cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Does early life exposure to exogenous sources of reactive oxygen species (ROS) increase the risk of respiratory and allergic diseases in children? A longitudinal cohort study
Creators: name: To, Teresa
name: Terebessy, Emilie
name: Zhu, Jingqin
name: Zhang, Kimball
name: Lakey, Pascale S.
name: Shiraiwa, Manabu
name: Hatzopoulou, Marianne
name: Minet, Laura
name: Weichenthal, Scott
name: Dell, Sharon D.
name: Stieb, David M.
Publisher: name: BioMed Central
Year: 2023

description: Background: Excess reactive oxygen species (ROS) can cause oxidative stress damaging cells and tissues, leading to adverse health effects in the respiratory tract. Yet, few human epidemiological studies have quantified the adverse effect of early life exposure to ROS on child health. Thus, this study aimed to examine the association of levels of ROS exposure at birth and the subsequent risk of developing common respiratory and allergic diseases in children. Methods 1,284 Toronto Child Health Evaluation Questionnaire (T-CHEQ) participants were followed from birth (born between 1996 and 2000) until outcome, March 31, 2016 or loss-to-follow-up. Using ROS data from air monitoring campaigns and land use data in Toronto, ROS concentrations generated in the human respiratory tract in response to inhaled pollutants were estimated using a kinetic multi-layer model. These ROS values were assigned to participants’ postal codes at birth. Cox proportional hazards regression models, adjusted for confounders, were then used to estimate hazard ratios (HR) with 95% confidence intervals (CI) per unit increase in interquartile range (IQR). Results After adjusting for confounders, iron (Fe) and copper (Cu) were not significantly associated with the risk of asthma, allergic rhinitis, nor eczema. However, ROS, a measure of the combined impacts of Fe and Cu in PM2.5, was associated with an increased risk of asthma (HR = 1.11, 95% CI: 1.02–1.21, p < 0.02) per IQR. There were no statistically significant associations of ROS with allergic rhinitis (HR = 0.96, 95% CI: 0.88–1.04, p = 0.35) and eczema (HR = 1.03, 95% CI: 0.98–1.09, p = 0.24). Conclusion These findings showed that ROS exposure in early life significantly increased the childhood risk of asthma, but not allergic rhinitis and eczema.
title: Sezione di Museologia Scientifica e Naturalistica, 2010: Volume Speciale
title: Volume Speciale
titleType: AlternativeTitle
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Presentazione...1-2
Programma...1-10
Biodiversità dal passato al futuro...1-4
Biodiversità e collezioni museali.Gestione e fruizione del patrimonio scientifico e storico del patrimonio italiano...21-41
Musei, collezioni e biodiversità. La biodiversità globale...42-56
Musei, collezioni e biodiversità. La biodiversità locale...57-76
Collezioni dei musei e analisi molecolari:potenzialità, problemi, criteri...77-82
Musei, colezioni e gestione del territorio. Ricerche sulla biodiversità...83-105
Educare alla biodiversità: riflessioni e proposte da condividere tra i soci...106-120
Alophophion mahunkai Vas 2024
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Alophophion
Alophophion mahunkai

