bluuebunny/crossref_metadata_2025_split huggingface dataset:
Advancing Clinical Decision Making Through Trauma-Informed Care in Pediatric Hearing Health Care
Authors: Sprouse Brittney J. 
Published: January 2024

Purpose:
Adverse childhood experiences affect early brain development and future health outcomes. The principles of trauma-informed care (TIC) incorporate safety, screening, understanding context, avoiding retraumatization, and discharge planning to provide optimal care for patients and families. Secondary traumatic stress is the trauma providers' experience when serving patients and families who have experienced trauma. The purpose of this article is to examine the impact of trauma, investigate the principles of TIC, and identify the ways to implement it in hearing health care.

Conclusions:
Providers working with children and families who have experienced trauma should be trained to provide a trauma-informed approach and learn the signs, symptoms, and risks of secondary traumatic stress. To improve the quality of care for children with hearing loss who have experienced trauma, their adverse experiences must be considered with trauma-informed techniques incorporated into the hearing health care model of care.
Optimized time varying parameters of the power balance equation model for electric arc furnaces
Authors: Babaei Zahra , Samet Haidar 
Published: January 2024

AbstractAn accurate model of electric arc furnaces (EAFs) is required to analyse their impact on the system's power quality. One of the well‐known approaches to model EAF is using the power balance equation. This model has two terms, each one has a coefficient named the model parameter. Also, both terms are powered to values, which are called model orders. So, the model includes two model parameters and two model orders. Model orders highly affect the modelling precision. The optimum model orders have not been obtained yet in previous studies. Here, based on many actual records from EAFs, the best model orders for refining, melting, and scrapping stages are attained. Unlike the original power balance equation which has constant model parameters, the first proposed model uses the attained optimal model orders with the time‐varying model parameters. In the second proposed model, the model orders are also considered time‐varying. Model parameters, which are updated every 10 ms, are obtained using autoregressive moving average (ARMA) models. The correctness of the models is assessed by calculating some important electric quantities using the actual data and the proposed models. Finally, the time‐varying parameters are generated using two MATLAB codes.
SWISS rectifier structure sector boundary current distortion suppression based on multi‐step predictive control
Authors: Cheng Zhun , Deng Jiangwei , Luo Bing , Zhang Yang 
Published: January 2024

AbstractThe SWISS rectifier is a three‐phase BUCK type Power Factor Correction rectifier with the advantages of adjustable output full voltage range, low voltage stress in the back stage devices, and high efficiency. However, because the voltage ripple of the input filter capacitor will cause the input current deviation, the input current of the SWISS rectifier will produce distortion at the sector boundary, which will affect the system performance. To this end, a multi‐stage predictive model method based on the spherical algorithm is presented. By predicting the grid‐side capacitor voltage and the input current state of the rectifier, the harmonic injection network switching tube is controlled in advance to supplement the grid‐side capacitor voltage, so that the grid‐side capacitor voltage approximately tracks the input voltage. Meanwhile, considering the current step that may be generated after the current distortion returns to normal, which leads to the resonance problem with the pre‐stage filter, this problem is incorporated into the value function and damping is optimized according to the feedback value. Finally, a 10‐kW SWISS rectifier on the SIMULINK platform is used to verify the feasibility of the new control method.
Galaxy main sequence and properties of low-mass Lyman-α emitters towards reionisation as viewed by VLT/MUSE and JWST/NIRCam
Authors: Goovaerts I. , Pello R. , Burgarella D. , Thai T. T. , Richard J. , Claeyssens A. , Tuan-Anh P. , Arango-Toro R. C. , Boogaard L. , Contini T. , Guo Y. , Langan I. , Laporte N. , Maseda M. 
Published: January 2024

