bluuebunny/crossref_metadata_2025_split huggingface dataset:
New Minerals from the Redmond Mine, North Carolina, USA: V. Finescreekite and Hayelasdiite, Two New Thiosulfate Minerals Containing Cubane-Like Pb4O4 Structural Units
Authors: Kampf Anthony R. , Smith Jason B. , Hughes John M. , Ma Chi , Emproto Christopher 
Published: March 2024

Abstract
The new minerals finescreekite, [Pb4(OH)4](S2O3)2 (IMA2022–030), and hayelasdiite, [Pb4O1.5(OH)2.5]2[Cu+5(S2O3)4(S2O2OH)2(H2O)]·4H2O (IMA2022–021), were found in the Redmond mine, Haywood County, North Carolina, USA, where they occur in a highly unusual secondary assemblage that comprises a variety of rare Pb-Zn-Cu sulfates, thiosulfates, and carbonates. Finescreekite was found in close association with anglesite, cubothioplumbite, redmondite, and steverustite. Hayelasdiite was found in close association with anglesite and steverustite. Finescreekite properties: colorless tablets to about 1.5 mm across; white streak; resinous to adamantine luster; brittle; Mohs hardness ∼ 2½; curved, stepped fracture; excellent cleavage on {001}, fair on {100}, {010}, and {110}; 5.675 g/cm3 calculated density; biaxial (−) with α = 2.00(1), β = 2.04(calc), γ = 2.065(calc), 2V = 75.9(5)°. Hayelasdiite properties: colorless prisms and blades to about 0.5 mm in length; white streak; vitreous to subadamantine luster; brittle; Mohs hardness ∼ 2½; curved fracture; perfect cleavage on {010}; 4.909 g/cm3 calculated density; biaxial (−) with α = 1.89(1), β = 1.95(calc), γ = 1.97(calc), 2V = 58(5)°. Electron probe microanalyses provided the empirical formulae [Pb4(OH)4](S2O3)1.76(SO4)0.24 and [Pb4.00O1.5(OH)2.5]2[Cu+5.00(S2O3)3.24(SO4)0.76(S2O2OH)2(H2O)]·4H2O for finescreekite and hayelasdiite, respectively. Finescreekite is Orthorhombic, P212121, a = 8.2330(9), b = 10.7128(13), c = 14.8256(13) Å, V = 1307.6(2) Å3, and Z = 4. Hayelasdiite is triclinic, P, a = 7.52089(15), b =14.9345(3), c = 17.9895(13) Å, α = 106.727(8), β = 90.966(6), γ = 90.031(6)°, V = 1934.79(16) Å3, and Z = 2. The structures of finescreekite (R1 = 0.061 for 1440 I &gt; 2σI) and hayelasdiite (R1 = 0.055 for 5636 I &gt; 2σI) both contain cubane-like Pb4O4 clusters, [Pb4(OH)4]4+ in finescreekite and [Pb4O1.5(OH)2.5]2.5+ in hayelasdiite. The structure of hayelasdiite also contains a decorated double chain with the formula [Cu+5(S2O3)4(S2O2OH)2(H2O)]5−.
Ser pintura para hacer refugios más que humanos: Fernández Cuesta y Yayoi Kusama
Authors: González Calvo Nerea , Amann Alcocer Atxu 
Published: March 2024

La negación de la libertad consiste en desvincular su trabajo del deseo. En el caso de las mujeres, el trabajo doméstico, tan imprescindible como invisible, se traduce en el cuidado del espacio en el que están encerradas y el de sus habitantes.
La subversión acontece cuando el trabajo se hace visible y se vincula al deseo personal. Es entonces cuando cada mujer se construye en el cuidado a ella misma, mediante acciones liberadoras que les facilitan salir de su encierro, rompiendo sus límites físicos y mentales.
María Ángeles Fernández Cuesta, “la pinturitas” y Yayoi Kusama son dos mujeres que a través de una acción gráfica, continua y libre, mediante el movimiento de sus cuerpos dejan huella y se apropian del espacio; toman el mundo como lienzo para compartir sus preocupaciones y obsesiones. Crean un imaginario radical que va más allá de las imágenes establecidas por el humanismo heteropatriarcal para incorporar narrativas más que humanas.
Patient Safety: Ultrasound-Assisted Buttock Fat Grafting for the Effectiveness of Aesthetic Results
Authors: Gallaga Towns Jesús Eduardo Daniel , Martínez Garza Lucia Isabel 
Published: March 2024

