On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

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. ...

Tsys using sky and absorber . Sensitivity using crosses from dipole 1. ... data taken with the dual pol array in position A0, focus=0. polA dipole 1 and polB dipole 2 were recorded. ... The phased array feed will have different values. processing: x101/100831/absorber.pro . ... Fit for: The Tsys offset, Gaussian amplitude, x,y offsets, major, minor axis widths, and ellipse rotation angle. 122 crosses were done in total. ... Top has the beam widths for each cross. * is the major axis beam width . ...

... Files . ... 00001 //# AxesMapping.h: Info about mapping array axes to another order 00002 //# Copyright (C) 2000,2001 00003 //# Associated Universities, Inc. ... 00095 // Another value gives the new axis number. 00096 // <br>It determines if axes are removed and/or reordered. 00097 explicit AxesMapping ( const IPosition & oldToNew); 00098 00099 // Copy constructor (copy semantics). ... 00133 IPosition posToNew ( const IPosition & pos) const ; 00134 00135 // Map a new position or shape to the old one...

Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . FileљList . FileљMembers . ... include . tcc . axeLim.h . ... 2 љ #include <boost/tr1/array.hpp> // so array works with old and new compilers . 3 љ #include " tcc/basics.h " . ... 19 љ std::tr1::array<double, 3> minPos ; . 20 љ std::tr1::array<double, 3> maxPos ; . 21 љ std::tr1::array<double, 3> vel ; . 22 љ std::tr1::array<double, 3> accel ; . 23 љ std::tr1::array<double, 3> jerk ; . ... std::tr1::array< double, 3 > . ...

... The sky position of a single source may be entered via the parameters ra , dec and (optionally) errorradius . ... In this mode, the output positions are printed to a single line of standard output. ... Source dec = <dec> deg. # # rawX rawY ccd On chip? +xxx.xx +xxx.xx xx x 123456789 123456789 12345678 . ... Source dec = <dec> deg. # # detX detY +xxxxx.x +xxxxx.x 123456789 12345678 . ... Source dec = <dec> deg. # # detX detY det err +xxxxx.x +xxxxx.x xxxxx.x 123456789 123456789 123456789 . ...

... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Glossary and Acronym List . ... ASCS : Aft Shroud Cooling System. ... CDBS : Calibration Data Base System; system for maintaining reference files and tables used to calibrate HST observation datasets. ... ICD : Interface Control Document; defines data structures used between software or systems to ensure compatibility. ... NICMOS : Near-Infrared Camera and Multi-Object Spectrometer. NIR : Near Infrared. ...

First results of X/S and X/Ka-band catalog combinations with full covariance information Andreas Iddink , Christopher Jacobs, Thomas Artz, Axel Nothnagel 22.09.2014 First results of S/X and X/Ka-band catalog combinations with full covariance information Andreas Iddink ­ 22.09.2014 Motivation Features of the ICRF2 ICRF2 (Defining- Sources ) 3414 ... Step: Import of the X/Ka catalog with full covariance information (Data provided by Christopher Jacobs et al. ...

home education > resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... Astronomy Education Bibliography . ... Astronomical Pseudo-Science . Moon Resource Guide . ... Astronomy of Many Cultures Resource Guide . ... Activity from NOVA to figure out your birthday in the Maya calendar (if you were born 1980 or after): http://www.pbs.org/wgbh/nova/teachers/activities/pdf/2804_maya.pdf . ... The Maya Astronomy Page (Dawn Jenkins): http://www.michielb.nl/maya/astronom.html . ...

... The derived position here agrees with the position from recent ATCA observations, RA=15h 01m 34.74s, Dec=39 18 39.2" (Tasker, private communication) which found the source unresolved. Because of the relatively large position offset, the reality of the fainter component 0.12" to the west is somewhat in doubt. However, the ATCA centroid position is offset by 0.3" to the south-east of the VLBA position, suggesting that the faint component may be part of more extended structure. ...

Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...

The Astronomy Net . Articles | AstroGuide | ... Forums . ... H ere you can find resouces to help understand perhaps the grandest of all sciences. ... Upcoming Sky Events . ... This site includes lists of manufacturers, vendors, software, etc. organized in the AstroGuide to help when you are looking to purchase your tools. ... Astronomy Articles . ... Are you interested in writing an article for the Astronomy Net? ... www.astronomy.net . ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... The generation of simulated sources whose physical properties are well understood is useful in assessing the functionality of point source analysis software. Qpsim is an IRAF/PROS task which will generate events from sources of given intensity, shape, and position and either overlay them on a flat background in a new QPOE file or inject them into an existing QPOE file. ... The simulated data can be a useful tool in calibrating point source analysis software. ...

Stellarium 0.12.3 . ... Renderer . FileљStructure . ... core . ... 29 љ Vec2f position; . ... 32 љ VertexP2 ( const Vec2f position) : position(position) {} . ... 43 љ Vec2f texCoord; . ... 46 љ VertexP3T2 ( const Vec3f & position, const Vec2f texCoord) . ... 50 љ VertexP3T2 ( const Vec2f pos, const Vec2f texCoord) . ... 64 љ VertexP3T2C4 ( const Vec3f & position, const Vec2f texCoord, const Vec4f & color) . ... 68 љ VertexP3T2C4 ( const Vec2f pos, const Vec2f texCoord, const Vec4f & color) . ...

... 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). ...

... ALMA . ... ARC Staff at ESO . ... The European ALMA Regional Centre (ARC) provides the interface between the ALMA project and the European science community. ... Below you can read the latest Announcements from the European ARC Network.. ... The call for 1-mm Very Long Baseline Interferometry (VLBI) proposals to use phased ALMA at Band 6 in Cycle 4, in collaboration with the Event Horizon Telescope Consortium (EHTC), will be released to coincide with the ALMA Cycle 4 Call for Proposals in March 2016...

... source code A class to hold all the information from a NIFS-produced data cube. ... Returns the data content of scidata as a numpy array. source code . ... Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. source code . ... source code Returns the data content of scidata as a numpy array. ... The fitscube instance is updated in-situ. source code Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. ...

This is possible if you do it in the following way, that is if you use the new continuation sign "&" at the end of the old line, but in position 73 so that it doesn't conflict with Fortran 77, and also choose the "&" sign as the almost arbitrary character in column 6, in order to get continuation according to Fortran 77. ... Comments are an incompatibility problem between Fortran 77 and Fortran 90, but of course not between fixed and free forms of Fortran 90 since the "!" is permitted in both. ...

... Helpful Computer Hints for Survival in this Class . ... Solar Radiation Data Base . Electronic Energy Journal . ... Answers to the First Midterm The Second Homework Assignment . ... WEEK #1 BASIC OVERVIEW OF THE PROBLEM . ... WEEK #2 SOLAR ENERGY BASICS . Solar Energy: Incident Energy on the Earth's Surface . ... WEEK #3 SOLAR ENERGY: ENERGY STORAGE and PHOTOVOLATIC CELLS . ... WEEK #4 SOLAR ENERGY: OTHER USES . ... WEEK #5 ENERGY STORAGE SYSTEMS . ... WEEK #9 PLANTS, POLLUTION AND PHYSICS . ...