bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENERAPAN METODE INKUIRI BERBASIS AUDIO VISUAL “MUSEUM BALI” DALAM MENUMBUHKAN MOTIVASI DAN KESADARAN SEJARAH
Authors: Ruli Rulianto 
Published: February 2022

Penelitian ini bertujuan untuk (1) mengetahui apakah penerapan metode inkuiri berbasis audio visual “Museum Bali” dapat menumbuhkan motivasi belajar mahasiswa, dan (2) mengetahui apakah penerapan metode inkuiri berbasis audio visual “Museum Bali” dapat menumbuhkan kesadaran sejarah mahasiswa. Penelitian ini merupakan penelitian tindakan kelas. Penelitian ini dilakukan dalam dua siklus dengan subjek penelitian seluruh mahasiswa semester III jurusan Pendidikan Sejarah Universitas Mahasaraswati Denpasar tahun akademik 2017-2018 sebanyak 26 orang. Metode yang digunakan pada penelitian ini adalah metode inkuiri. Hasil pembahasan menunjukkan bahwa motivasi belajar mahasiswa mengalami peningkatan, dengan indikator rasa ingin tahu mahasiswa meningkat setelah dilacak menggunakan angket motivasi pada proses belajar. Sementara itu, jika dikalkulasikan ke dalam angka maka pada siklus I sebanyak 16 mahasiswa belum mencapai ketuntasan dan 10 mahasiswa mencapai ketuntasan. Pada siklus II terjadi peningkatan, yakni sebanyak 17 mahasiswa mendapatkan skor 90, 3 mahasiswa memperoleh skor 110 sedangkan 6 mahasiswa mendapatkan skor 100. Dengan demikian dapat dikatakan bahwa sudah ada perubahan terhadap motivasi belajar mahasiswa secara signifikan. Sementara itu, aspek kesadaran sejarah mengacu pada rentang skor (100-120 Amat Baik), (90-99 Baik), (80-89 Cukup), (70-79 Kurang, dan (60-69 Sangat Kurang). Hasilnya menunjukkan bahwa data analisis tes angket kesadaran sejarah terhadap pembelajaran sejarah pada siklus I yaitu ada 13 mahasiswa mendapatkan skor terendah, 1 mahasiswa mendapatkan skor 77, 1 mahasiswa mendapatkan skor 78, 2 mahasiswa mendapatkan skor 79, 2 mahasiswa mendapatkan skor 80, 1 mahasiswa mendapat skor 86, 3 mahasiswa mendapatkan skor 88, dan 3 mahasiswa mendapatlan skor 89. Berdasarkan pedoman skor yang terdapat pada lembar observasi maka klasifikasi berada pada taraf Cukup. Pada siklus II, 19 mahasiswa mendapatkan skor di atas 90, 1 mahasiswa mendapatkan skor 112, 3 mahasiswa mendapatkan skor 103, dan 3 mahasiswa mendapatkan skor 120. Berdasarkan pedoman skor yang terdapat pada lembar observasi maka klasifikasi berada pada taraf Amat Baik.
PENGARUH SELF-CONCEPT AKADEMIK TERHADAP KEMANDIRIAN BELAJAR SISWA KELAS VI SEKOLAH DASAR SELAMA PANDEMI COVID-19
Authors: Archi Maulyda Mohammad , Indraswati Dyah , Erfan Muhammad , Widodo Arif , Nikmah Rahmatih Aisa 
Published: February 2022