A systematic review of the literature was carried out, whose basis is the structured and systematic integration of the information obtained in different research studies published in specialized journals, which was a search of records in the following databases: PubMed, SciELO and Science Direct of studies published in the last 10 years (2013-2023). The articles were searched in English and Spanish, Portuguese and once selected, they were read, with the due concentration of relevant information for this research. Two independent reviewers screened publications including those showing or not showing clinical evidence for "Ultrasound-assisted buttock fat grafting for the effectiveness of aesthetic outcomes ." We included 4 studies that met our selection criteria. We extracted data from: year of publication, author, country, population and outcomes. Conclusion: The use of real-time ultrasound allows injection into the subcutaneous plane of the skin, avoiding the deep plane where life-threatening complications such as fat embolism could occur.
Error Analysis for Rotating-drift-scan Charge-coupled Device Observation of Near-Earth Asteroids
Authors: Tang Kai , Pomazan Anton , Maigurova Nadiia , Song Yezhi , Yu Yong , Mao Yindun , Tang Zhenghong 
Published: March 2024

Abstract
The apparent velocities of near-Earth asteroids (NEAs) are usually high when they pass by Earth. Observing these fast-moving objects with long exposure times would cause their images to streak and significantly decrease the precision of astronomical measurements. The rotating-drift-scan (RDS) charge-coupled device technique is a promising approach to observe fast-moving NEAs during their close approaches to Earth. By rotating the camera of a telescope, an NEA can be observed in the time delay integration mode. This allows the asteroid to be imaged as a point source, even with a long exposure time. Here, we thoroughly present the RDS follow-up observation and orbit determination of a newly discovered NEA 2023 BJ7. This technique makes an impactful contribution to improving the NEA's orbit accuracy by extending the observation arc. A detailed statistical analysis of the astrometric error was conducted, revealing that RDS observations can achieve a competitive accuracy with an rms error of 0.″24 in right ascension and 0.″32 in declination. The instability of the telescope is thought to be the main reason affecting the internal precision. Furthermore, the RDS technique excels at observing fast-moving NEAs, as well as newly discovered NEAs without accurate ephemerides. For NEAs with rates of motion exceeding 10 deg day−1, the rms of RDS observation residuals is 0.″35 in the along-track direction and 0.″23 in the cross-track. With this technique, a network of small-aperture telescopes would substantially benefit our global NEAs monitoring system to ensure Earth’s safety from any asteroid impacts.
Precise Mass Measurement of OGLE-2013-BLG-0132/MOA-2013-BLG-148: A Saturn-mass Planet Orbiting an M Dwarf
Authors: Rektsini Natalia E. , Batista Virginie , Ranc Clément , Bennett David P. , Beaulieu Jean-Philippe , Blackman Joshua W. , Cole Andrew A. , Terry Sean K. , Koshimoto Naoki , Bhattacharya Aparna , Vandorou Aikaterini , Plunkett Thomas J. , Marquette Jean-Baptiste 
Published: March 2024

Abstract
We revisit the planetary microlensing event OGLE-2013-BLG-0132/MOA-2013-BLG-148 using Keck adaptive optics imaging in 2013 with NIRC2 and in 2020, 7.4 yr after the event, with OSIRIS. The 2020 observations yield a source and lens separation of 56.91 ± 0.29 mas, which provides us with a precise measurement of the heliocentric proper motion of the event μ
rel,hel = 7.695 ± 0.039 mas yr−1. We measured the magnitude of the lens in the K band as K
lens = 18.69 ± 0.04. Using these constraints, we refit the microlensing light curve and undertake a full reanalysis of the event parameters including the microlensing parallax π
E and the distance to the source D

S
. We confirm the results obtained in the initial study by Mróz et al. and improve significantly upon the accuracy of the physical parameters. The system is an M dwarf of 0.495 ± 0.054 M
⊙ orbited by a cold, Saturn-mass planet of 0.26 ± 0.028 M
Jup at projected separation r
⊥ = 3.14 ± 0.28 au. This work confirms that the planetary system is at a distance of 3.48 ± 0.36 kpc, which places it in the Galactic disk and not the Galactic bulge.
SOFIA/HAWC+ Far-Infrared Polarimetric Large Area CMZ Exploration Survey. I. General Results from the Pilot Program
Authors: Butterfield Natalie O. , Chuss David T. , Guerra Jordan A. , Morris Mark R. , Paré Dylan , Wollack Edward J. , Dowell C. Darren , Hankins Matthew J. , Karpovich Kaitlyn , Siah Javad , Staguhn Johannes , Zweibel Ellen 
Published: March 2024

