bluuebunny/crossref_metadata_2025_split huggingface dataset:
Examining where to go: pediatric psychology trainees’ perception of their graduate training in culture and diversity
Authors: Hess Courtney W , Rea Kelly E , Wruble Lauren P , Yee Shanique T , Bejarano Carolina M , Williford Desireé N , Gibler Robert C , Eshtehardi Sahar S , Fisher Rachel S , Morgan Casie H 
Published: June 2024

Abstract

Objective
Culture and diversity-related training is critical to the development of competent pediatric psychologists. Evaluation of training efforts have been conducted at the program level, yet evaluation of trainee experiences in culture and diversity-related training remains unassessed. This trainee-led study was the first formal assessment of pediatric psychology trainee experiences of culture and diversity-related training and the impact of training on their own cultural humility.

Methods
Study overview and a survey link was distributed across 2 listservs associated with the American Psychological Association (Division 53, Division 54) and sent directly to directors of graduate, internship, and fellowship training programs with a request to share with trainees. Surveys assessing integration of cultural training and trainee cultural humility were completed. Trainees also provided qualitative feedback regarding their multicultural training and development.

Results
Pediatric psychology trainees (N = 90) reported inconsistent integration of culture and diversity topics into their training. Of the 34 training areas assessed, 10 were perceived as thoroughly integrated into formal training by at least half of the respondents. Trainees often sought independent cultural training outside of their programs, and no relationship was detected between perceived integration of cultural training and trainee cultural competence.

Discussion
Results indicate room for improvement regarding integration of cultural training and a need to better understand driving forces behind trainees independently seeking training outside of their formal training programs. Moreover, understanding the aspects of training that are most contributory to trainee development is needed given that no relationship between training and development emerged in the current study.
The Plant PTM Viewer 2.0: in-depth exploration of plant protein modification landscapes
Authors: Willems Patrick , Sterck Lieven , Dard Avilien , Huang Jingjing , De Smet Ive , Gevaert Kris , Van Breusegem Frank 
Published: June 2024

Abstract
Post-translational modifications (PTMs) greatly increase protein diversity and functionality. To help the plant research community interpret the ever-increasing number of reported PTMs, the Plant PTM Viewer (https://www.psb.ugent.be/PlantPTMViewer) provides an intuitive overview of plant protein PTMs and the tools to assess it. This update includes 62 novel PTM profiling studies, adding a total of 112 000 modified peptides reporting plant PTMs, including 14 additional PTM types and three species (moss, tomato, and soybean). Furthermore, an open modification re-analysis of a large-scale Arabidopsis thaliana mass spectrometry tissue atlas identified previously uncharted landscapes of lysine acylations predominant in seed and flower tissues and 3-phosphoglycerylation on glycolytic enzymes in plants. An extra ‘Protein list analysis’ tool was developed for retrieval and assessing the enrichment of PTMs in a protein list of interest. We conducted a protein list analysis on nuclear proteins, revealing a substantial number of redox modifications in the nucleus, confirming previous assumptions regarding the redox regulation of transcription. We encourage the plant research community to use PTM Viewer 2.0 for hypothesis testing and new target discovery, and also to submit new data to expand the coverage of conditions, plant species, and PTM types, thereby enriching our understanding of plant biology.
The Efficacy of Whole Blood Resuscitation During Resuscitative Endovascular Balloon Occlusion of the Aorta (REBOA) to Mitigate Post-occlusion Circulatory Collapse: A Translational Model in Large Swine
Authors: Newberry Ryan K , Paredes R Madelaine , Barnard Ed B G , Redman Theodore T , Arana Allyson A , Maddry Joseph K , Glaser Jacob J , Rall Jason M 
Published: June 2024

ABSTRACT

Introduction
Uncontrolled torso hemorrhage is the primary cause of potentially survivable deaths on the battlefield. Zone 1 Resuscitative Endovascular Balloon Occlusion of the Aorta (REBOA), in conjunction with damage control resuscitation, may be an effective management strategy for these patients in the prehospital or austere phase of their care. However, the effect of whole blood (WB) transfusion during REBOA on post-occlusion circulatory collapse is not fully understood.

