cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dietary protein intake from different animal and plant sources plays a minor role in the bone health of adults with or without intermittent fasting for decades
Creators: name: Rodopaios, Nikolaos E.
name: Mougios, Vassilis
name: Koulouri, Alexandra-Aikaterini
name: Vasara, Eleni
name: Papadopoulou, Sousana K.
name: Skepastianos, Petros
name: Hassapidou, Maria
name: Kafatos, Anthony G.
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: Plant Biology
subject: Computational Biology

description: We examined whether bone health is related to protein intake from different sources by utilising a distinct, rare dietary pattern: avoidance of animal foods for approximately half of the year according to Christian Orthodox Church fasting. Four-hundred adults, of whom 200 had been following religious fasting for a median of 15 years and 200 were non-fasters, underwent anthropometry, measurements of bone mineral density (BMD) and bone mineral content (BMC), and completed a food frequency questionnaire. Groups did not differ significantly in anthropometric measures, BMD, or BMC. Fasters had higher consumption of seafood and lower consumption of red meat, poultry-eggs, dairy products, and grains-cereals than non-fasters. Protein intake from these food groups exhibited similar differences; overall, fasters had lower protein intake than non-fasters. BMD and BMC were positively, though weakly, correlated with red meat and poultry-egg consumption. Thus, protein intake seems to play a minor (if any) role in bone health.
A within-trial cost-effectiveness analysis of panitumumab compared with bevacizumab in the first-line treatment of patients with wild-type RAS metastatic colorectal cancer in the US
Creators: name: Graham, Christopher N.
name: Christodoulopoulou, Alexandra
name: Hediyyih N. Knox
name: Sabatelli, Lorenzo
name: Hechmati, Guy
name: Garawin, Tamer
name: Strickler, John H.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: Medicine
Pharmacology
Cancer
Science Policy

description: Aims: This analysis investigated the cost-effectiveness of panitumumab plus mFOLFOX6 (oxaliplatin, 5-fluorouracil, and leucovorin) compared with bevacizumab plus mFOLFOX6 in the first-line treatment of patients with wild-type RAS metastatic colorectal cancer (mCRC). Materials and methods: The cost-effectiveness analysis was developed from a third-party payer perspective in the US and was implemented using a partitioned survival model with health states for first-line treatment (progression-free), disease progression with and without subsequent active treatment, and death. Survival analyses of patients with wild-type RAS mCRC from the PEAK head-to-head clinical trial of panitumumab vs bevacizumab were performed to estimate time in the model health states. Additional data from PEAK informed the amount of each drug consumed, duration of therapy, subsequent therapy use, and toxicities related to mCRC treatment. Literature and US public data sources were used to estimate unit costs associated with treatment and duration of subsequent active therapies. Utility weights were calculated from patient-level data from panitumumab trials in the first-, second-, and third-line settings. A life-time perspective was taken with future costs and outcomes discounted at 3% per annum. Scenario, one-way, and probabilistic sensitivity analyses were performed. Results: Compared with bevacizumab, the use of panitumumab resulted in an incremental cost of US $60,286, and an incremental quality-adjusted life-year (QALY) of 0.445, translating into a cost per QALY gained of US $135,391 in favor of panitumumab. Results were sensitive to wastage and dose rounding assumptions modeled. Limitations: Progression-free and overall survival were extrapolated beyond the follow-up of the primary analysis using fitted parametric curves. Costs and quality of life were estimated from multiple and different data sources. Conclusions: The efficacy of panitumumab in extending progression-free and overall survival and improving quality of life makes it a cost-effective option for first-line treatment of patients with wild-type RAS mCRC compared with bevacizumab.
Uncertainty product of spherical wavelets
Creators: name: Iglewska-Nowak, Ilona
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 42C40

description: In the paper, asymptotic behavior of the uncertainty product for a family of zonal spherical wavelets is computed. The family contains the most popular wavelets, such as Gauss-Weierstrass, Abel-Poisson and Poisson wavelets and Mexican needlets. Boundedness of the uncertainty constant is in general not given, but it is a property of some of the wavelets from this class.
description: 12 pages
Buccinum crenulatum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum crenulatum

