ZSS 107 17:19:48 -41:18:14 new-HIZSS107 #FR Clipped rms: 0.0127 Jy #FN ( 41 out of 80 channels) #MC xaxis: optical #MX Maximum: 0.152 Jy at 3786.864 km/s #MN Minimum: - 0.027 Jy at 4111.852 km/s #NP Number of spectral points: 34 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 27.048 3898.770 94.667 Robust moments: 0 1 2 #MR 27.070 3887.686 81.464 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line ...

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 . ...

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. ...

... 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 . ...

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 | ...

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. ...

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 ...

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 . ...

... 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. ...

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 . ...

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 ...

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: . ...

... Telescope concept . ... The Submillimetron Project is dedicated to astronomical studies at the submillimeter and far infrared wavelengths using a cryogenic telescope located on the Russian segment of the International Space Station (ISS). The Astro Space Center of the Lebedev Institute of the Russian Academy of Sciences is responsible for developing the Submillimetron Project. ... Currently, the Astro Space Center is carrying out a pre-Project study under contract with the Russian Space Agency. ...

... The technology needed to implement a Distributed Astronomical Data Archive (DADA) is available today (e.g., Fullton 1993). Query interface standards are needed, however, before the DADA information will be discoverable. ... These parameters would be used to index each dataset in each catalog. ... The technology is available today to perform cross-catalog queries, to fetch the data at the click of a mouse, quickly to add new observation catalogs, and to distribute the load across multiple machines. ...

... The antenna system . ... A military radar system, consisting of two identical radars, was transferred to the Institute of Solar-Terrestrial Physics (ISTP). ... The system features a two-channel transmit-receive antenna. ... By changing the phase difference in the channels, one is able to modify the shape of the total channels' beam in the angle-of-elevation plane. ... The total beam is controlled by introducing the phase signal into the excitation signal of one of the channels. ... Peak power.. ...

Peremennye Zvezdy", . ... Type . Max . Min . ... type . ... USNO-A2.0 0900-17234449 . ... Comm. ... USNO-A2.0 0900-17238865 . ... USNO-A2.0 0900-17245476 . ... 2MASS 19582756+0454212 . ... Infrared colors J H = 0.654, H K = 0.132, J K = 0.786 (2MASS) are consistent with the K spectral type (Bessell and Brett 1988) and BY: classification. ... Infrared colors J H = 0.986, H K = 0.345, J K = 1.331 (2MASS) are consistent with the M spectral type (Bessell and Brett 1988) and SR classification. ...

... 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 . ...

... 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. ...

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 . ...

... 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. ...