| Íàéäåíî äîêóìåíòîâ: 286 (41 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.03ñåê. |
Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.puldb.ru/laza_gao/PUB/av_2.pdf.
http://www.puldb.ru/laza_gao/PUB/av_2.pdf.
21. Methods and results of radio cosmology. Appendix 12.
... Ãëàâà 2 . ... Ññûëêà èç Ãëàâû 4 ). ... 4.3 . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://sed.sao.ru/~vo/disser/app12.html -- 10.5 Êá -- 13.03.2007
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2) - sed.sao.ru/ )
22. Eclipse elements for Computer Ephemeris for 2016 (DE200/LE200).
Computer Ephemeris for 2016 from DE200/LE200. Elements of the Partial Lunar eclipse - 18 Aug 2016. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://space.univ.kiev.ua/ephem/16a/180816el.html -- 3.4 Êá -- 28.12.2015
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>8) - space.univ.kiev.ua/ )
23. EIT Server Input File Format
Suppose measuring system has 16 electrodes. ... If the measuring system doesn't perform redundant measurements, as the current injection through electrodes n and m is equivalent to the injection through electrodes m and n , corresponding redundant values should be set to zeros as in the following example: POLAR 16 0.000 0.908 0.513 0.313 0.202 0.280 0.752 0.000 0.000 0.869 0.351 0.243 0.297 0.311 0.340 0.000 0.000 0.000 1.358 0.484 0.205 0.212 0.355 1.214 0.000 ... EIT Gallery ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.cplire.ru/tserver/fileformat.html -- 6.5 Êá -- 12.06.2001
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>3) - www.cplire.ru/ )
24. http://www.mao.kiev.ua/images/postbyemail/IF2014_UA_all.pdf
JCR-Web 4.5 Marked List http://admin-apps.webofknowledge.com/JCR/JCR?RQ=L... 2014 JCR Science Edition MARKED JOURNAL LIST Sorted by: Impact Factor 2014 Total Cites 781 527 1496 395 283 85 195 600 126 130 623 580 446 152 39 201 5-Year Impact Immediacy 2014 Cited Eigenfactor Impact Factor Index Articles Half-life Score Factor 1.245 0.815 0.786 0.748 0.573 0.558 0.379 0.376 0.282 0.231 0.230 0.219 0.195 0.195 0.157 0.136 1.050 0.690 0.741 0.668 0.627 0 ...
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Òåêñò
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Ññûëêè http://www.mao.kiev.ua/images/postbyemail/IF2014_UA_all.pdf -- 62.4 Êá -- 30.06.2015
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
25. http://www.accuracy.puldb.ru/200810/C000.HTM
... 1.7 GSC 104 Italy, San 0.40 21 x 21' 2.5" 94 288 0.452 0.391 Marccello 2.0 GSC 106 Slovenia, 0.36 36 x 36' 2.0" 1265 5660 0.358 0.353 Crni vrh 2.4 USNO 113 Germany, 0.50 13 x 10' 2" 9 35 0.348 0.282 Schonbrunn 2.3 USNO 118 Slovakia, 0.57 14 x 10' 1.7" 7 41 0.154 0.121 Modra 3.3 USNO 122 France, 0.40 No data 8 24 0.100 0.071 Pises Obs. ... 2.2 USNO 715 USA, 0.30 23 x 15' 1.8" 8 27 0.321 0.153 Las Cruces 1.0 USNO 735 USA, 0.46 No data 15 64 0.369 0.246 George Obs. ... Germany 1.8 UCAC A77 Obs. ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.accuracy.puldb.ru/200810/C000.HTM -- 40.4 Êá -- 20.03.2009
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>20) - www.accuracy.puldb.ru/ )
26. Ôèçè÷åñêèå äàííûå ñïóòíèêîâ Óðàíà
ÔÈÇÈ×ÅÑÊÈÅ ÄÀÍÍÛÅ . ÑÏÓÒÍÈÊΠÓÐÀÍÀ . ... 13.70 + 0.04 . ... The masses of Uranus and its Major Satellites from Voyager Tracking Data and Earth-based Uranian Satellite Data," Astronomical Journal 103 , 2068. ... Voyager's Eleventh Discovery of a Satellite of Uranus and Phometry and the First Size Measurements of Nine Satellites", Icarus 151 , 69-77 . ... Uranus Satellites: Surface Properties", In Uranus (J. T. Bergstralh, E. D. Miner, and M. S. Matthews Eds.) pp. ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://lnfm1.sai.msu.ru/neb/rw/natsat/uraphyw.htm -- 29.8 Êá -- 26.06.2006
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>5) - lnfm1.sai.msu.ru/ )
27. http://www.arcetri.astro.it/irlab/luna/firpo/check.ps
... (FIRPO-TIRGO) w/error AR, Sun Aug 24 10:34:33 MET DST 1997 ############################################################# Sp:K4 irc10007 J 1.509 0.028 irc10007 J 1.65+/- 0.06 [ 0.05 ] 0.14 0.09 irc10007 H 0.961 0.006 irc10007 H 1.03+/- 0.04 [ 0.04 ] 0.07 0.05 irc10007 K 0.606 0.040 irc10007 K 0.85+/- 0.05 [ 0.03 ] 0.24 0.09 Sp:M2 irc10024 J 2.099 0.028 irc10024 J 2.31+/- 0.04 [ ...