description: Buccinum crenulatum [spec. nov.]
B. testa turrita, anfractibus margine crenatis.
Gvalt. test. t. 57. f. L.
Argenv. conch. t. 14. f. r.
Habitat in O. Africano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 741, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. IX 10 New Observations of Reverberation Mapping and Shortened H$β$ Lags
Creators: name: Du, Pu
name: Zhang, Zhi-Xiang
name: Wang, Kai
name: Huang, Ying-Ke
name: Zhang, Yue
name: Lu, Kai-Xing
name: Hu, Chen
name: Li, Yan-Rong
name: Bai, Jin-Ming
name: Bian, Wei-Hao
name: Yuan, Ye-Fei
name: Ho, Luis C.
name: Wang, Jian-Min
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: As one of the series of papers reporting on a large reverberation mapping campaign of super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs), we present the results of 10 SEAMBHs monitored spectroscopically during 2015-2017. Six of them are observed for the first time, and have generally higher 5100 Å luminosities than the SEAMBHs monitored in our campaign from 2012 to 2015; the remaining four are repeat observations to check if their previous lags change. Similar to the previous SEAMBHs, the H$β$ time lags of the newly observed objects are shorter than the values predicted by the canonical $R_{\mathrm{Hβ}}$-$L_{5100}$ relation of sub-Eddington AGNs, by factors of $\sim2-6$, depending on the accretion rate. The four previously observed objects have lags consistent with previous measurements. We provide linear regressions for the $R_{\mathrm{Hβ}}$-$L_{5100}$ relation, solely for the SEAMBH sample and for low-accretion AGNs. We find that the relative strength of Fe II and the profile of the H$β$ emission line can be used as proxies of accretion rate, showing that the shortening of H$β$ lags depends on accretion rates. The recent SDSS-RM discovery of shortened H$β$ lags in AGNs with low accretion rates provides compelling evidence for retrograde accretion onto the black hole. These evidences show that the canonical $R_{\mathrm{Hβ}}$-$L_{5100}$ relation holds only in AGNs with moderate accretion rates. At low accretion rates, it should be revised to include the effects of black hole spin, whereas the accretion rate itself becomes a key factor in the regime of high accretion rates.
description: 22 pages, 8 figures, 10 tables, accepted for publication in The Astrophysical Journal
The effect of probiotics, parabiotics, synbiotics, fermented foods and other microbial forms on immunoglobulin production: a systematic review and meta-analysis of clinical trials
Creators: name: Kazemi, Asma
name: Soltani, Sepideh
name: Nasri, Fatemeh
name: Clark, Cain C. T.
name: Kolahdouz-Mohammadi, Roya
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Science Policy

description: The aim of this systematic review and meta-analysis was to evaluate the effect of probiotics, parabiotics, synbiotics, fermented foods and other microbial forms on immunoglobulin production. We searched PubMed, Scopus, Web of Science, National Institute of Health Clinical Trials Register, and Cochrane Central Register of Clinical Trials, up to February 2020. All clinical trials that investigated the effects of oral intake of probiotics, parabiotics, synbiotics, fermented foods and other microbial forms on immunoglobulin (Ig)A, IgE, Japanese cedar pollen (JCP)-specific IgE, IgG, and IgM, for a duration of >7 days were included. Fifty-nine studies met the inclusion criteria, of these 54 studies were included in the analysis. The results indicated a significant increase in salivary IgA secretion rate (SMD = 0.21, 95% CI 0.02–0.39), while no significant effect was observed on other Igs. In conclusion, mentioned supplementation induced a small but significant effect on salivary secretion rate of IgA.
Poisson wavelets on $n$-dimensional spheres
Creators: name: Iglewska-Nowak, Ilona
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 42C40

