... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 1 Contents of the work A sample of H2O maser emission sources has been observed since 1980. ... Rudnitskij et al. ... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 4 Maser in a protoplanetary disc (S255) Flux density, Jy S255: H2O line profile 5 February 2002 Radial velocity, LSR, km/s Rudnitskij et al. ... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 12 ...

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... Purpose: The purpose of this program is to monitor the sensitivity, wavelength and detector calibrations of Side 2. Description: Four times per year (twice in Cycle 6) the following observations will be done: . ... SENSITIVITY MONITORING . ... Fraction of GO Programs Supported: All GHRS programs using gratings G160M (19%), G200M (7%), and G270M (15%). ... Observation: Internal-16 orbits (8 orbits for each of the 2 executions. Note: the internal orbits are full orbits). ...

... CI Cam is known to be a B[e] star and X-ray transient source. ... Figure 1. The light curve of CI Cam in residuals relative to the mean level of the slow variability (top) . The radial velocity curve of the HeII emission (middle) . ... The V light curve is shown in Figure 1 (top). ... Comparison of two CI Cam spectra in the region of HeII line. ... The radial velocity curve of HeII in CI Cam has a saw-tooth shape that may be an evidence of an elliptical orbit. ...

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... Torgashin Kotel'nilov Institute of Radio Engineering and Electronics, Russian Academy of Science, Mokhovaya 11, 125009, Moscow, Russia A Superconducting Integrated Receiver (SIR) [1, 2] was proposed more than 10 years ago and has since then been developed for practical applications [3]. ... In particular we have developed integrated receiver for novel balloon borne instrument TELIS (TErahertz and submillimeter LImb Sounder) [6, 7]. ... The SIR for TELIS covers frequency range 450 -650 GHz. ...

Reloading smiswww.iki.rssi.ru ...

... Fig.1 Left panel: GMRT map of integrated HI emission of XMD galaxy DDO 68 with angular resolution of 27"x22" (in greyscale) with superimposed contours of its optical B-band image from DSS-2. ... Top right panel: The same type of image, but for angular resolution of HI map of 17"x11". ... Top right panel: The integrated HI emission map with angular resolution of 8"x7" (greyscale) with superimposed contours of optical emission (smoothed to resolution of 7"). ...

... НЕПРЕРЫВНОГО МАТЕМАТИЧЕСКОГО ОБРАЗОВАНИЯ . ... Кружок ?Олимпиады и математика? ... Московская математическая олимпиада . Заочный математический конкурс . ... Устные математические олимпиады . Олимпиады по программированию . Математический праздник . Математические регаты . ... Математические бои . Олимпиада по геометрии им. И.Ф.Шарыгина . ... Программа ?Math in Moscow? Научные конкурсы . Творческий конкурс . ... График олимпиад . ... XXVII Математический праздник . ...

RF/Fiber Optic WDM Transceiver AC231W Features · 2000 MHz Bandwidth · 1.3 or 1.5 µm DFB Low Noise Laser · High Dynamic Range · WDM for bidirectional transmission · Internal Optical Isolator · Monitoring and Alarm Capability · Laser Disable · Singlemode Fiber Description The AC 231W is a linear, low noise RF fiber optic transceiver designed for fiber optic wireless systems and broadband RF applications. ... A laser and received optical power monitor and alarm is provided. ...

... Authors : V.V. Akimov , G.S.Bisnovatyi-Kogan , N.G. Leikov (Space Research Istitute, Moscow, Russia) . ... What differences CYGAM from traditional telescopes? Sky in the high-energy gamma-rays according to the data of SAS-2 (1972-1973), COS B (1975-1982), GAMMA 1 (1990-1992) and EGRET (1991-2000) . ... CYGAM characteristics according to results of Monte-Carlo simulations . What results may one expect after a year of CYGAM flight in the high apogee orbit? . ... Last updated on 10.06.03 ...

... 18-Jan-2010 16:45 . ... Muon_Telesc(hourly_values)/ . ... Muon_Telesc(minute_values)/ . ... Neutron_Monitors(daily_values)/ . ... Neutron_Monitors(hourly_values)/ . 15-Nov-2010 15:12 . Neutron_Monitors(minute_values)/ . ... Neutron_Monitors(monthly_values)/ . ...

. Astro Space Center . (Moscow Division) . Theoretical Astrophysics . QUAD : Quantum Astrophysics . Space Radio Astronomy . SED : Space Electronic . SCD : Space Constructions . ASMGSD : AstroSpace Missions Ground Support . RT-70 : Designe & Coordination RT-70 . DPD : Data Processing . INS_Lab : Information & Navigation Systems

... Field of interest: data analysis and interpretation of X-ray observations of BHC and NS systems, astrophysics of compact objects and related phenomena: X-ray , optical and radio observations , shocks and stellar winds, emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars ( signature of accreting BH), atoll- and Z-sources ( signature of accreting NS), modeling of INTEGRAL images % . ...

... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...

... You are here: start €Ё difx €Ё difx_monitor . ... difx:difx_monitor . ... Clients . ... To allow multiple clients to simultaneously receive this monitoring data, a monitor_server can be run which receives a copy of ALL visibilities and allows multiple clients to connect. The clients request which of the visibilities they require and monitor_server only sends on the products required (so e.g. a client can be run over a moderately slow link if it only requires a handful of products). ...

. annotation of talk . V.M.Malofeev, O.I.Malov (PRAO) . Detection of radioemission from Anomalous X-ray pulsar 1E2259+58 . We report on the discovery of pulsed radio emission with period 6.98 s from the first anomalous X-ray pulsar (AXP) 1E2259+586. The observations were made with the LPA FIAN in Pushchino at 111 MHz. The flux density about 70 mJy and the width of integrated pulse is close apon 120 ms. The dispersion measure is about 80 pc/cm 3 that gives the distance to pulsar 3.6 kpc.

... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...