... Search object | ... Extract mean data for a list of objects . ... DEC 1950 (degrees decimal value) . ... actual error on t . ... log10 of apparent diameter (d25 in 0.1') . ... actual error on logd25 . ... actual error on logr25 . ... actual error on brief . ... Apparent maximum rotation velocity of gas . ... actual error on vmaxg . ... Apparent maximum rotation velocity of stars . ... actual error on vmaxs . ... actual error on vdis . ... actual error on mg2 . ... actual error on m21 . ...

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• LEDA data base
• Documentation: LEDA: parameter:
• HyperLEDA documentation: parameter: bve

... subroutine CAL_getEffectiveArea(theta, phi, Elo, Ehi, area) use types real(kind=double), intent(in) :: theta, phi real(kind=double), intent(in) :: Elo, Ehi real(kind=double) :: area end subroutine . theta: off-axis angle position in the TELCOORD reference system at which the effective area curve is requested. phi: azimut angle position in the TELCOORD reference system at which the effective area curve is requested. ...

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• Parameters
• Input

... Correcting ETC Calculations of CCD Spectral Observations for CTE Effects . ... HST Overview . Overview . ... Post-Observation . ... ETC . ... ID: CL Script for Applying CTE Loss to Output of Spectroscopic ETC . ... However, the STIS ETC calculations do not incorporate these CTE effects as yet. ... The output from this script should then be used to calculate the appropriate input flux level for a second run of the ETC, which will then yield output which is corrected for the CTE effect. ...

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• PSF Effects
• Simulations
• Fine Guidance Sensor Instrument Handbook

... 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/~cima/bad_fits_1.txt
• http://www.naic.edu/~tghosh/software/pcheck.pro
• http://www.naic.edu/~phil/optics/tdposaug01/tdposforprf.html

... Impact on source motion in Galactic coordinate system is given by Kovalevsky (2003), Malkin (2011) l cos b = -A sin l, b = -A cos l sin b, where A = R0 02 /c is the galactocentric acceleration called hereafter the GA constant. ... We just have to return to the traditional many-centuries-old astrometric practice of modelling the position of a celestial object as a linear trend with two parameters: the position at the initial (conventional) epoch and the apparent (proper) motion. ... 2011). ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf

... 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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• Telescope Parameters
• lsst.coordConv: coordConv::Coord Class Reference
• lsst.coordConv: coordConv::PVTCoord Class Reference

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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• A Region mask for a radial profile in concentric, elliptical annuli
• *tvmark* - Mark pixel positions on the display
• Regions and Source Parameters

... CentralProcessor 0.11 documentation . ... Most of the time, these will be generated using the ACES footprint.py tool, and so all you need to specify are the footprint name, the position angle and pitch (separation of beams), and the frequency band you are observing in. ... If you have not loaded the ACES module, it is likely the footprint.py task will fail, and mosaicking will be disabled. ... User Parameters - Continuum Self-calibration . User Parameters - Continuum Source-finding . ...

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• Summary List of Setup File Parameters
• User Parameters - Continuum imaging CentralProcessor 0.11 documentation
• Fitting a tilted ring model to a warped galactic disk

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

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• Restrictions on the Scenario Parameters
• Initial parameters of compact stars
• Dependence on the Scenario Parameters and Initial Distributions

Next: Stellar models Up: Introduction Previous: Photometry Contents . In a hierarchical stellar system, the separation between two neighboring stars is always much smaller than the separation of this pair from the next companion in the system, be it another pair or a single star. ... They are also numerically easier to handle than non-hierarchical systems, since each pair can be described with the standard orbital parameters, and each star with a small number of physical parameters. ... System . ...

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• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• Command line procedures
• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• harak_e
• SCORPIO parameters
• Determination of atmospheric parameters and calculation of chemical composition

... 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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• Classification of Objects in the Guide Star Catalog
• The SuperCOSMOS Sky Surveys
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries

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

... The overall globular cluster population is divided by gap in the metallicity function at [Fe/H]=-1.0 into two discrete groups with well-defined maxima at [Fe/H]=-1.60?0.03 dex, and -0.60?0.04 dex. ... Clusters with extremely blue horizontal branches occupy a spherical volume of radius ~ 9 kpc, have high rotational velocities ( V rot =77?33 km/s), have substantial and equal negative radial and vertical metallicity gradients, and are, on average, the oldest group (the old-halo subsystem). ...

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• Vladimir Marsakov Publication List

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Polarization efficiency: size/shape/orientation effects
• Database of Optical Properties -- Level: subpage

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: Skybright Class Reference
• Stellarium: Refraction Class Reference
• Stellarium: TelescopeClientDirectNexStar 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 . ...

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• mod_session_crypto - Apache HTTP Server
• Determination of the Detector Parameters
• Tunable Kernel Parameters?

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

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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... 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
• Armagh Observatory