MAKING THE PROFILES . First of all you are expected to load a FITS file ("FILE"-"LOAD"). ... By pressing the middle button you copy the profile from the first profile window to the second one. ... An example: first integral can correspond to the profile of active region and second integral can correspond to the profile of quiet chromospheric region. ... The second profile (which is subtracted from the first one) you extract after clicking on "SUBTRACT"-"MARK QUIET PROFILE" and marking the region. ...

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Program: GETVAL Purpose: Get image values at given positions in a set Category: UTILITY File: getval.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (,subset): Maximum number of subsets is 1. ... The image values are formatted according the string entered in FORMAT= APPEND= Ok to append? ... The flag characters and their meanings are: - The result of the conversion is left- justified within the field. ... If the result of a conversion is longer than the field width, an asterisk is returned. ...

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• kpvslice: interactive position-velocity slicing

... COS/FUV Lifetime Position 3 Line Spread Functions and Cross-dispersion Spread Functions now available on the COS website . ... Line Spread Functions (LSF), which describe the one-dimensional line profile of an infinitely narrow spectral line from a point source, and Cross-dispersion Spread Functions (CDSF), which describe the cross-dispersion profile of a point source on the detector, are now available on the COS website (see http://www.stsci.edu/hst/cos/performance/spectral_resolution ). ...

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• COS FUV Spectra Shifted to New Lifetime Position.
• Summary of new COS Lifetime Position Characteristics
• ACS Data Handbook

... Circles are used to depict the source positions. ... A optional ID label can also be displayed alongside the circle, corresponding to the row num- ber of that source in the input source list. ... These circles are in fact DS9-type regions, which can be written out to a le for future use (for example, when running a later DS9 session) by setting withregionfile to true, and specifying the desired le name via the regionfile parameter. ... This is a text le containing region descriptions for each source...

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• http://xmm.vilspa.esa.es/sas/7.1.0/doc/srcdisplay.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/srcdisplay.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/srcdisplay.ps.gz

User should choose the type of coordinates and type of positions by marking corresponding radio button, first in the column headed Type and then in the column headed Positions . Rectangular coordinates are compatible only with choice Geometric . ... Remember that photographic or CCD observations are comparable with astrometric positions, whereas meridian observations are comparable with apparent ones. Observations made in horizontal coordinate system also are linked to apparent positions. ...

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OFFICIAL PRESS RELEASE . ... to the International Space Station . ... The vehicle and ISS docking is scheduled on 27 May 2004 with berthing to the axial docking port of Russian Service Module Zvezda. ... The prelaunch processing was directly led by the Technical Management (Yu.P. Semenov, Technical Manager of Russian Piloted Space Programs, General Designer of S.P. Korolev RSC Energia, Academician of the Russian Academy of Sciences). ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• PRESS RELEASE - S.P. KOROLEV ROCKET & SPACE CORPORATION ENERGIA

Instructions for using Menu-driven Axis Control Software . ... Altitude and azimuth axes use position feedback and the setting is in counts per second times 10. ... Use b to set the brakes and use c to clear the brakes for the corresponding axis, either azimuth or altitude. ... Use m to move to the previously specified position and velocity for the corresponding axis; either azimuth or altitude. ... Use g to move to the previously specified position and velocity for both the azimuth and altitude axis. ...

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• Plug-plate coordinate system
• TUI:Telescope:Offset Types
• TUI:Instruments:NICFPS:NICFPS window

... The keywords EXPRTIME and ZEROMAGN set the zero point for magnitudes. ... The program automatically determines a Point Spread Function when it gets proper initial values from the keywords SPROFIL. Initial values may be wrong by 0.1 each, and the program still can converge to the right Point Spread Function. ... The program looks for an initial point spread function into that descriptor at first and it uses data from the keywords SPROFILx when the descriptor DPROFILE is absent. ...

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• Event Handling
• Emission-line galaxies
• Closing down

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• Thesis Figures
• ON/OFF (Position Switching)
• on,off position switching offsets

Armagh Observatory, 16 January 2002: . Apostolos Christou and John McFarland have made the first detection, from anywhere in Ireland, of the shadow cast by a star of an asteroid as it passed over Armagh. Such events, known as asteroidal occultations, allow a precise fix to be made on the asteroid's position in space, and also an estimate of its size and shape. ... Asteroids are mostly small, rocky objects, lying hundreds of millions of miles from the Earth between Mars and Jupiter. ...

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

FSP1 : The time intervals corresponding to the INTERBALL TAIL PROBE (IB_TAIL) or GEOTAIL passage through the simulative magnetosphere boundary layer (BL) . ... FSP3 : That part of the FSP1 or FSP2 time intervals, which corresponds to the magnetic conjugations between any couple of the considered spacecraft. The value of the relative geocentric angular distance between magnetic field line's footprints is considered during FSP3 situation selection. ...

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• Satellite position in the SE and GSM coordinate systems
• Corrected Geomagnetic Coordinates
• The TAIL 1996/1997 campaign

... 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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• The AstroStat Slog astro-ph
• The AstroStat Slog positional citation effect
• The AstroStat Slog Blog Archive [ArXiv] The Importance of Being First: Position

Download Izmccd (~2.7 MB). ... If you want to calculate equatorial coordinates of object: . Click the " File " menu, and then click " Open " ; or press  on toolbar. Choose a file with image. ... Also see section " Viewing of image ". ... Before, if it is necessary, you must make an account dark current and flat field (See section " Preliminary processing of images ".) ... Measure the marked stars. ... Click the " Calculations " menu, and then click " Coordinates " or . ...

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... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA - Images of Camera

FSP1 : The time intervals corresponding to the INTERBALL TAIL PROBE (IB_TAIL) or GEOTAIL passage through the simulative magnetosphere boundary layer (BL) . ... FSP3 : That part of the FSP1 or FSP2 time intervals, which corresponds to the magnetic conjugations between any couple of the considered spacecraft. The value of the relative geocentric angular distance between magnetic field line's footprints is considered during FSP3 situation selection. ...

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• Pictures/Рисунки
• Fig11
• Corrected Geomagnetic Coordinates

... On-line Data . ... The program enables to find out the exact present Earth coordinates of the international space station and "Shuttle". ... J-Track - this program is similar to the previous one, however it knows how to display images and orbits of space vehicles. ... NASA SkyWatch - a program for those, who are fond of watching artificial space objects through the telescope, field - glass or with the unaided eye. ... Info: Industry news On-line Data Company ATLAS news Events We in press Contact . ...

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• Plan and technical specifications of the Baikonur cosmodrome, Russia's space

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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• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
• Space Telescope-European Coordinating Facility
• stecf.impol - Package Tasks

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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• Scan data
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• The star cluster Westerlund 1 and the positions of the magnetar and its

... 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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• Development of an ADS Data Dictionary Standard
• ASC Coordinate Transformation -- The Pixlib Library, II
• NICMOSlook and Calnic C: Slitless Spectra Extraction Tools

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Our BVR CCD photometric study of the globular cluster NGC 7006 permitted us to find two new suspected RR Lyrae variables. A cluster chart is presented with the position of known and suspected variables marked. ... According to the Catalogue of Variable Stars in Globular Clusters (Clement et al., 2001), it contains 76 variables, most of which are RR Lyrae variables, the RR1 to RR0 ratio being 8:55. ... for suspected and some of known variable stars. ...

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• Astronet > Sky Map, professional edition
• Hale Bopp: A Continuing Tail
• Астронет > Hale Bopp: A Continuing Tail