bluuebunny/crossref_metadata_2025_split huggingface dataset:
MEMBANGUN DAMAI MELALUI MEDIASI: STUDI TERHADAP PEMIKIRAN HAMKA DALAM TAFSIR AL-AZHAR
Authors: Taufiq Imam 
Published: June 2016

<em>Scholars have formulated theories on conflict and designed its resolution on the basis of their expertise. They may come from various disciples and backgrounds, such as economics, law, sociology and even religion. In the context of Islamic religion, Muslim scholars use the verses of the Qur’an regarding conflict and extract their meanings through exegetical thematic method. This method offers explanation of conflict resolution from the Qur’anic perspectives concerning the verses on multiculturalism. But how are the multicultural verses understood? This article elaborates Hamka’s model of exegesis on multicultural verses in his work of Tafsir al-Azhar on conflict resolution. It shows that the Qur’anic verses not only have resolution principles but also give instructions on how to apply them. The terms used by the Qur’an include al-ta‘aruf, al-arham and al-taqwa. These concepts promote mediation that is applicable in various contexts of conflict such as in family, society, custom and law. Multiculturalism verses in Hamka’s model also offers phases of conflict resolutions, beginning from clarification to planning and mediation control. His offer, at least, stimulates Muslims’ awareness about Islamic unity and human unity.</em>
Computer-Assisted In Sensu Exposure for Posttraumatic Stress Disorder: Development and Evaluation
Authors: Görg Nora , Priebe Kathlen , Deuschel Tilman , Schüller Martin , Schriner Friederike , Kleindienst Nikolaus , Ludäscher Petra , Schmahl Christian , Bohus Martin 
Published: June 2016

Background
Dissociative states during psychotherapy sessions reduce the benefit of exposure-based therapy for posttraumatic stress disorder (PTSD). Thus, in evidence-based therapeutic programs such as dialectical behavior therapy for PTSD (DBT-PTSD), therapists apply specific antidissociative skills to reduce dissociative features during in sensu exposure.

Objective
This study sought to examine the acceptance and feasibility of the MORPHEUS program.

Methods
Patients who underwent 12 weeks of residential DBT-PTSD treatment used MORPHEUS during exposure exercises in self-management. After the treatment, they filled out evaluation questionnaires.

Results
In sum, 26 patients receiving a 12-week standard DBT-PTSD program participated in this study; 2 participants could not be analyzed because of missing data. All the patients used MORPHEUS as often as it was required according to the DBT-PTSD treatment (2 to 5 times a week). The overall acceptance and feasibility as rated by the patients was high: for example, patients found the skills useful to block dissociation (mean 4.24 on a scale from 0 to 5, SD 0.24) and stated that they would use the program again (mean 4.72 on a scale from 0 to 5, SD 0.11). Furthermore, patients indicated that they would recommend MORPHEUS to a friend (mean 4.44 on a scale from 0 to 5, SD 0.12). In 82% (32/39) of the cases, the use of antidissociative skills was related to a decrease in dissociation. In 18% (5/39), dissociation remained unchanged or increased.

Conclusions
The evaluative data suggest high acceptability and feasibility of MORPHEUS. Further studies should evaluate the effectiveness of the skills applied during the program.

Trial Registration
World Health Organization International Clinical Trials Registry Platform: DRKS00006226; http://apps.who.int/trialsearch/Trial2.aspx?TrialID= DRKS00006226 (Archived by WebCite at http://www.webcitation.org/ 6hxuFbIUr)
The hand of God is over their hands(Q. 48:10): On the Notion of Covenant in al-Ṭabarī's Account of Karbala
Authors: Hylén Torsten 
Published: June 2016

