cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Topological Mott Insulators
Creators: name: Raghu, S.
name: Qi, Xiao-Liang
name: Honerkamp, C.
name: Zhang, Shou-Cheng
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider extended Hubbard models with repulsive interactions on a Honeycomb lattice and the transitions from the semi-metal phase at half-filling to Mott insulating phases. In particular, due to the frustrating nature of the second-neighbor repulsive interactions, topological Mott phases displaying the quantum Hall and the quantum spin Hall effects are found for spinless and spinful fermion models, respectively. We present the mean-field phase diagram and consider the effects of fluctuations within the random phase approximation (RPA). Functional renormalization group analysis also show that these states can be favored over the topologically trivial Mott insulating states.
description: 5 Pages, 4 figures
Additional file 1 of Association of dyslipidemia with the severity and mortality of coronavirus disease 2019 (COVID-19): a meta-analysis
Creators: name: Liu, Yanli
name: Pan, Yilong
name: Yin, Yuyao
name: Chen, Wenhao
name: Li, Xiaodong
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 1: Table SI: Quality assessment of included studies (cohort studies)
title: Mind Rain, The Journey of Accessing
Creators: name: Majedian, Shoora
Publisher: name: Emily Carr University of Art and Design
Year: 2021
Subjects: subject: Memory
valueUri: https://id.loc.gov/authorities/subjects/sh85083497
subject: Figurative painting
valueUri: https://id.loc.gov/authorities/subjects/sh89000109
subject: Painting
valueUri: https://id.loc.gov/authorities/subjects/sh85096661

description: The MFA thesis writing reflects how accessing memories assists me in constructing a new visual language for my representational paintings. Through the process of collecting visual references of objects, space and figures, from auto-ethnographic sources to Persian miniatures, I had the opportunities to look at their historical and cultural backgrounds and compose images that reflect my socio-political state. Material experimentations with surface qualities, sizes, as well as paint applications, let me experience different visual characters to bring more sensibility to my image. These layers of visual meaning and narrative are also trying to construct a historical account from my particular generation’s experiences. During an iterative studio process I was inspired to bring chaos to composition and appreciate uncertainty in mark-making. These methodologies also helped me to construct the unsettling expression that overlaps with the titles and small poems (translated from Farsi) that echoed my lived experiences.
Additional file 4: of Participation of father in perinatal care: a qualitative study from the perspective of mothers, fathers, caregivers, managers and policymakers in Iran
Creators: name: Vahideh Firouzan
name: Noroozi, Mahnaz
name: Mirghafourvand, Mojgan
name: Farajzadegan, Ziba
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Interview guide during the face-to-face interviews with deputy health managers and policymakers for the study conducted on participation of fathers in perinatal care from the perspective of mothers, fathers, caregivers, managers and policymakers in Tabriz Town, Iran, 2017 (See methods section for further description). (DOCX 16 kb)
title: ADCO, Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Cart. 184 (11 H 987), 105 folios, f. 0078
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/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0078, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0078, 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
Modelling dust rings in early-type galaxies through a sequence of radiative transfer simulations and 2D image fitting
Creators: name: Bonfini, P.
name: Gonzalez-Martin, O.
name: Fritz, J.
name: Bitsakis, T.
name: Bruzual, G.
name: Sodi, B. Cervantes
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A large fraction of early-type galaxies (ETGs) host prominent dust features, and central dust rings are arguably the most interesting among them. We present here `Lord Of The Rings' (LOTR), a new methodology which allows to integrate the extinction by dust rings in a 2D fitting modelling of the surface brightness distribution. Our pipeline acts in two steps, first using the surface fitting software GALFIT to determine the unabsorbed stellar emission, and then adopting the radiative transfer code SKIRT to apply dust extinction. We apply our technique to NGC 4552 and NGC 4494, two nearby ETGs. We show that the extinction by a dust ring can mimic, in a surface brightness profile, a central point source (e.g. an unresolved nuclear stellar cluster or an active galactic nucleus; AGN) superimposed to a `core' (i.e. a central flattening of the stellar light commonly observed in massive ETGs). We discuss how properly accounting for dust features is of paramount importance to derive correct fluxes especially for low luminosity AGNs (LLAGNs). We suggest that the geometries of dust features are strictly connected with how relaxed is the gravitational potential, i.e. with the evolutionary stage of the host galaxy. Additionally, we find hints that the dust mass contained in the ring relates to the AGN activity.
description: Accepted in MNRAS
การพัฒนาระบบแจ้งเตือนผู้สูงอายุด้วยกล่องจ่ายยาอัตโนมัติ
Creators: name: นันทพงศ์ โชติกาวินทร์
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: กล่องยา
ผู้สูงอายุ

