bluuebunny/crossref_metadata_2025_split huggingface dataset:
IMPLEMENTASI PROGRAM CORPORATE SOCIAL RESPONSIBILITY (CSR) DI PT. BANK PEMBANGUNAN DAERAH KALIMANTAN TENGAH
Authors: DIPERJA PURBA  , Riamona S.Tulis  
Published: February 2021

Fokus penelitian ini adalah Implementasi Program Corporate Social Responsibility (CSR) di PT. Bank Pembangunan Daerah Kalimantan Tengah. Rumusan masalah adalah bagaimana implementasi program Corporate Social Responsibility (CSR) di PT. Bank Pembangunan Daerah Kalimantan Tengah? Serta faktor-faktor apa saja yang menjadi penghambat implementasi program Corporate Social Responsibility (CSR) di PT. Bank Pembangunan Daerah Kalimantan Tengah?
Teori yang digunakan peneliti yaitu teori Implementasi Kebijakan dari Van Metter dan Van Horn yang dipengaruhi oleh enam variabel yaitu ukuran dan tujuan kebijakan, sumberdaya, karakteristik agen pelaksana, sikap/kecenderungan (disposition) para agen pelaksana, komunikasi antar organisasi dan aktivitas pelaksana, lingkungan sosial, ekonomi dan politik. Penelitian ini menggunakan metode penelitian kualitatif deskriptif. Data yang diperoleh berdasarkan informasi dari staff bagian CSR PT. Bank Pembangunan Daerah Kalimantan Tengah dan masyarakat penerima bantuan dana program CSR itu sendiri. Teknik pengumpulan data berupa observasi, wawancara dan dokumentasi. Selain itu teknik analisis datanya berupa tahap reduksi data, penyajian data dan penarikan kesimpulan/ verifikasi.
Hasil penelitian implementasi program CSR di PT. Bank Pembangunan Daerah Kalimantan Tengah belum terlaksana dengan optimal, hal ini terjadi karena sumber daya manusia yang mengelola CSR masih kurang mumpuni serta tidak ada divisi khusus yang mengelola CSR itu sendiri sehingga program CSR yang dilaksanakan Bank Kalteng selama ini tidak berjalan dengan baik.
KUALITAS PELAYANAN PEGAWAI KELURAHAN MENTENG KOTA PALANGKA RAYA DALAM PENERBITAN SURAT KETERANGAN TANAH (SKT)
Authors: IRMA DAMAYANTI BR PADANG  
Published: February 2021

Dalam melaksanakan pelayanan yang baik, Kantor Kelurahan Menteng Kota Palangka Raya perlu memperhatikan kualitas pelayanan yang diberikan melalui Transparansi, akuntabilitas, kondisional, partisipatif, kesamaanhak, dan keseimbangan hak dan kewajiban. Hal ini bertujuan untuk meningkatkan yang diinginkan oleh masyarakat itu sendiri. Kantor Kelurahan Menteng Kota Palangka Raya adalah salah satu pelayanan yang bersinggungan langsung dengan masyarakat, tentu saja harus ada upaya-upaya yang kongkrit dari pihak Kelurahan Menteng Kota Palangka Raya untuk meningkatkan layanan demi kenyamanan dan kepuasan seluruh masyarakat selaku menerima pelayanan dari pegawai.
Metode penelitian yang digunakan adalah metode kualitatif deskriptif. Dimana metode ini digunakan untuk mengetahui kualitas pelayanan pegawai yang diberikan oleh Kantor Kelurahan Menteng Kota Palangka Raya, subjek peneliti dari penelitian ini adalah Seksi Pemerintahan, dan masyarakat sekitar di Kelurahan Menteng Kota Palangka Raya yang pernah mengurus Surat Keterangan Tanah di instansi tersebut. Sedangkan untuk teknik pengumpulan data dilakukan melalui observasi, wawancara, dan dokumentasi.
Kesimpulan yang diperoleh dari penelitian ini menunjukkan bahwa kualitas pelayanan Kantor Kelurahan Menteng Kota Palangka Raya masih kurang maksimal. Hal ini dapat dilihat masih ada keluhan masyarakat terkait pelayanan yang diberikan.Kurangnya tanggungjawab dalam pelayanan, adanya diskriminasi antara masyarakat yang mengurus SKT dan adanya kendala-kendala yang dihadapi masyarakat, dan tidak ada kotak saran diKelurahan Menteng Kota Palangka Raya untuk menampung aspirasi masyarakat.
Partnership Model for Optimizing the Use of Village Funds
Authors: Mukhtar Sarman  
Published: February 2021

