cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Impact of CP-violating interference effects on MSSM Higgs searches
Creators: name: Fuchs, Elina
name: Weiglein, Georg
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Interference and mixing effects between neutral Higgs bosons in the MSSM with complex parameters are shown to have a significant impact on the interpretation of LHC searches for additional Higgs bosons. Complex MSSM parameters introduce mixing between the CP-even and CP-odd Higgs states and generate CP-violating interference terms. Both effects are enhanced in the case of almost degenerate states. Employing as an example an extension of a frequently used benchmark scenario by a non-zero phase $ϕ_{A_t}$, the interference contributions are obtained for the production of neutral Higgs bosons in gluon-fusion and in association with b-quarks followed by the decay into a pair of $τ$-leptons. While the resonant mixing increases the individual cross sections for the two heavy Higgs bosons $h_2$ and $h_3$, strongly destructive interference effects between the contributions involving $h_2$ and $h_3$ leave a considerable parameter region unexcluded that would appear to be ruled out if the interference effects were neglected.
description: 30 pages, 7 figures
Jacques model : a classifier of useless images for your seatizen sessions
Creators: name: Talpaert, Justine
Publisher: name: Zenodo
Year: 2023
Subjects: deep learning
checkpoint
classification
Seatizen

description: Jacques model is a checkpoint used by Jacques, a python package hat classifies useless images after having experienced the Seatizen's acquisition protocol (Seatizen project website). The checkpoint published here is used to load jacques and classify images to sort useful and useless images (blurred or collected out of the water).
Jacques model : a classifier of useless images for your seatizen sessions
Creators: name: Talpaert, Justine
Publisher: name: Zenodo
Year: 2023
Subjects: deep learning
checkpoint
classification
Seatizen

description: Jacques model is a checkpoint used by Jacques, a python package hat classifies useless images after having experienced the Seatizen's acquisition protocol (Seatizen project website). The checkpoint published here is used to load jacques and classify images to sort useful and useless images (blurred or collected out of the water). F1 score for v0 is 0.91.
Jacques model : a classifier of useless images for your seatizen sessions
Creators: name: Talpaert, Justine
name: Carpentier, Léanne
Publisher: name: Zenodo
Year: 2023
Subjects: deep learning
checkpoint
classification
Seatizen

description: Jacques model is a checkpoint used by Jacques, a python package that classifies useless images after having experienced the Seatizen's acquisition protocol (Seatizen project website). The checkpoint published here is used to load jacques and classify images to sort useful and useless images (blurred or collected out of the water). F1 score for v1 model is 0.98. You can also have a look a the metrics.csv and hparams.yaml to learn more about the model itself and the training conditions.
Additional file 3: of Parallel loss of introns in the ABCB1 gene in angiosperms
Creators: name: Parvathaneni, Rajiv
name: DeLeo, Victoria
name: Spiekerman, John
name: Debkanta Chakraborty
name: Devos, Katrien
Publisher: name: figshare
Year: 2017
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Multiple sequence alignment of monocot ABCB1 genes. AÂ multiple sequence alignment was generated for genomic and, for a few species, cDNA sequences of monocot ABCB1 genes obtained from available whole genome sequence data or sequenced ABCB1 genes. Differentially colored regions indicate exons and introns. (PDF 962Â kb)
Massive stars in advanced evolutionary stages, and the progenitor of GW150914
Creators: name: Hamann, Wolf-Rainer
name: Oskinova, Lidia
name: Todt, Helge
name: Sander, Andreas
name: Hainich, Rainer
name: Shenar, Tomer
name: Ramachandran, Varsha
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The recent discovery of a gravitational wave from the merging of two black holes of about 30 solar masses each challenges our incomplete understanding of massive stars and their evolution. Critical ingredients comprise mass-loss, rotation, magnetic fields, internal mixing, and mass transfer in close binary systems. The imperfect knowledge of these factors implies large uncertainties for models of stellar populations and their feedback. In this contribution we summarize our empirical studies of Wolf-Rayet populations at different metallicities by means of modern non-LTE stellar atmosphere models, and confront these results with the predictions of stellar evolution models. At the metallicity of our Galaxy, stellar winds are probably too strong to leave remnant masses as high as 30 solar masses, but given the still poor agreement between evolutionary tracks and observation even this conclusion is debatable. At the low metallicity of the Small Magellanic Cloud, all WN stars which are (at least now) single are consistent with evolving quasi-homogeneously. O and B-type stars, in contrast, seem to comply with standard evolutionary models without strong internal mixing. Close binaries which avoided early merging could evolve quasi-homogeneously and lead to close compact remnants of relatively high masses that merge within a Hubble time.
