bluuebunny/crossref_metadata_2025_split huggingface dataset:
Cover, Content, and Editorial Note from Pengabdianmu J Pengabdian Masyarakat Vol. 4 No. 1 March 2019
Authors: PengabdianMu J Pengabdian Masyarakat Chief Editor Of 
Published: April 2019

Assalamu�alaikum Wr. Wb.
Dear reader, now PengabdianMu: Jurnal Ilmiah Pengabdian kepada Masyarakat re-published on Volume 4 Issue 1 March 2019. The success of this publication is the result of good cooperation of all parties who maintain the publishing sustainability twice a year.
Alhamdulillah, form this edition PengabdianMu: Jurnal Ilmiah Pengabdian kepada Masyarakat has succeeded in gaining a proud achievement by successfully getting an accreditation rating on SINTA 4. This success cannot be separated from the support and prayer of all contributors, both material and non-material.
The publication of PengabdianMu: Jurnal Ilmiah Pengabdian kepada Masyarakat certainly participates in disseminating the results of community services in science and technology development conducted by lecturers and researchers especially from UM Palangkaraya and other universities.
This edition contains 11 articles consisting of Education, Social and Political, Islamic Studies, Engineering, and Health Science topics. Editorial boards are fully aware that there is still room for improvement in this edition, hence with all humility willing to accept constructive suggestions and feedback for improvements to the publication for the next editions.
The editorial board would like to thank the University, all editors and reviewers, and contributors of the scientific articles who have provided the repertoire in this issue. We hope that all parties, especially the contributors of the articles, could re-participate for the success of the publication in the next edition in September 2019.
Wassalamu�alaikum Wr. Wb.
Palangka Raya, March 2019
Editor-in-Chief,
signed
Dr. Nurul Hikmah Kartini, S.Si., M.Pd.
SENI GRAFIS INDONESIA KEMBALI KE “JALAN MASIF”
Authors: Rahman Deni 
Published: April 2019

<p>Siasat para praktisi grafis meng-eksklusifkan karya grafisnya agar setara dengan seni lukis, justru menjadikan seni grafis seolah-olah hanyalah sebagai salah satu teknik melukis. Untuk mendekatkan seni grafis pada masyarakat, menempuh “jalan masif” akan menjadi siasat yang ampuh. Hal ini akan menempatkan kembali seni grafis pada fitrahnya yaitu karya rupa multi impresi.</p><p> </p><p>kata kunci: seni grafis, masif</p>
What Will Parents Pay for Hands-on Ocean Conservation and Stewardship Education?
Authors: Schwarzmann Danielle , Nachbar Seaberry , Pollack Naomi , Leeworthy Vernon (Bob) , Hitz Sylvia 
Published: April 2019

Supported by the National Marine Sanctuary Foundation, the Ocean Guardian School (OGS) program is a federally funded grant program coordinated by the National Oceanic and Atmospheric Administration (NOAA) Office of National Marine Sanctuaries. OGS supports the educational goals of national marine sanctuaries (NMS) by funding hands-on ocean conservation and stewardship programs in both public and private schools. Schools apply for grants (up to $4,000) to implement school- or community-based conservation projects to educate students, while contributing to the health and protection of local watersheds and the world’s ocean. This study is the first to estimate the value that parents have for their child’s participation in an ocean conservation and stewardship program. Using a contingent choice survey, changes to student behaviour, parents’ support for the OGS program and the non-market economic value to parents of the six program attributes are estimated.
PENELITIAN TERHADAP MINAT MENJADI GURU AGAMA DAN KATEKIS DI STKIP WIDYA YUWANA MADIUN
Authors: Dewantara Agustinus Wisnu , Permana Natalis Sukma 
Published: April 2019

Catechetic is the coaching of children, youth and adults in the faith, which is specific to the delivery of the Christian movement, which is basically given organically and systematically, The Catholic Religion teacher deeply embraces her duties and mission through her work at school. This work is the duty and mission that comes from God himself. The Catholic Religion teacher is expected to earnestly live his vocation as a religious teacher. A Catholic teacher is an educator as well as a journalist. An educator or reporter will be able to carry out his duties well if he has a clear and correct understanding of what is actually the purpose of teaching Catholicism as a means of preaching the love of Jesus. A Religion Teacher is a person whose job is to teach another person or an emulated and imitated person. It means that the word is imitated and imitated by faith and deeds by dodging the Christian life.
STKIP Widya Yuwana is an institution owned by the diocese of Surabaya aimed at educating prospective catechists and religious teachers. The institute was originally founded by Paul Janssen, CM under the name AKI (Indonesian Catechetical Academy) which aims to produce a militant and powerful catechist. According to the times, AKI has changed into STKIP Widya Yuwana. As the name implies, this institution is then identified as a producer of religious teachers, and even the impression that this institution no longer exists on the path of Jansen's romance as a catechist producer, and turned into a producer of Catholic religious teachers.
This research is needed to photograph what really happened to the students. Is it true that the outward impression that graduates and students are more likely to be teachers? If so, what is the motivation behind it? Is it really a catechist profession is not promising, or indeed STKIP Widya Yuwana who had already lost the spirit of the founder of its predecessor?
SOBRE SUDOKUS E GRUPOS
Authors: Alegri Mateus , Silva Samuel Brito 
Published: April 2019

