bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kommemorativinschrift anlässlich der Stiftung von Opferfesten und Weihgaben durch einen Familienverband im Heiligtum von Dabla
Authors: STAAB Gregor , AKYÜREK ŞAHİN Nalan Eda , UZUNOĞLU Hüseyin 
Published: October 2023

This article is a continuation of the article published in the previous issue of Gephyra (Staab - Akyürek Şahin - Uzunoğlu 2023). The article analyses an inscription from the village of Ahmetler in the Pazaryeri district of Bilecik province, which was recorded by the Bilecik Museum authorities. The stone is not in the Bilecik Museum today but is probably still in the wall where it was built. The inscription was read from the photograph taken by the museum authorities, but the stone itself was not seen. The inscription is an epigram written in hexameter verse. The first two lines of the epigram are missing and probably remained under the cement on the wall. However, the rest of the lines are almost complete except line 1, which is poorly preserved. Since the stone was built into a wall, it is not clear whether the inscription carrier was an altar or a stele.
The person named Onesikrates, mentioned in lines 3 and 4 of the inscription, played an important role in this inscription. This person is the uncle of Hermias, the young Onesikrates and Ulpianus. It is understood that the uncle Onesikrates was the head of the family group mentioned in the poem. It is not known whether he took over the care of his nephews after the death of their father and whether they therefore all belonged to the same household. In any case, here as elsewhere, third-degree kinship reflects close family ties, especially in rural social structures. The uncle Onesicrates, who was also a soldier, appears as a central figure, and all the nephews mentioned are included in his oath or prayer. In line 4, the addressee, addressed in the second person (σύ θ᾿), must be the (local?) deity of the (local?) sanctuary of Dabla, to whom the wish to bestow property on the named individuals is expressed. It is known from the inscriptions that Zeus Bennios or Zeus Bronton was worshipped in this region. This inscription may have been erected in the sanctuary of one of these two gods. The article analyses the phrase Δαβλόνῳ παρὰ νηῷ in line 9 of the inscription and suggests that the name of the settlement may be Dabla. The inscription poetically describes the full financing of the three sacrificial feasts. The poem itself is thus identified as an expression of this praise for the donors.
Automatic imitation of speech is enhanced for non-native sounds
Authors: Wilt Hannah , Wu Yuchunzi , Evans Bronwen G. , Adank Patti 
Published: October 2023

AbstractSimulation accounts of speech perception posit that speech is covertly imitated to support perception in a top-down manner. Behaviourally, covert imitation is measured through the stimulus-response compatibility (SRC) task. In each trial of a speech SRC task, participants produce a target speech sound whilst perceiving a speech distractor that either matches the target (compatible condition) or does not (incompatible condition). The degree to which the distractor is covertly imitated is captured by the automatic imitation effect, computed as the difference in response times (RTs) between compatible and incompatible trials. Simulation accounts disagree on whether covert imitation is enhanced when speech perception is challenging or instead when the speech signal is most familiar to the speaker. To test these accounts, we conducted three experiments in which participants completed SRC tasks with native and non-native sounds. Experiment 1 uncovered larger automatic imitation effects in an SRC task with non-native sounds than with native sounds. Experiment 2 replicated the finding online, demonstrating its robustness and the applicability of speech SRC tasks online. Experiment 3 intermixed native and non-native sounds within a single SRC task to disentangle effects of perceiving non-native sounds from confounding effects of producing non-native speech actions. This last experiment confirmed that automatic imitation is enhanced for non-native speech distractors, supporting a compensatory function of covert imitation in speech perception. The experiment also uncovered a separate effect of producing non-native speech actions on enhancing automatic imitation effects.
Effects of Electromagnetic Field (1.8/0.9 GHz) Exposure on Spleen in Rats
Authors: KIZILOĞLU İlker , YILMAZ BOZOK Yeliz , TÜMKAYA Levent , AKAKIN Dilek , ŞENER AKÇORA Dila 
Published: October 2023

