(r11) IvoaExecMeetingTM56 < IVOA

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---+ IVOA Executive Committee Meeting (TM56)

*TM56 - Dec 16, 2014 (Telecon)*

*WebEx Info:*
| <a target="_blank" href="https://sao.webex.com/sao/j.php?MTID=m577db04a0ac4c15aead2f80386075069"> *Join WebEx meeting* </a> ||
| Meeting number: | 732 077 996 |
| Meeting password: | ivoa |
| ||
| *Join by phone* ||
| *<a target="_blank" href="tel:1-877-668-4493">1-877-668-4493</a>* Call-in toll-free number (US/Canada) ||
| *<a target="_blank" href="tel:1-650-479-3208">1-650-479-3208</a>* Call-in toll number (US/Canada) ||
| Access code: 732 077 996 ||

*Contents*
   * [[IvoaExecMeetingTM56#IVOA_Executive_Committee_Meeting][IVOA Executive Committee Meeting (TM54)]] 
      * [[IvoaExecMeetingTM56#Logistics][Logistics]]
      * [[IvoaExecMeetingTM56#Agenda][Agenda]]
      * [[IvoaExecMeetingTM56#Reports_from_the_Projects][Reports from the Projects]] 
         * [[IvoaExecMeetingTM56#Argentina_NOVA][Argentina - NOVA]]
         * [[IvoaExecMeetingTM56#ArVO][ArVO]]
         * [[IvoaExecMeetingTM56#AstroGrid][AstroGrid]]
         * [[IvoaExecMeetingTM56#Australia_VO][Australia-VO]]
         * [[IvoaExecMeetingTM56#BRAVO][BRAVO]]
         * [[IvoaExecMeetingTM56#China_VO][China-VO]]
         * [[IvoaExecMeetingTM56#ChiVO][ChiVO]]
         * [[IvoaExecMeetingTM56#CVO][CVO]]
         * [[IvoaExecMeetingTM56#Euro_VO][Euro-VO]]
         * [[IvoaExecMeetingTM56#ESAVO][ESAVO]]
         * [[IvoaExecMeetingTM56#France_VO][France VO]]
         * [[IvoaExecMeetingTM56#GAVO][GAVO]]
         * [[IvoaExecMeetingTM56#HVO][HVO]]
         * [[IvoaExecMeetingTM56#VObs_it][VObs.it]]
         * [[IvoaExecMeetingTM56#Japan_VO][Japan-VO]]
         * [[IvoaExecMeetingTM56#Ukraine_VO][Ukraine VO]]
         * [[IvoaExecMeetingTM56#VAO][VAO]]
         * [[IvoaExecMeetingTM56#RVO][RVO]]
         * [[IvoaExecMeetingTM56#SA3][SA^3]]
         * [[IvoaExecMeetingTM56#SVO][SVO]]
         * [[IvoaExecMeetingTM56#VO_India][VO-India]]
      * [[IvoaExecMeetingTM56#Report_from_the_TCG][Report from the TCG]]
      * [[IvoaExecMeetingTM56#Reports_from_the_WGs][Reports from the WGs]]

---++ <a name="Logistics"></a>Logistics

<span style="color: #000000; font-size: small;">Tuesday, Dec 16, 2014 (17:00-18:00 CET) </span>

