TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• TUI:Telescope:Offset window
• TUI:Telescope:Slew Window:Options:Keep Offsets
• Instrument Orientations and Offset Directions

On,off position switching is done to remove standing waves from the resulting spectra. ... 1,5,10,20,25,50,100 samples corresponding to great circle angular offsets of .004,.02,.04,.07,.09,.18, and .35 degrees. ... Page 1: rms vs great circle offset. ... Page 2: rms vs little circle offset. ... The rms increase correlates better with great rather than little circle offsets. the 1 usec standing wave starts to be seen in the .07 degree offsets. a .9 usec standing wave is seen at .35 degrees offset. ...

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• byu phased array feed.
• encoderOffsets
• a2186

... User Guide ] Key: offset A number of Miriad tasks either take or return celestial coordinates as offsets from some reference position -- invariably the observing center or the reference pixel. ... Offset celestial coordinates are always given in arcseconds on the sky. The offset, (x,y), is related to a true sky coordinate, (RA,DEC), by x = (RA - RA0) * cos(DEC0) y = DEC - DEC0 (These equations should be viewed as a definition, rather than a small angle approximation). ...

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• correlator:axis_offset [ATNF VLBI Wiki]
• casacore: casa::TableMeasOffsetDesc Class Reference
• casacore: casa::IPosition_global_functions_IPosition_Indexing Struct Reference

... HST . ... Data . ... HST Overview . ... Phase I Proposing . ... STIS . ... The offset angle between the STIS aperture axis and the spacecraft orientation reference vector U3 is about 45 degress for the STIS spectroscopic apertures. However, observers should be aware that each STIS aperture has a specific U3 offset angle which is close to, but not equal to 45-degrees. ... Table 1: Offset angles between the STIS spectroscopic apertures and the spacecraft orientation reference vector U3. ... 44.94 . ...

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• What is the offset in the U2 direction that can be taken before a gap appears?
• Offset between CCD and MAMA Coordinate Systems
• MAMA Offset correction table

... This paper describes a simple technique that cancels the DC offsets often found in Hubble Space Telescope's calibrated NICMOS images. ... Hubble Space Telescope NICMOS images often show quadrants with a slight mismatch in DC offset levels after the calibration process. ... Figure 1: NICMOS image showing DC offsets between quadrants. ... Figure: Same image depicted in Fig. 1 after being processed by the DC offset removal algorithm. ...

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• A Method for Minimizing Background Offset Errors When Creating Mosaics

Eyepieces Forum Message . ... Post . ... Secondary Offset . ... Post Message | ... Posted by Jarvis Krumbein on November 2, 2003 18:30:37 UTC . ... Secondary offset - gjeckes - November 2, 2003 - 21:41 UTC . ... www.astronomy.net . About 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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... Observatory . ... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > My OFFSET data are not processed. ... Observing Facilities . ... Instrumentation Development . ... Observing with ESO Telescopes . ... Data Reduction FAQ . ... Offset mode data containing only object or only sky data cannot be processed by the pipeline. ... The DataOrganiser in the current release will not mark such DataSets as incomplete and the recipe xsh_scired_slit_offset will fail. ...

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• ESO - How is the sky spectrum for OFFSET data produced?
• The Cross-correlations

... Transform a qpoe file according to the specified parameters. ... where Xshift, Yshift is the amount of shift in pixels. Any type of filtering can be applied to the input qpoe file, including region filtering. In addition, the size of the output event record can be different from the size of the input event record. ... The following will shift the x-axis by 3.2 pixels and the y-axis by -1.65 pixels, making the resulting qpoe file of small size: . ...

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Comedi Documentation . Prev . Next . comedi_get_buffer_offset -- streaming buffer status . ... int comedi_get_buffer_offset (comedi_t * device, unsigned int subdevice); . The function comedi_mark_buffer_read() is used on a subdevice that has a Comedi command in progress. This function returns the offset of the read pointer in the streaming buffer. This offset is only useful for memory mapped buffers. ... comedi_mark_buffer_read . ... comedi_get_timer ...

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... These offsets correct for low level noisy columns, by artificially suppressing their threshold values. ... 5 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag EPN ADUCONV 0055 2000 ­01­01T00:00:00 OFFSET GAIN NO EPN ADUCONV 0056 2000 ­06­11T03:00:00 OFFSET GAIN NO EPN ADUCONV 0057 2000 ­06­29T02:49:00 OFFSET GAIN NO EPN ADUCONV 0058 2000 ­07­01T08:07:00 OFFSET GAIN NO EPN ADUCONV 0059 2000 ­07­03T12:00:00 ...

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• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0211-1-0.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0062-1-0.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0090-1-0.ps.gz

... Калибровка снимков . Калибровка снимка - это удаление из него паразитной информации, которая включает в себя: темновой шум, горячие пиксели, шум считывания (ток смещения), а также тени от пыли на матрице и оптике. ... В первую очередь нам нужно получить мастер-кадр шума считывания (ток смещения), на западе снимок шума считывания называют Bias или Offset. Мастер-кадр шума считывания нам понадобится для вычитания из основных снимков (снимка объекта), снимков плоского поля, и темновых кадров. ...

