cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A network-based analysis of the cellular and genetic etiology of disease
Creators: name: Cornish, Alexander John
Publisher: name: Imperial College London
Year: 2016

description: Thousands of disease-associated loci have been identified in genome-wide association studies (GWAS). These loci can span multiple genes and identifying which, if any, of these genes are causal can be challenging. Multiple methods have been developed to identify causal genes, some of which use networks of physical interactions between proteins. The performance of many of these methods may however be limited by their failure to use data specific to the tissues and cell types that manifest each disease. Furthermore, many network-based approaches may be biased towards better-studied genes. In order to use data specific to a disease-manifesting cell type to identify disease- associated genes, it is first necessary to identify the disease-manifesting cell types. In this thesis, I report the development of the GSC (Gene Set Compactness) and GSO (Gene Set Overexpression) methods, which I use to identify associations between 352 diseases and 73 cell types. The GSC method identifies these associations using cell-type-specific protein-protein interaction (PPI) networks, which I generate by integrating PPI and gene expression data. Using text mining, it is demonstrated that these methods identify a large number of well-characterised disease-cell-type associations and associations that warrant further investigation. I also describe the development of ALPACA (Analysing Loci using Phenotypic And Cellular Associations), which identifies disease-associated genes using cell-type- specific PPI networks and phenotype data from humans and mice. I demonstrate that by taking a permutation-based approach, ALPACA avoids being biased towards better-studied genes. Furthermore, I demonstrate that using cell-type-specific networks, instead of generic networks, improves method performance. As the number of available tissue and cell-type-specific data continues to increase, methods that integrate these data will become increasingly important in understanding disease etiology.
Emex spinosa Campd.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Emex
Emex spinosa

description: Rumex spinosus Linnaeus, Species Plantarum 1: 337. 1753.
"Habitat in Creta." RCN: 2599.
Lectotype (Graham in Turrill & Milne-Redhead, Fl. Trop. E. Africa, Polygonaceae: 3. 1958): Herb. Linn. No. 464.36 (LINN).
Current name: Emex spinosa (L.) Campd. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 804, DOI: 10.5281/zenodo.291971
Search for the decay of a Higgs boson in the $\ell\ellγ$ channel in proton-proton collisions at $\sqrt{s} =$ 13 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A search for a Higgs boson decaying into a pair of electrons or muons and a photon is described. Higgs boson decays to a Z boson and a photon (H $\to$ Z$γ\to\ell\ellγ$, $\ell =$ e or $μ$), or to two photons, one of which has an internal conversion into a muon pair (H $\toγ^{*}γ\toμμγ$) were considered. The analysis is performed using a data set recorded by the CMS experiment at the LHC from proton-proton collisions at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosity of 35.9 fb$^{-1}$. No significant excess above the background prediction has been found. Limits are set on the cross section for a standard model Higgs boson decaying to opposite-sign electron or muon pairs and a photon. The observed limits on cross section times the corresponding branching fractions vary between 1.4 and 4.0 (6.1 and 11.4) times the standard model cross section for H $\toγ^{*}γ\toμμγ$ (H $\to$ Z$γ\to\ell\ellγ$) in the 120-130 GeV mass range of the $\ell\ellγ$ system. The H $\toγ^*γ\toμμγ$ and H $\to$ Z$γ\to\ell\ellγ$ analyses are combined for $m_\mathrm{H} =$ 125 GeV, obtaining an observed (expected) 95% confidence level upper limit of 3.9 (2.0) times the standard model cross section.
description: Replaced with the published version. Added the journal reference and the DOI. All the figures and tables can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/HIG-17-007 (CMS Public Pages)
Thasian Laws Concerning Wine and Vineyards
Creators: name: Perucca, Alessandro
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description: Engraved on this epigraph from Thasos are two laws promulgated within a short period of time between the end of the fifth and the beginning of the fourth century BC. Both deal with viticulture and the production of and trade in wine, a subject that is not new in Thasian legislation and which must have represented an important economic sector for the island. It seems clear that the main purpose of these laws was to prevent fraud concerning quantity, quality or terms of sale of the wine, although the loss of large sections of the inscription makes a complete understanding difficult.
description: Axon
Bwt fluctuation_Supplemental Table-JCEM.docx
Creators: name: Oh, Tae Jung
name: Moon, Jae Hoon
name: Choi, Sung Hee
name: Lim, Soo
name: Park, Kyong Soo
name: Cho, Nam H.
name: Jang, Hak Chul
Publisher: name: figshare
Year: 2018
Subjects: subject: 110306 Endocrinology
subject: FOS: Clinical medicine

