... The table that contains the event data - need to at least contain the columns named with the xcolumn , ycolumn , ecolumn parameters. colortablechoice . ... Choice parameter determining source of the color table that is to be used for the color coding. ... The name of the column that specifies the position of the event; passed to evselect as parameter xcolumn . ... The name of the column that specifies the scalar event attribute that is to be color-coded; passed to evselect as parameter zcolumn . ...

Еще в разделе: (Показать все результаты (>32372) - xmm.vilspa.esa.es/ )

Next: A New IRAF Catalog Access Tool for Astrometry . Up: Iraf Packages . ... Twofitlines is a tool developed within IRAF, optimized to be used with data containing multiple spectra along the spatial axis of the detector. A given spectral feature can be decomposed in one or several Gaussian components. ... A given spectral feature can be modeled using one or more components (currently only Gaussian profiles are available), . ... Close spectral features could be modeled simultaneously. ...

Еще в разделе: (Показать все результаты (>1993) - www.adass.org/ )

• ASC Data Analysis Architecture
• Building Software from Heterogeneous Environments
• Calculating the Position and Velocity Components of HST

... C CUse: C VOIGT gives the value of a multi-component gaussian. ... 1 CDERIV(1)- DERIV (3) -part. derivs. of component 1 C PAR (1+3*n)- PAR (3+3*n)-int,pos. of peak,dopp. fwhm ,lor. fwhm of cmp. n-1 C etc C C ---------------------------------------------------------------- CC C@ real function voigt ( real , real , integer ) C@ subroutine dvoigt( real , real , real , integer ) C FUNCTION VOIGT (X, PAR , NPAR ) N. 2 * SQRT ( LN(2) ) PARAMETER ( ...

Еще в разделе: (Показать все результаты (>16191) - www.atnf.csiro.au/ )

• uvsfit
• uvfit
• imfit

The wave complex KEM-3 is designed to measure the parameters of electromagnetic waves in the VLF and ULF ranges. ... The electric antenna is a 1.6 m long dipole made up by two spherical carbon EDS detectors each with a preamplifier. ... The same detector is also used for the VLF device. ... 1. component Ex: 0.1 Hz - 400 kHz; 5*10E(-8)HzE(-1/2) (2 kHz). 2. component Bx: 1.0 kHz - 50 kHz; 10E(-5) nT*HzE(-1/2) (2 kHz). 3. components Bx,y,z: 1.0 Hz - 2 kHz; 3*10E(-5) nT*HzE(-1/2) (100 Hz). ...

Еще в разделе: (Показать все результаты (>1015) - www.cosmos.ru/ )

• WAVE EXPERIMENTS ON TAIL PROBE

Find Similar Abstracts (with default settings below ) . ... Also-Read Articles . ... Parameters of the 41 Dra system components . ... 00/2001 . ... Stars: Binaries, Binaries: Fundamental Parameters, Binaries: Individual . ... 61B Based on spectral and speckle-interferometric observations of the system 41 Dra, model atmosphere parameters of the system components have been derived: component Aa - T eff = 6500K, lg g = 3.99, R = 1.87 R solar , component Ab - T eff = 6500K, lg g = 4.11, R = 1.61 R solar . ...

Еще в разделе: (Показать все результаты (>773) - jet.sao.ru/ )

• Spectrometric complex LRS

Next: Format of the Up: Auxiliary Data Previous: Description of the . For convenience in table handling only values for single lines or doublets (most of the observed cases) can be entered. If higher multiplicities are actually needed small changes have to be made in the table and program format. Possibility for 50 different atomic transitions. N.B. : in case of doublets, columns 3, 5, 7, 9, and 11 refer to the reddest component, and columns 4, 6, 8, 10 and 12 to the bluest. ...

Еще в разделе: (Показать все результаты (>2131) - www.sao.ru/ )

• HyperLEDA documentation: parameter: vmaxs
• Multivariate Statistical Methods
• HyperLEDA documentation: parameter: objtype

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

Еще в разделе: (Показать все результаты (>666) - www.ssau.ru/ )

... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

Еще в разделе: (Показать все результаты (>40071) - vo.astronet.ru/ )

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

Еще в разделе: (Показать все результаты (>422) - xray.sai.msu.ru/ )

• Change of Binary Parameters: Mass, Semi-major Axis and Eccentricity
• Other parameters of the evolutionary scenario
• Initial binary parameters

Irregular phenomena in the Earth Pole oscillation process and temporal variations of geopotential Valery Bondarenko, Vadim Perepelkin s The observed irregular phenomena in the Earth Pole oscillation process are very variety. ... These phenomena indicated in the IERS data are the "abnormal" fluctuation of the Earth Pole coordinates which owing to changing of the geodynamical parameters gives negative result in interpolation and forecast of the first approximation mathematical model. ... Fig. ...

