bluuebunny/crossref_metadata_2025_split huggingface dataset:
Associations Between Sociodemographic, Mental Health, and Mild Traumatic Brain Injury Characteristics With Lifetime History of Criminal Justice Involvement in Combat Veterans and Service Members
Authors: Gius Becky K , Fournier Lauren F , Reljic Tea , Pogoda Terri K , Corrigan John D , Garcia Amanda , Troyanskaya Maya , Hodges Cooper B , Miles Shannon R 
Published: August 2022

ABSTRACT

Introduction
Veterans and service members (V/SM) may have more risk factors for arrest and felony incarceration (e.g., posttraumatic stress disorder and at-risk substance use) but also more protective factors (e.g., access to health care) to mitigate behaviors that may lead to arrest. As such, understanding which factors are associated with criminal justice involvement among V/SM could inform prevention and treatment efforts. The current study examined relationships between lifetime history of arrests and felony incarceration and sociodemographic, psychological, and brain injury characteristics factors among combat V/SM.

Materials and Methods
The current study was a secondary data analysis from the Chronic Effects of Neurotrauma Consortium multicenter cohort study, approved by local institutional review boards at each study site. Participants were V/SM (N = 1,540) with combat exposure (19% active duty at time of enrollment) who were recruited from eight Department of Veterans Affairs and DoD medical centers and completed a baseline assessment. Participants were predominantly male (87%) and white (72%), with a mean age of 40 years (SD = 9.7). Most (81%) reported a history of at least one mild traumatic brain injury, with one-third of those experiencing three or more mild traumatic brain injuries (33%). Participants completed a self-report measure of lifetime arrest and felony incarceration history, a structured interview for all potential concussive events, the post-traumatic stress disorder checklist for Diagnostic and Statistical Manual of Mental Disorders, Fifth Edition (DSM-5), and the Alcohol Use Disorders Identification Test-Consumption. Three groups were compared on self-reported level of lifetime history of criminal justice system involvement: (1) no history of arrest or incarceration (65%); (2) history of arrest but no felony incarceration (32%); and (3) history of felony incarceration (3%).

Results
Ordinal regression analyses revealed that hazardous alcohol consumption (β = .44, P &lt; .001; odds ratio = 1.56) was positively associated with increased criminal justice involvement after adjusting for all other variables. Being married or partnered (β = −.44, P &lt; .001; odds ratio = 0.64) was negatively associated with decreased criminal justice involvement.

Conclusions
The rate of lifetime arrest (35%) in this V/SM sample was consistent with rates of arrests in the U.S. general population. One modifiable characteristic associated with lifetime arrest and felony incarceration was hazardous alcohol consumption. Alcohol use should be a top treatment target for V/SM at risk for arrest and those with history of criminal justice involvement.
SARS-CoV-19-associated Rhino-orbital and cerebral mucormycosis: clinical and radiological presentations
Authors: Mittal Ashima , Mahajan Nitika , Pal Singh Dhanota Devinder , Paul Birinder S , Ahluwalia Srishti , Ahluwalia Saumya , Galhotra Arnav , Gupta Veenu , Puri Sanjeev , Verma Rohit , Munjal Manish , Goel Sahil , Chopra Sumeet , Mahajan Rajesh , Ahluwalia Archana , Saggar Kavita , Singh Gagandeep 
Published: August 2022

Abstract
We describe presenting clinical and imaging manifestations of severe acute respiratory syndrome coronavirus-2 (SARS-CoV-2)-associated Rhino-oculo-cerebral mucormycosis (ROCM) in a hospital setting during the second wave of SARS-CoV-2 pandemic in India. Data on the presenting manifestations were collected from 1 March to 31 May 2021. Associations between clinical and imaging findings were explored, specifically: (1) the presence or absence of orbital pain and infiltration of a superior orbital fissure on imaging; (2) the presence of unilateral facial nerve palsy and pterygopalatine fossa infiltration and geniculate ganglion signal on contrast magnetic resonance imaging, and (3) vision loss and optic nerve findings on imaging. Orbital pain was reported by 6/36 subjects. A fixed, frozen eye with proptosis and congestion was documented in 26 (72%), complete vision loss in 23 (64%), and a unilateral lower motor neuron facial nerve palsy in 18 (50%). No association was found between the presence of orbital pain and superior orbital fissure infiltration on imaging. The ipsilateral geniculate ganglion was found to enhance more profoundly in 7/11 subjects with facial palsy and available magnetic resonance (MR) imaging, and the ipsilateral pterygopalatine fossa was found infiltrated in 14. Among 23 subjects with complete loss of vision, 9 (39%) demonstrated long-segment bright signal in the posterior optic nerve on diffusion MR images. We conclude that orbital pain might be absent in SARS-CoV-2-associated ROCM. Facial nerve palsy is more common than previously appreciated and ischemic lesions of the posterior portion of the optic nerve underlie complete vision loss.
The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
Authors: Richings Alexander J , Faucher-Giguère Claude-André , Gurvich Alexander B , Schaye Joop , Hayward Christopher C 
Published: August 2022

