bluuebunny/crossref_metadata_2025_split huggingface dataset:
Identifikasi Senyawa Fenol Beberapa Aksesi Teki (Cyperus rotundus L.) serta Pengaruhnya terhadap Perkecambahan Biji Borreria alata (Aubl.) DC.
Authors: Dewi Sangrani Annisa , Chozin Muhammad Ahmad , Guntoro Dan Dwi 
Published: October 2017

Purple nutsedge (Cyperus rotundus L.) is one of the important weeds in the world because of its ability to suppress the production of crops and difficult to control. C. rotundus residues can suppress the growth of others weeds. The experiments were conducted to identify the phenolic compound of C. rotundus from six different accessions and to determine the allelopathic effects of C. rotundus extracts on germination of Borreria alata (Aubl.) DC. The identification of phenolic compound was done using extract from all part of mature C. rotundus taken from different accessions and was analyzed using GC-MS. Analysis of C. rotundus extracts on germination of B. alata was designed using completely randomized design with three replications. The treatments were extract of C. rotundus from different accessions (from Cikarawang-Darmaga, Babakan-Darmaga, Ciawi, Megamendung, Cisarua, and Cianjur) with different concentration, 0.75 kg L-1 and 1.5 kg L-1. The result showed that C. rotundus from six accession had phenolic compond with different amounts. Cianjur accesion contained the most phenol content such as 2-furanmethanol; 1,4-benzenediol; 2-methoxy-4-vinylphenol; phenol, 2,6-dimethoxy; syringic acid; and 3-hydroxybenzoic acid. Germination test showed that C. rotundus extracts from different accessions and concentration had the same inhibitory effect on germination of B. alata.Keywords: Allelopathy, bioherbicide, purple nutsedge, weed management
Pewarisan Sifat Karakter Kualitatif dan Kuantitatif pada Hipokotil dan Kotiledon Cabai (Capsicum annuum L.)
Authors: Rtionga Arya Widura , Syukur Muhamad , Yunianti Rahmi , Sobir Dan 
Published: October 2017

Characters on hypocotyl dan cotyledon are very potential used for effective and efficient morphology marker for some crop plants. However, the information about the inheritance of qualitative and quantitative characters on hypocotyl and cotyledon of chili pepper was not available. The aim of this research was to determine the inheritance of qualitative and quantitative characters on hypocotyl and cotyledon of chili pepper. This research used purple chili pepper (P1 (IPB C20)), green chili pepper (P2 (IPB C2)), F1, F1R, BCP1, BCP2, and F2 populations. Analysis for qualitative characters used mendelian genetics analysis, whereas model genetic prediction for quantitative characters used join scaling test analysis. The result showed that hypocotyl and cotyledon color of chili pepper controlled by single gene. The gene controlling purple color was dominant than the gene controlling green color on hypocotyl, whereas the gene controlling green color was dominant than the gene controlling purple color on cotyledon. The additive-dominant genetic model with influence of additive-additive and additive-dominant interaction was suitable for hypocotyl length. The additive-dominant genetic model with influence of additive-dominant and dominant-dominant interaction was suitable for hypocotyls diameter. The additive-dominant genetic model with influence of additive-additive and dominant-dominant interaction was suitable for cotyledon width and cotyledon length. Keywords: genetic model, morfology marker, natural cross-pollination
Evaluation of a New and Simple Classification for Endoscopic Sinus Surgery
Authors: Kanai Kengo , Okano Mitsuhiro , Haruna Takenori , Higaki Takaya , Omichi Ryotaro , Makihara Sei-ichiro , Tsumura Munechika , Kariya Shin , Hirata Yuji , Nishizaki Kazunori 
Published: October 2017

