FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2023262283> ?p ?o ?g. }

• W2023262283 endingPage "L168" @default.
• W2023262283 startingPage "L163" @default.
• W2023262283 abstract "We present Advanced Camera for Surveys observations of MACSJ1149.5+2223, an X-ray luminous galaxy cluster at z=0.544 discovered by the Massive Cluster Survey. The data reveal at least seven multiply-imaged galaxies, three of which we have confirmed spectroscopically. One of these is a spectacular face-on spiral galaxy at z=1.491, the four images of which are gravitationally magnified by ~8<mu<~23. We identify this as an L* (M_B=-20.7), disk-dominated (B/T<~0.5) galaxy, forming stars at ~6Msol/yr. We use a robust sample of multiply-imaged galaxies to constrain a parameterized model of the cluster mass distribution. In addition to the main cluster dark matter halo and the bright cluster galaxies, our best model includes three galaxy-group-sized halos. The relative probability of this model is P(N_halo=4)/P(N_halo<4)>=10^12 where N_halo is the number of cluster/group-scale halos. In terms of sheer number of merging cluster/group-scale components, this is the most complex strong-lensing cluster core studied to date. The total cluster mass and fraction of that mass associated with substructures within R<=500kpc, are measured to be M_tot=(6.7+/-0.4)x10^14Msol and f_sub=0.25+/-0.12 respectively. Our model also rules out recent claims of a flat density profile at >~7sigma confidence, thus highlighting the critical importance of spectroscopic redshifts of multiply-imaged galaxies when modeling strong lensing clusters. Overall our results attest to the efficiency of X-ray selection in finding the most powerful cluster lenses, including complicated merging systems." @default.
• W2023262283 created "2016-06-24" @default.
• W2023262283 creator A5004193106 @default.
• W2023262283 creator A5022611236 @default.
• W2023262283 creator A5028898239 @default.
• W2023262283 creator A5035539608 @default.
• W2023262283 creator A5040248059 @default.
• W2023262283 creator A5042027319 @default.
• W2023262283 creator A5048025660 @default.
• W2023262283 creator A5048707483 @default.
• W2023262283 creator A5061818450 @default.
• W2023262283 creator A5064328569 @default.
• W2023262283 creator A5067307449 @default.
• W2023262283 creator A5080163935 @default.
• W2023262283 date "2009-12-07" @default.
• W2023262283 modified "2023-10-09" @default.
• W2023262283 title "<i>HUBBLE SPACE TELESCOPE</i> OBSERVATIONS OF A SPECTACULAR NEW STRONG-LENSING GALAXY CLUSTER: MACS J1149.5+2223 AT <i>z</i> = 0.544" @default.
• W2023262283 cites W1970754739 @default.
• W2023262283 cites W1977435885 @default.
• W2023262283 cites W1987312959 @default.
• W2023262283 cites W2022538907 @default.
• W2023262283 cites W2028471748 @default.
• W2023262283 cites W2039304323 @default.
• W2023262283 cites W2044093857 @default.
• W2023262283 cites W2053871165 @default.
• W2023262283 cites W2055520397 @default.
• W2023262283 cites W2062476095 @default.
• W2023262283 cites W2063734901 @default.
• W2023262283 cites W2068618869 @default.
• W2023262283 cites W2075739683 @default.
• W2023262283 cites W2087525524 @default.
• W2023262283 cites W2093456988 @default.
• W2023262283 cites W2101942176 @default.
• W2023262283 cites W2103038092 @default.
• W2023262283 cites W2106058713 @default.
• W2023262283 cites W2106221033 @default.
• W2023262283 cites W2111270537 @default.
• W2023262283 cites W2112796270 @default.
• W2023262283 cites W2116478593 @default.
• W2023262283 cites W2151173406 @default.
• W2023262283 cites W2151570583 @default.
• W2023262283 cites W2154669087 @default.
• W2023262283 cites W2155008346 @default.
• W2023262283 cites W3101182144 @default.
• W2023262283 cites W3102447698 @default.
• W2023262283 cites W3102810616 @default.
• W2023262283 cites W3103465215 @default.
• W2023262283 cites W3103868583 @default.
• W2023262283 cites W3103921369 @default.
• W2023262283 cites W3105163197 @default.
• W2023262283 cites W3121230951 @default.
• W2023262283 cites W3123764777 @default.
• W2023262283 cites W3125630950 @default.
• W2023262283 doi "https://doi.org/10.1088/0004-637x/707/2/l163" @default.
• W2023262283 hasPublicationYear "2009" @default.
• W2023262283 type Work @default.
• W2023262283 sameAs 2023262283 @default.
• W2023262283 citedByCount "100" @default.
• W2023262283 countsByYear W20232622832012 @default.
• W2023262283 countsByYear W20232622832013 @default.
• W2023262283 countsByYear W20232622832014 @default.
• W2023262283 countsByYear W20232622832015 @default.
• W2023262283 countsByYear W20232622832016 @default.
• W2023262283 countsByYear W20232622832017 @default.
• W2023262283 countsByYear W20232622832018 @default.
• W2023262283 countsByYear W20232622832019 @default.
• W2023262283 countsByYear W20232622832020 @default.
• W2023262283 countsByYear W20232622832021 @default.
• W2023262283 countsByYear W20232622832022 @default.
• W2023262283 countsByYear W20232622832023 @default.
• W2023262283 crossrefType "journal-article" @default.
• W2023262283 hasAuthorship W2023262283A5004193106 @default.
• W2023262283 hasAuthorship W2023262283A5022611236 @default.
• W2023262283 hasAuthorship W2023262283A5028898239 @default.
• W2023262283 hasAuthorship W2023262283A5035539608 @default.
• W2023262283 hasAuthorship W2023262283A5040248059 @default.
• W2023262283 hasAuthorship W2023262283A5042027319 @default.
• W2023262283 hasAuthorship W2023262283A5048025660 @default.
• W2023262283 hasAuthorship W2023262283A5048707483 @default.
• W2023262283 hasAuthorship W2023262283A5061818450 @default.
• W2023262283 hasAuthorship W2023262283A5064328569 @default.
• W2023262283 hasAuthorship W2023262283A5067307449 @default.
• W2023262283 hasAuthorship W2023262283A5080163935 @default.
• W2023262283 hasBestOaLocation W20232622831 @default.
• W2023262283 hasConcept C121332964 @default.
• W2023262283 hasConcept C1276947 @default.
• W2023262283 hasConcept C152268414 @default.
• W2023262283 hasConcept C156055797 @default.
• W2023262283 hasConcept C160147972 @default.
• W2023262283 hasConcept C164866538 @default.
• W2023262283 hasConcept C184665706 @default.
• W2023262283 hasConcept C199360897 @default.
• W2023262283 hasConcept C33024259 @default.
• W2023262283 hasConcept C41008148 @default.
• W2023262283 hasConcept C44870925 @default.
• W2023262283 hasConcept C98444146 @default.
• W2023262283 hasConceptScore W2023262283C121332964 @default.
• W2023262283 hasConceptScore W2023262283C1276947 @default.

• next