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 1, 15 ถึง 30
Summing One-Loop Graphs at Multi-Particle Threshold
Creators: name: Voloshin, M. B.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that the technique recently suggested by Lowell Brown for summing the tree graphs at threshold can be extended to calculate the loop effects. Explicit result is derived for the sum of one-loop graphs for the amplitude of threshold production of $n$ on-mass-shell particles by one virtual in the unbroken $λϕ^4$ theory. It is also found that the tree-level amplitude of production of $n$ particles by two incoming on-mass-shell particles vanishes at the threshold for $n > 4$.
description: 13 pages, LaTeX, TPI-MINN-92/45-T
title: Clermont-Ferrand. Bibliothèque du Patrimoine, MS 149, f3r
Creators: name: Bibliothèque du Patrimoine, Clermont-Ferrand
name: Clermont-Ferrand. Bibliothèque Du Patrimoine
name: Https://La.Wikisource.Org/Wiki/Usor:SZC_03 SZC 03
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024

description: Clermont-Ferrand. Bibliothèque du Patrimoine, MS 149, f3r
description: Source: https://la.wikisource.org/wiki/Vitae_sanctorum_(MS_149_Claromontensis)
description: Source: https://www.nakala.fr/10.34847/nkl.147d3z64
description: Source: Clermont Auvergne Métropole Library MS 149 Vitae sanctorum
description: Clermont-Ferrand. Bibliothèque du Patrimoine, MS 149, f3r
description: Clermont-Ferrand. Bibliothèque du Patrimoine, MS 149, f3r
การพัฒนาแอปพลิเคชันสำหรับถ่ายภาพประจำตัวนักศึกษา มหาวิทยาลัยพายัพจากเว็บแคเมราโดยใช้ภาษาโพรเซสซิง
Creators: name: ภูมินทร์ ดวงหาคลัง
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: แอปพลิเคชันสำหรับถ่ายภาพประจำตัวนักศึกษา
กระบวนการพัฒนาแอปพลิเคชันแบบรวดเร็ว
ภาษาโพรเซสซิง
เว็บแคเมรา

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 1, 31 ถึง 52
Merger rates in hierarchical models of galaxy formation. II: Comparison with N-body simulations
Creators: name: Lacey, Cedric
name: Cole, Shaun
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have made a detailed comparison of the results of large N-body simulations with the analytical description of the merging histories of dark matter halos presented in Lacey & Cole 1993, which is based on an extension of the Press- Schechter method (Bond etal 1991,Bower 1991). We find the analytical predictions for the halo mass function, merger rates and formation times to be remarkably accurate. The analytical model is however expected to apply for arbitrary Omega and general power spectra. Dark matter halos were identified in the simulations using two different methods. For halos selected at mean overdensities 100-200, the analytical mass function was found to provide a good fit to the simulations with a collapse threshold close to that predicted by the spherical collapse model, with a typical error of <30% over a range of 1000 in mass, which is the full dynamic range of our N-body simulations. This was insensitive to the type of filtering used. Over a range of 100 - 1000 in mass, there was also good agreement with the analytical predictions for merger rates, including their dependence on the masses of the two halos involved and the time interval being considered, and for formation times, including the dependence on halo mass and formation epoch. The analytical Press-Schechter mass function and its extension to halo lifetimes and merger rates thus provide a very useful description of the growth of dark matter halos through hierarchical clustering, and should providea valuable tool in studies of the formation and evolution of galaxies and galaxy clusters.
description: Available here as self unpacking postscript or as postscript file /pub/preprints/lacey_cole.ps by anonymous ftp from dust0.dur.ac.uk
การจัดการกลไกงานวิจัยด้วย Awesome table คณะเทคโนโลยีคหกรรมศาสตร์ มหาวิทยาลัยเทคโนโลยีราชมงคลกรุงเทพ
Creators: name: อรรถพล จันทร์สมุด
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: การจัดการกลไกงานวิจัย
Awesome table
คณะเทคโนโลยีคหกรรมศาสตร์
มหาวิทยาลัยเทคโนโลยีราชมงคลกรุงเทพ

