bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KINERJA KEUANGAN TERHADAP HARGA SAHAM PERUSAHAAN PERTAMBANGAN YANG TERDAFTAR DI BURSA EFEK INDONESIA
Authors: Abdullah Abdullah , Rachma Nur , Marlinah Andi 
Published: June 2023

Analisis Pengaruh Kinerja Keuangan terhadap Harga Saham pada Perusahaan Pertambangan yang terdaftar di Bursa Efek Indonesia. Penelitian ini bertujuan untuk mengetahui pengaruh Current Ratio, Debt to Equity Ratio, Return On Equity, Working Capital Turnover dan Earning Per Share secara parsial, maupun simultan terhadap Harga Saham. Populasi dalam penelitian ini adalah Perusahaan Sektor Pertambangan yang terdaftar di bursa efek Indonesia sebanyak 34 perusahaan. Sampel penelitian ini adalah 15 (limabelas) perusahaan yang dipilih berdasarkan criteria yaitu: Perusahaan Pertambangan yang terdaftar di Bursa Efek Indonesia Tahun 2019-2021; Menerbitkan laporan keuangan yang telah diaudit; Perusahaan sampel mempublikasikan laporan keuangan secara lengkap sesuai varibel penelitian selama periode pengamatan; Memiliki keuntungan (profit); dan pernah membagikan Cash Deviden selama periode pengamatan. Hasil penelitian ini menunjukkan bahwa Current Ratio (X1), Return On Equity (X3), Working Capital Turnover (X4) dan Earning Per Share (X5) berpengaruh positif dan signifikan terhadap harga saham, sedangkan Deb to Equity Ratio (X2) berpengaruh Negatif dan tidak signifikan terhdap Harga Saham. Secara Simultan Current Ratio (X1), Debt to Equity Ratio (X2), Return On Equity (X3), Working Capital Turnover (X4) dan Earning Per Share (X5) berpengaruh Positif dan Signifikan terhadap Harga Saham pada Perusahaan Pertambangan yang terdaftar di Bursa Efek Indonesia. Variabel yang berpengaruh dominan adalah Current Ratio (X1).
Analysis of the Influence of Financial Performance on Share Prices in Mining Companies Listed on the Indonesian Stock Exchange. This study aims to determine the effect of Current Ratio, Debt to Equity Ratio, Return On Equity, Working Capital Turnover and Earning Per Share partially or simultaneously on stock prices. The population in this study are Mining Sector Companies which are listed on the Indonesian stock exchange as many as 34 companies. The sample for this research is 15 (fifteen) companies selected based on criteria, namely: Mining Companies listed on the Indonesia Stock Exchange for 2019-2021; Publish audited financial reports; Sample companies publish complete financial reports according to the research variables during the observation period; Have a profit (profit); and have distributed cash dividends during the observation period. The results of this study indicate that the Current Ratio (X1), Return On Equity (X3), Working Capital Turnover (X4) and Earning Per Share (X5) have a positive and significant effect on stock prices, while the Deb to Equity Ratio (X2) has a negative and not significant to the stock price. Simultaneously Current Ratio (X1), Debt to Equity Ratio (X2), Return On Equity (X3), Working Capital Turnover (X4) and Earning Per Share (X5) have a Positive and Significant Effect on Stock Prices in Mining Companies Listed on the Stock Exchange Indonesian Securities. The variable that has the dominant influence is the Current Ratio (X1).
PENGARUH PROMOSI DAN KUALITAS PELAYANAN TERHADAP KEPUTUSAN WISATAWAN DAN DAMPAKNYA TERHADAP KEPUASAN (Studi di Kabupaten Pinrang)
Authors: Nur Syamsir , Idris Muhammad , Alam Syamsul 
Published: June 2023

