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http://www.atnf.csiro.au/news/newsletter/jun02/USNO_ATNF_VLBI.htm.

1. Description
... This task operates on event data in an event list. ... In the first two cases, the celestial coordinates of the reference point are taken respectively as the values of the RA_NOM , DEC_NOM or RA_OBJ , DEC_OBJ values in the input event file header. ... Although the OM attitude information may be more accurate, it will not be present throughout part of the observation, and as such, the default source for the attitude data should be "ahf". ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/attcalc/node3.html -- 11.0 Кб -- 28.06.2006
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Еще в разделе: (Показать все результаты (>9944) - xmm.vilspa.esa.es/ )

2. http://www.stsci.edu/~valenti/idl/struct_add_field.pro
pro struct_add_field, struct, tag, data, before=before, after=after $ , itag=itag ;Add a new field to an existing structure. ... Append new field . if itag gt 0 then begin ;target field occurs first new = create_ struct ( tags [0], rec.(0)) ;initialize structure for i=1, itag -1 do begin ;insert leading unchange new = create_ struct ( new , tags [i], rec.(i)) endfor new = create_ struct ( new , tag , data [0]) ;add new field endif else begin new = create_ struct ( ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~valenti/idl/struct_add_field.pro -- 5.6 Кб -- 22.06.2011
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3. http://www.atnf.csiro.au/computing/software/gipsy/tsk/rfits.dc1
Program: RFITS Purpose: Load FITS files from tape into a GIPSY set. ... Keywords: *** AUTO= Try to run in automatice mode [Y]. ... NODATA= Create only set headers [N]. ... Example: USER RFITS ,AUTO=N USER RFITS ,INTAPE=IMPORT USER RFITS ,INFILES=31 USER RFITS ,OUTSET=NGC4214 USER RFITS ,CTYPE1=RA-NCP USER RFITS ,CUNIT1= USER RFITS ,LIMITS1= USER RFITS ,GRID1= USER RFITS ,CTYPE2=DEC-NCP USER RFITS ,CUNIT2= USER RFITS ,LIMITS2= ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/tsk/rfits.dc1 -- 8.2 Кб -- 02.01.2000
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4. Blue Compact Galaxies from the Hambyrg/SAO Survey
Hamburg/SAO Survey (HSS) for Emission-Line Galaxies - New Wide-Angle Search for Blue Compact Galaxies (BCG) . ... New project named Hamburg/SAO Survey extends study of blue compact galaxies to new large wide-angle sample based on digitized objective-prism photoplates of the Hamburg Quasar Survey (HQS). ... 60%) of observed emission-line objects in accordance to the idea of use objective-prism wide-field surveys as favorable technique to search for narrow emission-line galaxies . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Current/HSS_eng.html -- 11.5 Кб -- 28.12.2006
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5. Heiles Symposium Presentations
P. Frisch - Warm partially ionized interstellar gas at the Sun . ... W. M. Goss - Time variations in small-scale galactic HI structure toward 3C138 . S. Stanimirovic - Does tiny-scale atomic structure exist in the ISM? ... T. Bania - The distance to molecular clouds via HI self-absorption . ... C. Heiles - Arecibo Millennium Survey statistics of magnetic field, column density and turbulence in the CNM . R. Crutcher - Magnetic fields in molecular clouds . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/heiles/Scientific_Presentations.html -- 7.2 Кб -- 23.08.2006
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6. Potential Energy
... This appartus will drop a mass from different heights. When the mass strikes the ground, some percentage of its original energy will be absorbed by the ground. ... The mass of the object (Mass) . The percentage of the energy which is absorbed by the surface on each "bounce" (EAS) . ... Start= Drop the ball after Energy, Mass and EAS have been set; resume after step or pause has been selected . Step = Drop the ball once and it rebounds to its maximum height and then pauses . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1998/ph101/pe1.html -- 5.4 Кб -- 13.10.1998
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7. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The low-resolution, Cassegrain mounted, FORS spectropolarimeter of the ESO Very Large Telescope is being extensively used for magnetic field surveys. Some of the new discoveries suggest that relatively strong magnetic fields may play an important role in numerous physical phenomena observed in the atmospheres as well as in the circumstellar environments of certain kinds of stars. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2013/640.html -- 7.2 Кб -- 09.09.2013
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8. What Really Exists Outside The Universe - an Astronomy Net Observation_reports
Astronomy Discussion Forums . ... What Really Exists Outside The Universe . ... Post Message | ... Picture a bowl of marbles. ... Each of the spheres in your marble bowl represents a single universe. Now in reality these marble spheres exist infinitly in numbers and are not limited to some sort of cosmic bowl. ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/observation_reports/messages/286.shtml -- 15.8 Кб -- 09.04.2016
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9. Lagrangian Points
... With enough velocity, a spacecraft can break loose from the Earth's gravity and enter an orbit around the Sun, like that of a planet. If it then orbits the Sun with the same period as the Earth--one year--it may keep a fixed position relative to Earth. ... If the distance is just right--about 4 times the distance to the Moon or 1/100 the distance to the Sun--the spacecraft, too, will need just one year to go around the Sun, and will keep its position between the Sun and the Earth. ...