Materials and Methods
Yorkshire male swine (n = 6 per group, 70–90 kg) underwent a 40% volume-controlled hemorrhage. After a 10-minute hemorrhagic shock period, a REBOA balloon was inflated in Zone 1. Fifteen minutes after inflation, 0, 1, or 3 units (450 mL/unit) of autologous WB was infused through the left jugular vein. Thirty minutes after initial balloon inflation, the balloon was deflated slowly over 3 minutes. Following deflation, normal saline was administered (up to 3,000 mL) and swine were observed for 2 hours. Survival (primary outcome), hemodynamics, and blood gas values were compared among groups. Statistical significance was determined by log-rank test, one-way ANOVA, and repeated measures ANOVA.

Results
Survival rates were comparable between groups (P = .345) with 66% of control, 33% of the one-unit animals, and 50% of the 3-unit animals survived until the end of the study. Following WB infusion, both the 1-unit and the 3-unit groups had significantly higher blood pressure (P &lt; .01), pulmonary artery pressure (P &lt; .01), and carotid artery flow (P &lt; .01) compared to the control group.

Conclusions
WB transfusion during Zone 1 REBOA was not associated with increased short-term survival in this large animal model of severe hemorrhage. We observed no signal that WB transfusion may mitigate post-occlusion circulatory collapse. However, there was evidence of supra-normal blood pressures during WB transfusion.
Glucagon-Like Peptide-1 Receptor Agonists and Sodium Glucose Cotransporter-2 Inhibitors and Cardiorespiratory Fitness Interaction
Authors: Ni David , Kokkinos Peter , Nylen Eric S 
Published: June 2024

ABSTRACT

Introduction
Cardiorespiratory fitness (CRF) is a stronger predictor of mortality than traditional risk factors and is a neglected vital sign of health. Enhanced fitness is a cornerstone in diabetes management and is most often delivered concurrently with pharmacological agents, which can have an opposing impact, as has been reported with metformin. Considering the rapid evolution of diabetes medications with improved cardiovascular outcomes, such as glucagon-like peptide-1 receptor agonists and sodium glucose cotransporter-2 inhibitors, it is of importance to consider the influence of these vis-a-vis effects on CRF.

Materials and Methods
Combining the words glucagon-like peptide-1 receptor agonists and sodium glucose cotransporter-2 inhibitors with cardiorespiratory fitness, an online search was done using PubMed, Embase, Scopus, Web of Science, Scientific Electronic Library Online, and Cochrane.

Results
There were only a few randomized controlled studies that included CRF, and the results were mostly neutral. A handful of smaller studies detected improved CRF using sodium glucose cotransporter-2 inhibitors in patients with congestive heart failure.

Conclusions
Since CRF is a superior prognosticator for cardiovascular outcomes and both medications can cause lean muscle mass loss, the current review highlights the paucity of relevant interactive analysis.
Cost Removed! Do Different Factors Influence Motivation for Vasectomy Reversal When Cost Is Not an Issue?
Authors: Maloney Trevor J , Swargaloganathan Piragash , Hawksworth Dorota J 
Published: June 2024

ABSTRACT

Introduction
Vasectomy is a relatively common procedure performed for the purposes of sterilization; however, up to 6% of men that undergo vasectomy wish for its reversal at some point. Few studies have examined the motivation behind vasectomy reversal (VR), especially within special populations, such as the U.S. Military. The aim of this study was to examine the motivations of U.S. Military service members (SMs) who opted for VR surgery, considering their unique access to free health care.

Materials and Methods
We conducted a retrospective record review of microsurgical VRs performed by a single surgeon (DJH) between January 2020 and May 2023. We evaluated patient’s age at which vasectomy was performed, age at VR, reasons for seeking VR surgical care, number of children fathered before the vasectomy, and the age of the current partner.

Results
A total of 106 patients underwent VR during the study period, and 102 of them had their medical records available for review. The average age at the time of vasectomy was 31.3 years, while the average age at VR was 40.2 years. The average spousal age at the time of seeking VR was 34.8 years. Before undergoing vasectomy, the men had fathered an average of 2.7 children. Most men were enlisted members of the military (68) and of all service branches, Army represented the greatest number (50). The vast majority of men (76) cited having a new partner after divorce as the primary motivation for seeking VR. Within this group, 57 were remarried, 15 were in a new relationship, 3 were newly engaged, and 1 desired fertility for future relationships. Additionally, 21 sought VR to have more children with the same spouse. Among them, motivating factors included changes to financial status and improvement in partner’s health condition. A minority of patients (2) desired VR due to post vasectomy pain syndrome or religious beliefs.