Penelitian bertujuan untuk menganalisis: 1) pengaruh langsung promosi dan kualitas pelayanan terhadap kepuasan wisatawan di Kabupaten Pinrang, 2) pengaruh langsung promosi dan kualitas pelayanan terhadap keputusan wisatawan di Kabupaten Pinrang, dan 3) pengaruh tidak langsung promosi dan kualitas pelayanan terhadap keputusan wisatawan melalui kepuasan di Kabupaten Pinrang.Desain penelitian ini menggunakan penelitian survey. Penelitian ini akan dilaksanakan pada di Kabupaten Pinrang pada bulan Oktober sampai November 2019. Populasi dalam penelitian adalah seluruh Wisatawan di Kabupaten Pinrang berjumlah 105 orang dijadaikan sampel. Teknik analisis data menggunakan analisis jalur (path analysis).
Hasil penelitian menunjukkan bahwa: 1) terdapat pengaruh positif dan signifikan secara langsung promosi dan kualitas pelayanan terhadap kepuasan wisatawan di Kabupaten Pinrang, 2) terdapat pengaruh positif dan signifikan secara langsung promosi dan kualitas pelayanan terhadap keputusan wisatawan di Kabupaten Pinrang, dan 3) terdapat pengaruh positif dan signifikan secara tidak langsung promosi dan kualitas pelayanan terhadap keputusan wisatawan melalui kepuasan di Kabupaten Pinrang,
PENGARUH SUPERVISI BIMBINGAN KONSELING DAN SIKAP PROFESIONAL TERHADAP KINERJA GURU PEMBIMBING SEKOLAH MENENGAH ATAS DI KABUPATEN MAJENE
Authors: Baya Nur , Razak Mashur , Alam Syamsul 
Published: June 2023

Penelitian ini dilakukan pada seluruh SMA di Kabupaten Majene.Teknik penarikan sampel adalah sampling jenuh (sensus), dimana semua populasi dijadikan sampel sebanyak 40 orang guru BK Sekolah Menengah Atas di Kabupaten Majene. Metode pengumpulan data yang diguanakan adalah angket dan studi dokumen. Metode analisis yang digunakan adalah analisis statistik deskriptif dan analisis regresi linear berganda.
Hasil penelitian menyimpulkan bahwa: Secara parsial menunjukkan bahwa variabel supervisi bimbingan konseling berpengaruh dominan terhadap kinerja guru pembimbing SMA, hal ini menunjukkan bahwa semakin baik supervisi bimbingan konseling dilakukan akan semakin meningkatkan kinerja guru pembimbing SMA di Kabupaten Majene. Secara parsial menunjukkan bahwa variabel sikap profesional berpengaruh terhadap kinerja pegawai, hal ini menunjukkan bahwa semakin tinggi sikap profesional guru akan semakin meningkatkan kinerja guru pembimbing SMA di Kabupaten Majene. Secara simultan menunjukkan bahwa variabel supervisi bimbingan konseling (X1) dan sikap profesional (X2) berpengaruh terhadap kinerja guru pembimbing SMA di Kabupaten Majene (Y) yang berarti bahwa peningkatan supervisi bimbingan konseling dan sikap profesional akan mempengaruhi peningkatan kinerja guru pembimbing SMA di Kabupaten Majene sebesar 59%
STRATEGI PENINGKATAN KINERJA PEGAWAI MELALUI PROGRAM PELATIHAN, KOMPETENSI DAN DISIPLIN KERJA PADA SEKRETARIAT DAERAH KABUPATEN JENEPONTO
Authors: Jumrah Jumrah , Echdar Saban , Maryadi Maryadi 
Published: June 2023

Penelitian ini bertujuan untuk menganalisis pengaruh Pelatihan, Kompetensi dan Disiplin Kerja terhadap Kinerja Pegawai secara parsial dan simultan, menganalisis variabel yang dominan berpengaruh terhadap Kinerja Pegawai. Penelitian ini menggunakan pendekatan kuantitatif, dengan sampel sebanyak 75, menggunakan analisis regresi linear berganda.
Hasil pengujian menunjukkan terdapat pengaruh positif dan signifikan pelatihan, kompensasi dan disiplin kerja secara parsial terhadap kinerja pegawai, terdapat pengaruh positif dan signifikan pelatihan, kompetensi dan disiplin kerja secara simultan terhadap kinerja pegawai, disiplin sebagai variabel paling dominan berpengaruh terhadap kinerja pegawai Sekretariat Daerah Kabupaten Jeneponto. Hasil perhitungan koefisien determinasi (R2) diperoleh hasil 0,416 yang berarti 41,6% variabel dependen (kinerja pegawai) dapat dijelaskan oleh variabel independent (pelatihan, kompetensi dan disiplin kerja), sedangkan sisanya 58,4% dijelaskan oleh variabel lain di luar penelitian ini.
PENGARUH HARGA,PROMOSI DAN KUALITAS PELAYANAN TERHADAP KEPUASAN PENGGUNA OJEK ONLINE DI KALANGAN MAHASISWA NOBEL
Authors: Putri Nur Azizah , Ngandoh Ali Murdhani , Ilham Bahrul Ulum 
Published: June 2023

