bluuebunny/crossref_metadata_2025_split huggingface dataset:
Analysis of a Single-Sever Queue with Disasters and Repairs Under Bernoulli Vacation Schedule
Authors: Ye Jingjing , Liu Liwei , Jiang Tao 
Published: March 2017

AbstractThis paper studies a single-sever queue with disasters and repairs, in which after each service completion the server may take a vacation with probabilityq(0≤q≤1), or begin to serve the next customer, if any, with probabilityp(= 1− q). The disaster only affects the system when the server is in operation, and once it occurs, all customers present are eliminated from the system. We obtain the stationary probability generating functions (PGFs) of the number of customers in the system by solving the balance equations of the system. Some performance measures such as the mean system length, the probability that the server is in different states, the rate at which disasters occur and the rate of initiations of busy period are determined. We also derive the sojourn time distribution and the mean sojourn time. In addition, some numerical examples are presented to show the effect of the parameters on the mean system length.
Revolutionary Reading, Evolutionary Toolmaking: (Re)development of Scholarly Reading and Annotation Tools in Response to an Ever Changing Scholarly Climate
Authors: MacGregor James B. , Joyce Michael , Hirsch Brett , Leitch Cara , Siemens Ray , Chiang Chia-Ning , Kopak Rick 
Published: March 2017

As the online scholarly landscape changes, so too must the tools used to traverse it. The Public Knowledge Project (PKP) Reading Tools provides readers a bridge from online scholarly content to a host of contextual information, to a number of discipline-specific search engines and databases, and to other tools. A lot has changed since it was originally released, such as the rise of Google Scholar as the de facto starting point for many novice (and not-so novice) researchers; the blurring line between desktop and web applications; and the increased professional use of social networking tools and websites. Recently, the University of Victoria's Electronic Textual Cultures Lab (ETCL), in cooperation with the PKP, undertook a study to determine the role and value of the existing Reading Tools, particularly in the context of Humanities Computing. The ETCL has also developed a prototype Professional Reading Environment which has been the basis for substantial analysis. Rick Kopak and Chia-Ning Chiang at the University of British Columbia (UBC) have undertaken a broad survey of the online annotation landscape, and have written a proposal for developing an annotation system for PKP software. This paper discusses how, using this research as a base and in cooperation with UBC and the PKP, the ETCL has begun a large-scale redevelopment of the PKP Reading Tools, extending the current toolset to include new social networking and research tools, as well as a robust personal annotation system, making social annotation possible between small groups and the public.
Homer and the New Testament as “Multitexts” in the Digital Age
Authors: Clivaz Claire 
Published: March 2017

The field of classical studies has undergone a radical transformation with the arrival of the digital age, particularly with regard to the editing of ancient texts. As Umberto Eco (2003) pointed out, the digital age may mean the end of the history of variants and of the notion of the “original text.” Among the texts of antiquity, the editing of Homer and of the New Testament are more especially susceptible to the effects of digital technology because of their numerous manuscripts. Whereas the “Homer Multitext” project recognizes that the notion of a synthetic critical edition is now seriously brought into question, the prototype of the online Greek New Testament continues to be based on the aim of obtaining a unique text, in the style of a printed critical edition. As it moves from a printed culture to the digital age, the editing of the Greek NT is also confronted by the emergence of non-Western scholarship. For example, the presence is to be noted of Arabic Muslim websites that examine Greek New Testament manuscripts but without directly interacting with Western scholarship.
Responding to Change and Transition in INKE’s Year 3
Authors: Siemens Lynne 
Published: March 2017

Use of project teams is increasing, however little is known about collaboration as it actually occurs over the life of projects. This paper explores the nature of collaboration within Implementing New Knowledge Environments (INKE) after three years of funded research. The third year is characterized by change and transition with new team members, partners, and sub-research areas. INKE continues to draw upon structures and processes, including team building activities, in-person meetings, multiple communication channels, evolving governance documents to support the collaboration, and incorporating collaboration-ready individuals. The paper concludes with recommendations for similar long term, large-scale project teams.
Re/collections: From Books to Blogs
Authors: Lay Ethna Dempsey 
Published: March 2017