description: 15.1.11 Alophophion mahunkai Vas, 2024 *
Distribution. Chile: Región de Arica y Parinacota (Vas 2024b).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 32, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
The ESO-VLT MIKiS survey reloaded: velocity dispersion profile and rotation curve of NGC 1904
Creators: name: Leanza, S.
name: Pallanca, C.
name: Ferraro, F. R.
name: Lanzoni, B.
name: Dalessandro, E.
name: Origlia, L.
name: Mucciarelli, A.
name: Valenti, E.
name: Tiongco, M.
name: Varri, A. L.
name: Vesperini, E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an investigation of the internal kinematic properties of M79 (NGC 1904). Our study is based on radial velocity measurements obtained from the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic globular clusters for more than 1700 individual stars distributed between $\sim 0.3^{\prime\prime}$ and $770^{\prime\prime}$ ($\sim14$ three-dimensional half-mass radii), from the center. Our analysis reveals the presence of ordered line-of-sight rotation with a rotation axis almost aligned along the East-West direction and a velocity peak of $1.5$ km s$^{-1}$ at $\sim 70^{\prime\prime}$ from the rotation axis. The velocity dispersion profile is well described by the same King model that best fits the projected density distribution, with a constant central plateau at $σ_0\sim 6$ km s$^{-1}$. To investigate the cluster rotation in the plane of the sky, we have analyzed the proper motions provided by the Gaia EDR3, finding a signature of rotation with a maximum amplitude of $\sim 2.0$ km s$^{-1}$ at $\sim 80^{\prime\prime}$ from the cluster center. Analyzing the three-dimensional velocity distribution, for a sub-sample of 130 stars, we confirm the presence of systemic rotation and find a rotation axis inclination angle of $37$° with respect to the line-of-sight. As a final result, the comparison of the observed rotation curves with the results of a representative N-body simulation of a rotating star cluster shows that the present-day kinematic properties of NGC 1904 are consistent with those of a dynamically old system that has lost a significant fraction of its initial angular momentum.
description: 30 pages, 20 figures, 8 tables, accepted for publication in ApJ
Limits on the hard X-ray emission from the periodic fast radio burst FRB 180916.J0158+65
Creators: name: Laha, Sibasish
name: Wadiasingh, Zorawar
name: Parsotan, Tyler
name: Lien, Amy
name: Younes, George
name: Zhang, Bing
name: Cenko, S. Bradley
name: Troja, Eleonora
name: Oates, Samantha
name: Nicholl, Matt
name: Meyer, Eileen
name: González, Josefa Becerra
name: Ghosh, Ritesh
name: Klingler, Noel
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: FRB 180916.J0158+65 is one of the nearest, periodically repeating, and actively bursting fast radio burst (FRB) which has been localized to the outskirts of a spiral galaxy. In this work we study the FRB with the hard X-ray $14-195$ keV data from the Burst Alert Telescope (BAT) on board The Neil Gehrels Swift Observatory. BAT uses coded mask technology giving a localization of $\lesssim 3$ arc-minute in the hard X-ray band, along with an accurate background estimation. BAT has been observing the source location in survey mode since February 2020. The survey mode observations involves background subtracted spectra, integrated over a time span ranging $300-2000$ seconds, at the source location (from Feb 2020-Jan 2022). We analyzed all the $\sim 230$ survey mode observations from BAT and checked for any signal in any of the observations. We did not detect any signal at $>5σ$ confidence level in any of the observations. We could estimate a $5σ$ upper limit on the $14-195$ keV flux, which ranged between $4.5\times 10^{-10} - 7.6\times 10^{-9}\, \rm erg\, cm^{-2}\, s^{-1}$. At the source distance this relates to a $5σ$ upper limit on luminosity of $5.08\times 10^{44}- 8.5\times 10^{45} \rm erg\, s^{-1}$. With this estimate, we could rule out any persistent X-ray emission, at the source location for these snapshots of BAT observations.
description: Accepted for publication in ApJ
title: Sezione di Museologia Scientifica e Naturalistica, 2011: Volume Speciale
title: Volume Speciale
titleType: AlternativeTitle
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Taphos 2011. 6th International Meeting on Taphonomy and Fossilization...1-95
Alophophion mallecoensis Alvarado 2014
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Alophophion
Alophophion mallecoensis

description: 15.1.12 Alophophion mallecoensis Alvarado, 2014
Distribution. Neotropical; Chile: Región de La Araucanía (Alvarado 2014).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 32, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
A quasar shedding its dust cocoon at redshift 2
Creators: name: Yi, Weimin
name: Brandt, W. N.
name: Ni, Q.
name: Ho, Luis C.
name: Luo, Bin
name: Yan, Wei
name: Schneider, D. P.
name: Paul, Jeremiah D.
name: Plotkin, Richard M.
name: Yang, Jinyi
name: Wang, Feige
name: He, Zhicheng
name: Chen, Chen
name: Wu, Xue-Bing
name: Bai, Jin-Ming
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the first near-IR spectroscopy and joint analyses of multi-wavelength observations for SDSS J082747.14+425241.1, a dust-reddened, weak broad emission-line quasar (WLQ) undergoing a remarkable broad absorption line (BAL) transformation. The systemic redshift is more precisely measured to be $z=2.070\pm0.001$ using H$β$ compared to $z=2.040\pm0.003$ using \mgii\ from the literature, signifying an extreme \mgii\ blueshift of $2140\pm530$ \kms\ relative to H$β$. Using the H$β$-based single-epoch scaling relation with a systematic uncertainty of 0.3 dex, its black hole (BH) mass and Eddington ratio are estimated to be $M_{\rm BH}\sim6.1\times10^8M_\odot$ and $λ_{\rm Edd}\sim0.71$, indicative of being in a rapidly accreting phase. Our investigations confirm the WLQ nature and the LoBAL$\rightarrow$HiBAL transformation, along with a factor of 2 increase in the \mgii+\feii\ emission strength and a decrease of 0.1 in $E(B-V)$ over two decades. The kinetic power of this LoBAL wind at $R\sim$15 pc from its BH is estimated to be $\sim$43\% of the Eddington luminosity, sufficient for quasar feedback upon its host galaxy albeit with an order-of-magnitude uncertainty. This quasar provides a clear example of the long-sought scenario where LoBAL quasars are surrounded by dust cocoons, and wide-angle nuclear winds play a key role in the transition for red quasars evolving into the commonly seen blue quasars.
description: 11 pages, 6 figures, accepted for publication in ApJ
E:Studio: Virtual City>Future City
Creators: name: Wilkins, Gretchen
name: Nazareth, Ian
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 330102
subject: Architectural design

