bluuebunny/crossref_metadata_2025_split huggingface dataset:
THE MOTHER'S PSYCHOLOGICAL RESPONSE TO CHANGES PSYCHOLOGICAL PARTURITION PARTURITION PERIOD BASED ON PARITY AND HOW LABOR IN RSUD SAYANG CIANJUR YEAR OF 2018
Authors: Rahmawati Naili 
Published: September 2019

The time of parturition or peurperium started after the birth of the placenta is up to 6 weeks (42 days) after, post-birth mothers will experience some changes in either the physical or psychological change change and some adjustments required by the mother. For those who cannot adjust to the psychological disorders-gangguang experience with a variety of syndromes or symptoms (postpartum stress). Figures for the incidence of baby blues or postpartum blues in Asia is quite high and varies between 26-85% and in Indonesia recorded between 50-70%. This research aims to know the mother's psychological response to changes psychological parturition parturition period based on parity and how childbirth in RSUD Sayang Cianjur year of 2018. Design research is descriptive research with cross sectional approach. The population in this research is the whole mom how can parturition spaces that are located in RSUD Sayang Cianjur while samples in this research was the mother of childbirth that is willing to be respondents and willing to fill out a questionnaire that has researchers prepare as many as 50 person. Data collection is done with the interview techniques using a questionnaire.Research results are obtained on the basis of parity that is as much as 15 people (60.0%), parturition multipara mother gave a positive response and as many as 14 people (56.0%), parturition primipara mother gave a negative response. For research results based on how labor i.e. as many as 12 people (60.0%), parturition maternity mother spontaneously give a positive response and as many as 16 people (53.3%) of mothers whose maternity parturition with action. Key words : psychological response, mother childbirth
ANAIS DA PRIMEIRA SEMANA CIENTÍFICA DA FACULDADE DA POLÍCIA MILITAR - FPM
Authors: FPM Faculdade da Polícia Militar 
Published: September 2019

A Primeira Semana Científica da Faculdade da Polícia Militar - FPM consistiu em uma excelente oportunidade para a integração de alunos e profissionais das áreas da Saúde Humana, Tecnologia e Ciência, promovendo discussões e reflexões sobre diferentes temas, além da experiência e formação acadêmica que os participantes tiveram nos quatro dias de imersão em conhecimento, com palestrantes altamente qualificados e reconhecidos no meio em que atuam. O evento aconteceu entre os dias 20 a 23 de maio de 2019, com palestras, conferências e apresentações de trabalhos. Os resumos apresentados e selecionados fazem parte deste Anais.
Mencari Jejak-jejak Autograf Perjanjian Lama di dalam Septuaginta
Authors: Kondoj Brando V. 
Published: September 2019

Untuk sekian lama, Septuaginta sebagai terjemahan Kitab Suci Ibrani yang pertama telah dipinggirkan dan tidak memperoleh tempat dalam usaha untuk mencari autograf (naskah asli Alkitab) Perjanjian Lama yang telah lama hilang itu. Namun demikian, perkembangan terbaru dalam studi terhadap naskah-naskah kuno Alkitab justru menunjukkan bahwa Septuaginta memiliki sumbangsih besar dalam pencarian autograf Perjanjian Lama. Hal ini dibuktikan melalui penggunaan metode kritik tekstual oleh para sarjana Alkitab, yakni dengan melakukan penelitian dan perbandingan terhadap naskah-naskah kuno Alkitab Perjanjian Lama, seperti Teks Masoret, Pentateukh Samaria, Gulungan Laut Mati, dan Septuaginta. Kata-kata kunci: Septuaginta, autograf Perjanjian Lama, metode kritik tekstual, Teks Masoret, Pentateukh Samaria, Gulungan Laut Mati. English : For too long the Septuagint, the first translation of the Hebrew Old Testament, has been sidelined and not given a credible hearing in seeking to discern the text of the original autographs of the Old Testament which have been lost in antiquity. Even though that has been the case, the new direction in recent textual studies, which has focused on the meaning of the original autographs of the Old Testament, has recognized that the Septuagint has a significant contribution to make within this field of study. This position has been supported by Biblical scholars who have employed the Text Critical method in determining the authoritative text of the Old Testament. They employ the Text Critical method in their comparison of the Masoretic Text, the Samaritan Pentateuch, The Dead Sea Scrolls and most recently, the Septuagint to find traces of the original OT autographs. Keywords: Septuagint, Old Testament autographs, text critical method, Masoretic Text, Samaritan Pentateuch, The Dead Sea Scrolls.
Religious Affections Jonathan Edwards dan Relevansinya bagi Ibadah Komunal
Authors: Samuel Lucky 
Published: September 2019

