bluuebunny/crossref_metadata_2025_split huggingface dataset:
Effects of Vocabulary and Implicit Linguistic Knowledge on Speech Recognition in Adverse Listening Conditions
Authors: Fletcher Annalise , McAuliffe Megan , Kerr Sarah , Sinex Donal 
Published: October 2019

Purpose
This study aims to examine the combined influence of vocabulary knowledge and statistical properties of language on speech recognition in adverse listening conditions. Furthermore, it aims to determine whether any effects identified are more salient at particular levels of signal degradation.

Method
One hundred three young healthy listeners transcribed phrases presented at 4 different signal-to-noise ratios, which were coded for recognition accuracy. Participants also completed tests of hearing acuity, vocabulary knowledge, nonverbal intelligence, processing speed, and working memory.

Results
Vocabulary knowledge and working memory demonstrated independent effects on word recognition accuracy when controlling for hearing acuity, nonverbal intelligence, and processing speed. These effects were strongest at the same moderate level of signal degradation. Although listener variables were statistically significant, their effects were subtle in comparison to the influence of word frequency and phonological content. These language-based factors had large effects on word recognition at all signal-to-noise ratios.

Discussion
Language experience and working memory may have complementary effects on accurate word recognition. However, adequate glimpses of acoustic information appear necessary for speakers to leverage vocabulary knowledge when processing speech in adverse conditions.
Prospective Evaluation of Cognitive Functions After Rehabilitation With Cochlear Implant or Hearing Aids: Preliminary Results of a Multicentric Study on Elderly Patients
Authors: Anzivino Roberta , Conti Guido , Di Nardo Walter , Fetoni Anna Rita , Picciotti Pasqualina Maria , Marra Camillo , Guglielmi Valeria , Fortunato Susanna , Forli Francesca , Paludetti Gaetano , Berrettini Stefano 
Published: October 2019

ObjectiveRecent literature has shown a growing interest in the relationship between presbycusis and cognitive decline, but significant evidence about the long-term benefit of rehabilitation on cognitive functions has not been reported yet. The aim of the study was to analyze audiological and neuropsychological performances in patients with cochlear implant (CI) or hearing aids (HAs) over time.Materials and MethodForty-four bilaterally deaf patients aged more than 60 years (25 with CI candidacy and 19 with HA candidacy) were enrolled. Patients were subjected to audiological evaluation, to a battery of neuropsychological tests (Mini-Mental State Examination [MMSE], Rey Auditory Verbal Learning Task [RAVLT], Rey–Osterreith Complex Figure Test, Digit/Corsi Span Forward and Backward, Multiple Features Target Cancellation, Trail-Making Test, Stroop Test, and Phonological and Semantic Word Fluency), and to a quality of life assessment (Short Form 36, Glasgow Benefit Inventory, Glasgow Health Status Inventory) at the baseline and after a long-term follow-up (6–12 months).ResultsSpeech recognition scores in quiet and in noise were significantly improved even 6 months after auditory rehabilitation. Significant differences between pre- and post-rehabilitation scores were reported in physical and emotional impacts in life, general global health, vitality, and social activities. MMSE and RAVLT scores were significantly improved in both groups after 6 months of follow-up, suggesting a global involvement of memory domain. Mnesic performances remained unchanged between the first and second follow-up, but a further significant improvement in executive functions (Stroop Test) was detected in patients with CI reevaluated 12 months after implantation. A significant correlation of the RAVLT with signal-to-noise ratio at +10 dB speech-in-noise scores and the MMSE with signal-to-noise ratio at 0 dB speech-in-noise scores suggests the pivotal role of executive functions in recognition in noisy environment.ConclusionsOur preliminary data confirm that hearing deprivation in aged patients represents a truly modifiable risk factor for cognitive decline, which can be positively faced by acoustic rehabilitation. The improvement of short- and long-term memory performances and the amelioration of executive and attentive functions suggest that hearing restoration with both HAs and CI may provide a recovery of superior cognitive domains probably through a reallocation of cortical resources altered by hearing deprivation.
Evidence-Based Recommendation for Bilateral Cochlear Implantation in Adults
Authors: Au Agnes , Dowell Richard C. 
Published: October 2019

Purpose
Most adult cochlear implant (CI) users in developed countries benefit from the use of a hearing aid in conjunction with their implant device (bimodal hearing). Benefits have also been documented for the use of bilateral CIs for speech perception in quiet, localization, and speech perception in noise. This study attempted to quantify speech perception results for bimodal and bilateral CIs in adults and provide a guide for those considering a 2nd CI.