Penelitian ini bertujuan mengetahui pengaruh self-concept akademik terhadap kemandirian belajar siswa kelas VI selama pandemi. Penelitian ini dilatarbelakangi adanya permasalahan bahwa masih terdapat banyak siswa yang kurang memiliki kemandirian dalam belajar pada jenjang pendidikan sekolah dasar, terutama saat pembelajaran berbasis online (daring) diberlakukan pada masa pandemi. Selain itu, ketika ujian berlangsung banyak siswa yang tidak mampu mengerjakan soalnya sendiri dan bertanya kepada teman di sampingnya. Penelitian ini menggunakan pendekatan kuantitatif-deskriptif. Jenis penelitian adalah penelitian korelasi. Subjek penelitian ini ialah siswa, berjumlah 40 siswa. Variabel yang dikaji yaitu self-concept akademik dan kemandirian belajar siswa. Data diambil melalui angket self-concept akademik dan kemandirian belajar siswa. Analisis penelitian ini menggunakan perhitungan analisis korelasi product moment dengan bantuan SPSS versi 23.0. Berdasarkan hasil analisis diperoleh hasil r tabel dengan N = 70 dan α= 5%, adalah 0,235. Sedangkan rhitung diperoleh besaran 0,769, maka rhitung > rtabel (0,769>0,235), berarti terdapat pengaruh positif dan signifikan, akibatnya Ho ditolak dan Ha diterima. Jadi kesimpulannya “Ada pengaruh yang positif dan signifikan self-concept akademik terhadap kemandirian belajar siswa kelas VI”. Artinya semakin tinggi self-concept akademik siswa maka semakin tinggi pula kemandirian belajarnya dan sebaliknya, apabila self-concept akademik rendah maka kemandirian belajar siswa rendah pula. Berdasarkan simpulan pada hasil penelitian siswa diharapkan dapat belajar dengan kesadaran diri tanpa adanya paksaan orangtua maupun guru serta dalam belajar tidak tergantung kepada orang lain. Guru diharapkan dapat memperhatikan self-concept akademik siswa dan berusaha meningkatkannya sehingga siswa dapat mempunyai kemandirian belajar tinggi dan dapat menyelesaikan tugas belajarnya dengan sempurna.
TYPES OF SPEAKING ACTIVITIES IN “BUKU BAHASA INGGRIS” FOR TOURISM VOCATIONAL HIGH SCHOOL
Authors: Yosefina Helenora Jem  , Ely H. Selamat  , Raymundus Beda  , Helena Saimun  
Published: February 2022

The use of textbooks as a media in teaching learning processes especially in English Language Teaching cannot be denied. That’s why this present study is intended to investigate types of speaking activities presented in buku Bahasa Inggris for Tourism Vocational High School. The content of an English text book was described and analyzed by using a descriptive qualitative method. Buku Bahasa Inggris kelas X had been chosen as the source of data. The collected data were analyzed through some steps such as (1) classifying the data into types of speaking activities (Acting from Script, Communication Games, Discussions, Paper Talk, Questionnaires, Simulation and Role Play) and (2) identifying the dominant type of speaking activities. The result indicates buku Bahasa Inggris Kelas X contains six types of speaking activities and it is dominated by speaking activity of prepared talk
POTRAIT INTERRELIGIOUS DIALOGUE OF CATHOLIC TRADERS AND MUSLIMS IN THE INPRES RUTENG MARKET
Authors: Fransiskus Sales Lega  , Marianus Supar Jelahut  
Published: February 2022

Dialogue is a way of being in the Church in a world characterized by religious and cultural diversity. This study aims to explore the interreligious dialogue of the traders at the Inpres Ruteng market. This research is urgent because the Inpres Ruteng market is a miniature of religious pluralism. This research uses a qualitative approach. The main instruments in collecting data were in-depth interviews and observations. The findings of this study indicate that two types of dialogue have been practiced by traders in Ruteng Inpres market, namely the dialogue of life and dialogue of works. These two types of dialogue have become part of the way of life of Catholic and Muslim traders in the Ruteng Inpres market. Two types of dialogue that have not yet appeared are the dialogue of faith experience and the theological dialogue. It is hoped that the strength of the dialogue on life and the dialogue of work is expected to be the strength to create a holistic and integral transformation in the lives of traders in the Ruteng Inpres market. Based on the findings of this study, the following two recommendations should be made. First, faith dialogue and theological dialogue need to be developed in order to build an adequate understanding of the uniques of the teachings of other religions. Developing a dialogue of faith and theological dialogue needs to be facilitated by the leaders of each religion. Second, further research is expected to focus on efforts to portray potential conflicts in the relationship between Catholic traders and Muslims in the Inpres Ruteng market. This is important so that the planning of preventive steps to prevent conflict can be done properly and measured.
Utekelezaji wa Mitalaa ya Kiswahili Vyuoni na Namna Unavyoathiri Utendakazi wa Walimu Wanaofundisha katika Shule za Upili
Authors: Mwanzi Jackline , Ipara Odeo Isaac , Simala Kenneth Inyani 
Published: February 2022

