The MAO NASU glass archive database: search and management tools
At the Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO NASU) the astronomical glass archive counts more than 50 000 of plates obtained in various observational projects during last 50 years of the past century. The local single-user database of glass archive, create...
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Головна астрономічна обсерваторія НАН України
2005
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Назва видання: | Кинематика и физика небесных тел |
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Цитувати: | The MAO NASU glass archive database: search and management tools / L. Pakuliak // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 573-576. — Бібліогр.: 1 назв. — англ. |
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irk-123456789-797252015-04-04T03:02:45Z The MAO NASU glass archive database: search and management tools Pakuliak, L. SS1: Virtual Observatories and Data Archives At the Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO NASU) the astronomical glass archive counts more than 50 000 of plates obtained in various observational projects during last 50 years of the past century. The local single-user database of glass archive, created on the basis of observational logs and partly on measurement results, has been transformed into an online multy-user system to provide a remote access to the plate archive. In the paper online tools for data searching and database management are presented. 2005 Article The MAO NASU glass archive database: search and management tools / L. Pakuliak // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 573-576. — Бібліогр.: 1 назв. — англ. 0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/79725 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України |
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SS1: Virtual Observatories and Data Archives SS1: Virtual Observatories and Data Archives Pakuliak, L. The MAO NASU glass archive database: search and management tools Кинематика и физика небесных тел |
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At the Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO NASU) the astronomical glass archive counts more than 50 000 of plates obtained in various observational projects during last 50 years of the past century. The local single-user database of glass archive, created on the basis of observational logs and partly on measurement results, has been transformed into an online multy-user system to provide a remote access to the plate archive. In the paper online tools for data searching and database management are presented. |
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Pakuliak, L. |
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Pakuliak, L. |
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Pakuliak, L. |
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The MAO NASU glass archive database: search and management tools |
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The MAO NASU glass archive database: search and management tools |
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The MAO NASU glass archive database: search and management tools |
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The MAO NASU glass archive database: search and management tools |
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The MAO NASU glass archive database: search and management tools |
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mao nasu glass archive database: search and management tools |
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Головна астрономічна обсерваторія НАН України |
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2005 |
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SS1: Virtual Observatories and Data Archives |
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http://dspace.nbuv.gov.ua/handle/123456789/79725 |
citation_txt |
The MAO NASU glass archive database: search and management tools / L. Pakuliak // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 573-576. — Бібліогр.: 1 назв. — англ. |
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Кинематика и физика небесных тел |
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AT pakuliakl themaonasuglassarchivedatabasesearchandmanagementtools AT pakuliakl maonasuglassarchivedatabasesearchandmanagementtools |
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2025-07-06T03:43:47Z |
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2025-07-06T03:43:47Z |
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THE MAO NASU GLASS ARCHIVE DATABASE:
SEARCH AND MANAGEMENT TOOLS
L. Pakuliak
Main Astronomical Observatory, NAS of Ukraine
27 Akademika Zabolotnoho Str., 03680 Kyiv, Ukraine
e-mail: pakuliak@mao.kiev.ua
At the Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO
NASU) the astronomical glass archive counts more than 50 000 of plates obtained in various ob-
servational projects during last 50 years of the past century. The local single-user database of
glass archive, created on the basis of observational logs and partly on measurement results, has
been transformed into an online multy-user system to provide a remote access to the plate archive.
In the paper online tools for data searching and database management are presented.
INTRODUCTION
At the Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO NASU) collected
a vast archive of glass astronegatives, obtained in frames of various observational projects, carried out at MAO
during last decades. Most of them cover separate sky areas, having interesting astronomical objects, except
for more than two thousands FON plates with a full coverage of the northern hemisphere with a small (25%)
overlap, as it was provided in Northern Sky Review Project (FON, after the completion of the project and
data proceeding – FONAK), carried out in 1987–1994. Time range of the archive covers 50 years (1947–1998).
The MAO plate archive started in 1950. The collection was partially presented earlier. Data for some plate
collections are shown in Table 1.