description: ContextBody-weight fluctuation (weight cycling) has been found to be associated with higher mortality and cardiovascular events in patients with coronary artery disease. However, there are very limited data regarding the relationship between body-weight fluctuation and health-related outcomes in the general population.MethodsWe examined whether body-weight fluctuation can associate incident diabetes mellitus and cardiovascular events, and mortality in a Korean population from the Korean Genome and Epidemiology Study. The intra-individual fluctuations of body weight were calculated by average successive variability (ASV), and health-related outcomes were collected every 2 years for 16 years in 3,678 participants.ResultsParticipants with a high ASV of body weight were more obese and had higher blood pressure and HbA1c levels at baseline than those with a low ASV of body weight. A one-unit increase in ASV of body weight was associated with increase in mortality (HR 1.46, 95% CI 1.32-1.62, P < 0.001). However, the association between the ASV of body weight and incident diabetes mellitus seemed to be influenced by baseline body mass index (BMI); negative effect in subjects with BMI < 25 kg/m2 (HR 1.36, 95% CI 1.11-1.65, P = 0.003) and protective effect in those with BMI ≥ 25 kg/m2 (HR 0.76, 95% CI 0.60-0.95, P = 0.014). There was no association between the ASV of body weight and cardiovascular event. ConclusionBody-weight fluctuation was associated with mortality. In addition, the effect of body-weight fluctuation on incident diabetes mellitus depended on the presence of obesity at baseline.
Interpretation of the galaxy structure surrounding the Local Supercluster
Creators: name: Paturel, Georges
name: Di Nella, Hélène
name: Theureau, Jean-Noël Terry et Gilles
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: After numerical simulations by E. Praton, we interprete the cocoon-like structure observed for the distribution of galaxies around us as an effect of infall velocities onto clusters. In this view structures like the Cocoon (or even like the Great-Wall) could be interpreted as observationnal artefacts.
description: 7 pages, 6 figures accepted by Comptes rendus de l'academie des sciences, Paris
Post Big Bang Processing of the Primordial Elements
Creators: name: Balbes, M. J.
name: Boyd, R. N.
name: Steigman, G.
name: Thomas, D.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore the Gnedin-Ostriker suggestion that a post-Big-Bang photodissociation process may modify the primordial abundances of the light elements. We consider several specific models and discuss the general features that are necessary (but not necessarily sufficient) to make the model work. We find that with any significant processing, the final D and $^3$He abundances, which are independent of their initial standard big bang nucleosynthesis (SBBN) values, rise quickly to a level several orders of magnitude above the observationally inferred primordial values. Solutions for specific models show that the only initial abundances that can be photoprocessed into agreement with observations are those that undergo virtually no processing and are already in agreement with observation. Thus it is unlikely that this model can work for any non-trivial case unless an artificial density and/or photon distribution is invoked.
description: 12 page Latex file (AASTEX style). Tarred, gzipped, and uuencoded postscript files of seven figures. Also available (with ps file of paper) at ftp://www-physics.mps.ohio-state.edu/pub/nucex/photo
Investigation of the nucleotide triphosphate diffusion into the active site of RNA polymerase
Creators: name: Genin, Nicolas Edmond
Publisher: name: Imperial College London
Year: 2016

description: RNA Polymerase can be seen as a mobile molecular structure orchestrating the movement of substrate NTP and nucleic acids, regulated by some control molecules (transcription factors) and the sequential interplay of the enzyme domains. For the last 15 years, loading of rNTPs into the active site of the enzymatic complex has been regarded more or less as a settled issue. Based on the first generated crystal structures, substrates were thought to load via a pathway termed secondary channel (CH2). The latter well-accepted paradigm regarding a fundamental aspect of the transcription process is refuted and a new model, relying on overlooked structural characteristics (CH3, CH4), and accommodating a large body of pre-existing information, is presented. Important implications involve notably the fact that CH2 is mainly an exit channel, and that NTPs are selected prior to delivery into the catalytic center. Overlapping partially with the new loading hypotheses, details about substrate discrimination, error recovery and the translocation mechanism, which has been an open question in the domain for the past 20 years, are discussed. Accelerated and Steered Molecular Dynamics simulations are computed and enable to gain informative insight about the dynamics of the diffusion process. In-depth conformational and electrostatic analyses are discussed and allow gauging propensity for substrate accommodation.
Janssen-Cilag - Karine Tabet
Creators: name: Leibowitch, Jacques (1942-2020)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: 1 fichier (13 pages).
description: 2 pièces jointes : diaporama sur ICCARRE et article de J. Leibowitch, et al., "Short cycles of antiretroviral drugs provide intermittent yet effective therapy: a pilot study in 48 patients with chronic HIV infection " paru dans le Faseb Journal en 2010..
Molecular Gas in the Perseus Cooling Flow Galaxy, NGC 1275
Creators: name: Bridges, Terry
name: Irwin, Judith
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The central arcminute of the Perseus cooling flow galaxy, NGC 1275, has been mapped with the JCMT in 12CO(2-1) at 21 arcsec resolution, with detections out to at least 36 arcsec (12 kpc). Within the limits of the resolution and coverage, the distribution of gas appears to be roughly E-W, consistent with previous observations of CO, X-ray, H alpha, and dust emission. The total detected molecular hydrogen mass is ~ 1.6 x 10^10 solar masses, using a Galactic conversion factor. The inner central rotating disk is apparent in the data, but the overall distribution is not one of rotation. Rather, the line profiles are bluewards asymmetric, consistent with previous observations in HI and [OIII]. We suggest that the blueshift may be due to an acquired mean velocity of ~ 150 km/sec imparted by the radio jet in the advancing direction. Within the uncertainties of the analysis, the available radio energy appears to be sufficient, and the interpretation is consistent with that of Bohringer et al. (1993) for displaced X-ray emission. We have also made the first observations of 13CO(2-1) and 12CO(3-2) emission from the central 21 arcsec region of NGC 1275 and combined these data with IRAM data supplied by Reuter et al. (1993) to form line ratios over equivalent, well-sampled regions. An LVG radiative transfer analysis indicates that the line ratios are not well reproduced by a single value of kinetic temperature, molecular hydrogen density, and abundance per unit velocity gradient. At least two temperatures are suggested by a simple two-component LVG model, possibly reflecting a temperature gradient in this region.
description: 12 pages, 5 figures, uses mn.sty, accepted for publication in MNRAS
Rotating stall in variable geometry compressors
Creators: name: Dodds, John
Publisher: name: Imperial College London
Year: 2016

