bluuebunny/crossref_metadata_2025_split huggingface dataset:
MANAJEMEN ASIP (ASI PERAH)MEMPENGARUHI KEBERHASILAN ASI EKSKLUSIF (STUDI KUANTITATIF PADA IBUYANG BEKERJA DI INSTANSI PEMERINTAHAN KOTA YOGYAKARTA)
Authors: Rosida Luluk , Putri Intan Mutiara 
Published: February 2020

Latar Belakang : Keberhasilan ASI Ekslusif pada ibu bekerja dipengaruhi oleh keberhasilan manajemen pemberian ASI perah (ASIP). Umumnya ibu yang gagal dalam manajemen ASIP akan segera memberikan susu formula karena merasa ASI ibu jumlahnya kurang, bahkan ada beberapa orang tua yang sengaja mengenalkan susu formula dari awal sebelum mulai bekerja. Bayi yang sudah mendapatkan susu formulacenderung berkurang frekuensi menyusuinya dan berdampak pada menurunnya produksi ASI.
Tujuan: Penelitian ini bertujuan untuk mengetahui hubunganmanajemen ASIP (asi perah) terhadap keberhasilan asi eksklusif (studi kuantitatif pada ibu yang bekerja di instansi pemerintahan kota yogyakarta)
Metode: Penelitian ini menggunakan jenis penelitian kuantitatif. Rancangan atau desain penelitian menggunakan pendekatan cross sectional.Sampel pada penelitian ini berjumlah 44 ibu yang memenuhi kriteria inklusi penelitian.Instrumen penelitian menggunakan kuesioner yang sudah dilakukan uji validitas dan reliabilitas. Metode analisis yang digunakan adalah uji statistik menggunakan analisis bivariat (Chi Square).
Hasil : Karakteristik responden berdasarkan umur ibu paling banyak pada kategori umur > 35 tahun yaitu sebanyak 36 responden (75%), paritas ibu paling banyak berada pada kategori ibu dengan multipara sebanyak 30 responden (62,5%) dan cara persalinan paling banyak adalah persalinan normal yaitu sebesar 32 responden (66,6%). Ibu bekerja yang menerapkan manajemen ASIP yang paling banyak adalah pada kategori tidak tepat yaitu sebanyak 28 responden (58,3%) dan mayoritas responden tidak berhasil memberikan ASI ekslusif yaitu sebanyak 31 responden (64,6%).Hasil uji chi squaremenunjukkannilai p-value : 0,000 (
LAMA PENGGUNAAN KB SUNTIK 3 BULAN DENGAN KEJADIAN SPOTTING DAN AMENORRHEA DI PMB DARMIATI NGEMPLAK BOYOLALI
Authors: Setyorini Catur , Lieskusumastuti Anita Dewi 
Published: February 2020

Latar Belakang : Kontrasepsi hormonal jenis KB suntikan di Indonesia semakin banyak dipakai karena kerjanya yang efektif, pemakaiannya yang praktis, harganya relative murah dan aman. Namun pemberian kontrasepsi suntikan sering menimbulkan gangguan haid seperti siklus haid memendek atau memanjang, perdarahan yang banyak atau sedikit, perdarahan tidak teratur atau perdarahan bercak (spotting) dan tidak haid sama sekali (amenorrhea), dimana gangguan haid ini biasanya bersifat sementara dan sedikit sekali mengganggu kesehatan.Tujuan penelitian ini untuk mengetahui lama penggunaan KB suntik 3 bulan dengan kejadian spotting dan amenorrhea di PMB Darmiati Ngemplak Boyolali Tahun 2019.
Metode : Jenis penelitian ini adalah penelitian analitik observasional, dengan pendekatan cross sectional. Populasi dalam penelitian ini adalah semua akseptor KB suntik 3 bulan di PMB Darmiati Ngemplak Boyolali pada Bulan Juli-Agustus 2019. Teknik pengambilan sampel dengan Accidental Sampling, sehingga sampelnya adalah akseptor KB suntik 3 bulan yang ditemui saat penelitian di PMB Darmiati Ngemplak Boyolali bulan Juli-Agustus 2019 sejumlah 50 responden. Metode pengumpulan data menggunakan data primer dan sekunder, sedangkan analisis data menggunakan uji statistik Chi Square.
Hasil : Hasil penelitian didapatkan mayoritas responden berusia 20-35 tahun sebanyak 25 responden (50%), mayoritas responden berpendidikan dasar (SD,SMP) sebanyak 42 responden (84%), mayoritas responden adalah multipara sebanyak 44 responden (88%), mayoritas responden menggunakan KB suntik 3 bulan ≥ 12 bulan sebanyak 41 responden (82%). Hasil uji statistic lama penggunaan KB suntik 3 bulan dengan kejadian spotting melalui uji chi square diketahui X2hitung 9,374 dengan p-value 0,002 dan hasil uji statistic lama penggunaan KB suntik 3 bulan dengan kejadian amenorrhea melalui uji chi square diketahui X2hitung 4,730 dengan p-value 0,03. Dimana nilai p
Implementasi Model Pendidikan Lingkungan UNESCO Di Sekolah Dasar
Authors: Supadmini Ni Kadek , Wisnu Budi Wijaya I Komang , Larashanti Ida Ayu Diah 
Published: February 2020

