Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 444757 (198 сайтов) ---- Время поиска: 1.62сек.   

Пред. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.eso.org/~ppadovan/survey/dxrbs_paper/node7.html.

21. GRB follow-up team
... Team . ... GRB mini-workshop 2006 . ... On April 8, 2005, an optical afterglow of the GRB 050408 was discovered with the SAO's telescopes (the 1-meter telescope Zeiss and 6-meter telescope BTA) within the framework of a joint BTA request (SAO RAS + IAA CSIC, Granada, Spain) on optical identification of gamma-ray bursts. We first detected a variable object only by our own data in the localization error-box reported by the space observatory HETE and then it was confirmed by our observations in SAO. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/grb/followup/GRB050408/GRB050408.html -- 7.1 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/grb/followup/GRB050408/GRB050408.html -- 7.1 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/grb/followup/GRB050408/GRB050408.html -- 7.1 Кб -- 10.04.2016
Похожие документы

22. Contributions by amateurs: SN1996X.
Visual Discovery of SN 1996X in NGC 5061. ... It was not until the IAU Circular was issued that we found out there had been an independent amateur photographic discovery of this supernova by Kesao Takamizawa of Japan. ... Earlier in the week, 660 galaxies had been observed during two nights we had use of the 40 inch telescope at Siding Spring. ... The supernova in NGC 5061 was first seen with the smaller telescope about 10pm local time on Friday, April 12 (April 12.5 UT). ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/1996x.htm -- 6.8 Кб -- 02.02.2012
Похожие документы

23. VISTA - Visible and Infrared Survey Telescope for Astronomy
... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...
[ Сохраненная копия ]  Ссылки http://www.vista.ac.uk/ -- 31.7 Кб -- 27.11.2014
Похожие документы
Еще в разделе: (Показать все результаты (>28) - www.vista.ac.uk/ )

24. Telescope nights at Armagh Planetarium | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . Colin Johnston . ... Telescopes and Observatories . ... January . ... By admin February 20, 2013 Posted in: Armagh Planetarium . ... M42, the Great Nebula in Orion, imaged through Armagh Planetarium?s telescope in January 2013. ... Image credit: Colin Johnston/Armagh Planetarium) . ... M31, the Andromeda Galaxy, imaged with the new telescope in January 2013. ... Armagh Planetarium?s new telescope in action in January 2013. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/telescope-nights-at-armagh-planetarium.html -- 48.1 Кб -- 09.04.2016
Похожие документы

25. A malfunction in one of the TESIS telescopes has been fixed
... Specialists from the TESIS Control Centre, at the FIAN Laboratory of Solar X-ray Astronomy, have succeeded in fixing a malfunction in one of the observatory's central telescopes, which occurred in the second half of May. ... The main version of events pointed to a malfunction in the drive mechanism's reducer, which is responsible for the rotational power from the main shaft of the motor to its output shaft, which is connected to the shutter. ... The TESIS observatory ї TESIS: www.tesis.lebedev.ru . ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/info/tesis_20090602_en.php -- 8.6 Кб -- 01.10.2012
Похожие документы

26. University of Louisville Research Telescope Photo Gallery
The telescope configured for measurements of exoplanet transit light curves is seen from the north side in this May 2010 photo. Lower portions of the dome have been insulated to reduce daytime heating by radiation from the warm metal dome. ... The interior of the dome is seen soon after the encoder upgrade in February 2007. ... Karen Collins, a research astronomer specializing in exoplanets, helped with the telescope installation in August 2006. ... kielkopf at louisville dot edu . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/rc24/rc24_gallery/index.html -- 5.3 Кб -- 11.05.2010
Похожие документы

27. Description of the RadioAstron project, english version
Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/support_eng.htm -- 14.3 Кб -- 10.05.2008
Похожие документы

28. A Night At The Telescope
... The computer is set up so that the software for whatever camera is running and the switch box set to channel B. This allows the monitor and keyboard upstairs to operate the computer. Now the telescope can be set up. ... In the North west of the dome, there is a motor that turns the dome. The dome opens with a motor that pulls the slit back. ... Each camera had a specific alignment with the telescope. ... The lights on the roof provide a nice target to center in all three telescopes. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node72.html -- 6.3 Кб -- 01.10.2012
Похожие документы

29. Remote telescopes
.
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~dmbiz/Lrobot.html -- 2.4 Кб -- 22.02.2003
Похожие документы
Еще в разделе: (Показать все результаты (>219) - comet.sai.msu.ru/ )

30. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt
... STScI-PR98-15 HUBBLE REVEALS DETAILS OF A NEWLY BORN PLANETARY NEBULA Astronomers have caught a peek at a rare moment in the final stages of a star's life: a ballooning shroud of gas cast off by a dying star flicking on its stellar light bulb. NASA's Hubble Space Telescope has captured the unveiling of the Stingray nebula (Hen-1357), the youngest known planetary nebula. ... A fast wind - material propelled outward from the hot central star -- compresses the gas and pushes the gas bubble outward. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt -- 6.4 Кб -- 30.01.2001
Похожие документы

31. HET: The New Largest Optical Telescope
Astronomy Picture of the Day . ... 26.12.1996 . ... To peer into our cosmos' unknown depths, astronomers must deploy new tools - and the classic new tool is a larger telescope. Pictured above is the new Hobby-Eberly Telescope (HET) which recently declared "first light" in western Texas. HET currently has the largest single mirror of any optical telescope -- 11 meters in diameter. ... HET 's huge size, on the other hand, allows it to see very dim objects and determine their spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/apod/1996-12-28 -- 14.6 Кб -- 11.01.2013
Похожие документы

