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- W2044769110 abstract "We report the results of a new 60 ks Chandra X-ray Observatory Advanced CCD Imaging Spectrometer S-array (ACIS-S) observation of the reddened, radio-selected, highly polarized ‘FeLoBAL’ quasar FIRST J1556+3517. We investigated a number of models of varied sophistication to fit the 531-photon spectrum. These models ranged from simple power laws to power laws absorbed by hydrogen gas in differing ionization states and degrees of partial covering. Preferred fits indicate that the intrinsic X-ray flux is consistent with that expected for quasars of similarly high luminosity, i.e. an intrinsic, dereddened and unabsorbed optical to X-ray spectral index of −1.7. We cannot tightly constrain the intrinsic X-ray power-law slope, but find indications that it is flat (photon index Γ = 1.7 or flatter at a >99 per cent confidence for a neutral hydrogen absorber model). Absorption is present, with a column density a few times 1023 cm−2, with both partially ionized models and partially covering neutral hydrogen models providing good fits. We present several lines of argument that suggest the fraction of X-ray emissions associated with the radio jet is not large. We combine our Chandra data with observations from the literature to construct the spectral energy distribution of FIRST J1556+3517 from radio to X-ray energies. We make corrections for Doppler beaming for the pole-on radio jet, optical dust reddening and X-ray absorption, in order to recover a probable intrinsic spectrum. The quasar FIRST J1556+3517 seems to be an intrinsically normal radio-quiet quasar with a reddened optical/UV spectrum, a Doppler-boosted but intrinsically weak radio jet and an X-ray absorber not dissimilar from that of other broad absorption line quasars." @default.
- W2044769110 created "2016-06-24" @default.
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- W2044769110 date "2013-10-23" @default.
- W2044769110 modified "2023-09-23" @default.
- W2044769110 title "The X-ray spectrum and spectral energy distribution of FIRST J155633.8+351758: a LoBAL quasar with a probable polar outflow" @default.
- W2044769110 cites W1524618787 @default.
- W2044769110 cites W1951204806 @default.
- W2044769110 cites W1966498099 @default.
- W2044769110 cites W1966935784 @default.
- W2044769110 cites W1968646907 @default.
- W2044769110 cites W1969912137 @default.
- W2044769110 cites W1971146070 @default.
- W2044769110 cites W1976615408 @default.
- W2044769110 cites W1977457396 @default.
- W2044769110 cites W1980726288 @default.
- W2044769110 cites W1987237508 @default.
- W2044769110 cites W1990103877 @default.
- W2044769110 cites W1990704789 @default.
- W2044769110 cites W1991752356 @default.
- W2044769110 cites W1996910901 @default.
- W2044769110 cites W1997076624 @default.
- W2044769110 cites W1998737144 @default.
- W2044769110 cites W1998759148 @default.
- W2044769110 cites W2003630083 @default.
- W2044769110 cites W2008712774 @default.
- W2044769110 cites W2009880431 @default.
- W2044769110 cites W2016572119 @default.
- W2044769110 cites W2017396100 @default.
- W2044769110 cites W2022902136 @default.
- W2044769110 cites W2025023223 @default.
- W2044769110 cites W2029344968 @default.
- W2044769110 cites W2032876430 @default.
- W2044769110 cites W2036259292 @default.
- W2044769110 cites W2040222334 @default.
- W2044769110 cites W2044069863 @default.
- W2044769110 cites W2044191473 @default.
- W2044769110 cites W2044610256 @default.
- W2044769110 cites W2047002529 @default.
- W2044769110 cites W2049952229 @default.
- W2044769110 cites W2052926897 @default.
- W2044769110 cites W2052990654 @default.
- W2044769110 cites W2053563078 @default.
- W2044769110 cites W2057953757 @default.
- W2044769110 cites W2061496112 @default.
- W2044769110 cites W2063365265 @default.
- W2044769110 cites W2067368901 @default.
- W2044769110 cites W2068601384 @default.
- W2044769110 cites W2069807844 @default.
- W2044769110 cites W2071344583 @default.
- W2044769110 cites W2074418452 @default.
- W2044769110 cites W2074868843 @default.
- W2044769110 cites W2075179680 @default.
- W2044769110 cites W2075224333 @default.
- W2044769110 cites W2075687999 @default.
- W2044769110 cites W2082174303 @default.
- W2044769110 cites W2091151158 @default.
- W2044769110 cites W2098463458 @default.
- W2044769110 cites W2110164985 @default.
- W2044769110 cites W2112615655 @default.
- W2044769110 cites W2119836155 @default.
- W2044769110 cites W2135212470 @default.
- W2044769110 cites W2146805014 @default.
- W2044769110 cites W2157823339 @default.
- W2044769110 cites W2157917411 @default.
- W2044769110 cites W2169204353 @default.
- W2044769110 cites W3099572316 @default.
- W2044769110 cites W3099634360 @default.
- W2044769110 cites W3099973496 @default.
- W2044769110 cites W3100556126 @default.
- W2044769110 cites W3100938569 @default.
- W2044769110 cites W3100976175 @default.
- W2044769110 cites W3101299994 @default.
- W2044769110 cites W3101630419 @default.
- W2044769110 cites W3101817379 @default.
- W2044769110 cites W3102302943 @default.
- W2044769110 cites W3102471238 @default.
- W2044769110 cites W3102531047 @default.
- W2044769110 cites W3103069129 @default.
- W2044769110 cites W3103078725 @default.
- W2044769110 cites W3103641717 @default.
- W2044769110 cites W3103882988 @default.
- W2044769110 cites W3104526308 @default.
- W2044769110 cites W3104855129 @default.
- W2044769110 cites W3105037366 @default.
- W2044769110 cites W3105378134 @default.
- W2044769110 cites W3105746951 @default.
- W2044769110 cites W3105794134 @default.