RFI Test - NETGEAR GSM7328FS Luis Quintero, Arecib o Observatory 17 Oct 2012 1 Intro duction This document shows RFI test (electric field only) info and results for the NETGEAR ProSafe GSM7328FS (see Fig. ... The red labels in the picture show the positions of two test points (1. front panel close to the cable and fiber transceiver, 2. close to the 120VAC power cable). ... 1] ETS LINDGREN, ETS Near-Field Probe Set Model 7405. ... Electric field test only. ... Figure 3: Electric Field Test Results. ...

... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...

. English . Russian KOI8 . Current server sed.sao.ru . Dissertation of Doctor of Sciences degree ( close to German Habilitation ) . A time to cast away stones, . and a time to gather stones together . Ecclesiastes, Ch. 3 ; 5 . Full gzipped PostScript version (in Russian) is here (2005), autoreferat (short thesis in Russian) is here . Main results of dissertation work . Continue...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Many of the fields are spatially . ... These include a pulsating white dwarf which appears to have a hot companion, a number of stars with A-type spectra that vary on a period in the range 20 35 min. Our primary goal is the discovery of new AM CVn systems: we find 66 sources which appear to show periodic modulation on a time-scales less than 40 min and a colour consistent with the known AM CVn systems. ...

pn Filter Wheel Closed Data . ... XMM-Newton SOC Home Page Conferences & Meetings . ... Data Analysis SAS News What is SAS? ... The following links contain pages to the merged Filter Wheel Closed event lists corresponding to the different EPIC-pn modes. ... Fast Modes . ... Burst Mode (BU) Below you can find relevant reports and proceedings about EPIC-pn Filter Wheel Closed exposures, such as spatial, temporal, and spectral properties of the internal background. ... EPIC-pn: background calibration . ...

... In Fig. 2 the spectrum of the host galaxy HS1035+4758 is shown, in which typical HII-galaxy narrow emission lines are seen: H 4861, [OIII] 4959,5007, H 6562, [NII] 6548,6584 and [SII] 6716,6731 ?. ... The spectral evolution of SN 1998bv is illustrated in Fig. ... The change of the spectrum between April 6 and 19 with clear reddening shortward of H during these 2 weeks indicates seemingly that the 1st spectrum was observed in the period between the 20th and 30th days after the peak of the light curve...

... astro-ph . ... Adams, F. C.. ... Allen, Paul D.. ... Bieging, John H.. ... Boss, Alan P.. ... Burgasser, Adam J.. Burrows, Adam. ... Butler, R. Paul. ... Cushing, Michael C.. ... Day-Jones, A. C.. ... Green, Richard F.. ... Hartung, Markus. ... Janson, Markus. ... Jones, Damien. Jones, H. R. A.. ... Kasper, Markus. Kelley, Michael S.. ... Kraus, Adam L.. ... Marley, Mark S.. ... Mathar, Richard J.. ... McCaughrean, Mark J.. McElwain, Michael. ... Monnier, John D.. ... Sosa, Richard G.. ...

... All the ELT pro jects present a segmented primary mirror. ... In 2001 Esposito [3] proposed the PWFS as phasing sensor for segmented mirrors, demonstrating, with numerical simulations, that the sensor can sense and control at the same time differential piston, tip and tilt of each segment. ... A new co-phasing loop has been arranged with the PWFS and the segmented mirror of NAOMI [6] (the AO system located at the telescope nasmith platform). ...

. The SiO (2-1) spectra of N6334 I(N) displayed below (off-source position plus 7-point mosaic) have been obtained in July, 2001, with the one baseline (CA03-CA04: 30m, 2 polarisations) 3mm prototype system of the Australia Telescope Compact Array . The SiO (2-1) rest frequency is 86.847 GHz. Uncalibrated SiO (2-1) emission spectra of N6334 I(N). Fields are: off-source (top left), W, NW, SW, center, NE, SE, E (bottom right). 15-07-2001 * B?rbel Koribalski

HI Distribution in the Region . of the Supernova Remnant G78.2+2.1 ( 2001 ). ... Based on RATAN-600 21 cm line observations with an angular resolution of 2.4' over a wide range of radial velocities, we analyze the neutral-hydrogen distribution in the region of the supernova remnant (SNR) G78.2+2.1. ... The brightness distribution of H I features at a radial velocity of +10 km/s after an extended background in the region of the Cygnus X radio source and SNR G78.2+2.1 has bee subtracted. ...