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 1, 53 ถึง 63
On the mechanism of trapped surface formation
Creators: name: Valls-Gabaud, David
name: Zannias, Thomas
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: By a combination of analytical and numerical methods, the density profile of a momentarily at rest spherical star is varied, and the corresponding response in the area of the spherical shells is monitored. It is shown that the inner apparent horizon (if it exists) must lie within or at most on the star's surface, while no such restriction is found for the outer apparent horizon. However, an apparent horizon lying in the vacuum region will always have non vanishing area, as long as the ADM mass of the system is non zero. Furthermore for density profiles not decreasing inwards, it appears that all spherical trapped surfaces lie on a thick spherical shell. Finally for a uniform density star a simple criterion is found, relating density and proper radius that guarantees the presence or absence of trapped regions.
description: PostScript, 9 pages with 3 figures (included)
A non-perturbative exploration of the high energy regime in $N_\text{f}=3$ QCD
Creators: name: Brida, Mattia Dalla
name: Fritzsch, Patrick
name: Korzec, Tomasz
name: Ramos, Alberto
name: Sint, Stefan
name: Sommer, Rainer
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using continuum extrapolated lattice data we trace a family of running couplings in three-flavour QCD over a large range of scales from about 4 to 128 GeV. The scale is set by the finite space time volume so that recursive finite size techniques can be applied, and Schrödinger functional (SF) boundary conditions enable direct simulations in the chiral limit. Compared to earlier studies we have improved on both statistical and systematic errors. Using the SF coupling to implicitly define a reference scale $1/L_0\approx 4$ GeV through $\bar{g}^2(L_0) =2.012$, we quote $L_0 Λ^{N_{\rm f}=3}_{\overline{\rm MS}} =0.0791(21)$. This error is dominated by statistics; in particular, the remnant perturbative uncertainty is negligible and very well controlled, by connecting to infinite renormalization scale from different scales $2^n/L_0$ for $n=0,1,\ldots,5$. An intermediate step in this connection may involve any member of a one-parameter family of SF couplings. This provides an excellent opportunity for tests of perturbation theory some of which have been published in a letter [1]. The results indicate that for our target precision of 3 per cent in $L_0 Λ^{N_{\rm f}=3}_{\overline{\rm MS}}$, a reliable estimate of the truncation error requires non-perturbative data for a sufficiently large range of values of $α_s=\bar{g}^2/(4π)$. In the present work we reach this precision by studying scales that vary by a factor $2^5= 32$, reaching down to $α_s\approx 0.1$. We here provide the details of our analysis and an extended discussion.
description: 40 pages, 11 figures
Additional file 2: of Gout prevalence and predictors of urate-lowering therapy use: results from a population-based study
Creators: name: Pisaniello, Huai
name: Lester, Susan
name: Gonzalez-Chica, David
name: Stocks, Nigel
name: Longo, Marie
name: Sharplin, Greg
name: Grande, Eleonora Dal
name: Gill, Tiffany
name: Whittle, Samuel
name: Hill, Catherine
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: Table S1. Prevalence of gout by age group and gender from the South Australian 2015 Health Omnibus Survey. Table S2. Birth country prevalence (percentage). Odds ratios are for the comparison of participants with and without gout. Table S3. (A) Coefficients from the multinomial logistic regression model for predictors of allopurinol use. (B) Predictor variables not included in the model for allopurinol use. (PDF 236 kb)
Google forms เพื่อการจองรถในสถาบันอุดมศึกษา กรณีศึกษา คณะเทคโนโลยีคหกรรมศาสตร์ มหาวิทยาลัยเทคโนโลยีราชมงคลกรุงเทพ
Creators: name: อรรถพล จันทร์สมุด
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: Google Forms เพื่อการจองรถ
สถาบันอุดมศึกษา
คณะเทคโนโลยีคหกรรมศาสตร์ มหาวิทยาลัยเทคโนโลยีราชมงคลกรุงเทพ

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 1, 64 ถึง 77
Correlations in orbital angular momentum of spatially entangled paired photons generated in parametric downconversion
Creators: name: Osorio, Clara I.
name: Molina-Terriza, Gabriel
name: Torres, Juan P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: What are the orbital angular momentum correlations between spatially entangled photon pairs generated in spontaneous parametric down-conversion? We show that the answer to this question can be given in two alternative, although complementary, ways. The answer posed in this letter explains satisfactorily the seemingly contradictory results obtained in different experiments, and theoretical approaches.
description: 4 pages, 3 figures. Submitted to PRA
Sign changes of Kloosterman sums and exceptional characters
Creators: name: Drappeau, Sary
name: Maynard, James
Publisher: name: arXiv
Year: 2018
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11L05, 11N36 (Primary), 11N75, 11L20, 11M20 (Secondary)

description: We prove that the existence of exceptional real zeroes of Dirichlet $L$-functions would lead to cancellations in the sum $\sum_{p\leq x} \Kl(1, p)$ of Kloosterman sums over primes, and also to sign changes of $\Kl(1, n)$, where $n$ runs over integers with exactly two prime factors. Our arguments involve a variant of Bombieri's sieve, bounds for twisted sums of Kloosterman sums, and work of Fouvry and Michel on sums of $\left| \Kl(1, n)\right|$.
description: 11 pages
The Farm-to-Fridge Value Chain: Participants’ Roles and Driving Productivity through Technology Interventions
Creators: name: Banerjee, Mohua
name: Kunamaneni, Suneel
name: Banerjee, Mohua
name: Kunamaneni, Suneel
Publisher: name: Unknown
Year: 2019
Subjects: subject: Agricultural and Food Policy
subject: Farm Management
subject: dairy
subject: value chain
subject: farm level profitability

