... Inst Data Fit allows one to determine various parameters needed for instrument data files, including: scale, orientation and the position of the rotator with respect to the instrument. ... Run Inst Data Fit. ... Specify all fields above the "Fit Scale and Orientation" button New Rot_Inst_ang . ... Modified the instructions so that new scale and orientation values are applied to the instrument block before measuring center-of-rotation data (to solve a problem brought to light by SPICam). ... R.O. ...

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• TUI:Telescope:Offset Types
• TUI:Introduction
• TCC User's Guide

During observation the target is placed at the aperture (PC1, WF2, WFALL, etc.) specified on the Phase II proposal. ... The POS TARG special requirement can be used when a position offset is needed. ... The exact directions of the offsets are parallel to the rows and columns of the CCD on which the aperture is specified. ... This is specified in the Phase II proposal using the ORIENT special requirement. ... Figure 7.9 shows the CCD orientation and aperture locations relative to the U3 axis. ...

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• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
• Fine Guidance Sensor Instrument Handbook
• WFPC2 Instrument Handbook

... AVERAGE/TABLE frame table xy_col outcol [size] . ... BACKGROUND/ECHELLE in out [radx,rady,step] [degree] [smooth] [method] . ... BACKGROUND/SMOOTH input output [radx,rady] [niter] [visu] . ... performs order definition and wavelength calibration . ... DISPLAY/ECHELLE image [g_flag] . ... Extract echelle orders and produces a frame in space pixel-order . ... LOAD/ECHELLE . display echelle orders (and optionally background) positions . ... Plots the overlap region between adjacent orders n and n+1 . ...

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• Using a Standard Star
• What was measured?

... The sky position of a single source may be entered via the parameters ra , dec and (optionally) errorradius . ... In this mode, the output positions are printed to a single line of standard output. ... Source dec = <dec> deg. # # rawX rawY ccd On chip? +xxx.xx +xxx.xx xx x 123456789 123456789 12345678 . ... Source dec = <dec> deg. # # detX detY +xxxxx.x +xxxxx.x 123456789 12345678 . ... Source dec = <dec> deg. # # detX detY det err +xxxxx.x +xxxxx.x xxxxx.x 123456789 123456789 123456789 . ...

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... To set the coordinates in E2000 use xpaset -p tel target [ra] [dec] All commands and arguments are lower case. ... Primary functions set or get values and provide basic control with the actions noted tel status [exit/on/off] manage xpatel and the telescope controller tel goto [on/off] go to target tel track [on/off] toggle track on and off tel guide [on/off] toggle precision guide on target tel target [#] [#] target coordinates [RA (h)] [ Dec (deg)] (E2000) tel ...

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• University of Louisville Research Telescope at Mount Kent
• Moore Observatory Remote/Robotic Telescope

On 12jan16 the turret failed to arrive on position. ... At that time i thought the problem was from the backlash board being misadjusted.. but it turned out to be a problem with the zero velocity offset of the dac that drives the motor amplifier (in velocity mode). ... The errors should be small when the turret is sitting at one position (while it is moving, the error will be large). plots of turret position and position offset for 1st day of each month for 2015 (.ps) ( .pdf ) . ...

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• on,off position switching offsets
• Details of Rotang
• byu phased array feed.

... TESIS . ... position: Head of the XRAS Laboratory, TESIS Main Designer and Instrument Manager . ... address: LPI, main building, room 177 . ... tel. (499) 132-65-96 . ... address: LPI, main building, room 173 . ... tel. (499) 135-80-81 . ... address: LPI, main building, room 275 . ... address: LPI, main building, room 173a . ... address: LPI, main building, room 174 . ... address: LPI, main building, room 179 . ... address: LPI, main building, room 180a . ... address: LPI, main building, room 178 . ...

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INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...

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• Lunar equatorial positions. Explanations for Computer Ephemeris.
• Lunar physical observations. Explanations for Computer Ephemeris.

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Circular polarization of the bright side of Iapetus versus wavelength, obtained with FORS2 at the ESO VLT during the night 2011-03-28 at a phase angle of 0.77 . ... It can be noted that a change in signal occurs in circular polarization observations that are taken after rotating the instrument by 90 degree with respect to the intial position angle on the sky. ...

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• Planetary positions
• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |

Next: Plotting Up: Polarisation Previous: Polarisation . Currently the receiver position angle is not read from the RPFITS file and a position angle of zero is assumed. ... It is possible that there is a phase offset between polarisation which will effect the phase of the cross polarisation correlation, and so give rise to spurious polarisation. rotate_xyphase can be used to correct for this error. ... ASAP> scans.rotate_xyphase(10.5) # Degrees . ...

