bluuebunny/crossref_metadata_2025_split huggingface dataset:
Personal Hygiene Habits dan Kejadian Flour Albus Patologis pada Santriwati PP AL-Munawwir, Yogyakarta
Authors: Nikmah Umi Sa'adatun , Widyasih Hesty 
Published: July 2018

Fluor albus adalah cairan yang dikeluarkan dari alat genital wanita dan dibagi menjadi dua yaitu keputihan fisiologis dan patologis. Keputihan bukan suatu penyakit, tetapi merupakan manifestasi dari hampir semua penyakit kandungan. Penyebab paling sering keputihan adalah infeksi. Personal hygiene habits merupakan salah satu faktor yang memegang peranan penting untuk menghindari infeksi yang dapat menyebabkan keputihan. Penelitian ini bertujuan untuk mengetahui korelasi antara personal hygiene habits dengan kejadian fluor albus patologis. Metode penelitian menggunakan desain cross sectional dengan populasi penelitian santri Pondok Pesantren Al-Munawwir Komplek Q. Pengambilan sampel dilakukan dengan purposive dan random sampling dengan besar sampel 106 santri. Alat pengumpulan data adalah kuesioner personal hygiene habits dan fluor albus. Analisis data menggunakan uji Chi-Square dan Coefficient Contingency. Hasil penelitian menunjukkan bahwa 52% santri memiliki personal hygiene habits yang buruk dan sebanyak 75,5 santri mengalami fluor albus patologis. Hasil uji statistik didapatkan p=0.000 dan C=0,517, sehingga terdapat hubungan yang positif dan signifikan antara personal hygiene habits dengan kejadian fluor albus patologis. Semakin buruk personal hygiene habits seseorang, maka keputihan yang dialaminya semakin besar bersifat patologis.
Google Tekelinde Haberciliğin Dönüşümü
Authors: Güzel Mehmet , Özmen Kürşat 
Published: July 2018

Bu çalışma, bugün rakipsiz bir bilgi ve
haber kaynağı olarak yükselen Google’ın, görünürdeki hizmetlerinin perde
arkasına bakmak ve kapitalist pazar ilişkileriyle şekillenen tekel konumunun
haberciliğe etkilerini ortaya koymak amacıyla yapılmıştır. Çalışmanın odağına,
Google’ın dijital dünyada ortaya koyduğu yeni iş modelinden en çok etkilenen
alanların başında gelen haber medyası yerleştirilmiştir. Çalışmada, Google’ın
dijital dünyada yeni üretim biçimi, dağıtım kanalları ve gelir elde etme
üçgeninde haberciliği nasıl etkilediği sorusunun cevabı işin sahasında yer alan
profesyonellerin görüş ve deneyimleri üzerinden betimlenmeye çalışılmıştır.

Araştırmada, konuyla ilişkili literatür çerçevesinde, Google’ın
ekonomi politiği, kullanıcı bilgilerinin metalaştırılarak reklam piyasasında
satılması ile ortaya çıkan durum merkeze alınarak açıklanmaya ve Google’ın
internet haber medyasında yarattığı dönüşüm ana hatlarıyla ortaya konmuştur. Niteliksel
araştırma yaklaşımının benimsendiği çalışmada bulgular, araştırma soruları ve verilerden
hareketle oluşturulmuş ve ana başlıklar altında aktarılmıştır. Araştırma
sonuçlarından yola çıkarak habercilik eğitimi ve bu alanda yapılacak çalışmalar
için öneriler sunulmuştur.
Postoperative Pyogenic Cervical Discovertebral Spondylitis
Authors: Sharma Krishna 
Published: July 2018

Postoperative cervical discovertebral spondylitis is an uncommon problem, especially if it occurs soon after another surgery somewhere else in the body. The diagnosis is late as the symptoms like neck pain, are initially ignored and may present later with features of unstable spine and neurological defi cits. Management is like for any other pygenic spondylitis and may need surgical debridement, decompression and fi xation. Overall prognosis is good with timely treatment. Since the neck problem occurs soon after a surgery elsewhere in the body, the previous surgery could be blamed for the present spondylitis. Thus this may add a medico-legal dimension to the problem. Nepal Journal of Neuroscience. Vol. 13, No. 2, 2016, Page: 81-87
Gas-assisted Growth of Protoplanets in a Turbulent Medium
Authors: Rosenthal M. M. , Murray-Clay R. A. , Perets H. B. , Wolansky N. 
Published: July 2018

