Calibration data from jun12 through dec12 was used to look at the system performance and pointing errors of various receivers. 06jun12 - model 18 installed. ... Prior to this, little power was getting into polB. 430 dome data used was after 19oct12. 28oct12: new sbn receiver installed . ... they had an exceptionally large pointing error for this receiver (say > 60 asecs) . ... The offsets for the other receivers are then computed relative to sbn using 2 or 4 sources.This was done back in apr-may12. ...

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• system Performance
• pntModelGradients
• Calibration Scans on Continuum Sources

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

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• Radio sources identfification

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... src . telMod.cc . ... 2 љ * Pointing model block . ... 11 љ const float RadPerArcsec = coordConv::RadPerDeg / coordConv::ArcsecPerDeg; . ... 27 љ void TelMod::loadPath (std::string const &filePath) { . ... 29 љ int retVal = tcsIntpm(filePath.c_str(), & _model ); . ... 47 љ std::string const &termName, . ... 75 љ std::vector<std::string> TelMod::getTermNames () const { . ... 125 љ std::ostream & operator<< (std::ostream &os, TelMod const &telMod) { . ...

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• sgs summary
• TUI:Scripts:Built In Scripts:NICFPS:Dither:Point Source
• Astrophysical Research Consortium - Apache Point Observatory

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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• Preparing your Data
• Making a Fake Observation
• USNO/ATNF_VLBI

Next: *imcnts* - Radial Profile Up: Radial Profiles and Projections Previous: *tabplot* - Displaying a . ... Input a spatially blocked and energy filtered image from above and use with the background determined from the broad-band background map. cl xray xr xspatial xs imcnts addbkg=no # Do not add the background error Source image file : xdata$snr.qp Source region descripter: c 503 513 50 p 503 513 0 360 n=10 # circular region centered on point ...

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• The AstroStat Slog Blog Archive Spurious Sources
• ECT: Evidence Evaluation Point!
• Spectral Extraction of Point Sources

Russian Academy of Sciences Pulkovo Observatory On systematic and stochastic errors of radio source position catalogues Zinovy Malkin Pulkovo Observatory and St. Petersburg State University malkin@gao.spb.ru JournИes 2013, Paris, France, September 2013 Topics to discuss The following topics related to the radio source position catalogues are considered: 1. ... A new approach to assess the external stochastic errors of radio source position catalogues has been presented. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/kurdubov.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm12c.pdf
• The Canadian S2 Correlator - Principles of Radio Interferometry

The Texas survey of radio sources covering -35.5{deg} < {delta} < 71.5{deg} at 365MHz . ... We present the Texas Survey of discrete radio sources between -35.5deg and 71.5deg declination (B1950), which was carried out at 365MHz with the Texas Interferometer during 1974-1983. ... The Texas Survey . ... The sources in the simpler model. ... Right Ascension 1950 . ... field separator . ... Some sources came from Version 6 of the Texas Survey ('TS6' in strp field) or Version 7 ('TS7' in strp field) . ...

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• Description of the RadioAstron project, english version

... 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
• Kalman Filtering in Chandra Aspect Determination
• ADASS 2003 Conference Proceedings

... Bojan Nikolic web pages (r. 329) . ... SCons user manual http://www.scons.org/doc/1.2.0/HTML/scons-user/book1.html . SCons man page (on web at http://www.scons.org/doc/HTML/scons-man.html , or man scons ) . ... SCons is a tool to build compile source code into (closer-to) executable format. ... Curiously, the shared-library SCons builder will accept multiple identical sources and pass them all to the linker, which will normally lead to ?multiple definition? errors. ... Introduction to SCons . ...

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• Monitoring of variable sources at 15 GHz
• exchange.h File Reference
• G332.4-0.4

Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... StelTextureBackend.hpp . ... 26 љ #include <QString> . ... 56 љ inline QString textureStatusName( const TextureStatus status) . ... 118 љ const QString& getName () const . ... 132 љ invariant(); . ... 143 љ const QString& getErrorMessage () const . ... 151 љ const QString path ; . ... 157 љ StelTextureBackend ( const QString& path ) . ... 200 љ void errorOccured ( const QString& error) . ... 232 љ void invariant() const . ...