Walimu wanaofundisha katika shule za upili hupata mafunzo yao ya kitaaluma kutoka katika vyuo vikuu mbalimbali. Wanapoandaliwa vyuoni, walimu hawa hupewa mafunzo kwa kutumia mitalaa tofauti inayoandaliwa katika vyuo vikuu hivyo. Baada ya kuhitimu, wao hutarajiwa kuutekeleza mtalaa mmoja unaoandaliwa na Taasisi ya Ukuzaji Mitalaa nchini Kenya (TUMIKE) ili ufundishwe katika shule zote za upili. Utafiti ulifanywa ili kudhihirisha iwapo mafunzo ya kitaaluma yanayotolewa vyuoni kuwaandaa walimu wa somo la Kiswahili yanawapa maarifa na stadi wanazohitaji kufundisha katika shule za upili baada ya kuhitimu. Makala haya yametokana na utafiti uliofanywa ili Kutathmini uhusiano baina ya mitalaa ya Kiswahili inayotumika katika vyuo vikuu vya umma nchini Kenya na mtalaa ambao umeandaliwa na TUMIKE ili kutekelezwa katika shule za upili. Utafiti ulifanyika katika vyuo vikuu vitano vya umma nchini Kenya. Muundo wa utafiti ulikuwa usoroveya elezi. Data ilikusanywa kwa njia ya usaili, uchanganuzi wa nyaraka na hojaji. Uchanganuzi wa data ulikuwa wa kitakwimu na kimaelezo. Utafiti uligundua kuwa uhusiano baina ya mitalaa rasmi ya Kiswahili ya vyuo vikuu vya umma na mtalaa wa Kiswahili wa shule za upili siyo wa moja kwa moja. Hali hii iliathiri utendakazi wa walimu walipotekeleza mtalaa wa shule za upili. Uhusiano mdogo uliopo baina ya mitalaa rasmi ya vyuo vikuu na mtalaa rasmi wa TUMIKE ulidhihirika kwa kuchunguza vipengele vikuu vya mtalaa ambavyo ni: malengo, mada, utekelezaji na tathmini. Utafiti unapendekeza pafanyike marekebisho ya mara kwa mara ya mtalaa wa TUMIKE kwa kuwahusisha walimu na waandalizi wao ili wakadirie malengo, mada, mbinu za utekelezaji na tathmini mintarafu maandalizi yanayotolewa kwa walimu.
Perbedaan Tumbuh Kembang pada Balita Usia 2-5 Tahun dengan Stunting dan Non-Stunting
Authors: Armayanti Luh Yenny , Putu Ayu Ratna Darmayanti  
Published: February 2022

Indonesia termasuk dalam salah satu negara dengan angka prevalensi stunting tertinggi di ASIA. Stunting akan sangat berpengaruh terhadap pertumbuhan dan perkembangan balita dan mempengaruhi masa depannya kelak. Penelitian ini bertujuan untuk menganalisis perbedaan perkembangan tumbuh kembang pada balita usia 2-5 tahun dengan stunting dan non stunting. Penelitian ini merupakan penelitian komparatif observasional dengan desain cross sectional. Sebanyak 49 balita usia 2-5 tahun menjadi responden dalam penelitian ini stunting yang berasal di daerah Blahbatuh Gianyar, yang ditentukan dengan menggunakan teknik simple random sampling. Alat pengumpulan data yang digunakan berupa KPSP, timbangan berat badan, Mikrotoa. Data dianalisis dengan menggunakan statistik deskriptif, dan komparatif dengan tingkat kepercayaan 95%. Berdasarkan hasil analisis data, didapatkan bahwa pada balita yang mengalami stunting, sebanyak 10 orang menunjukkan penyimpangan perkembangan dan 2 orang meragukan, sedangkan pada balita non stunting sebanyak 6 orang perkembangannya meragukan dan 31 orang perkembangannya sesuai usia. Pada balita nonstunting rerata berat badan dan tinggi badan 15,72±2,3 kg dan 99,29±7,6 cm. Sedangkan pada balita stunting rerata berat badan dan tinggi badan 9,25±1,19 kg dan 86,91±5,0 cm. Berdasarkan hasil uji komparasi ditemukan terdapat perbedaan signifikan perkembangan dan pertumbuhanbalita usia 2-5 tahun dengan stunting dan non stunting dengan nilai p-0,001 (<0,05). Terdapat perbedaan signifikan perkembangan balita usia 2-5 tahun dengan stunting dan non stunting. Diharapkan para orang tua untuk menjaga kebutuhan balita khususnya pemenuhan nutrisi sehingga kondisi stunting dapat dihindari dan balita dapat bertumbuh dan berkembang dengan optimal
Kata Kunci : Tumbuh Kembang, Balita, Stunting
Indeterminacy of International Law?
Authors: Severin Meier 
Published: February 2022