Abstract
Pebble accretion is a promising process for decreasing growth timescales of planetary cores, allowing gas giants to form at wide orbital separations. However, nebular turbulence can reduce the efficiency of this gas-assisted growth. We present an order-of-magnitude model of pebble accretion that calculates the impact of turbulence on the average velocity of small bodies, the radius for binary capture, and the sizes of the small bodies that can be accreted. We also include the effect of turbulence on the particle scale height, which has been studied in previous works. We find that turbulence does not prevent rapid growth in the high-mass regime: the last doubling time to the critical mass to trigger runaway gas accretion (M ∼ 10 M
⊕) is well within the disk lifetime, even for strong (α ≳ 10−2) turbulence. We find that, while the growth timescale is quite sensitive to the local properties of the protoplanetary disk, there are large regimes of parameter space over which large cores grow in less than the disk lifetime, if appropriately sized small bodies are present. Instead, the effects of turbulence are most pronounced for low planetary masses. For strong turbulence, the growth timescale is longer than the gas disk lifetime until the core reaches masses

. A “flow isolation mass,” at which binary capture ceases, emerges naturally from our model framework. We comment that the dependence of this mass on orbital separation is similar to the semimajor axis distribution of solar system cores.
The Evolution of Protoplanetary Disks: Probing the Inner Disk of Very Low Accretors
Authors: Thanathibodee Thanawuth , Calvet Nuria , Herczeg Gregory , Briceño César , Clark Catherine , Reiter Megan , Ingleby Laura , McClure Melissa , Maucó Karina , Hernández Jesús 
Published: July 2018

Abstract
We report FUV, optical, and NIR observations of three T Tauri stars in the Orion OB1b subassociation with Hα equivalent widths consistent with low or absent accretion and various degrees of excess flux in the mid-infrared. We aim to search for evidence of gas in the inner disk in HST Advanced Camera for Surveys/Solar Blind Channel spectra, and to probe the accretion flows onto the star using Hα and He i
λ10830 in spectra obtained at the Magellan and SOAR telescopes. At the critical age of 5 Myr, the targets are at different stages of disk evolution. One of our targets is clearly accreting, as shown by redshifted absorption at freefall velocities in the He i line and wide wings in Hα; however, a marginal detection of FUV H2 suggests that little gas is present in the inner disk, although the spectral energy distribution indicates that small dust still remains close to the star. Another target is surrounded by a transitional disk, with an inner cavity in which little sub-micron dust remains. Still, the inner disk shows substantial amounts of gas, accreting onto the star at a probably low but uncertain rate. The third target lacks both a He i line or FUV emission, consistent with no accretion or inner gas disk; its very weak IR excess is consistent with a debris disk. Different processes occurring in targets with ages close to the disk dispersal time suggest that the end of the accretion phase is reached in diverse ways.
ALMA Resolves C i Emission from the β Pictoris Debris Disk
Authors: Cataldi Gianni , Brandeker Alexis , Wu Yanqin , Chen Christine , Dent William , Vries Bernard L. de , Kamp Inga , Liseau René , Olofsson Göran , Pantin Eric , Roberge Aki 
Published: July 2018

Abstract
The debris disk around β Pictoris is known to contain gas. Previous ALMA observations revealed a CO belt at ∼85 au with a distinct clump, interpreted as a location of enhanced gas production. Photodissociation converts CO into C and O within ∼50 a. We resolve C i emission at 492 GHz using ALMA and study its spatial distribution. C i shows the same clump as seen for CO. This is surprising, as C is expected to quickly spread in azimuth. We derive a low C mass (between 5 × 10−4 and 3.1 × 10−3

), indicating that gas production started only recently (within ∼5000 a). No evidence is seen for an atomic accretion disk inward of the CO belt, perhaps because the gas did not yet have time to spread radially. The fact that C and CO share the same asymmetry argues against a previously proposed scenario where the clump is due to an outward-migrating planet trapping planetesimals in a resonance, nor can the observations be explained by an eccentric planetesimal belt secularly forced by a planet. Instead, we suggest that the dust and gas disks should be eccentric. Such a configuration, we further speculate, might be produced by a recent tidal disruption event. Assuming that the disrupted body has had a CO mass fraction of 10%, its total mass would be ≳3 M
Moon.
Glycinamide, a Glycine Precursor, Caught in the Gas Phase: A Laser-ablation Jet-cooled Rotational Study
Authors: Alonso E. R. , Kolesniková L. , Białkowska-Jaworska E. , Kisiel Z. , León I. , Guillemin J.-C. , Alonso J. L. 
Published: July 2018

