... region (region-6.2.2) [xmmsas_20030110_1802-5.4.1] . ... The region task will automatically determine the optimal source and background extraction regions for a detected source in an XMM observation. ... The regions are defined in sky coordinates. region will attempt to maximise the area of the extraction region for each source, whilst ensuring that the extraction regions of neighbouring sources do not overlap, and that the background extraction region for a given source excludes neighbouring...

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• Source and background regions

The FITS "World Coordinate System" (WCS) standard defines keywords and usage that provide for the description of astronomical coordinate systems in a FITS image header. ... I: "Representations of world coordinates in FITS" , Greisen, E.W. & Calabretta, M.R. (2002), Astronomy & Astrophysics , 395 , 1061-1075. ... This diagram illustrating Bonne's projection with conformal latitude +35 was produced by WCSLIB , a C implementation of the coordinate transformations defined in the FITS WCS papers. ...

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• casacore: Coordinates_module_internal_classes
• casacore: Lattices_module_internal_classes
• casacore: casa::LinearXform Class Reference

The Equatorial Inertial (GEI) coordinate system: . The X GEI axis is directed to the point of the spring equinox, . The Z GEI axis is coincide with the Earth's rotation axis, . The Y GEI supplements the right three. The Geographic (GEO) coordinate system: . ... The Solar Magnetic (SM) coordinate system: . ... About space physics coordinate transformation see Russel [1971] and Hapgood [1992] . ... M.A. Hapgood , Space physics coordinate transformations: A user guide // Planet Space Sci. ...

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• The magnetic conjugation numerical file description
• The FSP plot description
• The numerical file description

. This diagram illustrates how a background image may be repeated within the content and padding areas of a box. In this example, a background image is first centered within a box (established by the BODY element of the example). The box contains paragraphs of text, shown in gray to make them discrete. The image, a blue wavy line on a pale yellow background, is then repeated vertically, to the top and bottom of the BODY box. The effect is to create a wavy band down the center of the page. Return to image.

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• Long description of example of cell background calculation
• Long description of example illustrating background calculation
• Long description for example of clipping region

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

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• lsst.coordConv: coordConv::OtherCoordSys Class Reference
• lsst.coordConv: coordConv::FK4CoordSys Class Reference
• lsst.coordConv: coordConv::AppTopoCoordSys Class Reference

The Hubble Deep Field South (HDFS) is a Director's Discretionary program on HST in Cycle 7 to image, similarly to the Hubble Deep Field (North), a typical field at high galactic latitude in four wavelength passbands as deeply as reasonably possible. ... In addition to the WFPC2 field, HDFS will include a STIS field containing a QSO at z=2.25 identified by Hewett and Boyle. ... 30 Orbits F814W . 30 Orbits F606W . 30 Orbits F450W . ... 1 primary orbits with STIS/50CCD to image the QSO field . ...

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• The Hubble Deep Field -- Project Description
• cgvc 121
• Chapter?3: Fixed and Generic Targets

Next: Order Definition Up: Echelle Reduction Method Previous: Retrieving demonstration and . ... That is the mapping between the space wavelength, spectral order and the space sample x , line y in the raw image. ... Sections and describe the solution of this mapping. The second step in the reduction, described in Section , is to estimate the image background. ... In the rest of this Section the algorithms used in each step of the reduction are described. ...

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• WorldCoords(3)
• CATS home page
• WorldOrImageCoords(3)

... GSAOI Home . Instrument . ... The Gemini South Adaptive Optics Imager (GSAOI) is a near-infrared adaptive optics camera that will be used with the Multi-Conjugate Adaptive Optics (MCAO) system on the Gemini South 8-m telescope . ... Gemini's major instrumentation goal is to develop its Multi-Conjugate Adaptive Optics (MCAO) system for scientific use on Gemini South. ... Existing adaptive optics systems use a single natural guide star or artifical laser guide star to measure this image blur. ...

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• Gemini NIFS Brief Description.
• The repainted Farnham dome with the AITC in the background
• The High-Z SN Search Description

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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• SAI Open Star Clusters (SAI OCL) Catalog

... The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image projections. ... They were CRPIX n for the reference pixel location on pixel axis n , CRVAL n for the coordinate value at that pixel, CDELT n for the increment at that pixel in the coordinate value, and CTYPE n for the type of coordinate. ...