The most important (in)determinacy theses in international law since the 1920s are scrutinised in this book. As Severin Meier demonstrates, the extent of legal determinacy depends neither on some linguistic essence found in the text nor on theories that allegedly stand above practice. Instead, the (in)determinacy of law is shown to arise purely from practice. This reconceptualisation of a key discussion in legal philosophy provides a new perspective on the frame of meaning of legal norms.
Neutrino Properties with Ground-based Millimeter-wavelength Line Intensity Mapping
Authors: Moradinezhad Dizgah Azadeh , Keating Garrett K. , Karkare Kirit S. , Crites Abigail , Choudhury Shouvik Roy 
Published: February 2022

Abstract
Line intensity mapping (LIM) is emerging as a powerful technique to map the cosmic large-scale structure and to probe cosmology over a wide range of redshifts and spatial scales. We perform Fisher forecasts to determine the optimal design of wide-field ground-based millimeter-wavelength LIM surveys for constraining properties of neutrinos and light relics. We consider measuring the auto-power spectra of several CO rotational lines (from J = 2–1 to J = 6–5) and the [C ii] fine-structure line in the redshift range of 0.25 < z < 12. We study the constraints with and without interloper lines as a source of noise in our analysis, and for several one-parameter and multiparameter extensions of ΛCDM. We show that LIM surveys deployable this decade, in combination with existing cosmic microwave background (CMB; primary) data, could achieve order-of-magnitude improvements over Planck constraints on N
eff and M

ν
. Compared to next-generation CMB and galaxy surveys, a LIM experiment of this scale could achieve bounds that are a factor of ∼3 better than those forecasted for surveys such as EUCLID (galaxy clustering), and potentially exceed the constraining power of CMB-S4 by a factor of ∼1.5 and ∼3 for N
eff and M

ν
, respectively. We show that the forecasted constraints are not substantially affected when enlarging the parameter space, and additionally demonstrate that such a survey could also be used to measure ΛCDM parameters and the dark energy equation of state exquisitely well.
Reconstructing the Pleiades with Gaia EDR3
Authors: Heyl Jeremy , Caiazzo Ilaria , Richer Harvey B. 
Published: February 2022

Abstract
We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster within the Gaia EDR3 data set. We find nearly 1300 current cluster members and 289 former cluster candidates. Many of these candidates lie well in front of or behind the cluster from our point of view, so formerly they were considered cluster members, but their parallaxes put them more than 10 pc from the center of the cluster today. Over the past 100 Myr we estimate that the cluster has lost twenty percent of its mass including two massive white dwarf stars and the α
2 Canum Venaticorum type variable star, 41 Tau. All three white dwarfs associated with the cluster are massive (1.01–1.06 M
⊙) and have progenitors with main-sequence masses of about six solar masses. Although we did not associate any giant stars with the cluster, the cooling time of the oldest white dwarf of 60 Myr gives a firm lower limit on the age of the cluster.
Three-body Resonances in the Saturnian System
Authors: Ćuk Matija , El Moutamid Maryame 
Published: February 2022

