bluuebunny/crossref_metadata_2025_split huggingface dataset:
Optimalisasi Pengelolaan Usaha Bagi Pelaku UMKM Ikan Asin Bu Kaya Di Lingkungan VIII Kelurahan Belawan Bahari Kecamatan Medan Belawan
Authors: Hasugian Christnova , Sinurat Mangasa , Siallagan Hamonangan 
Published: July 2024

Kegiatan PKM ini dilaksanakan telah berlangsung dengan baik untuk mewujudkan peran perguruan tinggi dalam memberi pemikiran serta memotivasi masyarakat pengusaha ikan asin di Lingkungan VIII Kelurahan Belawan Bahari, Kecamatan Medan Belawan. Keberadaan pengusaha UMKM ikan asin di Kelurahan Belawan Bahari telah memiliki peran penting dalam mensuplai ikan asin sesuai kebutuhan masyarakat di Kecamatan Medan Belawan, bahkan sampai ke kota Medan dan kota lainnya. Akan tetapi para pengusaha belum mampu mengoptimalkan pengelolaan usaha baik dari segi; pemasaran digital, keterampilan Sumber Daya Manusia, kemampuan penyusunan laporan keuangan, dan pemahaman pemenuhan aturan hukum dalam mendukung legalitas berusaha Untuk menjalankan bisnis dengan sukses dan menghindari masalah keuangan di masa mendatang, perencanaan awal sangat penting untuk pengelolaan keuangan. Kegiatan pengabdian masyarakat melalui pelatihan ini telah menghapus perspektif dan pengetahuan sebelumnya yang menganggap penyusunan laporan keuangan tidak terlalu perlu dan tidak bermanfaat. Kegiatan PKM ini bertujuan untuk meningkatkan pengetahuan, pemahaman pengusaha, mengenai pengelolaan usaha ikan asin Bu Kaya Membantu proses pencatatan transaksi keuangan (pembukuan) secara sederhana. Menguraikan aspek hukum berkaitan dengan perijinan usaha, perlindungan konsumen, dan Hak Atas Kekayaan Intelektual (HAKI).
ИНТЕГРАЦИОННЫЙ ПОТЕНЦИАЛ ВУЗОВ И ИХ КООПЕРАЦИЯ С ОРГАНИЗАЦИЯМИ
Authors: Александрова Елена Васильевна , Иншаков Андрей Алексеевич 
Published: July 2024

Наращивание интеграционного потенциала ВУЗов в целях реализации совместных проектов в образовательной, научной, инновационной сферах становится одним из основных трендов развития высшего образования. Цель работы -проведение исследований, связанных с интеграцией научных, образовательных учреждений и их кооперацией с организациями реального сектора экономики. В статье использованы материалы публикаций, диссертаций, монографий ведущих ученых России.
Building up the integration potential of universities in order to implement joint projects in the educational, scientific, and innovative spheres is becoming one of the main trends in the development of higher education. The purpose of the work is to conduct research related to the integration of scientific and educational institutions and their cooperation with organizations of the real sector of the economy. The article uses materials from publications, dissertations, monographs of leading scientists of Russia.
Conocer las Experiencias en Cuidados Domiciliarios por Estudiantes de Enfermería
Authors: García Rodríguez Isaúl , Espinosa de los Monteros Melisa Islas , Escamilla Huerta Jocelyn Elizabeth , López Torres Ana Fabiola 
Published: July 2024

Introducción: Desde el año 2000, se ha trabajado en mejorar la calidad de la atención domiciliaria, con el propósito de elevar los estándares de los cuidados proporcionados por enfermera(o)s y estudiantes de enfermería. En la actualidad, el cuidado domiciliario impartido por estudiantes de enfermería carece de información, no obstante, se ha identificado que estos inician sus actividades laborales, aun estando en el desarrollo de sus estudios profesionales, principalmente por necesidad económica. Objetivo: Conocer las experiencias de los estudiantes de la Facultad de Enfermería de la Universidad Autónoma de Querétaro en el cuidado domiciliario. Metodología: Estudio transversal prospectivo de enfoque cualitativo, alcance descriptivo y diseño fenomenológico; donde se trabajará con estudiantes de segundo a octavo semestre. Se aplicará una entrevista a 10 sujetos, ya que el tipo de muestreo será no probabilístico a conveniencia. Se excluirán a aquellos que estén cursando primer semestre, servicio social y de posgrado. El consentimiento informado será parte de la ética del estudio. Resultados y Discusión. Conclusiones. Las experiencias son variables, puesto que, a pesar de los participantes brindan este tipo de cuidados, atraviesan por distintos desafíos que influyen en su percepción de la experiencia.
Radio Astrometry at Different Frequencies
Authors: Petrov Leonid 
Published: July 2024