This article is an analysis of the story of the killing of Ḥusayn b. ʿAlī at Karbala in 61/680, as it is presented by al-Ṭabarī. The main argument is that the notion of the divine covenant, which permeates the Qur'an, constitutes a framework through which al-Ṭabarī views this event. The Qur'anic idea of the covenant is read in structural/thematic continuity with the Hebrew Bible account of the covenant between Yahweh and the Hebrew people, which has, in turn, been traced back in its basic form to Late Bronze Era treaties between rulers and their vassals.The present study focuses on four speeches ascribed to Ḥusayn during the encounter he and his group had with the vanguard of the Kufan army led by al-Ḥurr. These are analysed in accordance with their use of Qur'anic covenant vocabulary. They are also categorised within the broader framework of the eight standard characteristics of Ancient West Asian and Biblical covenants, as presented by Mendenhall and Herion, which have recently been developed in a Qur'anic context by Rosalind Ward Gwynne. This article argues that al-Ṭabarī’s Karbala narrative presents the pact of loyalty to Ḥusayn as a clear extension of the divine covenant.
BetweenHistoryandTafsīr: Notes on al-Ṭabarī’s Methodological Strategies
Authors: Klar Marianna 
Published: June 2016

The bulk of the cited anecdotes in the most immediately relevant section pertaining to the Fall of Adam within al-Ṭabarī’s History consist solely of material that is duplicated in al-Ṭabarī’s commentary on But Satan made them slip in Q. 2:36. The duplicated material is not presented in the same order across the two works, but the extent of the overlap between the two sources is intriguing. In his introduction to the Tafsīr, published (in the form of public lectures) from 270/883–884 onwards, al-Ṭabarī (d. 310/923) gives a definition of his own methodology; the introduction to his History, the first volume of which was made public some 20 years later in 294/906–907, announces meanwhile a focus on the history of kings. Yet al-Ṭabarī does not provide any explicit elucidation of what this difference might entail. In areas where al-Ṭabarī’s subject matter spans both texts such a question seems especially pertinent.This article seeks to contribute to a more detailed understanding of how concepts of genre affected the material that was included by al-Ṭabarī in the History and the Tafsīr, and to expose the author's editorial techniques, with specific reference to the parallel versions of the story of Adam and the Fall al-Ṭabarī provided. It draws upon the preceding historical account of the Creation of Eve, and the material that frames the repentance narratives. It also seeks to ascertain whether the individual context of each Qur'anic pericope affected the presentation of material within the Tafsīr itself.
Universal multiplexable matK primers for DNA barcoding of angiosperms
Authors: Heckenhauer Jacqueline , Barfuss Michael H. J. , Samuel Rosabelle 
Published: June 2016

Premise of the study:PCR amplification of the matK barcoding region is often difficult when dealing with multiple angiosperm families. We developed a primer cocktail to amplify this region efficiently across angiosperm diversity.Methods and Results:We developed 14 matK primers (seven forward, seven reverse) for multiplex PCR, using sequences available in GenBank for 178 taxa belonging to 123 genera in 41 families and 18 orders. Universality of these new multiplexed primers was tested with 53 specimens from 44 representative angiosperm families in 23 different orders. Our primers showed high PCR amplification and sequencing success.Conclusions:These results show that our newly developed primers are highly effective for multiplex PCR and can be employed in future barcode projects involving taxonomically diverse samples across angiosperms. Using multiplex primers for barcoding will reduce the cost and time needed for PCR amplification.
Characterization of 19 microsatellite loci in the clonal monkshood Aconitum kusnezoffii (Ranunculaceae)
Authors: Ge Xing‐Yue , Tian Hao , Liao Wan‐Jin 
Published: June 2016

Premise of the study:Microsatellite loci were isolated and characterized from Aconitum kusnezoffii (Ranunculaceae) to estimate male and female reproductive success and evaluate the effects of clonal growth on sexual reproduction.Methods and Results:A genomic enrichment approach was used to develop microsatellite markers. In three investigated A. kusnezoffii populations, a total of 19 microsatellite loci were successfully amplified, and 13 of these loci were polymorphic. Most of the primer pairs designed for the identified loci also amplified corresponding microsatellite loci in A. barbatum var. puberulum and A. alboviolaceum.Conclusions:The identified microsatellite loci will be useful for quantifying male and female fitness in A. kusnezoffii and evaluating the effects of clonal growth on sexual reproduction.
ON THE LINEAR DAMPING RELATION FOR DENSITY WAVES IN SATURN’S RINGS
Authors: Schmidt Jürgen , Colwell Joshua E. , Lehmann Marius , Marouf Essam A. , Salo Heikki , Spahn Frank , Tiscareno Matthew S. 
Published: June 2016

