FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2059720487> ?p ?o ?g. }

• W2059720487 endingPage "9" @default.
• W2059720487 startingPage "1" @default.
• W2059720487 abstract "Following the successful mapping of the last scattering surface by the Wilkinson Microwave Anisotropy Probe (WMAP) and balloon experiments, the epoch of the first stars, when Population III stars formed, is emerging as the next cosmological frontier. It is not clear what these stars' properties were, when they formed, or how long their era lasted before leading to the stars and galaxies we see today. We show that these questions can be answered with the current and future measurements of the near-IR cosmic infrared background (CIB). Theoretical arguments suggest that Population III stars were very massive and short-lived stars that formed at z ~ 10-20 at rare peaks of the density field in the cold dark matter universe. Because Population III stars probably formed individually in small minihalos, they are not directly accessible to current telescopic studies. We show that these stars left a strong and measurable signature via their contribution to the CIB anisotropies for a wide range of their formation scenarios. The excess in the recently measured near-IR CIB anisotropies over that from normal galaxies can be explained by contribution from early Population III stars. These results imply that Population III were indeed very massive stars and that their epoch started at z ~ 20 and lasted past z ≲ 13. We show the importance of accurately measuring the CIB anisotropies produced by Population III with future space-based missions." @default.
• W2059720487 created "2016-06-24" @default.
• W2059720487 creator A5002625236 @default.
• W2059720487 creator A5031668992 @default.
• W2059720487 creator A5033500112 @default.
• W2059720487 creator A5059751886 @default.
• W2059720487 creator A5065163729 @default.
• W2059720487 date "2004-06-10" @default.
• W2059720487 modified "2023-10-01" @default.
• W2059720487 title "Detecting Population III Stars through Observations of Near‐Infrared Cosmic Infrared Background Anisotropies" @default.
• W2059720487 cites W1574701543 @default.
• W2059720487 cites W1588757845 @default.
• W2059720487 cites W1973368884 @default.
• W2059720487 cites W1974315074 @default.
• W2059720487 cites W1980514159 @default.
• W2059720487 cites W1980980788 @default.
• W2059720487 cites W1981046231 @default.
• W2059720487 cites W1984040414 @default.
• W2059720487 cites W1991026568 @default.
• W2059720487 cites W1995692817 @default.
• W2059720487 cites W2004168059 @default.
• W2059720487 cites W2019428480 @default.
• W2059720487 cites W2019771205 @default.
• W2059720487 cites W2020818391 @default.
• W2059720487 cites W2040488255 @default.
• W2059720487 cites W2040912209 @default.
• W2059720487 cites W2046952294 @default.
• W2059720487 cites W2053020072 @default.
• W2059720487 cites W2058983697 @default.
• W2059720487 cites W2062612172 @default.
• W2059720487 cites W2063051150 @default.
• W2059720487 cites W2065341238 @default.
• W2059720487 cites W2067181265 @default.
• W2059720487 cites W2075512945 @default.
• W2059720487 cites W2075884494 @default.
• W2059720487 cites W2086540357 @default.
• W2059720487 cites W2089820345 @default.
• W2059720487 cites W2094234733 @default.
• W2059720487 cites W2132802601 @default.
• W2059720487 cites W2134761558 @default.
• W2059720487 cites W2139503450 @default.
• W2059720487 cites W2140478436 @default.
• W2059720487 cites W2155711232 @default.
• W2059720487 cites W2159347590 @default.
• W2059720487 cites W2951034677 @default.
• W2059720487 cites W2951581092 @default.
• W2059720487 cites W3098003348 @default.
• W2059720487 cites W3098510299 @default.
• W2059720487 cites W3099112362 @default.
• W2059720487 cites W3099755318 @default.
• W2059720487 cites W3102398196 @default.
• W2059720487 cites W3104104726 @default.
• W2059720487 cites W3104870036 @default.
• W2059720487 cites W3105082704 @default.
• W2059720487 doi "https://doi.org/10.1086/386365" @default.
• W2059720487 hasPublicationYear "2004" @default.
• W2059720487 type Work @default.
• W2059720487 sameAs 2059720487 @default.
• W2059720487 citedByCount "78" @default.
• W2059720487 countsByYear W20597204872012 @default.
• W2059720487 countsByYear W20597204872013 @default.
• W2059720487 countsByYear W20597204872014 @default.
• W2059720487 countsByYear W20597204872015 @default.
• W2059720487 countsByYear W20597204872016 @default.
• W2059720487 countsByYear W20597204872017 @default.
• W2059720487 countsByYear W20597204872018 @default.
• W2059720487 countsByYear W20597204872019 @default.
• W2059720487 countsByYear W20597204872020 @default.
• W2059720487 countsByYear W20597204872021 @default.
• W2059720487 countsByYear W20597204872022 @default.
• W2059720487 countsByYear W20597204872023 @default.
• W2059720487 crossrefType "journal-article" @default.
• W2059720487 hasAuthorship W2059720487A5002625236 @default.
• W2059720487 hasAuthorship W2059720487A5031668992 @default.
• W2059720487 hasAuthorship W2059720487A5033500112 @default.
• W2059720487 hasAuthorship W2059720487A5059751886 @default.
• W2059720487 hasAuthorship W2059720487A5065163729 @default.
• W2059720487 hasBestOaLocation W20597204871 @default.
• W2059720487 hasConcept C121332964 @default.
• W2059720487 hasConcept C1276947 @default.
• W2059720487 hasConcept C144024400 @default.
• W2059720487 hasConcept C149923435 @default.
• W2059720487 hasConcept C150846664 @default.
• W2059720487 hasConcept C207297109 @default.
• W2059720487 hasConcept C2908647359 @default.
• W2059720487 hasConcept C33024259 @default.
• W2059720487 hasConcept C44870925 @default.
• W2059720487 hasConcept C60318249 @default.
• W2059720487 hasConcept C62520636 @default.
• W2059720487 hasConcept C69672822 @default.
• W2059720487 hasConcept C85725439 @default.
• W2059720487 hasConcept C87485669 @default.
• W2059720487 hasConcept C98444146 @default.
• W2059720487 hasConceptScore W2059720487C121332964 @default.
• W2059720487 hasConceptScore W2059720487C1276947 @default.
• W2059720487 hasConceptScore W2059720487C144024400 @default.
• W2059720487 hasConceptScore W2059720487C149923435 @default.
• W2059720487 hasConceptScore W2059720487C150846664 @default.

• next