description: 5 pages, to be published in the Proceedings of the IAU Symposium No. 329 "The lives and death-throes of massive stars"
Additional file 3: Table S3. of Changes in urinary risk profile after short-term low sodium and low calcium diet in recurrent Swiss kidney stone formers
Creators: name: Seeger, Harald
name: Kaelin, Andrea
name: Ferraro, Pietro
name: Weber, Damian
name: Jaeger, Philippe
name: Ambuehl, Patrice
name: Robertson, William
name: Unwin, Robert
name: Wagner, Carsten
name: Mohebbi, Nilufar
Publisher: name: figshare
Year: 2017
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Plasma and urine chemistry at baseline and after seven days on diet from patients with calcium oxalate containing kidney stones which successfully reduced their sodium excretion on low-calcium low-sodium diet. (DOCX 16Â kb)
Additional file 2: of Parallel loss of introns in the ABCB1 gene in angiosperms
Creators: name: Parvathaneni, Rajiv
name: DeLeo, Victoria
name: Spiekerman, John
name: Debkanta Chakraborty
name: Devos, Katrien
Publisher: name: figshare
Year: 2017
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Maximum likelihood protein tree of analyzed ABCB1 (in blue) and ABCB19 (in red) sequences. TheÂ maximum likelihood tree wasÂ generated by RAxML from alignments of analyzed ABCB1 and ABCB19 proteins. Protein names are as listed in Additional file 1: Table S1. ABCB1 and ABCB19 proteins are color-coded in blue and red, respectively. (PDF 394Â kb)
Indirect controllability of some linear parabolic systems of m equations with m-1 controls involving coupling terms of zero or first order
Creators: name: Duprez, Michel
name: Lissy, Pierre
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 93B05, 93B07, 35K40

description: This paper is devoted to the study of the null and approximate controllability for some classes of linear coupled parabolic systems with less controls than equations. More precisely, for a given bounded domain in R^N, we consider a system of m linear parabolic equations (m > 2) with coupling terms of first and zero order, and m-1 controls localized in some arbitrary nonempty open subset. In the case of constant coupling coefficients, we provide a necessary and sufficient condition to obtain the null or approximate controllability in arbitrary small time. In the case m = 2 and N = 1, we also give a generic sufficient condition to obtain the null or approximate controllability in arbitrary small time for general coefficients depending on the space and times variables, provided that the supports of the coupling terms intersect the control domain. The results are obtained thanks to the fictitious control method together with an algebraic method and some appropriate Carleman estimates.
Additional file 1 of Reduction of peripheral regulatory T cells in active rheumatoid arthritis patients with coronary artery disease
Creators: name: Wang, Yanyan
name: Su, Rui
name: Li, Baochen
name: Guo, Qiaoling
name: Hu, Fangyuan
name: Yu, Xiaopu
name: Ma, Mingxia
name: Wang, Lizhi
name: Gao, Chong
name: Li, Xiaofeng
name: Wang, Caihong
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1. Table S1-S3. The number and percentages of lymphocyte and CD4+T cell subset in different groups; Table S4. Cytokine levels in the RA-CAD and pure RA groups; Figure S1-S2. Phenotypic characterization of lymphocyte and CD4+T cell subsets via flow cytometry; Figure S3. Correlation between Treg number and disease activity indicators when a sample with uniquely high Treg number was excluded.
Additional file 4: Figure S4. of Anti-aggregant tau mutant promotes neurogenesis
Creators: name: Joseph, Maria
name: Anglada-Huguet, Marta
name: Paesler, Katharina
name: Mandelkow, Eckhard
name: Eva-Maria Mandelkow
Publisher: name: figshare
Year: 2017
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Ki67 positive cells are increased in anti-aggregant slices at DIV30. OHSCs were cultured until DIV30. The slices were then fixed and immunostained with NeuN antibody for neurons and Ki67, a marker of proliferating cells. Note that with advanced age the level of proliferation is higher in anti-aggregant TauRDÎ KPP slices (top row), compared with controls (bottom). (PDF 113 kb)
A hadronic minute-scale GeV flare from quasar 3C 279?
Creators: name: Petropoulou, M.
name: Nalewajko, K.
name: Hayashida, M.
name: Mastichiadis, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The flat spectrum radio quasar 3C 279 is a known $γ$-ray variable source that has recently exhibited minute-scale variability at energies $>100$ MeV. One-zone leptonic models for blazar emission are severely constrained by the short timescale variability that implies a very compact emission region at a distance of hundreds of Schwarzschild radii from the central black hole. Here, we investigate a hadronic scenario where GeV $γ$-rays are produced via proton synchrotron radiation. We also take into account the effects of the hadronically initiated electromagnetic cascades (EMC). For a $γ$-ray emitting region in rough equipartition between particles and kG magnetic fields, located within the broad-line region (BLR), the development of EMC redistributes the $γ$-ray luminosity to softer energy bands and eventually leads to broad-band spectra that differ from the observed ones. Suppression of EMC and energy equipartition are still possible, if the $γ$-ray emitting region is located beyond the BLR, is fast moving with Doppler factor ($>70$), and contains strong magnetic fields ($>100$ G). Yet, these conditions cannot be easily met in parsec-scale jets, thus disfavouring a proton synchrotron origin of the Fermi-LAT flare.
