Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 219786 (169 сайтов) ---- Время поиска: 0.52сек.   

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

Показаны документы, содержащие фрагменты текста из документа
http://www.stsci.edu/software/tinytim/tinytim_faq.html.

1. ESO - Why do I get the message that "no slits could be detected", even though
... Data Handling and Products > Data Reduction FAQ > Why do I get the message that "no slits could be detected", even though in the raw frames I can clearly see the slits? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... ESO Annual Reports . ... Seminars at ESO Santiago . ... Seminars at ESO Garching . ... ESO Telescope Bibliography . ... Last Update: 04.04.14 ESO . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/data-processing/faq/why-do-i-get-the-message-that-no-slits-could-be-detected.html -- 22.5 Кб -- 10.04.2016
Похожие документы

2. CIMA Frequently Asked Questions
Why are there different versions of CIMA? Which version of CIMA should I choose? ... There is no CIMA log in my project directory --- what happened? ... If You are a normal, happy observer, You should choose the CIMA version with the highest version number, since that version contains the latest improvements and bug fixes. ... This means that programs like the data quick-look display and various ALFA instrument displays all exist in several versions just like the CIMA observing session itself. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~cima/cima_faq.html -- 8.2 Кб -- 01.03.2012
Похожие документы

3. K-band Arcetri Obscured Supernova Search - Detected Supernovae
Detected Supernovae . The search have produced till now the detections of 4 SNe. ... This result highlights the power of infrared monitoring in detecting Obscured SNe and indicates that optical surveys are probably missing a significant fraction of SNe, especially in obscured systems such as starburst galaxies. ... In Fig. we show the archival SOFI image of NGC3256 (left) and the first image obtained in 2001 (right) where SN2001db has been detected. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/SNe/supernovae.html -- 8.2 Кб -- 02.10.2008
Похожие документы
Еще в разделе: (Показать все результаты (>8795) - www.arcetri.astro.it/ )

4. Zeiss Gd20 last observed
. Click on star markers for catalogue data. Zeiss 20sm guide last observed FITS -image with WCS-header. Source image . Detected objects . Catalogue objects . Overlay . DSS1 .
[ Сохраненная копия ]  Ссылки http://www.sao.ru/tb/webcam/zeiss_gd20.html -- 8.3 Кб -- 05.08.2015
Похожие документы

5. ASKAP Frequently Asked Questions
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Quickly find out more about ASKAP with answers to these 'frequently asked questions': . ... Once built, ASKAP will form part of CSIRO's Australia Telescope National Facility along with existing telescopes at Parkes, Narrabri and Mopra. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/projects/askap/faq.html -- 52.2 Кб -- 08.04.2016
Похожие документы

6. XWare > APOD
... LP 944-20: A Failed Star Flares . ... The Crab Nebula in Blue and White . ... Comet LINEAR Extends . ... Many sky watchers are closely following Comet C/1999 S4 LINEAR and wondering if it will develop an impressive tail or become visible to the naked eye later this month. ... Comet C/1999 S4 LINEAR is rapidly approaching both the Earth and the Sun from the outer Solar System, and should be at its brightest around 2000 July 25 in the early evening sky of northern observers. ... 1999 2000 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=82&d=2002-09 -- 15.5 Кб -- 12.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>53152) - www.astronet.ru/ )

7. XMM Science Objectives
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/science_top.html -- 1.5 Кб -- 12.11.1998
Похожие документы
Еще в разделе: (Показать все результаты (>4432) - xmm.vilspa.esa.es/ )

8. Stars as Observed in the Infrared
The figure below shows what stellar spectra are like in this wavelength range. All stars hotter than about 3000 K effective temperature radiate like a hot blackbody at these long wavelengths, possibly with a very few atomic lines (of Hydrogen, in the A-type stars) or molecular bands (the CO band overtone near 2.25 microns for example, in K-type stars and G-type stars). ... unusual features: mixed chemistry sources, Wolf-Rayet stars, ice bands, featureless carbon-star spectra ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/stars.html -- 4.1 Кб -- 14.06.2010
Похожие документы

9. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Radio luminosity - spectral type plot for all ultracool dwarfs observed at 4.9 GHz. ... Whilst no radio emission was detected from any of the targets, significant upper limits were placed on the radio luminosities that are below the luminosities of previously detected ultracool dwarfs. Combining our results with those from the literature gives a detection rate for dwarfs in the spectral range M7 тАУ L3.5 of тИ® 9%. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2012/625.html -- 7.1 Кб -- 20.11.2012
Похожие документы

10. Detection of Radio Transients and Variable Radio Sources Using the Archive Data
... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
Похожие документы

11. http://hea-www.harvard.edu/~saku/Telescope.pdf
Basic observing: Sky flats==twilight flats. Good because get uniform light. Bad because very short time available to obtain. Also may get stars within the field; for this do several different sky patches and take the mode or median. Dome flats. ... Bad because sometimes illumination is not good enough (Saku question: what is good?) Dome flats scale by integration time. Lamps for wavelength calibrations frequently. Acquire object frequently. Sky flats==twilight flats. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~saku/Telescope.pdf -- 16.4 Кб -- 01.03.2011
Похожие документы