Artikel ini mencoba untuk membahas kontribusi dari salah satu tulisan penting Jonathan Edwards, yaitu A Treatise Concerning Religious Affections, bagi ibadah komunal. Sebagaimana karya ini bermanfaat dalam mengevaluasi kerohanian seseorang dan merumuskan apa itu spiritualitas yang autentik, risalah ini juga dapat bermanfaat di dalam mengevaluasi dan merancang ibadah komunal. Berfokus pada tiga tanda pertama dari dua belas indikator spiritualitas yang sejati menurut Edwards, tulisan ini mengusulkan bahwa risalah ini dapat berfungsi sebagai penawar dari tiga pemahaman menyimpang dalam ibadah komunal: ibadah yang legalistik, narsisistik, dan terapeutik. Kata-kata kunci: Jonathan Edwards, Afeksi Religius, Ibadah Komunal, Spiritualitas English : This article attempts to discuss one of the important writings of Jonathan Edwards, A Treatise Concerning Religious Affections, and its contribution to corporate worship. Since this work has been helpful in evaluating one’s spirituality and in formulating what the authentic spirituality is, this treatise can be also useful in evaluating and designing corporate worship. Focusing on the first three signs of gracious affections according to Edwards, this paper suggests that this treatise can serve as an antidote for three distorted notions in corporate worship, namely legalistic, narcissistic, and therapeutic worship. Keywords: Jonathan Edwards, Religious Affections, Corporate Worship, Spirituality
Konsep Kebenaran Allah Menurut Rasul Paulus di dalam Surat Roma
Authors: Alinurdin David 
Published: September 2019

Bagaimana Allah membenarkan orang-orang percaya di dalam proses keselamatan masih menjadi perdebatan di dalam kekristenan. Ada golongan yang berpandangan tindakan pembenaran Allah bersifat forensik dengan mengimputasikan kebenaran Kristus kepada seorang percaya sehingga ia mendapatkan status benar di hadapan Allah. Ada pula yang berpandangan pembenaran Allah itu bersifat moral dan transformatif dengan mengimpartasikan kebenaran Kristus di dalam diri orang percaya. Dan belakangan ini muncul pandangan New Perspective on Paul (NPP) yang merombak konsep pembenaran Allah tidak lagi bersifat forensik maupun etis, melainkan bersifat eklesiologis dengan memasukkan orang percaya di dalam komunitas umat Allah. Tulisan ini mengupas beberapa perikop kunci dari surat Paulus kepada jemaat di Roma guna memperlihatkan bahwa konsep kebenaran Allah dan karya pembenaran-Nya yang dipahami Paulus bersifat menyeluruh mencakup ketiga aspek tersebut.
How God justifies believers in the process of salvation is still under debate within Christianity. There are groups who view God’s justification as forensic by imparting the truth of Christ to a believer so that the believer attains a right status before God. Some view God’s justification as moral and transformative by imparting the truth of Christ in believers. And lately there is a New Perspective on Paul (NPP) that envisions overhauling the concept of God’s justification in that it is neither forensic nor moral, but is ecclesiological by including believers in the community of God’s people. This paper examines some key passages from Paul’s letter to the church in Rome to show that the concept of God’s truth and his justification, as understood by Paul, is comprehensive in that it encompasses all three aspects.
Pregenealogical Coherence dan Teks Awal Markus 1:41
Authors: Kristianto Stefanus 
Published: September 2019

