bluuebunny/crossref_metadata_2025_split huggingface dataset:
Entorno a la dudosa clasificación de escrituras judiciales. / The doubtful classification of judicial deeds.
Authors: Piccon Augusto 
Published: June 2022

SUMARIO
Introducción. Desarrollo. A- ¿En base a qué clasificamos? B - ¿A partir de qué hablamos de escrituras judiciales? *Escrituras de recopilación de antecedentes judiciales. C- Origen de la clasificación: *Escrituras de Protocolización: Casos. El término Técnico. ¿Fin que persigue? ¿Es una Escritura? Designación del Escribano. Transcripción. Escrituras de Ejecución Forzada. D- Criterios de la relación del expediente. Modelos de la Doctrina según: Falbo Dalessio. Villalba Welsh, Heguy. Conclusión.ABSTRACT
Introduction. Developing. A- On what basis do we classify? B - From what do we speak of judicial deeds? *Writs of compilation of judicial antecedents. C- Origin ofthe classification: * Protocolization Deeds: Cases. The technical term. End pursued? Is it a Scripture? Appointment of the Notary. Transcription. Deeds of Forced Execution. D- Criteria of the relation of the file. Models of the Doctrine according to: Falbo Dalessio. Villalba Welsh, Heguy. Conclution.
EFEKTIVITAS PENDIDIKAN KESEHATAN STUNTING DENGAN METODE DARING TERHADAP PERILAKU PENCEGAHAN STUNTING
Authors: Ditya Yankusuma Setiani  , Sriwiyati Lilik 
Published: June 2022

Latar Belakang : Stunting adalah kondisi dimana balita memiliki panjang atau tinggi badan yang kurang jika dibandingkan dengan umur. Kecamatan Kebonarum Klaten masih terdapat balita dengan stunting yaitu 2 % dari 1000 anak. Mayoritas ibu tidak mengetahui tentang pencegahan stunting.

Tujuan dan Manfaat : Mengetahui kefektifan pendidikan kesehatan stunting dengan metode daring terhadap perilaku pencegahan stunting

Subjek dan Metode : Responden penelitian ini adalah 31 orang. Desain penelitian quasy experimental dengan rancangan pre test dan post test. Data dianalisis dengan Paired T-Test.

Hasil Penelitian : Untuk nilai rata-rata perilaku sebelum diberi penyuluhan 13,48 dan sesudah diberi penyuluhan 13,94 dan hasil paired t-test 0,000 maka dapat disimpulkan bahwa ada peningkatan perilaku pencegahan setelah diberi peyuluhan.
Kesimpulan : Pendidikan kesehatan secara daring efektif untuk meningkatkan perilaku pencegahan stunting.

Kata kunci : Pendidikan Kesehatan, Perilaku Pencegahan Stunting, Daring

THE EFFECTIVENESS OF STUNTING HEALTH EDUCATION WITH ONLINE METHODS ON STUNTING PREVENTION BEHAVIORIN THE VILLAGE OF CENTRAL KLATEN REGENCY

Ditya Yankusuma Setiani, Lilik Sriwiyati

INSTITUTE OF HEALTH SCIENCE OF PANTI KOSALA, Sukoharjo, Central Java, Indonesia

Abstract

Background: Stunting is a condition where toddlers have a length or height that is less than their age. In Kebonarum District, Klaten, there are still toddlers with stunting, which is 2% of 1000 children. The majority of mothers do not know about stunting prevention.The Aim of the study: Knowing the effectiveness of stunting health education with online methods on stunting prevention behaviorSubjects and Methods: The respondents of this study were 31 people. Quasy experimental research design with pre test and post test designs. Data were analyzed by Paired T-Test.Research results: the average value of behavior before being given counseling is 13.48 and after being given counseling is 13.94 and the paired t-test result is 0.000, it can be concluded that there is an increase in preventive behavior after being given counseling.Conclusion: Online health education is effective to improve stunting prevention behavior.

