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11021. Презентация PowerPoint
Prague, August 16, 2006 . Another problem that was making it difficult to automatically merge GCVS and survey catalogs has been recently solved: 'old' variable stars also had only very rough coordinates. The GCVS has been identified, on a star-by-star basis, with positional catalogs. ... The total number of stars we were unable to identify, at least tentatively, is only 200, most of them from two or three sources of especially unreliable positional information. ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0006.htm -- 6.4 Кб -- 04.09.2006
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11022. Презентация PowerPoint
. Prague, August 16, 2006 . Same star: A.V. Khruslov, PZP, 2005, 5 , No. 8 . Problems with automatic period determination and classification. One of the Galaxy's longest- period fundamental-mode Cepheids in the ASAS-3 light- curve gallery
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0032.htm -- 7.8 Кб -- 04.09.2006
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11023. http://www.sai.msu.su/gcvs/future/iaupraha.files/master03.htm
. Образец заголовка . Образец текста . Второй уровень . Третий уровень . Четвертый уровень . Пятый уровень . ?дата/время? . ?нижний колонтитул? . ?#?
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/master03.htm -- 2.6 Кб -- 04.09.2006
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11024. http://www.sai.msu.su/gcvs/future/iaupraha.files/master03.xml
-microsoft-com:office:powerpoint xmlns:oa= urn:schemas-microsoft-com:office:activation o:shapelayout v: ext = edit o:idmap v: ext = edit data= 1 / /o:shapelayout p:colorscheme colors= #FFFFFF,#000000,#808080,#000000,#00CC99,#3333CC,#CCCCFF,#B2B2B2 / v:background id= _x0000_s1025 o:bwmode= white fillcolor= white [0] v: ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/master03.xml -- 4.5 Кб -- 04.09.2006
[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master03.xml -- 4.5 Кб -- 04.09.2006
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[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master03.xml -- 4.5 Кб -- 04.09.2006
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11025. http://www.sai.msu.su/gcvs/future/iaupraha.files/pres.xml
xml xmlns:v= urn:schemas-microsoft-com:vml xmlns:o= urn:schemas-microsoft-com: office : office xmlns:p= urn:schemas-microsoft-com: office :powerpoint xmlns:oa= urn:schemas-microsoft-com: office :activation p:presentation sizeof= screen gridspacingx= 46448 gridspacingy= 46448 p:master id= 3 slidesn = 0,0 type = main ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/pres.xml -- 4.4 Кб -- 04.09.2006
[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/pres.xml -- 4.4 Кб -- 04.09.2006
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[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/pres.xml -- 4.4 Кб -- 04.09.2006
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11026. Презентация PowerPoint
Prague, August 16, 2006 . The main GCVS problem is that it is no longer a GENERAL catalogue of variable stars (in fact, it even never was). The GCVS always was a catalogue of galactic variables, with a minor number of extragalactic stars that were included mainly by misunderstandings. ... Recently, many thousands of new variable stars were discovered in automatic survey projects (for example, some 30000 non-GCVS stars solely in the ASAS-3 project). ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0001.htm -- 7.1 Кб -- 04.09.2006
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11027. Презентация PowerPoint
. N.N. Samus . Institute of Astronomy (Russian Acad. Sci.), . Sternberg Astronomical Institute (Moscow University), . and Eurasian Astronomical Society . Problems and Prospects . of the GCVS . The XXVI th ? General Assembly of the IAU . Prague, Czech Republic . August 16, 2006
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0003.htm -- 8.0 Кб -- 04.09.2006
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11028. Презентация PowerPoint
... Since GCVS IV, there was no new GCVS edition. ... Main reasons for the automatic-survey new variables remaining outside the GCVS for a long time: • ? different level of detail of the classification systems, no perfect software for automatic classification available; • ? individual approach to each star that was always used in the GCVS cannot be applied any longer, but the experience of automatically- updated catalogs evidences for the number of errors ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0004.htm -- 7.3 Кб -- 04.09.2006
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11029. Презентация PowerPoint
Prague, August 16, 2006 . ... The history of variable-star catalogues is a kind of permanent crisis due to wrong decisions (Argelander?s system of designating variable stars using letters; the attempt of the ?Astronomische Gesellschaft? to issue catalogues every year; the tradition of globular-cluster variables kept outside the general catalogue; etc.) ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0028.htm -- 6.4 Кб -- 04.09.2006
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11030. Презентация PowerPoint
Prague, August 16, 2006 . ... The GCVS has no IAU financial support since 1994, so we are not discussing money. ... However, it must be finished, with a new modern version prepared for all ?old? GCVS stars, including those from Name-Lists, with current knowledge incorporated and improved classification system applied. ... Also, people like GCVS star names, use them, ? and want their discoveries to be named. We can ask other people, with better resources than in Russia, to continue. ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0029.htm -- 7.4 Кб -- 04.09.2006
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11031. Презентация PowerPoint
Prague, August 16, 2006 . ... We can decide to merge the GCVS with automatic surveys now. I have already outlined the difficulties and will give some examples illustrating the problems slightly later. Steve Kawaler?s suggestion: ?The GCVS personnel might play a role as a `meta-catalog? ? a central `index? of survey-based catalogs of variable stars?. ... If we want to have a good meta-catalog, the difficulties I have mentioned in relation to merging the catalogues still should be considered. ...
