Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources
Tinn Thongmeearkom, Colin J. Clark, Rene P. Breton, Marta Burgay, Lars Nieder, Oliver G. Dodge, Brian McGloughlin, Ewan D. Barr, Sarah Buchner, Benjamin W. Stappers, Joanna Berteaud, Elizabeth C. Ferrara, Paulo C. C. Freire, Lina Levin, Scott M. Ransom, Laila Vleeschower

TL;DR
This study used MeerKAT UHF observations to discover 15 new pulsars from Fermi-LAT sources, confirming gamma-ray associations and demonstrating UHF's superior sensitivity over L band for faint pulsar detection.
Contribution
First UHF-band survey of Fermi-LAT sources with MeerKAT, discovering new pulsars and demonstrating UHF's advantages over L band in sensitivity and detection rate.
Findings
Discovered nine new millisecond pulsars and six slow pulsars.
Confirmed gamma-ray associations for seven MSPs through joint timing.
UHF observations outperform L band in detecting faint gamma-ray pulsars.
Abstract
The Fermi Large Area Telescope (LAT) provides advantages for radio pulsar searches by enabling efficient target selection. We can confidently point radio telescopes to the positions of Fermi unidentified gamma-ray sources that have a high probability of hosting a pulsar. As part of Transients and Pulsars with MeerKAT (TRAPUM), we conducted a survey of Fermi-LAT sources using the Ultra High Frequency (UHF; 544-1088 MHz) receiver of the MeerKAT radio telescope. We observed 79 sources that were identified as pulsar-like candidates using a random forest technique from the Fermi-LAT Fourth Source Catalogue. We observed each target for 10 minutes at two separate epochs. As a result, we discovered nine new millisecond pulsars (MSPs) and six slow pulsars. Based on the radio discoveries, we also searched for gamma-ray pulsations, confirming that seven of the newly discovered MSPs are associated…
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