Keywords: Health Education, Stunting Prevention Behavior, Online
RHETORIC DA'WAH MEDINA PERIOD
Authors: Tohir Sya’roni 
Published: June 2022

Tujuan Penelitian : penelitian ini bertujuan untuk mengetahui bagaimana Retorika Da’wah Periode Madinah. Hasil penelitian : Rethorika da’wah ialah keterampilan berbahasa secara efektif, memuaskan dan kecerdasan dalam menyampaikan dan menampilkan ajaran Islam yang dapat digunakan untuk menyeru dan mengajak orang (manusia) ke dalam agama Islam, serta mempelajarinya, mengamalkannya dan mensyiarkannya dengan baik. Allah subahanahu wa ta’ala dalam firman-firman-Nya banyak menyeru kepada hamba-hamba-Nya dengan seruan yang khithabnya (komunikannya) umum (hai manusia), ada yang khitabnya kepada golongan tertentu seperti hai orang-orang yang beriman, hai ahlul kitab, hai bani Israil, hai orang-orang kafir, ada juga yang sangat khusus seperti : “hai hamba-hambaku,” ya adam” dan “ya Ibrohim”. Seruan-seruan ini dapat menggabarkan kasih saying, sanjungan, penghormatan, kedekatan, ketegasan, keberanian, kemuliaan dan ketinggian martabat komunikator dan lain-lain. Bila diteliti lebih mendalam lagi, Bahasa seruan itu juga ada yang dipengaruhi oleh kontek situasi dan kondisi komunikator. Kapan dan di mana komunikator itu berada dan dalam situasi menang atau kalah. Bermartabat, sederajat atau hina di hadapan komunikannya. Kesimpulan : retorika da’wah rasulullah shallallahu ‘alaihi wa sallam pada periode Madinah ada yang besifat umum dan retorika khusus pula. Ada retorika yang menggambarkan bahwa islam itu memiliki ‘izzah (martabat yang tinggi). Retorika Islam yang santun, retorika islam itu mulia dan bermartabat. Retorika Islam itu adalah retorika yang singkat, padat, jelas, lugas, tegas, bahasanya mudah dan indah.
The Transmission Spectrum of WASP-17 b From the Optical to the Near-infrared Wavelengths: Combining STIS, WFC3, and IRAC Data Sets
Authors: Saba Arianna , Tsiaras Angelos , Morvan Mario , Thompson Alexandra , Changeat Quentin , Edwards Billy , Jolly Andrew , Waldmann Ingo , Tinetti Giovanna 
Published: June 2022

Abstract
We present the transmission spectrum of the inflated hot Jupiter WASP-17 b, observed with the STIS and WFC3 instruments aboard the Hubble Space Telescope, allowing for a continuous wavelength coverage from ∼0.4 to ∼1.7 μm. Observations taken with IRAC channels 1 and 2 on the Spitzer Space Telescope are also included, adding photometric measurements at 3.6 and 4.5 μm. HST spectral data were analyzed with Iraclis, a pipeline specialized in the reduction of STIS and WFC3 transit and eclipse observations. Spitzer photometric observations were reduced with the TLCD-LSTM method, utilizing recurrent neural networks. The outcome of our reduction produces incompatible results between STIS visit 1 and visit 2, which leads us to consider two scenarios for G430L. Additionally, by modeling the WFC3 data alone, we can extract atmospheric information without having to deal with the contrasting STIS data sets. We run separate retrievals on the three spectral scenarios with the aid of TauREx 3, a fully Bayesian retrieval framework. We find that, independently of the data considered, the exoplanet atmosphere displays strong water signatures and, potentially, the presence of aluminum oxide and titanium hydride. A retrieval that includes an extreme photospheric activity of the host star is the preferred model, but we recognize that such a scenario is unlikely for an F6-type star. Due to the incompleteness of all STIS spectral light curves, only further observations with this instrument would allow us to properly constrain the atmospheric limb of WASP-17 b, before the James Webb Space Telescope or Ariel will come online.
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): How Do Dense Core Properties Affect the Multiplicity of Protostars?
Authors: Luo 罗 Qiu-yi 秋怡 , Liu 刘 Tie 铁 , Tatematsu Ken’ichi , Liu Sheng-Yuan , Li Pak Shing , di Francesco James , Johnstone Doug , Goldsmith Paul F. , Dutta Somnath , Hirano Naomi , Lee Chin-Fei , Li Di , Kim Kee-Tae , Won Lee Chang , Lee Jeong-Eun , Liu Xun-chuan , Juvela Mika , He Jinhua , Qin Sheng-Li , Liu Hong-Li , Eden David , Kwon Woojin , Sahu Dipen , Li Shanghuo , Xu Feng-Wei , Zhang Si-ju , Hsu Shih-Ying , Bronfman Leonardo , Sanhueza Patricio , Pelkonen Veli-Matti , Zhou Jian-wen , Liu Rong , Gu Qi-lao , Wu Yue-fang , Mai Xiao-feng , Falgarone Edith , Shen Zhi-Qiang 
Published: June 2022

