... Also the measured signals are affected by detector transients, altering the final results considerably. We present the design and the main features of a software package, developed in order to support the absolute calibration of the instrument. ... In case the fit is not successful, the average of the last 30% of the data is taken as the final signal. ... The two different symbols represent individual calibrations of the final background signals, using the first or the second FCS-signal. ...

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• Prototypical Operations Support Tools for NASA Interferometer Missions:
• Distribution of the OPUS Data Processing System
• ADASS 2003 Conference Proceedings

... Left: A POSSM plot of the uncalibrated spectrum of DA 193 at 1.66 GHz on a baseline Bear Lakes to Noto. ... The phase slope as a function of frequency is clear evidence for a small delay error in the correlator model. Right: The same data as shown on the left, but corrected for a delay error and a residual fringe rate. ... Left: A VPLOT plot of the uncalibrated amplitude (upper frame) and uncalibrated phase (lower frame) as a function of time for the source DA 193 on a baseline HartRAO to Noto. ...

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• INTAS99.4

COPRATES CHASMA NORTH WALL INTERIOR LAYERED DEPOSIT: LAYER MEASUREMENTS AND COMPARISON WITH JUVENTAE CHASMA ILDS USING MARS EXPRESS HIGH RESOLUTION STEREO CAMERA (HRSC) DERIVED TOPOGRAPHY Michael, G.1, E. Hauber1, K. Gwinner1, R. Stesky2 ... Planets, Freie Universitaet, Berlin, Germany 5ESTEC, ESA, Noordwijk, The Netherlands Introduction: The interior layered deposit ( ILD ) in the north wall of Coprates ... The lesser section of the ILD is confined by a ridge of the chasma wall. ...

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Next: Principal Areas of Research Up: annrep Previous: Contents Contents . The Armagh Observatory, founded in 1790 by Archbishop Richard Robinson, is a modern astronomical research institute with a rich heritage. ... Overall, around 25 astronomers of graduate or postdoctoral status are actively studying Stellar Astrophysics, the Sun, Solar System astronomy, and the Earth's climate. ... The Armagh Observatory participates in the UK Research Assessment Exercise, held in 1992, 1996 and again in 2001. ...

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. . (MPIfR/ ), . . ( /MPIfR), . . (MPIfR//), . . (MPIfR) . . (1.4-15.4 ) VLBA 20 - . . 20 . >1 ~1 <1 () () . ~1 (). >1 ~1 <1 >1 ~1 <1 (1>2) 1 2 =1 - . VLBA 20 . 9 : 1.4-15.4 . NRAO's Very Long Baseline Array (VLBA) Image courtesy of NRAO/AUI and Earth image courtesy of the SeaWiFS Project NASA/GSFC and ORBIMAGE VLBA Lobanov (1998 A&A, 330, 79), () , , k=1 k k=0.98 +/-0.11, k=1. k 0952+179 k=2.7 +/-1.7 k=0.98 +/-0.11, k=1. 20 . 9 1.4-15.4 VLBA. . : 1 mas 1.4 5.0 , 0.2 mas 5.0 15 . ().

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• http://hea.iki.rssi.ru/integral06/papers/J36_Wunderer03-23Feb07_03:04:03.pdf

Впечатление художника о молекулярном диске, окружающем предполагаемую черную дыру в ядре галактики NGC 4258. ... Геометрия и динамика диска были аккуратно определены из наблюдений на интерферометре Very Long Baseline Array (VLBA), NRAO, США. ... Reprinted from: Proceedings of the Natinal Academy of Sciences. Vol.92, Number 5, December 5, 1995, by the National Radio Astronomy Obervatory with the permission of National Academy of Sciences. ...

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. This is a new popup window - close it when you are done . Submitted by Paul Valleli on 01/16/2007 15:59:15 . 25 Meter Radio telescope . Down in the valley from McDonald Obs. is one 25 meter Radio telescope antenna of an array that stretches around the world for VLBI - very long baseline interferometer . Logon to post a follow-up comment or review comments from others . Copyright (c) Amateur Telescope Makers of Boston, Inc. About Us Contact Us

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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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... In this paper, results are presented on studies which have been performed to investigate the impact of the cut-off elevation angle and elevation-dependent weighting on the EOP estimates and baseline length repeatability. ... He tested his method with the actual CONT05 observations. ... This gave an impulse to the present work where some results are presented of investigation of the impact of the CEA and EDW on the baseline length repeatability (BLR) and Earth rotation parameters (EOP) estimates. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/skurikhina.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/soffel.pdf
• http://www.gao.spb.ru/english/publ-s/viii-rfs/p011.pdf

... After all we cannot send a probe to the star Altair to confirm that it is 17 light years away. ... The "Bessel determined that the star 61 Cygni was about ten light years away" Earth goes around the Sun in one year, so in six month it is in the opposite position in its orbit. ... In 1838 Bessel determined that the star 61 Cygni had a parallax of 0.314 arcseconds and therefore the star was about ten light years away (today the distance is more precisely measured to be 11.4 light years). ...

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Stellarium 0.12.3 . ... Plugins . ... FileљStructure . FileљList . FileљMembers . plugins . Satellites . src . gsatellite . sgp4unit.h . ... 7 љ * this file contains the sgp4 procedures for analytical propagation . 8 љ * of a satellite. the code was originally released in the 1980 and 1986 . ... Generated on Sat Aug 10 2013 17:12:43 for Stellarium by љ 1.8.3.1 ...