Еще в разделе: (Показать все результаты (>279) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/publ/miller_malkin_ivsgm-2008.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/zotov.pdf
• Phase light curves of young binary systems

Next: A Simple Example With Up: CHIRPLET TRANSFORM SUBSPACES Previous: CHIRPLET TRANSFORM SUBSPACES . We begin by discussing the CF plane, and then present an argument for re-parameterizing this plane in terms of two frequency indices, leading to what we will be calling ``frequency-frequency'' (FF) analysis. ... Computing the CF plane of a signal, s ( t ), is equivalent to correlating the signal with a family of chirps that are parameterized by chirprate, c and center frequency, . ... Figure 7 . ...

Еще в разделе: (Показать все результаты (>1224) - crydee.sai.msu.ru/ )

• SunSoft
• Footnotes
• Notation

In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

Еще в разделе: (Показать все результаты (>527) - www.cplire.ru/ )

• Getting Started in Actor Prolog. Analyzing Web Sites.
• Research Activities of InformChaos Lab.
• Getting Started in Actor Prolog. Component-Oriented Programming.

... Observers may find that they wish to perform parts of the pipeline reduction again on their data using these tasks. Typical examples will be to re-perform cosmic ray rejection, altering the input parameters or using data from separate datasets, or to perform one-dimensional spectral extraction on long-slit data or to modify the input parameters (e.g., aperture extraction box, or background region) when doing one-dimensional spectral extraction for echelle data. ... Rectify spectral images. ...

Еще в разделе: (Показать все результаты (>14556) - www.stsci.edu/ )

• An Ultraviolet-to-Radio Broadband Spectral Atlas of Nearby Galaxies
• CCD Parameters table
• CSPICE Routines: VPACK_C

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Measured radial velocities for the primary (full symbols) and secondary (empty symbols), phased with the orbital period of 5.9051102 0.0000023 days. ... HD 98088 is a synchronised, double-lined spectroscopic binary system with a magnetic Ap primary component and an Am secondary component. ... The magnetic field in the primary is predominantly dipolar, with the positive pole oriented approximately towards the secondary. ...

Еще в разделе: (Показать все результаты (>1510) - star.arm.ac.uk/ )

... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...

Еще в разделе: (Показать все результаты (>202) - mavr.sao.ru/ )

• IRAS01005+7910
• Hardware sector, archive 2004
• Galaxy sector, archive 2006

True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... parameters were derived from bright shell at N . Abundance of O-like element was set to zero asumming Typ1 I SN( Hughes et al., 1995 ). source=(xswabs * xsvraymond) . reduce chi^2 = 7.41398 . ... DataSet 1: 153 data points -- 144 degrees of freedom. Statistic value = 1067.61 . ... DataSet 3: 90 data points -- 76 degrees of freedom. ... Back to SNR J0519.5-6902 Index . Chandra Supernova Remnant Catalog . ...

Еще в разделе: (Показать все результаты (>2533) - hea-www.harvard.edu/ )

• The AstroStat Slog ICA
• The AstroStat Slog Blog Archive [MADS] Law of Total Variance
• *search_grid* - Grid of - default mode

The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...

Еще в разделе: (Показать все результаты (>580) - www.ipa.nw.ru/ )

• Keywords_75
• IAA EOP Service

... Wind Baffle Parameters . ... As part of this analysis, the volume, mass, center of gravity and mass moment of inertia of the telescope and optics support structure (OSS) were computed. ... The total moment of inertia of the circular floor panel, wind baffle and telescope in azimuth should be correct to 30% but is dependent on estimates of the mass of equipment supported below and above the circular floor panel. ... Table 8 : Masses and mass moments of inertia of the wind baffle components. ...

Еще в разделе: (Показать все результаты (>460) - www.apo.nmsu.edu/ )

• lsst.coordConv: coordConv::Coord Class Reference

Next: Coherent integration Up: Astrometry data reduction Previous: Introduction Contents . ... In order to increase the SNR for these data, we coherently integrate the complex visibility for typically 200 ms. The coherent integration is done using the COBRA procedure cohstrictor . In order to provide the necessary input file for this step, the following CONSTRICTOR parameters should be used. ... The .coh extension is standard for coherent integration. ... NumAv = 100. ... Pass on metrology data . ...

Еще в разделе: (Показать все результаты (>13495) - www.eso.org/ )

• The Hierarchical Stellar Systems Model Format
• OYSTER Lab
• TQS tools: documentation and tools

... Velocity allipcoid parameters as functions of heigt above the Galactic disk for the complete sample of F -stars (left) and a young ( t 3 Gyr) metal-rich ( [Fe/H] -0.13 ) group (reght). ... next figure | previous figure . ...

Еще в разделе: (Показать все результаты (>83) - ip.rsu.ru/ )

• Vladimir Marsakov Abstracts