bluuebunny/crossref_metadata_2025_split huggingface dataset:
Les usagers professionnels des prévisions météorologiques probabilistes : des rapports à l'incertitude variés
Authors: Breton Éléanor 
Published: November 2023

Le rapport à l'incertitude des événements météorologiques et au risque qu'ils peuvent constituer pour les biens et les personnes est un enjeu devenu essentiel dans le contexte de dérèglement climatique que nous connaissons. Il est ainsi intéressant d'ouvrir la boîte noire des relations entretenues par les usagers professionnels météo-sensibles à l'égard de l'incertitude des prévisions afin d'en mesurer la complexité. Nous proposons ici de les envisager depuis la perspective sociologique, rarement empruntée sur ce terrain, comparativement aux approches psychologiques et économiques, en mettant en évidence certaines variables clés (météo-sensibilité continue ou segmentée, métier, expertise, rapport au risque, rapport au marché notamment). Les combinaisons singulières de ces variables produisent des rapports différents à l'information météorologique en fonction des usagers, utiles pour saisir leurs dispositions à s'approprier les prévisions probabilistes.
The relationship between the uncertainty of meteorological events and the risk they can pose to people and property has become an essential issue in the context of climate disruption. It is therefore interesting to open the black box of the relationships maintained by weather-sensitive professional users with regard to forecast uncertainty, in order to measure their complexity. We propose here to consider these relationships from a sociological perspective, which is rarely used in this field compared to psychological and economic approaches, by highlighting certain key variables (continuous or segmented weather-sensitivity, profession, expertise, relationship to risk, relationship to the market, etc.). The singular combinations of these variables produce different relationships to meteorological information, depending on the user, which is useful for grasping their disposition to appropriate probabilistic forecasts.
Retour d'expérience de l'inondation de Gaklé (Extrême-Nord au Cameroun) du 24 au 25 juillet 2018
Authors: Bouba Lucas , Samba Assomo Philippe 
Published: November 2023

Les analyses des données issues d'un observatoire hydrométéorologique, une reconnaissance des facteurs géomorphologiques environnants, ainsi qu'une analyse de l'évolution spatio-temporelle de l'orage grâce à l'imagerie satellitaire de Météosat, ontpermis de reconstituer les causes de l'inondation catastrophique survenue du 24 au 25 juillet 2018 à Gaklé dans l'Extrême-Nord au Cameroun. La combinaison de plusieurs facteurs peut expliquer l'inondation : (i) un contexte climatique caractérisé par une fréquence élevée des événements pluviométriques journaliers de classe P3 (cumul > 40 mm) ayant entraîné une forte humidité des sols ; (ii) une localisation de l'orage dans sa phase la plus sévère, dans un contexte de morphologie de terrain favorable à la crue de la rivière qui traverse Gaklé. En définitive, le retour d'expérience de cette inondation a permis de fournir à l'opinion des informations nécessaires pour améliorer la connaissance des facteurs d'occurrence des inondations dans la partie soudano-sahélienne du Cameroun.
Data from a hydrometeorological observatory subjected to statistical analyzes of time series, recognition of surrounding geomorphological factors, as well as an analysis of the spatio-temporal evolution of the storm using Meteosat satellite imagery, made it possible to reconstruct the causes of the catastrophic flood that occurred from July 24 to 25, 2018 in Gaklé in the peri-urban area of Maroua in the Far-North of Cameroon. The combination of several factors can explain the flooding: (i) a climatic context characterized by a high frequency of daily rainfall events of class P3 (with a cumulative > 40 mm) resulting in high soil humidity; (ii) location of the storm in its most severe phase in a context of land morphology favourable to the flooding of the river that crosses Gaklé. Ultimately, the experience feedback from this flood has made it possible to provide public opinion with the information necessary to improve knowledge of the factors of occurrence of floods in the Sudano-Sahelian part of Cameroon.
Enhancing Maternal Baby Massage Behavior in Makassar City through AH Baby Massage-Based Training
Authors: Harun Ayatullah , Amir Fatmawati 
Published: November 2023

