New Opportunities 2010 and Beyond: The High-Energy/Radio Connection High Energy Missions Timeline XMM, Suzaku.. ... Hard X-ray Sky EXIST Wide-Field Hard X-ray Imaging: EXIST ·~20X more sensitive than Swift or INTEGRAL and cover full sky ·Detect ~104 sources, 10 positions, 3-600 keV spectra ·unique temporal survey: full sky imaging each orbit High Energy Telescope HET (10-600keV) (6 x 3 coded aperture telescopes; 131o x 65o FoV) Low Energy Telescope LET (3-30 ...

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• http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/dos/OS2.TXT
• http://www.naic.edu/~phil/usrproj/a1946/24sep04_doit.pro
• http://www.naic.edu/~phil/calcb/040924doit.pro

... The hard gamma radiation from AGN is produced most probably in the relativistic jets observed in the considerable part of these objects. In the center of AGN (and may be of all other galaxies) there is a supermassive black hole surrounded by the accretion disk, which is the source of the energy in these objects. ... The problem of particle acceleration in the AGN jets is very important: the time of the electron energy losses in the jets is usually much less than their life time. ... next page . ...

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• Multi-element X-ray detection module
• Space Research Institute (IKI) Seminar
• ANO "Cosmos-NT"

... Programme . ... Its emission is detected from radio to -rays. Despite the fact that Centaurus A is one of the best studied extragalactic objects the origin of its hard X-ray and soft -ray emission is still poorly understood. ... A review of hard X-ray and -ray emission will be given (keV up to GeV) and the contribution of this observations to models of the Centaurus A emission wil be discssed. If no other talk addresses the newly reported emission > 250 GeV, this will be included.) . ...

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• tHermes key definitions
• lbaops:lbamar2008:vx014acdlog [ATNF VLBI Wiki]
• VLBI Wiki | PmWiki / PmWikiPhilosophy

... Mirror hard points, Galil channels A-D, are at nominal positions for observations . Lateral link drives, Galil channels E & F, are at nominal positions for observations . Install telescope-wind baffle turnbuckles . ... Remove wind baffle (see wind baffle rem. proc.) . ... Remove remaining 2 pair of wind baffle counterweights . ... Move wind baffle + telescope to zenith "bird bath", install pin, apply telescope altitude brake, depress emergency stop button and disable wind baffle drive . ...

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• Astrophysical Research Consortium - Apache Point Observatory
• Untitled Document

GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

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• High Energy Astrophysics Department at IKI RAN
• Сазонов Сергей Юрьевич (ИКИ РАН)
• Поутанен Юрий Иормович (Oulu Univ.)

... Flux density at 1 GHz (/Jy): 2720 . ... 1991, ApJ, 373, 146. ... ADS . ... VLA at 1.4 GHz and 4.8 GHz (both 1".3), for polarisation studies. ... VLA at 1.4 GHz and 4.8 GHz, for proper motion studies. ... 151 MHz observations for bulk expansion studies. ... Chandra observations, showing outer shock. ... Fesen et al. ... Spitzer observations. ... Chandra observations of rim. ... 2006, ApJ, 636, 848. ... 2006, ApJ, 647, L41. -ray line observations. ... Spitzer and Chandra observations for 3-D structure...

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• G11.2-0.3
• OptInt PmWiki : Pm Wiki Philosophy
• OptInt PmWiki : PmWiki / Pm Wiki Philosophy

... stars . ... Finding twin Earths is harder than we thought . Astronomers need a handful of transits to decipher a planet's atmosphere and possibly confirm the existence of the first twin Earth. ... If an earthlike world is nearby, though, then by adding observations of a number of transits, astronomers should be able to detect biomarkers like methane or ozone. ... They are also cooler and dimmer than the Sun, as well as smaller, which makes finding an earthlike planet transiting an M star easier. ...

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• In the protoplanetary disk, pebbles turn from rocks to asteroids to
• White dwarf pulses like a pulsar | Astronomy.com
• Phoenix continues sample-collection tests | Astronomy.com

These pages collect together references to many pictures of the solar system that can be found on the Net. ... Since I originally compiled this list the number of relevant images has grown tremendously. ... http://www.jpl.nasa.gov/pictures/ . ... ftp://dftnic.gsfc.nasa.gov/images/gifs/ . ... http://www.jpl.nasa.gov/galileo/images.html . http://www.jpl.nasa.gov/magellan/images.html . ... http://nssdc.gsfc.nasa.gov/image/planetary/ . ... NASA Image Access Homepage (Planetary Photojournal) . ...