description: BACKGROUND: The article: "E:Studio: Virtual City>Future City" focuses on the relationship between urban education and the production of the city itself, explored through a project called 'e:Studio'. It was published in Urban Pamphleteer - a series launched by the Urban Lab+ at the University College London (UCL). Urban Pamphleteer #5: Global Education for Urban Futures selected articles and projects from an international group of entries. It was launched at the Bartlett in London, coinciding with the symposium 'Global Urban Higher Education: the Challenges and Potentials of Internationalisation.' CONTRIBUTION: The article discusses the 'e:Studio' project, in terms of the need to enhance local, face-to-face design collaboration with remote, globally networked online interaction, especially for urban, design-based practices. It outlines the structural and conceptual approach to the e:studio platform, a model for blended urban collaboration and education designed for implementation in design programs at RMIT University. The accompanying symposium presentation 'Global Constructs: a platform for comparative, collaborative urban education' expanded this project to a global context. The research sits at the intersection of urban-based design research, teaching and practice, focusing on technologies of collaboration. It contributes to research in educational and professional technology, design and the production of urban knowledge. SIGNIFICANCE: The significance of the article is evidenced by its publication in a peer-reviewed (abstract only), international publication and symposium/paper presentation. UCL Urban Lab+ - a globally renowned university and well-established urban research unit - is the publisher and host, alongside academic partners which are also highly-ranked, globally positioned educational institutions.
Sezione di Museologia Scientifica e Naturalistica, Vol 7 (2011)
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Le ichnocenosi delle successioni sedimentarie Eocenico-Mioceniche affioranti tra il Lago Trasimeno e l'Alpe di Poti (Appennino Settentrionale)...1-104
Revisiting the role of bars in AGN fuelling with propensity score sample matching
Creators: name: Silva-Lima, Luiz A.
name: Martins, Lucimara P.
name: Coelho, Paula R. T.
name: Gadotti, Dimitri A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The high luminosity displayed by an active galactic nucleus (AGN) requires that gas be transported to the centre of the galaxy by some mechanism. Bar-driven processes are often pointed out in this context and a number of studies have addressed the bar-AGN connection, but with conflicting results. Some of the inconsistencies can be explained by the different spatial- and timescales involved in bar-driven gas inflows, accretion by the central black hole, and AGN emission. However, the discrepant results could also be due to sample biases, because both the AGN activity determination and the bar detection are influenced by the method employed. We revisit the bar-AGN connection in a sample of galaxies from SDSS, looking for evidence of the influence of bars on AGN activity. We determine AGN activity by emission line diagnostics and the properties of the bar were previously estimated with \texttt{BUDDA}, which performs 2D bulge-bar-disk decomposition. Before comparing active and inactive galaxies, we made a careful selection of the sample to minimise selection biases. We created control samples by matching them with the AGN sample using propensity score matching. This technique offers an analytical approach for creating control samples given some object parameters. We find that AGN are preferentially found in barred galaxies and that the accretion rate is higher in barred galaxies, but only when different M-$σ$ relations are used to estimate the black hole mass M$_\bullet$ in barred and unbarred galaxies (from the central velocity dispersion $σ$). On the other hand, we find no correlation between activity level and bar strength. Altogether, our results strengthen theoretical predictions that the bar is an important mechanism in disc galaxies, creating a gas reservoir to feed AGN, but they also indicate that other mechanisms can play a major role, particularly at scales
'Back from the Front', Art, Memory and the Aftermath of War (Original Textual Work)
Creators: name: Gough, Paul
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 360699
subject: Visual arts not elsewhere classified