Context. Faint, star-forming galaxies are likely to play a dominant role in cosmic reionisation. Great strides have been made in recent years to characterise these populations at high redshifts (z > 3). Now, for the first time, with JWST photometry beyond 1 μm in the rest frame, we can derive accurate stellar masses and position these galaxies on the galaxy main sequence.
Aims. We seek to assess the place of 96 individual Lyman-α emitters (LAEs) selected behind the A2744 lensing cluster with MUSE IFU spectroscopy on the galaxy main sequence. We also compare the derived stellar masses to Lyman-α luminosities and equivalent widths to better quantify the relationship between the Lyman-α emission and the host galaxy.
Methods. These 96 LAEs lie in the redshift range of 2.9 < z < 6.7, with their range of masses extending down to 106 M⊙ (over half with M⋆ < 108 M⊙). We used the JWST/NIRCam and HST photometric catalogues from the UNCOVER project, giving us excellent wavelength coverage from 450 nm to 4.5 μm. We also performed an SED fitting using CIGALE, fixing the redshift of the LAEs to the secure, spectroscopic value. This combination of photometric coverage with spectroscopic redshifts allows us to robustly derive stellar masses for these galaxies.
Results. We found a main sequence relation for these low-mass LAEs of log SFR = (0.88 ± 0.07 − 0.030 ± 0.027 × t) log M⋆ − (6.31 ± 0.41 − 0.08 ± 0.37 × t). This is in relative agreement with the best-fit results of prior collated studies; however, here we see a steeper slope and a higher normalisation. This indicates that low-mass LAEs towards the epoch of reionisation lie above the typical literature main sequence relations derived at lower redshift and higher masses. In addition, by comparing our results to UV-selected samples, we can see that while low-mass LAEs lie above these typical main sequence relations, they are likely not singular in this respect at these particular masses and redshifts. While low-mass galaxies have been shown to play a significant role in cosmic reionisation, our results point to the likelihood that LAEs hold no special position in this regard.
TELAMON: Effelsberg monitoring of AGN jets with very-high-energy astroparticle emission
Authors: Eppel F. , Kadler M. , Heßdörfer J. , Benke P. , Debbrecht L. , Eich J. , Gokus A. , Hämmerich S. , Kirchner D. , Paraschos G. F. , Rösch F. , Schulga W. , Sinapius J. , Weber P. , Bach U. , Dorner D. , Edwards P. G. , Giroletti M. , Kraus A. , Hervet O. , Koyama S. , Krichbaum T. P. , Mannheim K. , Ros E. , Zacharias M. , Zensus J. A. 
Published: January 2024

Aims.We introduce the TELAMON program which is using the Effelsberg 100-m telescope to monitor the radio spectra of active galactic nuclei (AGN) under scrutiny in astroparticle physics, specifically TeV blazars and candidate neutrino-associated AGN. Here, we present and characterize our main sample of TeV-detected blazars.Methods.We analyzed the data sample from the first ∼2.5 yr of observations between August 2020 and February 2023 in the range from 14 GHz to 45 GHz. During this pilot phase, we observed all 59 TeV-detected blazars in the Northern Hemisphere (i.e., Dec > 0°) known at the time of observation. We discuss the basic data reduction and calibration procedures used for all TELAMON data and introduce a sub-band averaging method used to calculate average light curves for the sources in our sample.Results.The TeV-selected sources in our sample exhibit a median flux density of 0.12 Jy at 20 mm, 0.20 Jy at 14 mm, and 0.60 Jy at 7 mm. The spectrum for most of the sources is consistent with a flat radio spectrum and we found a median spectral index (S(ν)∝να) ofα = −0.11. Our results on flux density and spectral index are consistent with previous studies of TeV-selected blazars. Compared to the GeV-selected F-GAMMA sample, TELAMON sources are significantly fainter in the radio band. This is consistent with the double-humped spectrum of blazars being shifted towards higher frequencies for TeV-emitters (in particular for high-synchrotron peaked BL Lac type objects), which results in a lower radio flux density. The spectral index distribution of our TeV-selected blazar sample is not significantly different from the GeV-selected F-GAMMA sample. Moreover, we present a strategy to track the light curve evolution of sources in our sample for future variability and correlation analysis.
Correlation between accretion rate and free-free emission in protoplanetary disks
Authors: Rota A. A. , Meijerhof J. D. , van der Marel N. , Francis L. , van der Tak F. F. S. , Sellek A. D. 
Published: January 2024

