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1. WCSLIB: wcslib.h Source File
WCSLIB љ 5.15 . ... Files . ... wcslib.h . ... 3 љ WCSLIB 5.15 - an implementation of the FITS WCS standard. ... Use it to include all . ... 3282 љfunction name, source file, line number, and an error message which may be . ... 3296 љEach of the @ref structs "structs" in @ref overview "WCSLIB" includes a . ... int wcsfree(struct wcsprm *wcs) . ... int wcsset(struct wcsprm *wcs) . ... int wcsperr(const struct wcsprm *wcs, const char *prefix) . ... int wcsini(int alloc, int naxis, struct wcsprm *wcs) . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/mcalabre/WCS/wcslib/wcslib_8h_source.html -- 25.1 Кб -- 10.04.2016
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2. http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/user/v2_0/NETZWERK.LST
netzwerk.h 9 #include prog.h 10 #include time.h 11 void netopen(void) 12 { 13 #include extern .c 14 long tmo; 15 int al; 16 tmo = 20; /* 20ms time out */ 17 ad.fhost = 0x8ee1e489;/* Host address: 137.228.225.142 */ 18 ad.lsocket = 9010; /* Local socket # */ 19 ad.fsocket = 1000; /* Foreign socket # */ 20 ad.protocol = STREAM; 21 if (neustart != 0) goto c2; 22 alarm = net_getdesc(); 23 if ( alarm 0) 24 { 25 neustart = 0; 26 ... extern far function *** *** net_connect . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/user/v2_0/NETZWERK.LST -- 9.8 Кб -- 06.03.2001
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3. lsst.coordConv: include/coordConv/mathUtils.cc Source File
lsst.coordConv љ unknown . ... Files . ... include . ... mathUtils.cc . ... 12 љ inline void rot2D ( double &rotX, double &rotY, double x, double y, double ang) { . 13 љ double sinAng = sind (ang); . 14 љ double cosAng = cosd (ang); . ... 21 љ // put angle into range (-360, 360), then finish the job . 22 љ double wrappedAng = std::fmod(ang, 360); . ... 53 љ double wrappedAng = refAng + wrapCtr (ang - refAng); . ... void rot2D(double &rotX, double &rotY, double x, double y, double ang) . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/coordConv/html/include_2coord_conv_2math_utils_8cc_source.html -- 19.5 Кб -- 07.05.2015
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4. Source Positions
Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/EGRET2/node7.html -- 9.0 Кб -- 08.05.1998
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5. Astrometric alignment of the input source coordinates
... Get a list of the number of unique ``windows'' in the input source-list files (a window has a unique set of WINDOWX0, WINDOWDX, WINDOWY0, WINDOWDY and BINBPE parameters. ... Find the source-list that has the most sources in that window. For each other source-list in the window, compute the RA/DEC offsets that are needed to be added to their RAs/Decs to align with the reference source-list coordinates. ... Subtract the mean offsets from the RA/Dec coordinates of the reference source-list. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omsrclistcomb/node7.html -- 6.1 Кб -- 02.07.2008
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6. *imcnts* - Radial Profile of an extended source at the field center
Next: *tabplot* - Displaying a Up: Radial Profiles and Projections Previous: Radial Profiles and Projections . Obtain a radial distribution of counts for the source centered at x = 503, y = 513, in the data image xdata$snr.qp . The background is taken locally from an annulus outside the source region. ... Region descriptors can also be given on the command line, but they must be enclosed by quotes. xs> imcnts xdata$snr ``a 503 513 0 50 n=5'' . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node103.html -- 7.0 Кб -- 01.10.2012
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7. The Cross-correlations
... The actual cross-correlations were done as follows: north of WGACAT was correlated with the GB6 catalog with a correlation radius of one arc minute. ... We therefore cross-correlated WGACAT with the GB6 and PMN radio catalogs with a 1.5 arcmin radius. ... As a result of this experiment, we then added to the WGACAT/PMN candidate list the 29 unclassified sources obtained from the 1.5 arcmin correlation and having PSPC offsets arcmin, ratio between X-ray/radio offset and positional error , and . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node5.html -- 11.3 Кб -- 03.12.2003
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8. Stellarium: core/renderer/StelGLUtilityFunctions.hpp Source File
Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... StelGLUtilityFunctions.hpp . ... 42 љ inline GLint glAttributeType( const AttributeType type) . ... 46 љ case AttributeType_Vec2f: . ... 49 љ return GL_FLOAT; . ... 68 љ inline const char * glslAttributeName( const AttributeInterpretation interpretation) . ... 72 љ case AttributeInterpretation_Position: return "vertex" ; . ... 267 љ inline bool glTextureSizeWithinLimits( const QSize size, const TextureDataFormat format) . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/StelGLUtilityFunctions_8hpp_source.html -- 40.3 Кб -- 28.02.2014
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9. Energy and the Environment: Resources for a Networked World
Links and Resources for Energy and the Environment . The world is finally becoming globally aware that exponential resource usage in combination with finite reserves is a recipe that ensures our great grandchildren won't be born. ... National Environmental Information Service . ... Electronic Energy Journal . ... Sustainable Development Dimensions , including sections on Environmental information , Environmental policy, planning and management and Energy for development . ... Acid Rain Resource . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/energy.html -- 6.5 Кб -- 05.04.2000
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10. WFC3 Data Handbook
... WFC3 Data Handbook > Chapter 5: WFC3-UVIS Sources of Error > 5.5 Image Anomalies . ... Ghosts appear as images of the pupil formed from the light of a bright target in, or near the UVIS detector FOV. ... Further details concerning these ghosts may be found in WFC3 ISR 2007-09. ... Specifically, in full-frame, unbinned UVIS readouts, the CT level is ~2x10 -4 of the source when the target is in quadrants A or C and about 8x10 -5 when the target is in quadrants B or D ( WFC3 ISR 2009-03 ). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/HST_overview/documents/datahandbook/hst/wfc3/documents/handbooks/currentDHB/Chapter5_uvis_error6.html -- 121.6 Кб -- 12.04.2016
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