer algorithms to associate on the basis of positional coordinates two very large tables, with at least 100.000 entries. (associate tool). Tests gave various un-satisfactory performance figures, which were reported back to industry. Local expertise has been accumulated and a new development path is considered. Implementation of visualization tools is started at 1/11/2002. WP3: The federated database for documents and source code, CVS, has been set up at the various partner institutes, providing the first basic computer network infrastructure. The database has been populated with first versions of prototype source code, documentation and also internet web site data. This system provides the first backbone for a common partner wide development network. Evaluations of the scalability of various databases into the Terabyte regime have been prepared for the design review in May 2002. We have assessed the suitability of Oracle9i for ASTRO-WISE. The scalability to Terabyte database size has been demonstrated by us. In addition, Oracle9i provides all the necessary object-oriented features needed to cleanly interface to the rest of the ASTRO-WISE system. Federating the database over Europe is currently not covered by Oracle9i directly, but its capability of Advanced Replication can be used in an upgrade path to the eventual ASTRO-WISE aimed federation. After the selection and the settling of the Oracle contract a first basic test implementation was prepared. This test implementation worked satisfactory with the image pipeline (see WP1) and subsequently further development work for the real implementation has been scooped. A detailed work plan for the second project year has been made. WP4 OAC: a Beowulf cluster is installed at the OAC and is fully operational since 17/02/2002. The cluster has eight slave nodes each dual processor PIII 1 GHz, 512 MB RAM 40 GB EIDE disk and two master nodes each with two processor PIII 1 GHz, 1 GB RAM, one RAID array with 350 GB HD. The masters are connected via Gigabit Ethernet to a network switch and the connection between the switch and the slave nodes is via Fast Ethernet. In order to define the best hardware/configuration solution for the ASTRO-WISE data centers, an astronomical application benchmark tool has been realized. The tool allows to measure the time needed to perform standard astronomical image processing application like image calibration production, source extraction, re-sampling and background subtraction. The tool is also able to profile the CPU, memory and network usage. In this way a better understanding of the cluster resources usage is available allowing a tuning of the system for the specific application. The tool will also be used to compare performance figures at the various partners sites. USM: as of January 2002, the USM has a fully operational Beowulf cluster. The rationale was to create a system with maximal inter-node data rates, high I/O, and large on-chip memory, in a very user-friendly set-up with a high level of hardware support from the manufacturer. As a result, USM has opted for a "turn-key" solution based on Compaq ProLiant rack-mounted PC cluster. The system's 8 nodes, each of which is composed of dual Pentium III 1.1 GHz processors with 6 GB of RAM, are interconnected via a 2 Gbit Myrinet switch with fibre ports. The rack and Myrinet switch will allow an expansion to 32 processors in the future. Storage is centrally distributed on the master node and comprises 12 x 72GB = 780 GB in a RAID5 configuration. The Beowulf controller will allow for a future expansion to a 10 TB total storage. Aside from the Beowulf cluster, we have also installed 4 individual PC workstations that will, eventually, be connected to the cluster to give the user a local storage and work area. Each PC has a RAID array with 815.5 GB at RAID level 3/5, allowing for a total of 4.26 TB of storage. The USM Beowulf PC cluster is running Slackware Linux 8.0 under an openMosix Linux kernel. OpenMosix is a Linux kernel extension for automatic active load balancing between the cluster nodes, and gives users and applications the illusion of one single computer with n CPUs. OpenMosix is perfectly scalable and adaptive and may be used to connect the workstation PC's to the central Beowulf to create a 12 node cluster. Terapixs new cluster of PCs arrived at IAP on January 24, 2002. The cluster is made of 5 nodes linked through Gigabit Ethernet. Each node is a bi-processor machine with 2 AMD MP1800+ processors, 2GB of DDR memory and 700GB of RAID5 storage space ("scratch" disk). RAID5 management is handled in hardware by 3Ware 7850 PCI cards. The whole thing is running Mandrake Linux 8.2 (which has built-in support for the XFS filesystem we are using for our data storage). Extensive tests have shown that data can be moved from one node to another at about 60MB/s sustained. Home-made benchmarks have shown this system to be far more competitive than many more expensive solutions. The machines started production in June 2002 for CFH12k and WIFI data. In December 2002 TERAPIX shall receive 2 more RAID5 arrays (Fibre-channel interface), providing an extra 5.2 TB of storage space for our cluster. NOVA: A fileserver, hosting ASTRO-WISEs central CVS repositories, Oracle Enterprise manager and server and 0.6 Tbyte of disk space was installed. Plans for an extensive dozens of Tbyte RAID disk system were made. WP5: A comparison in terms of performance and costs of several storage systems has been performed. SCSI, FC, EIDE RAID external and internal solutions have been tested. A clear result is that the EIDE disks with 3ware controller on PCI bus (internal solution) gives by far the best performance. Partner sites plan installations in the second year. WP6: Under highlights, section 2.1.2, the several WP6 coordination activities have been listed. Beyond these, we mention our quarterly meetings, minutes and Action items as listed on our web site. 