... Classes . ... casa::FunctionTraits< T > . ... Function data types for parameters and arguments. ... Actual template type. typedef T . ... Type for arguments. typedef AutoDiff < T > . ... FunctionTraits defines relationships between the data types of result, parameters and arguments of function objects. This templated class contains a number of typedefs that describe the relationship between different numeric data types used for the calculation of Function and the function parameter and arguments. ...

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• casacore: casa::FunctionWrapper< T > Class Template Reference
• casacore: casa::CompoundFunction< T > Class Template Reference
• casacore: casa::Image2DConvolver< T > Class Template Reference

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

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• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: TextParams Struct Reference
• Stellarium: TextureParams Struct Reference

... Reference Data for Calibration and Tools . ... If you would like to receive an e-mail every time a new COS reference file is delivered and the database is updated, you can subscribe to the cos_reffiles_upd mailing list. ... Burst Parameters Table . ... The high voltage reference table gives the times when the FUV high voltage was changed More... hv . ... The walk corection reference table gives parameters for correcting the pixel coordinates XCORR and YCORR of FUV TIME-TAG data More... walk . ...

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• File and Table Structures
• CDBS FOS Page
• Chapter 11: Advanced Camera for Surveys (ACS)

... int . write_oi_array (fitsfile *fptr, oi_array array, int extver, int *status) . Write OI_ARRAY fits binary table. ... write_oi_target (fitsfile *fptr, oi_target targets, int *status) . ... write_oi_wavelength (fitsfile *fptr, oi_wavelength wave, int extver, int *status) . ... write_oi_vis (fitsfile *fptr, oi_vis vis, int extver, int *status) . ... write_oi_vis2 (fitsfile *fptr, oi_vis2 vis2, int extver, int *status) . ... write_oi_t3 (fitsfile *fptr, oi_t3 t3, int extver, int *status) . ...

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• read_fits.c File Reference
• exchange.h File Reference
• DUST: dustiface.h File Reference

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• DIRT: The Dust InfraRed Toolbox
• ADASS 2003 Conference Proceedings
• The SuperCOSMOS Sky Surveys

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... ahf/fixed/om . ... Value specifying RA of S/C's attitude in the equatorial, earth-centred reference frame (if attitudelabel =fixed) . ... Values specifying Dec of S/C's attitude in the equatorial, earth-centred reference frame (if attitudelabel =fixed) . ... Values specifying position angle of S/C's attitude in the equatorial, earth-centred reference frame (if attitudelabel =fixed) (see comments) . ...

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• Calling Parameters

The reduction of a given magnitude m to bt is given by: . bt = a.m + b + c.(logr25 - <logr25>) . ... e.(logd25 - <logd25>) . f.(de1950 - <de1950>) . where a, b, c, d, e, f, <logr25>, <t>, <logd25> and <de1950> are constant values given in the table here below for each reference taken into account. The mean bt magnitude is calculated as a weighted mean where the weight (last column) is derived from each source of magnitude as the inverse square of the mean standard deviation. ...

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• References
• Session Parameters
• OPTOPUS Commands and Parameters

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

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• Orbits in the period / acceleration plane
• WAPP Signal Processing Page
• ALFA Receiver Temperature Polynomial Fit

... Files . ... tcc.msg.formatObjFields Namespace Reference . ... Definition at line 36 of file formatObjFields.py . ... Definition at line 107 of file formatObjFields.py . ... Definition at line 115 of file formatObjFields.py . ... Definition at line 129 of file formatObjFields.py . ... Definition at line 122 of file formatObjFields.py . ... Definition at line 213 of file formatObjFields.py . ... Definition at line 139 of file formatObjFields.py . ... Definition at line 247 of file formatObjFields.py ....