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Òåêñò
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Ññûëêè http://www.arcetri.astro.it/irlab/luna/firpo/check.ps -- 14.9 Êá -- 28.07.2005
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>10) - www.arcetri.astro.it/ )
28. St.Petersburg optical observations
... Optical calibrations for AZT-8 and LX-200 . ... preliminary . ... 0235+164 . AO 0235+16 . ... 0420 014 . PKS 0420 01 . ... 0528+134 . PKS 0528+134 . ... 0647+250 . 1ES 0647 . ... 0716+714 . S5 0716+71 . ... PKS 0735+17 . ... PKS 1222 . ... PKS 1510 08 . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.astro.spbu.ru/staff/vlar/OPTlist.html -- 99.5 Êá -- 11.09.2012
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2) - www.astro.spbu.ru/ )
29. http://www.gao.spb.ru/english/as/publ/gorshkov_astvest_2007.pdf
... ×. ó. Ùã?Ýã, ÙÞ,Üfl (øëÞÝã,âÝfl) âêãÜãßÛ~ÒâÝfl ãÇâÒ,êãÛfl úÔ÷, ûÜÝê-øÒêÒÇë,, øãâêëäÛÞ , ÒÝ^Û 06.06.2005 ,,. ýÝ ÜÑÀ,ÒßÀÒ ,ãÞÜÀ õÝã,Û^ (Markowitz wobble - MW) äÒâê,Þflê âãÇãØ Ý,ÑÛ,,ßãÜÛ~ÒâÝÛÒ ÝãÞÒÇÜÛfl âÒÜÒ,,ã äãÞâ ñÒßÞÛ â äÒÛããß ãÝãÞã 30 ÞÒê Û ßäÞÛêëãØ 0.02''-0.03''. ûÒ,ÒãÔêÞÜêÛ~ÒâÝãÒ ÝãÞÒÇÜÛÒ (North Atlantic Oscillation - NAO), iÝêÒÛÑëÒßãÒ ÝëäÜãßâ?êÇÜÀßÛ fl,ÞÒÜÛflßÛ , âÛâêÒßÒ êßãâéÒÜã-ãÝÒÜÛ~ÒâÝÛi äã^Òââã, êã,,ã Ò,,ÛãÜ, , â,ã ã~ÒÒÈ, ÛßÒÒê ,Û^ÛÛ fl ßÒêÒããÞã,,Û~ÒâÝÛi äßÒêã, , ?ÛãÝãØ äãÞãâÒ ~âêãê. ...
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Òåêñò
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Ññûëêè http://www.gao.spb.ru/english/as/publ/gorshkov_astvest_2007.pdf -- 451.9 Êá -- 19.11.2012
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>5) - www.gao.spb.ru/ )
30. http://www.iki.rssi.ru/ofo/pdf/preprint_Fobos.pdf
... 100 . ... 500 . 4 , 40 (500600 ) . ... 0.5 ( ). , ~0.2 3 . ... 300 , 5- . ... 5.1. , : , , : , , 12 12 40 40 200 200 8000 8000 0.45 0.45 1.5 1.5 7.5 7.5 300 300 30 100 500 20000 , 6080 2 5 . ... 5.2. : (.. ) (300 ), 670 200 . ... 7.1). 3 1 7.1. 1. 2. 3. 300 4. 3 ( 45 4.5 ) 3 ( 1.2 1 ) 0.51 15 ( 0.20.4 0.6 ) 300 10 10 . ... 7.2. , (10 ). , 0.51 , 0.20.4 200400 , ~15 , 6 , . ... 7.2). , 1 ( ), 5 7 ( ). 7.2. () 10 740 1 35 206 500 18 51 300 11 19 2.1 0.19 0.021 100 30 10 300 , -1 -2 50%, . ...
