bluuebunny/crossref_metadata_2025_split huggingface dataset:
Evaluating the Dear MD to Be Podcast as an Equity, Diversity and Inclusion resource: a cross-sectional survey analysis
Authors: Kherani Imaan Zera , Osei-Yeboah Clara , Bushra Maham , Mahendiran Meera , Inibhunu Happy , Mylopoulos Maria , Law Marcus 
Published: November 2024

Background: Equity-deserving groups are communities marginalized from institutional power by oppressive forces (e.g., racism, sexism, homophobia, ableism). Dear MD to Be is a medical-student-led podcast created to interview physicians of intersectional backgrounds about their institutional experience. This study aims to evaluate the podcast as a tool for knowledge, mentorship, and psychological safety for equity-deserving listeners.
Methods: Between February and March 2022, we recruited medical students across all levels of training from English-speaking Canadian medical schools using email listservs and social media. We disseminated a cross-sectional questionnaire assessing demographics, knowledge gained from podcast engagement, attitudes towards podcasts as a tool for mentorship, and psychological/emotional gains from the podcast content. We conducted descriptive and frequency analyses of quantitative data and applied thematic analysis to qualitative data.
Results: Thirty-eight individuals completed the entire survey from all levels of training, with 97% self-identifying with at least one equity-deserving group. 100% agreed that the Dear MD to Be podcast was an accessible form of mentorship; participants appreciated self-pacing mentorship and interacting with many narratives. Listeners gleaned lessons about wellness, advocacy work, allyship, cultural imposter syndrome, and navigating discrimination. Furthermore, most listeners felt represented, empowered, and legitimized by podcast content.
Conclusions: Podcasts can serve as a medium for accessible equity-centred mentorship. By disseminating multiple underrepresented narratives in medicine, the Dear MD to Be podcast serves as a source of EDI knowledge while contributing to learner safety.
PROFIL DEMOGRAFI DAN EFIKASI DIRI PADA PENDERITA DM TIPE II
Authors: Manoppo Arlien Jeannete 
Published: November 2024

Diabetes Melitus Tipe II (DMT2) merupakan masalah kesehatan global dengan prevalensi yang terus meningkat, mencapai 171 juta penderita pada 2021 dan diperkirakan menjadi 366 juta pada 2030. Komplikasi serius dari penyakit ini dapat menyebabkan angka kematian yang tinggi, sehingga pengelolaan mandiri menjadi krusial. Profil demografi seperti usia, jenis kelamin, tingkat pendidikan, pekerjaan, serta pendapatan memainkan peran dalam efikasi diri, yang berdampak pada keberhasilan pengelolaan penyakit. Oleh karena itu, penelitian ini bertujuan untuk menguji perbedaan antara profil demografi dengan efikasi diri pada penderita DMT2. Desain deskriptif komparasi dan cross-sectional diterapkan pada 60 sampel di salah satu puskesmas, Minahasa Utara yang diseleksi menggunakan teknik convenience sampling. The Diabetes Mellitus Management Self-Efficacy Scale (DMSES) digunakan untuk mengukur efikasi diri sedangkan profil demografi diukur dengan checklist. Uji Independent T-Test, One-way ANOVA dan Pearson Correlation digunakan sebagai uji bivariat. Mayoritas responden memiliki efikasi diri yang baik (83,3%), namun tidak ditemukan perbedaan yang signifikan antara profil demografi (usia, jenis kelamin, pendidikan, pekerjaan, dan pendapatan) dengan efikasi diri pada penderita DMT2 (p>0,05). Meskipun tidak ada perbedaan signifikan dalam aspek demografi penderita DMT2, hampir semua responden menunjukkan efikasi diri yang baik, mencerminkan kesadaran dan manajemen aktif dalam pengelolaan penyakit mereka
Type II Diabetes (T2D) represents a burgeoning global health concern, with its prevalence escalating from 171 million cases in 2021 to a projected 366 million by 2030. The potentially lethal complications associated with this disease underscore the critical importance of effective self-management strategies. Demographic factor including age, gender, educational attainment, occupation, and income, play pivotal roles in shaping patients' self-efficacy, which in turn significantly influences disease management outcomes. This study aims to explore the potential disparities in self-efficacy among T2D patients across various demographic profiles. A descriptive comparative and cross-sectional design was employed, involving a sample of 60 participants from a community health center in North Minahasa, selected through convenience sampling. The Diabetes Mellitus Management Self-Efficacy Scale (DMSES) was utilized to assess self-efficacy, while demographic profiles were measured using a checklist. Independent T-Test, One-way ANOVA, and Pearson Correlation were applied as bivariate tests. The majority of respondents demonstrated good self-efficacy (83.3%); however, no significant differences were found between demographic profiles (age, gender, education, occupation, and income) and self-efficacy in individuals with T2D (p > 0.05). While no significant demographic differences were observed among T2D patients, nearly all respondents exhibited good self-efficacy, reflecting an active awareness and management of their condition.
VLT/MUSE Detection of Accretion/Ejection Associated with the Close Stellar Companion in the HT Lup System
Authors: Jorquera Sebastián , Bonnefoy Mickaël , Pérez Laura M. , Chauvin Gaël , Aguinaga Adrian , Dougados Catherine , Julo Rémi , Demars Dorian , Andrews Sean M. , Ricci Luca , Zhu Zhaohuan , Kurtovic Nicolas T. , Cuello Nicolás , Bai Xue-Ning , Birnstiel Til , Dullemond Cornellis , Guzmán Viviana V. 
Published: November 2024