Abstract
During the transition phase from a prestellar to a protostellar cloud core, one or several protostars can form within a single gas core. The detailed physical processes of this transition, however, remain unclear. We present 1.3 mm dust continuum and molecular line observations with the Atacama Large Millimeter/submillimeter Array toward 43 protostellar cores in the Orion molecular cloud complex (λ Orionis, Orion B, and Orion A) with an angular resolution of ∼0.″35 (∼140 au). In total, we detect 13 binary/multiple systems. We derive an overall multiplicity frequency (MF) of 28% ± 4% and a companion star fraction (CSF) of 51% ± 6%, over a separation range of 300–8900 au. The median separation of companions is about 2100 au. The occurrence of stellar multiplicity may depend on the physical characteristics of the dense cores. Notably, those containing binary/multiple systems tend to show a higher gas density and Mach number than cores forming single stars. The integral-shaped filament of the Orion A giant molecular cloud (GMC), which has the highest gas density and hosts high-mass star formation in its central region (the Orion Nebula cluster), shows the highest MF and CSF among the Orion GMCs. In contrast, the λ Orionis GMC has a lower MF and CSF than the Orion B and Orion A GMCs, indicating that feedback from H ii regions may suppress the formation of multiple systems. We also find that the protostars comprising a binary/multiple system are usually at different evolutionary stages.
The In Situ Origins of Dwarf Stellar Outskirts in FIRE-2
Authors: Kado-Fong Erin , Sanderson Robyn E. , Greene Jenny E. , Cunningham Emily C. , Wheeler Coral , Chan T. K. , El-Badry Kareem , Hopkins Philip F. , Wetzel Andrew , Boylan-Kolchin Michael , Faucher-Giguère Claude-André , Huang Song , Quataert Eliot , Starkenburg Tjitske 
Published: June 2022

Abstract
Extended, old, and round stellar halos appear to be ubiquitous around high-mass dwarf galaxies (108.5 < M
⋆/M
⊙ < 109.6) in the observed universe. However, it is unlikely that these dwarfs have undergone a sufficient number of minor mergers to form stellar halos that are composed of predominantly accreted stars. Here, we demonstrate that FIRE-2 (Feedback in Realistic Environments) cosmological zoom-in simulations are capable of producing dwarf galaxies with realistic structures, including both a thick disk and round stellar halo. Crucially, these stellar halos are formed in situ, largely via the outward migration of disk stars. However, there also exists a large population of “nondisky” dwarfs in FIRE-2 that lack a well-defined disk/halo and do not resemble the observed dwarf population. These nondisky dwarfs tend to be either more gas-poor or to have burstier recent star formation histories than the disky dwarfs, suggesting that star formation feedback may be preventing disk formation. Both classes of dwarfs underscore the power of a galaxy’s intrinsic shape—which is a direct quantification of the distribution of the galaxy’s stellar content—to interrogate the feedback implementation in simulated galaxies.
Study of Transverse Oscillations in Coronal Loops Excited by Flares and Eruptions
Authors: Conde C. Sandra M. , Jain Rekha , Jatenco-Pereira Vera 
Published: June 2022