Introduction: Current baby massage interventions have been shown to be effective in boosting baby growth so it is important to socialize baby massage to improve parents behavior so that they can do baby massage independently. The aim of this study was to evaluate the effectiveness of baby massage training based on the AH Baby Massage application to enhance mother's intentions, mother knowledge, mother attitude and mother skills doing baby massage.
Methods: This research uses quantitative methods with the design of one group pretest – posttest. To a mother who has a baby of 35 mothers in the area of work practice Bidan Independent District Biringkanaya City of Makassar.
Results: The results of the study were obtained, there were differences in the mother's intentions, the mother’s knowledge of her attitude and her skills in performing baby massages before and after the intervention of baby massage training based on the AH Baby Massage application with (p value < 0.05). Conclusion: The conclusion of the baby massage training based on the AH Baby Massage app has been shown to improve the mother's intentions, knowledge, attitude and skills of the mother doing baby massage so it requires the role of Puskesmas, health care and kader involvement in socializing baby massage.
Nursing Protocol: Oral Health in Older Patients
Authors: Tkacheva O. N. , Sharashkina N. V. , Runikhina N. K. , Kotovskaya Yu. V. 
Published: November 2023

In the presented article, the authors consider the problem of oral care for older patients with functional or cognitive impairments. This protocol outlines the process for assessing the oral cavity on patient’s admission and at each shift, explaining how to inform the therapist of any abnormalities when evaluating the oral health condition, and how to determine the extent to which oral care can be managed by the patient himself or herself. When providing oral care, measures are taken to prevent aspiration.
Hernia de Garengeot, Reporte de Caso Clínico
Authors: Campo González Leonardo Enrique , Pérez Otálora Deivis Alfonso , Llinas Burgos Lilibeth 
Published: November 2023

Las hernias contenedoras del apéndice cecal constituyen una rareza en la práctica médica habitual. La hernia femoral que contiene el apéndice fue descrita por primera vez por René-Jacques Croissant De Garengeot en 1731. Presentamos un caso clínico de una hernia de Garengeot, un hallazgo intraoperatorio de un saco herniario que contiene este órgano motivo por el cual se realiza el reporte del caso de un paciente masculino de 71 años quien ingresa a cirugía programado en la Clínica Misericordia Internacional de Barranquilla para herniorrafía inguinal derecha, al momento de realizar el procedimiento se encontró una hernia de Garengeot.
Fomento de las Competencias Investigativas de los Estudiantes de Básica y Media
Authors: Ortiz Franco Juan Vicente , Caicedo Mora Maria Raquel 
Published: November 2023

La formación en investigación es una habilidad fundamental que se desarrolla desde los primeros momentos de vida de los seres humanos, que debe continuar a través de la formación desde educación inicial hasta más allá de la universidad. En el sistema educativo colombiano se tiene escaso conocimiento y se encuentra con limitadas acciones organizadas que conduzcan al desarrollo de esta habilidad investigativa. La presente investigación se concentra en recoger los elementos característicos de una experiencia de formación en investigación desarrollada con 40 estudiantes de los grados 6º a 11º y 5 docentes de una Institución Educativa de Sevilla Valle. La pregunta de investigación planteada es ¿Cuáles son las habilidades investigativas que desarrollan los estudiantes utilizando como estrategia las Ferias de la Ciencia y la construcción de proyectos en el área técnica? El objetivo propuesto a alcanzar consiste en identificar la incidencia en el desarrollo de habilidades investigativas que alcancen los estudiantes en las Ferias de la Ciencia y cómo la construcción de proyectos en el área técnica continúa fortaleciendo dicha formación. El enfoque investigativo es cualitativo con enfoque etnográfico puesto que los participantes tanto profesores como estudiantes aportan sus experiencias y reflexionan en torno a una problemática. Para el levantamiento de la información se construyen dos instrumentos convalidados con el juicio de 4 profesores con experiencia investigativa. Los aportes de esta investigación contribuyen a identificar aciertos y vacíos posibles de mejora para potenciar las habilidades investigativas en estudiantes de los niveles de básica y media. La fundamentación teórica se basa en: Maldonado, Retana y Rivas.
FORMULATION, AND CHARACTERIZATION OF NANOSTRUCTURED LIPID CARRIER (NLC) CONTAINING QUERCETIN
Authors: Rahayu Asti , Putri Astrid Kusuma , Ambarwati Nadya , Sari Fithri Farchah Frischah , Putra Rizky Anugrah Dirgantara 
Published: November 2023

