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. ...

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

Next: Dynamic Scheduling Up: Scan Times Previous: Dealing with Formatter Reconfigurations Contents . The nominal scan start time, if set using DWELL , is the time good data is expected to be available. ... The more modern systems, especially the Mark5C recorders and the software correlators, approach this ideal and the recordings are started at the time specified in the VEX file for the start of good data. ... A recording scan is the time between stops of the recording media. ...

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• MINPAUSE
• DURation
• START

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...

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• Program use
• Detector Performance
• mod_session_crypto - Apache HTTP Server

... solve : find optimum fit in a grid of model spectra . ... It initiates an optimisation by starting with a grid of theoretical spectra, defined by model or read_grid , a set of starting parameters and an observed spectrum. ... The parameters to be optimised include: T eff , log g , n A , v sin i , v rad being effective temperature, surface gravity, an abundance variable, rotation velocity and radial velocity for one or two stars, and R 2 / R 1 being the relative radius of the second star, if present....

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• FFIT - Command Syntax

Next: The Optopus session Up: Using the Optopus Previous: Using the Optopus . The commands in the Optopus package have to initialised by setting the Optopus context with the MIDAS command SET/CONTEXT OPTOPUS . ... Since almost all commands in the package work, both in input and in output, on MIDAS tables, another important task of the user at the start of an Optopus session will be to create a MIDAS table from the ASCII file where the data about the objects to be observed are being kept. ...

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• Starting the whole thing
• Saving and Loading Session Parameters
• Commands

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. ...

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• Getting Started in Actor Prolog. Analyzing Web Sites.
• Getting Started in Actor Prolog. Hello World.
• Getting Started in Actor Prolog. Underdetermined Sets.

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... Constraints . ... in equation 1 must exceed this value for a source to pass. mindetml . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. minmaskfrac . ... For a source to pass, ii_DET_ML must be mindetml and ii_MASKFRAC must be minmaskfrac for at least one of the instruments ii. numhexchar . ... 3.5 1.0 1.0 . ...

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• Index

... This page will contain a form to pass parameter values for a on-line working code producing figures illustrating the dependence of optical properties of different scatterers on their parameters. Specify the parameters and press start calculation button to produce a figure. ... Independent variable: x v a/b alpha Re(m)? another? ... Number of curves: 1 2 3 . ... Curve #1: . Particle shape: sphere spheroid another? TE/TM mode: TE TM . Other parameters: x= Re(m)= Im(m)= a/b= alpha= . ...

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Next: What We Will Up: Improved Prescription Retrieval and Previous: Prescription-Based Optical Modeling . ... Prescription retrieval provides a means of improving estimates of prescription parameters by computer processing of image data (Fig. ... Prescription retrieval takes as a starting point the . ... The prescription retrieval process takes image data as input. ... The best results are obtained using several images simultaneously, preferably images that use different field and focus points. ...

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• STIS PSF Library Input Tool...Help
• Deconvolution
• Python: module constraint_window

... ratios Evolution Equations with · Now write · Evolution equations now · Define trajectories via Cosmic Trajectories Dust =0 de Sitter phase Radiation =1/3 Initial singularity Cosmic Trajectories · For a range of initial conditions, models re-focus around the flat ... case · For decoupled matter and radiation can solve the equations exactly · Solutions governed by two constants: Non-Euclidean Geometry · Axioms of ...

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• http://www.mrao.cam.ac.uk/~rachael/compphys/examples/quantum.f90

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• Parameters
• OYSTER
• OLAS integration test suites

... The various Inst :Focus scripts allow you to take a series of exposures over a range of secondary mirror focus values, report the resulting FWHMs and optionally adjust the focus to the estimated best value. ... Slitviewer scripts assume the focus star is on the boresight. ... Focus scripts runs in three phases: . ... The script moves the boresight so the focus star is visible next to the slit, sets the focus to Center Focus, takes an exposure and tries to measure the star's FWHM. ...

