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093081

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DataCite Commons2025-01-29 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/093081.html
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We propose to observe the X-ray brightest and one of the firstgamma-ray-detected BAL quasars B3 1520+437 simultaneously with NuSTARand XMM-Newton for exposures 40 ksec and 20 ksec respectively. Theproposed observations will allow us to (i) check whether strong soft X-rayabsorption one of the most prominent characteristics of most BAL quasarsalso exists in the polar outflows and to check whether face-on BAL quasarsare otherwise X-ray normal and (ii) precisely estimate the jet powerlocation of the emission region along the jet bulk Lorentz factor andproperties of the electron energy distribution. [truncated! Please see actual data for full text]
提供机构:
European Space Agency
创建时间:
2025-01-29
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