cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Pooled extracellular receptor-ligand interaction screening using CRISPR activation
Creators: name: Zheng-Shan Chong
name: Ohnishi, Shuhei
name: Yusa, Kosuke
name: Wright, Gavin
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Table S1. A table listing the gRNAs sequences targeting the promoter regions for the named genes. The gene symbol, accession number of the target transcript and chromosomal location are provided. Table S2. A table detailing the sequences of the synthesized DNA fragments and PCR primers used for plasmid construction and sequencing, primers used for q-RT-PCR, and primers for gRNA library preparation and amplification. Table S3. A table providing the sources, and where appropriate, clone names of the primary monoclonal and conjugated secondary antibodies used in this study. (PDF 553 kb)
title: Disinvestment? Out of the question. Managing German business subsidiaries in apartheid South Africa during the tenure of P.W. Botha, 1978-1989
Creators: name: Sud, Gaurav Pratap
Publisher: name: London School of Economics and Political Science (LSE)
Year: 2021

description: This thesis re-evaluates the case for business disinvestment from South Africa during the tenure of P.W. Botha (1978-1989). Using neglected corporate archives as well as oral testimony by former directors, the thesis scrutinizes the decision-making processes employed by the outlier on disinvestment – German business. Through seven case studies, the thesis illustrates how Apartheid policies, rather than being the foundation for business success, were the originators of enduring financial and operational woes. By continuing operations, management faced enduring uncertainty whilst grappling with the fallout from Botha’s reform and security measures. This research highlights that not only was international business entangled to an unprecedented degree with Botha’s policy agenda, but also that established narratives presented by anti-apartheid stakeholders on disinvestment require more critical evaluation. Most importantly, it illustrates that the ‘last decade of apartheid’ deserves a wider interdisciplinary approach that includes an engagement with the voice of management. For, these foreign corporate responses go beyond the historic South African context by having spearheaded several institutions, processes and interlinkages that define today’s globalised world.
Thermal conduction in accretion disk coronae
Creators: name: Maciolek-Niedzwiecki, Andrzej
name: Krolik, Julian H.
name: Zdziarski, Andrzej A.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the effects of thermal conduction in a hot, active corona above an accretion disk. We assume that all of the dissipative heating takes place in the corona. We find that the importance of conduction decreases with increases in the local dissipative compactness of the corona, l_{diss,loc}, and increases with increasing abundance of electron-positron pairs. For l_{diss,loc} < 1, a significant fraction of the energy released in the corona may be carried away by the conductive flux, leading to formation of a relatively hot transition layer below the base of the corona. Comptonization of disk radiation in such a layer may account for the presence of soft X-ray excesses in the spectra emitted by disk-corona systems.
description: 15 pages, 6 figures, accepted for publication in ApJ
Novel Mechanism for Streptokinase-induced Hypotension in Myocardial Infarction: Retrospective Analyses
Creators: name: Khalid, Karniza
name: Ahmad, Raja Elina Afzan Raja
name: Sze Yee Lui
name: Tong, Alwin Yu Hoong
name: Abidin, Ida Zaliza Zainal
Publisher: name: Zenodo
Year: 2020
Subjects: Hypotension
Myocardial Infarction
Streptokinase
Retrospective
Analysis
Novel Mechanism

description: Introduction Therapy with intravenous streptokinase (STK) for patients with acute myocardial infarction is often complicated with hypotension. The aim of the study is to investigate the extent of STK-induced hypotension in the local setting and determine the possible role of alteration in serum protein in the development of this event. Materials and Methods This is a retrospective cross-sectional study involving data transcription of acute myocardial infarction cases in Hospital Tuanku Fauziah, Perlis from the year 2015 to 2018. Patients requiring prior haemodynamic stabilisation prior to streptokinase administration (i.e. requiring inotropic support or glyceryl trinitrate (GTN) infusion prior to streptokinase), or prior cardiopulmonary resuscitation (CPR) were excluded. Results Out of the total 594 medical records screened for eligibility, 412 patients were selected based on the pre-defined criteria. The mean age of the study participants was 59.3 ± 0.66 years old. Majority were male (n=303, 82.8%) and of Malay descent (n=328, 89.6%). Anterior myocardial infarction was more common compared to the inferior site (50.1% vs. 41.7%). There were 109 (26.5%) patients who developed STK-induced hypotension whereas 259 (62.9%) with no complication. The yearly prevalence of STK-induced hypotension in our centre ranges from 27.0% to 38.5% (p=0.435). Multiple logistic regression (MLR) showed that Killip classification and baseline heart rate positively predict the development of hypotension in patients with acute myocardial infarction receiving streptokinase (controlled for age, gender, baseline CK, location of MI, and baseline SBP/DBP). We found that with every 1 unit decrement of baseline heart rate, the risk of hypotension will increase by 2.6%. Additionally, patients with Killip III and IV have 5 times higher risk of developing STK-induced hypotension as compared to those with Killip I. Discussion / Conclusion . The yearly prevalence of streptokinase-induced hypotension is similar to other worldwide multicentre studies, ranging from 27.0% to 38.5%. Our study suggests streptokinase may have preferential proteolytic activity against serum albumin as patients with hypotension had a significantly lower serum albumin as compared to those without hypotension, following streptokinase therapy. The observed reduction in serum albumin level in patients with hypotension may result in reduced serum viscosity, subsequently affects the total peripheral resistance with a resultant drop in blood pressure. Therefore, our study suggests the novel role of serum albumin in the pathophysiology of STK-induced hypotension that was never before studied.