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• ROTATION
• kpvslice: interactive position-velocity slicing
• News Results

... Meade Instruments Corporation . ... Microscope Instruction Manual . ... Meade Model 9600 Microscope Introduction. The Meade Model 9600 Microscope is a precision instrument with the important advantage of a binocular eyepiece head. ... Your Meade Model 9600 Microscope requires some minor assembly of the Eyepiece and Objective Lenses. ... The Meade Model 9600 Microscope offers magnifications of 100X, 400X, and 1000X with the 10X eyepiece, 125X, 500X, and 1250X when used with the 12.5X eyepiece. ...

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• Meade Instruments Corporation - ETX-90EC and Autostar Frequently Asked...
• Meade Instruments Corporation - Meade Model 9460 Microscope Instruction Manual
• Meade Instruments Corporation - Meade Model 9400 Microscope Instruction Manual

hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)

Next: The Transmission Gratings Up: The Instruments Previous: The Instruments . ... A conventional cross-grid charge detector reads out the photo-induced charge cloud and the electronics determine an arrival time to 16s, and the position with a resolution of about 18 m or 0.37 arcsec. ... The Massachusetts Institute of Technology's Center for Space Research, in collaboration with Lincoln Laboratories, developed the detector system and manufactured the CCDs; Lockheed-Martin integrated the instrument. ...

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• The Instruments

The polar oval complete and partially visibility for the optical instruments on board of the AURORAL PROBE are shown by different symbols . The polar diagram of the Spacecraft positions magnetic mapping during polar oval visibility for the UVAI and UVSIPS cameras. The polar diagram shows the Spacecraft corrected geomagnetic co-ordinates : co-latitude - local time . ... The real time visibility (Moscow time MT=UT+3h). Date is shown along the X-axis, the MT - along the Y-axis. ...

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• Trigonometry beyond 90 degrees
• The Wind Spacecraft
• Navigation--lesson plan #8

polimplot -- Plot a polarization vector map . ... inpol = "" [name] . Input linear polarization image (in %) to plot. inpopa = "" [name] . Input image for position angle of linear polarization vectors (degrees). poi_err = "" [boolean] . ... Name of corresponding polarization position angle error image (degrees). ... This task is a flexible tool for plotting a polarization vector map from two images of the polarization and the position angle of the polarization vector. ...

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• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)
• Correct positioning | ESO United States
• Correct positioning | ESO

... All the ELT pro jects present a segmented primary mirror. ... In 2001 Esposito [3] proposed the PWFS as phasing sensor for segmented mirrors, demonstrating, with numerical simulations, that the sensor can sense and control at the same time differential piston, tip and tilt of each segment. ... A new co-phasing loop has been arranged with the PWFS and the segmented mirror of NAOMI [6] (the AO system located at the telescope nasmith platform). ...

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• Mechanics and Cryogenics
• Procedures for Observations
• Converting Modules from Apache 1.3 to Apache 2.0 - Apache HTTP Server

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• QPOE Files
• Fixing and Freeing Region Markers

Telescope Tip-Tilt Secondary Mirror The tip-tilt secondary mirror on the ANU 2.3 m telescope · Measures and adjusts image position at 30 Hz · Corrects image blur produced by turbulence in the Earth's atmosphere · Both the tip-tilt secondary mirror and the 2.3 m telescope were designed and constructed by RSAA ...

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• Untitled1
• GSAOI Instrument Description Page
• Gemini NIFS May 2002 First Cool Down.

The Wind spacecraft. ... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... For additional details and updates, see the home page of the "Wind" mission. Exploration" home page (index) Glossary . ...

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• Corrected Geomagnetic Coordinates
• Seasons of the Year
• FM-3I Instrument

... The SIRTF Science Center is developing two Web-based tools that will be used during operations. One tool is for Quality Analysis. ... The basic design requirements for the QA tool are (1) that it provide an easy way of looking at all the data, observation by observation, and (2) that it provide an easy way to specify status and comments for each observation. ... The data accessed by this tool consists of meta-data in the central database as well as the actual data files in the archive. ...

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• WinTICS-24 Version 2.0 and PFITS-An Integrated Telescope/CCD Control Interface
• Three Instruments in Four Years: The UCO/Lick Data-Driven Toolkit
• ADASS 2003 Conference Proceedings