... 389Voges+ IX/10A ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999) ================================================================================ The ROSAT all-sky survey bright source catalogue. ... At a brightness limit of 0.1cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. Broad band images are available for a subset of the flagged sources from http://wave.xray.mpe.mpg.de/rosat/catalogues/rass-bsc . ... 0 Source countrate (4) 70- 78 E9.3 ct/s e_Count ?= ...

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• Source Positions
• ROSAT catalog
• The ROSAT All-Sky Survey Faint Source Catalogue

Slews: Fast and Slow Fast Slew Status XMMSL1 : catalogue of slew sources released May 2006 Revs 314-978, 5180 detections, 2692 clean sources , 259 hard (2-10 keV) sources , 6200 square degrees, attitude error=8 (1 sigma) Read et al, 2006, PASJ - Scientific highlights Esquej et al, 2007, A A ґ High variability galaxies Saxton et al, 2007, A A (in prep) ґ Full description SOFT 0.2-2 keV HARD 2-12 keV Fast ... Total of 10,000 deg^2; about 4000 clean sources. ...

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• XMM Deep Survey Simulations
• Description
• The contour method of calculating source region shape

True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Distance: 8kpc(galactic center ) . ... Radio . ... Radio Images Page . ... Exposure uf . ... Exposure uf Exposure time of unfiltered event file . Exposure f Exposure time of filtered event file . ... Event 2 FITS File . ... AUX file . ... see fit detail page for more about the fit. see chandra spectrum page for region used. ... Radio Images . ... 2002 , ApJ, 581, 1148 : Chandra and radio . ... Main Page | Galactic SNR | ...

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• BEHR: Bayesian Estimation of Hardness Ratios
• SAO RSDC Home Page - RRA - PSPC
• Chandra Images for G332.4-00.2

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Date: Thu, 22 May 1997 19:29:43 GMT . From: < castejon@kbw350.chem.yale.edu > . How the resources limits (filesize, cpu,etc) can be changed? . Messages . 1. Setting resource limits by Jukka Santala .

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• Setting resource limits
• research field
• Program parameters

... Authors: Paolo Padovani 1,2,3 , Raffaella Morganti 4 , Joachim Siebert 5 , Fausto Vagnetti 3 , Andrea Cimatti 6 We present new BeppoSax LECS, MECS and PDS observations of five lobe-dominated, broad-line active galactic nuclei selected from the 2-Jy sample of southern radio sources. These include three radio quasars and two broad-line radio galaxies. ... The collected data cover the energy range 0.1-10 keV, reaching ~50keV for one source (Pictor A). ... huizinga@stsci.edu . ...

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• The Nature of Luminous X-Ray Sources with Mid-Infrared Counterparts
• Herschel Key Program Heritage: a Far-Infrared Source Catalog for the Magellanic
• Hard Science/Soft Skills

The Future of Continuum Source Finding for ASKAP SSPs Paul Hancock Sydney Institute for Astronomy (SIfA) Source Finding today > Generic SF programs are available - Tend to be quite basic - Require post-processing > More refined SF programs - Telescope/Survey specific - Effective - Hard to transfer to other Telescopes/Surveys > ASKAP will require a refined program > "How well do the currently available source finding programs work on the simulated ASKAP data?" What do we want from a SF program? ...

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• Duchamp Source Finder
• Source Fitting and Positions
• VSOP Observing Schedule

... Chandra Resolves the Hard X Ray Background . ... Chandra , NASA Explanation: It is everywhere but nobody knew why. ... The above photograph shows that about 80 percent of the apparently diffuse hard X-ray background can be resolved into very many very faint sources. ... Publications with keywords: Chandra - x-ray background - cosmic microwave background radiation . Publications with words: Chandra - x-ray background - cosmic microwave background radiation . ... Chandra X Ray Telescope . ...

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• Астронет > Chandra Resolves the Hard X Ray Background
• Journal "Peremennye Zvezdy"
• XWare > APOD

... 2000 January 14 . Chandra Resolves the Hard X-Ray Background . ... Chandra , NASA . ... In every direction at all times, the sky glows in X-rays . ... Yesterday results were released using data from the recently launched Chandra X-Ray Observatory that appears to have resolved much of this mystery. The above photograph shows that about 80 percent of the apparently diffuse hard X-ray background can be resolved into very many very faint sources. ... About APOD | ...