Quercetin, like triterpenoids, decreases blood glucose levels. Quercetin has several limitations including low solubility, low percutaneous permeability, and low bioavailability. The formulation of quercetin preparations in a Nanostructured Lipid Carrier (NLC) system is one solution to increase its solubility. The quercetin NLC system was successfully formulated by the high shear homogenization method at a speed of 6000 rpm. The solid lipid glyceryl monostearate and sunflower oil play important roles in the formation of NLC. The physicochemical characteristics examined in this study included the particle size, dispersion, viscosity, pH, and entrapment efficiency. The particle size of NLC quercetin ranges from 22.98 ± 0.008 nm to 41.04 ± 0.082 nm, with p-values < 0.05. The dispersion power of quercetin NLC ranges from 5.12 ± 0.11 cm to 7.01 ± 0.28 cm, p values < 0.05. The resulting pH range is 7.3 ± 0.01 to 7.4 ± 0.01, and the resulting viscosity is 223.7 ± 9.8 cps to 492.0 ± 0.0 cps. Entrapment efficiency range of (62.20 ± 0.245)% to (86.17 ± 0.287)% ( p < 0.05). The ratio of solid lipid concentration to liquid lipid concentration in NLC quercetin has a significant effect on particle size, dispersion, and entrapment efficiency.
Keywords: Nanostructured Lipid Carrier, Quercetin, Lipid, Glyceryl Monosterate, Sunflower Oil
A Lithium Depletion Age for the Carina Association
Authors: Wood Mackenna L. , Mann Andrew W. , Barber Madyson G. , Bush Jonathan L. , Milburn Reilly P. , Thao Pa Chia , Schmidt Stephen P. , Tofflemire Benjamin M. , Kraus Adam L. 
Published: November 2023

Abstract
The dispersed remnants of stellar nurseries, stellar associations, provide unparalleled samples of coeval stars critical for studies of stellar and planetary formation and evolution. The Carina Stellar Association is one of the closest stellar associations to Earth, and yet measurements of its age have varied from 13 to 45 Myr. We aim to update the age of Carina using the lithium depletion boundary (LDB) method. We obtain new measurements of the Li 6708 Å absorption feature in likely members using optical spectra from the Goodman High Throughput Spectrograph on SOAR and NRES on LCO. We detect the depletion boundary at M

K
≃ 6.8 (M5). This age is consistent within uncertainties across six different models, including those that account for magnetic fields and spots. We also estimate the age through analysis of the group’s overall variability, and by comparing the association members’ color–magnitude diagram to stellar evolutionary models using a Gaussian Mixture Model, recovering ages consistent with the LDB. Combining these age measures we obtain an age for the Carina association of

41

−
5

+
3

Myr. The resulting age agrees with the older end of previous age measurements and is consistent with the lithium depletion age for the neighboring Tucana-Horologium moving group.
Early Planet Formation in Embedded Disks (eDisk). XII. Accretion Streamers, Protoplanetary Disk, and Outflow in the Class I Source Oph IRS 63
Authors: Flores Christian , Ohashi Nagayoshi , Tobin John J. , Jørgensen Jes K. , Takakuwa Shigehisa , Li Zhi-Yun , Lin Zhe-Yu Daniel , van ’t Hoff Merel L. R. , Plunkett Adele L. , Yamato Yoshihide , Sai (Insa Choi) Jinshi , Koch Patrick M. , Yen Hsi-Wei , Aikawa Yuri , Aso Yusuke , de Gregorio-Monsalvo Itziar , Kido Miyu , Kwon Woojin , Lee Jeong-Eun , Lee Chang Won , Looney Leslie W. , Santamaría-Miranda Alejandro , Sharma Rajeeb , Thieme Travis J. , Williams Jonathan P. , Han Ilseung , Narayanan Suchitra , Lai Shih-Ping 
Published: November 2023

Abstract
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the Class I source Oph IRS 63 in the context of the Early Planet Formation in Embedded Disks large program. Our ALMA observations of Oph IRS 63 show a myriad of protostellar features, such as a shell-like bipolar outflow (in 12CO), an extended rotating envelope structure (in 13CO), a streamer connecting the envelope to the disk (in C18O), and several small-scale spiral structures seen toward the edge of the dust continuum (in SO). By analyzing the velocity pattern of 13CO and C18O, we measure a protostellar mass of M
⋆ = 0.5 ± 0.2 M
⊙ and confirm the presence of a disk rotating at almost Keplerian velocity that extends up to ∼260 au. These calculations also show that the gaseous disk is about four times larger than the dust disk, which could indicate dust evolution and radial drift. Furthermore, we model the C18O streamer and SO spiral structures as features originating from an infalling rotating structure that continuously feeds the young protostellar disk. We compute an envelope-to-disk mass infall rate of ∼10−6
M
⊙ yr−1 and compare it to the disk-to-star mass accretion rate of ∼10−8
M
⊙ yr−1, from which we infer that the protostellar disk is in a mass buildup phase. At the current mass infall rate, we speculate that soon the disk will become too massive to be gravitationally stable.
Revisiting Galaxy Evolution in Morphology in the Cosmic Evolution Survey Field (COSMOS-ReGEM). I. Merging Galaxies
Authors: Ren Jian , Li Nan , Liu F. S. , Cui Qifan , Fu Mingxiang , Zheng Xian Zhong 
Published: November 2023