ABSTRACT
We revisit the equation for viscous damping of density waves derived from linearized theory and show that the damping is not only determined by the magnitudes of shear and bulk viscosity. Modifications arise from the dependence of the viscosity on the ring’s surface mass density. This was noted more than 30 years ago by Goldreich & Tremaine (1978b). Still, to date the consequences have not been explored. In the literature these terms have been neglected throughout when fitting the rings’ viscosity from observations of wave damping. Therefore, one must suspect that these viscosities, as well as the dispersion velocities inferred from them, suffer from systematic bias, which might be small or significant, depending on the local conditions in the ring. We show that the modified damping formula, to linear order, is related to the stability threshold for viscous overstability and argue that the appearance of density waves may be altered by this instability.
THE UBIQUITY OF COEVAL STARBURSTS IN MASSIVE GALAXY CLUSTER PROGENITORS
Authors: Casey Caitlin M. 
Published: June 2016

ABSTRACT
The universe’s largest galaxy clusters likely built the majority of their massive >1011
M

galaxies in simultaneous, short-lived bursts of activity well before virialization. This conclusion is reached based on emerging data sets for

proto-clusters and the characteristics of their member galaxies, in particular, rare starbursts and ultraluminous active galactic nuclei (AGN). The most challenging observational hurdle in identifying such structures is their very large volumes, ∼104 comoving Mpc3 at

, subtending areas of approximately half a degree on the sky. Thus, the contrast afforded by an overabundance of very rare galaxies in comparison to the background can more easily distinguish overdense structures from the surrounding, normal density field. Five

proto-clusters from the literature are discussed in detail and are found to contain up to 12 dusty starbursts or luminous AGN galaxies each, a phenomenon that is unlikely to occur by chance even in overdense environments. These are contrasted with three higher-redshift (

) dusty star-forming galaxy (DSFG) groups, whose evolutionary fate is less clear. Measurements of DSFGs’ gas depletion times suggest that they are indeed short-lived on ∼100 Myr timescales, and accordingly the probability of finding a structure containing more than 8 such systems is ∼0.2%, unless their “triggering” is correlated on very large spatial scales, ∼10 Mpc across. The volume density of DSFG-rich proto-clusters is found to be comparable to all of the >1015
M

galaxy clusters in the nearby universe, which is a factor of five larger than expected in some simulations. Some tension still exists between measurements of the volume density of DSFG-rich proto-clusters and the expectation that they are generated via short-lived episodes, as the latter suggests that only a fraction (

) of all proto-clusters should be rich with DSFGs. However, improved observations of proto-clusters over large regions of sky will certainly shed more light on the assembly of galaxy clusters, and whether or not they build their galaxies through episodic bursts as suggested here.
ON THE CONSERVATION OF THE VERTICAL ACTION IN GALACTIC DISKS
Authors: Vera-Ciro Carlos , D’Onghia Elena 
Published: June 2016

ABSTRACT
We employ high-resolution N-body simulations of isolated spiral galaxy models, from low-amplitude, multi-armed galaxies to Milky Way-like disks, to estimate the vertical action of ensembles of stars in an axisymmetrical potential. In the multi-armed galaxy the low-amplitude arms represent tiny perturbations of the potential, hence the vertical action for a set of stars is conserved, although after several orbital periods of revolution the conservation degrades significantly. For a Milky Way-like galaxy with vigorous spiral activity and the formation of a bar, our results show that the potential is far from steady, implying that the action is not a constant of motion. Furthermore, because of the presence of high-amplitude arms and the bar, considerable in-plane and vertical heating occurs that forces stars to deviate from near-circular orbits, reducing the degree at which the actions are conserved for individual stars, in agreement with previous results, but also for ensembles of stars. If confirmed, this result has several implications, including the assertion that the thick disk of our Galaxy forms by radial migration of stars, under the assumption of the conservation of the action describing the vertical motion of stars.
STAR CLUSTERS IN M31. VII. GLOBAL KINEMATICS AND METALLICITY SUBPOPULATIONS OF THE GLOBULAR CLUSTERS
Authors: Caldwell Nelson , Romanowsky Aaron J. 
Published: June 2016

ABSTRACT
We carry out a joint spatial–kinematical–metallicity analysis of globular clusters (GCs) around the Andromeda Galaxy (M31), using a homogeneous, high-quality spectroscopic data set. In particular, we remove the contaminating young clusters that have plagued many previous analyses. We find that the clusters can be divided into three major metallicity groups based on their radial distributions: (1) an inner metal-rich group ([Fe/H] >