Method
Speech perception outcomes were reviewed for 1,394 adults with acquired hearing loss who received a CI at the Melbourne Cochlear Implant Clinic between 2000 and 2015.

Results
Bimodal and bilateral users significantly outperformed unilateral CI users on consonant–vowel–consonant word recognition in quiet. For the bilateral group, word recognition scores with the 1st CI were predictive of 2nd CI word scores. The analysis suggested that bimodal users who were gaining less than 19% benefit from the nonimplanted ear were likely to perform better with a 2nd implant.

Conclusions
CI users who score less than 19% on consonant–vowel–consonant words in the nonimplanted ear have a good chance of benefiting from a 2nd implant. Consideration of many other factors including age, hearing goals, medical factors, and the risk to residual hearing also needs to play a part in recommending a 2nd CI.
Electrocochleography: New Uses for an Old Test and Normative Values
Authors: Ferraro John A. , Kileny Paul R. , Grasel Signe S. 
Published: October 2019

Purpose
This article combines the results of 3 studies that were presented at the HeAL 2018 Conference in Lake Como, Italy, in June 2018. Each study involved electrocochleography (ECochG), a neurodiagnostic evaluation that has been used clinically for over 80 years but whose applications continue to expand. The 1st study describes recent research wherein ECochG was recorded from asymptomatic subjects who were siblings or offspring of patients with a confirmed diagnosis of Ménière's disease (MD). Our results provide evidence that ECochG may be helpful in not only diagnosing MD but also predicting it as well. Second, case studies are described where ECochG was important in both diagnosing superior semicircular canal dehiscence and monitoring the repair of this condition during surgery. Finally, although ECochG has been practiced clinically for over 8 decades, the protocols for recording, measuring, and interpreting the electrocochleogram continue to lack standardization among clinicians and scientists. We thus present normative data for some of these features based on noninvasive recordings made from the tympanic membrane from 100 normal hearing subjects.

Conclusions
Although the primary use of ECochG continues to be in the diagnosis of MD, we report on 2 additional clinical applications for this important test of inner ear/auditory nerve function. First, a preliminary study on a small sample of subjects indicates that ECochG may also be useful in predicting MD prior to the onset of symptoms in individuals who may be genetically predisposed to developing it. Second, through a series of case studies, we demonstrate how ECochG is used to help diagnose superior semicircular canal dehiscence and monitor the status of the inner ear during the surgical repair of this condition. Finally, normative values for clinically important components of the electrocochleogram based on tympanic membrane recordings have been established from a large sample of subjects.
Speech-Language Pathologists' Comfort Providing Intervention to Children With Traumatic Brain Injury: Results From a National Survey
Authors: Pelatti Christina Yeager , Bush Erin J. , Farquharson Kelly , Schneider-Cline Whitney , Harvey Judy , Carter Mary W. 
Published: October 2019

Purpose
This exploratory study examined speech-language pathologists' (SLPs) clinical experience and work environment characteristics impacting comfort with providing intervention to children with traumatic brain injury (TBI).

Method
This study included 162 SLPs who responded to a national survey about their comfort providing intervention to children with TBI, clinical experience (i.e., years of experience treating children with TBI, TBI preprofessional training and professional development, and licensure/credentialing), and work environment (i.e., work setting, caseload size, geographic location).

Results
Findings from latent class analysis revealed 3 distinct groups of SLPs based on their comfort with providing services to children with TBI: those with low comfort, moderate comfort, and high comfort. Further analyses revealed statistically significant differences across the 3 groups in the areas of years of experience treating children with TBI, professional development, work setting, TBI caseload size, and geographic location.