Penelitian ini menggunakan metode kuantitatif. Data dikumpulkan melalui kuesioner dan diolah dengan menggunakan SPSS. Penelitian ini mengambil sampel sebanyak 68 mahasiswa.
Hasil penelitian menunjukkan bahwa (1) Harga tidak berpengaruh signifikan terhadap kepuasan pengguna ojek online dikalangan Mahasiswa Nobel. (2) Promosi berpengaruh signifikan terhadap kepuasan pengguna ojek online dikalangan Mahasiswa Nobel. (3) Kualiatas Pelayanan berpengaruh secara parsial terhadap kepuasan pengguna ojek online dikalangan Mahasiswa Nobel. (4) Secara simultan Harga, Promosi, dan Kualitas Pelayanan berpengaruh terhadap variabel dependen Y(Kepuasaan Pengguna)
Responsible Cannabis Sales: A Narrative Review Considering Interventions for Dispensary Staff to Address Cannabis Harms
Authors: Lange James E. , Moyers Susette A. , Croff Julie M. 
Published: June 2023

An industry of cannabis sales outlets (often called dispensaries) has proliferated in response to state-sanctioned legalization. This paper focuses on the interaction of dispensary sales staff (budtenders) and consumers, which likely has a substantial impact on the consumer experience. To date, there has been little consideration on this aspect of dispensary sales environment, in which staff provide guidance regarding cannabis products. Training programs for alcohol sales are frequently mandated; in contrast, budtender trainings are not currently required or otherwise regulated by state agencies, and therefore, do not address consumer or community safety. This paper explores responsible cannabis sales training and practice. Differences between cannabis and alcohol sales environments, including product diversity, consumer education and motivations, and market maturity are described. Dispensary staff training, along with management policies may improve the quality of product education, and therefore, improve the safety to consumers and communities.
Pembangunan Prototype Aplikasi Mobile Android Untuk Mendukung Sistem Penjualan Dan Promosi UMKM Jihaz Toys Desa Sayati Kabupaten Bandung Jawa Barat
Authors: Roro Santi  , Rahmanesa Abdur 
Published: June 2023

Semakin meningkatnya penggunaan perangkat smartphone untuk berbagai aktivitas, terutama pada saat kondisi seluruh dunia mengalami Pandemik COVID-19. Anjuran pemerintah yang merujuk pada anjuran WHO dalam menghadapi kondisi sekarang untuk melakukan pembatasan aktivitas sosial, sangat berdampak pada berbagai aspek kehidupan terutama permasalahan ekonomi. Kondisi ini menyebabkan akses komunikasi melalui internet terutama melalui smartphone semakin meningkat, karena hal ini menjadi solusi termudah untuk tetap berkomunikasi dan melakukan aktivitas sosial. Kemudahan menggunakan perangkat smartphone menjadi bagian dari gaya hidup, selain sebagai komunikasi sosial smartphone juga digunakan untuk komunikasi penunjang ekonomi. Melalui penelitian ini penulis tertarik untuk mencari solusi melalui kemudahan memanfaatkan perangkat dan aplikasi mobile untuk digunakan dalam beraktivitas mendukung sistem penjualan dan promosi UMKM. Penulis mengunakan beberapa aplikasi mobile android sosial media dan marketplace yang sudah ada dalam Play Store untuk digunakan pada sistem penjualan dan promosi, serta menambahkan aplikasi (prototype) mobile android sebagai tambahan dan pendukung untuk menangani beberapa aktivitas yang tidak dapat ditangani oleh beberapa aplikasi yang sudah ada tersebut. Harapannya adalah dengan penerapan aplikasi ini dapat memudahkan aktivitas penjualan dan promosi UMKM sehingga tidak ada keraguan untuk melakukan digitalisasi pada usahanya.
Absorption-line Observations of
H3+
and CO in Sight Lines Toward the Vela and W28 Supernova Remnants
Authors: Indriolo Nick 
Published: June 2023