description: The value chain of the Indian dairy industry consists of dairy farmers, collection centres, chilling centres, processing plants, retailers and consumers. The objectives of the study are to map the processes and operational challenges existing in the dairy value chain, estimate profitability of the participants at the farm-levels to gauge their potential in undertaking entrepreneurial initiatives, study roles of the privately-owned processing plants in the supply chain, and identify business models of startups in the dairy ecosystem who drive productivity through technology interventions. Exploratory research through multiple field visits, in-depth interviews and personal observations in West Bengal (eastern India) and Bangalore have formed the basis of this study. Using case study format, the roles of the different intermediaries in the value chain have been analysed to develop insights on their entrepreneurial abilities and intent. The findings reveal the largely fragmented, unorganized dairy industry where the channel members majorly operate in silos with linkages only to their immediate backward and forward partners, in a myopic manner. At the farm level, only the chilling centres have sufficient profitability to undertake value-adding entrepreneurial initiatives. The marginal dairy farmers are at subsistence level and hence unable to participate in value creation. The private processing plants are corporate entrepreneurs and their interactions with chilling centres are confined to that of supplier-manufacturer, to ensure seamless supply of milk for their manufacturing processes. They do not engage with the small dairy farmers. In these circumstances, new-age start-ups that create social impact while operating as a viable, for-profit organization, effectively bridge the gaps in the dairy value chain by intervening at all its nodal points and providing technology solutions to create additional value. Farmers are at the core of the dairy processes as they produce the milk and any improvement in the value chain ultimately gets back to the farmer through better prices and better market linkages.
การพัฒนาเครื่องพ่นฆ่าเชื้อโรคที่พื้นสำหรับเท้าและรองเท้า แบบอัตโนมัติ
Creators: name: บุญสืบ โพธิ์ศรี
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: เครื่องพ่นฆ่าเชื้อ
ไมโครคอนโทรลเลอร์อาดุยโน่
ไวรัสโคโรนา 2019