Conclusions
Our findings reveal that most SLPs feel comfortable providing intervention to children with TBI; however, differences in characteristics across groups suggest that specific steps can be taken to ensure increased comfort for all SLPs working with this population. Practicing SLPs may increase their level of comfort through professional development and hands-on, mentored experience with TBI. Efforts such as these may influence the quality of service provision and expand the population of SLPs who feel comfortable treating children with TBI. Future research is needed to further examine how comfort and SLP characteristics directly impact the quality of speech and language intervention and long-term outcomes of children with TBI.
Going With the Flow: An Examination of Entrainment in Typically Developing Children
Authors: Wynn Camille J. , Borrie Stephanie A. , Pope Kiersten A. 
Published: October 2019

Purpose
Conversational entrainment is the tendency for individuals to modify their behavior to more closely converge with the behavior of their communication partner and is an important aspect of successful interaction. Evidence of entrainment in adults is robust, yet research regarding its development in children is sparse. Here, we investigate the emergence of entrainment skills in typically developing children.

Method
Data were collected from a total of 50 typically developing children between the ages of 5 and 14 years. Children participated in a quasiconversational paradigm with a virtual interlocutor. Speech rate of the interlocutor was digitally manipulated to produce fast and slow speech rate conditions.

Results
Data from the fast and slow conditions were compared using linear mixed models. Results indicated that children, regardless of age, did not alter their speech to match the rate of the virtual interlocutor.

Conclusions
Findings suggest that entrainment in children may not be as robust as entrainment in adults and therefore not adequately captured with the current experimental paradigm. Modifications to the current paradigm will help identify a methodology sufficiently sensitive to capture the speech alignment phenomenon in children and provide much needed information regarding the typical stages of entrainment development.
Design and implementation of microstrip dual‐band filtering power divider using square‐loop resonator
Authors: Mirzaei M. , Sheikhi A. 
Published: October 2019

This Letter presents a dual‐band filtering power divider (FPD) by employing square‐loop resonator loaded by open stubs. The even‐ and odd‐mode equivalent circuits of the proposed resonator are analysed and design equations are derived. For demonstration, the power divider (PD) is fabricated and measured. The simulated results of the PD not only show a good selectivity but also it does good isolation. Finally, the comparisons of the measured and simulated results of the dual‐band FPD are presented, which are in good agreement. The measured results show that the dual‐band FPD has better than −30/−36 dB isolation, −16.5/−18 dB return loss, and −3.9/−4.0 dB insertion loss at centre frequencies of 3.1 and 5.3 GHz, respectively.
Radiation thermo-chemical models of protoplanetary disks
Authors: Thi W. F. , Lesur G. , Woitke P. , Kamp I. , Rab Ch. , Carmona A. 
Published: October 2019

Context. Disks around pre-main-sequence stars evolve over time by turbulent viscous spreading. The main contender to explain the strength of the turbulence is the magnetorotational instability model, whose efficiency depends on the disk ionization fraction.
Aims. Our aim is to compute self-consistently the chemistry including polycyclic aromatic hydrocarbon (PAH) charge chemistry, the grain charging, and an estimate of an effective value of the turbulence α parameter in order to find observational signatures of disk turbulence.
Methods. We introduced PAH and grain charging physics and their interplay with other gas-phase reactions in the physico-chemical code PRODIMO. Non-ideal magnetohydrodynamics effects such as ohmic and ambipolar diffusion are parametrized to derive an effective value for the turbulent parameter αeff. We explored the effects of turbulence heating and line broadening on CO isotopologue submillimeter lines.
Results. The spatial distribution of αeff depends on various unconstrained disk parameters such as the magnetic parameter βmag or the cosmic ray density distribution inside the protoplanetary disk s. The inner disk midplane shows the presence of the so-called dead zone where the turbulence is almost inexistent. The disk is heated mostly by thermal accommodation on dust grains in the dead zone, by viscous heating outside the dead zone up to a few hundred astronomical units, and by chemical heating in the outer disk. The CO rotational lines probe the warm molecular disk layers where the turbulence is at its maximum. However, the effect of turbulence on the CO line profiles is minimal and difficult to distinguish from the thermal broadening.
Conclusions. Viscous heating of the gas in the disk midplane outside the dead zone is efficient. The determination of α from CO rotational line observations alone is challenging.
Disc kinematics and stability in high-mass star formation
Authors: Ahmadi A. , Kuiper R. , Beuther H. 
Published: October 2019

