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Google doc v5.1 RadioAstron International Science Council Tsargrad Hotel (Boyarsky room) Breakfast starts at 8am Monday, June 18 ( Tsargrad hotel) 10:00 N. Kardashev: Welcome 10:15 K. Kellermann: Goals of meeting and approval of agenda 10:30 Introductions of members and guests 10:45 RISC Terms of Reference Supporting documents: RISC ToR draft 11:30 Break 12:00 M. Popov: SRT in-orbit tests and basic parameters 12:30 Y. Kovalev: Fringe Search: ...

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Mercury Spring 2010 Table of Contents . This artist s impression shows the transiting exoplanet Corot-9b. Credit: ESO / L. Cal ada. First Temperate Exoplanet . ... Combining observations from the CoRoT satellite and the ESO HARPS instrument, astronomers have discovered the first . ... Designated Corot-9b, the . ... If you enjoyed this excerpt from a feature article and would like to receive our quarterly Mercury magazine, we invite you to join the ASP and receive 4 issues a year. ...

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... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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... Sciences) - (01.03.02 - Astrophysics and Radioastronomy), Main Astronomical Observatory of Ukrainian National Academy of Sciences, Kyiv, Ukraine. ... Sciences) (01.03.03 - Geliophysics and Solar System Physics), Main Astronomical Observatory of Ukrainian National Academy of Sciences, Kyiv, Ukraine. ... 1977 - 1981 - Engineer, Main Astronomical Observatory, Ukrainian National Academy of Sciences, Kiev, Ukraine . ... Institute: Main Astronomical Observatory of Ukrainian National Academy of Sciences . ...

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... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...

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AstroScript program to calculate the equation of time = MST - RST} {Set the default values for the various quantities} set_ time _zone(0) set_daylight_saving(0) set_longitude(0,0,0) set_latitude(0,0,0) set_height(0) set_decimal_places(0) set_local_civil_ time (12,0,0) {Clear the screen and display the title in light grey on black} set_normal_text (7) display _title(The equation of time ) {Find the moment when the ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Radio telescope 's beam General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Radio telescope's beam . ...

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... 2, JUNE 2003 1039 Properties of a High-Tc dc SQUID Radiofrequency Amplifier Alexey S. Kalaboukhov, Michael A. Tarasov, Ants Lohmus, Zdravko G. Ivanov, and Oleg V. Snigirev Abstract--We present an experimental investigation of a radiofrequency amplifier based on a bicrystal high- dc SQUID designed for the frequency range 500­3000 MHz. ... Maximum power gain was found to be 16 dB at 520 MHz for a SQUID with 8 turn input coil. ... Digital Object Identifier 10.1109/TASC.2003.814145 T Fig. ...

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