Neste trabalho exibiremos algumas relações entre a teoria matemática que abrange o jogo Sudoku, os quadrados latinos, e a teoria de grupos finitos. Na terceira seção exibiremos um critério que estabelece se um quadrado latino de ordem $n$ é a tabela de Cayley de um grupo de igual ordem. Na última seção trabalharemos com o conceito de ortogonalidade entre quadrados latinos, e utilizando o conceito de grupos finitos, exibiremos um contra-exemplo para uma famosa conjectura de Euler. Resaltamos que o único pré-requisitos para o perfeito entendimento deste artigo é o teorema de Cayley para grupos finitos, de modo que a teoria desenvolvida aqui é aplicável no ensino universitário.
The Impact of a Financial Capability Program on the Financial Well-being of Medical Practitioners
Authors: Anthony Rajna , Fazil Sabri Mohamad 
Published: April 2019

The main objective of this study is to determine the impact of a financial capability program on the financial well-being of medical practitioners in the public hospitals in Selangor, Malaysia. Its specific aims were to determine the levels of financial capability, financial satisfaction and financial practice of medical practitioners before and after a financial capability program intervention. A total of 100 medical practitioners were randomly assigned to intervention (50%) and control groups (50%) after both completing the financial capability initial assessment and evaluation (pre-test) questionnaire. The intervention group participants attended a series of five two hour one on one coaching session while the control group did not. After a four month duration both the groups completed the post evaluation (post-test). There were equal numbers of males and females in the intervention sample compared to 19 males and 31 females in the control group. The findings showed that the paired samples t-test detected the difference between the means scores of financial capability, financial satisfaction and financial practice of the medical practitioners in the two groups (control and intervention) from time 1 (pre intervention) and time 2 (post intervention). There was no statistically significant difference found in the financial capability, financial satisfaction and financial practice scores between the two groups (intervention and control) prior to the program intervention (time 1). But the post program intervention (time 2) showed statistically significant (p<0.001) difference between the intervention group and the control group confirming a positive impact. The results of this study can be a starting point in using coaching techniques as part of ongoing education program.
Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey
Authors: Miyatake Hironao , Battaglia Nicholas , Hilton Matt , Medezinski Elinor , Nishizawa Atsushi J. , More Surhud , Aiola Simone , Bahcall Neta , Bond J. Richard , Calabrese Erminia , Choi Steve K. , Devlin Mark J. , Dunkley Joanna , Dunner Rolando , Fuzia Brittany , Gallardo Patricio , Gralla Megan , Hasselfield Matthew , Halpern Mark , Hikage Chiaki , Hill J. Colin , Hincks Adam D. , Hložek Renée , Huffenberger Kevin , Hughes John P. , Koopman Brian , Kosowsky Arthur , Louis Thibaut , Madhavacheril Mathew S. , McMahon Jeff , Mandelbaum Rachel , Marriage Tobias A. , Maurin Loïc , Miyazaki Satoshi , Moodley Kavilan , Murata Ryoma , Naess Sigurd , Newburgh Laura , Niemack Michael D. , Nishimichi Takahiro , Okabe Nobuhiro , Oguri Masamune , Osato Ken , Page Lyman , Partridge Bruce , Robertson Naomi , Sehgal Neelima , Sherwin Blake , Shirasaki Masato , Sievers Jonathan , Sifón Cristóbal , Simon Sara , Spergel David N. , Staggs Suzanne T. , Stein George , Takada Masahiro , Trac Hy , Umetsu Keiichi , Engelen Alex van , Wollack Edward J. 
Published: April 2019

