... It also sends commands to the trolley micro to switch between track mode and slew mode. ... Laser head (7702) Linear interferometer (7002) Retroreflector(7003) Various mirrors Beam expanders Fibre optic pickup Measurement board(2002) Datum switch(Sony SETP151) A schematic layout is shown below in Fig 1 Optical fibres connect the receiver to the measurement board and from the laser to the reference input on the measurement board. ... Reset the datum latch circuit. ...

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• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.DesignDocumentation/vmesoftware.pdf,1200671764
• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.DesignDocumentation/vmesoftware.pdf
• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.DesignDocumentation/vmesoftware.pdf,1200916642

... mm] CAMCOORD1 2 translation in X . ... mm] CAMCOORD2 origin in SACCOORD - X . ... mm] origin of telescope frame in SACCOORD - X . ... X-coordinate of center of PIXCOORD1 pixel (RAWX0/RAWY0) in CAMCOORD1 system . ... absolute uncertainty associated with X0 (currently unused) . ... absolute uncertainty associated with EULER_PHI (currently unused) . ... absolute uncertainty associated with EULER_THETA (currently unused) . ... absolute uncertainty associated with EULER_PSI (currently unused) . ...

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This diagram illustrates the effects of absolutely positioning a box. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. All text outside the "outer" box has been flowed into lines 1 and 2. The "outer" box is positioned absolutely so that it occupies the lower right quadrant of the document window. ... The lines, as they appear in the image, contain: 1 Beginning of body contents. End of 2 body contents. ... Inner 7 contents. End of 8 outer contents. ...

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• Long description illustrating absolute positioning with respect to the initial
• Long description for example illustrating positioning with respect to a
• Long description for example with unclipped overflow

... Even the maximum velocity can't be applied yet, due to the acceleration limit. ... The algorithm used is as follows: When the integral term is being used, the correction velocity is given by Vcor = kP ( x-xDES ) + kI therefore, the change in one cycle is ( x-xDES ) dt Vcor = kP ( x-xDES ) + kI ( x-xDES ) t Vcor = kP [( x-xDES ) - ( x-xDES ) old ]+ kI ( x-xDES ) old t Vcor = kP ( x-xDES ) + (kI t - kP) ( x-xDES ) old Vcor = kP ( x-xDES ) + q( x-xDES ) ...

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• http://www.naic.edu/~phil/turret/encoder.html
• turret history
• td_move_nuts

... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document ?Programmatic Requirements for Gemini Instrumentation Development? states the requirements for the Software Maintenance Manual . ...

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• The High-Z SN Search Description

COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 8: Target Acquisitions > 8.5 ACQ/PEAKXD Acquisition Mode . ... The target XD location is assumed to be the median position (NUV) or mean position (FUV) of the collapsed spectrum. ... If the target is centered in the aperture, but the Y walk shifts its spectrum in the XD direction, then the ACQ/PEAKXD algorithm will miscalculate its centroid and move the target away from the aperture center. ...

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• Introduction
• Sample Shifting
• A Brief Description of the Instrument and Its Operation

... A response matrix is a discrete representation of a given instrument's response to incoming photons. ... This presentation is a preliminary report on MKRMF, a new tool developed by the Chandra X-ray Science Center (CXC), to calculate RMFs appropriate for the variety of science instruments on-board Chandra (Wise 1998). ... These external redistribution functions are stored using a new FITS format developed by the CXC for encapsulating functions. ... axes file : . ... list file : . ... CXC RMF Format ...

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• ADASS 2003 Conference Proceedings
• Calculating the Position and Velocity Components of HST
• Modeling AXAF Obstructions with the Generalized Aperture Program.

Software Forum Message . Forums: . ... Discussion Forums | Astronomy Software Discussion | Post . ... Star Positions.. Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Your Description Is To Vague. - an Astronomy Net Education Forum Message
• I Think What You're Saying Is Not A Deeply-considered Position - an Astronomy
• Well, That's A Pretty Emotional Response! - an Astronomy Net Exploration Forum

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

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... B=Command, 12AB=Azm, comma, 4000=Alt. ... Example: if the desired position is 220°, then POSITION_24BIT = (220/360)*224 = 10,252,743 Separate POSITION_24BIT into three bytes such that (POSITION_24BIT = PosHigh*65536 + PosMed*256 + PosLow). Exampe: PosHigh = 156, PosMed = 113, PosLow = 199 Send the following 8 bytes: a. Azm Slow Goto: 80, 4, 16, 23, PosHigh, PosMed, PosLow, 0 b. Alt Slow Goto: 80, 4, 17, 23, PosHigh, PosMed, PosLow, 0 The number 35 is returned from the handcontrol 4. ...