Abstract
The very long baseline interferometry technique allows us to determine the positions of thousands of radio sources using the absolute astrometry approach. I have investigated the impacts of a selection of observing frequencies in a range from 2 to 43 GHz in single-band, dual-band, and quad-band observing modes on astrometric results. I processed seven data sets in a range of 72,000 to 6.9 million observations, estimated source positions, and compared them. I found that source positions derived from dual-band, quad-band, and 23.6 GHz single-band data agree at a level below 0.2 mas. Comparison of independent data sets allowed me to assess the error levels of individual catalogs: 0.05–0.07 mas per position component. Further comparison showed that individual catalogs have systematic errors at the same level. The positions from 23.6 GHz single-band data show systematic errors related to the residual ionosphere contribution. Analysis of source position differences revealed systematic errors along jet directions at a level of 0.09 mas. Network-related systematic errors affect all the data, regardless of frequency. Comparison of position estimates allowed me to derive the stochastic error model that closes the error budget. Based on the collected evidence, I have made a conclusion that the development of frequency-dependent reference frames of the entire sky is not warranted. In most cases dual-band, quad-band, and single-band data at a frequency of 22 GHz and higher can be used interchangeably, which allows us to exploit the strength of a specific frequency setup for given objects. Mixing observations at different frequencies causes errors not exceeding 0.07 mas.
The Web Epoch of Reionization Lyα Survey (WERLS). I. MOSFIRE Spectroscopy of z ∼ 7–8 Lyα Emitters*
Authors: Cooper Olivia R. , Casey Caitlin M. , Akins Hollis B. , Magee Jake , Melendez Alfonso , Fong Mia , Urbano Stawinski Stephanie M. , Kartaltepe Jeyhan S. , Finkelstein Steven L. , Larson Rebecca L. , Jung Intae , Bista Ash , Champagne Jaclyn B. , Chávez Ortiz Óscar A. , Coffin Sadie , Cooper M. C. , Drakos Nicole , Faisst Andreas L. , Franco Maximilien , Fujimoto Seiji , Gillman Steven , Gozaliasl Ghassem , Harish Santosh , Hutchison Taylor A. , Koekemoer Anton M. , Kokorev Vasily , Lertprasertpong Jitrapon , Liu Daizhong , Long Arianna S. , Papovich Casey , Rich R. Michael , Robertson Brant E. , Talia Margherita , Vanderhoof Brittany N. , Weaver John R. , Whitaker Katherine E. , Zavala Jorge A. 
Published: July 2024

