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) . ...

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• casacore: fits/FITS/FITSError.h Source File
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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 . ...

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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) . ...

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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. ...

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• The ROSAT All-Sky Survey Faint Source Catalogue
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... 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. ...

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• Algorithm

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'' . ...

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... 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 . ...

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• Untitled Document
• Sample Identification

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) . ...

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• core/StelTexture.hpp Source File

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 . ...

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• Lecture XVIII.
• Geothermal Energy

... 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 ). ...

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... Mathematics is relatively straightforward library to use again. ... double x; x = sqrt(63.9); . ... double acos( double x) -- Compute arc cosine of x. double asin( double x) -- Compute arc sine of x. double atan( double x) -- Compute arc tangent of x. double atan2( double y, double x) -- Compute arc tangent of y/x. double ceil( double x) -- Get smallest integral value that exceeds x. double cos( double x) -- Compute cosine of angle in radians ...

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• The C Preprocessor
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... The VSOP Survey Continuum Source List . The radio sample for the VSOP continuum survey was defined to include all extragalactic radio sources with: . a total flux density at 5 GHz, S>=1.0 Jy . ... The sample also included all sources in the sky with a 5 GHz flux density S>5 Jy, regardless of spectral index and galactic latitude. ... The source would then be included in the VSOP sample (three of the sources were found with a flux density above 1 Jy and added to the sample). ...

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• source comment

.

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• NAG's Fortran 90
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• XFree86/OS2 project

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• ADASS 2002 Conference Proceedings
• Space Science Education Resource Directory
• Cheating Poisson: A Biased Method for Detecting Faint Sources in All-Sky Survey

... Flux density at 1 GHz (/Jy): 35? ... Radio: Incomplete shell, including wide `v' of emission to east with small flat-spectrum source at apex. ... X-ray: Pulsar detected, with faint extension. ... Molonglo at 408 MHz (3': S=38 Jy). ADS . ... Optical detection. ... Becker & Helfand 1985, Nature, 313, 115. ... 1985, MNRAS, 212, 975. Pulsar detection. ... 1991, MNRAS, 253, 7P. Pulsar and remnant association. ... Pulsar observations, including proper motion. ... 2001, ApJ, 562, L163. ...

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• Bojan Nikolic -- Compiling CASA revisited
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... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

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Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences PUL Analysis Center Pulkovo IVS Analysis Center (PUL) 2009 Annual Rep ort Zinovy Malkin, Natalia Miller, Elena Popova Abstract This report briefly presents the PUL IVS Analysis Center activities during 2009 and plans for the coming year. The main topics of the investigations of PUL staff in that period were ICRF related studies, computation and analysis of EOP series, and VLBI2010 related issues. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm13r.pdf

... Now, all three programs come in one easy to build package. ... Unfortunately, because it is the only brand of F90 compiler I have access to, the source codes can only be guaranteed to build with Intel Fortran Compiler v6.0 , and now with the newer v7.1 . ... Binary RPM - RedHat 8.0 Binary RPM Package (~2.8 MB) [ How to install ] . Source RPM - Source RPM package (~1.7MB) [ How to install ] . ... Source RPM - Source RPM package (~2.5MB) [ How to install ] . ... Chris Winter, 2007 . ...

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home education > resources . ... Resources . ... Astronomical Pseudo-Science . ... Black Holes: An Introductory Resource List . ... http://www.astrosociety.org/2012 . ... Fraknoi, A. "Dealing with Astrology, UFOs, and Faces on Other Worlds: Guide to Astronomical Pseudo-science in Classroom," Astronomy Edu cation Review, (2004): http://dx.doi.org/10.3847/AER2003022 . ... The Skeptic's Dictionary: An excellent source of brief reviews, references, and links on dozens of areas of pseudo-science. ...

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• ASP: The Astronomy of Many Cultures: A Resource Guide

XmCCD ----- The programs provided here offer a Linux graphical user interface to astronomical and scientific CCD cameras. ... It is the latest one they offer and the files included allow support for Android and Mac OS X. This distribution of XmCCD includes source code to utilize the SBIG shared library libsbigudrv.so with a Motif-based graphical user interface. ... The XmCCD source package includes and will install: SAOimage ds9 xpa cfitsio SAOimage is the primary image display for XmCCD. ...

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• http://www.astro.louisville.edu/software/sbig/xmccd-5.1/README
• Moore Observatory Astronomical Software Resources