... The parameters of powspec are computed from the parameters of efftplot , such that for each energy band, only one time-averaged PDS is computed. Then for each energy band, efftplot reads the PDS into the FITS file produced by powspec , and plots it with the PGPLOT library. ... The PDS is calculated in data segments of Nbins bins. ... 1 : PDS is normalized such that the (white) noise level expected corresponds to a power value of 2. ... 2 : as =2, but the expected white noise level is subtracted. ...

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. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

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This diagram gives one visual rendering of a table that has been marked up especially for aural rendering. The table has a centered caption above it that reads "Travel Expense Report". ... In order to group information in a useful way, the table has a central column group with three columns, labeled "Meals", "Hotels", and "Transport" from left to right. The table's first column (to the left of the central column group) lists days of travel and labels these days with the city visited. ...

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• Long description of example illustrating precedence in the collapsing borders
• Long description of example of cell background calculation
• Long description for italic forms

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

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• Database of Optical Constants -- Level: welcome

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... AT Deep Fields Home б б б |б б б  ATHDFS Home б б б |б б б  Project Details б б б |б б б  Data б б б |б б б  Catalogues б б б |б б б  Publications б б б |б б б  ATHDFS Team Pages (password required) б б  . ... Column (1) --- Source ID number Column (2) --- Source name. ...

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• casacore: Mathematics_module
• casacore: casa::ScalarRecordColumnDesc Class Reference
• casacore: casa::SubTableDesc Class Reference

... Short description of Intel families (.ps) ( .pdf ) . ... Cpu Type . ... 512 . ... 0.000 . ... Intel Xeon 2.40GHz . ... Intel Xeon 2.66GHz . ... Intel Xeon 3.06GHz . ... 2.6.18-274.18.1.el5.centos.plus . AMD Opteron 246 . ... Intel Xeon 5130 @ 2.00GHz . ... 6144 . ... 3.10.0-327.10.1.el7.centos.plus.x86_64 . Intel Xeon L5430 @ 2.66GHz . ... Cpu type: The type of cpu(s) used in the computer. xeon X55xx is the nehalem intel processor. processing: phil/admin/cpuinfo.pl home_~phil ...

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• satellite prediction routines
• fccCodesForPR
• rotaPlatToSky

grdgradient - Compute directional derivative or gradient from 2-D grd file representing z(x,y) grdgradient in _ grdfile -G out _ grdfile [ -A azim [/ azim2 ] ] [ -D [ c ][ o ][ n ] ] [ -L flag ] [ -M ] [ -N [ e ][ t ][ amp ][/ sigma [/ offset ]] ] [ -S slopefile ] [ -V ] grdgradient may be used to compute the directional derivative in a given direction ( -A ), or the direction ( -S ) [and the magnitude ( -D )] of the vector gradient of the data. ... If amp is not given, default amp = 1. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/spectrum1d.html
• http://xray.sai.msu.ru/~ivan/gmt/man/psscale.html
• http://xray.sai.msu.ru/~ivan/gmt/man/grdmask.html

... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...

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• Reference Clock Options
• APOD: December 23, 1996 - The Hills of Ganymede
• xntpd - Network Time Protocol (NTP) daemon

... This section describes three functions which have been created to cleanup defects in images. The first two functions for cleaning rows and columns are particularly useful for CCD--images. ... These can often be removed with the commands: MODIFY/COLUMN INPUT OUTPUT [C or V] [columns] . ... This is particularly useful for removing the permanent defects which may exist in the CCD--frames and which cannot be removed by the MODIFY/COLUMN or MODIFY/ROW commands. ...

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• All Sky Catalog at 2.7 GHz
• Order Definition
• WSRT deep surveys

... In our numerical experiments we have mainly considered two test objects provided by R. Hanisch and characterized by different types of brightness distribution; one of the objects simulates an elliptical galaxy and the other one a star cluster with size 512 512 and 256 256 pixels, respectively. ... The best performances in the restoration of the star cluster image are provided by the R-L algorithm and the LWPOS one; they give accuracies of 6%and 5%, respectively (see Table 1). ...

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• Target Identification
• CSPICE Routines: RAXISA_C
• Description of the Reconstruction Methods

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

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• lsst.coordConv: coordConv::PVT Class Reference
• lsst.coordConv: coordConv::PVTCoord Class Reference
• lsst.coordConv: coordConv::Coord Class Reference

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...