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arxiv: 2605.22516 · v2 · pith:HN2ADL63new · submitted 2026-05-21 · 🌌 astro-ph.HE · astro-ph.IM

Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station

Pith reviewed 2026-05-25 05:43 UTC · model grok-4.3

classification 🌌 astro-ph.HE astro-ph.IM
keywords pulsar timingLOFARlow-frequency radioneutron starspulsar surveystiming solutionsradio astronomypulsar follow-up
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The pith

A single international LOFAR station can detect and deliver coherent timing solutions for 17 pulsars at 150 MHz.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper shows that the Irish LOFAR station, operated as a standalone telescope, has enough sensitivity to follow up pulsar candidates announced by various surveys and to build timing models at 150 MHz. From 33 candidates observed between 2020 and 2023, 22 were detected and 17 received long-term monitoring across 590 hours, yielding coherent solutions for every source. Seven of the solutions are new; the other ten match independent results. This matters because the surge in new pulsar discoveries has outstripped the capacity of traditional timing programs, and low-frequency stations offer an under-used route to keep timing models current.

Core claim

The authors used the Irish LOFAR station in local mode to monitor 17 pulsars at 150 MHz over 590 hours and obtained coherent timing solutions for all of them. Seven sources had no prior reported timing solutions; the remaining ten agree with solutions published by other groups. The work demonstrates that the 14 international LOFAR stations are positioned to perform long-term follow-up of survey candidates beyond standard campaigns at those telescopes.

What carries the argument

Long-term monitoring campaign with the Irish LOFAR station at 150 MHz, which supplies the sensitivity and frequency coverage needed to produce coherent timing solutions from single-station data.

If this is right

  • International LOFAR stations can absorb part of the follow-up load for newly discovered pulsars.
  • Timing models can be built for a larger fraction of the pulsar population without competing for time at dedicated timing arrays.
  • Low-frequency data become routinely available for dispersion-measure and emission studies of these sources.
  • The scientific return from recent wide-field surveys increases because more sources receive basic timing characterisation.
  • Pressure on observing time at higher-frequency facilities is reduced for routine monitoring.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Other international LOFAR stations could run parallel campaigns, multiplying the number of sources that receive low-frequency timing.
  • The same single-station approach could be tested on future survey discoveries announced at higher frequencies to check detection rates at 150 MHz.
  • Combined low-frequency timing solutions may reveal frequency-dependent effects in pulse profiles or dispersion measures that higher-frequency data alone miss.
  • This method offers a low-cost way to maintain timing for the growing population of pulsars that lack dedicated follow-up resources.

Load-bearing premise

The 17 selected candidates are real pulsars that remain detectable and phase-coherent at 150 MHz with the sensitivity of one LOFAR station over multi-year timescales.

What would settle it

Inability to obtain phase-connected timing solutions across the 17 sources or systematic disagreement between the new 150 MHz solutions and independent timing measurements at other frequencies.

Figures

Figures reproduced from arXiv: 2605.22516 by D. J. McKenna, E. F. Keane, J. McCauley, P. T. Gallagher.

Figure 1
Figure 1. Figure 1: — A period-period derivative phase space plot of known pulsars, with the sources timed as a part of this work highlighted. This plot was generated with the aid of psrqpy (Pitkin 2018). (v2.6.0), 94.3 ms, as opposed to the original survey pe￾riod, the latter of which was used for this work and is present in the ephemeris, 364.9 ms. This does not appear to be an integer multiple of the final rotation period,… view at source ↗
Figure 2
Figure 2. Figure 2: — The Stokes I frequency-averaged folded profiles of the sources detected and monitored as a part of this work. The x-axis labels cover the full folded pulse profile of each source in seconds, while the y-axis contains off-axis-normalised emission in arbitrary units [PITH_FULL_IMAGE:figures/full_fig_p012_2.png] view at source ↗
read the original abstract

