... The spectroscopic model of the source gives , the number of photons received per cm and per second at the earth, from sky position and at energy (differential per solid angle and energy). The number of photons, , detected (per second) in pixel and in PI energy bin centered at is obtained by multiplying by the effective area and applying the response matrix: . ... The correspondence between sky position and detector coordinates depends on the telescope's pointing. ...

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. ...

. This diagram illustrates how the definition of a pixel depends on the users distance from the viewing surface (paper or screen). The image depicts the user looking at two planes, one 28 inches (71 cm) from the user, the second 140 inches (3.5 m) from the user. An expanding cone is projected from the user's eye onto each plane. Where the cone strikes the first plane, the projected pixel is .28 mm high. Where the cone strikes the second plane, the projected pixel is 1.4mm high. Return to image.

lsst.coordConv љ unknown . ... Classes . ... coordConv::OtherCoordSys Class Reference . ... OtherCoordSys (std::string const &name, double date=0, DateTypeEnum dateType= DateType_None , bool isMean =false) . ... virtual Coord љ . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom ( CoordSys const &fromCoordSys, Coord const &fromCoord, Site const &site, double tai=0) const . ... virtual Coord coordConv::OtherCoordSys::removePM . ...

... Classes . ... casa::FuncExprData . ... Destructor. map< String , ExprOperator > & . ... const map< String , ExprOperator >& casa::FuncExprData::binary1 . ... const map< String , ExprOperator >& casa::FuncExprData::binary2 . ... const map< String , ExprOperator >& casa::FuncExprData::function . ... const map< String , ExprOperator >& casa::FuncExprData::special . ... const map< String , ExprOperator >& casa::FuncExprData::unary1 . ... const map< String , ExprOperator >& casa::FuncExprData::unary2 . ...

... Each HST Science Instrument requires its own local coordinate system and apertures to support both target acquisition and small angle motions (SAMs). ... Any location within the field of view of a NICMOS camera can be specified by the POSTARG special requirement (described in the HST Phase II Proposal Instructions). ... Each NICMOS camera has two primary apertures. One is positioned at the geometric center of the detector and the other at an optimal position close to the center. ... 128,128 . ...

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. ...

Lutsenko Olena L. (PhD, Psychology, Associate Professor) Filonenko Anna (Master, Psychology, Lecturer) School of Psychology V. N.Karazin Kharkiv National University COURSE DESCRIPTIONS ­ PSYCHOLOGY OF LEADERSHIP Title and N of module 1­ Leadership Theories Themes 1. ... Ethical leadership. ... Organizational Behavior and Human Decision Processes, 95 , 140-155. ... Socializing the newcomer: The mediating role of leader-member exchange.Organizational Behavior and Human Decision Processes, 119, 114-125. ...

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

... 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 . ...

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. ...