Abstract
We present weak-lensing measurements using the first-year data from the Hyper Suprime-Cam Strategic Survey Program on the Subaru telescope for eight galaxy clusters selected through their thermal Sunyaev–Zel’dovich (SZ) signal measured at 148 GHz with the Atacama Cosmology Telescope Polarimeter experiment. The overlap between the two surveys in this work is 33.8 square degrees, before masking bright stars. The signal-to-noise ratio of individual cluster lensing measurements ranges from 2.2 to 8.7, with a total of 11.1 for the stacked cluster weak-lensing signal. We fit for an average weak-lensing mass distribution using three different profiles, a Navarro–Frenk–White profile, a dark-matter-only emulated profile, and a full cosmological hydrodynamic emulated profile. We interpret the differences among the masses inferred by these models as a systematic error of 10%, which is currently smaller than the statistical error. We obtain the ratio of the SZ-estimated mass to the lensing-estimated mass (the so-called hydrostatic mass bias 1−b) of

, which is comparable to previous SZ-selected clusters from the Atacama Cosmology Telescope and from the Planck Satellite. We conclude with a discussion of the implications for cosmological parameters inferred from cluster abundances compared to cosmic microwave background primary anisotropy measurements.
The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity
Authors: Moe Maxwell , Kratter Kaitlin M. , Badenes Carles 
Published: April 2019

Abstract
There is now strong evidence that the close binary fraction (P < 104 days; a < 10 au) of solar-type stars (M
1 ≈ 0.6–1.5

) decreases significantly with metallicity. Although early surveys showed that the observed spectroscopic binary (SB) fractions in the galactic disk and halo are similar (e.g., Carney–Latham sample), these studies did not correct for incompleteness. In this study, we examine five different surveys and thoroughly account for their underlying selection biases to measure the intrinsic occurrence rate of close solar-type binaries. We reanalyze (1) a volume-limited sample of solar-type stars, (2) the Carney-Latham SB survey of high proper motion stars, (3) various SB samples of metal-poor giants, (4) the APOGEE survey of radial velocity (RV) variables, and (5) eclipsing binaries (EBs) discovered by Kepler. The observed APOGEE RV variability fraction and Kepler EB fraction both decrease by a factor of ≈4 across −1.0 < [Fe/H] < 0.5 at the 22σ and 9σ confidence levels, respectively. After correcting for incompleteness, all five samples/methods exhibit a quantitatively consistent anticorrelation between the intrinsic close binary fraction (a < 10 au) and metallicity: F
close = 53% ± 12%, 40% ± 6%, 24% ± 4%, and 10% ± 3% at [Fe/H] = −3.0, −1.0, −0.2 (mean field metallicity), and +0.5, respectively. We present simple fragmentation models that explain why the close binary fraction of solar-type stars strongly decreases with metallicity while the wide binary fraction, close binary fraction of OB stars, and initial mass function are all relatively constant across −1.5 ≲ [Fe/H] < 0.5. The majority of solar-type stars with [Fe/H] ≲ −1.0 will interact with a stellar companion, which has profound implications for binary evolution in old and metal-poor environments such as the galactic halo, bulge, thick disk, globular clusters, dwarf galaxies, and high-redshift universe.
Prolonged Kelvin–Helmholtz Waves at Dawn and Dusk Flank Magnetopause: Simultaneous Observations by MMS and THEMIS
Authors: Lu S. W. , Wang C. , Li W. Y. , Tang B. B. , Torbert R. B. , Giles B. L. , Russell C. T. , Burch J. L. , McFadden J. P. , Auster H. U. , Angelopoulos V. 
Published: April 2019

Abstract
The Kelvin–Helmholtz (K-H) waves predominantly excited at the Earth’s low-latitude magnetopause were suggested to be dawn–dusk asymmetric. We report a prolonged simultaneous observations of the K-H waves on the dawn and dusk magnetopause by Magnetospheric Multiscale (MMS) and THEMIS-A (THA) spacecraft, respectively. The quasi-periodic K-H waves on both flanks have unambiguous low-density and high-speed patterns. The wave periods vary gradually on both flanks, with similar average periods (303 ± 107 s for MMS and 266 ± 102 s for THA). The lag time between the variations of the wave periods is close to the wave propagation time from THA to MMS, which suggests that the K-H waves generate and propagate quasi-symmetrically on both flanks. Larger local magnetic shear angles are observed on the trailing edges by MMS than by THA, which is probably due to the strong magnetic field distortion during the tailward propagation. The increased magnetic shear may excite magnetic reconnection, thus contributing to the formation of the low-latitude boundary layer.
The MESAS Project: Long-wavelength Follow-up Observations of Sirius A
Authors: White Jacob Aaron , Aufdenberg J. , Boley A. C. , Devlin M. , Dicker S. , Hauschildt P. , Hughes A. G. , Hughes A. M. , Mason B. , Matthews B. , Moór A. , Mroczkowski T. , Romero C. , Sievers J. , Stanchfield S. , Tapia F. , Wilner D. 
Published: April 2019