Extrapolation for meson screening masses from imaginary to real chemical potential
Creators: name: Ishii, Masahiro
name: Miyahara, Akihisa
name: Kouno, Hiroaki
name: Yahiro, Masanobu
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We first extend our formulation for the calculation of $π$- and $σ$-meson screening masses to the case of finite chemical potential $μ$. We then consider the imaginary-$μ$ approach, which is an extrapolation method from imaginary chemical potential ($μ=i μ_{\rm I}$) to real one ($μ=μ_{\rm R}$). The feasibility of the method is discussed based on the entanglement Polyakov-loop extended Nambu--Jona-Lasinio (EPNJL) model in 2-flavor system. As an example, we investigate how reliable the imaginary-$μ$ approach is for $π$- and $σ$-meson screening masses, comparing "screening masses at $μ_{\rm R}$ in the method" with "those calculated directly at $μ_{\rm R}$". We finally propose the new extrapolation method and confirm its efficiency.
description: 9 pages, 11 figures
Additional file 5: of Body proportions for the facilitation of walking, running and flying: the case of partridges
Creators: name: JesĂşs Nadal
name: Ponz, Carolina
name: Margalida, Antoni
Publisher: name: figshare
Year: 2018
Subjects: subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: All partridge samples confidence intervals and correlation coefficients. (DOCX 28â kb)
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0387
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Petot, Frédéric
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0387, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0387, 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
Typhlopone brevinodosa Westwood 1840
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1877
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Typhlopone
Typhlopone brevinodosa

description: 31. Typhlopone brevinodosa Mayr,
Wien. Zool. Bot. Ges. 1862. 737.
Keren (Beccari). Molti esemplari di tutte le dimensioni da 2,5 fino a 7 millim.
Questa specie e molto affine alla T. punctata Sm., di cui ripete la forma e la statura; differisce per la punteggiatura assai meno forte sul capo e sul torace; il capo e meno largamente incavato indietro, con gli angoli posteriori piu rotondati, meno prominenti; nei grandi individui la forma del capo e piu parallela; il pigidio e conformato come nella T. punctata, mediocremente ristretto indietro; il suo margine posteriore ha due larghe incisure separate da una sporgenza angolare mediana, limitate all' esterno da una piccola spina. Si riconosce poi facilmente dalla T. oraniensis, alla quale Mayr 1 ' aveva riferita come varieta, per la punteggiatura piu forte, il capo piu breve, scavato indietro, il nodo del picciuolo meno lungo e piu largo e la struttura del pigidio.
description: Published as part of Emery, C., 1877, Catalogo delle formiche esistenti nelle collezioni del Museo Civico di Genova. Parte prima. Formiche provenienti dall Viaggio dei signori Antinori, Beccari e Issel nel Mar Rosso e nel paese dei Bogos., pp. 363-381 in Annali del Museo Civico di Storia Naturale Giacomo Doria (Genova) 9 on pages 363-381
Lepton pair production by high-energy neutrino in an external electromagnetic field
Creators: name: Kuznetsov, A. V.
name: Mikheev, N. V.
name: Rumyantsev, D. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The process of the lepton pair production by a neutrino propagating in an external electromagnetic field is investigated in the framework of the Standard Model. Relatively simple exact expression for the probability as the single integral is obtained, which is suitable for a quantitative analysis.
description: 9 pages, LATEX, 2 PS figures, submitted to Modern Physics Letters A
Global and local polarization of $Λ$ hyperons in Au+Au collisions at 200 GeV from STAR
Creators: name: Niida, Takafumi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: New results on global polarization of $Λ$ hyperons in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV reveal non-zero signal on the order of a few tenths of a percent. Compared with lower energy results, the current measurement shows that the polarization decreases at higher collision energy, the trend being well reproduced by theoretical calculations. The polarization is found to be larger in more peripheral collisions, as well as in the in-plane than in the out-of-plane direction. The signal seems to depend on the asymmetry between positive and negative charge in each event, which may indicate an influence of the axial current induced by the magnetic field. In addition, the first measurement of a local polarization along the beam direction was performed. The results show a quadrupole modulation relative to the second-order event plane, as expected from the elliptic flow.
