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• W4220687620 endingPage "075102" @default.
• W4220687620 startingPage "075102" @default.
• W4220687620 abstract "Abstract The application of fast radio bursts (FRBs) as probes for investigating astrophysics and cosmology requires proper modelling of the dispersion measures of the Milky Way ( <?CDATA $ DM_{rm MW} $?> ) and host galaxy ( <?CDATA $ DM_{rm host} $?> ). <?CDATA $ DM_{rm MW} $?> can be estimated using the Milky Way electron models, such as the NE2001 model and YMW16 model. However, <?CDATA $ DM_{rm host} $?> is hard to model due to limited information on the local environment of the FRBs. In this study, using 17 well-localized FRBs, we search for possible correlations between <?CDATA $DM_{rm host} $?> and the properties of the host galaxies, such as the redshift, stellar mass, star-formation rate, age of galaxy, offset of the FRB site from the galactic center, and half-light radius. We find no strong correlation between <?CDATA $ DM_{rm host} $?> and any of the host properties. Assuming that <?CDATA $DM_{rm host} $?> is a constant for all host galaxies, we constrain the fraction of the baryon mass in the intergalactic medium today to be <?CDATA $ f_{rm IGM,0}=0.78_{-0.19}^{+0.15} $?> . If we model <?CDATA $ DM_{rm host} $?> as a log-normal distribution, however, we obtain a larger value, <?CDATA $ f_{rm IGM,0}= 0.83_{-0.17}^{+0.12} $?> . Based on the limited number of FRBs, no strong evidence for a redshift evolution of <?CDATA $ f_{rm IGM} $?> is found." @default.
• W4220687620 created "2022-04-03" @default.
• W4220687620 creator A5018449715 @default.
• W4220687620 creator A5027164510 @default.
• W4220687620 creator A5065772623 @default.
• W4220687620 date "2022-07-01" @default.
• W4220687620 modified "2023-09-27" @default.
• W4220687620 title "Search for correlations between host properties and DM _host of fast radio bursts: constraints on the baryon mass fraction in IGM *" @default.
• W4220687620 cites W1967094474 @default.
• W4220687620 cites W2036423640 @default.
• W4220687620 cites W2036639372 @default.
• W4220687620 cites W2042553000 @default.
• W4220687620 cites W2045912997 @default.
• W4220687620 cites W2078483536 @default.
• W4220687620 cites W2121795427 @default.
• W4220687620 cites W2201489770 @default.
• W4220687620 cites W2280104906 @default.
• W4220687620 cites W2288589145 @default.
• W4220687620 cites W2289905436 @default.
• W4220687620 cites W2296285603 @default.
• W4220687620 cites W2296660619 @default.
• W4220687620 cites W2347092838 @default.
• W4220687620 cites W2563744641 @default.
• W4220687620 cites W2571196594 @default.
• W4220687620 cites W2782530178 @default.
• W4220687620 cites W2885497170 @default.
• W4220687620 cites W2889445544 @default.
• W4220687620 cites W2913441758 @default.
• W4220687620 cites W2922352734 @default.
• W4220687620 cites W2940147897 @default.
• W4220687620 cites W2955902629 @default.
• W4220687620 cites W2982829710 @default.
• W4220687620 cites W2988203737 @default.
• W4220687620 cites W2997632089 @default.
• W4220687620 cites W3003668048 @default.
• W4220687620 cites W3016506979 @default.
• W4220687620 cites W3029501268 @default.
• W4220687620 cites W3030369513 @default.
• W4220687620 cites W3030414242 @default.
• W4220687620 cites W3088355124 @default.
• W4220687620 cites W3094691047 @default.
• W4220687620 cites W3098520916 @default.
• W4220687620 cites W3098764749 @default.
• W4220687620 cites W3099394385 @default.
• W4220687620 cites W3099453376 @default.
• W4220687620 cites W3099983421 @default.
• W4220687620 cites W3100040870 @default.
• W4220687620 cites W3100054713 @default.
• W4220687620 cites W3100196086 @default.
• W4220687620 cites W3100401081 @default.
• W4220687620 cites W3100513703 @default.
• W4220687620 cites W3100664724 @default.
• W4220687620 cites W3101090726 @default.
• W4220687620 cites W3101197687 @default.
• W4220687620 cites W3101263812 @default.
• W4220687620 cites W3101287716 @default.
• W4220687620 cites W3101338961 @default.
• W4220687620 cites W3101400699 @default.
• W4220687620 cites W3101536471 @default.
• W4220687620 cites W3101745821 @default.
• W4220687620 cites W3101879206 @default.
• W4220687620 cites W3102014803 @default.
• W4220687620 cites W3103255237 @default.
• W4220687620 cites W3103437717 @default.
• W4220687620 cites W3103969210 @default.
• W4220687620 cites W3103974490 @default.
• W4220687620 cites W3104025957 @default.
• W4220687620 cites W3104539364 @default.
• W4220687620 cites W3104552357 @default.
• W4220687620 cites W3104780305 @default.
• W4220687620 cites W3104987194 @default.
• W4220687620 cites W3105507702 @default.
• W4220687620 cites W3105602981 @default.
• W4220687620 cites W3105847478 @default.
• W4220687620 cites W3106016811 @default.
• W4220687620 cites W3106307049 @default.
• W4220687620 cites W3106323259 @default.
• W4220687620 cites W3106371390 @default.
• W4220687620 cites W3106373846 @default.
• W4220687620 cites W3110713537 @default.
• W4220687620 cites W3119143432 @default.
• W4220687620 cites W3132160370 @default.
• W4220687620 cites W3133559635 @default.
• W4220687620 cites W3135312907 @default.
• W4220687620 cites W3135543454 @default.
• W4220687620 cites W3140651708 @default.
• W4220687620 cites W3171329438 @default.
• W4220687620 cites W3183569244 @default.
• W4220687620 cites W3195222562 @default.
• W4220687620 cites W3202097581 @default.
• W4220687620 cites W3215502559 @default.
• W4220687620 cites W3217181905 @default.
• W4220687620 cites W4205650896 @default.
• W4220687620 cites W4205845447 @default.
• W4220687620 cites W4206329711 @default.
• W4220687620 cites W4226106036 @default.
• W4220687620 cites W4288079944 @default.
• W4220687620 doi "https://doi.org/10.1088/1674-1137/ac5e92" @default.

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