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• Titan Press Release
• Electrons
• How to tell a sine from a cosine

... 12, 2015 Abell 2063 MAC 1522 +0828 May 09 2010 31 Ser Ser Ser Ser Ser Ser Ser Ser Ser Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy 17mmT4 EF,VS,UB,NND,AV FIRST THEN HOLDS, AGC 2063 ,R=P MAC 1522 +0829 May 09 2010 31 17mmT4 EF,ES,* IN NUC,VERY FAINT HALO AROUND *,SUSP, AGC ...

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• http://www.wro.org/scodova/RNGC_by_Abell14.pdf
• http://www.wro.org/scodova/RNGC_by_Abell151.pdf
• http://www.wro.org/scodova/RNGC_by_Abell147.pdf

... Bus Hound may be the very first product of its kind -- a software bus analyzer for capturing device I/O and protocol. ... When the capture buffer fills to capacity, Bus Hound can be configured to stop the capture process or continue capturing, keeping the most recent acquired data. ... IDE : Bus Hound captures command and data transfers for ATA and ATAPI devices. ... B us Hound captures I/O using a device driver. ... The below figure demonstrates how Bus Hound captures data for SCSI devices. ...

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• LWN: Driver porting: Device model overview
• From Power Up To Bash Prompt: The Filesystem
• Directory of Personnel

... Do you know why we have seasons on Earth? ... Even if you offer students the great activities developed by the Harvard researchers, or the great activities in ASP's teacher resource book, The Universe at Your Fingertips , your students still won't learn anything unless they work hard and think about their work. ... But none of these are worth a hoot unless they are also accompanied by hard work on students' part. ... The key to success in astronomy is the same as it is in everything else: hard work....

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• ASP: Now, Voyager
• ASP: Editorial: Down With the Geeks
• ASP: The topsy-turveying of planets, stars, and lava lamps

Geometry of X-ray sources in accreting black-hole binaries Andrzej A. Zdziarski N. Copernicus Astronomical Center, Warsaw The structure of the X-ray sources in the hard spectral state of accreting black-hole binaries has been a subject of intense debate. The paradigm dominant for many years postulated that the accretion disc in the hard state is truncated at some radius >> the innermost stable orbit (ISCO) whereas the disc reaches the ISCO in the soft state. ...

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• Ya.B. Zeldovich All-Moscow Seminar of Astrophysicists

. Remove a file that has hard links to it the same way as you would remove any other file: rm filename(s) . Any files that were created by making hard links to the filename will continue to exist in their own right. Removing a file to which symbolic links have been made has a different effect. Although the linkname remains, the actual file that this name points to does not. Trying to use a command on the linkname will give you the message: command : filename : No such file or directory .

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• UNIXhelp Glossary - "F"
• Linking directories

The First Law (1): Energy is Conserved in a closed system: . ... We usually consider work and heat flow as the two kinds of energy . The Second Law (2): The Law of Entropy: . ... The amount of disorder increases . ... You can not go from a disordered system to an ordered system without inputting more energy (this is the most important attribute of the second law) . ... In no way can we recover work of that this disordered system without putting energy into the system. ... More on Thermodynamics . ...

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• U of O High Energy Physics Seminars

... Up: User Interfaces and Visualization . Previous: DASHA-2: Improving Visualization and Processing of Photometric Data with IDL Objects . ... Smirnov, O. & Malkov, O. 1999, in ASP Conf. ... 172, Astronomical Data Analysis Software and Systems VIII, eds. D. M. Mehringer, R. L. Plante, & D. A. Roberts (San Francisco: ASP), 442 . ... XSKYMAP is a widget-based IDL application for visualization of astronomical catalogs. Since then XSKYMAP has grown into a powerful sky catalog visualization tool. ...

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• ADASS 2003 Conference Proceedings
• Integrating the ZGSC and PPM at the Galileo Telescope for On-line Control of
• Real Time Linux and the WTTM Project

. home . product . gallery . contact .

37. Project: PAHs

38. Some Autostar Hard Reset ? (Proc.Trap 2) error ! - Астрономия и компьютеры

39. Evidences of supercritical accretion onto black hole in SS433

40. http://www.schools.keldysh.ru/school1413/eng/Bad/main.html