Next: Pass band integrations Up: Fit scenarios Previous: Triple with velocity curves Contents . Fit all three masses, as well as the inclination of one of the pairs. That not any combination of orbital inclinations is allowed can be seen from the fact that the triple consists of two double-lined binaries and only one mass solution exists for a given inclination. ... Christian Hummel 2015-04-28 ...

Еще в разделе: (Показать все результаты (>17080) - www.eso.org/ )

• How DFS components access databases

. Next: CALgetEncircledEnergy Up: CALgetPSFmap Previous: Output Contents . For the SciSim CCF, one of the following CCF components shall be used depending on the selected telescope. XRT1_XPSF_????_SCISIM.CCF XRT2_XPSF_????_SCISIM.CCF XRT3_XPSF_????_SCISIM.CCF For the XMM CCF, one of the following CCF components shall be used depending on the selected telescope. XRT1_XPSF_????_SCISIM.CCF XRT2_XPSF_????_SCISIM.CCF XRT3_XPSF_????_SCISIM.CCF . Michael Smith 2011-09-20

Еще в разделе: (Показать все результаты (>6096) - xmm.vilspa.esa.es/ )

• RGS Related CAL Routines
• List of CCF Components used
• Components

Properties of the interstellar gas clouds . ... The angular resolution of this Survey was 2.4' x 130', velocity resolution was 6.3 km/s, r.m.s. fluctuations of antenna temperature (T a ) was 0.25 K. All clouds with kinematical distances r a Some selection effects were discovered and our statistic results were corrected for them. Figure 1. ... In the very high mass range the number of neutral gas clouds may be decreased because of gravitational instability or/and molecularization. ...

Еще в разделе: (Показать все результаты (>900) - jet.sao.ru/ )

• Iron abundance in the atmospheres of components of the binary system 41...
• GRB follow-up team
• Parameters of the 41 Dra system components

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

Еще в разделе: (Показать все результаты (>3897) - www.naic.edu/ )

• Chapter 5. Listing of Installed Components
• HI Self-Absorption in the Canadian Galactic Plane Survey: First Results
• Pulsar Highlights - Best Limits on Dipolar Gravitational Wave Emission

... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...

Еще в разделе: (Показать все результаты (>4225) - hea-www.harvard.edu/ )

• Comments on: [ArXiv] component separation methods By: hlee By: Sam Leach
• The AstroStat Slog component separation
• The AstroStat Slog principle component analysis

... Dodson, Legge et al, ApJ, 2003 Spectral Line Sources Ї Requirement of high brightness temperatures means no thermal emission Ї Masers: Galactic Extragalactic Ї OH, H2O Ї OH, H2O, SiO, CH3OH Ї Galactic extra-galactic HI absorption VLBI arrays Ї VLBA (Very Long Baseline Array) Dedicated US array of ten 25m telescopes 330 MHz ґ 90 GHz Ї EVN (European VLBI Network) Formal collaboration of radio telescopes in Europe, Asia and South Africa ~15 telescopes 15m to 100m 330 MHz ґ 22/43 GHz ...

Еще в разделе: (Показать все результаты (>9500) - www.atnf.csiro.au/ )

• casacore: ComponentModels_module
• odnh3
• casacore: components/ComponentModels/GaussianShape.h File Reference

The spectrophotometrical complex of the 6-m telescope in Nasmyth-1 focus . ... A new sample of 360 blue compact galaxies with a strong star formation was build on the base of the Second Byurakan Survey. ... More that 20 galaxies with the extremely low-abundances of heavy elements in the range of 1/30-1/10 of the Sun's one, were found. ... During the 15-years observation term near 500 spectra of the unique source SS~433, from which the relativistic jets were found for the first time, were obtained. ...

Еще в разделе: (Показать все результаты (>1848) - www.sao.ru/ )

• A fast-scan extragalactic source survey at 4.755 GHz
• Principal Components Analysis
• Group IAG

... Mass ratio of SS433 components is q = M X / MV = 0.2 В 0.3 . ... The spectum corresponds to precessional moment T3, i.e. when the angle between jet axis and the line of sight is equal 60 degrees. 10 -2 10 -3 lg I, phot/cm2/sec/keV 10 -4 10 -5 10 100 lg h, keV Cherepashchuk A.M.,Sunyaev R.A., Fabrika S.N., Postnov K.A. et al./ ... 5 10 100 Tcor = 20keV lg h, keV Mjet = 21020 g / s Lk = 61039 erg / s Angle dependence of SS433 spectrum In the figure the angle dependence for SS433 spectrum is shown. ...