Since 2015, the Government has allocated village development funds in the form of Village Fund policies of IDR 20.7 trillion, then in 2016 it increased to IDR 46.9 trillion, and continues to increase in the following years. However, based on field research in a number of regions in Indonesia, it turns out that the use of Village Funds is not optimal, some of which have been proven wrongly targeted, not transparent in use, and not accountable in reporting. The aspect of planning activities and the quality of human resources implementing policies and coordination between parties that should play a role are still a major problem.
The PPP (Public-Private Partnership) model is actually intended for the development of large-scale projects, such as the construction of highways or seaports and airports. But by taking the substance of cooperation from the parties that each have strengths, the PPP model (and its variants) may be applicable in the use of Village Funds. Using secondary data analysts, the following article discusses the theoretical aspects of the advantages of the PPP model. This model is juxtaposed with cases of success in building the economic self-reliance of rural communities with the help of private parties and academics. It is assumed that the partnership model can be an alternative solution to further optimize the use of Village Funds in order to reduce poverty in rural areas.
ANALISIS INDEKS KEPUASAN MASYARAKAT DI KANTOR DINAS KEPENDUDUKAN DAN PENCATATAN SIPIL KOTA PALANGKA RAYA
Authors: Mahda Cahyati Ningruma  , Bhayu Rhama  , Imanuel Jaya  
Published: February 2021

Pelayanan publik yang berkualitas adalah pelayanan yang mampu memenuhi harapan dan melampaui harapan-harapan dari masyarakat yang dilayani. Beberapa masyarakat mengeluhkan pelayanan publik yang diberikan oleh Kantor Dinas Kependudukan dan Pencatatan Sipil Kota Palangka Raya. Penelitian ini bertujuan untuk menganalisis indeks kepuasan masyarakat terhadap pelayanan publik di Kantor Dinas Kependudukan dan Pencatatan Sipil Kota Palangka Raya yang mengacu pada Kepmenpan Nomor 25 Tahun 2004 dengan menggunakan teori dimensi SERVQUAL oleh Zeithaml et.al (1990) yaitu terdiri dari dimensi tangible (berwujud), reliability (kehandalan), responsiveness (respon/ketanggapan), assurance (jaminan), dan empathy (empati).
Metode yang digunakan dalam penelitian ini adalah penelitian kuantitatif deskriptif dengan menggunakan pendekatan metode survey. Teknik pengambilan sampel menggunakan teknik non probability sampling dengan jenis accidental sampling. Jumlah sampel dalam penelitian ini adalah 100 responden. Teknik pengumpulan data dilakukan dengan cara observasi, kuesioner (angket) dan dokumentasi.
Hasil penelitian menunjukkan bahwa nilai indeks kepuasan masyarakat di Kantor Dinas Kependudukan dan Pencatatan Sipil Kota Palangka Raya adalah sebesar 2,963 dan nilai indeks kepuasan masyarakat setelah dikonversikan sebesar 74,075 dengan mutu pelayanan berada pada kategori “B” dan kinerja unit pelayanan “BAIK”. Berdasarkan hasil penelitian yang diperoleh dari perhitungan indeks kepuasan masyarakat dapat disimpulkan bahwa pelayanan publik di Kantor Dinas Kependudukan dan Pencatatan Sipil Kota Palangka Raya dapat dikatakan berkualitas baik dan tidak seperti yang dikeluhkan. Hanya penilaian subjektif dari beberapa orang yang mengatakan pelayanan publik masih belum baik, namun perlu untuk ditingkatkan.
Kinerja Keuangan Usaha Mikro dan Kecil
Authors: Winbaktianur  , Siregar Liesma Maywarni 
Published: February 2021