12. SKA-3 Results Page
SKA-3 instrument consists of two energy-angle ( EA ) electrostatic analyzers and two energy-mass ( EM ) time-of-flight analyzers. ... Here you can find more details about SKA-3 instrumentation set. ... Case 218 . ... satellite's trajectory in geomagnetic frame ( blue coloured), UFSIPS scan location and observation moment ( red coloured), interval of the SKA-3 observations ( green coloured) . ... a view of the Nothern polar region at the moment of UFSIPS observations, the scan location is red coloured. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/ska-3.htm -- 8.3 Кб -- 07.08.1997
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/ska-3.htm -- 8.3 Кб -- 07.08.1997
Похожие документы

13. Has dark matter ever been detected in or around the Milky Way Galaxy? |
... Gravitational wave search provides insights into galaxy evolution and mergers . ... milky way . ... Astronomy for Kids . ... Has dark matter ever been detected in or around the Milky Way Galaxy? ... While some scientists claim theyт??ve seen evidence of a т??windт?? of dark-matter particles, most members of the astronomy community believe this was a false detection and direct observation of this mysterious material hasnт??t happened yet. ... Get instant access to subscriber content on Astronomy.com!...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/News-Observing/Ask%20Astro/2013/01/Dark%20matter.aspx -- 63.3 Кб -- 10.04.2016
Похожие документы

14. http://comet.sai.msu.ru/~gmr/AC/AC1573.pdf
ASTRONOMICHESKII TSIRKULYAR No.1573, 2010 April 12 1995 2009 . A Comparison of the Latitudinal Variations of the Methane Absorption Bands on Saturn's Disk at Equinoxes 1995 and 2009 Abstract. The observations of Saturn at last equinox 2009 have detected significant differences of the latitudinal variations of the methane absorption from observed at 1995 equinox . ... 1995 . 2008- 2009 , ­ . ... 4 ( 580-880 ) , (.1) , 2008-2009 . ... 2 , 4 725 1995 2009 . ... 1995 2009 15 , 1980 1995 . ...
[ Текст ]  Ссылки http://comet.sai.msu.ru/~gmr/AC/AC1573.pdf -- 236.4 Кб -- 06.03.2012
Похожие документы
Еще в разделе: (Показать все результаты (>40) - comet.sai.msu.ru/ )

15. Discussion
Next: Gamma-Ray Bursts Up: Detection rate of binary Previous: Detection rate of binary . Figure: A schematic dependence of the detection rate ratio on the detector sensitivity (the upper scale) and the limiting distance from which binary NS (1.4+1.4M , the middle scale) and binary BH (8.5+8.5M , the bottom scale) mergings can be detected. ... At the end of this segment evolutionary effects can affect the detection ratio (the dashed line). ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/kionewht/node11.html -- 6.7 Кб -- 16.06.2000
Похожие документы

16. Astro-2 and the UIT Experiment
We report here on those proposed UIT targets that, in fact, were successfully acquired. ... Note on Filters: . A1 centered at 2500 angstroms with a width of 1200 angstroms . ... Sextans A is a low mass dwarf companion to the Milky Way Galaxy. It is sufficiently close that it is easily resolved into its individual stars. ... An exposure of 1100 seconds through the A1 and B1 filters was obtained. NGC 2903 Is a relatively nearby mostly face-on galaxy with active star formation. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/uit-t4.html -- 3.5 Кб -- 07.10.1996
Похожие документы
Еще в разделе: (Показать все результаты (>315) - zebu.uoregon.edu/ )

17. Amateur Telescope Makers of Boston
... A star party is a gathering of amateur astronomers who set up their telescopes and observe the dynamic night sky. ... Star parties are best scheduled during first quarter and waxing gibbous Moon. During full moon, the moon is so bright it obscures a view of other celestial objects and even the Moon is best viewed when NOT full. ... We will consult local weather forecasters and make a decision by 2:00p on the day of the star party. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
[ Сохраненная копия ]  Ссылки http://www.atmob.org/library/starparties.php -- 9.6 Кб -- 09.04.2016
Похожие документы

18. APOD: 2012 September 5 - Airglow Over Germany
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2012 September 5 . Airglow Over Germany . ... Explanation: Does air glow? ... Pictured above between the beige clouds, above the curving Earth, behind the streaking airplane, and in front of the sparkling stars are some green bands of airglow . ... About APOD | ... NASA Official: Phillip Newman Specific rights apply . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap120905.html -- 5.7 Кб -- 03.02.2013
Похожие документы

19. Pink Black Holes: Frequently Asked Questions
... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/pink/FAQ.html -- 6.9 Кб -- 01.10.2012
Похожие документы

20. 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. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
Похожие документы
Еще в разделе: (Показать все результаты (>69) - vo.astronet.ru/ )

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 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