Abstract
We present the first results from the Web Epoch of Reionization Lyα Survey (WERLS), a spectroscopic survey of Lyα emission using Keck I/MOSFIRE and LRIS. WERLS targets bright (J < 26) galaxy candidates with photometric redshifts of 5.5 ≲ z ≲ 8 selected from pre-JWST imaging embedded in the Epoch of Reionization (EoR) within three JWST deep fields: CEERS, PRIMER, and COSMOS-Web. Here, we report 11 z ∼ 7–8 Lyα emitters (LAEs; three secure and eight tentative candidates) detected in the first five nights of WERLS MOSFIRE data. We estimate our observed LAE yield is ∼13%, which is broadly consistent with expectations assuming some loss from redshift uncertainty, contamination from sky OH lines, and that the Universe is approximately half-ionized at this epoch, whereby observable Lyα emission is unlikely for galaxies embedded in a neutral intergalactic medium. Our targets are selected to be UV-bright, and span a range of absolute UV magnitudes with −23.1 < M
UV < −19.8. With two LAEs detected at z = 7.68, we also consider the possibility of an ionized bubble at this redshift. Future synergistic Keck+JWST efforts will provide a powerful tool for pinpointing beacons of reionization and mapping the large-scale distribution of mass relative to the ionization state of the Universe.
Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS
Authors: Long Arianna S. , Antwi-Danso Jacqueline , Lambrides Erini L. , Lovell Christopher C. , de la Vega Alexander , Valentino Francesco , Zavala Jorge A. , Casey Caitlin M. , Wilkins Stephen M. , Yung L. Y. Aaron , Arrabal Haro Pablo , Bagley Micaela B. , Bisigello Laura , Chworowsky Katherine , Cooper M. C. , Cooper Olivia R. , Cooray Asantha R. , Croton Darren , Dickinson Mark , Finkelstein Steven L. , Franco Maximilien , Gould Katriona M. L. , Hirschmann Michaela , Hutchison Taylor A. , Kartaltepe Jeyhan S. , Kocevski Dale D. , Koekemoer Anton M. , Lucas Ray A. , McKinney Jed , Nere Rachel , Papovich Casey , Pérez-González Pablo G. , Pirzkal Nor , Santini Paola 
Published: July 2024

Abstract
Substantial populations of massive quiescent galaxies at z ≥ 3 challenge our understanding of rapid galaxy growth and quenching over short timescales. In order to piece together this evolutionary puzzle, more statistical samples of these objects are required. Established techniques for identifying massive quiescent galaxies are increasingly inefficient and unconstrained at z > 3. As a result, studies report that as much as 70% of quiescent galaxies at z > 3 may be missed from existing surveys. In this work, we propose a new empirical color selection technique designed to select massive quiescent galaxies at 3 ≲ z ≲ 6 using JWST NIRCam imaging data. We use empirically constrained galaxy spectral energy distribution (SED) templates to define a region in the F277W − F444W versus F150W − F277W color plane that captures quiescent galaxies at z > 3. We apply these color selection criteria to the Cosmic Evolution Early Release Science (CEERS) Survey and use SED fitting on sources in the region to identify 44 candidate z ≳ 3 quiescent galaxies. Over half of these sources are newly discovered and, on average, exhibit specific star formation rates of poststarburst galaxies. Most of these sources would not be discovered using canonical UVJ diagrams. We derive volume density estimates of n ∼ 1–4 × 10−5 Mpc−3 at 3 < z < 5, finding excellent agreement with existing reports on similar populations in the CEERS field. Thanks to NIRCam’s wavelength coverage and sensitivity, this technique provides an efficient tool to search for large samples of these rare galaxies.
A Hot Core in the Group-dominant Elliptical Galaxy NGC 777
Authors: O’Sullivan Ewan , Rajpurohit Kamlesh , Schellenberger Gerrit , Vrtilek Jan , David Laurence P. , Babul Arif , Olivares Valeria , Ubertosi Francesco , Kolokythas Konstantinos , Babyk Iurii , Loubser Ilani 
Published: July 2024

Abstract
NGC 777 provides an example of a phenomenon observed in some group-central ellipticals, in which the temperature profile shows a central peak, despite the short central cooling time of the intragroup medium. We use deep Chandra X-ray observations of the galaxy, supported by uGMRT 400 MHz radio imaging, to investigate the origin of this hot core. We confirm the centrally peaked temperature profile and find that the entropy and cooling time both monotonically decline to low values (2.62

−
0.18

+
0.19

keV cm2 and

71.3

−
13.1

+
12.8

Myr, respectively) in the central ∼700 pc. Faint diffuse radio emission surrounds the nuclear point source, with no clear jets or lobes but extending to ∼10 kpc on the northwest–southeast axis. This alignment and extent agree well with a previously identified filamentary Hα + [N ii] nebula. While cavities are not firmly detected, we see X-ray surface brightness decrements on the same axis at 10–20 kpc radii, which are consistent with the intragroup medium having been pushed aside by expanding radio lobes. Any such outburst must have occurred long enough ago for lobe emission to have faded below detectability. Cavities on this scale would be capable of balancing radiative cooling for at least ∼240 Myr. We consider possible causes of the centrally peaked temperature profile, including gravitational heating of gas as the halo relaxes after a period of active galactic nucleus jet activity, and heating by particles leaking from the remnant relativistic plasma of the old radio jets.
Age of Massive Galaxies at Redshift 8
Authors: López-Corredoira M. , Melia F. , Wei J.-J. , Gao C.-Y. 
Published: July 2024

