FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100612386> ?p ?o ?g. }

• W3100612386 endingPage "43" @default.
• W3100612386 startingPage "43" @default.
• W3100612386 abstract "We present a general framework for incorporating astrophysical information into Bayesian parameter estimation techniques used by gravitational wave data analysis to facilitate multi-messenger astronomy. Since the progenitors of transient gravitational wave events, such as compact binary coalescences, are likely to be associated with a host galaxy, improvements to the source sky location estimates through the use of host galaxy information are explored. To demonstrate how host galaxy properties can be included, we simulate a population of compact binary coalescences and show that for ∼8.5% of simulations within 200 Mpc, the top 10 most likely galaxies account for a ∼50% of the total probability of hosting a gravitational wave source. The true gravitational wave source host galaxy is in the top 10 galaxy candidates ∼10% of the time. Furthermore, we show that by including host galaxy information, a better estimate of the inclination angle of a compact binary gravitational wave source can be obtained. We also demonstrate the flexibility of our method by incorporating the use of either the B or K band into our analysis." @default.
• W3100612386 created "2020-11-23" @default.
• W3100612386 creator A5026870642 @default.
• W3100612386 creator A5038272398 @default.
• W3100612386 creator A5086586889 @default.
• W3100612386 date "2014-10-13" @default.
• W3100612386 modified "2023-10-03" @default.
• W3100612386 title "A BAYESIAN APPROACH TO MULTI-MESSENGER ASTRONOMY: IDENTIFICATION OF GRAVITATIONAL-WAVE HOST GALAXIES" @default.
• W3100612386 cites W1553648889 @default.
• W3100612386 cites W1851157365 @default.
• W3100612386 cites W1963750967 @default.
• W3100612386 cites W1965356879 @default.
• W3100612386 cites W1970091694 @default.
• W3100612386 cites W1974046066 @default.
• W3100612386 cites W1996706920 @default.
• W3100612386 cites W2005280645 @default.
• W3100612386 cites W2008831524 @default.
• W3100612386 cites W2011215868 @default.
• W3100612386 cites W2012291066 @default.
• W3100612386 cites W2015058037 @default.
• W3100612386 cites W2029083557 @default.
• W3100612386 cites W2031941608 @default.
• W3100612386 cites W2033202457 @default.
• W3100612386 cites W2036809080 @default.
• W3100612386 cites W2037953664 @default.
• W3100612386 cites W2041673535 @default.
• W3100612386 cites W2045527130 @default.
• W3100612386 cites W2049176663 @default.
• W3100612386 cites W2070203621 @default.
• W3100612386 cites W2071998148 @default.
• W3100612386 cites W2078907077 @default.
• W3100612386 cites W2081587002 @default.
• W3100612386 cites W2082865060 @default.
• W3100612386 cites W2084955838 @default.
• W3100612386 cites W2086503365 @default.
• W3100612386 cites W2087010948 @default.
• W3100612386 cites W2090334442 @default.
• W3100612386 cites W2090568279 @default.
• W3100612386 cites W2103373677 @default.
• W3100612386 cites W2104950841 @default.
• W3100612386 cites W2107350153 @default.
• W3100612386 cites W2112587052 @default.
• W3100612386 cites W2125317842 @default.
• W3100612386 cites W2126450676 @default.
• W3100612386 cites W2141120919 @default.
• W3100612386 cites W2148010487 @default.
• W3100612386 cites W2150995848 @default.
• W3100612386 cites W2159546027 @default.
• W3100612386 cites W2160753031 @default.
• W3100612386 cites W2963509052 @default.
• W3100612386 cites W2964340496 @default.
• W3100612386 cites W2978278853 @default.
• W3100612386 cites W3098220822 @default.
• W3100612386 cites W3098553117 @default.
• W3100612386 cites W3099316544 @default.
• W3100612386 cites W3101445189 @default.
• W3100612386 cites W3102649643 @default.
• W3100612386 cites W3103365574 @default.
• W3100612386 cites W3103494666 @default.
• W3100612386 cites W3104042284 @default.
• W3100612386 cites W3105278005 @default.
• W3100612386 cites W3106265194 @default.
• W3100612386 cites W3121560983 @default.
• W3100612386 cites W3123262349 @default.
• W3100612386 cites W3123605675 @default.
• W3100612386 cites W3123661811 @default.
• W3100612386 cites W4233096186 @default.
• W3100612386 cites W2123016013 @default.
• W3100612386 doi "https://doi.org/10.1088/0004-637x/795/1/43" @default.
• W3100612386 hasPublicationYear "2014" @default.
• W3100612386 type Work @default.
• W3100612386 sameAs 3100612386 @default.
• W3100612386 citedByCount "42" @default.
• W3100612386 countsByYear W31006123862014 @default.
• W3100612386 countsByYear W31006123862015 @default.
• W3100612386 countsByYear W31006123862016 @default.
• W3100612386 countsByYear W31006123862017 @default.
• W3100612386 countsByYear W31006123862018 @default.
• W3100612386 countsByYear W31006123862019 @default.
• W3100612386 countsByYear W31006123862020 @default.
• W3100612386 countsByYear W31006123862021 @default.
• W3100612386 countsByYear W31006123862022 @default.
• W3100612386 countsByYear W31006123862023 @default.
• W3100612386 crossrefType "journal-article" @default.
• W3100612386 hasAuthorship W3100612386A5026870642 @default.
• W3100612386 hasAuthorship W3100612386A5038272398 @default.
• W3100612386 hasAuthorship W3100612386A5086586889 @default.
• W3100612386 hasBestOaLocation W31006123862 @default.
• W3100612386 hasConcept C121332964 @default.
• W3100612386 hasConcept C1276947 @default.
• W3100612386 hasConcept C144024400 @default.
• W3100612386 hasConcept C149923435 @default.
• W3100612386 hasConcept C174802034 @default.
• W3100612386 hasConcept C190330329 @default.
• W3100612386 hasConcept C205327720 @default.
• W3100612386 hasConcept C2908647359 @default.
• W3100612386 hasConcept C44870925 @default.
• W3100612386 hasConcept C98444146 @default.

• next