); (2) a group with intermediate metallicity (with median [Fe/H] = −1); and (3) a metal-poor group, with [Fe/H] <

. The metal-rich group has kinematics and spatial properties like those of the disk of M31, while the two more metal-poor groups show mild prograde rotation overall, with larger dispersions—in contrast to previous claims of stronger rotation. The metal-poor GCs are the least concentrated group; such clusters occur five times less frequently in the central bulge than do clusters of higher metallicity. Despite some well-known differences between the M31 and Milky Way GC systems, our revised analysis points to remarkable similarities in their chemodynamical properties, which could help elucidate the different formation stages of galaxies and their GCs. In particular, the M31 results motivate further exploration of a metal-rich GC formation mode in situ, within high-redshift, clumpy galactic disks.
TIMING THE EVOLUTION OF QUIESCENT AND STAR-FORMING LOCAL GALAXIES
Authors: Pacifici Camilla , Oh Sree , Oh Kyuseok , Lee Jaehyun , K. Yi Sukyoung 
Published: June 2016

ABSTRACT
Constraining the star formation histories (SFHs) of individual galaxies is crucial for understanding the mechanisms that regulate their evolution. Here, we combine multi-wavelength (ultraviolet, optical, and infrared) measurements of a very large sample of galaxies (∼230,000) at z < 0.16, with physically motivated models of galaxy spectral energy distributions to extract constraints on galaxy physical parameters (such as stellar mass and star formation rate) as well as individual SFHs. In particular, we set constraints on the timescales in which galaxies form a certain percentage of their total stellar mass (namely, 10%, 50%, and 90%). The large statistics allows us to average such measurements over different populations of galaxies (quiescent and star-forming) and in narrow ranges of stellar mass. As in the downsizing scenario, we confirm that low-mass galaxies have more extended SFHs than high-mass galaxies. We also find that at the same observed stellar mass, galaxies that are now quiescent evolve more rapidly than galaxies that are currently still forming stars. This suggests that stellar mass is not the only driver of galaxy evolution, but plays along with other factors such as merger events and other environmental effects.
THE SDSS-IV EXTENDED BARYON OSCILLATION SPECTROSCOPIC SURVEY: LUMINOUS RED GALAXY TARGET SELECTION
Authors: Prakash Abhishek , Licquia Timothy C. , Newman Jeffrey A. , Ross Ashley J. , Myers Adam D. , Dawson Kyle S. , Kneib Jean-Paul , Percival Will J. , Bautista Julian E. , Comparat Johan , Tinker Jeremy L. , Schlegel David J. , Tojeiro Rita , Ho Shirley , Lang Dustin , Rao Sandhya M. , McBride Cameron K. , Zhu Guangtun Ben , Brownstein Joel R. , Bailey Stephen , Bolton Adam S. , Delubac Timothée , Mariappan Vivek , Blanton Michael R. , Reid Beth , Schneider Donald P. , Seo Hee-Jong , Rosell Aurelio Carnero , Prada Francisco 
Published: June 2016

ABSTRACT
We describe the algorithm used to select the luminous red galaxy (LRG) sample for the extended Baryon Oscillation Spectroscopic Survey (eBOSS) of the Sloan Digital Sky Survey IV (SDSS-IV) using photometric data from both the SDSS and the Wide-field Infrared Survey Explorer. LRG targets are required to meet a set of color selection criteria and have z-band and i-band MODEL magnitudes z < 19.95 and 19.9 < i < 21.8, respectively. Our algorithm selects roughly 50 LRG targets per square degree, the great majority of which lie in the redshift range 0.6 < z < 1.0 (median redshift 0.71). We demonstrate that our methods are highly effective at eliminating stellar contamination and lower-redshift galaxies. We perform a number of tests using spectroscopic data from SDSS-III/BOSS ancillary programs to determine the redshift reliability of our target selection and its ability to meet the science requirements of eBOSS. The SDSS spectra are of high enough signal-to-noise ratio that at least ∼89% of the target sample yields secure redshift measurements. We also present tests of the uniformity and homogeneity of the sample, demonstrating that it should be clean enough for studies of the large-scale structure of the universe at higher redshifts than SDSS-III/BOSS LRGs reached.
Their Emotions and Ours: A Single History?
Authors: Konstan David 
Published: June 2016