Context. In the disc-mediated accretion scenario for the formation of the most massive stars, high densities and high accretion rates could induce gravitational instabilities in the disc, forcing it to fragment and produce companion objects.
Aims. We investigate the effects of inclination and spatial resolution on the observable kinematics and stability of discs in high-mass star formation.
Methods. We studied a high-resolution 3D radiation-hydrodynamic simulation that leads to the fragmentation of a massive disc. Using RADMC-3D we produced 1.3 mm continuum and CH3CN line cubes at different inclinations. The model was set to different distances, and synthetic observations were created for ALMA at ~80 mas resolution and NOEMA at ~0.4′′.
Results. The synthetic ALMA observations resolve all fragments and their kinematics well. The synthetic NOEMA observations at 800 pc with linear resolution of ~300 au are able to resolve the fragments, while at 2000 pc with linear resolution of ~800 au only a single structure slightly elongated towards the brightest fragment is observed. The position–velocity (PV) plots show the differential rotation of material best in the edge-on views. A discontinuity is seen at a radius of ~250 au, corresponding to the position of the centrifugal barrier. As the observations become less resolved, the inner high-velocity components of the disc become blended with the envelope and the PV plots resemble rigid-body-like rotation. Protostellar mass estimates from PV plots of poorly resolved observations are therefore overestimated. We fit the emission of CH3CN (12K−11K) lines and produce maps of gas temperature with values in the range of 100–300 K. Studying the Toomre stability of the discs, we find low Q values below the critical value for stability against gravitational collapse at the positions of the fragments and in the arms connecting the fragments for the resolved observations. For the poorly resolved observations we find low Q values in the outskirts of the disc. Therefore, although we could not resolve any of the fragments, we are able to predict that the disc is unstable and fragmenting. This conclusion is valid regardless of our knowledge about the inclination of the disc.
Conclusions. These synthetic observations reveal the potential and limitations of studying discs in high-mass star formation with current (millimetre) interferometers. While the extremely high spatial resolution of ALMA reveals objects in extraordinary detail, rotational structures and instabilities within accretion discs can also be identified in poorly resolved observations.
The Araucaria project: High-precision orbital parallax and masses of eclipsing binaries from infrared interferometry
Authors: Gallenne A. , Pietrzyński G. , Graczyk D. , Pilecki B. , Storm J. , Nardetto N. , Taormina M. , Gieren W. , Tkachenko A. , Kervella P. , Mérand A. , Weber M. 
Published: October 2019

Context. The precise determinations of stellar mass at ≲1% provide important constraints on stellar evolution models. Accurate parallax measurements can also serve as independent benchmarks for the next Gaia data release.
Aims. We measured the masses and distance of binary systems with a precision level better than 1% using a fully geometrical and empirical method.
Methods. We obtained the first interferometric observations for the eclipsing systems AI Phe, AL Dor, KW Hya, NN Del, ψ Cen and V4090 Sgr with the VLTI/PIONIER combiner, which we combined with radial velocity measurements to derive their three-dimensional orbit, masses, and distance.
Results. We determined very precise stellar masses for all systems, ranging in precision from 0.04% to 3.3%. We combined these measurements with the stellar effective temperature and linear radius to fit stellar isochrones models and determined the age of the systems. We also derived the distance to the systems with a precision level of 0.4%.
Conclusions. The comparison of theoretical models with stellar parameters shows that stellar models are still deficient in simultaneously fitting the stellar parameters (Teff, R and M) with this level of precision on individual masses. This stresses the importance of precisely measuring the stellar parameters to better calibrate stellar evolution models. The precision of our model-independent orbital parallaxes varies from 24 μas as to 70 μas and the parallaxes provide a unique opportunity to verify whether the future Gaia measurements have systematic errors.
Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
Authors: Choplin Arthur , Tominaga Nozomu , Ishigaki Miho N. 
Published: October 2019

