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http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/16:47:55-00:23:08.measure.

1. http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/16:39:41-56:52:35.measure
HIP 791 16:39:41 -56:52:35 new #FR Clipped rms: 0.0132 Jy #FN ( 42 out of 65 channels) #MC xaxis: optical #MX Maximum: 0.211 Jy at 1504.615 km/s #MN Minimum: -0.027 Jy at 1331.502 km/s #NP Number of spectral points: 19 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 18.902 1468.637 35.290 Robust moments: 0 1 2 #MR 18.454 1469.378 27.806 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line centre : 1468.024 1467.617 #MXW ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/multibeam/HIPASS-BGC/tables/measure/16:39:41-56:52:35.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. 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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4. comedi_get_maxdata
. Comedi Documentation . Prev . Next . comedi_get_maxdata -- maximum sample of channel . #include <comedilib.h> . lsampl_t comedi_get_maxdata (comedi_t * device, unsigned int subdevice, unsigned int channel); . The function comedi_get_maxdata() returns the maximum valid data value for channel chan of subdevice subdevice belonging to the comedi device device This function returns 0 on error. Prev . Home . Next . comedi_maxdata_is_chan_specific . Up . comedi_get_n_ranges
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/sts/linux/comedi/doc/func-ref-comedi-get-maxdata.html -- 3.8 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/sts/linux/comedi/doc/func-ref-comedi-get-maxdata.html -- 3.8 Кб -- 11.09.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/sts/linux/comedi/doc/func-ref-comedi-get-maxdata.html -- 3.8 Кб -- 02.10.2012
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5. 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. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/2016/Weather_Dec15_pr.html -- 10.9 Кб -- 14.01.2016
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6. 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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7. lsst.tcc: tcc::AxeLim Class Reference
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Classes . Files . ... tcc::AxeLim Class Reference . include < axeLim.h > . std::tr1::array < double, 3 >љ . ... Note: AxeLim uses separate arrays for position, velocity, etc. instead of containing a vector of AxisLim, so that the load/dump file format is backward compatible with the old TCC. ... std::tr1::array <double, 3> tcc::AxeLim::accel . ... std::tr1::array <double, 3> tcc::AxeLim::jerk . ... std::tr1::array <double, 3> tcc::AxeLim::maxPos . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/html/classtcc_1_1_axe_lim.html -- 16.9 Кб -- 14.09.2015
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8. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/prefs/README
A prefs.ccd file should be located in /usr/local/observatory/prefs on the computer to which the camera is attached. ... Parameters that will be read by prefs.ccd are -- ccd.frame_count_multi Sets the maximum number of frames in multi mode Default is 10 Minimum is 2 No maximum ccd. filter _max Sets the number of filters in the filter wheel Should be less than or equal to the number of slots available ccd. filter _01 to ccd. filter _10 Labels for each ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/prefs/README -- 1.9 Кб -- 29.11.2012
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9. Stellarium: varstar Struct Reference
Stellarium 0.12.3 . ... FileљStructure . ... varstar Struct Reference . QStringљ . ... Magnitude at maximum brightness. ... Magnitude flag code. ... First minimum magnitude or amplitude. ... Second minimum magnitude or amplitude. ... The photometric system for magnitudes. ... Definition at line 41 of file StarMgr.hpp . ... QString varstar::photosys . ... QString varstar::stype . ... QString varstar::vtype . ... The documentation for this struct was generated from the following file: . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/structvarstar.html -- 14.8 Кб -- 28.02.2014
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10. The AstroStat Slog Blog Archive A test for global maximum
... Archives . ... If getting the first derivative (score function) and the second derivative (empirical Fisher information) of a (pseudo) likelihood function is feasible and checking regularity conditions is viable, a test for global maximum (Li and Jiang, JASA, 1999, Vol. 94, pp. 847-854) seems to be a useful reference for verifying the best fit solution. I didn?t see any ways to confirm that best fit results from XSPEC or Sherpa are a global maximum without searching whole parameter space. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/a-test-for-global-maximum/index.html -- 23.2 Кб -- 01.03.2014
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11. Halloween and the Ghost Head Nebula
Astronomy Picture of the Day . ... 31.10.2010 . ... Since the fifth century BC, Halloween has been celebrated as a cross-quarter day , a day halfway between an equinox (equal day / equal night) and a solstice (minimum day / maximum night in the northern hemisphere). ... Similar to the icon of a fictional ghost , NGC 2080 is actually a star forming region in the Large Magellanic Cloud , a satellite galaxy of our own Milky Way Galaxy. ... Publications with keywords: Ghost Head Nebula - NGC 2080 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/apod/2010-10-31 -- 15.0 Кб -- 31.10.2010
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12. Plan and technical specifications of the Baikonur cosmodrome, Russia's space
... Space flight . ... Baikonur . ... Space camp . Space Hotel . ... On May 5, 1957 acceptance act of the first launch complex was signed, and as early as on May 6, 1957 the first "R-7" missile was erected on the site. The cosmodrome consists of nine launch complexes with fourteen launchers, thirty-four engineering complexes, three fuelling stations for space vehicles and two aerodromes. ... Services / Baikonur: General description Technical description Shedule of launches Photo gallery Price . ...