Diskusi teks Markus 1:41 merupakan salah satu diskusi teks yang paling menarik. Mayoritas sarjana menganggap bahwa bacaan σπλαγχνισθεὶς adalah bacaan sekunder, meskipun bacaan ini didukung oleh mayoritas saksi. Dalam tulisan ini, penulis akan menunjukkan bahwa bukti yang didapat dari analisis pregenealogical coherence makin memperkuat validitas bukti eksternal dalam mendukung bacaan σπλαγχνισθεὶς sebagai teks awal. Karena itu, bukti eksternal yang konklusif ini tidak boleh diabaikan begitu saja. Di akhir tulisan, penulis akan mendiskusikan secara singkat kemungkinan transkripsional (transcriptional probability) mengapa penyalin mengubah bacaan σπλαγχνισθεὶς menjadi ὀργισθείς. Kata-kata kunci: Kritik Teks Perjanjian Baru, Pregenealogical Coherence, Coherence-Based Genealogical Method, Markus 1:41, Teks Awal Discussion as to the text of Mark 1:41 is one of the most interesting textual discussions. Although most witnesses support the primacy of the reading σπλαγχνισθεὶς, most scholars consider that the reading is secondary. In this paper, the writer intends to show that the pregenealogical coherence analysis on the text strengthens the validity of the external evidences in supporting σπλαγχνισθεὶς as the initial text. These conclusive external evidences, therefore, must not be set aside. At the end of this paper, the writer will discuss in brief as to why the scribes altered the reading σπλαγχνισθεὶς to be ὀργισθείς. Keywords: New Testament Textual Criticism, Pregenealogical Coherence, Coherence-Based Genealogical Method, Mark 1:41, Initial Text
The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources
Authors: González-López Jorge , Decarli Roberto , Pavesi Riccardo , Walter Fabian , Aravena Manuel , Carilli Chris , Boogaard Leindert , Popping Gergö , Weiss Axel , Assef Roberto J. , Bauer Franz Erik , Bertoldi Frank , Bouwens Richard , Contini Thierry , Cortes Paulo C. , Cox Pierre , da Cunha Elisabete , Daddi Emanuele , Díaz-Santos Tanio , Inami Hanae , Hodge Jacqueline , Ivison Rob , Le Fèvre Olivier , Magnelli Benjamin , Oesch Pascal , Riechers Dominik , Rix Hans-Walter , Smail Ian , Swinbank A. M. , Somerville Rachel S. , Uzgil Bade , van der Werf Paul 
Published: September 2019

Abstract
The Atacama Large Millimeter/submillimeter Array (ALMA) SPECtroscopic Survey in the Hubble Ultra Deep Field (HUDF) is an ALMA large program that obtained a frequency scan in the 3 mm band to detect emission lines from the molecular gas in distant galaxies. Here we present our search strategy for emission lines and continuum sources in the HUDF. We compare several line search algorithms used in the literature, and critically account for the line widths of the emission line candidates when assessing significance. We identify 16 emission lines at high fidelity in our search. Comparing these sources to multiwavelength data we find that all sources have optical/infrared counterparts. Our search also recovers candidates of lower significance that can be used statistically to derive, e.g., the CO luminosity function. We apply the same detection algorithm to obtain a sample of six 3 mm continuum sources. All of these are also detected in the 1.2 mm continuum with optical/near-infrared counterparts. We use the continuum sources to compute 3 mm number counts in the sub-millijansky regime, and find them to be higher by an order of magnitude than expected for synchrotron-dominated sources. However, the number counts are consistent with those derived at shorter wavelengths (0.85–1.3 mm) once extrapolating to 3 mm with a dust emissivity index of β = 1.5, dust temperature of 35 K, and an average redshift of z = 2.5. These results represent the best constraints to date on the faint end of the 3 mm number counts.
The Nearby Very Low Mass Triple Star LHS 1070
Authors: Xia Fang , Fu Yanning , Wang Xiaoli 
Published: September 2019

Abstract
The component masses and kinematic parameters of the triple star LHS 1070 are redetermined by using the three-body model. It is shown that the discrepancy between new observations and the two-body fitting results is due to the three-body effects, which justifies the necessity of using the three-body model. Numerical integration shows that the three-body system remains integrated and its hierarchical configuration remains unchanged since the formation of the components. This implies that the triple star may not be formed by a three-body encounter. Also, the possibility that the most massive component is itself a tightly bounded binary is excluded based on the redetermined dynamical mass. The improved dynamical masses of the three components are greatly helpful to constrain at the lower end of the stellar empirical mass–luminosity relation.
The SDO/EVE Solar Irradiance Coronal Dimming Index Catalog. I. Methods and Algorithms
Authors: Mason James Paul , Attie Raphael , Arge Charles N. , Thompson Barbara , Woods Thomas N. 
Published: September 2019