Table 1. Some plate collections from the MAO NASU glass archive
Scientific projects Telescopes Scale (′′/min) Period Lim.magn. Num. of plates
– Galaxies DLA,DWA, DSA 38, 103, 295 1950–1990 16.0m, 16.0, 12.0–13.0 1100, 300, 100
– Radio Sources DAZ, Zeiss-600 69, 28 1986–1989 18.0, 18.5 20, 100
– Selected areas DWA,DSA, TCA 103, 295, 172 1949–1990 16.0, 14.0, 12.8 400, 2080, 840
Fundamental stars DLA,DWA 38, 103 1956–1990 14.5, 15.5 1770, 150
Special programs DLA,DWA, DSA 38, 103, 295 1949–1987 15.5, 16.0, 16.0 2760, 230, 3000
Northern Sky Survey (FON) DWA, DAZ 103, 60 1981–1993 16.0, 17.0 2400, 90
Planets and their satellites DLA,DWA, Zeiss-600 38, 103, 28 1960–1990 15.0, 14.0, 16.0 1300, 300, 250
Minor planets DLA,DWA, DSA 38, 103, 295 1949–1996 14.0, 14.5, 13.0 557, 1100, 20
Comets DWA,DSA, TCA 103, 295, 172 1976–1996 16.0, 14.0, 12.8 625, 270, 10
List of telescopes in Table 1: DLA – Double Long-Focus Astrograph (D/F = 40/550 refractor);
DWA – Double Wide-Angle Astrograph (D/F = 40/200 refractor);
AZT-2 – (D/F = 70/315 reflector);
DSA – Double Short-Focus Astrograph (D/F = 12/70 refractor);
DAZ – Zeiss Double Astrograph (D/F = 40/300 refractor);
TCA – Three-Cameras Astrograph (D/F = 11/170 refractor).
Other plate collections include more then 4 000 geostationary satellite plates, 1 000 Moon plates, about
10 000 active solar formation plates, more than 50 000 stellar and planetary spectra plates. During the FON
Project observations, it became necessary to create an electronic archive of observed plates and the digital
database of plates content on the basis of that archive and measured data obtained after measurements of
plates on the measuring machine PARSEC of MAO NASU. Lately that archive was enhanced with data of first
epoch plates from others observational projects and the current electronic archive of glass plates was formed.
c© L. Pakuliak, 2004
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DATABASE OF THE ASTRONOMICAL GLASS PLATE ARCHIVE
The first version of the electronic plate archive was made in the FOXBASE+ environment on DOS platform.
It included data of practically all plates from project FON (FONAK), projects on galaxies, fundamental stars,
variable stars, as well as special programs, the MEGA projects, for which the plates have been taken with
DLA and DWA (Table 1). The software package consisted of the administrative interface for database integrity
support, backup and data correction and of the user interface for the optimal request construction.
On certain stage of plates’ digitization, the necessity appeared to transform the local single-user database into
an online multy-user system to provide a remote access to the plate archive and to involve the MAO database
into the world database of glass archives. And more on, the archive of FON measurements and the conserved
measured data of plates of other projects give an opportunity to not only select data of plates, but to obtain
a kind of “quick-view” of plate content before the digitization procedure would be completed.
Online astronegative database has been constructed on the basis of the relational database management
system MySQL.
MySQL Server was originally developed to handle large databases and today it offers a rich and useful set
of functions, making its connectivity, speed, and security highly suited for accessing databases on the Internet.
MySQL Server is installed on the web-server (Debian GNU/Linux) of MAO NASU. The MySQL Database
Software is a client/server system that consists of a multi-threaded SQL server that supports different backends,
several different client programs and libraries, administrative tools, and a wide range of programming interfaces
(APIs) and ODBC (Open-DataBase-Connectivity) support for Win32 as well. For non-commercial purposes
the MySQL software is an Open Source/Free Software product under the terms of the GNU General Public
License.
Currently, the database includes the following plate collections (Table 2):
Table 2. Plate collections, included into the online database
Northern Sky Survey (FON) 2229 records
Sky areas with Galaxies, Radio Sources, Selected areas 1097 records
Fundamental stars 1769 records
Special programs (clusters, star associations, variable stars, double stars, etc.) 2091 records
Main Meridional Section of the Galaxy (MEGA) 261 records
Minor planets 1097 records
Comets, clusters, SS bodies (DWAA) 3208 records
Plate collection of Three-Cameras Astrograph (clusters mostly) 1093 records
Plate collection of AZT-2 (70-cm reflector) 1124 records
Total 13969 records
The structure of database (Fig. 1) consists of data tables, connective tables, auxiliary tables and authorization
tables. Such a division in according with different functionality permits an easy supplement of database with
new collections and a high flexibility in constructing SQL-queries.