Abstract
We revisit the evolution of galaxy morphology in the Cosmic Evolution Survey field over the redshift range 0.2 ≤ z ≤ 1, using a large and complete sample of 33,605 galaxies with a stellar mass of log(M
*/M
⊙) > 9.5 with significantly improved redshifts and comprehensive nonparametric morphological parameters. Our sample has 13,881 (∼41.3%) galaxies with reliable spectroscopic redshifts and more accurate photometric redshifts with a σ
NMAD ∼ 0.005. This paper is the first in a series that investigates merging galaxies and their properties. We identify 3594 major merging galaxies through visual inspection and find 1737 massive galaxy pairs with log(M
*/M
⊙) >10.1. Among the family of nonparametric morphological parameters including C, A, S, Gini, M
20, A
O, and D
O, we find that the outer asymmetry parameter A
O and the second-order momentum parameter M
20 are the best tracers of merging features compared to other combinations. Hence, we propose a criterion for selecting candidates of violently star-forming mergers: M
20 > − 3A
O + 3 at 0.2 < z < 0.6 and M
20 > − 6A
O + 3.7 at 0.6 < z < 1.0. Furthermore, we show that both the visual merger sample and the pair sample exhibit a similar evolution in the merger rate at z < 1, with

R
∼

(
1
+
z
)

1.79
±
0.13

for the visual merger sample and

R
∼

(
1
+
z
)

2.02
±
0.42

for the pair sample. The visual merger sample has a specific star formation rate that is about 0.16 dex higher than that of nonmerger galaxies, whereas no significant star formation excess is observed in the pair sample. This suggests that the effects of mergers on star formation differ at different merger stages.
Ejecta, Rings, and Dust in SN 1987A with JWST MIRI/MRS
Authors: Jones O. C. , Kavanagh P. J. , Barlow M. J. , Temim T. , Fransson C. , Larsson J. , Blommaert J. A. D. L. , Meixner M. , Lau R. M. , Sargent B. , Bouchet P. , Hjorth J. , Wright G. S. , Coulais A. , Fox O. D. , Gastaud R. , Glasse A. , Habel N. , Hirschauer A. S. , Jaspers J. , Krause O. , Lenkić L. , Nayak O. , Rest A. , Tikkanen T. , Wesson R. , Colina L. , van Dishoeck E. F. , Güdel M. , Henning Th. , Lagage P.-O. , Östlin G. , Ray T. P. , Vandenbussche B. 
Published: November 2023

Abstract
Supernova (SN) 1987A is the nearest supernova in ∼400 yr. Using the JWST MIRI Medium Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer rings in the mid-infrared 12,927 days (35.4 yr) after the explosion. The spectra are rich in line and dust continuum emission, both in the ejecta and the ring. The broad emission lines (280–380 km s−1 FWHM) that are seen from all singly-ionized species originate from the expanding ER, with properties consistent with dense post-shock cooling gas. Narrower emission lines (100–170 km s−1 FWHM) are seen from species originating from a more extended lower-density component whose high ionization may have been produced by shocks progressing through the ER or by the UV radiation pulse associated with the original supernova event. The asymmetric east–west dust emission in the ER has continued to fade, with constant temperature, signifying a reduction in dust mass. Small grains in the ER are preferentially destroyed, with larger grains from the progenitor surviving the transition from SN into SNR. The ER dust is fit with a single set of optical constants, eliminating the need for a secondary featureless hot dust component. We find several broad ejecta emission lines from [Ne ii], [Ar ii], [Fe ii], and [Ni ii]. With the exception of [Fe ii] 25.99 μm, these all originate from the ejecta close to the ring and are likely to be excited by X-rays from the interaction. The [Fe ii] 5.34 to 25.99 μm line ratio indicates a temperature of only a few hundred K in the inner core, which is consistent with being powered by 44 Ti decay.
CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Robbins Grady , Meisner Aaron M. , Schneider Adam C. , Burgasser Adam J. , Kirkpatrick J. Davy , Gagné Jonathan , Hsu Chih-Chun , Moranta Leslie , Casewell Sarah , Marocco Federico , Gerasimov Roman , Faherty Jacqueline K. , Kuchner Marc J. , Caselden Dan , Cushing Michael C. , Alejandro Sherelyn ,   The Backyard Worlds: Planet 9 Collaboration,   The Backyard Worlds: Cool Neighbors Collaboration
Published: November 2023

