cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Retinal dynamic vascular biomarkers of arterial stiffness
Creators: name: Rezaeian, Mahdieh
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Arterial stiffness is an independent predictor of cardiovascular events. Cardiovascular diseases have been the leading causes of mortality across the globe over the past 15 years. There is a growing recognition of the links between small and large vessels impairment in arterial stiffness. However, fundamental aspects of small-artery stiffness are poorly understood and need further research. Retinal microvasculature provides direct access to the microcirculation easily and non-invasively. Previous studies suggest microvascular remodelling occurs in association with arterial stiffness. Assuming retinal vessels display the same changes seen in other small resistance arteries, they should also undergo structural changes in response to arterial stiffness. The current research investigates whether dynamic characteristics of retinal vessels including pulsatility and arterial pulse transit time derived from diameter waveforms are associated with large artery stiffening. This thesis presents a novel method for the measurement of pulsatile diameter changes both in the human and rat retinal vessels. Experimental studies in rats demonstrated retinal arteriolar narrowing and reduced arterial pulse amplitude in presence of hypertension. In addition, a strong positive correlation was found between pulse wave velocity in retinal arteries and increasing blood pressure. These observations are in accordance with known vasoconstriction-induced inward remodelling of resistance vessels and pressure dependence of arterial stiffness as suggested from previous studies in large arteries. Furthermore, a clinical study on a group of elderly volunteers showed a strong positive linear relationship between pulse wave velocity in retinal arteries and pulse wave velocity measured between carotid and femoral arteries as the gold-standard clinical marker of arterial stiffness, for the first time. Moreover, in the identification of the theoretical value of the pulse wave velocity in retinal arteries, an in-vitro experiment was conducted to measure the elastic modulus of the retinal arteries for the first time and a wave speed in order of cm/s was estimated which is two orders of magnitude slower than pulse wave velocity in large arteries. Investigation of dynamic characteristics of retinal vessels may help to provide insights into the pathophysiology and development of stiffness in small arteries. It can also help in possible therapeutic strategies not only in hypertension and arterial stiffness but also in a range of ocular and vascular-related pathogenesis.
CMB-induced radio quenching of high-redshift jetted AGNs with highly magnetic hotspots
Creators: name: Wu, Jianfeng
name: Ghisellini, Gabriele
name: Hodges-Kluck, Edmund
name: Gallo, Elena
name: Ciardi, Benedetta
name: Haardt, Francesco
name: Sbarrato, Tullia
name: Tavecchio, Fabrizio
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In an effort to understand the cause of the apparent depletion in the number density of radio-loud AGNs at $z>3$, this work investigates the viability of the so-called Cosmic Microwave Background (CMB) quenching mechanism of intrinsically jetted, high-z AGNs, whereby Inverse Compton scattering of CMB photons off electrons within the extended lobes results in a substantial dimming of the lobe synchrotron emission at GHz frequencies, while simultaneously boosting their diffuse X-ray signal. We focus on five $z>3.5$ radio galaxies that have sufficiently deep Chandra exposure (> 50 ks) to warrant a meaningful investigation of any extended X-ray emission. For those objects with evidence for statistically significant extended X-ray lobes (4C 41.17 and 4C 03.24), we combine the Chandra measurements with literature data at lower frequencies to assemble the systems' Spectral Energy Distributions (SEDs), and utilize state-of-the-art SED modelling (Ghisellini et al. 2015) -- including emission from the disk, torus, jet, hotspots, and lobes -- to infer their physical parameters. For both radio galaxies, the magnetic energy density in the hotspots is found to exceed the energy density in CMB photons, wheres the opposite is true for the lobes. This implies that any extended synchrotron emission likely originates from the hotspots themselves, rather than the lobes. Conversely, Inverse Compton scattering of CMB photons dominates the extended X-ray emission from the lobes, which are effectively "radio-quenched". As a result, CMB quenching is effective in these systems in spite of the fact that the observed X-ray to radio luminosity ratio does not bear the signature $(1+z)^4$ dependence of the CMB energy density.
description: MNRAS in press; 17 pages, 8 figures, 4 tables
Additional file 1 of Hollow polydopamine nanoparticles loading with peptide RL-QN15: a new pro-regenerative therapeutic agent for skin wounds
Creators: name: Sun, Huiling
name: Wang, Ying
name: He, Tiantian
name: He, Dingwei
name: Hu, Yan
name: Fu, Zhe
name: Wang, Yinglei
name: Sun, Dandan
name: Wang, Junsong
name: Liu, Yixiang
name: Shu, Longjun
name: He, Li
name: Deng, Ziwei
name: Yang, Xinwang
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1: Table S1. Surface areas, pore diameter and pore volume of HPDA nanoparticles. Figure S1. Biodistribution and clearance of HPDA and HPDAlR.
