Matches in SemOpenAlex for { <https://semopenalex.org/work/W2103496122> ?p ?o ?g. }
- W2103496122 endingPage "125" @default.
- W2103496122 startingPage "125" @default.
- W2103496122 abstract "We present the first study to synthesize results from five different exoplanet surveys using three independent detection methods: microlensing, radial velocity, and direct imaging. The constraints derived herein represent the most comprehensive picture of the demographics of large-separation (>~ 2 AU) planets orbiting the most common stars in our Galaxy that has been constructed to date. We assume a simple, joint power-law planet distribution function of the form d^2N_{pl}/[dlog(m_p)dlog(a)] = A(m_p/M_{Sat})^{alpha}(a/2.5 AU)^{beta} with an outer cutoff radius of the separation distribution function of a_{out}. Generating populations of planets from these models and mapping them into the relevant observables for each survey, we use actual or estimated detection sensitivities to determine the expected observations for each survey. Comparing with the reported results, we derive constraints on the parameters {alpha, beta, A, a_{out}} that describe a single population of planets that is simultaneously consistent with the results of microlensing, RV, and direct imaging surveys. We find median and 68% confindence intervals of alpha = -0.86^{+0.21}_{-0.19} (-0.85^{+0.21}_{-0.19}), beta = 1.1^{+1.9}_{-1.4} (1.1^{+1.9}_{-1.3}), A = 0.21^{+0.20}_{-0.15} dex^{-2} (0.21^{+0.20}_{-0.15} dex^{-2}), and a_{out} = 10^{+26}_{-4.7} AU (12^{+50}_{-6.2} AU) assuming hot-start (cold-start) planet evolutionary models. These values are consistent with all current knowledge of planets on orbits beyond ~2 AU around M dwarfs." @default.
- W2103496122 created "2016-06-24" @default.
- W2103496122 creator A5070040153 @default.
- W2103496122 creator A5088539346 @default.
- W2103496122 date "2016-03-08" @default.
- W2103496122 modified "2023-09-27" @default.
- W2103496122 title "SYNTHESIZING EXOPLANET DEMOGRAPHICS: A SINGLE POPULATION OF LONG-PERIOD PLANETARY COMPANIONS TO M DWARFS CONSISTENT WITH MICROLENSING, RADIAL VELOCITY, AND DIRECT IMAGING SURVEYS" @default.
- W2103496122 cites W1966079298 @default.
- W2103496122 cites W1966393173 @default.
- W2103496122 cites W1979896643 @default.
- W2103496122 cites W1995011483 @default.
- W2103496122 cites W2001265656 @default.
- W2103496122 cites W2002702371 @default.
- W2103496122 cites W2008059488 @default.
- W2103496122 cites W2008129175 @default.
- W2103496122 cites W2012898691 @default.
- W2103496122 cites W2023276174 @default.
- W2103496122 cites W2023856858 @default.
- W2103496122 cites W2024770774 @default.
- W2103496122 cites W2026840775 @default.
- W2103496122 cites W2043836523 @default.
- W2103496122 cites W2045109688 @default.
- W2103496122 cites W2047712469 @default.
- W2103496122 cites W2049884523 @default.
- W2103496122 cites W2056968313 @default.
- W2103496122 cites W2059365121 @default.
- W2103496122 cites W2066481832 @default.
- W2103496122 cites W2083250837 @default.
- W2103496122 cites W2101871480 @default.
- W2103496122 cites W2102759231 @default.
- W2103496122 cites W2106752330 @default.
- W2103496122 cites W2119029888 @default.
- W2103496122 cites W2122383266 @default.
- W2103496122 cites W2130979480 @default.
- W2103496122 cites W2133775827 @default.
- W2103496122 cites W2136840156 @default.
- W2103496122 cites W2140137154 @default.
- W2103496122 cites W2140881079 @default.
- W2103496122 cites W2150756303 @default.
- W2103496122 cites W2159561097 @default.
- W2103496122 cites W2159697822 @default.
- W2103496122 cites W2160869102 @default.
- W2103496122 cites W2162210754 @default.
- W2103496122 cites W2162975616 @default.
- W2103496122 cites W2166068066 @default.
- W2103496122 cites W2170750689 @default.
- W2103496122 cites W2177545076 @default.
- W2103496122 cites W2200601985 @default.
- W2103496122 cites W3022668787 @default.
- W2103496122 cites W3098134353 @default.
- W2103496122 cites W3099143351 @default.
- W2103496122 cites W3099146730 @default.
- W2103496122 cites W3099230470 @default.
- W2103496122 cites W3099569883 @default.
- W2103496122 cites W3099896971 @default.
- W2103496122 cites W3100312073 @default.
- W2103496122 cites W3100446832 @default.
- W2103496122 cites W3101298061 @default.
- W2103496122 cites W3101689680 @default.
- W2103496122 cites W3102119723 @default.
- W2103496122 cites W3102487611 @default.
- W2103496122 cites W3102938219 @default.
- W2103496122 cites W3104853564 @default.
- W2103496122 cites W3105649543 @default.
- W2103496122 cites W3105657417 @default.
- W2103496122 cites W3105667095 @default.
- W2103496122 cites W4237977832 @default.
- W2103496122 cites W4292310538 @default.
- W2103496122 doi "https://doi.org/10.3847/0004-637x/819/2/125" @default.
- W2103496122 hasPublicationYear "2016" @default.
- W2103496122 type Work @default.
- W2103496122 sameAs 2103496122 @default.
- W2103496122 citedByCount "86" @default.
- W2103496122 countsByYear W21034961222016 @default.
- W2103496122 countsByYear W21034961222017 @default.
- W2103496122 countsByYear W21034961222018 @default.
- W2103496122 countsByYear W21034961222019 @default.
- W2103496122 countsByYear W21034961222020 @default.
- W2103496122 countsByYear W21034961222021 @default.
- W2103496122 countsByYear W21034961222022 @default.
- W2103496122 countsByYear W21034961222023 @default.
- W2103496122 crossrefType "journal-article" @default.
- W2103496122 hasAuthorship W2103496122A5070040153 @default.
- W2103496122 hasAuthorship W2103496122A5088539346 @default.
- W2103496122 hasBestOaLocation W21034961221 @default.
- W2103496122 hasConcept C100905312 @default.
- W2103496122 hasConcept C121332964 @default.
- W2103496122 hasConcept C125125069 @default.
- W2103496122 hasConcept C1276947 @default.
- W2103496122 hasConcept C144024400 @default.
- W2103496122 hasConcept C149923435 @default.
- W2103496122 hasConcept C150846664 @default.
- W2103496122 hasConcept C163479331 @default.
- W2103496122 hasConcept C178635117 @default.
- W2103496122 hasConcept C2780084366 @default.
- W2103496122 hasConcept C2908647359 @default.
- W2103496122 hasConcept C32848918 @default.
- W2103496122 hasConcept C38652104 @default.