description: The design and operation of gas-turbine engines is heavily influenced by the off-design stability of the compressor, which limits obtainable performance and may result in aeroelastic vibration issues. Whilst Variable Stator Vanes (VSVs) are widely used to mitigate this problem, research considering the mismatching effect of VSVs away from their optimal settings is limited. In this thesis, a high-speed variable geometry compressor is studied at part-speed conditions and VSV setting adjustments are made to deliberately trigger stable rotating stall and study its behaviour. Examination of unsteady measurements reveals two "families'' of rotating stall, each at different frequencies, where the dominant behaviour depends upon the VSV settings. Stall in the front stage is shown to consist of a spatially non-uniform and time-varying pattern of short lengthscale cells, which couple with rotor vibration and propagate as noise. Second stage stall is a longer lengthscale uniform disturbance consisting of fewer stall cells. The stalling pressure amplitudes are also found to correlate well to blade loading parameters from a one-dimensional meanline model. Steady and unsteady CFD simulations at these stalled conditions confirm that the behaviour is due to regions of stall in the front stage tip region together with the hub of the second stage. These CFD calculations naturally result in the formation of stall cells and give a credible match to the experiment. Inviscid reasoning explains how this flowfield is due to spanwise static pressure gradients arising from part-speed closure of the VSVs. Finally, the non-dimensional cell propagation speed (Vstall/U) for each family of stall is shown to be uniquely determined by the VSV settings. This appears to be linked to the axial flow velocity local to the cell and suggests that cell speed may be restated in a more universal non-dimensional form. Furthermore, simulations show the importance of flowfield coupling mechanisms in determining the number of stall cells, which are also driven largely by the VSV settings.
Additional file 2 of A qualitative study on the involvement of adolescents and young adults (AYAs) with cancer during multiple research phases: “plan, structure, and discuss”
Creators: name: van Ham, Camila Rosalinde
name: Burgers, Vivian Wilhelmina Gerarda
name: Sleeman, Sophia Helena Eva
name: Dickhout, Annemiek
name: Harthoorn, Niels Christiaan Gerardus Laurus
name: Manten-Horst, Eveliene
name: van Eenbergen, Mies Christina
name: Husson, Olga
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: Additional file 2. Research cycle.
Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
Creators: name: Frieman, J.
name: Hill, C.
name: Stebbins, A.
name: Waga, I.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore the cosmological implications of an ultra-light pseudo-Nambu-Goldstone boson. With global spontaneous symmetry breaking scale $f \simeq 10^{18}$ GeV and explicit breaking scale comparable to MSW neutrino masses, $M \sim 10^{-3}$ eV, such a field, which acquires a mass $m_ϕ\sim M^2/f \sim H_0$, would have become dynamical at recent epochs and currently dominate the energy density of the universe. The field acts as an effective cosmological constant for several expansion times and then relaxes into a condensate of coherent non-relativistic bosons. Such a model can reconcile dynamical estimates of the density parameter, $Ω_m \sim 0.2$, with a spatially flat universe, and can yield an expansion age $H_0 t_0 \simeq 1$ while remaining consistent with limits from gravitational lens statistics.
description: 15 pages (including 2 figs.), uuencoded compressed postscript; also available on www at http://www-astro-theory.fnal.gov/ under Publications
Joaquín Torres-García and Guillermo de Torre: An Itinerary in Letters
Creators: name: García-Sedas, Pilar
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description:
This article addresses the epistolary relationship between the Uruguayan painter Joaquín Torres-García and the writer Guillermo de Torre, responsible of the construction of an international intellectual network. Their correspondence shows the intellectual connection between the two in a geographical journey that took them through Spain, France, Argentina, and Uruguay and, at the same time, in an artistic journey that began in 1919 with the emergence of Ultraism. Based on the concepts set out by Hoock-Demarle, the letters object of this study are an essential tool to offer a transnational vision of the mediation work carried out in the field of art theorization and the active participation of both in the circulation of symbolic goods such as books and magazines. This correspondence also reveals aspects of their personalities that shine through moments of indignation and depression, in shared illusions and aspirations that influence the search for a common goal: the theorization of ‘arte nuevo’.

