bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KUALITAS PELAYANAN TERHADAP KEPUASAN PELANGGAN PADA WARUNG MAKAN BAKSO DAN MIE AYAM BADALI DESA BAHUNGIN KECEMATAN KELUA KABUPATEN TABALONG
Authors: Hasanah Nurul , Rahmah Audina 
Published: April 2024

Penelitian ini bertujuan untuk mengetahui apakah kualitas pelayanan secara simultan mempunyai pengaruh terhadap kepuasan pelanggan Warung Makan Bakso dan Mie Ayam Dadali Desa Bahungin Kecematan Kelua Kabupaten Tabalong.
Populasi penelitian ini adalah konsumen Warung Makan Bakso Dan Mie Ayam Badali. Sampel yang diambil sebanyak 86 responden dengan mengunakan teknik insidental sampling. Data dikumpulkan dengan kuesioner sebagai metode pokok dan dokumentasi sebagai metode pelengkap. Metode analisis data yang digunakan adalah kuantitatif dengan menggunakan uji kualitas data seperti uji validitas, uji reliabilias dan uji F.
Berdasarkan hasil penelitian dan pengujian dari data yang didapatkan, penulis menyimpulkan bahwa Tangibles (Bukti Fisik), Reliability (Keandalan), Assurance (Jaminan) dan Empathy (Empati) serta Responsiveness (Daya Tangkap) berpengaruh positif pada kepuasan pelanggan. Hal itu disimpulkan dengan melihat hasil uji hipotesis secara simultan (Uji F) yang menunjukkan kalau nilai F hitung (9,73) lebih besar dari nilai F tabel (2,33) yang berarti bahwa Ho ditolak dan Ha diterima atau dapat variabel bebas X1, X2, X3, X4, dan X5 (secara simultan) berpengaruh terhadap variabel terikat (Y).
PENGARUH HARGA TERHADAP KEPUTUSAN PEMBELIAN KOSMETIK WARDAH DI TOKO RANUM KOSMETIK AMUNTAI
Authors: Handayani Ramona , Maulidah Siti 
Published: April 2024

Penelitian ini dilakukan untuk meneliti pengaruh harga terhadap keputusan pembelian yang di latar belakangi karena banyak orang yang menyukai produk kosmetik wardah. Serta untuk mengetahui dan menganalisis pengaruh harga terhadap keputusan pembelian kosmetik wardah pada konsumen.
Penelitian ini menggunakan 65 responden sebagai sampel penelitian dan teknik pengumpulan sampel menggunakan metode non probability sampling. Metode analisis data yang digunakan adalah analisis kuantitatif yang meliputi uji validitas, uji reliabilitas, uji normalitas, uji linearitas, uji korelasi ( uji regresi linear sederhana).
Data yang diuji kemudian diolah dengan Software SPSS versi 20, dari 13 pernyataan hasil uji validitas dinyatakan valid. Hal ini dapat dinyatakan nilai Rhitung > 0,244. Untuk hasil uji reliabilitas pada kedua variabel tersebut adalah 0,795 dan 0,897 > 0,60. Data dikatakan reliabel apabila cronbach alpa > 0,60. Untuk hasil uji normalitas diketahui nilai signifikansi 0,214 > 0,05, maka dapat disimpulkan bahwa nilai residual berdistribusi normal. Sedangkan hasil uji linearitas diketahui nilai sig. Deviations from Linearity 0,000 < 0,05, maka tidak terdapat hubungan yang linear antara variabel bebas dengan variabel terikat.
Berdasarkan kesimpulan yang penulis kemukakan diatas, maka penulis memberikan saran yang mungkin dapat menjadi pertimbangan bagi penjual. Sarannya yaitu mempertahankan harga yang dapat dijangkau masyarakat agar masyarakat tetap memilih produk Wardah tersebut, karena harga merupakan jumlah nilai yang diberikan pelanggan kepada pembeli untuk mendapatkan keuntungan dari produk yang dijual
Instance maps as an organising concept for complex experimental workflows as demonstrated for (nano)material safety research
Authors: Punz Benjamin , Brajnik Maja , Dokler Joh , Amos Jaleesia D , Johnson Litty , Reilly Katie , Papadiamantis Anastasios G , Green Etxabe Amaia , Walker Lee , Martinez Diego S T , Friedrichs Steffi , Weltring Klaus M , Günday-Türeli Nazende , Svendsen Claus , Ogilvie Hendren Christine , Wiesner Mark R , Himly Martin , Lynch Iseult , Exner Thomas E 
Published: April 2024