Abstract
Supernova remnants act as particle accelerators, providing the cosmic-ray protons that permeate the interstellar medium and initiate the ion–molecule reactions that drive interstellar chemistry. Enhanced fluxes of cosmic-ray protons in close proximity to supernova remnants have been inferred from observations tracing particle interactions with nearby molecular gas. Here I present observations of

H

3

+

and CO absorption, molecules that serve as tracers of the cosmic-ray ionization rate and gas density, respectively, in sight lines toward the W28 and Vela supernova remnants. Cosmic-ray ionization rates inferred from these observations range from about 2 to 10 times the average value in Galactic diffuse clouds (∼3 × 10−16 s−1), suggesting that the gas being probed is experiencing an elevated particle flux. While it is difficult to constrain the line-of-sight locations of the absorbing gas with respect to the supernova remnants, these results are consistent with a scenario where cosmic rays are diffusing away from the acceleration site and producing enhanced ionization rates in the surrounding medium.
Removal of Active Region Inflows Reveals a Weak Solar Cycle Scale Trend in the Near-surface Meridional Flow
Authors: Mahajan Sushant S. , Sun 孙 Xudong 旭东 , Zhao 赵 Junwei 俊伟 
Published: June 2023

Abstract
Using time–distance local helioseismology flow maps within 1 Mm of the solar photosphere, we detect inflows toward activity belts that contribute to solar-cycle scale variations in the near-surface meridional flow. These inflows stretch out as far as 30° away from the active region centroids. If active region neighborhoods are excluded, the solar-cycle-scale variation in the background meridional flow diminishes to below 2 m s−1, but still shows systematic variations in the absence of active regions between sunspot cycles 24 and 25. We therefore propose that the near-surface meridional flow is a three-component flow made up of a constant baseline flow profile that can be derived from quiet-Sun regions, variations due to inflows around active regions, and solar-cycle-scale variation of about 2 m s−1. Torsional oscillation, on the other hand, is found to be a global phenomenon, i.e., exclusion of active region neighborhoods does not significantly affect its magnitude or phase. This nonvariation in torsional oscillation with distance away from active regions and the three-component breakdown of the near-surface meridional flow serve as vital constraints for solar dynamo models and surface flux-transport simulations.
Interpretation of Flat Energy Spectra Upstream of Fast Interplanetary Shocks
Authors: Perri Silvia , Prete Giuseppe , Zimbardo Gaetano , Trotta Domenico , Wilson III Lynn B. , Lario David , Servidio Sergio , Valentini Francesco , Giacalone Joe 
Published: June 2023

Abstract
Interplanetary shocks are large-scale heliospheric structures often caused by eruptive phenomena at the Sun, and represent one of the main sources of energetic particles. Several interplanetary (IP) shock crossings by spacecraft at 1 au have revealed enhanced energetic-ion fluxes that extend far upstream of the shock. Surprisingly, in some shock events ion fluxes with energies between 100 keV and about 2 MeV acquire similar values (which we refer to as “overlapped” fluxes), corresponding to flat energy spectra in that range. In contrast, closer to the shock the fluxes are observed to depend on energy. In this work, we analyze three IP-shock-related energetic particle events observed by the Advanced Composition Explorer spacecraft where flat ion energy spectra were observed upstream of the shock. We interpret these observations via a velocity-filter mechanism for particles in a given energy range. In particular, ions with velocity parallel to the local magnetic field larger than the speed of the upstream plasma, in the reference frame of the shock, can easily propagate back upstream, while lower-energy ions tend to be confined to the shock front, thus reducing their fluxes far upstream and giving rise to flat energy spectra. The velocity-filter mechanism has been corroborated from observations of particle flux anisotropy by the Solid-State Telescope of Wind/3DP.
ALMA Observation of a z ≳ 10 Galaxy Candidate Discovered with JWST
Authors: Yoon Ilsang , Carilli C. L. , Fujimoto Seiji , Castellano Marco , Merlin Emiliano , Santini Paola , Yun Min S. , Murphy Eric J. , Jung Intae , Casey Caitlin M. , Finkelstein Steven L. , Papovich Casey , Fontana Adriano , Treu Tommaso , Letai Jonathan 
Published: June 2023

