... Abstract Find the vector in a specified plane that maps to a specified vector in another plane under orthogonal projection. ... Brief_I/O Variable I/O Description -------- --- -------------------------------------------------- vin I The projected vector. projpl I Plane containing vin. invpl I Plane containing inverse image of vin. vout O Inverse projection of vin. found O Flag indicating whether vout could be calculated. ... Detailed_Output vout is the inverse orthogonal projection of vin. ...

Blackholes Forum Message . Forums: . ... Discussion Forums | Blackholes I | Post . ... No There's Another Mistake . Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Usage: oicopy [--target_id n] [--arrname array] [--overwrite] [--flag vis/vis2/t3amp/t3] infile outfile -t/--target_id: only copies records for specified TARGET_ID -a/--arrname: only copies tables with specified ARRNAME -o/--overwrite: overwrite output file -f/--flag: flag all data of specified type (vis/vis2/t3amp/t3) Other switches will be added later. """ __revision__ = '$Revision: 1.4 $' import sys, getopt, os, string import oi_fits, pyfits, ieee def readfile(fileName): """Read FITS file. ...

... casa::OrderedMap< key, value > . ... OrderedMap (const value &dflt, uInt size) . ... OrderedMap (const OrderedMap < key, value > &other) . ... OrderedMap<key,value> is a template class derived from Map . ... template<class key, class value> . ... const key& casa::OrderedMap < key, value >::getKey . ... const value& casa::OrderedMap < key, value >::getVal . ... uInt casa::OrderedMap < key, value >::incr . ... uInt casa::OrderedMap < key, value >::ntot . ... uInt casa::OrderedMap < key, value >::nused...

... region (region-7.9.3) [xmmsas_20080701_1801-8.0.0] . ... The basic source region shape is a circle. There are three ways to assign the radius, specified via the parameter radiusstyle : . radiusstyle =`userfixed'. ... In this choice, the task uses for the source region radius that value which encloses energyfraction of the total flux under the Point Spread Function (PSF). ... At present the effect of this reprojection on the source region contours is ignored and circles are retained. ...

Next: External Functions Up: Fitting of Data Previous: The Corrected Gauss--Newton . ... Basic functions are either defined in the system or defined by the user as external FORTRAN routines. ... Basic functions are specified by the name, the independent variable(s) and parameter(s), with optional guesses for the parameters, following the syntax: name(var1[, ];par1[, ]) [par1=value] . ... Parameters are defined by unique names after the semicolon in the function specification. ...

Next: Power Law fit to Up: Spectral Analysis Previous: Error Determination . With PROS2.3 all fitting is performed using Poisson statistics , rather than Gaussian, so that results will be correct even for small counts ( ) in some channels. Power Law fit to a Point Source . Raymond Model . Two-Temperature Raymond Model . Limiting Energy Channels Input to the Fit . Multiple Data Sets . ... Fit a source with a small number of net counts . Inspection of results . ...

In Actor Prolog a resident is a special mechanism that helps processes to inspect state of other processes. A resident observes the state of a specified (target) process and if the state of the process changes (for instance, after message handling) it proves a specified predicate of the process. ... Work of the resident. ... Any change of the list of target processes or arguments of resident function results in activation of the resident and repeated collection of information in the target worlds. ...

The ntpq and xntpdc utility programs can be used to debug reference clocks, either on the server itself or from another machine elsewhere in the network. The server is compiled, installed and started using the command-line switches described in the xntpd page. ... First, use the pe and as commands to display billboards showing the peer configuration and association IDs for all peers, including the radio clock peers. ... The most useful are the clockstat and commands described in the document page. ...

... Linear limb darkening coefficients are taken from tables published by Van Hamme (1993, AJ 106, 2096). limb_stars Compute limb darkening fit coefficients for all stars. limb_star ( spectrum _char , filter _char ) Function. Return linear limb darkening coefficient integrated over specified bandpass. Example: print, limb_star('G0I','V') . ... Return factor to multiply the uniform disk diameter with in order to get a limb darkened diameter using the specified linear limb darkening coefficient. ...

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... TuiNodeActivate Class Reference . ... voidљ . ... TuiNodeActivate (const QString &text, QObject *receiver, const char *method, TuiNode *parent=NULL, TuiNode *prev=NULL) . Create a TuiNodeActivate node. ... virtual TuiNodeResponse љ . handleKey (int key) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual TuiNode *љ . ... virtual voidљ . ... Contains the numbers of the parent nodes in the hierarchy. ...

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. ...

... public class WindowManager . ... This class consists of static methods used to manage ImageJ's windows. ... static void . ... Adds the specified window to the Window menu. static boolean . ... Returns a reference to the active image or null if there isn't one. static ImageWindow . ... Makes the image contained in the specified window the active image. static void . ... Returns the first image that has the specified title or null if it is not found. public static void addWindow (java.awt.Frame win) ....

. To change your current working directory use the command: cd pathname . where pathname specifies the directory that you want to move to. The pathname can be given as either a full pathname or a relative pathname . Examples . Did You Know? .

... include <string.h> . char *stpcpy ( char *dest, char *src) - Copy one string into another. int strcmp( char * string1 , char * string2 ) - Compare string1 and string2 to determine alphabetic order. char *strcpy( char * string1 , char * string2 ) - Copy string2 to stringl. char *strerror( int errnum) - Get error message corresponding to specified error number. int strlen( ...

... SSAU History . SSAU roadmap . ... The participants got unique knowledge during the four very busy days of training at the School of Astronautics, they heard firsthand about the life at the International Space Station and the work in space, they even were able to try on the suit for the spacecraft flight and the gloves, in which Oleg Artemyev worked in open space. ... If I lived another life, I would have studied in SSAU at the Engine Building Department , - shared his thoughts Oleg Artemyev. ...

Allows you to specify a drift scan: motion at a constant velocity along a great circle. ... The path starts at the new object position (though the telescope actually intersects the path later, see Subtleties ). ... Note that the units are always /sec for both axes. ... The velocity along the path is 0.01 /sec. ... The path is assumed to start when you hit the Slew button (more precisely, when the TCC parses the command). However, it takes the telescope awhile to slew to meet the specified path. ...

Hipparchus (and possibly Aristarchus before him) also derived the Moon's distance from the duration of a lunar eclipse . Because the Earth casts a much larger shadow than the Moon, such an eclipse usually darkens the entire Moon, for several hours. ... If the Sun is assumed to be very distant, and if the Moon crosses the middle of the shadow (if not, corrections must be made), the width of the shadow is expected to be about 2r , twice the Earth's radius r . ... Last updated 4 February 1999 Moon. ...

... Apache HTTP Server Version 2.4 . ... On systems with multiple users, each user can be permitted to have a web site in their home directory using the UserDir directive. Visitors to a URL http://example.com/~username/ will get content out of the home directory of the user " username ", out of the subdirectory specified by the UserDir directive. ... Per-user web directories . ... the URL http://example.com/~rbowen/file.html will be translated to the file path /home/rbowen/public_html/file.html . ...