Observations of Magnetar SGR J1830–0645 and Pulsar J0250+5854 at 111 MHz

Search observations of radio signals from the new magnetar SGR J1830–0645 have been carried out since January 2021 and up to the present at the Pushchino Radio Astronomy Observatory of the Lebedev Physics Institute of Russian Academy of Sciences (PRAO LPI) at a frequency of 111 MHz with the Large Ph...

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Bibliographic Details
Published in:Astronomy reports 2022-11, Vol.66 (11), p.981-988
Main Authors: Losovsky, B. Ya, Glushak, A. P.
Format: Article
Language:English
Subjects:
Astronomy
Flux density
Magnetars
Observations and Techniques
Phased arrays
Physics
Physics and Astronomy
Pulsars
Radio astronomy
Radio signals
Signal processing
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Summary:Search observations of radio signals from the new magnetar SGR J1830–0645 have been carried out since January 2021 and up to the present at the Pushchino Radio Astronomy Observatory of the Lebedev Physics Institute of Russian Academy of Sciences (PRAO LPI) at a frequency of 111 MHz with the Large Phased Array (LPA). According to results of processing observations for 2021, periodic or pulsed radio signals were not detected. The upper limit for estimating the radio flux density of SGR J1830–0645 at 111 MHz is 500 mJy. The 23.5 s radio pulsar J0250+5854 was used as a control radio source. Its flux density at 111 MHz was measured to be 9.6 ± 1.6 mJy. We performed pulse timing, measured and calculated the parameters of J0250+5854.
ISSN:1063-7729
1562-6881
DOI:10.1134/S1063772922110130