Abstract
The accretion/ejection processes in T Tauri stars are fundamental to their physical evolution, while also impacting the properties and evolution of the circumstellar material at a time when planet formation takes place. To date, the characterization of ongoing accretion processes in stellar pairs at 5–50 au scales has been challenging as high-angular resolution spectrographs are required to extract the spectral features of each component. We present the analysis of spectroscopic observations of the tight (160 mas, 25 au) T Tauri system HT Lup A/B, obtained with MUSE at the Very Large Telescope in 2021 March and July. We focus on constraining the accretion/ejection processes and variability of the secondary component HT Lup B by searching for accretion tracers by applying high-resolution spectral differential imaging techniques. We retrieve strong (signal-to-noise ratio > 5) Hα, Hβ, and [O i]λ6300 emission in both epochs. The Hα and Hβ line fluxes showcase high variability, with variations up to 200%–300% between epochs. The fluxes are consistent with accretion rates of 3× 10−9
M
⊙ yr−1 and 8 × 10−10
M
⊙ yr−1 for the first and second epochs, respectively. We attribute the increased accretion activity during the first night to a “burst-like” event, followed by a relaxation period more representative of the common accretion activity of the system. The [O i]λ6300 line profiles remain relatively similar between epochs and suggest ejection rates on the order of 10−9−10−10
M
⊙ yr−1, compatible with moderate disk wind emission. Our results also indicate that the accretion processes of HT Lup B are compatible with Classical T Tauri stars, unlike previous classifications.
High-redshift, Small-scale Tests of Ultralight Axion Dark Matter Using Hubble and Webb Galaxy UV Luminosities
Authors: Winch Harrison , Rogers Keir K. , Hložek Renée , Marsh David J. E. 
Published: November 2024

Abstract
We calculate the abundance of UV-bright galaxies in the presence of ultralight axion (ULA) dark matter (DM), finding that axions suppress their formation with a non-trivial dependence on redshift and luminosity. We set limits on axion DM using UV luminosity function (UVLF) data, excluding a single axion as all the DM for m
ax < 10−21.6 eV and limiting axions with

−
26
≤
log
(

m

ax

/

eV
)
≤
−
23

to be less than 22% of the DM (both at 95% credibility). These limits use UVLF measurements from 24,000 sources from the Hubble Space Telescope (HST) at redshifts 4 ≤ z ≤ 10. We marginalize over a parametric model connecting halo mass and UV luminosity. Our results bridge a window in axion mass and fraction previously unconstrained by cosmological data, between large-scale cosmic microwave background and galaxy clustering and the small-scale Lyα forest. These high-z measurements provide a powerful consistency check of low-z tests of axion DM, including the recent hint for a sub-dominant ULA DM fraction in Lyα forest data. We also consider a sample of 25 spectroscopically confirmed high-z galaxies from the James Webb Space Telescope (JWST), finding these data to be consistent with HST. Combining HST and JWST UVLF data does not improve our constraints beyond HST alone, but future JWST measurements have the potential to improve these results. We also find an excess of low-mass halos (<109
M
⊙) at z < 3, which could be probed by subgalactic structure probes (e.g., stellar streams, satellite galaxies, and strong lensing).
DESI Massive Poststarburst Galaxies at z ∼ 1.2 Have Compact Structures and Dense Cores
Authors: Zhang Yunchong , Setton David J. , Price Sedona H. , Bezanson Rachel , Khullar Gourav , Newman Jeffrey A. , Aguilar Jessica Nicole , Ahlen Steven , Andrews Brett H. , Brooks David , Claybaugh Todd , de la Macorra Axel , Dey Biprateep , Doel Peter , Gaztañaga Enrique , Gontcho A Gontcho Satya , Greene Jenny E. , Juneau Stephanie , Kehoe Robert , Kisner Theodore , Kriek Mariska , Leja Joel , Manera Marc , Meisner Aaron , Miquel Ramon , Moustakas John , Prada Francisco , Rossi Graziano , Sanchez Eusebio , Schubnell Michael , Siudek Małgorzata , Spilker Justin , Sprayberry David , Suess Katherine A. , Tarlé Gregory , Zou Hu ,   DESI Collaboration
Published: November 2024