description: Rassegna iberistica
Rumex tingitanus Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex tingitanus

description: Rumex tingitanus Linnaeus, Systema Naturae, ed. 10, 2: 991. 1759.
["Habitat in Barbaria, Hispania. Alstroemer."] Sp. Pl., ed. 2, 1: 479 (1762). RCN: 2595.
Lectotype (Siddiqi & El-Taife in Jafri & El-Gadi, Fl. Libya 106: 21. 1983): Löfling 276a, Herb. Linn. No. 464.28 (LINN).
Current name: Rumex tingitanus L. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 804, DOI: 10.5281/zenodo.291971
The mechanism of energy expenditure of oxyntomodulin
Creators: name: Scott, Rebecca Victoria
Publisher: name: Imperial College London
Year: 2017

description: The gut hormone oxyntomodulin is an attractive potential treatment for obesity as it reduces food intake and increases energy expenditure in rats and in man. However, the mechanisms by which OXM increases energy expenditure are not known. Oxyntomodulin has a short half-life in vivo, so long-acting analogues are being developed for both obesity pharmacotherapy and to help us understand the physiology of OXM. This thesis uses the novel oxyntomodulin analogue, OX2, to investigate the energy expenditure effects of oxyntomodulin. The first part of this thesis shows that OX2 increases energy expenditure acutely, as directly measured in CLAMS metabolic cages. Metabolic cage and pair-feeding studies show this increase in energy expenditure is sustained with prolonged administration of the oxyntomodulin analogue. The increase in energy expenditure occurs via activation of the glucagon receptor, as shown in studies using the GLP-1 antagonist Ex9-39, and comparing OX2 to the GLP-1 specific analogue OX2-Glu3. Metabolic cage data shows that oxyntomodulin increases energy expenditure via altering metabolic processes rather than physical activity. The second part of this thesis investigates which pathways are affected by OXM. Using 6-hydroxydopamine to cause a chemical sympathectomy, this thesis demonstrates that the sympathetic nervous system is important in controlling the energy expenditure effects of OXM. Chronic administration of OX2 suppressed many metabolic pathways, including brown adipose tissue thermogenesis and organ growth. However, protein metabolisms and lipolysis were both increased, leading to a reduction in both body fat and body protein. The final part of this thesis then shows OX2 has acute, as well as chronic, effects on protein metabolism. The findings in this thesis provide a basis for further investigations into the metabolic effects of oxyntomodulin. The thesis also underlines the importance of understanding these processes before oxyntomodulin analogues can be used in the treatment of obesity.
Vibrational spectroscopic characterization, quantum chemical, molecular docking and molecular dynamics investigations of cyclo(L-phenylalanyl-L-proline), an anticancer agent
Creators: name: Oktemer, Tugce Sinem
name: Celik, Sefa
name: Ozel, Aysen E.
name: Akyuz, Sevim
name: Er, Alev
Publisher: name: Taylor & Francis
Year: 2025
Subjects: Biophysics
Biochemistry
Physical Sciences not elsewhere classified
Cell Biology
Pharmacology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Computational Biology