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 2, 1 ถึง 16
Study of $B_{c}^{-}$ ${\to}$ $J/ψπ^{-}$, $η_{c}π^{-}$ Decays with QCD Factorization
Creators: name: Sun, Junfeng
name: Xue, Guifeng
name: Yang, Yueling
name: Lu, Gongru
name: Du, Dongsheng
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The $B_{c}$ ${\to}$ $J/ψπ$, $η_{c}π$ decays are studied in the scheme of the QCD factorization approach. The branching ratios are calculated with the asymptotic distribution amplitude of the pion. The charm quark mass effect is considered. We find that the mass effect on the branching ratios is small.
description: 20 pages, 3 figures, 3 tables
Robo-AO Kepler Survey V: The effect of physically associated stellar companions on planetary systems
Creators: name: Ziegler, Carl
name: Law, Nicholas M.
name: Baranec, Christoph
name: Howard, Ward
name: Morton, Tim
name: Riddle, Reed
name: Duev, Dmitry A.
name: Salama, Maïssa
name: Jensen-Clem, Rebecca
name: Kulkarni, S. R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The Kepler light curves used to detect thousands of planetary candidates are susceptible to dilution due to blending with previously unknown nearby stars. With the automated laser adaptive optics instrument, Robo-AO, we have observed 620 nearby stars around 3857 planetary candidates host stars. Many of the nearby stars, however, are not bound to the KOI. In this paper, we quantify the association probability between each KOI and detected nearby stars through several methods. Galactic stellar models and the observed stellar density are used to estimate the number and properties of unbound stars. We estimate the spectral type and distance to 145 KOIs with nearby stars using multi-band observations from Robo-AO and Keck-AO. We find most nearby stars within 1" of a Kepler planetary candidate are likely bound, in agreement with past studies. We use likely bound stars as well as the precise stellar parameters from the California Kepler Survey to search for correlations between stellar binarity and planetary properties. No significant difference between the binarity fraction of single and multiple planet systems is found, and planet hosting stars follow similar binarity trends as field stars, many of which likely host their own non-aligned planets. We find that hot Jupiters are ~4x more likely than other planets to reside in a binary star system. We correct the radius estimates of the planet candidates in characterized systems and find that for likely bound systems, the estimated planetary candidate radii will increase on average by a factor of 1.77, if either star is equally likely to host the planet. We find that the planetary radius gap is robust to the impact of dilution, and find an intriguing 95%-confidence discrepancy between the radius distribution of small planets in single and binary systems.
description: 19 pages, 12 figures, submitted to AAS Journals
Incremental Training of Deep Convolutional Neural Networks
Creators: name: Istrate, Roxana
name: Malossi, Adelmo Cristiano Innocenza
name: Bekas, Costas
name: Nikolopoulos, Dimitrios
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We propose an incremental training method that partitions the original network into sub-networks, which are then gradually incorporated in the running network during the training process. To allow for a smooth dynamic growth of the network, we introduce a look-ahead initialization that outperforms the random initialization. We demonstrate that our incremental approach reaches the reference network baseline accuracy. Additionally, it allows to identify smaller partitions of the original state-of-the-art network, that deliver the same final accuracy, by using only a fraction of the global number of parameters. This allows for a potential speedup of the training time of several factors. We report training results on CIFAR-10 for ResNet and VGGNet.
The role of lipoxin A4 in regulating ion transport and airway surface liquid dynamics in cystic fibrosis bronchial epithelium
Creators: name: Al-Alawi, Mazen
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: The thesis reports novel findings on the role of LXA4 in inodulating the airway surface liquid (ASL) layer height and in particular expanding the deficient ASL observed in CF as a novel means to augmenting existing therapy. Lipoxin A4 (LXA4) is produced at inflammatory sites, and exerts antiinflammatoiy effects and has been reported to be reduced in cystic fibrosis (CF) airways. The altered Cl- secretion and Na+ hyperabsorption in CF affects the ASL height and leads to a defective mucociliary clearance, chronic infection, inflammation and progressive lung destruction. The role of LXA4 in modulating ion transport and ASL height in CF and non-CF airway epithelia was investigated. CF (CuFi-1) and non-CF (NuLi-1) bronchial epithelial cell lines were grown into well-differentiated epithelia. LXA4 effects were explored using laser confocal inicroscopy to measure ASL height, short-circuit current to investigate ion transporters activity, and ATP assay to measure ATP release at the apical side of CF epithelia. LXA4 (1 nM) treatment for 15 minutes, increased ASL height in Nuli-1 and CuFi-1 epithelia. The stimulatory effect of LXA4 on ASL height was inhibited by the LXA4 receptor FPR2/ALX inhibitor, boc-2; in addition to bumetanide, reactive blue and extracellular hexolinase, while amiloride was showed an additive effect to LXA4. LXA4 was activated Cl- secretion and inhibited Na+ absorption in the CF epithelia. In addition, LXA4 stimulated an apical Boc-2 sensitive release of ATP in CF epithelia. This thesis provides evidence for a novel effect of LXA4 involving the FPR2/ALX receptor, apical ATP release and purinoreceptor activation, inhibition of Na+ absorption and stimulation of Cl+ secretion in CF and non-CF epithelia to finally increase ASL height. These effects open up a new therapeutic avenue in the treatment of CF.
Additional file 5: of Hepatitis B virus infection among pregnant women in Ethiopia: a systematic review and Meta-analysis of prevalence studies
Creators: name: Kindie Kebede
name: Dejene Abateneh
name: Alemayehu Belay
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Sub-group meta-analysis by study site among pregnant women in Ethiopia. (DOCX 1401 kb)
GAME: GAlaxy Machine learning for Emission lines
Creators: name: Ucci, Graziano
name: Ferrara, Andrea
name: Pallottini, Andrea
name: Gallerani, Simona
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an updated, optimized version of GAME (GAlaxy Machine learning for Emission lines), a code designed to infer key interstellar medium physical properties from emission line intensities of UV/optical/far infrared galaxy spectra. The improvements concern: (a) an enlarged spectral library including Pop III stars; (b) the inclusion of spectral noise in the training procedure, and (c) an accurate evaluation of uncertainties. We extensively validate the optimized code and compare its performance against empirical methods and other available emission line codes (PYQZ and HII-CHI-MISTRY) on a sample of 62 SDSS stacked galaxy spectra and 75 observed HII regions. Very good agreement is found for metallicity. However, ionization parameters derived by GAME tend to be higher. We show that this is due to the use of too limited libraries in the other codes. The main advantages of GAME are the simultaneous use of all the measured spectral lines, and the extremely short computational times. We finally discuss the code potential and limitations.
description: 11 pages, 8 figures (appendix: 7 pages, 10 figures). Accepted for publication in MNRAS
title: Virtual Loops: Deconstructing Painting to Explore the Aesthetics of Mediation
Creators: name: Burke, Mollie
Publisher: name: Emily Carr University of Art and Design
Year: 2021
Subjects: subject: Painting
valueUri: https://id.loc.gov/authorities/subjects/sh85096661
subject: Painting, Abstract
valueUri: https://id.loc.gov/authorities/subjects/sh85096683
subject: Abstraction
valueUri: https://id.loc.gov/authorities/subjects/sh85000258
subject: Installations (Art)
valueUri: https://id.loc.gov/authorities/subjects/sh85066731
subject: Technology in art
valueUri: https://id.loc.gov/authorities/subjects/sh85133190