Conclusions
Our study demonstrates that the primary driver for seeking VR surgical care among SMs was the desire for fertility with a new partner, which correlates with trends in the civilian sector. Approximately 20% of the men cited the wish to have more children with the same partner as their motivation. Non-fertility reasons, such as religious beliefs and post vasectomy pain syndrome, were also observed, albeit less frequently.
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
Authors: Klein M , Mohr J J , Bocquet S , Aguena M , Allen S W , Alves O , Ansarinejad B , Ashby M L N , Bacon D , Bayliss M , Benson B A , Bleem L E , Brodwin M , Brooks D , Bulbul E , Burke D L , Canning R E A , Carlstrom J E , Rosell A Carnero , Carretero J , Chang C L , Conselice C , Costanzi M , Crites A T , da Costa L N , Pereira M E S , Davis T M , De Vicente J , Desai S , de Haan T , Dobbs M A , Doel P , Ferrero I , Flores A M , Frieman J , George E M , Giannini G , Gladders M D , Gonzalez A H , Grandis S , Gruen D , Gruendl R A , Gutierrez G , Halverson N W , Hinton S R , Holder G P , Hollowood D L , Holzapfel W L , Honscheid K , Hrubes J D , Huang N , James D J , Khullar G , Kim K , Knox L , Kraft R , Kéruzoré F , Lee A T , Luong-Van D , Mahler G , Mantz A , Marrone D P , Marshall J L , McDonald M , McMahon J J , Mena-Fernández J , Menanteau F , Meyer S S , Miquel R , Myles J , Padin S , Pieres A , Plazas Malagón A A , Pryke C , Reichardt C L , Reil K , Roberson J , Romer A K , Romero C , Ruhl J E , Saliwanchik B R , Salvati L , Sanchez E , Saro A , Schaffer K K , Schrabback T , Schubnell M , Sevilla-Noarbe I , Sharon K , Shirokoff E , Smith M , Somboonpanyakul T , Stalder B , Stanford S A , Stark A A , Strazzullo V , Suchyta E , Swanson M E C , Tarle G , To C , Vanderlinde K , Vieira J D , von der Linden A , Weaverdyck N , Williamson R , Wiseman P , Young M 
Published: June 2024

ABSTRACT
We present an extension to a Sunyaev–Zel’dovich Effect (SZE) selected cluster catalogue based on observations from the South Pole Telescope (SPT); this catalogue extends to lower signal to noise than the previous SPT–SZ catalogue and therefore includes lower mass clusters. Optically derived redshifts, centres, richnesses, and morphological parameters together with catalogue contamination and completeness statistics are extracted using the multicomponent matched filter (MCMF) algorithm applied to the S/N &gt; 4 SPT–SZ candidate list and the Dark Energy Survey (DES) photometric galaxy catalogue. The main catalogue contains 811 sources above S/N = 4, has 91 per cent purity, and is 95 per cent complete with respect to the original SZE selection. It contains in total 50 per cent more clusters and twice as many clusters above z = 0.8 in comparison to the original SPT-SZ sample. The MCMF algorithm allows us to define subsamples of the desired purity with traceable impact on catalogue completeness. As an example, we provide two subsamples with S/N &gt; 4.25 and S/N &gt; 4.5 for which the sample contamination and cleaning-induced incompleteness are both as low as the expected Poisson noise for samples of their size. The subsample with S/N &gt; 4.5 has 98 per cent purity and 96 per cent completeness and is part of our new combined SPT cluster and DES weak-lensing cosmological analysis. We measure the number of false detections in the SPT-SZ candidate list as function of S/N, finding that it follows that expected from assuming Gaussian noise, but with a lower amplitude compared to previous estimates from simulations.
The MOSDEF survey: properties of warm ionized outflows at z = 1.4–3.8
Authors: Weldon Andrew , Reddy Naveen A , Coil Alison L , Shapley Alice E , Siana Brian , Price Sedona H , Kriek Mariska , Mobasher Bahram , Song Zhiyuan , Wozniak Michael A 
Published: June 2024