Abstract
When a coronal mass ejection departs, it leaves behind a temporary void. That void is known as coronal dimming, and it contains information about the mass ejection that caused it. Other physical processes can cause parts of the corona to have transient dimmings, but mass ejections are particularly interesting because of their influence in space weather. Prior work has established that dimmings are detectable even in disk-integrated irradiance observations, i.e., Sun-as-a-star measurements. The present work evaluates four years of continuous Solar Dynamics Observatory Extreme Ultraviolet Experiment (EVE) observations to greatly expand the number of dimmings we may detect and characterize, and collects that information into James’s EVE Dimming Index catalog. This paper details the algorithms used to produce the catalog, provides statistics on it, and compares it with prior work. The catalog contains 5051 potential events (rows), which correspond to all robustly detected solar eruptive events in this time period as defined by >C1 flares. Each row has a corresponding 27,349 elements of metadata and parameterizations (columns). In total, this catalog is the result of analyzing 7.6 million solar ultraviolet light curves.
On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure
Authors: Golightly E. C. A. , Nixon C. J. , Coughlin E. R. 
Published: September 2019

Abstract
The tidal disruption of stars by supermassive black holes (SMBHs) can be used to probe the SMBH mass function, the properties of individual stars, and stellar dynamics in galactic nuclei. Upcoming missions will detect thousands of tidal disruption events (TDEs), and accurate theoretical modeling is required to interpret the data with precision. Here we analyze the influence of more realistic stellar structure on the outcome of TDEs; in particular, we compare the fallback rates—being the rate at which tidally disrupted debris returns to the black hole—from progenitors generated with the stellar evolution code mesa to

and γ = 5/3 polytropes. We find that mesa-generated density profiles yield qualitatively different fallback rates as compared to polytropic approximations, and that only the fallback curves from low-mass (1 M
⊙ or less), zero-age main-sequence stars are well fit by either a

or 5/3 polytrope. Stellar age has a strong affect on the shape of the fallback curve, and can produce characteristic timescales (e.g., the time to the peak of the fallback rate) that greatly differ from the polytropic values. We use these differences to assess the degree to which the inferred black hole mass from the observed light curve can deviate from the true value, and find that the discrepancy can be at the order of magnitude level. Accurate stellar structure also leads to a substantial variation in the critical impact parameter at which the star is fully disrupted, and can increase the susceptibility of the debris stream to fragmentation under its own self-gravity. These results suggest that detailed modeling is required to accurately interpret observed light curves of TDEs.
Measuring the D/H Ratios of Exoplanets and Brown Dwarfs
Authors: Morley Caroline V. , Skemer Andrew J. , Miles Brittany E. , Line Michael R. , Lopez Eric D. , Brogi Matteo , Freedman Richard S. , Marley Mark S. 
Published: September 2019

Abstract
The relative abundance of deuterium and hydrogen is a potent tracer of planet formation and evolution. Jupiter and Saturn have protosolar atmospheric D/H ratios, a relic of substantial gas accretion from the nebula, while the atmospheres of Neptune and Uranus are enhanced in D by accretion of ices into their envelopes. For terrestrial planets, D/H ratios are used to determine the mechanisms of volatile delivery and subsequent atmosphere loss over the lifetime of the planet. Planets and brown dwarfs more massive than ∼13 M
J quickly fuse their initial D reservoir. Here, we simulate spectra for giant exoplanets and brown dwarfs (2 M
Neptune to ∼10 M
Jupiter) from T
eff = 200–1800 K including both CH3D and HDO to determine the observability of these dominant deuterium isotopologues in mid-infrared thermal emission spectra. Colder objects have stronger molecular features in their spectra, due to the temperature dependence of molecular cross sections. CH3D is easier to observe than HDO at all temperatures considered, due to the strength of its absorption bands and locations of features at wavelengths with few other strong absorption features. We predict that for nearby cool brown dwarfs, the CH3D abundance can be measured at high signal to noise with the James Webb Space Telescope (JWST); for objects from 200 to 800 K closer than 10 pc, a protosolar D/H ratio would be readily observable in 2.5 hr. Moderately young Jupiter-mass planets (100–300 Myr) and young Neptunes (10 Myr) may be discovered with JWST and provide the best targets for detecting deuterium on an exoplanet in the coming decade. Future telescope designs should consider the importance of isotopes for understanding the formation and evolution of planetary atmospheres.
A Wind-based Unification Model for NGC 5548: Spectral Holidays, Nondisk Emission, and Implications for Changing-look Quasars
Authors: Dehghanian M. , Ferland G. J. , Peterson B. M. , Kriss G. A. , Korista K. T. , Chatzikos M. , Guzmán F. , Arav N. , De Rosa G. , Goad M. R. , Mehdipour M. , van Hoof P. A. M. 
Published: September 2019