---++ <span style="line-height: 19px;">Agenda TM56</span>

   1 Roll Call and Agenda (JE)
   1 Minutes of <a target="_top" href="http://wiki.ivoa.net/internal/IVOA/IvoaRepMin/ivoa-fm55-20141009.pdf">FM55</a>
   1 Review of <a target="_top" href="http://wiki.ivoa.net/internal/IVOA/IvoaExecMeetingTM56/actions-for-tm56-20141216.pdf"><span style="font-family: Verdana, Arial, Helvetica, sans-serif; color: #000000;">Actions</span></a>
   1 Project Reports [Significant Events Only]
   1 <span style="background-color: transparent;">Discussion of progress on US VO coordination initiatives (BB)</span>
   1 TCG status
   1 Approval of new IVOA Recommendation(s) [Standing Item]
   1 Summary of agreement about IVOA documents in the ADS
   1 IVOA Draft Note on Web Assets
   1 DRAFT Charter for IVOA Operations Group
   1 <span style="background-color: transparent;">Exec review membership of CSP</span>
   1 Review terms up for Expiration
   1 <span style="background-color: transparent;"> </span> <span style="background-color: transparent;">Discuss IVOA potential participation at the IAU GA @ Hawaii, Aug 3-14, 2015 </span>
   1 <span style="background-color: transparent;"> </span> <span style="background-color: transparent;">Future Interops</span> 
      * <span style="background-color: transparent;">Spring 2015 - Sesto, Italy / Jun 15-19</span>
      * <span style="background-color: transparent;">Fall 2015 - Sydney, Austalia (after ADASS)</span>
      * Spring 2016 - VO China offered (May2014); S Africa offered (Oct2014)
      * Fall 2016 - Trieste, Italy (Oct 21-23; after ADASS)
   1 <span style="white-space: pre; background-color: transparent;">Date of Next Exec Meeting</span>
   1 <span style="white-space: pre; background-color: transparent;">Review of Actions Items (JE)</span><span style="background-color: transparent;"> </span>
<span style="font-size: 17px; font-weight: bold; line-height: 1em;"><a name="Argentina_NOVA"></span><span style="font-size: 17px; font-weight: bold; line-height: 1em;"></a></span><span style="color: #630000; font-size: 17px; font-weight: bold; line-height: 1em; background-color: transparent;">Argentina - NOVA</span>

---

---+++ <a name="ArVO"></a>ArVO

---

<span style="font-size: 17px; font-weight: bold; line-height: 1em;"><a name="AstroGrid"></span><span style="font-size: 17px; font-weight: bold; line-height: 1em;"></a></span><span style="color: #630000; font-size: 17px; font-weight: bold; line-height: 1em; background-color: transparent;">AstroGrid</span>

---

---+++ <a name="Australia_VO"></a>Australia-VO

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---+++ <a name="BRAVO"></a>BRAVO

---+++ <a name="China_VO"></a>China-VO

China-VO 2014, the 13th annual workshop of the China-VO project, was held from Nov. 26 to 29. More than 100 persons attended the workshop. The theme of the China-VO 2014 is "Big Data in Astronomy".<br /><br />The second WWT planetarium was completed at Astronomy Department of Beijing Normal University. The inauguration was held on Oct. 15, 2014.
---+++ <a name="ChiVO"></a>ChiVO

---+++ <a name="CVO"></a>CVO

---

---+++ <a name="Euro_VO"></a>Euro-VO

---+++ <a name="ESAVO"></a>ESAVO

---

---+++ <a name="France_VO"></a>France VO

---+++ <a name="GAVO"></a>GAVO

---+++ <a name="HVO"></a>HVO

---

---+++ <a name="VObs_it"></a>VObs.it

<span style="font-family: Times New Roman; font-size: small;"> </span>

---+++ <a name="Japan_VO"></a>Japan-VO

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<span style="font-size: 17px; font-weight: bold; line-height: 1em;"><a name="Ukraine_VO"></span><span style="font-size: 17px; font-weight: bold; line-height: 1em;"></a></span><span style="color: #630000; font-size: 17px; font-weight: bold; line-height: 1em; background-color: transparent;">Ukraine VO</span>

---

---+++ <a name="VAO"></a>VAO

---

---+++ <a name="RVO"></a>RVO

<div id="_mcePaste">1. The database of Moscow astronomical plate collection and <span style="background-color: transparent;">maintenance of the General Catalogue of Variable Stars (INASAN and SAI </span><span style="background-color: transparent;">MSU, led by Nikolai Samus) </span></div>

