bluuebunny/crossref_metadata_2025_split huggingface dataset:
Peningkatan Kapasitas Karyawan PT Brand Mark dalam Literasi Finansial
Authors: Irhamni Firly , Mufidha Aulia Ulul , Haridyanti Amyra , Iskandar Muhammad Rijal 
Published: August 2023

<p><em>Tujuan kegiatan pengabdian di PT</em><em>.</em><em> Brand Mark adalah untuk memberikan wawasan dan meningkatkan skill dan kemampuan pengelolaan keuangan pribadi para pegawainya. Sering kali masyarakat yang produktif seperti para pegawai PT</em><em>.</em><em> Brand Mark kurang memperhatikan pengelolaan keuangan personalnya, dengan alasan kesibukan pekerjaan, deadline, dan merasa aman karena memiliki pendapatan rutin. Karena konsumtif dan belanja yang berlebihan, akibatnya perencanaan keuangan di masa depan kurang optimal. </em><em>Metode dan pendekatan yang kami gunakan </em><em>dengan melakukan observasi awal dan FGD pendahuluan kepada 3 karyawan terpilih secara acak, dilanjutkan pendampingan dan seminar tentang pengelolaan keuangan personal. Hasil evaluasi dan post-test dilakukan dengan survei sejumlah pertanyaan terkait pengetahuan dan pemahaman peserta yang diolah dengan </em><em>Wilcoxon signed rank test </em><em>yang menunjukkan peningkatan pengetahuan dan kemampuan signifikan dibanding sebelum pendampingan disampaikan. Dapat disimpulkan bahwa kegiatan ini berhasil memenuhi sasaran dan memiliki kebermanfaatan untuk mitra dengan diperolehnya wawasan baru mengenai pentingnya kesadaran para pegawai dalam memahami konsep literasi keuangan personal dan pengelolaan keuangan dasar.</em></p><p><strong>Kata kunci: <em>Literasi Keuangan, Pegawai, Pengelolaan Keuangan Personal</em></strong><strong><em></em></strong></p>
ANALISIS USAHA TERNAK SAPI PADA KELOMPOK TANI BESARANG DI DESA NATAI SEDAWAK KECAMATAN SUKAMARA KABUPATEN SUKAMARA KALIMANTAN TENGAH
Authors: Mudhita Ida Ketut , Sumiati Alam , Rubiansyah M , Musnaini  
Published: August 2023

Penelitian ini dilakukan di Kelompok Tani Besarang Desa Natai Sedawak Kecamatan Sukamara Kabupaten Sukamara. Tujuan penelitian untuk mengindetifikasi profil kelompok ternak,karakteristik peternak, karakteristik usaha ternak, dan tata laksana usaha ternak, serta menganalisis tingkat pendapatan dan tipologi usaha ternak sapi potong di Kelompok Tani Besarang Desa Natai Sedawak Kecamatan Sukamara. Responden dalam penelitian ini, adalah seluruh anggota Kelompok Tani Besarang yang berjumlah sepuluh peternak. Berdasarkan hasil penelitian diketahui, bahwa profil kelompok Tani Besarang berdiri dari tahun 2016, memiliki 10 anggota. Karakteristik peternak yaitu rata-rata peternak berumur 57 tahun, pendidikan rata-rata SD, pekerjaan utama rata-rata petani., pengalaman beternak rata-rata 12-16 tahun, dan jumlah tanggungan keluarga 3-5 orang sebesar 100%. Permodalan peternak 100% modal individu, dalam status kepemilikan ternak 100% milik sendiri, luas lahan yang digunakan untuk menggembala ternak kurang lebih 50 Ha. Penanganan kesehatan dengan pemberian obat cacing maksimal 6 bulan 1 kali, pemasaran hasil 30% oleh blantik dan 70% jual sendiri, area pemasaran Kecamatan Sukamara 60% dan Kecamatan Pantai Lunci 40%. Pendapatan di Kelompok Tani Besarang peternak sebesar Rp. 63.360.000 dalam 1 tahun dengan hitungan rata-rata dari jumlah semua anggota ternak. Penerimaan sebesar Rp. 85.000.000 dan total biaya produksi Rp. 21.640.000-,. Nilai R/C Ratio sebesar 3,92 menunjukan usaha ternak yang menguntungkan dan kontribusi sebesar 13,86 % dari total pendapatan usaha merupakan usaha sampingan karena kontribusi termasuk < 30%.
Hubungan Kualitas Pelayanan dengan Kepatuhan Pemeriksaan Kehamilan (K4) pada Ibu Hamil TM III di BPM Dyah Surti Gonilan Sukoharjo 2017
Authors: Sari Ajeng Novita , Sab’ngatun Sab’ngatun 
Published: August 2023

