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A luminous fast radio burst that probes the Universe at redshift 1.

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Title: A luminous fast radio burst that probes the Universe at redshift 1.
Authors: Ryder, S. D., Bannister, K. W., Bhandari, S., Deller, A. T., Ekers, R. D., Glowacki, M., Gordon, A. C., Gourdji, K., James, C. W., Kilpatrick, C. D., Lu, W., Marnoch, L., Moss, V. A., Prochaska, J. X., Qiu, H., Sadler, E. M., Simha, S., Sammons, M. W., Scott, D. R., Tejos, N.
Source: Science (pre-March 2025). 10/20/2023, Vol. 382 Issue 6668, p294-299. 6p. 1 Color Photograph, 1 Diagram, 2 Graphs.
Subjects: Solar radio bursts, Interstellar medium, Redshift, Extragalactic distances, Plasma turbulence, Universe
Abstract: Fast radio bursts (FRBs) are millisecond-duration pulses of radio emission originating from extragalactic distances. Radio dispersion is imparted on each burst by intervening plasma, mostly located in the intergalactic medium. In this work, we observe the burst FRB 20220610A and localize it to a morphologically complex host galaxy system at redshift 1.016 ± 0.002. The burst redshift and dispersion measure are consistent with passage through a substantial column of plasma in the intergalactic medium and extend the relationship between those quantities measured at lower redshift. The burst shows evidence for passage through additional turbulent magnetized plasma, potentially associated with the host galaxy. We use the burst energy of 2 × 1042 erg to revise the empirical maximum energy of an FRB. [ABSTRACT FROM AUTHOR]
Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Psychology and Behavioral Sciences Collection
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  Data: A luminous fast radio burst that probes the Universe at redshift 1.
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  Data: <searchLink fieldCode="AR" term="%22Ryder%2C+S%2E+D%2E%22">Ryder, S. D.</searchLink><br /><searchLink fieldCode="AR" term="%22Bannister%2C+K%2E+W%2E%22">Bannister, K. W.</searchLink><br /><searchLink fieldCode="AR" term="%22Bhandari%2C+S%2E%22">Bhandari, S.</searchLink><br /><searchLink fieldCode="AR" term="%22Deller%2C+A%2E+T%2E%22">Deller, A. T.</searchLink><br /><searchLink fieldCode="AR" term="%22Ekers%2C+R%2E+D%2E%22">Ekers, R. D.</searchLink><br /><searchLink fieldCode="AR" term="%22Glowacki%2C+M%2E%22">Glowacki, M.</searchLink><br /><searchLink fieldCode="AR" term="%22Gordon%2C+A%2E+C%2E%22">Gordon, A. C.</searchLink><br /><searchLink fieldCode="AR" term="%22Gourdji%2C+K%2E%22">Gourdji, K.</searchLink><br /><searchLink fieldCode="AR" term="%22James%2C+C%2E+W%2E%22">James, C. W.</searchLink><br /><searchLink fieldCode="AR" term="%22Kilpatrick%2C+C%2E+D%2E%22">Kilpatrick, C. D.</searchLink><br /><searchLink fieldCode="AR" term="%22Lu%2C+W%2E%22">Lu, W.</searchLink><br /><searchLink fieldCode="AR" term="%22Marnoch%2C+L%2E%22">Marnoch, L.</searchLink><br /><searchLink fieldCode="AR" term="%22Moss%2C+V%2E+A%2E%22">Moss, V. A.</searchLink><br /><searchLink fieldCode="AR" term="%22Prochaska%2C+J%2E+X%2E%22">Prochaska, J. X.</searchLink><br /><searchLink fieldCode="AR" term="%22Qiu%2C+H%2E%22">Qiu, H.</searchLink><br /><searchLink fieldCode="AR" term="%22Sadler%2C+E%2E+M%2E%22">Sadler, E. M.</searchLink><br /><searchLink fieldCode="AR" term="%22Simha%2C+S%2E%22">Simha, S.</searchLink><br /><searchLink fieldCode="AR" term="%22Sammons%2C+M%2E+W%2E%22">Sammons, M. W.</searchLink><br /><searchLink fieldCode="AR" term="%22Scott%2C+D%2E+R%2E%22">Scott, D. R.</searchLink><br /><searchLink fieldCode="AR" term="%22Tejos%2C+N%2E%22">Tejos, N.</searchLink>
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  Data: <searchLink fieldCode="JN" term="%22Science+%28pre-March+2025%29%22">Science (pre-March 2025)</searchLink>. 10/20/2023, Vol. 382 Issue 6668, p294-299. 6p. 1 Color Photograph, 1 Diagram, 2 Graphs.
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  Data: <searchLink fieldCode="DE" term="%22Solar+radio+bursts%22">Solar radio bursts</searchLink><br /><searchLink fieldCode="DE" term="%22Interstellar+medium%22">Interstellar medium</searchLink><br /><searchLink fieldCode="DE" term="%22Redshift%22">Redshift</searchLink><br /><searchLink fieldCode="DE" term="%22Extragalactic+distances%22">Extragalactic distances</searchLink><br /><searchLink fieldCode="DE" term="%22Plasma+turbulence%22">Plasma turbulence</searchLink><br /><searchLink fieldCode="DE" term="%22Universe%22">Universe</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: Fast radio bursts (FRBs) are millisecond-duration pulses of radio emission originating from extragalactic distances. Radio dispersion is imparted on each burst by intervening plasma, mostly located in the intergalactic medium. In this work, we observe the burst FRB 20220610A and localize it to a morphologically complex host galaxy system at redshift 1.016 ± 0.002. The burst redshift and dispersion measure are consistent with passage through a substantial column of plasma in the intergalactic medium and extend the relationship between those quantities measured at lower redshift. The burst shows evidence for passage through additional turbulent magnetized plasma, potentially associated with the host galaxy. We use the burst energy of 2 × 1042 erg to revise the empirical maximum energy of an FRB. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=pbh&AN=173075041
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        Text: English
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        Type: general
      – SubjectFull: Interstellar medium
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      – SubjectFull: Redshift
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      – SubjectFull: Universe
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