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1. Python: module build_PRD_dataset
build_PRD_dataset (version 4/16/04) . ... o Modified 8/28/03 KWC - Create work directory, renamed . ... to build_prd_files. o Modified 1/28/04 KWC - Add support for a list of files in a pickle. o Modified 2/ 3/04 RSK - Add support for user change directory. o Modified 3/12/04 RSK - Add processing for differencing output with . ... o Modified 4/ 1/04 KWC - Fix definition of new_user_file_dict, make . file differencing an option. o Modified 4/16/04 KWC - Use new prd_file_data, difference_PRD_files . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/spst/UnixTransition/doc/build_PRD_dataset.html -- 11.5 Кб -- 08.04.2016
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2. VLBI Wiki | TidNotes / FilePrep
... Go to new wiki . ... TidNotes / . ... define ifds 06132201809x ifd=,,nor,nor lo=lo1,1380,usb,lcp,1.0,0 patch=lo1,1h,2h,3h,4h,5h,6h,7h,8h,9h,10h,11h,12h,13h,14h enddef define vclba 06132201825x vc01=285.99,16.00,ul vc02=285.99,16.00,ul vc03=285.99,16.00,ul vc04=285.99,16.00,ul vc05=285.99,16.00,ul vc06=285.99,16.00,ul vc07=285.99,16.00,ul vc08=285.99,16.00,ul vc09=285.99,16.00,ul vc10=285.99,16.00,ul vc11=285.99,16.00,ul vc12=285.99,16.00,ul vc13=285.99,16.00,ul vc14=285.99,16.00,ul . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/vlbi/wiki/index.php?n=TidNotes.FilePrep -- 11.9 Кб -- 12.04.2016
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3. Change history
... September 17,2008 New parameter (removescatteredlight) is introduced to enable removing scattered light features by the task omgprep . May, 01, 2008 Modified the call to omgrism plot in order to produce the PostScript file with spectra extraction regions plotted over the grism rotated image. ... July 15, 2004: V1.0.7 Default options for the spectra extraction region are changed from 3 to 6 pixels to avoid the possibility of missing some of the spectra (SPR-3355) . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omgchain/node2.html -- 7.0 Кб -- 22.10.2008
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4. pulsedPwrIntoAlfa
... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/mbeam/biasChange_sep08.html -- 5.6 Кб -- 22.09.2008
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5. Extended IDL Help
This page was created by the IDL library routine mk_html_help . ... mk_html_help . at the IDL command line prompt. ... to calculate CHIANTI line intensities and continua, to create a synthetic spectrum. ... WRITTEN : Ver.1, 7-Nov-01, Giulio Del Zanna (GDZ) and Peter Young (PRY) MODIFICATION HISTORY: V.2, 7-Nov-01, GDZ . Fixed a small bug (now the spectrum plot is always plotted within the widget), and modified the option to add continua. ... Added extended details in the ascii output spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/chianti/chianti_5.1/list_headers.html -- 26.9 Кб -- 15.09.2005