description: In this paper, Poisson wavelets on $n$-dimensional spheres, derived from Poisson kernel, are introduced and characterized. We compute their Gegenbauer expansion with respect to the origin of the sphere, as well as with respect to the field source. Further, we give recursive formulae for their explicit representations and we show how the wavelets are localized in space. Also their Euclidean limit is calculated explicitly and its space localization is described. We show that Poisson wavelets can be treated as wavelets derived from approximate identities and we give two inversion formulae.
description: 17 pages
The estimated intake of palm oil in Spain and Germany
Creators: name: Hearty, Aine P.
name: Berg, Iekje
name: Coenradie, Alwin
name: Drieduite, Nicolette
name: Gambelli, Luisa
name: Logman, Margaret
name: Soler, Jordi
name: Tiesinga, Imkje
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Palm oil is one of the most widely used vegetable oils by the food industry but there is limited information on actual intake. A detailed intake assessment of palm oil for Spain and Germany was conducted. For Spain, mean palm oil intakes ranged from 2.06 g/day in the elderly to 4.54 g/day in children and adolescents, while high-level intakes ranged from 10.34 g/day in the elderly to 20.88 g/day in toddlers. For Germany, mean palm oil intakes ranged from 3.06 g/day in toddlers to 6.22 g/day in the very elderly, while high-level intakes ranged from 13.61 g/day in toddlers to 30.10 g/day in the elderly. For both countries, the main contributing food categories to mean palm oil intake were biscuits, cakes, bread, breakfast cereal and margarine. In summary, the present paper provides a realistic assessment of the intake of palm oil in two EU countries for different population groups.
Προγνωστική δημοσιογραφία δεδομένων : Η περίπτωση της αθλητικής δημοσιογραφίας
Creators: name: Παγούνας, Άγγελος Θωμά
Publisher: name: Aristotle University of Thessaloniki
Year: 2025
Subjects: προγνωστική δημοσιογραφία
αθλητισμός
στοίχημα
predictive journalism
sports
betting

description: Ο σκοπός της διπλωματικής εργασίας ήταν η αναλυτική παρουσίαση της προγνωστικής δημοσιογραφίας, εστιάζοντας στην αθλητική δημοσιογραφία και τη διερεύνηση της κατάστασης στον ελληνικό μιντιακό χώρο σχετικά με τη δημοσίευση αθλητικών άρθρων που εμπίπτουν σε αυτή την κατηγορία. Επιπλέον, μέσω ποσοτικής έρευνας, εξετάστηκε η στάση των αναγνωστών απέναντι σε άρθρα προγνωστικής δημοσιογραφίας. Στην εργασία, προσδιορίστηκαν τα χαρακτηριστικά της προγνωστικής δημοσιογραφίας, η οποία ορίστηκε ως ένα αναδυόμενο είδος δημοσιογραφίας που ενσωματώνει εκτιμήσεις και προβλέψεις. Η μελέτη των δημοσιευμένων άρθρων έδειξε ότι η ελληνική αθλητική δημοσιογραφία χωρίζεται σε δύο κατηγορίες: άρθρα με προγνωστικά αγώνων και άρθρα με έμμεσα προγνωστικά αγώνων. Για την διερεύνηση των στάσεων των Ελλήνων αναγνωστών έγινε ποσοτική έρευνα με δομημένο ερωτηματολόγιο σε ένα δείγμα ευκολίας Ν=20 άτομα, κυρίως παίκτες στοιχήματος. Τα αποτελέσματα έδειξαν ότι η πλειοψηφία του δείγματος είναι εξοικειωμένοι με τον όρο «προγνωστική δημοσιογραφία» και ενδιαφέρεται για την ανάγνωση αυτών των άρθρων. Αν και το 80% ανέφερε ότι διαβάζει άρθρα πριν από έναν αγώνα, το 45% ανέφερε ότι δεν επηρεάζεται αυτά. Το 50% εμπιστεύεται συγκεκριμένες πηγές προγνωστικών και εκφράζει την επιθυμία για αξιόπιστες και τεκμηριωμένες πληροφορίες.
description: The purpose of the Dissertation was the analytical presentation of predictive journalism, focusing on sports journalism and the investigation of the situation in the Greek media sector regarding the publication of sports articles that fall into this category. Furthermore, through a quantitative survey, the attitude of readers towards articles of predictive journalism was examined. In the paper, the characteristics of predictive journalism were identified, which was defined as an emerging genre of journalism that incorporates assessments and predictions. The study of published articles showed that Greek sports journalism is divided into three categories: articles with match predictions, articles with indirect predictions and articles on artificial intelligence, with the first two categories predominating. To investigate the attitudes of Greek readers, a quantitative survey with a structured questionnaire was conducted on a convenience sample of N=20 people, mainly bettors. The results showed that most of the sample are familiar with the term "predictive journalism" and are interested in reading these articles. Although 80% reported reading articles before a match, 45% reported not being influenced by them. 50% trusted specific sources of predictive journalism and expressed a desire for reliable and informed information.
Boiling crisis dynamics: low gravity experiments at high pressure
Creators: name: Nikolayev, Vadim
name: Garrabos, Yves
name: Lecoutre, Carole
name: Charignon, T.
name: Hitz, Denis
name: Chatain, Denis
name: Guillaument, Romain
name: Marre, Samuel
name: Beysens, Daniel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Physics (physics.class-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: To understand the boiling crisis mechanism, one can take advantage of the slowing down of boiling at high pressures, in the close vicinity of the liquid-vapor critical point of the given fluid. To preserve conventional bubble geometry, such experiments need to be carried out in low gravity. We report here two kinds of saturated boiling experiments. First we discuss the spatial experiments with SF$_6$ at 46$^\circ$ C. Next we address two ground-based experiments under magnetic gravity compensation with H$_2$ at 33 K. We compare both kinds of experiments and show their complementarity. The dry spots under vapor bubbles are visualized by using transparent heaters made with metal oxide films. We evidence two regimes of the dry spots growth: the regime of circular dry spots and the regime of chain coalescence of dry spots that immediately precedes the heater dryout. A recent H$_2$ experiment is shown to bridge the gap between the near-critical and low pressure boiling experiments.
Additional file 1 of Differential effects of sound interventions tuned to 432 Hz or 443 Hz on cardiovascular parameters in cancer patients: a randomized cross-over trial
Creators: name: Hohneck, Anna
name: Rodríguez, Ánxelo Maia
name: Weingärtner, Simone
name: Merx, Kirsten
name: Sarodnick, Felicitas
name: von Gagern, Fritjof
name: Mavratzas, Athanasios
name: Burkholder, Iris
name: Schumacher, Gerhard
name: Hofmann, Wolf-Karsten
name: Hofheinz, Ralf-Dieter
Publisher: name: figshare
Year: 2025
Subjects: Medicine
Cell Biology
Neuroscience
Biological Sciences not elsewhere classified
Science Policy
Mental Health