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• Planetary Picture List
• Sternberg Astronomical Institute
• The Gimp Page

11 august 2014/Monday: Arriving, Registration . ... The variation of solar flare coronal X-ray source spatial properties. ... Melnikov V.F., Charikov Yu.E., Kudriavtsev I.V. Directivity of X-ray and gamma-ray emission from different parts of flaring magnetic loops. ... E., Melnikov V.F. Angular characteristics of polarization degree of hard X-ray emission from different parts of flaring magnetic loops. ... The thick target model and analytical calculations of the hard X-ray emission from solar flares. ...

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... Science . ... Science Users Information Science Software ESO-MIDAS jump to navigation jump to content . ... Science Software . ... ESO-MIDAS . ... ESO-MIDAS uses software standards provided by most computer manufactures, and runs on UNIX or Linux based platforms, as well as on Mac OSX systems. ... RedHat based, e.g. Scientific Linux, CentOS . ... Ubuntu based, e.g. Kubuntu, Ultimate Edition, Linux Mint . ... Debian based, e.g. aptosid . ... based on Linux/X11 emulation software Cygwin_NT-5.1 . ...

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• ROSAT BL Lac Spectra
• Different X-ray Spectra
• Sample Identification

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• ADASS 2003 Conference Proceedings
• QPSIM: An IRAF/PROS Tool for Source Simulation
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing

... 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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• NVSS Source Search ($Revision: 1.6 $ - running v2.17)
• G11.2-0.3
• The 7C(G) survey

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 Ї~20X more sensitive than Swift or INTEGRAL and cover full sky ЇDetect ~104 sources, 10 positions, 3-600 keV spectra Їunique 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/vscience/schedule/2013Fall/CamilotagP2717.pdf
• Calibration Scans on Continuum Sources
• ON/OFF (Position Switching)

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Located in the middle of Hard Labor Creek State Park in Rutledge, Georgia (~50 miles east of downtown Atlanta), the observatory is a resource for professional and amateur astronomers. However, an additional service of HLCO has been to the public - bringing the wonders of the Universe to Georgia residents. ... Web Site . ... Web . ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Astronomy articles, forums, listings, and other resources about Astronomy.

... Chandra Observation of LMXB in M84 . We present characteristics of the X-ray point source population in the M84 field as observed by Chandra ACIS-S. We find the galactic sources in M84 follow the stellar light profile, which imposes similar formation histories for stars in both single and binary systems. After correcting for incompleteness in the source detection, we find a log N-log S similar to that of the elliptical galaxy NGC4697. ...

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• Discussion and conclusions
• Scientific Interests
• Sources in the LMC: comments to the Table 2

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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• "Exploration" as a Classroom Resource
• Plasma source [Oulu]

... Seminar archive . ... 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. ... On the other hand, there have been numerous claims in recent years that the disc extends to the ISCO in the hard state. ...

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... This flare was observed simultaneously in H alpha, ratio (at microwave and millimeґ ter wavelenghts), and soft and hard Xґrays (by the Yohkoh spacecraft) with high spatial and moderate spectral resolution. ... Analysis of the microwave/hard Xґray/soft Xґray emission from individual sources provides information on the radio emission mechanisms, the energetic electron population, the magnetic field strenght, and plasma denґ sity. ...

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• IAJ: Resources: Observatories
• Hard disks
• Examples of hard disk allocation

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

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OPTICAL IDENTIFICATIONS OF INTEGRAL / RXTE SOURCES WITH 1.5-METER OPTICAL TELESCOPE RTT150 I.Bikmaev (1,2), M.Revnivtsev (3,4) , R.Burenin (3) R.Sunyaev (3,4) , N.Sakhibullin (1,2) (1) Kazan State University, Kremlevskaya Str., ... 1, D-85741, Garching bei MЭnchen , Germany (3 (4) ABSTRACT We present the first results of our project on optical identifications of INTEGRAL / RXTE hard X-ray sources by using scientific instrumentations of the 1.5meter joint Russian-Turkish optical telescope RTT150. ...

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• http://hea.iki.rssi.ru/integral/catalog/ReadMe.html
• High Energy Astrophysics Department at IKI RAN
• Russian Turkish 1.5-m telescope