Abstract
We report the observation by the Atacama Large Millimeter/submillimeter Array (ALMA) of a z ≳ 10 galaxy candidate (GHZ1) discovered from the GLASS–JWST Early Release Science Program. Our ALMA program aims to detect the [O iii] emission line at the rest-frame frequency 3393.0062 GHz (88.36 μm) and far-IR continuum emission with the spectral window setup seamlessly covering a 26.125 GHz frequency range (10.10 < z < 11.14). A total of 7 hr of on-source integration was employed, using four frequency settings to cover the full range (1.7 hr per setting), with 0.″7 angular resolution. No line or continuum is clearly detected, with 5σ upper limits on the line emission of 0.93 mJy beam−1 at 25 km s−1 channel−1 and on the continuum emission of 30 μJy beam−1. We report marginal spectral (at 225 km s−1 resolution) and continuum features (4.1σ and 2.6σ peak signal-to-noise ratio, respectively), within 0.″17 from the JWST position of GHZ1. This spectral feature implies z = 10.38 and needs to be verified with further observations. Assuming that the best estimate of photometric redshift (

z
=

10.60

−
0.60

+
0.52

) is correct, the model of the galaxy’s broadband spectral energy distribution for the 3σ upper limit of the continuum flux from GHZ1 suggests that GHZ1 has a small amount of dust (M

d
≲ 104
M
⊙) at a high temperature (T

d
≳ 90 K). The 5σ upper limit on the [O iii]88μm line luminosity and the inferred star formation rate of GHZ1 are consistent with the properties of low-metallicity dwarf galaxies. We also report serendipitous clear detections of six continuum sources at the locations of the JWST galaxy counterparts in the field.
Digging into the Interior of Hot Cores with the ALMA (DIHCA). III. The Chemical Link between NH2CHO, HNCO, and H2CO
Authors: Taniguchi Kotomi , Sanhueza Patricio , Olguin Fernando A. , Gorai Prasanta , Das Ankan , Nakamura Fumitaka , Saito Masao , Zhang Qizhou , Lu Xing , Li Shanghuo , Chen Huei-Ru Vivien 
Published: June 2023

Abstract
We have analyzed the NH2CHO, HNCO, H2CO, and CH3CN (13CH3CN) molecular lines at an angular resolution of ∼0.″3 obtained by the Atacama Large Millimeter/submillimeter Array Band 6 toward 30 high-mass star-forming regions. The NH2CHO emission has been detected in 23 regions, while the other species have been detected toward 29 regions. A total of 44 hot molecular cores (HMCs) have been identified using the moment 0 maps of the CH3CN line. The fractional abundances of the four species have been derived at each HMC. In order to investigate pure chemical relationships, we have conducted a partial correlation test to exclude the effect of temperature. Strong positive correlations between NH2CHO and HNCO (ρ = 0.89) and between NH2CHO and H2CO (0.84) have been found. These strong correlations indicate their direct chemical links; dual-cyclic hydrogen addition and abstraction reactions between HNCO and NH2CHO and gas-phase formation of NH2CHO from H2CO. Chemical models including these reactions can reproduce the observed abundances in our target sources.
Shaken or Stirred: The Diffuse Interstellar Medium with Exceptionally High SiO Abundance
Authors: Rybarczyk Daniel R. , Stanimirović Snežana , Gusdorf Antoine 
Published: June 2023