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• Stellarium: core/renderer/StelGLUtilityFunctions.hpp Source File
• Stellarium: core/renderer/StelTextureLoader.hpp Source File
• core/StelTexture.hpp Source File

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 . ... Please be patient, and point out any discrepancies or errors on the developer/ pages directly to the dev@httpd.apache.org mailing list. ... Apache 1.3 API Notes . Apache 2.0 Hook Functions . Request Processing in Apache 2.0 . ... Converting Modules from Apache 1.3 to Apache 2.0 . ... Apache 2.x Thread Safety Issues . ... Licensed under the Apache License, Version 2.0 . ...

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• Developer Documentation for the Apache HTTP Server 2.4 - Apache HTTP Server
• mod_dumpio - Apache HTTP Server
• mod_cgi - Apache HTTP Server

... 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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• IRAF/STECF 2-D spectrum point source / background decomposition package
• Sample Identification
• Previously Identified Sources

Peremennye Zvezdy", . ... Star Name: . 1RXS J190331.9+104353, EQ J190331.9+104353.1 . ... This variable star was discovered by Barsukova (2004) in the vicinity of the hard X-ray source and microquasar candidate 1RXS J190333.1+104355 (Paredes et al., ... Our variable star is located outside the error circles of these sources but very close to the western border of the ROSAT X-ray error circle. ... The light curve shape is typical of Mira Ceti type stars. ... Light Curve . ... Data Source . ...

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• Астронет > Англо-Русский Словарь
• Астронет > The X-ray Sources of M31
• The X-ray Sources of M31

This module provides for execution of CGI scripts. ... Module Identifier: cgi_module Any file that has the mime type application/x-httpd-cgi or handler cgi-script (Apache 1.1 or later) will be treated as a CGI script, and run by the server, with its output being returned to the client. ... Debugging CGI scripts has traditionally been difficult, mainly because it has not been possible to study the output (standard output and error) for scripts which are failing to run properly. ... Status: mod_cgi . ...

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• Server-Wide Configuration
• Apache module mod_imap
• Apache suEXEC Support

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The K2 optical (top panel) and MAXI X-ray (lower panel) light curves of Sco X-1. ... The error on the optical photometry is negligible and the error on the X-ray points are typically 1 percent. ... We also find evidence that this behaviour has a typical systemic timescale of 4.8 days, which we interpret as a possible disc precession period in the system. Finally, we confirm the complex optical vs. ...

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• IAJ: Resources: Observatories
• WD Merger Movie: POV-Ray stars
• Mysterious music source revealed | International Year of Astronomy in Ireland |

home education > resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... Resources . ... Astronomy Education Bibliography . ... Astronomical Pseudo-Science . ... Black Holes: An Introductory Resource List . ... Astronomy . ... Space Science Education Resource Directory . ... http://www.aas.org/education/ancientuniverse.html . National Center for Science Education: Best web site for keeping up with issues in this area, with many articles, resources, and links. http://www.ncseweb.org . ...

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• ASP: Black Holes: An Introductory Resource List
• ASP: Educational Resources
• ASP: Resource Center

... Page not found . ... Задачей КА Mars Express, является выполнение научных исследований, которые не состоялись из-за аварии российского КА Марс 96. ... Mars Express будет запущен в начале июня 2003 года с Байконура ракетой-носителем "Союз-Фрегат". Выход на орбиту Марса планируется на 26 декабря 2003 года. ... КА Mars Express также будет выступать в качестве ретранслятора для посадочных ступеней других международных миссий по исследованию Марса. ...

18. Astronomy articles, forums, listings, and other resources about Astronomy.

19. Practical Astrophysics

20. Data sources