Abstract
Glycinamide, a glycine precursor, has been successfully generated in the gas phase by laser ablation of its hydrochloride salt, and its microwave spectrum, recorded from 6 to 16 GHz using a Chirped Pulse Fourier Transform Microwave (LA-CP-FTMW) spectrometer, is reported for the first time. The existence of a single structure stabilized by a Na–H ⋯ NtH2 hydrogen bond has been revealed in the supersonic expansion. The complex nuclear quadrupole coupling hyperfine structure due to the two 14N nuclei has been completely resolved and analyzed using a Molecular Beam Fourier Transform Microwave spectrometer in combination with laser ablation (LA-MB-FTMW spectrometer). The first precise data obtained on this glycine precursor could be of great importance for possible future identifications in the interstellar medium.
Globular Clusters in a Cosmological N-body Simulation
Authors: Carlberg Raymond G. 
Published: July 2018

Abstract
Stellar dynamical model globular clusters are introduced into reconstituted versions of the dark matter halos of the Via Lactea II (VL-2) simulation to follow the star cluster tidal mass-loss and stellar stream formation. The clusters initially evolve within their local sub-galactic halo, later being accreted into the main halo. Stars are continually removed from the clusters, but those that emerged in the sub-galactic halos are dispersed in a wide stream when accreted into the main halo. Thin tidal streams that survive to the present can begin to form once a cluster is in the main halo. A higher-redshift start places the star clusters in denser halos, where they are subject to stronger tides leading to higher average mass-loss rates. A z = 3 start leads to a rich set of star streams, with nearly all within 100 kpc having a remnant progenitor star cluster in the stream. In contrast, with a z = 8 start, all star clusters that are accreted onto the main halo are completely dissolved. These results are compared to the available data on Milky Way streams, where the majority of streams do not have clearly associated globular clusters, which, if generally true, suggests that there were at least twice as many massive globular clusters at high redshift.
Hematological profile in natural progression of giardiasis: kinetics of experimental infection in gerbils
Authors: Gil Frederico Ferreira , Ventura Luciana Laranjo Amorim , Fonseca Joice Freitas , Saniago Helton Costa , Busatti Haendel , Santos Joseph Fabiano Guimarães , Gomes Maria Aparecida 
Published: July 2018

Introduction: The clinical manifestations of giardiasis and its impact are harmful to children, and may cause deficits in their physical and cognitive development. The pathogenic mechanisms are usually unknown and the available reports can be controversial.
Methodology: The present study aimed to know, for the first time, the evolution of the hematological profile of the gerbils, experimentally infected with Giardia lamblia, up to the infection’s resolution. Hematological variables have been tested.
Results: White blood cells have not presented meaningful alterations during the course of the infection. A significant reduction in the number of red blood cells (p = 0.021), in the concentration of hemoglobin (p = 0.029) and in the value of the hematocrit (p = 0.016) has been observed, starting from the second week of infection, ratifying an anemia related to giardiasis. Reduction in the level of serum iron starting from the third week of infection, despite not being significant, could suggest the participation of iron in the anemia. However, the weight of the animals was kept and the hematimetric parameters started to return to the basic values after the parasitological cure without iron reposition.
Conclusions: The outcomes found suggest the idea that not only malabsorption but also other mechanisms such as chronic inflammation may be implicated in iron deficiency anemia in giardiasis and may explain how asymptomatic patients may have anemia without malabsorption. In this context, considering the highlighting character of the anemia in our study, we believe that anemia should be investigated in children with giardiasis. And in the cases of anemia without a definite etiology, giardiasis should also be investigated.
Incidence and antibiotic susceptibility of MRSA infections in a Saudi Arabian Hospital: a 10-year surveillance study
Authors: Al-Hamad Arif Mansour , Alfaraj Afaq Ali , Altowaileb Jaffar , Al-Shamlan Sameer Mahdi , Leskafi Hussam , Alsubeikhy Fatimah Abdullah , Abbas Hussein Radhi 
Published: July 2018