description: The molecular structure and spectral properties of cyclo(L-Phenylalanyl-L-Proline) dipeptide, which has several biological activities, were investigated. Firstly, conformational preference of the cyclo(L-Phenylalanyl-L-Proline) was searched and obtained lowest energy conformer of the cyclic dipeptide was then optimized using Density Functional Theory with wb97xd/6-311++G(d,p) level of theory. A detailed vibrational spectral analysis has been carried out and assignments of the fundamental modes have been proposed. The experimental vibrational wavenumbers of the investigated compound display good agreement with the computed values. The Frontier Molecular Orbitals, Molecular Electrostatic Potential and electronic transitions of the investigated compound were discussed. In addition, the 1H and 13C NMR chemical shifts of the cyclic dipeptide were calculated and the results were compared with the experimental values. Also, to evaluate the anticancer potential, molecular docking studies of cyclo(L-Phenylalanyl-L-Proline) within the ATP-binding sites of both wild type (EGFRWT; ID: 4HJO) and mutant (EGFRT790M; ID: 3W2O) Epidermal Growth Factor Receptor were performed. The results indicated that cyclo(Phe-Pro) has high binding affinities toward both EGFRWT (−6.6 kcal/mol) and EGFRT790M (−7.7 kcal/mol) receptors, thus, has good anticancer activity and also has potential to overcome drug resistance in therapy. Molecular dynamics simulations on cyclo(L-Phenylalanyl-L-Proline)-wild type complex were conducted through a 50-nanosecond timed to investigate the ligand-receptor interactions in more detail, and to determine the binding free energy accurately. The binding free energy of the cyclo(L-Phenylalanyl-L-Proline)-wild type complex was calculated to be −27.18 kcal/mol.
Constraints on the Chemical Enrichment History of the Perseus Cluster of Galaxies from High-Resolution X-ray Spectroscopy
Creators: name: Simionescu, A.
name: Nakashima, S.
name: Yamaguchi, H.
name: Matsushita, K.
name: Mernier, F.
name: Werner, N.
name: Tamura, T.
name: Nomoto, K.
name: de Plaa, J.
name: Leung, S. -C.
name: Bamba, A.
name: Bulbul, E.
name: Eckart, M. E.
name: Ezoe, Y.
name: Fabian, A. C.
name: Fukazawa, Y.
name: Gu, L.
name: Ichinohe, Y.
name: Ishigaki, M. N.
name: Kaastra, J. S.
name: Kilbourne, C.
name: Kitayama, T.
name: Leutenegger, M.
name: Loewenstein, M.
name: Maeda, Y.
name: Miller, E. D.
name: Mushotzky, R. F.
name: Noda, H.
name: Pinto, C.
name: Porter, F. S.
name: Safi-Harb, S.
name: Sato, K.
name: Takahashi, T.
name: Ueda, S.
name: Zha, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: High-resolution spectroscopy of the core of the Perseus Cluster of galaxies, using the $Hitomi$ satellite above 2 keV and the $XMM$-$Newton$ Reflection Grating Spectrometer at lower energies, provides reliable constraints on the abundances of O, Ne, Mg, Si, S, Ar, Ca, Cr, Mn, Fe, and Ni. Accounting for all known systematic uncertainties, the Ar/Fe, Ca/Fe, and Ni/Fe ratios are determined with a remarkable precision of less than 10%, while the constraints on Si/Fe, S/Fe, and Cr/Fe are at the 15% level, and Mn/Fe is measured with a 20% uncertainty. The average biases in determining the chemical composition using archival CCD spectra from $XMM$-$Newton$ and $Suzaku$ range typically from 15-40%. A simple model in which the enrichment pattern in the Perseus Cluster core and the proto-solar nebula are identical gives a surprisingly good description of the high-resolution X-ray spectroscopy results, with $χ^2=10.7$ for 10 d.o.f. However, this pattern is challenging to reproduce with linear combinations of existing supernova nucleosynthesis calculations, particularly given the precise measurements of intermediate $α$-elements enabled by $Hitomi$. We discuss in detail the degeneracies between various supernova progenitor models and explosion mechanisms, and the remaining uncertainties in these theoretical models. We suggest that including neutrino physics in the core-collapse supernova yield calculations may improve the agreement with the observed pattern of $α$-elements in the Perseus Cluster core. Our results provide a complementary benchmark for testing future nucleosynthesis calculations required to understand the origin of chemical elements.
description: MNRAS in press
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Cart. 168 (11 H 66), f. 0187r
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/2010
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0187r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.3 (2e moitié XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 168 (11 H 66), f. 0187r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
The Use of Serious Games as an Educational and Dissemination Tool for Archaeological Heritage
Creators: name: Mariotti, Samanta
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description:

In the last decades, digital technologies have pervaded every aspect of the production of archaeological knowledge and they have been massively used to communicate the past. This contribution analyses the potential and benefits of serious games as they appear a promising tool for engaging the users in active learning of cultural contents, for attracting new audiences and promoting knowledge and awareness around archaeological heritage. Moreover, the need for multidisciplinary collaborations between archaeologists and developers and the necessity of assessment studies on learning levels to implement their effectiveness will be highlighted.

