bluuebunny/crossref_metadata_2025_split huggingface dataset:
KUALITAS PELAYANAN PUSKESMAS ASEMBAGUS DAN KEPUASAN PASIEN DI KECAMATAN ASEMBAGUS KABUPATEN SITUBONDO
Authors: Susanto Hari 
Published: May 2024

Kesehatan merupakan hal yang sangat diinginkan oleh semua makhluk hidup di muka bumi ini. Karena kondisi tubuh yang sakit, akan membuat seseorang menjadi tidak produktif, karena itu, kesehatan adalah kebutuhan utama bagi setiap manusia. sehingga diperlukan adanya pelayanan kesehatan yang layak. Hal ini menjadikan lembaga kesehatan dituntut untuk meningkatkan kualitas pelayanannya agar lebih baik, salah satunya adalah puskesmas yang ada di masing-masing kecamatan. Puskesmas merupakan organisasi fungsional yang langsung memberikan pelayanan kepada masyarakat tertentu dalam bentuk usaha-usaha kesehatan setiap orang. Sedangkan fungsi puskesmas di antaranya adalah menyembuhkan penyakit dan pemulihan kesehatan perorangan, memelihara dan meningkatkan kesehatan serta mencegah penyakit. Puskesmas memberikan pelayanan yang berkualitas agar dapat memberikan rasa puas pada masyarakat/pasien. Kepuasan pasien dalam pelayanan kesehatan sangat penting untuk diperhatikan karena dapat menggambarkan kualitas pelayanan di tempat pelayanan kesehatan tersebut. Penelitian ini bertujuan ingin melihat adanya keterpengaruhan kualitas pelayanan terhadap kepuasan pasien yang dilakukan oleh Puskesmas Asembagus Kabupaten Situbondo, dan mengetahui berapa besarnya pengaruh tersebut. Penelitian dilaksanakan di Puskesmas Asembangus Kabupaten Situbondo dengan menggunakan metode kuantitatif. Sampel penelitian adalah pasien Puskesmas Asembagus secara isendetil berjumlah 41 orang. Hasil penelitian menyatakan bahwa kualitas pelayanan berpengaruh terhadap kepuasan pasien halmana diperoleh Fhitung sebesar 5,685 > Ftabel = 4,09. Besarnya pengaruh kualitas pelayanan terhadap kepuasan pasien sebesar 2,384 (lebih besar daripada t tabel=2,02). Nilai R2 sebesar 0,127 (12,7%), menunjukkan bahwa persentase pengaruh variabel kualitas pelayanan mampu menjelaskan sebesar 12,7% variasi kepuasan pasien di Puskesmas Asembagus Kabupaten Situbondo, sedangkan sisanya sebesar 87,3% dipengaruhi oleh faktor varibel lainnya.
PENGAWASAN, MOTIVASI PIMPINAN DAN KINERJA PEGAWAI DI DINAS PEMBERDAYAAN MASYARAKAT DAN DESA KABUPATEN SITUBONDO
Authors: Susanto Hari 
Published: May 2024

Keberhasilan organisasi pemerintah dapat diukur dari kinerja pegawainya yang didukung diantaranya oleh keuangan, tata kelola serta dinamika eksternalnya. Upaya meningkatkan kinerja pegawainya dengan meningkatkan kualitas dan kuantitas sumberdaya manusia, di antaranya melalui pengawasan dan motivasi para pegawainya. Dilakukan pengawasan karena hal ini untuk mengurangi kesalahan serta penyimpangan dalam dalam bekerja. Pengawasan bertujuan agar hasil pekerjaan diperoleh secara efisien dan efektif sesuai dengan rencana yang ditetapkan oleh organisasi. Sedangkan motivasi pimpinan berfungsi memberikan inspirasi, semangat dan dorongan kepada bawahannya untuk bekerja sesuai tujuan organisasinya. Motivasi adalah dorongan yang menciptakan kegairahan kerja seseorang agar mau bekerja sama, bekerja efektif dan terintegrasi dengan segala daya upaya untuk mencapai tujuan. Penelitian bertujuan ingin mengetahui adanya pengaruh pengawasan dan motivasi pimpinan terhadap kinerja pegawai, serta mengetahui berapa besarnya pengaruh tersebut. Penelitian dengan metode kuantitatif dilaksanakan di Di Dinas Pemberdayaan Masyarakat Dan Desa Kabupaten Situbondo. Sampel penelitian adalah seluruh pegawai berjumlah 45 orang. Hasil penelitian menyatakan bahwa pengawasan dan motivasi secara simultan berpengaruh terhadap kinerja pegawai, dimana diperoleh Fhitung sebesar 61,384>Ftabel=3,22. Besarnya pengaruh pengawasan(tx1) sebesar 9,555 dan motivasi(tx2) sebesar 2,872 terhadap kinerja pegawai. Nilai keduanya lebih besar daripada nilai ttabel sebesar 2.014.Nilai R2 sebesar 0,746 (74,6%), menunjukkan persentase keterikatan hubungan antara kedua variabel mampu menjelaskan sebesar 74,6% terhadap variabel kinerja pegawai, sisanya sebesar 25,4% dipengaruhi faktor varibel lainnya.
PENGEMBANGAN SUMBER DAYA APARATUR BERBASIS KOMPETENSI PADA PEMERINTAH KABUPATEN SITUBONDO
Authors: Fitriyah Nina Sa'idah 
Published: May 2024