Introduction: Methicillin-resistant Staphylococcus aureus (MRSA) infections remain prevalent and are associated with significant morbidity and mortality. The aim of the present study was to investigate the epidemiology of MRSA infections and antibiotic susceptibility in Qatif, Saudi Arabia.
Methodology: All patients who had positive culture for S. aureus from January 1, 2006 through December 31, 2015 were enrolled and analyzed in WHONET, a free database software developed by the World Health Organization (WHO). Patients’ data were collected from electronic medical records and traditional chart reviews to determine whether MRSA acquisition was likely to have been in the community or in the healthcare facility. Susceptibility results for community-associated (CA)-MRSA were compared with isolates from healthcare setting.
Results: A total of 3395 patients with S. aureus infections were analyzed, with an overall annual MRSA incidence of 25 cases per 100,000 patients (27% of total S. aureus isolates). While the majority (64%) of MRSA infections occurred in healthcare setting, CA-MRSA isolation increased steadily from 23% in 2006 to 60% in 2015, exceeding rate of isolation of healthcare-associated (HA)-MRSA. Skin and soft tissue, the lung and blood stream were the most common sites of infection, with 20% to 35% of MRSA infections occurring in pediatric patients. In the inpatient setting, the majority of infections due to MRSA were in surgical wards and critical care units. Compared with CA-MRSA, HA-MRSA isolates turned out to be more frequently resistant against ciprofloxacin, clindamycin, erythromycin, tetracycline, and trimethoprim/sulfamethoxazole.
Conclusions: Staphylococcus aureus continues to cause multiple site infections with a relatively stable methicillin-resistance rate, but the isolation of MRSA from the community is increasing.
Dissemination of ST101 blaOXA-48 producing Klebsiella pneumoniae at tertiary care setting
Authors: ElMahallawy Hadir , Zafer Mai Mahmoud , Al-Agamy Mohamed , Amin Magdy Aly , Mersal Mai Muhammed , Booq Rayan Yousef , Alyamani Essam , Radwan Samah 
Published: July 2018

Introduction: The worldwide dissemination of the acquired carbapenemases in Gram-negative bacteria is a strongly expressed demand for the emergence of post antibiotic era. The aim of this study was to test the production of carbapenemase by Klebsiella pneumoniae strains isolated from hospitalized cancer patients and to investigate the genetic relationship of carbapenemase producing carbapenem resistant K. pneumoniae using multilocus sequence typing (MLST).
Methodology: Antibiotic susceptibility testing and phenotypic testing for extended spectrum b-lactamases (ESBL) and carbapenemases production were performed. PCR amplification of ESBL and carbapenemase genes was performed. MLST was done to detect the genetic relatedness of the isolates.
Results: Our data showed all strains were sensitive to colistin. Carba NP test was positive in thirty-one carbapenem resistant K. pneumoniae isolates and 26 out of 34 K. pneumoniae isolates were metallo-beta-lactamases (MBL) positive. All carbapenemase-positive isolates were ESBL CTX-M-1-like positive. blaOXA-48 gene was detected in 25 isolates (80.65%) and 21 isolates (67.75%) produced blaNDM-1 like enzyme. VIM and KPC genes were not identified in this study. Association of blaOXA-48 like and blaNDM-1 like was found in 15 (48.39%) isolates, while the coproduction of OXA-48-like and IMP-1 was revealed in only one K. pneumoniae isolate. MLST revealed ten distinct sequence types (STs).
Conclusion: Here we have documented the coexistence of NDM-type and OXA-48-like, and the coproduction of OXA-48-like and IMP in carbapenem resistant K. pneumoniae in patients with cancer. The dominant clone of the OXA-48-like-producing K. pneumoniae isolates from Egypt was ST101 epidemic clone belonging to clonal complex 101, an association that has been reported worldwide. The second most frequent ST was ST383.ST11 was assigned to OXA-48-producing K. pneumoniae.
Collections Management and High-Throughput Digitization using Distributed Cyberinfrastructure Resources
Authors: Motz Gary , Zimmerman Alexander , Cook Kimberly , Bancroft Alyssa 
Published: July 2018

