No Pulsar Companion Around the Nearest Low Mass White Dwarf
Tilemachos M. Athanasiadis, Nataliya K. Porayko, John Antoniadis,, David Champion, Olaf Wucknitz, Benedetta Ciardi, Matthias Hoeft, Michael, Kramer

TL;DR
This study conducted a sensitive radio search for a pulsar companion around the nearest low-mass white dwarf but found no evidence of such a pulsar, constraining the existence of detectable radio pulsars in this system.
Contribution
First targeted deep radio search for a pulsar companion around the nearest low-mass white dwarf, setting new limits on its possible pulsar presence.
Findings
No pulsed radio signals detected from the system.
Excludes the presence of a detectable radio pulsar in the binary.
Achieved sensitivity of ~3 mJy for a 10-ms pulsar at low DM.
Abstract
2MASS J050051.85093054.9 is the closest known low-mass helium-core white dwarf in a binary system. We used three high-band international LOFAR stations to perform a targeted search for a pulsar companion, reaching sensitivities of ~3 mJy for a 10-ms pulsar at a DM = 1 pccm. No pulsed signal was detected, confidently excluding the presence of a detectable radio pulsar in the system.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Pulsars and Gravitational Waves Research · Astronomy and Astrophysical Research