<span style="background-color: transparent;">In March, 2014, a new electronic version of the GCVS was made available </span><span style="background-color: transparent;">to the astronomical community. </span><span style="background-color: transparent;">We started working on the next, 81st Name-List of Variable Stars, </span><span style="background-color: transparent;">which will contain about 6000 objects. A half of the list will be ready </span><span style="background-color: transparent;">for publication by the end of 2014. </span><span style="background-color: transparent;">As usual, many dozens of corrections to the electronic GCVS </span><span style="background-color: transparent;">have been introduced during 2014. A new scanner for digitizing </span><span style="background-color: transparent;">the Moscow collection of astronomical plates was introduced by the end of 2013, </span><span style="background-color: transparent;">and we continued scanning. We also proceed with discoveries of new variable stars</span>
<div id="_mcePaste">using digitized plates. 1011 new variable stars were discovered <span style="background-color: transparent;">in a field in Cassiopeia. Two oral talks on the variable stars </span><span style="background-color: transparent;">from the digitizing project were presented (March, Prague; July, Sofia). </span><span style="background-color: transparent;">The work on the new system of automatic classification of variable stars for the GCVS, </span><span style="background-color: transparent;">based on photometric data, was continued. </span></div>

References

Sokolovsky, K.V., Antipin, S.V., Zubareva, A.M., et al. 2014,
<div id="_mcePaste">New variable stars on digitized plates of the Moscow collection.</div> <div id="_mcePaste">Field SA9. Astronomy Reports, 58, 319.</div>

Kazarovets, E.V., Pastukhova, E.N. 2014, 37 Mira Type Stars from the NSV Catalog:
<div id="_mcePaste">Recovery and Light Elements. Peremennye Zvezdy Prilozhenie/Variable Stars Supplement,</div> <div id="_mcePaste">V. 14, No. 9.</div>

2. Working group "RVO data" (INASAN, led by Dana Kovaleva)

The Binary Star Database (BDB) beta version is available <span style="background-color: transparent;">at http://bdb.inasan.ru/ . The BDB includes all catalogued data </span><span style="background-color: transparent;">on physical and astrometric parameters of binaries and multiples </span><span style="background-color: transparent;">of various types. BDB provides a tool for effective managing </span><span style="background-color: transparent;">of the catalogues of binary stars into the IVO. Organization </span><span style="background-color: transparent;">of the information is based on the careful cross-identification </span><span style="background-color: transparent;">of the objects. This year, the new data catalogues has been added, </span><span style="background-color: transparent;">and the new approach to the solution of cross-identification problem </span><span style="background-color: transparent;">was developed. A new consistent scheme for identification of objects </span><span style="background-color: transparent;">in binary and multiple stars, BSDB (Binary Star DataBase), </span><span style="background-color: transparent;">is developed and implemented. The scheme allows to link properly data </span><span style="background-color: transparent;">with the relevant objects in the stellar system. The list of all binary </span><span style="background-color: transparent;">and multiple stars cross-identifiers (preliminarily named </span><span style="background-color: transparent;">Identification List of Binaries, ILB) is being created and will be used </span><span style="background-color: transparent;">to improve BDB request processing. IVO standards implementation into BDB is discussed. </span><span style="background-color: transparent;">The database request batch mode is being tested.</span>

References

<div id="_mcePaste">Kovaleva D.A., Kaygorodov P.V., Kalinichenko L.A., Malkov O.Yu., Skvortsov N.A.</div> <div id="_mcePaste">"On the problems of designation and cross-identification of multiple objects in astronomy",</div> <div id="_mcePaste">2014, in: Proc. of the 16th All-Russian Conference</div> <div id="_mcePaste">"Digital Libraries: Advanced Methods and Technologies" (RCDL-2014),</div> <div id="_mcePaste">Eds. L.A.Kalmykova, M.R.Kogalovskyi. Dubna,</div> <div id="_mcePaste">The Joint Institute for Nuclear Research, 198-204.</div>