Exploring teacher perspectives on the relationship between teacher-student interactions and the classroom engagement of students with behavioural difficulties
Creators: name: Good, Phillip
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: This research employed a qualitative design to examine two dimensions of teachers’ experiences with students presenting with challenging behaviours: teachers-student interaction, and classroom engagement. A total of 15 teachers from three Catholic schools were involved in the study, five teachers from each participating school. The three schools included: (1) a coeducational primary school; (2) a mainstream secondary school for boys; and (3) a special behavioural secondary school for boys. The study employed one-on-one semi-structured teacher interviews. Teachers’ own classroom experiences, along with their perceptions of the impact of the wider school context on outcomes for students with behavioural difficulties, were examined. An Interpretive Phenomenological Analysis (IPA) approach was used in the analysis of interview data. Findings: A narrative of caring for the wellbeing of students with challenging behaviour was embedded in the interview data from all fifteen teachers. The teachers reported the complexity of student behavioural challenges and factors that inhibited positive teacher-student interaction and relationships, as well as consequences for not meeting school expectations. However, developing caring and positive relationships with students - giving them a voice, providing students with clear expectations, rules and boundaries – was seen as key to the formation of positive teacher-student interactions, positive student classroom engagement, and an optimal environment for learning. Limitations: This research was limited by the relatively small participant numbers, and it may be that the emphasis on caring reflected a philosophical approach emphasised and reinforced within the Catholic school system.
Additional file 1: Figure S1. of Targeting the cross-talk between Urokinase receptor and Formyl peptide receptor type 1 to prevent invasion and trans-endothelial migration of melanoma cells
Creators: name: Ragone, Concetta
name: Minopoli, Michele
name: Ingangi, Vincenzo
name: Botti, Giovanni
name: Fratangelo, Federica
name: Pessi, Antonello
name: Stoppelli, Maria
name: Ascierto, Paolo
name: Ciliberto, Gennaro
name: Motti, Maria
name: Carriero, Maria
Publisher: name: figshare
Year: 2017
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Uncropped images of immunoblots. Full blots from Fig. 1b, Inset of the Fig. 2a, c, Fig. 4b, and Fig. 7a. (PDF 164Â kb)
Steep Decay Phase Shaped by the Curvature Effect. II. Spectral Evolution
Creators: name: Lin, Da-Bin
name: Mu, Hui-Jun
name: Liang, Yun-Feng
name: Liu, Tong
name: Gu, Wei-Min
name: Lu, Rui-Jing
name: Wang, Xiang-Gao
name: Liang, En-Wei
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We derive a simple analytical formula to describe the evolution of spectral index $β$ in the steep decay phase shaped by the curvature effect with assumption that the spectral parameters and Lorentz factor of jet shell is the same for different latitude. Here, the value of $β$ is estimated in 0.3$-$10keV energy band. For a spherical thin shell with a cutoff power law (CPL) intrinsic radiation spectrum, the spectral evolution can be read as a linear function of observer time. For the situation with Band function intrinsic radiation spectrum, the spectral evolution may be complex. If the observed break energy of radiation spectrum is larger than 10keV, the spectral evolution is the same as that shaped by jet shells with a CPL spectrum. If the observed break energy is less than 0.3keV, the value of $β$ would be a constant. Others, the spectral evolution can be approximated as a logarithmal function of the observer time in generally.
description: 24 pages, 13 figures, accepted for publication in ApJ
Exactly solved mixed spin-(1,1/2) Ising-Heisenberg distorted diamond chain
Creators: name: Lisnyi, Bohdan
name: Strecka, Jozef
Publisher: name: arXiv
Year: 2016
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The mixed spin-(1,1/2) Ising-Heisenberg model on a distorted diamond chain with the spin-1 nodal atoms and the spin-1/2 interstitial atoms is exactly solved by the transfer-matrix method. An influence of the geometric spin frustration and the parallelogram distortion on the ground state, magnetization, susceptibility and specific heat of the mixed-spin Ising-Heisenberg distorted diamond chain are investigated in detail. It is demonstrated that the zero-temperature magnetization curve may involve intermediate plateaus just at zero and one-half of the saturation magnetization. The temperature dependence of the specific heat may have up to three distinct peaks at zero magnetic field and up to four distinct peaks at a non-zero magnetic field. The origin of multipeak thermal behavior of the specific heat is comprehensively studied.
description: 15 pages, 10 figures
title: Дискретная математика
title: Учебное пособие
titleType: Subtitle
Creators: name: Хусаинов А.А.
