The Wide-Field Plate Database: A New Tool in Observational Astronomy

Author(s):  
M. K. Tsvetkov ◽  
K. Y. Stavrev ◽  
K. P. Tsvetkova ◽  
E. H. Semkov ◽  
A. S. Mutafov ◽  
...  
1998 ◽  
Vol 179 ◽  
pp. 462-464
Author(s):  
M.K. Tsvetkov ◽  
K.Y. Stavrev ◽  
K.P. Tsvetkova ◽  
E.H. Semkov ◽  
A.S. Mutafov ◽  
...  

Since the first applications of wide-field photography in astronomy nearly 2 million plates and films have been obtained and stored in archives all over the world. The Wide-Field Plate Database (WFPDB) provides astronomers with detailed information about the wide-field photographic observations. Its preparation started in 1991 as one of the main projects initiated by the Working Group on Wide Field Imaging at the IAU Commission 9.


1994 ◽  
Vol 161 ◽  
pp. 359-364 ◽  
Author(s):  
M.K. Tsvetkov ◽  
K.Y. Stavrev ◽  
K.P. Tsvetkova ◽  
P.V. Ivanov ◽  
M.S. Iliev

The present status of the work on the creation of a Wide-Field Plate Database is reported. It is planned to collect the available information for about 1.5 million plates from 187 wide-field instruments in 71 institutes/observatories. The source data are from 213 plate catalogues, 65 of them in computer-readable form. The structure and content of the Wide-Field Plate Database, now including 51 observation catalogues with more than 300,000 plates, is presented.


2014 ◽  
Vol 335 (4) ◽  
pp. 440-447
Author(s):  
A.V. Poghosyan ◽  
W. Pfau ◽  
K.P. Tsvetkova ◽  
M. Mugrauer ◽  
M.K. Tsvetkov ◽  
...  

2000 ◽  
Vol 9 (4) ◽  
Author(s):  
M. K. Tsvetkov ◽  
M. Stavinschi ◽  
K. P. Tsvetkova ◽  
Κ. Y. Stavrev ◽  
H. D. Lukarski ◽  
...  

1994 ◽  
Vol 161 ◽  
pp. 141-145
Author(s):  
H.H. Heyer ◽  
J. Quebatte ◽  
H. Zodet

The recent years have seen a clear trend in observational astronomy towards digital detectors, but they are only able to cover sky fields which are significantly smaller than what is possible with photographic plates. In consequence, there has been a tendency to concentrate on small sky areas and individual objects. Nevertheless, many large-scale structures can only be well comprehended if the observed fields are much larger than such CCD-frames. Similarly, the use of more than one passband adds important information for a better understanding of the nature of large structures. We demonstrate this by showing here a two-field composite of IC 1396 (Palomar/ESO Atlas), and a four-field composite from the ESO R-Atlas, covering an area of more than 100 square degrees around IC 4628 in Scorpius/Ara.


1995 ◽  
Vol 148 ◽  
pp. 148-155 ◽  
Author(s):  
Milcho Tsvetkov ◽  
Konstantin Stavrev ◽  
Katya Tsvetkova ◽  
Asen Mutafov ◽  
Michail-Ernesto Michailov

AbstractThe contemporary state of the Schmidt/Maksutov telescope plate archives and their unification in an Index Plate Catalogue as part of the Wide Field Plate Database is presented.


2001 ◽  
Vol 24 (3) ◽  
pp. 231-231 ◽  
Author(s):  
Mucho. K. Tsvetkov

The Sofia Sky Archive Data Center (SSADC) was developed on the base of the Wide-Field Plate Database (WFPDB – http://www.skyarchive.org) as a project of the Working Group on Sky Surveys, Commission 9 of the IAU, and is dedicated to saving plate collections. The center manages 12 PCs connected in a local computer network and a PDS 1010 microdensitometer donated by the European Southern Observatory. The main field of operation is the WFPDB development, plate digitization and image processing for different astronomical tasks in South- and East Europe (Russia, Ukraine, Armenia, etc.), and as a regional coordinator especially for the neighbour countries – Romania, Yugoslavia, Macedonia, Greece and Turkey. The main problem in the way of the WFPDB development is the creation of the computer-readable plate catalogues of the original logbooks because the speed of converting the logbooks in a computer-readable form is very low. The message is: we have to find the way to accelerate this important part of the project where the role of the developing countries in this direction should be very important. (Co-authors are: K. Tsvetkova, K. Stavrev V. Popov, H. Lukarski, A. Borisova, M-E. S. Michailov and G. Borisov of Sofia, Bulgaria, and S. Christov, Bulgarian South-West University).


1995 ◽  
Vol 148 ◽  
pp. 170-173
Author(s):  
R. H. McNaught ◽  
D. I. Steel ◽  
K. S. Russell ◽  
G. V. Williams

AbstractWe describe our routine identification of images of asteroids and comets on plates and films in the U.K. Schmidt Telescope archive. The asteroids of most interest to us are those which approach the Earth, and whenever such an object is found (by anyone) we perform backintegrations in order to determine whether the object may have been recorded on any UKST plate taken since 1973. In many cases the object is found (‘precovered’) and measured, allowing an accurate orbit to be determined soon after its discovery; other studies such as long-term dynamical investigations, or predictions of future close approaches to the Earth, are then possible. Similar programs using other wide-field plate archives are to be encouraged, since valuable scientific results may be derived.


1995 ◽  
Vol 151 ◽  
pp. 412-415
Author(s):  
M.K. Tsvetkov ◽  
K.Y. Stavrev ◽  
K.P. Tsvetkova ◽  
A.S. Mutafov

AbstractThe current status of a database containing information on wide-field observations stored in plate archives all over the world is presented. The database will permit on-line access to information on nearly 2 · 106 wide-field (⪆ 1 degree) plates and films, obtained over more than a century with about 200 telescopes and cameras.


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