... An input dataset with at least one table. ... The table of interest must contain: . FRAME column, of type 32-bit signed int . CCDID column, of type 8-bit int. In the case of the PN instrument, the allowed range of values is [0,1,2]. In the case of the PN instrument, an additional column . QUADRANT column, of type 8-bit int. The allowed range of value is [0,1,2,3]. is also required. If the parameter withsettings is false, then the table must also contain the following attributes: . ...

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• Data-set
• dataset

... User Guide ] Task: uvmodel Purpose: Add, subtract, etc, a model from a uv data set. Categories: uv analysis UVMODEL is a MIRIAD task that modifies a visibility dataset by combining or replacing it a model. ... Key: vis Input visibility data file. No default Key: model Input model cube. ... Key: line The visibility linetype to use, in the standard form, viz: type,nchan,start,width,step Generally if there is an input model, this defaults to the linetype parameters used to construct the map. ...

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• Miscellaneous Analysis Tasks
• BBSYN2
• DOPSRC

The sections <Directory> , <Location> and <Files> can contain directives which only apply to specified directories, URLs or files respectively. Also htaccess files can be used inside a directory to apply directives to that directory. ... The order of merging is: . ... If multiple <Directory> sections apply to the same directory they are processed in the configuration file order. ... Using the options in question is only possible inside a <Directory> section (or a .htaccess file). ...

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• Apache module mod_access
• Apache module mod_auth_anon.c

... HST Phase II Proposal Instructions for Cycle 20 > Chapter 12: Cosmic OriginsSpectrograph (COS) > OBSERVING MODES > 12.11 Mode = TIME-TAGConfig = COS/NUV . ... Note: No wavelength should be specified if MIRRORA or MIRRORB is the Spectral Element. ... BUFFER-TIME . ... FP-POS = ALL indicates that the specified exposure time will be the exposure time for each FP-POS position. The values FP-POS=1, 2 or 4 will result in the exposure being taken at an offset from the specified central wavelength. ...

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• Mode = ACCUMConfig = ACS/WFC
• Changes in Treatment of STIS GO-WAVECAL Exposures (TARGET=WAVE)
• CSPICE Routines: EKCII_C

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. ...

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• Stellarium: LabelMgr Class Reference
• Stellarium: TriangleIterator< V > Class Template Reference

... Apache HTTP Server Version 2.2 . ... 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 . ...

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• Access LEDA from Aladin
• mod_suexec - Apache HTTP Server
• mod_authz_host - Apache HTTP Server

... Apache HTTP Server Version 2.2 . ... 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 . ...

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• mod_suexec - Apache HTTP Server
• mod_authz_host - Apache HTTP Server
• mod_mem_cache - Apache HTTP Server

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 . ...

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• The XPA Name Server (xpans)
• Autoconfigure of Frame #1
• *srcinten* - Calculate Source Intensity

... The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image projections. ... They were CRPIX n for the reference pixel location on pixel axis n , CRVAL n for the coordinate value at that pixel, CDELT n for the increment at that pixel in the coordinate value, and CTYPE n for the type of coordinate. ...

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• Exploring Interactive Archive Data Presentation at the COSSC
• Numerical Observatory: a Web Site for the Retrieval, Analysis, and
• Building Software from Heterogeneous Environments

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... Amateur Telescope Makers Association, ATMA 18 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

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• Amateur Telescope Making Journal, AstroGuide Listing
• Communications For Your Astronomy Event - an Astronomy Net Article
• Help Needed On Adding Additional Objects To FITS Images... - an Astronomy Net

... D.1 Grammar . ... D.3 Comparison of tokenization in CSS2 and CSS1 . This appendix is normative. ... STRING ] S* ]? ']' ; pseudo : ':' [ IDENT | ... LENGTH S* | ... return CDC;} ~= { return INCLUDES;} |= { return DASHMATCH;} { string } { return STRING ;} { ident } { return IDENT ;} # {name} { return HASH;} @import { return IMPORT_SYM;} @page { return PAGE_SYM;} @media { return MEDIA_SYM;} @font-face { return FONT_FACE_SYM;} @charset { return CHARSET_SYM;} @ { ...

