Найдено документов: 238201 (166 сайтов) ---- Время поиска: 0.42сек. |
Показаны документы, содержащие фрагменты текста из документа
http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6EB58216-43A8-44DE-99AB-7C5558758C0B%7D.
http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6EB58216-43A8-44DE-99AB-7C5558758C0B%7D.
1. ESO - ESO-MIDAS Releases and Distribution
... Public . Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Publications with ESO Data . ... ESO-MIDAS . ... The short statement of the GNU license is included in every MIDAS file; the full text is included as a separate file in the ESO-MIDAS Release. ... Manual pages,installation guides and other documentation are generally released together with the source code and can also be obtained from the ESO-MIDAS ftp account (see below). ...
[
Сохраненная копия
]
Ссылки http://www.eso.org/sci/software/esomidas/midas-distrib.html -- 27.7 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>66223) - www.eso.org/ )
2. Siding Spring Survey
T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...
[
Сохраненная копия
]
Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>487) - www.mso.anu.edu.au/ )
3. Distribution Policy
... The MIDAS system is available, free of charge, to all non--profit research institutes, whereas other organisations or companies may be charged a nominal fee to cover distribution. Institutes interested in using MIDAS must sign a User Agreement before they receive MIDAS. The necessary forms can be obtained by contacting the Data Analysis Group at ESO/Munich. ... The current system at ESO/Munich is frozen several months prior to the official release. ...
[
Сохраненная копия
]
Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node9.html -- 5.5 Кб -- 23.02.1996
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1016) - www.sao.ru/ )
4. http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf
... The areas between the contours were measured automatically. The results of the measurement are represented on fig.1 The graphic shows the distribution of the height levels against their areas. ... USGS, USA Fig.1 The dependence of the distribution of the heights levels versus the area occupied Fig.2 The distribution of the areas of heights levels in the northern and southern hemispheres Fig.3 The distributions of the areas heights levels in eastern and western hemispheres of Mars ...
[
Текст
]
Ссылки http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf -- 166.4 Кб -- 06.10.2008
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>116) - selena.sai.msu.ru/ )
5. Spectral energy distribution
... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...
[
Сохраненная копия
]
Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
Похожие документы
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node8.html -- 17.5 Кб -- 01.10.2012
Похожие документы
Еще в разделе:
(Показать все результаты (>657) - jet.sao.ru/ )
6. NStars2A: Proper motions - the NLTT and 2MASS
... We are obtaining Cousins (B)VRI photometry for the brighter southern stars. Initial results from observations of stars from NLTT sample 1 were obtained from the South African Astronomical Observatory, and are presented by Reid, Kilkenny Cruz (AJ 2002). ... Figure C2.2 compares the 2MASS near-infrared and SAAO optical photometry of the NLTT dwarfs against data for well-studied nearby stars. ... Weis . ... Bessell, M.S. Weis, E.W. 1987, PASP 99, 642 . ... NStars proper motions index . ...
[
Сохраненная копия
]
Ссылки http://www.stsci.edu/~inr/nstars2c.html -- 11.7 Кб -- 08.06.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>12975) - www.stsci.edu/ )
7. Test of the Initial Mass-Ratio Distribution
Next: Phenomenological Kick Velocity Up: Restrictions on the Scenario Previous: The COOC Criterion (Criterion . ... The results of testing and parameters without kick velocity are presented in the form of "topographical maps" (i.e. as isolines) of constant ``COOC'' criterion in the plane calculated separately for each of the binary species listed in Table 4 (Figures 16 - 20 ). The total COOC criterion calculated with equal weights is shown in Figure 21 . ...
[
Сохраненная копия
]
Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node44.html -- 11.0 Кб -- 26.02.1997
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>357) - xray.sai.msu.ru/ )
8. *qpspec* - Extraction of Photon Distributions from QPOE files
Next: Spectral Extraction of Point Up: Spectral Analysis Previous: Structure of the Spectral . A pulse height distribution can be extracted from a QPOE file only if the event structure is `large', `region', or `full'. ... With the new RDF format files, the output from qpspec for most instruments is split into three files: . ... source off-axis histogram . ... background off-axis histogram . For Einstein IPC, there are no off-axis histogram files, but there is a BAL histogram file, _bal.tab. ...
[
Сохраненная копия
]
Ссылки http://hea-www.harvard.edu/PROS/PUG/node141.html -- 6.2 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1632) - hea-www.harvard.edu/ )
9. The summary plot of time distribution of the multisatellites magnetic
The summary plot shows the monthly time distribution of all predicted magnetic conjugations between four spacecraft considered. ... To show the time of conjugation, in frame of the corresponding day for each SC the corresponding colour and line are used: . for the first SC the red color and the first line are used, . ... On the plot the SC names are shown by the corresponding colours. The summary plot permit to find the simultaneous magnetic conjugations of 3 and even 4 satellites. ...