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• TUI:Scripts:Built In Scripts:NICFPS:Data Cube
• what to do with the trace data
• Astrophysical Research Consortium - Apache Point Observatory

Rotang can either be run from the command line as described here or through the alfa_ang GUI . ... To run rotang at Arecibo: . Start IDL . ... rotang, Date , RA , Dec , Time , /choice . Here Date takes the format YYMMDD (e.g. 041128 for the 28 th of November, 2004). ... Rotang also calculates the Azimuth and Zenith Angle fir every source. If the Zenith Angle is greater than 20 degrees, then the program will return that the source is down and will not calculate an optimum ALFA angle. ...

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• WAPP File Format Page
• CIMA Data Taking Modes
• The Mock Spectrometer

... News . ... Research areas . ... English News . ... In the spring of this year the scientists of Samara State Aerospace University (SSAU) will proceed to integrated exploration environment in the near-Earth space and its impact on the engineered materials of spacecraft. ... This spring it will be launched into space by the first carrier rocket from the new Russian space launcher complex Vostochniy. ... The equipment set is designed and manufactured in SSAU Institute of Space Device Engineering (ISDE)...

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• SSAU starts cooperation with the Republic of Korea
• The Tenth International Summer Space School starts this week
• Business Club Starts at SSAU

... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...

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... CREATE FULLTEXT PARSER -- create a parser for full-text search . CREATE FULLTEXT PARSER prsname START= start_function GETTOKEN gettoken_function END end_function LEXTYPES lextypes_function [ HEADLINE headline_function ] ; . CREATE FULLTEXT PARSER will create a new parser used to break document onto lexemes. If a schema name is given (for example, CREATE FULLTEXT PARSER myschema.prsname ... ) then the parser is created in the specified schema. ... DROP FULLTEXT PARSER ...

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• Looking behind the Gimp
• GIMP Effects: Rounded Text
• MaDgimp: Fire Effect

... The grid of values can be built around any parameter by explicitly giving the center point of the grid (in response to the model descriptor prompt). ... Please choose the grid axes: model componet number for the first axis (1): cr first axis parameter (norm|index|temp|galacticNh|intrinsicNh): temp half range of first axis parameter (0.4): 0.25 number of steps in the first axis (1:) (7): 5 model component number for the second axis (1): 2 second axis ...

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• *timfilter* - List start & stop times of good data intervals
• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog effective area

New reduction of minor planets photographic plates obtained with Pulkovo Normal Astrograph A.A. Berezhnoy Pulkovo Observatory of RAS, Saint-Petersburg, Russia Minor Planet observations at Pulkovo Periodical observations of 14 bright asteroids named Selected Minor Planets (SMP) were performed at Pulkovo since 1948 within the international framework started by works of B.V. Numerov and D. Brouwer. ... 108 133 113 74 124 67 97 88 14 84 64 5 20 19 Epochs (YYYY.MM) 1200 Mean values of total obs. ...

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• The Pul-3 astrometric catalogue (Second edition). Data access form.
• Proper motions of 59766 stars with respect to galaxies in 149 areas of the sky
• The Pul_ERS astrometric catalogue. Data access form

. The Doppler Effect . Spectroscopy . Wavelengths . The Electromagnetic Spectrum . Spectrographs . PPT Slide . What’s this got to do with velocities? . The Doppler Effect: . How does this affect the spectra? . The Maths . Example. Author: Paul Francis . Email: pfrancis@mso.anu.edu.au . Home Page: http://msowww.anu.edu.au/~pfrancis/astr1001/ . Other information: . Course Notes for ASTR1001 Astronomy

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• Library and heliostat tower before start of cleanup.
• Exterior painting has started
• Starting on the business manager's old office.

Stellarium 0.12.3 . ... StelCircleArcRenderer Class Reference . Provides functions to draw circle arcs using StelRenderer . ... drawGreatCircleArc (const Vec3d &start, const Vec3d &stop, const SphericalCap *clippingCap=NULL, void(*viewportEdgeIntersectCallback)(const Vec3d &screenPos, const Vec3d &direction, void *userData)=NULL, void *userData=NULL) . ... Create a circle arc renderer to draw multiple circle arcs . ... void(*)(const Vec3d &screenPos, const Vec3d &direction, void *userData)љ . ...

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• Stellarium: StelScriptMgr Class Reference
• Stellarium: StelQGLTextureBackend Class Reference
• Stellarium: StelSkyLayer Class Reference