description: 5 pages, 1 figure, accepted for publication
Pubertal development and self-regulation of behavior: a systematic review
Creators: name: França, Thiago
name: Segura, Isis
name: Miranda, Mônica
name: Pompeia, Sabine
Publisher: name: Open Science Framework
Year: 2022

description: Self-regulation of behavior is an essential ability for living a healthy and productive life. It matures during adolescence, when self-regulation failures are still likely to be involved in higher risk taking and behaviors that increase vulnerability. Most studies have addressed this issue considering development over chronological ages, which happens in tandem with changes in adolescents’ environment and social milieu, as well as with changes in pubertal status. The timing and tempo of pubertal development, however, varies widely among individuals and so it is not adequately represented by age. Recent studies have suggested that puberty may in fact be a more important factor in determining brain and behavioral changes in adolescence than age. Understanding how puberty influences the development of self-regulation may therefore enable a better understanding of how this crucial function develops during adolescence, which could in turn be useful for designing public policies for prevention and intervention to promote adolescents’ health and well-being, to create better educational strategies and to determine adolescents’ rights and their accountability. Recent years have seen a growing interest on puberty, which led to an increasing number of studies incorporating measures of pubertal status. But how much knowledge about the effects of puberty on self-regulation have we gained from these studies? How much progress have we made in disentangling the effects of puberty on self-regulation from the effects of other changes happening during adolescence, such as those more closely correlated with increases in age or grades? To answer these questions we will apply the methods of systematic review to locate and integrate the literature studying the development of self-regulation along pubertal development.
On the Structural Origin of the Catalytic Properties of Inherently Strained Ultrasmall Decahedral Gold Nanoparticles
Creators: name: Walsh, Michael
name: Yoshida, Kenta
name: Kuwabara, Akihide
name: Pay, Mungo
name: Gai, Pratibha
name: Boyes, Edward
Publisher: name: arXiv
Year: 2017
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A new mechanism for reactivity of multiply twinned gold nanoparticles resulting from their inherently strained structure provides a further explanation of the surprising catalytic activity of small gold nanoparticles. Atomic defect structural studies of surface strains and quantitative analysis of atomic column displacements in the decahedral structure observed by aberration corrected transmission electron microscopy reveal an average expansion of surface nearest neighbor distances of 5.6 percent, with many strained by more than 10 percent. Density functional theory calculations of the resulting modified gold d-band states predict significantly enhanced activity for carbon monoxide oxidation. The new insights have important implications for the applications of nanoparticles in chemical process technology, including for heterogeneous catalysis.
MOESM1 of The influence of dopamine-beta-hydroxylase and catechol O-methyltransferase gene polymorphism on the efficacy of insulin detemir therapy in patients with type 2 diabetes mellitus
Creators: name: Bozek, Tomislav
name: Blazekovic, Antonela
name: Matea Perkovic
name: Jercic, Kristina
name: Sustar, Aleksandra
name: Smircic-Duvnjak, Lea
name: Outeiro, Tiago
name: Pivac, Nela
name: Borovecki, Fran
Publisher: name: figshare
Year: 2017
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Additional tables.
Using Collisions of AGN Outflows with ICM Shocks as Dynamical Probes
Creators: name: Jones, T. W.
name: Nolting, Chris
name: O'Neill, B. J.
name: Mendygral, P. J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In this paper we lay out a simple set of relationships connecting the dynamics of fast plasma jets to the dynamical state of their ambient media. The objective is to provide a tool kit that can be used to connect the morphologies of radio AGNs in galaxy clusters to the dynamical state of the local ICM. The formalism is intended to apply to jets whether they are relativistic or non-relativistic. Special attention is paid to interactions involving ICM shocks, although the results can be applied more broadly. Our formalism emphasizes the importance of the relative Mach number of the impacting ICM flow and the internal Mach number of the AGN jet in determining how the AGN outflows evolve.