Publisher: name: Амурский гуманитарно-педагогический государственный университет, Ай Пи Ар Медиа
Year: 2019

description: В учебном пособии даны основы дискретной математики: конечные множества и отношения, комбинаторный анализ, производящие функции и рекуррентные соотношения, деревья, хроматические функции графов, а также функции Мебиуса на конечных частично упорядоченных множествах. Учебное пособие предназначено для студентов, обучающихся по направлениям подготовки 01.03.01 «Математика», 01.03.02 «Прикладная математика и информатика», 38.03.05 «Бизнес-информатика» и изучающих дисциплину «Дискретная математика». Также будет полезно студентам других специальностей и направлений подготовки.
Additional file 1: of Validity of mobile electronic data capture in clinical studies: a pilot study in a pediatric population
Creators: name: NiederhĂ¤Usern, Belinda Von
name: Saccilotto, Ramon
name: SchĂ¤Delin, Sabine
name: Ziesenitz, Victoria
name: Benkert, Pascal
name: Marie-Luise Decker
name: Hammann, Anya
name: Bielicki, Julia
name: Pfister, Marc
name: Pauli-Magnus, Christiane
Publisher: name: figshare
Year: 2017
Subjects: subject: Space Science
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Development of mobile application. (PDF 74Â kb)
BTAS: A Library for Tropical Algebra
Creators: name: Humayun, Ahsan
name: Asif, Dr. Muhammad
name: Hanif, Dr. Muhammmad Kashif
Publisher: name: arXiv
Year: 2017
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: GPUs are dedicated processors used for complex calculations and simulations and they can be effectively used for tropical algebra computations. Tropical algebra is based on max-plus algebra and min-plus algebra. In this paper we proposed and designed a library based on Tropical Algebra which is used to provide standard vector and matrix operations namely Basic Tropical Algebra Subroutines (BTAS). The testing of BTAS library is conducted by implementing the sequential version of Floyd Warshall Algorithm on CPU and furthermore parallel version on GPU. The developed library for tropical algebra delivered extensively better results on a less expensive GPU as compared to the same on CPU.
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 181 (11 H 754), 165 folios, f. 0055
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0055, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0055, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 2: Table S2. of Historical isolation and contemporary gene flow drive population diversity of the brown alga Sargassum thunbergii along the coast of China
Creators: name: Li, Jing-Jing
name: Hu, Zi-Min
name: Sun, Zhong-Min
name: Yao, Jian-Ting
name: Liu, Fu-Li
name: Fresia, Pablo
name: Duan, De-Lin
Publisher: name: figshare
Year: 2017
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Sequences of 7 rbc spacer haplotypes and primers of 11 microsatellite markers. (DOCX 15 kb)
Additional file 1 of Barriers to medication adherence in a rural-urban dual economy: a multi-stakeholder qualitative study
Creators: name: Xu, Jacqueline
name: Zhao, Mengxi
name: Vrosgou, Athina
name: Yu, Natalie Chin Wen
name: Liu, Chelsea
name: Zhang, Han
name: Ding, Chunxi
name: Roth, Noelle Wyman
name: Pan, Yuesong
name: Liu, Liping
name: Wang, Yilong
name: Wang, Yongjun
name: Bettger, Janet Prvu
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1. Interview Guide.
