bluuebunny/crossref_metadata_2025_split huggingface dataset:
Estudio métrico sobre la actividad investigadora usando el software libre R: el caso del sistema universitario gallego
Authors: Tarrío-Saavedra Javier , Orois Elena , Naya Salvador 
Published: January 2018

Este trabajo representa una nueva alternativa para el estudio, clasificación y comparación de la producción científica de centros de investigación, utilizando las funciones de tratamiento de datos del paquete Citan del software estadístico R. En particular, se muestra el análisis bibliométrico de las publicaciones de las universidades de A Coruña, Santiago de Compostela y Vigo, en el periodo 2000-2011, recopiladas por la base de datos Scopus. Entre las técnicas usadas se aplicaron modelos de Lotka y Price, modelización no paramétrica y paramétrica de los datos, así como el cálculo y análisis de indicadores de la cantidad y calidad de la producción científica, los índices h y g, y otros menosconocidos como los rp1, lp, Ge1, Ge5 y Slp1. Como novedad, se propone una variante del índice h (hh) que define el grupo de investigadores que forman la élitemás productiva de cada universidad y estima su calidad investigadora.AbstractThis work represents a new alternative for the study, classification and comparison of the scientific production corresponding to research entities. It consists on the application of statistical data processing functions available in the R software’s Citan package. In particular, the bibliometric study of publications of universities of A Coruña, Santiago de Compostela and Vigo, in the period 2000-2011, compiled by the Scopus database. The study was conducted using the statistical analysis of the data, the application of models of Lotka and Price, nonparametric and parametric modeling (Pareto) of the data, and the calculation and analysis of indicators of the scientific production like the h and g indexes, and others lesser known as rp1, lp, Ge1, Ge5 and Slp1. A novelty consists in a variant of the h index (hh) that defines the group of researchers who are the most productive of each university, the elite, and estimates the researching quality of such representative elites.
Családon belüli erőszak egy irodalmi mű alapján. (Móricz Zsigmond: „A világ végén már szép és jó”)
Authors: Pápai-Tarr Ágnes 
Published: January 2018

In my study I am going to present a rather complicated issue, namely a few problems of domestic violence based on a less-known short story by the Hungarian writer Zsigmond Móricz. I chose this story because it is still relevant today, it could even be set in 2017, as it basically depicts domestic violence in its complexity. This story by Móricz proves that the phenomenon of domestic violence is not at all new, given that in the beginning or the middle of the 20th century we can see the same complex social problem which present-day criminal law has to face. Hungarian society 50 or 100 years ago was not exempt from domestic violence either. We may also claim that the factors enhancing domestic violence were even stronger than today. The story aligns several dimensions of domestic violence, as it shows examples of both child and wife abuse. I am going to analyse the crimes depicted by Móricz according to the criminal laws effective today, and I just tangentially touch upon the judgment of the offences in the age of writing. This way, first I analyse the questions of child abuse, focusing on the right of punishment, which is still relevant in today’s criminal system as a cause for miscarriage. Then I present a detailed analysis of the bearing of case of partner abuse in the framework of violence in relationships, which exists in Hungarian criminal law since 2013.
TOGOG & SEMAR: DEHUMANIZATION, ANTI-HUMAN, POST-HUMAN
Authors: Setyobudi Imam 
Published: January 2018

The core of Wayang stories (Mahabharata, Bharatayuda, Ramayana) is the reflection of human that is always continuously in crisis and emergency situations and conditions. Tragic. Wayang stories raise humanity problems so that the existences of human conception experience the perpetuity of dehumanization, existential instability and ambiguous. The killing of the essence of the human existence purpose on earth. It is an issue fundamentally of anti-human.Shadow play perspective does not rest on human understanding or Knight (Pandawa, Kurawa, Rama, Giant), the heaven God (Bathara Guru), and/or Prabu Khresna, incarnation of Wisnhu God. Wayang stories evoke Togog and Semar angle. Liyan. Grassroots. The general public. Amorphous: No Man is not a knight instead of a brahmana is not god instead of giant.Arises a question that is closely related to the presence of Togog and Semar. Why do shadow play stories present the figure of the them, while the authentic story of the Mahabharata and Ramayana India version does not exist at all? Are Togog and Semar truly actualization of post-human aesthetic and post-human anthropology ideas?The substance of this writing ask us to discuss regarding the idea of Togog and Semar in shadow play into the realm of post-human discourse as a result of dehumanization signs in the frame of shadow play stories. The main focus of the discussion focused on the position of Togog and Semar as the figure as linuwih or great beyond human (knight) and god. Study restriction on the context of Purwa Java Gagrak Jogja and Solo wayang; similarly in East Java, Sunda and Bali, there are also those two figures.
Resetting the Compass: An Immersive Intervention to Develop Abilities in Construction Management
Authors: Smallwood John , Allen Christopher 
Published: January 2018

