FRB 20180916B (previously known as FRB 180916.J0158+65, and less formally known as FRB 180916 or "R3"), is a repeating Fast radio burst (FRB) discovered in 2018 by astronomers at the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Telescope. According to a study published in the 9 January 2020 issue of the journal Nature, CHIME astronomers, in cooperation with the radio telescopes at European VLBI Network (VLBI) and the optical telescope Gemini North on Mauna Kea, Hawaii, were able to pinpoint the source of FRB 180916 to a location within a Milky Way-like galaxy named SDSS J015800.28+654253.0. This places the source at redshift 0.0337, approximately 457 million light-years from the Solar System.
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| - FRB 180916.J0158+65 (en)
- FRB 180916.J0158+65 (ru)
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| - FRB 20180916B (previously known as FRB 180916.J0158+65, and less formally known as FRB 180916 or "R3"), is a repeating Fast radio burst (FRB) discovered in 2018 by astronomers at the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Telescope. According to a study published in the 9 January 2020 issue of the journal Nature, CHIME astronomers, in cooperation with the radio telescopes at European VLBI Network (VLBI) and the optical telescope Gemini North on Mauna Kea, Hawaii, were able to pinpoint the source of FRB 180916 to a location within a Milky Way-like galaxy named SDSS J015800.28+654253.0. This places the source at redshift 0.0337, approximately 457 million light-years from the Solar System. (en)
- FRB 180916.J0158+65 (наиболее известен как FRB 180916 или «R3», а также как FRB 20180916B) — повторяющийся быстрый радиовсплеск, обнаруженный в 2018 году с помощью радиотелескопа в ходе Канадского эксперимента по картированию интенсивности водорода. Возмущение было зафиксировано 9 января 2020 года в обсерватории Джемини, Мауна-Кеа и исходило из галактики , находящейся на расстоянии 457 миллионов световых лет. (ru)
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| - SDSS J015800.28+654253.0 (en)
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| - FRB 20180916B (previously known as FRB 180916.J0158+65, and less formally known as FRB 180916 or "R3"), is a repeating Fast radio burst (FRB) discovered in 2018 by astronomers at the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Telescope. According to a study published in the 9 January 2020 issue of the journal Nature, CHIME astronomers, in cooperation with the radio telescopes at European VLBI Network (VLBI) and the optical telescope Gemini North on Mauna Kea, Hawaii, were able to pinpoint the source of FRB 180916 to a location within a Milky Way-like galaxy named SDSS J015800.28+654253.0. This places the source at redshift 0.0337, approximately 457 million light-years from the Solar System. (en)
- FRB 180916.J0158+65 (наиболее известен как FRB 180916 или «R3», а также как FRB 20180916B) — повторяющийся быстрый радиовсплеск, обнаруженный в 2018 году с помощью радиотелескопа в ходе Канадского эксперимента по картированию интенсивности водорода. Возмущение было зафиксировано 9 января 2020 года в обсерватории Джемини, Мауна-Кеа и исходило из галактики , находящейся на расстоянии 457 миллионов световых лет. (ru)
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