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• Index of /software/sbig/archive/xmccd-4.1/xmccd-4.1e/xpa-2.1.14
• Index of /software/xmtel/archive/xmtel-3.1/docs/nexstar

Stellarium 0.12.3 . ... Classes . ... File Structure . Class List . Class Index . Class Hierarchy . Class Members . List of all members | ... Position Struct Reference . ... More... #include < InterpolatedPosition.hpp > . ... Definition at line 37 of file InterpolatedPosition.hpp . The documentation for this struct was generated from the following file: . home/aw/devel/stellarium/trunk/plugins/TelescopeControl/src/clients/ InterpolatedPosition.hpp . ...

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• Stellarium: TelescopeClient Class Reference
• Stellarium: VertexP3T2 Struct Reference
• Stellarium: VertexP3T2C4 Struct Reference

... Classes . Files . ... casa::MeasComet . ... MeasComet (const String &path) . ... MeasComet (const Table &tabin, const String &path) . ... Get the name of the comet. const MVPosition & . ... get ( MVPosition &returnValue, Double date) const . ... Construct a table from the name and the input table. casa::MeasComet::MeasComet . ... Get the end of the table (in MJD). const String & casa::MeasComet::getName . ... Get the start of the table (in MJD). const MVPosition & casa::MeasComet::getTopo . ...

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• WCSLIB: sph.h File Reference
• casacore: casa::MSFeedEnums Class Reference
• casacore: casa::SolarPos Class Reference

lsst.tcc   1.2.2-3-g89ecb63 . ... Classes . Files . ... tcc::AxeLim Class Reference . include < axeLim.h > . std::tr1::array < double, 3 >  . ... Note: AxeLim uses separate arrays for position, velocity, etc. instead of containing a vector of AxisLim, so that the load/dump file format is backward compatible with the old TCC. ... std::tr1::array <double, 3> tcc::AxeLim::accel . ... std::tr1::array <double, 3> tcc::AxeLim::jerk . ... std::tr1::array <double, 3> tcc::AxeLim::maxPos . ...

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• lsst.tcc: tcc::PVAJT Class Reference
• lsst.coordConv: coordConv::PVT Class Reference
• lsst.coordConv: coordConv::Coord Class Reference

The electronics of LonGSp is composed of two main parts: "upper" electronics, that is situated near the instrument, and the "lower" electronics, put in the control room. ... There is also the main electronics box that contains the amplifiers and the A/D converters for the four output signals from the detector, the sequence memory which generates the proper timing clocks, and a logic for converting the 16-bit parallel data from the array to a serial format. ...

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• ab - Apache HTTP server benchmarking tool - Apache HTTP Server
• mod_sed - Apache HTTP Server
• mod_ext_filter - Apache HTTP Server

... The first of the equations defines the position of the spectral orders, m , in the raw image, while the second equation gives, for each order, the dispersion relation in one dimension. ... where the coefficients are computed using least squares techniques on a grid , i.e. sample number and line number of points located within the spectral orders of the image. These points in the grid are found automatically by an order--following algorithm, normally using the FLAT or STD image. ...

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• HyperLEDA documentation: compilation of cz measurements (a110)
• HyperLEDA documentation: (distance_method_codes) method codes for distance
• General Description

... To load the PROS software: . cl xray []----------------------------------------------------[] [] PROS RELEASE VERSION 2.4 [] [] October, 1995 [] [] [] [] Before using this version rerun mkiraf [] [] [] [] For answers mail hotseat [] []----------------------------------------------------[] The following general information is available via the help command: help topic: description : pros description of all help options available in pros bugs ...

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• Chandra Images for G359.2-00.8
• Chandra Images for G000.1-00.1
• Chandra Images for SNRJ 0540.1-6919

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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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)

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)
• dfosBackup

For the selected intervals of the UT the co-ordinates of 4 spacecraft are shown with 10-min step. ... The region designations used in the numerical files. The simulative geophysical region models . ...

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• ASCII files description
• The numerical file description
• Space physics cordinate systems