... In the following table we list only the best results for each GPU: GPU b oard ATI 7950 3GB ATI 6950 1GB ATI 7770 1GB CPU Intel Core i5-2400 AMD Athlon II X4 630 Intel CoreDuo Quad CPU Q6600 Driver version 12.6 11.6 12.6 B uffe r numbe 32K 32K 32K 32K 32K 32K lenght and r of buffers B в 512 B в 512 B в 256 B в 512 B в 128 B в 512 M a x S p eed MSample/s 225MS/s Double 370MS/s Single 200MS/s Double 310MS/s Single 60MS/s Double 160MS/s Single Figure 1: SpectralGpu Logo Version 1.0, November 2012. ...

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• Digital backends

The capability to use the WAPPs in dual board mode for single pixel receivers was added in CIMA version 2.3 with first observations performed on 1 April 2007. This is the mode when the two boards of each WAPP are used as independent spectrometers allowing each WAPP to cover up to 200 MHz bandwidth. ... If You select to use dual board mode, all enabled WAPPs will be running in dual board mode. ... When using dual board mode, both boards on the same WAPP will use the same bandwidth. ...

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• tiedowns
• testing radar dataking 31oct13
• pdev_birdies_25jun07

Next: *evalvg* - Generate Time Up: QPOE Utilities Previous: *qplintran* Apply . Read a list of input qpoe files (including filters) and produce an appended output qpoe file. ... Any type of filtering can be applied to the input qpoe file, including region filtering. ... cl> xray xr> xdataio xp> page merge.lst # an ascii file listing the two input qp files xdata$rp110590.qp[time=(1606720.00:1607484.00)] xdata$rp110590.qp[time=(1611613.00:1612817.00)] xp> qpappend @merge.lst ``'' merge.qp large . ...

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• *fold* - Make a folded light curve
• *qplintran* -- Apply linear transformation to a qp file through filter
• *qpshift* -- Shift qp file by an offset in x and y

... The COMBINE/CCD command offers the possibility to combine a number of input images using different combining methods. COMBINE/CCD takes three input parameters at maximum: the exposure type of the images to be combined, the input frames themselves and and output frame. ... In the case of DO input (association) table, from the name of the output calibration frame in the table the command extracts the names of all requested single calibration frames and combines these frames in the output frame. ...

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• Entry points
• Structure of Tables
• Input/Output Redirection in Midas

... Image Area Store Area 240x120 24µm Gain Registers OP 8 Gain Registers Store Area OP 7 240x120 24µm Gain Registers OP 6 OP 1 OP 5 16 July 2008 Javier Reyes The design challenges des ges · Very fast read-out speed: up to 1500 fps speed: up to · Very low read-out noise. read-out ­ Effective ... · Very stable high-voltage clocks high-voltage · Low power consumption power consumption · Reduce volume: 19 x 23.5 x 7.5 cm 16 July 2008 Javier ...

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• http://www.eso.org/projects/www.eso.org.projects.ngc/General/16072008-lmehrgan.pdf

Next: Some Alternative Non-Linear Methods Up: Combining Mosaics and Single Previous: The Linear Method - . ... The non-linear combination uses the task mosmem (and the maximum entropy principle) to perform a joint deconvolution of the mosaic and single-dish images. ... Usage of mosmem is similar to that in Section 21.6 , expect that there are now two parameter values for the map , beam , rmsfac and q keywords, with these corresponding to the mosaic and single-dish values (in that order). ... MOSMEM . ...

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• Some Theory and Preparing the Single-Dish Data
• Input Parameters to the Self-Calibration Tasks
• immerge

... The algorithm has been successfully applied to both real and simulated astronomical data (Jefferies , 1993; Jefferies 1993) and its ability to accurately preserve photometry in the observed image has been demonstrated. ... In order to investigate the algorithm's performance without the influence of detector and photon noise we took the ``truth'' data set and convolved it with the given PSF to generate a noiseless image. ... The restored object and the two restored PSF's are shown in Fig. ...

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• Python: module code
• GOODS/ACS Mosaics for CDF-S and HDF-N GOODS: The Great Observatories Origins
• WFC3 Data Handbook

On this page you can compute thermodynamics, opacity and nuclear reaction rates for conditions which exist inside the Sun. ... Logarithmic partial derivative dlogP/dlogT (hi_t) . Logarithmic partial derivative dlogP/dlogRHO (hi_rho) . Logarithmic partial derivative dlogP/dlogX (hi_x) . Logarithmic partial derivative dlogU/dlogT (ksi_t) . ... Input field size does not limit the amount of data entered; you can type or paste thousands of lines (10,000 lines tested with output size over 5MB). ...

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• Equation of state for solar modeling

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... yes . ... If weightstyle =`gti', the task attempts to obtain a list of Good Time Intervals (GTIs), the exact way these are supplied being dictated via the parameter gtistyle ; these GTIs are ANDed with the attitude time bins; the net GTI in each bin provides the weight. gtistyle . ... If gtistyle =`user', the task obtains a single, simple GTI for all chip images from the parameters tstart and tstop . ...

