Astronet Ïîèñê ïî àñòðîíîìè÷åñêèì ñàéòàì English Russian
       
        Òî÷íàÿ ôîðìà ñëîâ   Î ïðîåêòå   Ñàéòû   Ñïðàâêà
Íàéäåíî äîêóìåíòîâ: 272610 (174 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.65ñåê.   

Ïðåä. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | Ñëåä.

Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf.

21. Natural Satellites Service. Saturn coorbital satellites ephemerides
Natural Satellites Service. Special ephemerides . Ephemerides of the coorbital satellites of Saturn . for infrared observations . ... It is a good idea to use the disk of Saturn to occult or to eclipse the bright ring and to observe the satellites as they pass through superior conjunction. ... The next epoch when these observations are possible arrives in 2013. ... 2020/01/05 – 2020/03/29, . ... 2033/10/10 – 2033/11/22, . ... New observations of Saturn's coorbital satellites” - Icarus. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://lnfm1.sai.msu.ru/neb/nss/coorb/nsscooa.htm -- 3.7 Êá -- 13.12.2007
Ïîõîæèå äîêóìåíòû

22. ÎÒ×ÅÒ
... Radio astronomical tests of the engineering model of the space radio telescope (SRT) were completed in Pushchino - see Results . ... Monitoring of the development of the upgrade on-board 1.35-cm receiver (R-SRT-1.35 cm): . ... EM Engineering Model . ... OHCFS-SRT Space Radio Telescope On-board Heterodyne and Clock Frequency Synthesizer set . OHFS-SRT Space Radio Telescope On-board Hydrogen Frequency Standard . ORFS-SRT Space Radio Telescope On-board Rubidium Frequency Standard . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.asc.rssi.ru/RadioAstron/archives/2004/month_notic/dec_mar.html -- 23.7 Êá -- 03.11.2011
Ïîõîæèå äîêóìåíòû

23. Accuracy of World positional CCD observations of the numbered minor planets
... Contact A Problem of an estimation of accuracy of the asteroid CCD observations . The Minor Planet Center supported by the Interntional Astronomical Union is the main office for keeping observational data of the small Solar System bodies and their investigations. ... At Pulkovo Observatory we are estimating an accuracy of the CCD asteroid observations obtained by amateurs and professional astronomers all over the World using the MPC database. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.accuracy.puldb.ru/PROBLEM.HTM -- 3.9 Êá -- 05.12.2007
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>104) - www.accuracy.puldb.ru/ )

24. Radio sources identfification
... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://mavr.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Êá -- 02.10.2012
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Êá -- 01.10.2012
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://jet.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Êá -- 01.10.2012
Ïîõîæèå äîêóìåíòû

25. Bright Supernova pages - List of GRB
List of supernova GRB (Gamma Ray Burst) . This is a list of Gamma Ray Burst . ... Page re-generated at: Mon, Mar 28, 2016 8:13:30 PM Earliest Supernova Latest Max SN Host Galaxy Observation R.A. Decl. offset from host Mag Mag Type Reference Discoverer 1998bw ESO 184-G82 1998 04 28 19 35 03.31 -52 50 46.65 0.0 14.0** 13.5 Ib IAUC 6895 ESO aka GRB980425 1997cy Anon. ... 2008 10 07 22 39 50.58 -40 08 48.3 0.0W 0.0S 18.0** 16.4 Ic CBET 1602 M. Della Valle et. el. aka GRB 081007 2009nz Anon. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.rochesterastronomy.org/snimages/grblist.html -- 8.9 Êá -- 29.03.2016
Ïîõîæèå äîêóìåíòû

26. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
[ Òåêñò ]  Ññûëêè http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Êá -- 15.12.2015
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1480) - vo.astronet.ru/ )