Objective In 2013, the Japanese Rhinologic Society proposed a simple classification for endoscopic sinus surgery (ESS). This classification consists of five procedures (type I, fenestration of the ostiomeatal complex, with uncinectomy and widening of the natural ostium; type II, single-sinus procedure, with manipulating the inside of the sinus; type III, polysinus procedure; type IV, pansinus procedure; type V, extended procedure beyond the sinus wall). The clinical relevance of this classification in chronic rhinosinusitis (CRS) and paranasal sinus cyst was evaluated. Study Design A retrospective validation study. Methods A total of 122 patients (195 sinuses) who underwent ESS in Okayama University Hospital in 2012 were enrolled. The relationships between the ESS classification and the clinical course, including the operation time, bleeding amounts during surgery and postoperative changes of olfaction, the computed tomography (CT) score, and nasal airway resistance were analyzed. Results A total of 195 ESS procedures were classified into type I (n = 3), type II (n = 17), type III (n = 91), type IV (n = 82), and type V (n = 2). The major phenotypes of type II, III, and IV ESS were paranasal sinus cyst (68%), CRS without nasal polyps (77%), and CRS with nasal polyps (55%), respectively, and the difference was significant. The degree of ESS based on this classification was positively and significantly correlated with the operation time and bleeding amounts. As a whole, olfaction, CT score, and nasal airway resistance were significantly improved after surgery. The degree of improvement was similar between type III and type IV ESS. Conclusion This simple classification for ESS reflected the perioperative burden of the disease.
Reflexiones sobre el impacto del comportamiento mediático en las políticas de seguridad en México
Authors: López de Alba Gómez Alejandra 
Published: October 2017

El presente artículo analiza desde una perspectiva teórica el impacto de la información en el diseño y ejecución de las políticas de seguridad, haciendo hincapié en la situación de México en los últimos años. A efectos de mostrar un panorama más amplio, se enuncian algunos ejemplos internacionales que muestran que la información presentada, a través de los medios de comunicación no puede ser considerada como un fenómeno aislado, sino que ha llegado a convertirse un componente de peso de la toma de decisiones en materia de seguridad.
Para este fin, se propone que las partes involucradas, Estado y medios de comunicación consideren en todo momento que la i nformación en materia de seguridad puede ser parte de operaciones de información, y así aminorar los riesgos de revelar secretos que desvíen las políticas de seguridad, sin menoscabar el derecho a la libertad de expresión y el derecho a la información.
Influence of short-term dietary starch inclusion on the equine cecal microbiome1
Authors: Warzecha C M , Coverdale J A , Janecka J E , Leatherwood J L , Pinchak W E , Wickersham T A , McCann J C 
Published: October 2017

Abstract
The objective of this study was to determine bacterial community profiles of the equine cecum in response to abrupt inclusion of varying levels of dietary starch. Seven cecally cannulated Quarter Horse geldings (497 to 580 kg) were used in a crossover design with two 28-d periods and a 28-d washout between each. Horses were randomly assigned to dietary treatments consisting of a commercial concentrate offered as fed at either 0.6 (low starch [LS]) or 1.2% BW (high starch [HS]) daily that was divided into 2 meals at 12-h intervals. Prior to the start of each period, horses were allowed ad libitum access to coastal bermudagrass (Cynodon dactylon) hay. Concentrate was fed on d 1 with no adaptation. Cecal fluid was collected on d 1 at h 0 and at 3, 6, 9, and 12 h relative to the initial concentrate meal on d 1. Additional samples were collected 6 h after feeding on d 2, 3, and 7 of each period. Cecal contents were used to determine pH and VFA concentrations and extract microbial DNA. The V4 through V6 region of 16S rRNA gene was amplified using PCR and sequenced on the Roche 454 FLX platform. Sequence analysis was performed with QIIME, and data were analyzed using the MIXED procedure of SAS. Cecal pH tended to decrease (P = 0.09) in horses fed HS in the first 12 h after the first concentrate meal and remained lower (P ≤ 0.05) the following 7 d. Total VFA were greater (P ≤ 0.05) in horses fed HS in the initial 12 h and 7 d after addition of concentrate. Species richness determined using the Chao1 index was unchanged (P &gt; 0.20) over the initial 12 h and decreased (P = 0.01) over 7 d for both treatments. Community diversity determined using the Shannon index tended to decrease (P = 0.06) over the 7 d. Relative abundances of Paraprevotellaceae were greater (P ≤ 0.05) in HS in the first 12 h. Over 7 d, relative abundances of Paraprevotellaceae, Veillonellaceae, and Succinivibrionaceae were greater (P ≤ 0.05) in HS compared with LS. Abrupt and short-term exposure to dietary starch does alter cecal fermentation and microbial community structure in horses, but the impact on horse health is unknown.
Corans maghrébins copiés du XIIe au XVIIe siècle. conservés dans les musées et Bibliothèques de France autres que la BnF
Authors: Guesdon Marie-Geneviève 
Published: October 2017