Sumber daya manusia merupakan faktor yang paling penting dan paling menentukan dalam setiap organisasi. Sumber daya manusia merupakan penentu jalan tidaknya ataupun maju mundurnya organisasi. Sebaik apapun sistem yang telah disusun atau dilengkapi dengan apapun sarana dan prasarana yang tersedia dalam organisasi, tanpa didukung oleh keberadaan sumber daya manusia yang memiliki kemampuan yang memadai, maka berbagai kelengkapan tersebut tidak akan berarti banyak bagi keberadaan organisasi, dengan sumber daya manusia pula, sistem sarana dan prasarana yang ada dalam organisasi dapat terus disempurnakan sesuai dengan perkembangan kebutuhan bagi percepatan menyelesaikan tugas. Sumber daya aparatur yang berkualitas merupakan prasyarat dalam meningkatkan mutu penyelenggaraan negara serta kepada masyarakat. Dalam undang-undang Nomor 5 tahun 2014 (pasal 70) ditegaskan: (1) setiap pegawai ASN memiliki hak dan kesempatan umtuk pengembangan kompetensi, antara lain melaluipendidikan dan pelatihan (diklat), kursus, seminar, dan penataran; (2) dalam pengembangan kompetensi setiap instansi Pemerintah wajib menyusun rencana pengembangan kompetensi tahunan.
Jenis penelitian ini menggunakan penelitian deskriptif dengan metode pendekatan kualitatif. Lokasi penelitian di Badan Pengembangan dan Kepegawaian Sumber Daya Manusia Kabupaten Situbondo Jawa Timur. Teknik penentu informan menggunakan purposive sampling yang meliputi Dinas Kepala dinas, Sekretaris Dinas, Kepala Bidang, Aparatur Sipil Negara pada Badan Pengembangan dan Kepegawaian Sumber Daya Manusia sebagai Keynote adalah Kepala Bidang Pengembangan Sumber daya Manusia. Jenis data yang digunakan adalah data sekunder dan primer. Teknik pengumpulan data menggunakan wawancara mendalam, observasi dan study pustaka. Teknik analisis data dalam penelitian ini dilakukan dalam tiga tahap yaitu reduksi data, penyajian data dan penarikan kesimpulan.
Hasil penelitian ini adalah Program pengembangan sumber daya aparatur yang diterapkan akan optimal apabila seluruh aparatur sipil negara memiliki tiga kompetensi yang berkembang (kompetensi manajerial, kompetensi teknis, kompetensi sosial kultural), sehingga menghasilkan aparatur sipil yang professional. Sehingga dengan ketiga kompetensi yang diperoleh aparatur sipil negara dapat membangun hardskill dan softskill aparatur sipil negara.
Visual word identification beyond common words: The role of font and letter case in brand names
Authors: Labusch Melanie , Duñabeitia Jon Andoni , Perea Manuel 
Published: May 2024

AbstractWhile abstractionist theories of visual word recognition propose that perceptual elements like font and letter case are filtered out during lexical access, instance-based theories allow for the possibility that these surface details influence this process. To disentangle these accounts, we focused on brand names embedded in logotypes. The consistent visual presentation of brand names may render them much more susceptible to perceptual factors than common words. In the present study, we compared original and modified brand logos, varying in font or letter case. In Experiment 1, participants decided whether the stimuli corresponded to existing brand names or not, regardless of graphical information. In Experiment 2, participants had to categorize existing brand names semantically – whether they corresponded to a brand in the transportation sector or not. Both experiments showed longer response times for the modified brand names, regardless of font or letter-case changes. These findings challenge the notion that only abstract units drive visual word recognition. Instead, they favor those models that assume that, under some circumstances, the traces in lexical memory may contain surface perceptual information.
Ameliorating Effects of Arsenic-Induced Toxicity On The Histology Of Vagina And Reproductive Hormones Of Female Sprague Dawley Rats
Authors: Mir Amaidah , Mir Urfa Zaryab , Yasmeen Maria , Ahmad Mushtaq , Huma Kanwal , Khurshid Iram Kehkashan 
Published: May 2024