Human and the environment have an interdependence relationship. The human survival is depends on the environmental condition and vise versa. In fact, the degradation of environmental quality is mostly happen due to human activities. Therefore, it is necessary to apply the environmental education since primary school age. UNESCO has developed the environmental education model consists of three conceptual, they are education about the environment, education in the environment and education for the environment. This UNESCO environmental education development model is suitable to be applied in primary school for inside or outside classroom activities. The teacher’s role in implementing the environmental education model is as a model, motivator, developer and evaluator.
Hubungan Status Gizi dengan Perkembangan Anak Usia 3 – 5 tahun di Posyandu Tawangsari Mojosongo Jebres Surakarta
Authors: Hanifah Lilik , Riawati Danik 
Published: February 2020

Abstrak
Masa balita yang disebut dengan golden periode, merupakan masa pertumbuhan dan perkembangan yang paling pesat pada otak manusia, masa ini otak bersifat plastis dibandingkan dengan orang dewasa sehingga balita sangat terbuka dan peka dalam menerima berbagai macam pembelajaran dan pengayaan baik bersifat positif maupun negatif. Oleh karena itu kita harus memberi masukan dan nilai-nilai yang postiif, menghindari masukan yang bersifat negatif dan sedapat mungkin memberikan asupan gizi yang adekuat, memberikan stimulasi yang baik dan benar, serta memberikan pelayanan kesehatan yang terbaik bagi anak, sehingga tercapai tumbuh kembang yang optimal.1 Tujuan penelitian ini adalah untuk mengetahui hubungan status gizi dengan perkembangan anak usia 3 – 5 Tahun di Posyandu Tawangsari Mojosongo Jebres Surakarta.
Jenis penelitian ini adalah observasional analitik dengan rancangan cross sectional. Populasi penelitian adalah anak usia 3 – 5 tahun di Posyandu Tawangsari, Mojosongo, Jebres, Surakarta. Sampel penelitian sebanyak 40 anak dengan teknik simple random sampling. Analisis data menggunakan chi square.
Hasil penelitian menunjukkan bahwa ada hubungan status gizi dengan perkembangan pada anak usia 3 – 5 tahun. Semakin tinggi status gizi anak semakin meningkat pula perkembangan anak. Hubungan tersebut secara statistik signifikan (OR= 2,785). Nilai p value adalah 0.000 berarti terdapat hubungan status gizi dengan perkembangan pada anak usia 3 – 5 tahun.
REPRESENTASI CINTA PADA ALLAH DALAM SYAIR RABIâ€™AH AL-ADAWIYAH DAN SYAIR HUSAIN MANSHUR AL-HALLAJ (Kajian Sastra Bandingan)
Authors: Nurhayati Tati 
Published: February 2020

This article aims to examine and describe the representation love for God in the poems both of Rabi'ah al-Adawiyah and al-Hallaj. This study is a comparative literature study, in order to find the relation between the two poems. The method used in this study is descriptive analysis method and comparative method. The results of this study show the meaning of Rabi'ah al-Adawiyahâ€™s love poems and al-Hallaj's love poems. Then it was found that there was a relation between similarities or similarities in terms of the main meanings both of poems, there were also differences in terms of certain meanings and in terms of the style of presentation.
Key word: Representation of Love in Allah, Rabi'ah al-Adawiyahâ€™s poems, al-Hallaj's poems.

