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1. The ROSAT All-Sky Survey Bright Source Catalogue
... 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 ?= ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/RASS-BSC2.html -- 25.1 Кб -- 18.03.2015
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2. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Saxton.pdf
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 ­ High variability galaxies Saxton et al, 2007, A A (in prep) ­ Full description SOFT 0.2-2 keV HARD 2-12 keV Fast ... Total of 10,000 deg^2; about 4000 clean sources. ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Saxton.pdf -- 1689.7 Кб -- 13.05.2014
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3. Chandra Images for G000.1-00.1
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 | ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G000.1-00.1/ -- 11.0 Кб -- 27.02.2014
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4. resources hard limits
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 .
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/linux/khg/HyperNews/get/khg/66.html -- 2.5 Кб -- 23.03.2000
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5. STScI Preprint #1317
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1317/prep1317.html -- 5.7 Кб -- 23.05.2000
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6. http://www.atnf.csiro.au/research/workshops/2010/sourcefinding/Hancock.pdf
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? ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/research/workshops/2010/sourcefinding/Hancock.pdf -- 519.9 Кб -- 10.05.2010
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7. Chandra Resolves the Hard X Ray Background
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1162742 -- 15.9 Кб -- 10.11.2006
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8. APOD: 2000 January 14 - Chandra Resolves the Hard X Ray Background
... 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 | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap000114.html -- 4.7 Кб -- 01.10.2012
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9. RADIOSUN Workshop 2014
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. ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/english/personal/radiosun/program.html -- 7.7 Кб -- 25.06.2015
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10. ESO - ESO-MIDAS Hard- and Software Requirements
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/software/esomidas/midas-require.html -- 30.3 Кб -- 10.04.2016
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11. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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12. G111.7-2.1
... 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. ... Spitz