FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2790802271> ?p ?o ?g. }

• W2790802271 endingPage "4371" @default.
• W2790802271 startingPage "4362" @default.
• W2790802271 abstract "To study the full formation and evolution history of galaxy clusters and their population, high resolution simulations of the latter are flourishing. However comparing observed clusters to the simulated ones on a one-to-one basis to refine the models and theories down to the details is non trivial. The large variety of clusters limits the comparisons between observed and numerical clusters. Simulations resembling the local Universe down to the cluster scales permit pushing the limit. Simulated and observed clusters can be matched on a one-to-one basis for direct comparisons provided that clusters are well reproduced besides being in the proper large scale environment. Comparing random and local-Universe like simulations obtained with differently grouped observational catalogs of peculiar velocities, this paper shows that the grouping scheme used to remove non-linear motions in the catalogs that constrain the simulations affects the quality of the numerical clusters. With a less aggressive grouping scheme - galaxies still falling onto clusters are preserved - combined with a bias minimization scheme, the mass of the dark matter halos, simulacra for 5 local clusters - Virgo, Centaurus, Coma, Hydra and Perseus - is increased by 39% closing the gap with observational mass estimates. Simulacra are found on average in 89% of the simulations, an increase of 5% with respect to the previous grouping scheme. The only exception is Perseus. Since the Perseus-Pisces region is not well covered by the used peculiar velocity catalog, the latest release let us foresee a better simulacrum for Perseus in a near future." @default.
• W2790802271 created "2018-03-29" @default.
• W2790802271 creator A5005644291 @default.
• W2790802271 creator A5050368575 @default.
• W2790802271 date "2018-03-03" @default.
• W2790802271 modified "2023-10-18" @default.
• W2790802271 title "Galaxy clusters in simulations of the local Universe: a matter of constraints" @default.
• W2790802271 cites W1479809817 @default.
• W2790802271 cites W1821343735 @default.
• W2790802271 cites W1947575852 @default.
• W2790802271 cites W1947909385 @default.
• W2790802271 cites W1954069964 @default.
• W2790802271 cites W1984631803 @default.
• W2790802271 cites W1996528251 @default.
• W2790802271 cites W2000265182 @default.
• W2790802271 cites W2006547515 @default.
• W2790802271 cites W2013403927 @default.
• W2790802271 cites W2019511225 @default.
• W2790802271 cites W2024149319 @default.
• W2790802271 cites W2024931169 @default.
• W2790802271 cites W2031263070 @default.
• W2790802271 cites W2042956136 @default.
• W2790802271 cites W2045026061 @default.
• W2790802271 cites W2048990175 @default.
• W2790802271 cites W2049203344 @default.
• W2790802271 cites W2049317540 @default.
• W2790802271 cites W2057332312 @default.
• W2790802271 cites W2062513449 @default.
• W2790802271 cites W2069557863 @default.
• W2790802271 cites W2069944955 @default.
• W2790802271 cites W2089311248 @default.
• W2790802271 cites W2089374432 @default.
• W2790802271 cites W2093969344 @default.
• W2790802271 cites W2113391777 @default.
• W2790802271 cites W2128759530 @default.
• W2790802271 cites W2139937287 @default.
• W2790802271 cites W2159478752 @default.
• W2790802271 cites W2162210948 @default.
• W2790802271 cites W2163090913 @default.
• W2790802271 cites W2180808049 @default.
• W2790802271 cites W2214077841 @default.
• W2790802271 cites W2227479743 @default.
• W2790802271 cites W2228605776 @default.
• W2790802271 cites W2234483448 @default.
• W2790802271 cites W2259792253 @default.
• W2790802271 cites W2286741996 @default.
• W2790802271 cites W2401966916 @default.
• W2790802271 cites W2418259467 @default.
• W2790802271 cites W2511441103 @default.
• W2790802271 cites W2515276161 @default.
• W2790802271 cites W2521336726 @default.
• W2790802271 cites W2586930307 @default.
• W2790802271 cites W2592842931 @default.
• W2790802271 cites W2612531948 @default.
• W2790802271 cites W2964217547 @default.
• W2790802271 cites W3037484794 @default.
• W2790802271 cites W3098221464 @default.
• W2790802271 cites W3098588194 @default.
• W2790802271 cites W3099020808 @default.
• W2790802271 cites W3099469494 @default.
• W2790802271 cites W3099469848 @default.
• W2790802271 cites W3100655566 @default.
• W2790802271 cites W3101168514 @default.
• W2790802271 cites W3101584731 @default.
• W2790802271 cites W3103048770 @default.
• W2790802271 cites W3103093820 @default.
• W2790802271 cites W3104019486 @default.
• W2790802271 cites W3105439606 @default.
• W2790802271 cites W3105813593 @default.
• W2790802271 cites W3105900570 @default.
• W2790802271 cites W3125501372 @default.
• W2790802271 doi "https://doi.org/10.1093/mnras/sty505" @default.
• W2790802271 hasPublicationYear "2018" @default.
• W2790802271 type Work @default.
• W2790802271 sameAs 2790802271 @default.
• W2790802271 citedByCount "15" @default.
• W2790802271 countsByYear W27908022712018 @default.
• W2790802271 countsByYear W27908022712019 @default.
• W2790802271 countsByYear W27908022712020 @default.
• W2790802271 countsByYear W27908022712022 @default.
• W2790802271 countsByYear W27908022712023 @default.
• W2790802271 crossrefType "journal-article" @default.
• W2790802271 hasAuthorship W2790802271A5005644291 @default.
• W2790802271 hasAuthorship W2790802271A5050368575 @default.
• W2790802271 hasBestOaLocation W27908022714 @default.
• W2790802271 hasConcept C121332964 @default.
• W2790802271 hasConcept C1276947 @default.
• W2790802271 hasConcept C144024400 @default.
• W2790802271 hasConcept C149923435 @default.
• W2790802271 hasConcept C156055797 @default.
• W2790802271 hasConcept C159249277 @default.
• W2790802271 hasConcept C164866538 @default.
• W2790802271 hasConcept C199360897 @default.
• W2790802271 hasConcept C2908647359 @default.
• W2790802271 hasConcept C41008148 @default.
• W2790802271 hasConcept C44870925 @default.
• W2790802271 hasConcept C83160514 @default.
• W2790802271 hasConcept C84999194 @default.

• next