Masalah Kesehatan Ibu dan Anak (KIA) merupakan masalah nasional yang perlu mendapat prioritas utama karena sangat menentukan kualitas Sumber Daya Manusia (SDM) pada generasi mendatang. Tingginya Angka Kematian Ibu (AKI) menunjukkan bahwa pelayanan ANC sangat mendesak untuk ditingkatkan baik dari segi jangkauan maupun kualitas pelayanannya.Tujuan penelitian ini adalah untuk mengetahui hubungan kualitas pelayanan dengan kepatuhan pemeriksaan kehamilan (K4) pada ibu hamil Trimester III di BPM Dyah Surti Gonilan Sukoharjo tahun 2017.
Jenis penelitian ini menggunakan deskriptif kuantitatif dengan rancangan cross sectional. Populasi dalam penelitian ini adalah Ibu hamil Trimester III yang melakukan pemeriksaan kehamilan di BPM Dyah Surti Gonilan Sukoharjo dengan sampel sebanyak 37 responden dengan teknik accidental sampling.Teknik pengumpulan data menggunakan kuesioner dan checklist.Teknik analisis data menggunakan chi square.
Hasil penelitian menunjukkan bahwa mayoritas umur responden adalah 20-35 tahun sebanyak 22 orang (59,6%) dengan tingkat pendidikan tinggi sebanyak 27 responen (73,0%) dan mayoritas responden bekerja yaitu sebanyak 24 orang (64,9%). Mayoritas responden yaitu sebanyak 22 orang (59,5%) menyatakan bahwa kualtias pelayanan ANC dalam kategori baik. Mayoritas responden yaitu sebanyak 23 responden (62,2%) menyatakan patuh dalam pemeriksaan kehamilan. Ada hubungan yang bermakna antara kualitas pelayanan ANC dengan kepatuhan pemeriksaan kehamilan Ibu hamil Trimester III yang melakukan pemeriksaan kehamilan di BPM Dyah Surti Gonilan Sukoharjo dengan nilai X2 = 5,268 dan p value0,022 < 0,05.
MENINGKATKAN KETERAMPILAN MENYIMAK CERITA FABEL MELALUI MODEL PAIRED STORYTELLING MELALUI MEDIA WAYANG KARTUN DI KELAS II MI BPPI CISAAT DENGAN TEKNIK PROJECT BASE LEARNING (PJBL)
Authors: Nurkaidah  , Dwi Kartika Susanti  
Published: August 2023

This study was conducted to overcome the problem of lack of enthusiasm and concentration of students when the teacher explains in front of the class in class II MI BPPI Cisaat. The purpose of the study was to improve listening skills to fable stories through the Paired Storytelling model using cartoon puppet media with the application of Project Based Learning (PjBL) techniques in the class.
This study involved 26 students (12 boys and 14 girls) as subjects. Data were collected through observation methods and written tests. The results showed an increase in students' listening skills. In the first cycle, the average class score was 69 with a percentage of listening skills completeness of 70.91% (sufficient category) and learning outcomes completeness of 61.5% (unfinished category). In the second cycle, with the application of the Paired Storytelling model using cartoon puppet media and Project Based Learning (PjBL) techniques, the average class score increased to 82. The percentage of listening skills completeness increased to 81.73% (good category) with a percentage of learning outcomes completeness of 84.6% (complete category).
Comparative analysis between the results of the first and second cycles shows a significant improvement in students' listening skills in dealing with fable stories in class II MI BPPI Cisaat. This research encourages a better and deeper understanding of listening skills through the implemented learning model.
Komunikasi Pemasaran Bolu Amor Sukabumi dalam Meningkatkan Brand Awarenessdi Masa Pandemi Covid-19
Authors: Neskisyah Affan Neskisyah Ramadhan , Melisa Agustina  
Published: August 2023