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/Education/wlagran.html -- 11.9 Кб -- 24.03.2006
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10. Organization of data
... The data inside CHAMELEON is organized in tables (e.g. ScanTable), structures (e.g. GenConfig), arrays of structures (e.g. scans), and plain arrays (e.g. VisSq). ... RawData: unaveraged, typically 2 ms integrations, flat arrays (bin counts, laser positions, quad cell counts) . ... ScanData: scan averaged data ( scans, bgscans ), output from CHAMELEON, as well as data used in AMOEBA, velocities (spectrosopy) , positions (relative astrometry), magnitudes (photometry), arrays of structures . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node216.html -- 6.8 Кб -- 28.04.2015
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11. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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12. Lagrangian Points
... With enough velocity, a spacecraft can break loose from the Earth's gravity and enter an orbit around the Sun, like that of a planet. If it then orbits the Sun with the same period as the Earth--one year--it may keep a fixed position relative to Earth. ... If the distance is just right--about 4 times the distance to the Moon or 1/100 the distance to the Sun--the spacecraft, too, will need just one year to go around the Sun, and will keep its position between the Sun and the Earth. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/Education/wlagran.html -- 11.9 Кб -- 21.12.2007
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13. XWare > APOD
... Starting in the 1400s astronomers erected large instruments here to enable them to measure star and planet positions with increasing accuracy. ... A new star, likely the brightest supernova in recorded human history, appeared in planet Earth's sky in the year 1006 AD. ... Alpha Centauri: The Closest Star System . ... The closest star system to the Sun is the Alpha Centauri system. Of the three stars in the system, the dimmest -- called Proxima Centauri -- is actually the nearest star. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=71&d=2005-02 -- 14.8 Кб -- 12.04.2016
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14. astro-ph
... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=T. -- 19.7 Кб -- 13.04.2016
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15. Data analysis and Spatial Corrections
Next: A Preliminary Investigation Up: Spatial Corrections of ROSAT Previous: Introduction . ... These tasks bin a time sorted photon event list based on an assigned phase that corresponds to the 402 second period of the wobble. ... The fundamental limitation of this method is how many source counts you have for centroiding each binned image section. ... Once the phase binned qpoes have been shifted in x,y so as to align the source centroid, they are restacked using 'qpappend_ftsi'. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node199.html -- 5.3 Кб -- 01.10.2012
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16. lsst.tcc: tcc::GuideProbe Class Reference
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Classes . Files . ... GuideProbe . ... tcc::GuideProbe Class Reference . include < inst.h > . ... std::tr1::array < double, 2 >љ . ... does this probe exist? ... std::tr1::array <double, 2> tcc::GuideProbe::ctr . ... bool tcc::GuideProbe::exists . ... std::tr1::array <double, 2> tcc::GuideProbe::maxXY . ... std::tr1::array <double, 2> tcc::GuideProbe::minXY . ... double tcc::GuideProbe::rot_gim_ang . ... std::tr1::array <double, 2> tcc::GuideProbe::rot_gp_xy . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/classtcc_1_1_guide_probe.html -- 14.5 Кб -- 14.09.2015
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17. Dynamic HTML in Communicator
Contents] [Previous page] [Next page] Index] . This book describes how to use Dynamic HTML to incorporate style sheets, positioned content, and downloadable fonts in your web pages. ... Introducing Style Sheets . ... Style Sheets in Communicator . Using Cascading Style Sheets to Define Styles . ... Defining Style Sheets with the <STYLE> Tag . Defining Style Sheets in External Files . ... Combining Style Sheets . ... Style Sheets Ink Home Page . ... Positioning HTML Content Using Styles . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/dhtml/dynhtml/contents.htm -- 9.5 Кб -- 13.08.1997
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18. Data bases of Natural Satellites. Documentation. Structure
Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/DocStructe.htm -- 11.4 Кб -- 18.05.2009
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19. Laboratory of spectroscopy of defect structures ISSP RAS
... Kveder V.V. Corresponding member of RAS, Professor, Dr.S. director of ISSP, professor . 118 ГЛК . ... Bredikhin S.I. Dr.S. deputy director, head of LSDS . 115 ГЛК . ... Dolganov V.K. Dr.S. principal research scientist . ... Gasparov V.A. Dr.S. leading senior scientist . ... Kedrov V.V. Dr.S. leading senior scientist . ... Turanov A.N. Dr.S. leading senior scientist . ... Shevchenko S.A. Dr.S. senior scientist . ... Steinman E.A. Dr.S. leading senior scientist . ... senior scientist . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lsds/en/personal.html -- 13.1 Кб -- 09.04.2016
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20. http://www.mso.anu.edu.au/pfrancis/string/ausrelease.doc
... The remote area was formed very early, at a time when the Universe was a fifth of its present age and the presence of the galaxy string defies existing models, which can not explain how a string this big could have formed so long ago. ... The simulations tell us that you cannot take the matter in the early Universe and line it up in strings this large," Dr Francis said. ... But in the early Universe, most galaxies had not yet formed, and most dark matter clouds will not yet contain a galaxy. ...
[ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/string/ausrelease.doc -- 69.0 Кб -- 06.01.2004
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