... Default . ... The descriptions below focus on the meaning of each filename parameter, leaving the exact details of the inferred default value to be explained in the algorithm section. evlist . ... file . The response matrix file (OGIP-compliant format). ... If a spectrum file is not provided ( withspectrum =no) this parameter specifies the INDEX number of a source in the source description list (parameter srclist ), and thereby the incidence angle and selection regions for the response matrix. ...

Еще в разделе: (Показать все результаты (>13961) - xmm.vilspa.esa.es/ )

Next: Parameters of the starburst Up: The Model Previous: Initial parameters of compact . ... If the rate of accretion from one star to another is sufficiently high (e.g., the mass transfer occurs on a timescale a few times shorter than the thermal Kelvin-Helmholz time for the normal companion) or the compact object is engulfed by a giant companion, the common envelope (CE) stage of the binary evolution can set in (see Paczynski 1976; van den Heuvel 1983). ...

Еще в разделе: (Показать все результаты (>547) - xray.sai.msu.ru/ )

• Effect of sources evolution on
• Dependence on the Scenario Parameters and Initial Distributions
• Initial Distributions of Binary Parameters

... We now describe the input parameters to the self-calibration tasks. ... For selfcal , you need not perform source , dra , or ddec selection if you use the selradec option (see below). minants : The minimum number of antenna that must be present before the tasks will attempt to find a solution. ... and phase : This determines whether the self-calibration tasks solve for just phase ( options=phase , which is the default) or amplitude and phase solution ( options=amplitude ). mfs : . ...

Еще в разделе: (Показать все результаты (>9922) - www.atnf.csiro.au/ )

• Preprocessing for Selavy CentralProcessor 0.11 documentation
• User Parameters - Pipeline & job control CentralProcessor 0.11 documentation
• List of Frequency File Parameters

The principal designation is the name, amongst the different possible names, chosen to identify the object because it is considered as the most reliable to cross-link to other databases or archives (eg. ... We recommend that authors of tables or catalogues identify their objects with the principal name, the celestial position plus possibly a name specific to the context (for example in a paper studying 3C sources use also the 3C name). ... HyperLeda . ...

Еще в разделе: (Показать все результаты (>1955) - www.sao.ru/ )

• Estimated parameters
• Gain steps
• Permanent telescope parameters

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...

Еще в разделе: (Показать все результаты (>221) - www.wdcb.ru/ )

• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/Type...

Next: Results Up: HST Image Restoration with Previous: The FMAPE Algorithm . ... Up to now, we have considered to be an adjustable parameter belonging to object space that is constant for a given image. ... To solve this problem several approaches have been presented in this conference (Katsaggelos 1994, Lucy 1994, Puetter 1994, Stark et al. ... Our approach consists in the introduction of a space variant hyperparameter in the Bayesian framework. ... 3 is space variant in the object space. ...

Еще в разделе: (Показать все результаты (>11517) - www.stsci.edu/ )

• Description of the Reconstruction Methods
• Prescription Retrieval
• Herschel Images and Results for the Magellanic Clouds

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

Еще в разделе: (Показать все результаты (>2196) - hea-www.harvard.edu/ )

• Parameters
• Period Criteria
• Model Spectra for Spectral-Fitting Program

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 (>293) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/personal/malkin/publ/zm09b.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm09a.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf

... The possibility to use the electrostatic approximation to calculate the polarizability allows one to consider practically any shape scatterers - from the regular ones (ellipsoid, cylinder, disc) [ 7 , 274 ] to those with an arbitrary shape, structure and anisotropy [ 308 , 309 , 313 , 405 ] (in the last case the polarizability tensor should be found numerically) - using the theory of the Rayleigh scattering. ...

Еще в разделе: (Показать все результаты (>373) - www.astro.spbu.ru/ )

• Database of Optical Properties -- Level: subpage
• Database of Optical Properties -- Level: subsubpage
• Nebular Abundances For PNe of Different Central Star Masses

... 8, ``Celestial Mechanics'', 2002 Investigation of stability of NEAs orbital resonance motions by numerical methods L. E. Bykova Tomsk State University, Tomsk, Russia The problem of orbital stability of resonance Near­Earth asteroids (NEAs) is considered. Most of NEAs have multiple close approaches to the inner ma­ jor planets. ... The technique of the investigation of NEAs orbital stability has been devel­ oped by author on the basis of the construction of possible motion domains (R) of asteroids. ...