Abstract
The 180 day Space Telescope and Optical Reverberation Mapping campaign on NGC 5548 discovered an anomalous period, the broad-line region (BLR) holiday, in which the emission lines decorrelated from the continuum variations. This is important since the correlation between the continuum-flux variations and the emission-line response is the basic assumption for black hole (BH) mass determinations through reverberation mapping. During the BLR holiday the high-ionization intrinsic absorption lines also decorrelated from the continuum as a result of the variable covering factor of the line-of-sight (LOS) obscurer. The emission lines are not confined to the LOS, so this does not explain the BLR holiday. If the LOS obscurer is a disk wind, its streamlines must extend down to the plane of the disk and the base of the wind would lie between the BH and the BLR, forming an equatorial obscurer. This obscurer can be transparent to ionizing radiation, or can be translucent, blocking only parts of the spectral energy distribution, depending on its density. An emission-line holiday is produced if the wind density increases only slightly above its transparent state. Both obscurers are parts of the same wind, so they can have associated behavior in a way that explains both holidays. A very dense wind would block nearly all ionizing radiation, producing a Seyfert 2 and possibly providing a contributor to the changing-look active galactic nucleus phenomenon. Disk winds are very common and we propose that the equatorial obscurers are too, but mostly in a transparent state.
Geographical distribution of cervical cancer in Odisha: A 5-year retrospective study at a regional cancer center
Authors: Hota Pradeep Kumar , Panda Niharika , Nayak Bhagyalaxmi , Samantaray Sagarika 
Published: September 2019

Abstract
Background: Cancer cervix and breast are the two major female health problems in India. A hospital-based, 5-year (2010–2014) retrospective study was conducted at a regional cancer center of Odisha to analyze the present burden of cancer cervix in this state, which has a population of more than 45.5 million at present. Materials and Methods: All the patients suffering from cancer cervix that was treated by radiotherapy during 2010–2014 at this center were analyzed year wise for age, stage of disease, and native area. Results: Based on the Census 2011 data, it was calculated and found that from the low-literacy area on an average of 4.62 cervical cancer patients per million, from the medium-literacy area 6.56 patients per million, and from high-literacy area 19.11 patients per million of population have received radiotherapy in this hospital. More than 60% of patients with cervical cancer were from stage IIIB and in the age group of 50–55 years. Discussion: Odisha has 83.7% female population in rural areas with literacy rate below 50%. Due to lack of awareness and unavailability of cancer care facilities at their reach, they mainly depend on various alternative medicines in unscientific manner for their health care. Conclusion: Strengthening of existing regional cancer center, development of oncology wings in all medical college hospitals by providing basic radiotherapy facilities, emphasizing more on district cancer control programs, decentralizing of NGO schemes, and facilitating with more cancer screening and awareness programs may help better registration, prevention, and treatment of cancer in Odisha.
Assessment of quality of life in resectable gastric cancer patients undergoing chemoradiotherapy as adjuvant treatmentLetter to the Editor
Authors: Pruthi Deep Shankar , Ahmad Mushtaq , Gupta Meenu , Bansal Saurabh , Nautiyal Vipul , Saini Sunil 
Published: September 2019

Abstract
Introduction: Quality of life (QOL) is increasingly recognized as an important endpoint in cancer therapies. However, few data are available on QOL in patients who have received radiotherapy as adjuvant treatment for cancer stomach. Methods: Thirty patients who underwent curative resection were enrolled and received chemoradiotherapy (45 Gy in 25 fractions using three-dimensional conformal radiotherapy technique), together with 5-fluorouracil and leucovorin. The European Organization for Research and Treatment of Cancer QOL questionnaire C30 and STO Q22 was assessed at four time points: pre- and postchemoradiotherapy and at 1-month and 6-month follow-up. Results: Mean age of the patients was 54 years. Male:female ratio was 4:1. Stage II and Stage III disease was present in 60% and 30% of patients, respectively. All patients were able to complete the chemoradiotherapy protocol. Our study found out significant impairment in QOL for emotional functioning, fatigue, nausea and vomiting and dyspnea. Results showed that QOL levels decrease postchemoradiotherapy; however, QOL levels returned to baseline at 1-month and 6-month follow-up period. Conclusion: Chemoradiotherapy as adjuvant treatment for cancer stomach patients who have undergone resection with curative intent is a safe and well-tolerated regimen with respect to QOL.