Context. The nature of the early generation of massive stars can be inferred by investigating the origin of the extremely metal-poor (EMP) stars, likely formed from the ejecta of one or a few previous massive stars.
Aims. We investigate the rotational properties of early massive stars by comparing the abundance patterns of EMP stars with massive stellar models including rotation.
Methods. Low metallicity 20 M⊙ massive stellar models with eight initial rotation rates between 0 and 70% of the critical velocity are computed. Explosions with strong fallback are assumed. The ejected material is considered to fit individually the abundance patterns of 272 EMP stars with −4 <  [Fe/H] <  −3.
Results. With increasing initial rotation, the [C/H], [N/H], [O/H], [Na/H], [Mg/H], and [Al/H] ratios in the massive star ejecta are gradually increased (up to ∼4 dex) while the 12C/13C ratio is decreased. Among the 272 EMP stars considered, ∼40 − 50% are consistent with our models. About 60 − 70% of the carbon-enhanced EMP star sample can be reproduced against ∼20 − 30% for the carbon-normal EMP star sample. The abundance patterns of carbon-enhanced EMP stars are preferentially reproduced with a material coming from mid to fast rotating massive stars. The overall velocity distribution derived from the best massive star models increases from no rotation to fast rotation. The maximum is reached for massive stars having initial equatorial velocities of ∼550 − 640 km s−1.
Conclusions. Although subject to significant uncertainties, these results suggest that the rotational mixing operating in between the H-burning shell and the He-burning core of early massive stars played an important role in the early chemical enrichment of the Universe. The comparison of the velocity distribution derived from the best massive star models with velocity distributions of nearby OB stars suggests that a greater number of massive fast rotators were present in the early Universe. This may have important consequences for reionization, the first supernovae, or integrated light from high redshift galaxies.
Dusty phenomena in the vicinity of giant exoplanets
Authors: Arkhypov O. V. , Khodachenko M. L. , Hanslmeier A. 
Published: October 2019

Context. Hitherto, searches for exoplanetary dust have focused on the tails of decaying rocky or approaching icy bodies only at short circumstellar distances. At the same time, dust has been detected in the upper atmospheric layers of hot jupiters, which are subject to intensive mass loss. The erosion and/or tidal decay of hypothetic moonlets might be another possible source of dust around giant gaseous exoplanets. Moreover, volcanic activity and exozodiacal dust background may additionally contribute to exoplanetary dusty environments.
Aims. In the present study, we look for photometric manifestations of dust around different kinds of exoplanets (mainly giants).
Methods. We used linear approximation of pre- and post-transit parts of the long-cadence transit light curves (TLCs) of 118 Kepler objects of interest after their preliminary whitening and phase-folding. We then determined the corresponding flux gradients G1 and G2, respectively. These gradients were defined before and after the transit border for two different time intervals: (a) from 0.03 to 0.16 days and (b) from 0.01 to 0.05 days, which correspond to the distant and adjoining regions near the transiting object, respectively. Statistical analysis of gradients G1 and G2 was used for detection of possible dust manifestation.
Results. It was found that gradients G1 and G2 in the distant region are clustered around zero, demonstrating the absence of artifacts generated during the light curve processing. However, in the adjoining region, 17 cases of hot jupiters show significantly negative gradients, G1, whereas the corresponding values of G2 remain around zero. The analysis of individual TLCs reveals the localized pre-transit decrease of flux, which systematically decreases G1. This effect was reproduced with the models using a stochastic obscuring precursor ahead of the planet.
Conclusions. Since only a few TLCs show the presence of such pre-transit anomalies with no analogous systematic effect in the post-transit phase, we conclude that the detected pre-transit obscuration is a real planet-related phenomenon. Such phenomena may be caused by dusty atmospheric outflows or background circumstellar dust compressed in front of the mass-losing exoplanet, the study of which requires dedicated physical modeling and numeric simulations. Of certain importance may be the retarding of exozodiacal dust relative to the planet by the Poynting-Robertson effect leading to dust accumulation in electrostatic or magnetic traps in front of the planet.