27. Àñòðîíîìèÿ â Ñàíêò-Ïåòåðáóðãñêîì óíèâåðñèòåòå |
...  ÷åòâåðã, 14 àïðåëÿ 2016 ã., ñîñòîèòñÿ ñåìèíàð êàôåäðû àñòðîôèçèêè. Ïîâåñòêà äíÿ . ... Íà÷àëî â 11 ÷àñ.15 ìèí. Àóä. ...  ÷åòâåðã, 31 ìàðòà 2016 ã., ñîñòîèòñÿ ñåìèíàð êàôåäðû àñòðîôèçèêè . ...  ÷åòâåðã, 24 ìàðòà 2016 ã. , ñîñòîèòñÿ ñåìèíàð êàôåäðû. ...  ÷åòâåðã, 17 ìàðòà 2016 ã. , ñîñòîèòñÿ çàñåäàíèå êàôåäðû. ... ÎÑÏ ÍÈÈ ÏÌÌ Íàöèîíàëüíîãî èññëåäîâàòåëüñêîãî Òîìñêîãî ãîñóäàðñòâåííîãî óíèâåðñèòåòà) . ... Copyright 2016 Àñòðîíîìèÿ â Ñàíêò-Ïåòåðáóðãñêîì óíèâåðñèòåòå . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astro.spbu.ru/ -- 44.8 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>380) - www.astro.spbu.ru/ )

28. Detection of unique bright radio flare of X-ray binary
... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Êá -- 10.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://mavr.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû

29. Generation from In-Orbit Data
. Next: XAreaEf Up: XPSF Previous: Generation from Ground Calibration Contents . The multi-Gaussian fit is based on in-orbit observations of bright p[oint sources. In particular, it accounts for the triangular shape of the FM2 telescope. The King function parameters have been calculated from fits to the radial profiles of bright point sources observed in-orbit. Michael Smith 2011-09-20
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node663.html -- 3.3 Êá -- 20.09.2011
Ïîõîæèå äîêóìåíòû

30. Optical systems and devices
To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.mao.kiev.ua/lao/optical_systems_eng.html -- 19.6 Êá -- 12.01.2010
Ïîõîæèå äîêóìåíòû

31. http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1366tp.ps
Proposal Identi cation No.: A1366 Date Received: 1999-Sep-27 16:55:20 Technical Page Proposal Type: Regular General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 75 Hours Proposal Title: 21-cm Observations of Nearby Low Surface Brightness Galaxies : Investigating the LSB Tully-Fisher Relation ABSTRACT: In spite of the diôculty in detecting low surface brightness ( LSB ) ...
[ Òåêñò ]  Ññûëêè http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1366tp.ps -- 86.8 Êá -- 19.04.2004
Ïîõîæèå äîêóìåíòû

32. Îáñåðâàòîðèÿ
... GRB060712 ( GCN5303 ) The first R image was at 2006-07-12 21:10:32 UT, 72 s after notice time and 212 s after the GRB time. ... HETE Alert 4006 ( GCN 4549 ) - MASTER promt optical limit time . ... GCN 4173 | ... GRB050410 ( GCN 3221 5 h after Swift GRB trigger time . ... GRB05017 ( GCN 2954 19m at between 2h and 4h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . GRB05017 ( GCN 2953 17m at 2h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://observ.pereplet.ru/work.shtml -- 14.9 Êá -- 27.02.2014
Ïîõîæèå äîêóìåíòû

33. Paul Francis -- Astronomical Constants
... 1 erg = 0.1 microjoules . 1 Jansky = 10**-26 watts per metre square per hertz . 1 Angstrom = 0.1 nanometres . ... 1 Astronomical unit = 1.4960 times 10**11 m . ... Mass of Sun = 1.989 times 10**30 kg . ... Mass of the Earth = 5.976 times 10**24 kg . Mass of Jupiter = 318 times mass of Earth . Solar constant = 1.37 kW per metre . c= 3 times 10**8 metres per second . ... Mass of Proton = 1836.1 times mass of electron . ... Stefan Boltzmann constant = 5.67 times 10**-8 W m**-2 K**-4 . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.mso.anu.edu.au/pfrancis/constants.html -- 2.9 Êá -- 01.10.2012
Ïîõîæèå äîêóìåíòû

34. http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf
Dynamic Shack-Hartmann System RAPID V. G. Orlov, V. V. Voitsekhovich Instituto de AstronomÌa, UNAM, MÈxico CONACYT project E9507-1020P UNAM PAPIIT IN104910 Telescopes OAN OAN- SPM 2.1m telescope 1.5m telescope 0.84m telescope 2.1m telescope OAN-Tonanzintla 1m telescope Astronomical site SPM Observing statistics 1982-2002 (Tapia+ 2007 ) Photometric nights : 64.1% Spectroscopic ... Rapid - Dynamic Shack-Hartmann All modern telescopes demand installation of adaptive system. ...
[ Òåêñò ]  Ññûëêè http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf -- 1652.8 Êá -- 18.10.2010
Ïîõîæèå äîêóìåíòû