Plusieurs bibliothèques et musées français conservent dans leurs fonds des manuscrits ou des fragments du Coran qui ont été copiés dans l'Occident musulman entre le XIIe et le XVIIe siècle, mais n'ont parfois pas été correctement identifiés. Si on laisse de côté la Bibliothèque nationale de France, sa collection ayant été déjà décrite de manière exhaustive, le présent article rassemble de l'information sur des manuscrits possédant ces caractéristiques, tirée de divers catalogues et bases de données où ils sont décrits. [Various libraries and museums in France have in their holdings Qur'an manuscripts and fragments copied in the Western Islamic World between the twelfth and seventeenth centuries that are sometimes not properly identified. Leaving aside the Bibliothèque nationale de France, since its collection has already been fully described, the present paper collates information about such manuscripts from the various disparate catalogues or databases in which they are described.]
Le prince et la nourrice
Authors: Déroche François 
Published: October 2017

Le manuscrit du Coran dit « de la Nourrice » est l'un des plus célèbres de la collection de Kairouan, maintenant conservée au Musée des arts islamiques de Raqqada. Son origine est exceptionnellement bien connue grâce à un texte qui équivaut à un colophon et donne la date d'achèvement en ramadan 410/janvier 1020—ou légèrement plus tôt. Les dimensions remarquables de cette copie (environ 445x300 mm), sa calligraphie spectaculaire et son enluminure frappent l'imagination. Près de 2000 feuillets ont été préservés et une étude détaillée sera nécessaire pour comprendre cet important épisode de la calligraphie et de l'art du livre dans l'Ifriqiya ziride. Le présent article représente une première étape dans cette direction et montre que différents copistes et/ou enlumineurs ont été impliqués dans la réalisation de cet exemplaire en soixante volumes. Il tente de replacer ce superbe manuscrit dans le contexte de son époque. [The so-called ‘Qur'an of the Nurse’ is one of the most famous manuscripts from the Qayrawān collection, now in the Museum of Islamic arts in Raqqada. Its provenance is exceptionally well documented, with the equivalent of a colophon giving the date of completion in Ramaḍān 410/January 1020 or slightly before. The outstanding size of the copy (c. 445x300 mm), and its dramatic calligraphy and illumination capture the imagination. About 2,000 folios have survived and a full study of the manuscript is required in order to understand this important episode of calligraphy and art of the book in Zirid Ifriqiyya. The present paper is a first step towards this goal and shows that various copyists and/or illuminators have been involved in the production of the sixty-volume set. It tries to put this magnificent manuscript into the context of this period.]
Un concurrent du Coran en Occident musulman du Xe/XVIe à l'aube du XIIe/XVIIIe siècle: les Dalāʾil al-khayrāt d'al-Jazūlī
Authors: Abid Hiba 
Published: October 2017

Près d'un siècle après sa composition, le livre de prières sur le Prophète du mystique marocain al-Jazūlī (m. 869/1465), les Dalāʾil al-Khayrāt, commença à circuler de façon intensive à travers le monde musulman sunnite jusqu'à devenir, très rapidement, le texte religieux le plus copié après le Coran. Au-delà de cette proximité avec le Livre de la révélation, les exemplaires du bréviaire partagent un certain nombre de traits matériels et ornementaux avec les manuscrits coraniques. C'est ce que révèle l'examen de copies produites en Occident musulman entre le Xe/XVIe et le XIIe/XVIIIe siècles, dans lesquelles nous rencontrons des particularités codicologiques ou des formules ornementales jusqu'alors strictement réservées aux Corans maghrébins. Ce mimétisme est très certainement le signe de la révérence et de la sacralité accordées au livre de prières comme le montre par ailleurs la présence, dans certains exemplaires, de texte fournissant des instructions sur la pureté rituelle préalable avant la récitation des prières, similaire à celle que requiert la lecture du Coran. [Nearly a century after it was written by the Moroccan Ṣūfī Sīdī b. Sulaymān al-Jazūlī (d. 869/1465), the book of salutations [on the Prophet Muḥammad] entitled the Dalāʾil al-khayrāt, widely circulated throughout the Muslim Sunnī world. It soon became one of the most copied religious books after the Qur'an. Most importantly, it appears that the Dalāʾil manuscripts share a great amount of material and decorative features with the Qur'an manuscripts. Indeed, examination of copies produced in the Muslim West from the tenth/sixteenth century to the twelfth/eighteenth century reveals that several material characteristics of the manuscripts and their ornamentation closely follow those of Qur'an manuscripts in North Africa. This ‘imitation’ certainly indicates the esteem in which the Dalāʾil was held and the extent to which it was viewed with religious deference in Islamic piety. This is reinforced by some examples of texts appended to a few surviving manuscripts, in which instructions to the reader on attaining ritual purity before reciting or holding the book are provided.]
ALMA Multiple-transition Molecular Line Observations of the Ultraluminous Infrared Galaxy IRAS 20551–4250: Different HCN, HCO+, and HNC Excitation, and Implications for Infrared Radiative Pumping
Authors: Imanishi 今西 Masatoshi 昌俊 , Nakanishi 中西 Kouichiro 康一郎 , Izumi 泉 Takuma 拓磨 
Published: October 2017