Nanosafety assessment, which seeks to evaluate the risks from exposure to nanoscale materials, spans materials synthesis and characterisation, exposure science, toxicology, and computational approaches, resulting in complex experimental workflows and diverse data types. Managing the data flows, with a focus on provenance (who generated the data, for what purpose) and quality (how the data was generated, using which protocol, with which controls), as part of good research output management, is necessary to maximise the re-use potential and value of the data. The concept of Instance Maps has been developed and evolved to visualise experimental nanosafety workflows and to bridge the gap between the theoretical principles of FAIR (Findable, Accessible, Interoperable and Re-usable) data and the everyday practice of experimental researchers. While Instance Maps can be created for completed studies or publications, they are most effective when applied at the study design stage to associate the workflow with the nanomaterials, environmental conditions, method descriptions, protocols, biological and computational models to be used and the data flows arising from study execution. Application of the Instance Map Tool (described herein) to research workflows of increasing complexity is presented to demonstrate its utility, starting from assessment of nanomaterials transformations in complex media, and documentation of nanomaterial synthesis, functionalisation and characterisation, to description of the culturing of ecotoxicity model organisms Daphnia magna and their use in acute and chronic standardised tests for nanomaterials ecotoxicity assessment, and visualisation of complex workflows in human immunotoxicity assessment using cell lines and primary cellular models. These examples showcase the use of the Instance Map approach for coordination of materials and data flows in complex multi-partner collaborative projects, and to support demonstration case studies. Finally, areas for future development of the Instance Map approach and tool are highlighted.
The Star Formation History in Local Group Galaxies. I. Ten Dwarf Galaxies
Authors: Ren 任 Yi 逸 , Jiang 姜 Biwei 碧沩 , Wang 王 Yuxi 钰溪 , Yang 杨 Ming 明 , Yan 闫 Zhiqiang 智强 
Published: April 2024

Abstract
The star formation histories (SFHs) of galaxies provide valuable insights into galaxy evolution and stellar physics. Understanding the SFHs enables the study of chemical enrichment of galaxies, star formation triggered by interactions, and the behavior of various stellar populations. This work investigates the SFHs of ten dwarf galaxies in the Local Group (LG), which spans a wide range of types, masses, luminosities, and metallicities. The analysis is based on our new sample of the member stars in the LG after removing foreground dwarf stars by using information from the near-infrared color–color diagram and Gaia astrometry. The sample includes the most complete and pure red supergiants and asymptotic giant branch stars to gain valuable insights into the recent SFHs of the galaxies. A fitting method based on the color–magnitude diagram (CMD) is introduced to measure the SFH. The Padova isochrones are used to generate initial model CMDs, accounting for photometric errors and completeness through star-field simulations to match the completeness and error distributions of the observed CMDs. Subsequently, the SFHs, distance modulus, and metallicity of the ten dwarf galaxies are determined by fitting the CMDs. The results indicate that the star formation rates of dwarf irregulars show a gradual increase, while those of dwarf ellipticals exhibit a gradual decrease from the past to the present. Furthermore, this work shows that the star formation activity in dwarf ellipticals persisted up to 30 Myr ago. A significant increasing feature in the SFH of NGC 6822 reveals star formation activity triggered by an interaction event.
Distinguishing ΛCDM from Evolving Dark Energy with Om Two-point Statistics: Implications from the Space-borne Gravitational-wave Detector
Authors: Liu Yuting , Cao Shuo , Zheng Xiaogang , Biesiada Marek , Jiang Jianyong , Liu Tonghua 
Published: April 2024

Abstract
The Omh
2(z

i
, z

j
) two-point diagnostics was proposed as a litmus test of the ΛCDM model, and measurements of the cosmic expansion rate H(z) have been extensively used to perform this test. The results obtained so far suggested a tension between observations and predictions of the ΛCDM model. However, the data set of H(z) direct measurements from cosmic chronometers and baryon acoustic oscillations was quite limited. This motivated us to study the performance of this test on a larger sample obtained in an alternative way. In this paper, we propose that gravitational-wave (GW) standard sirens could provide large samples of H(z) measurements in the redshift range of 0 < z < 5, based on the measurements of the dipole anisotropy of luminosity distance arising from the matter inhomogeneities of the large-scale structure and the local motion of the observer. We discuss the effectiveness of our method in the context of the space-borne DECi-herz Interferometer Gravitational-wave Observatory, based on a comprehensive H(z) simulated data set from binary neutron star merger systems. Our results indicate that in the GW domain, the Omh
2(z

i
, z

j
) two-point diagnostics could effectively distinguish whether ΛCDM is the best description of our Universe. We also discuss the potential of our methodology in determining possible evidence for dark energy evolution, focusing on its performance on the constant and redshift-dependent dark energy equation of state.
Ultrafast Compact Binary Mergers
Authors: Beniamini Paz , Piran Tsvi 
Published: April 2024