Abstract
Poststarburst galaxies (PSBs) are young quiescent galaxies that have recently experienced a rapid decrease in star formation, allowing us to probe the fast-quenching period of galaxy evolution. In this work, we obtained Hubble Space Telescope (HST)/WFC3 F110W imaging to measure the sizes of 171 massive (

log
(

M
*

/

M
⊙

)
∼

11
)

spectroscopically identified PSBs at 1 < z 1.3 selected from the DESI Survey Validation luminous red galaxy sample. This statistical sample constitutes an order of magnitude increase from the ∼20 PSBs with space-based imaging and deep spectroscopy. We perform structural fitting of the target galaxies with pysersic and compare them to quiescent and star-forming galaxies in the 3D-HST survey. We find that these PSBs are more compact than the general population of quiescent galaxies, lying systematically ∼0.1 dex below the established size–mass relation. However, their central surface mass densities are similar to those of their quiescent counterparts (

log

(

Σ

1

kpc

/

(

M

⊙

kpc

−
2

)
)
∼
10.1

). These findings are easily reconciled by later ex situ growth via minor mergers or a slight progenitor bias. These PSBs are round in projection (b/a
median ∼ 0.8), suggesting that they are primarily spheroids, not disks, in 3D. We find no correlation between the time since quenching and light-weighted PSB sizes or central densities. This disfavors apparent structural growth due to the fading of centralized starbursts in this galaxy population. Instead, we posit that the fast quenching of massive galaxies at this epoch occurs preferentially in galaxies with preexisting compact structures.
ALMASOP. The Localized and Chemically Rich Features near the Bases of the Protostellar Jet in HOPS 87
Authors: Hsu Shih-Ying , Lee Chin-Fei , Liu Sheng-Yuan , Johnstone Doug , Liu Tie , Takahashi Satoko , Bronfman Leonardo , Chen Huei-Ru Vivien , Dutta Somnath , Eden David J. , Evans Neal J. , Hirano Naomi , Juvela Mika , Kuan Yi-Jehng , Kwon Woojin , Lee Chang Won , Lee Jeong-Eun , Li Shanghuo , Liu Chun-Fan , Liu Xunchuan , Luo Qiuyi , Qin Sheng-Li , Sahu Dipen , Sanhueza Patricio , Shang 尚 Hsien 賢 , Tatematsu Kenichi , Yang Yao-Lun 
Published: November 2024

Abstract
HOPS 87 is a Class 0 protostellar core known to harbor an extremely young bipolar outflow and a hot corino. We report the discovery of localized, chemically rich regions near the bases of the two-lobe bipolar molecular outflow in HOPS 87 containing molecules such as H2CO, 13CS, H2S, OCS, and CH3OH, the simplest complex organic molecule (COM). The locations and kinematics suggest that these localized features are due to jet-driven shocks rather than being part of the hot-corino region encasing the protostar. The COM compositions of the molecular gas in these jet-localized regions are relatively simpler than those in the hot-corino zone. We speculate that this simplicity is due to either the liberation of ice with a less complex chemical history or the effects of shock chemistry. Our study highlights the dynamic interplay between the protostellar bipolar outflow, disk, inner-core environment, and the surrounding medium, contributing to our understanding of molecular complexity in solar-like young stellar objects.
Investigating the Cosmological Rate of Compact Object Mergers from Isolated Massive Binary Stars
Authors: Boesky Adam P. , Broekgaarden Floor S. , Berger Edo 
Published: November 2024