description: This thesis document outlines the key concepts and research practices I undertook to explore the aesthetics of mediating digital and analog logics through materiality and painterly abstraction. It culminated in a body of work of 8 paintings and a ﬁnal thesis exhibition from March 22 to April 1 at Emily Carr University of Art and Design. This work builds on my practice as an abstract painter to deconstruct painting and use a site responsive installation method to explore the optical dimensions of borders, boundaries, and surfaces to negotiate between digital and analog logics. This interest in a medial condition coupled with the impact of Covid 19 focused my observational and material research to center around the site and idea of LCD and plasma screens of personal computing devices. The screen mediates between two categories of digital and analog, and in an attempt to study communication loops between these two categories I use digital processes of laser cutters, 3D scanners, and 3D printers as well as analog processes of silicone casting and paint drying to explore diﬀerent variations of transmutation. The materials I choose are based on visual eﬀect and the relationship with transparency/translucency and opacity/obscuring. Through fusing an expanded painting practice (using ﬂat, painterly elements) with the spatial and sculptural (using the actuality and volume of sculpture) I want to consider the digital as a state of abstraction that is constantly mediated between the analog forms of real. This research draws on the theories of the media archaeology of colour by Carolyn L Kane for my selection of colours and surfaces, Alexander Galloway’s conception of the digital as an epistemological category that exists outside of personal computing devices, and Bernhard Siegert’s notion of cultural techniques to frame the screen as a material technic that reinforces ideas and divisions of digital and analog, while these categories and ways of thinking have long historical precedents.
Additional file 3: of Participation of father in perinatal care: a qualitative study from the perspective of mothers, fathers, caregivers, managers and policymakers in Iran
Creators: name: Vahideh Firouzan
name: Noroozi, Mahnaz
name: Mirghafourvand, Mojgan
name: Farajzadegan, Ziba
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Interview guide during the face-to-face interviews with health care providers (midwives, gynecologists and nurses) for the study conducted on participation of fathers in perinatal care from the perspective of mothers, fathers, caregivers, managers and policymakers in Tabriz Town, Iran, 2017 (See methods section for further description). (DOCX 16 kb)
Solution space of 2+1 gravity on ${\bf R} \times T^2$ in Witten's connection formulation
Creators: name: Louko, Jorma
name: Marolf, Donald M.
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the space ${\cal M}$ of classical solutions to Witten's formulation of 2+1 gravity on the manifold ${\bf R} \times T^2$. ${\cal M}$ is connected, unlike the spaces of classical solutions in the cases where $T^2$ is replaced by a higher genus surface. Although ${\cal M}$ is neither Hausdorff nor a manifold, removing from ${\cal M}$ a set of measure zero yields a manifold which is naturally viewed as the cotangent bundle over a non-Hausdorff base space~${\cal B}$. We discuss the relation of the various parts of ${\cal M}$ to spacetime metrics, and various possibilities of quantizing~${\cal M}$. There exist quantizations in which the exponentials of certain momentum operators, when operating on states whose support is entirely on the part of ${\cal B}$ corresponding to conventional spacetime metrics, give states whose support is entirely outside this part of~${\cal B}$. Similar results hold when the gauge group ${\rm SO}_0(2,1)$ is replaced by ${\rm SU}(1,1)$.
description: 23 pages, REVTeX v3.0, SU-GP-93/7-6, CGPG-93/8-3. (Discussion on the gauge equivalence of degenerate and nondegenerate metrics extended.)
ระบบสัญญาอัจฉริยะสำหรับการจำหน่ายหญ้าเนเปียร์ให้โรงไฟฟ้าชีวมวลที่อำเภอปะคำ จังหวัดบุรีรัมย์
Creators: name: ประสิทธิ์ จิโรจน์กุล
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: ระบบสัญญาอัจฉริยะ
บล็อกเชน
โรงไฟฟ้าชีวมวล
วิสาหกิจชุมชน
หญ้าเนเปียร์

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 2, 17 ถึง 32
Radiative $D^*$ Decay Using Heavy Quark and Chiral Symmetry
Creators: name: Amundson, J. F.
name: Boyd, C. G.
name: Jenkins, E.
name: Luke, M.
name: Manohar, A. V.
name: Rosner, J. L.
name: Savage, M. J.
name: Wise, M. B.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The implications of chiral $SU(3)_L \times SU(3)_R$ symmetry and heavy quark symmetry for the radiative decays $D^{*0}\to D^0γ$, $D^{*+}\to D^+γ$, and $D_s^*\to D_sγ$ are discussed. Particular attention is paid to $SU(3)$ violating contributions of order $m_q^{1/2}$. Experimental data on these radiative decays provide constraints on the $D^* Dπ$ coupling.
description: 9 pages plus 3 pages of figures in POSTSCRIPT file appended to TeX file (uses harvmac.tex and tables.tex), UCSD/PTH 92-31, CALT-68-1816, EFI-92-45, CERN-TH.6650/92
First hydrodynamics simulations of radiation forces and photoionization feedback in massive star formation
Creators: name: Kuiper, Rolf
name: Hosokawa, Takashi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the first simulations of the formation and feedback of massive stars which account for radiation forces as well as photoionization feedback (along with protostellar outflows). In two different accretion scenarios modeled, we determine the relative strength of these feedback components and derive the size of the reservoir from which the forming stars gained their masses. We find that protostellar outflows alone limit the stellar mass growth only in an accretion scenario with a finite mass reservoir; when including accretion and ram pressure from large scales (> 0.1 pc), protostellar outflows do not limit stellar mass growth at all. Photoionization and HII regions dominate the feedback ladder only at later times and only on large scales. Specifically, photoionization yields a broadening of the bipolar outflow cavities and a reduction of the gravitational infall momentum by about 50 percent, but does not limit the stellar mass accretion. On the other hand, we find radiation forces restrain the gravitational infall toward the circumstellar disk, impact the gravito-centrifugal equilibrium at the outer edge of the disk, and eventually shut down stellar accretion completely. The most massive star formed in the simulations accreted 95 solar masses before disk destruction; this mass was drawn-in from an accretion reservoir of approximately 240 solar masses and 0.24 pc in radius. In the regime of very massive stars, the final mass of these stars is controlled by their own radiation force feedback.
description: 22 pages, accepted for publication at A&A
Additional file 10: of Structural complexity of the co-chaperone SGTA: a conserved C-terminal region is implicated in dimerization and substrate quality control
Creators: name: MartĂ­Nez-Lumbreras, Santiago
name: Krysztofinska, Ewelina
name: Thapaliya, Arjun
name: Spilotros, Alessandro
name: Matak-Vinkovic, Dijana
name: Salvadori, Enrico
name: Roboti, Peristera
name: Nyathi, Yvonne
name: Muench, Janina
name: Roessler, Maxie
name: Svergun, Dmitri
name: High, Stephen
name: Isaacson, Rivka
Publisher: name: figshare
Year: 2018
Subjects: Biochemistry
Cell Biology
Developmental Biology
Computational Biology