[
Òåêñò
]
Ññûëêè http://www.iki.rssi.ru/ofo/pdf/preprint_Fobos.pdf -- 957.4 Êá -- 26.05.2008
[ Òåêñò ] Ññûëêè http://www.cosmos.ru/ofo/pdf/preprint_Fobos.pdf -- 957.4 Êá -- 26.05.2008
Ïîõîæèå äîêóìåíòû
[ Òåêñò ] Ññûëêè http://www.cosmos.ru/ofo/pdf/preprint_Fobos.pdf -- 957.4 Êá -- 26.05.2008
Ïîõîæèå äîêóìåíòû
31. http://www.issp.ac.ru/lhpp/PapersMeletov/paper88.pdf
... , 3, Ô. Ô. ÙÛääÛëâ4, ø. Ù. ÷ëßã,1, øãâêëäÛÞ , ÒÝ^Û 12.03.2008 ,,. øãâÞÒ ãÇãêÝÛ 27.05.2008 ,,. 2 ýÒiÜÛ~ÒâÝÛÒ âÞãÚÜãâêÛ äÛ âãÑÜÛÛ ÝÛãâêê Þfl ÛââÞÒã,ÜÛfl ÞÒÝêãÜÜã,,ã äß,,ÜÛêÜã,,ã ÒÑãÜÜâ (.ä..) äÛ ,, ÒÞÛÒ ,Ài êÒßäÒêëi â,flÑÜÀ â ã,,ÜÛ~ÒÜÜÀßÛ ÑßÒßÛ ÝßÒÀ Þfl ãÇÑ ^ã, Û äÑÛêÜÀßÛ âÛ,,ÜÞßÛ ãê ÒÒ ßêÒÛÞ. ùäêÛßÞÈÜÀß Ò?ÒÜÛÒß fl, ÞflÒêâfl ÛâäãÞÈÑã,ÜÛÒ ,ëâêÒÜÜã,,ã Ý,^Ò,ã,,ã , äãßÒÒßã,,ã ,ÜëêÈ ÒÑãÜêã Û âãäflÚÒÜÜã,,ã â êÒäÞããÇßÒÜÜÛÝãß ÝÛãâêê , äÛ êãß ãiÞÚÒÜÛÒ ...
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Òåêñò
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Ññûëêè http://www.issp.ac.ru/lhpp/PapersMeletov/paper88.pdf -- 226.8 Êá -- 18.02.2014
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2) - www.issp.ac.ru/ )
32. http://www.adass.org/adass/proceedings/adass03/reprints/P7-9.pdf
... We present a new technique to segregate old and young stellar populations in galactic spectra using machine learning methods. We used an ensemble of classifiers, each classifier in the ensemble specializes in young or old populations and was trained with locally weighted regression and tested using ten-fold cross-validation. ... In this work we propose a Machine Learning (ML) method to determine the age of stellar populations in synthetic galactic spectra. ... Combine results in an ensemble. ...