Context. The inner regions of protoplanetary disks are believed to be the primary locations of planet formation and the processes that influence the global evolution of the disk, such as magnetohydrodynamic winds and photoevaporation. Transition disks with large inner dust cavities are ideal targets for studying the inner regions (of tens of au) of disks, as this is where the central emission can be fully disentangled from the outer disk emission.
Aims. We present a homogeneous multiwavelength analysis of the continuum emission in a sample of 11 transition disks. We investigate the nature of the central emission close to the star, distinguishing between thermal dust and free-free emission.
Methods. We combined spatially resolved measurements of continuum emission from the archival Atacama Large Millimeter/Submillimeter Array data with centimeter-wave (cm-wave) observations from the literature to study the spectral indices of the inner and outer disks separately.
Results. While the emission from the outer disks is consistent with thermal dust emission, 10 out of 11 of the spectral indices estimated for the central emission close to the star suggest that this emission is free-free emission that is likely associated with an ionized jet or a disk wind. We found no correlation between the free-free luminosity and the accretion luminosity or the X-ray luminosity and this argues against an explanation based on a potential photoevaporative wind. A sub-linear correlation between the ionized mass loss rate and the accretion rate onto the star was observed, suggesting the origin is drawn from the ionized jet.
Conclusions. The relative lack of millimeter-dust (mm-dust) grains in the majority of inner disks in transition disks indicates that either such dust grains have drifted quickly towards the central star, that grain growth is less efficient in the inner disk, or that grains rapidly grow to planetesimal sizes in the inner disk. The observed correlation between the ionized mass loss rate and the accretion rate suggests the outflow is strictly connected to stellar accretion and that accretion in these disks is driven by a jet.
More fundamental than the fundamental metallicity relation
Authors: Sánchez-Menguiano Laura , Sánchez Sebastián F. , Sánchez Almeida Jorge , Muñoz-Tuñón Casiana 
Published: January 2024

Context One of the most fundamental scaling relations in galaxies is observed between metallicity and stellar mass – the mass-metallicity relation (MZR) – although recently a stronger dependence of the gas-phase metallicity with the galactic gravitational potential (ΦZR) has been reported. Further dependences of metallicity on other galaxy properties have been revealed, with the star formation rate (SFR) being one of the most studied and debated secondary parameters in the relation (the so-called fundamental metallicity relation).
Aims. In this work we explore the dependence of the gas-phase metallicity residuals from the MZR and ΦZR on different galaxy properties in the search for the most fundamental scaling relation in galaxies.
Methods. We applied a random forest regressor algorithm on a sample of 3430 nearby star-forming galaxies from the SDSS-IV MaNGA survey. Using this technique, we explored the effect of 147 additional parameters on the global oxygen abundance residuals obtained after subtracting the MZR. Alternatively, we followed a similar approach with the metallicity residuals from the ΦZR.
Results. The stellar metallicity of the galaxy is revealed as the secondary parameter in both the MZR and the ΦZR, ahead of the SFR. This parameter reduces the scatter in the relations ∼10 − 15%. We find the 3D relation between gravitational potential, gas metallicity, and stellar metallicity to be the most fundamental metallicity relation observed in galaxies.
Signs of magnetic star-planet interactions in HD 118203
Authors: Castro-González A. , Lillo-Box J. , Correia A. C. M. , Santos N. C. , Barrado D. , Morales-Calderón M. , Shkolnik E. L. 
Published: January 2024

Context. Planetary systems with close-in giant planets can experience magnetic star-planet interactions that modify the activity levels of their host stars. The induced activity is known to strongly depend on the magnetic moment of the interacting planet. Therefore, such planet-induced activity should be more readily observable in systems with close-in planets in eccentric orbits, since those planets are expected to rotate faster than in circular orbits. However, no evidence of magnetic interactions has been reported in eccentric planetary systems to date.Aims. We intend to unveil a possible planet-induced activity in the bright (V= 8.05 ± 0.03 mag) and slightly evolved star HD 118203, which is known to host an eccentric (e= 0.32 ± 0.02) and close-in (a= 0.0864 ± 0.0006 au) Jupiter-sized planet.Methods. We characterized the planetary system by jointly modelling 56 ELODIE radial velocities and four sectors of TESS photometry. We computed the generalized Lomb-Scargle periodogram of the TESS, ELODIE, and complementary ASAS-SN data to search for planet-induced and rotation-related activity signals. We studied the possible origins of the stellar variability found, analysed its persistence and evolution, and searched for possible links with the eccentric orbital motion of HD 118203 b.Results. We found evidence of an activity signal within the TESS photometry that matches the 6.1-day orbital period of its hosted planet HD 118203 b, which suggests the existence of magnetic star-planet interactions. We did not find, however, any additional activity signal that could be unambiguously interpreted as the rotation of the star, so we cannot discard stellar rotation as the actual source of the signal found. Nevertheless, both the evolved nature of the star and the significant orbital eccentricity make the synchronous stellar rotation with the planetary orbit very unlikely.Conclusions. The planetary system HD 118203 represents the best evidence that magnetic star–planet interactions can be found in eccentric planetary systems, and it opens the door to future dedicated searches in such systems that will allow us to better understand the interplay between close-in giant planets and their host stars.
Appel à projets « Réacteurs innovants » : vers de plus en plus de fluidité
Authors: Dupin Ludovic 
Published: January 2024