description: 11 pages, 5 figures. Submitted to Physics of Plasmas
Energy-Efficient Coordinated Multi-Cell Multigroup Multicast Beamforming with Antenna Selection
Creators: name: Tervo, Oskari
name: Tran, Le-Nam
name: Pennanen, Harri
name: Chatzinotas, Symeon
name: Juntti, Markku
name: Ottersten, Björn
Publisher: name: arXiv
Year: 2017
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: This paper studies energy-efficient coordinated beamforming in multi-cell multi-user multigroup multicast multiple-input single-output systems. We aim at maximizing the network energy efficiency by taking into account the fact that some of the radio frequency chains can be switched off in order to save power. We consider the antenna specific maximum power constraints to avoid non-linear distortion in power amplifiers and user-specific quality of service (QoS) constraints to guarantee a certain QoS levels. We first introduce binary antenna selection variables and use the perspective formulation to model the relation between them and the beamformers. Subsequently, we propose a new formulation which reduces the feasible set of the continuous relaxation, resulting in better performance compared to the original perspective formulation based problem. However, the resulting optimization problem is a mixed-Boolean non-convex fractional program, which is difficult to solve. We follow the standard continuous relaxation of the binary antenna selection variables, and then reformulate the problem such that it is amendable to successive convex approximation. Thereby, solving the continuous relaxation mostly results in near-binary solution. To recover the binary variables from the continuous relaxation, we switch off all the antennas for which the continuous values are smaller than a small threshold. Numerical results illustrate the superior convergence result and significant achievable gains in terms of energy efficiency with the proposed algorithm.
description: 6 pages, 5 figures, accepted to IEEE ICC 2017 - International Workshop on 5G RAN Design
Properties of the cosmological filament between two clusters: A possible detection of a large-scale accretion shock by $Suzaku$
Creators: name: Akamatsu, H.
name: Fujita, Y.
name: Akahori, T.
name: Ishisaki, Y.
name: Hayashida, K.
name: Hoshino, A.
name: Mernier, F.
name: Yoshikawa, K.
name: Sato, K.
name: Kaastra, J. S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report on the results of a $Suzaku$ observation of the plasma in the filament located between the two massive clusters of galaxies Abell 399 and Abell 401. Abell 399 ($z$=0.0724) and Abell 401 ($z$=0.0737) are expected to be in the initial phase of a cluster merger. In the region between the two clusters, we find a clear enhancement in the temperature of the filament plasma from 4 keV (expected value from a typical cluster temperature profile) to $kT\sim$6.5 keV. Our analysis also shows that filament plasma is present out to a radial distance of 15' (1.3 Mpc) from a line connecting the two clusters. The temperature profile is characterized by an almost flat radial shape with $kT\sim$6-7 keV within 10' or $\sim$0.8 Mpc. Across $r$=8'~from the axis, the temperature of the filament plasma shows a drop from 6.3 keV to 5.1 keV, indicating the presence of a shock front. The Mach number based on the temperature drop is estimated to be ${\cal M}\sim$1.3. We also successfully determined the abundance profile up to 15' (1.3 Mpc), showing an almost constant value ($Z$=0.3 solar) at the cluster outskirt. We estimated the Compton $y$-parameter to be $\sim$14.5$\pm1.3\times10^{-6}$, which is in agreement with $Planck$'s results (14-17$\times10^{-6}$ on the filament). The line of sight depth of the filament is $l\sim$1.1 Mpc, indicating that the geometry of filament is likely a pancake shape rather than cylindrical. The total mass of the filamentary structure is $\sim$7.7$\times10^{13}~\rm M_{\odot}$. We discuss a possible interpretation of the drop of X-ray emission at the rim of the filament, which was pushed out by the merging activity and formed by the accretion flow induced by the gravitational force of the filament.
description: 8 pages, 8 figures, accepted for publication in A&A
Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
Creators: name: Franck, J. R.
name: McGaugh, S. S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Candidate Cluster and Protocluster Catalog (CCPC) contains 218 galaxy overdensities com- posed of more than 2000 galaxies with spectroscopic redshifts spanning the first few Gyrs after the Big Bang (2.0 < z < 6.6). We use Spitzer archival data to track the underlying stellar mass of these overdense regions in various temporal cross sections by building rest-frame near-infrared luminosity functions across the span of redshifts.This exercise maps the stellar growth of protocluster galaxies, as halos in the densest environments should be the most massive from hierarchical accretion. The characteristic apparent magnitude, m*(z), is relatively flat from 2.0 < z < 6.6, consistent with a passive evolution of an old stellar population. This trend maps smoothly to lower redshift results of cluster galaxies from other works. We find no difference in the luminosity
description: 22 pages and 9 figures. Accepted to the Astrophysical Journal
Lettre de Jean-François Séguier à non id. (minute), s.d.