Objective: To find out the toxic effects of arsenic on the histology of the vagina and reproductive hormones of female Sprague Dawley rats.
Methods: 60 female Sprague Dawley rats were divided into control group A and experimental group B with 30 rats in each group. The gross weight of all the rats was checked before and at the end of the experiment. After one week of acclimatization, the control group was administered 10ml of distilled water by oral gavage daily for 14 days and the experimental group was administered 4µg of sodium arsenite dissolved in 10ml of distilled water by oral gavage daily for 14 days. After being euthanized by chloroform inhalation on day 15, blood from each rat was drawn by a single intra-cardiac puncture and stored for biochemical analysis. After that, rats were sacrificed and the whole reproductive tract was removed and vaginal sections were prepared and stained with hematoxylin and eosin (H&E ). The histological parameters were analyzed by using Image J software. Whereas, biochemical parameters e.g. serum LH and FSH levels were analyzed by ELISA.
Results: After exposure to a low dose of arsenic administered for a short period, the gross weight of rats, weight of reproductive tract, height of vaginal epithelium and serum FSH and LH values were significantly reduced in experimental animals as compared to control animals with p-value < 0.05.
Conclusion: Low dose of arsenic given via contaminated drinking water for a short period is very toxic to the female reproductive tract which is evident by the histological changes in the vagina and deranged hormonal profile of female Sprague Dawley rats.
Keywords: Arsenic, FSH, Free radicals, LH, Oxidative stress, Vagina.
An Empirical Study On Imaging Sensitivity Of SKA1-LOW Based on Point Source Sensitivity
Authors: Xie 谢 Zhaotong 兆彤 , Wang 王 Feng 锋 , Mei 梅 Ying 盈 , Deng 邓 Hui 辉 , Zhu 朱 Yunjin 云瑾 
Published: May 2024

Abstract
The Square Kilometre Array (SKA) radio telescope will achieve unparalleled sensitivity and angular resolution, substantially progressing our research into the formation and development of the early universe. Sensitivity is one of the most critical telescope metrics, often used to determine the observing mode and observing time of a radio source. It is also used to determine imaging parameters to balance imaging sensitivity and spatial resolution during data processing. In this paper, to meet the needs of continuum imaging pipeline data processing for the SKA1-LOW telescope, we derive equations for point-source-sensitivity (PSS) calculations under multichannel, multipolarization, discrete frequency sampling, discrete time sampling, and different weighting schemes. After validating the correctness of the equation, we improved and refined the sensitivity calculation application in the Radio Astronomy Simulation, Calibration, and Imaging Library, and further calculated the variation of the PSS versus angular resolution for the full-scale SKA1-LOW with different weighting schemes, and provided SKA1-LOW broadband image performance as functions of angular scale for four frequencies. These results can provide not only a theoretical basis for the construction and commissioning of the SKA1-LOW telescope but also guidance for imaging processing in future scientific data processing.
Discovery of a Second Eclipsing, ​​​​​Bursting Neutron Star Low-mass X-Ray Binary in the Globular Cluster Terzan 6
Authors: van den Berg Maureen , Homan Jeroen , Heinke Craig O. , Pooley David A. , Wijnands Rudy , Bahramian Arash , Miller-Jones James C. A. 
Published: May 2024

Abstract
We have analyzed Chandra and Suzaku observations of the globular cluster Terzan 6, made when the recurrent transient GRS 1747–312 was in quiescence. Our analysis reveals the presence of a second eclipsing, bursting neutron star low-mass X-ray binary in the central regions of the cluster, in addition to GRS 1747–312. The new source, which we name Terzan 6 X2, is located only ∼0.″7 away from GRS 1747–312 in the 2021 Chandra images. The detection of a 5.14 ks long eclipse in the light curve of X2 at a time not predicted by the ephemeris of GRS 1747–312 confirms that it is an unrelated source. Using the Suzaku light curve from 2009, which, in addition to a type I X-ray burst, also showed an eclipse-like feature, we constrain the orbital period to be longer than 16.27 hr. The 0.5–10 keV luminosities of X2 vary in the range of ∼0.24–5.9 × 1034 erg s−1 on timescales of months to years. We have identified a plausible optical counterpart of X2 in Hubble Space Telescope F606W and F814W images. This star varied by 2.7 mag in V
606 between epochs separated by years. In the cluster color–magnitude diagram, the variable counterpart lies in the blue-straggler region when it was optically bright, about 1.1–1.7 mag above the main-sequence turn-off. From the orbital period–density relation of Roche-lobe filling stars, we find the mass-donor radius to be ≳0.8 R
⊙.
Bayesian Survey of the Dense Matter Equation of State Built upon Skyrme Effective Interactions
Authors: Beznogov Mikhail V. , Raduta Adriana R. 
Published: May 2024