description: Figure S10. 15NÂ - {1H} heteronuclear NOE measurements of different SGTA constructs; in all cases, the domain boundaries and linker regions are similar. (PDF 142 kb)
Additional file 2: of Simultaneous E-cadherin and PLEKHA7 expression negatively affects E-cadherin/EGFR mediated ovarian cancer cell growth
Creators: name: Rea, Katia
name: Roggiani, Francesca
name: Cecco, Loris De
name: Raspagliesi, Francesco
name: Carcangiu, Maria
name: Nair-Menon, Joyce
name: Bagnoli, Marina
name: Bortolomai, Ileana
name: Mezzanzanica, Delia
name: Canevari, Silvana
name: Kourtidis, Antonis
name: Anastasiadis, Panos
name: Tomassetti, Antonella
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: 60506 Virology

description: Figure S1. IHC with anti-E-cadherin on: upper panel, FFPE sections from fallopian tubal epithelium; and lower panel, eight FFPE samples of solid masses from HG-SOC patients. Control, a section only processed with the secondary antibody. Bar, 50 μm. Figure S2a. Representative phase contrast images of OAW42 MCAs and evaluation of live/dead cells; bar, 50 μm. The empty box highlights the image reported in Fig. 1f. b. Upper panel: representative phase contrast images of MCAs of control (CO) and E-cadh siRNA-treated OAW42 cells grown in Matrigel® for 6 days. Lower panel: measurement of OAW42 MCA area using ImageJ software. c. Control (CO) or E-cadherin siRNA-treated OVCAR5 cells. Upper panel: cell viability assay performed on silenced OVCAR5 cells; the number of cells was evaluated. Lower panel: E-cadherin levels in OVCAR5 cells after 5 days of culture. d. E-cadherin levels in treated cells of Fig. 2c. Control, (CO) or pooled E-cadherin siRNA. e. Western blotting on lysates from OAW42 starved (−) or EGF treated cells. Figure S3. Representative phase contrast images or fluorescent marked OAW42 and OVCAR5 live/dead cells; bar, 100 μm. Figure S4a. Western blotting on total cell lysates from six EOC cell lines. b. IF on fixed Caco2, OAW42, and OVCAR5 cells. c. Upper panel: representative western blotting on lysates from Caco2 cells infected with a control (NT) or with PLEKHA7 shRNA (shPLEKHA7). Starved cells (−). Lower left panel: western blotting with anti-PLEKHA7 Ab. Lower right panel: quantitative P-EGFR/EGFR ratio on PLEKHA7 silenced cells as above. Figure S5a. Confocal IF performed on LZRS or LZRS-PLEKHA7 infected OAW42 cells. Bar, 20 μm. The panel reports the stacks with single Ab of the merge images of Fig. 5d. b. Left panel: representative phase contrast images of LZRS or PLEKHA7 OAW42 MCAs grown in Algimatrix™. Right panel: cell viability assay of cells extracted from the sponge. (PDF 791 kb)
Simulating Self-gravitating Hydrodynamic Flows
Creators: name: Mueller, Ewald
name: Steinmetz, Matthias
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An efficient algorithm for solving Poisson's equation in two and three spatial dimensions is discussed. The algorithm, which is described in detail, is based on the integral form of Poisson's equation and utilizes spherical coordinates and an expansion into spherical harmonics. The solver can be applied to and works well for all problems for which the use of spherical coordinates is appropriate. We also briefly discuss the implementation of the algorithm into hydrodynamic codes which are based on a conservative finite--difference scheme.
description: 15 pages, compressed uu-encoded postscript file (232kB), to appear in Computer Physics Communications, special issue Computational Hydrodynamics in Astrophysics
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0283
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/2012
name: Petot, Frédéric
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: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0283, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
A galaxy lacking dark matter
Creators: name: van Dokkum, Pieter
name: Danieli, Shany
name: Cohen, Yotam
name: Merritt, Allison
name: Romanowsky, Aaron J.
name: Abraham, Roberto
name: Brodie, Jean
name: Conroy, Charlie
name: Lokhorst, Deborah
name: Mowla, Lamiya
name: O'Sullivan, Ewan
name: Zhang, Jielai
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Studies of galaxy surveys in the context of the cold dark matter paradigm have shown that the mass of the dark matter halo and the total stellar mass are coupled through a function that varies smoothly with mass. Their average ratio M_{halo}/M_{stars} has a minimum of about 30 for galaxies with stellar masses near that of the Milky Way (approximately 5x10^{10} solar masses) and increases both towards lower masses and towards higher masses. The scatter in this relation is not well known; it is generally thought to be less than a factor of two for massive galaxies but much larger for dwarf galaxies. Here we report the radial velocities of ten luminous globular-cluster-like objects in the ultra-diffuse galaxy NGC1052-DF2, which has a stellar mass of approximately 2x10^8 solar masses. We infer that its velocity dispersion is less than 10.5 kilometers per second with 90 per cent confidence, and we determine from this that its total mass within a radius of 7.6 kiloparsecs is less than 3.4x10^8 solar masses. This implies that the ratio M_{halo}/M_{stars} is of order unity (and consistent with zero), a factor of at least 400 lower than expected. NGC1052-DF2 demonstrates that dark matter is not always coupled with baryonic matter on galactic scales.
description: To appear in the 29 March issue of Nature
Relativistic energy of a moving spherical capacitor
Creators: name: Braga, Nelson R. F.
name: Sophia, Gustavo
Publisher: name: arXiv
Year: 2007
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: We discuss the relativistic transformation of the energy of a charged spherical capacitor. The energy stored in the electromagnetic fields observed by an uniformly moving frame is related to that of the rest frame by a factor different from $γ$. Considering the energy and the stresses in the capacitor shells we show that the total energy of the system satisfies the expected relativistic transformation.
description: 8 pages, 3 figures
นวัตกรรมเพื่อส่งเสริมผู้ประกอบการรายย่อยด้วยเทคโนโลยีบล็อกเชน
Creators: name: ภุมรินทร์ ปาละนันทน์
Publisher: name: มหาวิทยาลัยแม่โจ้
Year: 2022
Subjects: ตัวแทนจำหน่าย
บล็อกเชน
โทเคนดิจิทัล
เวิร์ดเพรสส์