Abstract
We present measurements of periodicity for transverse loop oscillations during the periods of activity of two remote and separated (both temporally and spatially) flares. The oscillations are observed in the same location more than 100 Mm away from the visible footpoints of the loops. Evidence for several possible excitation sources is presented. After close examination, we find that the eruptions during the flaring activities play an important role in triggering the oscillations. We investigate periodicities using time–distance, fast Fourier transform, and wavelet techniques. Despite different excitation sources in the vicinity of the loops and the changing nature of amplitudes, the periodicity of multiple oscillations is found to be 4–6 min.
First Experimental Confirmation of the CH3O + H2CO → CH3OH + HCO Reaction: Expanding the CH3OH Formation Mechanism in Interstellar Ices
Authors: Santos Julia C. , Chuang Ko-Ju , Lamberts Thanja , Fedoseev Gleb , Ioppolo Sergio , Linnartz Harold 
Published: June 2022

Abstract
The successive addition of H atoms to CO in the solid phase has been hitherto regarded as the primary route to form methanol in dark molecular clouds. However, recent Monte Carlo simulations of interstellar ices alternatively suggested the radical-molecule H-atom abstraction reaction CH3O + H2CO → CH3OH + HCO, in addition to CH3O + H → CH3OH, as a very promising and possibly dominating (70%–90%) final step to form CH3OH in those environments. Here, we compare the contributions of these two steps leading to methanol by experimentally investigating hydrogenation reactions on H2CO and D2CO ices, which ensures comparable starting points between the two scenarios. The experiments are performed under ultrahigh vacuum conditions and astronomically relevant temperatures, with H:H2CO (or D2CO) flux ratios of 10:1 and 30:1. The radical-molecule route in the partially deuterated scenario, CHD2O + D2CO → CHD2OD + DCO, is significantly hampered by the isotope effect in the D-abstraction process, and can thus be used as an artifice to probe the efficiency of this step. We observe a significantly smaller yield of D2CO + H products in comparison to H2CO + H, implying that the CH3O-induced abstraction route must play an important role in the formation of methanol in interstellar ices. Reflection-absorption infrared spectroscopy and temperature-programmed desorption-quadrupole mass spectrometry analyses are used to quantify the species in the ice. Both analytical techniques indicate constant contributions of ∼80% for the abstraction route in the 10–16 K interval, which agrees well with the Monte Carlo calculations. Additional H2CO + D experiments confirm these conclusions.
New Polarimetric Data for the Galilean Satellites: Europa Observations and Modeling
Authors: Kiselev Nikolai , Rosenbush Vera , Muinonen Karri , Kolokolova Ludmilla , Savushkin Aleksandr , Karpov Nikolai 
Published: June 2022

Abstract
This paper is dedicated to a long-standing problem of the shape of the negative branch of polarization (NBP) for Jupiter's moon Europa, determination of which is crucial for the characterization of the icy regolith on this satellite and similar objects, as well as for further progress in understanding light scattering by particulate surfaces. To establish the shape of Europa's NBP, in 2018–2021 we accomplished high-precision disk-integrated polarimetry of Europa in the UBVR
I bands using the identical two-channel photoelectric polarimeters mounted on the 2.6 m Shajn reflector of the Crimean Astrophysical Observatory and the 2 m telescope of the Peak Terskol Observatory. We found that the polarization dependence on the phase angle in each filter is an asymmetric curve with a sharp polarization minimum