description: Field of enquiry (published texts, practice-based studio works, curatorial) is framed within the discourse of cultural memory, within the iconography of war and peace, with a particular focus on contemporary representations of recent war by living artists. Gough is selected and shown in the Imperial War Museum, London: New Zealand War Memorial, Wellington; The Canadian War Museum, Ottawa, Canada. Key exponents of the representation of war and peace include many of the artists that Gough invited to be in these exhibitions and recorded in the accompanying large-scale and online catalogue. Research questions: How does the informed studio practitioner create visual language capable of capturing the vast scale of global warfare; What practice-based approach is best deployed to convey the essentials of trauma, recovery, peace and commemoration; How can practice-based enquiry inform the field of memory studies within the greater discourse of practice-based studio arts, photography, jewellery, media; How can these lines of enquiry be captured on-line and book format through a catalogue of text, image and provocation? Significance: On-line e-catalogue; 208 full colour page catalogue. https://itunes.apple.com/us/book/back-from-the-front/id980887643?mt=11 Invitations to contribute to academic debate, conferences, peer-reviewed publications, exhibitions, battlefield conservation and the heritage of sites of memory: Significant attention from media; including Al Jazeera television; G2 Guardian Newspaper, 27/7; Royal Academy Week. Significant online debate: Dr David Kelly biographer - 'Robert Lewis Review' http://robertlewis.com/blog/shock-awe-academy/ Brothers in Art / Brothers in Arms' in Country Life; Frances Spalding The Literary Review, 8/14; Gough on 'Free thinking', BBC Radio 3, 10pm 1st July 2014 ; http://www.bbc.co.uk/programmes/b048bm10 Gough commissioned by British Library http://www.bl.uk/world-war-one/articles/why-paint-war-british-and-belgian-artists
Shallow Transits -- Deep Learning II: Identify Individual Exoplanetary Transits in Red Noise using Deep Learning
Creators: name: Dvash, Elad
name: Peleg, Yam
name: Zucker, Shay
name: Giryes, Raja
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Image and Video Processing (eess.IV)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In a previous paper, we have introduced a deep learning neural network that should be able to detect the existence of very shallow periodic planetary transits in the presence of red noise. The network in that feasibility study would not provide any further details about the detected transits. The current paper completes this missing part. We present a neural network that tags samples that were obtained during transits. This is essentially similar to the task of identifying the semantic context of each pixel in an image -- an important task in computer vision, called `semantic segmentation', which is often performed by deep neural networks. The neural network we present makes use of novel deep learning concepts such as U-Nets, Generative Adversarial Networks (GAN), and adversarial loss. The resulting segmentation should allow further studies of the light curves which are tagged as containing transits. This approach towards the detection and study of very shallow transits is bound to play a significant role in future space-based transit surveys such as PLATO, which are specifically aimed to detect those extremely difficult cases of long-period shallow transits. Our segmentation network also adds to the growing toolbox of deep learning approaches which are being increasingly used in the study of exoplanets, but so far mainly for vetting transits, rather than their initial detection.
description: 16 pages, 14 figures, accepted for publication in the Astronomical Journal
Data visualization as an intervention for pediatric chronic pain : a pilot feasibility study protocol for a randomized controlled crossover trial
Creators: name: Boerner, Katelynn E.
name: Desai, Unma
name: MacLean, Karon
name: Munzner, Tamara
name: Foladare, Haley
name: Gill, Javed
name: Oberlander, Tim F.
Publisher: name: BioMed Central
Year: 2023

description: Background: Chronic pain is a common and costly condition in youth, associated with negative implications that reach far beyond the pain experience itself (e.g., interference with recreational, social, and academic activities, mental health sequelae). As a self-appraised condition, pain experience is influenced by patient’s biases and meaning-making in relation to their symptoms and triggers. We propose that interacting with self-reported data will impact the experience of pain by altering understanding and expectations of symptom experience and how pain interacts with other factors (e.g., sleep, emotions, social interactions). In this study, we aim to establish the feasibility and acceptability of using a data visualization platform to track and monitor symptoms and their relationship with other factors, versus simply daily reporting of symptoms using a smartphone-based Ecological Momentary Assessment (EMA). Methods This protocol is for a randomized, single-center, open-label crossover trial. We aim to recruit 50 typically developing youth aged 12–18 years with chronic pain to take part in two phases of data collection. The trial will utilize an A-B counterbalanced design in which participants will be randomly assigned to receive either Part A (EMA alone for 7 days) or Part B (EMA plus visualization platform for 7 days) first and then receive the opposite phase after a 7-day break (washout period). Key outcomes will be participant reports of acceptability and feasibility, EMA completion rates, barriers, and perceptions of the benefits or risks of participation. Secondary exploratory analyses will examine the relationship between EMA-reported symptoms over time and in relation to baseline measures, as well as pilot data on any improvements in symptoms related to engaging with the data visualization platform. Discussion This protocol describes the feasibility and pilot testing of a novel approach to promoting self-management and facilitating symptom appraisal using visualized data. We aim to determine whether there is a sufficient rationale, both from the perspective of feasibility and patient satisfaction/acceptability, to conduct a larger randomized controlled trial of this intervention. This intervention has the potential to support clinical care for youth with chronic pain and other conditions where self-appraisal and understanding of symptom patterns are a critical component of functional recovery. Trial registration Open Science Framework doi: https://doi.org/10.17605/OSF.IO/HQX7C . Registered on October 25, 2021, osf.io/hqx7c
title: Sezione di Museologia Scientifica e Naturalistica, 2005: Volume Speciale
title: Volume Speciale
titleType: AlternativeTitle
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Fugagnoli A. and Bassi D. (Eds) 2005. Giornata di Studi Paleontologici "Prof. C. Loriga Broglio". Ferrara, 18th June 2004
description: Foreword...1-4
Geochemical changes at the Permian–Triassic transition in Southern Alps and adjacent area: a review...5-12
Bivalve reefs from the Upper Triassic of Iran...13-24
Feeding specializations in Late Triassic fishes...25-32
Biofacies evolution in the Triassic platforms of the Dolomites, Italy...32-44
Calcimicrobial oncoid coatings from the Pliensbachian Massone Member (Calcari Grigi Formation, Trento Platform, Italy). Preliminary communication....45-50
The Middle Eocene siliceous sponges from Val di Chiampo (Lessini Mountains, northern Italy)...51-62
The Upper Eocene crustose coralline algal pavement in the Colli Berici, north-eastern Italy...63-74
Pliocene foraminifera of Piedmont (north-western Italy): a synthesis of recent studies...75-88
New stratigraphic and taphonomic data from the late Pleistocene deposits of the San Teodoro Cave (North-Eastern Sicily, Italy)...89-98
Mammalian faunas and environment from the Würmian Glacial Maximum of the Italian peninsula (approx. 22±2 ka cal BP)...99-104
Paleoecological interpretation of a Holocene sand body in the coastal area of Phetchaburi, Gulf of Thailand...105-114
Bryozoans and serpuloideans in skeletobiont communities from the Pleistocene of Sicily: spatial utilisation and competitive interactions...115-124
Onset of depression and anxiety among patients with gout after diagnosis : a population-based incident cohort study
Creators: name: Howren, Alyssa
name: Sayre, E. C.
name: Choi, Hyon K.
name: Aviña-Zubieta, J. Antonio
name: Shojania, Kam
name: Park, Jamie Y.
name: De Vera, Mary
Publisher: name: BioMed Central
Year: 2024