[
Сохраненная копия
]
Ссылки http://www.iki.rssi.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
Похожие документы
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/descr/sumplot.htm -- 2.5 Кб -- 19.11.1999
Похожие документы
Еще в разделе:
(Показать все результаты (>1037) - www.cosmos.ru/ )
10. HIPASS Bright Galaxy Catalog
B?rbel Koribalski (ATNF) + HIPASS and ZOA teams . Velocities are color coded in bins of 1000 km/s: . dark blue . ... light blue . cross . 1000 . green . ... HVCs? ... All the new galaxies, most of which are at |b| All the new galaxies are marked in blue, HI clouds in green and HVCs in orange. (plot by Malte Marquarding, aips++). bkoribal @ atnf.csiro.au ...
[
Сохраненная копия
]
Ссылки http://www.atnf.csiro.au/people/bkoribal/BGals/sky_distribution.html -- 3.3 Кб -- 02.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>6662) - www.atnf.csiro.au/ )
11. http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf
Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...
[
Текст
]
Ссылки http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf -- 1659.8 Кб -- 24.09.2008
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>365) - www.mao.kiev.ua/ )
12. The Network Time Protocol (NTP) Distribution
... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...
[
Сохраненная копия
]
Ссылки http://www.sai.msu.su/~er/xntp/ -- 8.7 Кб -- 21.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2786) - www.sai.msu.su/ )
13. Starlink's Software Distribution System
... Up: Software Systems and Tools . ... The Starlink Software is a collection of astronomical packages and utilities comprising over 120 separate components. When built, the system needs between 500 and 650 MB disk space (without source) making it ideal for distribution on CD-ROM. Each component has been individually packaged into an easy-to-install bundle for users to obtain over the Internet via a ``point and click'' WWW interface from the Starlink Software Store. ...
[
Сохраненная копия
]
Ссылки http://www.adass.org/adass/proceedings/adass98/blymj/ -- 10.9 Кб -- 16.07.1999
Похожие документы
Похожие документы
14. weight on turret floor
The weight and positions for the objects on the rotary floor were obtained from ecastro on nov03 and used to plot the weight distribution on the rotary floor. ... The figure shows the weight distribution by turret position. ... Fig 1 top: Each object on the floor is plotted with its weight vs its turret position. Fig 1 middle: The weight is averaged by turret position quadrant to show the imbalance in weight distribution. ... The turret position is that of the receiver or read off of the drawing. ...
[
Сохраненная копия
]
Ссылки http://www.naic.edu/~phil/turret/turretweight.html -- 8.2 Кб -- 20.06.2013
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1929) - www.naic.edu/ )
15. The Galaxy Gallery Page VII: Infrared Imaging
.
[
Сохраненная копия
]
Ссылки http://zebu.uoregon.edu/ir.html -- 4.7 Кб -- 07.10.1996
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>214) - zebu.uoregon.edu/ )
16. Distribution (ImageJ API)
... Class . ... FRAMES NO FRAMES All Classes . ... FIELD | CONSTR | METHOD . DETAIL: FIELD | ... java.lang.Object ij.plugin.Distribution . ... public class Distribution . ... This plugin implements the Analyze/Distribution command. ... This method is called when the plugin is loaded. void . ... Constructor Detail public Distribution () . ... This method is called when the plugin is loaded. 'arg', which may be blank, is the argument specified for this plugin in IJ_Props.txt. ...
[
Сохраненная копия
]
Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/Distribution.html -- 12.0 Кб -- 02.12.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>246) - www.astro.louisville.edu/ )
17. Index of /lk/source
... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...
[
Сохраненная копия
]
Ссылки http://scan.sai.msu.ru/lk/source/ -- 2.9 Кб -- 09.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3) - scan.sai.msu.ru/ )
18. Spatial dependence and averaging
... The task calculates an average RMF over the spatial region used to extract the source spectrum. ... Essentially a grid is placed over the source region and the redistribution parameters calculated at each point. ... By means of command line parameters the averaging may be performed assuming that the flux distribution is that of the point spread function (PSF), a flat uniform distribution or it may be defined explicitly by supplying the task with an image containing the source region. ...
[
Сохраненная копия
]
Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/rmfgen/node10.html -- 6.9 Кб -- 02.07.2008
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3806) - xmm.vilspa.esa.es/ )
19. (Untitled)
To construct two-dimension distribution of minor planets user should specify elements/ parameters/ function that will be plotted as abscissas and ordinates. In three-dimension case one should add to them the element plotted on Z axis. ... Though you may choose elements plotted along different axes at will, often there is good reason to plot such elements as a, n, or n" along X axis (two-dimension distributions) and to plot them along Y axis in three-dimension case. ...
[
Сохраненная копия
]
Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user8zse.htm -- 3.4 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>438) - www.ipa.nw.ru/ )
20. How do galaxies form? - New discovery from European Southern Observatory |
Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Stars . ... Space Flight . ... A galaxy is born: This artist's impression shows a young galaxy, about two billion years after the Big Bang, accreting material from the surrounding hydrogen and helium gas and forming many young stars. ... Galaxies, distant from us in space and time, have been in the news recently. ... Astronomers at the European Southern Observatory have observed another process which helped primordial galaxies grow. ...
[
Сохраненная копия
]
Ссылки http://www.armaghplanet.com/blog/another-galaxy-far-far-away-seen-by-hst-and-eso.html -- 42.6 Кб -- 09.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2787) - www.armaghplanet.com/ )
Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
Комментарии, вопросы? Пишите: info@astronet.ru или сюда