Bolu Amor Sukabumi implemented Integrated Marketing Communication to increase brand awareness during the Covid-19 pandemic. This research describes Bolu Amor Sukabumi's marketing communication strategy in strengthening brand awareness. The concept of Integrated Marketing Communication (IMC) was used as the basis of this research, involving various marketing activities. A qualitative method with a descriptive approach was used, as well as purposive sampling for the selection of four main informants. The research revealed six elements of integrated marketing communication implemented by Bolu Amor Sukabumi.

First, in the advertising aspect, Bolu Amor Sukabumi focuses on the use of posters, banners, and social media to reach the audience. Second, the Publicity and Public Relations aspect involves collaboration with the wider community, although publicity still needs to be improved. Third, Sales Promotion attracts customers through various attractive promotions. Fourth, Direct Marketing utilizes electronic shopping and practical payment systems. Fifth, Event and Experience involves sponsorship of government activities, schools, charity events, and community empowerment. Sixth, Online and Social Media Marketing involves platforms such as Instagram, Facebook, and TikTok, with a dedicated team producing unique content and attractive designs. In conclusion, Bolu Amor Sukabumi adopted IMC strategies with various approaches to strengthen brand awareness amidst the pandemic.
Lensing in the Blue. II. Estimating the Sensitivity of Stratospheric Balloons to Weak Gravitational Lensing
Authors: McCleary Jacqueline E. , Everett Spencer W. , Shaaban Mohamed M. , Gill Ajay S. , Vassilakis Georgios N. , Huff Eric M. , Massey Richard J. , Benton Steven J. , Brown Anthony M. , Clark Paul , Holder Bradley , Fraisse Aurelien A. , Jauzac Mathilde , Jones William C. , Lagattuta David , Leung Jason S.-Y. , Li Lun , T. Luu Thuy Vy , Nagy Johanna M. , Netterfield C. Barth , Paracha Emaad , Redmond Susan F. , Rhodes Jason D. , Schmoll Jürgen , Sirks Ellen , Tam Sut Ieng 
Published: August 2023

Abstract
The Superpressure Balloon-borne Imaging Telescope (SuperBIT) is a diffraction-limited, wide-field, 0.5 m, near-infrared to near-ultraviolet observatory designed to exploit the stratosphere’s space-like conditions. SuperBIT’s 2023 science flight will deliver deep, blue imaging of galaxy clusters for gravitational lensing analysis. In preparation, we have developed a weak-lensing measurement pipeline with modern algorithms for PSF characterization, shape measurement, and shear calibration. We validate our pipeline and forecast SuperBIT survey properties with simulated galaxy cluster observations in SuperBIT’s near-UV and blue bandpasses. We predict imaging depth, galaxy number (source) density, and redshift distribution for observations in SuperBIT’s three bluest filters; the effect of lensing sample selections is also considered. We find that, in three hours of on-sky integration, SuperBIT can attain a depth of b = 26 mag and a total source density exceeding 40 galaxies per square arcminute. Even with the application of lensing-analysis catalog selections, we find b-band source densities between 25 and 30 galaxies per square arcminute with a median redshift of z = 1.1. Our analysis confirms SuperBIT’s capability for weak gravitational lensing measurements in the blue.
White-light Superflare and Long-term Activity of the Nearby M7-type Binary EI Cnc Observed with GWAC System
Authors: Li Hua-Li , Wang Jing , Xin Li-Ping , Bai Jian-Ying , Han Xu-Hui , Cai Hong-Bo , Huang Lei , Lu Xiao-Meng , Qiu Yu-Lei , Wu Chao , Li Guang-Wei , Deng Jing-Song , Xu Da-Wei , Yang Yuan-Gui , Wang Xiang-Gao , Liang En-Wei , Wei Jian-Yan 
Published: August 2023