description: Background: Gout may be associated with an increased incidence of mental health disorders, however, published findings have been limited and inconsistent. Therefore, our objective was to conduct a population-based cohort study to evaluate the incidence of depression and anxiety after gout diagnosis. Methods: We used linked population-based administrative health data in British Columbia, Canada that includes information on demographics, outpatient visits, and inpatient visits from the period of January 1, 1990 to March 31, 2018. We assessed depression and anxiety using validated International Classification of Diseases, 9th and 10th Revision coding algorithms. We applied multivariable Cox proportional hazard models to evaluate incident depression and anxiety among patients with gout in comparison to non-gout controls, adjusting for age, sex, neighbourhood income quintile, residence, comorbidities, and health care utilization. Results: We included 157,426 incident cases of gout (60.2% male; mean age 57.1 years) and 157,426 non-gout controls (60.2% male; mean age 56.9 years). The incidence rate of depression among individuals with gout and non-gout controls was 12.9 (95% confidence interval [CI] 12.7–13.2) and 11.1 (95% CI 10.9–11.4) per 1000 person-years, respectively. The incidence rate of anxiety for those with gout was 5.4 (95% CI 5.3–5.5) per 1000 person-years and for non-gout controls was 4.6 (95% CI 4.4–4.7) per 1000 person-years. Individuals with gout had an increased onset of depression (adjusted hazard ratio [aHR], 1.08; 95% CI 1.05–1.11) and anxiety (aHR, 1.10; 95% CI 1.05–1.14) compared to non-gout controls. Conclusion: Our population-based study shows an increased incidence of depression and anxiety following gout diagnosis in comparison to non-gout controls. Findings suggest the importance of considering psychiatric impacts in addition to the physical impacts of gout.
Searching for pulsars associated with polarised point sources using LOFAR: Initial discoveries from the TULIPP project
Creators: name: Sobey, C.
name: Bassa, C. G.
name: O'Sullivan, S. P.
name: Callingham, J. R.
name: Tan, C. M.
name: Hessels, J. W. T.
name: Kondratiev, V. I.
name: Stappers, B. W.
name: Tiburzi, C.
name: Heald, G.
name: Shimwell, T.
name: Breton, R. P.
name: Kirwan, M.
name: Vedantham, H. K.
name: Carretti, Ettore
name: Grießmeier, J. -M.
name: Haverkorn, M.
name: Karastergiou, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Discovering radio pulsars, particularly millisecond pulsars (MSPs), is important for a range of astrophysical applications, such as testing theories of gravity or probing the magneto-ionic interstellar medium. We aim to discover pulsars that may have been missed in previous pulsar searches by leveraging known pulsar observables (primarily polarisation) in the sensitive, low-frequency radio images from the Low-Frequency Array (LOFAR) Two-metre Sky Survey (LoTSS), and have commenced the Targeted search, using LoTSS images, for polarised pulsars (TULIPP) survey. For this survey, we identified linearly and circularly polarised point sources with flux densities brighter than 2 mJy in LoTSS images at a centre frequency of 144 MHz with a 48 MHz bandwidth. Over 40 known pulsars, half of which are MSPs, were detected as polarised sources in the LoTSS images and excluded from the survey. We have obtained beam-formed LOFAR observations of 30 candidates, which were searched for pulsations using coherent de-dispersion. Here, we present the results of the first year of the TULIPP survey. We discovered two pulsars, PSRs J1049+5822 and J1602+3901, with rotational periods of P=0.73 s and 3.7 ms, respectively. We also detected a further five known pulsars (two slowly-rotating pulsars and three MSPs) for which accurate sky positions were not available to allow a unique cross-match with LoTSS sources. This targeted survey presents a relatively efficient method by which pulsars, particularly MSPs, may be discovered using the flexible observing modes of sensitive radio telescopes such as the Square Kilometre Array and its pathfinders/precursors, particularly since wide-area all-sky surveys using coherent de-dispersion are currently computationally infeasible.
description: 15 pages, 7 figures, 3 tables. Accepted for publication in A&A
Alophophion mapuche Alvarado 2014
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Alophophion
Alophophion mapuche

