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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• Details of Rotang

Finally, the radial velocity is also expressed in the reference frame of the Cosmic Background Radiation. This velocity is noted v3k . It is calculated from the heliocentric velocity v using the total solar motion of 360 km/s towards the direction defined by the B1950 equatorial coordinates B 11.25 H - 5.6 deg (Lubin Villela 1986). v3k = v + 360 cos(theta) Where theta is: cost(theta) = sin(de3k) sin (de1950) + cos (de3k) cos(de1950) cos(al3k - al1950) . ...

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• Documentation: LEDA: parameter: vrot
• HyperLEDA documentation: parameter: celpos
• Documentation: LEDA: parameter:

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... yes . ... If weightstyle =`gti', the task attempts to obtain a list of Good Time Intervals (GTIs), the exact way these are supplied being dictated via the parameter gtistyle ; these GTIs are ANDed with the attitude time bins; the net GTI in each bin provides the weight. gtistyle . ... If gtistyle =`user', the task obtains a single, simple GTI for all chip images from the parameters tstart and tstop . ...

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... CentralProcessor 0.11 documentation . ... These parameters govern all processing used for the calibrator observation. ... The dynamic flagging step can also optionally include antenna or baseline flagging. Then the bandpass table is calculated with cbpcalibrator , which requires MSs for all beams to be given. ... Second amplitude threshold applied when flagging 1934 data [hardware units - before calibration] . ... Name of the CASA table used for the bandpass calibration parameters. ...

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• User Parameters - Continuum imaging CentralProcessor 0.11 documentation
• User Parameters - Pipeline & job control CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation

Stellarium 0.12.3 . ... TextParams Struct Reference . Parameters specifying how to draw text. ... TextParams (const float x, const float y, const QString &string) . Construct TextParams with default parameters. ... TextParams ( Vector3 < F > &position3D, StelProjectorP projector , const QString &string) . Construct TextParams to draw text at a 3D position, using specified projector. ... string љ . ... Text string to draw. ... The required string parameter is also set, as is the projector. ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: gTime Class Reference

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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• Parameters of binary compact star evolution
• Initial binary parameters
• Dependence on the Scenario Parameters and Initial Distributions

... use frames summary class fields routine details file attributes . GLS routines to calculate linear fit . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = linearize_mr( time , ramp ) . ... result = cephes_ndtri( y0 ) . ... Lines: . ... McCabe complexity: . ...

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• covar2ellipse.pro (JWST Pipeline routines in IDL)
• Index
• Appendix: Recipe File XML Format GPI Data Pipeline 1.0 documentation

... overview of pyQC . ... output used by . ... All pyQC scripts and modules share a similar structure. Python offers to group functions, classes, etc. into modules which can be imported by different scripts. ... In order to avoid confusion if names are used by different (especially external) modules, the QC scripts use the 'from' statement only for pyQC modules, i.e.: . ... For other modules, the simple 'import' statement is used: . ... Python modules are also used for keeping script configuration. ...

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• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• Preparation of parameter file
• Parameters

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/perminov.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/tsyba.pdf
• Pulkovo NEO Page: Ephemeris Support

... Parameters of the Moon-perturbed orbit . ... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. The initial state vector is given in the inertial coordinate system in epoch J2000.0. ... The orbit has initial perigee radius Rp=7000.0 km, initial apogee radius Ra=343000.0 km and initial period T=8.453 days. ...

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• Results of measurements of SRT antenna parameters in Pushchino

... dust_AbsXSec . Absorption Cross section. typedef void . ... Calculates the equilibrium temperature given the absorption cross section and a radiation field. double . ... Calculates the absortion cross section of a species/size of dust grain . ... The grain absorption cross section . ... The absorption cross section of the grain . ... Calculates the equilibrium emission at wavelength lambda from a (large) grain at temperature T and with absorption cross section xsection. double dust_EquiT . ...

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• exchange.h File Reference
• write_fits.c File Reference
• read_fits.c File Reference

Following designations of elements/ parameters are used in AMPLE. ... mean anomaly . ... Node . ... Apart conventional orbital elements AMPLE gives possibility to calculate for each minor planet the following often used functions: . ... MOID . ... To calculate MOID user should order the name or the number of the major or minor planet through dialog. ... To calculate CT user should order the name or the number of the major or minor planet through dialog as it is proposed for MOID calculation. ...

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• ENGAMPLE
• Parameters of lightcurves of minor planets
• Table of Minor planet lightcurve parameters

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... Files . ... All љ Classes љ Namespaces љ Files љ Functions љ Variables љ Typedefs љ Enumerations љ Enumerator љ Macros љ Pages . ... tcc.parse.getCoordSys Namespace Reference . ... Obtain a coordinate system from a parsed parameter. ... Make a coordinate system from its name and date. ... if the coordinate system is unrecognized . Definition at line 31 of file getCoordSys.py . ... coordinate system date, or None for default date . ...

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• lsst.coordConv: coordConv::PVTCoord Class Reference
• lsst.tcc: tcc.msg.formatObjFields Namespace Reference
• lsst.coordConv: coordConv::OtherCoordSys Class Reference

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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• IMCCE-SAI: Natural Satellites Data Center (NSDC). Parameters
• The determination of parameters of the gravity anomalies sources
• IMCCE-SAI: Natural Satellites Service. Parameters and constants

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

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• Model Spectra for Spectral-Fitting Program
• Regions and Source Parameters
• The AstroStat Slog parameter estimation

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 . ...

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• Determination of the Detector Parameters
• mod_macro - Apache HTTP Server
• mod_session_crypto - Apache HTTP Server

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

... The predicted MIR's ground tracks, which pass near INSPIRE net, are available in this home page. The track consists from magnetic footprints calculated by magnetic mapping from MIR positions with 30 s step. ... For each time some of the INSPIRE net place are selected as soon as its coordinates are close to the MIR magnetic footprint (the geocentric angular distance between SP and footprint is less then 2.1 deg) . Back to the Top . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• IKI SSC, INTMINS APRIL99
• Multipoint correlations of the solar wind parameters observed by several
• Tail Probe | Matrix of Transformation Tail Probe | Matrix of Transformation

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• A Python-based IRAF Task Parameter Editor
• ASC Coordinate Transformation -- The Pixlib Library, II
• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed

... 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 . ...

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