This study considers the contemporary post-literacy moment and its kinship to the historical change from Anglo-Saxon orality to English literacy, by suggesting a parallel between the scholarship of Walter Ong and the new media scholar Lev Manovich. Their perspectives on communication and textuality inform the conversation about how contemporary first-year writers make meaning. Student writers exhibit remix as a kind of new orality, some sequel to literacy. This notion speaks to the students’ orientation as digital composers, for whom the written word has been displaced as the primary way to present knowledge. Primary data is drawn from student invention blogs.
Inference and Linking on the Humanist’s Semantic Web
Authors: Simpson John Edward 
Published: March 2017

The Semantic Web promises that the pools of semantic data it interweaves together will enable people to find information that they could not otherwise find by revealing knowledge not explicitly visible in the distributed source data. In order for this promise to be fulfilled within the humanities, the Semantic Web data being created must have certain features, but what are they? This article provides some background on Semantic Web inferencing and then argues that there are three things that humanists can do to prepare their data to participant in this sort of inference generation: add more data, reciprocate links across repositories, and add metadata specifically to support inferencing.
History Moves: Mobilizing Public Histories in Post-Digital Space
Authors: Wizinsky Matthew , Brier Jennifer 
Published: March 2017

Similar to most cultural forms today, history is collected, edited, manipulated, stored, displayed, distributed, and otherwise produced through a complex network of post-digital techniques and media. It is often produced only by historians. History Moves is a public history project that aims to produce cogent and collective historical experiences within the cultural frame of mutable and highly distributed media forms. It does this by bringing history, design, and historical subjects into conversation to shape public space. The project uses a participatory process that mobilizes people to interpret history by mobilizing digital and analogue media. History Moves transforms historical subjects into history-makers while simultaneously and repeatedly transfiguring media into forms that are engaging and accessible to widely distributed audiences. This article recounts a case study where History Moves worked with a group of women living with HIV/AIDS to present a history of the epidemic and a women’s history of Chicago. We suggest that the example provides a model for how to build participatory digital history projects and collaborative history displays.
StructureMorph: Creating Scholarly 3D Models for a Convergent, Digital Publishing Environment
Authors: Bonnett John , Anderson Mark , Tang Wei , Farrimond Brian , Robichaud Léon 
Published: March 2017

Background: The StructureMorph project rests on the premise that future publishing platforms will converge multiple applications, such as geographic information systems (GIS) and game engines, and multiple paradigms of computing, such as desktop computing and high-performance computing. Convergent platforms will also present design challenges for scholars.Analysis: In this contribution, one response to these challenges is presented: the Complex Object. Complex Objects are 4D models that alter their shape and surface appearance in response to user interaction, and changes in world time. They also to mimic the behaviours of 2D polygons as configured in geographic information systems, graphically linking attribute data with spatial locales.Conclusion and implications: This article discusses the concept of the Complex Object and describes the software and workflow devised to support its creation.
THE DIVERSITY OF REPTILES ON SEVERAL HABITAT TYPES IN CAMPUS AREA OF SRIWIJAYA UNIVERSITY INDRALAYA, OGAN ILIR
Authors: Saptalisa Wenny , Yustian Indra , Setiawan Arum 
Published: March 2017

The Diversity of Reptiles on Several Habitat Types in Campus Area of Sriwijaya University Indralaya, Ogan Ilir was aimed to determine the diversity of amphibian species present in this area. The research has been done in March until May 2015, in the campus of the Sriwijaya University, Indralaya. The method in this study is use the transect method by placing seventh transect line on line with the direction of cutting contour lines. Data collection techniques using the Visual Encounter Survey (VES) and Pit-Fall Trap method in combination with the Straight Line Method and Fence (Drift Fence). Results from this study recorded 11 species of amphibians from five families of the Anura Order. Average diversity index at Sriwijaya University Indralaya region is 1.70 which fall into the medium category. Keywords : Sriwijaya university, amphibians, transect,diversity
LIFE HISTORY ANNELIDA: POLYCHAETA IN AN ESTUARY OF THE OMUTA-GAWA RIVER, KYUSHU, JAPAN
Authors: Hanafiah Zazili 
Published: March 2017

