Program: TRACE Purpose: TRACE plots image values at user given positions as function of distance to a plot centre (in 2-d (sub)sets). Category: ANALYSIS, PLOTTING File: trace.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (, subset): Only one subset is allowed. ... XYBOX= Give size of box around one pixel: [3,3] The resulting value at a selected position is an average of the pixels in the defined box around that position. ... POSITION= Give position x, y: Physical values are allowed. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/tsk/pbcorr.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/sub/gdspos.dc2
• Source Fitting and Positions

Kermit writes data as FITS files which are fairly standard but nonetheless there are a few details you may want to be aware of. Kermit FITS files contain an NxNxM array of 32 bit integers. ... The values stored in the 32 bit integers are the sum total of counts read at that pixel during the exposure. ... To achieve this normalization, you almost certainly want to normalize the image by dividing it by the NREADS FITS keyword value. ... The current focus position is stored as the FOCUS keyword. ...

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• COS Data Handbook
• PSF Variations with Field Position
• Chapter 4: Solar System Targets

Routines can now be called with keyword arguments and can use default arguments, that means that some arguments can be given with keywords instead of position and some do not have to be given at all, in which case a standard or default value is used. ... IMPLICIT NONE INTERFACE SUBROUTINE SOLVE (A, B, N) INTEGER, INTENT (IN) : : N REAL, INTENT(OUT) : : A REAL, INTENT(IN), OPTIONAL : : B END SUBROUTINE SOLVE END INTERFACE REAL X ! ... You will use keyword arguments and default arguments so that . ...

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• Dynamic HTML in Communicator
• Long description for example illustrating positioning with respect to a

... 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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• HyperLEDA documentation: (auxdistance) auxiliary table for distance catalog
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XMM-Newton Science Analysis System Page: 1 imsample July 9, 2007 Abstract This task takes as inputs a ts image and a list ( ts table) of positions in the image pixel coordinates. The task samples the image at each of the positions and writes the result to a speci ed column in the ts table. ... At present, the list of positions (which must be a binary table extension in a FITS le) must contain columns which give the position in image pixel coordinates. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/imsample.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/imsample.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/imsample.ps.gz

... 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. ...

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• Keywords_369
• Keywords_65
• Keywords_26

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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• The Favourable Spatial Position Criteria
• The Favourable Spatial Position
• Lagrangian Points

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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• optics
• ON/OFF (Position Switching)

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)

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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• ESO - ALMA
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• ESO - How do I interpret the SEQ TIME keyword values?

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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• Spatial Region Coordinates
• zhtools
• The AstroStat Slog Blog Archive [ArXiv] The Importance of Being First: Position

... Positions in 2000 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2001 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2002 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2003 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . Positions in 2004 - Jan - Feb - Mar - Apr - May - Jun - Jul - Aug - Sep - Oct - Nov - Dec . ...

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• IDLINES: identifying spectral lines
• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• Armagh Observatory

For all keywords that contain a red and a blue value, the blue value comes first. ... The full pathname, but without the trailing "b.fit" and "r.fit", that would be given to the next exposure if the basename argument is not given to the expose command. ccdHeaters=float,float . ... bluelambda2=float [M] . The center wavelength for the given grating: the 1 or 2 indicates the grating bay. The bluelambda and redlambda keywords match one set of these, depending on the position of the turret. ...

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• TUI:Telescope:User Catalogs
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. Next: Initial velocity Up: Space and velocity distributions Previous: Space and velocity distributions . Following Paczynsky (1990), we assume initial space distribution of young neutron stars to be varying exponentially with distance from the Galactic center and from the Galactic plane, that is probability distribution for young neutron star positions can be written in the form . with kpc, and pc. Mike E. Prokhorov . Fri Jul 19 19:16:07 MSD 1996

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... 7C(G) catalogue -------------------------------------------------------------------------------- See also: J/A+AS/110/419 : 7C: 151MHz survey of region RA=17h, DE=+65deg (Visser+, 1995) J/MNRAS/282/779 : 7C: 151MHz survey of region 9-16h 20-35deg (Waldram+ 1996) J/MNRAS/298/637 : 7C: 151MHz survey of 3 regions (Pooley+, 1998) Byte-by-byte Description of file: catalog.dat ---------------------------------------------------- ...

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• NVSS Source Search ($Revision: 1.6 $ - running v2.17)

... 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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• IRAF Multiple Extensions FITS (MEF) Files Interface
• Development of an ADS Data Dictionary Standard
• ADASS 2003 Conference Proceedings

. Computer Ephemeris. Lunar equatorial positions. Explanations. Each row contains at 0 h and 12 h of Time Dynamical Terrestrial: month, day, apparent right ascension (hours, minutes, seconds), apparent declination (degrees, minutes, seconds of arc) and geocentric distance (in Earth's radii).

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• Central meridian positions for physical observations of Uranus for Computer
• Central meridian positions for physical observations of Saturn for Computer
• Central meridian positions for physical observations of Neptune for Computer

I/146 Positions and Proper Motions (Roeser+ 1988) ================================================================================ Catalogue of Positions and Proper Motions Roeser S., Bastian U. =1988A .. ... 449R ================================================================================ ADC_Keywords: Positional data; Proper motions Description: PPM North gives J2000 positions and proper motions of 181,731 stars north of -2.5 degrees declination. ... The mean epoch is near 1931. ...

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• Positions and Proper Motions - South
• Supplement to the PPM Star Catalogue

Radio Interferometry Principles . Radio Interferometry Signal Processing . ... A radio interferometer consists of a pair of directional antennas that are tuned to receive radio emissions from a source in a desired RF band. ... The antennas are pointed at the radio source of interest and are set up to receive the signal and process it into a form suitable for transmission to the correlator. ... In connected element interferometry, the digital signal goes directly to the correlator. ...

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• PULK GNSS station

Создание тестовой базы данных Kafedra BEGIN; DROP TABLE lectures; DROP TABLE students; DROP TABLE semestrs ; DROP TABLE courses ; DROP TABLE balls; COMMIT; */ BEGIN; /* Лекторы */ CREATE TABLE lectures ( id_lect INTEGER PRIMARY KEY, surname VARCHAR (50) NOT NULL , name VARCHAR (20) NOT NULL , patronim VARCHAR (50) NOT NULL , phone VARCHAR (20) NOT NULL , mail VARCHAR (20) NOT ...

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• Dome position
• New spectra of R CrB
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