Abstract
We present the first data release of the Far-Infrared Polarimetric Large Area CMZ Exploration (FIREPLACE) survey. The survey was taken using the 214 μm band of the HAWC+ instrument with the SOFIA telescope (19.″6 resolution; 0.7 pc). In this first data release we present dust polarization observations covering a ∼0.°5 region of the Galactic center’s central molecular zone (CMZ), approximately centered on the Sgr B2 complex. We detect ∼25,000 Nyquist-sampled polarization pseudovectors, after applying the standard SOFIA cuts for minimum signal-to-noise ratios in fractional polarization and total intensity of three and 200, respectively. Analysis of the magnetic field orientation suggests a bimodal distribution in the field direction. This bimodal distribution shows enhancements in the distribution of field directions for orientations parallel and perpendicular to the Galactic plane, which are suggestive of a CMZ magnetic field configuration with polodial and torodial components. Furthermore, a detailed analysis of individual clouds included in our survey (i.e., Sgr B2, Sgr B2-NW, Sgr B2-Halo, Sgr B1, and Cloud E/F) shows they have fractional polarization values of 1%–10% at 214 μm, with most of the emission having values <5%. A few of these clouds (i.e., Sgr B2 and Cloud E/F) show relatively low fractional polarization values toward their cores and higher fractional polarization values toward their less dense peripheries. We also observe higher fractional polarization toward compact H ii regions, which could indicate an enhancement in the grain alignment in the dust surrounding these sources.
Relevance of the P+O2 Reaction for PO Formation in Astrochemical Environments: Electronic Structure Calculations and Kinetic Simulations
Authors: García de la Concepción Juan , Cavallotti Carlo , Barone Vincenzo , Puzzarini Cristina , Jiménez-Serra Izaskun 
Published: March 2024

Abstract
Phosphorus monoxide (PO) is a key brick of prebiotic chemistry since it is a potential precursor of phosphates, which are present in all living systems. Prompted by the lack of information on the different processes involved in the formation of PO, we have revisited and analyzed in detail the P(4
S) + O2(3Σ−) and P(4
S) + O2(1Δ) reactions leading to PO. The former process has been widely studied from both experimental and theoretical points of view, however, with contradictory results. We have used high-level quantum-chemical calculations to accurately describe the reaction mechanisms. Next, rate constants have been computed using a master equation approach based on ab initio transition state theory. By incorporating the P(4
S) + O2(3Σ−) reaction in an astrochemical model, we have found that this reaction cannot be overlooked when aiming at a complete understanding of the PO abundance in regions dominated by shocks with speeds below 40 km s−1.
2.5D Magnetohydrodynamic Simulation of the Formation and Evolution of Plasmoids in Coronal Current Sheets
Authors: Mondal Sripan , Srivastava Abhishek K. , Pontin David I. , Yuan Ding , Priest Eric R. 
Published: March 2024

Abstract
In the present paper, using MPI-AMRVAC, we perform a 2.5D numerical magnetohydrodynamic simulation of the dynamics and associated thermodynamical evolution of an initially force-free Harris current sheet subjected to an external velocity perturbation under the condition of uniform resistivity. The amplitude of the magnetic field is taken to be 10 G, typical of the solar corona. We impose a Gaussian velocity pulse across this current sheet that mimics the interaction of fast magnetoacoustic waves with a current sheet in the corona. This leads to a variety of dynamics and plasma processes in the current sheet, which is initially quasi-static. The initial pulse interacts with the current sheet and splits into a pair of counterpropagating wavefronts, which form a rarefied region that leads to an inflow and a thinning of the current sheet. The thinning results in Petschek-type magnetic reconnection followed by a tearing instability and plasmoid formation. The reconnection outflows containing outward-moving plasmoids have accelerated motions with velocities ranging from 105 to 303 km s−1. The average temperature and density of the plasmoids are found to be 8 MK and twice the background density of the solar corona, respectively. These estimates of the velocity, temperature, and density of the plasmoids are similar to values reported from various solar coronal observations. Therefore, we infer that the external triggering of a quasi-static current sheet by a single-velocity pulse is capable of initiating magnetic reconnection and plasmoid formation in the absence of a localized enhancement of resistivity in the solar corona.
Long-term Study of the First Galactic Ultraluminous X-Ray Source Swift J0243.6+6124 Using NICER
Authors: Chhotaray Birendra , Jaisawal Gaurava K. , Nandi Prantik , Naik Sachindra , Kumari Neeraj , Ng Mason , Gendreau Keith C. 
Published: March 2024