Aim: To evaluate potential effects of whole-body 900 and 1800 MHz electromagnetic field (EMF) exposure on the rat spleen.
Material and Methods: The study was conducted on 9 Sprague–Dawley rats. Pregnant rats were assigned into 3 groups: 900 MHz EMF-exposure, 1800 MHz EMF-exposure and controls.
Results: Under light microscope, myeloid series cells, erythrocytes and megakaryocytes were observed in all groups. In the red pulp, dilated sinusoids were observed in both 900 and 1800 prenatal 24-hour groups with more prominent findings in the 1800 prenatal 24-hour group. Fused white pulps were apparent in 900 group while there was increase in the irregular white pulps (varying in size) with destruction in the1800 group. Biochemical evaluation showed that spleenmalondialdehyde level was higher while glutathione level waslower in the 900 MHz-exposure and 1800 MHz-exposuregroups compared to controls (p
PKM Praktik Economy Digital Dan Participatory Approach Untuk Penguatan Kelembagaan Paguyuban Pedagang Pasar Seni Sukawati
Authors: DEWI Kadek Goldina Puteri Dewi , DEWI Anak Agung Istri Krisna Gangga , NURAK Anastacia Patricia Novlina 
Published: October 2023

Pemanfaatan teknologi dan digitalisasi dalam dunia ekonomi sangat menunjang dalam pemasaran suatu produk tak terlebih produk lokal. Pengembangan ekonomi digital ini juga didorong oleh adanya pergeseran perilaku masyarakat yang cenderung menggunakan platform digital di berbagai sektor. Pasar Seni Sukawati termasuk salah satu pasar seni tradisional di Bali, yang mendapat hibah dari pemerintah pusat untuk direvitalisasi menjadi Pasar Seni Modern. Perubahan pada Pasar Seni Sukawati (revitalisasi) menuntut para pedagang untuk terus berevolusi ke arah yang lebih baik. Hal ini menjadi permasalahan yang besar bagi pedagang pasar seni Sukawati karena membutuhkan proses adaptasi dari revitalisasi jumlah kunjungan dan pendapatan pedagang yang masih sedikit. Berdasarkan adanya beberapa permasalahan yang dihadapi mitra, maka kegiatan program kemitraan masyarakat ini memiliki tujuan untuk pemberdayaan paguyuban pedagang Pasar Seni Sukawati dengan digitalisasi ekonomi (economy digital) yaitu memberikan sosialisai dan pelatihan pembuatan laporan keuangan akuntansi yang terdigitalisasi, Menyusun dan mempraktikan strategi promosi yang terdigitalisasi, dan pendekatan partisipan (participatory approach) yakni kegiatan agar mampu mengenal, memahami, dan menangani permasalahan dalam penyelenggaraan organisasi.
Penerapan Pemotongan Tunjangan Kinerja Anggota Bid Tik Polda Bali Yang Ditentukan Dalam Kehadiran Jumlah Kerja
Authors: AMARTHA Made Putra Jaya , MARTINI I.A. Oka 
Published: October 2023

Tunjangan kinerja dapat menjadi salah satu faktor yang meningkatkan kedisiplinan karyawan di dalam kehadiran anggota BID TIK Polda Bali. Kinerja yang baik mencerminkan hasil pekerjaan yang optimal, sesuai dengan standar organisasi, dan secara keseluruhan mendukung tercapainya tujuan organisasi tersebut. Tujuan penelitian ini yaitu untuk mengetahui penerapan pemotongan tunjangan kinerja berdasar tingkat kehadiran jumlah kerja di BID TIK Polda Bali. Penelitian berupa observasi deskriptif dengan mengamati kehadiran dan tunjangan 65 anggota. Terdapat 65 anggota dengan persentase 78% dengan kehadiran penuh dan 22% tidak hadir satu hari per bulan Juni-Juli 2023. Tingkat kehadiran mempengaruhi tunjangan kinerja dengan kategori kelas jabatan sebagai berikut kelas 13 (Rp8,562,000); kelas 11 (Rp5,183,000); kelas 10 (Rp4,551,000); kelas 9 (Rp3,781,000); kelas 8 (Rp3,319,000); kelas 7 (Rp2,928,000) dan kelas 5 (Rp2,493,000). Berdasarkan kehadiran dan kelas jabatan terdapat 14 anggota mengalami pemotongan. Pemotongan izin dengan dikalikan 1% tunjangan. Dengan rincian 1 anggota kelas jabatan 7,9 dan 10, serta 11 anggota kelas jabatan 5. Total pengurangan sebesar Rp386.830 per Juni-Juli 2023. Saran berupa apel berkala dengan komunikasi kebijakan; penjelasan insentif dan konsekuensi; motivasi penguatan positif; edukasi pentingnya kehadiran; identifikasi hambatan kehadiran, penyuluhan kesehatan dan kesejahteraan.
ELemental abundances of Planets and brown dwarfs Imaged around Stars (ELPIS). I. Potential Metal Enrichment of the Exoplanet AF Lep b and a Novel Retrieval Approach for Cloudy Self-luminous Atmospheres
Authors: Zhang 张 Zhoujian 周健 , Mollière Paul , Hawkins Keith , Manea Catherine , Fortney Jonathan J. , Morley Caroline V. , Skemer Andrew , Marley Mark S. , Bowler Brendan P. , Carter Aarynn L. , Franson Kyle , Maas Zachary G. , Sneden Christopher 
Published: October 2023

