... Standard-star files, however, must also have the standard photometric values (in place of the rough MAG column). The column label should be the usual name of the magnitude or index in the column, e.g., V or U-B or c1; see Table . ... MIDAS table files do not distinguish between upper and lower case in column labels. Thus, while it is possible to use 'u-b' as a column label for the uvby system, it cannot be distinguished from 'U-B' by programs or MIDAS procedures that read these files. ...

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• Standard stars
• Standard orientation
• Displaying Tables

... FIELD | ... static int . ... Field Detail static final int AREA . ... Constant Field Values . static final int MEAN . ... static final int STD_DEV . ... static final int MODE . ... static final int MIN_MAX . ... static final int CENTROID . ... static final int CENTER_OF_MASS . ... static final int PERIMETER . ... static final int LIMIT . ... static final int RECT . ... static final int LABELS . ... static final int ELLIPSE . ... static final int INVERT_Y . ... static final int CIRCULARITY . ...

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• PGM_Reader (ImageJ API)

... The standard lbn cal diode was compared to the standard diode. Using the standard diode value and the insertion loss the lbn cal value was computed every 25 MHz from 1200 MHz to 1600 Mhz. ... After the measurement, the insertion loss from the standard diode to the output of the coupler was measured over the frequency range 1200 to 1400 Mhz. ... The major uncertainty in the measurement is in the standard diode ENR and the insertion loss of the waveguide transition. ... freq [Mhz] . ...

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• encoderOffsets
• measured_operating_values
• ALFA Performance at 1665 MHz

These routines are meant to provide a simple to use asynchronous line reading facility. ... arln_read_float . Read a floating point value from the user. arln_read_int . ... Read a line from the user. float arln_read_float (CONST char *prompt, float default_value) . ... If no input is given, the routine returns a default value. ... Returns: The value. ... This routine will prompt the user for a single boolean value. ... flag arln_read_line (char *buffer, unsigned int length, CONST char *prompt) . ...

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• casacore: casa::AipsrcVector< T > Class Template Reference
• casacore: casa::AipsrcValue< T > Class Template Reference
• difx:vdifio [ATNF VLBI Wiki]

... This article is part of the LWN Porting Drivers to 2.6 series . This article serves as a sort of final resting place for various small changes in the kernel programming API which do not fit elsewhere. The kdev_t type has been removed from the kernel; everything which works with device numbers should now use the dev_t type. ... Consider using these while fixing your code; the next time the type of i_rdev changes, you will be happier. ... Driver porting: miscellaneous changes, designated inits . ...

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• Looping and Iteration
• Advanced Pointer Topics
• exit()

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• Astronomy HyperText Book: Stellar Evolution
• U of O High Energy Physics Seminars

... Abstract Find the minimum of a set of double precision values. ... Brief_I/O Variable I/O Description -------- --- -------------------------------------------------- n I The number of double precision values to compare.. ... Detailed_Input n is the number of double precision values in the set whose minimum is to be determined... represents a variable argument list. ... 2) If the number of double precision values supplied does not match the argument n, the action of this routine is not defined. ...

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• A Guide to Kermit Data
• CSPICE Routines: MAXD_C
• CSPICE Routines: SCE2C_C

To read standard input into a shell script use the read command. For example: echo "Please enter your name:" read name echo "Welcome to Edinburgh $name" . This prompts the user for input, assigns this to the variable name and then displays the value of this variable to standard output . ... For example: echo "Please enter your surname\n" echo "followed by your first name: \c" read name1 name2 echo "Welcome to Glasgow $name2 $name1" . ...

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• UNIXhelp Glossary - "B"
• Mail program files
• Redirecting standard input and output

spectrum1d - compute auto- [and cross- ] spectra from one [or two] timeseries. spectrum1d [ x [ y ] file ] -S segment _ size ] [ -C ] [ -D dt ] [ -N name _ stem ] [ -V ] [ -W ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] spectrum1d reads X [and Y] values from the first [and second] columns on standard input [or x [ y ] file ]. ... Units same as ypower. name _ stem .npower Power spectral density of the noise output. Units same as ypower. name _ stem .gain Gain spectrum, or modulus of the transfer function. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/minmax.html
• http://xray.sai.msu.ru/~ivan/gmt/man/splitxyz.html
• http://xray.sai.msu.ru/~ivan/gmt/man/surface.html

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... The image dataset to be smoothed. outset . ... This parameter is read if smoothstyle =`simple' is chosen and prescribes the shape or type of convolver to use to smooth the image. width . ... See section 3.3 for further details. normalize . ... If set, the task reads from parameter invarianceset an image of the variances (squares of the standard deviations) of the input image values. invarianceset . ...