ABSTRACT
Interstellar chemistry is important for galaxy formation, as it determines the rate at which gas can cool, and enables us to make predictions for observable spectroscopic lines from ions and molecules. We explore two central aspects of modelling the chemistry of the interstellar medium (ISM): (1) the effects of local stellar radiation, which ionizes and heats the gas, and (2) the depletion of metals on to dust grains, which reduces the abundance of metals in the gas phase. We run high-resolution (400 M⊙ per baryonic particle) simulations of isolated disc galaxies, from dwarfs to Milky Way-mass, using the fire galaxy formation models together with the chimes non-equilibrium chemistry and cooling module. In our fiducial model, we couple the chemistry to the stellar fluxes calculated from star particles using an approximate radiative transfer scheme; and we implement an empirical density-dependent prescription for metal depletion. For comparison, we also run simulations with a spatially uniform radiation field, and without metal depletion. Our fiducial model broadly reproduces observed trends in H i and H2 mass with stellar mass, and in line luminosity versus star formation rate for [C ii]$_{158 \rm {\mu m}}$, [O i]$_{63 \rm {\mu m}}$, [O iii]$_{88 \rm {\mu m}}$, [N ii]$_{122 \rm {\mu m}}$, and H α6563Å. Our simulations with a uniform radiation field predict fainter luminosities, by up to an order of magnitude for [O iii]$_{88 \rm {\mu m}}$ and H α6563Å, while ignoring metal depletion increases the luminosity of carbon and oxygen lines by a factor ≈ 2. However, the overall evolution of the galaxy is not strongly affected by local stellar fluxes or metal depletion, except in dwarf galaxies where the inclusion of local fluxes leads to weaker outflows and hence higher gas fractions.
The H i gas disc thickness of the ultra-diffuse galaxy AGC 242019
Authors: Li Xin , Shi Yong , Zhang Zhi-Yu , Chen Jianhang , Yu Xiaoling , Wang Junzhi , Gu Qiusheng , Li Songlin 
Published: August 2022

ABSTRACT
Ultra-diffuse galaxies (UDGs) are as faint as dwarf galaxies but whose sizes are similar to those of spiral galaxies. A variety of formation mechanisms have been proposed, some of which could result in different disc thicknesses. In this study, we measure the radial profile of the H i scale height (hg) and flaring angle (hg/R) of AGC 242019 through the joint Poisson–Boltzmann equation based on its well spatially-resolved H i gas maps. The mean H i scale height of AGC 242019 is $\langle h_{\rm g}\rangle \approx 537.15 \pm 89.4\,{\rm pc}$, and the mean flaring angle is $\langle h_{\rm g}/R \rangle\approx 0.19 \pm 0.03$. As a comparison, we also derive the disc thickness for a sample of 14 dwarf irregulars. It is found that the H i disc of AGC 242019 has comparable thickness to dwarfs. This suggests that AGC 242019 is unlikely to experience much stronger stellar feedback than dwarf galaxies, which otherwise leads to a thicker disc for this galaxy.
High mass flow rate in a BAL outflow of quasar SDSS J1130 + 0411
Authors: Walker Andrew , Arav Nahum , Byun Doyee 
Published: August 2022