Kalinichenko L.A., Kovalev D.Yu., Kovaleva D.A., Malkov O.Yu.
<div id="_mcePaste">"Introduction into Analysis of Methods and Tools for Hypothesis-Driven</div> <div id="_mcePaste">Scientific Experiment Support", 2014, in: Proc. of the 16th All-Russian Conference</div> <div id="_mcePaste">"Digital Libraries: Advanced Methods and Technologies" (RCDL-2014),</div> <div id="_mcePaste">Eds. L.A.Kalmykova, M.R.Kogalovskyi. Dubna,</div> <div id="_mcePaste">The Joint Institute for Nuclear Research, 177-196.</div>

Dluzhnevskaya O.B., Kaygorodov P.V., Kovaleva D.A., Malkov O.Yu.
<div id="_mcePaste">"BDB: The Binary Star Database" 2014, in ADASS XXIII Conference,</div> <div id="_mcePaste">eds. N. Manset, P. Forshay. Waikoloa, Hawaii, Sep 2013, ASP Conf. Ser.,</div> <div id="_mcePaste">Vol. 485, 247-250.</div>

Kaygorodov P.V., Kovaleva D.A., Dluzhnevskaya O.B., Malkov O.Yu.
<div id="_mcePaste">Binary star database (BDB) internals, 2014, Russian Digital Libraries, 17, 1</div>

Kaygorodov P.V., Kovaleva D.A., Malkov O.Yu.
<div id="_mcePaste">"Design and Implementation of BDB, the Binary Star Database" 2014,</div> <div id="_mcePaste">in Setting a new standard in the analysis of binary stars conference,</div> <div id="_mcePaste">eds. Kresimir Pavlovski, Andrew Tkachenko, Guillermo Torres.</div> <div id="_mcePaste">Leuven, Sep 2013, EAS Publication Series, Vol. 64, 405-406.</div>

Malkov O.Yu., Kaygorodov P.V., Kovaleva D.A., Oblak E., Debray B.
<div id="_mcePaste">"Binary star database BDB: datasets and services" 2014, <span style="background-color: transparent;">Astronomical and Astrophysical Transactions, 28, N 3, 235-244.</span></div>

O.Yu.Malkov, O.B.Dluzhnevskaya, P.V.Kaygorodov, D.A.Kovaleva, N.A.Skvortsov
<div id="_mcePaste">"On identification and cross-identification of celestial objects", 2014, <span style="background-color: transparent;">Russian Digital Libraries, in press</span></div>

Kovaleva D.A., Debray B., Kaygorodov P.V., Malkov O.Yu., Oblak E.
<div id="_mcePaste">"VO-accessible Binary star DataBase BDB" 2014, Astronomy and Computing, <span style="background-color: transparent;">submitted</span></div>

Avvakumova E., Kaygorodov P., Kovaleva D., Malkov O.
<div id="_mcePaste">"The Binary star DataBase (BDB): the new service providing basic data for binary and multiple systems" 2014,</div> <div id="_mcePaste">in Binary Systems, their Evolution and Environments Conference, <span style="background-color: transparent;">Ulaanbaatar, Mongolia, Sep 2014,</span></div> <div id="_mcePaste">http://mongolia.csp.escience.cn/, id.G1.</div>

Conferences

Malkov O.Yu., "Binary star database BDB". Invited talk at All-Russian
<div id="_mcePaste">scientific conference "Information systems in fundamental science. Big data".</div> <div id="_mcePaste">SAO RAS, Nizhny Arkhyz (21-26.07.2014)</div>

Malkov O.Yu. "On identification and cross-identification of celestial objects"
<div id="_mcePaste">Invited talk at Fourth All-Russian Symposium</div> <div id="_mcePaste">"Infrastructure of Scientific Informational Resources and Systems",</div> <div id="_mcePaste">StPetersbourg (6-8.10.2014)</div>

Kovaleva D.A. "On the problems of designation and cross-identification
<div id="_mcePaste">of multiple objects in astronomy", Talk at 16th All-Russian Conference</div> <div id="_mcePaste">"Digital Libraries: Advanced Methods and Technologies" (RCDL-2014),</div> <div id="_mcePaste">Dubna (13-16.10.2014)</div>

