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http://hea-www.harvard.edu/ChandraSNR/G189.1+03.0C/chandra_spectra.cgi.
http://hea-www.harvard.edu/ChandraSNR/G189.1+03.0C/chandra_spectra.cgi.
1. Chandra Images for G011.2-00.3
. True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . Images show regions used to extract spectra . Regions with red strikes are excluded . Background was subtracted from a region around or close to the SNR. Back to G011.2-00.3 Index . Chandra Supernova Remnant Catalog . Main Page | Galactic SNR | Magellanic Cloud SNR . True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR .
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G011.2-00.3/chandra_spectra.cgi -- 5.0 Кб -- 02.10.2012
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2. How to extract MOS spectra of a point-like source and associated matrices
... This thread contains a step-by-step recipe to extract MOS spectra of a point-like source observed in Imaging mode and to create associated response matrices, starting from a calibrated, concatenated event list (either produced with emproc or available as PPS product; here it has the assumed file name MOS.fits ). ... The users should note that the SAS metatask xmmselect allows them to interactively define source and background regions (via ds9) and to run backscale on the fly. ...
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Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/MOS_spectrum_thread.html -- 11.6 Кб -- 15.06.2007
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3. The Parkes 6 cm Galactic Survey
... 1Haynes+ A catalogue at 5 GHz of 915 sources in the Galactic plane is presented. Sources with a peak beam brightness temperature of at least 0.2 K above the surrounding background are included, except in confused regions; a point source of 0.2 K corresconds to 0.26 Jy. ... It was assumed that Hydra A was a point source with a peak flux density of 13 Jy at 5 GHz; this is equivalent to a mean beam brightness temperature of 10.0 K for a beamwidth of 4.1x4.4'. ...
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Ссылки http://www.sao.ru/cats/doc/PKSGAL.html -- 6.0 Кб -- 18.03.2015
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4. Radio sources identfification
... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...
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Ссылки http://mavr.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
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5. casacore: images/Regions/WCCompound.h Source File
... Classes . Files . ... File List . File Members . images . Regions . ... 00087 // The image regions have to contain WCRegion objects, otherwise an 00088 // exception is thrown. 00089 // group 00090 WCCompound ( const ImageRegion region1, const ImageRegion region2); 00091 WCCompound ( const ImageRegion * region1, 00092 const ImageRegion * region2 = 0, 00093 const ImageRegion * region3 = 0, 00094 const ImageRegion * region4 = 0, 00095 const ...
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Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/WCCompound_8h_source.html -- 26.8 Кб -- 14.02.2011
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6. Detection of polarized radiation sources with unusual spectral characteristics
... Solar flare activity is produced by the processes of accumulation and release of energy in an active region. ... In the framework of study of solar active regions, producing powerful flares the researchers from the RATAN-600 radio telescope have detected sources with features in the form of a sharp drop in the intensity of polarized radiation in various parts of the recorded frequency range (2-16GHz), sometimes changing the sign of polarization. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
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7. 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. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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8. A Spitzer Space Telescope Far-infrared Spectral Atlas of Compact Sources in the
We present far-infrared spectra, ЮЛ = 52-93 ЮМm, obtained with the Spitzer Space Telescope in the spectral energy distribution mode of its Multiband Imaging Photometer for Spitzer instrument, of a selection of luminous compact far-infrared sources in the Small Magellanic Cloud (SMC). ... We compare these results with those obtained in the Large Magellanic Cloud (LMC). ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2010AJ....139.1553V.html -- 5.8 Кб -- 21.01.2016
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9. INTEGRAL 9-year Galactic Survey
... Flux Sign Expo . ... 0.13 PHA . ... The map above is movable . ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. All maps are convolved with instrumental point spread function (PSF) which is Gaussian ( =5'). Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ...
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Ссылки http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php?key=GAL-Survey-115-clean&ei=3®ion=1&map=expo -- 17.3 Кб -- 10.04.2016
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10. http://www.naic.edu/~astro/School/Talks/large_pdf/handson_gbt2_2.pdf
... GRAPHICS SOURCE: W3OH (STAR FORMING REGION) SOURCE: TCOM (STAR) SOURCE: RHYA (STAR) SOURCE: WLEO (STAR) SOURCE: ARP220 (EXTRAGLACTIC SOURCE) Results SOURCE S W 3OH TCom RH ya W Leo Arp220 DIST ANCE S (pc) 2200 1253 617 1220 Z=0.018 TYPE SFR * * * EG INT. FLUX (Jy Km/s) 432.34 1.97 17.05 1.34 52.20 L/L (SNR) 3.6 10(6.8) 5.2 10(14.9) 1.1 10(5.9) 3.4 10(12.7) 6 Tsys (K ) 41.52 RM S/Calc 0.02/0.017 0.01/0.009 0.01/0.008 0.01/0.009 0.008/0.006 9 15.05 8 16.67 9 15.17 16.33 512 (701.9) Table 1. ...