SMEs is one of the basic forms of business stance developed from an individual or a group of people. In practice there has been a lot of support given to this business category even though the products or services is still small competing with medium and large businesses. Planning and control needs to be done which is the goal the main thing is to achieve the goal. Planning is made for facilitate the assessment or evaluation of business activities. Performance appraisal is important to see to what extent the business that is carried out has reached the goal, financial performance how much profit is obtained in a period. The purpose of this research is to discuss the importance of conducting a performance appraisal micro and small scale entrepreneurship. The method of this paper is library research. In discussion, it will describe what assessment is performance, performance appraisal factors and indicators as well as terminated with the benefit of doing a financial performance appraisal.
Keywords: Micro and Small Enterprises, performance appraisal, entrepreneurship
Pengaruh Kepemimpinan dan Pengembangan Karir Terhadap Niat untuk Tinggal dengan Keterikatan Kerja sebagai Intervening
Authors: Kriswanta Kriswanta , Mulyono Ari , Iskandar Herli , Haris Pratama Faisal , Wiji Astuti Dwi , Aulia Alafta 
Published: February 2021

Penelitian bertujuan menguji pengaruh kepemimpinan dan pengembangan karir pada perusahaan penggilingan baja di kabupaten Bekasi terhadap niat untuk tinggal dengan keterikatan kerja sebagai intervening. Data diperoleh dari kuesioner yang diberikan kepada 61 karyawan. Pendekatan yang dilakukan adalah dengan penelitian kuantitatif dengan analisis struktural menggunakan Smart PLS 3. Penelitian menemukan bahwa pengembangan karir berpengaruh terhadap keterikatan kerja dan ikut mempengaruhi niat untuk tinggal. Kepemimpinan tidak berpengaruh terhadap keterikatan kerja dan niat untuk tinggal, tetapi hal ini perlu menjadi perhatian khusus bagi perusahaan.
This study aims to examine the influence of leadership and career development in steel milling companies in Bekasi district on the intention to stay with work engagement as an intervening. Data obtained from questionnaires given to 61 employees. The approach taken is quantitative research with structural analysis using Smart PLS 3. The study found that career development affects work engagement and also influences the intention to stay. The leadership does not affect work engagement and the intention to stay, but this needs special attention for the company.
PENGARUH PERUBAHAN ORGANISASI DAN BUDAYA ORGANISASI TERHADAP PENINGKATAN EFEKTIVITAS KERJA KARYAWAN PADA PT. TELKOM REGIONAL VII SULAWESI SELATAN
Authors: Abdullah Salma 
Published: February 2021

Penelitian ini bertujuan untuk mengetahui Pengaruh Perubahan Organisasi dan Budaya Organisasi dalam Meningkatan Efektivitas Kerja pada PT. Telkom Regional VII Sulawesi. Pendekatan penelitian ini termasuk dalam jenis penelitian eksplanatori yang bersifat menguji hipotesis melalui kajian tentang Pengaruh Perubahan dan Budaya Organisasi dalam Meningkatan Efektivitas Kerja pada PT. Telkom Regional VII Sulawesi. Penelitian ini termasuk dalam jenis penelitian eksplanatori dengan menggunakan pendekatan kuantitatif melalui uji parameter dalam menjawab hipotesis.Pengumpulan data dilakukan secara cross-section melalui kuesioner. Penentuan sampel menggunakan Simple random sampling dengan jumlah sampel sebanyak 35 responden. Metode analisis data yang digunakan dalam pengujian hipotesis Analisis Regresi berganda. Hasil penelitian memberikan bukti bahwa Variabel perubahan organisasi dan Variabel budaya organisasi berpengaruh secara signifikan terhadap efektivitas kerja karyawan.
PENGELOLAAN PASAR TRADISIONAL DALAM SINERGITAS PASAR MODERN DI INDONESIA
Authors: Gani Mustafa 
Published: February 2021