P

min

≈
−
0.3
%

at phase angle

α

min

≤
0
.°
4

, after which the polarization degree gradually increases to positive values, passing the inversion angle at α
inv ≈ 6° − 7°. Within the error limits, the parameters P
min,

α

min

, and α
inv of the NPB are independent of the wavelength in the visible spectrum. The polarization curve clearly demonstrates the so-called polarization opposition effect (POE). Our analysis of the previous and new polarimetric observations of Europa allows us to conclude that the POE is caused by coherent backscattering of sunlight on microscopic icy grains covering Europa’s surface. Computer modeling with the numerical radiative transfer coherent backscattering method demonstrates that the best fit to the polarimetric observations and geometric albedo of Europa is provided by a regolith layer of elementary single-scattering albedo ∼0.985 and extinction mean free path length 2π
l/λ
eff ≈ 150, λ
eff representing the effective wavelength in the UBVR
I spectral bands.
Observational Study on Outcomes after Radioiodine Ablation in Hyperthyroid Patients
Authors: Pamnani Harsha , Jindal Radhika , Khare Jaideep , Sharma Monika , Siddiqui Asim , Wangnoo Subhash K. 
Published: June 2022

Introduction:
Radio-active Iodine (RAI) is a safe, definitive, and cost-effective modality of treatment that is used as the first line of treatment for Graves’ hyperthyroidism by most endocrinologists. Very few reports are available from India, observational follow-up data is needed to determine the meaningful prognostic outcomes of RAI ablation in the Indian population.

Aims:
To study the outcomes in hyperthyroid patients undergoing RAI ablation.

Materials and Methods:
This observational cohort study was conducted at Department of Endocrinology at Indraprastha Apollo Hospital, New Delhi. A total of 82 hyperthyroid patients who underwent RAI ablation between June 2014 to June 2018 were enrolled. RAI dose was calculated arbitrarily in most cases; often by an empirical fixed dose based on the goiter size and RAIU. The patients were reviewed at 1, 3 and 6 months post-RAI ablation. During follow-up, along with a detailed clinical examination, free T4, free T3 and TSH were checked.

Results:
The dose of I-131 varied from 6 mCi to 14 mCi. Most of the patients were given RAI in the dose of 7.1-10 mci. About 63.4% of patients achieved hypothyroidism in 6 months, 6.1% in 1 month, 37.8% in 3 months, and 19.5% in 6 months. Gender, age, etiology of hyperthyroidism, baseline thyroid function, goiter, and ophthalmopathy did not affect outcomes after RAI ablation. Those who were not treated with antithyroid drugs prior to RAI therapy were found to have higher rates of conversion to a hypothyroid state.

Conclusion:
RAI can be given safely as the first line of treatment in Graves’ disease and antithyroid drug naïve patients respond better to therapy.
Clinicopathological Characteristics and Treatment Outcome of Patients with Metastatic Differentiated Thyroid Cancer
Authors: Aziz Abdul , Khan Sajjad Ali , Suchal Zafar A. , Islam Najmul 
Published: June 2022

Background and Objective:
Differentiated thyroid carcinoma (DTC) is a slow-growing tumour with 20% of the cases having distant metastasis. Its prognosis can vary by its histological characteristics, extension and spread. The data on metastatic DTC patients in Pakistan is scarce; therefore, the purpose of our study was to assess the clinicopathological characteristics and treatment outcomes of metastatic DTC in our population.

Methods:
This retrospective, single-centre study was carried out on 117 patients with metastatic DTC with their age at diagnosis, gender, tumour size and extent and spread of the tumour, and its histologic characteristic recorded. The treatment they received and the outcome in terms of status, at last, follow-up were also recorded.