Abstract
We present the results obtained from detailed X-ray timing and spectral studies of X-ray pulsar Swift J0243.6+6124 during its giant and normal X-ray outbursts between 2017 and 2023 observed by the Neutron star Interior Composition Explorer (NICER). We focused on a timing analysis of the normal outbursts. A distinct break is found in the power density spectra of the source. The corresponding break frequency and slopes of the power laws around the break vary with luminosity, indicating a change in the accretion dynamics with the mass accretion rate. Interestingly, we detected quasiperiodic oscillations within a specific luminosity range, providing further insights into the underlying physical processes. We also studied the neutron star spin period evolution and a luminosity variation in the pulse profile during the recent 2023 outburst. The spectral analysis was conducted comprehensively for the giant and all other normal outbursts. We identified a double transition at luminosities of ≈7.5 × 1037 and 2.1 × 1038 erg s−1 in the evolution of continuum parameters like the photon index and cutoff energy with luminosity. This indicates three distinct accretion modes experienced by the source, mainly during the giant X-ray outburst. A soft blackbody component with a temperature of 0.08–0.7 keV is also detected in the spectra. The observed temperature undergoes a discontinuous transition when the pulsar evolves from a sub- to super-Eddington state. Notably, in addition to an evolving 6–7 keV iron line complex, a 1 keV emission line was observed during the super-Eddington state of the source, implying X-ray reflection from the accretion disk or outflow material.
Suicide Probability Among Patients With Schizophrenia and Bipolar Disorder
Authors: Yüksel Arzu , Yilmaz Emel Bahadir , Dikmen Sema Nur Türkoğlu 
Published: March 2024

Purpose:
To evaluate the possibility of suicide and related factors among individuals with schizophrenia and bipolar disorder (BD).

Method:

Data were collected for 270 individuals registered in a community mental health center using the Suicide Probability Scale (SPS). Subsequently,
t
test and multiple linear regression analyses were conducted on independent samples.

Results:
There was no statistically significant difference found between mean SPS scores of participants with schizophrenia and BD. However, hostility subscale mean scores of participants with schizophrenia were higher than those of participants with BD, and the difference was statistically significant. Sex, family history of mental illness, need for help with medication, suicidal ideation in the past 10 days, and number of suicide attempts were important predictors of suicide probability.

Conclusion:

Individuals with schizophrenia and BD and in remission should be evaluated periodically for the possibility of suicide. [
Journal of Psychosocial Nursing and Mental Health Services, 62
(8), 37–45.]
Advancing Behavioral Health Equity Through Telehealth and Remote Training of Newly Certified Psychiatric–Mental Health Nurse Practitioners
Authors: Chinnis Simone , Robidoux Hannah , Harrold S. Akeya , Lauerer Joy 
Published: March 2024

Purpose:
Rural communities are disproportionately impacted by acute shortages of mental health providers. This problem, combined with complex behavioral health conditions, elicited the need for a university-based, remote telepsychiatric traineeship for newly board certified psychiatric–mental health nurse practitioners (PMHNPs).

Method:
The Psychiatric Advanced Practice Registered Nurse TechNology Enhanced Residency (PARTNER) Program was developed to advance behavioral health equity by increasing state-wide access to care, removing geographical barriers, and enhancing PMHNP workforce readiness by strengthening trainees' ability to manage complex behavioral health conditions.

Results:
In a southeastern state over a period of 3 years, six PMHNPs cumulatively provided behavioral health services to 1,195 patients, managed >118 diagnoses, and completed 3,535 visits, with 95.6% of visits comprising provision of care to patients residing in rural areas.

Conclusion:

Care was provided through the implementation of a collaborative-interdisciplinary-care model provided by route of telehealth and comprising a partnership between PMHNPs and patients' primary care providers. The training program enhanced providers' clinical proficiency, improved patient outcomes, and increased the number of skilled providers trained to manage patients with complex behavioral health conditions. [
Journal of Psychosocial Nursing and Mental Health Services, 62
(8), 19–24.]
Le soutien de l’enseignant d’EPS pour engager les élèves “difficiles” de lycée professionnel dans le travail en classe : des moments partagés entre l’enseignant et ses élèves au cours d’une année scolaire
Authors: Girard Amélina , Gal-Petitfaux Nathalie , Vors Olivier 
Published: March 2024