Students’ post-intervention perceptions of an event provide insight relative to their understanding and appreciation of the intervention, as well as the impact thereof.Experience and anecdotal evidence indicate that Honours students experience challenges in terms of completing the academic year.The purpose of the study reported on is to determine the impact of a one-day team building event on participants directed at, inter alia, developing their ability to manage themselves, work as a team, and interface with each other, and their ability to strategise, plan, evolve tactics, and take action, based upon a self-administered questionnaire survey conducted in a South African university. The students were surveyed after the completion of the event.The salient findings include - the team building activities impacted on participants in many ways, contributed to an enhancement of their ability to strategise, plan, evolve tactics, and take action, and participants enjoyed and benefited from the team building activities.It can be concluded that the one-day team building event had the desired impact in terms of the development of participants’ ability to manage themselves, work as a team, and interface with each other, and their ability to strategise, plan, evolve tactics, and take action.It is recommended that the one-day team building event continue to be staged at the beginning of the Honours year, and that the post-event research be conducted on an annual basis.
RED TIDE DETECTION USING Seawifs STANDARD CHOLOROPHYLL-a ALGORITHM IN SOUTHEAST KOREAN WATERS
Authors: Winarso Gathot 
Published: January 2018

Cochlodinium polykrikoides red tides have occurred in summer every year at coastal waters of the South Korea. Chlorophyll-a concentration data estimated from ocean color satellite SeaWiFS (Sea-viewing Wide Field-of-view Sensor) were used to detect the red tide in this study. The high value of chlorophyll-a concentration used to detect red tide was analyzed and compared with red tide map produced by National Fisheries Research and Development Institute of Korea (NFRDI). Based on SeaWiFS data and NFRDI red tide map, it was found that high chlorophyll-a concentration of ≥ 5 mg/m3in SeaWiFS images corresponded to the red-tide occurrence with some limitations.
DETECTING THE SPATIAL DISTRIBUTION OF SETTLEMENTS ON VOLCANIC REGION USING IMAGE LANDSAT-8 OLI IMAGERY
Authors: Suwarsono . , Khomarudin M. Rokhis 
Published: January 2018

Geologically, Indonesia region is on track ring of fire, brings the consequence that the danger of volcanic eruption could occur at any time. Information sites where the settlement is located in the affected areas on emergency response process is needed in quick time. The availability of up to date data is important because it illustrates the actual condition of the region. Active volcanic landforms ranging from the crater to footslope in general is prone area to volcanic eruption, either by the threat of lava flows, pyroclastic falls, or lahars. This study aims to detect the spatial distribution of the settlement on volcanic region using Landsat-8 OLI. Parameters used for the detection of settlements is Normalized Difference Build-up Index (NDBI). Research methods include radiometric correction, delineation of the boundaries of volcanic landforms, NDBI value extraction, extraction of settlement areas, as well as the accuracy assesment. Study area is Sinabung Volcano region located in the province of North Sumatera. Recently, the volcano experienced a devastating and catastrophic eruption. The results showed that the spatial distribution of settlements on volcanic landforms can be detected quickly from Landsat-8 OLI based on NDBI parameters with a sufficient degree of accuracy.
Animality, Biopolitics, and Umwelt in Amitav Ghosh’s The Hungry Tide
Authors: Tsai Robin Chen-Hsing 
Published: January 2018