description: magazén
title: Petrae 16/1/9/1
Creators: name: Maurin, Louis
name: Navarro-Caballero, Milagros
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: autel,marbre

description: Source: Ausonius UMR 5607 CNRS - Université Bordeaux Montaigne
description: Coverage: Bordeaux, Aquitaine, France
description: Coverage: antiquité romaine
description: Dédicace à Auguste et au Génie de la cité des Bituriges Vivisques
Additional file 1 of A qualitative study on the involvement of adolescents and young adults (AYAs) with cancer during multiple research phases: “plan, structure, and discuss”
Creators: name: van Ham, Camila Rosalinde
name: Burgers, Vivian Wilhelmina Gerarda
name: Sleeman, Sophia Helena Eva
name: Dickhout, Annemiek
name: Harthoorn, Niels Christiaan Gerardus Laurus
name: Manten-Horst, Eveliene
name: van Eenbergen, Mies Christina
name: Husson, Olga
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: Additional file 1. Interview prompts.
Soft X-ray transient light curves as standard candles: exponential versus linear decays
Creators: name: Shahbaz, T.
name: Charles, P. A.
name: King, A. R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A recent paper by King and Ritter (1998: hereafter KR) proposed that the light curves of soft X-ray transients (SXTs) are dominated by the effect of irradiation of the accretion disc by the central X-rays. This prevents the onset of the cooling wave which would otherwise return the disc to the quiescent state, and so prolongs the outbursts beyond those in dwarf nova discs. KR show that the decay of the resulting X-ray light curve should be exponential or linear depending on whether or not the observed peak X-ray luminosity is sufficient to ionize the outer edge of the accretion disc. Here we examine the observed X-ray decays, and show that they are exponential or linear according as the peak luminosity is greater or smaller than the critical value defined by KR, strongly suggesting that the light curves are indeed irradiation--dominated. We show further that the occurrence of an exponential or linear decay tends to favour the same type of decay in subsequent outbursts, so that systems usually show only one or the other type. We use the equations of KR and the observed X-ray light curve to determine the size $R_{h}$ of the hot disc at the peak of the outburst. For exponential decays, $R_{h}$ is found to be comparable to the circularization radius, as expected since the disc consists entirely of material transferred from the secondary since the previous outburst. Further, $R_h$ is directly proportional to the time at which one sees the secondary maximum ($t_{s}$), as expected if $t_{s}$ is the viscous timescale of the irradiated disc. This implies that the orders of magnitude of the viscosity parameter alpha and disc aspect ratio H/R are such that alpha (H/R)~0.01. Observation of a secondary maximum calibrates the peak luminosity and gives an eqaution for the distance to the source.
description: 7 pages latex, 6 figures, Accepted by MNRAS
Poetry in the Era of Social Networks: The Case of Faraḥ Šammā
Creators: name: De Blasio, Emanuela
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description:

The research focuses on the linguistic and content analysis of the poems of the young poetess of Palestinian origin Faraḥ Šammā. The peculiarity of this artist consists in using the Internet and in particular videos on YouTube to recite her poems orally. As a Spoken Word artist, Faraḥ Šammā has grasped in the tool of video channels the way to transmit her compositions as she does in the course of her live performances. Starting from a reflection on the role of orality and poetry in the Arab cultural tradition and on how this literary form is inserted in the context of the new digital communication media, the work focuses on examining the thematic and linguistic aspects of the selected corpus. The goal is to extend the analysis to other forms of poetry, less conventional but which can help to open a wider glimpse into the knowledge of new literary phenomena in the Arab world.

description: Annali di Ca’ Foscari. Serie orientale
Measurement-based quantum control of mechanical motion
Creators: name: Rossi, Massimiliano
name: Mason, David
name: Chen, Junxin
name: Tsaturyan, Yeghishe
name: Schliesser, Albert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Controlling a quantum system based on the observation of its dynamics is inevitably complicated by the backaction of the measurement process. Efficient measurements, however, maximize the amount of information gained per disturbance incurred. Real-time feedback then enables both canceling the measurement's backaction and controlling the evolution of the quantum state. While such measurement-based quantum control has been demonstrated in the clean settings of cavity and circuit quantum electrodynamics, its application to motional degrees of freedom has remained elusive. Here we show measurement-based quantum control of the motion of a millimetre-sized membrane resonator. An optomechanical transducer resolves the zero-point motion of the soft-clamped resonator in a fraction of its millisecond coherence time, with an overall measurement efficiency close to unity. We use this position record to feedback-cool a resonator mode to its quantum ground state (residual thermal occupation n = 0.29 +- 0.03), 9 dB below the quantum backaction limit of sideband cooling, and six orders of magnitude below the equilibrium occupation of its thermal environment. This realizes a long-standing goal in the field, and adds position and momentum to the degrees of freedom amenable to measurement-based quantum control, with potential applications in quantum information processing and gravitational wave detectors.
description: New version with corrected detection efficiency as determined with a NIST-calibrated photodiode, added references and revised structure. Main conclusions are identical. 41 pages, 18 figures
ZHAOv18-M2-mode-2.mat
Creators: name: Zhao, Zhongxiang
Publisher: name: figshare
Year: 2018
Subjects: subject: Oceanography
subject: FOS: Earth and related environmental sciences

