... A form allowing access to any MPEC is at the bottom of this page. ... Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Prepared using the Tamkin Foundation Computer Network MPC @CFA.HARVARD.EDU URL http://www.minorplanetcenter.org/iau/ mpc .html 2010 NJ1 Observations: K10N01J * K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J K10N01J ... C51 WISE. ...

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• http://www.winer.org/Downloads/MPEC2010-A35.pdf
• http://www.winer.org/Downloads/MPEC2010-A36.pdf
• http://www.winer.org/Downloads/MPEC2010-A37.pdf

... Copyrightї1997 Bob Yen (byen@ix.netcom.com) (http://www.comet-track.com/hb/hb.html) . ... Information on Comet Hale-Bopp for the Non-Astronomer Hale-Bopp rotates about twice a day (3/14/97) . ... The Comet Observation Home Page was been selected to receive the Griffith Observatory Star Award for the week of February 2 - 8, 1997 for excellence in promoting astronomy to the public through the World Wide Web. ... Typically, about 1,000 individual users/computers access this page every day. ...

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• Laboratory of Non-equilibrium Electronic Processes - HomePage
• Department of Special Materials Processing
• Laboratory of Nonequilbrium Electron Processes (LNEP)

Overview -------- The quick processing ftps, demultiplexes and searches the resulting individual pixels at low resolution (32 x 3.125 MHz channels and 1.024 ms sampling). ... The results are written to /home/alfa/realtime/results on the ASP but are best viewed through the php web server (see below). ... Start the processing. ... Notes on the Candidate Viewer ----------------------------- The candidate viewer can be run from any browser on any computer on the AO network, not just ASP. ...

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• http://www.naic.edu/alfa/ealfa/meeting2/handouts/NAIC_guidelines.pdf
• http://www.naic.edu/alfa/galfa/meetings/3/galfa3_agenda.pdf
• http://www.naic.edu/~phil/notes/idlspcproc.html

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

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• Archive of observations of feed-cabine N1
• Process Control and Management
• Process Control

... Class . Use . ... FRAMES NO FRAMES All Classes . Packages that use ColorProcessor . ij.plugin.filter . ij.process . Uses of ColorProcessor in ij.plugin.filter . ... BackgroundSubtracter. rollingBallBrightnessBackground ( ColorProcessor ip, double radius, boolean createBackground, boolean lightBackground, boolean useParaboloid, boolean doPresmooth, boolean correctCorners) . ... Uses of ColorProcessor in ij.process . ... ColorProcessor . ... Used by the FFT class. ...

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• ij.process Class Hierarchy (ImageJ API)
• ij.plugin.filter (ImageJ API)
• Uses of Class ij.process.FloatProcessor (ImageJ API)

... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....

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... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

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• Arcetri Extragalactic Group
• Lunar Orbiter to the Moon (1966 - 1967)
• Pluto - Hubble Space Telescope

... Projects . ... High Energy Astrophysics department at IKI, Moscow, is carrying out research in various fields of X-ray astronomy: physical processes in the vicinity of compact sources of x-ray emission, x-ray observations using Russian space observatories MIR/KVANT and GRANAT, development of scientific instrumentation for the SPECTRUM-X-GAMMA mission and International Space Station (ISS), participation in the INTEGRAL project and observations on the RTT-150 optical telescope. 2016 IKI RAN ...

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• The 6th INTEGRAL Workshop "The Obscured Universe"
• z90-program
• GRANAT Home Page

On combined processing of different space geodetic observations . ... A software for combined processing of different space geodetic observations is developed along with the work on the co-location of various observational techniques at the observatories of Quasar VLBI network. ... Various aspects of the combined processing of different types of space geodetic observations are also discussed. ... space geodetic observations, combined processing, normal equations, software package, SINEX-format. ...

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• IAA EOP Service
• LAB Ephem. Astronomy-ERA
• (Untitled)

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

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• Hardware sector, archive 2013
• Hardware sector, archive 2009
• The dust jets in the nucleus of comet 29P/Schwassmann-Wachmann 1

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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This composite image is based on observations from the New Horizons Ralph/LEISA instrument made at 6:25 a.m. EDT on July 14, 2015, when New Horizons was 50,000 miles (81,000 kilometers) from Charon. The spatial resolution is 3 miles (5km) per pixel. The LEISA data were downlinked October 1 4, 2015, and processed into a map of Charon s 2.2 micron ammonia-ice absorption band. ... The ammonia absorption map from LEISA is shown in green on the LORRI image. ...

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• Supernova simulations reveal new processes | Astronomy.com
• Processing your sketch | Astronomy.com

... Advises . Contact Advises . As an advise for amateurs we would like to underline: if it's possible, try to observe 3 asteroid positions per night and do not neglect to observe the Numbered Minor Planets in your telescope field of view as a "by product" of your observational programs. ... We think such estimations ought to be produced every morning after CCD observations of the moving celestial objects by observer himself. ...

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... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... ISS Russian Segment . ... Rocket Space Complexes . Sea Launch . ... Launches Chronology . ... Land Launch . ... Land Launch - Complex Content | ... Contribution of RSC Energia to the Russian Rocket-Space Technology . ... RSC Energia: Progress MS-02 docked with the ISS.' ... ROCKET SPACE COMPLEXES . ...

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• S.P. Korolev RSC Energia - International Space Station
• RSC "Energia" - Launchers

System of astrometric databases of Pulkovo observatory. 26-inch refractor . Pulkovo system of astrometric databases consists of three databases, which contain results of processing photographic and CCD observations, obtained with the 26-inch refractor and the Normal astrograph of Pulkovo observatory. Pulkovo photographic catalogs: Pul-2, Pul-3 (Pul-3 SE), Pul ERS . Results of photographic and CCD observations of Solar system objects . ... Normal Astrograph ...

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... Data processing and storage : · Processing time with Groningen cluster may exceed observation time , especially if thermal noise or high dynamic range or high resolution (international baselines) is requested · Other resources for data analysis should be investigated · Involvement of FZ JЭlich (1 PB storage and cluster processing ) is considered and will be tested, data transfer between Groningen and ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• Determination of the relative orientation between radio and dynamical reference
• Astrophysics Group Fringes and Power Spectra from COAST

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38. Astronaut Bio: Bruce McCandless II

39. Intro

40. Follow Up - an Astronomy Net Observation_reports Forum Message