32. Pulkovo NEO Page: Estimation of Accuracy of the Observations
Pulkovo NEO Page . ... NEA Accuracy Estimation . ... The estimation of accuracy of the current CCD observations of asteroids and comets is constantly performed at Pulkovo Observatory. ... The (O-C) values, so called "Observed" minus "Calculated" positions, characterize numerically the observations of any observatory, both professional and amateur, during a short period (one or several close nights). ... So the (O-C) values for these objects nearly entirely define the errors of observations. ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/personal/neo/eng/accuracy/p01.htm -- 9.8 Кб -- 26.11.2013
Похожие документы
Еще в разделе: (Показать все результаты (>335) - www.gao.spb.ru/ )

33. Three-telescope interferometry allows astrophysicists to observe how black
... Observing . ... Behemoth black hole found in an unlikely place . ... black holes . ... Three-telescope interferometry allows astrophysicists to observe how black holes are fueled . ... This three-telescope interferometry is a major milestone toward directly imaging the growth phase of supermassive black holes," said Sebastian Hoenig from the University of California, Santa Barbara, one of the astrophysicists who utilized this technique to observe the AGN at the center of galaxy NGC 3783. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2012/05/three-telescope-interferometry-allows-astrophysicists-to-observe-how-black-holes-are-fueled -- 69.9 Кб -- 10.04.2016
Похожие документы

34. Technical Details
... Technique of supervision of solar atmosphere active formations with the Multichannel Flare Spectrograph. Consider in details now a method of observations of fast processes in solar chromosphere with Multichannel Flare Spectrograph (MFS) installed in Ondrejov Observatory (Czech Republic). ... The working spectral range lies between IR CaII 8542 A and K CaII 3870 A. To observe solar image on the spectrograph's slit a lens, narrow-band H-alpha filter (4) ("Daystar") and CCD-chamber are used. ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/~kupry/technote.html -- 5.7 Кб -- 13.01.2009
Похожие документы
Еще в разделе: (Показать все результаты (>580) - lnfm1.sai.msu.ru/ )

35. III International Astronomy Olympiad, Problems to solve
Text of these problems is available also in other languages : . ... What can one see in the Moon's sky more often - the Sun or the Earth? ... There are about of 250 millions of stars in the elliptical galaxy M32 (a satellite of Andromeda galaxy). ... The masses of Capella's components. ... You are proposed to estimate the masses of Capella's components, using our observational data. ... A galaxy's mass. ... Estimate the mass of FGC 1908 and compare it to the mass of our galaxy. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/iao/1998/problems/vi98us_e.html -- 13.6 Кб -- 15.04.2011
Похожие документы

36. Magnification (Power) And Using Eyepieces - an Astronomy Net Article
Magnification (Power) And Using Eyepieces . ... To determine power in a telescope, divide the focal length of the telescope by the focal length of the eyepiece. By exchanging an eyepiece of one focal length for another, you can increase or decrease the power of the telescope. For example, a 25mm eyepiece used on a telescope with a 1000mm focal length would yield a power of 40x (1000 / 25 = 40) and a 10mm eyepiece used on the same telescope would yield a power of 100x (1000 / 10 = 100). ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/articles/26/ -- 17.6 Кб -- 09.04.2016
Похожие документы

37. Posting to VSNet
Posting Observations . ... You will need to subscribe to vsnet-acc (to allow you access to post your observations). ... VSNet has several different e-mail sigs, and sub sigs. ... These list are controlled by a software package called " Majordomo ", which allows you to subscribe and unsubscribe yourself from these list with an e-mail message (automated). ... Once you have subscribed to vsnet-acc (which will only send you a welcome message back and nothing else) you can post to the other list. ...
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/vsnet.html -- 11.3 Кб -- 10.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>899) - www.rochesterastronomy.org/ )

38. Radioastrophysical Observatory ISTP RAS SB
RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Possibilities of observing . ... Investigations of the SSRT 5.7 GHz radio maps in conjunction with images obtained in other emission ranges, suggested the following conclsions: . ... Solar images obtained in line H a ;(on the left, 16:11 UT, Big Bear observatory) and in the microwave emission (on the right, 04:04 UT, SSRT) 4 march 1997 . ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/rad22en.shtml -- 16.1 Кб -- 27.02.2014
Похожие документы
Еще в разделе: (Показать все результаты (>42) - ssrt.iszf.irk.ru/ )

39. (Untitled)
When entering Identification section user should open the file with observed positions of objects which are to be identified (the file may be first created). ... Format of observations must coincide with that of optic observations in which they are published by Minor Planet Center (observed position may be presented as “accurate” or “approximate” one): . ... observed right ascension (in hours, minutes, and seconds of time (“accurate position”) or in hours and minutes (“approximate position”) . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user712s.htm -- 3.4 Кб -- 10.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>762) - www.ipa.nw.ru/ )

40. Astro-2 and the UIT Experiment
... Note on Filters: . ... NGC 3351 is a mostly face-on late type spiral galaxy. It is marked by a bar like feature in its central regions and a strong inner ring of star formation. ... The galaxy was imaged through the A1,B1 and B5 filters over a total exposure time of 1936 seconds. ... The galaxy was imaged through the A1 filter for 450 seconds and the B1 filter for 1084 seconds. ... The galaxy was imaged through the A1 and V1 filters over a total exposure time of 1200 seconds. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/uit-t3.html -- 4.9 Кб -- 07.10.1996
Похожие документы

Пред. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | След.


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования