cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Entropy-SGD optimizes the prior of a PAC-Bayes bound: Generalization properties of Entropy-SGD and data-dependent priors
Creators: name: Dziugaite, Gintare Karolina
name: Roy, Daniel M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: We show that Entropy-SGD (Chaudhari et al., 2017), when viewed as a learning algorithm, optimizes a PAC-Bayes bound on the risk of a Gibbs (posterior) classifier, i.e., a randomized classifier obtained by a risk-sensitive perturbation of the weights of a learned classifier. Entropy-SGD works by optimizing the bound's prior, violating the hypothesis of the PAC-Bayes theorem that the prior is chosen independently of the data. Indeed, available implementations of Entropy-SGD rapidly obtain zero training error on random labels and the same holds of the Gibbs posterior. In order to obtain a valid generalization bound, we rely on a result showing that data-dependent priors obtained by stochastic gradient Langevin dynamics (SGLD) yield valid PAC-Bayes bounds provided the target distribution of SGLD is ε-differentially private. We observe that test error on MNIST and CIFAR10 falls within the (empirically nonvacuous) risk bounds computed under the assumption that SGLD reaches stationarity. In particular, Entropy-SGLD can be configured to yield relatively tight generalization bounds and still fit real labels, although these same settings do not obtain state-of-the-art performance.
description: 18 pages, 6 figures; combines ICML camera ready with supplementary materials
Additional file 1: of Adapting clinical practice guidelines for diabetic retinopathy in Kenya: process and outputs
Creators: name: Nyawira Mwangi
name: Muchai Gachago
name: Gichangi, Michael
name: Gichuhi, Stephen
name: Kibata Githeko
name: Atieno Jalango
name: Jefitha Karimurio
name: Kibachio, Joseph
name: Muthami, Lawrence
name: Ngugi, Nancy
name: Carmichael Nduri
name: Nyaga, Patrick
name: Nyamori, Joseph
name: Zindamoyen, Alain
name: Covadonga Bascaran
name: Foster, Allen
Publisher: name: figshare
Year: 2018
Subjects: 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: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Search strategy for â Adapting Clinical Practice Guidelines for Diabetic Retinopathy in Kenyaâ (PDF 568 kb)
A two-pion exchange three-nucleon force based on a realistic pi-N interaction
Creators: name: Saito, T. -Y.
name: Haidenbauer, J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The contribution of a $ππ$-exchange three-body force to the three-nucleon binding energy is calculated in terms of a $πN$ amplitude. The latter is based on a meson-theoretical model of $πN$ interaction developed by the Jülich group. Similar to a previous study based on simple phenomenological $πN$ potentials a very small effect of the resulting three-body force is found. Possible origins of the two-orders-of-magnitude descrepancy between the present result and the values obtained for the Tucson-Melbourne three-body force are investigated. Evidence is provided that this discrepancy is most likely due to strikingly different off-shell properties of the $πN$ amplitudes underlying the two approaches.
description: 22 pages, 8 figures; to appear in Eur. Phys. J. A
Additional file 3 of High expression of RABL6 promotes cell proliferation and predicts poor prognosis in esophageal squamous cell carcinoma
Creators: name: Feng, Yanfen
name: Yan, Shumei
name: Huang, Yuhua
name: Huang, Qitao
name: Wang, Fang
name: Lei, Yiyan
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 3.
EL CONSUMO DE DROGAS EN LA SENTENCIA N°  C-221/94 DE LA  CORTE CONSTITUCIONAL COLOMBIANA: UN CASO TRÁGICO  A propósito del pensamiento de Carlos Santiago Nino
Creators: name: Jaime David Abanto Torres
Publisher: name: Zenodo
Year: 2007

description:  SUMARIO Introducción. 1. El rol del Estado. 2. La dignidad de la persona. 3. El caso. 4. Consideraciones de la Corte en mayoría. 5. Consideraciones de la Corte en minoría. 6. Razonabilidad y Proporcionalidad. 7. Alternativas para combatir el consumo de drogas. Conclusiones.
Highly polarized structures in the near-nuclear regions of Cygnus A: intrinsic anisotropy within the cones?
Creators: name: Tadhunter, C. N.
name: Sparks, W.
name: Axon, D. J.
name: Bergeron, L.
name: Jackson, N. J.
name: Packham, C.
name: Hough, J. H.
name: Robinson, A.
name: Young, S.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present near-IR imaging polarimetry observations of the nucleus of Cygnus A, taken with the NICMOS camera of the HST at a wavelength of 2.0 microns.These maps reveal a highly collimated region of polarized emission straddling the nucleus and extending to a radius of 1.2 arcseconds. Remarkably, this feature coincides with one, but only one, limb of the edge-brightened bicone structure seen in the total intensity image. The high degree (P_k ~ 25%) and orientation of the extended polarization feature are consistent with a scattering origin. Most plausibly, the detection of polarization along only one limb of the bicone is a consequence of intrinsic anisotropy of the near-IR continuum within the radiation cones, with the direction of maximum intensity of the near-IR radiation field significantly displaced from the direction of the radio axis. The unresolved nuclear core source is also highly polarized (P_k > 28%), with a position angle close to the perpendicular to the radio axis. Given that this high degree of nuclear polarization can only be explained in terms of dichroic extinction if the dichroic mechanism is unusually efficient in Cygnus A, it is more likely that the nuclear polarization is due to the scattering of nuclear light in an unresolved scattering region close to the AGN. In this case, the flux of the core source in the K-band is dominated by scattered rather than transmitted quasar light, and previous extinction estimates based on K-band photometry of the core substantially underestimate the true nuclear extinction.
description: 12 pages, 1 figure, to be published in MNRAS
The Error Probability of Sparse Superposition Codes with Approximate Message Passing Decoding
Creators: name: Rush, Cynthia
name: Venkataramanan, Ramji
Publisher: name: arXiv
Year: 2017
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: Sparse superposition codes, or sparse regression codes (SPARCs), are a recent class of codes for reliable communication over the AWGN channel at rates approaching the channel capacity. Approximate message passing (AMP) decoding, a computationally efficient technique for decoding SPARCs, has been proven to be asymptotically capacity-achieving for the AWGN channel. In this paper, we refine the asymptotic result by deriving a large deviations bound on the probability of AMP decoding error. This bound gives insight into the error performance of the AMP decoder for large but finite problem sizes, giving an error exponent as well as guidance on how the code parameters should be chosen at finite block lengths. For an appropriate choice of code parameters, we show that for any fixed rate less than the channel capacity, the decoding error probability decays exponentially in $n/(\log n)^{2T}$, where $T$, the number of AMP iterations required for successful decoding, is bounded in terms of the gap from capacity.
description: 27 pages. IEEE Transactions on Information Theory
Orchestration of Starbirth Activity in Disk Galaxies: New Perspectives from Ultraviolet Imaging
Creators: name: Waller, William H.
name: Stecher, Theodore P.
name: Telescope, the Ultraviolet Imaging
name: Team, Science
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Ultraviolet imaging of nearby disk galaxies reveals the star-forming activity in these systems with unprecedented clarity. UV images recently obtained with the Shuttle-borne Ultraviolet Imaging Telescope (UIT) reveal a remarkable variety of star-forming morphologies. The respective roles of tides, waves, and resonances in orchestrating the observed patterns of starbirth activity are discussed in terms of the extant UV data.
description: Paper format (latex); length of paper (4); 2 encapsulated postscript figure files; uses AIP Press files aipproc.cls, aipproc.sty; Journal Reference: to be published in proceedings in "Star Formation, Near and Far", Proceedings of the 7th annual Astrophysics Conference in Maryland, Steve Holt, Lee G. Mundy, editors
A simple and natural interpretations of the DAMPE cosmic-ray electron/positron spectrum within two sigma deviations
Creators: name: Niu, Jia-Shu
name: Li, Tianjun
name: Xu, Fang-Zhou
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The DArk Matter Particle Explorer (DAMPE) experiment has recently announced the first results for the measurement of total electron plus positron fluxes between 25 GeV and 4.6 TeV. A spectral break at about 0.9 TeV and a tentative peak excess around 1.4 TeV have been found. However, it is very difficult to reproduce both the peak signal and the smooth background including spectral break simultaneously. We point out that the numbers of events in the two energy ranges (bins) close to the 1.4 TeV excess have $1σ$ deficits. With the basic physics principles such as simplicity and naturalness, we consider the $-2σ$, $+2σ$, and $-1σ$ deviations due to statistical fluctuations for the 1229.3~GeV bin, 1411.4~GeV bin, and 1620.5~GeV bin. Interestingly, we show that all the DAMPE data can be explained consistently via both the continuous distributed pulsar and dark matter interpretations, which have $χ^{2} \simeq 17.2 $ and $χ^{2} \simeq 13.9$ (for all the 38 points in DAMPE electron/positron spectrum with 3 of them revised), respectively. These results are different from the previous analyses by neglecting the 1.4 TeV excess. At the same time, we do a similar global fitting on the newly released CALET lepton data, which could also be interpreted by such configurations. Moreover, we present a $U(1)_D$ dark matter model with Breit-Wigner mechanism, which can provide the proper dark matter annihilation cross section and escape the CMB constraint. Furthermore, we suggest a few ways to test our proposal.
description: 18 pages, 6 figures, 5 tables. Figures and Bibs updated
Identifying Biomarkers from Transcriptomic Signatures in Renal Allograft Biopsies Using Deceased and Living Donors
Creators: name: Yang, Bin
name: Sylvius, Nicolas
name: Luo, Jinli
name: Yang, Cheng
name: Da, Zhanyun
name: Crotty, Charlottelrm
name: Nicholson, Michael L.
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine
subject: biomarkers
subject: differentially expressed genes
subject: fibrosis
subject: immunity
subject: inflammation
subject: transplant kidney injury

description: The survival of transplant kidneys using deceased donors (DD) is inferior to living donors (LD). In this study, we conducted a whole-transcriptome expression analysis of 24 human kidney biopsies paired at 30 minutes and 3 months post-transplantation using DD and LD. The transcriptome profile was found significantly different between two time points regardless of donor types. There were 446 differentially expressed genes (DEGs) between DD and LD at 30 minutes and 146 DEGs at 3 months, with 25 genes common to both time points. These DEGs reflected donor injury and acute immune responses associated with inflammation and cell death as early as at 30 minutes, which could be a precious window of potential intervention. DEGs at 3 months mainly represented the changes of adaptive immunity, immunosuppressive treatment, remodeling or fibrosis via different networks and signaling pathways. The expression levels of 20 highly DEGs involved in kidney diseases and 10 genes dysregulated at 30 minutes were found correlated with renal function and histology at 12 months, suggesting they could be potential biomarkers. These genes were further validated by quantitative polymerase chain reaction (qPCR) in 24 samples analysed by microarray, as well as in a validation cohort of 33 time point unpaired allograft biopsies. This analysis revealed that SERPINA3, SLPI and CBF were up-regulated at 30 minutes in DD compared to LD, while FTCD and TASPN7 were up-regulated at both time points. At 3 months, SERPINA3 was up-regulated in LD, but down-regulated in DD, with increased VCAN and TIMP1, and decreased FOS, in both donors. Taken together, divergent transcriptomic signatures between DD and LD, and changed by the time post-transplantation, might contribute to different allograft survival of two type kidney donors. Some DEGs including FTCD and TASPN7 could be novel biomarkers not only for timely diagnosis, but also for early precise genetic intervention at donor preservation, implantation and post-transplantation, in particular to effectively improve the quality and survival of DD.
Isospin Breaking and Instantons in QCD Nucleon Sum Rules
Creators: name: Forkel, Hilmar
name: Nielsen, Marina
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study isospin breaking instanton corrections to the operator product expansion of the nucleon correlation functions. After a comparison with quark model calculations based on the 't Hooft interaction, we examine the role of instantons in the corresponding QCD sum rules. Instanton contributions are found to be absent in the chirally even sum rule, but significant in the chirally-odd one. They improve the consistency of both sum rules and favor a value of the isovector quark condensate close to the chiral estimate.
description: 28 pages, REVTEX file and 5 Postscript figures
Additional file 2: of In-depth proteomic analyses of Haliotis laevigata (greenlip abalone) nacre and prismatic organic shell matrix
Creators: name: Mann, Karlheinz
name: Cerveau, Nicolas
name: Gummich, Meike
name: Fritz, Monika
name: Mann, Matthias
name: Jackson, Daniel
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: Hematology
subject: Plant Biology

description: Table S1. Organic matrix yields. This docx-file shows the organic matrix yields of individual shell fractions as determined by weighing after lyophilisation of acidic extracts. (DOCX 14Â kb)
ML-SIM: universal reconstruction of structured illumination microscopy images using transfer learning.
Creators: name: Christensen, Charles N
name: Ward, Edward N
name: Lu, Meng
name: Lio, Pietro
name: Kaminski, Clemens F
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021

description: Structured illumination microscopy (SIM) has become an important technique for optical super-resolution imaging because it allows a doubling of image resolution at speeds compatible with live-cell imaging. However, the reconstruction of SIM images is often slow, prone to artefacts, and requires multiple parameter adjustments to reflect different hardware or experimental conditions. Here, we introduce a versatile reconstruction method, ML-SIM, which makes use of transfer learning to obtain a parameter-free model that generalises beyond the task of reconstructing data recorded by a specific imaging system for a specific sample type. We demonstrate the generality of the model and the high quality of the obtained reconstructions by application of ML-SIM on raw data obtained for multiple sample types acquired on distinct SIM microscopes. ML-SIM is an end-to-end deep residual neural network that is trained on an auxiliary domain consisting of simulated images, but is transferable to the target task of reconstructing experimental SIM images. By generating the training data to reflect challenging imaging conditions encountered in real systems, ML-SIM becomes robust to noise and irregularities in the illumination patterns of the raw SIM input frames. Since ML-SIM does not require the acquisition of experimental training data, the method can be efficiently adapted to any specific experimental SIM implementation. We compare the reconstruction quality enabled by ML-SIM with current state-of-the-art SIM reconstruction methods and demonstrate advantages in terms of generality and robustness to noise for both simulated and experimental inputs, thus making ML-SIM a useful alternative to traditional methods for challenging imaging conditions. Additionally, reconstruction of a SIM stack is accomplished in less than 200 ms on a modern graphics processing unit, enabling future applications for real-time imaging. Source code and ready-to-use software for the method are available at http://ML-SIM.github.io.
Additional file 6: of Views on and experiences of electronic cigarettes: a qualitative study of women who are pregnant or have recently given birth
Creators: name: Bowker, Katharine
name: Orton, Sophie
name: Cooper, Sue
name: Naughton, Felix
name: Whitemore, Rachel
name: Lewis, Sarah
name: Bauld, Linda
name: Sinclair, Lesley
name: Coleman, Tim
name: Dickinson, Anne
name: Ussher, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Topic Guide Follow up used. Brief description of the data: Topic guide for women for postpartum follow-up interview who in first interview (during pregnancy) said that they were currently using ECs or had previously used them. (DOCX 26 kb)
Quark-Hadron Phase Transitions in Young and Old Neutron Stars
Creators: name: Steiner, A.
name: Prakash, M.
name: Lattimer, J. M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The mixed phase of quarks and hadrons which might exist in the dense matter encountered in the varying conditions of temperature and trapped neutrino fraction in proto-neutron stars is studied. The extent that the mixed phase depends upon the thermodynamical parameters as well as on the stiffness of matter in the hadronic and quark phases is discussed. We show that hadronic equations of state that maximize the quark content of matter at a given {\it density} generally minimize the extent of the mixed phase region in a neutron star of a given mass, and that only in extreme cases could a pure quark star result. For both the Nambu Jona-Lasinio and MIT bag quark models, neutrino trapping inhibits the appearance of a mixed phase which leads to possible proto-neutron star metastability. The main difference between the two quark models is the small abundance of strange quarks in the former. We also demonstrate that $\partial T/\partial n<0$ along adiabats in the quark-hadron mixed phase, opposite to what is found for the kaon condensates-hadron mixed phase. This could lead to core temperatures which are significantly lower in stars containing quarks than in those not containing quarks.
description: 16 pages, 8 figures
title: Einfluss der Qualitätsermittlung kollaborativ erstellter Informationen auf die Gestaltung interorganisationaler Krisenmanagementsysteme
Creators: name: Christofzik, Désirée
name: Reuter, Christian
Publisher: name: GITO mbH Verlag für Industrielle Informationstechnik und Organisation
Year: 2022

description: In dieser Arbeit analysieren wir die Gesamtqualität kollaborativ erstellter Informationen als Aggregation der Qualität von Einzelinformationen indem wir die Angemessenheit verschiedener Funktionen in Abhängigkeit von der jeweiligen Fragestellung betrachten. Ziel ist die Herausstellung von Implikationen für das Design kollaborativer Systeme. Die Untersuchung findet am Beispiel des interorganisationalen Krisenmanagements statt. Nach einer Darstellung möglicher Aggregationsfunktionen zeigen wir auf Basis qualitativ-empirischer Untersuchungen exemplarische Anwendungsfälle aus dem interorganisationalen Krisenmanagement auf. Anhand dieser werden Implikationen für das Design und die Implementierung von Softwarekomponenten für die Vernetzung der beteiligten Akteure gezogen und gezeigt, dass die jeweilige Fragestellung hierbei von besonderer Bedeutung ist.
title: 02_0330
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
The progression of disorder-specific brain pattern expression in schizophrenia over 9 years.
Creators: name: Lieslehto, Johannes
name: Jääskeläinen, Erika
name: Kiviniemi, Vesa
name: Haapea, Marianne
name: Jones, Peter B
name: Murray, Graham K
name: Veijola, Juha
name: Dannlowski, Udo
name: Grotegerd, Dominik
name: Meinert, Susanne
name: Hahn, Tim
name: Ruef, Anne
name: Isohanni, Matti
name: Falkai, Peter
name: Miettunen, Jouko
name: Dwyer, Dominic B
name: Koutsouleris, Nikolaos
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021

description: Age plays a crucial role in the performance of schizophrenia vs. controls (SZ-HC) neuroimaging-based machine learning (ML) models as the accuracy of identifying first-episode psychosis from controls is poor compared to chronic patients. Resolving whether this finding reflects longitudinal progression in a disorder-specific brain pattern or a systematic but non-disorder-specific deviation from a normal brain aging (BA) trajectory in schizophrenia would help the clinical translation of diagnostic ML models. We trained two ML models on structural MRI data: an SZ-HC model based on 70 schizophrenia patients and 74 controls and a BA model (based on 561 healthy individuals, age range = 66 years). We then investigated the two models' predictions in the naturalistic longitudinal Northern Finland Birth Cohort 1966 (NFBC1966) following 29 schizophrenia and 61 controls for nine years. The SZ-HC model's schizophrenia-specificity was further assessed by utilizing independent validation (62 schizophrenia, 95 controls) and depression samples (203 depression, 203 controls). We found better performance at the NFBC1966 follow-up (sensitivity = 75.9%, specificity = 83.6%) compared to the baseline (sensitivity = 58.6%, specificity = 86.9%). This finding resulted from progression in disorder-specific pattern expression in schizophrenia and was not explained by concomitant acceleration of brain aging. The disorder-specific pattern's progression reflected longitudinal changes in cognition, outcomes, and local brain changes, while BA captured treatment-related and global brain alterations. The SZ-HC model was also generalizable to independent schizophrenia validation samples but classified depression as control subjects. Our research underlines the importance of taking account of longitudinal progression in a disorder-specific pattern in schizophrenia when developing ML classifiers for different age groups.
Probe $CP$-violating $Hγγ$ coupling through interferometry
Creators: name: Wan, Xia
name: Wang, You-Kai
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The diphoton invariant mass distribution of interference between $gg\to H \to γγ$ and $gg\to γγ$ is almost antisymmetric around the Higgs mass $M_H$. We propose a new observable $A_{\text{int}}$ to quantify this effect, which is a ratio of a sign-reversed integral around $M_H$ ( e.g. $\int^{M_H}_{M_H-5~\mbox{GeV}} -\int_{M_H}^{M_H+5~\mbox{GeV}}$) and the cross section of the Higgs signal. We study $A_{\text{int}}$ both in Standard Model (SM) and new physics with various $CP$-violating $Hγγ$ couplings. The $A_{\text{int}}$ in SM could reach a value of $10\%$, while for $CP$-violating $Hγγ$ couplings $A_{\text{int}}$ could range from $10\%$ to $-10\%$, which is probable to be detected in HL-LHC experiment. The $A_{\text{int}}$ with both $CP$-violating $Hγγ$ and $Hgg$ couplings are also studied and its value range is further extended.
description: 8 pages, 7 figures, to be published in Chinese Physics C
Additional file 5: of Views on and experiences of electronic cigarettes: a qualitative study of women who are pregnant or have recently given birth
Creators: name: Bowker, Katharine
name: Orton, Sophie
name: Cooper, Sue
name: Naughton, Felix
name: Whitemore, Rachel
name: Lewis, Sarah
name: Bauld, Linda
name: Sinclair, Lesley
name: Coleman, Tim
name: Dickinson, Anne
name: Ussher, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Topic Guide postpartum never used. Brief description of the data: Topic guide for women who are postpartum and have never used ECs. (DOC 56 kb)
An Empirical Test and Calibration of H II Region Diagnostics
Creators: name: Kennicutt,, R. C.
name: Bresolin, F.
name: French, H.
name: Martin, P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present spectrophotometry in the 3600-9700 A region for a sample of 39 H II regions in the Galaxy and Magellanic Clouds, for which independent information is available on the spectral types and effective temperatures of the ionizing stars. The spectra have been used to evaluate nebular diagnostics of stellar temperature, metal abundance, and ionization parameter, and compare the observed behavior of the line indices with predictions of nebular photoionization models. We observe a strong degeneracy between forbidden-line sequences produced by changes in stellar Teff and metal abundance, which severely complicates the application of many forbidden-line diagnostics to extragalactic H II regions. Our data confirm however that the Edmunds and Pagel [O II]+[O III] abundance index and the Vilchez and Pagel `eta' index provide more robust diagnostics of metal abundance and stellar effective temperature, respectively. A comparison of the fractional helium ionization of the H II regions with stellar temperature confirms the reliability of the spectral type vs Teff calibration for the relevant temperature range Teff < 38000 K. We use empirical relations between the nebular hardness indices and Teff to reinvestigate the case for systematic variations in the stellar effective temperatures and the upper IMFs of massive stars in extragalactic H II regions. The data are consistent with a significant softening of the ionizing spectra (consistent with cooler stellar temperatures) with increasing metal abundance, especially for Z less than solar. However unresolved degeneracies between Z and Teff still complicate the interpretation of this result.
description: 28 pages, 14 figures, 2 tables. To appear in The Astrophysical Journal
On the Hasse principle for quartic hypersurfaces
Creators: name: Marmon, Oscar
name: Vishe, Pankaj
Publisher: name: arXiv
Year: 2017
Subjects: subject: Number Theory (math.NT)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 11D72 (Primary) 11P55, 14G05 (Secondary)

description: We establish the Hasse principle for smooth projective quartic hypersurfaces of dimension greater than or equal to 28 defined over $\mathbb{Q}$.
description: 50 pages, 1 figure, revision
Additional file 27: of In-depth proteomic analyses of Haliotis laevigata (greenlip abalone) nacre and prismatic organic shell matrix
Creators: name: Mann, Karlheinz
name: Cerveau, Nicolas
name: Gummich, Meike
name: Fritz, Monika
name: Mann, Matthias
name: Jackson, Daniel
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Figure S2. Sequences and repeat structure of uncharacterized major proteins. Sequence regions covered by identified peptides are shown in bold green. Predicted signal sequence peptides are underlined. Collagen triple-helical sequences are in italics. In sequence alignments identical amino acids are shaded yellow. (DOCX 75Â kb)
New Collider Bound on Light Gravitino Mass
Creators: name: Dicus, Duane A.
name: Nandi, S.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In supergravity theories with a very light gravitino, the gluino decays dominantly to a gluon and a gravitino. This results in a much larger missing $E_T$ for the multijet final states in hadronic colliders. We use the latest Tevatron data for the multijet final states to set a new absolute lower bound of 3.0 x 10^{-13} GeV for the light gravitino mass.
description: 9 pages, Latex, macros and 2 figures not included
Resummed Photon Spectra for WIMP Annihilation
Creators: name: Baumgart, Matthew
name: Cohen, Timothy
name: Moult, Ian
name: Rodd, Nicholas L.
name: Slatyer, Tracy R.
name: Solon, Mikhail P.
name: Stewart, Iain W.
name: Vaidya, Varun
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We construct an effective field theory (EFT) description of the hard photon spectrum for heavy WIMP annihilation. This facilitates precision predictions relevant for line searches, and allows the incorporation of non-trivial energy resolution effects. Our framework combines techniques from non-relativistic EFTs and soft-collinear effective theory (SCET), as well as its multi-scale extensions that have been recently introduced for studying jet substructure. We find a number of interesting features, including the simultaneous presence of SCET$_{\text{I}}$ and SCET$_{\text{II}}$ modes, as well as collinear-soft modes at the electroweak scale. We derive a factorization formula that enables both the resummation of the leading large Sudakov double logarithms that appear in the perturbative spectrum, and the inclusion of Sommerfeld enhancement effects. Consistency of this factorization is demonstrated to leading logarithmic order through explicit calculation. Our final result contains both the exclusive and the inclusive limits, thereby providing a unifying description of these two previously-considered approximations. We estimate the impact on experimental sensitivity, focusing for concreteness on an SU(2)$_{W}$ triplet fermion dark matter - the pure wino - where the strongest constraints are due to a search for gamma-ray lines from the Galactic Center. We find numerically significant corrections compared to previous results, thereby highlighting the importance of accounting for the photon spectrum when interpreting data from current and future indirect detection experiments.
description: 55+25 pages, 11+2 figures; v3, updated an expression in the appendix to make it applicable at higher order - no impact on the results in this work
Statistical properties of SGR 1806-20 bursts
Creators: name: Gogus, Ersin
name: Woods, Peter M.
name: Kouveliotou, Chryssa
name: van Paradijs, Jan
name: Briggs, Michael S.
name: Duncan, Robert C.
name: Thompson, Christopher
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present statistics of SGR 1806-20 bursts, combining 290 events detected with RXTE/PCA, 111 events detected with BATSE and 134 events detected with ICE. We find that the fluence distribution of bursts observed with each instrument are well described by power laws with indices 1.43, 1.76 and 1.67, respectively. The distribution of time intervals between successive bursts from SGR 1806-20 is described by a lognormal function with a peak at 103 s. There is no correlation between the burst intensity and either the waiting times till the next burst or the time elapsed since the previous burst. In all these statistical properties, SGR 1806-20 bursts resemble a self-organized critical system, similar to earthquakes and solar flares. Our results thus support the hypothesis that the energy source for SGR bursts is crustquakes due to the evolving, strong magnetic field of the neutron star, rather than any accretion or nuclear power.
description: 11 pages, 4 figures, To appear in ApJ Letters
title: Integraal Plan Boven-Zeeschelde: sub report 16. Effect of the C-alternatives on the hydrodynamics
Creators: name: Bi, Qilong
name: Vanlede, Joris
name: Smolders, Sven
name: Mostaert, Frank
Publisher: name: Flanders Hydraulics Research
Year: 2021

description: In the project “Integral Plan for the Upper Sea Scheldt”, a 3D Scaldis-model of the tidal Scheldt estuary is used to analyse the effects of several bathymetry alternatives under different climate scenarios (boundary conditions). This report focuses on the effects of C alternatives on the hydrodynamics under 3 different boundary conditions: A0CN, AminCL and AplusCH. The model results are analysed in terms of water levels, harmonic components, velocities, and tidal asymmetry. The input for the subsequent ecotope analysis (inundation frequency, frequency of the flow velocity that exceeds 0.65 m/s and frequency of the bed shear stress that exceeds 1 Pa) is also presented .
description: Title : FHR reports. Flanders Hydraulics Research: Antwerp Volume : 13_131_16 Issue : Pagination : VIII, 60 + 36 p. app.
Derivation of the Lamb Shift using an Effective Field Theory
Creators: name: Labelle, Patrick
name: Zebarjad, S. Mohammad
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We rederive the $O(α^5)$ shift of the hydrogen levels in the non-recoil ($m_e/m_P \to 0$) limit using Nonrelativistic QED (NRQED), an effective field theory developed by Caswell and Lepage (Phys. Lett. 167B, 437 (1986)). Our result contains the Lamb shift as a special case. Our calculation is far simpler than traditional approaches and has the advantage of being systematic. It also clearly illustrates the need to renormalize (or ``match'') the coefficients of the effective theory beyond tree level.
description: 15 pages, 11 Postscript figures, uses Latex2e and epsf.tex
W-STEM website
Creators: name: García-Holgado, A.
name: García-Peñalvo, F. J.
Publisher: name: Zenodo
Year: 2019
Subjects: CBHE, EU, gender, STEM, W-STEM

description: Presentation of the novelties of the W-STEM project website, made in the 2nd face-to-face meeting of the W-STEM ERASMUS + Capacity-building in Higher Education European Project (Ref. 598923-EPP-1-2018-1-ES-EPPKA2-CBHE-JP), which was held in the Universidad del Norte, Barranquilla (Colombia), 27-29 November 2019.
description: W-STEM (Building the future of Latin America: engaging women into STEM) is a project funded under European Union ERASMUS + Capacity-building in Higher Education Programme (598923-EPP-1-2018-1-ES-EPPKA2-CBHE-JP). The European Commission support for the production of this publication does not constitute an endorsement of the contents which reflects the views only of the authors, and the Commission cannot be held responsi­ble for any use which may be made of the information contained therein.
Building a stem cell-based primate uterus.
Creators: name: Bergmann, Sophie
name: Schindler, Magdalena
name: Munger, Clara
name: Penfold, Christopher A
name: Boroviak, Thorsten E
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021

description: Funder: Wellcome Trust
description: The uterus is the organ for embryo implantation and fetal development. Most current models of the uterus are centred around capturing its function during later stages of pregnancy to increase the survival in pre-term births. However, in vitro models focusing on the uterine tissue itself would allow modelling of pathologies including endometriosis and uterine cancers, and open new avenues to investigate embryo implantation and human development. Motivated by these key questions, we discuss how stem cell-based uteri may be engineered from constituent cell parts, either as advanced self-organising cultures, or by controlled assembly through microfluidic and print-based technologies.
Additional file 4: of Views on and experiences of electronic cigarettes: a qualitative study of women who are pregnant or have recently given birth
Creators: name: Bowker, Katharine
name: Orton, Sophie
name: Cooper, Sue
name: Naughton, Felix
name: Whitemore, Rachel
name: Lewis, Sarah
name: Bauld, Linda
name: Sinclair, Lesley
name: Coleman, Tim
name: Dickinson, Anne
name: Ussher, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Topic Guide postpartum users or used. Brief description of the data: Topic guide for women who are postpartum and are currently using ECs or have previously used them. (DOCX 28 kb)
Fine structure of alpha decay in odd nuclei
Creators: name: Mirea, M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Using an alpha decay level scheme, an explanation for the fine structure in odd nuclei is evidenced by taking into account the radial and rotational couplings between the unpaired nucleon and the core of the decaying system. It is stated that the experimental behavior of the alpha decay fine structure phenomenon is directed by the dynamical characteristics of the system.
description: 8 pages, 3 figures, REVTex, submitted to Physical Review C
Testing gravity on cosmological scales with cosmic shear, cosmic microwave background anisotropies, and redshift-space distortions
Creators: name: Ferté, Agnès
name: Kirk, Donnacha
name: Liddle, Andrew R.
name: Zuntz, Joe
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use a range of cosmological data to constrain phenomenological modifications to general relativity on cosmological scales, through modifications to the Poisson and lensing equations. We include cosmic microwave background anisotropy measurements from the Planck satellite, cosmic shear from CFHTLenS and DES-SV, and redshift-space distortions from BOSS data release 12 and the 6dF galaxy survey. We find no evidence of departures from general relativity, with the modified gravity parameters constrained to $Σ_0 = 0.05^{+0.05}_{-0.07}$ and $μ_0 = -0.10^{+0.20}_{-0.16}$, where $Σ_0$ and $μ_0$ refer to deviations from general relativity today and are defined to be zero in general relativity. We also forecast the sensitivity to those parameters of the full five-year Dark Energy Survey and of an experiment like the Large Synoptic Survey Telescope, showing a substantial expected improvement in the constraint on $Σ_0$.
description: 12 pages, 10 figures
Media representations of opposition to the 'junk food advertising ban' on the Transport for London (TfL) network: A thematic content analysis of UK news and trade press.
Creators: name: Thompson, Claire
name: Clary, Christelle
name: Er, Vanessa
name: Adams, Jean
name: Boyland, Emma
name: Burgoine, Thomas
name: Cornelsen, Laura
name: De Vocht, Frank
name: Egan, Matt
name: Lake, Amelia A
name: Lock, Karen
name: Mytton, Oliver
name: Petticrew, Mark
name: White, Martin
name: Yau, Amy
name: Cummins, Steven
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021
Subjects: Regulation
Media
Advertising
Childhood Obesity

description: BackgroundAdvertising of less healthy foods and drinks is hypothesised to be associated with obesity in adults and children. In February 2019, Transport for London implemented restrictions on advertisements for foods and beverages high in fat, salt or sugar across its network as part of a city-wide strategy to tackle childhood obesity. The policy was extensively debated in the press. This paper identifies arguments for and against the restrictions. Focusing on arguments against the restrictions, it then goes on to deconstruct the discursive strategies underpinning them.MethodsA qualitative thematic content analysis of media coverage of the restrictions (the 'ban') in UK newspapers and trade press was followed by a document analysis of arguments against the ban. A search period of March 1, 2018 to May 31, 2019 covered: (i) the launch of the public consultation on the ban in May 2018; (ii) the announcement of the ban in November 2018; and (iii) its implementation in February 2019. A systematic search of printed and online publications in English distributed in the UK or published on UK-specific websites identified 152 articles.ResultsArguments in favour of the ban focused on inequalities and childhood obesity. Arguments against the ban centred on two claims: that childhood obesity was not the 'right' priority; and that an advertising ban was not an effective way to address childhood obesity. These claims were justified via three discursive approaches: (i) claiming more 'important' priorities for action; (ii) disputing the science behind the ban; (iii) emphasising potential financial costs of the ban.ConclusionThe discursive tactics used in media sources to argue against the ban draw on frames widely used by unhealthy commodities industries in response to structural public health interventions. Our analyses highlight the need for interventions to be framed in ways that can pre-emptively counter common criticisms.
The Asiago-ESO/RASS QSO Survey. I.The Catalog and the Local QSO Luminosity Function
Creators: name: Grazian, A.
name: Cristiani, S.
name: D'Odorico, V.
name: Omizzolo, A.
name: Pizzella, A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper presents the first results of a survey for bright quasars (V < 14.5 and R<15.4) covering the North Hemisphere at galactic latitudes |b|>30. The photometric database is derived from the GSC and USNO catalogs. Quasars are identified on the basis of their X-ray emission measured in the ROSAT All Sky Survey. The surface density of quasars brighter than 15.5 mag turns out to be $9 \pm 1 \cdot 10^{-3} deg^{-2}$, about 3 times higher than that estimated by the PG survey. The quasar optical Luminosity Function (LF) at $0.04 < z \le 0.3$ is computed and shown to be consistent with a Luminosity Dependent Luminosity Evolution of the type derived by La Franca and Cristiani (1997) in the range $0.3 < z \le 2.2$. The predictions of semi-analytical models of hierarchical structure formation agree remarkably well with the present observations.
description: 54 pages Latex, with 7 PostScript figures. Some minor changes. Astronomical Journal, in press
Extragalactic Results from the Infrared Space Observatory
Creators: name: Genzel, Reinhard
name: Cesarsky, Catherine J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: More than a decade ago the IRAS satellite opened the realm of external galaxies for studies in the 10 to 100 micron band and discovered emission from tens of thousands of normal and active galaxies. With the 1995-1998 mission of the Infrared Space Observatory the next major steps in extragalactic infrared astronomy became possible: detailed imaging, spectroscopy and spectro-photometry of many galaxies detected by IRAS, as well as deep surveys in the mid- and far- IR. The spectroscopic data reveal a wealth of detail about the nature of the energy source(s) and about the physical conditions in galaxies. ISO's surveys for the first time explore the infrared emission of distant, high-redshift galaxies. ISO's main theme in extragalactic astronomy is the role of star formation in the activity and evolution of galaxies.
description: 106 pages, including 17 figures. Ann.Rev.Astron.Astrophys. (in press), a gzip'd pdf file (667kB) is also available at http://www.mpe.mpg.de/www_ir/preprint/annrev2000.pdf.gz