Abstract
Recent James Webb Space Telescope data analyses have shown that massive red galaxies existed at redshifts z ≳ 6, a discovery that is difficult to understand in the context of standard cosmology (ΛCDM). Here, we analyze these observations more deeply, by fitting a stellar population model to the optical and near-infrared photometric data. These fits include a main stellar population in addition to a residual younger population and with the same extinction for both (a lower extinction for the younger population is unphysical). Extra stellar populations or the inclusion of an active galactic nucleus component do not significantly improve the fits. These galaxies are being viewed at very high redshifts, with an average 〈z〉 ≈ 8.2, when the ΛCDM Universe was only ≈600 Myr old. This result conflicts with the inferred ages of these galaxies, however, which were on average between 0.9 and 2.4 Gyr old within a 95% confidence level. Given the sequence of star formation and galaxy assembly in the standard model, these galaxies should instead be even younger than 290 Myr on average, for which our analysis assigns a probability of only <3 × 10−4 (≳3.6σ tension). This outcome may indicate the need to consider nonstandard cosmologies. Nevertheless, our conclusions result from several approximations in stellar astrophysics and extinction, so they should be taken with a grain of salt. Further research is necessary to corroborate the possible existence of galaxies older than the ΛCDM Universe at their observed redshifts.
Atmospheric Waves Driving Variability and Cloud Modulation on a Planetary-mass Object
Authors: Plummer Michael K. , Wang 王 Ji 吉 , Artigau Étienne , Doyon René , Suárez Genaro 
Published: July 2024

Abstract
Planetary-mass objects and brown dwarfs at the transition (T
eff ∼ 1300 K) from relatively red L dwarfs to bluer mid-T dwarfs show enhanced spectrophotometric variability. Multiepoch observations support atmospheric planetary-scale (Kelvin or Rossby) waves as the primary source of this variability; however, large spots associated with the precipitation of silicate and metal clouds have also been theorized and suggested by Doppler imaging. We applied both wave and spotted models to fit near-infrared (NIR), multiband (Y/J/H/K) photometry of SIMP J013656.5+093347 (hereafter SIMP0136) collected at the Canada–France–Hawaii Telescope using the Wide-field InfraRed Camera. SIMP0136 is a planetary-mass object (12.7 ± 1.0 M
J) at the L/T transition (T2 ± 0.5) known to exhibit light-curve evolution over multiple rotational periods. We measure the maximum peak-to-peak variability of 6.17% ± 0.46%, 6.45% ± 0.33%, 6.51% ± 0.42%, and 4.33% ± 0.38% in the Y, J, H, and K bands, respectively, and find evidence that wave models are preferred for all four NIR bands. Furthermore, we determine that the spot size necessary to reproduce the observed variations is larger than the Rossby deformation radius and Rhines scale, which is unphysical. Through the correlation between light curves produced by the waves and associated color variability, we find evidence of planetary-scale, wave-induced cloud modulation and breakup, similar to Jupiter’s atmosphere and supported by general circulation models. We also detect a 93.°8 ± 7.°4 (12.7σ) phase shift between the H − K and J − H color time series, providing evidence for complex vertical cloud structure in SIMP0136's atmosphere.
CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI
Authors: Ronayne Kaila , Papovich Casey , Yang Guang , Shen Lu , Dickinson Mark , Kennicutt Robert , Alavi Anahita , Arrabal Haro Pablo , Bagley Micaela B. , Burgarella Denis , Le Bail Aurélien , Bell Eric F. , Cleri Nikko J. , Cole Justin , Costantin Luca , de la Vega Alexander , Daddi Emanuele , Elbaz David , Finkelstein Steven L. , Grogin Norman A. , Holwerda Benne W. , Kartaltepe Jeyhan S. , Kirkpatrick Allison , Koekemoer Anton M. , Lucas Ray A. , Magnelli Benjamin , Mobasher Bahram , Pérez-González Pablo G. , Prichard Laura , Rafelski Marc , Rodighiero Giulia , Sunnquist Ben , Teplitz Harry I. , Wang Xin , Windhorst Rogier A. , Yung L. Y. Aaron 
Published: July 2024

