Discovery of a 36-minute long-period transient ASKAP J142431.2-612611
Joshua Pritchard, Tara Murphy, Dougal Dobie, Emil Lenc, Akash Anumarlapudi, Manisha Caleb, Sophia Grainger, Natasha Hurley-Walker, David L. Kaplan, Samuel J. McSweeney, Jackson Mitchell-Bolton, Kovi Rose, Rahul Sengar, Ziteng Wang, Jayde Willingham, and Andrew Zic

TL;DR
A new long-period radio transient with a 36-minute cycle was discovered, showing unique polarisation behavior and intermittent activity, expanding understanding of such transient sources.
Contribution
This paper reports the first detection of a 36-minute long-period radio transient with unique polarisation characteristics and intermittent activity, adding to the known class of long-period transients.
Findings
Detected a 36-minute period radio transient ASKAP J142431.2-612611.
Observed stable, highly polarised pulse profile evolving from elliptical to linear polarisation.
Source exhibited intermittent activity, switching off after eight days.
Abstract
We report the discovery of a new long-period radio transient, ASKAP J142431.2-612611, with a 36 minute period, identified in the Australian SKA Pathfinder Evolutionary Map of the Universe survey. We detected pulsed emission from ASKAP J142431.2-612611 over a period of eight days during follow-up observations with the Australia Telescope Compact Array, after which the source appears to have switched off. No optical or near-infrared counterpart is detected in archival surveys or in targeted Gemini South FLAMINGOS-2 observations. During its active state, the source exhibits a stable pulse profile with fractional polarisation consistent with 100%, evolving from elliptically to linearly polarised and tracing a well-defined great-circle trajectory on the Poincar\'e sphere. We show that this behaviour is consistent with fully linearly polarised intrinsic emission modified by propagation…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