description: Supplementary Material 1
Frustration and anisotropic exchange in ytterbium magnets with edge-shared octahedra
Creators: name: Rau, Jeffrey G.
name: Gingras, Michel J. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider the structure of anisotropic exchange interactions in ytterbium-based insulating rare-earth magnets built from edge-sharing octahedra. We argue the features of trivalent ytterbium and this structural configuration allow for a qualitative determination of the different anisotropic exchange regimes that may manifest in such compounds. The validity of such super-exchange calculations is tested through comparison to the well-characterized breathing pyrochlore compound Ba$_3$Yb$_2$Zn$_5$O$_{11}$. With this in hand, we then consider application to three-dimensional pyrochlore spinels as well as two-dimensional honeycomb and triangular lattice systems built from such edge-sharing octahedra. We find an extended regime of robust emergent weak anisotropy with dominant antiferromagnetic Heisenberg interactions as well as smaller regions with strong anisotropy. We discuss the implications of our results for known compounds with the above structures, such as the spinels AYb$_2$X$_4$ (A = Cd, Mg, X = S, Se), the triangular compound YbMgGaO$_4$, which have recently emerged as promising candidates for observing unconventional magnetic phenomena. Finally, we speculate on implications for the R$_2$M$_2$O$_7$ pyrochlore compounds and some little studied honeycomb ytterbium magnets.
description: 25 pages, 9 figures
Semi-continuous and discrete wavelet frames on $n$-dimensional spheres
Creators: name: Iglewska-Nowak, Ilona
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 42C40

