The Agile filter wheel controller can be accessed via telnet to agile-rotator on port 4100. Close the socket when you are finished (there is no disconnect command). ... Always prefix filterwheel commands with "fw ". ... If you mistype a command that does not have an "fw " prefix then you'll get whatever the rotator controller outputs. ... Returns status . Move filterwheel slot n , where 1 n 6. ... low-level stepper motor controller status . ... high-level filter wheel controller status . ...

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NCR 53CF94, 53CF96 FLYER INFORMATION The NCR 53CF94 and 53CF96 Fast SCSI Controllers are high-performance CMOS devices conforming to ANSI standards X3.131-1986 (SCSI-1) and X3.131-199X (SCSI-2) for the Small Computer Systems Interface (SCSI). ... The NCR 53CF94 and 53CF96 feature 10 megabytes per second (MB/s) Fast SCSI-2 data transfers, improved single-ended SCSI operation, a 24-bit transfer counter, and enhanced SCSI-2 command functionality. ...

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... Welcome to the ADLab home page! Advanced Design Laboratory of the Special Astrophysical Observatory is concerned with research on low light level imaging and development of scientific digital imaging systems. About ADLab . ... Current project "A New Generation Multipurpose CCD Controller" . Project Contents . ... Publications on the Project . ... Other Web Sites of Interest . Created: 24 March 1998 . ... people have visited our web site. ... Copyright 1998 Advanced Design Laboratory. ...

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... spectrum . ... nsource <n> : choice of source function (def: 3=Feautrier) . noptype <n> : choice of continuous opacity (def: 1=Kiel) . nhedat <nhedat> : choice of HeI data (BCS or Mon treal) (def: 1=BCS) . ... read_model <filename>: read model atmosphere in QUB/STERNE2 format . ... wavmax <w_max> : distance from line centre to compute . ... nvturb <n vt > : number of points in -dependent v turb . ... tau_exp <n> : increase resolution of optical depth scale by adding additional points . ...

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Remembering the name of a command and how it is used can be difficult. Assigning your own name for a command - an alias - is very easy. Assigning an alias is done with the command: alias name definition . The syntax of the alias command is different for each shell. Follow the guidelines and examples for the shell that you are using. ... Creating an alias with the C shell . ... Creating an alias with the Korn shell . Creating an alias with the Bourne Again SHell . ...

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Astronomical Data Analysis Software and Systems XII ASP Conference Series, Vol. ... Fasti is a controller architecture originally developed for fast infrared astronomical array detectors, and intended to be powerful and extendible. ... Fasti Layout Commands Data flow Buffered data User's Host Embedded Controller Commands BFD- FIFO Buffer SVB - Sequence generator Generated waveforms Analog data 2 CADC Boards Conditioned control signals ASD - Signal conditioning Detector Figure 1. version 2. ...

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• DIRT: The Dust InfraRed Toolbox
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Each Apache module is described using a common format that looks like this: . Status: status . ... This indicates how tightly bound into the Apache Web server the module is; in other words, you may need to recompile the server in order to gain access to the module and its functionality. ... A module with "Extension" status is not normally compiled and loaded into the server. ... Modules which are not included with the base Apache distribution ("third-party modules") may use the "External" status. ...

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• Definitions of terms used to describe Apache directives
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... champ name : Source ID in the format explained in the Definitions section. ra : RA in decimal degrees. ... pos_error : Source count extraction radius in arcseconds. netB : net counts in B-band. See Definitions section. error_netB : error of net counts in B-band. see Definitions section. netS : S-band net counts, defined analogously to netB . ... See Definitions section. C21 : X-ray color. ... C32 : X-ray color. See Definitions section. rateB : B-band count rate in ksec. ...

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... Advances in International Accounting is a refereed, academic research annual, that is devoted to publishing articles about advancements in the development of accounting and its related disciplines from an international perspective. ... title='LG Стиральная машина LG - LG' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . ... Цвет: серый . Коллекция: Весна-лето 2016 . ... Материал верха: искусственная замша . ... Материал подошвы: искусственный материал . ...

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ELF-VLF ADVANCED SIGNAL ANALYZER AND SAMPLER SAS-2 . ... Therefore the SAS-2 must be input signals in the band 20Hz…16kHz (or 20kHz) from as other SI. In this case the SAS-2 must get the wide-band ELF-VLF input signal form the . ... e) Onboard Time: The time is needed to program scheduled data collections ! ... MODE 2 : In this mode the SAS-2 investigates that the input signals appearing in the three (six) input channels are a whistler or not. ... Address of input channel is added to each sample. ...

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... Classes . ... StelQGLViewport Class Reference . ... Definition at line 84 of file StelQGLViewport.hpp . ... Definition at line 132 of file StelQGLViewport.hpp . ... Definition at line 337 of file StelQGLViewport.hpp . ... Definition at line 351 of file StelQGLViewport.hpp . ... Definition at line 304 of file StelQGLViewport.hpp . ... Definition at line 359 of file StelQGLViewport.hpp . ... Definition at line 247 of file StelQGLViewport.hpp . ... Definition at line 148 of file StelQGLViewport.hpp . ...

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and 42 % 27-11-1999 Andr\'as Holl % 2.31: 02-05-2001 % % Konkoly Observatory, Budapest, Hungary % Use the following documentstyle definition : % \documentstyle[twoside, ibvs2, epsf]{article} % or % \documentstyle[twoside]{article} % \input ibvs2.sty % \input epsf.sty % epsf is only needed for figures % IBVS.STY screen message \ typeout {} \ typeout {IBVS.STY Ver. 2.31 - 02-05-2001 } \ typeout {Information Bulletin on Variable Stars - Konkoly Observatory} \ ...

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. Enter an expression . Result: .

14. http://site2010.sai.msu.ru/static/doc/RShomali_site2010.pdf

15. Observing Resources for Amateur Astronomers ? Part 3: Advanced Observers ?

16. Марсианское время

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