description: An empirical internal tide model for the mode-2 M2 internal tide, constructed using 25 years of satellite altimetry data. The mapping method is described in a paper under review by JGR-Oceans. The model covers the global ocean from -65 to 65 in latitude and 0-360 in longitude. The regular grid is 0.1 degrees by 0.1 degrees. The SSH amplitude is in cm and the phase is in Greenwich.
Galaxy Selection and the Surface Brightness Distribution
Creators: name: McGaugh, S. S.
name: Bothun, G. D.
name: Schombert, J. M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Optical surveys for galaxies are biased against the inclusion of low surface brightness (LSB) galaxies. Disney (1976) suggested that the constancy of disk central surface brightness noticed by Freeman (1970) was not a physical result, but instead was an artifact of sample selection. Since LSB galaxies do exist, the pertinent and still controversial issue is if these newly discovered galaxies constitute a significant percentage of the general galaxy population. In this paper, we address this issue by determining the space density of galaxies as a function of disk central surface brightness. Using the physically reasonable assumption (which is motivated by the data) that central surface brightness is independent of disk scale length, we arrive at a distribution which is roughly flat (i.e. approximately equal numbers of galaxies at each surface brightness) faintwards of the Freeman (1970) value. Brightwards of this, we find a sharp decline in the distribution which is analogous to the turn down in the luminosity function at $L^*$. An intrinsically sharply peaked ``Freeman Law'' distribution can be completely ruled out, and no Gaussian distribution can fit the data. Low surface brightness galaxies (those with central surface brightnesses fainter than $22~B\sb$) comprise $\gtrsim 1/2$ the general galaxy population, so a representative sample of galaxies at $z = 0$ does not really exist at present since past surveys have been insensitive to this component of the general galaxy population.
description: uuencoded compressed, tarred postscript. The preprint is also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html
Rumex verticillatus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex verticillatus

description: Rumex verticillatus, spec. nov.
4. Rumex floribus hermaphroditis: valvulis integerrimis: omnibus graniferis, foliis lanceolatis: vaginis cylindricis.
 Lapathum aquaticum, foliis longis angustis acutis, floribus ad genicula verticillatim congestis. Gron. virg. 39.
 Habitat in Virginia . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 334, DOI: 10.5281/zenodo.3931989
The Height Structure of the Solar Atmosphere from the EUV Perspective
Creators: name: Zhang, J.
name: White, S. M.
name: Kundu, M. R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the structure of the solar chromosphere and transition region using full Sun images obtained with the Extreme Ultraviolet Imaging Telescope (EIT) aboard the Solar and Heliospheric Observatory (SOHO) spacecraft. The limb seen in the EIT coronal images (taken in lines of Fe IX/X at 171 Å, Fe XII at 195 Åand Fe XV at 284 Å) is an absorption limb predicted by models to occur at the top of the chromosphere where the density of neutral hydrogen becomes significant ($\sim10^{10}$ cm$^{-3}$). The transition-region limb seen in He II 304 Åimages is an emission limb. We find: (1) the limb is higher at the poles than at the equator both in the coronal images (by 1300 $\pm$ 650 km) and the 304 Åimages (by 3500 $\pm$ 120 0 km); and (2) the 304 Ålimb is significantly higher than the limb in the coronal images. The height difference is 3100 $\pm$ 1200 km at the equator, and 6600 $\pm$ 1200 km at the poles. We suggest that the elevation of the 304 Ålimb above the limb in the coronal images may be due to the upper surface of the chromosphere being bumpy, possibly because of the presence of spicules. The polar extension is consistent with a reduced heat input to the chromosphere in the polar coronal holes compared with the quiet--Sun atmosphere at the equator.
description: 6 pages, 2 figures
Rumex verticillatus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex verticillatus