Creators: name: Séguier, Jean-François
name: Jean-François Séguier
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022
Subjects: Librairie

description: Monsieur, votre lettre du 10 septembre ne m’est parvenue que depuis peu de jours. J’ai été charmé de recevoir de vos nouvelles qui m’ont été très agréable. J’y ai lu les marques les plus distinctes de votre politesse à mon égard puisque vous voulez bien m’offrir si obligeamment un exemplaire de l’ouvrage de M. Hunter dont je regrette infiniment la perte. Toutes les personnes qui s’appliquent à la connaissance des médailles y sont extrêmement sensibles. J’ai vu les soins que vous avez déjà pris pour me faire parvenir cet exemplaire par Mrs MacSmyth avocat d’Edimburg. Ensuite comme il arriva depuis et qu’il ne peut s’en charger par M. Giraudy marchand de vin à Nice où il lui sera aisé de le remettre à M. Brickbeck consul de la nation anglaise dans la ville de Nice dont je suis fort connu et qui m’a fait ci devant passer bien des paquets de livres d’Angleterre lorsqu’il se rendait à Marseille. Si vos Messieurs consuls se destinent à venir ici, je serai charmé de les voir et de leur offrir mes services dans tout ce qui dépend de moi, de même que M. Pieyre le jeune qui m’a chargé de vous faire ses remerciements du pistolet que vous lui [avez] envoyé et qu’il recevra cet article à l’égard du restant de la commission qu’il vous avait donnée. Il vous en remercie et vous prie ne pas l’envoyer attendu que la personne pour qui il vous avait prié n’est plus ici. Il sera aussi empressé que moi à obliger M. Giraudy en tout qui dépendra de lui.
Je n’ai pas manqué de parler à M. Razoux de tout ce que vous me dîtes d’obligeant à son sujet. Il avait été charmé de pouvoir avoir l’honneur d’être assuré et d’appartenir à l’illustre société royale. Ayez la bonté de lui continuer votre amitié dont il est fort jaloux. Il continue à s’occuper fort utilement et a mérité de plus en plus l’honneur de lui appartenir. Il a été charmé d’apprendre que l’illustre Monsieur Banks en est le président.
Si <…> j’en aurais plutôt donner de mes nouvelles et ajouté à mes remerciements.
S’il était nécessaire de faire parvenir à Paris le volume de Hunter que vous me destinez, on pourra l’adresser à M. d’Henin conseiller de la cour des aides rue Quanquempoix qui acquittera le port franc de la caisse et qui aura le soin de me le faire parvenir s’il est nécessaire.
J’ai l’honneur d’être avec respect, Monsieur & c.
description: Source: [établissement de conservation] Nîmes, Bibliothèque Carré d'Art [cote] ms. 417, fol. 148
description: created: 0000-00-00
Non-resonant Collider Signatures of a Singlet-Driven Electroweak Phase Transition
Creators: name: Chen, Chien-Yi
name: Kozaczuk, Jonathan
name: Lewis, Ian M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We analyze the collider signatures of the real singlet extension of the Standard Model in regions consistent with a strong first-order electroweak phase transition and a singlet-like scalar heavier than the Standard Model-like Higgs. A definitive correlation exists between the strength of the phase transition and the trilinear coupling of the Higgs to two singlet-like scalars, and hence between the phase transition and non-resonant scalar pair production involving the singlet at colliders. We study the prospects for observing these processes at the LHC and a future 100 TeV $pp$ collider, focusing particularly on double singlet production. We also discuss correlations between the strength of the electroweak phase transition and other observables at hadron and future lepton colliders. Searches for non-resonant singlet-like scalar pair production at 100 TeV would provide a sensitive probe of the electroweak phase transition in this model, complementing resonant di-Higgs searches and precision measurements. Our study illustrates a strategy for systematically exploring the phenomenologically viable parameter space of this model, which we hope will be useful for future work.
description: 34 pages + 4 appendices, 13 figures. Comments welcome!
Additional file 1: of The development of a nursing subset of patient problems to support interoperability
Creators: name: R. Kieft
name: E. Vreeke
name: E. De Groot
name: P. Volkert
name: A. Francke
name: D. Delnoij
Publisher: name: figshare
Year: 2017
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Overview of patient problems (level of occurrence compared to level of reported influence). (DOCX 17Â kb)
Narrowing down the possible explanations of cosmic acceleration with geometric probes
Creators: name: Dhawan, Suhail
name: Goobar, Ariel
name: Mörtsell, Edvard
name: Amanullah, Rahman
name: Feindt, Ulrich
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Recent re-calibration of the Type Ia supernova (SNe~Ia) magnitude-redshift relation combined with cosmic microwave background (CMB) and baryon acoustic oscillation (BAO) data have provided excellent constraints on the standard cosmological model. Here, we examine particular classes of alternative cosmologies, motivated by various physical mechanisms, e.g. scalar fields, modified gravity and phase transitions to test their consistency with observations of SNe~Ia and the ratio of the angular diameter distances from the CMB and BAO. Using a model selection criterion for a relative comparison of the models (the Bayes Factor), we find moderate to strong evidence that the data prefer flat $Λ$ CDM over models invoking a thawing behaviour of the quintessence scalar field. However, some exotic models like the growing neutrino mass cosmology and vacuum metamorphosis still present acceptable evidence values. The bimetric gravity model with only the linear interaction term can be ruled out by the combination of SNe~Ia and CMB/BAO datasets whereas the model with linear and quadratic interaction terms has a comparable evidence value to standard $Λ$ CDM. Thawing models are found to have significantly poorer evidence compared to flat $Λ$ CDM cosmology under the assumption that the CMB compressed likelihood provides an adequate description for these non-standard cosmologies. We also present estimates for constraints from future data and find that geometric probes from oncoming surveys can put severe limits on non-standard cosmological models.