description: 15.1.13 Alophophion mapuche Alvarado, 2014
Distribution. Neotropical; Chile: Región de Coquimbo (Alvarado 2014); Región de Valparaíso (Alvarado 2014).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 32, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Supplementary document for Ultrafast dynamics and internal processing mechanism of silica glass under double-pulse femtosecond laser irradiation - 7151667.pdf
Creators: name: Ren, Guoqi
name: Ito, Yusuke
name: Yoshizaki, Reina
name: Sun, Huijie
name: Hattori, Junya
name: Sugita, Naohiko
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Supplement 1
Supplementary document for Recalibration of the nonlinear optical coefficients of BaGa₄Se₇ crystal using second-harmonic-generation method - 5541028.pdf
Creators: name: Zhao, XueZhi
name: Bai, Jinzhou
name: li, chunxiao
name: wang, zhengping
name: Yao, Jiyong
name: Tan, Rongqing
name: Xu, Xin-guang
Publisher: name: Optica Publishing Group
Year: 2025
Subjects: Uncategorized

description: Supplement 1
title: Sezione di Museologia Scientifica e Naturalistica, 2007: Volume Speciale
title: Volume Speciale
titleType: AlternativeTitle
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Introduzione e Indice...I-VII
Ambiente e Territorio...1-14
Modalità insediative...15-49
Strategie di sussistenza...50-102
Arte e spiritualità...103-124
Evoluzione biologica e culturale...125-156
Tecnologie applicate alla ricerca archeologica...157-198
Supplementary document for Recalibration of the nonlinear optical coefficients of BaGa₄Se₇ crystal using second-harmonic-generation method - 5541028.pdf
Creators: name: Zhao, XueZhi
name: Bai, Jinzhou
name: li, chunxiao
name: wang, zhengping
name: Yao, Jiyong
name: Tan, Rongqing
name: Xu, Xin-guang
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Supplement 1
Sezione di Museologia Scientifica e Naturalistica, Vol 2 (2006)
Creators: name: Sezione Di Museologia Scientifica E Naturalistica
Publisher: name: Sezione di Museologia Scientifica e Naturalistica
Year: 2013

description: Foraminiferal shell structures: exoskeleton and endoskeleton....1
Foraminiferal shell structures: additional cavity systems produced by supplemental skeletons....2
Initiation of Alfvénic turbulence by Alfven wave collisions: A numerical study
Creators: name: Shestov, S. V.
name: Voitenko, Y. M.
name: Zhukov, A. N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: In the framework of compressional magnetohydrodynamics (MHD), we numerically studied the commonly accepted presumption that the Alfvénic turbulence is generated by the collisions between counter-propagating Alfvén waves (AWs). In the conditions typical for the low-beta solar corona and inner solar wind, we launched two counter-propagating AWs in the three-dimensional simulation box and analyzed polarization and spectral properties of perturbations generated before and after AW collisions. The observed post-collisional perturbations have different polarizations and smaller cross-field scales than the original waves, which supports theoretical scenarios with direct turbulent cascades. However, contrary to theoretical expectations, the spectral transport is strongly suppressed at the scales satisfying the classic critical balance of incompressional MHD. Instead, a modified critical balance can be established by colliding AWs with significantly shorter perpendicular scales. We discuss consequences of these effects for the turbulence dynamics and turbulent heating of compressional plasmas. In particular, solar coronal loops can be heated by the strong turbulent cascade if the characteristic widths of the loop substructures are more than ten times smaller than the loop width. The revealed new properties of AW collisions have to be incorporated in the theoretical models of AW turbulence and related applications.
description: 9 pages, 9 figures
The Abyssinian Contortionist
Creators: name: Carlin, David
Publisher: name: RMIT University
Year: 2024
Subjects: classificationCode: 360201
subject: Creative writing (incl. scriptwriting)

