High-resolution imaging of two radio quasars at the end of the reionization epoch

Krisztina Perger; Yingkang Zhang; Sándor Frey; Tao An; Krisztina E. Gabányi; Leonid I. Gurvits; Chorng Yuan Hwang; Ekaterina Koptelova; Zsolt Paragi; Ailing Wang

High-resolution imaging of two radio quasars at the end of the reionization epoch

Krisztina Perger, Yingkang Zhang, Sándor Frey, Tao An, Krisztina E. Gabányi, Leonid I. Gurvits, Chorng Yuan Hwang, Ekaterina Koptelova, Zsolt Paragi, Ailing Wang

天文研究所

研究成果: 雜誌貢獻 › 會議論文 › 同行評審

1 引文斯高帕斯（Scopus）

摘要

There are approximately 250 quasars discovered at redshift z ≥ 6, of which only a handful were detected in radio bands, and even fewer were imaged with the highest resolution very long baseline interferometry (VLBI) technique. Here we report the results of our dual-frequency observations with the Very Long Baseline Array (VLBA) of two such recently discovered quasars, VIKING J231818.35-311346.3 at z = 6.44 and FIRST J233153.20+112952.11 at z = 6.57. Both extremely distant sources were imaged with VLBI for the first time. The radio properties of the former are consistent with those of quasars with young radio jets. The latter has an UV/optical spectrum characteristic of BL Lac objects, of which no others have been found beyond redshift 4 so far. Our VLBA observations revealed a flat-spectrum compact radio source.

原文	???core.languages.en_GB???
文章編號	024
期刊	Proceedings of Science
卷	428
出版狀態	已出版 - 22 8月 2023
事件	15th European VLBI Network Mini-Symposium and Users' Meeting, EVN 2022 - Cork, Ireland 持續時間: 11 7月 2022 → 15 7月 2022

引用此

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title = "High-resolution imaging of two radio quasars at the end of the reionization epoch",

abstract = "There are approximately 250 quasars discovered at redshift z ≥ 6, of which only a handful were detected in radio bands, and even fewer were imaged with the highest resolution very long baseline interferometry (VLBI) technique. Here we report the results of our dual-frequency observations with the Very Long Baseline Array (VLBA) of two such recently discovered quasars, VIKING J231818.35-311346.3 at z = 6.44 and FIRST J233153.20+112952.11 at z = 6.57. Both extremely distant sources were imaged with VLBI for the first time. The radio properties of the former are consistent with those of quasars with young radio jets. The latter has an UV/optical spectrum characteristic of BL Lac objects, of which no others have been found beyond redshift 4 so far. Our VLBA observations revealed a flat-spectrum compact radio source.",

author = "Krisztina Perger and Yingkang Zhang and S{\'a}ndor Frey and Tao An and Gab{\'a}nyi, {Krisztina E.} and Gurvits, {Leonid I.} and Hwang, {Chorng Yuan} and Ekaterina Koptelova and Zsolt Paragi and Ailing Wang",

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T1 - High-resolution imaging of two radio quasars at the end of the reionization epoch

AU - Perger, Krisztina

AU - Zhang, Yingkang

AU - Frey, Sándor

AU - An, Tao

AU - Gabányi, Krisztina E.

AU - Gurvits, Leonid I.

AU - Hwang, Chorng Yuan

AU - Koptelova, Ekaterina

AU - Paragi, Zsolt

AU - Wang, Ailing

PY - 2023/8/22

Y1 - 2023/8/22

N2 - There are approximately 250 quasars discovered at redshift z ≥ 6, of which only a handful were detected in radio bands, and even fewer were imaged with the highest resolution very long baseline interferometry (VLBI) technique. Here we report the results of our dual-frequency observations with the Very Long Baseline Array (VLBA) of two such recently discovered quasars, VIKING J231818.35-311346.3 at z = 6.44 and FIRST J233153.20+112952.11 at z = 6.57. Both extremely distant sources were imaged with VLBI for the first time. The radio properties of the former are consistent with those of quasars with young radio jets. The latter has an UV/optical spectrum characteristic of BL Lac objects, of which no others have been found beyond redshift 4 so far. Our VLBA observations revealed a flat-spectrum compact radio source.

AB - There are approximately 250 quasars discovered at redshift z ≥ 6, of which only a handful were detected in radio bands, and even fewer were imaged with the highest resolution very long baseline interferometry (VLBI) technique. Here we report the results of our dual-frequency observations with the Very Long Baseline Array (VLBA) of two such recently discovered quasars, VIKING J231818.35-311346.3 at z = 6.44 and FIRST J233153.20+112952.11 at z = 6.57. Both extremely distant sources were imaged with VLBI for the first time. The radio properties of the former are consistent with those of quasars with young radio jets. The latter has an UV/optical spectrum characteristic of BL Lac objects, of which no others have been found beyond redshift 4 so far. Our VLBA observations revealed a flat-spectrum compact radio source.

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M3 - 會議論文

AN - SCOPUS:85150160922

SN - 1824-8039

VL - 428

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 024

T2 - 15th European VLBI Network Mini-Symposium and Users' Meeting, EVN 2022

Y2 - 11 July 2022 through 15 July 2022

ER -

High-resolution imaging of two radio quasars at the end of the reionization epoch

摘要

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