Pengelolaan Pasar Tradisional dalam sinergitas pasar modern yang menjadi fokus masalah adalah Bagaimana pengembangan pasar tradisional sebagai mitra Pasar modern di Indonesia Jenis penelitian kualitatif melalui pendektan fenomenologi Hasil penelitian menunjukkan bahwa keberadaan pasar tradisional sangat penting dan strategis baik ditinjau dari aspek ekonomi,sosial,budaya dan politik, kehadiran pasar tradisional dengan konsep kesederhanaan dan harga yang terjangkau akan mengairahkan ekonomi sehingga proses perputaran barang akan lancar,keberadaan pasar tradisional perlu dibenahi dan diolah agar kehadirannya tetap mampu dipertahankan dan tidak tergilas oleh kehadiran pasar modern
Spin Change of Asteroid 2012 TC4 Probably by Radiation Torques
Authors: Lee Hee-Jae , Ďurech Josef , Vokrouhlický David , Pravec Petr , Moon Hong-Kyu , Ryan William , Kim Myung-Jin , Kim Chun-Hwey , Choi Young-Jun , Bacci Paolo , Pollock Joe , Apitzsch Rolf 
Published: February 2021

Abstract
Asteroid 2012 TC4 is a small (∼10 m) near-Earth object that was observed during its Earth close approaches in 2012 and 2017. Earlier analyses of light curves revealed its excited rotation state. We collected all available photometric data from the two apparitions to reconstruct its rotation state and convex shape model. We show that light curves from 2012 and 2017 cannot be fitted with a single set of model parameters; the rotation and precession periods are significantly different for these two data sets, and they must have changed between or during the two apparitions. Nevertheless, we could fit all light curves with a dynamically self-consistent model assuming that the spin states of 2012 TC4 in 2012 and 2017 were different. To interpret our results, we developed a numerical model of its spin evolution in which we included two potentially relevant perturbations: (i) gravitational torque due to the Sun and Earth and (ii) radiation torque, known as the Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effect. Despite our model simplicity, we found that the role of gravitational torques is negligible. Instead, we argue that the observed change of its spin state may be plausibly explained as a result of the YORP torque. To strengthen this interpretation, we verify that (i) the internal energy dissipation due to material inelasticity and (ii) an impact with a sufficiently large interplanetary particle are both highly unlikely causes of its observed spin state change. If true, this is the first case where the YORP effect has been detected for a tumbling body.
Comparison of Observed Galaxy Properties with Semianalytic Model Predictions Using Machine Learning
Authors: Simet Melanie , Chartab Nima , Lu Yu , Mobasher Bahram 
Published: February 2021

Abstract
With current and upcoming experiments such as the Wide Field Infrared Survey Telescope, Euclid, and Large Synoptic Survey Telescope, we can observe up to billions of galaxies. While such surveys cannot obtain spectra for all observed galaxies, they produce galaxy magnitudes in color filters. This data set behaves like a high-dimensional nonlinear surface, an excellent target for machine learning. In this work, we use a lightcone of semianalytic galaxies tuned to match Cosmic Assembly Near-infrared Deep Legacy Survey (CANDELS) observations from Lu et al. to train a set of neural networks on a set of galaxy physical properties. We add realistic photometric noise and use trained neural networks to predict stellar masses and average star formation rates (SFRs) on real CANDELS galaxies, comparing our predictions to SED-fitting results. On semianalytic galaxies, we are nearly competitive with template-fitting methods, with biases of 0.01 dex for stellar mass, 0.09 dex for SFR, and 0.04 dex for metallicity. For the observed CANDELS data, our results are consistent with template fits on the same data at 0.15 dex bias in

and 0.61 dex bias in the SFR. Some of the bias is driven by SED-fitting limitations, rather than limitations on the training set, and some is intrinsic to the neural network method. Further errors are likely caused by differences in noise properties between the semianalytic catalogs and data. Our results show that galaxy physical properties can in principle be measured with neural networks at a competitive degree of accuracy and precision to template-fitting methods.
Three-dimensional Hydrodynamics Simulations of Precollapse Shell Burning in the Si- and O-rich Layers
Authors: Yoshida Takashi , Takiwaki Tomoya , Kotake Kei , Takahashi Koh , Nakamura Ko , Umeda Hideyuki 
Published: February 2021

