Search for periodic emission of five gamma-ray pulsars at the frequency of 111 MHz
arXiv:2204.06785 · doi:10.1134/S1063772921100401
Abstract
The search for pulsar (periodic) emission of five gamma-ray pulsars was carried out using the summed power spectra and the summed periodograms. No harmonics corresponding to the known pulsar periods were found. The upper estimations of the integral flux density of the pulsars J0357+3205 (<0.5 mJy), J0554+3107 (<0.5 mJy), J1958+2846 (<0.5 mJy), J2021+4026 (<0.4 mJy), and J2055+2539 (<0.55 mJy) is obtained.
Published in Astronomy Reports and translated from russian version of paper by Yandex translator with correction scientific lexis. 6 page, 1 figure, 1 table
References in corpus (11)
- Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
- Optimal periodicity searching: Revisiting the Fast Folding Algorithm for large-scale pulsar surveys
- Detection of new pulsars at the frequency 111 MHz
- Search and detection of pulsars in the monitoring observations at the frequency 111 MHz
- The LOFAR Tied-Array All-Sky Survey: Timing of 21 pulsars including the first binary pulsar discovered with LOFAR
- Deep searches for decameter wavelength pulsed emission from radio-quiet gamma-ray pulsars
- A detailed X-ray investigation of PSR J2021+4026 and -Cygni supernova remnant
- Search for pulsars in the summed power spectra at a frequency of 111 MHz
- Detection of two new RRATs at 111 MHz
- MAGIC Upper Limits for two Milagro-detected, Bright Fermi Sources in the Region of SNR G65.1+0.6
- Search for periodic radio emission of gamma pulsar J0357+3205