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• Stellarium: gSatWrapper Class Reference

... Also the measured signals are a#ected by detector transients, altering the final results considerably. ... The sequence is bounded by two measurements of the FCS , to fix the responsivity for the baseline correction 0 200 400 600 800 1000 measurement time [s] 0.00 0.02 0.04 0.06 0.08 0.10 Volt/second bg source fitted baseline 2. FCS 1. FCS source initial drifting signal corrected signal bg FCS source background signal internal calibration signal source signal corrected ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/rosej.ps.gz

NIST Spetial Publication 500-220 . Guide on Open System Environment (OSE) Procurements . ... An Open System Environment encompasses the functionality needed to provide interoperability, portability, and scalability of computerized applications across networks of heterogeneous, multi-vendor hardware/software/communications platforms. ... The Open System Environment concept has become ubiquitous throughout both the public and private sectors. ... ACQUIRING AN OPEN SYSTEM ENVIRONMENT 11 . ...

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... Bad Astronomy . ... Mad Science . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... The name "parsec" is indeed a distance of 3.26 light years. ... First off, we need to know about "parallax". ... A great example is easy to show: hold a thumb up in front of your face, about 20 centimeters away. ... That angle is called the parallax angle, and it depends on two things: how far apart your eyes are (the baseline ), and how far away your thumb is. ... 2008 Phil Plait. ...

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Permitted Context: %math . ... This is represented in HTML math by: <array> <row><item>a_11_<item>a_12_<item> <item>a_1n_ <row><item> <item> <item> <item> <row><item>a_n1_<item>a_n2_<item> <item>a_nn_ </array> . ... This is represented by: <array coldef="C+C+C+C=C"> <row><item>a_11_x_1_<item>a_12_x_2_<item> <item>a_1n_x_n_<item>b_1_ <row><item>a_21_x_1_<item>a_22_x_2_<item> <item>a_2n_x_n_<item>b_2_ <row><item colspan=5> <row><item>a_n1_x_1_<item>a_n2_x_2_<item> <item>a_nn_x_n_<item>b_n_ </array> . ...

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• Table Rows

... xntpd is an operating system daemon which sets and maintains the system time-of-day in synchronism with Internet standard time servers. xntpd is a complete implementation of the Network Time Protocol (NTP) version 3, as defined by RFC-1305, but also retains compatibility with version 1 and 2 servers as defined by RFC- 1059 and RFC-1119, respectively. xntpd does all computations in 64-bit fixed point arithmetic and requires no floating point support. ... Specify the name and path of the log file. ...

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• FTS Parser Example
• Zen: tsearchd
• Configuration Options

Quantum Painleve-Calogero Correspondence A. Zabrodin Moscow, September 20, 2011 (Based on joint work with A. Zotov) Painleve equations Compatibility of linear problems Zero curvature condition is equivalent to Painleve equation Example (Painleve I) Hamiltonian structure There is a time-dependent Hamiltonian H(p, q; T) such that Painleve equation is equivalent to H(p, q; T) is a polynomial in p,q (K.Okamoto) Painleve-Calogero correspondence (P.Painleve, 1906; Yu. ...

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... XPS D450 Dell / Dimension XPS R400 Dell / Dimension XPS R450 Dell / Dimension XPS T550 Dell / Dimension 4100 NEW I Processor Type Pentium III Pentium II Pentium III Pentium II Pentium III Pentium II Pentium II Pentium II Pentium II Pentium III Pentium III Core Logic Chipset 820 440LX 440BX 440FX 820 440LX 440BX 440BX 440BX 440BX 815E 850i 440BX ... 04/10/2001 CUSL2 BIOS version 1002. ... III. ...

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• Power GrabberTM

Grace project file # @version 50120 @page size 792, 612 @page scroll 5% @page inout 5% @link page off @ map font 0 to Times-Roman , Times-Roman @ map font 1 to Times-Italic , Times-Italic @ map font 2 to Times-Bold , Times-Bold @ map font 3 to Times-BoldItalic , Times-BoldItalic @ map font 4 to Helvetica , Helvetica @ ...

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• http://www.astro.louisville.edu/software/alsvid/alsvid-current/src/INSTALL
• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.1/TODO
• http://www.astro.louisville.edu/shared_skies/archive/select/messier/m4/20070402/magi_magv.agr

... Issue 7 -- Short Contributions AG 2005 Kln 1 Infrared Interferometry of the Seyfert Galaxy NGC 1068 G. WEIGELT 1 , Y. Y. BALEGA 2 , T. BECKERT 1 , W. J. DUSCHL 3 , K.­H. HOFMANN 1 , A. B. MEN'SHCHIKOV 4 , D. SCHERTL 1 , M. WITTKOWSKI 5 1 Max­Planck Institut fr Radioastronomie, Auf dem Hgel 69, 53121 Bonn, Germany 2 Special Astrophysical Observatory, Nizhnij Arkhyz, Zelenchuk region, Karachai­Cherkesia 357147, Russia 3 Institut fr Theoretische Astrophysik, Universitt Heidelberg, Albert­Ueberle­Str. ...

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