description: 4 pages, 7 figures, Proceedings of Quark Matter 2018, Venice, Italy (May 13-19, 2018)
The chemical composition of $α$ Cen AB revisited
Creators: name: Morel, Thierry
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a fully self-consistent, line-by-line differential abundance analysis of $α$ Cen AB based on high-quality HARPS data. Various line lists are used and analysis strategies implemented to improve the reliability of the results. Abundances of 21 species with a typical precision of 0.02-0.03 dex are reported. We find that the chemical composition of the two stars is not scaled solar (e.g. Na and Ni excess, depletion of neutron-capture elements), but that their patterns are strikingly similar, with a mean abundance difference (A - B) with respect to hydrogen of -0.01$\pm$0.04 dex. Much of the scatter may be ascribed to physical effects that are not fully removed through a differential analysis because of the mismatch in parameters between the two components. We derive an age for the system from abundance indicators (e.g. [Y/Mg] and [Y/Al]) that is slightly larger than solar and in agreement with most asteroseismic results. Assuming coeval formation for the three components belonging to the system, this implies an age of about $\sim$6 Gyrs for the M dwarf hosting the terrestrial planet Proxima Cen b. After correction for Galactic chemical evolution effects, we find a trend between the abundance ratios and condensation temperature in $α$ Cen A akin to that of the Sun. However, taking this finding as evidence for the sequestration of rocky material locked up in planets may be premature given that a clear link between the two phenomena remains to be established. The similarity between the abundance pattern of the binary components argues against the swallowing of a massive planet by one of the stars after the convective zones have shrunk to their present-day sizes.
description: Accepted for publication in A&A. 24 pages, 8 figures. Abstract abridged
Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
Creators: name: Garratt-Smithson, L.
name: Wynn, G. A.
name: Power, C.
name: Nixon, C. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the effects of gradual heating on the evolution of turbulent molecular clouds of mass $2\times 10^6$ M$_\odot$ and virial parameters ranging between $0.7-1.2$. This gradual heating represents the energy output from processes such as winds from massive stars or feedback from High Mass X-ray binaries (HMXBs), contrasting the impulsive energy injection from supernovae (SNe). For stars with a mass high enough that their lifetime is shorter than the life of the cloud, we include a SN feedback prescription. Including both effects, we investigate the interplay between slow and fast forms of feedback and their effectiveness at triggering/suppressing star formation. We find that SN feedback can carve low density chimneys in the gas, offering a path of least resistance for the energy to escape. Once this occurs the more stable, but less energetic, gradual feedback is able to keep the chimneys open. By funneling the hot destructive gas away from the centre of the cloud, chimneys can have a positive effect on both the efficiency and duration of star formation. Moreover, the critical factor is the number of high mass stars and SNe (and any subsequent HMXBs) active within the free-fall time of each cloud. This can vary from cloud to cloud due to the stochasticity of SN delay times and in HMXB formation. However, the defining factor in our simulations is the efficiency of the cooling, which can alter the Jeans mass required for sink particle formation, along with the number of massive stars in the cloud.
description: 35 pages, 46 figures, accepted for publication in MNRAS
Implications of using systematic decomposition structures to organize building LCA information: A comparative analysis of national standards and guidelines- IEA EBC ANNEX 72
Creators: name: Soust-Verdaguer, B.
name: García Martínez, A.
name: Llatas, C.
name: Gómez De Cózar, J. C.
name: Allacker, K.
name: Trigaux, D.
name: Alsema, E.
name: Berg, B.
name: Dowdell, D.
name: Debacker, W.
name: Frischknecht, R.
name: Ramseier, L.
name: Veselka, J.
name: Volf, M.
name: Hajek, P.
name: Lupíšek, A.
name: Malik, Z.
name: Habert, G.
name: Hollberg, A.
name: Lasvaux, S.
name: Peuportier, B.
name: Pomponi, F.
name: Wastiel, L.
name: Gomes, V.
name: Zara, O.
name: Gomes, M.
name: Gusson Baiocchi, A.
name: Pulgrossi, L.
name: Ouellet-Plamondon, C.
name: Moncaster, A.
name: Bari, R. Di
name: Horn, R.
name: Lenz, K.
name: Balouktsi, Maria
name: Lützkendorf, Thomas
name: Röck, M.
name: Hoxha, E.
name: Passer, A.