The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
Creators: name: Danieli, Shany
name: van Dokkum, Pieter
name: Merritt, Allison
name: Abraham, Roberto
name: Zhang, Jielai
name: Karachentsev, I. D.
name: Makarova, L. N.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We obtained follow-up HST observations of the seven low surface brightness galaxies discovered with the Dragonfly Telephoto Array in the field of the massive spiral galaxy M101. Out of the seven galaxies, only three were resolved into stars and are potentially associated with the M101 group at $D=7\text{ Mpc}$. Based on HST ACS photometry in the broad F606W and F814W filters, we use a maximum likelihood algorithm to locate the Tip of the Red Giant Branch (TRGB) in galaxy color-magnitude diagrams. Distances are $6.38^{+0.35}_{-0.35}, 6.87^{+0.21}_{-0.30}$ and $6.52^{+0.25}_{-0.27} \text{ Mpc}$ and we confirm that they are members of the M101 group. Combining the three confirmed low luminosity satellites with previous results for brighter group members, we find the M101 galaxy group to be a sparsely populated galaxy group consisting of seven group members, down to $M_V = -9.2 \text{ mag}$. We compare the M101 cumulative luminosity function to that of the Milky Way and M31. We find that they are remarkably similar; In fact, the cumulative luminosity function of the M101 group gets even flatter for fainter magnitudes, and we show that the M101 group might exhibit the two known small-scale flaws in the $Λ\textrm{CDM}$ model, namely `the missing satellite' problem and the `too big to fail' problem. Kinematic measurements of M101$'$s satellite galaxies are required to determine whether the `too big to fail' problem does in fact exist in the M101 group.
description: Accepted for publication in ApJ
Integrated magnetics: contributions to improved processing and interpretation of magnetic gradient tensor data, new methods for source location and estimation of magnetisation, and predictive magnetic exploration models
Creators: name: Clark, David Alan
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: This thesis presents methods for processing and interpreting magnetic gradient tensor data, new approaches to estimation of source magnetisations from analysis of magnetic anomalies, and improved geological interpretation of magnetic surveys using magnetic petrological principles and predictive magnetic exploration models. The thesis emphasises the importance of an approach that integrates an understanding of the geological processes that create and destroy magnetic minerals with extra information obtained from magnetic gradient tensor data, and with petrophysical and palaeomagnetic information, to derive better geological models and to improve exploration success.
Quantum Speed Limit for Change of Basis
Creators: name: Naseri, Moein
name: Macchiavello, Chiara
name: Bruß, Dagmar
name: Horodecki, Paweł
name: Streltsov, Alexander
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum speed limits provide ultimate bounds on the time required to transform one quantum state into another. Here, we extend the notion of quantum speed limits to collections of quantum states, investigating the time for converting a basis of states into an unbiased one. We provide tight bounds for systems of dimension smaller than 5, and general bounds for multi-qubit systems and Hilbert space dimension $d$. For two-qubit systems, we show that the fastest transformation implements two Hadamards and a swap of the qubits simultaneously. We further prove that for qutrit systems the evolution time depends on the particular type of the unbiased basis. We also investigate speed limits for coherence generation, providing the minimal time to establish a certain amount of coherence with a unitary evolution.
description: 13 pages, 2 figures
Additional file 2: of Medical overuse and quaternary prevention in primary care â A qualitative study with general practitioners
Creators: name: Alber, Kathrin
name: Kuehlein, Thomas
name: Schedlbauer, Angela
name: Schaffer, Susann
Publisher: name: figshare
Year: 2017
Subjects: subject: Medicine
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 60506 Virology

description: Timeline/Mapping â Evidence-based medicine and guidelines. (PDF 1486 kb)
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 685
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 685, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 685, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
CHIME FRB: An application of FFT beamforming for a radio telescope
Creators: name: Ng, C.
name: Vanderlinde, K.
name: Paradise, A.
name: Klages, P.
name: Masui, K.
name: Smith, K.
name: Bandura, K.
name: Boyle, P. J.
name: Dobbs, M.
name: Kaspi, V.
name: Renard, A.
name: Shaw, J. R.
name: Stairs, I.
name: Tretyakov, I.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have developed FFT beamforming techniques for the CHIME radio telescope, to search for and localize the astrophysical signals from Fast Radio Bursts (FRBs) over a large instantaneous field-of-view (FOV) while maintaining the full angular resolution of CHIME. We implement a hybrid beamforming pipeline in a GPU correlator, synthesizing 256 FFT-formed beams in the North-South direction by four formed beams along East-West via exact phasing, tiling a sky area of ~250 square degrees. A zero-padding approximation is employed to improve chromatic beam alignment across the wide bandwidth of 400 to 800 MHz. We up-channelize the data in order to achieve fine spectral resolution of $Δν$=24 kHz and time cadence of 0.983 ms, desirable for detecting transient and dispersed signals such as those from FRBs.