Abstrak
Artikel ini bertujuan untuk mengkaji dan memaparkan mengenai representasi cinta pada Allah dalam syair Rabiâ€™ah al-Adawiyah dan syair al-Hallaj. Kajian ini merupakan kajian sastra banding, guna menemukan keterkaitan antara kedua syair tersebut. Metode yang digunakan dalam kajian ini adalah metode deskriptif analisis dan metode komparatif. Hasil dari penelitian ini menunjukkan makna dalam syair cinta Rabiâ€™ah al-Adawiyah dan syair cinta al-Hallaj. Kemudian ditemukan adanya keterkaitan kemiripan atau persamaan dalam segi makna pokok kedua syair tersebut, juga terdapat perbedaan pada segi makna tertentu dan dari segi gaya penyajiannya.
Kata Kunci:Representasi Cinta Pada Allah, Syair Rabiâ€™ah al-Adawiyah,Syair al-Hallaj.
Filsafat Pendidikan Islam dalam Perspektif al-Ghazali dan Ibnu Khaldun
Authors: Fathorrahman Fathorrahman 
Published: February 2020

In-depth, comprehensive, systematic and radical discussion of the educational problems above is the most appropriate alternative. The philosophical approach is very appropriate to unravel the tangled thread of the problem of education in Indonesia, especially Islamic education. The reason is that the majority of Indonesian Muslims are still bound by the thought of liberalism and conservatism. So that Islamic education as a whole is divided
Abstrak
Pembahasan mendalam, menyeluruh, sistematis dan juga radikal terhadap problematika pendidikan di atas adalah alternatif yang paling tepat. Pendekatan filsafat sangat tepat untuk mengurai benang kusut problematika pendidikan di Indonesia, khusunya pendidikan Islam. Pasalnya, masyarakat Indonesia yang mayoritas Muslim, masih saja terbelenggu oleh pemikiran antara liberalisme dan konservatisme. Sehingga pendidikan Islam secara kesuluruhan terbelah
Implementasi Imtaq dalam Kehidupan Mahasiswa
Authors: Aisyah Siti 
Published: February 2020

A moral crisis is a precarious condition in a society or group in which there is a deterioration or damage to actions, attitudes, morals and character. This moral crisis is seen in Indonesian society, both among young people, even parents and even small children. This moral crisis is indicated by the proliferation of acts that approach adultery or even adultery, the culture of smoking or even illegal drugs and intoxicants (khamr). In addition, the existence of a community that is disturbing the community or even criminal and brutal acts that have mushroomed in the community has also triggered a moral crisis. Not only that, but there are still many more indications of a moral crisis found in society.
Abstrak
Krisis moral adalah suatu kondisi genting dalam suatu masyarakat atau kelompok yang mana terjadinya kemerosotan atau kerusakan perbuatan, sikap, akhlak dan budi pekerti. Krisis moral ini terlihat di dalam masyarakat Indonesia, baik itu pada kalangan pemuda, orang tua bahkan kalangan anak kecil sekali pun. Krisis moral ini terindikasi dengan maraknya perbuatan yang mendekati zina atau bahkan zina, kebudayaan merokok atau bahkan obat-obatan terlarang dan minuman memabukkan (khamr). Selain itu juga adanya komunitas yang meresahkan masyarakat atau bahkan tindak kriminal dan brutal yang menjamur di masyarakat juga memicu adanya krisis moral. Tidak hanya itu, namun masih banyak lagi indikasi krisis moral yang terdapat di dalam masyarakat.
Membangun Kreatifitas Generasi Muslim
Authors: Hendriyadi H. Imam 
Published: February 2020

The holy koran, itâ€™s contains all fields of human life, there are related to economic, political, socio-cultural, science and technology, to the problem of morality and personality development. All of that contained in the qur an. In fact, it is also true to say that al qur an is legislation as well as a basic human in living life.