General plate data store in data tables divided by instrumental or project factor because of a structure of
a record differs widely for different collections (Table 3). Fields set in every data table consists of mandatory
fields, the same ones in every collection, and special fields, unique for the collection.
Connective tables include data, which describe common characteristics of instruments, programs, emulsions,
etc., as well as identificator fields for binding common data with data of every collection.
The auxiliary table “list of fields” includes the description of every data table structure and is necessary for
the formalization of SQL-queries when searching of data. The table of authorization includes data of permitted
users and their personal information in order to give the access for the administrative part of the database user
interface.
The electronic database of the plate data archive is searchable. The search engine for data search was built
on PHP+MySQL web facilities and for the moment it is capable to search plates in the area of any radius around
the point with center coordinates, telescope, collection, colour band, exposition duration, period of observation,
etc., inserted into the SQL-query constructor form as search parameters. The result of searching returns as
a HTML-page with general data of selected plates, covering the area of interest. It is possible to search data as
in a separate collection, and so as in the whole database.
The user interface permits user to browse detailed plate data for every plate, identified by its log-book
name, to browse a complete set of plate data for the collection as a whole and to view the overall description of
collections.
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Figure 1. The structure of database
Table 3. An example of MySQL-table structure for the MEGA observational project
No Field Type Default Extra Index Field Description
1 NumPlate Int(10) Default Autoincrement Primary Plate ID
2 PlateName Varchar(12) 0 Number of plate in a log
3 RA Double NULL Center coordinates
4 D Double NULL Center coordinates
5 EPlate Int(10) 0 Epoch of center coordinates
6 LimMag Int(10) 0 Limited magnitude
7 DPlate Int (10) 0 Date
8 Obj Varchar(50) 0 Astronomical objects
9 XNum Tinyint(4) 0 Number of expositions
10 X1 Float 0 Duration of 1st exposure
11 X2 Float 0 Duration of 2nd exposure
12 X3 Float 0 Duration of 3rd exposure
13 DimP Varchar(20) Dimensions
14 Temp Float 0 Temperature
15 Press Float 0 Pressure
16 TAngle Float 0 Hour angle
17 Qual Varchar(20) Quality
18 Emulsion Varchar(20) NULL Emulsion and filter
19 Colour Varchar(4) NULL Colour
20 Observer Varchar(20) Observer
21 Note Text Notes
22 Telescope Varchar(100) NULL Telescope
23 Scale Int(11) 0 Scale
24 Program Varchar(255) NULL Observational project
25 Station Varchar(255) NULL Observational site
26 Digitals Varchar(255) NULL Scan index or measurements file index
27 Tstamp Timestamp(14) NULL Timestamp
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The administrative module of the user interface gives a possibility to update data in records of every data
table or to add single plates to the proper collection. Massive data loading or creation of new data tables is
carried out by means of MySQL environment, not through the user interface. An access to administrative tools
of user interface is realized by means of PHP Basic Authentication and is permitted for authorized users only.
The database is available on the web-site of the Main Astronomical Observatory of NAS of Ukraine at
[http://www.mao.kiev.ua/ardb/].
PROSPECTS
The further development of user package of tools for database management and data search include following
tasks (in the order of complexity growing):
1. Realization of building of sketches of selected plates overlapping.
2. Improvement of the database expansion tools by means of WWW-interface.
3. Realization of data extracting in various output formats; dumping selected data into files and transmission
them into the user computer by HTTP or email (in a case of a vast data set).
4. Realization of “quick-view” of plate content on the basis of plate scanning or measurements.
[1] Pakulyak L. K., Golovnya V. V., Sergeeva T. P. Wide Field Plate Archive of MAO NAS of Ukraine: electronic plate
collection and first results of database application // New deal in European Astronomy: Trends and Perspectives:
Abstr. Intern. Conf. JENAM-2003, Budapest, Aug. 25–30, 2003.–P. 112.
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