Abstract
We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 μm polycyclic aromatic hydrocarbon luminosities from the integrated emission of galaxies at z ∼ 0–2. We utilize multiband photometry covering 0.2–160 μm from the Hubble Space Telescope, CFHT, JWST, Spitzer, and Herschel for galaxies in the Cosmic Evolution Early Release Science (CEERS) Survey. We perform spectral energy distribution (SED) modeling of these data to measure dust-corrected far-UV (FUV) luminosities, L
FUV, and UV-derived SFRs. We then fit SED models to the JWST/MIRI 7.7–21 μm CEERS data to derive rest-frame 7.7 μm luminosities, L
770, using the average flux density in the rest-frame MIRI F770W bandpass. We observe a correlation between L
770 and L
FUV, where

log

L

770

∝
(
1.27
±
0.04
)
log

L

FUV

. L
770 diverges from this relation for galaxies at lower metallicities, lower dust obscuration, and for galaxies dominated by evolved stellar populations. We derive a “single-wavelength” SFR calibration for L
770 that has a scatter from model estimated SFRs (σ
ΔSFR) of 0.24 dex. We derive a “multiwavelength” calibration for the linear combination of the observed FUV luminosity (uncorrected for dust) and the rest-frame 7.7 μm luminosity, which has a scatter of σ
ΔSFR = 0.21 dex. The relatively small decrease in σ suggests this is near the systematic accuracy of the total SFRs using either calibration. These results demonstrate that the rest-frame 7.7 μm emission constrained by JWST/MIRI is a tracer of the SFR for distant galaxies to this accuracy, provided the galaxies are dominated by star formation with moderate-to-high levels of attenuation and metallicity.
« As you like it » : les noms d’assonance lyciens‑grecs
Authors: Réveilhac Florian 
Published: July 2024

En Lycie, zone de contacts linguistiques entre lycien et grec notamment, les anthroponymes indigènes ont fait l’objet de différentes stratégies d’adaptation de la langue source à la langue cible : emprunt proprement dit, emprunt assimilé, calque et nom d’assonance. À la suite de travaux fondateurs menés dans d’autres zones de contacts du monde gréco-romain, cette contribution examine la question des noms d’assonance lyciens-grecs, c’est‑à‑dire pouvant recevoir une interprétation à la fois en lycien et en grec. Dans un premier temps, il s’agit d’établir des critères d’identification pour ces anthroponymes en tenant compte des spécificités de l’aire lycienne. Nous proprosons, ensuite, à travers l’étude de cas précis, une typologie des noms d’assonance lyciens-grecs qui prend en considération à la fois le point de vue de la langue source et celui de la langue cible.
Une isoglosse des dialectes doriens du sud‑est de la mer Égée
Authors: Nieto Izquierdo Enrique 
Published: July 2024

La finale ‑εια, issue de l’adjonction du suffixe *‑ja (gén. *‑jās), se retrouve dans le second élément de certains composés anthroponymiques au féminin, notamment dans des racines en sifflante, tant nominales (Ξενοκράτ‑εια, de κράτος) que d’origine verbale (Δαμοκρίν‑εια, de κρίνω). En dehors de ces catégories, il y a des exemples, caractéristiques des dialectes doriens de la mer Égée (Théra, Anaphè, Cos, Rhodes, Astypalée, etc.), où le suffixe ‑εια (‑εα après perte de yod secondaire intervocalique, contracté ultérieurement en ‑η) semble s’être étendu de manière inattendue à d’autres féminins comme Ξειναγορεια (← ‑αγόρα), Ἰσανορεια, Τιμανορη (← ‑άνειρα, ‑άνδρα), Ἀναξιλεα (← ‑λάϝα), Πεισιροδεα, Φιλοροδη (← ‑ρόδα), etc. Après avoir écarté d’autres explications, y compris la prétendue origine ionienne de la finale ‑η, l’auteur arrive à la conclusion que ces formes en ‑ε(ι)α (> ‑η) remontent en dernier lieu au suffixe patronymique et ctétique ‑εία (masc. ‑ειος) qu’on trouve souvent dans les noms de patrai, abondamment attestés dans les îles doriennes : Εὐωνακτίδειοι (← Εὐωνακτίδας), Λυκώνειοι (← Λύκων), etc. Les féminins en ‑εία auraient alors une accentuation de paroxyton (Ξειναγορεία, Πεισιροδέα) et leur avatar contracté en ‑ῆ, à l’accent périspomène (Φιλοροδῆ), les distinguerait des formes de féminin en ‑η (< ‑ᾱ) ioniennes et/ou de koinè.
E pluribus unum
Authors: Alonso Déniz Alcorac 
Published: July 2024