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Ссылки http://www.sai.msu.su/gcvs/future/iaupraha.files/slide0030.htm -- 6.3 Кб -- 04.09.2006
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11032. http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master03.htm
. Образец заголовка . Образец текста . Второй уровень . Третий уровень . Четвертый уровень . Пятый уровень . 'дата/время' . 'нижний колонтитул' . '#'
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/master03.htm -- 2.6 Кб -- 04.09.2006
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11033. Презентация PowerPoint
Prague, August 16, 2006 . The main GCVS problem is that it is no longer a GENERAL catalogue of variable stars (in fact, it even never was). The GCVS always was a catalogue of galactic variables, with a minor number of extragalactic stars that were included mainly by misunderstandings. ... Recently, many thousands of new variable stars were discovered in automatic survey projects (for example, some 30000 non-GCVS stars solely in the ASAS-3 project). ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0001.htm -- 7.1 Кб -- 04.09.2006
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11034. Презентация PowerPoint
. N.N. Samus . Institute of Astronomy (Russian Acad. Sci.), . Sternberg Astronomical Institute (Moscow University), . and Eurasian Astronomical Society . Problems and Prospects . of the GCVS . The XXVI th General Assembly of the IAU . Prague, Czech Republic . August 16, 2006
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0003.htm -- 8.0 Кб -- 04.09.2006
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11035. Презентация PowerPoint
... Since GCVS IV, there was no new GCVS edition. ... Main reasons for the automatic-survey new variables remaining outside the GCVS for a long time: different level of detail of the classification systems, no perfect software for automatic classification available; individual approach to each star that was always used in the GCVS cannot be applied any longer, but the experience of automatically- updated catalogs evidences for the number of errors ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0004.htm -- 7.3 Кб -- 04.09.2006
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11036. Презентация PowerPoint
Prague, August 16, 2006 . ... The history of variable-star catalogues is a kind of permanent crisis due to wrong decisions (Argelander's system of designating variable stars using letters; the attempt of the 'Astronomische Gesellschaft' to issue catalogues every year; the tradition of globular-cluster variables kept outside the general catalogue; etc.) ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0028.htm -- 6.4 Кб -- 04.09.2006
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11037. Презентация PowerPoint
Prague, August 16, 2006 . ... The GCVS has no IAU financial support since 1994, so we are not discussing money. ... However, it must be finished, with a new modern version prepared for all 'old' GCVS stars, including those from Name-Lists, with current knowledge incorporated and improved classification system applied. ... Also, people like GCVS star names, use them, and want their discoveries to be named. We can ask other people, with better resources than in Russia, to continue. ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0029.htm -- 7.4 Кб -- 04.09.2006
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11038. Презентация PowerPoint
Prague, August 16, 2006 . ... We can decide to merge the GCVS with automatic surveys now. I have already outlined the difficulties and will give some examples illustrating the problems slightly later. Steve Kawaler's suggestion: 'The GCVS personnel might play a role as a `meta-catalog' - a central `index' of survey-based catalogs of variable stars'. ... If we want to have a good meta-catalog, the difficulties I have mentioned in relation to merging the catalogues still should be considered. ...
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Ссылки http://www.sai.msu.su/groups/cluster/gcvs/future/iaupraha.files/slide0030.htm -- 6.3 Кб -- 04.09.2006
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11039. http://www.sai.msu.su/gcvs/gcvs/nl78/5721-t3.txt
# IBVS 5721-t3.txt #Author: Kazarovets, E.V.; Samus, N.N.; Durlevich, O.V.; Kireeva, N.N.; Pastukho va, E.N. #Comment: The 78th Name-List of Variable Stars, Table E3 #IBVSdataKey: name-list No. Name R.A.,Decl., 2000.0 Max Min Type Ref. Epoch Period M-m Spectrum h m s o ' " m m JD200000+ d 780001 V956 Cas 00 05 05.4 +59 39 01. 14.2 17.2 B IS: 001 002 780002 CD Scl 00 06 20.8 -35 17 13. 12.7 14.2 V RRAB 130 004 52068.835 0.57769 20 A0 780003 V439 And 00 06 36.8 +29 01 17. 6.13 ( 0.04 ) V BY 005 DM K0Ve 780004
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Ссылки http://www.sai.msu.su/gcvs/gcvs/nl78/5721-t3.txt -- 181.4 Кб -- 10.08.2006
[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/gcvs/nl78/5721-t3.txt -- 181.4 Кб -- 10.08.2006
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[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/gcvs/nl78/5721-t3.txt -- 181.4 Кб -- 10.08.2006
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11040. http://www.sai.msu.su/gcvs/gcvs/nl78/e2.TXT
V956 Cas = 780001 = NSV 00016 V956 Cas = 780001 = S 10134 CD Scl = 780002 = CSV 5836 CD Scl = 780002 = GSC 06995.00681 CD Scl = 780002 = NSV 00029 CD Scl = 780002 = S 5222 V439 And = 780003 = 1RXS J000636.8+290112 V439 And = 780003 = BD +28 4704 V439 And = 780003 = BS 8 V439 And = 780003 = GSC 01735.00927 V439 And = 780003 = GSC 01735.02532 V439 And = 780003 = Gl 5 V439 And = 780003 = HD 166 (K0) V439 And = 780003 = HIP 544 V439 And = 780003 = IDS 0001.4N2829A V439 And = 780003 = IRAS 00040+2844 V439 And =
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Ссылки http://www.sai.msu.su/gcvs/gcvs/nl78/e2.TXT -- 188.2 Кб -- 04.08.2006
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[ Сохраненная копия ] Ссылки http://www.sai.msu.su/groups/cluster/gcvs/gcvs/nl78/e2.txt -- 188.2 Кб -- 04.08.2006
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