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Giulia Mantovani

Publications and source records attributed to Giulia Mantovani.

3 recordsLinked to original sources

Designing Ambiguity-Aware Clerical Review: A Stratified Sampling Framework for Record Linkage and Deduplication

Clerical review of candidate record pairs remains the de facto gold standard for evaluating record linkage, but it is resource-intensive and often designed informally. We propose a design-based framework that treats clerical review as finite-population sampling over fine-grained strata defined by match weight, comparison pattern, record-level ambiguity, and demographic group. Match-probability bands are constructed from model-based score deciles. Within bands, strata combine comparison patterns with an ambiguity factor derived from matchability and conditional candidate perplexity. A band-specific margin-of-error profile encodes substantive priorities, such as tighter precision in high-score bands, while a single scaling parameter enforces the overall clerical budget. We evaluate the framework using a labelled dataset deduplicated in Splink, comprising 50,000 records and approximately 478,000 candidate pairs. We compare a baseline design reviewing about 23% of pairs with a budget-constrained design reviewing about 7%. The baseline accurately estimates global and band-specific match rates, while sampled distributions of comparison patterns, gender, and ambiguity broadly track the population. Under the budget design, global error approximately doubles, with the largest band-level errors in middle-score bands where matches, non-matches, and ambiguous cases are intermixed. Accuracy in the highest-score bands and the band-wise ambiguity profile are largely preserved, although representativeness by comparison pattern and gender declines. The framework generalises to other clerical-review objectives and can incorporate gold-standard data as prior information for design and calibration. It makes explicit the negotiable trade-offs between workload, precision, representativeness, and coverage of linkage uncertainty.

stat.ME

Relativistic Fe K alpha line study in Seyfert 1 galaxies observed with Suzaku

We present an analysis of a sample of Seyfert 1 galaxies observed with Suzaku. The aim of this work is to examine critically the evidence for a relativistic Fe K alpha line in the X-ray spectra of these AGN. The sample was compiled from those sources in which a relativistic component was missing in at least one XMM-Newton observation. We analysed the Suzaku spectra of these objects in order to have more constraints on the high energy emission, including the Compton reflection hump. The results show that the relativistic Fe K alpha line is detected (at >95% confidence) in all sources observed with high signal-to-noise ratio (e.g. where the counts in the 5-7 keV energy band are > 4 x 10^4). This is in agreement with the idea that relativistic lines are a ubiquitous feature in the spectra of Seyfert galaxies, but are often difficult to detect without very high quality data. We also investigate the relation between the Fe K alpha line and the reflection continuum at high energies. For most of the sample, the strength of the reflection component is consistent with that of the line. There are exceptions in both senses, however i.e. where the reflection continuum is strong but with weak line emission, and vice versa. These observations present a challenge for standard reflection models.

astro-ph.HE

Relativistic iron K alpha line detection in the Suzaku spectra of IC 4329A

We present an analysis of five Suzaku observations of the bright Seyfert1 galaxy IC 4329A. The broad energy band and high signal-to-noise ratio of the data give new constraints on the iron K alpha line profile and its relationship with the Compton hump at higher energies. The Fe K bandpass is dominated by a narrow core (EW=57 eV) at 6.4 keV consistent with neutral material. Using a physically-motivated model, our analysis also reveals the presence of a broad Iron K alpha line (EW=124 eV), most likely produced in the inner part of the accretion disk and blurred by general relativistic effects. This component is not immediately evident from the individual spectra, but is clearly present in the stacked residuals of all five observations, and has high statistical significance. This highlights the difficulty in identifying broad iron lines in AGN, even in data with very high signal-to-noise ratio, as they are difficult to disentangle from the continuum. The data are consistent with the narrow and broad iron line components tracking the Compton Hump, but do not provide clear evidence that this is the case. An additional narrow FeXXVI emission line at 6.94 keV is also seen, suggesting the presence of ionized material relatively distant from the central region. There is also a hint of variability, so the precise origin of this line remains unclear.

astro-ph.HE