The LOFAR search for radio pulsars and fast transients in M33, M81 & M82

TL;DR

This study used LOFAR to search for radio pulsars and fast transients in nearby galaxies M33, M81, and M82, setting new limits on their brightness and finding no sources, thus constraining extragalactic pulsar populations.

Contribution

First deep LOFAR observations of M33, M81, and M82 for pulsar and transient detection, establishing new flux limits and constraining extragalactic pulsar brightness.

Findings

No pulsars or transients detected in the targeted galaxies.

Set stricter flux density limits than previous surveys.

Nearby galaxies lack bright pulsars comparable to Milky Way pulsars.

Abstract

The radio pulsar and rotating radio transient populations are only known in and near the Milky Way. Investigating such populations in other galaxies requires deep pulsar and transient searches. We performed 4-h radio observations of nearby galaxies M33, M81 and M82 with LOFAR. Our main purpose was to characterise the bright end of the pulsar population in other galaxies, and compare it to that of the Milky Way. We searched for extragalactic radio pulsars through a periodic-pulse search, and for sporadic fast radio transients through a single-pulse search. We coherently combined at most 23 LOFAR Core High-Band Antenna (HBA) stations and covered M33, M81, and M82 in their entirety using multiple tied-array beams. No pulsating sources or single pulses were found. We have, therefore established stricter limits on the extragalactic pulsar flux density at lower frequencies than those obtained in previous Arecibo, GBT, and WSRT searches. We conclude that in nearby galaxies M33, M81, and M82 there are no pulsars shining toward Earth with pseudo luminosities greater than a few times that of the brightest pulsars in our Milky Way.