ABSTRACT
We present the analysis of the absorption troughs of six outflows observed in quasar SDSS J1130 + 0411 ($z$ ≈ 3.98) with radial velocities ranging from −2400 to $-15\, 400$ km s−1. These spectra were taken with the Very Large Telescope/Ultraviolet and Visual Echelle Spectrograph over the rest-frame wavelength range of 1135–1890 Å. In the main outflow system ($v$ ≈ −3200 km s−1), we identify Fe ii and several Fe ii* absorption troughs, as well as Si ii and Si ii* troughs, which we use to determine the electron number density $\log n_e = 2.6_{-0.7}^{+0.8}$ cm−3. Using the column densities of these and other ions, we determine a photoionization solution with hydrogen column density $\log N_H = 21.44_{-0.33}^{+0.24}$ cm−2 and ionization parameter $\log U_H = -1.75_{-0.45}^{+0.28}$. From these values, we derive the distance $R = 16_{-11}^{+23}$ kpc, the average mass flow rate $\dot{M} = 4100_{-2400}^{+6600}$ M⊙ yr−1, and the kinetic luminosity $\log \dot{E}_k = 46.13_{-0.37}^{+0.41}$ erg s−1. This $\dot{E}_k$ is $1.4_{-0.8}^{+2.2}$ per cent of the quasar’s Eddington luminosity, and therefore contributes significantly to AGN feedback.
ATOMS: ALMA three-millimeter observations of massive star-forming regions – XII: Fragmentation and multiscale gas kinematics in protoclusters G12.42+0.50 and G19.88−0.53
Authors: Saha Anindya , Tej Anandmayee , Liu Hong-Li , Liu Tie , Issac Namitha , Lee Chang Won , Garay Guido , Goldsmith Paul F , Juvela Mika , Qin Sheng-Li , Stutz Amelia , Li Shanghuo , Wang Ke , Baug Tapas , Bronfman Leonardo , Xu Feng-Wei , Zhang Yong , Eswaraiah Chakali 
Published: August 2022

ABSTRACT
We present new continuum and molecular line data from the ALMA Three-millimeter Observations of Massive Star-forming regions (ATOMS) survey for the two protoclusters, G12.42+0.50 and G19.88−0.53. The 3 mm continuum maps reveal seven cores in each of the two globally contracting protoclusters. These cores satisfy the radius–mass relation and the surface mass density criteria for high-mass star formation. Similar to their natal clumps, the virial analysis of the cores suggests that they are undergoing gravitational collapse ($\rm \alpha _{vir} \lt \lt 2$). The clump to core scale fragmentation is investigated and the derived core masses and separations are found to be consistent with thermal Jeans fragmentation. We detect large-scale filamentary structures with velocity gradients and multiple outflows in both regions. Dendrogram analysis of the H13CO+ map identifies several branch and leaf structures with sizes ∼ 0.1 and 0.03 pc, respectively. The supersonic gas motion displayed by the branch structures is in agreement with the Larson power law indicating that the gas kinematics at this spatial scale is driven by turbulence. The transition to transonic/subsonic gas motion is seen to occur at spatial scales of ∼0.1 pc indicating the dissipation of turbulence. In agreement with this, the leaf structures reveal gas motions that deviate from the slope of Larson’s law. From the large-scale converging filaments to the collapsing cores, the gas dynamics in G12.42+0.50 and G19.88−0.53 show scale-dependent dominance of turbulence and gravity and the combination of these two driving mechanisms needs to be invoked to explain massive star formation in the protoclusters.
E
iso–Ep correlation of gamma-ray bursts: calibration and cosmological applications
Authors: Jia X D , Hu J P , Yang J , Zhang B B , Wang F Y 
Published: August 2022

ABSTRACT
Gamma-ray bursts (GRBs) are the most explosive phenomena and can be used to study the expansion of Universe. In this paper, we compile a long GRB sample for the Eiso–Ep correlation from Swift and Fermi observations. The sample contains 221 long GRBs with redshifts from 0.03 to 8.20. From the analysis of data in different redshift intervals, we find no statistically significant evidence for the redshift evolution of this correlation. Then we calibrate the correlation in six subsamples and use the calibrated one to constrain cosmological parameters. Employing a piece-wise approach, we study the redshift evolution of dark energy equation of state (EOS), and find that the EOS tends to be oscillating at low redshift, but consistent with −1 at high redshift. It hints at dynamical dark energy at 2σ confidence level at low redshift.
Acetaldehyde binding energies: a coupled experimental and theoretical study
Authors: Ferrero S , Grieco F , Ibrahim Mohamed A-S , Dulieu F , Rimola A , Ceccarelli C , Nervi C , Minissale M , Ugliengo P 
Published: August 2022