Abstract
Stellar white-light flares are believed to play an essential role in the physical and chemical properties of the atmosphere of the surrounding exoplanets. Here we report an optical monitoring campaign on the nearby flaring system EI Cnc carried out by the Ground-based Wide Angle Camera (GWAC) and its dedicated follow-up telescope. A superflare, coming from the brighter component EI CncA, was detected and observed, in which four components are required to properly model the complex decay light curve. The lower limit of flare energy in the R − band is estimated to be 3.3 × 1032 erg. A total of 27 flares are additionally detected from the GWAC archive data with a total duration of 290 hr. The inferred cumulative flare frequency distribution follows a quite shallow power-law function with a slope of β = − 0.50 ± 0.03 over the energy range between 1030 and 1033 erg, which reinforces the trend that stars cooler than M4 show enhanced superflare activity. The flares identified in EI Cnc enable us to extend the τ–E relationship previously established in the white-light superflares of solar-type stars down to an energy as low as ∼1030erg (i.e., by 3 orders): τ ∝ E
0.42±0.02, which suggests a common flare mechanism for stars with a type from M to solar-like and implies an invariant of B
1/3
υ
A in the white-light flares.
Sudden Extreme Obscuration of a Sun-like Main-sequence Star: Evolution of the Circumstellar Dust around ASASSN-21qj
Authors: Marshall Jonathan P. , Ertel Steve , Kemper Francisca , del Burgo Carlos , Otten Gilles P. P. L. , Scicluna Peter , Zeegers Sascha T. , Ribas Álvaro , Morata Oscar 
Published: August 2023

Abstract
ASASSN-21qj is a distant Sun-like star that recently began an episode of deep dimming events after no prior recorded variability. Here we examine archival and newly obtained optical and near-infrared data of this star. The deep aperiodic dimming and absence of previous infrared excess are reminiscent of KIC 8462852 (“Boyajian’s Star”). The observed occultations are consistent with a circumstellar cloud of submicron-sized dust grains composed of amorphous pyroxene, with a minimum mass of 1.50 ± 0.04 × 10−9
M
⊕ derived from the deepest occultations, and a minimum grain size of

0.29

−
0.18

+
0.01

μ
m

assuming a power-law size distribution. We further identify the first evidence of near-infrared excess in this system from NEOWISE 3.4 and 4.6 μm observations. The excess emission implies a total circumstellar dust mass of around 10−6
M
⊕, comparable to the extreme, variable disks associated with terrestrial planet formation around young stars. The quasiperiodic recurrence of deep dips and the inferred dust temperature (ranging from 1800 to 700 K across the span of observations) independently point to an orbital distance of ≃0.2 au for the dust, supporting the occulting material and excess emission being causally linked. The origin of this extended, opaque cloud is surmised to be the breakup of one or more exocometary bodies.
Formation of Gaps in Self-gravitating Debris Disks by Secular Resonance in a Single-planet System. II. Toward a Self-consistent Model
Authors: Sefilian Antranik A. , Rafikov Roman R. , Wyatt Mark C. 
Published: August 2023

Abstract
High-resolution observations of several debris disks reveal structures such as gaps and spirals, suggestive of gravitational perturbations induced by underlying planets. Most existing studies of planet–debris disk interactions ignore the gravity of the disk, treating it as a reservoir of massless planetesimals. In this paper, we continue our investigation into the long-term interaction between a single eccentric planet and an external, massive debris disk. Building upon our previous work, here we consider not only the axisymmetric component of the disk’s gravitational potential, but also the nonaxisymmetric torque that the disk exerts on the planet (ignoring for now only the nonaxisymmetric component of the disk self-gravity). To this goal, we develop and test a semianalytic “N-ring” framework that is based on a generalized (softened) version of the classical Laplace–Lagrange secular theory. Using this tool, we demonstrate that even when the disk is less massive than the planet, not only can a secular resonance be established within the disk that leads to the formation of a wide gap, but that the very same resonance also damps the planetary eccentricity e