Abstract
Saturn has a dynamically rich satellite system, which includes at least three orbital resonances between three pairs of moons: Mimas–Tethys 4:2, Enceladus–Dione 2:1, and Titan–Hyperion 4:3 mean-motion resonances. Studies of the orbital history of Saturn’s moons usually assume that their past dynamics was also dominated solely by two-body resonances. Using direct numerical integrations, we find that three-body resonances among Saturnian satellites were quite common in the past, and could result in a relatively long-term, but finite capture time (10 Myr or longer). We find that these three-body resonances are invariably of the eccentricity type and do not appear to affect the moons’ inclinations. While some three-body resonances are located close to two-body resonances (but involve the orbital precession of the third body), others are isolated, with no two-body arguments being near resonance. We conclude that future studies of the system’s past must take full account of three-body resonances, which have been overlooked in the past work.
AGC 226178 and NGVS 3543: Two Deceptive Dwarfs toward Virgo
Authors: Jones Michael G. , Sand David J. , Bellazzini Michele , Spekkens Kristine , Cannon John M. , Mutlu-Pakdil Burçin , Karunakaran Ananthan , Beccari Giacomo , Magrini Laura , Cresci Giovanni , Inoue John L. , Fuson Jackson , Adams Elizabeth A. K. , Battaglia Giuseppina , Bennet Paul , Crnojević Denija , Caldwell Nelson , Guhathakurta Puragra , Haynes Martha P. , Muñoz Ricardo R. , Seth Anil , Strader Jay , Toloba Elisa , Zaritsky Dennis 
Published: February 2022

Abstract
The two sources AGC 226178 and NGVS 3543, an extremely faint, clumpy, blue stellar system and a low surface brightness dwarf spheroidal, are adjacent systems in the direction of the Virgo cluster. Both have been studied in detail previously, with it being suggested that they are unrelated normal dwarf galaxies or that NGVS 3543 recently lost its gas through ram pressure stripping and AGC 226178 formed from this stripped gas. However, with Hubble Space Telescope Advanced Camera for Surveys imaging, we demonstrate that the stellar population of NGVS 3543 is inconsistent with being at the distance of the Virgo cluster and that it is likely a foreground object at approximately 10 Mpc, whereas the stellar population of AGC 226178 is consistent with it being a very young (10–100 Myr) object in the Virgo cluster. Through a reanalysis of the original ALFALFA H i detection, we show that AGC 226178 likely formed from gas stripped from the nearby dwarf galaxy VCC 2034, a hypothesis strengthened by the high metallicity measured with MUSE VLT observations. However, it is unclear whether ram pressure or a tidal interaction is responsible for stripping the gas. Object AGC 226178 is one of at least five similar objects now known toward Virgo. These objects are all young and unlikely to remain visible for over ∼500 Myr, suggesting that they are continually produced in the cluster.
The Lunar Geophysical Network Landing Sites Science Rationale
Authors: Fuqua Haviland Heidi , Weber Renee C. , Neal Clive R. , Lognonné Philippe , Garcia Raphaël F. , Schmerr Nicholas , Nagihara Seiichi , Grimm Robert , Currie Douglas G. , Dell’Agnello Simone , Watters Thomas R. , Panning Mark P. , Johnson Catherine L. , Yamada Ryuhei , Knapmeyer Martin , Ostrach Lillian R. , Kawamura Taichi , Petro Noah , Bremner Paul M. 
Published: February 2022