Results:
The mean age of diagnosis was found to be 46.6 ± 17.2 years with an almost equal male to female ratio. The most common site of metastasis was the lung followed by bone. Papillary carcinoma was the most common subtype with 89.7% of the cases followed by follicular carcinoma occurring in 7.7%. The overall survival in years was found to be 5.6 ± 2.6 years. Ninety-six per cent had complete surgical resection followed by radioactive iodine (RAI) in 91.5%.

Conclusion:
Our study shows that the most significant factors in predicting the outcome in metastatic DTC are age, an extrathyroidal extension of the primary tumour and distant metastasis. However, further multicentric studies done on a much larger population will be needed to further support and strengthen our results.
Prevalence & spectrum of congenital anomalies at a tertiary care centre in north India over 20 years (1998-2017)
Authors: Kumar Jogender , Saini Shiv Sajan , Sundaram Venkataseshan , Mukhopadhyay Kanya , Dutta Sourabh , Kakkar Nandita , Kumar Praveen 
Published: June 2022

Background & objectives:
Congenital anomalies lead to significant morbidity and mortality. Systematically published data on the prevalence and spectrum of congenital anomalies from India are scarce. This study was aimed to ascertain the prevalence, spectrum, trend, and outcome of congenital anomalies at a tertiary care centre in north India over two decades.

Methods:
Electronic records of all live births from January 1998 to December 2017 were retrieved, and the neonates with congenital anomaly were included in this retrospective analysis. International Statistical Classification of Diseases and Related Health Problems, tenth revision (ICD-10) was used for uniformity and international comparison. The further sub-categorization was done as per the WHO birth defects surveillance manual. The prevalence of individual as well as overall congenital anomalies was calculated. Run charts were used to analyze the trends.

Results:
In the two decades studied (1998-2017), there were 86850 live births, of which 1578 [1.82%, 95% confidence interval (CI): 1.73-1.91%] neonates had a major congenital anomaly. The overall prevalence of anomalies was 182 (95% CI: 173-191) per 10,000 live births. Malformation of the circulatory system was the most common (28.0%) followed by musculoskeletal (18.6%) and urinary system (14.3%). Congenital anomaly-related death rate was 6.78 per 1000 live births. No significant trend was observed in the annual prevalence, individual malformations or contribution of congenital anomalies to overall mortality over the two decades.

Interpretation & conclusions:
Our results showed a high prevalence of congenital anomalies which could be responsible for significant mortality, warranting the need for a national surveillance programme and birth defect services. It is important to have a national database to know the overall burden and spectrum of congenital anomalies in the country.
Tobacco use among college students in Kerala, India
Authors: Jaisoorya T.S. , Ganjekar Sundarnag , Menon Priya G. , Nair B. Sivasankaran , Rani Anjana , Thennarassu K. 
Published: June 2022

Background & objectives:
Despite tobacco use among college students being a major health concern, data remain sparse from India. It is in this background that this study aimed to report the prevalence of tobacco use and its psychosocial correlates among college students in the State of Kerala, India.

Methods:
A total of 5784 students from 58 colleges from Ernakulam district, Kerala, selected by cluster random sampling and were provided with self-administered questionnaire. In addition to socio-demographic profile, the questionnaire incorporated alcohol, smoking, and substance involvement screening test (ASSIST, for assessing tobacco use and its severity, lifetime use of other substances); Kessler’s scale (psychological distress) and Barkeley’s scale (attention deficit hyperactivity disorder symptoms). Screening questions were used for assessing lifetime suicidality and sexual abuse.

Results:
The lifetime prevalence of tobacco use was 8.6 per cent (21.5% males and 1.4% female). Among users, hazardous and dependent use defined using ASSIST scores was 63.3 and 2.9 per cent, respectively. Tobacco use was associated with older age, being male, urban residence, having a part-time job, use of alcohol and illicit drugs and academic failures.

Interpretation & conclusions:
Although the prevalence of tobacco use in our study was relatively low, the proportionately higher rates of hazardous use and its association with the negative correlates suggest that more needs to be done to prevent its deleterious consequences.