FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1618343387> ?p ?o ?g. }

• W1618343387 endingPage "92" @default.
• W1618343387 startingPage "92" @default.
• W1618343387 abstract "ABSTRACT We present a method to constrain galaxy parameters directly from three-dimensional data cubes. The algorithm compares directly the data with a parametric model mapped in <?CDATA $x,y,lambda $?> <?MML <mml:math> <mml:mi>x</mml:mi> <mml:mo>,</mml:mo> <mml:mi>y</mml:mi> <mml:mo>,</mml:mo> <mml:mi>λ</mml:mi> </mml:math>?> coordinates. It uses the spectral line-spread function and the spatial point-spread function (PSF) to generate a three-dimensional kernel whose characteristics are instrument specific or user generated. The algorithm returns the intrinsic modeled properties along with both an “intrinsic” model data cube and the modeled galaxy convolved with the 3D kernel. The algorithm uses a Markov Chain Monte Carlo approach with a nontraditional proposal distribution in order to efficiently probe the parameter space. We demonstrate the robustness of the algorithm using 1728 mock galaxies and galaxies generated from hydrodynamical simulations in various seeing conditions from 0.″6 to 1.″2. We find that the algorithm can recover the morphological parameters (inclination, position angle) to within 10% and the kinematic parameters (maximum rotation velocity) to within 20%, irrespectively of the PSF in seeing (up to 1.″2) provided that the maximum signal-to-noise ratio (S/N) is greater than ∼3 pixel −1 and that the ratio of galaxy half-light radius to seeing radius is greater than about 1.5. One can use such an algorithm to constrain simultaneously the kinematics and morphological parameters of (nonmerging) galaxies observed in nonoptimal seeing conditions. The algorithm can also be used on adaptive optics data or on high-quality, high-S/N data to look for nonaxisymmetric structures in the residuals." @default.
• W1618343387 created "2016-06-24" @default.
• W1618343387 creator A5022894838 @default.
• W1618343387 creator A5027516481 @default.
• W1618343387 creator A5053050177 @default.
• W1618343387 creator A5068252137 @default.
• W1618343387 creator A5088924579 @default.
• W1618343387 date "2015-08-27" @default.
• W1618343387 modified "2023-09-30" @default.
• W1618343387 title "GalPaK^3D: A BAYESIAN PARAMETRIC TOOL FOR EXTRACTING MORPHOKINEMATICS OF GALAXIES FROM 3D DATA" @default.
• W1618343387 cites W1820140616 @default.
• W1618343387 cites W1970587228 @default.
• W1618343387 cites W1979829845 @default.
• W1618343387 cites W1990491187 @default.
• W1618343387 cites W1997010649 @default.
• W1618343387 cites W2003243598 @default.
• W1618343387 cites W2003264328 @default.
• W1618343387 cites W2016189541 @default.
• W1618343387 cites W2019198220 @default.
• W1618343387 cites W2043544014 @default.
• W1618343387 cites W2057816597 @default.
• W1618343387 cites W2064064569 @default.
• W1618343387 cites W2065560654 @default.
• W1618343387 cites W2066675108 @default.
• W1618343387 cites W2071741925 @default.
• W1618343387 cites W2079227246 @default.
• W1618343387 cites W2081425105 @default.
• W1618343387 cites W2096000415 @default.
• W1618343387 cites W2101942176 @default.
• W1618343387 cites W2105927762 @default.
• W1618343387 cites W2110198441 @default.
• W1618343387 cites W2117060658 @default.
• W1618343387 cites W2117962806 @default.
• W1618343387 cites W2132745107 @default.
• W1618343387 cites W2135296228 @default.
• W1618343387 cites W2138309709 @default.
• W1618343387 cites W2141003628 @default.
• W1618343387 cites W2146434002 @default.
• W1618343387 cites W2154481929 @default.
• W1618343387 cites W2154762550 @default.
• W1618343387 cites W2157389393 @default.
• W1618343387 cites W2188589973 @default.
• W1618343387 cites W2789944975 @default.
• W1618343387 cites W2949396216 @default.
• W1618343387 cites W3098183032 @default.
• W1618343387 cites W3100206188 @default.
• W1618343387 cites W3100340969 @default.
• W1618343387 cites W3100427722 @default.
• W1618343387 cites W3100753765 @default.
• W1618343387 cites W3102467437 @default.
• W1618343387 cites W3103488511 @default.
• W1618343387 cites W3103868583 @default.
• W1618343387 cites W3105535190 @default.
• W1618343387 cites W3106221437 @default.
• W1618343387 cites W3106322441 @default.
• W1618343387 cites W3106327842 @default.
• W1618343387 cites W3121302146 @default.
• W1618343387 cites W3122334058 @default.
• W1618343387 cites W3123966025 @default.
• W1618343387 cites W3124945482 @default.
• W1618343387 cites W3126143209 @default.
• W1618343387 cites W4289815557 @default.
• W1618343387 cites W4293241892 @default.
• W1618343387 cites W4295094139 @default.
• W1618343387 cites W4301011223 @default.
• W1618343387 doi "https://doi.org/10.1088/0004-6256/150/3/92" @default.
• W1618343387 hasPublicationYear "2015" @default.
• W1618343387 type Work @default.
• W1618343387 sameAs 1618343387 @default.
• W1618343387 citedByCount "90" @default.
• W1618343387 countsByYear W16183433872015 @default.
• W1618343387 countsByYear W16183433872016 @default.
• W1618343387 countsByYear W16183433872017 @default.
• W1618343387 countsByYear W16183433872018 @default.
• W1618343387 countsByYear W16183433872019 @default.
• W1618343387 countsByYear W16183433872020 @default.
• W1618343387 countsByYear W16183433872021 @default.
• W1618343387 countsByYear W16183433872022 @default.
• W1618343387 countsByYear W16183433872023 @default.
• W1618343387 crossrefType "journal-article" @default.
• W1618343387 hasAuthorship W1618343387A5022894838 @default.
• W1618343387 hasAuthorship W1618343387A5027516481 @default.
• W1618343387 hasAuthorship W1618343387A5053050177 @default.
• W1618343387 hasAuthorship W1618343387A5068252137 @default.
• W1618343387 hasAuthorship W1618343387A5088924579 @default.
• W1618343387 hasBestOaLocation W16183433871 @default.
• W1618343387 hasConcept C11413529 @default.
• W1618343387 hasConcept C121332964 @default.
• W1618343387 hasConcept C41008148 @default.
• W1618343387 hasConcept C44870925 @default.
• W1618343387 hasConcept C98444146 @default.
• W1618343387 hasConceptScore W1618343387C11413529 @default.
• W1618343387 hasConceptScore W1618343387C121332964 @default.
• W1618343387 hasConceptScore W1618343387C41008148 @default.
• W1618343387 hasConceptScore W1618343387C44870925 @default.
• W1618343387 hasConceptScore W1618343387C98444146 @default.
• W1618343387 hasIssue "3" @default.
• W1618343387 hasLocation W16183433871 @default.

• next