Abstract
We present 3D hydrodynamics simulations of shell burning in two progenitors with zero-age main-sequence masses of 22 and 27 M
⊙ for ∼65 and 200 s up to the onset of gravitational collapse, respectively. The 22 and 27 M
⊙ stars are selected from a suite of 1D progenitors. The former and the latter have an extended Si- and O-rich layer with a width of ∼109 cm and ∼5 × 109 cm, respectively. Our 3D results show that turbulent mixing occurs in both of the progenitors with the angle-averaged turbulent Mach number exceeding ∼0.1 at the maximum. We observe that an episodic burning of O and Ne, which takes place underneath the convection bases, enhances the turbulent mixing in the 22 and 27 M
⊙ models, respectively. The distribution of nucleosynthetic yields is significantly different from that in 1D simulations, namely, in 3D more homogeneous and inhomogeneous in the radial and angular direction, respectively. By performing a spectrum analysis, we investigate the growth of turbulence and its role of material mixing in the convective layers. We also present a scalar spherical harmonics mode analysis of the turbulent Mach number. This analytical formula would be helpful for supernova modelers to implement the precollapse perturbations in core-collapse supernova simulations. Based on the results, we discuss implications for the possible onset of the perturbation-aided neutrino-driven supernova explosion.
Dynamical Masses and Stellar Evolutionary Model Predictions of M Stars
Authors: Pegues Jamila , Czekala Ian , Andrews Sean M. , Öberg Karin I. , Herczeg Gregory J. , Bergner Jennifer B. , Ilsedore Cleeves L. , Guzmán Viviana V. , Huang Jane , Long Feng , Teague Richard , Wilner David J. 
Published: February 2021

Abstract
In this era of Gaia and ALMA, dynamical stellar mass measurements, derived from spatially and spectrally resolved observations of the Keplerian rotation of circumstellar disks, provide benchmarks that are independent of observations of stellar characteristics and their uncertainties. These benchmarks can then be used to validate and improve stellar evolutionary models, the latter of which can lead to both imprecise and inaccurate mass predictions for pre-main-sequence, low-mass (≤0.5 M
⊙) stars. We present the dynamical stellar masses derived from disks around three M stars (FP Tau, J0432+1827, and J1100–7619) using ALMA observations of 12CO (J = 2–1) and 13CO (J = 2–1) emission. These are the first dynamical stellar mass measurements for J0432+1827 and J1100–7619 (0.192 ± 0.005 M
⊙ and 0.461 ± 0.057 M
⊙, respectively) and the most precise measurement for FP Tau (0.395 ± 0.012 M
⊙). Fiducial stellar evolutionary model tracks, which do not include any treatment of magnetic activity, agree with the dynamical stellar mass measurement of J0432+1827 but underpredict the mass by ∼60% for FP Tau and by ∼80% for J1100–7619. Possible explanations for the underpredictions include inaccurate assumptions of stellar effective temperature, undetected binarity for J1100–7619, and that fiducial stellar evolutionary models are not complex enough to represent these stars. In the former case, the stellar effective temperatures would need to be increased by amounts ranging from ∼40 to ∼340 K to reconcile the fiducial stellar evolutionary model predictions with the dynamically measured masses. In the latter case, we show that the dynamical masses can be reproduced using results from stellar evolutionary models with starspots, which incorporate fractional starspot coverage to represent the manifestation of magnetic activity. Folding in low-mass M stars from the literature and assuming that the stellar effective temperatures are imprecise but accurate, we find tentative evidence of a relationship between fractional starspot coverage and observed effective temperature for these young, cool stars.
Laboratory Study of the Torus Instability Threshold in Solar-relevant, Line-tied Magnetic Flux Ropes
Authors: Alt Andrew , Myers Clayton E. , Ji Hantao , Jara-Almonte Jonathan , Yoo Jongsoo , Bose Sayak , Goodman Aaron , Yamada Masaaki , Kliem Bernhard , Savcheva Antonia 
Published: February 2021

