Package . Class . ... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ... These links take you to the next or previous class, interface, package, or related page. ...

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

Next: Identification and Analysis of Binary Star Systems using Probability Theory . ... We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. ... In the case of slowly rotating stars one can use the zero-rotation approximation to describe stellar pulsations. Such a model was used already by Cugier, Dziembowski & Pamyatnykh (1994) to study nonadiabatic observables of Cephei stars. ...

... The filter extensions include a region expression, to cover cases where we know there are spatial variations, and the transmission values corresponding to each energy bin datum. ... CAL_getFilterTransmission() : Retrieve filter transmission data as a function of energy for the THIN1 filter; the function exists in two flavors the second of which integrates the efficiency curve over a specified energy range . ... Columns: . ... The description of the region in which the transmission values are valid. ...

... Scripnichenko V. I., Vinogradova T. A., Zheleznov N. B. AMPLE - integrated multi-purpose software package for minor planets. Version 1.3. Ключевые слова: малые планеты, эфемериды, астрометрия, элементы орбит, О-С, идентификация, пластинка, трек, орбита, обсерватория, объектно-ориентированные технологии. ... Начиная с версии 1.3, в AMPLE предоставляется новая возможность - вычисление эфемерид и вычисление (О-С) для объектов, которые отсутствуют в базе данных пакета. ...

... Space-time distribution of matter at the epoch Z=0.4--3.5 by analysis of absorbtion systems in QSO spectra" . A statistical analysis of distributions of C IV and Mg II absorption-line systems observed in QSO spectra within the cosmological redshift interval Z abs =0.2-3.2 is presented. ... The isotropy (or anisotropy) of the distribution is verified by comparing of independent distributions of the absorption systems in opposite hemispheres with their various orientations. ...

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Next: Scattering properties Up: Polarization properties (transmitted radiation) Previous: Linear polarization: wavelength dependence . Traditionally, the main problem considered in connection with circular interstellar polarization is the meaning of the wavelength where changes the sign . ... This is also demonstrated by Fig. 19 (lower panel) which shows the wavelength dependence of the factors of linear and circular polarization for particles of magnetite as was done by Shapiro ([ 1975 ]). ...

. On the plot the Spacecraft visibility relative to the groundbased station is shown as a function of the Moscow time . Date is shown along the X-axis, the Moscow time (MT=UT + 3 hours) - along the Y-axis. The Spacecraft visibility relative to the corresponding groundbased station is labelled with the 1-hour step. The Spacecraft passing through the selected simulative geophysical regions are shown as well by the corresponding symbols.

Time Standard and Ensemble Pulsar Time Scale Ding Chen, George & Dick, Bill 20100928, Orange National Time Service Center. ... Ensemble Pulsar Time Scale(EPT) : (TAI - EPT ) = k = ( 2 k k =1 N ^ k (TAI - PTk ) + 2 z ,k ( T )) -2 PPTA is the best project to establish the new independent ensemble time scale which will take contribution to both GW detection and BIPM. ... Ensemble Pulsar Time Scale is more stable than the AT of some clock laboratory on long term scale. ...

... NICMOS data are represented by five arrays for each readout. ... Samples array. ... Each downlinked readout is always represented by these five arrays ( Figure 13.4 ). Multiple readouts in the same dataset (e.g., MULTIACCUM data) are represented by repeated sets of these five arrays ( Figure 13.5 ). ... For data where multiple samples of the array were obtained during the integration, the samples array denotes the number of samples for each pixel in the corresponding science image. ...

hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

... Vladimir A. Borodin . ... Corresponding Member of Russian Academy of Sciences . General Director of Experimental Factory of Scientific Engineering with Special Design Department, Russian Academy of Sciences . Vladimir A. Borodin is a well-known physicist working in the field of flux crystal growth and development of applicable automated equipment. ... In 2006€а V.A.Borodin was elected€а a corresponding member of the Russian Academy of Sciences (Scientific Engineering Division). ...

FSP1 : The time intervals corresponding to the INTERBALL TAIL PROBE (IB_TAIL) or GEOTAIL passage through the simulative magnetosphere boundary layer (BL) . ... FSP3 : That part of the FSP1 or FSP2 time intervals, which corresponds to the magnetic conjugations between any couple of the considered spacecraft. The value of the relative geocentric angular distance between magnetic field line's footprints is considered during FSP3 situation selection. ...

The galactic absorption is computed from Schlegel's maps . Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds", Schlegel et al 1998 . ... For Galactic objects, ag is also provided, although it does not correspond to the real extinction toward a given object (because it integrates the extinction through the whole depth of the Galaxy; for nearby objects it over-estimates the extinction). ... ag(I342)=ag(Schlegel)*3.50 . ... ag(I10)=ag(Schlegel)*3.50 . ...

. F IGURE . 10. Dependence of cluster metallicity on (a) Galactocentric distance and (b) distance from the Galactic plane. The filled and open circles correspond to the young and old halos, respectively, and the straight lines are the corresponding rms regressions. The small square shows the old-halo cluster excluded from computations based on a 3 criterion. discussion in the text | privious figure | next figure .

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Title: Superconducting Flux-Flow Oscillators for THz Integrated Receiver Authors: V.P. Koshelets (1, 2), P.N. Dmitriev (1), A.B. Ermakov (1, 2), L.V. Filippenko (1), A.S. Sobolev (1), M.Yu. ... The concept of a fully Superconducting Integrated Receiver (SIR) has been developed and experimentally proven in a tight collaboration between the Institute of Radio Engineering and Electronics (IREE-Moscow) and the SRON Netherlands Institute for Space Research. ...

... A Massive Star in NGC 6357 . ... One such massive star, near the center of NGC 6357, is framed above carving out its own interstellar castle with its energetic light from surrounding gas and dust. ... This image of Saturn could not have been taken from Earth. ... Since Earth is much closer to the Sun than Saturn, only the day side of the ringed planet is visible from the Earth. ... Sixteen years ago, Comet Hale-Bopp rounded the Sun and offered a dazzling spectacle in planet Earth's night. ...