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• lsst.tcc: tcc.parse.getCoordSys Namespace Reference
• lsst.tcc: tcc.parse.getPVTList Namespace Reference
• lsst.coordConv: coordConv::OtherCoordSys Class Reference

Find Similar Abstracts (with default settings below ) . ... Also-Read Articles . ... Parameters of the 41 Dra system components . ... 00/2001 . ... Stars: Binaries, Binaries: Fundamental Parameters, Binaries: Individual . ... 61B Based on spectral and speckle-interferometric observations of the system 41 Dra, model atmosphere parameters of the system components have been derived: component Aa - T eff = 6500K, lg g = 3.99, R = 1.87 R solar , component Ab - T eff = 6500K, lg g = 4.11, R = 1.61 R solar . ...

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• References
• C Standard Library Functions
• Access via e-mail

... Append the name of the output grid file. ... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / Je lon0 / lat0 / scale (Equidistant). ...

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• Initial Distributions of Binary Parameters
• Parameters of the starburst
• Initial binary parameters

... Forum: The Linux Kernel Hackers' Guide . Keywords: kernel tuning, file handles, Bus error . ... In a recent comp.os.linux. article I saw a reference to tunable kernel parameters, which I think may help me with a problem I'm having with expireover on a Debian 1.2, Inn 1.4 unoff4 news server. ... I'm runnming 2.0.27, 64mb ram, raid 0 on three 2gb drives for /var/spool/news. ... I've been looking for some docs on tuning kernel parameters like file handles, and can't seem to find it. ...

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• Determination of the Detector Parameters

wcs2dr -- Convert WCS header information into drizzle parameters for image registration wcs2dr image refim . images = "" [file name] . ... The style for the output listing. ... cl wcs2dr @files ref style= para # drizzle .data= test1 drizzle .shft_fr= output drizzle .shft_un= output drizzle .align= center drizzle .xsh= 552.733 drizzle .ysh= 482.749 drizzle .scale= 1.009 drizzle .rot= - 2.871 # drizzle .data= test2 drizzle .shft_fr= output drizzle .shft_un= output ...

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• SEEING (V1.3) --- Apr00 --- SEEING (V1.3)

The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...

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• Magnetic mapping file description
• The magnetic conjugation conception
• STDA files

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• Nebular Abundances For Extragalactic PNe
• Database of Optical Properties -- Level: database
• Database of Optical Properties -- Level: subpage

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

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• Catalogue 5 of WDC-B

Next: Up: Optical Interferometer Script Data Previous: Optical Interferometer Script Data . ... Programmer's reference . ... The plot selection widget . ... Astrometry . ... Script library files . ... Introduction . ... Data files . ... Basic widget procedures . Load data . ... File usage . ... Data and auxilliary files . ... Output files . ... Open the data file . ... Open a data file . Access a data file . ... Accessing data files . ... NPOI raw data files . ... NPOI raw packet data files . ...

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• Optical Interferometer Script Data Reduction Version 8 for IDL
• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)
• Running CONSTRICTOR

... In some cases where memory space is at a premium, it is possible to tailor the configuration to remove such features as reference clock driver support, debugging support, and so forth. ... The following lines are used in this file: . ... The DEFS_LOCAL line defines global flags that apply to all machines. Ordinarily, the only flags included are the -DDEBUG , which includes the debugging code, and -DREFCLOCK , which includes basic reference clock support. ... D_INCLUDE_BSD_SOURCE . ...

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• Generic Reference Driver
• Debugging Hints for Reference Clock Drivers
• Reference Clock Options

Next: *pllist* - Look at Up: Regions and Source Parameters Previous: Regions and Source Parameters . ... cl> xray xr> ximages xi> plcreate region description: c 6930 9390 240 reference image file or 2 dims for mask: xdata$rp110590.qp output mask data file [root.pl]: rp110590 # =rp110590.pl file . ... xi> plcreate region descriptor: saoimage # default output file from SAOimage reference image file or 2 dims for mask: xdata$rp110590.qp output mask data file [root.pl]: rp110590 # =rp110590.pl file . ...

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• Possible Pitfalls
• *qplintran* -- Apply linear transformation to a qp file through filter
• ISDN References

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• Astronomy HyperText Book
• Astronomy HyperText Book: Stellar Evolution
• Cosmological Issues for Theorists