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http://www.arcetri.astro.it/irlab/instr/spectralgpu/doc/spegpu_progress_1.pdf.

1. http://www.arcetri.astro.it/irlab/instr/spectralgpu/doc/spegpu_summary.pdf
... 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. ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/instr/spectralgpu/doc/spegpu_summary.pdf -- 53.6 Кб -- 16.11.2012
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2. WAPP Dual Board Mode
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. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~cima/cima_dual_board.html -- 6.0 Кб -- 01.03.2012
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3. *qpappend* -- Append a list of input qpoes to produce a single qpoe file
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 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node53.html -- 6.2 Кб -- 01.10.2012
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4. Input and Output
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node44.html -- 5.9 Кб -- 23.02.1996
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5. http://www.eso.org/projects/www.eso.org.projects.ngc/General/16072008-jreyes.pdf
... 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 ...
[ Текст ]  Ссылки http://www.eso.org/projects/www.eso.org.projects.ngc/General/16072008-jreyes.pdf -- 2808.3 Кб -- 20.07.2008
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6. The Non-Linear Method - MOSMEM
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 . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node195.html -- 12.2 Кб -- 10.04.2016
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7. Application to Simulated Data
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/christouj.dir/section3_2.html -- 6.6 Кб -- 18.04.1994
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8. Solar modeling input physics (thermodynamics, opacity, nuclear reactions)
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). ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/physics/phys.php -- 6.3 Кб -- 01.10.2012
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