Abstract
AF Lep A+b is a remarkable planetary system hosting a gas-giant planet that has the lowest dynamical mass among directly imaged exoplanets. We present an in-depth analysis of the atmospheric composition of the star and planet to probe the planet’s formation pathway. Based on new high-resolution spectroscopy of AF Lep A, we measure a uniform set of stellar parameters and elemental abundances (e.g., [Fe/H] = −0.27 ± 0.31 dex). The planet’s dynamical mass (

2.8

−
0.5

+
0.6

M
Jup) and orbit are also refined using published radial velocities, relative astrometry, and absolute astrometry. We use petitRADTRANS to perform chemically consistent atmospheric retrievals for AF Lep b. The radiative–convective equilibrium temperature profiles are incorporated as parameterized priors on the planet’s thermal structure, leading to a robust characterization for cloudy self-luminous atmospheres. This novel approach is enabled by constraining the temperature–pressure profiles via the temperature gradient

(
d
ln
T

/

d
ln
P
)

, a departure from previous studies that solely modeled the temperature. Through multiple retrievals performed on different portions of the 0.9–4.2 μm spectrophotometry, along with different priors on the planet’s mass and radius, we infer that AF Lep b likely possesses a metal-enriched atmosphere ([Fe/H] > 1.0 dex). AF Lep b’s potential metal enrichment may be due to planetesimal accretion, giant impacts, and/or core erosion. The first process coincides with the debris disk in the system, which could be dynamically excited by AF Lep b and lead to planetesimal bombardment. Our analysis also determines T
eff ≈ 800 K,

log
(
g
)
≈
3.7

dex, and the presence of silicate clouds and disequilibrium chemistry in the atmosphere. Straddling the L/T transition, AF Lep b is thus far the coldest exoplanet with suggested evidence of silicate clouds.
Developing a Drift Rate Distribution for Technosignature Searches of Exoplanets
Authors: Li Megan G. , Sheikh Sofia Z. , Gilbertson Christian , He Matthias Y. , Isaacson Howard , Croft Steve , Sneed Evan L. 
Published: October 2023

Abstract
A stable-frequency transmitter with relative radial acceleration to a receiver will show a change in received frequency over time, known as a “drift rate.” For a transmission from an exoplanet, we must account for multiple components of drift rate: the exoplanet’s orbit and rotation, the Earth’s orbit and rotation, and other contributions. Understanding the drift rate distribution produced by exoplanets relative to Earth, can (a) help us constrain the range of drift rates to check in a Search for Extraterrestrial Intelligence project to detect radio technosignatures, and (b) help us decide validity of signals-of-interest, as we can compare drifting signals with expected drift rates from the target star. In this paper, we modeled the drift rate distribution for ∼5300 confirmed exoplanets, using parameters from the NASA Exoplanet Archive (NEA). We find that confirmed exoplanets have drift rates such that 99% of them fall within the ±53 nHz range. This implies a distribution-informed maximum drift rate ∼4 times lower than previous work. To mitigate the observational biases inherent in the NEA, we also simulated an exoplanet population built to reduce these biases. The results suggest that, for a Kepler-like target star without known exoplanets, ±0.44 nHz would be sufficient to account for 99% of signals. This reduction in recommended maximum drift rate is partially due to inclination effects and bias toward short orbital periods in the NEA. These narrowed drift rate maxima will increase the efficiency of searches and save significant computational effort in future radio technosignature searches.
ALMA 300 pc Resolution Imaging of a z = 6.79 Quasar: No Evidence for Supermassive Black Hole Influence on the C ii Kinematics
Authors: Meyer Romain A. , Neeleman Marcel , Walter Fabian , Venemans Bram 
Published: October 2023