Abstract
Y dwarfs, the coolest known spectral class of brown dwarfs, overlap in mass and temperature with giant exoplanets, providing unique laboratories for studying low-temperature atmospheres. However, only a fraction of Y dwarf candidates have been spectroscopically confirmed. We present Keck/NIRES near-infrared spectroscopy of the nearby (d ≈ 6–8 pc) brown dwarf CWISE J105512.11+544328.3. Although its near-infrared spectrum aligns best with the Y0 standard in the J band, no standard matches well across the full YJHK wavelength range. The CWISE J105512.11+544328.3 NH3-H = 0.427 ± 0.0012 and CH4-J = 0.0385 ± 0.0007 absorption indices and absolute Spitzer [4.5] magnitude of 15.18 ± 0.22 are also indicative of an early-Y dwarf rather than a late-T dwarf. CWISE J105512.11+544328.3 additionally exhibits the bluest Spitzer [3.6]−[4.5] color among all spectroscopically confirmed Y dwarfs. Despite this anomalously blue Spitzer color given its low luminosity, CWISE J105512.11+544328.3 does not show other clear kinematic or spectral indications of low metallicity. Atmospheric model comparisons yield a log(g) ≤ 4.5 and T
eff ≈ 500 ± 150 K for this source. We classify CWISE J105512.11+544328.3 as a Y0 (pec) dwarf, adding to the remarkable diversity of the Y-type population. JWST spectroscopy would be crucial to understanding the origin of this Y dwarf’s unusual preference for low-gravity models and blue 3–5 μm color.
CAHA/PPAK Integral-field Spectroscopic Observations of M81. II. Testing Photoionization Models in a Spatially Resolved LINER
Authors: Li Zongnan , Li Zhiyuan , García-Benito Rubén , Jin Yifei 
Published: November 2023

Abstract
The origin of the low-ionization nuclear emission-line region (LINER) prevalent in local galaxies and its relationship with supermassive black holes have been debated for decades. We perform a comprehensive evaluation of traditional photoionization models against the circumnuclear ionized gas in M81, for which recent CAHA/PPAK integral-field spectroscopic observations reveal a LINER characteristic out to a galactocentric radius of ∼1 kpc. Constructed with the photoionization code cloudy, the models have the novel aspect of their primary parameters being well constrained by extensive observations of a prototypical low-luminosity active galactic nucleus (LLAGN) and an old stellar bulge in M81. Additionally, these models incorporate a reasonably broad range of uncertain nebular properties. It is found that the integrated photoionization by the LLAGN and hot, low-mass stars distributed in the bulge can roughly reproduce the observed radial intensity distributions of the Hα, Hβ, and [N ii] lines, with the bulge stars dominating the ionizing flux at radii ≳200 pc. However, the models generally fail to reproduce a similarly declining profile of the [O iii] line or an accordingly flat profile of the [O iii]/Hβ ratio. This clearly points to a deficiency of ionizing photons in the outer regions despite an extended photoionization source. The discrepancy might be alleviated if much of the observed [O iii] line arose from a bulge-filling, low-density gas surrounding a denser, Hα-emitting disk, or by a higher AGN luminosity in the recent past. The case of M81 has important implications for the ionization mechanism of LINERs and low-ionization emission-line regions in general.
Constraining the AGN Luminosity Function from JWST with the X-Ray Background
Authors: Padmanabhan Hamsa , Loeb Abraham 
Published: November 2023

Abstract
We predict the X-ray background (XRB) expected from the population of quasars detected by the James Webb Space Telescope spectroscopic surveys over the redshift range z ∼ 4–7. We find that the measured UV emissivities imply a ∼10 times higher unresolved XRB than constrained by current experiments. We illustrate the difficulty of simultaneously matching the faint end of the quasar luminosity function and the XRB constraints. We discuss possible origins and consequences of this discrepancy.
Quelle science pour quel socialisme ? Pratiques et représentations de la science dans le socialisme européen
Authors: Prochasson Christophe 
Published: November 2023

Les études ayant mis en évidence les liens qu’ont entretenus science et socialisme ne se comptent plus. On rouvre ici le dossier en mettant en avant trois configurations qui guidèrent cette rencontre. Sans réduire l’histoire des rapports entre science et socialisme à une succession d’étapes, chacune marquée par des formes différentes de lucidité scientifique, il est possible de distinguer trois paradigmes : le premier appartient à la sphère physico-mathématique, le deuxième est attaché aux sciences naturelles, le troisième se confond presque avec la sociologie.