Avvakumova E.A. "The Binary star DataBase (BDB): the new service
<div id="_mcePaste">providing basic data for binary and multiple systems", Poster paper at:</div> <div id="_mcePaste">"Binary Systems, their Evolution and Environments" Conference,</div> <div id="_mcePaste">Ulaanbaatar, Mongolia, Sep 2014</div>

3. Working group "Technologies of RVO information structures"
<div id="_mcePaste">(IPI RAS, led by Leonid Kalinichenko)</div>

In 2014 at the Institute of Informatics Problems in cooperation with colleagues from INASAN <span style="background-color: transparent;">investigations for developing virtual observatories have been conducted, focused on: investigation and </span><span style="background-color: transparent;">development of conceptual approach to astronomical problem solving and demonstration of its benefits </span><span style="background-color: transparent;">for particular cases; development of multiple object identification system and common approach to their </span><span style="background-color: transparent;">cross-identification; investigation of methods to support lifecycle of hypothesis-dviven research and </span><span style="background-color: transparent;">experiments; investigation of anomaly detection methods for various kinds of data.</span>

Investigation of conceptual approach to scientific problem solving

Astronomy as a data-intensive science becomes more and more dependent on the fast growing datasets <span style="background-color: transparent;">from various epochs, spectral ranges and instruments. Up to now researchers continue to be committed to </span><span style="background-color: transparent;">the approach according to which particular catalogs are selected prior to the problem statement, so that </span><span style="background-color: transparent;">the problem is defined in the terms of specific catalogs. Due to that problem specification and solving </span><span style="background-color: transparent;">become tightly tied to specific catalogs and services.</span>

Dominance of such approach impedes the problem solving methods reuse with other datasets as well as <span style="background-color: transparent;">collecting methods to apply in new researches. Virtual observatories stress this deficiency serving generally </span><span style="background-color: transparent;">as data archives today instead of serving also as libraries of analytic methods applicable to astronomical </span><span style="background-color: transparent;">objects and phenomena, not to catalog lines.</span>

In this regard using conceptual approach is noteworthy. It is built on the problem domain knowledge <span style="background-color: transparent;">allowing formulation of problem solving algorithms and data analysis methods in terms of the domain </span><span style="background-color: transparent;">concepts without reference to catalogs thus getting rid of the mentioned deficiencies. Catalogs in their </span><span style="background-color: transparent;">turn are mapped into the problem domain specifications and used to solve problems formulated in the </span><span style="background-color: transparent;">domain terms.</span>

<span style="background-color: transparent;"><br /></span>
<div id="_mcePaste">Benefits of conceptual approach application has been demonstrated on solving of problems related to <span style="background-color: transparent;">searching for secondary photometric standard candidates, detection photometric redshift of galaxies, </span><span style="background-color: transparent;">construction of binary and multiple star repository from heterogeneous databases, classification of </span><span style="background-color: transparent;">eclipsing stars. These problems have been formulated and solved over specifications of widely applied </span><span style="background-color: transparent;">knowledge dimensions in astronomy such as photometric systems, astronomical objects, multiple star </span><span style="background-color: transparent;">systems and others, and defined in the respective domain terms independently of the existing catalogs [1].</span></div>

Development of multiple object identification system and cross-identification approach

This work continues and develops research focused on solving of problems arising in the comprehensive <span style="background-color: transparent;">analysis of heterogeneous data sets by available arsenal of scientific methods and tools to identify useful </span><span style="background-color: transparent;">information and to gain new knowledge. Problems of identification and crossmatching of multiple objects </span><span style="background-color: transparent;">in astronomy were observed with a focus on systematization of identification and integrating of </span><span style="background-color: transparent;">multidimensional observational data of different types. Existing methods of identification of single and </span><span style="background-color: transparent;">multiple astronomical objects have been reviewed. BSDB scheme has been daveloped and implemented in </span><span style="background-color: transparent;">Binary star database (BDB). Problems and solutions in cross-identification methods have been correlated </span><span style="background-color: transparent;">to entity resolution methods in computer science including data schema mathing, data indexing in order to </span><span style="background-color: transparent;">reduce pairwise enumeration, data comparison methods, selection of data identifying unique objects or </span>
<div id="_mcePaste">allowing to estimate similarity [2].</div>

