... 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 . ...

transfer_sms_files_to_opus (version 14.04.22) . ... transfer_sms_files_to_opus.py . ... USAGE: do transfer_sms_files_to_opus <smsname> [<cmdtime>] [<type>] . ... convert_to_opus_time (spss_time =None ) . ... format into an OPUS time (YYYYJJJHHMMSS format). ftp_sms_files (input_data =None ) . ... query_for_sms_for_opus (sms_id =None , pass_id =None , file_type =None , replan_time =None ) . ... This will be one id per record in the output file. run (sms_name =None , cmd_time =None , send_type ='ALL' ) . ...

... eparam* - edit parameter files . ... Type ``<esc>-?'' within a parameter editor for more details on commands. *tupar* - Edit table headers . Table files (* .tab ) consist of a header including a variety of parameters and the table itself. It is possible to edit the header using tupar and the table with tedit provided you have write-access to the file. ... Works like emacs but uses <ctrl> D to exit. *hedit* - edit image file header . qphedit* - edit .qp file headers . ...

Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...

... Class . ... METHOD . ... java.lang.Object ij.plugin.filter.UnsharpMask . ... public class UnsharpMask . ... Unsharp masking subtracts a blurred copy of the image and rescales the image to obtain the same contrast of large (low-frequency) structures as in the input image. ... This method is invoked by a Generic Dialog if any of the inputs have changed (CANCEL does not trigger it; OK and running the dialog from a macro only trigger the first DialogListener added to a GenericDialog). void . ...

... new LaTeX template, approved version . ... only minor changes for task version 1.4 . ... applies to task version 1.5: . ... applies to task version 1.6: minor updates . ... applies to task version 3.0: new parameter names . ... applies to task version 3.1: parameter gain file removed . ... applies to task version 5.0: new parameter randomization_on . ... applies to task version 5.1: new optional parameter srcposition . ... Null values, high/low accuracy gain/cti correction, new errors and warnings ....

... JavaScript version 1.3 provides the following new features and enhancements: . ... See the Client-Side JavaScript Guide for details. ... Changes to the Array object. ... The push method returns the new length of the array rather than the last element added to the array. ... Changes to the Date object. ... Added a day parameter to the setMonth method. ... Added the apply method, which allows you to apply a method of another object in the context of a different object (the calling object). ...

... 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 ...

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... This is a first attempt at writing the lessons I learned when trying to convert the mod_mmap_static module to Apache 2.0. ... So the name gets a small change from mmap_init to mmap_post_config . ... server_rec *s . ... server config */ . create per-server config structures */ . ... merge server config */ . merge per-server config structures */ . ...

... StelScriptMgr Class Reference . ... const QStringљ . ... Stops any running script. ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getDescription . ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getLicense . ... Get the rate at which the script is running as a multiple of the normal execution rate. void StelScriptMgr::pauseScript . ...

... Fortran . Storage rules Dummy argument is a quantity in the specification of a procedure, function or subroutine. Actual argument is a quantity in the call of a procedure, function or subroutine. ... Becomes 101 END PROGRAM EXAMPLE SUBROUTINE SUB(X, Y, Z) IMPLICIT NONE REAL, INTENT(IN) :: X REAL, INTENT(INOUT) :: Y REAL, INTENT(OUT) :: Z Y = Y**2 Z = X + Y END SUBROUTINE SUB In Fortran there is really only one kind of argument usage, called argument association. ...

... to_tsquery( [ configuration , ] querytext text) RETURNS TSQUERY . ... Query rewriting is a set of functions and operators for tsquery type. ... We'll expand query supernovae using table-driven rewriting rules. =# create table aliases (t tsquery primary key, s tsquery); =# insert into aliases values(to_tsquery('supernovae'), to_tsquery('supernovae|sn')); =# select rewrite(to_tsquery('supernovae'), 'select * from aliases') && to_tsquery('crab'); ?column? --------------------------------- ( 'supernova'...

... fdldelay ( baseline [, spectrometer , /scan ]) Function. Return residual FDL delay for specified baseline. ... The scan keyword specifies whether or not all records belonging to the scan will be returned. If not, then only the records associated with the currently loaded bincount data (if any) will be returned. ... Return complex Fourier transform of visibility with respect to wavenumber, computed at delay values d . ... Return white light phase delay for complex visibility . ...

Main Page Data Structures File List Data Fields Globals . ... Go to the source code of this file. struct . ... Data for OI_ARRAY FITS table. ... write_oi_array (fitsfile *fptr, oi_array array, int extver, int *status) . ... Data for OI_ARRAY FITS table. typedef struct _target target . ... Data for OI_TARGET FITS table. typedef struct _oi_wavelength oi_wavelength . Data for OI_WAVELENGTH FITS table. typedef struct _oi_vis_record oi_vis_record . ... fptr , . ... array data struct, see exchange.h . ...

... Some commands are not yet documented. bin . ... expose . ... number . ... If basename is not specified, the filenames are determined by the ICC's path , name , places , and number If neither red nor blue is specified, both images will be saved. ... Returns: basename , name , number path , places . ... For example, with path= /export/images/DD01 , name= bias. , places= 3 , and number= 11 , the blue image file would be /export/images/DD01/bias.011b.fits . ... name , number , places , path , basename ,...

Next: Semi-major axis change Up: Change of Binary Parameters: Previous: Change of Binary Parameters: . The mass of the star that loses matter is . Accordingly, the mass of the accreting star is . where is the accretion rate   of the captured matter. ... In the case of compact accretors, we require the rate of their mass increase to be limited by the accretion energy output equal to the critical Eddington luminosity   . ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

November 5, 2001 (Monday) Xiao-Gang He, National Taiwan University . ... Tuesday, 2:00 pm, 472 Willamette Hall . Fall 2000 . Winter 2001 . Spring 2001 . ... Recent data from type Ia supernovae show that our universe is currently expanding with an accelerating rate. ... I will also discuss how structure formation is affected. 4:00pm, 318 Willamette Hall . ... To facilitate interpretation of this result, model independent analyses are also presented. 2:00 pm, 472 Willamette Hall . ...

... Bad Astronomy . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... The length of the shadow depends on the height of an object (like a mountain or a human) and how high up the Sun is. ... We can calculate the length of the shadow if we know the Sun's angle above the horizon and the object's height. ... The Earth spins 360 degrees in 24 hours, which means it spins 1 degree in 4 minutes; that in turn means the Sun moves 1 degree every 4 minutes in the sky. ...

... The Multiple Extension FITS (MEF) file interface is an IRAF library providing facilities for general file operations upon FITS multi-extension files. ... The Multiple Extensions FITS (MEF) interface consists of a number of routines to mainly read a FITS Primary Data Unit or an Extension Unit and manipulate the data at a file level. ... Read the FITS header of a MEF file that matches the EXTNAME or EXTVER keyword values or if not specified, read the extension number `group'. ... The header filename. ...