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• Colors and backgrounds

TH setINDI 1 .SH NAME setINDI \- set one or more writable INDI property values .SH SYNOPSIS \fBsetINDI [options] device.property.e1[;e2...]=v1[;v2...] ... \fP .SH DESCRIPTION .na .nh .PP setINDI connects to an indiserver and sends commands to set new values for specified properties. ... TP -p <p> connect using alternate port p; the default is 7624. ... SH EXIT STATUS The setINDI program exits with a status of 0 if it suceeded in setting the new value for each specified property. ...

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• RoiProperties (ImageJ API)
• DirectoryChooser (ImageJ API)
• ij.io (ImageJ API)

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. ...

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• TUI:Telescope:User Catalogs
• TUI:Instruments:DIS:DIS window
• TUI:Scripts:Built In Scripts:(Inst):Focus

... Note you are not allowed to nest FORM elements! ... Forms are created by placing input fields within paragraphs, preformatted text, lists and tables. ... Notice the use of the NAME attribute to name each field : TITLE Sample Questionaire /TITLE H1 Sample Questionaire /H1 P Please fill out this questionaire: FORM METHOD=post ACTION= http://www.hal.com/sample P Your name : input name = name size= 48 P input name = male type =radio Male P input ...

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• Font Style Elements
• Figures
• Suspending commands with the sleep command

... GRIN lenses for telecommunication optics applications ? GTC (gradient telecom) lenses. ... GTC lenses are used in different fiber-optic devices: collimators, couplers, isolators and WDM etc . ... 2.Diameter . GTC lenses diameters are 1.0 mm, 1.8 mm, 3.0 mm and 4.0mm. ... 1.0 mm -3.0 mm diam GTC lenses are supplied in 0.22P, 0.23P, 0.25P, 0.27P and 0.29P length. 4.0 mm diam GTC lenses are supplied in 0.11P length. ... GTC . ... 3 scratches with 5mkm max width and 200mkm max length are allowed . ...

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The NTP standard specifies an extension which provides cryptographic authentication of received NTP packets. ... The specification allows any one of possibly 4 billion keys, numbered with 32-bit key identifiers, to be used to authenticate an association. ... In the case of MD5, the keys are 64 bits (8 bytes). xntpd reads its keys from a file specified using the -k command line option or the keys statement in the configuration file. ... A zero key in NTP format would be specified as 8080808080808080 . ...

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• Monitoring Options
• Debugging
• SN 1989B Light Curve Analysis.

Next: Introduction Up: Ceilidh - On Line C Tutoring System Previous: Ceilidh - On Line C Tutoring System . ... On line course notes . Automatic Assessment of C programs . Template programs are provided to start you on an exercise. ... Automatic Compilation of programs . Programs can be run against test data and user specified data . CEILIDH will be used to help mark your coursework. ... CEILIDH marks a program in many ways: it analyses style, efficiency, `prettiness' and output. ...

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• Chapter 11. Specifying OpenGL Environment Variable Settings
• Ideal Backend for E-ALFA
• Standard On

... The current cable tray route specified in the UTE-FTT interface document MRO-ICD-EIE-0032d gives a length of 5.5m from the edge of the optical table to the bottom of Q5, the rack containing the FTT electronics. ... ACTION: - MRO will examine the cable route in detail and estimate the length of cable between the worst case camera position on the optical table and the position of the FTT space in Q5. ... Heat must be extracted from the camera's peltier cooler and also from the camera enclosure. ...

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• OptInt PmWiki : PmWiki / Page List Templates
• OptInt PmWiki : PmWiki / Available Actions
• OptInt PmWiki : PmWiki / Forms

Next: Bias correction of visibilities Up: Discussion of reduction issues Previous: Discussion of reduction issues Contents . With the advent of the 6-way NPOI configuration in which the observer can switch in and out stations, the number of participating stations can change throughout the night. This is equivalent to VLBI, where different sub-arrays are observing. ... It is handled using a field in the scan table ( scantable.station ), which, for every scan, indicates which stations were used. ...

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• EVM and ETRM specification for ESO instruments
• List procedures
• Stellar models