Massimiliano Picciani, responsable de l’appel à projets « Réacteurs nucléaires innovants » pour Bpifrance, tire les premiers enseignements de cette méthode originale lancée en 2022 sous l’impulsion d’Emmanuel Macron dans le cadre de France 2030.
Entwicklung der Verbstellung im Deutschen – eine Studie zu typischen und atypischen Verläufen anhand elizitierter Sprachproduktion
Authors: Lawatsch Kim , Kauschke Christina 
Published: January 2024

ZusammenfassungIm dritten Lebensjahr erwerben Kinder mit typischer Grammatikentwicklung die Grundzüge der Satzstruktur und der Verbstellung im deutschen Hauptsatz. Auch in den folgenden Jahren sind noch Weiterentwicklungen und Ausdifferenzierungen der grundlegenden Fähigkeiten zu erwarten. Der vorliegende Beitrag untersucht die Realisierung der Verbstellung und assoziierter grammatischer Strukturen im Vorschulalter mit einem Verfahren, das für die Neuauflage der „Patholinguistischen Diagnostik bei Sprachentwicklungsstörungen“ (PDSS) neu entwickelt wurde. Grundlage ist die im Zuge der Normierung der PDSS erhobene, elizitierte Sprachproduktion von 241 monolingual aufwachsenden Kindern zwischen 3;0 und 6;11 Jahren. Anhand dieser Daten konnten zwölf Meilen- und zehn Grenzsteine zeitlich eingeordnet werden. Darüber hinaus wurde die Stichprobe in zwei Subgruppen aus Kindern mit alterstypischen grammatischen Fähigkeiten bzw. grammatischen Schwächen aufgeteilt. Im Gruppenvergleich zeigte sich, dass die Kinder der zweiten Subgruppe relevante Zielstrukturen später produzieren und länger an nicht-zielsprachlichen Übergangsstrukturen festhalten.
Are Questionnaires Helpful To Predict Exercise-Induced
Bronchoconstriction (EIB) And Exercise-Induced Laryngeal Obstruction
(EILO)?
Authors: Dreßler Melanie , Lassmann Hannah , Eichhorn Celine , Trischler Jordis , Hutter Martin , Zielen Stefan , Schulze Johannes 
Published: January 2024

Abstract
Objective Exercise induced laryngeal obstruction (EILO) is an important
differential diagnosis to exercise induced bronchoconstriction (EIB) and
diagnosed via continuous laryngoscopy while exercising (CLE). However,
availability of CLE is limited to specialized centres. And without CLE EILO is
often misdiagnosed as EIB. Therefore it is essential to carefully preselect
potential EILO candidates. Aim of this study was to investigate whether two
short questionnaires -Asthma Control Test (ACT) and Dyspnea Index (DI)
evaluating upper airway-related dyspnea- can differentiate between EIB and
EILO.
Methods Patients with dyspnea while exercising were analysed with an
exercise challenge in the cold chamber (ECC) to diagnose EIB in visit 1 (V1), as
appropriate a CLE in visit 2 (V2, 4–6 weeks after V1) and ACT and DI in
V1 and V2. EIB patients were treated with asthma medication after V1.
Results Complete dataset of 36 subjects were gathered. The ACT showed
lower values in V2 in EILO compared to EIB patients. A lack of improvement in
ACT in V2 after asthma medication of EIB patients is suspicious for additional
EILO diagnosis. The DI showed higher values in V1 in EILO compared to EIB
patients. A score≥30 can predict a positive CLE reaction.
Conclusion ACT and DI are valuable tools in preselecting CLE candidates to
assure timely diagnostic despite limited diagnostic capabilities.
Hsa_circ_0092355 Accelerates Papillary Thyroid Cancer Progression by
Regulating the miR-543/PDE5A Pathway
Authors: Sun Zhijun , Zhang Min , Ye Yangmei , Yang Leilei 
Published: January 2024