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• Input Files
• Input
• Index

Flexible frame grabbing to PC over PCI bus from area & line scan cameras . ... Analog input up to 20 MHz and digital input up to 32 Mbytes/Sec. ... The LPG-132 will easily interface to virtually any analog or digital camera and provides lightning fast PCI transfers at an amazingly attractive price. The LPG-132 will interface with any camera or sensor at data rates up to 32 Mbytes/Sec. ... The LPG-132 comes in two configurations - one for analog input and the other for digital inputs. ...

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• FPG Power Grabber

Comedi Documentation . ... I assume that your hardware device is in your computer, and that you know the relevant details about it, i.e., what kind of card it is, the I/O base, the IRQ, jumper settings related to input ranges, etc. To tell the comedi kernel module that you have a particular device, and some information about it, you will be running the comedi_config command. ... The overall info gives information about the device -- basically the same information as /proc/comedi. ...

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• Linux PCI-HOWTO: General tips for PCI-Motherboard + Linux NCR PCI SCSI
• Arrays and Strings
• Application-specific functions

To read standard input into a shell script use the read command. For example: echo "Please enter your name:" read name echo "Welcome to Edinburgh $name" . This prompts the user for input, assigns this to the variable name and then displays the value of this variable to standard output . ... For example: echo "Please enter your surname\n" echo "followed by your first name: \c" read name1 name2 echo "Welcome to Glasgow $name2 $name1" . ...

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• Redirecting standard input and output
• Redirecting standard input
• Fill-Out Forms

L1 Simulation Upgrade December 6th, 2004 BaBar Collaboration Meeting SLAC Eric Torrence University of Oregon Eric Torrence 1/15 December 2004 Phase 0 (Now) DchDigis EmcDigis EmtSim trgDC L1Accept This IS the current SP6 (14.4.X) Base simulation code unchanged, but interface elements are updated (Digis, TsfLUT) Remaining changes are inside black blob Eric Torrence 2/15 December ... Done · L1DZpdTrackDigi - cellLocation and cellPhi are not currently being simulated. ...

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• Energy From the Oceans
• Lecture XVII.

... Previous: Calibration with the ISOPHOT Interactive Analysis (PIA) . ... This article is devoted to a description of the image processing capabilities of PIA, on the basis of the different mapping strategies with ISOPHOT. ... As input for mapping processing, PIA uses ISOPHOT data which has been reduced to the level of sky brightness (in MJy/sr) for each raster (and chopper) step and per detector pixel, together with the associated pointing information per raster point. ...

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• An Automatic Astronomical Classifier Based on Topological Neural Networks
• The IDL Wavelet Workbench
• On the Need for Input Data Control in Pipeline Reductions

... В разделе По форуму . ... На форуме начался конкурс - Астрофотография месяца: АПРЕЛЬ! ... Форум . ... Дополнительные форумы ? Горизонты науки о Вселенной (Модераторы: Дмитрий Вибе , AlAn ) . Обсуждаем проблемы современной астрономии, астрофизики и смежных наук. ... Тема / Автор . Ответов / Просмотров . Последний ответ . ... Автор Дмитрий Вибе . 16 Ответов . 418 Просмотров . ... Автор Сергей Попов ? ... 5 102 Просмотров . ... О разделе Горизонты науки о Вселенной. ... Автор Ах . ...

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• Часто Задаваемые Вопросы (ЧАВО или FAQ) - стр. 1 - Практическая астрономия
• Астрофотография - стр. 1 - Практическая астрономия
• Астрономические наблюдения - стр. 1 - Практическая астрономия

Next: Correlator Products . Previous: RSOG Post-Observation Products . ... Merged Correlator Input Log . Calibration and Flag files . SRT Amplitude Calibration Data . ... Phase Calibration (PCal) Data . ... DPC to Correlators . What: The RSOG produces the `merged' correlator input log file based on the Data Processing Logs supplied by the GTSs and on Executed Sequence of Events supplied by GOCG to produce a single correlator input log for all the GTSs for each observation. ...

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Hide Zen home . ... Index . ... Do we really need them for database indexing ? ... We need simple numbering scheme, so that for any given point we could easily calculate the number of "pixel", this is what HealPix provides and lacks HTM. ... During Rtree queries the number of index blocks read is several times greater than during Q3C queries. ... But in Q3C scheme, as we showed before, the circle is segmented, so we extract from the database only a few percents more data than occur in the circle. ...

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• Zen: LoadingSDSS
• APOD: June 11, 1998 - SOHOs Twin Sungrazers
• APOD: July 16, 1998 - X Ray Triple Jet

... While Sfit accepts input from "stdio", it is more natural to save/edit commands in a file (eg "solve_input.sfit") and run the code simply by entering > Sfit solve_input.sfit [linelist] . ... The model grid (3.4MB) produced by Example 1 and a selection of input spectra ( f008 f036 f068 f304 f354 ), together with SFIT output files are also given in this folder . ... The model grid (2.8MB) produced by Example 3 and an input spectrum together with SFIT output files are also given in this folder . ...

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• Influence of Climate Variables on Tree-Ring Widths of Different Species
• Spectrum v1 - Input Syntax
• Spectrum v1 - Examples

OptInt PmWiki : Pm Wiki / Forms . ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...

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• OptInt PmWiki : MROIDelayLineSW / VME
• OptInt PmWiki : Forms
• Bojan Nikolic -- Input format for Out-Of-Focus (OOF) holography software

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

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• AI SPbU library of scattering codes
• Model realization and some results
• Database of Optical Constants -- Level: welcome