description: 31 pages, 9 figures, to be submitted to JCAP. Comments welcome
Additional file 1: Table S1. of Economic burden of community-acquired pneumonia among elderly patients: a Japanese perspective
Creators: name: Konomura, Keiko
name: Nagai, Hideaki
name: Akazawa, Manabu
Publisher: name: figshare
Year: 2017
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Definition of the six categories for the breakdown of total treatment costs. Table S2. Definition of comorbidities and their medications. Table S3. Definition of drug use. Table S4. The median treatment costs and treatment period, and death rate of invasive pneumococcal disease (IPD). (PDF 586Â kb)
Additional file 2: Table S2. of Changes in urinary risk profile after short-term low sodium and low calcium diet in recurrent Swiss kidney stone formers
Creators: name: Seeger, Harald
name: Kaelin, Andrea
name: Ferraro, Pietro
name: Weber, Damian
name: Jaeger, Philippe
name: Ambuehl, Patrice
name: Robertson, William
name: Unwin, Robert
name: Wagner, Carsten
name: Mohebbi, Nilufar
Publisher: name: figshare
Year: 2017
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Plasma and urine chemistry in patients with calcium oxalate containing kidney stones at baseline and after seven days on low-calcium low-sodium diet. (DOCX 15Â kb)
OH Survey along Sightlines of Galactic Observations of Terahertz C+
Creators: name: Tang, Ningyu
name: Li, Di
name: Heiles, Carl
name: Yue, Nannan
name: Dawson, J. R.
name: Goldsmith, Paul F.
name: Krčo, Marko
name: McClure-Griffiths, N. M.
name: Wang, Shen
name: Zuo, Pei
name: Pineda, Jorge L.
name: Wang, Jun-Jie
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have obtained OH spectra of four transitions in the $^2Π_{3/2}$ ground state, at 1612, 1665, 1667, and 1720 MHz, toward 51 sightlines that were observed in the Herschel project Galactic Observations of Terahertz C+. The observations cover the longitude range of (32$^\circ$, 64$^\circ$) and (189$^\circ$, 207$^\circ$) in the northern Galactic plane. All of the diffuse OH emissions conform to the so-called 'Sum Rule' of the four brightness temperatures, indicating optically thin emission condition for OH from diffuse clouds in the Galactic plane. The column densities of the HI `halos' N(HI) surrounding molecular clouds increase monotonically with OH column density, N(OH), until saturating when N(HI)=1.0 x 10$^{21}$ cm$^{-2}$ and N (OH) $\geq 4.5\times 10^{15}$ cm$^{-2}$, indicating the presence of molecular gas that cannot be traced by HI. Such a linear correlation, albeit weak, is suggestive of HI halos' contribution to the UV shielding required for molecular formation. About 18% of OH clouds have no associated CO emission (CO-dark) at a sensitivity of 0.07 K but are associated with C$^+$ emission. A weak correlation exists between C$^+$ intensity and OH column density for CO-dark molecular clouds. These results imply that OH seems to be a better tracer of molecular gas than CO in diffuse molecular regions.
description: 13 pages, 12 figures, accepted for publication in ApJ
The Other Art of Computer Programming. Milestone 2: LOGO. 1960s
Creators: name: Tarr, Melanie
Publisher: name: Edith Cowan University
Year: 2019
Subjects: Computer Science

description: A comic on early computer science in the 1960s based on LOGO. This comic helps to explain abstract concepts and is illustrated by hand. It may be used as a visual aid by teachers for education purposes.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000633
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
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: Châtelet
subject: registre

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000633
A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
Creators: name: Rieder, Michael
name: Teyssier, Romain
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Magnetic fields in galaxies are believed to be the result of dynamo amplification of initially weak seed fields, reaching equipartition strength inside the interstellar medium. The small-scale dynamo appears to be a viable mechanism to explain observations of strong magnetic fields in present-day and high-redshift galaxies, considering the extreme weakness of seed fields predicted by battery mechanisms or primordial fields. Performing high-resolution adaptive mesh magneto-hydrodynamic simulations of a small mass, isolated cooling halo with an initial magnetic seed field strength well below equipartition, we follow the small-scale dynamo amplification from supernova-induced turbulence up to saturation of the field. We find that saturation occurs when the average magnetic pressure reaches only 3 % to 5 % of the turbulent pressure. The magnetic energy growth transitions from exponential to linear, and finally comes to halt. The saturation level increases slightly with grid resolution. These results are in good agreement with theoretical predictions for magnetic Prandtl numbers of order $\mathrm{Pr_M} \sim 1$ and turbulent Mach numbers of order $\mathrm{M} \sim 10$. When we suppress supernova feedback after our simulation has reached saturation, we find that turbulence decays and that the gas falls back onto a thin disk with the magnetic field in local equipartition. We propose a scenario in which galactic magnetic fields are amplified from weak seed fields in the early stages of the Universe to sub-equipartition fields, owing to the turbulent environment of feedback-dominated galaxies at high redshift, and are evolved further in a later stage up to equipartition, as galaxies transformed into more quiescent, large spiral disks.