ABSTRACT
Acetaldehyde is one of the most common and abundant gaseous interstellar complex organic molecules found in cold and hot regions of the molecular interstellar medium. Its presence in the gas-phase depends on the chemical formation and destruction routes, and its binding energy (BE) governs whether acetaldehyde remains frozen on to the interstellar dust grains or not. In this work, we report a combined study of the acetaldehyde BE obtained via laboratory temperature programmed desorption (TPD) experiments and theoretical quantum chemical computations. BEs have been measured and computed as a pure acetaldehyde ice and mixed with both polycrystalline and amorphous water ice. Both calculations and experiments found a BE distribution on amorphous solid water that covers the 4000–6000 K range when a pre-exponential factor of $1.1\times 10^{18}\, \mathrm{s}^{-1}$ is used for the interpretation of the experiments. We discuss in detail the importance of using a consistent couple of BE and pre-exponential factor values when comparing experiments and computations, as well as when introducing them in astrochemical models. Based on the comparison of the acetaldehyde BEs measured and computed in the present work with those of other species, we predict that acetaldehyde is less volatile than formaldehyde, but much more than water, methanol, ethanol, and formamide. We discuss the astrochemical implications of our findings and how recent astronomical high spatial resolution observations show a chemical differentiation involving acetaldehyde, which can easily explained due to the different BEs of the observed molecules.
Engine-fed kilonovae (mergernovae) – I. Dynamical evolution and energy injection/heating efficiencies
Authors: Ai Shunke , Zhang Bing , Zhu Zhaohuan 
Published: August 2022

ABSTRACT
A binary neutron star merger is expected to be associated by a kilonova, transient optical emission powered by radioactive decay of the neutron-rich ejecta. If the post-merger remnant is a long-lived neutron star, additional energy injection to the ejecta is possible. In this first paper of a series, we study the dynamical evolution of the engine-fed kilonova (mergernova) ejecta in detail. We perform a semi-analytical study of the problem by adopting a modified mechanical blastwave model that invokes interaction between a Poynting-flux-dominated flow and a non-magnetized massive ejecta. Shortly after the engine is turned on, a pair of shocks would be excited. The reverse shock quickly reaches the wind-acceleration region and disappears (in a few seconds), whereas the forward shock soon breaks out from the ejecta (in 102–103 s) and continues to propagate in the surrounding interstellar medium. Most of the energy injected into the blastwave from the engine is stored as magnetic energy and kinetic energy. The internal energy fraction is fint &lt; 0.3 for an ejecta mass equal to 10−3 M⊙. Overall, the energy injecting efficiency ξ is at most ∼0.6 and can be as small as ∼0.04 at later times. Contrary to the previous assumption, efficient heating only happens before the forward shock breaks out of the ejecta with a heating efficiency ξt ∼ (0.006 − 0.3), which rapidly drops to ∼0 afterwards. The engine-fed kilonova light curves will be carefully studied in Paper II.
Comparing reflection and absorption models for the soft X-ray variability in the NLS1 AGN UGC 11763
Authors: Jiang Jiachen , Gallo Luigi C , Grupe Dirk , Parker Michael L 
Published: August 2022

ABSTRACT
We present a spectral analysis of two XMM–Newton observations of the narrow-line Seyfert 1 galaxy UGC 11763. UGC 11763 shows very different soft X-ray spectral shapes in the two observations separated by 12 yr. Three spectral models are considered to explain the multi-epoch X-ray variability of UGC 11763, one based on the relativistic disc reflection model, one based on multiple partially covering absorbers combined with the warm corona model, and a hybrid model. In the first model, the X-ray variability of UGC 11763 is caused by the emission from a compact coronal region with a variable size. The resulting disc reflection component changes accordingly. A warm absorption model with a modest column density is required in this model too. In the partially covering absorption scenario, the X-ray variability of UGC 11763 is caused by the variable covering factors of two absorbers located within a region of r &lt; ≈100rg. Moreover, the temperature and strength of the warm corona have to change significantly too to explain the variable underlying soft X-ray emission. Lastly, we investigate the possibility of variable intrinsic power-law emission from the hot corona combined with variable absorption in UGC 11763 without changing the geometry of the corona in the third model. This hybrid model provides a slightly better fit than the partially covering absorption model with improvements in fitting the iron emission band. Current CCD-resolution data cannot distinguish these spectral models for UGC 11763. Future high-resolution X-ray missions, e.g. Athena and XRISM, will test them by resolving different spectral components.
A multifidelity emulator for the Lyman-α forest flux power spectrum
Authors: Fernandez M A , Ho Ming-Feng , Bird Simeon 
Published: August 2022

ABSTRACT
In this work, we extend our recently developed multifidelity emulation technique to the simulated Lyman-α forest flux power spectrum. Multifidelity emulation allows interpolation of simulation outputs between cosmological parameters using many cheap low-fidelity simulations and a few expensive high-fidelity simulations. Using a test suite of small-box (30 Mpc h−1) simulations, we show that multifidelity emulation is able to reproduce the Lyman-α forest flux power spectrum well, achieving an average accuracy when compared to a test suite of $0.8\, {\rm {per\ cent}}$. We further show that it has a substantially increased accuracy over single-fidelity emulators, constructed using either the high- or low-fidelity simulations only. In particular, it allows the extension of an existing simulation suite to smaller scales and higher redshifts.
Does locomotive syndrome severity predict future fragility fractures in community-dwelling women with osteoporosis?
Authors: Asahi Ryoma , Nakamura Yutaka , Koike Yoshinao , Kanai Masayoshi , Watanabe Kento , Yuguchi Satoshi , Kamo Tomohiko , Azami Masato , Ogihara Hirofumi , Asano Satoshi 
Published: August 2022

ABSTRACT

Objectives
We investigated whether the locomotive syndrome (LS) severity affects future fragility fractures in osteoporosis patients.