description: BACKGROUND This research sits within the field of nonfiction literary practice, specifically intervening in debates around new forms and approaches to autobiography, memoir and biography within a post-human, post-Cartesian and post-colonial understanding of embodied voice. It forms part of a body of work including my previous memoir Our father who wasn't there and numerous shorter essay/memoir works that investigate questions of voice, narrativity and subject/object relationships. Key practitioners and theorists in this field include Solnit, Kapuscinsky, Gornick, Klaus, Maggie Nelson and many others. CONTRIBUTION This work asks how one can approach writing the story of another person's life, across differences of gender, culture and geography. It places the 'story' of Sosina Wogayehu, an Ethiopian-Australian asylum-seeker, within a broader context of the history of Western cultural perceptions of Africa. It does so using techniques of personal reflection and narration, combined with ethnographic observation and historical research. It breaks new ground by dramatizing, within its narrative structure, the question of how stories are told and by whom, within a 'negotiated memoir' (Carlin 2011). SIGNIFICANCE The subject of the book is an internationally renowned circus performer. The book intervenes in vital international issues including zenophobia, race relations and asylum seekers. Subsequent to the book's publication, Sosina Wogayehu has been granted $20,000 by DFAT towards establishing a new circus school in Addis Ababa. The book received funding of $11,000 from Harold Mitchell Foundation and was published by innovative trade publisher UWA Publishing. It has been nationally reviewed in Australia and spotlighted at multiple festivals and conferences in the US, The Philippines and Australia. Two leading Australian arts festivals are now commissioning an adaptation of the book into a stageplay.
Testing the empirical relationship between Forbush decreases and cosmic ray diurnal anisotropy
Creators: name: Alhassan, Jibrin Adejoh
name: Okike, Ogbonnaya
name: Chukwude, Augustine Ejikeme
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The abrupt aperiodic modulation of cosmic ray (CR) flux intensity, often referred to as Forbush decrease (FD), plays a significant role in our understanding of the Sun-Earth electrodynamics. Accurate and precise determination of FD magnitude and timing are among the intractable problems in FD-based analysis. FD identification is complicated by CR diurnal anisotropy. CR anisotropy can increase or reduce the number and amplitude of FDs. It is therefore important to remove its contributions from CR raw data before FD identification. Recently, an attempt was made, using a combination of Fourier transformed technique and FD-location machine to address this. Thus, two FD catalogs and amplitude diurnal variation (ADV) were calculated from filtered (FD1 and ADV) and raw (FD2) CR data. In the current work, we test the empirical relationship between FD1, FD2, ADV, and solar-geophysical characteristics. Our analysis shows that two types of magnetic fields-interplanetary (IMF) and geomagnetic (Dst) govern the evolution of CR flux intensity reductions.
description: 17 pages, 5 figures, 9 tables, Accepted in Research in Astronomy and Astrophysics
Alophophion mapudungun Alvarado 2014
Creators: name: Araujo, Rodrigo O.
name: Fernandes, Daniell R. R.
name: Pos, Davide Dal
name: Giovanni, Filippo Di
name: Moreira-Muñoz, Andrés
name: Pádua, Diego G.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Alophophion
Alophophion mapudungun

description: 15.1.14 Alophophion mapudungun Alvarado, 2014 *
Distribution. Chile: Región de Atacama (Alvarado 2014); Región de Coquimbo (Alvarado 2014); Región de Valparaíso (Alvarado 2014).
description: Published as part of Araujo, Rodrigo O., Fernandes, Daniell R. R., Pos, Davide Dal, Giovanni, Filippo Di, Moreira-Muñoz, Andrés & Pádua, Diego G., 2025, Unveiling the secrets of South American Darwin wasps, part I: a comprehensive checklist of the Chilean Ichneumonidae (Hymenoptera: Ichneumonoidea), pp. 1-51 in Zootaxa 5631 (1) on page 32, DOI: 10.11646/zootaxa.5631.1.1, http://zenodo.org/record/15326657
Ventricular septal rupture complicating acute myocardial infarction
Creators: name: David, Arthur
Publisher: name: EURORAD
Year: 2016
Subjects: subject: Cardiac
subject: Veins / Vena cava
subject: CT
subject: Diagnostic procedure
subject: Ischaemia / Infarction

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 83 years
description: Clinical History: A 83 year-old male patient was admitted in our institution because of cardiogenic shock and 1-day history of chest pain. Bedside echocardiography was performed by the emergency physician and revealed hyperechoic pericardial effusion. Final Diagnosis: Ventricular septal rupture.
Convective Penetration in Early-Type Stars
Creators: name: Jermyn, Adam S.
name: Anders, Evan H.
name: Lecoanet, Daniel
name: Cantiello, Matteo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Observations indicate that the convective cores of stars must ingest a substantial amount of material from the overlying radiative zone, but the extent of this mixing and the mechanism which causes it remain uncertain. Recently, Anders et al. (2021) developed a theory of convective penetration and calibrated it with 3D numerical hydrodynamics simulations. Here we employ that theory to predict the extent of convective boundary mixing in early-type main-sequence stars. We find that convective penetration produces enough mixing to explain core masses inferred from asteroseismology and eclipsing binary studies, and matches observed trends in mass and age. While there are remaining uncertainties in the theory, this agreement suggests that most convective boundary mixing in early-type main-sequence stars arises from convective penetration. Finally, we provide a fitting formula for the extent of core convective penetration for main-sequence stars in the mass range from $1.1-60 M_\odot$.
description: 10 pages, 8 figures. Accepted in ApJ
Semi-synthetic bile acids as novel drug candidate in liver diseases: physico-chemical characterization and HPLC-ES-MS/MS methods for their quali-quantitative analysis in different experimental animal models
Creators: name: Camborata, Cecilia <1987>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2015
Subjects: CHIM/01 Chimica analitica