The research was conducted at four　stations in the Omuta-gawa River, Kyushu, Japan from December 2003 to July 2005. The results of the monthly survey clearly indicated that Hediste japonica has one generation per year. The reproductive period of this species is from late December to late February, and also occurred on H. diaroma, that it has one generation per year. The reproductive period of this species in the Omuta-gawa River is from middle December to late April, when reproductive swarming of mature adults occurs. This reproductive period is much longer than that of H. japonica. Both Hediste species, spawning, fertilization and early development occur in water column with a long pelagic larval life. Keywords: life history, Hediste japonica, H. diadroma, reproductive period, estuary
CHARACTERISTICS OF MACROZOOBENTHOS COMMUNITY WITH SUBSTRATES TYPE AT WARKUK RIVER DISTRICK OF WARKUK RANAU SELATAN, OKU SELATAN REGENCY, SOUTH SUMATERA
Authors: Hamudin Frianti , Fauziah - , Hanafiah Zazili 
Published: March 2017

The research about Characteristic of Macrozoobenthos Community With Substrates Type At Warkuk River Districk of Warkuk Ranau Selatan, OKU Selatann Regency, South Sumatera has been conducted from May 2013 to December 2015. This study aims to analysis of characteristic and makrozoobenthos composition in substrat type, analysis about physic and chemistry condition at Warkuk River. Determination of sampling sites were conducted by Random Sampling. The Sample of macrozoobenthos were identified at the Laboratory of Research Institute for Inland Fisheries Mariana, Palembang. From the results obtained, are grouped into 3 classes of macrozoobenthos namely Insecta, Gastropoda and Oligochaeta, which is classified into 9 orders consists of 14 families, 16 spesies. Density ranging from 1155,56 to 1755,56 individuals/m2. Level of diversity are high, ranging from 1,95 to 2,41 and dominance index ranging from 0,31 to 0,40. Family Biotic Index (FBI) ranging from 3,47 to 3,98 with the water quality category of excellent.Key words : Warkuk River, Macrozoobenthos, Substrat Type
A SIMPLE PROTOCOL FOR SOMATIC EMBRYOGENESIS INDUCTION OF IN VITRO SUGARCANE ( Saccharum officinarum. L) BY 2,4-D AND BAP
Authors: Widuri Laily Ilman , Dewanti Parawita , Sugiharto Bambang 
Published: March 2017

Induction of in vitro sugarcane through somatic embryogenesis technique influenced by addition of plant growth regulator. The objective of this research was to determine appropriate formulation medium for indirect somatic embryogenesis induction on two potential sugarcane SUT Event 02 and PS 881. This research carried out in three steps, callus induction, callus proliferation, and shoot regeneration. Explants taken from basal of in vitro plantlet one month SUT Event 02 and PS 881 resulted from shoot regeneration previously. Five different medium formulas applied for callus induction and one formula for proliferation and shoot regeneration. Research using completely randomized design (CRD) factorial with five different formulation induction mediums. The result showed that the best respond of indirect somatic embryogenesis on SUT Event 02 and PS 881 was medium containing 3 mgL-1of 2,4-D.
FOOD HABITS AND FEEDING HABITS OF BARRAMUNDI FISH (Lates calcarifer Block) IN TERUSAN DALAM (INSIDE CANAL) WATERS, EAST COAST OF SOUTH SUMATERA PROVINCE
Authors: Ridho Mohammad Rasyid , Patriono Enggar 
Published: March 2017