Abstrak
Al-Qur an, pada hakekatnya memuat seluruh bidang kehidupan manusia, baik terkait dengan aspek ekonomi, politik, sosial-budaya, maupun ilmu pengetahuan dan teknologi, hingga masalah moralitas dan pembangunan kepribadian. Semua itu termaktub dalam Al-Qur an. Bahkan, benar juga jika dikatakan bahwa Al-Qur an merupakan undang-undang dan peraturan umum, sekaligus merupakan kaedah dasar manusia dalam menjalani kehidupannya.
OGLE-2016-BLG-1227L: A Wide-separation Planet from a Very Short-timescale Microlensing Event
Authors: Han Cheongho , Udalski Andrzej , Gould Andrew ,   (Leading Authors), Albrow Michael D. , Chung Sun-Ju , Hwang Kyu-Ha , Jung Youn Kil , Lee Chung-Uk , Ryu Yoon-Hyun , Shin In-Gu , Shvartzvald Yossi , Yee Jennifer C. , Zang Weicheng , Cha Sang-Mok , Kim Dong-Jin , Kim Hyoun-Woo , Kim Seung-Lee , Lee Dong-Joo , Lee Yongseok , Park Byeong-Gon , Pogge Richard W. , Jee M. James , Kim Doeon , Kim Chun-Hwey , Kim Woong-Tae ,   (The KMTNet Collaboration), Mróz Przemek , Szymański Michał K. , Skowron Jan , Poleski Radek , Soszyński Igor , Pietrukowicz Paweł , Kozłowski Szymon , Ulaczyk Krzysztof ,   (The OGLE  Collaboration)
Published: February 2020

Abstract
We present the analysis of the microlensing event OGLE-2016-BLG-1227. The light curve of this short-duration event appears to be a single-lens event affected by severe finite-source effects. Analysis of the light curve based on a single-lens single-source (1L1S) model yields very small values of the event timescale,

days, and the angular Einstein radius,

mas, making the lens a candidate of a free-floating planet. Close inspection reveals that the 1L1S solution leaves small residuals with an amplitude of ΔI ≲ 0.03 mag. We find that the residuals are explained by the existence of an additional widely separated heavier lens component, indicating that the lens is a wide-separation planetary system rather than a free-floating planet. From Bayesian analysis, it is estimated that the planet has a mass of

and it is orbiting a low-mass host star with a mass of

located with a projected separation of

au. The planetary system is located in the Galactic bulge with a line-of-sight separation from the source star of

kpc. The event shows that there is a range of deviations in the signatures of host stars for apparently isolated planetary lensing events and that it is possible to identify a host even when a deviation is subtle.
WISE 2150-7520AB: A Very Low-mass, Wide Comoving Brown Dwarf System Discovered through the Citizen Science Project Backyard Worlds: Planet 9*
Authors: Faherty Jacqueline K. , Goodman Sam , Caselden Dan , Colin Guillaume , Kuchner Marc J. , Meisner Aaron M. , Gagné Jonathan , Schneider Adam C. , Gonzales Eileen C. , Bardalez Gagliuffi Daniella C. , Logsdon Sarah E. , Allers Katelyn , Burgasser Adam J. ,   The Backyard Worlds: Planet 9 Collaboration
Published: February 2020