Tsai explores Ghosh’s novel in relation to intersecting histories of both human and nonhuman violence. Set in the tide country of the Sundarbans in Bangladesh and India, the novel dramatizes vulnerable forms of life, including endangered river dolphins and dispossessed people, threatened not only by storms and floods stemming from global warming but also by the neo-imperialist violence of the state. Tsai’s reading of the novel draws upon the concept of the Umwelt from Jakob von Uexküll, as well as the fields of animality studies, biopolitics, systems theory, and phenomenology, in order to argue for what he calls a “critical bioregionalism” in which advocacy for vulnerable places needs to be attentive to the overlapping forms and histories of violence that connect human and nonhuman inhabitants.
Servius, Cicero and the Res Publica of Justinian
Authors: Harries Jill 
Published: January 2018

Cicero’s correspondence with Servius after the death of Tullia
justifies cultural attitudes which denied legal agency to the
populus;Servius’ juristic successors also perpetuated the role of elite
legal thinkers as “procurators” and Pomponius’ history of jurisprudence did not acknowledge the transition from ‘Republic” to Empire, which removed constitutional agency from the populus.
Servius, Cicero and the successor jurists thus paved the way for
the res publica of the autocrat Justinian.
Impulsive Synchronisation: A Conversation on Military Technologies and Audiovisual Arts
Authors: Satz Aura , Parikka Jussi 
Published: January 2018

Stemming from their common interest in media archeology and the idea of the air as a medium of encrypted signals, Satz and Parikka explore the themes emerging from Satz's film installation 'Impulsive Synchronisation' (2013). Satz has used various technologies as the subject of her work, including the Chladni plate, mechanical music, phonograph grooves and optical sound, looking at how such objects tap into ideas of knowledge and communication in their use of notation systems, languages or codes. Satz is also interested in bringing to the fore key female figures largely excluded from mainstream historical discourse in an ongoing engagement with the question of women’s contributions to labour, technology and scientific knowledge. The starting point for ‘Impulsive Synchronisation’ was a 'Secret Communication System' patented during World War II by Hollywood star Hedy Lamarr and American composer George Antheil. This invention of 'frequency hopping', designed to protect radio-controlled torpedoes from enemy disruption by distributing the signal over many frequencies and synchronising the transmitter and receiver in rapidly changing patterns, has become the basis for today's spread-spectrum technology. In Satz’s work, these technologies are referenced to explore visual, musical and data notation, as well as its encryption, synchronisation and decipherment.
Kinematics of the Horsehead Nebula and IC 434 Ionization Front in CO and C+
Authors: Bally John , Chambers Ed , Guzman Viviana , Keto Eric , Mookerjea Bhaswati , Sandell Goran , Stanke Thomas , Zinnecker Hans 
Published: January 2018

Abstract
Stratospheric Observatory for Infrared Astronomy [C ii] 157 μm, APEX 860 μm J = 3−2 CO, and archival James Clerk Maxwell Telescope J = 2−1 CO and 13CO observations of the Horsehead Nebula are presented. The photon-dominated region (PDR) between the Orion B molecular cloud and the adjacent IC 434 H ii region is used to study the radial velocity structure of the region and the feedback impacts of UV radiation. Multiple west-facing cloud edges are superimposed along the line of sight with radial velocities that differ by a few kilometers per second. The Horsehead lies in the foreground blueshifted portion of the Orion B molecular cloud and is predominantly illuminated from the rear. The mean H2 density of the Horsehead,

, results in a spatially thin PDR where the photoablation flow has compressed the western cloud edge to an H2 density of

. The associated [C ii] 157 μm layer has a width L < 0.05 pc. The background parts of the Orion B cloud in the imaged field consist of a clumpy medium surrounded by molecular gas with H2 densities lower by one to two orders of magnitude. Along the straight part of the IC 434 ionization front, the PDR layer probed by [C ii] 157 μm emission is much thicker with L ∼ 0.5 pc. A possible model for the formation and evolution of this edge-on ionization front and PDR is presented. The [C ii] data were independently analyzed and published by Pabst et al.
HATS-50b through HATS-53b: Four Transiting Hot Jupiters Orbiting G-type Stars Discovered by the HATSouth Survey*
Authors: Henning Th. , Mancini L. , Sarkis P. , Bakos G. Á. , Hartman J. D. , Bayliss D. , Bento J. , Bhatti W. , Brahm R. , Ciceri S. , Csubry Z. , Val-Borro M. de , Espinoza N. , Fulton B. J. , Howard A. W. , Isaacson H. T. , Jordán A. , Marcy G. W. , Penev K. , Rabus M. , Suc V. , Tan T. G. , Tinney C. G. , Wright D. J. , Zhou G. , Durkan S. , Lazar J. , Papp I. , Sari P. 
Published: January 2018

