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- W2016271714 abstract "The distances of about thirty gamma-ray bursts (GRBs) are known. The most remote one is at |$z sim 4.5$|, and the remaining more dimmer GRBs are supposed to be more remote. If we can estimate the distances for the dimmer GRBs, their distances should be much beyond |$z sim 4.5$|. Two independent studies to estimate their distances were previously conducted. One was based on the variability–luminosity relation, and the other was based on the lag–luminosity relation. However, these relations can apply only for a very limited range of luminosity. In this paper, we introduce the viewing angles and use a new lag-luminosity relation by Ioka and Nakamura (2001, ApJ, 554, L163), which is capable of explaining the luminosity of the nearest GRBs. By applying the new relation, we infer the star-formation history out to |$z sim 4$|. Our result shows an increasing trend of star-formation out to |$z sim 4$|. However, the lag–luminosity relation itself is still a matter of debate, and thus this work is a tentative approach. For example, we have used only eight known GRB distances. Our result should be checked and calibrated by future data with Swift, observing more distant GRBs." @default.
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- W2016271714 date "2003-10-25" @default.
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- W2016271714 title "One Approach to the Star-Formation History Inferred from the GRB Lag–Luminosity Relation" @default.
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- W2016271714 doi "https://doi.org/10.1093/pasj/55.5.l65" @default.
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