Methods
In this retrospective cohort study, 315 women with osteoporosis (mean follow-up period, 2.8 years) were reviewed, of whom 244 were included in the analysis. At baseline, we obtained medical information, bone mineral density of the lumbar spine and femoral neck, and sagittal vertical axis. Additionally, LS risk was assessed using the two-step test, stand-up test, and 25-question geriatric locomotive function scale scores. The LS risk test results were used to classify LS severity, which was rated on a 4-point scale from stage 0 (robust) to 3 (worsening). Cox proportional hazards regression analysis was used to determine the association of the severity with future fragility fracture.

Results
Fragility fractures occurred in 37 of 315 participants (11.8%). This study showed that sagittal vertical axis (hazard ratio = 1.014; 95% confidence interval, 1.005–1.023; p value = 0.003) and LS severity (hazard ratio =1.748; 95% confidence interval, 1.133–2.699; p = 0.012) were independent risk factors for incidence of fragility fracture.

Conclusions
This study revealed the LS severity to predicted fragility fractures. We suggested that the progression of LS associated with osteoporosis increases the fracture risk.
A case report of two systemic lupus erythematosus pregnancies with early placental exposure to belimumab: Case report with review
Authors: Nakai Takehiro , Ikeda Yukihiko , Yamaguchi Kenichi , Asano Takahiro , Iwata Futoshi , Kidoguchi Genki , Fukui Sho , Ozawa Hiroki , Kawaai Satoshi , Kitada Ayako , Suda Masei , Nomura Atsushi , Tamaki Hiromichi , Okada Masato 
Published: August 2022

ABSTRACT
Since its approval for the management of systemic lupus erythematosus (SLE), belimumab has been widely used. However, its pregnancy safety profile has been underinvestigated. We present the pregnancy outcomes of two cases of early placental exposure to belimumab and summarise the pregnancy outcomes in previous reports regarding placental exposure to belimumab. Case 1 describes a 27-year-old woman with an 18-year history of SLE and lupus nephritis class III. We introduced belimumab 19 months prior to conception to control her proteinuria and discontinued its use at 5 weeks and 5 days of gestation. Her lupus activity was stable throughout pregnancy, and at 37 weeks and 1 day of gestation, she delivered a healthy girl with no anomaly. At delivery, the girl was small for gestational age, but at the 1-year follow-up, there was no delay in her growth or any serious infection. Case 2 describes a 32-year-old woman with a 15-year history of SLE. We introduced belimumab 9 months prior to conception and discontinued its use at 7 weeks and 1 day of gestation. Although her lupus was well controlled without belimumab, a missed abortion occurred, which was possibly due to foetal factors. Although there is accumulating data on the safety of belimumab use during pregnancy, it seems necessary to cautiously use this medication in pregnant women, until further analyses are conducted.
Programmable RNA base editing with a single gRNA-free enzyme
Authors: Han Wenjian , Huang Wendi , Wei Tong , Ye Yanwen , Mao Miaowei , Wang Zefeng 
Published: August 2022

Abstract
Programmable RNA editing enables rewriting gene expression without changing genome sequences. Current tools for specific RNA editing dependent on the assembly of guide RNA into an RNA/protein complex, causing delivery barrier and low editing efficiency. We report a new gRNA-free system, RNA editing with individual RNA-binding enzyme (REWIRE), to perform precise base editing with a single engineered protein. This artificial enzyme contains a human-originated programmable PUF domain to specifically recognize RNAs and different deaminase domains to achieve efficient A-to-I or C-to-U editing, which achieved 60–80% editing rate in human cells, with a few non-specific editing sites in the targeted region and a low level off-target effect globally. The RNA-binding domain in REWIREs was further optimized to improve editing efficiency and minimize off-target effects. We applied the REWIREs to correct disease-associated mutations and achieve both types of base editing in mice. As a single-component system originated from human proteins, REWIRE presents a precise and efficient RNA editing platform with broad applicability.