Publisher: name: IOP Publishing
Year: 2020

description: The application of the Life Cycle Assessment (LCA) technique to a building requires the collection and organization of a large amount of data over its life cycle. The systematic decomposition method can be used to classify building components, elements and materials, overcome specific difficulties that are encountered when attempting to complete the life cycle inventory and increase the reliability and transparency of results. In this paper, which was developed in the context of the research project IEA EBC Annex 72, we demonstrate the implications of taking such approach and describe the results of a comparison among different national standards/guidelines that are used to conduct LCA for building decomposition. Methods: We initially identified the main characteristics of the standards/guidelines used by Annex participant countries. The "be2226" reference office building was used as a reference to apply the different national standards/guidelines related to building decomposition. It served as a basis of comparison, allowing us to identify the implications of using different systems/standards in the LCA practice, in terms of how these differences affect the LCI structures, LCA databases and the methods used to communicate results. We also analyzed the implications of integrating these standards/guidelines into Building Information Modelling (BIM) to support LCA. Results: Twelve national classification systems/standards/guidelines for the building decomposition were compared. Differences were identified among the levels of decomposition and grouping principles, as well as the consequences of these differences that were related to the LCI organization. In addition, differences were observed among the LCA databases and the structures of the results. Conclusions: The findings of this study summarize and provide an overview of the most relevant aspects of using a standardized building decomposition structure to conduct LCA. Recommendations are formulated on the basis of these findings.
Quark Mass Matrix with a Structure of a Rank One Matrix Plus a Unit Matrix
Creators: name: Fusaoka, H.
name: Koide, Y.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A quark mass matrix model $M_q=M_e^{1/2} O_q M_e^{1/2} $ is proposed where $M_e^{1/2}={\rm diag}(\sqrt{m_e},\sqrt{m_μ},\sqrt{m_τ})$ and $O_q$ is a unit matrix plus a rank one matrix. Up- and down-quark mass matrices $M_u$ and $M_d$ are described in terms of charged lepton masses and additional three parameters (one in $M_u$ and two in $M_d$). The model can predict reasonable quark mass ratios (not only $m_u/m_c$, $m_c/m_t$, $m_d/m_s$ and $m_s/m_b$, but also $m_u/m_d$) and Kobayashi-Maskawa matrix elements.
description: 8 pages, Latex, no figures
Hierarchical Quark Mixing and Bimaximal Lepton Mixing on the Same Footing
Creators: name: Kim, C. S.
name: Kim, J. D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that not only the hierarchical quark CKM mixing matrix but also the "bimaximal" lepton flavor mixing matrix can be derived from the same mass matrix ansatz based on the broken permutation symmetry, by assuming the hierarchy of neutrino masses to be $m_1\simeq m_2 <
description: 12 Pages, LaTeX, no figures, corrected hep-ph number and a PACS number
Kinematics of the Galaxy from OB Stars with Data from the Gaia DR2 Catalogue
Creators: name: Bobylev, V. V.
name: Bajkova, A. T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have selected and analyzed a sample of OB stars with known line-of-sight velocities determined through ground-based observations and with trigonometric parallaxes and proper motions from the Gaia DR2 catalogue. Some of the stars in our sample have distance estimates made from calcium lines. A direct comparison with the trigonometric distance scale has shown that the calcium distance scale should be reduced by 13\%. The following parameters of the Galactic rotation curve have been determined from 495 OB stars with relative parallax errors less than 30\%: $(U,V,W)_\odot=(8.16,11.19,8.55)\pm(0.48,0.56,0.48)$ km s$^{-1}$, $Ω_0=28.92\pm0.39$ km s$^{-1}$ kpc$^{-1}$, $Ω^{'}_0=-4.087\pm0.083$ km s$^{-1}$ kpc$^{-2}$ and $Ω^{''}_0=0.703\pm0.067$ km s$^{-1}$ kpc$^{-3}$, where the circular velocity of the local standard of rest is $V_0=231\pm5$ km s$^{-1}$ (for the adopted $R_0=8.0\pm0.15$ kpc). The parameters of the Galactic spiral density wave have been found from the series of radial, $V_R,$ residual tangential, $ΔV_{circ}$, and vertical, $W,$ velocities of OB stars by applying a periodogram analysis. The amplitudes of the radial, tangential, and vertical velocity perturbations are $f_R=7.1\pm0.3$ km s$^{-1}$, $f_θ=6.5\pm0.4$ km s$^{-1}$, and $f_W=4.8\pm0.8$ km s$^{-1}$, respectively; the perturbation wavelengths are $ λ_R=3.3\pm0.1$ kpc, $λ_θ=2.3\pm0.2$ kpc, and $ λ_W=2.6\pm0.5$ kpc; and the Sun's radial phase in the spiral density wave is $ (χ_\odot)_R=-135\pm5^\circ$, $(χ_\odot)_θ=-123\pm8^\circ$, and $ (χ_\odot)_W=-132\pm21^\circ$ for the adopted four-armed spiral pattern.
description: 16 pages,6 figures, 1 table
Hidden Symmetry of the Yang--Coulomb System
Creators: name: Mardoyan, L. G.
name: Sissakian, A. N.
name: Ter--Antonyan, V. M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The bound system composed of the Yang monopole coupled to a particle of the isospin by the SU(2) and Coulomb interaction is considered. The generalized Runge--Lenz vector and the SO(6) group of hidden symmetry are established. It is also shown that the group of hidden symmetry make it possible to calculate the spectrum of the system by a pure algebraic method.