description: 14 pages, 14 figures, submitted to MNRAS. Part I (The kinematic phase) can be found at https://doi.org/10.1093/mnras/stv2985 (journal article) or at arXiv:1506.00849
On the Distribution of Extrema for a Class of Lévy Processes
Creators: name: Najafabadi, Amir T. Payandeh
name: Kucerovsky, Dan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: Suppose Xt is either a regular exponential type Levy process or a Levy process with a bounded variation jumps measure. The distribution of the extrema of Xt play a crucial role in many financial and actuarial problems. This article employs the well known and powerful Riemann-Hilbert technique to derive the characteristic functions of the extrema for such Levy processes. An approximation technique along with several examples is given.
description: 12 Pages
IslandFAST: A Semi-numerical Tool for Simulating the Late Epoch of Reionization
Creators: name: Xu, Yidong
name: Yue, Bin
name: Chen, Xuelei
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the algorithm and main results of our semi-numerical simulation, islandFAST, which is developed from the 21cmFAST and designed for the late stage of reionization. The islandFAST predicts the evolution and size distribution of the large scale under-dense neutral regions (neutral islands), and we find that the late Epoch of Reionization (EoR) proceeds very fast, showing a characteristic scale of the neutral islands at each redshift. Using islandFAST, we compare the impact of two types of absorption systems, i.e. the large scale under-dense neutral islands versus small scale over-dense absorbers, in regulating the reionization process. The neutral islands dominate the morphology of the ionization field, while the small scale absorbers dominate the mean free path of ionizing photons, and also delay and prolong the reionization process. With our semi-numerical simulation, the evolution of the ionizing background can be derived self-consistently given a model for the small absorbers. The hydrogen ionization rate of the ionizing background is reduced by an order of magnitude in the presence of dense absorbers.
description: 15 pages, 8 figures
Quantum Oscillations in the Chiral Magnetic Conductivity
Creators: name: Kaushik, Sahal
name: Kharzeev, Dmitri E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In strong magnetic field the longitudinal magnetoconductivity in 3D chiral materials is shown to exhibit a new type of quantum oscillations arising from the chiral magnetic effect (CME). These quantum CME oscillations are predicted to dominate over the Shubnikov-de Haas (SdH) ones in chiral materials with an approximately conserved chirality of quasiparticles at strong magnetic fields. The phase of quantum CME oscillations differs from the phase of the conventional SdH oscillations by $π/2$.
description: 5 pages, 3 figures
D5.3 Dissemination Activities Report-first year report
Creators: name: Esteves, Sofia
name: Varandas, Nuno
name: Tucker, Charlotte
name: Doguchi, Keiko
Publisher: name: Zenodo
Year: 2020
Subjects: IoT
Security
Dissemination
Promotion
Events
Articles
Newsletters
Workshops
Webinars
Conferences

description: The current deliverable shows dissemination activities that have been implemented at project and partner level during the first period, according to the Action Plan set at the beginner of the project.
Additional file 3: Figure S3. of Anti-aggregant tau mutant promotes neurogenesis
Creators: name: Joseph, Maria
name: Anglada-Huguet, Marta
name: Paesler, Katharina
name: Mandelkow, Eckhard
name: Eva-Maria Mandelkow
Publisher: name: figshare
Year: 2017
Subjects: Biochemistry
Cell Biology
Neuroscience
Developmental Biology
Cancer

description: DCX positive cells are increased in the anti-aggregant slices at DIV30. OHSCs were cultured until DIV30. The slices were then fixed and immunostained with NeuN antibody for neurons and DCX antibody for progenitor cells. DCX positive cells appear in controls and in the anti-aggregant slices in all regions of the hippocampus. The figure shows the CA3 and DG regions from the control and anti-aggregant slices at DIV30. Arrows indicate DCX+ cell bodies. Note the increase in DCX+ positive cells in the anti-aggregant TauRDÎ KPP slices compared to the age-matched controls. (PDF 183 kb)
Integrated optics prototype beam combiner for long baseline interferometry in the L and M bands
Creators: name: Tepper, Jan
name: Labadie, Lucas
name: Diener, Romina
name: Minardi, Stefano
name: Pott, Jörg-Uwe
name: Thomson, Robert R.