description: The physico-chemical characterization, structure-pharmacokinetic and metabolism studies of new semi synthetic analogues of natural bile acids (BAs) drug candidates have been performed. 
Recent studies discovered a role of BAs as agonists of FXR and TGR5 receptor, thus opening new therapeutic target for the treatment of liver diseases or metabolic disorders. Up to twenty new semisynthetic analogues have been synthesized and studied in order to find promising novel drugs candidates. 
In order to define the BAs structure-activity relationship, their main physico-chemical properties (solubility, detergency, lipophilicity and affinity with serum albumin) have been measured with validated analytical methodologies. Their metabolism and biodistribution has been studied  in “bile fistula rat”, model where each BA is acutely administered through duodenal and femoral infusion and bile collected at different time interval allowing to define the relationship between structure and intestinal absorption and hepatic uptake ,metabolism and systemic spill-over. 
One of the studied analogues, 6α-ethyl-3α7α-dihydroxy-5β-cholanic acid, analogue of CDCA (INT 747, Obeticholic Acid (OCA)), recently under approval for the treatment of cholestatic liver diseases, requires additional studies to ensure its safety and lack of toxicity when administered to patients with a strong liver impairment.
For this purpose, CCl4 inhalation to rat causing hepatic decompensation (cirrhosis) animal model has been developed and used to define the difference of OCA biodistribution in respect to control animals trying to define whether peripheral tissues might be also exposed as a result of toxic plasma levels of OCA, evaluating also the endogenous BAs biodistribution.
An accurate and sensitive HPLC-ES-MS/MS method is developed to identify and quantify all BAs in biological matrices (bile, plasma, urine, liver, kidney, intestinal content and tissue) for which a sample pretreatment have been optimized.
Generating unrepresented proportions of geological facies using Generative Adversarial Networks
Creators: name: Abdellatif, Alhasan
name: Elsheikh, Ahmed H.
name: Graham, Gavin
name: Busby, Daniel
name: Berthet, Philippe
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: In this work, we investigate the capacity of Generative Adversarial Networks (GANs) in interpolating and extrapolating facies proportions in a geological dataset. The new generated realizations with unrepresented (aka. missing) proportions are assumed to belong to the same original data distribution. Specifically, we design a conditional GANs model that can drive the generated facies toward new proportions not found in the training set. The presented study includes an investigation of various training settings and model architectures. In addition, we devised new conditioning routines for an improved generation of the missing samples. The presented numerical experiments on images of binary and multiple facies showed good geological consistency as well as strong correlation with the target conditions.
Biomedical engineering for healthy ageing. Predictive tools for falls
Creators: name: Palumbo, Pierpaolo <1986>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2015
Subjects: ING-INF/06 Bioingegneria elettronica e informatica

description: Falls are common and burdensome accidents among the elderly. About one third of the population aged 65 years or more experience at least one fall each year. Fall risk assessment is believed to be beneficial for fall prevention. This thesis is about prognostic tools for falls for community-dwelling older adults.
We provide an overview of the state of the art. We then take different approaches: we propose a theoretical probabilistic model to investigate some properties of prognostic tools for falls; we present a tool whose parameters were derived from data of the literature; we train and test a data-driven prognostic tool. Finally, we present some preliminary results on prediction of falls through features extracted from wearable inertial sensors.
Heterogeneity in validation results are expected from theoretical considerations and are observed from empirical data. Differences in studies design hinder comparability and collaborative research. According to the multifactorial etiology of falls, assessment on multiple risk factors is needed in order to achieve good predictive accuracy.
Non-thermal emission in hyper-velocity and semi-relativistic stars
Creators: name: Martinez, J. R.
name: del Palacio, S.
name: Bosch-Ramon, V.
name: Romero, G. E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Context. There is a population of runaway stars that move at extremely high speeds with respect to their surroundings. The fast motion and the stellar wind of these stars, plus the wind-medium interaction, can lead to particle acceleration and non-thermal radiation. Aims. We characterise the interaction between the winds of fast runaway stars and their environment, in particular to establish their potential as cosmic-ray accelerators and non-thermal emitters. Methods. We model the hydrodynamics of the interaction between the stellar wind and the surrounding material. We self-consistently calculate the injection and transport of relativistic particles in the bow shock using a multi-zone code, and compute their broadband emission from radio to $γ$-rays. Results. Both the forward and reverse shocks are favourable sites for particle acceleration, although the radiative efficiency of particles is low and therefore the expected fluxes are in general rather faint. Conclusions. We show that high-sensitivity observations in the radio band can be used to detect the non-thermal radiation associated with bow shocks from hypervelocity and semi-relativistic stars. Hypervelocity stars are expected to be modest sources of sub-TeV cosmic rays, accounting perhaps for a $\sim 0.1$% of that of galactic cosmic rays.
description: 11 pages, 8 figures, accepted for publication section 2. Astrophysical processes of Astronomy and Astrophysics