description: 6 pages, LaTeX file
Developing a Game (Inner Dragon) Within a Leading Smartphone App for Smoking Cessation: Design and Feasibility Evaluation Study
Creators: name: White, JS
name: Salem, MK
name: Toussaert, S
name: Westmaas, J Lee
name: Raiff, BR
name: Crane, D
name: Warrender, E
name: Lyles, C
name: Abroms, L
name: Thrul, Johannes
Publisher: name: La Trobe
Year: 2024
Subjects: classificationCode: 360502
subject: Computer gaming and animation

description: Background: Several stand-alone smartphone apps have used serious games to provide an engaging approach to quitting smoking. So far, the uptake of these games has been modest, and the evidence base for their efficacy in promoting smoking cessation is still evolving. The feasibility of integrating a game into a popular smoking cessation app is unclear. Objective: The aim of this paper was to describe the design and iterative development of the Inner Dragon game within Smoke Free, a smartphone app with proven efficacy, and the results of a single-arm feasibility trial as part of a broad program that seeks to assess the effectiveness of the gamified app for smoking cessation. Methods: In phase 1, the study team undertook a multistep process to design and develop the game, including web-based focus group discussions with end users (n=15). In phase 2, a single-arm study of Smoke Free users who were trying to quit (n=30) was conducted to assess the feasibility and acceptability of the integrated game and to establish the feasibility of the planned procedures for a randomized pilot trial. Results: Phase 1 led to the final design of Inner Dragon, informed by principles from psychology and behavioral economics and incorporating several game mechanics designed to increase user engagement and retention. Inner Dragon users maintain an evolving pet dragon that serves as a virtual avatar for the users’ progress in quitting. The phase-2 study established the feasibility of the study methods. The mean number of app sessions completed per user was 13.8 (SD 13.1; median 8; range 1-46), with a mean duration per session of 5.8 (median 1.1; range 0-81.1) minutes. Overall, three-fourths (18/24, 75%) of the participants entered the Inner Dragon game at least once and had a mean of 2.4 (SD 2.4) sessions of game use. The use of Inner Dragon was positively associated with the total number of app sessions (correlation 0.57). The mean satisfaction score of participants who provided ratings (11/24, 46%) was 4.2 (SD 0.6) on a 5-point scale; however, satisfaction ratings for Inner Dragon were only completed by 13% (3/24) of the participants. Conclusions: Findings supported further development and evaluation of Inner Dragon as a beneficial feature of Smoke Free. The next step of this study is to conduct a randomized pilot trial to determine whether the gamified version of the app increases user engagement over a standard version of the app.
Cooperative reliable response from sloppy gene-expression dynamics
Creators: name: Inoue, Masayo
name: Kaneko, Kunihiko
Publisher: name: arXiv
Year: 2018
Subjects: subject: Molecular Networks (q-bio.MN)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Gene expression dynamics satisfying given input-output relationships were investigated by evolving the networks for an optimal response. We found three types of networks and corresponding dynamics, depending on the sensitivity of gene expression dynamics: direct response with straight paths, amplified response by a feed-forward network, and cooperative response with a complex network. When the sensitivity of each gene's response is low and expression dynamics is sloppy, the last type is selected, in which many genes respond collectively to inputs, with local-excitation and global-inhibition structures. The result provides an insight into how a reliable response is achieved with unreliable units, and on why complex networks with many genes are adopted in cells.
X-ray Shapes of Distant Clusters: the Connection to Blue Galaxy Fractions
Creators: name: Wang, Q. Daniel
name: Ulmer, Melville P.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Based on ROSAT PSPC pointed observations, we have determined the aggregate X-ray shapes of 10 distant (z = 0.17-0.54) rich clusters: A2397, A222, A520, A1689, A223B, A1758, A2218, A2111, A2125, and CL0016+16. Four of the clusters have global X-ray ellipticities greater than 0.2, as measured on a scale of diameter 3 h_{50}^{-1} Mpc. These strongly elongated clusters tend to show substantial amounts of substructure, indicating that they are dynamically young systems. Most interestingly, the global X-ray ellipticities of the clusters correlate well with their blue galaxy fractions; the correlation coefficient is 0.75 with a 90% confidence range of 0.44-0.92. This correlation suggests that blue cluster galaxies originate in the process of cluster formation, and that the blue galaxy proportion of a cluster decreases as the intracluster medium relaxes onto equipotential surfaces.