<div id="_mcePaste">Analysis of Methods and Tools for Hypothesis-Driven Scientific Experiment Support</div>

The objective of this study is to analyze, collect and systematize information on the role of hypotheses in <span style="background-color: transparent;">the data intensive research process as well as on support of hypothesis formation, evaluation, selection </span><span style="background-color: transparent;">and refinement in course of the natural phenomena modeling and scientific experiments. Facilities of </span><span style="background-color: transparent;">informatics for support of hypothesis-driven experiments, considered in the paper, are aimed at the </span><span style="background-color: transparent;">conceptualization of scientific experiments, hypothesis formulation and browsing in various domains </span><span style="background-color: transparent;">(including biology, biomedical investigations, neuroscience, astronomy), automatic organization of </span><span style="background-color: transparent;">hypothesis-driven experiments. Examples of scientific researches applying hypotheses considered in the </span><span style="background-color: transparent;">paper include modeling of population and structure synthesis of the Galaxy, connectome-related </span><span style="background-color: transparent;">hypothesis testing, studying of temperature trends in Australia, analysis of stock markets applying the </span><span style="background-color: transparent;">EMN (efficient market hypothesis), as well as algorithmic generation of hypotheses in the IBM Watson </span><span style="background-color: transparent;">project. An introduction into the state of the art of the hypothesis-driven research presented in the paper </span><span style="background-color: transparent;">opens a way for investigation of the generalized approaches for efficient organization of hypothesis-driven </span><span style="background-color: transparent;">experiments applicable for various branches of data intensive sciences [3].</span>

Survey of anomaly detection methods for data intensive research

<span style="background-color: transparent;">An approach to classify different anomaly detection methods according to the way the data is presented. </span><span style="background-color: transparent;">Different applications of the outlier analysis in various cases have been summarized. end we Specific </span><span style="background-color: transparent;">features of the methods suitable for the outlier analysis problem have been overviewed. Future plans </span><span style="background-color: transparent;">include working on the anomaly detection in various fields (e.g. finding peculiar objects in massive digital </span><span style="background-color: transparent;">sky astronomy surveys) [4].</span>

References

1. Skvortsov N.A., Avvakumova E.A., Briukhov D.O., Vovchenko A.E.,
<div id="_mcePaste">Volnova A.A., Dluzhnevskaya O.B., Kaygorodov P.V., Kalinichenko L.A., Knyazev A.Y., Kovaleva D.A. Malkov</div> <div id="_mcePaste">O.Y., Pozanenko A.S., Stupnikov S.A.</div> <div id="_mcePaste">Problem solving in astronomy using conceptual approach //</div> <div id="_mcePaste">Astrophysical Bulletin, accepted</div>

2. Kovaleva D.A., Kaygorodov P.V., Malkov O.Y., Kalinichenko L.A., Skvortsov N.A.
<div id="_mcePaste">Problems of Designation and Cross-Identification of Multiple Objects in</div> <div id="_mcePaste">Astronomy. // RCDL 2014. Dubna: JINR, 2014, p. 198-204</div> <div id="_mcePaste">http://ceur-ws.org/Vol-1297/125-131_paper-19.pdf</div>

3. Kalinichenko L.A., Kovalev D.Y., Kovaleva D.A., Malkov O.Y. Introduction into Analysis of Methods and
<div id="_mcePaste">Tools for Hypothesis-Driven Scientific Experiment Support. // 16th Russian Conference on Digital Libraries</div> <div id="_mcePaste">RCDL 2014 Proceedings. Dubna: JINR, 2014. P. 177-196; http://ceur-ws.org/Vol-1297/104-123_paper-</div> <div id="_mcePaste">17.pdf</div>