p
via a process known as resonant friction. The resulting gap is initially nonaxisymmetric (akin to those observed in HD 92945 and HD 206893), but evolves to become more axisymmetric (similar to that in HD 107146) as e

p
(t) → 0 with time. We also develop analytic understanding of these findings, finding good quantitative agreement with the outcomes of the N-ring calculations. Our results may be used to infer both the dynamical masses of (gapped) debris disks and the dynamical history of the planets interior to them, as we exemplify for HD 206893.
Calculation and Uncertainty of Fast Radio Burst Structure Based on Smoothed Data
Authors: Sutinjo Adrian T. , Scott Danica R. , James Clancy W. , Glowacki Marcin , Bannister Keith W. , Cho 조 Hyerin 혜린 , Day Cherie K. , Deller Adam T. , Perrett Timothy P. , Shannon Ryan M. 
Published: August 2023

Abstract
Studies of the time-domain structure of fast radio bursts (FRBs) require an accurate estimate of the FRB dispersion measure in order to recover the intrinsic burst shape. Furthermore, the exact dispersion measure is itself of interest when studying the time evolution of the medium through which multiple bursts from repeating FRBs propagate. A commonly used approach to obtain the dispersion measure is to take the value that maximizes the FRB structure in the time domain. However, various authors use differing methods to obtain this structure parameter and do not document the smoothing method used. Furthermore, there are no quantitative estimates of the error in this procedure in the FRB literature. In this article, we present a smoothing filter based on the discrete cosine transform, and show that computing the structure parameter by summing the squares of the derivatives and taking the square root (that is, the 2-norm,

Σ

(
d

/

dt
)

2

) immediately lends itself to the calculation of the uncertainty of the structure parameter. We illustrate this with FRB 20181112A and FRB 20210117A data, which were detected by the Australian Square Kilometre Array Pathfinder, and for which high-time-resolution data are available.
Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations
Authors: Vermette Benjamin , Salcedo Ciro , Mori Kaya , Gerber Julian , Yoon Kyung Duk , Bridges Gabriel , Hailey Charles J. , Haberl Frank , Hong Jaesub , Grindlay Jonathan , Ponti Gabriele , Ramsay Gavin 
Published: August 2023

Abstract
We report timing and broadband spectral analysis of a Galactic X-ray source, CXOGBS J174517.0−321356 (J1745), with a 614 s periodicity. Chandra discovered the source in the direction of the Galactic Bulge. Gong proposed that J1745 was either an intermediate polar (IP) with a mass of ∼1 M
⊙, or an ultracompact X-ray binary (UCXB). To confirm J1745's nature, we jointly fit XMM-Newton and NuSTAR spectra, ruling out a UCXB origin. We have developed a physically realistic model that considers a finite magnetosphere radius, X-ray absorption from the preshock region, and reflection from the white-dwarf (WD) surface to properly determine the IP properties, especially its WD mass. To assess systematic errors on the WD mass measurement, we consider a broad range of specific accretion rates (

m

̇

=
0.6
–
44

g cm−2 s−1) based on the uncertain source distance (d = 3–8 kpc) and fractional accretion area (f = 0.001–0.025). Our model properly implements the fitted accretion column height in the X-ray reflection model and accounts for the underestimated mass accretion rate due to the (unobserved) soft X-ray blackbody and cyclotron cooling emissions. We found that the lowest accretion rate of

m

̇

= 0.6 g cm−2 s−1, which corresponds to the nearest source distance and maximum f value, yields a WD mass of (0.92 ± 0.08)M
⊙. On the other hand, as long as the accretion rate is

m

̇

≳
3

g cm−2 s−1, the WD mass is robustly measured to be (0.81 ± 0.06)M
⊙, nearly independent of

m

̇

. The derived WD mass range is consistent with the mean WD mass of nearby IPs. Assuming spin equilibrium between the WD and accretion disk, we constrained the WD magnetic field to B ≳ 7 MG, indicating that it could be a highly magnetized IP. Our analysis presents the most comprehensive methodology for constraining the WD mass and B field of an IP by consolidating the effects of cyclotron cooling, finite magnetospheric radius, and accretion column height.
Can Cold Jupiters Sculpt the Edge-of-the-multis?
Authors: Sobski Nicole , Millholland Sarah C. 
Published: August 2023