description: Submitted to ApJL, 9 pages including 2 figures
Audit of tenecteplase in ST-segment-elevation myocardial infarction in a secondary hospital in Malaysia: A retrospective case series
Creators: name: Chua, Kin Wei
name: Sreevali Muthuvadivelu
name: Rosilawati Abdul Rani
name: Siew Chin Ong
name: Narwani Hussin
name: Wee Kooi Cheah
Publisher: name: Zenodo
Year: 2020
Subjects: Tenecteplase
ST-segment-elevation myocardial infarction
Retrospective
Case Series
Malaysia
Myocardial infarction
Secondary Hospital
Audit

description: Introduction Little is known about the impacts of tenecteplase(TNK) on clinical outcomes in Malaysia. We aimed to evaluate the effectiveness and safety of TNK in patients presenting with ST-segment-elevation myocardial infarction (STEMI) in clinical practice at Taiping Hospital. Materials and Methods This was a single-center retrospective case series based on medical records of STEMI patients who were admitted to the cardiac care unit at Taiping Hospital between January 2016 and May 2019. The mortality status and date were obtained via data linkage with the National Registration Department of Malaysia. Results Data of 30 patients with STEMI who were administered weight-adjusted TNK were analyzed. The patients’ mean age was 62 years(SD±14years), and 77% of them were males. The median time-to-treatment(TTT) was 265min(IQR 228,660) and the clinically successful thrombolysis(CST) rate was 79%. The overall all-cause in-hospital mortality rate was 33%. The patients with TTT360 min(50%)(p=0.12). Kaplan-Meier curves showed relatively higher 30-day- and 1-year-survival values in patients with TTT<=360 min(p=0.20 and p=0.03, respectively). There was only 1 case(3%) of major bleeding requiring blood transfusion(HAS-BLED score=5). No instances of ischemic stroke, non-major bleeding, in-hospital reinfarction, and allergic reaction were reported. Conclusion The mortality-related outcomes of TNK in STEMI were influenced by TTT, with TTT<=360min providing better prognosis. The bleeding-related complications caused by TNK were minimal, if administered to low-risk patients. Further study is needed to compare its profile with that of streptokinase, which is commonly used in the current clinical practice.
Heavy Higgs production and decay via $e^+e^-\to Z^0 H^0 \to b\bar bZ^0Z^0$ and irreducible backgrounds at Next Linear Colliders
Creators: name: Moretti, Stefano
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The complete matrix element for $e^+e^-\ar b\bar bZ^0Z^0$ has been computed at tree--level and applied to $Z^0H^0$--production followed by $Z^0\ar b\bar b$ and $H^0\ar Z^0Z^0$, including all the irreducible background, at Next Linear Colliders. We find that, assuming flavour identification of the $Z^0$--decay products, this channel, together with $e^+e^-\ar b\bar bW^+W^-$ in which $Z^0H^0\ar (b\bar b)(W^+W^-$), can be important for the study of the parameters of the Standard Model Higgs boson over the heavy mass range $2M_{Z^0}\Ord M_{H^0}\Ord 2{m_t}$.
description: 24 pages, LaTeX (uses Feynman), 7 figures (.ps files or hardcopies of figs.2-7 available upon request)
SO(3) Gauge model for neutrino masses and oscillations
Creators: name: Wu, Yue-Liang
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I mainly describe neutrino masses and oscillations in the gauge model with $SO(3)_{F}$ lepton flavor symmetry and with two Higgs triplets. It is shown how the maximal mixing between $ν_μ$ and $ν_τ$ neutrinos comes out naturally after spontaneous breaking of the symmetry. The nearly two-flavor mixing scenario is resulted naturally from an approximate permutation symmetry between the two Higgs triplets. The hierarchy between the neutrino mass-squared differences, which is needed for reconciling both solar and atmospheric neutrino data, leads to an almost maximal mixing between $ν_{e}$ and $ν_μ$ neutrinos. Thus the model favors the intriguing bi-maximal mixing scenario.The three Majorana neutrino masses are allowed to be nearly degenerate and large enough to play a significant cosmological role. The model can also lead to interesting phenomena on lepton-flavor violations via the $SO(3)_{F}$ gauge interactions.
description: latex, no figures, invited talk at the Sixth Topical Seminar on Neutrino and Astroparticle Physics, San Miniato, Italy, May 1999, to appear in Nucl. Phys. B (Proc. Suppl.)
MPEC 2024-D57 : 2024 DL
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 DL

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
[Querido hijo : Adoro los dulces, soy un consumidor contumáz de dulces]
Creators: name: Manuel, Vázquez Portal
name: Vázquez Portal, Manuel
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: Prison de Boniato
Conditions de détention

description: Destinataire : Cervantes García, Agustín
description: Description : L'auteur de la lettre le remercie pour son envoi de friandises. Il évoque : la liberté, leur lutte, Cuba, la patrie, son frère Jorge, une société libre et juste, et fait un éloge de son correspondant. Il souligne son importance dans la lutte contre leurs oppresseurs et qu'il pense publier ses lettres. Il lui demande de faire sortir cette lettre afin qu'elle soit publiée (note verticale marge gauche de la dernière page).