Abstract
We report the discovery of four close-in transiting exoplanets (HATS-50b through HATS-53b), discovered using the HATSouth three-continent network of homogeneous and automated telescopes. These new exoplanets belong to the class of hot Jupiters and orbit G-type dwarf stars, with brightness in the range V = 12.5–14.0 mag. While HATS-53 has many physical characteristics similar to the Sun, the other three stars appear to be metal-rich (

), larger, and more massive. Three of the new exoplanets, namely HATS-50b, HATS-51b, and HATS-53b, have low density (HATS-50b:

,

; HATS-51b:

,

; HATS-53b:

,

) and similar orbital periods (

days,

days,

days, respectively). Instead, HATS-52b is more dense (mass

and radius

) and has a shorter orbital period (

days). It also receives an intensive radiation from its parent star and, consequently, presents a high equilibrium temperature (

K). HATS-50 shows a marginal additional transit feature consistent with an ultra-short-period hot super Neptune (upper mass limit 0.16

), which will be able to be confirmed with TESS photometry.
Bayesian Model Testing of Ellipsoidal Variations on Stars due to Hot Jupiters
Authors: Gai Anthony D. , Knuth Kevin H. 
Published: January 2018

Abstract
A massive planet closely orbiting its host star creates tidal forces that distort the typically spherical stellar surface. These distortions, known as ellipsoidal variations, result in changes in the photometric flux emitted by the star, which can be detected within the data from the Kepler Space Telescope. Currently, there exist several models describing such variations and their effect on the photometric flux. By using Bayesian model testing in conjunction with the Bayesian-based exoplanet characterization software package EXONEST, the most probable representation for ellipsoidal variations was determined for synthetic data and the confirmed hot Jupiter exoplanet Kepler-13A b. The most preferred model for ellipsoidal variations observed in the Kepler-13 light curve was determined to be EVIL-MC. Among the trigonometric models, the Modified Kane & Gelino model provided the best representation of ellipsoidal variations for the Kepler-13 system and may serve as a fast alternative to the more computationally intensive EVIL-MC. The computational feasibility of directly modeling the ellipsoidal variations of a star are examined and future work is outlined. Providing a more accurate model of ellipsoidal variations is expected to result in better planetary mass estimations.
The Origin and Evolution of Nucleosynthetic Sr Isotope Variability in Calcium and Aluminum-rich Refractory Inclusions
Authors: Myojo Kunihiro , Yokoyama Tetsuya , Okabayashi Satoki , Wakaki Shigeyuki , Sugiura Naoji , Iwamori Hikaru 
Published: January 2018

Abstract
Nucleosynthetic isotope anomalies in meteorites are useful for investigating the origin of materials in the protoplanetary disk and dynamical processes of planetary formation. In particular, calcium and aluminum-rich inclusions (CAIs) found in chondrites are key minerals for decoding the initial conditions of the solar system before the accretion of small planetary bodies. In this study, we report isotopic analyses for three Allende CAIs, fluffy type A (FTA), type B, and fine-grained spinel rich (FS) inclusions, with a specific emphasis on the measurements of 84Sr/86Sr ratios. It was found that the average μ
84Sr values (106 relative deviations from a standard material) were 175, 129, and 56 ppm for the samples of FTA, type B, and FS inclusions, respectively. Additionally, the FTA samples exhibited heterogeneous μ
84Sr values, while those for the type B and FS inclusions were homogeneous within individual inclusions. The elevated μ
84Sr values were most likely explained by the relative enrichment of r-process nuclides in the CAI formation region. The variation of μ
84Sr values between the FTA and type B inclusions, as well as within the FTA inclusion, suggests the presence of multiple CAI source reservoirs with distinct isotopic compositions, which is either inherited from isotopic heterogeneity in the molecular cloud or caused by the selective destruction of r-process-enriched supernova grains via nebular thermal processing. On the other hand, the reaction between a refractory precursor of the FS inclusion and a gaseous reservoir enriched in Mg, Si, and 16O resulted in the lowest μ
84Sr values for the FS inclusion.
“Red” but Not “Dead”: Actively Star-forming Brightest Cluster Galaxies at Low Redshifts
Authors: Runge James , Yan Haojing 
Published: January 2018