description: 4 pages, 3 figures, submitted to the XXXII International Union of Radio Science General Assembly & Scientific Symposium (URSI GASS) 2017
Potential roles of serum ATPase and AMPase in predicting diagnosis of colorectal cancer patients
Creators: name: Shi, Mengchen
name: Tian, Yu
name: He, Lingyuan
name: Zhang, Jingdan
name: Yang, Xiangling
name: Liu, Huanliang
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Colorectal cancer (CRC) is a common gastrointestinal cancer with high incidence and mortality rates. CRC may be associated with regulation of circulating nucleotides. This study aimed to evaluate the serum levels of nucleotide-metabolizing enzymes (ATPase and AMPase) in patients with CRC and to explore the clinical diagnostic value of these enzymes. The gene set variation analysis (GSVA) score of the ATP-adenosine signature was calculated using tumor samples from The Cancer Genome Atlas (TCGA). ATP-adenosine signaling plays a central role in CRC progression. A total of 135 subjects, including 87 patients with CRC and 48 healthy controls, were included. The serum levels of ATPase and AMPase in the CRC group were significantly higher than those in the control group (P < 0.05). Furthermore, ATP and AMP hydrolysis levels significantly increased in the advanced CRC group (P < 0.05). ATP and AMP hydrolysis was decreased by the ENTPDase inhibitors (POM-1 and ARL67156) and CD73 inhibitor (APCP). The sensitivities of ATPase and AMPase were 95.4% and 75.9%, respectively, which were higher than those of CEA (67.8%) and CA19-9 (72.4%). The specificities of ATPase and AMPase were 69.9% and 73.9%, respectively, which were higher than that of CA19-9 (47.8%). The combination of CEA, ATPase, and AMPase demonstrated high sensitivity (92.0%) and specificity (87.0%). Collectively, ATPase and AMPase activities are upregulated in CRC with considerable diagnostic significance. The combination of CEA, ATPase, and AMPase may provide a novel approach for CRC screening.
Additional file 1 of Phosphorylation of NF-κBp65 drives inflammation-mediated hepatocellular carcinogenesis and is a novel therapeutic target
Creators: name: Xu, Xuan
name: Lei, Yiming
name: Chen, Lingjun
name: Zhou, Haoxiong
name: Liu, Huiling
name: Jiang, Jie
name: Yang, Yidong
name: Wu, Bin
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Figure S1. Deficiency of hepatocytes p65 attenuated hepatocellular carcinogenesis in mice. (a) AFP levels of WT and L-p65-KO mice. (b) Quantification of average liver weight versus body weight in WT and L-p65-KO mice. (c) Maximal size of liver tumors measured by a caliper. (d) Average tumor numbers at 9 months. All values are mean ± SD (n = 10 for each group). P < 0.05 by using Student’s t-test.
Testing spatial models of genetic connectivity for European Raja clavata and Sepia officinalis in response to seascape resistance
Creators: name: Luland, Holly
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Predicting influences of habitat distribution and heterogeneity on species gene flow is now widely acknowledged as a key step in optimising effective marine management practices. Commonly applied models of geographic influence such as isolation by distance (IBD) and isolation by oceanic distances (IBO), though often effective at predicting the genetic connectivity of pelagic species, fail to incorporate potential influences of habitat by single corridor or multiple corridors on the genetic and movement connectivity for non-pelagic and demersal-obligate species, as found on continental shelf systems. Least-cost path (LCP) and isolation by resistance (IBR); a novel approach based on Circuit Theory principles of random walk, counters these limitations by integrating the effects of single and multiple pathways on connectivity by distances taken between locations over habitat shapes of assigned resistances optimised a priori. Applications of these models have been largely restricted to terrestrial systems despite the potential for improving predictions of connectivity for marine habitat specialists. Using available genetic, distribution and habitat data from two co-distributed and predominately demersal species Sepia officinalis and Raja clavata, we were able to identify that IBO explained the connectivity of R. clavata while S. officinalis connectivity was influenced by IBR and the LCP by habitat configuration. With this study we provide a simple framework for developing tests of genetic connectivity that indicate some of the processes underpinning patterns of genetic structure.
