... The Spectrum Extraction window is activated by clicking on the button in the Main window and contains options for fitting the sky and extracting spectra. ... The window provides two buttons and for an interactive definition of the limits of the sky and the object. Clicking one of the these buttons activates a cursor in the display window. ... The name of the resulting sky file is defined in the text field Sky (image or constant): which includes the default value sky . ...

... Packet Format . ... The TCC broadcasts UDP packets containing position information. ... Packet Header . ... int4 . ... double . ... pos, vel double . ... pos, vel, time double . ... See the TCC Message Keywords Dictionary for full definitions of most items in the "data" section of the packet. pos, vel double is a structure containing two doubles: "pos" and "vel"; it contains the same information as the TCC's "coordinates" (p,v,t triplets), but with time given by the "TAIDate" entry in the packet. ...

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. ...

... Files . ... File List . File Members . casa . ... Defines . ... this file contains all the compiler specific defines . ... Define the canonical sizes of the built-in data types. #define . ... Define for each data format if a conversion is needed from the local format to the canonical format (or vice-versa). #define . ... Define for each data format if a conversion is needed from the local format to the canonical format (or vice-versa). ... Definition at line 66 of file CanonicalConversion.h . ...

... Analysis of in-orbit data closely follow the CSL data analysis. Stars with known astrometric positions are matched with their image centroids. ... The measured position, the expected position and the offset between the measured and expected positions are calculated and written into a file. ... select catalogued positions for different observations/pointings (e.g. positions of objects in photometric sequence) . ... The new distortion map was generated from in-flight observations of the G153 field. ...

... To run the <LAYER> version of the example, select: flower.htm . ... However, if the page had several layers with absolute positions, and you wanted to place another layer in a relative position to one of the existing layers, you could use inline JavaScript to calculate the value for LEFT or TOP . ... In this example, there is really no need to use inline JavaScript to position the last flower layer, since you could just let the TOP value default to its natural value, as in the other flower layers. ...

Optical Filters . The WFPC2 camera configuration and filter set require a substantial number of apertures for full utilization of its capabilities. ... An additional set of aperture names have been defined for use with the WFPC2 filters which require partial rotations. ... The pixel coordinates of these apertures will be reviewed on a regular basis to reflect changes in CCD and filter cosmetics. ... The aperture name is generally the same as the (rotated) filter name. ...

... NEWS . WHEN : typically 3 weeks before the official deadline , i.e. date by which the new DFS release has to be operational on the mountain. ... complete list of performed tests. ... description of the new bugs raised during this Integration phase. ... HOW: Integration Acceptance meeting at DFS level with: . ... If needed, specific Integration acceptance meetings at DFS project level and SCCB meetings may be organized to prepare this Integration acceptance meeting. Before this meeting, . ...

... to_tsquery( [ configuration , ] querytext text) RETURNS TSQUERY . ... Query rewriting is a set of functions and operators for tsquery type. ... We'll expand query supernovae using table-driven rewriting rules. =# create table aliases (t tsquery primary key, s tsquery); =# insert into aliases values(to_tsquery('supernovae'), to_tsquery('supernovae|sn')); =# select rewrite(to_tsquery('supernovae'), 'select * from aliases') && to_tsquery('crab'); ?column? --------------------------------- ( 'supernova'...

... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...

Stellarium 0.12.3 . ... FileљStructure . FileљList . ... core . ... StelSphereGeometry.hpp File Reference . ... operator<< (QDataStream &out, const SphericalRegionP &region) . ... boolљ . sideHalfSpaceContains (const Vec3d &v1, const Vec3d &v2, const Vec3d &p) . ... greatCircleIntersection (const Vec3d &p1, const Vec3d &p2, const Vec3d &p3, const Vec3d &p4, bool &ok) . ... greatCircleIntersection (const Vec3d &p1, const Vec3d &p2, const Vec3d &nHalfSpace, bool &ok) . ... const Vec3d &љ . ...

... Acronyms and Abbreviations AMOS Advanced Mechanical and Optical Systems (UTM vendor) EIE FTT FLC ICD ISS European Industrial Engineering (UTE vendor) Fast Tip-Tilt First Light Camera Interface Control Document Interferometer Supervisory System NAS NMT NOT TBC TBD UT UTE UTM Narrow-field Acquisition System New Mexico Tech Nasmyth Optical ... Interface design description 2.5 FTT/NAS to ISS ICD This ICD describes the software interfaces of the FTT/NA system to the ISS. ...

... JavaScript 1.2: added name , text , x , and y properties Using the HTML A tag or calling the String.anchor method. The JavaScript runtime engine creates an Anchor object corresponding to each A tag in your document that supplies the NAME attribute. It puts these objects in an array in the document.anchors property. ... A string specifying the anchor's name. text . ... The horizontal position of the anchor's left edge, in pixels, relative to the left edge of the document. y . ... Anchor . ...

SCCSWHAT( @(#)c1.err 2.29 88/02/25 18:18:00 ) */ /* fatals */ 1001 Internal Compiler Error\n\t\t( compiler file '%s', line %d)\n\t\tContact Microsoft Technical Support 1002 out of heap space 1003 error count exceeds ... off]" 4086 "expected [1 | ...

... Documentation for the Python objects defined by the project is divided into separate pages for each package, module, and class. The API documentation also includes two pages containing information about the project as a whole: a trees page, and an index page. ... A description of the package. ... A summary of the classes defined by the package. ... The module contents frame contains a list of every submodule, class, type, exception, function, and variable defined by a module or package. ...

Perhaps the greatest theoretical achievement of physics in the 19th century was the discovery of electromagnetic waves. ... It is possible to use this to define a unit of electric charge, as the charge which repels a similar charge at a distance of, say, 1 meter, with a force of unit strength (actual formulas make this precise). ... But "field" originally only meant the force a magnet or an electric charge could expect at a point in space, if it were placed there. ...

The first field of each line starts at 0 (zero); the second is 1 (one) and so on. To define which field to sort on you give the position of the field at which to start the sort followed by the position at which to end the sort. The position at which to start the sort is given as the number of fields to skip to get to this position. ... tells sort to skip the first two fields. The position at which to stop the sort is given as the number of the field at the end of which the sort stops. ...

... Equinox of object coordinates BJ = 18.87 / bJ magnitude UMBJ = -0.69 / u - bJ colour BJMR = 0.22 / bJ - r colour NOBS = 1 / Number of 2dF observations available IS_ BEST = 'TRUE ' / TRUE if this file contains the best 2dF observa DATEBEST= '24/09/00' / Date of best 2dF observation (DD/MM/YY) ID_ BEST = 'QSO ' / ID from best 2dF observation QUALBEST= 11 / Data quality flag from best 2dF observation Z_ ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . ... Installation of the ground receiving station on the premises of M.V. Keldysh Institute of Applied Mathematics, the Russian Academy of Sciences, software upgrading to receive the information signal from board the ISS RS. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... sin f = y / r . cos f = x / r . ... They are now viewed as new definitions of the sine and cosine, for the polar angle f given by x and y ( a slightly different way of formulating this definition is described further below ). ... sin 2 f + cos 2 f = 1 . ... Angle . ... Many trigonometry texts define the sine and cosine slightly differently, using the so-called unit circle . ... Then the distance AB ("the sine line") equals sin a , and the distance OA ("the cosine line") equals cos a . ...