Abstract
Brightest cluster galaxies (BCGs) are believed to have assembled most of their stars early in time and therefore should be passively evolving at low redshifts and appear “red-and-dead.” However, there have been reports that a minority of low-redshift BCGs still have ongoing star formation rates (SFRs) of a few to even

. Such BCGs are found in “cool-core” (“CC”) clusters, and their star formation is thought to be fueled by “cooling flow.” To further investigate the implications of low-redshift, star-forming BCGs, we perform a systematic search using the 22 μm data (“W4” band) from the Wide-field Infrared Survey Explorer (WISE) on the GMBCG catalog, which contains 55,424 BCGs at

identified in the Sloan Digital Sky Survey (SDSS). Our sample consists of 389 BCGs that are bright in W4 (“W4BCGs”), most being brighter than 5 mJy. While some (

) might host active galactic nuclei, most W4BCGs should owe their strong mid-IR emissions to dust-enshrouded star formation. Their median total IR luminosity (L
IR) is

(SFR ∼50

, and 27% of the whole sample has

(SFR >100

). Using 10 W4BCGs that have Chandra X-ray data, we show that 7 of them are possibly in CC clusters. However, in most cases (five out of seven) the mass deposition rate cannot account for the observed SFR. This casts doubt on the idea that cooling flows are the cause of the star formation in non-quiescent BCGs.
Supercritical Accretion onto a Non-magnetized Neutron Star: Why is it Feasible?
Authors: Takahashi Hiroyuki R. , Mineshige Shin , Ohsuga Ken 
Published: January 2018

Abstract
To understand why supercritical accretion is feasible onto a neutron star (NS), we carefully examine the accretion flow dynamics by 2.5-dimensional general relativistic radiation magnetohydrodynamic (RMHD) simulations, comparing the cases of accretion onto a non-magnetized NS and that onto a black hole (BH). Supercritical BH accretion is relatively easy, since BHs can swallow excess radiation energy, so that radiation flux can be inward in its vicinity. This mechanism can never work for an NS, which has a solid surface. In fact, we find that the radiation force is always outward. Instead, we found significant reduction in the mass accretion rate due to strong radiation-pressure-driven outflow. The radiation flux F
rad is self-regulated such that the radiation force balances with the sum of gravity and centrifugal forces. Even when the radiation energy density greatly exceeds that expected from the Eddington luminosity

E

rad

≃

F

rad

τ

/

c
>

10

2

L

Edd

/

(
4
π

r

2

c
)

, the radiation flux is always kept below a certain value, which makes it possible not to blow all the gas away from the disk. These effects make supercritical accretion feasible. We also find that a settling region, where accretion is significantly decelerated by a radiation cushion, is formed around the NS surface. In the settling region, the radiation temperature and mass density roughly follow

T

rad

∝

r

−
1

and

ρ
∝

r

−
3

, respectively. No settling region appears around the BH, so matter can be directly swallowed by the BH with supersonic speed.
On the Synchrotron Spectrum of GRB Prompt Emission
Authors: Xu Siyao , Yang Yuan-Pei , Zhang Bing 
Published: January 2018

Abstract
The prompt emission spectrum of gamma-ray bursts is characterized by a smoothly joint broken power-law spectrum known as the Band function. The typical low-energy photon index is

, which poses a challenge to standard synchrotron radiation models. We investigate the electron energy spectrum as a result of the interplay among adiabatic stochastic acceleration (ASA), particle injection, and synchrotron cooling. In the ASA-dominated low-energy range, ASA enables an efficient hardening of the injected energy spectrum to approach a spectral index −1. In the synchrotron cooling-dominated high-energy range, the injected high-energy electrons undergo fast synchrotron cooling and have a softer photon spectrum. With the energy range of the injected electrons broadly covering both the ASA- and synchrotron cooling-dominated ranges, the resulting photon number spectrum has low- and high-energy indices of

and

, respectively. The break energy is of the order of ∼100 keV, depending on the turbulence properties.