Find Similar Abstracts . ... The birth of a closed universe, and the anthropogenic principle . ... 7, Oct. 1981, p. 579-581.) Soviet Astronomy Letters, vol. ... Oct. 1981, p. 322, 323. ... Thus a universe having the properties we observe may in fact have been singled out by the anthropogenic principle. Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

... This document and the attached postscript figure document an analysis that I did to determine the optimum midpoint and required ranges for both the rotator and azimuth for the 2.5 M telescope. ... I simulate a series of drift scans on the sky for tracks that cover the northern survey area. These tracks cover the range in survey latitude of -60 to +60 degrees, spaced by 10 degrees. ... Along each track the azimuth, elevation, and position angle of the CCD is computed at 1 minute intervals. ...

LOC Web-site . The 13 th International Astronomy Olympiad has been held successfully in Trieste (Italy) on October 13-21, 2008. ... There were 19 teams participated in the XIII IAO: . ... Monday, October 13 - Day of arrival . Tuesday, October 14 - Day of opening ceremony . ... M.G.Gavrilov (IAO Chairman) - Chairman, . C.Boehm (Trieste, XIII IAO-2008 LOC Chairman), . ... Dr. Michael G. Gavrilov, Founding Chairman and Coordinator of the International Astronomy Olympiad (IAO) . ...

... Close Up of the Lagoon Nebula . ... 16.08.2004 . ... Credit: Canada-France-Hawaii Telescope , J.-C. Cuillandre ( CFHT ), Coelum Explanation: Stars are battling gas and dust in the Lagoon Nebula but the photographers are winning. ... The speculator portion of the Lagoon Nebula taken by the CFHT was created from light emitted by hydrogen (shown in red) and light emitted by oxygen (shown in green). ... Publications with keywords: M8 - Lagoon Nebula . ... Stars and Dust of the Lagoon Nebula . ...

. September 9 - 14, 1996. Close to the apogee of the Auroral Probe orbit in the morning sector of magnetosphere at L > 8 the energy fluxes of ions with some maximums were regularly recorded. These maximums are probably connected with the registration of multicomponent ion flow containing H + , He + , N + +O + , N 2 + +O 2 + +NO + . The total flux of ions with the energy E < 25 eV is 4ћ10 7 - 5ћ10 8 cm -2 s -1 .

Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences PUL Analysis Center Pulkovo IVS Analysis Center (PUL) 2009 Annual Rep ort Zinovy Malkin, Natalia Miller, Elena Popova Abstract This report briefly presents the PUL IVS Analysis Center activities during 2009 and plans for the coming year. The main topics of the investigations of PUL staff in that period were ICRF related studies, computation and analysis of EOP series, and VLBI2010 related issues. ...

... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...

... 8, ``Celestial Mechanics'', 2002 CCD observations of planetary satellites and occultations and close approachments of stars by asteroids with 26­ inch refractor of Pulkovo observatory T. P. Kiseleva, I. S. Izmailov, M. A. Mozhaev Pulkovo Observatory, St. Petersburg, Russia ST--6 CCD camera has been used with 26-- inch Refractor at Pulkovo for ob­ servations of ... These estimates are \Sigma0:015 arcsec and \Sigma0:014 arcsec for X and Y correspondingly. ...

... Two algorithms have been used to simultaneously solve for the sky, gain, and offset for simulated sets of dithered images. ... When solving for sky and gain, achieves machine precision on noiseless data; for noisy data, solution within noise. ... When solving for sky and gain, achieves machine precision on noiseless data; for noisy data, solution slightly different from Fixsen-Arendt solution, but within noise. ... Figure 2: MIPS truth image, and full MIPS dither pattern . ...

... The spectrum of the Sgr B2 molecular cloud has been surveyed between 215 and 265 GHz towards 3 positions, the dense cores Sgr B2(N)and Sgr B2(M), and the quiescent core Sgr B2(NW). ... The Sgr B2 molecular cloud, located approximately 100 pc from the Galactic Centre and with a mass of , is one of the most extreme cases among star formation sites ( Lis & Goldsmith (1991) ). ... Of the 3 observed positions Sgr B2(N) has the strongest line emission in most molecular species with a few exceptions. ...