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January 18, 20260 citations

A survey for radio pulsars and transients in the 10 pc region around Sgr A*

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GDG. DesvignesRER.P. EatoughYMY.P. MenMax Planck Institute for Radio Astronomy

Key Points

  • This research aims to survey the 10 pc region around Sgr A* for new radio pulsars and transients.
  • Conducted survey using Effelsberg radio telescope at 4 to 8 GHz frequencies.
  • Utilized full-Stokes data for pulsar and transient searches.
  • Implemented periodicity, acceleration, and jerk searches for candidate scoring.
  • Performed dedicated linear polarisation search for slow transients.
  • Detected the magnetar SGR J1745-2900 again but found no new discoveries.
  • Identified a faint single pulse candidate and several weak periodicity candidates.
  • Survey sensitivity is insufficient to detect a population of millisecond pulsars.

Abstract

Here we report on a new survey for pulsars and transients in the 10,pc region around using the Effelsberg radio telescope at frequencies between 4 to 8 GHz. Our calibrated full-Stokes data were searched for pulsars and transients using , , and . Polarisation information is used in the scoring of the candidates. Our periodicity acceleration and jerk searches allowed us to maintain good sensitivity towards binary pulsars in ≳ 10-hr orbits. In addition we performed a dedicated search in linear polarisation for slow transients. While our searches yielded no new discovery beyond the redetection of the magnetar SGR J1745-2900, we report on a faint single pulse candidate in addition to several weak periodicity search candidates. After thoroughly assessing our survey's sensitivity, we determined that it is still not sensitive to a population of millisecond pulsars. Next generation radio interferometers can overcome the limitations of traditional single-dish pulsar searches of the Galactic Centre. PulsarX TransientX PRESTO

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Cite This Study

Desvignes et al. (2025) studied this question.

synapsesocial.com/papers/696c789ceb60fb80d1396cd8https://doi.org/10.1051/0004-6361/202556381/pdf
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