description: Notes : Lettre envoyée depuis la Prison de Aguadores. Numérotation des pages avec des chiffres encerclés dans la marge supérieure, au stylo noir. Sur la quatrième page, dans la marge supérieure, les annotations : 'Yolanda' et 'Hector Macello 873 4165', au stylo bleu.
description: Source: Cote : MVP-B-2003-09-10
description: Source: Localisation du document : États-Unis, Miami (Floride)
title: ADCO, Cartulaire de Fontenay, premier fragment (XIIIe siècle), Cart. 201 (15 H 9), 175 folios, f. 003v
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/2009
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios, f. 003v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
Dorylus atriceps Shuck
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1877
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Dorylus
Dorylus atriceps

description: 32. Dorylus atriceps Shuck.
Ann. of nat. hi'st. V. 1840. 323. Ainsaba (Beccavi); un solo.
Questo esemplare e di colore assai piu chiaro di quello descritto dal Shuckard, ma dc 1 resto e conforme alla descrizione; tutto testaceo, col capo piceo, gli scapi e le mandibole ferruginei; 1 ' ala anteriore destra offre un rudimento di una 2. a costola ricorrente (Shuckard nota l'istessa anomalia nell' ala sinistra del suo esemplare).
(Estratto dagli Annali del Mus. Civ. di St. Nat. di Genova, Vol. IX, 1876 - 77 â 27 Marzo - 3 Aprile 1877).
Genova. Tip. Sordo-muti.
description: Published as part of Emery, C., 1877, Catalogo delle formiche esistenti nelle collezioni del Museo Civico di Genova. Parte prima. Formiche provenienti dall Viaggio dei signori Antinori, Beccari e Issel nel Mar Rosso e nel paese dei Bogos., pp. 363-381 in Annali del Museo Civico di Storia Naturale Giacomo Doria (Genova) 9 on pages 363-381
Reacting fluids in the expanding Universe: A new mechanism for entropy production
Creators: name: Zimdahl, Winfried
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It is shown that two reacting cosmological fluids, each of them perfect on its own, which exchange energy and momentum without preserving particle numbers, give rise to an entropy producing `reactive' bulk stress of the system as a whole, as soon as the detailed balance between decay and inverse decay processes is perturbed. This demonstrates explicitly that particle generation is dynamically equivalent to an effective bulk pressure. We derive a semiquantitative formula for the corresponding new kinetic coefficient and evaluate the latter for the out-of-equilibrium decay of heavy, nonrelativistic particles into radiation. It turns out that the associated reactive bulk viscosity may be more than one order of magnitude larger than the conventional bulk viscosity, calculated, e.g., in radiative hydrodynamics.
description: 13 pages, Revtex, submitted to MNRAS
Additional file 4: of Body proportions for the facilitation of walking, running and flying: the case of partridges
Creators: name: JesĂşs Nadal
name: Ponz, Carolina
name: Margalida, Antoni
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Covariance analysis for pairs of parameters. (DOCX 26â kb)
Monomorium gracillimum Smith
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1877
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Monomorium
Monomorium gracillimum

description: M. gracillimum Smith
Proc. Lin. Soc. Zool. 1 S 61, 34 Â« (Myrmica) - [[worker]]. Laevissima, testacea, abdomine fusco, basi pallescente, capite latiusculo, latitudine vix longiore, lateribus rotundata, postice vix emarginato, sparse subtiliter punctato, antennis gracilibus, thorace impresso, nodis subaequalibus angustis. hong. 2 â 2,6 millim. [[queen]]. Testacea, regione oculorum fusca, thoracis dorso, nodis et abdomine magis miuusve brunnescentibus, pedibuspaludis, capite parce grosse punctata, antennis gracilibus, scapo regionem ocellorum superante. Long. 0,5 â 7 millim.; alae hyalinae costis dilutis, absque cellula discoidali. [[male]]. Brunneus, capite fusco, antennis pedibusque dilute flavis, capite trapezoidea, antennis gracillbus, apice attenuatis, scapo articulo flagelli primo vix sesqui-longiore. Long. 3,2 millim. Gerusalemme (De Saulcy). La [[worker]] si distingue da quella del M. basale pel capo pia breve, piu rotondato sui lati, meno scavato in dietro e per le antenne piu gracili.
description: Published as part of Emery, C., 1877, Catalogo delle formiche esistenti nelle collezioni del Museo Civico di Genova. Parte prima. Formiche provenienti dall Viaggio dei signori Antinori, Beccari e Issel nel Mar Rosso e nel paese dei Bogos., pp. 363-381 in Annali del Museo Civico di Storia Naturale Giacomo Doria (Genova) 9 on pages 363-381
Non-abelian gauge theories as a consequence of perturbative quantum gauge invariance
Creators: name: Aste, Andreas
name: Scharf, G"unter
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show for the case of interacting massless vector bosons, how the structure of Yang-Mills theories emerges automatically from a more fundamental concept, namely perturbative quantum gauge invariance. It turns out that the coupling in a non-abelian gauge theory is necessarily of Yang-Mills type plus divergence- and coboundary couplings. The extension of the method to massive gauge theories is briefly discussed.