Abstract
Gravitational-wave (GW) detectors are observing compact object mergers from increasingly far distances, revealing the redshift evolution of the binary black hole (BBH)—and soon the black hole–neutron star (BHNS) and binary neutron star (BNS)—merger rate. To help interpret these observations, we investigate the expected redshift evolution of the compact object merger rate from the isolated binary evolution channel. We present a publicly available catalog of compact object mergers and their accompanying cosmological merger rates from population synthesis simulations conducted with the COMPAS software. To explore the impact of uncertainties in stellar and binary evolution, our simulations use two-parameter grids of binary evolution models that vary the common-envelope efficiency with mass transfer accretion efficiency and supernova (SN) remnant mass prescription with SN natal kick velocity, respectively. We quantify the redshift evolution of our simulated merger rates using the local (z ∼ 0) rate, the redshift at which the merger rate peaks, and the normalized differential rates (as a proxy for slope). We find that although the local rates span a range of ∼103 across our model variations, their redshift evolutions are remarkably similar for BBHs, BHNSs, and BNSs, with differentials typically within a factor 3 and peaks of z ≈ 1.2–2.4 across models. Furthermore, several trends in our simulated rates are correlated with the model parameters we explore. We conclude that future observations of the redshift evolution of the compact object merger rate can help constrain binary models for stellar evolution and GW formation channels.
The Mass and Redshift Dependence of Halo Star Clustering
Authors: Tan Zhenlin , Wang Wenting , He Jiaxin , Zhang Yike , Rodriguez-Gomez Vicente , Han Jiaxin , Li Zhaozhou , Yang Xiaohu 
Published: November 2024

Abstract
We adopt the two-point correlation function (2PCF) as a statistical tool to quantify the spatial clustering of halo stars for galaxy systems spanning a wide range in host halo virial mass (

11.25
<

log

10

M

200
c

/

M

⊙

<
15

) and redshifts (0 < z < 1.5) from the IllustrisTNG simulations. Consistent with a previous study, we identify clear correlations between the strength of the 2PCF signals and galaxy formation redshifts, but over a much wider mass range. We find that such correlations are slightly stronger at higher redshifts and get weakened with the increase of host halo mass. We demonstrate that the spatial clustering of halo stars is affected by two factors: (1) the clustering gets gradually weakened as time passes (phase mixing); (2) newly accreted stars at more recent times would increase the clustering. For more massive galaxy systems, they assemble late, and the newly accreted stars would increase the clustering. The late assembly of massive systems may also help to explain the weaker correlations between the 2PCF signals and the galaxy formation redshifts in massive halos, as their 2PCFs are affected more by recently accreted stars, while formation redshift characterizes mass accretion on a much longer timescale. We find that the orbits of satellite galaxies in more massive halos maintain larger radial anisotropy, reflecting the more active accretion state of their hosts while also contributing to their stronger mass loss rates.
Visual Quality, Patient Satisfaction, and Photic Phenomena With a Diffractive Intraocular Lens and Its New Evolved Materials Version
Authors: Rementería-Capelo Laureano A. , Contreras Inés , Gros-Otero Juan , Mariñas Laura , Ruiz-Alcocer Javier 
Published: November 2024

Purpose
To assess the visual quality, patient satisfaction, and photic phenomena 3 and 12 months after the implantation of two similar diffractive intraocular lenses (IOLs) manufactured with different materials.

Methods
This retrospective observational study included patients with the AcrySof PanOptix IOL or the Clareon Pan-Optix IOL (both Alcon Laboratories, Inc). Three and 12 months after the surgery, binocular contrast sensitivity under photopic conditions was measured. The presence of dysphotopsias and difficulties when driving in dim light conditions was also reported. Patient satisfaction was assessed through the Catquest 9-SF questionnaire and patients also reported the need for additional spectacles at different distances. Twelve months after the surgery, the presence of posterior capsule opacification and glistening was reported.

Results
The study included 59 patients. Contrast sensitivity was stable in both groups 12 months after the surgery, the proportion of patients that always perceived halos decreased approximately 15%, and difficulties when driving at night were minimized. Both groups showed high and similar rates of satisfaction with their vision and achieved spectacle independence rates greater than 85% at the two visits. The presence of posterior capsule opacification was similar for both groups, whereas 64% and 90% of the eyes were free of glistening in the AcrySof and Clareon groups, respectively.

Conclusions
Both diffractive IOLs offer consistent visual outcomes and high rates of patient satisfaction during the initial 12 months after surgery. The results also suggest that the novel material may better preserve the transparency of the IOL in the long term.