Abstract
We present our ALMA multi-transition molecular line observational results for the ultraluminous infrared galaxy IRAS 20551−4250, which is known to contain a luminous buried active galactic nucleus and shows detectable vibrationally excited (v
2 = 1f) HCN and HNC emission lines. The rotational J = 1–0, 4–3, and 8–7 of HCN,

, and HNC emission lines were clearly detected at a vibrational ground level (v = 0). Vibrationally excited (v
2 = 1f) J = 4–3 emission lines were detected for HCN and HNC, but not for

. Their observed flux ratios further support our previously obtained suggestion, based on J = 3–2 data, that (1) infrared radiative pumping plays a role in rotational excitation at v = 0, at least for HCN and HNC, and (2) HCN abundance is higher than

and HNC. The flux measurements of the isotopologue H13CN,

, and HN13C J = 3–2 emission lines support the higher HCN abundance scenario. Based on modeling with collisional excitation, we constrain the physical properties of these line-emitting molecular gases, but find that higher HNC rotational excitation than HCN and

is difficult to explain, due to the higher effective critical density of HNC. We consider the effects of infrared radiative pumping using the available 5–30 μm infrared spectrum and find that our observational results are well-explained if the radiation source is located at 30–100 pc from the molecular gas. The simultaneously covered very bright CO J = 3–2 emission line displays a broad emission wing, which we interpret as being due to molecular outflow activity with the estimated rate of

.
Deep CO(1–0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
Authors: Rudnick Gregory , Hodge Jacqueline , Walter Fabian , Momcheva Ivelina , Tran Kim-Vy , Papovich Casey , da Cunha Elisabete , Decarli Roberto , Saintonge Amelie , Willmer Christopher , Lotz Jennifer , Lentati Lindley 
Published: October 2017

Abstract
We present an extremely deep CO(1–0) observation of a confirmed z = 1.62 galaxy cluster. We detect two spectroscopically confirmed cluster members in CO(1–0) with signal-to-noise ratio

. Both galaxies have log(

/

) > 11 and are gas rich, with

/(

+

) ∼ 0.17–0.45. One of these galaxies lies on the star formation rate (SFR)–

sequence, while the other lies an order of magnitude below. We compare the cluster galaxies to other SFR-selected galaxies with CO measurements and find that they have CO luminosities consistent with expectations given their infrared luminosities. We also find that they have gas fractions and star formation efficiencies (SFE) comparable to what is expected from published field galaxy scaling relations. The galaxies are compact in their stellar light distribution, at the extreme end for all high-redshift star-forming galaxies. However, their SFE is consistent with other field galaxies at comparable compactness. This is similar to two other sources selected in a blind CO survey of the HDF-N. Despite living in a highly quenched protocluster core, the molecular gas properties of these two galaxies, one of which may be in the process of quenching, appear entirely consistent with field scaling relations between the molecular gas content, stellar mass, star formation rate, and redshift. We speculate that these cluster galaxies cannot have any further substantive gas accretion if they are to become members of the dominant passive population in

clusters.
The EDGE–CALIFA Survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
Authors: Utomo Dyas , Bolatto Alberto D. , Wong Tony , Ostriker Eve C. , Blitz Leo , Sanchez Sebastian F. , Colombo Dario , Leroy Adam K. , Cao Yixian , Dannerbauer Helmut , Garcia-Benito Ruben , Husemann Bernd , Kalinova Veselina , Levy Rebecca C. , Mast Damian , Rosolowsky Erik , Vogel Stuart N. 
Published: October 2017

