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http://www.sai.msu.su/gcvs/gcvs/GCVS5/ReadMe.htm.

1. General Catalogue of Variable Stars: Vols I-III (the new electronic version).
New GCVS Versions for Three Southern Constellations Peremennye Zvezdy (Variable Stars) 27, No. ... We are currently working on a version of the General Catalogue of Variable Stars (GCVS) revised taking into account the new data accumulated since the 4th GCVS edition. ... It will contain all stars of the 4th GCVS edition plus a complete catalogue of the stars added to the GCVS in the Name Lists of Variable Stars Nos. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/gcvs/gcvs/GCVS5/ReadMe.htm -- 12.1 Кб -- 08.12.2010
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2. CSPICE Routines: OSCELT_C
... Abstract Determine the set of osculating conic orbital elements that corresponds to the state (position, velocity) of a body at some epoch. ... In general, the elements found by this routine can have two kinds of problems: - The elements are not accurate but still represent the input state accurately. ... One recommended "sanity check" on the outputs is to supply them to the CSPICE routine conics_c and compare the resulting state vector with the one supplied to this routine. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~sontag/spicedocs/cspice/oscelt_c.html -- 9.9 Кб -- 17.12.2005
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3. casacore: casa::TableMeasOffsetDesc Class Reference
... Classes . ... Definition of a Measure Offset in a Table . ... TableMeasOffsetDesc (const Measure &offset) . ... Get the (non-variable) measure offset for this column. ... Create the Measure column to be used as the measure offset column TableMeasValueDesc valDesc(td, "OffsetCol" ); TableMeasDesc<MEpoch> offset(valDesc); // Create the offset descriptor TableMeasOffsetDesc offsetDesc(offset); . ... All measures in the columns will have the same offset. casa::TableMeasOffsetDesc::TableMeasOffsetDesc . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1TableMeasOffsetDesc.html -- 43.1 Кб -- 14.02.2011
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4. Description
... The radial PSF distribution of the filter FilterId is tabulated in the extension PSF- FilterId . ... radial PSF of U-filter . ... radial PSF of UVW1-filter . ... radial PSF of UV grism 1st order (TBC) . ... The value of the cumulative PSF is normalized to 1.0 at this fixed aperture radius. The aperture radius is listed for each filter elements in the keyword APERTURE. ... Therefore the aperture radius is listed separately for each filter in the keyword APERTURE of the filter extensions. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node948.html -- 10.1 Кб -- 20.09.2011
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5. http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf
... We present a pro ject of an Information system on binary stars (ISBS). ... Stars from the following catalogues will be included in the first version of ISBS: Catalog of orbital elements , masses and luminosities of close double stars ( Svechnikov Bessonova 1984); The catalogue of approximate photometric and absolute elements of eclipsing variable stars ( Svechnikov Kuznetsova 1990); The catalogue of orbital elements , masses and luminosities of detached main-sequence ...
[ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf -- 96.0 Кб -- 27.08.2004
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6. Journal "Peremennye Zvezdy"
Peremennye Zvezdy ( Variable Stars ) 33 , No. ... I present the discovery of an eclipsing component in light variations of the known High-Amplitude Delta Scuti star GSC 1374-01131 based on the Catalina Surveys publicly available data. ... From a single night of their observations, the variable was classified as a HADS (High-Amplitude Delta Scuti) star, with the light elements: . ... The light curves of GSC 1374-01131 based on Catalina data, folded with periods of pulsations and eclipses. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1279785 -- 11.4 Кб -- 12.02.2013
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7. Introduction to Astronomy
Subject of Astronomy. ... Celestial Sphere. ... Spherical Frames of Reference: Horisontal and Equatorial Coordinates, Ecliptical System. ... Transformation of Celestial Coordinates. ... Change of Object Coordinates as a Result of Diurnal Rotation of Celestial Sphere. Phenomenons, Which Lead to Celestial Coordinates Change. ... Motion of Equator, Ecliptic, and Their Poles. ... Diurnal Solar Motion on Different Latitudes. ... Time Equation. ... Apparent Motions and Configuration of Planets. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/vstup_do_astr_e.html -- 7.1 Кб -- 23.02.2005
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8. Principal Components Analysis
... Among the objectives of Principal Components Analysis are the following. dimensionality reduction; љ . the determining of linear combinations of variables; љ . ... identification of groups of objects or of outliers. ... Finding a set of principal axes allows the objects to be adequately characterised on a smaller number of (artificial) variables. ... Reduction of dimensionality is practicable if the first new axes account for approximately 75 % or more of the variance. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node213.html -- 7.2 Кб -- 23.02.1996
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9. 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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10. IBIS: Technical Description
The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/IBIS/IBIS_description.html -- 33.6 Кб -- 13.12.2015