Abstract
Compact systems of multiple close-in super-Earths/sub-Neptunes (compact multis) are a ubiquitous outcome of planet formation. It was recently discovered that the outer edges of compact multis are located at smaller orbital periods than expected from geometric and detection biases alone, suggesting some truncation or transition in the outer architectures. Here we test whether this edge-of-the-multis might be explained in any part by distant giant planets in the outer regions (≳1 au) of the systems. We investigate the dynamical stability of observed compact multis in the presence of hypothetical giant (≳0.5 M
Jup) perturbing planets. We identify what parameters would be required for hypothetical perturbing planets if they were responsible for dynamically sculpting the outer edges of compact multis. Edge-sculpting perturbers are generally in the range of P ∼ 100–500 days for the average compact multi, with most between P ∼ 200 and 300 days. Given the relatively close separation, we explore the detectability of the hypothetical edge-sculpting perturbing planets, finding that they would be readily detectable in transit and radial velocity data. We compare to observational constraints and find it unlikely that dynamical sculpting from distant giant planets contributes significantly to the edge-of-the-multis. However, this conclusion could be strengthened in future work by a more thorough analysis of the detection yields of the perturbing planets.
Universal Upper End of the Stellar Initial Mass Function in the Young and Compact LEGUS Clusters
Authors: Jung Dooseok Escher , Calzetti Daniela , Messa Matteo , Heyer Mark , Sirressi Mattia , Linden Sean T. , Adamo Angela , Chandar Rupali , Cignoni Michele , Cook David O. , Dobbs Clare L. , Elmegreen Bruce G. , Evans Aaron S. , Fumagalli Michele , Gallagher John S. , Hunter Deidre A. , Johnson Kelsey E. , Kennicutt Robert C. , Krumholz Mark R. , Schaerer Daniel , Sabbi Elena , Smith Linda J. , Tosi Monica , Wofford Aida 
Published: August 2023

Abstract
We investigate the variation in the upper end of the stellar initial mass function (uIMF) in 375 young and compact star clusters in five nearby galaxies within ∼5 Mpc. All the young stellar clusters (YSCs) in the sample have ages ≲ 4 Myr and masses above 500 M
⊙, according to standard stellar models. The YSC catalogs were produced from Hubble Space Telescope images obtained as part of the Legacy ExtraGalactic UV Survey (LEGUS) Hubble treasury program. They are used here to test whether the uIMF is universal or changes as a function of the cluster’s stellar mass. We perform this test by measuring the Hα luminosity of the star clusters as a proxy for their ionizing photon rate, and charting its trend as a function of cluster mass. Large cluster numbers allow us to mitigate the stochastic sampling of the uIMF. The advantage of our approach relative to previous similar attempts is the use of cluster catalogs that have been selected independently of the presence of Hα emission, thus removing a potential sample bias. We find that the uIMF, as traced by the Hα emission, shows no dependence on cluster mass, suggesting that the maximum stellar mass that can be produced in star clusters is universal, in agreement with previous findings.
La donnée, objet et outil de la médiation scientifique : l’exemple du Dôme
Authors: Millet François 
Published: August 2023

Le Dôme est un espace culturel qui mène et accompagne des projets de recherche participative. La question des données est au cœur des méthodologies qu’il déploie, que ce soit avec son fablab, dans l’héritage de la culture du logiciel libre, ou en invitant les participants à recueillir des données scientifiques pour nourrir des programmes de recherche ou d’innovation. Constituant tantôt la « matière première », tantôt la finalité des projets du Dôme, François Millet analyse pourquoi les données impactent sa pérennité, voire son modèle économique, comme elles imposent de mettre à jour certaines modalités déontologiques dans ses pratiques de médiation.