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grdgradient - Compute directional derivative or gradient from 2-D grd file representing z(x,y) grdgradient in _ grdfile -G out _ grdfile [ -A azim [/ azim2 ] ] [ -D [ c ][ o ][ n ] ] [ -L flag ] [ -M ] [ -N [ e ][ t ][ amp ][/ sigma [/ offset ]] ] [ -S slopefile ] [ -V ] grdgradient may be used to compute the directional derivative in a given direction ( -A ), or the direction ( -S ) [and the magnitude ( -D )] of the vector gradient of the data. ... If amp is not given, default amp = 1. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grdreformat.html
• Media

import imagingsim_utils import iofits4 def SnapshotMovie(): Illustrate effect of a screen blowin across fnamein= ../ casasim /base/pointsrc.ms.fits screenname = temp/t4.fits for t in range(0, 2000, 180.0) : uvblow.BlowSimple(fnamein, screenname , 6, 6, ../ casasim /windmovie/pint-t%g.ms.fits % t, phasescale =4.0, toffset=t) def LongInteg(): A 50 min obs with 10s integrations fnamein= ../ ...

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• http://www.mrao.cam.ac.uk/~jsy1001/dimmwit/calibration.txt
• http://www.mrao.cam.ac.uk/~bn204/alma/memo-turb/uvblow.py
• OptInt PmWiki : Workstation | History

from visual import * scene = display(range=(20,20,20),width=1280,height=800) scene.background = color .black Delta_t = 0.02 t = 0 # Set up particle grid size = 0.15 grid = [] vel0 = vector (0,0.65,0) colour = (0.7,0.6,0.5) rad = 0.2 spacing = 0.10 baseangle = 0.2 # Head pos0 = vector (10,1.0,0) grid.append(sphere( pos = pos0 ,radius=2.0* rad , vel=vel0, color = colour )) # Body pos0 = vector (10,1.0,0) ...

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• http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_model.txt
• http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_modela.txt
• http://www.mso.anu.edu.au/~bessell/FTP/bessell.cfile

Next: TESTTA/CCD Up: Test Commands Previous: TESTBA/CCD . ... Test F1: Creation of the combined flat frame, using only those flat frames in the input catalogue that have exposure times falling within the allowed range. The combined flat is corrected for the bias offset. ... A combined low count flat frame corrected for the bias offset; . ... The combined low count flat field is corrected for the mean bias offset, stored in the keyword BIASMEAN , filled by the command TESTB/CCD . ...

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• Overscan correction and trimming
• Location of slitlets and flat-field correction
• rotatelogs - Piped logging program to rotate Apache logs - Apache HTTP Server

... New offset/filter box. A new filter/box is available. ... It is lighter, smaller and sturdier than the filter/clock and offset boxes used till now. ... The offset is stabilized to a few parts in a million. ... Notice that only positions 0-3 are meaningful, while values of 4 and above will leave the signal unfiltered. The box has one input BNC, and two output BNC: one outputs the signal with the same polarity as the input, the other reverses the signal (remember that FIRPO has negative output). ...

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• rotatelogs - Piped logging program to rotate Apache logs - Apache HTTP Server
• FIRPO News

Physical and dynamical parameters of particles in outbursting Comet 17 P/Holmes . ... The time depending offset between the center of brightness and center of mass of the comet nucleus has been determined on the ground of positional observations of the comet. ... The motion of these particles allowed subsequent offset between the center of brightness and center of mass of the comet nucleus to be obtained from positional observations. ... comet, dynamical model, outburst, brightness. ...

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• Keywords_69

ntptrace [ -vdn ] [ -r retries ] [ -t timeout ] [ server ] . ntptrace determines where a given Network Time Protocol (NTP) server gets its time from, and follows the chain of NTP servers back to their master time source. ... Note that the stratum is the server hop count to the primary source, while the synchronization distance is the estimated error relative to the primary source. ... Prints verbose information about the NTP servers. ...

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• Introduction to Layers
• MaDgimp: Mercury Effect
• Hands On; Tiled Backgrounds

fitshdr - FITS-file headers manipulation tool fitshdr [options] [FITSfile_name] . ... fitshdr [options] --edit FITSfile_name . ... If You want to modify headers of FITSFILE using new FITS-header lines from HEADER file (or from stdin), You have to use this option (You can skip this option, if -H or --header option is used). ... Empty header lines are not displayed (in 'dump' mode only). --line-offsets . ... In 'dump' mode: file offset will be displayed for each header line. --no-line-offsets . ...

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Comparing files in... D:\WORK with files in... D:\WORK Comparing ARCHI-FR.EXE with ARCHI-MY.EXE - Compare failure. Offset 1fe96h Source = 75h Destination = 90h Offset 1fe97h Source = 7h Destination = 90h 2 Mismatches - Ending comparison.

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• http://crydee.sai.msu.ru/ftproot/pub/rec/games/unsorted/thegame.hnt
• http://crydee.sai.msu.ru/ftproot/pub/rec/games/Cracks-Solutions-Cheats/Populous/populous.hnt
• http://crydee.sai.msu.ru/ftproot/pub/rec/games/Cracks-Solutions-Cheats/Dallas_Quest/dallas.hnt