Abstract
We report the discovery of WISE 2150-7520AB (W2150AB): a widely separated (∼341 au) very low-mass L1 + T8 co-moving system. The system consists of the previously known L1 primary 2MASS J21501592-7520367 and a newly discovered T8 secondary found at position 21:50:18.99–75:20:54.6 (MJD = 57947) using Wide-field Infrared Survey Explorer data via the Backyard Worlds: Planet 9 citizen science project. We present Spitzer ch1 and ch2 photometry (ch1–ch2 = 1.41 ± 0.04 mag) of the secondary and Folded-port InfraRed Echellette prism spectra of both components. The sources show no peculiar spectral or photometric signatures, indicating that each component is likely field age. Using all observed data and the Gaia DR2 parallax of 41.3593 ± 0.2799 mas for W2150A we deduce fundamental parameters of log(L
bol/L
☉) = −3.69 ± 0.01, T
eff = 2118 ± 62 K, and an estimated mass = 72 ± 12 M
Jup for the L1 and log(L
bol/L
☉) = −5.64 ± 0.02, T
eff = 719 ± 61 K, and an estimated mass = 34 ± 22 M
Jup for the T8. At a physical separation of ∼341 au this system has E
bin = 1041 erg, making it the lowest binding energy system of any pair with M
tot < 0.1 M
Sun not associated with a young cluster. It is equivalent in estimated mass ratio, E
bin, and physical separation to the ∼2 Myr M7.25 + M8.25 binary brown dwarf 2MASS J11011926-7732383AB (2M1101AB) found in the Chameleon star-forming region. W2150AB is the widest companion system yet observed in the field where the primary is an L dwarf or later.
Evidence for a Multipolar Magnetic Field in SGR J1745-2900 from X-Ray Light-curve Analysis
Authors: de Lima Rafael C. R. , Coelho Jaziel G. , Pereira Jonas P. , Rodrigues Claudia V. , Rueda Jorge A. 
Published: February 2020

Abstract
SGR J1745-2900 was detected from its outburst activity in 2013 April and it was the first soft gamma repeater (SGR) detected near the center of the Galaxy (Sagittarius A*). We use 3.5 yr Chandra X-ray light-curve data to constrain some neutron star (NS) geometric parameters. We assume that the flux modulation comes from hot spots on the stellar surface. Our model includes the NS mass, radius, a maximum of three spots of any size, temperature and positions, and general relativistic effects. We find that the light curve of SGR J1745-2900 could be described by either two or three hot spots. The ambiguity is due to the small amount of data, but our analysis suggests that one should not disregard the possibility of multi-spots (due to a multipolar magnetic field) in highly magnetized stars. For the case of three hot spots, we find that they should be large and have angular semiapertures ranging from 16° to 67°. The large size found for the spots points to a magnetic field with a nontrivial poloidal and toroidal structure (in accordance with magnetohydrodynamics investigations and Neutron Star Interior Composition Explorer’s (NICER) recent findings for PSR J0030+0451) and is consistent with the small characteristic age of the star. Finally, we also discuss possible constraints on the mass and radius of SGR J1745-2900 and briefly envisage possible scenarios accounting for the 3.5 yr evolution of SGR J1745-290 hot spots.
Two New Outbursts and Transient Hard X-Rays from 1E 1048.1-5937
Authors: Archibald R. F. , Scholz P. , Kaspi V. M. , Tendulkar S. P. , Beardmore A. P. 
Published: February 2020

Abstract
Since its discovery, 1E 1048.1−5937 has been one of the most active magnetars, both in terms of radiative outbursts, and changes to its spin properties. Here we report on a continuing monitoring campaign with the Neil Gehrels Swift Observatory X-ray Telescope in which we observe two new outbursts from this source. The first outburst occurred in 2016 July, and the second in 2017 December, reaching peak 0.5–10 keV absorbed fluxes of

erg s−1 cm−2 and

erg s−1 cm−2, respectively, factors of ∼5 and ∼4 above the quiescent flux. Both new outbursts were accompanied by spin-up glitches with amplitudes of

Hz and

Hz, respectively. Following the 2016 July outburst, we observe, as for past outbursts, a period of delayed torque fluctuations, which reach a peak spin-down of 1.73 ± 0.01 times the quiescent rate, and which dominates the spin evolution compared to the spin-up glitches. We also report an observation near the peak of the first of these outbursts with NuSTAR in which hard X-ray emission is detected from the source. This emission is well characterized by an absorbed blackbody plus a broken power law, with a power-law index above 13.4 ± 0.6 keV of