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Òåêñò
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Ññûëêè http://www.adass.org/adass/proceedings/adass03/reprints/P7-9.pdf -- 223.0 Êá -- 27.08.2004
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
33. spectrographic optical design
... Optical Prescription . ... Radius=625. 000 Source at infinity s c s n a2 a4 a6 k 1 -8.889e-005 0.00 -1.00028 0.000e + 000 0.000e + 000 3.81e-022 -1.285e+ 000 2 -1.390e-004 -3644.44 1.00028 0.000e + 000 0.000e + 000 1.79e-019 -1.197e+001 3 0.000e + 000 3619.89 1.46080 2.321e-005 -1.173e-010 -7.87e-017 0.000e + 000 4 0.000e + 000 12.00 1.00028 0.000e + 000 0.000e + 000 0.00e+ 000 0.000e + ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19961022_SpecOpticalDesign/19961022.html -- 11.3 Êá -- 18.05.1999
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>4) - www.apo.nmsu.edu/ )
34. http://www.buran.ru/other/ako_06-05.pdf
... × ëÜãß ,ÛÜêÒ Þfl ÑßÒÒÜÛfl ÝÒêÀ ?Ýãâßãâ-ÑÒßÞflË ãÇfiß ÑÝÇÛÜÜã,,ã ãêâÒÝ fl,Üã ÜÒ i,êÞã, Û ãäãÞÜÛêÒÞÈÜÀØ ãÇfiß 2 ß3 Ò?ÛÞÛ äãÞë~ÛêÈ Ñ â~fiê ëßÒÜÈ?ÒÜÛfl Ñäâ êãäÞÛ ,. üÜÀØ ùû Û ÛãÞãÝ^ÛãÜÜÀØ Ñ,Ò~ÛÝ ÛßÒÞÛ Ñ,ã~Û,ÒßÀÒ Ü ãÇÛêÒ ,ÜÒ?ÜÛÒ ÜêÒÜÜÀ, ÝãêãÀÒ âÇâÀ,ÞÛâÈ äÒÒ âiããß â ãÇÛêÀ . ùêÞÛ~ÛêÒÞÈÜãØ ~ÒêãØ ÇãÒ ,Ài ,ÛÜêã, fl,ÞflÞâÈ ,ãÑßãÚÜãâêÈ ,ÀäãÞÜÒÜÛfl ßÜfi, äã ÛÑßÒÜÒÜÛ äÞãâÝãâêÛ ãÇÛêÀ Þfl äã,êãÜã,,ã äãiã Ü ãÜãØ Û êãØ ÚÒ êã~ÝãØ ÑÒßÜãØ äã,ÒiÜãâêÛ (äÛ ,ÀäãÞÜÒÜÛÛ ...
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Òåêñò
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Ññûëêè http://www.buran.ru/other/ako_06-05.pdf -- 393.2 Êá -- 08.04.2010
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>3) - www.buran.ru/ )
35. Magnetic field found on Tau Bootis | Astronomy.com
... Observing . ... Magnetic field found on Tau Bootis . ... The magnetic field of the planet-hosting star tau Bootis. ... They detected that the magnetic field of Tau Bootis, a one billion year old star, has a mass of one and a half solar masses and is located nearly 50 light years from the Earth. ... This is just a little more than the Sun's magnetic field, but in structure, tau Bootis is much more complex than the Sun. ... Only registered members of Astronomy.com are allowed to comment on this...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.astronomy.com/news/2006/11/magnetic-field-found-on-tau-bootis -- 69.4 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
36. http://www.izmiran.rssi.ru/~obridko/papers/348rus.pdf
... 1?ßiÛÜâÝfl ðÑë~ÒÜã âäÒÒÞÒÜÛÒ ß,, ÜÛêÜã ,,ã äãÞfl âãÞÜÒ ~Üã,,ã ,Òê ,ÇÞÛÑÛ ñÒßÞÛ Û âãäãâê,ÞÒÜã â êÒß, ~êã ãÚÛÞãâÈ äã ÝÞââÛ~ÒâÝãØ ßãÒÞÛ. øãÝÑÜã, ~êã ,ëi,Ò?ÛÜÜãâêÈ âäÒÒÞÒÜÛfl ÑÜ~ ÒÜÛØ ßÒÚäÞÜÒêÜã,,ã ß,, ÜÛêÜã ,,ã äãÞfl , ãÇÜëÚÒÜÜfl ÜÒÒ, ÜÒ fl,ÞflÒêâfl êÒéÝêãß ëâÒÜÒÜÛfl, ãêÚÒê ÒÞÈÜë âêëÝêëë ß,, ÜÛêÜã ,,ã äãÞfl ,ÜëêÛ âÒÝêã. øÛ êãß ÇãÞÒÒ ~âêã ,âêÒ~Òêâfl ß,,ÜÛêÜãÒ äãÞÒ äãÞflÜãâêÛ, ... ÕãÞÒÒ êã,,ã ,,Ûâêã,,ßß âêÞ ?ÛÒ Û ÑÜ~ÒÜÛfl ßÝâÛßëßã, (äÛÝã,) Ü Û,,ßßÒ âÒÜÒ~âã,Ài ÑÜ~ÒÜÛØ âããê,Òêâê,ëê Á4.5 ÜýÞ. ...
