WCSLIB љ 5.15 . ... DataљStructures . ... fitskey Struct Reference . ... fitshdr() returns an array of fitskey structs, each of which contains the result of parsing one FITS header keyrecord. ... Returned ) Keyvalue data type: . ... Returned ) Logical ( fitskey::type == 1) and 32-bit signed integer ( fitskey::type == 2) data types in the fitskey::keyvalue union. int64 fitskey::k . Returned ) 64-bit signed integer ( fitskey::type == 3) data type in the fitskey::keyvalue union. int fitskey::l . ...

... 2003/01/10, MWB, fixed multi-line query error. ... Does nothing helpful to identify/report bad SQL syntax. ;- pro mysqlquery2,lun, query ,info, $ FORMAT =fmt,HEAD= heads , CMD = cmd ,VERBOSE=verbose,$ ngood = ngood ; Zero the output variables, so there's no risk of accidentally ; re-processing a previous result if something went wrong. heads = '' ; lun and query string are manditory, as are at least one output ; variable (unless the / CMD flag is set) if (keyword_set( ...

Next: General CCF Components Up: Calibration Access and Data Previous: List of CAL Routines Contents . This section contains descriptions of the structure of CCF constituents. ... The calibration team of the SOC is also providing additional CCF components where required in conjunction with data that were generated with SciSim. ... These CCF components are generated on a need basis and are identical in structure to the real life components. ... Generation from Ground Calibration Data . ...

ImageIO - Reference Counted C++ Class for Reading and Writing Images . include ImageIO .h // types of image data (these mostly correspond to the FITS BITPIX values) enum ImageDataType { UNKNOWN_ IMAGE = -1, // unknown type BYTE_ IMAGE = 8, // 8 bit images X_ IMAGE = -8, // special, color scaled, X image data SHORT_ IMAGE = 16, // 16 bit signed USHORT_ IMAGE = -16, // 16 bit unsigned LONG_ IMAGE = 32, // 32 bit integer FLOAT_ IMAGE = -32 // 32 bit floating point }; ...

lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...

... AINTRO- USING THE CGEN ROUTINES: . ... CGENPLOT - PLOT GENERATOR DATA . Next Routine] [ List of Routines ] help,d[500].geni[2],/st ** Structure CGEN1, 40 tags, length=160, data length=160: DEVTYPE LONG 3 CTRLSW LONG 2 STATE LONG 3 FAULTCODE LONG 0 FAULTTYPE LONG 0 KWPERCENT FLOAT 76.0000 TOTKWST FLOAT 755.000 NFPA110 LONG 24576 EXTENDEDST LONG 0 FREQ FLOAT 59.0000 TOTPF FLOAT 0.921850 TOTKVA FLOAT 821.000 TOTKW FLOAT 755.000 TOTKVAR FLOAT 319.000 VOLTSAB ...

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

The HyperNews Linux KHG Discussion Pages . Forum: Tour of the Linux kernel source . Keywords: configuration makefile . Date: Wed, 22 May 1996 17:34:39 GMT . From: Steffen Moeller < steffen@di.unito.it > . ... Or is this too trivial for a Hacker's Guide? ... If there's some positive feedback I'd like to start on this myself, but I'd need some help - at least for the language. ... Editing services available... by Michael K. Johnson . ... Kernel configuration by Venkatesha Murthy G. ...

Most radio and modem clocks used for a primary (stratum-1) NTP server utilize serial ports operating at speeds of 9600 baud or greater. ... In order to reduce these errors, a set of special line disciplines and stream modules can be configured in the Unix kernel. ... Note that not all Unix kernels support line disciplines and of those that do, not all support System V streams. ... There are two line disciplines and a special streams module included in the distribution. ...

Stellarium 0.12.3 . ... TextParams Struct Reference . Parameters specifying how to draw text. ... TextParams (const float x, const float y, const QString &string) . Construct TextParams with default parameters. ... TextParams ( Vector3 < F > &position3D, StelProjectorP projector , const QString &string) . Construct TextParams to draw text at a 3D position, using specified projector. ... string љ . ... Text string to draw. ... The required string parameter is also set, as is the projector. ...

... DevHlp_Security This devhlp allows to open a file for read access in the Init routine of a BASEDEV . ... returned: size of file SYIOpenFile ends Valid at INIT time only. ... This routine uses the corresponding function of the miniFSD , not normal file I/O, thus access is restricted. ... Although the size argument of the data structure implies, I'd recommend to better not read more than 32K at a time. ... DL = 044h This function will return the table of security helper functions for file access. ...

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...

... IDX+1) ; * if float, assumed to refer to IDSTR.( ... IDX +1) idxtr= idstr .( idx [0]+1L) ncomp= n_elements (idxtr.WVL) tnam =tag_names(idxtr) nflds= n_elements ( tnam ) for i=0,nflds-1 do begin if tnam [i] eq 'WVL' then xWVL=idxtr.WVL if tnam [i] eq 'Z' then xZ=idxtr.Z if tnam [i] eq 'ION' then xION=idxtr.ION if tnam [i] eq 'LABL' then xLABL =idxtr.LABL if tnam [i] eq 'FLUX' then xFLUX=idxtr.FLUX if tnam [i] eq 'FLUXERR' then xFLUXERR=idxtr.FLUXERR if ...

SAI VO . ... Web Services . Catalog Access Services . ... SAI Web Services . ... This service aims to automatically match stars in FITS image provided with catalogue and add the correct WCS keywords to its FITS header. ... Service Web Interface . ... The service is available here To use it, you has to provide the image as a Base64-encoded string, along with the rough information on image field of view size and center (the latter may be deduced from FITS header keywords like 'RA' and 'DEC'). ...

... 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). ...

... overview of pyQC . ... output used by . ... All pyQC scripts and modules share a similar structure. Python offers to group functions, classes, etc. into modules which can be imported by different scripts. ... In order to avoid confusion if names are used by different (especially external) modules, the QC scripts use the 'from' statement only for pyQC modules, i.e.: . ... For other modules, the simple 'import' statement is used: . ... Python modules are also used for keeping script configuration. ...

... Files with sunspot magnetic fields data ============================================== Column Format Description ______________________________________________ 1-2 I2 Day of month 3-4 I2 Month (numerical) 5-8 I4 Year 9 A1 Blank 10-13 I4 UT in hhmm 14 A1 Blank 15-19 A5 Sc - atmospheric flutter in arc sec 20 A1 Blank 21-25 A5 S - quality of the Sun image 26-27 A2 Blank 28-31 A4 Number of sunspots (numbering from unit every day ) 32 A1 ...

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...