description: วารสารแม่โจ้เทคโนโลยีสารสนเทศและนวัตกรรม, 8, 2, 33 ถึง 48
Particle Creation in a universe filled by radiation and dust-like matter
Creators: name: Villalba, Victor M.
Publisher: name: arXiv
Year: 1993
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this article the particle creation process of scalar and spin 1/2 particles in a spatially open cosmological model associated with a universe filled by radiation and dustlike matter. The Klein-Gordon and Dirac equations are solved via separation of variables. After comparing the{\it \ in }and% {\it \ out} vacua, we obtain that the number of created particles corresponds to Planckian and Fermi-Dirac distributions for the scalar and Dirac cases
description: 16pp. IVIC-CFLE-93/03
When fast and slow interfaces grow together: connection to the half-space problem of the Kardar-Parisi-Zhang class
Creators: name: Ito, Yasufumi
name: Takeuchi, Kazumasa A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We study height fluctuations of interfaces in the $(1+1)$-dimensional Kardar-Parisi-Zhang (KPZ) class, growing at different speeds in the left half and the right half of space. Carrying out simulations of the discrete polynuclear growth model with two different growth rates, combined with the standard setting for the droplet, flat, and stationary geometries, we find that the fluctuation properties at and near the boundary are described by the KPZ half-space problem developed in the theoretical literature. In particular, in the droplet case, the distribution at the boundary is given by the largest-eigenvalue distribution of random matrices in the Gaussian symplectic ensemble, often called the GSE Tracy-Widom distribution. We also characterize crossover from the full-space statistics to the half-space one, which arises when the difference between the two growth speeds is small.
description: 7 pages, 7 figures
title: UMass ADVANCE STEM Pandemic Effects by Gender and Time of Hire 2022
Creators: name: Liu, Shuyin
name: Misra, Joya
name: Smith-Doerr, Laurel
Publisher: name: University of Massachusetts Amherst
Year: 2023

description: In this research brief, we describe some of the key findings from this survey, focusing on patterns among STEM faculty by gender and new hires (whether they joined UMass before or since 2019, given the impact of the pandemic on faculty life). We explore whether and how the intersection of gender and time of hire affect STEM faculty decision-making, feelings of inclusion, and research collaboration.