Search arXiv⌕ Search

arXiv · 2610.24003

Missing Light, Misleading Confidence: Optical-Module Readout Loss and Signal Reliability in Neutrino Telescopes

Abstract

Optical neutrino telescopes reduce the photomultiplier signals of an optical module or string segment to compact multichannel summaries, and readout loss can make these summaries unreliable. We asked whether availability-based quality gates, which accept a summary when enough of the readout was live, can certify a summary of inter-channel statistical consistency (called coherence here; not optical coherence) under readout loss, and where they fail. We used public IceCube pulses (9,484 string records) and the released hits of KM3NeT event KM3-230213A with controlled readout loss, together with a replay of real KM3NeT readout flags. In a two-by-two design we compared a published recursive support state with direct mask support, and calibrated every threshold on development records. The support state is a function of the mask and added no information. On IceCube the support-gated rule retained 0.16 percentage points more usable summaries, an effect of the window at which support was read that reversed sign at a looser tolerance; on KM3NeT it accepted nothing. The gates accepted only records with nearly intact masks, including records whose charge had been depleted by signal-dependent loss that the mask does not record. Pulse loss during live acquisition and timing jitter passed every availability gate, which then accepted summaries of which up to 66% were unreliable. Availability flags are therefore necessary but not sufficient, and signal-based checks are needed. This work uses public data and is not an IceCube or KM3NeT Collaboration result.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Thammarat Yawisit, Pittaya Pannil. 2026-10-15. Missing Light, Misleading Confidence: Optical-Module Readout Loss and Signal Reliability in Neutrino Telescopes. https://arxiv.org/abs/2610.24003

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Error Propagation from Integral Moments and Spectral Derivatives of Stokes Profiles to Magnetic Observables

We aim to derive convenient analytic estimations of magnetic inference errors, which can be used to inform and facilitate the creation of the science-traceability matrix of a polarimetric instrument. In order to do this, we study the general problem of the propagation of Poissonian noise in polarized light signals to derived data products of the Stokes profiles, namely integral moments of arbitrary orders and spectral derivatives of the intensity. In particular, we derive the errors on the longitudinal and transversal projections of the magnetic field inferred from the weak-field approximation (WFA) of the Zeeman effect. The propagated errors on magnetic inference are traced back to the signal- to-noise ratio (SNR) of the observations. The results can be used to quantify the contributions of different environmental and instrumental conditions (spectral line width, spectral resolution, line spread function, stray light) to the overall error on the inferred quantities. Our tests indicate that the integral-moment method of inference is comparable to the local derivative in a predictable way.

astro-ph.IM↗

Plate-YOLO: An End-to-End Object Detection Framework for Robust Astrometric Registration of Historical Plates

Historical astronomical plates provide a long temporal baseline for time-domain astrophysics, but degradation and structural artifacts can hinder automated astrometric calibration. We present Plate-YOLO, a framework that combines source detection and stellar classification in one detector and supplies source catalogs to a separate astrometric solver. The detector adapts YOLOv5 with Space-to-Depth feature rearrangement, SimAM attention, a high-resolution P2 head, and a Normalized Wasserstein Distance loss for small bounding boxes. A Gaia-guided fine-tuning procedure uses initially solved plates to construct labels for a new archive. On 150 UBAI plates for which the conventional pipeline had failed, the Chinese-trained model solved 40 plates, and target-archive fine-tuning recovered a further 106, giving an overall recovery rate of 146/150 (97.3%). In the reported hardware configuration, source extraction took 6.61 s per plate for Plate-YOLO and 16.73 s for SExtractor. These results demonstrate the practical value of adapting source detection to degraded historical plates.

astro-ph.IM↗

Consistency and precision of very long baseline interferometry source coordinate time series

Coordinate time series of extragalactic radio sources from very long baseline interferometry observations are widely used to evaluate source positional stability, select stable sources for celestial reference frames, assess reference-frame axis stability, and investigate source-related astrometric variability. Their external consistency, realistic errors, and relation to processing strategies and analysis configurations remain to be investigated. We aim to compare coordinate time series solutions from different analysis centers and investigate how processing strategies and configurations contribute to their differences. We collected eight solutions from seven analysis centers and selected 496 common sources after data selection, reference-frame alignment, and extraction of common observing sessions. Inter-solution differences were characterized with pairwise positional offsets and correlation analysis, and realistic positional errors with the N-cornered-hat (NCH) method and bootstrap resampling. Most solutions have median weighted root mean square (WRMS) values of a few hundred microarcseconds $(\mathrm{μas})$, and the median NCH-derived precision is about 200-300 $\mathrm{μas}$ in right ascension and 250-400 $\mathrm{μas}$ in declination. Solutions with similar strategies, software, or source constraints show higher consistency, with more similar WRMS values, stronger correlations, and closer precision estimates. Consistency is affected not only by the global or independent mode distinction but also by detailed analysis configuration. NCH-derived precision depends on declination, being poorer in the southern sky, and stabilizes with more observing sessions. Processing strategies and configurations introduce marginal differences; solutions remain generally consistent. Inter-solution comparisons independently estimate realistic stochastic errors beyond formal errors.

astro-ph.IM↗