Next: Specifying Pixels in Up: MIDAS Data Structures Previous: Specifying Keywords . The MIDAS table file system is described in detail in chapter 5 of this volume. Here we just explain briefly how to access the various elements in a table file. To do so, it is necessary to specify the table name , the column and the row . ... would display the element in column 3 of row 10 in table file tname.tbl . ... All table commands default the data files to tables with extension .tbl . ...

... disprm Struct Reference . ... Returned ) Pointer to the first element of an array of int* containing pointers to the first elements of the arrays of integer distortion parameters for each axis. double ** disprm::dparm . Returned ) Pointer to the first element of an array of double* containing pointers to the first elements of the arrays of floating point distortion parameters for each axis. int disprm::i_naxis . ... Returned ) The number of distortion functions. struct wcserr * disprm::err . ...

... NOTES: ; This routine automatically determines which axis is wavelength and ; which axes are RA and Dec. ... ;VOPT , ZOPT , $ AWAV , VELO , BETA ] for i = 0,n_elements(wave_axes_types)-1 do begin axis_lambda = where( strmid( astr.ctype ,0,4) eq wave_axes_types[i], lambdact) if lambdact eq 1 then break endfor ; ; Check for NONSTANDARD LAMBDA axis type produced by Gemini GMOS IRAF ; ; pipeline ; if lambdact eq 0 then begin ; axis_lambda = where( strmid( astr.ctype ,0,6) eq ...

Main Page Data Structures File List Data Fields Globals . Array element. More... #include < exchange.h > . char . ... diameter . double . ... Corresponds to one row of an OI_ARRAY FITS table. char _element::tel_name[17] . char _element::sta_name[17] . int _element::sta_index . float _element::diameter . double _element::staxyz[3] . The documentation for this struct was generated from the following file: . exchange.h . ...

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Static Public Member Functions . CLIProcessor Class Reference . ... argsGetOption (const QStringList &argList, QString shortOpt, QString longOpt) . Check if a QStringList has a CLI-style option in it (before the first ). ... Retrieve the argument to an option from a QStringList. ... Check if a QStringList has a yes/no CLI-style option in it, and find out the argument to that parameter. ... a long-form option string, e.g. "&ndash;help" . ...

This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...

The NTP Version 3 daemon currently supports several different radio, satellite and modem reference clocks plus a special pseudo-clock used for backup or when no other clock source is available. Detailed descriptions of individual device drivers and options can be found in the Reference Clock Drivers page. Additional information can be found in the pages referenced there, including the Debugging Hints for Reference Clock Drivers and How To Write a Reference Clock Driver pages. ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . Classes . ... NamespaceљList . ... All љ Classes љ Namespaces љ Files љ Functions љ Variables љ Typedefs љ Enumerations љ Enumerator љ Macros љ Pages . tcc . ... tcc.parse.cmdParse Namespace Reference . ... A class that holds command definitions, and can parse tcc commands. ... defљ . ... Return the index of keyword in list allowing unique abbreviations and independent of case. ... Constructs a generic TCC command from pyparsing elements. ...

... Next: Star Finding and Up: Image Restoration and Previous: Multiresolution and Astronomical . ... Design improvements continue to be made in the filter developed using mathematical morphology principles for the Infrared Astronomical Satellite ( IRAS ) images. The purpose of this filter is to eliminate Galactic cirrus emission from extragalactic fields. ... With an appropriate normalization, the filter curve was applied to each pixel in the image to remove the Galactic cirrus. ...