[
J Refract Surg
. 2024;40(11):e877–e883.]
Visual Outcomes After Cataract Surgery With the Light Adjustable Lens in Japanese Patients With and Without Prior Corneal Refractive Surgery
Authors: Ichikawa Kei , Sakai Yukihiro , Toda Hiroto , Kato Yukihito , Ichikawa Kazuo 
Published: November 2024

Purpose
To describe Light Adjustable Lens (RxSight, Inc) (LAL) visual and refractive outcomes in a Japanese patient population with and without prior refractive surgery.

Methods
In this retrospective chart review of patients with cataract in a private eye clinic, 34 eyes from 21 patients underwent cataract surgery with LAL implantation. Eyes underwent light treatment to adjust the patients' refraction after implantation to meet individual visual goals. Standard visual and refractive outcomes were collected. Contrast sensitivity (to assess quality of vision), clinical defocus and vergence curves (to assess range of vision), and patient satisfaction were also collected.

Results
The mean prediction error of the light adjustment was −0.04 ± −0.48. Thirty-one eyes (91%) and 33 eyes (97%) were within ±0.25 and ±0.50 diopters (D) of manifest spherical equivalent target, respectively. Thirty-two eyes (94%) had residual refractive cylinder of 0.50 D or less. The full depth of focus was 3.68 D. Monocular contrast sensitivity shows frequencies equivalent to a normal population aged 50 to 60 years. The mean satisfaction score was 8.8 (scale: 1 to 10). There were no adverse events and no eyes lost corrected distance visual acuity from the light treatment.

Conclusions
LALs in cataract refractive surgery hold great promise, including for the Japanese population, which have unique ocular biometrics. By providing a safe procedure and the ability for postoperative adjustments, the LAL provided a tailored approach to vision correction, ultimately improving patient outcomes and satisfaction.

[
J Refract Surg
. 2024;40(11):e854–e862.]
L’élevage diversifie ses relations aux cultures en plaines cultivées : étude en région AuRA
Authors: Rapey Hélène , Cochetel Cécile , Hostiou Nathalie , Houdart Marie 
Published: November 2024

De nouvelles synergies végétal-animal sont recherchées dans les filières agricoles, mais les freins restent nombreux. Dans ce contexte, cette étude porte sur les élevages de petites zones céréalières et sur leurs échanges de matières entre ateliers d’élevages et de cultures, intra- et inter-exploitations. L’analyse de 32 enquêtes en ferme montre que ces élevages sont divers quant à leur dimension, orientation et commercialisation, en dépit de leur petit nombre. La taille de ces exploitations a peu évolué ces dix dernières années, mais leurs échanges intra- et inter-exploitations se sont diversifiés et la plupart ne prévoient pas d’arrêter l’élevage. Ceci appelle à ne pas minimiser le rôle et la dynamique de ces élevages dans les synergies cultures-élevage en zone céréalière.
Editorial Expression of Concern: Lipid-lowering therapy in patients with coronary heart disease: an Italian real-life survey. Results from the Survey on Risk FactOrs and CardiovascuLar secondary prevention and drug strategieS (SOFOCLES) in Italy
Authors: Monaldi Archives for Chest Disease Editors The 
Published: November 2024

The Editors and the Publisher have been alerted to concerns about this article (DOI: 10.4081/monaldi.2024.2972 ), and an investigation is in progress. In the interim, we alert readers that these concerns have been raised.
This Expression of Concern will remain in place until the investigation is completed and any further needs for appropriate action have been taken.
Stress-Strength Reliability Bayesian of Generalized Exponential-Poisson Distriution for Complete Data
Authors: Nada S Karam  , Hajer M AbdAwon  
Published: November 2024

In this paper, a Bayesian analysis is made to estimate the Reliability of two stress-strength model systems. First: the reliability of one component strengths X under stress Y. Second: reliability of one component strength under two stresses. Where X and Y are independent Generalized Exponential-poison random variables with (α, λ, θ) and (β, λ, θ), parameters respectively. The analysis is concerned based on complete data samples using gamma prior under eight different loss functions (Quadratic, Squared error, Weighted, Linear exponential, precautionary, De Groot, Entropy, and non-Linear exponential). The estimators are compared by Mean squared error criteria due to a simulation study and find that the best performance of the estimators found in order as (Quadratic, Weighted, Linear exponential and non-Linear exponential.