Abstract
The duration of orbital decay induced by gravitational waves (GWs) is often the bottleneck of the evolutionary phases going from star formation to a merger. We show here that kicks imparted to the newly born compact object during the second collapse generically result in a GW merger time distribution behaving like

dN

/

d
log
t
∝

t

2

/

7

at short durations, leading to ultrafast mergers. Namely, a nonnegligible fraction of neutron star binaries, formed in this way, will merge on a timescale as short as 10 Myr, and a small fraction will merge even on a timescale less than 10 kyr. The results can be applied to different types of compact binaries. We discuss here the implications for binary neutron star mergers. These include unique short gamma-ray bursts (GRBs), eccentric and misaligned mergers, r-process enrichment in the very early Universe and in highly star-forming regions, and possible radio precursors. Interestingly, we conclude that among the few hundred short GRBs detected so far, a few must have formed via this ultrafast channel.
Solar Energetic Particle and the Heliospheric Current Sheet
Authors: Liou Kan , Wu Chin-Chun 
Published: April 2024

Abstract
The effect of the heliospheric current sheet (HCS) on the propagation of solar energetic particles (SEPs) remains poorly known. In this study we address this question by surveying energetic (∼2.0–9.6 MeV nucleon–1) helium data acquired by the energetic particle acceleration, composition, and transport (EPACT) sensor on board the Wind spacecraft. A superposed epoch analysis of 319 HCS crossings made by Wind reveals a sharp drop in the SEP fluxes at the HCS for the low-energy channels and little change across the HCS for the high-energy channels. To help understand the statistical result, we studied a total of 15 SEP flux dropout (a decrease of ∼50% or more) events that coincided with the crossing of the HCS. One of the common features of these SEP events is that they were initiated in the western hemisphere but far away from the longitude of HCS crossings, suggesting that the source of SEPs was well connected initially but was cut off later after Wind moved to the opposite hemisphere (e.g., HCS crossing). Further analysis of the events suggests that the percentage of flux dropouts decreases with increasing energy. It is suggested that a strong scattering of MeV helium may have occurred as the particle gyroradius is comparable to the thickness of the current sheet. This study clearly provides solid evidence for the HCS as a barrier to suppressing SEP flux of MeV energies from the onset hemisphere to the other.
Circumnuclear Multiphase Gas in the Circinus Galaxy. VI. Detectability of Molecular Inflow and Atomic Outflow
Authors: Baba Shunsuke , Wada Keiichi , Izumi Takuma , Kudoh Yuki , Matsumoto Kosei 
Published: April 2024

Abstract
Recent submillimeter observations have revealed signs of parsec-scale molecular inflow and atomic outflow in the nearest Seyfert 2 galaxy, the Circinus galaxy. To verify the gas kinematics suggested by these observations, we performed molecular and atomic line transfer calculations based on a physics-based 3D radiation-hydrodynamic model, which has been compared with multiwavelength observations in this paper series. The major-axis position–velocity diagram (PVD) of CO(3–2) reproduces the observed faint emission at the systemic velocity, and our calculations confirm that this component originates from failed winds falling back to the disk plane. The minor-axis PVD of [C i](3
P
1–3
P
0), when created using only the gas with positive radial velocities, presents a sign of blueshifted and redshifted offset peaks similar to those in the observation, suggesting that the observed peaks indeed originate from the outflow, but that the model may lack outflows as strong as those in the Circinus galaxy. Similar to the observed HCN(3–2), the similar dense-gas tracer HCO+(3–2) can exhibit nuclear spectra with inverse P-Cygni profiles with ∼0.5 pc beams, but the line shape is azimuthally dependent. The corresponding continuum absorbers are inflowing clumps at 5–10 pc from the center. To detect significant absorption with a high probability, the inclination must be fairly edge-on (≳85°), and the beam size must be small (≲1 pc). These results suggest that HCN or HCO+ and [C i] lines are effective for observing parsec-scale inflows and outflows, respectively.
The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)*
Authors: Zeimann Gregory R. , Debski Maya H. , Schneider Donald P. , Bowman William P. , Drory Niv , Hill Gary J. , Lee Hanshin , MacQueen Phillip , Shetrone Matthew 
Published: April 2024