description: 12 pages, latex, no figures
The Cosmic Evolution of Magnesium Isotopes
Creators: name: Vangioni, E.
name: Olive, K. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The abundance of magnesium in the interstellar medium is a powerful probe of star formation processes over cosmological timescales. Magnesium has three stable isotopes, 24Mg, 25Mg, 26Mg, which can be produced both in massive and intermediate-mass (IM) stars with masses between 2 and 8 M_\odot. In this work, we use constraints on the cosmic star formation rate density (SFRD) and explore the role and mass range of intermediate mass stars using the observed isotopic ratios. We compare several models of stellar nucleosynthesis with metallicity-dependent yields and also consider the effect of rotation on the yields massive stars and its consequences on the evolution of the Mg isotopes. We use a cosmic evolution model updated with new observational SFRD data and new reionization constraints coming from 2018 Planck collaboration determinations. We find that the main contribution of 24Mg comes from massive stars whereas 25Mg and 26Mg come from intermediate mass stars. To fit the observational data on magnesium isotopic ratios, an additional intermediate mass SFRD component is preferred. Moreover, the agreement between model and data is further improved when the range of IM masses is narrowed towards higher masses (5-8 M_\odot). While some rotation also improves the fit to data, we can exclude the case where all stars have high rotational velocities due to an over-production of 26Mg.
description: 12 pages, 17 figures
Camponotus angusticeps Emery, 1886, n. sp.
Creators: name: Emery, C.
Publisher: name: Zenodo
Year: 1886
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Camponotus
Camponotus angusticeps

description: 1. Camponotus angusticeps n. sp.
[[worker]] minor. Nigra, mandibulis, articalationibus pedum tar sisque piceo-ru-fescentibus, opaca, creberrime punctata, sparse pilosa, pube adpressa, in abdomine densissima ibique und ' neo-sericea; caput latitudine maxima plus duplo longius (fig. 1),. lateribus subrectis, fere parallelus, postico trun-catum, angiitis rotundatus; mandibulae 7 - dentatae, dente apicali magno, acuto, subtilissime punctatae et punctis majoribus piligeris sparsae; clypeus carinatus, antice lobatus; area frontalis indistincta; thorax dorso aequali, arcuato; squama ovata later aliter visa cunei formis: pedes graciles. L. 7 1 / 2 â 8 1 / 2 mm.
Por la densa pubescenza ricorda il C. micans Nyl. ed ha uno splendore sericeo marezzato ancora piu intenso e di colore grigio bronzino. La forma del capo e affatto speciale e non rassomiglia a quella di nessun altro Camponotus a me noto. Ho veduto due soli esemplari che mi pare siano [[worker]] minori. Rimano problematica la forma dell' [[worker]] maggiore.
description: Published as part of Emery, C., 1886, Alcune formiche africane., pp. 355-366 in Bollettino della Societa Entomologica Italiana 18 on page 355
The HI content of dark matter halos at $z\approx 0$ from ALFALFA
Creators: name: Obuljen, Andrej
name: Alonso, David
name: Villaescusa-Navarro, Francisco
name: Yoon, Ilsang
name: Jones, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We combine information from the clustering of HI galaxies in the 100% data release of the Arecibo Legacy Fast ALFA survey (ALFALFA), and from the HI content of optically-selected galaxy groups found in the Sloan Digital Sky Survey (SDSS) to constrain the relation between halo mass $M_h$ and its average total HI mass content $M_{\rm HI}$. We model the abundance and clustering of neutral hydrogen through a halo-model-based approach, parametrizing the $M_{\rm HI}(M_h)$ relation as a power law with an exponential mass cutoff. To break the degeneracy between the amplitude and low-mass cutoff of the $M_{\rm HI}(M_h)$ relation, we also include a recent measurement of the cosmic HI abundance from the $α$.100 sample. We find that all datasets are consistent with a power-law index $α=0.44\pm 0.08$ and a cutoff halo mass $\log_{10}M_{\rm min}/(h^{-1}M_\odot)=11.27^{+0.24}_{-0.30}$. We compare these results with predictions from state-of-the-art magneto-hydrodynamical simulations, and find both to be in good qualitative agreement, although the data favours a significantly larger cutoff mass that is consistent with the higher cosmic HI abundance found in simulations. Both data and simulations seem to predict a similar value for the HI bias ($b_{\rm HI}=0.875\pm0.022$) and shot-noise power ($P_{\rm SN}=92^{+20}_{-18}\,[h^{-1}{\rm Mpc}]^3$) at redshift $z=0$.
description: 17 pages, 11 figures. Comments welcome