S AO's New Generation Multipurpose CCD Controller . ... In the 1990?s considerable advances have been made in the world over technology of manufacturing scientific image detectors with high photoelectric characteristics, which called for the creation of new complex array controllers to operate such detectors. ... very low readout noise; . ... Quite a few teams of researchers and engineers are ingaged in the development of controllers. ... development, SPICE modelling and design of modules; . ...

... The mirrorCtrl mirror controller actor controls one telescope mirror. It accepts desired orientation and commands mirror motion accordingly. ... It is presently designed to command a Galil mirror controller , but one may add support for other low-level motion controllers. mirrorCtrl is written pure Python. ... Home the desired actuators, where actuator list is a comma-separated list of actuator letters A through F (but some mirrors have fewer than 6 actuators). 2.5m M1 valid actuators: A-F . ...

... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...

... The fitting package in STSDAS (Space Telescope Science Data Analysis System) relies on two basic techniques (one linear and one non-linear) for fitting functions to data. ... Results show that both methods may generate biased coefficients (at the ~few percent level), and over or under-estimate error bars (at the ~10 percent level), in particular from low signal-to-noise data. ... Function coefficient errors are computed directly from the covariance matrix. ... Abscissa is signal-to-noise. ...

Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

Random numbers ­ a note · How can a computer generate a "random" number? ... Maximal sequence length is m 30/10/2007 Computational Physics 2007 Distributions · Basic generator is uniform on [0,m]. ... 30/10/2007 Computational Physics 2007 Generators · Many random number generators: ­ f95 intrinsic functions · call random_number (harvest) . ... 30/10/2007 Computational Physics 2007 How "random"? ... 30/10/2007 Computational Physics 2007 About software How can it go wrong? ...

. Next: Generation from In-Orbit Data Up: EPN_ADUCONV Previous: Description Contents . Ground calibration data obtained from extensive measurements of X-ray emission lines and synchrotron lines (mainly flat fields). The gains of the individual readout nodes are derived by comparing the positions of the CTE corrected calibration lines (in ADU) with their energies. Michael Smith 2011-09-20

... An explanation of the general VLT control system architecture is given. Two generations of ESO VLT CCD Controller systems (ACE and FIERA) are described, and a comparison between them is presented, considering both the architecture and the performances. 1) The ESO VLT Control System . ... two . ... To achieve the readout requirements of the new generation CCD devices the LCU was replaced with a SPARC CPU, connected to the CCD Electronics through a 150 MBytes/sec full duplex optical fiber link. ...

Next: Time Series Analysis Up: No Title Previous: Command Syntax Summary . This manual is intended as a guide to the use of the digital stellar photometry reduction program DAOPHOT II: The Next Generation. ... In DAOPHOT II: The Next Generation all of the major algorithms and actual FORTRAN coding are done by Stetson, with the exception of those Figaro, IRAF, or MIDAS routines which are used for the image input and output. Stetson is solely responsible for bugs and algorithm-related problems. ...

... user-defined data file formats . ... better integration with a user's analysis routines To add such functionality to SAOimage, we developed the XPA Messaging System that allows X programs to define points of public access through which data and commands can be exchanged with external programs. ... We have utilized XPA to develop "SAOimage: The Next Generation" (SAOtng), an extensible image display service that can cooperate with other processes and programs. ... SAOtng help pages . ...

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. ...

... ATNF Home . About ATNF . ... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Our people overview . ... Publications overview . ... ATNF facilities . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Images . ... The MAPPIT (Masked APerture Plane Interference Telescope) instrument has been used for NRM observations at the 3.9m Anglo-Australian Telescope. ...

... Energetic magnetospheric ions are often unstable to the electromagnetic ion cyclotron (EMIC) instability . ... generation of EMIC waves below the proton gyrofrequency , and . ... Depending on the local proton gyrofrequency, the frequency of the EMIC waves varies: in the magnetosphere we deal with the ULF range (more precisely 0.1-5 Hz), while in the auroral field lines we have ELF waves (tens or hundreds of Hz; see radio frequencies and flickering aurora ). ... Space Physics Text Book of Oulu ...

... Meade Instruments Corporation . ... Autostar Computer Controller Instruction Manual . Autostar Computer Controller . ... NOTE: This manual covers both Model #495 Autostar and #497 ETX Autostar Computer Controllers. ... Autostar Primary Menus and Options . ... Chapter 3: Alignment . ... Guided Tour Menu . ... Chapter 5: Autostar Menu Functions . ... Meade Autostar Computer Controller . ... Meade #505 Connector Cable Set Manual . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...

... 10003 REM **BEGIN CONFIG** 10004 REM <MAP>configuration</MAP><REM>Saved Configuration.< ... ENC 0 /ENC DAC 0 /DAC STEP 0 /STEP DAC2 0 /DAC2 STEP2 0 /STE 10006 REM P2 ALG 0 /ALG ALGMODE 0 /ALGMODE IOMODE 0 /IOMODE EXIO 0 /EXIO ENCEX ... 10010 REM 0?0?0?0?0?0?< ... NAME_A /ACRMAPPING ACRAXIS SIGTYPE 7 /SIGTYPE STEPMODE 0 /STEPMODE SIGNDX 0 10011 REM /SIGNDX TAG_DRIVE Aries EPL /TAG_DRIVE TAG_DRIVERES 8000 /TAG_DRIVERES TAG_DACGAIN 3276 REM> 11000 REM **END CONFIG** ...

... Автокресло F 1000 K синее Sparco - универсальная модель для детей от 9 месяцев до 12 лет. ... Цвет: Синий, Черный . ... Цвет: разноцветный . ... Размер FR: 86 . Пол: Женский . Леггинсы Z Generation. ... Артикул: HC34EFRX35 Цвет: черный Состав: 100% кожа натуральная Размеры: высота 27 см, ширина 26 см, глубина 3 см, длина съемного ремешка регулируется Особенности: внутри - одно основное отделение Страна дизайна: США Страна производства: Китай . ... Материал верха: искусственная кожа . ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... This will include: efficient polarized and unpolarized spectrum synthesis; critical compilations of atomic data; determination of fundamental physical parameters; quantitative spectroscopy for abundance determination; magnetic field detection and modelling. ... Evelyne Alecian (Royal Military College of Canada) . ... Abundance analysis in magnetic and non magnetic stars (part I) . ... COFFEE BREAK . ... Herbig Ae/Be stars ....

Analysis of general features of the chaotic system behavior and investigation of the properties of concrete chaotic sources. ... Analysis of information properties of chaotic systems and chaotic oscillations as concrete objects for information processing and comunications. ... This hypothesis gives a possibility of designing simple mathematical structures accomplishing various processes of information processing using chaos. ... Activities | ... E-mail: chaos@mail.cplire.ru ...

... Radiative Transfer & Galaxy modelling . 09:30- 10:00 Nick Kylafis - Radiative transfer in spiral galaxies . ... 10:30- 11:00 Coffee break . ... 12:00- 12:30 Angelos Misiriotis - Dust in near-by edge-on spiral galaxies from the 2MASS Large Galaxy Atlas. ... for the Study of Gas and Dust in Galaxies . ... 15:00- 15:30 Leslie Hunt - Bulges and disks in spiral galaxies: clues for secular evolution? ... 09:00- 09:30 Edvige Corbelli - Dust and gas as tracers of star formation in M33 . ...