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http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/13:37:30-39:52:56.measure.

1. http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/12:47:26-77:34:17.measure
new #FR Clipped rms: 0.0082 Jy #FN ( 31 out of 37 channels) #MC xaxis: optical #MX Maximum: 0.146 Jy at 416.000 km/s #MN Minimum: 0.002 Jy at 455.689 km/s #NP Number of spectral points: 6 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 4.692 413.964 11.804 Robust moments: 0 1 2 #MR 4.373 414.104 7.259 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line centre : 413.118 414.591 #MXW Line width : ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/12:47:26-77:34:17.measure -- 2.0 Кб -- 23.07.2007
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2. Arcetri Correlation Spectrometer
This instrument is a spectometer with . ... maximum resolution of 40 Hz (8.4 m/s at 1.4 GHz) . ... The control software has been developed using Object Oriented analysis and modelling techniques ( Arcetri report 3/98 ). ... n. 3/93: ARCOS - Arcetri Correlation Spectrometer: Clock Generation module . n. 13/93: ARCOS - Arcetri Correlation Spectrometer: Project status report . ... n. 3/98: Software Analysis for the Arcetri COrrelation Spectrometer . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/Radio/instr/arcos/arcos.html -- 3.5 Кб -- 02.10.2008
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3. Produce a spectral data set using the PROS task 'xray.xspectral.qpspec'
Next: Create an XSPEC compatible Up: PHA Distributions Previous: PHA Distributions . ... bkgd = "none" background qpoe file . ... table = "raysm" root name for output files [root_obs.tab, etc.] ... (detx = "chipx") type of binning . ... binning = "pha") type of binning . ... The relevant numbers are the T13 parameters (TLMIN13 and TLMAX13) in the header to the binary extension file (can be viewed with the ftools task 'fv' or by unix 'more' or 'less'). ... to produce the 'root_obs.tab' file. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node214.html -- 5.8 Кб -- 01.10.2012
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4. SPUTNIK home page
... 0,50-0,59 (0,50-0,59) µm . ... Swath Width . ... at end of visibilty area . ... Visibility Area Width . ... Ground Resoultion in Nadir: . along swath . ... across swath . ... Ground Resolution at End of Visibilty Area: . ... 200 lines per second . ... at least 200 . Ground resolution corresponds to normal flihgt altitude 650 km. For more information send a mail to: info@sputnik.infospace.ru . ...
[ Сохраненная копия ]  Ссылки http://sputnik.infospace.ru/resurs/engl/msue_e.htm -- 8.3 Кб -- 21.01.2002
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5. ASP: Star Science in the Autumn Sky
Once students get the hang of it, they can find and measure the brightness of Delta Cephei in a few minutes. ... of Delta Cephei . ... Oct. ... The following table lists the measurements of Delta Cephei made by one amateur astronomer in autumn 1990. ... 4.0 . ... This activity is a simplified version of one that appeared in Hands-On Astrophysics, a series of activities prepared by the American Association of Variable Star Observers with support from the National Science Foundation. << previous page | ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/32/starscience4.html -- 18.8 Кб -- 02.10.2012
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6. Optical static Fourier spectrometer
Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/~lapchuk/my_web/Spectrometer.htm -- 10.1 Кб -- 21.02.2000
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7. http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2002/Oal_IAU209.ps
Dopita, S. Kwok and R.S. Sutherland, eds. Di raction-limited speckle interferometry and modeling of the circumstellar envelope of R CrB at maximum and minimum light K. Ohnaka, T. Blocker, K.-H. Hofmann, N. R. Ikhsanov, G. Weigelt Max-Planck-Institut fur Radioastronomie, 53121 Bonn, Germany Y. Balega Special Astrophysical Observatory, Nizhnij Arkhyz, 35147, Russia V. I. Shenavrin, B. F. Yudin Sternberg Astronomical Institute, 119899 Moscow, Russia ...
[ Текст ]  Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2002/Oal_IAU209.ps -- 55.2 Кб -- 03.08.2004
[ Текст ]  Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/Oal_IAU209.ps -- 55.2 Кб -- 24.02.2010
[ Текст ]  Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2002/Oal_IAU209.ps -- 55.2 Кб -- 24.02.2010
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8. INTAS99.4
Image analysis of the VLBI experiment INTAS99.4 . PI: I. Molotov (GAO, Russia) . Analyst: A. Pushkarev (GAO, Russia; CrAO, Ukraine) . ... Frequency: 1.66 GHz . ... Antennas and their characteristics at 1.66 GHz . ... Bear Lakes (Russia) . ... Svetloe (Russia) . ... Pushchino (Russia) . ... CALIBRATION . Amplitude Calibration . Phase Calibration . ... 0420-014 . ... Quasar . ... 0420-014.gif . ... 0420+022 . ... 0420+022.gif . ... 0552+398 . ... 1308+326 . ... 1345+125 . ... 1803+784 . ...
[ Сохраненная копия ]  Ссылки http://astra.prao.psn.ru/Molotov/Webpage/intas99_en.html -- 9.3 Кб -- 06.04.2005
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9. Armagh Observatory
... Armagh Observatory, 5 January 2016: Armagh Observatory reports that December 2015 was much wetter than average, the wettest December on record at Armagh, that is, since records of daily precipitation began at Armagh in 1838. ... The month was slightly duller than average, with 15 of the 31 days having no recorded strong sunshine at all. ... The long-term (1838-2010) average December precipitation at Armagh is 77.44 mm and the most recent 30-year (1981-2010) average precipitation is 77.23 mm. ...