Abstract
The nonrelativistic model of nuclear matter (NM) with zero-range Skyrme interactions is employed within a Bayesian approach in order to study the behavior of the neutron star (NS) equation of state (EOS). A minimal number of constraints from nuclear physics and ab initio calculations of pure neutron matter (PNM) are imposed together with causality and a lower limit on the maximum mass of an NS to all our models. Our key result is that accounting for correlations among the values that the energy per neutron in PNM takes at various densities and that are typically disregarded efficiently constrains the behavior of the EOS at high densities. A series of global NS properties, e.g., maximum mass, central density of the maximum mass configuration, minimum NS mass that allows for direct URCA, and radii of intermediate and massive NSs, appear to be correlated with the value of effective neutron mass in PNM at 0.16 fm−3. Together with similar studies in the literature our work contributes to a better understanding of the NS EOS as well as its link with the properties of dense NM.
Probing Electromagnetic Gravitational-wave Emission Coincidence in a Type I Binary-driven Hypernova Family of Long Gamma-Ray Bursts at Very High Redshift
Authors: Bianco C. L. , Mirtorabi M. T. , Moradi R. , Rastegarnia F. , Rueda J. A. , Ruffini R. , Wang 王 Y. 瑜 , Della Valle M. , Li 李 Liang 亮 , Zhang 张 S. R. 书瑞 
Published: May 2024

Abstract
The repointing time of the X-Ray Telescope (XRT) instrument on the Neil Gehrels Swift Observatory satellite has posed challenges in observing and studying the early X-ray emissions within ≈40 s after a gamma-ray burst (GRB) trigger. To address this issue, we adopt a novel approach that capitalizes on the cosmological time dilation in GRBs with redshifts ranging from 3 to 9. Applying this strategy to Swift/XRT data, we investigate the earliest X-ray emissions of 368 GRBs from the Swift catalog, including short and long GRBs. We compare the observed time delay between the GRB trigger and the initial Swift/XRT observation, measured in the GRB observer frame, and the corresponding cosmological rest-frame time delay (RTD). This technique is here used in the analysis of GRB 090423 at z = 8.233 (RTD ∼8.2 s), GRB 090429B at z ≈ 9.4 (RTD ∼10.1 s), and GRB 220101A at z = 4.61 (RTD ∼14.4 s). The cosmological time dilation enables us to observe the very early X-ray afterglow emission in these three GRBs. We thus validate the observation of the collapse of the carbon–oxygen core and the coeval newborn neutron star (νNS) formation triggering the GRB event in the binary-driven hypernova (BdHN) scenario. We also evidence the νNS spin-up due to supernova ejecta fallback and its subsequent slowing down due to the X-ray/optical/radio synchrotron afterglow emission. A brief gravitational-wave signal may separate the two stages owing to a fast-spinning νNS triaxial-to-axisymmetric transition. We also analyze the long GRB redshift distribution for the different BdHN types and infer that BdHNe II and III may originate the NS binary progenitors of short GRBs.
CHANG-ES. XXX. 10 kpc Radio Lobes in the Sombrero Galaxy
Authors: Yang Yang , Li Jiang-Tao , Wiegert Theresa , Li Zhiyuan , Guo Fulai , Irwin Judith , Wang Q. Daniel , Dettmar Ralf-Juergen , Beck Rainer , English Jayanne , Ji Li 
Published: May 2024