, similar to those observed in both persistent and transient magnetars. The hard X-ray results are broadly consistent with models of electron/positron cooling in twisted magnetic field bundles in the outer magnetosphere. However, the repeated outbursts and associated torque fluctuations in this source remain puzzling.
The Roles of Mass and Environment in the Quenching of Galaxies. II.
Authors: Contini E. , Gu Q. , Ge X. , Rhee J. , Yi S. K. , Kang X. 
Published: February 2020

Abstract
We take advantage of an analytic model of galaxy formation coupled to the merger tree of an N-body simulation to study the roles of environment and stellar mass in the quenching of galaxies. The model has been originally set in order to provide the observed evolution of the stellar mass function as well as reasonable predictions of the star formation rate–stellar mass relation, from high redshift to the present time. We analyze the stellar mass and environmental quenching efficiencies and their dependence on stellar mass, halo mass (taken as a proxy for the environment), and redshift. Our analysis shows that the two quenching efficiencies are dependent on redshift and stellar and halo mass, and that the halo mass is also a good proxy for the environment. The environmental quenching increases with decreasing redshift and is inefficient below log M
* ∼ 9.5, reaches the maximum value at log M
* ∼ 10.5, and decreases again, becoming poorly efficient at very high stellar mass (log M
* ≳ 11.5). Central and satellites galaxies are mass quenched differently: for the former, the quenching efficiency depends very weakly on redshift but strongly on stellar mass; for the latter, it strongly depends on both stellar mass and redshift in the range

. According to the most recent observational results, we find that the two quenching efficiencies are not separable: intermediate-mass galaxies, as well as intermediate/massive galaxies in more massive halos, are environmentally quenched faster. At stellar masses lower than log M
* ≲ 9.5, both quenching mechanisms become inefficient, independently of the redshift.
Ion-scale Electromagnetic Waves in the Inner Heliosphere
Authors: Bowen Trevor A. , Mallet Alfred , Huang Jia , Klein Kristopher G. , Malaspina David M. , Stevens Michael , Bale Stuart D. , Bonnell J. W. , Case Anthony W. , Chandran Benjamin D. G. , Chaston C. C. , Chen Christopher H. K. , Dudok de Wit Thierry , Goetz Keith , Harvey Peter R. , Howes Gregory G. , Kasper J. C. , Korreck Kelly E. , Larson Davin , Livi Roberto , MacDowall Robert J. , McManus Michael D. , Pulupa Marc , Verniero J. L. , Whittlesey Phyllis ,   (The PSP/FIELDS and PSP/SWEAP Teams)
Published: February 2020

Abstract
Understanding the physical processes in the solar wind and corona that actively contribute to heating, acceleration, and dissipation is a primary objective of NASA’s Parker Solar Probe (PSP) mission. Observations of circularly polarized electromagnetic waves at ion scales suggest that cyclotron resonance and wave–particle interactions are dynamically relevant in the inner heliosphere. A wavelet-based statistical study of circularly polarized events in the first perihelion encounter of PSP demonstrates that transverse electromagnetic waves at ion resonant scales are observed in 30–50% of radial field intervals. Average wave amplitudes of approximately 4 nT are measured, while the mean duration of wave events is on the order of 20 s; however, long-duration wave events can exist without interruption on hour-long timescales. Determination of wave vectors suggests propagation parallel/antiparallel to the mean magnetic field. Though ion-scale waves are preferentially observed during intervals with a radial mean magnetic field, we show that measurement constraints, associated with single spacecraft sampling of quasi-parallel waves superposed with anisotropic turbulence, render the measured coherent ion-wave spectrum unobservable when the mean magnetic field is oblique to the solar wind flow; these results imply that the occurrence of coherent ion-scale waves is not limited to a radial field configuration. The lack of radial scaling of characteristic wave amplitudes and duration suggests that the waves are generated in situ through plasma instabilities. Additionally, observations of proton distribution functions indicate that temperature anisotropy may drive the observed ion-scale waves.