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 T0 kick-off WP6 OK Nov01 T0 kick-off- prepare design review for all WP1,2,3,4 and 5 OK NOV01/Mar02 T0 + 1Q design review WP1, 2 and 3; procurement WP4 and 5 OK Paris May02 T0 + 2Q import pipeline OK Fall 02 T0 + 2Q procure WP4,WP5 start sub-component installation OK summer 02 T0 + 3Q WP1 fully operational with first version of WP4 and 5 OK dec 02 deliverable: operational pipeline at partners centres (WP1) 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. At the right side of the table we have indicated in bold the completion dates of the various planned activities. However, the acquisition of new EU funded personnel was more difficult and took more time than anticipated. Particularly, it was difficult to find the persons with the proper profile with both a scientific R&D background and the specific knowledge of the IT we employ. Eventually, we decided to recruit relatively young and less experienced persons and train them ourselves. A very successful training course with 30 attendants was held at the Leiden University Lorentz center. The strategy with own trained young staff seems to work, but it will require extra time before the implementation phase II is at full swing. 2.4 Planned activities in the next period In spite of the relatively late recruitment of new personnel, the project still follows its original schedule as outline in Annex I of the contract. During the second year the project will start Phase II evaluate and prepare for mass productions, which means a thorough evaluation of the prototypes as developed during the first year. In the second year it is planned to publish the first full version of the integrated Architectural and detailed design of the system. First versions of the database will be populated, using the newly developed tools. Test versions of this software will be exported to partner sites and the collaborative federation is expected to take shape. Partner sites will be able to address and contribute to the 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 during the reporting period: Architectural Design Document version 0.2. CVS distributed project documentation CVS distributed source code Prototype image pipeline Hardware, parallel computers installs at OAC, USM and Terapix Hardware, central fileserver and database installed at NOVA ASTRO-WISE web site with internal reports on various WP evaluation 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 evaluations have supported our views on the feasibility of the project. A discordant note is the later availability of trained implementers, mentioned above, which will cause a shift in the schedule. 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 see cost statements): Wpall: AstroWise pre-Kick-off meeting meeting at Leiden (Amsterdam)- 21/11/2001 WP3: CERN Geneva-S CERN database workshop, expert exchange on very large databases such as employed by AstroWise 28/1 30/1 2002 WP6: Inauguration +Kick-off meeting at Kapteyn 12 /13 March 2002 Groningen-NL WP6: AstroWise PI meeting at Terapix- Conceptual Design Review AstroWise17 May 2002, Paris F WP3: SPIE conference Presentation on AstroWise Db concepts 22-31 August 2002 Hawaii- US WP1, WP3: Oort Workshop Leiden exchange with US leading wide field imaging project/ Sloan Digital Sky SurveyNL 16/6 18/6 WP3-WP6-coordination with AVO: Conference Virtual Observatories of the future, Garching bei Munchen-D 9/6 12/6 2002 WP3: Oracle headquarters 8 May brainstorm including ASTRO-GRID/contract negotiations- Reading Uk WP3: Workvisit Napoli-I 4-10 May 2002 WP all: Lorentz center Leiden AstroWise training course attended by 35 persons, mostly funded by AstroWise- Leiden NL 28/10 1/11 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 close agreement to what was outlined in the contract, but clearly the work which involved the new personnel was delayed because of the later arrival of these people. Now, with new staff available at all the sites we expect the project to run well in the coming year. The acquisition of new personnel took more time than planned, essentially due to lack of qualified candidates. Consequently, we have organized a training programme to educate young persons for the new positions. This has been a success - an intensive one-week course was organized in October in Leiden. Newly recruited ASTRO-WISE funded personnel started at: OAC: 1 Januari 2003 1 scientific programmer Terapix: 1 November 2002 1 scientific programmer NOVA: 1 October 2002: 1 scientific programmer + 0.5 junior programmer USM: 1 May 2002: 1 scientific programmer ESO: 1 November 2001 1 scientific programmer; 1 May 2002 1 scientific programmer 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 1 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 1 /year 1 /year1 [month] [month] [hours]NOVA 41 74 52 16 9 28 220 60/3 160/41 496 AC NOVA/co-or 12 12 24 24/0 0/0 0 VISTA 22 22 6/0 16 /2 0 ESO 30 72 18 6 6 8 140 36/2.5 104/18 2891 FC OAC 33 34 18 7 14 12 118 30/0 88/17 0 AC TERAPIX 10 28 27 14 79 48/9 31/1 1230 FF USM 20 24 3 7 6 8 68 18/5 50/6 988 AC Total 134 232 130 36 35 104 671 222/19.5 449/85 5605 One partner, ESO, is delayed with defining and starting up their contribution. A review on their possible contribution was held summer 2002 and the outcome will be incorporated in the management plan for the second year. The subcontractor VISTA attended all meetings. 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. The later start of new personnel creates a surplus, which we plan to spend at a later date. Cost-Statement form E3 lists the transferred sums from Coordinator to partners. These sums match to Table Advance of the Contract, after correction for the pre-payment made by the coordinator of the Oracle licenses, which are budgeted as Other specific costs for each partner (except ESO). 6. SUPPLEMENTARY INFORMATION Annex 1 List of Publications/Patents (1) ASTRO-WISE: Architectural Design Review Version 0.2 Internal Report 64 pages (2)ASTRO-WISE : An Astronomical Wide field imaging System for Europe -see  HYPERLINK "http://www.astro-wise.org./doc_nova.html" www.astro-wise.org./doc_nova.html E.A. Valentijn and K.H Kuijken . Invited paper to appear in the Conference Proceedings of the conference: Towards an International Virtual Observatory ESA/ESO/NASA/NSF June 2002 Garching bei Munchen (3) Simple query comparison between a relational database and an object-oriented database, Proceedings of SPIE conference Hawaii, 2002, P. Didelon and B. 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