Abstract
Coronal mass ejections (CMEs) occur when long-lived magnetic flux ropes (MFRs) anchored to the solar surface destabilize and erupt away from the Sun. This destabilization is often described in terms of an ideal magnetohydrodynamic instability called the torus instability. It occurs when the external magnetic field decreases sufficiently fast such that its decay index,

, is larger than a critical value,

, where

for a full, large aspect ratio torus. However, when this is applied to solar MFRs, a range of conflicting values for

is found in the literature. To investigate this discrepancy, we have conducted laboratory experiments on arched, line-tied flux ropes and applied a theoretical model of the torus instability. Our model describes an MFR as a partial torus with foot points anchored in a conducting surface and numerically calculates various magnetic forces on it. This calculation yields better predictions of

that take into account the specific parameters of the MFR. We describe a systematic methodology to properly translate laboratory results to their solar counterparts, provided that the MFRs have a sufficiently small edge safety factor or, equivalently, a large enough twist. After this translation, our model predicts that

in solar conditions falls near

and within a larger range of

, depending on the parameters. The methodology of translating laboratory MFRs to their solar counterparts enables quantitative investigations of CME initiation through laboratory experiments. These experiments allow for new physics insights that are required for better predictions of space weather events but are difficult to obtain otherwise.
The 60 pc Environment of FRB 20180916B
Authors: Tendulkar Shriharsh P. , Gil de Paz Armando , Kirichenko Aida Yu. , Hessels Jason W. T. , Bhardwaj Mohit , Ávila Fernando , Bassa Cees , Chawla Pragya , Fonseca Emmanuel , Kaspi Victoria M. , Keimpema Aard , Kirsten Franz , Lazio T. Joseph W. , Marcote Benito , Masui Kiyoshi , Nimmo Kenzie , Paragi Zsolt , Rahman Mubdi , Payá Daniel Reverte , Scholz Paul , Stairs Ingrid 
Published: February 2021

Abstract
Fast radio burst FRB 20180916B in its host galaxy SDSS J015800.28+654253.0 at 149 Mpc is by far the closest-known FRB with a robust host galaxy association. The source also exhibits a 16.35 day period in its bursting. Here we present optical and infrared imaging as well as integral field spectroscopy observations of FRB 20180916B with the WFC3 camera on the Hubble Space Telescope and the MEGARA spectrograph on the 10.4 m Gran Telescopio Canarias. The 60–90 milliarcsecond (mas) resolution of the Hubble imaging, along with the previous 2.3 mas localization of FRB 20180916B, allows us to probe its environment with a 30–60 pc resolution. We constrain any point-like star formation or H ii region at the location of FRB 20180916B to have an Hα luminosity L
Hα
≲ 1037 erg s−1, and we correspondingly constrain the local star formation rate to be ≲10−4 M⊙ yr−1. The constraint on Hα suggests that possible stellar companions to FRB 20180916B should be of a cooler, less massive spectral type than O6V. FRB 20180916B is 250 pc away (in projected distance) from the brightest pixel of the nearest young stellar clump, which is ∼380 pc in size (FWHM). With the typical projected velocities of pulsars, magnetars, or neutron stars in binaries (60–750 km s−1), FRB 20180916B would need 800 kyr to 7 Myr to traverse the observed distance from its presumed birth site. This timescale is inconsistent with the active ages of magnetars (≲10 kyr). Rather, the inferred age and observed separation are compatible with the ages of high-mass X-ray binaries and gamma-ray binaries, and their separations from the nearest OB associations.
Spectroscopic Confirmation of an M6 Dwarf Companion to the Nearby Star BD-08 2582
Authors: Low Ryan , Burgasser Adam J. , Reylé Céline , Gerasimov Roman , Hsu Chih-Chun , Theissen Christopher A. 
Published: February 2021

Abstract
We report resolved optical spectroscopy for the nearby low-mass stellar system BD-08 2582AB. We confirm prior unpublished reports of the existence of the secondary, and the spectral data indicate a secondary type of M6 Ve, consistent with spectrophotometric estimates from Gaia astrometry. The secondary exhibits Hα emission at a level equivalent to other M6 dwarfs, and has a metallicity index in line with its well-studied solar-metallicity K7/M0 primary.