ABSTRACT
We use the large spectroscopic data set of the MOSFIRE Deep Evolution Field survey to investigate the kinematics and energetics of ionized gas outflows. Using a sample of 598 star-forming galaxies at redshift 1.4 &lt; z &lt; 3.8, we decompose [O iii] and $\rm {H}\,\alpha$ emission lines into narrow and broad components, finding significant detections of broad components in 10 per cent of the sample. The ionized outflow velocity from individual galaxies appears independent of galaxy properties, such as stellar mass, star formation rate (SFR), and SFR surface density (ΣSFR). Adopting a simple outflow model, we estimate the mass-, energy-, and momentum-loading factors of the ionized outflows, finding modest values with averages of 0.33, 0.04, and 0.22, respectively. The larger momentum- than energy-loading factors, for the adopted physical parameters, imply that these ionized outflows are primarily momentum driven. We further find a marginal correlation (2.5σ) between the mass-loading factor and stellar mass in agreement with predictions by simulations, scaling as ηm$\propto M_{\star }^{-0.45}$. This shallow scaling relation is consistent with these ionized outflows being driven by a combination of mechanical energy generated by supernovae explosions and radiation pressure acting on dusty material. In a majority of galaxies, the outflowing material does not appear to have sufficient velocity to escape the gravitational potential of their host, likely recycling back at later times. Together, these results suggest that the ionized outflows traced by nebular emission lines are negligible, with the bulk of mass and energy carried out in other gaseous phases.
Plasma lensing interpretation of FRB 20201124A bursts at the end of September 2021
Authors: Chen Xuechun , Hu Bin , Wang Pei , Zheng Wenwen , Li Di , Er Xinzhong 
Published: June 2024

ABSTRACT
When radio photons propagate through a non-uniform electron density volume, the plasma lensing effect can induce an extreme magnification to the observed flux at certain frequencies. Because the plasma lens acts as a diverging lens, it can extremely suppress the observed flux when aligned with the source. These two properties can theoretically cause a highly magnified fast radio burst (FRB) to become faint or even disappear for a period of time. In this paper, we interpret that the significant increase in burst counts followed by a sudden quenching in FRB 20201124A in September 2021 can be attributed to plasma lensing. Based on the one-dimensional Gaussian lens model, we search for double main-peak structures in the spectra just before its extinction on 2021 September 29. After the de-dispersion and de-scintillation procedures, we find eight bursts with double main-peaks at stable positions. There are three parameters in our modelling, the height N0, width a of the lens and its distance DLS to the source. We reformulate them as a combined parameter ${P}_0 \propto \left(\frac{a}{\mathrm{au}}\right)\sqrt{\frac{\mathrm{kpc}}{D_{\mathrm{LS}}} \frac{\mathrm{pc}\mathrm{cm}^{-3}}{N_0} }$. The frequency spectra can give an accurate estimation of P0 corresponding to $\left(\frac{a}{\mathrm{au}}\right)\sqrt{\frac{\mathrm{kpc}}{D_{\mathrm{LS}}} \frac{\mathrm{pc}\mathrm{cm}^{-3}}{N_0} } \approx 28.118$, while the time of arrival only give a relatively loose constraint on a2/DLS. Comparing with the observation dynamic spectra, we suggest that for a plasma lens in host galaxy, e.g. DLS ≈ 1 kpc, the width of lens can not be larger than 40 au. At last, we estimate the relative transverse motion velocity between the lens and source, $v\approx 98\left(\frac{a}{\mathrm{au}}\right)\mathrm{km\,s^{-1}}$.
Radiative properties of plasmoids and plasmoid mergers in magnetic reconnection
Authors: Zhang Haocheng , Dong Lingyi , Giannios Dimitrios 
Published: June 2024