Abstract
We present Atacama Large Millimeter/submillimeter Array (ALMA) [C ii] 158 μm and dust continuum observations of the z = 6.79 quasar J0109–3047 at a resolution of 0.″045 (∼300 pc). The dust and [C ii] emission are enclosed within a ∼500 pc radius, with the central beam (r < 144 pc) accounting for ∼25% (8%) of the total continuum ([C ii]) emission. The far-infrared (FIR) luminosity density increases radially from ∼5 × 1011
L
⊙ kpc−2 to a central value of ∼70 × 1011
L
⊙ kpc−2 (SFRD ∼50–700 M
⊙yr−1 kpc−2). The [C ii] kinematics are dispersion dominated with a constant velocity dispersion of 137 ± 6 km s−1. The constant dispersion implies that the underlying mass distribution is not centrally peaked, consistent with the expectations of a flat gas mass profile. The lack of an upturn in velocity dispersion within the central beam is inconsistent with a black hole mass greater than M
BH < 6.5 × 108
M
⊙ (2σ level), unless highly fine-tuned changes in the interstellar medium properties conspire to produce a decrease of the gas mass in the central beam comparable to the black hole mass. Our observations therefore imply either that (a) the black hole is less massive than previously measured, or (b) the central peak of the FIR and [C ii] emission are not tracing the location of the black hole, as suggested by the tentative offset between the near-infrared position of the quasar and the ALMA continuum emission.
Are “Changing-look” Active Galactic Nuclei Special in the Coevolution of Supermassive Black Holes and Their Hosts? I.
Authors: Wang J. , Zheng W. K. , Brink T. G. , Xu D. W. , Filippenko A. V. , Gao C. , Xie C. H. , Wei J. Y. 
Published: October 2023

Abstract
The nature of the so-called “changing-look” (CL) active galactic nucleus (AGN), which is characterized by spectral-type transitions within ∼10 yr, remains an open question. As the first in our series of studies, we attempt here to understand the CL phenomenon from the view of the coevolution of AGNs and their host galaxies (i.e., if CL-AGNs are at a specific evolutionary stage) by focusing on the SDSS local “partially obscured” AGNs in which the stellar population of the host galaxy can be easily measured in the integrated spectra. A spectroscopic follow-up program using the Xinglong 2.16 m, Lick/Shane 3 m, and Keck 10 m telescopes enables us to identify in total nine CL-AGNs from a sample of 59 candidates selected by their mid-infrared variability. Detailed analysis of these spectra shows that the host galaxies of the CL-AGNs are biased against young stellar populations and tend to be dominated by intermediate-age stellar populations. This motivates us to propose that CL-AGNs are probably particular AGNs at a specific evolutionary stage, such as a transition stage from “feast” to “famine” fueling of the supermassive black hole. In addition, we reinforce the previous claim that CL-AGNs tend to be biased against both a high Eddington ratio and a high bolometric luminosity, suggesting that the disk-wind broad-line-region model is a plausible explanation of the CL phenomenon.
Multipoint Observations of the Dynamics at an ICME Sheath–Ejecta Boundary
Authors: Ala-Lahti Matti , Pulkkinen Tuija I. , Ruohotie Julia , Akhavan-Tafti Mojtaba , Good Simon W. , Kilpua Emilia K. J. 
Published: October 2023

Abstract
The radial evolution of interplanetary coronal mass ejections (ICMEs) is dependent on their interaction with the ambient medium, which causes ICME erosion and affects their geoefficiency. Here, an ICME front boundary, which separates the confined ejecta from the mixed, interacted sheath–ejecta plasma upstream, is analyzed in a multipoint study examining the ICME at 1 au on 2020 April 20. A bifurcated current sheet, highly filamented currents, and a two-sided jet were observed at the boundary. The two-sided jet, which was recorded for the first time for a magnetic shear angle <40°, implies multiple (patchy) reconnection sites associated with the ICME erosion. The reconnection exhaust exhibited fine structure, including multistep magnetic field rotation and localized structures that were measured only by separate Cluster spacecraft with the mission inter-spacecraft separation of 0.4–1.6 R
E. The mixed plasma upstream of the boundary with a precursor at 0.8 au lacked coherency at 1 au and exhibited substantial variations of southward magnetic fields over radial (transverse) distances of 41–237 R
E (114 R
E). This incoherence demonstrates the need for continuous (sub)second-resolution plasma and field measurements at multiple locations in the solar wind to adequately address the spatiotemporal structure of ICMEs and to produce accurate space weather predictions.
Crowded No More: The Accuracy of the Hubble Constant Tested with High-resolution Observations of Cepheids by JWST
Authors: Riess Adam G. , Anand Gagandeep S. , Yuan Wenlong , Casertano Stefano , Dolphin Andrew , Macri Lucas M. , Breuval Louise , Scolnic Dan , Perrin Marshall , Anderson Richard I. 
Published: October 2023