Additional file 1: Table S1. of Historical isolation and contemporary gene flow drive population diversity of the brown alga Sargassum thunbergii along the coast of China
Creators: name: Li, Jing-Jing
name: Hu, Zi-Min
name: Sun, Zhong-Min
name: Yao, Jian-Ting
name: Liu, Fu-Li
name: Fresia, Pablo
name: Duan, De-Lin
Publisher: name: figshare
Year: 2017
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Sampling locality, code, coordinates, sample size and RuBisCo spacer (rbc spacer) haplotype distribution in each Sargassum thunbergii population. (DOCX 15 kb)
Anyon condensation and confinement transition in a Kitaev spin liquid bilayer
Creators: name: Hwang, Kyusung
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Transitions between quantum spin liquids (QSLs) are fundamental problems lying beyond the Landau paradigm and requiring a deep understanding of the entanglement structures of QSLs called topological orders. The novel concept of anyon condensation has been proposed as a theoretical mechanism, predicting various possible transitions between topological orders, but it has long been elusive to confirm the mechanism in quantum spin systems. Here, we introduce a concrete spin model that incarnates the mechanism of anyon condensation transition. Our model harbors two topological QSLs in different parameter regions, a non-abelian Kitaev spin liquid (KSL) bilayer state and a resonating valence bond (RVB) state. The bilayer-KSL-to-RVB transition indeed occurs by the mechanism of anyon condensation, which we identify by using parton theories and exact diagonalization studies. Moreover, we observe "anyon confinement" phenomena in our numerical results, akin to the quark confinement in high energy physics. Namely, non-abelian Ising anyons of the bilayer KSL are confined in the transition to the RVB state. Implications and extensions of this study are discussed in various aspects such as (i) anyon-condensed multilayer construction of the Kitaev's sixteenfold way of anyon theories, (ii) additional vison condensation transition from the RVB to a valence bond solid (VBS) in the Kitaev bilayer system, (iii) dynamical anyon condensation in a non-Hermitian Kitaev bilayer, (iv) generalizations of our model to other lattice geometries, and (v) experimental realizations. This work puts together the two fascinating QSLs that are extensively studied in modern condensed matter and quantum physics into a concrete spin model, offering a comprehensive picture that unifies the anyon physics of the Kitaev spin liquids and the resonating valence bonds.
description: 21 pages, 13 figures, 3 tables
Farnesane sesquiterpenoids from Rubus delavayi and their anti-Trichinella spiralis activities
Creators: name: Hao, Yi
name: Luo, Xiao-Lei
name: Wang, Min
name: Liu, Rong
name: Zhang, Wei
name: Xiao, Chao-Jiang
name: Jiang, Bei
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Biochemistry
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Two new farnesane sesquiterpenoid glycosides, rubusdelosides A and B (1 and 4), together with five known farnesane sesquiterpenoids (2, 3, and 5-7), and two known meroterpenoids (8 and 9), were isolated from water extract of the herbs of R. delavayi. Their structures were identified by the comprehensive analyses of physicochemical properties and spectroscopic data (NMR and HR-ESI-MS). Compounds 1-8 showed moderate in vivo anti-T. spiralis activities.
Ambitwistor superstring in the Green-Schwarz formulation
Creators: name: Chandia, Osvaldo
name: Vallilo, Brenno Carlini
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we construct the ambitwistor superstring in the Green-Schwarz formulation. The model is obtained from the related pure spinor version. We show that the spectrum contains only ten dimensional supergravity and that kappa symmetry in a curved background implies some of the standard constraints.
description: Latex, 12 pages. Minor changes
Additional file 1: of Medical overuse and quaternary prevention in primary care â A qualitative study with general practitioners
Creators: name: Alber, Kathrin
name: Kuehlein, Thomas
name: Schedlbauer, Angela
name: Schaffer, Susann
Publisher: name: figshare
Year: 2017
Subjects: subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Interview guide â Medical overuse and quaternary prevention in primary care. (PDF 286 kb)
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00315
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00315, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
The Oblique Orbit of WASP-107b from K2 Photometry
Creators: name: Dai, Fei
name: Winn, Joshua N.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Observations of nine transits of WASP-107 during the {\it K2} mission reveal three separate occasions when the planet crossed in front of a starspot. The data confirm the stellar rotation period to be 17 days --- approximately three times the planet's orbital period --- and suggest that large spots persist for at least one full rotation. If the star had a low obliquity, at least two additional spot crossings should have been observed. They were not observed, giving evidence for a high obliquity. We use a simple geometric model to show that the obliquity is likely in the range 40-140$^\circ$, i.e., both spin-orbit alignment and anti-alignment can be ruled out. WASP-107 thereby joins the small collection of relatively low-mass stars hosting a giant planet with a high obliquity. Most such stars have been observed to have low obliquities; all the exceptions, including WASP-107, involve planets with relatively wide orbits ("warm Jupiters", with $a_{\rm min}/R_\star \gtrsim 8$). This demonstrates a connection between stellar obliquity and planet properties, in contradiction to some theories for obliquity excitation.