AbstractCircRNAs have been found to participate in the progression of various tumors. In
the present study, we aimed to clarify the role of hsa_circ_0092355 in papillary
thyroid cancer (PTC) cell development. RT-qPCR was used to determine the
expression of hsa_circ_0092355, miR-543, and PDE5A. PTC cell proliferation was
ascertained via a cell colony formation assay and the CCK-8 test. Western
blotting was performed to examine the expression levels of PDE5A and
apoptosis-associated proteins (Bcl-2 and Bax) in PTC cells. A scratch wound
assay was performed to measure the migration of PTC cells. A mouse xenograft
test was performed to assess the effects of hsa_circ_0092355 in vivo. RIP
and dual-luciferase reporter assays confirmed the association between miR-543
and hsa_circ_0092355 or PDE5A. Associations between miR-543, hsa_circ_0092355,
and PDE5A were evaluated using Pearson’s correlation coefficient.
Upregulation of hsa_circ_0092355 was observed in PTC tissues. The
hsa_circ_0092355 knockdown blocked the proliferation and migration of PTC cells
and induced apoptosis. Moreover, hsa_circ_0092355 knockdown blocked PTC
xenograft tumor growth in vivo. The miR-543 inhibitor could reverse the
changes induced by hsa_circ_0092355 knockdown by hsa_circ_0092355 targeting
miR-543. Furthermore, miR-543 suppresses PTC progression by downregulating PDE5A
expression. Our findings suggest that the PTC tumor promoter hsa_circ_0092355
may promote carcinogenesis by controlling the miR-543/PDE5A pathway.
Maternal and Neonatal Morbidities by Race in College-Educated Women
Authors: Kern-Goldberger Adina R. , Madden Nigel , Baptiste Caitlin , Friedman Alexander , Gyamfi-Bannerman Cynthia 
Published: January 2024

Abstract
Objective Non-Hispanic black and Hispanic women experience significantly higher adverse maternal and neonatal outcomes compared with non-Hispanic white women. The purpose of this study is to explore whether disparities in obstetric outcomes exist by race among women who are college-educated.
Study Design This is a retrospective cohort study from a multicenter observational cohort of women undergoing cesarean delivery. Women were defined as “college-educated” if they reported completion of a 4-year college degree. Race/ethnicity was categorized as non-Hispanic white, non-Hispanic black, Hispanic, Asian, Native American, or unknown. The primary outcome was a composite of maternal morbidity, and a composite of neonatal morbidity was evaluated as a secondary outcome. A multivariable logistic regression model was then utilized to assess associations of race with the primary and secondary outcomes.
Results A total of 2,540 women were included in the study. After adjusting for potential confounding variables, maternal morbidity was found to be significantly higher for college-educated non-Hispanic black women compared with non-Hispanic white women (odds ratio [OR] 1.77, 95% confidence interval [CI] 1.12–2.80). The incidence of neonatal morbidity was significantly higher for non-Hispanic black (OR 1.91, 95% CI 1.31–2.79) and Hispanic (OR 3.34, 95% CI 2.23–5.01) women.
Conclusion In this cohort, the odds of cesarean-related maternal and neonatal morbidities were significantly higher for college-educated non-Hispanic black women, compared with their non-Hispanic white counterparts. This demonstrates that even among women with higher level education, racial and ethnic disparities persist in obstetric outcomes.
“Clock dial pattern”, a radiologic clue to neuro-chikungunya diagnosis: a case series
Authors: Fraiman Pedro Henrique Almeida , Freire Mariana , Fernandes Bruno , Palitot Felipe , Mota Nathalia , Sequerra Eduardo , Santos Glauco , Dourado Mario Emilio , Godeiro-Junior Clecio de Oliveira , Moreira-Neto Manuel 
Published: January 2024

Abstract
Background Chikungunya is a mosquito-borne disease caused by the chikungunya virus (CHIKV) and can lead to neurological complications in severe cases.
Objective This study examined neuroimaging patterns in chikungunya cases during two outbreaks in Brazil to identify specific patterns for diagnosis and treatment of neuro-chikungunya.
Methods Eight patients with confirmed chikungunya and neurological involvement were included. Clinical examinations and MRI scans were performed, and findings were analyzed by neuroradiologists. Data on age, sex, neurological symptoms, diagnostic tests, MRI findings, and clinical outcomes were recorded.
Results Patients showed different neuroimaging patterns. Six patients exhibited a “clock dial pattern” with hyperintense dotted lesions in the spinal cord periphery. One patient had thickening and enhancement of anterior nerve roots. Brain MRI revealed multiple hyperintense lesions in the white matter, particularly in the medulla oblongata, in six patients. One patient had a normal brain MRI.
Conclusion The “clock dial pattern” observed in spinal cord MRI may be indicative of chikungunya-related nervous system lesions. Isolated involvement of spinal cord white matter in chikungunya can help differentiate it from other viral infections. Additionally, distinct brainstem involvement in chikungunya-associated encephalitis, particularly in the rostral region, sets it apart from other arboviral infections. Recognizing these neuroimaging patterns can contribute to early diagnosis and appropriate management of neuro-chikungunya.