Еще в разделе: (Показать все результаты (>555) - www.ipa.nw.ru/ )

• http://www.ipa.nw.ru/conference/2002/sovet/PS/PROKHOR.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/NEISHTAD.PS
• Keywords_99

Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...

Еще в разделе: (Показать все результаты (>531) - www.cplire.ru/ )

• Getting Started in Actor Prolog. Oil Production.
• Project 6 - RFBR - Multilayer epitaxial heterostructures of high-temperature
• SYNCHRONIZATION OF DRIVE-RESPONSE SYSTEMS ON CONDITION OF A LARGE MISMATCH OF

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

Еще в разделе: (Показать все результаты (>6912) - www.arcetri.astro.it/ )

• Determination of the Detector Parameters
• New Features in this Release
• mod_session_crypto - Apache HTTP Server

... Using the uvby -photometry and proper motion data for about 5500 F stars within 80 pc from the Sun, we have studied velocity ellipsoid parameters and obtained the following results. 1) The sizw of all wllipsoid semiaxes increase systematically for groups of stars with the decrease of both temperature (at constant metallicity) and metallicity (at constant temperature). ... As a result, each of the three parameters - temperature, metallicity and velocity dispersion - is an age indicator. ...

Еще в разделе: (Показать все результаты (>68) - ip.rsu.ru/ )

• Vladimir Marsakov Publication List
• Mid Scales Role

... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...

Еще в разделе: (Показать все результаты (>2278) - crydee.sai.msu.ru/ )

• Tutorial on Fortran 90, Digital UNIX
• Notation
• The pyramidal (multi-resolution) CCT

. Intervals of available data are coded by blue color. To read availability charts user should know the descriptor ("name") of the KP subset of interest. Table annotations include also number of version for each subset. Plot resolution is exactly one pixel per hour. Data are considered as available if at least one data point is present during that hour.

Еще в разделе: (Показать все результаты (>608) - www.iki.rssi.ru/ )

• AZ Key parameters, 1998
• AZ key parameters, 1996
• Plasma waves [Oulu]

Measuring\Omega and \Lambda with Type Ia Supernovae J.C. Niemeyer Max­Planck­Institut fЁur Astrophysik Karl­Schwarzschild­Strasse 1, D­85748 Garching, Germany B. Leibundgut European Southern Observatory Karl­Schwarzschild­Strasse 2, D­85748 Garching, Germany The explosive carbon incineration of white dwarfs produces very luminous events with no hydrogen in their spectra ­ Type Ia supernovae (SNe Ia). ... Their determination of\Omega and \Lambda is based on the analysis of 7 supernovae at redshifts z ? ...

Еще в разделе: (Показать все результаты (>7622) - www.eso.org/ )

• pyQC: script structure
• Preparation of parameter file
• OYSTER Lab

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

Еще в разделе: (Показать все результаты (>1616) - star.arm.ac.uk/ )

• Armagh Observatory
• Influence of Climate Variables on Tree-Ring Widths of Different Species
• Sfit Control Language: Classified Listing

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 (>1672) - www.adass.org/ )

• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• A Python-based IRAF Task Parameter Editor
• Building Software from Heterogeneous Environments

Arecibo Upgrade Notes INSTRUMENTAL POLARIZATION : POLARIZATION ISOLATION ERRORS IN STOKES PARAMETERS Jim Cordes Joe Lazio 22 May 1996 Summary The purpose of this memo is to: (1) demonstrate how polarization isolation is related to errors in Stokes parameters ; (2) estimate a tolerable level of errors in Stokes parameters due to amplitude and ... However, the errors in Stokes parameters are not so small: Eq. 4 indicates that the polarized flux is in error by ffi ъ ё 22%. ...

Еще в разделе: (Показать все результаты (>2724) - www.naic.edu/ )

• http://www.naic.edu/~astro/aotms/backends/96-01.pdf
• http://www.naic.edu/aisr/worldday/wd_intro.html
• CIMA Configuration Files

... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Nuclear activity and environment Effect of environment on AGN is not completely clear yet. ... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Effect of the mass Mass slices ­ optical and radio AGN overall interaction one-on-one interaction relative location 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Stratified study Stratifed study that considers several strata of mass. ...

Еще в разделе: (Показать все результаты (>1216) - www.mrao.cam.ac.uk/ )

• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l5.pdf
• http://www.mrao.cam.ac.uk/~bn204/phd_era/publications/ursi-oof-a0poster.pdf
• http://www.mrao.cam.ac.uk/~cjld1/pages/geometryandcosmology2.pdf