[ Сохраненная копия ]  Ссылки http://www.atlasaerospace.net/eng/baykonur-tech.htm -- 32.9 Кб -- 09.04.2016
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13. Server Pool Management
... The defaults for each variable are: MinSpareServers 5 MaxSpareServers 10 StartServers 5 There is an absolute maximum number of simultaneous children defined by a compile-time limit which defaults to 256 and a "MaxClients" directive which specifies the number of simultaneous children that will be allowed. ... If you need more than 256 simultaneous children, you need to modify both HARD_SERVER_LIMIT and MaxClients. In versions before 1.2, HARD_SERVER_LIMIT defaulted to 150. ...
[ Сохраненная копия ]  Ссылки http://neptun.sai.msu.su/manual/process-model.html -- 3.6 Кб -- 20.06.2002
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14. East Siberian Center for the Earth's Ionosphere Research. Maximum usable
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The on-line prediction procedure is based on the Newton interpolation formulae for a uniform distribution of the variable with first, second and third argument powers restrictions (Kurkin V.I. , Polekh N.M., Tchistyakova L.V. MAF operative prognosis for oblique ionosphere sounding// Issledovaniya po geomagnrtismu, aeronomii i phisike Solntsa. ... Prediction MUF calculation for the next 15 minutes; . ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/lchmen/op_proghen.htm -- 4.8 Кб -- 02.06.2001
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15. 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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16. Communications For Your Astronomy Event - an Astronomy Net Article
Communications For Your Astronomy Event . Articles | ... Some manufacturers have received approval to market radios that are certified for use in both the Family Radio Service (FRS) and the General Mobile Radio Service (GMRS). ... FRS radios have a maximum power of Ѕ watt (500 milliwatt) effective radiated power and integral (non-detachable) antennas. ... FRS and GMRS Channel 1 . ... The FRS/GMRS radios I have transmit more than 1/2 watt when on channels 1-7 and 15-22. ... www.astronomy.net . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/articles/28/frsgmrs.html -- 21.0 Кб -- 09.04.2016
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17. http://cgm.iszf.irk.ru/irkt/info.htm
... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...
[ Сохраненная копия ]  Ссылки http://cgm.iszf.irk.ru/irkt/info.htm -- 6.1 Кб -- 28.11.2002
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18. 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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19. Discovery Channel спонсирует постройку большого телескопа своего имени
... Сегодня: 10 апреля 2016 г. Компания Discovery Communications, которой принадлежит известный телевизионный канал познавательных программ Discovery Channel, стала спонсором разработки и строительства нового телескопа обсерватории Lowell в штате Аризона. ... Как было объявлено, основная миссия телескопа - это исследовательская работа и участие в научных программах NASA, Национального научного фонда и других подобных организаций. ... Шаттл Discovery стартовал . ...
[ Сохраненная копия ]  Ссылки http://news.cosmoport.com/2005/07/26/3.htm -- 22.7 Кб -- 10.04.2016
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20. GIRA - Two Channel Photometric Restoration
... We report on the status of a two channel photometric restoration technique and its current implementation as an IRAF task called GIRA. This method is particularly suited to stellar photometric measurements in crowded fields or in images where an extended structured background is present. ... One such method is a two channel photometric restoration method known as GIRA first conceived by one of us (L. B. Lucy) and which is under development at the ST-ECF (Pirzkal et al. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P2-55/ -- 16.8 Кб -- 11.10.2000
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