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• Using XML and Java for Astronomical Instrument Control
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in
• The VizieR System for Accessing Astronomical Data

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

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• Description of program searchdup
• mod_remoteip - Apache HTTP Server
• HwB: ATA Internal Connector (Offline)

bToJ - convert coordinates from B1950 to J2000. outputFile The routine reads from standard input and writes to standard output. bToJ converts B1950 coordinates to J2000 format. ... The input file format is: Key hhmmss.s ddmmss.s One entry per line. ... Enter input from the the terminal, output goes to the terminal. bToJ xxxsrcname 202020 101010 .. user enters the b1950 coords xxxsrcname 202243.9408 101950.2285 .. program outputs the J2000 coordinates. ctrl-D to exit . ...

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• Description
• Project Description
• wst idl routines

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...

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• Description of the RadioAstron project, russion version

Next: DETAILED LIST OF ROSAT Up: PROS USERS GUIDE Previous: List of Related Documents . This section lists all PROS tasks (some of which are not described in this guide) and some useful IRAF tasks which are included. ... converts FITS to images and/or tables . ... delete a list of images . ... convert an Einstein FITS file into an IRAF/PROS QPOE file . ... convert a list of IRAF/PROS IMAGE files into RDF compatible format . ... convert a list of IRAF/PROS QPOE files into RDF compatible format . ...

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• Smithsonian Astrophysics Observatory Predoctoral Fellowships, 2004
• Converting the XPA API to 2.0
• Funtools and DS9 Image Display

Comedi Documentation . ... Next . comedi_perror -- print a Comedilib error message . ... When a Comedilib function fails, it usually returns -1 or NULL, depending on the return type. ... This error number can be converted to a human-readable form by the functions comedi_perror() and comedi_strerror(). ... In particular, Comedilib functions sometimes return an error that is generated inside the C library; the comedi error message in this case is the same as the C library. ... comedi_strerror ...

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• comedi_strerror
• comedi_errno
• SCORPIO-2 project: description

The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

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• Run_state
• HdrDownloader
• ESO - Description of End-to-End Operations

grdvector - Plot vector fields from grdfiles grdvector compx . ... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/psimage.html
• http://xray.sai.msu.ru/~ivan/gmt/man/gmtconvert.html
• http://xray.sai.msu.ru/~ivan/gmt/man/pshistogram.html

... Telescopes . ... Diameter of circular antenna . ... Number of antenna elements . ... Geometrical area . ... Effective area of full circle . ... Wavelength range . ... Frequency range . ... 2 arcsec . ... Flux density limit . ... Absolute brightness temperature limit . 0.050 mK . ...

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• Small telescopes short description
• Preparing and Submitting Tabular Data

... description: . ... product: . ... vendor: . ... version: . ... capabilities: . ... physical id: . ... Intel Corp. physical id: . ... clock: . ... bus info: . ... bus_master system:1 UNCLAIMED . ... bus_master display:0 UNCLAIMED . ... vga bus_master cap_list . ... uhci bus_master . ... ehci bus_master cap_list . ... pci normal_decode bus_master pcmcia . ... pcmcia bus_master cap_list . ... bus_master cap_list . ... bus_master cap_list mii autonegotiation 100bt-fd 100bt 10bt-fd 10bt ethernet physical...

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• Gadget Box PPS Level Converter and CHU Modem
• Zen: sncat design
• tickadj - set time-related kernel variables

Multichannel Flare Spectrograph . ... phi - the angle between the green vertical line passing through the solar disk image and the violet radius vector "r" of the object located at the center of the spectrograph slit- red cross. positive - clockwise, negative - counterclockwise . ... mx = x coordinate of the coelostat main mirror . ... x : carthesian solar coordinate alog axis parallel to solar equator (in arcsec) . y : carthesian solar coordinate alog axis parallel to solar axis (in arcsec) ...

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• HSFA 2 technical description Technical Details
• Anna Mel'nik - Description of the catalog
• Natural Satellites Service. Special Ephemerides