Pulsar timing is a foundational part of pulsar research to triage the most interesting systems and to characterise properties (rotational or otherwise) of the population of these extreme objects. Due to the efficiency of a number of sensitive and/or wide-field surveys in recent years, the number of new pulsars discoveries is growing year-on-year, and most of these lack even basic timing parameter measurements. This work aims to demonstrate the capabilities of international Low Frequency Array (LOFAR) stations operating as single telescopes to follow-up, time and characterise these sources, offering new insight into the emission properties of these neutron stars, and support efforts to build timing models for these sources. Between 2020 and 2023 we used the local-mode allocation of the Irish LOFAR station to follow-up 33 pulsar candidates announced from various surveys at different observing frequencies to determine if an international LOFAR station has sufficient sensitivity to detect and time these sources. From the 33 pulsars selected, 22 pulsars were detected and 17 were selected for long-term monitoring across 590 hours of observing time. This has resulted in coherent timing solutions for all of these sources at 150 MHz -- 7 of these have never had any reported timing solutions, the remaining 10 solutions agree well with announcements from others since the beginning of our project. For a fraction of sources announced by surveys each year, the 14 international LOFAR stations are well placed to follow-up survey candidates for long-term pulsar monitoring beyond the standard timing campaigns performed at these telescopes to date, reducing the pressure on observing time availability at these observatories, and enabling the full scientific potential of these pulsars to be realised.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 3 minor

Summary. The manuscript reports follow-up observations of 33 pulsar candidates using the Irish LOFAR station in local mode between 2020 and 2023. From these, 22 were detected and 17 selected for long-term monitoring totaling 590 hours, yielding coherent timing solutions at 150 MHz for all 17 sources. Seven solutions are presented as new; the remaining ten are stated to agree with independent announcements from other groups.

Significance. If the timing solutions hold, the work shows that individual international LOFAR stations can perform effective long-term pulsar timing follow-up at low frequencies. This capability could complement survey discoveries, reduce demand on other facilities, and enable population studies of emission properties for newly found pulsars. The reported agreement for the ten overlapping sources supplies direct empirical support for the pipeline.

minor comments (3)
  1. The abstract and introduction would benefit from a brief statement of the typical TOA precision or timing residual RMS achieved for the 17 sources to allow immediate assessment of solution quality.
  2. Section describing the candidate selection criteria (from the 33 initial targets) should explicitly list the survey frequencies and flux-density thresholds used, as these directly affect the claimed detection rate of 22/33.
  3. A short table or paragraph comparing the new 150 MHz solutions (period, DM, position) against the independent announcements for the ten overlapping sources would strengthen the validation claim.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their positive assessment of the manuscript, the recognition of its significance for demonstrating single-station LOFAR timing capabilities, and the recommendation for minor revision. No major comments were raised in the report.

Circularity Check

0 steps flagged

No significant circularity identified

full rationale

The paper reports direct observational results: detection and coherent timing of 17 pulsars from 590 hours of Irish LOFAR data at 150 MHz, with 7 new solutions and 10 agreeing with independent announcements. Timing solutions are obtained via standard TOA extraction and fitting procedures applied to the collected data. No equations, parameters, or claims reduce by construction to prior fitted values within the paper; no self-citations are load-bearing for the central result; no ansatzes or uniqueness theorems are invoked. The agreement with external announcements supplies independent validation. The derivation chain is self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The paper relies on standard pulsar timing techniques and the assumption that the candidates are real pulsars detectable at 150 MHz. No free parameters, new axioms, or invented entities are introduced in the abstract.

axioms (1)
  • domain assumption Standard assumptions in pulsar timing analysis such as the validity of the timing model and dispersion measure corrections.
    Implicit in any pulsar timing work at radio frequencies.

pith-pipeline@v0.9.0 · 5861 in / 1191 out tokens · 23290 ms · 2026-05-25T05:43:20.920425+00:00 · methodology

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Reference graph

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