description: Rumex verticillatus Linnaeus, Species Plantarum 1: 334. 1753.
"Habitat in Virginia." RCN: 2579.
Type not designated.
Original material: Herb. Linn. No. 464.5 (LINN).
Current name: Rumex verticillatus L. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 804, DOI: 10.5281/zenodo.291971
Legge di Taso sugli onori ai caduti in guerra e alle loro famiglie
Creators: name: Giannotti, Andrea
name: Proietti, Giorgia
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description: The stele, to be displayed in the civic prytaneion, preserves a public decree concerning honours for the war dead, norms and limitations to their public mourning, as well as provisions for the fallen’s fathers and sons. The decree, dated to mid-4th century B.C. on a paleographical basis, has been recently connected with the war the Thasians fought against the Thracians to protect their colony Datos/Krenides between 360 and 356 B.C. The first section (ll. 4-14) concerns public honours for the war dead, while the second section (ll. 14-49) deals with public provisions for the war dead’s fathers and sons. Concerning both the special treatment of the war dead and the welfare in favour of the war orphans, a useful comparison can be drawn from the analogue Athenian practice in Classical times.
description: Axon
The Low Redshift Lyman Alpha Forest in Cold Dark Matter Cosmologies
Creators: name: Dave', Romeel
name: Hernquist, Lars
name: Katz, Neal
name: Weinberg, David
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the physical origin of the low-redshift Lyman alpha forest in hydrodynamic simulations of four CDM cosmologies. Our main conclusions are insensitive to the cosmological model but depend on our assumption that the UV background declines at low redshift. We find that the expansion of the universe drives rapid evolution of dN/dz (the number of absorbers per unit z) at z > 1.7, but that at lower redshift the fading of the UV background counters the influence of expansion, leading to slow evolution. At every redshift, weaker lines come primarily from moderate fluctuations of the diffuse, unshocked IGM, and stronger lines originate in shocked or radiatively cooled gas of higher overdensity. However, the neutral hydrogen column density associated with structures of fixed overdensity drops as the universe expands, so an absorber at z = 0 is dynamically analogous to an absorber with neutral hydrogen column density 10 to 50 times higher at z = 2-3. We find no clear distinction between lines arising in "galaxy halos" and lines arising in larger scale structures; however, galaxies tend to lie near the dense regions of the IGM that produce strong Lyman alpha lines. The simulations provide a unified physical picture that accounts for the most distinctive observed properties of the low redshift Lyman alpha forest: (1) a sharp transition in the evolution of dN/dz at z ~ 1.7, (2) stronger evolution for absorbers of higher equivalent width, (3) a correlation of increasing Lyman alpha equivalent width with decreasing galaxy impact parameter, and (4) a tendency for stronger lines to arise in close proximity to galaxies while weaker lines trace more diffuse large scale structure. (Abridged)
description: 57 pages, 18 figures, submitted to ApJ
Evita in Italy
Creators: name: Rodríguez, Fernando Diego
Publisher: name: Fondazione Università Ca’ Foscari Venezia, Italia
Year: 2021

description: During the summer of 1947, Eva Duarte de Perón, wife of the Argentinean Republic President, visited several European countries followed by a large entourage. This article focuses exclusively on her visit to Italy, the longest stage of her trip and perhaps the least studied. The abundance of news that this voyage produced enabled the creation of new perspectives and the formulation of new questions concerning Eva Perón, a central figure in Argentinian history. The chosen perspective stresses the political and socio-economic character of Evita’s journey, avoiding the stereotypes of a ‘glamorous diva’ that were constructed at the time and influenced the subsequent interpretations of that event.
description: Rassegna iberistica
Additional file 1 of Cord blood antimicrobial peptide LL37 levels in preterm neonates and association with preterm complications
Creators: name: Ren, Zhuxiao
name: Mo, Wenhui
name: Yang, Liling
name: Wang, Jianlan
name: Zhang, Qi
name: Zhong, Zhicheng
name: Wei, Wei
name: Liu, Zhipeng
name: Wu, Zhiping
name: Yao, Yao
name: Yang, Jie
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Mental Health
subject: Hematology

description: Additional file 1: Supplemental Table 1. Multiple regression analysis model for perinatal factors that may affect the concentration of LL37 in plasma 48–72 hours after birth. Supplemental Table 2. The main preterm complications in infants < 32 weeks and < 28 weeks.
Karakosta et al - Cord leptin predicts child neurposychological development - Supplementary Tables
Creators: name: Karakosta, Polyxeni
Publisher: name: figshare
Year: 2018
Subjects: subject: 110306 Endocrinology
subject: FOS: Clinical medicine
subject: 111706 Epidemiology
subject: FOS: Health sciences

description: Supplementary Table S1:Data for the trajectory model selection
Supplementary Table S2: Background characteristics of the study population (subjects with available cord leptin levels and at least one assessment of neuropsychological development of cognition from birth to 6 years) based on cord leptin status; Rhea birth cohort, Crete Greece (n=429).Supplementary Table S3: Background characteristics of the study population included in the analysis and lost to follow up.
Supplementary Table S4:Association of cord leptin with child neuropsychological development, after i. excluding preterm and/or low birth weight neonates, and iii. additional adjusting for ponderal index.
Supplementary document for Deep learning enables confocal laser-scanning microscopy with enhanced resolution - 5428101.pdf
Creators: name: Wang, Weibo
name: Wu, Biwei
name: Baoyuan, Zhang
name: Ma, Jie
name: Tan, Jiubin
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Supplement 1