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1. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/anchor.htm
... JavaScript 1.2: added name , text , x , and y properties Using the HTML A tag or calling the String.anchor method. The JavaScript runtime engine creates an Anchor object corresponding to each A tag in your document that supplies the NAME attribute. It puts these objects in an array in the document.anchors property. ... A string specifying the anchor's name. text . ... The horizontal position of the anchor's left edge, in pixels, relative to the left edge of the document. y . ... Anchor . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/anchor.htm -- 13.7 Кб -- 07.10.1999
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2. Long description for example illustrating positioning with respect to a
This diagram illustrates the effects of absolutely positioning a box ("inner") with respect to a containing block established by a relatively positioned ancestor ("outer"). ... The "inner" box has been positioned relative to the top and left edges of the "outer" element's first inline box. ... The reference edges for positioning the "inner" box are indicated in the diagram by thick dashed lines. ... 1 Beginning of body contents.| ... 4 [(+200, -100)] 5 Inner 6 contents. ... Inner contents" is blue. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/css2/images/longdesc/flow-abs-rel-desc.html -- 2.9 Кб -- 08.05.1998
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3. Zen: CASDB
... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/oddmuse/index.cgi/CASDB -- 11.9 Кб -- 11.04.2016
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4. STDA files
... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/descr/stda.htm -- 14.7 Кб -- 12.05.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/descr/stda.htm -- 14.7 Кб -- 12.05.1999
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5. Database of Optical Properties -- Level: subpage
A small paper prepared by V.Tishkovets, P.Litvinov, and S.Beletsky (Kharkov Univ., Ukraina) provides the reader with a brief description of the problem, its solution, the developed software and its training (the PDF version of the paper is here ). ... Please, select the PAS subdirectory for the Pascal version of the code, and the FORT subdirectory for the Fortran version. A brief description of files and their purposes is given in our user notes (their PostScript version is here ). ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/A-PERC/ -- 2.6 Кб -- 19.11.2010
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6. Suppression of detector noise at low energies
... While there is practically no detector noise present at energies above , X-ray data below are considerably contaminated by noise events, which become more and more dominant towards the lowest transmitted energies (Fig. ... Investigations of 40 hours of in-orbit calibration data with the filter wheel closed, taken over a period of more than two years, showed that the noise properties vary with position and energy, but are fairly stable in time for most areas on the detector. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/epreject/node7.html -- 10.4 Кб -- 15.11.2007
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7. POLARIZATION PROPERTIES OF TWO PULSARS
Polarization properties of two pulsars R. N. Manchester (ATNF, CSIRO, Australia) . ... Abstract Mean pulse polarization properties at 1.4, 4.6 and 8.3 GHz and rotation measures are presented for two pulsars with unusually wide profiles. PSR J0437-4715 is a millisecond pulsar with significant emission over at least 80% of the pulse period. It shows a complicated variation of linear position angle across the pulse indicating substantial departures from a dipole field structure. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Simon.Johnston/papers/poln.html -- 2.4 Кб -- 02.10.2012
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8. patriot 12 meter telescope
... File format . ... The p12mProg is the AO control program for the 12 meter telescope. ... the time from the tick, till when we complete the status read from the device. ... P12M_STAT_BLK struct (read from controller via group read at tick) . ... azimuth master 32bit status word . ... dbl . ... azimuth error read from controller. ... azimuth velocity read back from controller deg/sec . ... elevation position read back from controller. stBlk.elErr_D . ... elevation velocity read back from controller . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/software/datataking/p12m/logFileFmt.html -- 28.6 Кб -- 28.01.2015
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9. Chapter 3: Fixed and Generic Targets
Table 3.1: Designations of Special Targets . Table 3.2: Target Categories . Table 3.3: Descriptive Keywords for STAR and EXT-STAR . Table 3.4: Descriptive Keywords for STELLAR CLUSTER and EXT-CLUSTER . Table 3.5: Descriptive Keywords for GALAXY . ... Table 3.13: Bright-Object Constraints . The use of "FIXED_TARGETS" and "GENERIC_TARGETS" are described in this chapter. ... In this chapter, each heading has a description followed by a keyword in square brackets (e.g., [ Number] ). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/P2PI/ch03_targ_fixed.html -- 8.2 Кб -- 22.05.2008
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10. Stellarium: SatellitesListFilterModel Class Reference
Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... SatellitesListFilterModel Class Reference . Custom proxy model allowing filtering by satellite group and flag. ... getFilterFlag () const . ... setFilterFlag (const SatFlag &flag) . QStringљ . ... setFilterGroup (const QString &groupId) . ... setSecondaryFilters (const QString &groupId, const SatFlag &flag) . ... Definition at line 27 of file SatellitesListFilterModel.hpp . ... QString SatellitesListFilterModel::filterGroup . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classSatellitesListFilterModel.html -- 12.1 Кб -- 28.02.2014
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11. Spatial Region Coordinates
... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/RD/funtools/regcoords.html -- 8.7 Кб -- 01.10.2012
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12. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/indiutil/getINDI.1
TH getINDI 1 .SH NAME getINDI \- get INDI property values .SH SYNOPSIS \fBgetINDI [options] [device.property.element ...]\fP .SH DESCRIPTION .na .nh .PP getINDI connects to an indiserver and reports the current value of one or more properties. ... PP The last component of the property specification is usually the element name, but may be a reserved name to indicate an attribute of the property as a whole. ... TP -p <p> connect using alternate port p; the default is 7624. ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/indiutil/getINDI.1 -- 4.3 Кб -- 03.08.2011
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13. LHPP ISSP RAS
... About: Dr. Antonov was born in Ryazan in 1950; graduated in Solis State Physics from the Faculty of General and Applied Physics of Moscow Institute of Physics and Technology in 1973; got a PhD degree in 1977 and the degree of Doctor of Sciences from the Institute of Solid State Physics RAS in 1985. ... 1973 – 1975 Probational Researcher, ISSP RAS, Chernogolovka . ... 2003 – present Head of the Laboratory of High-Pressure Physics, ISSP RAS, Chernogolovka . ... LHPP ISSP RAS © 2004 All rights reserved...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lhpp/antonoven.html -- 9.3 Кб -- 31.03.2016
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14. V652HER AND MERGED BINARY WHITE DWARF MODELS
Next: DIRECT MASSES FOR BXCIR Up: EXTREME HELIUM STARS: PULSATION Previous: PULSATION PROPERTIES . As already indicated, V652Her is an important EHe star because its relatively short pulsation period and large amplitude pulsations allow its overall dimensions to be determined with high precision. ... Saio & Nomoto (1998) made the first successful models for the merger of two carbon-oxygen white dwarfs, and prompted Saio & Jeffery (2000) to attempt models for the merger of two helium white dwarfs. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/research/ehe_review/node6.html -- 13.7 Кб -- 25.01.2002
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15. Methods and instruments to measure/monitor major site properties
... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...
[ Сохраненная копия ]  Ссылки http://site2010.sai.msu.ru/section/2 -- 9.2 Кб -- 09.04.2016
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16. Orbital Properties of the Solar System
. Mars is "behind" the sun from the earth's point of view and is therefore not visible in the nighttime sky (i.e. its up in the daytime). Venus it at greatest elongation and appears in the western sky as a bright object for 2-3 hours after sunset .
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/disted/ph121/l4.html -- 5.5 Кб -- 06.01.2005
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17. Be/X-ray binaries and candidates
... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~raguzova/BeXcat/ -- 5.8 Кб -- 09.01.2015
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18. The ROSAT AGN
... We present 5GHz high resolution VLA observations of 2,127 radio-- and X-ray--emitting sources found in both the Green Bank (GB) 5GHz radio catalog and the ROSAT All-Sky Survey (RASS). We report core flux densities and positions accurate to =-0.5". ... This table has 1861 rows and 9 columns giving: Catalog source name, RA and DEC (J2000), observation code, S/N ratio, VLA core flux density at 5 GHz (mJy), Green Bank flux density at 5 GHz (mJy), error in Green Bank flux density (mJy), and Notes. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/ROSAT_Laur.html -- 3.8 Кб -- 18.03.2015
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19. Calculating the Position and Velocity Components of HST
... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/aket.html -- 12.3 Кб -- 03.11.2000
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20. CO in NGC 1530, aperture synthesis of a barred spiral
... NGC 1530 is one of the largest barred spiral galaxies in the northern sky, with bright CO emission. ... To trace molecular gas, we observed the line, with the IRAM Interferometer. ... Properties of NGC 1530 and observational results . ... Then in a frame rotating with the potential, the periodic orbits are ellipses either parallel to the bar ( ) or perpendicular ( ), depending on the radius of the orbit. ... We observed the molecular gas in the bar of NGC 1530, a barred SBb spiral in the line. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/reynaud/reynaud.html -- 12.6 Кб -- 08.12.2003
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