Abstract
The Lunar Geophysical Network (LGN) mission is proposed to land on the Moon in 2030 and deploy packages at four locations to enable geophysical measurements for 6–10 yr. Returning to the lunar surface with a long-lived geophysical network is a key next step to advance lunar and planetary science. LGN will greatly expand our primarily Apollo-based knowledge of the deep lunar interior by identifying and characterizing mantle melt layers, as well as core size and state. To meet the mission objectives, the instrument suite provides complementary seismic, geodetic, heat flow, and electromagnetic observations. We discuss the network landing site requirements and provide example sites that meet these requirements. Landing site selection will continue to be optimized throughout the formulation of this mission. Possible sites include the P-5 region within the Procellarum KREEP Terrane (PKT; (lat: 15°; long: −35°), Schickard Basin (lat: −44.°3; long: −55.°1), Crisium Basin (lat: 18.°5; long: 61.°8), and the farside Korolev Basin (lat: −2.°4; long: −159.°3). Network optimization considers the best locations to observe seismic core phases, e.g., ScS and PKP. Ray path density and proximity to young fault scarps are also analyzed to provide increased opportunities for seismic observations. Geodetic constraints require the network to have at least three nearside stations at maximum limb distances. Heat flow and electromagnetic measurements should be obtained away from terrane boundaries and from magnetic anomalies at locations representative of global trends. An in-depth case study is provided for Crisium. In addition, we discuss the consequences for scientific return of less than optimal locations or number of stations.
Concepts for the Future Exploration of Dwarf Planet Ceres’ Habitability
Authors: Castillo-Rogez Julie , Brophy John , Miller Kelly , Sori Michael , Scully Jennifer , Quick Lynnae , Grimm Robert , Zolensky Michael , Bland Michael , Buczkowski Debra , Raymond Carol , Hendrix Amanda , Prettyman Thomas , Sekine Yasuhito , Titus Timothy , Williams David , Backes Paul , Barge Laura , Ermakov Anton , Galassi Andrew , Moreland Scott , Zacny Kris 
Published: February 2022

Abstract
Dwarf planet Ceres is a compelling target for future exploration because it hosts at least regional brine reservoirs and potentially ongoing geological activity. As the most water-rich body in the inner solar system, it is a representative of a population of planetesimals that were likely a significant source of volatiles and organics to the inner solar system. Here we describe possible medium-class (around $1 billion) mission concepts that would determine both Ceres’ origin and its current habitability potential. Habitability is addressed through a combination of geological, geophysical, and compositional investigations by (i) searching for evidence from orbit of past and ongoing geological activity near landforms interpreted as brine-driven volcanic structures and (ii) probing the brine distribution below one of these regions with electromagnetic sounding (in situ). Two approaches were considered for compositional measurements, which address both habitability and origins: (1) in situ exploration at two sites and (2) sample return from a single site. Both concepts targeted material at Occator crater, which is one of the youngest features on Ceres (∼20 Ma) and a site rich in evaporites evolved from recently erupted brine sourced from a region >35 km deep. We conclude that a sample return architecture from these young evaporite deposits offers greater science return by enabling high-resolution analysis of organic matter (trapped in salt minerals) and isotopes of refractory elements for a similar cost and less science risk than in situ analyses. This manuscript describes the six science objectives and the two implementation concepts considered to achieve those objectives.
Crater Distributions of Uranus's Mid-sized Satellites and Implications for Outer Solar System Bombardment
Authors: Kirchoff Michelle R. , Dones Luke , Singer Kelsi , Schenk Paul 
Published: February 2022

Abstract
Outer solar system impact bombardment is largely unconstrained. Although recent data from the Jupiter, Saturn, and Pluto systems have produced new constraints, analysis is incomplete without inclusion of the Uranus system. We reanalyze Uranus system crater populations with recent improvements in processing of Voyager 2 imaging. No consensus in crater populations on mid-sized Uranian satellites, Miranda, Ariel, Umbriel, Titania, and Oberon, was resolved during the Voyager era. For satellites with available data, we find variability in crater size–frequency distributions (SFDs) for diameters (D) < 10 km. Most terrains on Miranda show a shallower slope (ratio of smaller to larger craters is smaller), while Inverness Corona on Miranda and Ariel's terrains show a steeper slope (ratio increases). For D > 10 km, satellites with available data show a steeper slope. Shallower-sloped SFDs for D < 10 km and steeper slopes for D > 10 km agree with Pluto system data—a proxy for the heliocentric impactor population originating from the Kuiper Belt—implying these SFDs represent heliocentric bombardment in the Uranus system. The shallow-sloped population for smaller diameters is also observed on Jovian satellites, but not on mid-sized, heavily cratered Saturnian satellites or Triton (Neptune), which have steeper slopes. This implies the heliocentric impactor population originating from the Kuiper Belt reaches throughout the outer solar system, but that the Saturnian, Neptunian, and maybe Uranian systems also might have their own planet-specific impactors. Finally, we find Ariel appears overall younger than the other Uranian satellites, supporting relatively recent geologic activity.