FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100855941> ?p ?o ?g. }

• W3100855941 endingPage "133" @default.
• W3100855941 startingPage "133" @default.
• W3100855941 abstract "There is evidence that magnetized material along the line of sight to distant quasars is detectable in the polarization properties of the background sources. The polarization properties appear to be correlated with the presence of intervening MgII absorption, which is thought to arise in outflowing material from star forming galaxies. In order to investigate this further, we have obtained high spectral resolution polarization measurements, with the VLA and ATCA, of a set of 49 unresolved quasars for which we have high quality optical spectra. These enable us to produce a Faraday Depth spectrum for each source, using Rotation Measure Synthesis. Our new independent radio data confirms that interveners are strongly associated with depolarization. We characterize the complexity of the Faraday Depth spectrum using a number of parameters and show how these are related, or not, to the depolarization and to the presence of MgII absorption along the line of sight. We argue that complexity and structure in the Faraday Depth distribution likely arise from both intervening material and intrinsically to the background source and attempt to separate these. We find that the strong radio depolarization effects associated with intervening material at redshifts out to $z approx 1$ arise from inhomogeneous Faraday screens producing a dispersion in Rotation Measure across individual sources of around 10~rad/m$^2$. This is likely produced by disordered fields with strengths of at least $3;mu$G." @default.
• W3100855941 created "2020-11-23" @default.
• W3100855941 creator A5012431420 @default.
• W3100855941 creator A5028071403 @default.
• W3100855941 creator A5032344817 @default.
• W3100855941 creator A5053935358 @default.
• W3100855941 creator A5057238445 @default.
• W3100855941 creator A5066077016 @default.
• W3100855941 creator A5070521432 @default.
• W3100855941 date "2016-09-29" @default.
• W3100855941 modified "2023-10-18" @default.
• W3100855941 title "FARADAY ROTATION MEASURE SYNTHESIS OF INTERMEDIATE REDSHIFT QUASARS AS A PROBE OF INTERVENING MATTER" @default.
• W3100855941 cites W1563718207 @default.
• W3100855941 cites W1649074782 @default.
• W3100855941 cites W1665346145 @default.
• W3100855941 cites W1839132220 @default.
• W3100855941 cites W1874693742 @default.
• W3100855941 cites W1877230173 @default.
• W3100855941 cites W1979050809 @default.
• W3100855941 cites W1980346622 @default.
• W3100855941 cites W1984635727 @default.
• W3100855941 cites W1984879627 @default.
• W3100855941 cites W1987883530 @default.
• W3100855941 cites W1987936139 @default.
• W3100855941 cites W1993977025 @default.
• W3100855941 cites W1995114536 @default.
• W3100855941 cites W2002706261 @default.
• W3100855941 cites W2007468939 @default.
• W3100855941 cites W2019450729 @default.
• W3100855941 cites W2038275661 @default.
• W3100855941 cites W2056866161 @default.
• W3100855941 cites W2057209307 @default.
• W3100855941 cites W2058373358 @default.
• W3100855941 cites W2059001712 @default.
• W3100855941 cites W2068340869 @default.
• W3100855941 cites W2073265904 @default.
• W3100855941 cites W2101307399 @default.
• W3100855941 cites W2142516705 @default.
• W3100855941 cites W2148307523 @default.
• W3100855941 cites W2159060260 @default.
• W3100855941 cites W2264368166 @default.
• W3100855941 cites W3098539272 @default.
• W3100855941 cites W3098601964 @default.
• W3100855941 cites W3103415081 @default.
• W3100855941 cites W3103462129 @default.
• W3100855941 cites W3103539009 @default.
• W3100855941 cites W3103583886 @default.
• W3100855941 cites W3104011010 @default.
• W3100855941 cites W3104121946 @default.
• W3100855941 cites W3105037954 @default.
• W3100855941 cites W4290035193 @default.
• W3100855941 cites W4290035235 @default.
• W3100855941 doi "https://doi.org/10.3847/0004-637x/829/2/133" @default.
• W3100855941 hasPublicationYear "2016" @default.
• W3100855941 type Work @default.
• W3100855941 sameAs 3100855941 @default.
• W3100855941 citedByCount "31" @default.
• W3100855941 countsByYear W31008559412016 @default.
• W3100855941 countsByYear W31008559412017 @default.
• W3100855941 countsByYear W31008559412018 @default.
• W3100855941 countsByYear W31008559412019 @default.
• W3100855941 countsByYear W31008559412020 @default.
• W3100855941 countsByYear W31008559412021 @default.
• W3100855941 countsByYear W31008559412022 @default.
• W3100855941 countsByYear W31008559412023 @default.
• W3100855941 crossrefType "journal-article" @default.
• W3100855941 hasAuthorship W3100855941A5012431420 @default.
• W3100855941 hasAuthorship W3100855941A5028071403 @default.
• W3100855941 hasAuthorship W3100855941A5032344817 @default.
• W3100855941 hasAuthorship W3100855941A5053935358 @default.
• W3100855941 hasAuthorship W3100855941A5057238445 @default.
• W3100855941 hasAuthorship W3100855941A5066077016 @default.
• W3100855941 hasAuthorship W3100855941A5070521432 @default.
• W3100855941 hasBestOaLocation W31008559411 @default.
• W3100855941 hasConcept C108948954 @default.
• W3100855941 hasConcept C115260700 @default.
• W3100855941 hasConcept C121332964 @default.
• W3100855941 hasConcept C1276947 @default.
• W3100855941 hasConcept C135041427 @default.
• W3100855941 hasConcept C147789679 @default.
• W3100855941 hasConcept C185592680 @default.
• W3100855941 hasConcept C205049153 @default.
• W3100855941 hasConcept C207230154 @default.
• W3100855941 hasConcept C2780928442 @default.
• W3100855941 hasConcept C33024259 @default.
• W3100855941 hasConcept C44870925 @default.
• W3100855941 hasConcept C4839761 @default.
• W3100855941 hasConcept C62520636 @default.
• W3100855941 hasConcept C98444146 @default.
• W3100855941 hasConceptScore W3100855941C108948954 @default.
• W3100855941 hasConceptScore W3100855941C115260700 @default.
• W3100855941 hasConceptScore W3100855941C121332964 @default.
• W3100855941 hasConceptScore W3100855941C1276947 @default.
• W3100855941 hasConceptScore W3100855941C135041427 @default.
• W3100855941 hasConceptScore W3100855941C147789679 @default.
• W3100855941 hasConceptScore W3100855941C185592680 @default.
• W3100855941 hasConceptScore W3100855941C205049153 @default.
• W3100855941 hasConceptScore W3100855941C207230154 @default.

• next