Cette étude vise à comprendre la construction d’une relation de soutien entre l’enseignant d’EPS et les élèves de lycée professionnel considérés comme un public difficile. L’engagement de ces élèves dans le travail se révèle être au cœur des préoccupations des enseignants intervenant dans ces contextes tant leur rapport à l’école est distant. Le soutien de l’enseignant apparait comme un levier privilégié pour favoriser l’engagement dans le travail de ces élèves. Il s’agit alors, dans le cadre théorique du Cours d’action (Theureau, 2015), de comprendre comment ce soutien est vécu par l’enseignant et ses élèves au cours de l’année et comment il se construit dans leurs interactions.L’étude a été menée au cours d’une année scolaire dans quatre lycées professionnels : 12 classes ont participé à l’étude quantitative rendant compte de la perception du soutien social de leur enseignant d’EPS (CASSS, Malecki et Elliott, 1999), quatre de ces classes ont été suivies pour une analyse qualitative basée sur des entretiens d’autoconfrontation. Le recueil de données s’est effectué à trois périodes de l’année selon trois étapes : (1) enregistrement audio-visuel, (2) passation du questionnaire CASSS (Malecki et Elliott, 1999), (3) entretiens d’auto- confrontation avec les élèves et leur enseignant d’EPS. Les résultats montrent que la relation soutenante de l’enseignant envers les élèves se construit tout au long de l’année, notamment lors de moments de soutien partagés synchroniquement et diachroniquement.
Skin testing: A valuable screening tool to identify allergy to anesthetic agents
Authors: Gull Ayaz , Bisati Aariba Z , Qureshi Taha A , Shafi Tabasum , Imran Sheikh , Ashraf Qazi , Rasool Roohi 
Published: March 2024

Abstract
Anaphylaxis is a rapid-onset, life-threatening allergic reaction that needs immediate medical intervention. Typically, immunoglobulin E (IgE) mediated, these reactions necessitate skin testing for assessing drug hypersensitivity. A 31-year-old woman with cervical carcinoma, scheduled for a total hysterectomy with bilateral salpingo-oophorectomy under general anesthesia (GA), experienced preoperative urticaria and palpitations, during a blood transfusion. Administering intravenous (IV) pheniramine, ranitidine, and dexamethasone resolved symptoms, allowing surgery under GA. However, post atracurium injection, she developed generalized urticaria and mild hypotension. IV pheniramine and hydrocortisone stabilized her, prompting surgery deferral for an allergology workup. The skin testing was performed, and all drugs tested negative. To prevent non-IgE-mediated reactions, a preoperative regimen of pheniramine 25 mg, prednisolone 50 mg, and famotidine 20 mg was recommended. Subsequently, surgery was performed under GA, using propofol and rocuronium, with the whole perioperative period remaining uneventful. This case underscores the imperative role of skin testing in elucidating perioperative drug usage amid suspected or encountered drug allergies.
Exploring the nexus: Asthma prevalence, smoking habits, and medication adherence among urban slum dwellers of Delhi
Authors: Saroj Shyam Kanhaiya , Kumar Raj , Kumar Manoj 
Published: March 2024

Abstract

BACKGROUND:
Asthma is chronic lung disease. Reducing exposure to tobacco smoke is vital for both primary prevention of asthma and disease management. Adherence to medical advice is crucial for the effectiveness of treatments. This research explores the connected dynamics of smoking habits, asthma prevalence, and medication adherence among urban slum dwellers.

METHODS:
A door-to-door survey was conducted in two urban slums of Delhi, employing a random sampling method to study 318 households comprehensively. Two proficient research volunteers administered a questionnaire designed to assess smoking habits, asthma prevalence, adherence to prescribed medications, and devices used by individuals with asthma.

RESULTS:
The overall prevalence of asthma was found at 1.6%, with gender-specific rates of 0.9% and 0.7% for males and females, respectively, with a mean age of 35.62 years (standard deviation = 15.93) in the population of 1376 individuals. Within the cohort of asthmatic patients, 13.6% exhibited severe asthma. Despite their asthma diagnosis, 9.1% were current active smokers, and 18.2% transitioned to the use of smokeless tobacco. The odds ratio for being asthmatic in smokers as compared to nonsmokers was 2.11 (95% confidence interval: 0.81–5.46, P = 0.1224). A significant proportion of patients displayed lapses in adhering to prescribed medication regimens.

CONCLUSION:
The current study sheds light on a concerning trend of negligence observed in both medical adherence and smoking habits among asthmatic patients. The findings underscore the imperative for targeted interventions and educational initiatives aimed at enhancing adherence to medical regimens and mitigating smoking behaviors within this vulnerable patient population. Addressing these factors is pivotal for enhancing comprehensive asthma management, alleviating associated risks, and promoting more favorable long-term health outcomes.