Matches in SemOpenAlex for { <https://semopenalex.org/work/W2915397710> ?p ?o ?g. }
- W2915397710 endingPage "85" @default.
- W2915397710 startingPage "85" @default.
- W2915397710 abstract "We measure the average deflection of cosmic microwave background photons by quasars at $langle z rangle =1.7$. Our sample is selected from the Sloan Digital Sky Survey to cover the redshift range $0.9leq zleq2.2$ with absolute i-band magnitudes of $M_ileq-24$ (K-corrected to z=2). A stack of nearly 200,000 targets reveals an 8$sigma$ detection of Planck's estimate of the lensing convergence towards the quasars. We fit the signal with a model comprising a Navarro-Frenk-White density profile and a 2-halo term accounting for correlated large scale structure, which dominates the observed signal. The best-fitting model is described by an average halo mass $log_{10}(M_{rm h}/h^{-1}M_odot)=12.6pm0.2$ and linear bias $b=2.7pm0.3$ at $z=1.7$, in excellent agreement with clustering studies. We also report of a hint, at a 90% confidence level, of a correlation between the convergence amplitude and luminosity, indicating that quasars brighter than $M_ilesssim -26$ reside in halos of typical mass ${M_{rm h}approx 10^{13},h^{-1}M_odot}$, scaling roughly as ${M_{rm h}propto L_{rm opt}^{3/4}}$ at ${M_ilesssim-24}$, in good agreement with physically-motivated quasar demography models. Although we acknowledge this luminosity dependence is a marginal result, the observed $M_{rm h}$-$L_{rm opt}$ relationship could be interpreted as a reflection of the cutoff in the distribution of black hole accretion rates towards high Eddington ratios: the weak trend of $M_{rm h}$ with $L_{rm opt}$ observed at low luminosity becomes stronger for the most powerful quasars, which tend to be accreting close to the Eddington limit." @default.
- W2915397710 created "2019-03-02" @default.
- W2915397710 creator A5004910438 @default.
- W2915397710 creator A5005678872 @default.
- W2915397710 creator A5023302727 @default.
- W2915397710 creator A5045208440 @default.
- W2915397710 creator A5061482160 @default.
- W2915397710 creator A5085763615 @default.
- W2915397710 date "2019-03-27" @default.
- W2915397710 modified "2023-10-11" @default.
- W2915397710 title "The Halo Mass of Optically Luminous Quasars at <i>z</i> ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background" @default.
- W2915397710 cites W1602726146 @default.
- W2915397710 cites W1925976652 @default.
- W2915397710 cites W1972053729 @default.
- W2915397710 cites W1973368884 @default.
- W2915397710 cites W1976579441 @default.
- W2915397710 cites W1983211222 @default.
- W2915397710 cites W2004976613 @default.
- W2915397710 cites W2007204176 @default.
- W2915397710 cites W2027535639 @default.
- W2915397710 cites W2047002529 @default.
- W2915397710 cites W2048502125 @default.
- W2915397710 cites W2051694884 @default.
- W2915397710 cites W2054103046 @default.
- W2915397710 cites W2056330559 @default.
- W2915397710 cites W2062713883 @default.
- W2915397710 cites W2084345763 @default.
- W2915397710 cites W2105265841 @default.
- W2915397710 cites W2116045290 @default.
- W2915397710 cites W2123019532 @default.
- W2915397710 cites W2127477503 @default.
- W2915397710 cites W2134712793 @default.
- W2915397710 cites W2137023092 @default.
- W2915397710 cites W2148567160 @default.
- W2915397710 cites W2156368504 @default.
- W2915397710 cites W2160005571 @default.
- W2915397710 cites W2169866137 @default.
- W2915397710 cites W2204578610 @default.
- W2915397710 cites W2211491388 @default.
- W2915397710 cites W2345492478 @default.
- W2915397710 cites W2560866266 @default.
- W2915397710 cites W2608279899 @default.
- W2915397710 cites W2614934774 @default.
- W2915397710 cites W2615760052 @default.
- W2915397710 cites W2741744820 @default.
- W2915397710 cites W3099268282 @default.
- W2915397710 cites W3100110286 @default.
- W2915397710 cites W3100574878 @default.
- W2915397710 cites W3102678232 @default.
- W2915397710 cites W3102761395 @default.
- W2915397710 cites W3103268559 @default.
- W2915397710 cites W3104637165 @default.
- W2915397710 cites W3122369081 @default.
- W2915397710 cites W3122853321 @default.
- W2915397710 cites W3123662149 @default.
- W2915397710 cites W3125319234 @default.
- W2915397710 cites W3125978220 @default.
- W2915397710 doi "https://doi.org/10.3847/1538-4357/ab0894" @default.
- W2915397710 hasPublicationYear "2019" @default.
- W2915397710 type Work @default.
- W2915397710 sameAs 2915397710 @default.
- W2915397710 citedByCount "13" @default.
- W2915397710 countsByYear W29153977102019 @default.
- W2915397710 countsByYear W29153977102020 @default.
- W2915397710 countsByYear W29153977102022 @default.
- W2915397710 countsByYear W29153977102023 @default.
- W2915397710 crossrefType "journal-article" @default.
- W2915397710 hasAuthorship W2915397710A5004910438 @default.
- W2915397710 hasAuthorship W2915397710A5005678872 @default.
- W2915397710 hasAuthorship W2915397710A5023302727 @default.
- W2915397710 hasAuthorship W2915397710A5045208440 @default.
- W2915397710 hasAuthorship W2915397710A5061482160 @default.
- W2915397710 hasAuthorship W2915397710A5085763615 @default.
- W2915397710 hasBestOaLocation W29153977101 @default.
- W2915397710 hasConcept C120665830 @default.
- W2915397710 hasConcept C121332964 @default.
- W2915397710 hasConcept C135041427 @default.
- W2915397710 hasConcept C184665706 @default.
- W2915397710 hasConcept C207297109 @default.
- W2915397710 hasConcept C33024259 @default.
- W2915397710 hasConcept C44870925 @default.
- W2915397710 hasConcept C68498078 @default.
- W2915397710 hasConcept C85725439 @default.
- W2915397710 hasConcept C98444146 @default.
- W2915397710 hasConceptScore W2915397710C120665830 @default.
- W2915397710 hasConceptScore W2915397710C121332964 @default.
- W2915397710 hasConceptScore W2915397710C135041427 @default.
- W2915397710 hasConceptScore W2915397710C184665706 @default.
- W2915397710 hasConceptScore W2915397710C207297109 @default.
- W2915397710 hasConceptScore W2915397710C33024259 @default.
- W2915397710 hasConceptScore W2915397710C44870925 @default.
- W2915397710 hasConceptScore W2915397710C68498078 @default.
- W2915397710 hasConceptScore W2915397710C85725439 @default.
- W2915397710 hasConceptScore W2915397710C98444146 @default.
- W2915397710 hasFunder F4320320006 @default.
- W2915397710 hasIssue "1" @default.
- W2915397710 hasLocation W29153977101 @default.
- W2915397710 hasLocation W29153977102 @default.