... RESWRI uses the 1 sigma error-field to calculate its errors. ... Maximum number of rings is 512. ... Example: USER reswri reswri Version 1.2 (Nov 24 1998) USER RESWRI INSET=drop 2 inset2=drop 1 Set drop has 3 axes RA-NCP from -134 to 115 DEC-NCP from -116 to 135 PARAM-GAUSSFIT from 1 to 11 Set drop has 3 axes RA-NCP from -134 to 115 DEC-NCP from -116 to 135 PARAM-GAUSSFIT from 1 to 11 USER RESWRI BOX= BOX range for set drop : RA-NCP from -134 to 115 DEC-NCP from -116 to 135 ...

Еще в разделе: (Показать все результаты (>24380) - www.atnf.csiro.au/ )

• http://www.atnf.csiro.au/computing/software/gipsy/tsk/astrom.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/sub/skyfit.dc2
• imfit

... File name for the fits binary table containing X-ray source positions and their errors. opticalset . ... File name for the fits binary table containing optical source positions and their errors. findrotation . ... boolean . ... name of B magnitude column . ... column name of optical catalogue position RA . ... column name of optical catalogue position DEC . ... column name of optical catalogue position error . ... column name of X-ray source position RA . ... column name of X-ray source position DEC...

Еще в разделе: (Показать все результаты (>14854) - xmm.vilspa.esa.es/ )

traxy -- Transform an X,Y position from input to output pixel position using the same conventions as drizzle traxy xin yin . xin = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... So, if an object on an input image at a certain position is drizzled with a given set of parameters then the position of that object on the output can be predicted using traxy with the same parameter values. ...

Еще в разделе: (Показать все результаты (>244) - www.stecf.org/ )

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

This page gives the name and meaning of the various parameters which can be queried in HyperLeda through SQL requests . ... real . ... actual error on t . ... log 10 of apparent major axis diameter d25 at 25 mag.arcsec -2 (d25 in 0.1') . ... actual error on logd25 . ... Apparent maximum rotation velocity of gas . ... log 10 of apparent corrected diameter (dc in 0.1') . ... total apparent corrected B-magnitude . ... total apparent corrected U-B color . ... Questions: leda@univ-lyon1.fr ...

Еще в разделе: (Показать все результаты (>2188) - www.sao.ru/ )

• HyperLEDA documentation: parameter: pa
• HyperLEDA documentation: parameter: celpos
• EXTRACT HOMOGENIZED DATA FOR A LIST OF OBJECTS

... 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 ...

Еще в разделе: (Показать все результаты (>319) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/personal/malkin/publ/zm14e.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/kurdubov.pdf

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

Еще в разделе: (Показать все результаты (>552) - xray.sai.msu.ru/ )

• Initial Distributions of Binary Parameters
• Dependence on the Scenario Parameters and Initial Distributions
• Initial binary parameters

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 (>3883) - hea-www.harvard.edu/ )

• The AstroStat Slog parameter estimation
• *tvmark* - Mark pixel positions on the display
• Regions and Source Parameters

Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

Еще в разделе: (Показать все результаты (>14707) - www.stsci.edu/ )

• Index
• CSPICE Routines: OSCELT_C
• Obsolescent Acquisition Parameters

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. ...

Еще в разделе: (Показать все результаты (>65899) - www.eso.org/ )

• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• OYSTER Lab
• The Hierarchical Stellar Systems Model Format

... 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 . ...

Еще в разделе: (Показать все результаты (>754) - www.apo.nmsu.edu/ )

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

... 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. ...

Еще в разделе: (Показать все результаты (>166) - www.asc.rssi.ru/ )

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. ...

Еще в разделе: (Показать все результаты (>999) - astro.uni-altai.ru/ )

• Stellarium: Skybright Class Reference
• Stellarium: gSatTEME Class Reference
• Stellarium: StelGeometryBuilder Class Reference

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 (>7384) - www.arcetri.astro.it/ )

... 8, ``Celestial Mechanics'', 2002 First results of GPS orbit determination with GRAPE package using a square--root information filter M. O. Keshin Institute of Applied Astronomy, St. Petersburg, Russia The zero--differenced carrier phase measurements contain the distance be­ tween the phase centres of receiver and transmitter antennas biased by unknown integer number of cycles (phase ambiguities). ... In the case of GPS the problem of solar radiation pressure modelling is of primary importance. ...

Еще в разделе: (Показать все результаты (>650) - www.ipa.nw.ru/ )

• http://www.ipa.nw.ru/conference/wpltn2012/docs/25/1320%20yagudina.pdf
• (Untitled)
• Keywords_128

... rotang, Date, RA, Dec, Time, accS, ast=ast, ha=ha, lst=lst, jd=jd, az=az, za=za, sep=sep, rotang=rotang, alfabeams=alfabeams . ... It is thus possible to specify, for instance: rotang, ... , ha=haHr, lst=lstHr, ast=astHr . ... alfa_angle - script to launch the GUI . alfa_ang.pro - the GUI: provides input to rotang and a graphical display of the results. rotang.pro - the main routine of the program: finds the required time, the other associated times, Az and ZA using ao_idl routines. ...

Еще в разделе: (Показать все результаты (>3895) - www.naic.edu/ )

• AGES Database Search
• Orbits in the period / acceleration plane

... 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. ...

Еще в разделе: (Показать все результаты (>1668) - www.adass.org/ )

• Calculating the Position and Velocity Components of HST
• The SuperCOSMOS Sky Surveys
• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed

... This appartus will drop a mass from different heights. When the mass strikes the ground, some percentage of its original energy will be absorbed by the ground. ... The percentage of the energy which is absorbed by the surface on each "bounce" (EAS) . ... The impact velocity of the object will also be given at each bounce. ... Start= Drop the ball after Energy, Mass and EAS have been set; resume after step or pause has been selected . ... Reset = Reset experiment to intial values . ...

Еще в разделе: (Показать все результаты (>369) - zebu.uoregon.edu/ )

... define constants real, parameter :: g = 9.8 real, parameter :: pi = 3.1415927 integer :: n, i real :: a, u, delt real :: ttot, t, x, y ! Read values for u and a from terminal write(*,*) 'Enter initial speed u:' read(*,*) u write(*,*) 'Enter initial angle a in degrees:' read(*,*) a ! ... Read value for time interval from terminal write(*,*) 'Enter time interval:' read(*,*) delt if (delt <= 0.0) stop 'Invalid time interval!' Calculate number of time intervals n = ttot / delt ! ...

Еще в разделе: (Показать все результаты (>3641) - www.mrao.cam.ac.uk/ )

• http://www.mrao.cam.ac.uk/~rachael/compphys/examples/cell_list.f90
• NVSS Source Search (10-July-1998) Help for NVSS Source Catalog Search
• OptInt PmWiki : PmWiki / Markup Expressions

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 . ...

Еще в разделе: (Показать все результаты (>1164) - www.cosmos.ru/ )

• STDA files
• Multipoint correlations of the solar wind parameters observed by several
• IKI SSC INTMINS APRIL98

Hideyuki Saio Simon Jeffery are exploring models for the evolution of stars formed by the merger of two white dwarfs. The attached movie provides a simulation of the major events involved in the merger process. ... An initial binary system consists of two white dwarfs of masses M 1 and M 2 (given) with an orbital period ( P ). ... We adopt a simple expression for the white dwarf radius as a function of mass (in solar units): . ... The merged star evolution is simulated by a quadratic expansion . ...

Еще в разделе: (Показать все результаты (>2853) - star.arm.ac.uk/ )

• Armagh Observatory
• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• SCL Sfit SLV Commands