Abstract
We report the discovery of the 10 kpc scale radio lobes in the Sombrero galaxy (NGC 4594), using data from the Continuum Halos in Nearby Galaxies—an Expanded Very Large Array Survey project. We further examine the balance between the magnetic pressure inside the lobes and the thermal pressure of the ambient hot gas. At the radii r of ∼(1–10) kpc, the magnetic pressure inside the lobes and the thermal pressure of the ambient hot gas are generally in balance. This implies that the jets could expand into the surroundings to at least r ∼ 10 kpc. The feedback from the active galactic nucleus jet responsible for the large-scale lobes may help to explain the unusually high X-ray luminosity of this massive quiescent isolated disk galaxy, although more theoretical work is needed to further examine this possibility.
Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655−40
Authors: Keshet Noa , Behar Ehud , Kallman Timothy R. 
Published: May 2024

Abstract
Supernovae are responsible for the elemental enrichment of the galaxy, and some are postulated to leave behind a black hole. In a stellar binary system, the supernova pollutes its companion, and the black hole can accrete back its own debris and emit X-rays. In this sequence of events, which is only poorly understood, winds are ejected and observed through X-ray absorption lines. Measuring abundances of elements in the wind can lead to inferences about the historical explosion and possibly identify the long-gone progenitor of the compact object. Here, we reanalyze the uniquely rich X-ray spectrum of the 2005 outburst of GRO J1655−40. We reconstruct the absorption measure distribution (AMD) of the wind and find that it increases sharply with ionization from H-like O up to H-like Ca and then flattens out. The AMD is then used to measure the relative abundances of 18 different elements. The present abundances are in partial agreement with a previous work with discrepancies mostly for low-Z elements. The overabundance of odd-Z elements hints at a high-metallicity, high-mass (≃25 M
⊙) progenitor. Interestingly, the abundances are different from those measured in the companion atmosphere, indicating that the wind entrains lingering ambient supernova debris. This can be expected since the current total stellar mass of the binary (<10 M
⊙) is much less than the progenitor mass.
TriOS Schwarzschild Orbit Modeling: Robustness of Parameter Inference for Masses and Shapes of Triaxial Galaxies with Supermassive Black Holes
Authors: Pilawa Jacob , Liepold Emily R. , Ma Chung-Pei 
Published: May 2024

Abstract
Evidence for the majority of the supermassive black holes in the local Universe has been obtained dynamically from stellar motions with the Schwarzschild orbit superposition method. However, there have been only a handful of studies using simulated data to examine the ability of this method to reliably recover known input black hole masses M
BH and other galaxy parameters. Here, we conduct a comprehensive assessment of the reliability of the triaxial Schwarzschild method at simultaneously determining M
BH, stellar mass-to-light ratio M*/L, dark matter mass, and three intrinsic triaxial shape parameters of simulated galaxies. For each of 25 rounds of mock observations using simulated stellar kinematics and the TriOS code, we derive best-fitting parameters and confidence intervals after a full search in the 6D parameter space with our likelihood-based model inference scheme. The two key mass parameters, M
BH and M*/L, are recovered within the 68% confidence interval, and other parameters are recovered between the 68% and 95% confidence intervals. The spatially varying velocity anisotropy of the stellar orbits is also well recovered. We explore whether the goodness-of-fit measure used for galaxy model selection in our pipeline is biased by variable complexity across the 6D parameter space. In our tests, adding a penalty term to the likelihood measure either makes little difference, or worsens the recovery in some cases.
Infrared Properties of Carbon Stars in Our Galaxy
Authors: Suh Kyung-Won 
Published: May 2024

Abstract
We explore the characteristics of carbon stars within our Galaxy through a comprehensive analysis of observational data spanning visual and infrared (IR) bands. Leveraging data sets from IRAS, the Infrared Space Observatory, Akari, the Midcourse Space Experiment, the Two Micron All Sky Survey, the Wide-field Infrared Survey Explorer (WISE), Gaia DR3, AAVSO, and the SIMBAD object database, we conduct a detailed comparison between the observational data and theoretical models. To facilitate this comparison, we introduce various IR two-color diagrams (2CDs), IR color–magnitude diagrams (CMDs), and spectral energy distributions (SEDs). We find that the CMDs, which utilize the latest distance and extinction data from Gaia DR3 for a substantial number of carbon stars, are very useful for distinguishing carbon-rich asymptotic giant branch (CAGB) stars from extrinsic carbon stars that are not in the AGB phase. To enhance the accuracy of our analysis, we employ theoretical radiative transfer models for dust shells around CAGB stars. These theoretical dust shell models demonstrate a commendable ability to approximate the observations of CAGB stars across various SEDs, 2CDs, and CMDs. We present the infrared properties of known pulsating variables and explore the infrared variability of the sample stars by analyzing WISE photometric data spanning the last 14 years. Additionally, we present a novel catalog of CAGB stars, offering enhanced reliability and a wealth of additional information.