Abstract
We present results from the EDGE survey, a spatially resolved CO(1−0) follow-up to CALIFA, an optical Integral Field Unit survey of local galaxies. By combining the data products of EDGE and CALIFA, we study the variation in molecular gas depletion time (τ
dep) on kiloparsec scales in 52 galaxies. We divide each galaxy into two parts: the center, defined as the region within

, and the disk, defined as the region between 0.1 and

. We find that 14 galaxies show a shorter τ
dep (∼1 Gyr) in the center relative to that in the disk (τ
dep ∼ 2.4 Gyr), which means the central region in those galaxies is more efficient at forming stars per unit molecular gas mass. This finding implies that the centers with shorter τ
dep resemble the intermediate regime between galactic disks and starburst galaxies. Furthermore, the central drop in τ
dep is correlated with a central increase in the stellar surface density, suggesting that a shorter τ
dep is associated with molecular gas compression by the stellar gravitational potential. We argue that varying the CO-to-H2 conversion factor only exaggerates the central drop of τ
dep.
A Face-on Accretion System in High-mass Star Formation: Possible Dusty Infall Streams within 100 AU
Authors: Motogi Kazuhito , Hirota Tomoya , Sorai Kazuo , Yonekura Yoshinori , Sugiyama Koichiro , Honma Mareki , Niinuma Kotaro , Hachisuka Kazuya , Fujisawa Kenta , Walsh Andrew J. 
Published: October 2017

Abstract
We report on interferometric observations of a face-on accretion system around the high-mass young stellar object, G353.273+0.641. The innermost accretion system of 100 au radius was resolved in a 45 GHz continuum image taken with the Jansky-Very Large Array. Our spectral energy distribution analysis indicated that the continuum could be explained by optically thick dust emission. The total mass of the dusty system is ∼0.2 M
☉ at minimum and up to a few M
☉ depending on the dust parameters. 6.7 GHz CH3OH masers associated with the same system were also observed with the Australia Telescope Compact Array. The masers showed a spiral-like, non-axisymmetric distribution with a systematic velocity gradient. The line-of-sight velocity field is explained by an infall motion along a parabolic streamline that falls onto the equatorial plane of the face-on system. The streamline is quasi-radial and reaches the equatorial plane at a radius of 16 au. This is clearly smaller than that of typical accretion disks in high-mass star formation, indicating that the initial angular momentum was very small, or the CH3OH masers selectively trace accreting material that has small angular momentum. In the former case, the initial specific angular momentum is estimated to be 8 × 1020 (

M
☉)

cm2 s−1, or a significant fraction of the initial angular momentum was removed outside of 100 au. The physical origin of such a streamline is still an open question and will be constrained by the higher-resolution (∼10 mas) thermal continuum and line observations with ALMA long baselines.
Probing the Metal Enrichment of the Intergalactic Medium at z = 5–6 Using the Hubble Space Telescope
Authors: Cai Zheng , Fan Xiaohui , Dave Romeel , Finlator Kristian , Oppenheimer Ben 
Published: October 2017

Abstract
We test the galactic outflow model by probing associated galaxies of four strong intergalactic C iv absorbers at z = 5–6 using the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) ramp narrowband filters. The four strong C iv absorbers reside at z = 5.74, 5.52, 4.95, and 4.87, with column densities ranging from N
C iv
= 1013.8 to 1014.8 cm−2. At z = 5.74, we detect an i-dropout Lyα emitter (LAE) candidate with a projected impact parameter of 42 physical kpc from the C iv absorber. This LAE candidate has a Lyα-based star formation rate (SFRLyα
) of 2 M
⊙ yr−1 and a UV-based SFR of 4 M
⊙ yr−1. Although we cannot completely rule out that this i-dropout emitter may be an [O ii] interloper, its measured properties are consistent with the C iv powered galaxy at z = 5.74. For C iv absorbers at z = 4.95 and z = 4.87, although we detect two LAE candidates with impact parameters of 160 and 200 kpc, such distances are larger than that predicted from the simulations. Therefore, we treat them as nondetections. For the system at z = 5.52, we do not detect LAE candidates, placing a 3σ upper limit of SFRLyα
≈ 1.5 M
⊙ yr−1. In summary, in these four cases, we only detect one plausible C iv source at z = 5.74. Combining the modest SFR of the one detection and the three nondetections, our HST observations strongly support that smaller galaxies (SFRLyα
≲ 2 M
⊙ yr−1) are main sources of intergalactic C iv absorbers, and such small galaxies play a major role in the metal enrichment of the intergalactic medium at z ≳ 5.