Observations of Transient Phenomena in BSA Radio Survey at 110 MHz

Самодуров, В. А.; Pozanenko, A.; Rodin, A. E.; Churakov, D. D.; Dumskij, D. V.; Исаев, Е. А.; Kazantsev, A. N.; Логвиненко, С. В.; Oreshko, V. V.; Toropov, M. O.; Volobueva, Maria I.

doi:10.1007/978-3-319-57135-5_10

Cited by 4 publications

(2 citation statements)

References 4 publications

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“…This time in milliseconds is shown under the transient name. Table 1 lists the main parameters of the new 25 RRATs together with additional information for eight RRATs published earlier by Samodurov et al (2017);Tyul'bashev et al (2018) and in RRATalog. The first column contains the RRAT's name in the J2000 notation.…”

Section: Observations and Resultsmentioning

confidence: 99%

Detection of 25 new rotating radio transients at 111 MHz

Tyul’bashev

Malofeev

2018

A&A

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Nearly all fast radio RRAT-type transients that are pulsars with rare pulses have been previously detected using decimetre wavelengths. We present here 34 transients detected at metre wavelengths in our daily monitoring at declinations −9 • ≤ δ ≤ +42 • . 25 transients are new RRATs. We confirmed the detection of 7 RRATs based on our early observations. One of the 34 detected transients was determined to be a new pulsar J1326+3346. At the same time, out of 35 RRATs detected at the decimetre wavelengths and included in the studied area, only one was detected by us J1848+1518. The periods of 6 RRATs were found from the time of arrival of single pulses. Three quarters of all RRATs were observed more than once and the total number of RRATs in the area studied has doubled.

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Section: Observations and Resultsmentioning

confidence: 99%

Detection of 25 new rotating radio transients at 111 MHz

Tyul’bashev

Malofeev

2018

A&A

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“…Inspection of recent publications shows that the strongest transients, J0139+3310 and J1005+3015, were apparently already detected at 111 MHz in earlier six-frequency BSA monitoring observations (Samodurov (2017)). During the period from July 2012 through October 2013, 34 pulses at the coordinates 2000 = 1 ℎ 38 30 ± 30 and 2000 = 33 41 ′ ± 15 ′ and with = 21 ± 3 pc/cm 3 were found; 12 pulses at the coordinates 2000 = 10 ℎ 05 05 ± 30 and 2000 = 30 10 ′ ± 15 ′ with = 18 ± 2 pc/cm 3 were found.…”

Section: Resultsmentioning

confidence: 90%

Detection of Five New RRATs at 111 MHz

Tyul'bashev,

Malofeev

et al. 2022

Preprint

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Results of 111-MHz monitoring observations carried out on the Big Scanning Antenna of the Pushchino Radio Astronomy Observatory during September 1-28, 2015 are presented. Fifty-four pulsating sources were detected at declinations −9 < < 42 . Forty-seven of these are known pulsars, five are new sources, and two are previously discovered transients. Estimates of the peak flux densities and dispersion measures are presented or all these sources.

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Detection of Five New RRATs at 111 MHz

Tyul’bashev

Malofeev

et al. 2018

Astron. Rep.

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Observations of Transient Phenomena in BSA Radio Survey at 110 MHz

Cited by 4 publications

References 4 publications

Detection of 25 new rotating radio transients at 111 MHz

Detection of 25 new rotating radio transients at 111 MHz

Detection of Five New RRATs at 111 MHz

Detection of Five New RRATs at 111 MHz

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