Abstract
Modeling the submillimeter to centimeter emission of stars is challenging due to a lack of sensitive observations at these long wavelengths. We launched an ongoing campaign to obtain new observations entitled Measuring the Emission of Stellar Atmospheres at Submillimeter/millimeter wavelengths (MESAS). Here we present Atacama Large Millimeter/submillimeter Array, Green Bank Telescope, and Very Large Array observations of Sirius A, the closest main-sequence A-type star, that span from 1.4 to 9.0 mm. These observations complement our previous millimeter data on Sirius A and are entirely consistent with the PHOENIX stellar atmosphere models constructed to explain them. We note that accurate models of long-wavelength emission from stars are essential not only to understand fundamental stellar processes, but also to determine the presence of dusty debris in spatially unresolved observations of circumstellar disks.
A Discovery of Young Radio Sources in the Cores of Giant Radio Galaxies Selected at Hard X-Rays
Authors: Bruni G. , Panessa F. , Bassani L. , Chiaraluce E. , Kraus A. , Dallacasa D. , Bazzano A. , Hernández-García L. , Malizia A. , Ubertini P. , Ursini F. , Venturi T. 
Published: April 2019

Abstract
Giant radio galaxies (GRG) are the largest single entities in the universe, having a projected linear size exceeding 0.7 Mpc, which implies that they are also quite old objects. They are not common, representing a fraction of only ∼6% in samples of bright radio galaxies. While a census of about 300 of these objects has been built in the past years, still no light has been shed on the conditions necessary to allow such an exceptional growth, whether of environmental nature or linked to the inner accretion properties. Recent studies found that samples of radio galaxies selected from hard X-ray active galactic nuclei catalogs selected from the International Gamma-Ray Astrophysics Laboratory (INTEGRAL)/the Imager on Board the INTEGRAL Satellite and Swift/the Burst Alert Telescope (thus at energies >20 keV) present a fraction of GRG four times larger than what is found in radio-selected samples. We present radio observations of 15 nuclei of hard-X-ray-selected GRG, finding for the first time a large fraction (61%) of young radio sources at the center of Mpc-scale structures. Being at the center of GRG, these young nuclei may be undergoing a restarting activity episode, suggesting a link between the detected hard X-ray emission—due to the ongoing accretion—and the reactivation of the jets.
In Vivo Toxicity Study of Ethanolic Extracts of Evolvulus alsinoides & Centella asiatica in Swiss Albino Mice
Authors: Yadav Mukesh Kumar , Singh Santosh Kumar , Singh Manish , Mishra Shashank Shekhar , Singh Anurag Kumar , Tripathi Jyoti Shankar , Tripathi Yamini Bhusan 
Published: April 2019

AIM: We aimed to investigate several parameters after the in vivo acute and sub-acute administration of ethanolic extracts from E. alsinoides & C. asiatica.
METHODS: Malignant Ovarian Germ Cell Tumors for in vivo toxicity study guidelines 423 and 407 of Organization for Economic Co-operation and Development (OECD) were followed for acute and sub-acute toxicity assays respectively. For LD50 evaluation, a single dose of ethanolic extracts of Evolvulus alsinoides L. (EEA) and ethanolic extracts of Centella asiatica (ECA) was orally administered to mice at doses of 200, 400, 800, 1600 and 2000 mg/kg. Then the animals were observed for 72 hours. For acute toxicity evaluation, a single dose of both extracts was orally administered to mice at doses of 300, 600, 1200 and 2000 mg/kg and the animals were observed for 14 days. In the sub-acute study, the extracts were orally administered to mice for 28 days at doses of 300, 600, 1200 and 2000 mg/kg. To assess the toxicological effects, animals were closely observed on general behaviour, clinical signs of toxicity, body weight, food and water intake. At the end of the study, it was performed biochemical and hematological evaluations, as well as histopathological analysis from the following organs: brain, heart, liver, and kidney.
RESULTS: The oral administration of E. alsinoides and C. asiatica ethanolic extracts, i.e. EEA 300, EEA 600, EEA 1200, EEA 2000, ECA 300, ECA 600, ECA 1200 & ECA 2000 mg/kg doses showed no moral toxicity effect in LD50, acute and sub-acute toxicity parameters.
CONCLUSION: In this study, we had found that E. alsinoides & C. asiatica extract at different doses cause no mortality in acute and sub-acute toxicity study. Also, histopathology of kidney, liver, heart, and brain showed no alterations in tissues morphology.
Comprendre l’activité d’enseignant(e)s utilisant des formes pédagogiques coopératives nouvelles dans le secondaire
Authors: Leblanc Serge , Sauvaire-Maltrana Céline 
Published: April 2019

