The position of the objects on the sky were generally measured to a precision between 1 and 4 arcsec. ... For the stars, the position is always at epoch 2000, whatever J2000 or B1950 coordinates are printed. ... The celestial position is given as coordinates in 4 different systems: . ... B1950 . ... Galactic coordinates in the reference frame called "new" system, adopted by IAU in 1958. Galactic pole at B124900.0+272400, node at ra=282.25,l=33 deg (inclination 62.6 deg). ... 1 arcsec . ...

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• HyperLEDA documentation: parameter: pa
• OPTOPUS Commands and Parameters
• Starting up

The following parameters as a function of the universal time are enclosed in this file. 1. no . ... Universal time date (YYYYMMDD) . ... Universal time (.hhmmss) . ... Geomagnetic local time in the satellite position . ... geomagnetic latitude . ... co-ordinate - . ... system . ... co-ordinate system . ... Solar-ecliptic co-ordinate - . ... Satellite velocity . ...

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• IKI SSC INTMINS APRIL98
• Multipoint correlations of the solar wind parameters observed by several
• Magnetic mapping

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" | ...

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• *tvmark* - Mark pixel positions on the display
• Parameters
• Listing and Printing Files, Parameters, and Tables

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 (V2.00) --- November00 --- POLIMPLOT (V2.00)
• Plot data from the WDS
• Stellar parameters from calibrations of spectral types

... It takes a set of grid positions and a set of sky coordinates to fit the parameters. ... Category: MATH File: skyfit.c Author: K.G. Begeman Use: INTEGER SKYFIT( X , Input DOUBLE PRECISION ARRAY Y , Input DOUBLE PRECISION ARRAY A , Input DOUBLE PRECISION ARRAY D , Input DOUBLE PRECISION ARRAY N , Input INTEGER XF , Output DOUBLE PRECISION ARRAY YF , Output DOUBLE PRECISION ARRAY FPAR , In/Output DOUBLE PRECISION ... X Contains x grid coordinates. ...

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• User Parameters - Mosaicking Continuum images CentralProcessor 0.11
• Central Processor Manager CentralProcessor 0.11 documentation
• casacore: casa::GaussianConvert Class Reference

... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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• MCP Menu documentation
• lsst.coordConv: coordConv::OtherCoordSys Class Reference
• lsst.coordConv: coordConv::Coord Class Reference

Shell scripts can act like standard UNIX commands and take arguments from the command line. Arguments are passed from the command line into a shell program using the positional parameters $1 through to $9 . Each parameter corresponds to the position of the argument on the command line. ... For example: cat printps # This script converts ASCII files to PostScript # and sends them to the PostScript printer ps1 # It uses a local utility "a2ps" a2ps $* | lpr -Pps1 printps elm.txt vi.ref msg . ...

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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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• Where are the tunable parameters of the kernel?
• Kernel tunable parameters
• Tunable Kernel Parameters?

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   . ... Text string to draw. ... The required string parameter is also set, as is the projector. ...

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• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: Skybright Class Reference
• Stellarium: Refraction Class Reference

... Execute) Back Status Jacks Limits # ListCtrl $ Caption =Jack Limits: $ ColumnName0 = Name $ ColumnName1 =Status $ StructName1 =Limits.Actual Back Drive Status # ListCtrl $ Caption =Drive Status: $ ColumnName0 = Name $ ColumnName1 =Status $ StructName1 =Jacks Alarms.Actual Back Positions # ListCtrl $ Caption =Jack Positions: $ ColumnName0 = Name $ ColumnName1 =Position $ ...

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• http://www.naic.edu/~tghosh/software/pcheck.pro
• http://www.naic.edu/~cima/bad_fits_1.txt
• http://www.naic.edu/~phil/hardware/byuPhasedAr/rfischercode/userhelp.txt

... 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/personal/malkin/publ/zm12i.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm14e.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf

... The operators will be explained as they are used. The general notion to keep in mind is that any combination of these operators results in a 2- D affine coordinate transformation in the TF plane, which may be represented using the homogeneous coordinates often used in computer graphicsfoley. ... S _t_c,f_c = g_t_c,f_c,(_t) | ... We denote a time shift to the position , with an operator that has a multiplicative law of composition : (Table 1). ... Note that these two operators do not commute. ...

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• Tutorial on Fortran 90, Digital UNIX
• Footnotes
• Keyword arguments and default arguments

... spectrum . ffit . ... grids . ... These commands read in a grid of model spectra. ... Values for the parameters are taken from the input models themselves, to avoid mixups. The syntax of the command arguments is precise. model{ . ... If there is only one spectrum to fit, one should set default parameters for the secondary which lie within the model grid, with <L_2/L> being a very small value. ... The output is saved in a file <file.fit> , where <file> was the name of the spectrum being fitted. ...

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• Sfit Control Language: Classified Listing
• SCL Sfit Genetic Commands
• SCL Sfit SYN Commands

... There is an opportunity to perform O-C calculations for objects which are absent in the data base of the package. Such objects can be described by orbital elements or by initial coordinates and velocities. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ... For example, the designations of objects in the list can occupy the last position in each line. ...

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• ENGAMPLE
• Keywords_128
• IAA GPS Analysis Center

... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...

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• TwoFitlines: An Spectrum and Line Analysis Tool
• The SuperCOSMOS Sky Surveys
• ASC Coordinate Transformation-The Pixlib Library

Basics of magnetosphere satellite experiment. Main steps of data processing. Modern conception of Earth magnetosphere. ... Empirical models of the bow shock, magnetopause and neutral current sheet positions. Main principles of construction of empirical magnetospheric magnetic field models. ... Current systems in the Earth magnetosphere. Chapman- Ferraro current. ... Tsyganenko 1996 model and its application to satellite data processing. ... Basics of statistical data analysis. ...

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• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2016 (DE200/LE200).

... First ask for the controlling parameters} set_string (s1,10) ask_for_string (Maximum step size [days],s1) set_maximum_step(s1) set_string (s1,100) ask_for_string (Maximum number of steps in the search,s1) set_number_of_iterations(s1) set_string (s1,1e-6) ask_for_string (Tolerance,s1) set_tolerance(s1) new_line write_string (Allowed coordinate types are true, apparent, and topocentric) new_line set_string (s1,true) ...

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• http://www.mrao.cam.ac.uk/~rachael/compphys/examples/cell_list.f90
• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLineSW.RequirementsReview/ICS_if.pdf
• Command line interface to libAIR and water vapour column retrieval Bojan

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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Calculation attitude parameters: . ... Axes position of the GSE system relative to the s/c coordinate system is determinated by 3 angles Alpha , Betha and Gamma . Alpha and Betha determinate coordinates of a new XGSE axis, while Gamma determinates YGSE or ZGSE. ... String in the attitude file look like this: . ... 980307 09 16 21 604 -665.00 233.00 264.00 . ... 980307 09 16 30 604 -669.00 336.00 113.00 . ... 980307 09 16 42 604 -672.00 359.00 -114.00 . ... Angles Alpha Beta Gamma (rad) . ...

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• List of currently available KP AZ.
• AZ Key parameters, 1997
• AZ Key parameters, 1998

... 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
• Texas Survey of radio sources at 365MHz