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http://www.naic.edu/~phil/hardware/pdev/rmsVsMixergain_24apr08.html.

1. http://www.naic.edu/~phil/obsproblems/apr03PolBDrift/apr03sbc1PolBDrifts.html
... list of all files with drifts 15apr03 to 27may03 baseband mixer chassis was tested on the bench and the tubular lowpass filters (k&E) (100 mhz) after the mixer were causing the problem. ... 10apr03 shows drift of sbc1B with the outputs of the IF2 switched sbc1B, sbc2b. The drift remains in sbc1B so the problem is after this switch (in the correlator). 14apr03 The cables leaving the attenuator box in the correlator were switched (sbc1b and sbc2b). ... At sample 4600 i retightened the switched cables....
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/obsproblems/apr03PolBDrift/apr03sbc1PolBDrifts.html -- 11.1 Кб -- 29.06.2003
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2. Detection of Radio Transients and Variable Radio Sources Using the Archive Data
... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Zhelenkova/ -- 6.9 Кб -- 10.04.2016
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3. Monitoring of variable sources at 15 GHz
The Ryle Telescope was used for some years for monitoring variable sources (in addition to its role in source-surveys related to the Sunyaev-Zeldovitch studies). The instrument is now transformed into the "AMI large array": see the AMI pages for details. ... The rebuild took place between 2006 June and mid-2008; between these dates there is no useful data available. ... For some sources there are many plots, organised by date: . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~guy/ -- 3.6 Кб -- 24.02.2015
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4. ADASS 2002 Conference Proceedings
Next: Status of the BIMA Image Pipeline . ... We describe all the steps of the standard reduction including per pixel error propagation: Bias correction, treatment of bad pixels, flatfielding, and filtering of cosmic ray events. ... We build difference images via image convolution with a technique called OIS (optimal image subtraction, Alard & Lupton 1998), proceed with PSF-fitting, relative photometry on all pixels and finally apply an automatic detection of variable sources. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/P4-4/ -- 14.6 Кб -- 13.03.2003
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5. lsst.tcc: python/tcc/cmd/showInstrument.py Source File
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . ... cmd . showInstrument.py . ... 35 љ kwStrs.append( "Inst=%s; InstPos=%s; GCView=%s" % ( . ... 48 љ kwStrs.append( "IImScale=%0.4f, %0.4f; IImCtr=%0.2f, %0.2f; IImLim=%0.2f, %0.2f, %0.2f, %0.2f" % ( . ... 61 љ kwStrs.append( "GImScale=%0.4f, %0.4f; GImCtr=%0.2f, %0.2f; GImLim=%0.2f, %0.2f, %0.2f, %0.2f" % ( . ... 69 љ kwStrs.append( "GImScale=NaN, NaN; GImCtr=NaN, NaN; GImLim=NaN, NaN, NaN, NaN" ) . ... tcc.cmd.showFocus.showFocus . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/show_instrument_8py_source.html -- 23.7 Кб -- 14.09.2015
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6. casacore: casa/Logging/LogFilter.h Source File
... Files . ... casa . Logging . ... 00001 //# LogFilter.h: Filter LogMessages on message priority 00002 //# Copyright (C) 1996,2000,2003 00003 //# Associated Universities, Inc. ... 00108 LogMessage::Priority lowestPriority () const ; 00109 00110 private : 00111 LogMessage::Priority lowest_p ; 00112 }; 00113 00114 00115 inline LogMessage::Priority LogFilter::lowestPriority () const 00116 { 00117 return lowest_p ; 00118 } 00119 00120 00121 00122 } //# NAMESPACE CASA - END 00123 00124 #endif . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/LogFilter_8h_source.html -- 19.5 Кб -- 14.02.2011
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7. *imcnts* - Azimuthal profile of an extended source
Next: *imcnts* - Radial Profile Up: Radial Profiles and Projections Previous: *tabplot* - Displaying a . ... Input a spatially blocked and energy filtered image from above and use with the background determined from the broad-band background map. cl xray xr xspatial xs imcnts addbkg=no # Do not add the background error Source image file : xdata$snr.qp Source region descripter: c 503 513 50 p 503 513 0 360 n=10 # circular region centered on point ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node105.html -- 4.4 Кб -- 01.10.2012
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8. Database of Optical Constants -- Level: welcome
The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/JPDOC/ -- 10.8 Кб -- 19.11.2010
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9. di_eks
... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/len/di_eks_e.htm -- 16.9 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/len/di_eks_e.htm -- 16.9 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/len/di_eks_e.htm -- 16.9 Кб -- 24.02.2010
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10. Setting shell variables
To define a temporary value to a shell variable use the command: set variable_name = value . The value of this variable will remain set until you exit from this shell. The value of this variable is not exported to other C shells when they are invoked. To give a lasting value to a shell variable: . ... Use an editor to open your .cshrc ( .tcshrc ) file and add the line: set variable_name = value . ... This adds the value of the shell variable to your shell's present environment. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/environment/sh_var.html -- 2.5 Кб -- 17.01.1997
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11.