Research about the food habits and feeding habits of Barramundi (Lates calcarifer Block) in Terusan Dalam (inside canal) waters, East coast of South Sumatera Province, had been done during March to June 2012. The purpose of this research was to analyze the food habits and feeding habits of Barramundi (Lates calcarifer Block) on Terusan Dalam (inside canal) waters, East coast of South Sumatera Province. Sampling method of the fish was purposive sampling method using Tangsi net. The results of this research showed that the number of fish from March to June totaled 31 individuals of fish. Based on the Relative Importance Index (RII), the natural food of Barramundi (Lates calcarifer Block) in March to June 2012 consisted of shrimp as the main food with the Relative Importance Index 72.37-99.51%, the fish was as the complement food with the Relative Importance Index 11.33-27.63%, and as the additional food was the worm with Relative Importance Index 0.49%.Keywords: Barramundi, food habits, feeding habits
Religion and Mythology in the Chilembwe Rising of 1915 in Nyasaland and the Easter Rising of 1916 in Ireland: Preparing for the End Times?
Authors: Thompson T. Jack 
Published: March 2017

Superficially there are many parallels between the Chilembwe Rising of 1915 in Nyasaland and the Easter Rising of 1916 in Ireland – both were anti-colonial rebellions against British rule. One interesting difference, however, occurs in the way academics have treated John Chilembwe, leader of the Nyasaland Rising, and Patrick Pearse, one of the leaders of the Irish Rising and the man who was proclaimed head of state of the Provisional government of Ireland. For while much research on Pearse has dealt with his religious ideas, comparatively little on Chilembwe has looked in detail at his religious motivation – even though he was the leader of an independent church.This paper begins by looking at some of the major strands in the religious thinking of Pearse, before going on to concentrate on the people and ideas which influenced Chilembwe both in Nyasaland and the United States. It argues that while many of these ideas were initially influenced by radical evangelical thought in the area of racial injustice, Chilembwe's thinking in the months immediately preceding his rebellion became increasingly obsessed by the possibility that the End Time prophecies of the Book of Daniel might apply to the current political position in Nyasaland. The conclusion is that much more academic attention needs to be given to the millennial aspects of Chilembwe's thinking as a contributory motivation for rebellion.
Collisions of Terrestrial Worlds: The Occurrence of Extreme Mid-infrared Excesses around Low-mass Field Stars
Authors: Theissen Christopher A. , West Andrew A. 
Published: March 2017

Abstract
We present the results of an investigation into the occurrence and properties (stellar age and mass trends) of low-mass field stars exhibiting extreme mid-infrared (MIR) excesses (

). Stars for the analysis were initially selected from the Motion Verified Red Stars (MoVeRS) catalog of photometric stars with Sloan Digital Sky Survey, 2MASS, and WISE photometry and significant proper motions. We identify 584 stars exhibiting extreme MIR excesses, selected based on an empirical relationship for main-sequence

colors. For a small subset of the sample, we show, using spectroscopic tracers of stellar age (Hα and Li i) and luminosity class, that the parent sample is most likely comprised of field dwarfs (

Gyr). We also develop the Low-mass Kinematics (LoKi) galactic model to estimate the completeness of the extreme MIR excess sample. Using Galactic height as a proxy for stellar age, the completeness-corrected analysis indicates a distinct age dependence for field stars exhibiting extreme MIR excesses. We also find a trend with stellar mass (using r − z color as a proxy). Our findings are consistent with the detected extreme MIR excesses originating from dust created in a short-lived collisional cascade (≲100,000 years) during a giant impact between two large planetismals or terrestrial planets. These stars with extreme MIR excesses also provide support for planetary collisions being the dominant mechanism in creating the observed Kepler dichotomy (the need for more than a single mode, typically two, to explain the variety of planetary system architectures Kepler has observed), rather than different formation mechanisms.
Source Population and Acceleration Location of Suprathermal Heavy Ions in Corotating Interaction Regions
Authors: Filwett R. J. , Desai M. I. , Dayeh M. A. , Broiles T. W. 
Published: March 2017