35. The COOC Criterion (Criterion of Observations versus Calculations)
... In order to compare the number of different evolutionary stages obtained and X-ray luminosity of the chosen X-ray sources with the observed galactic values we use the sum of C/O+O/C , where C and O are the calculated and observed values of a given binary type, respectively. If we make comparison for a number of different binary species (for example, we compare the number of CV, number of X-ray pulsars,   total X-ray luminosity of LMXB, etc.), we write this criterion in the form: . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://xray.sai.msu.ru/~mystery/articles/review/node43.html -- 5.0 Êá -- 26.02.1997
Ïîõîæèå äîêóìåíòû

36. http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/plates2.pdf
New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...
[ Òåêñò ]  Ññûëêè http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/plates2.pdf -- 1667.0 Êá -- 05.01.2013
Ïîõîæèå äîêóìåíòû

37. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz
... The Co­Addition Technique Applied to Images of Galaxy Cores W. W. Zeilinger Institut f˜ur Astronomie, University of Vienna, T˜urkenschanzstraúe 17, A­1180 Wien, Austria P. Crane, P. GrosbÜl and A. Renzini European Southern Observatory, Karl­Schwarzschild Straúe 2, D­85748 Garching, Germany Abstract. ... One may therefore take full advantage of the high resolution FOC images by co­adding them with (high signal­to­noise) ground­ based data. ... References Crane, P. et al. ...
[ Òåêñò ]  Ññûëêè http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz -- 76.9 Êá -- 12.06.2006
Ïîõîæèå äîêóìåíòû

38. Doug Burke: Publications List
... D. J. Burke and J. Patrick Henry . The Astrophysical Journal, submitted. ... S. Brough, W. J. Couch, C. A. Collins, T. Jarrett, D. J. Burke , R. G. Mann . ... D. A. Wake, C. A. Collins, R. C. Nichol, L. R. Jones, D. J. Burke . ... R. Sadat, A. Blanchard, S. C. Vauclair, D. H. Lumb, J. Bartlett, A. K. Romer, J.-P. Bernard, M. Boer, P. Marty, J. Nevalainen, D. J. Burke , C. A. Collins, R. C. Nichol, . ... S. Majerowicz, D. M. Neumann, A. K. Romer, R. C. Nichol, D. J. Burke , C. A. Collins . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://hea-www.harvard.edu/~dburke/pubs.html -- 16.7 Êá -- 01.10.2012
Ïîõîæèå äîêóìåíòû

39. Astronomy Terms - To Help You Study The Universe - an Astronomy Net Article
Astronomy Terms - To Help You Study The Universe . Articles | ... Learning about the universe, or the study of astronomy, can be fun for the individual or for the whole family. ... Learning a few simple terms will help you with this fascinating study. ... You will use a telescope or binoculars for your observation of the sky at night. ... Celestial Terms . ... Meteor or a shooting star – the light caused when a meteoroid burns up in Earth's . ... www.astronomy.net . About Astronomy Net | ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astronomy.net/articles/33/ -- 16.8 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû

40. AAL Homepage
MAIN PAGE . ... Nova Cygni August 1975! ... 1975/76: Comet West! ... Dr. Richard West (4th from left) & AAL members visiting SES Betzdorf on occasion of our club's 25th anniversary - October 1996 . Comet West Information . ... It was the brightest comet visible from Earth since Comet West in 1976. ... 1997: Comet Hale-Bopp! ... Thus Comet Hale-Bopp never got closer to Earth than Earth gets to the Sun. ... Comet Hale-Bopp JPL Page . ... 1999: Total solar eclipse over Luxembourg! ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.aal.lu/HIGHLIGHTS_1970-2000/ -- 22.1 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>49) - www.aal.lu/ )

Ïðåä. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | Ñëåä.


Àñòðîíåò | Íàó÷íàÿ ñåòü | ÃÀÈØ ÌÃÓ | Ïîèñê ïî ÌÃÓ | Î ïðîåêòå | Àâòîðàì

Êîììåíòàðèè, âîïðîñû? Ïèøèòå: info@astronet.ru èëè ñþäà

Rambler's Top100 RFBR ßíäåêñ öèòèðîâàíèÿ