Finding high-redshift gamma-ray bursts in tandem near-infrared and optical surveys

被引：0
|
作者：
S. Campana
G. Ghirlanda
R. Salvaterra
O. A. Gonzalez
M. Landoni
G. Pariani
A. Riva
M. Riva
S. J. Smartt
N. R. Tanvir
S. D. Vergani
机构：
[1] INAF,STFC UK Astronomy Technology Centre
[2] Osservatorio astronomico di Brera,Astrophysics Research Centre, School of Mathematics and Physics
[3] INFN,School of Physics and Astronomy
[4] Sezione di Milano-Bicocca,GEPI, Observatoire de Paris
[5] INAF,undefined
[6] Istituto di Astrofisica Spaziale e Fisica cosmica,undefined
[7] The Royal Observatory,undefined
[8] INAF,undefined
[9] Osservatorio astrofisico di Torino,undefined
[10] Queen’s University Belfast,undefined
[11] University of Leicester,undefined
[12] PSL University,undefined
[13] CNRS,undefined
来源：
Nature Astronomy | 2022年 / 6卷
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摘要：
Gamma-ray bursts are linked to the most distant objects in the Universe, but detecting them is a rare event. With a dedicated near-infrared telescope to observe in tandem with the optical Vera Rubin Observatory, ten or so high-redshift (z ≳ 6) gamma-ray bursts could potentially be detected every year.
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页码：1101 / 1104
页数：3
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