Y a-t-il une histoire de l’émotion dans la longue durée ? Si les émotions sont des invariants à travers l’histoire et les sociétés, du passé au présent, dans ce cas (c’est-à-dire indépendamment des conditions spécifiques qui les suscitent) elles n’ont pas d’histoire en tant que telles. En revanche, si les émotions sont culturellement construites, et donc soumises au changement, est-ce l’émotion particulière qui évolue ou bien une nouvelle qui remplace l’ancienne ? Évidemment on peut affirmer que certaines réponses primitives, quasi-émotionnelles, sont transculturelles, tandis que les émotions complexes sont construites à partir de ces affects élémentaires, et changent d’une culture à l’autre. Cet article offre deux études de cas de l’évolution émotionnelle – la transformation de la pitié en compassion et celle du regret en repentance – et propose, pour conclure, l’idée que nous pouvons tracer des schèmes ou des convergences à travers une série de sentiments, lorsqu’une matrice émotionnelle se dissout et une nouvelle se cristallise.
Le corps social à l’origine de l’invention du mot « émotion »
Authors: Hochner Nicole 
Published: June 2016

Bien que les historiens analysent les émotions des sociétés passées, le terme émotion lui-même est un mot récent qui n'apparaît qu'au courant du XVe siècle. Cette « invention », qui se fait en France, se dissémine rapidement dans d'autres langues, comme en anglais par exemple. À l'origine le mot « émotion » a une signification politique et désigne un soulèvement ou une révolte populaire. Cette étude se propose d'examiner le contexte précis de gestation et d'apparition du mot émotion, qui n'a curieusement suscité aucun examen systématique jusqu'à nos jours. En comblant cette lacune, on pourra mieux comprendre la dimension politique originelle du terme et, surtout, prouver que ce ne sont pas nécessairement les agitations et les perturbations politiques qui secouent la France qui suffisent pour expliquer l'apparition de ce nouveau terme. Il est indéniable que les réalités politiques ont leur place dans le contexte culturel et politique de l'invention du terme « émotion », mais cet article prouve que l'élément indispensable et constitutif à la formation du mot « émotion » est la référence au corps imaginaire de la société qui est profondément bouleversée par Nicole Oresme. Cet article démontrera comment et pourquoi le corps politique doit être considéré comme le berceau métaphorique du mot « émotion » qui depuis a perdu sa teneur politique.
Current estimates of biogenic emissions from eucalypts uncertain for southeast Australia
Authors: Emmerson Kathryn M. , Galbally Ian E. , Guenther Alex B. , Paton-Walsh Clare , Guerette Elise-Andree , Cope Martin E. , Keywood Melita D. , Lawson Sarah J. , Molloy Suzie B. , Dunne Erin , Thatcher Marcus , Karl Thomas , Maleknia Simin D. 
Published: June 2016

Abstract. The biogenic emissions of isoprene and monoterpenes are one of the main drivers of atmospheric photochemistry, including oxidant and secondary organic aerosol production. In this paper, the emission rates of isoprene and monoterpenes from Australian vegetation are investigated for the first time using the Model of Emissions of Gases and Aerosols from Nature version 2.1 (MEGANv2.1); the CSIRO chemical transport model; and atmospheric observations of isoprene, monoterpenes and isoprene oxidation products (methacrolein and methyl vinyl ketone). Observations from four field campaigns during three different seasons are used, covering urban, coastal suburban and inland forest areas. The observed concentrations of isoprene and monoterpenes were of a broadly similar magnitude, which may indicate that southeast Australia holds an unusual position where neither chemical species dominates. The model results overestimate the observed atmospheric concentrations of isoprene (up to a factor of 6) and underestimate the monoterpene concentrations (up to a factor of 4). This may occur because the emission rates currently used in MEGANv2.1 for Australia are drawn mainly from young eucalypt trees (< 7 years), which may emit more isoprene than adult trees. There is no single increase/decrease factor for the emissions which suits all seasons and conditions studied. There is a need for further field measurements of in situ isoprene and monoterpene emission fluxes in Australia.