Cette contribution examine certaines données linguistiques qui pourraient constituer des preuves de variation dans la carte dialectale de la Crète au Ιer millénaire. La distribution de certaines isoglosses dans les inscriptions dès la seconde moitié du viie s. jusqu’à ca 400 av. J.‑C. contredit, au moins partiellement, l’impression d’une carte dialectale monolithique de la Crète. Dans la partie occidentale, à la suite de la colonisation des Éginètes, Kydonia et d’autres localités de la côte nord présentent des spécificités doriennes qui les écartent linguistiquement de la Crète centrale. Par ailleurs, à côté de certaines isoglosses communes à toutes les cités de la Crète centrale, le dorien des inscriptions archaïques de cette région est loin d’être monolithique, comme le montre la distribution de quelques caractéristiques phonologiques, morphologiques, syntaxiques et lexicales.
Lire, écrire, soigner. La circulation des remèdes dans une communauté religieuse urbaine (Rome, xvie-xviie siècles)
Authors: Tomassetti Stefano 
Published: July 2024

L’article analyse un recueil manuscrit de recettes médicinales (env. 1590-1643) et met en lumière son contexte de production et d’usage : l’oratoire de Santa Maria in Vallicella à Rome. Ce livre est à la fois un texte, un outil de lecture et un bloc-notes. Son analyse matérielle témoigne des façons dont il a été produit, en révélant l’utilisation de sources manuscrites et de livres imprimés conservés dans la bibliothèque oratorienne, et un mélange de pratiques d’écriture et lecture. L’article met aussi en évidence le rôle des parcours informels et oraux dans la diffusion du savoir médical à la Vallicella, en soulignant également la façon dont les soins y étaient pratiqués, que ce soit par des soignants professionnels ou à travers le partage de savoirs et de savoir-faire thérapeutiques entre les prêtres oratoriens. Le but est d’estimer la contribution de ces derniers à la formation du recueil et, finalement, de montrer que la compilation de recettes était une composante d’un plus vaste processus de circulation des connaissances médicales, qu’il convient d’inscrire dans un milieu social et culturel spécifique.
L’enseignement laïque des faits religieux peut-il contribuer à la formation politique ?
Authors: Husser Anne-Claire 
Published: July 2024

S’il est fréquent de mettre en avant la contribution d’une meilleure connaissance des religions au « vivre ensemble » au sens où celle-ci favoriserait la tolérance, l’apport de l’enseignement des faits religieux à la formation politique proprement dite est plus rarement exploré. Le principe de neutralité religieuse s’applique à l’institution et non aux publics qu’elle accueille, mais l’exercice de la citoyenneté ne s’en inscrit pas moins dans l’horizon d’une vision laïque du débat public et de la délibération. Dans ces conditions, les points de vue religieux semblent par avance disqualifiés en tant qu’emprunts d’une indépassable particularité. Moyennant souvent un certain effort de traduction en langage séculier, ces derniers participent pourtant à la vie politique réelle à l’instar d’autres groupes convictionnels ou groupes d’intérêts. Ignorer cette composante politique des faits religieux ou cette composante religieuse du débat public, n’est-ce pas exposer l’éducation scolaire à la citoyenneté à une forme d’abstraction idéaliste ?