ABSTRACT
Magnetic reconnection is often considered as the primary particle acceleration mechanism in a magnetized blazar zone environment. The majority of radiation in the reconnection layer comes from plasmoids and their mergers. In particular, plasmoid mergers can produce strong multiwavelength flares and major variations in synchrotron polarization signatures. However, radiative properties of plasmoid mergers have not been well explored due to difficulties in tracking the merging processes. Here we use an image processing method that combines the magnetic vector potential and density to identify isolated and merging plasmoids. We find that this method can clearly distinguish radiation contributions from isolated plasmoids, merging plasmoids, and the primary current sheet of reconnection. This new method enables us to study the radiative properties of plasmoids and mergers statistically. Our results show that isolated plasmoids have similar emissivity regardless of their sizes, and they generally have non-zero polarization degree (PD) due to their quasi-circular shape. Flares due to plasmoid mergers have relative amplitudes that are antiproportional to the size ratio of the plasmoids participating in the mergers. Finally, only mergers between plasmoids of comparable sizes (width ratio ≲5) can lead to significant spectral hardening and polarization angle (PA) variations; the amplitude of the PA variations is between 0 and 180° and has a mean value of 90°. Our analyses on 2D simulations can pave the way for future analyses and machine learning techniques on radiative properties of 3D magnetic reconnection simulations.
Astrophysical parameter inference on accreting white dwarf binaries using gravitational waves
Authors: Yi Sophia , Lau Shu Yan , Yagi Kent , Arras Phil 
Published: June 2024

ABSTRACT
Accreting binary white dwarf systems are among the sources expected to emanate gravitational waves that the Laser Interferometer Space Antenna (LISA) will detect. We investigate how accurately the binary parameters may be measured from LISA observations. We complement previous studies by performing our parameter estimation on binaries containing a low-mass donor with a thick, hydrogen-rich envelope. The evolution is followed from the early, pre-period minimum stage, in which the donor is non-degenerate, to a later, post-period minimum stage with a largely degenerate donor. We present expressions for the gravitational-wave amplitude, frequency, and frequency derivative in terms of white dwarf parameters (masses, donor radius, etc.), where binary evolution is driven by gravitational-wave radiation and accretion torques, and the donor radius and logarithmic change in radius (ηd) due to mass-loss are treated as model parameters. We then perform a Fisher analysis to reveal the accuracy of parameter measurements, using models from Modules for Experiments in Stellar Astrophysics (mesa) to estimate realistic fiducial values at which we evaluate the measurement errors. We find that the donor radius can be measured relatively well with LISA observations alone, while we can further measure the individual masses if we have an independent measurement of the luminosity distance from electromagnetic observations. When applied to the parameters of the recently discovered white dwarf binary ZTF J0127+5258, our Fisher analysis suggests that we will be able to constrain the system’s individual masses and donor radius using LISA’s observations, given Zwicky Transient Facility’s (ZTF’s) measurement of the luminosity distance.
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
Authors: Thompson Oliver A , Richings Alexander J , Gibson Brad K , Faucher-Giguère Claude-André , Feldmann Robert , Hayward Christopher C 
Published: June 2024

ABSTRACT
Our ability to trace the star-forming molecular gas is important to our understanding of the Universe. We can trace this gas using CO emission, converting the observed CO intensity into the H$_2$ gas mass of the region using the CO-to-H$_2$ conversion factor ($X_{\rm{{\small CO}}}$). In this paper, we use simulations to study the conversion factor and the molecular gas within galaxies. We analysed a suite of simulations of isolated disc galaxies, ranging from dwarfs to Milky Way-mass galaxies, that were run using the fire-2 subgrid models coupled to the chimes non-equilibrium chemistry solver. We use the non-equilibrium abundances from the simulations, and we also compare to results using abundances assuming equilibrium, which we calculate from the simulation in post-processing. Our non-equilibrium simulations are able to reproduce the relation between CO and H$_2$ column densities, and the relation between $X_{\rm{{\small CO}}}$ and metallicity, seen within observations of the Milky Way. We also compare to the xCOLD GASS survey, and find agreement with their data to our predicted CO luminosities at fixed star formation rate. We also find the multivariate function used by xCOLD GASS overpredicts the H$_2$ mass for our simulations, motivating us to suggest an alternative multivariate function of our fitting, though we caution that this fitting is uncertain due to the limited range of galaxy conditions covered by our simulations. We also find that the non-equilibrium chemistry has little effect on the conversion factor (&lt;5 per cent) for our high-mass galaxies, though still affects the H$_2$ mass and $L_{\rm{{\small CO}}}$ by $\approx$25 per cent.