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Ссылки http://www.naic.edu/~astro/School/Talks/large_pdf/handson_gbt2_2.pdf -- 126.0 Кб -- 18.07.2005
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11. The 7C(G) survey
... Full details of the observations, data reduction and calibration of this survey, and the production of the 7C(G) compact source list, are described in Vessey & Green (1998, MNRAS, 294, 607) . ... b |<5њ, with a resolution of about 1.2 ? ... The survey consisted of 24 fields, spaced 3њ.5 in l , and alternating between b = +3њ and -3њ, but with a gap near l = 110њ. ... Please refer to the source list description for details of the entries ; the catalogue itself is available as: . ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/7C_G/ -- 8.7 Кб -- 05.04.2000
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12. The Cross-correlations
... The actual cross-correlations were done as follows: north of WGACAT was correlated with the GB6 catalog with a correlation radius of one arc minute. ... We therefore cross-correlated WGACAT with the GB6 and PMN radio catalogs with a 1.5 arcmin radius. ... As a result of this experiment, we then added to the WGACAT/PMN candidate list the 29 unclassified sources obtained from the 1.5 arcmin correlation and having PSPC offsets arcmin, ratio between X-ray/radio offset and positional error , and . ...
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Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node5.html -- 11.3 Кб -- 03.12.2003
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13. Population Synthesis of X-ray Sources at the Galactic Center
Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node72.html -- 6.7 Кб -- 01.03.1997
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14. The BD+40 region (Abstract)
... Near-IR broad-band imaging of V1318 Cygni reveals the presence of two distinct stellar components oriented north-south, a result recently reported by Aspin et al. ... The distribution of the high density molecular gas traced by the CS J emission is highly concentrated around V1318 and V1686 Cygni, while the total column density of gas traced by the J shows a ridge morphology centered on these sources. ... A molecular outflow has been detected in CO J . ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/bd40_fig_aa/abstract.html -- 4.1 Кб -- 11.09.2007
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15. Astro-2 and the UIT Experiment
... Ultraviolet photons have short wavelength and high energy and thus come from sources which have fairly high temperatures. ... Star formation regions in nearby galaxies . Star formation regions in our own galaxy . ... In addition, the background glow of the night sky is at a minimum level at around 2000 angstroms. ... It is hoped that these very diffuse galaxies can be more easily imaged at a wavelength where the noise from a background of finite brightness is at its minimum. ...
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Ссылки http://zebu.uoregon.edu/uit-ms.html -- 2.5 Кб -- 07.10.1996
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16. Stellarium: core/StelSphericalIndexMultiRes.hpp Source File
... 40 љ template < class FuncObject> void processIntersectingRegions ( const SphericalRegionP & region, FuncObject& func) const . ... 44 љ const RootNode* node = treeForRadius[i-1]; . ... 87 љ const Vec3d & c0 = triangle.getConvexContour().at(0); . ... 195 љ template < class FuncObject> void processIntersectingRegions ( const Node& node, const SphericalRegionP & region, FuncObject& func) const . ... 212 љ template < class FuncObject> void processAll ( const Node& node, FuncObject& func) const . ...
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Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/StelSphericalIndexMultiRes_8hpp_source.html -- 38.5 Кб -- 28.02.2014
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17. SAI SN RESEARCH GROUP
Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...
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18. Test access to the platforms of electronic resources of McGraw-Hill Education
... Pre-university education . ... The NEICON consortium provides free test access to three platforms of electronic resources of McGraw-Hill Education company: . ... ACCESS ENGINEERING (www.accessengineeringlibrary.com ) is the largest platform in the area of technology and engineering science. It contains over 250 key items as well as interactive graphs, tables and video materials. ... ACCESS MEDICINE (www.accessmedicine.com) is the basic medicinal platform of McGraw-Hill Education. ...
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Ссылки http://www.ssau.ru/engnews/10157/ -- 23.8 Кб -- 27.09.2013
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19. ASP: Family ASTRO: Resource Lists and Background Reading
Family ASTRO Event Leaders can follow the links below to find a number of resources and more background reading to help them with their Astronomy Events and expand their knowledge on the topics covered in our series of Leader Kits for educators. ... Print and Web Resources on the Night Sky . ... If you have questions about Family ASTRO, see our Frequently Asked Questions for Educators and Astronomers page , or our Frequently Asked Questions for Families and Friends page. ...
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Ссылки http://www.astrosociety.org/edu/family/resources/resources.html -- 7.0 Кб -- 02.10.2012
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20. X-Rays from the Galactic Core
... X-Rays from the Galactic Core . ... CXC , NASA Explanation: Using the orbiting Chandra X-ray Observatory, astronomers have taken this long look at the core of our Milky Way galaxy, some 26,000 light-years away. ... This suggests that this supermassive black hole has been starved by a lack of infalling material. ... Publications with keywords: X-ray - Milky Way - Galactic Center - Sgr A - black hole . Publications with words: X-ray - Milky Way - Galactic Center - Sgr A - black hole . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1201098 -- 14.8 Кб -- 06.11.2004
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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