Abstract
We have analyzed the ∼20–320 keV nucleon−1 suprathermal (ST) heavy ion abundances in 41 corotating interaction regions (CIRs) observed by the Wind spacecraft from 1995 January to 2008 December. Our results are: (1) the CIR Fe/CNO and NeS/CNO ratios vary with the sunspot number, with values being closer to average solar energetic particle event values during solar maxima and lower than nominal solar wind values during solar minima. The physical mechanism responsible for the depleted abundances during solar minimum remains an open question. (2) The Fe/CNO increases with energy in the 6 events that occurred during solar maximum, while no such trends are observed for the 35 events during solar minimum. (3) The Fe/CNO shows no correlation with the average solar wind speed. (4) The Fe/CNO is well correlated with the corresponding upstream ∼20–320 keV nucleon−1 Fe/CNO and not with the solar wind Fe/O measured by ACE in 31 events. Using the correlations between the upstream ∼20–40 keV nucleon−1 Fe/CNO and the ∼20–320 keV nucleon−1 Fe/CNO in CIRs, we estimate that, on average, the ST particles traveled ∼2 au along the nominal Parker spiral field line, which corresponds to upper limits for the radial distance of the source or acceleration location of ∼1 au beyond Earth orbit. Our results are consistent with those obtained from recent surveys, and confirm that CIR ST heavy ions are accelerated more locally, and are at odds with the traditional viewpoint that CIR ions seen at 1 au are bulk solar wind ions accelerated between 3 and 5 au.
The Abundance of Atmospheric CO2 in Ocean Exoplanets: a Novel CO2 Deposition Mechanism
Authors: Levi A. , Sasselov D. , Podolak M. 
Published: March 2017

Abstract
We consider super-Earth sized planets which have a water mass fraction large enough to form an external mantle composed of high-pressure water-ice polymorphs and also lack a substantial H/He atmosphere. We consider such planets in their habitable zone, so that their outermost condensed mantle is a global, deep, liquid ocean. For these ocean planets, we investigate potential internal reservoirs of CO2, the amount of CO2 dissolved in the ocean for the various saturation conditions encountered, and the ocean-atmosphere exchange flux of CO2. We find that, in a steady state, the abundance of CO2 in the atmosphere has two possible states. When wind-driven circulation is the dominant CO2 exchange mechanism, an atmosphere of tens of bars of CO2 results, where the exact value depends on the subtropical ocean surface temperature and the deep ocean temperature. When sea-ice formation, acting on these planets as a CO2 deposition mechanism, is the dominant exchange mechanism, an atmosphere of a few bars of CO2 is established. The exact value depends on the subpolar surface temperature. Our results suggest the possibility of a negative feedback mechanism, unique to water planets, where a reduction in the subpolar temperature drives more CO2 into the atmosphere to increase the greenhouse effect.
The Metallicity Distribution and Hot Jupiter Rate of the Kepler Field: Hectochelle High-resolution Spectroscopy for 776 Kepler Target Stars
Authors: Guo Xueying , Johnson John A. , Mann Andrew W. , Kraus Adam L. , Curtis Jason L. , Latham David W. 
Published: March 2017

Abstract
The occurrence rate of hot Jupiters from the Kepler transit survey is roughly half that of radial velocity surveys targeting solar neighborhood stars. One hypothesis to explain this difference is that the two surveys target stars with different stellar metallicity distributions. To test this hypothesis, we measure the metallicity distribution of the Kepler targets using the Hectochelle multi-fiber, high-resolution spectrograph. Limiting our spectroscopic analysis to 610 dwarf stars in our sample with

> 3.5, we measure a metallicity distribution characterized by a mean of

, in agreement with previous studies of the Kepler field target stars. In comparison, the metallicity distribution of the California Planet Search radial velocity sample has a mean of

, and the samples come from different parent populations according to a Kolmogorov–Smirnov test. We refit the exponential relation between the fraction of stars hosting a close-in giant planet and the host star metallicity using a sample of dwarf stars from the California Planet Search with updated metallicities. The best-fit relation tells us that the difference in metallicity between the two samples is insufficient to explain the discrepant hot Jupiter occurrence rates; the metallicity difference would need to be ≃0.2–0.3 dex for perfect agreement. We also show that (sub)giant contamination in the Kepler sample cannot reconcile the two occurrence calculations. We conclude that other factors, such as binary contamination and imperfect stellar properties, must also be at play.