name: Nolte, Stefan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In the last few years, integrated optics (IO) beam combiners have facilitated the emergence of 4-telescope interferometers such as PIONIER or GRAVITY, boosting the imaging capabilities of the VLTI. However, the spectral range beyond 2.2microns is not ideally covered by the conventional silica based IO. Here, we propose to consider new laser-written IO prototypes made of GLS glasses, a material that permits access to the mid-infrared spectral regime. Our goal is to conduct a full characterization of our mid-IR IO 2-telescope coupler in order to measure the performance levels directly relevant for long-baseline interferometry. We focus in particular on the exploitation of the L and M astronomical bands. We use a dedicated Michelson-interferometer setup to perform Fourier Transform spectroscopy on the coupler and measure its broadband interferometric performance. We also analyze the polarization properties of the coupler, the differential dispersion and phase degradation as well as the modal behavior and the total throughput. We measure broadband interferometric contrasts of 94.9% and 92.1% for unpolarized light in the L and M bands. Spectrally integrated splitting ratios are close to 50% but show chromatic dependence over the considered bandwidths. Additionally, the phase variation due to the combiner is measured and does not exceed 0.04rad and 0.07rad across the band L and M band, respectively. The total throughput of the coupler including Fresnel and injection losses from free-space is 25.4%. The laser-written IO GLS prototype combiners prove to be a reliable technological solution with promising performance for mid-infrared long-baseline interferometry. In the next steps, we will consider more advanced optical functions as well as a fiber-fed input and revise the optical design parameters in order the further enhance the total throughput and achromatic behavior.
Solving an Integral Equation Arising from the Ruin Probability of Long-term Bonus-Malus Systems
Creators: name: Kucerovsky, Dan
name: Najafabadi, Amir T. Payandeh
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: This article studies in detail the solution of an integral equation due to Rongming et al. [13]. The methods involve complex analysis. As an application, we find the ruin probability of a given Bonus-Malus system in a steady state. We obtain closed form solutions for the ruin probability in certain cases, and we characterize these cases. We give conditions for the Laplace transform of a ruin probability to extend to a meromorphic function in the complex plane, we prove a very general and almost sharp inequality of Lundberg type, and we extend our results to a doubly stochastic situation.
description: 23Pages
Additional file 1: Table S1. of Changes in urinary risk profile after short-term low sodium and low calcium diet in recurrent Swiss kidney stone formers
Creators: name: Seeger, Harald
name: Kaelin, Andrea
name: Ferraro, Pietro
name: Weber, Damian
name: Jaeger, Philippe
name: Ambuehl, Patrice
name: Robertson, William
name: Unwin, Robert
name: Wagner, Carsten
name: Mohebbi, Nilufar
Publisher: name: figshare
Year: 2017
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Plasma and urine chemistry in female and male patients with calcium oxalate containing kidney stones at baseline and after seven days on low-calcium low-sodium diet. (DOCX 22Â kb)
Additional file 12: of Parallel loss of introns in the ABCB1 gene in angiosperms
Creators: name: Parvathaneni, Rajiv
name: DeLeo, Victoria
name: Spiekerman, John
name: Debkanta Chakraborty
name: Devos, Katrien
Publisher: name: figshare
Year: 2017
Subjects: Biochemistry
Molecular Biology
Developmental Biology
Computational Biology

description: Mixed model for ABCB1 intron variance in the Poales explained by both intron loss and intron gain events. Intron loss events are shown by red stars and a minus sign (â ) followed by the intron that was lost. Intron gain events are shown by green stars and a plus sign (+) followed by the intron that was gained. Members of the grass family are represented in black while non-grass monocots are in blue. The vertical bars indicate different grass subfamilies. (PDF 922Â kb)
Spintronic virtual neural network by a voltage controlled ferromagnet for associative memory
Creators: name: Taniguchi, Tomohiro
name: Imai, Yusuke
Publisher: name: arXiv
Year: 2024
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Recently, an associative memory operation by a virtual oscillator network, consisting of a single spintronic oscillator, was examined to solve issues in conventional, real oscillators-based neural networks such as inhomogeneities between the oscillators. However, the spintronic oscillator still carries issues dissipating large amount of energy because it is driven by electric current. Here, we propose to use a single ferromagnet manipulated by voltage-controlled magnetic anisotropy (VCMA) effect as a fundamental element in a virtual neural network, which will contribute to significantly reducing the Joule heating caused by electric current. Instead of the oscillation in oscillator networks, magnetization relaxation dynamics were used for the associative memory operation. The associative memory operation for alphabet patterns is successfully demonstrated by giving correspondences between the colors in a pattern recognition task and the sign of a perpendicular magnetic anisotropy coefficient, which could be either positive or negative via the VCMA effect.
description: 18 pages, 5 figures, publication information was added