Cette étude porte sur des formes pédagogiques coopératives, peu répandues dans l’enseignement du secondaire. Elles se veulent être une alternative aux deux formats pédagogiques anciens et très répandus : le cours dialogué et le travail individuel écrit. Conduite dans le cadre de l’anthropologie cognitive située, cette étude montre comment l’activité de trois enseignant(e)s expérimenté(e)s (histoire-géographie, français et mathématique) qui ont fait évoluer leurs pratiques pédagogiques dans cette orientation, se restructure au niveau de l’organisation de l’espace-temps, de l’exploitation des supports ou des artefacts et au niveau des modes d’interactions entre les élèves, mais aussi entre le groupe et l’enseignant. Elle met également en évidence des préoccupations communicationnelle et relationnelle très présentes et une posture d’accompagnement plus que d’enseignement qui éloignent ces enseignant(e)s de la culture scolaire traditionnelle. Dans un contexte éducatif français où les réformes successives débouchent sur des échecs tant au niveau de l’amélioration des résultats des élèves que du bien-être à l’école, comprendre les raisons d’agir de ces enseignant(e)s et identifier les conditions qui leur ont permis d’opérer des transformations effectives de leurs pratiques de classe semble très utile pour alimenter la formation initiale et continue.
Faire de la recherche fondamentale de terrain dans les établissements scolaires : orientations épistémologiques et implications méthodologiques
Authors: Moussay Sylvie , Escalié Guillaume , Chaliès Sébastien 
Published: April 2019

Dans le présent article, l’objectif est de décrire la recherche fondamentale de terrain (Clot, 2008a, 2008b ; Wisner, 1995) telle que nous la concevons dans nos programmes de recherche et telle que nous la mettons en œuvre, dans les établissements scolaires avec les professionnels de l’enseignement. Sont présentés les orientations épistémologiques et théoriques ainsi que les choix méthodologiques que nos études à visées transformative et épistémique adoptent pour mener une recherche fondamentale de terrain. Dans ce contexte, l’article développe la problématique des relations chercheur(s) et professionnel(s) en décrivant les processus de co-construction de l’objet d’étude et d’élaboration collective des transformations de l’activité que la méthode d’entretien d’autoconfrontation permet de faire émerger au cours de la recherche. Trois études illustrent cette démarche de recherche fondamentale de terrain menée avec des enseignants en milieu scolaire. Une mise en discussion de ces trois études à propos des conditions du développement de l’activité des enseignants permet de souligner des points d’accord et de débat avec d’autres travaux qui se réclament d’une recherche fondamentale de terrain.
The Selective Expansion and Targeted Accumulation of Bone Marrow–Derived Macrophages Drive Cardiac Vasculitis
Authors: Stock Angus T. , Collins Nicholas , Smyth Gordon K. , Hu Yifang , Hansen Jacinta A. , D’Silva Damian B. , Jama Hamdi A. , Lew Andrew M. , Gebhardt Thomas , McLean Catriona A. , Wicks Ian P. 
Published: April 2019

Abstract
The adult heart contains macrophages derived from both embryonic and adult bone marrow (BM)-derived precursors. This population diversity prompted us to explore how distinct macrophage subsets localize within the heart, and their relative contributions in cardiac disease. In this study, using the reciprocal expression of Lyve-1 and Ccr2 to distinguish macrophages with distinct origins, we show that, in the steady state, both embryonic (Lyvepos) and BM-derived (Ccr2pos) macrophages populate the major vessels of the heart in mice and humans. However, cardiac macrophage populations are markedly perturbed by inflammation. In a mouse model of Kawasaki disease, BM-derived macrophages preferentially increase during acute cardiac inflammation and selectively accumulate around major cardiac vessels. The accumulation of BM-derived macrophages coincides with the loss of their embryonic counterparts and is an initiating, essential step in the emergence of subsequent cardiac vasculitis in this experimental model. Finally, we demonstrate that the accumulation of Ccr2pos macrophages (and the development of vasculitis) occurs in close proximity to a population of Ccr2 chemokine ligand–producing epicardial cells, suggesting that the epicardium may be involved in localizing inflammation to cardiac vessels. Collectively, our findings identify the perivascular accumulation of BM-derived macrophages as pivotal in the pathogenesis of cardiac vasculitis and provide evidence about the mechanisms governing their recruitment to the heart.