Abstract
The Hobby–Eberly Telescope (HET) VIRUS Parallel Survey (HETVIPS) is a blind spectroscopic program that sparsely covers approximately two-thirds of the celestial sphere and consists of roughly 252 million fiber spectra. The spectra were taken in parallel mode with the Visible Integral-field Replicable Unit Spectrograph (VIRUS) instrument when the HET was observing a primary target with other HET facility instruments. VIRUS can simultaneously obtain approximately 35,000 spectra covering 3470–5540 Å at a spectral resolution of ≈800. Although the vast majority of these spectra cover blank sky, we used the Pan-STARRS1 Data Release 2 Stacked Catalog to identify objects encompassed in the HETVIPS pointings and extract their spectra. This paper presents the first HETVIPS data release, containing 493,012 flux-calibrated spectra obtained through 2023 March 31, as well as a description of the data processing technique. Each of the object spectra were classified, resulting in a catalog of 74,196 galaxies, 4,087 quasars, 259,396 stars, and 154,543 unknown sources.
The Near-infrared Ca ii Triplet as a Stellar Activity Indicator: A Library and Comparative Study
Authors: Huang 黄 Xin 鑫 , He 何 Yuji 玉吉 , Bai 白 Zhongrui 仲瑞 , Yuan 袁 Hailong 海龙 , Yang 杨 Mingkuan 明宽 , Zhou 周 Ming 明 , Dong 董 Yiqiao 义乔 , Wang 汪 Mengxin 梦欣 , He 贺 Han 晗 , Zhang 张 Jinghua 敬华 , Chu 褚 Yaoquan 耀泉 , Zhao 赵 Yongheng 永恒 , Zhang 张 Yong 勇 , Zhang 张 Haotong 昊彤 
Published: April 2024

Abstract
We have established and released a new stellar index library of the Ca ii triplet, which serves as an indicator for characterizing the chromospheric activity of stars. The library is based on data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low-Resolution Spectroscopic Survey (LRS) Data Release 9. To better reflect the chromospheric activity of stars, we have defined new indices R and R
+. The library includes measurements of R and R
+ for each Ca ii infrared triplet (IRT) from 699,348 spectra of 562,863 F, G, and K-type solar-like stars with a signal-to-noise ratio higher than 100, as well as the stellar atmospheric parameters and basic information inherited from the LAMOST LRS catalog. We compared the differences between the three individual indices of the Ca ii triplet and also conducted a comparative analysis of

R

λ
8542

+

to the Ca ii H and K S and

R

HK

+

index databases. We observe the fraction of less active stars decreases with T
eff and the fraction of more active stars first decreases with decreasing temperature and turns to increase with decreasing temperature at 5800 K. We also find that a significant fraction of stars that show a high activity index in both Ca ii H and K and IRT are binaries with low activity; some of them could be discriminated in the Ca ii H and K S index and

R

λ
8542

+

space. This new stellar library serves as a valuable resource for studying chromospheric activity in stars and can be used to improve our comprehension of stellar magnetic activity and other astrophysical phenomena.
Tidal Disruption of Planetesimals from an Eccentric Debris Disk Following a White Dwarf Natal Kick
Authors: Akiba Tatsuya , McIntyre Selah , Madigan Ann-Marie 
Published: April 2024

Abstract
The surfaces of many white dwarfs are polluted by metals, implying a recent accretion event. The tidal disruption of planetesimals is a viable source of white dwarf pollution and offers a unique window into the composition of exoplanet systems. The question of how planetary material enters the tidal disruption radius of the white dwarf is currently unresolved. Using a series of N-body simulations, we explore the response of the surrounding planetesimal debris disk as the white dwarf receives a natal kick caused by anisotropic mass loss on the asymptotic giant branch. We find that the kick can form an apse-aligned, eccentric debris disk in the range 30–240 au, which corresponds to the orbits of Neptune, the Kuiper Belt, and the scattered disk in our solar system. In addition, many planetesimals beyond 240 au flip to counterrotating orbits. Assuming an isotropic distribution of kicks, we predict that approximately 80% of white dwarf debris disks should exhibit significant apsidal alignment and a fraction of counterrotating orbits. The eccentric disk is able to efficiently and continuously torque planetesimals onto radial, star-grazing orbits. We show that the kick causes both an initial burst in tidal disruption events as well as an extended period of 100 Myr where tidal disruption rates are consistent with observed mass accretion rates on polluted white dwarfs.
Travailler, travailler encore
Authors: Raulet Gérard 
Published: April 2024