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• Input Files

... Data Reduction FAQ > Negative pixel values in the 2D spectrum image are not being ignored by the standard extraction procedure. ... The X-Shooter pipeline flags but does not ignore those pixels that are negative in its algorithms including standard extraction. ... If a reset anomaly has not occurred in your data, and negative pixels are causing a problem, then simply add 2097152 to the value of the parameter decode-bp to start treating negative pixels in the raw data as bad pixels by ignoring them. ...

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• OYSTER Lab
• A standard recipe
• Imaging simulations

A problem, that can arise when moving from Fortran 77 to Fortran 90, is dependent on a usual deviation from the standard, and has to do especially with user programs. ... With many Fortran 77 implementations we wrote PROGRAM TEST REAL X WRITE(*,10) 10 FORMAT('Give X = ',$) READ(*,*) X WRITE(*,*) X END In Fortran 90 we use "non-advancing I/O" instead. ... In some old Fortran dialects the statement TYPE was used to write on a typewriter terminal and PRINT was used to write on the line printer. ...

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• Tutorial on Fortran 90, Digital UNIX
• Keyword arguments and default arguments
• Summary of Fortran 77 statements

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• SFIT2 - Command Syntax
• Spectrum - control
• CD-ROM's

ntpq [ -inp ] [ -c command ] [ host ] [ ... ] . ntpq is used to query NTP servers which implement the recommended NTP mode 6 control message format about current state and to request changes in that state. ... Requests to read and write arbitrary variables can be assembled, with raw and pretty-printed output options being available. ntpq can also obtain and print a list of peers in a common format by sending multiple queries to the server. ... Causes output from query commands to be "cooked" . ...

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• Tsearch2 and Unicode/UTF-8
• HSV is Groo-V!
• Authentication Options

OptInt PmWiki . ... Forms . ... This page explains how you can embed input forms into wiki pages. ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...

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• OptInt PmWiki : PmWiki / Forms
• OptInt PmWiki : PmWiki / Page File Format
• A Calculation of derivatives

repetition index means value+1: ; 0 means 1 iteration, 2 means 3 iterationis, 255 (the max) ; means 256 iterations ; This apply on BOTH loop and output mask, so (LINE @ 0) means LINE for 1 ; clock cycle ; some symbols ; ZERO equ #0 ; all void BASE equ ZERO ; standard no operation pattern PIXEL equ #01 ; xclock XSYNC equ #02 ; xsync LINE equ #04 ; yclock YSYNC equ #08 ; ysync RSTX equ #10 ; Reset of all Quadrants SOCX ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientguide/glossary.htm
• Block Device Drivers
• CHIANTI atomic database

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9

... Next: FITS Checksum Verification Up: Data Models and Previous: A Proposed Convention . ... The FITSIO Subroutine Library has been available for 3 years, and has matured into a stable, full-featured interface for reading and writing FITS format files. ... The FITSIO subroutine library for reading and writing FITS files is now three years old and is used by many projects as the standard programming interface for accessing FITS format data files. ...

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• IRAF Multiple Extensions FITS (MEF) Files Interface
• SDFITS: A Standard for Storage and Interchange of Single Dish Data
• ADASS 2003 Conference Proceedings

... Events can be selected based on a flexible set of user-specified criteria that allows column values to be compared with numeric values, header parameters, functions, or other column values. To do this, we use a technique in which a filter specification is converted into a tiny C program, which is compiled and linked automatically so that events can be fed to this program and filter results returned to the calling program. ... short PHA . ... select events whose pha value is exactly 10 . ...

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• Model Spectra for Spectral-Fitting Program
• Mapping Pixel Values to Screen Intensity
• Reading Einstein FITS files

Last updated 5 November 2003 by JMD . Last link checked 9 October 2003 by JCB . Data from 191 observations of stars with the ARCES were analyzed to calculate exposure times to reach particular signal-to-noise values for bright standard stars. ... An exponential fit to the data shows pretty good agreement and allows for forecasting to fainter stars beyond the limit of the data set ( V ~ 12). The fit was used to calculate the exposure times in the table below: . ...

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• TUI:Telescope:User Catalogs
• Astrophysical Research Consortium - Apache Point Observatory
• TUI:TUI Menu:Preferences Window