description: Submitted to AAS journals
Characterizing the Population of Bright Infrared Sources in the Small Magellanic Cloud
Creators: name: Kraemer, K. E.
name: Sloan, G. C.
name: Wood, P. R.
name: Jones, O. C.
name: Egan, M. P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We used Spitzer's Infrared Spectrograph (IRS) to observe stars in the Small Magellanic Cloud (SMC) selected from the Midcourse Space Experiment (MSX) Point Source Catalog. We concentrate on the dust properties of oxygen-rich evolved stars, which show less alumina than Galactic stars. This difference may arise from the SMC's lower metallicity, but it could be a selection effect: the SMC sample includes more stars which are brighter and thus more massive. The distribution of SMC stars along the silicate sequence looks more like that of Galactic red supergiants than asymptotic giant branch stars (AGBs). While many are definitively AGBs, several SMC stars show evidence of hot bottom burning. Other sources show mixed chemistry (oxygen-rich and carbon-rich features), including supergiants with PAH emission. MSX SMC 134 may be the first confirmed silicate/carbon star in the SMC, and MSX SMC 049 is a post-AGB candidate. MSX SMC 145, previously a candidate OH/IR star, is actually an AGB star with a background galaxy at z=0.16 along the same line-of-sight. We consider the overall characteristics of all the {\em MSX} sources, the most infrared-bright objects in the SMC, in light of {\em Spitzer}'s higher sensitivity and resolution, and compare them with the object types expected from the original selection criteria. This population represents what will be seen in more distant galaxies by the James Webb Space Telescope (JWST). Color-color diagrams using the IRS spectra and JWST mid-infrared filters show how one can separate evolved stars from young stellar objects (YSOs) and distinguish among different YSO classes.
description: Accepted for publication in ApJ
Strange stars in $f(R)$ theories of gravity in the Palatini formalism
Creators: name: Panotopoulos, Grigoris
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In the present work we study strange stars in $f(R)$ theories of gravity in the Palatini formalism. We consider two concrete well-known cases, namely the $R+R^2/(6 M^2)$ model as well as the $R-μ^4/R$ model for two different values of the mass parameter $M$ or $μ$. We integrate the modified Tolman-Oppenheimer-Volkoff equations numerically, and we show the mass-radius diagram for each model separately. The standard case corresponding to the General Relativity is also shown in the same figure for comparison. Our numerical results show that the interior solution can be vastly different depending on the model and/or the value of the parameter of each model. In addition, our findings imply that i) for the cosmologically interesting values of the mass scales $M,μ$ the effect of modified gravity on strange stars is negligible, while ii) for the values predicting an observable effect, the modified gravity models discussed here would be ruled out by their cosmological effects.
description: 10 pages, 2 figures
Constraints on the location of the gamma-ray emission region for the gamma-ray-loud radio source GB 1310+487
Creators: name: Kang, Shiju
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We employ a single-zone leptonic jet model, with synchrotron, synchrotron self-Compton (SSC) and external Compton (EC) process, to reproduce the quasi-simultaneous multi-wavelength spectral energy distributions in active and quiescent states of the narrow-line gamma-ray-loud radio source GB 1310+487. In the case of the EC process, the external seed photons from both broad line region (BLR) and dust torus are considered by assuming that the gamma-ray emission region is located at the outside boundary of the BLR and inside the dust torus. Comparing the energy density of external photon fields $U_{\rm BLR}$ obtained by model fitting with that constrained from the BLR observations. We find that the location of the gamma-ray emitting region of GB 1310+487 can be tightly constrained at the outer edge of the BLR (the dissipation distance of the $γ$-ray emission region from central black hole $r_{\rm diss} \sim {\rm~a~few~times~of}~R_{\rm BLR}$). The ratio of magnetic energy and emitting-electron energy in the radiation blob ($ε_{B}=L_{B}/L_{\rm e}$) is gradually increased from Flare 1, Flare 2 to Post-Flare, where the magnetic energy increase and matter energy decrease. These results suggest that the conversion of the magnetic field and the matter (radiation electrons) energy and the location of the $γ$-ray emission region (or ambient photon field) may play an important role in different radiation states of GB 1310+487.