4. Kalinichenko L. A, Shanin I., Taraban I. Methods for Anomaly Detection: a Survey // 16th Russian
<div id="_mcePaste">Conference on Digital Libraries RCDL 2014 Proceedings. Dubna: JINR, 2014. P. 42-47. http://ceur-</div> <div id="_mcePaste">ws.org/Vol-1297/020-25_paper-5.pdf</div>

4. Working group "The service of the electronic library of the astronegatives <span style="background-color: transparent;">produced on Zvenigorod Observatory" (INASAN, led by Sergei V. Vereshchagin)</span>
<div id="_mcePaste">The service and support in working order the digital archives was continued. <span style="background-color: transparent;">The scanning and cataloging process for the Zvenigorod Astrograph plates </span><span style="background-color: transparent;">was doing with data reduction to a standard format according to WFPDB instruction </span><span style="background-color: transparent;">(some more than 100 plates was scanned. </span><span style="background-color: transparent;">The online information about our work, science groups, tools, volumes and </span><span style="background-color: transparent;">characteristic of the plate and film libraries is presented: </span></div> <div id="_mcePaste"><span style="white-space: pre;"> </span>1) on the INASAN site http://www.inasan.ru/rus/scan/;</div> <div id="_mcePaste"><span style="white-space: pre;"> </span>2) in the Wide Field Plate Data Base in Bulgaria http://wfpdb.org /search/search.cgi</div> <div id="_mcePaste"><span style="white-space: pre;"> </span> (Getting data about archive and each plate, viewing of the negatives, <span style="background-color: transparent;">selection plates by the parameters. In the search to use: IDobs - "ZVN", </span><span style="background-color: transparent;">IDins - "040" for Astrograph, IDins - "021" for AFU.);</span></div> <div id="_mcePaste">3) About the Zvenigorod Observatory Telescopes:</div> <div id="_mcePaste"><span style="white-space: pre;"> </span>http://www.inasan.ru/eng/zvenigorod/instr.html</div>

<div id="_mcePaste">References</div>

1. S.V.Vereshchagin and N.V.Chupina
<div id="_mcePaste">"Photoplates digital archives of the INASAN Zvenigorod Astronomical Observatory".</div> <div id="_mcePaste">International workshop on scientific use,</div> <div id="_mcePaste">digitization and preserving astronomical photographic records.</div> <div id="_mcePaste">Prague, Villa Lanna, March 18-21, 2014</div> <div id="_mcePaste">http://www.astroplate.cz/</div>

2. S.V.Vereshchagin and N.V.Chupina
<div id="_mcePaste">Zvenigorod Observatory Scans Arhive Electonic Bibliotecs and</div> <div id="_mcePaste">Perspective methods and thechnologis, an electronic collections, Dubna,</div> <div id="_mcePaste">2014, in: Proc. of the 16th All-Russian Conference</div> <div id="_mcePaste">"Digital Libraries: Advanced Methods and Technologies" (RCDL-2014),</div> <div id="_mcePaste">Eds. L.A.Kalmykova, M.R.Kogalovskyi. Dubna,</div> <div id="_mcePaste">The Joint Institute for Nuclear Research, 411-415.</div>
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---+++ <a name="SA3"></a>SA^3

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---+++ <a name="SVO"></a>SVO

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---+++ <a name="VO_India"></a>VO-India

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---++ <a name="Report_from_the_TCG"></a>Report from the TCG

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---++ <a name="Reports_from_the_WGs"></a>Reports from the WGs

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Topic attachments
I	Attachment	History	Action	Size	Date	Who	Comment
pdf	20141216-IVOAOpsCharter-DRAFT.pdf	r1	manage	102.6 K	2014-12-16 - 13:03	ChristopheArviset
Topic revision: r11 - 2014-12-18 - JanetEvans
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