FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2022356181> ?p ?o ?g. }

• W2022356181 endingPage "S221" @default.
• W2022356181 startingPage "S207" @default.
• W2022356181 abstract "Five on-plane regions within +/- 0.8deg of the Galactic center were observed with the Hard X-ray Detector (HXD) and the X-ray Imaging Spectrometer (XIS) onboard Suzaku. From all regions, significant hard X-ray emission was detected with HXD-PIN up to 40 keV, in addition to the extended plasma emission which is dominant in the XIS band. The hard X-ray signals are inferred to come primarily from a spatially extended source, rather than from a small number of bright discrete objects. Contributions to the HXD data from catalogued X-ray sources, typically brighter than 1 mCrab, were estimated and removed using information from Suzaku and other satellites. Even after this removal, the hard X-ray signals remained significant, exhibiting a typical 12--40 keV surface brightness of 4E-10 erg cm-2 s-1 deg-2 and power-law-like spectra with a photon index of 1.8. Combined fittings to the XIS and HXD-PIN spectra confirm that a separate hard tail component is superposed onto the hot thermal emission, confirming a previous report based on the XIS data. Over the 5--40 keV band, the hard tail is spectrally approximated by a power law of photon index ~2, but better by those with somewhat convex shapes. Possible origins of the extended hard X-ray emission are discussed." @default.
• W2022356181 created "2016-06-24" @default.
• W2022356181 creator A5008122738 @default.
• W2022356181 creator A5022197033 @default.
• W2022356181 creator A5024955707 @default.
• W2022356181 creator A5028070930 @default.
• W2022356181 creator A5033311537 @default.
• W2022356181 creator A5034026655 @default.
• W2022356181 creator A5042164470 @default.
• W2022356181 creator A5050905248 @default.
• W2022356181 creator A5060279814 @default.
• W2022356181 creator A5061572980 @default.
• W2022356181 creator A5067428193 @default.
• W2022356181 creator A5077781477 @default.
• W2022356181 creator A5086937144 @default.
• W2022356181 creator A5087278101 @default.
• W2022356181 creator A5089397488 @default.
• W2022356181 date "2008-02-20" @default.
• W2022356181 modified "2023-10-06" @default.
• W2022356181 title "Suzaku Detection of Extended/Diffuse Hard X-Ray Emission from the Galactic Center" @default.
• W2022356181 cites W1973961020 @default.
• W2022356181 cites W1978691390 @default.
• W2022356181 cites W1984008682 @default.
• W2022356181 cites W1995610322 @default.
• W2022356181 cites W2004958367 @default.
• W2022356181 cites W2013584294 @default.
• W2022356181 cites W2018773775 @default.
• W2022356181 cites W2020919928 @default.
• W2022356181 cites W2022585345 @default.
• W2022356181 cites W2028501240 @default.
• W2022356181 cites W2032372224 @default.
• W2022356181 cites W2034937893 @default.
• W2022356181 cites W2045737159 @default.
• W2022356181 cites W2046225530 @default.
• W2022356181 cites W2048206598 @default.
• W2022356181 cites W2069889589 @default.
• W2022356181 cites W2070229824 @default.
• W2022356181 cites W2077161655 @default.
• W2022356181 cites W2082518108 @default.
• W2022356181 cites W2085499291 @default.
• W2022356181 cites W2087044161 @default.
• W2022356181 cites W2094947514 @default.
• W2022356181 cites W2095842507 @default.
• W2022356181 cites W2098787786 @default.
• W2022356181 cites W2100235733 @default.
• W2022356181 cites W2112912708 @default.
• W2022356181 cites W2124515698 @default.
• W2022356181 cites W2125570493 @default.
• W2022356181 cites W2126271344 @default.
• W2022356181 cites W2138831523 @default.
• W2022356181 cites W2158746059 @default.
• W2022356181 cites W3033709371 @default.
• W2022356181 cites W3099183279 @default.
• W2022356181 cites W3099745664 @default.
• W2022356181 cites W3100116223 @default.
• W2022356181 cites W3105505278 @default.
• W2022356181 cites W3106152066 @default.
• W2022356181 doi "https://doi.org/10.1093/pasj/60.sp1.s207" @default.
• W2022356181 hasPublicationYear "2008" @default.
• W2022356181 type Work @default.
• W2022356181 sameAs 2022356181 @default.
• W2022356181 citedByCount "20" @default.
• W2022356181 countsByYear W20223561812012 @default.
• W2022356181 countsByYear W20223561812013 @default.
• W2022356181 countsByYear W20223561812016 @default.
• W2022356181 countsByYear W20223561812017 @default.
• W2022356181 crossrefType "journal-article" @default.
• W2022356181 hasAuthorship W2022356181A5008122738 @default.
• W2022356181 hasAuthorship W2022356181A5022197033 @default.
• W2022356181 hasAuthorship W2022356181A5024955707 @default.
• W2022356181 hasAuthorship W2022356181A5028070930 @default.
• W2022356181 hasAuthorship W2022356181A5033311537 @default.
• W2022356181 hasAuthorship W2022356181A5034026655 @default.
• W2022356181 hasAuthorship W2022356181A5042164470 @default.
• W2022356181 hasAuthorship W2022356181A5050905248 @default.
• W2022356181 hasAuthorship W2022356181A5060279814 @default.
• W2022356181 hasAuthorship W2022356181A5061572980 @default.
• W2022356181 hasAuthorship W2022356181A5067428193 @default.
• W2022356181 hasAuthorship W2022356181A5077781477 @default.
• W2022356181 hasAuthorship W2022356181A5086937144 @default.
• W2022356181 hasAuthorship W2022356181A5087278101 @default.
• W2022356181 hasAuthorship W2022356181A5089397488 @default.
• W2022356181 hasBestOaLocation W20223561811 @default.
• W2022356181 hasConcept C105795698 @default.
• W2022356181 hasConcept C120665830 @default.
• W2022356181 hasConcept C121332964 @default.
• W2022356181 hasConcept C125245961 @default.
• W2022356181 hasConcept C1276947 @default.
• W2022356181 hasConcept C132552067 @default.
• W2022356181 hasConcept C159317903 @default.
• W2022356181 hasConcept C183582522 @default.
• W2022356181 hasConcept C183852935 @default.
• W2022356181 hasConcept C2779328170 @default.
• W2022356181 hasConcept C33390570 @default.
• W2022356181 hasConcept C33923547 @default.
• W2022356181 hasConcept C42061751 @default.
• W2022356181 hasConcept C44870925 @default.
• W2022356181 hasConcept C4839761 @default.

• next