description: Accepted for publication in ApJ. 9 pages, 1 figure, 1 table. arXiv admin note: text overlap with arXiv:1606.00438
Additional file 1: of The role of isolation on contrasting phylogeographic patterns in two cave crustaceans
Creators: name: PĂŠrez-Moreno, Jorge
name: BalĂĄzs, Gergely
name: Wilkins, Blake
name: GĂĄbor Herczeg
name: Bracken-Grissom, Heather
Publisher: name: figshare
Year: 2017
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Additional tables with information regarding evolutionary models selected for phylogenetic analyses, the genetic loci sequence and primers employed, accession numbers for data deposited in GenBank, and Genealogical Sorting Index estimates for all populations of Asellus aquaticus and Niphargus hrabei. (DOCX 56 kb)
Modelling short term equilibrium and long term change in a natural way
Creators: name: McLeod, Doug
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Why would an agent produce and supply something if it got nothing in return? In order to investigate how complex systems, such as biological and economic systems, organize themselves, McLeod (2015) constructs a simple economic model for a biological system. In the context of a dimension model, it was shown that if exchange of resources between creatures is based on relative scarcity, we get a similar outcome to that produced by a market economy, even though such exchanges are not reciprocal. Specifically the ‘biological economy’ constructed in McLeod (2015) promotes the development of specialization and interdependence, and the number of creatures increases over time. These may be construed as large scale, or system, trends. The work presented in this thesis extends McLeod (2015). It develops a multi–sector general equilibrium model of an economy in which resource-based processes are modelled, in order to understand evolution from an economic perspective. The model is based on habitual behaviour represented by Markov chains. It applies particularly, but not exclusively, to biological systems and to pre–market human economies. Interestingly, the interplay between producers of scarce resources and consumers of those resources generates various kinds of agent number and system trajectories. These range from expanding to collapsing and oscillating to stable, depending on the ‘efficiency’ of the agents. Such dynamics occur even though we do not assume any explicit law of motion, objective function, or maximisation principle. The model demonstrates that: (̧ ‘–) mutation/learning will cause a progressive increase in the specialization, interdependence and size of the economy; and (̧ ‘–̧ ‘–) a path dependent outcome is possible. Overall, the work contributes to our economic understanding of systems by grounding the dynamics of those systems in the cut and thrust of evolutionary competition, rather than in the more aloof view of agent behaviour suggested by abstract optimization economics.
Additional file 1 of A novel homozygous variant of COL2A1 in a Chinese male with type II collagenopathy: a case report
Creators: name: Zhang, Qianwen
name: Yao, Ruen
name: Li, Qun
name: Li, Xin
name: Feng, Biyun
name: Chang, Guoying
name: Wang, Jian
name: Wang, Xiumin
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Variants filtering processes . Table S2. Significant variants found in the patient. Table S3. Clinical manifestations of patients with type II collagenopathies with homozygous mutations in different domains. Figure S1. Radiographs of the proband’s father. A, B. The cervical spine. C, D. The thoracic spine. F. The right pelvis. E, G. The lumbar spine. Figure S2. Radiographs of the proband’s mother. A, B. The Tervical spine. C, D. The thoracic spine. E, F. The right knee. G, H. The lumbar spine. Figure S3. Radiographs of the proband’s brother. A, B. The cervical spine. C, D. The thoracic and lumbar spine. E, F. The right knee.
title: История
title: Учебно-методическое пособие
titleType: Subtitle
Creators: name: Баранникова Н.В.
Publisher: name: Амурский гуманитарно-педагогический государственный университет, Ай Пи Ар Медиа
Year: 2019

description: Учебно-методическое пособие «История» адаптировано для изучения дисциплины с использованием дистанционных образовательных технологий. Помимо теоретического материала включает вопросы для самоконтроля, творческие задания. Предназначено для изучения дисциплины «История» по направлению подготовки высшего образования 44.03.01 «Педагогическое образование». Кроме того, учебно-методическое пособие будет полезно студентам других специальностей и направлений, изучающих данную дисциплину.