Collections digitization relies increasingly upon computational and data management resources that occasionally exceed the capacity of natural history collections and their managers and curators. Digitization of many tens of thousands of micropaleontological specimen slides, as evidenced by the effort presented here by the Indiana University Paleontology Collection, has been a concerted effort in adherence to the recommended practices of multifaceted aspects of collections management for both physical and digital collections resources. This presentation highlights the contributions of distributed cyberinfrastructure from the National Science Foundation-supported Extreme Science and Engineering Discovery Environment (XSEDE) for web-hosting of collections management system resources and distributed processing of millions of digital images and metadata records of specimens from our collections.
The Indiana University Center for Biological Research Collections is currently hosting its instance of the Specify collections management system (CMS) on a virtual server hosted on Jetstream, the cloud service for on-demand computational resources as provisioned by XSEDE. This web-service allows the CMS to be flexibly hosted on the cloud with additional services that can be provisioned on an as-needed basis for generating and integrating digitized collections objects in both web-friendly and digital preservation contexts. On-demand computing resources can be used for the manipulation of digital images for automated file I/O, scripted renaming of files for adherence to file naming conventions, derivative generation, and backup to our local tape archive for digital disaster preparedness and long-term storage.
Here, we will present our strategies for facilitating reproducible workflows for general collections digitization of the IUPC nomenclatorial types and figured specimens in addition to the gigapixel resolution photographs of our large collection of microfossils using our GIGAmacro system (e.g., this slide of conodonts). We aim to demonstrate the flexibility and nimbleness of cloud computing resources for replicating this, and other, workflows to enhance the findability, accessibility, interoperability, and reproducibility of the data and metadata contained within our collections.
This Old Herbarium: APHIS Compliance and Renovation Planning
Authors: Gardner Erika 
Published: July 2018

With the continuous evolution of permitting regulations the Department of Botany at the National Museum of Natural History (NMNH) in Washington D.C., invited an agent from the United States Department of Agriculture (USDA), Animal and Plant Health Inspection Service (APHIS) to discuss requirements for obtaining import permits for plant specimens. This meeting lead to the planning of restructuring existing procedures, workflows and modifications to the physical workspaces within our facilities. It also prompted the collection management staff to be well versed in the current regulations.
APHIS requires individuals applying for a permit to submit a Standard Operational Procedure document (SOP) of their facilities. The APHIS agent will review the sterile entry procedures in the SOP and determine if the facility qualifies. Before we drafted our final SOP, we researched SOPs from other APHIS compliant herbaria.
Most of the facilities at NMNH, constructed in 1910 and 1965, predates climate control and pest management best practice standards. After meeting with the APHIS agent, we reevaluated our packing and unpacking procedures. It was apparent that the frontline to combat pests should be as close to the shipping office entry point as possible. The ideal room is our drying room located next to the shipping office. Other room renovations where specimen processing occurs will be discussed in detail. PowerPoint is a major tool that helped with the visualization of the renovations. However, modifying and renovating spaces within the museum is not an easy feat because of the large scale coordinating efforts within the institution.
Beyond the physical changes, there has been unexpected changes as to the role of collection staff in the permitting process. The APHIS requirements have created new challenges. Collection management staff are now sources of information about what collectors need to know before applying for a permit. Collection staff must also know about the various tools available for answering collectors’ questions, such as being well versed in the USDA Phytosanitary export database (PExD). Overall, new restrictions and guild lines create unexpected changes for the overall form and function of collection management.
Dis-moi comment tu traites tes vieux et je te dirai dans quelle société tu vis
Authors: Bourdaire-Mignot Camille , Gründler Tatiana 
Published: July 2018

Alors que le Comité consultatif national d’éthique est engagé depuis des mois sur le front des états généraux de la bioéthique, il a profité d’un court répit entre la fin des consultations citoyennes et la remise de son rapport au Gouvernement pour rendre cet avis sur un autre sujet qui le préoccupe : le vieillissement. À partir de constats connus et quasi inchangés depuis 1998, le Comité consultatif national d’éthique rend un nouvel avis sur le vieillissement. Il entend manifestement bousculer notre société en dénonçant ses modèles dominants peu adaptés aux problématiques liées au grand âge et propose d’agir pour intégrer pleinement les personnes âgées dans notre société. Une société tournée vers ses vieux, tel est l’avenir !
IL-22: There Is a Gap in Our Knowledge
Authors: Zenewicz Lauren A 
Published: July 2018

Abstract
IL-22 is a critical cytokine in modulating tissue responses during inflammation. IL-22 is upregulated in many chronic inflammatory diseases, making IL-22 biology a potentially rewarding therapeutic target. However, this is complicated by the dual-natured role of IL-22 in inflammation, as the cytokine can be protective or inflammatory depending on the disease model. Although scientific interest in IL-22 has increased considerably in the past 10 y, there is still much we do not know about the environmental, cellular, and molecular factors that regulate the production and function of this cytokine. A better understanding of IL-22 biology will allow us to develop new or improved therapeutics for treating chronic inflammatory diseases. In this article, I will highlight some of the outstanding questions in IL-22 biology.