Еще в разделе: (Показать все результаты (>598) - www.iki.rssi.ru/ )

• Examples of the raw magnetic field information, obtained with the MIF-M
• Geomagnetic Kp Index

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

Еще в разделе: (Показать все результаты (>891) - www.cosmos.ru/ )

• Wave complex KEM-3

... Астронет | ... Термин "component" . ... компонента . ... составляющие [компоненты] радиоизлучения Солнца . ... составляющие [компоненты] солнечного радиоизлучения . ... основная компонента (радиоизлучения Солнца) . ... составляющая (радиоизлучения всплесков IV типа) в сантиметровом диапазоне (радиоизлучения Солнца) . ... жесткий компонент (напр. корпускулярного излучения) . ... спорадическая [быстрая] компонента (радиоизлучения Солнца) . ... составляющие [компоненты] радиоизлучения (напр. ...

Еще в разделе: (Показать все результаты (>74155) - www.astronet.ru/ )

• Spacecraft Rosetta Shows Comet has Two Components
• Астронет > Spacecraft Rosetta Shows Comet has Two Components
• Journal "Peremennye Zvezdy"

... The continuum of the Orion Nebula's template contains the nebular contribution plus a combination of Kurucz model atmospheres to simulate the stellar contribution. The fluxes of the UV, optical and near-IR emission lines from different sources are also incorporated into the template (J.R. Walsh, private comm.) The continuum of the planetary nebula has a nebular component and a hot stellar component simulated by an 80000K black body. ...

Еще в разделе: (Показать все результаты (>13639) - www.stsci.edu/ )

• Thermal and Nonthermal Infrared Emission from M87
• STScI Preprint #1221
• Fine Guidance Sensor Instrument Handbook

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... We present the numerical simulations for an electron-beam-driven and loss-cone-driven electron cyclotron maser (ECM) with different plasma parameters and different magnetic field strengths for a relatively small region and short time-scale in an attempt to interpret the recent discovered intense radio emission from ultracool dwarfs. ... A wide frequency band should therefore be covered by future radio observations. ...

Еще в разделе: (Показать все результаты (>1979) - star.arm.ac.uk/ )

• Armagh Observatory Preprint No. ???
• Doppler Imaging and Flare Activity on HR1099

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

Еще в разделе: (Показать все результаты (>286) - www.gao.spb.ru/ )

• Phase light curves of young binary systems

... 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 (>242) - mavr.sao.ru/ )

• IRAS01005+7910
• Galaxy sector, archive 2009
• Optical component of GRB080319B

REDSHIFT DETERMINATION OF GALAXIES IN TWO- COMPONENT EXPANDING MODEL OF UNIVERSE T.S. Kozhanov et al. ... This equation is found for mass and massless particles on the background of mixed model of the Universe (dust+radiation) at di erent values of space curvature (k = 1; 0). ... The asymptotic equations of the scale factor at di erent values of the ratio of baryons matter density to the radiation density for plane, open and close cosmological models is obtained. ...

Еще в разделе: (Показать все результаты (>2880) - www.mrao.cam.ac.uk/ )

• OptInt PmWiki : Component Documentation | History
• OptInt PmWiki : Component Documentation
• OptInt PmWiki : MROIDelayLine / Component Documentation

. AIAA Paper 94-2323 . Jacques Lewalle, jlewalle@syr.edu

Еще в разделе: (Показать все результаты (>936) - crydee.sai.msu.ru/ )

• A Simple Example With a Single Chirp Component

... Equipment . ... The scientific-methodical work is an important component of the LSR work, which should satisfy the needs of employees of other laboratories of the ISSP RAS both in structure investigations and in interpretation of the obtained results. ... It consists of measurements and determination of required characteristics of a specimen, like phase composition, single crystal orientation, dimension and form of structure components, chemical composition. ... Copyright 2005 LSR ISSP RAS . ...

Еще в разделе: (Показать все результаты (>863) - www.issp.ac.ru/ )

• III International Astronomy Olympiad, Problems to solve
• II-VI compound crystal growth, HPVB & HPVZM basics

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

Еще в разделе: (Показать все результаты (>3) - scan.sai.msu.ru/ )

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 (>1636) - www.adass.org/ )

• Image Reconstruction with Few Strip-Integrated Projections: Enhancements by
• Calculating the Position and Velocity Components of HST
• A Computer-Based Technique for Automatic Description and Classification of

Detected Supernovae . The search have produced till now the detections of 4 SNe. ... This result highlights the power of infrared monitoring in detecting Obscured SNe and indicates that optical surveys are probably missing a significant fraction of SNe, especially in obscured systems such as starburst galaxies. ... In Fig. we show the archival SOFI image of NGC3256 (left) and the first image obtained in 2001 (right) where SN2001db has been detected. ...

Еще в разделе: (Показать все результаты (>8517) - www.arcetri.astro.it/ )

• HwB: Macintosh Serial Connector (Offline)
• Microwave components: few tests
• First VLT Colour Photo of a Strange Galaxy (ESO PR Photo 19/98)