Abstract
Interstellar shocks, a key element of stellar feedback processes, shape the structure of the interstellar medium (ISM) and are essential for the chemistry, thermodynamics, and kinematics of interstellar gas. Powerful, high-velocity shocks are driven by stellar winds, young supernova explosions, more evolved supernova remnants, cloud–cloud collisions, and protostellar outflows, whereas the existence and origin of much-lower-velocity shocks (≲10 km s−1) are not understood. Direct observational evidence for interstellar shocks in diffuse and translucent ISM environments has been especially lacking. We present the most sensitive survey to date of SiO—often considered an unambiguous tracer of interstellar shocks—in absorption, obtained with the Northern Extended Millimeter Array interferometer. We detect SiO in five of eight directions probing diffuse and translucent environments without ongoing star formation. Our results demonstrate that SiO formation in the diffuse ISM (i.e., in the absence of significant star formation and stellar feedback) is more widespread and effective than previously reported. The observed SiO line widths are all ≲4 km s−1, excluding high-velocity shocks as a formation mechanism. Yet, the SiO abundances we detect are mostly 1–2 orders of magnitude higher than those typically assumed in quiescent environments and are often accompanied by other molecular transitions whose column densities cannot be explained with UV-dominated chemical models. Our results challenge the traditional view of SiO production via stellar feedback sources and emphasize the need for observational constraints on the distribution of Si in the gas phase and grain mantles, which are crucial for understanding the physics of grain processing and the diffuse interstellar chemistry.
Measuring the Orbit Drift of Near-Earth Asteroids by the Yarkovsky Effect
Authors: Liu Xin , Hou Xi-Yun , Yang Zhi-Tao , Gan Qing-Bo , Zhang Yao 
Published: June 2023

Abstract
The Yarkovsky effect causes the semimajor axis drift of near-Earth asteroids. The drift can be detected by a precise orbit determination process. Using the proposed algorithm, 2233 out of 27,078 near-Earth asteroids are chosen as the initial candidates. Out of these initial candidates, 769 have a measurable Yarkovsky effect with a signal-to-noise ratio (S/N) larger than 1, and 166 have a measurable Yarkovsky effect with an S/N larger than 3. The ratio between retrograde and prograde near-Earth asteroids is plotted with respect to their size. An average ratio of 2 is found for asteroids with an absolute magnitude between 14 and 21. The measurement work is carried out based on orbit determination software developed by the authors that considers a high-precision dynamical model.
Secular Spin–Orbit Resonances of Black Hole Binaries in AGN Disks
Authors: Li Gongjie , Bhaskar Hareesh Gautham , Kocsis Bence , Lin Douglas N. C. 
Published: June 2023

Abstract
The spin–orbit misalignment of stellar-mass black hole (sBH) binaries provides important constraints on the formation channels of merging sBHs. Here, we study the role of secular spin–orbit resonance in the evolution of an sBH binary component around a supermassive BH (SMBH) in an AGN disk. We consider the sBH’s spin precession due to the J
2 moment introduced by a circum-sBH disk within the warping/breaking radius of the disk. We find that the sBH’s spin–orbit misalignment (obliquity) can be excited via spin–orbit resonance between the sBH binary’s orbital nodal precession and the sBH spin precession driven by a massive circum-sBH disk. Using an α-disk model with Bondi–Hoyle–Lyttleton accretion, the resonances typically occur for sBH binaries with semimajor axis of 1 au and at a distance of ∼1000 au around a 107
M
⊙ SMBH. The spin–orbit resonances can lead to high sBH obliquities and a broad distribution of sBH binary spin–spin misalignments. However, we note that the Bondi–Hoyle–Lyttleton accretion is much higher than that of Eddington accretion, which typically results in spin precession being too low to trigger spin–orbit resonances. Thus, secular spin–orbit resonances can be quite rare for sBHs in AGN disks.
Electron Dynamics in Strong Turbulence within the Diffusion Region during Magnetopause Magnetic Reconnection
Authors: Li Zhi , Pan Xu 
Published: June 2023

Abstract
Magnetic reconnection has been proposed to play an important role in energy dissipation in space plasma. The diffusion region is an essential place for generation of energetic electrons. However, the mechanism responsible for the generation of these energetic electrons in such a confined region remains elusive. Here a diffusion region of asymmetric reconnection is observed at the turbulent magnetopause. The diffusion region is a rather structured region where two dynamical filamentary currents at subion scale were observed. Intense electron flow and nonideal electric field inside the filamentary currents induced significant energy dissipation. Concurrently, the electron parallel temperature between the current layers increases from 58 to 80 eV. Direct evidence indicates that the electrons inside the three-dimensional diffusion region are accelerated by the parallel electric fields inside the current layers and are effectively heated by the turbulence between them.