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Òåêñò
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/348rus.pdf -- 225.3 Êá -- 14.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2) - www.izmiran.rssi.ru/ )
37. http://selena.sai.msu.ru/Kozl/Publications/AstVest5_04KozlovaLO.pdf
... × ÇãêÒ ÛÑë~ÒÜÀ ÝêÒÀ, âäãÞãÚÒÜÜÀÒ , äãÞflÜÀi ãÇÞâêfli õÒÝëÛfl Û óëÜÀ . úââ~ÛêÜ äÞãÈ äãâêãflÜÜã ÑêÒÜÒÜÜÀi ãÇÞâêÒØ , äãÞflÜÀi ØãÜi ãÇãÛi êÒÞ, Þfl óëÜÀ - â ë~Òêãß ÛÑßÒÜÒÜÛØ äãÞãÚÒÜÛfl äãÞâ ,ÒÜÛfl óëÜÀ ãêÜãâÛêÒÞÈÜã äãÞâ ÝÞÛäêÛÝÛ Ñ 18.6 ÞÒê, Þfl õÒÝëÛfl - , êÒ~ÒÜÛÒ ßÒÝëÛÜâÝÛi âãÞÜÒ~ÜÀi âëêãÝ. úââ~ÛêÜÀ ÛÑßÒÜÒÜÛfl êÒßäÒêëÀ , ÝêÒi , âã,äÛi äã âäãÞãÚÒÜÛ â ãÇÞâêflßÛ äã,À?ÒÜÜã,,ã âãÒÚÜÛfl ,ããã Þfl ... 36 ÝêÒã, âãÒÚê äãâêãflÜÜë êÒÜÈ, äÞãÈ ÝãêããØ âãâê,ÞflÒê ßÒÜÒÒ 10% ãê äÞãÛ ÝêÒ. ...
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Ññûëêè http://selena.sai.msu.ru/Kozl/Publications/AstVest5_04KozlovaLO.pdf -- 851.3 Êá -- 22.04.2013
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2) - selena.sai.msu.ru/ )
38. Journal Impact Factors
. Ïîðòàë | Ñîäåðæàíèå | Î íàñ | Àâòîðàì | Íîâîñòè | Ïåðâàÿ äåñÿòêà | Äèñêóññèîííûé êëóá | Íàó÷íûé ôîðóì | Îòïðàâèòü îòêðûòêó . Ïåðâàÿ äåñÿòêà "Ðóññêîãî ïåðåïëåòà" Òåìû äíÿ: . | Îáðàùåíèå ê Äìèòðèþ Îëåãîâè÷ó Ðîãîçèíó ïî òåìå "êîñìè÷åñêèå óãðîçû": êàê ñäåëàòü ñèñòåìó ïðåäóïðåæäåíèÿ? . Ðåéòèíã ó÷åíûõ Ðîññèè . Êîíêóðñ êóðèðóåò ïðîôåññîð ÌÃÓ Â.Ì. Ëèïóíîâ . Ìåñòî ó÷àñòíèêà êîíêóðñà îïðåäåëÿåòñÿ àâòîìàòè÷åcêè ñ ó÷åòîì ìèðîâîãî óðîâíÿ ïóáëèêàöèé ó÷åíîãî. Ïîñòàâüòå íàø áàííåð . Íàóêà â "Ðóññêîì ïåðåïëåòå" . Ïðåæäå,
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Ññûëêè http://www.pereplet.ru/nauka/sciall/impact95-98.shtml -- 223.6 Êá -- 11.04.2016
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
39. http://www.sao.ru/blcat/
... Data Usage Policy . ... Export main Table and RATAN-600 data . ... RATAN data . ... Blazar type . ... Data explorer . ... LSP . BLac . RBL . ... BL~Lac . ... BL~Lac~cand. ... ISP . ... XBL . ... BLac.can . ...
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Ñîõðàíåííàÿ êîïèÿ
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Ññûëêè http://www.sao.ru/blcat/ -- 177.1 Êá -- 09.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://mavr.sao.ru/blcat/ -- 177.1 Êá -- 09.04.2016
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[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://mavr.sao.ru/blcat/ -- 177.1 Êá -- 09.04.2016
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40. http://vega.inp.nsk.su/catalogs/tycho.pdf
... Contents of the Tycho Catalogue Over view of the Tycho Catalogue: The Tycho Catalogue provides astrometr y (positions, parallaxes and proper motions) and two-colour photometr y (in B T and VT ) for more than one million stars brighter than VT = 11.5 mag. ... Stars in ver y dense clusters and other dense fields thus leaving the resulting Tycho Catalogue incomplete in such regions `R' in Field T42). ... The number of non-Hipparcos stars with Tycho Catalogue parallaxes larger than 40 + 4 mas is 1245. ...
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Ññûëêè http://vega.inp.nsk.su/catalogs/tycho.pdf -- 159.4 Êá -- 12.01.2000
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