Next: Auxiliary Data Up: Spectral Analysis Previous: Convolution and Deconvolution . Interactive continuum determination can be done with the command NORMALIZE/SPECTRUM as mentioned above. There are commands to measure the position of spectral features. ... Measurements of line strengths and equivalent widths can be obtained with the command INTEGRATE/LINE . ... The fitting package permits the determination of line parameters and additional modelling of the data. ...

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... In order for FOS to have observed a target, that target must, naturally, have been located in the instrument aperture. ... An FOS Onboard target acquisition: Used either a Binary Acquisition (ACQ/BINARY), a Peakup or Peakdown (ACQ/PEAK), an interactive acquisition (INT ACQ), an early FOS Image (ACQ) or a firmware acquisitions (ACQ/FIRMWARE). ... The overwhelming majority of FOS target acquisitions used the onboard acquisition modes ACQ/BINARY and ACQ/PEAK. ... High wavelength accuracy. ...

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• Fine Guidance Sensor Instrument Handbook
• Obsolescent Acquisition Parameters
• FOS Data Handbook

... Pre-university education . ... For the year Samara State Aerospace University moved up in the ranking of Vladimir Potanin Foundation from the 44th to the 10th place and added three positions in the ranking of universities reputation Expert RA in the field of Engineering, natural and exact sciences . Samara State Aerospace University has significantly improved its position in the ranking of universities of Vladimir Potanin Charitable Foundation at the end of academic year 2014-2015. ...

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• SSAU rose in the world ranking of universities Webometrics for 1379 positions

... Format of the orbital elements | Estimation of the extrapolation errors | Version 1" of the orbital elements collection, determined by KIAM during flight and used for operations planning . Version 2" of the of the orbital elements collection, modified by IKI during flight and recommended for the orbital calculations during scientific data processing . ... Three kinds of the INTERBALL Auroral probe (IB_AUR) orbital elements' collections are presented here. ... IKI RAN | SSC IKI RAN | ...

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• About modification of the INTERBALL orbital elements
• STDA files
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... Next: 7 kslice_3d: slicing data Up: Karma User Manual Previous: 5 Volume Rendering a . The <kpvslice> programme allows you to use a two-dimensional image to define a slice through a three-dimensional data cube. ... The slice is drawn on the total column density or velocity field map, and the corresponding position-velocity diagram will appear in the other window. ... To load the cube, press the Cubes button in the left window and select a cube file. ... The image is displayed in the left window. ...

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• velplot
• clplot
• HI Catalogs Galaxy Properties

Each receiver has a turret position to place the horn at the focus. ... current . 14may04 (02may04 survey) . ... sbn rcv . ... 14feb04 horn survey . ... 13feb04 (13 feb04 survey) . ... sbn . ... mod14/sbn/mar03 . ... survey feb04. mod15/may04 . ... horn move,survey,model may04 . ... horn move, survey feb04 . ... horn move,survey,model may04 Notes: . ... After the may04 surveys, sbn and lbw were not moved in the x direction (za) because there was no room in the hole in the turret floor. home_~phil ...

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• Test of Position Switching with a Specified Off Position
• Programmer Position in Astronomy
• AGES Database Search

... 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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• On-line Access to Very Large Catalogues
• ADASS 2003 Conference Proceedings
• NICMOSlook and Calnic C: Slitless Spectra Extraction Tools

... This can be used to overlay the position of fiducial stars onto an image, for example. Positions can be input manually or from a list. To position marks interactively display the image and then cl> noao no> images im> tv tv> tvmark 1 STDIN interactive+ type . to put dot at cursor position type + to put cross at cursor position type c to put circle at cursor position (must specify hidden parameter ``radii'') <ctrl>d to exit . ...

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• The AstroStat Slog Blog Archive [Jobs] postdoc position at UC Berkeley
• *tvimcontour* - Overlay contours and/or source positions on the display
• *skypix* -- conversion of pixel position to sky coordinates

... This task needs as input, in addition to the spectrum and detector map, the position of the source in question. ... The task gets this information from one of two sources: from the centre of the source region in the input spectrum (if the parameter withsourcepos false ), or explicitly from the user ( withsourcepos true ). If the latter, the user can choose to specify the position in one of four coordinate systems: EQPOS, POS, TEL and DET. ... Conversion to DET coordinates . ...

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... 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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• PhD position, Centre for Astronomy, NUI Galway: deadline 18 July 2008 |
• Postgraduate Positions
• Research Technician Post

Chair of solid state physics . ... position in MIPT: . Professor, Head of the Solid State Physics Chair . position in ISSP: . ... scientific degree: . Dr. S. e-mail: . kveder@issp.ac.ru . ... Professor, Deputy Head of the Solid State Physics Chair . ... zverev@issp.ac.ru . ... Secretary of the Solid State Physics Chair . ... povarova@issp.ac.ru . ... dev@issp.ac.ru . ... kulakovs@issp.ac.ru . ... maksimov@issp.ac.ru . ... Professor, Dean of the General and Applied Physics Department . ...

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... Luminosity (L) · · · · A source's luminosity is the power that it emits in radiation. ... NB Astronomers often say `flux' when they mean `flux density' · SI units are Wm-2Hz -1 -26 filter · Also used are Jy 10 Wm-2Hz -1 E= РРРF d dA dt Specific Intensity, Surface Brightness (I) · Specific intensity (or surface brightness) is the power received (or emitted) per unit area per unit frequency per unit solid angle. ч F at surface of a spherical source = I · · Specific intensity is independent of distance...

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• Determination of the relative orientation between radio and dynamical reference
• NVSS Image ftp service Documentation Help for NVSS Image ftp service
• VLSS Image ftp service Documentation Help for VLSS Image ftp service

... FIELD | ... static int . ... Field Detail static final int AREA . ... Constant Field Values . static final int MEAN . ... static final int STD_DEV . ... static final int MODE . ... static final int MIN_MAX . ... static final int CENTROID . ... static final int CENTER_OF_MASS . ... static final int PERIMETER . ... static final int LIMIT . ... static final int RECT . ... static final int LABELS . ... static final int ELLIPSE . ... static final int INVERT_Y . ... static final int CIRCULARITY . ...

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• FFTFilter (ImageJ API)

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

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• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• ST-ECF Grism Spectrum Software for NICMOS Grism Data

... They are the offset in arcseconds for the x and y inst plane offset, the exposure time in seconds, and the number of exposures at each position. ... A point about offsets should be made here. The dither program uses absolute instrument plane offsets, so you should use object plane offsets to center up on the chip so that the script starts from where you centered up. INST and OBJ offsets are independent so an object offset will not be zeroed out by and inst plane offset, just added to it. ...

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• TUI:Tidbits:Entering Sexagesimal Positions
• M1 Airflow Lab Tests
• Guider Image Controller Overview

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. ...

17. ENGAMPLE

18. http://www.mso.anu.edu.au/coala/form.html

19. Stellarium: BigStarCatalogExtension::StarWrapperBase Class Reference

20. I Think What You're Saying Is Not A Deeply-considered Position - an Astronomy