La tradition utopique compte autant de projets de société promettant l’avènement d’une ère de loisirs que de projets dans lesquels le travail demeure le pilier de la cohésion sociale. Cette double lignée continue d’inspirer certains programmes politiques, mais à la différence des années 1970 une sorte de résignation semble s’être répandue. Cet article propose, au contact de l’histoire des idées politiques et de la philosophie politique contemporaine, de réexaminer les paradigmes de la conception du travail et de sa place dans la société, et de dresser un bilan des théories et utopies sociales qui ont imaginé comment le règne de la liberté peut s’établir sur le règne de la nécessité. La relecture de la tradition utopique permet de faire justice d’une série de lieux communs. Par exemple la crainte qu’une organisation communautaire trop parfaite, « communiste », ne dissuade de travailler – un argument qui ne cesse de polluer toute réflexion sur une conception sociale globale (et non libéraleindividuelle) de la question du travail.
Les silences de la langue paternelle, transmission et « écrypture »
Authors: Farkas Olivia 
Published: April 2024

Partant d’un lapsus, celui d’« écrypture », condensation des signifiants « crypte » et « écriture », ce texte interroge la non-transmission de la langue maternelle du père qualifiée de « langue paternelle » dans les situations de trauma et d’exil, en appui sur les ouvrages d’auteurs hongrois comme décor de l’histoire familiale. À la génération suivante, comment les cryptes paternelles auraient-elles contribué à la transmission des éléments traumatiques vécus avant l’exil ?
La langue maternelle et le langage de la tendresse. Perdus et retrouvés
Authors: Koritar Endre 
Published: April 2024

Cet article explore l’impact des premières expériences esthétiques sur le développement de la psyché. Le bain sonore de l’environnement du fœtus puis du nouveau-né est enregistré en tant que mémoire implicite dans l’inconscient non refoulé et transmet un sentiment d’appartenance ou d’aliénation en fonction de la nature des relations objectales maternelles précoces. Dans le cas d’un enfant déplacé de sa culture maternelle précoce, par la fuite et l’émigration, l’acculturation, la perte des images, des sons et odeurs familiers de sa culture d’origine, ce sont autant de stress supplémentaires. Tout comme la perte de la musicalité de la langue. Nous présentons ici le cas clinique d’un jeune patient qui a pu faire le deuil de sa langue maternelle et de sa culture tardivement, après avoir pu revenir sur son lieu de naissance. L’expérience esthétique de sa confrontation à la culture de son village natal et la remémoration de ses premières expériences de vie auprès des personnes qui lui avaient prodigué leurs soins ont ouvert les cryptes de traumatismes longtemps enfouis du passé et l’ont amené au cours de l’analyse à explorer les régions souterraines de son esprit. Cet article soutient que c’est son instinct d’autoconservation qui l’a conduit à la recherche de son passé. Le travail analytique de construction et de reconstruction lui a fourni le récit ayant pu réanimer son instinct de vie affaibli en redonnant du sens et un but à son existence.
Freud, un Janus bifrons ? Freud et sa « psychologie de l’enfant » au tournant du siècle
Authors: Kamieniak Jean-Pierre 
Published: April 2024

Si l’objet majeur des recherches du futur conquistador résidait bien dans le devenir libidinal désormais inconscient du sujet humain, faisant de ce dernier un être pulsionnel dès ses débuts aux conduites recouvertes par cette amnésie infantile qu’il identifiera en 1905, il n’en reste pas moins que jusqu’à la publication de L’interprétation du rêve – activité pédiatrique, éducation, analyse d’adultes, paternage et auto-analyse aidant –, c’est un véritable portrait psychologique de l’enfant qu’il brosse à grands traits, partagé qu’il est entre ce laboratoire que sont ses Lettres à l’ami Fließ et cette publication officielle fondamentale de 1900. Aussi est-ce à la fréquentation de cet espace hétérogène, si ce n’est contradictoire, que le lecteur est convié.
Scolarisation obligatoire et fécondité des femmes en Indonésie
Authors: de Talancé Marine 
Published: April 2024

L’allongement de la scolarisation obligatoire en Indonésie a changé les trajectoires d’éducation, maritales et, in fine, les comportements de fécondité des femmes, particulièrement pour les groupes ethniques pratiquant traditionnellement le prix de la fiancée. Codes JEL : I25, J13.