Abstract
High-resolution James Webb Space Telescope (JWST) observations can test confusion-limited Hubble Space Telescope (HST) observations for a photometric bias that could affect extragalactic Cepheids and the determination of the Hubble constant. We present JWST NIRCAM observations in two epochs and three filters of >320 Cepheids in NGC 4258 (which has a 1.5% maser-based geometric distance) and in NGC 5584 (host of SN Ia 2007af), near the median distance of the SH0ES HST SN Ia host sample and with the best leverage among them to detect such a bias. JWST provides far superior source separation from line-of-sight companions than HST in the near-infrared to largely negate confusion or crowding noise at these wavelengths, where extinction is minimal. The result is a remarkable >2.5× reduction in the dispersion of the Cepheid period–luminosity relations, from 0.45 to 0.17 mag, improving individual Cepheid precision from 20% to 7%. Two-epoch photometry confirmed identifications, tested JWST photometric stability, and constrained Cepheid phases. The P–L relation intercepts are in very good agreement, with differences (JWST−HST) of 0.00 ± 0.03 and 0.02 ± 0.03 mag for NGC 4258 and NGC 5584, respectively. The difference in the determination of H0 between HST and JWST from these intercepts is 0.02 ± 0.04 mag, insensitive to JWST zero-points or count rate nonlinearity thanks to error cancellation between rungs. We explore a broad range of analysis variants (including passband combinations, phase corrections, measured detector offsets, and crowding levels) indicating robust baseline results. These observations provide the strongest evidence yet that systematic errors in HST Cepheid photometry do not play a significant role in the present Hubble Tension. Upcoming JWST observations of >12 SN Ia hosts should further refine the local measurement of the Hubble constant.
Jet Lorentz Factor Constraint for GRB 221009A Based on the Optical Depth of the TeV Photons
Authors: Gao Duan-Yuan , Zou Yuan-Chuan 
Published: October 2023

Abstract
The recent detection of teraelectronvolt (TeV) photons from the record-breaking gamma-ray burst GRB 221009A during its prompt phase poses challenges for constraining its Lorentz factor. We reevaluate the constraints on the jet Lorentz factor considering a two-zone model, wherein the TeV photons originate from the external shock region while the lower-energy MeV photons come from the internal prompt emission region. By properly accounting for the evolution of the MeV photon spectrum and light curve, we calculate the optical depth for TeV photons and derive a minimum Lorentz factor of about 300. It is consistent with the afterglow modeling for the TeV emission.
Exemple de coconstruction d’un programme d’empowerment en faveur de la santé des personnes vivant avec des troubles psychiques
Authors: Guillermet Élise , Meunier-Beillard Nicolas , Costa Marie , Defaut Marion , Millot Isabelle , Demassiet Vincent , Roelandt Jean-Luc , Denis Frédéric 
Published: October 2023

Introduction : Au sein de la population présentant des troubles psychiques sévères et persistants, on observe une surreprésentation des facteurs de risque et des pathologies cardiovasculaires. Une personne chez qui un diagnostic de schizophrénie ou de troubles bipolaires a été porté aurait deux à trois fois plus de risque de mourir d’une maladie cardiovasculaire que la population générale. But de l’étude : Dans le cadre du projet « Collaboration patient-soignant pour une meilleure prise en charge des troubles cardiovasculaires des patients souffrant de troubles psychiques au long cours » (COPsyCAT), un programme d’ empowerment a été coconstruit pour réduire ces inégalités de santé. La prise en compte de l’expérience et des besoins des patients, de leurs aidants et des professionnels de santé est au cœur de chacune des étapes méthodologiques suivies pour la création du programme. Résultats : Les parties prenantes ont défini le programme comme devant viser l’amélioration de la qualité de vie et non la réduction du risque cardiovasculaire. Des outils ont été sélectionnés selon leur maniabilité pour permettre l’orientation autogérée des patients, de telle sorte que les contraintes inhérentes aux cloisonnements entre psychiatrie et soins primaires soient contournées. Le programme se base sur la mutualisation des ressources existantes sur un territoire. Pouvoir d’agir individuel et construction de contexte favorable à la santé sont ainsi pensés pour se renforcer mutuellement et agir sur des leviers réformateurs. Conclusions : Cet article décrit concrètement les étapes grâce auxquelles le programme d’ empowerment COPsyCAT a été conçu, en coconstruction par les chercheurs de l’étude, les usagers et associations d’usagers et les professionnels de santé à partir de leurs savoirs expérientiels. La faisabilité du programme et l’appropriation des outils en situation réelle va être prochainement évaluée. La mesure de l’efficacité du programme sur le risque cardiovasculaire viendra dans un second temps.