description: The paper shows that under some mild conditions $n$-dimensional spherical wavelets derived from approximate identities build semi-continuous frames. Moreover, for sufficiently dense grids Poisson wavelets on $n$-dimensional spheres constitute a discrete frame. In the proof we only use the localization properties of the reproducing kernel and its gradient.
description: 28 pages
МOТИВAЦИЯ ПЕДAГOГИЧЕСКOЙ ДЕЯТЕЛЬНOСТИ, ФOРМИРOВAНИЕ ПЕДAГOГИЧЕСКOЙ НAПРAВЛЕННOСТИ СПЕЦИAЛИСТA ПO ФИЗИЧЕСКOЙ КУЛЬТУРЕ
Creators: name: Мирбабаев, Музаффар
name: Раимов, Шахзод
Publisher: name: Zenodo
Year: 2024

description: Нaстрoеннoсть нa педaгoгическую деятельнoсть в сфере физическoй культуры и спoртa прoявляется еще в шкoльнoм вoзрaсте в мoтивaх выбoрa oднoй из физкультурнo-педaгoгических прoфессий, кoтoрaя трaнсфoрмируется в мoтивaцию учебнoй деятельнoсти в вузе и, дaлее в педaгoгическую нaпрaвленнoсть прoфессиoнaльнoй деятельнoсти.
Optical Luminosities and Mass--to--Light Ratios of Nearby Galaxy Clusters
Creators: name: Girardi, M.
name: Borgani, S.
name: Giuricin, G.
name: Mardirossian, F.
name: Mezzetti, M.
name: ;
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze a sample of 105 clusters having virial mass homogeneously estimated and for which galaxy magnitudes are available with a well defined high degree of completeness. In particular, we consider a subsample of 89 clusters with B_j band galaxy magnitudes taken from the COSMOS/UKST Southern Sky Object Catalogue. We compute cluster luminosities L_{B_j} within several clustercentric distances and within the virialization radius R_{vir}. In particular, we use the luminosity function and background counts estimated by Lumsden et al. (1997) on the Edinburgh/Durham Southern Galaxy Catalogue. We analyze the effect of several uncertainties connected to photometric data, fore/background removal, and extrapolation below the completeness limit of the photometry, in order to assess the robustness of our cluster luminosity estimates. We draw our results on the relations between luminosity and dynamical quantities from the COSMOS sample by considering mass and luminosities determined within the virialization radius. We find a very good correlation between cluster luminosity, L_{B_j}, and galaxy velocity dispersion, sigma_v, with L_{B_j} proportional to sigma_v^{2.1--2.3}. Our estimate of typical value for the mass-to-light ratio is M/L_{B_j} about 250 (in solar units). We do not find any correlation of M/L_{B_j} with cluster morphologies, i.e. Rood--Sastry and Bautz--Morgan types, and only a weak significant correlation with cluster richness. We find that mass has a slight, but significant, tendency to increase faster than the luminosity does, M proportional to L_{B_j}^{1.2--1.3}. We verify the robustness of this relation against a number of possible systematics.
description: 18 pages, 6 eps figures, accepted by ApJ
Towards a comprehensive compendium of factors impacting language  dynamics in post-globalized scenarios: Presenting principles,  paradigms and frameworks for use in the emerging science of  language dynamics
Creators: name: Rao Mandavilli, Sujay
Publisher: name: Zenodo
Year: 2024

description: The objective of this paper is to present comprehensive principles of language spread that are applicable in post-globalized scenarios, by expanding upon and consolidating our already-published works in which had we studied different aspects of diachronic and synchronic linguistics and language dynamics including language dynamics in India. Admittedly, these principles and theories cannot be comprehensive, inclusive or wide-ranging enough to account for all dimensions of language spread in all possible scenarios at this juncture. However, we recommend a repository-type and a nomotheticapproach which will allow for principles drawn from new and varied case studies and fieldwork from different contexts around the world to be generalized and extended to other contexts, with suitable annotations and clarifications regarding their anticipated general or context-specific use. These approaches are particularly relevant in post-globalized scenarios which we expect to be the norm, barring exceptions, given that the factors working in favour of a global long term, political, economic and technological socio-cultural integration are expected to outweigh those working against it. Thus, non contact-based scenarios are expected to be over-arching in the twenty-first century, and are expected to take precedence over contact-based scenarios in many cases, even though the latter can both directly and indirectly impact the former. Therefore, this paper takes into account work already done in the field of sociolinguistics, applied sociolinguistics, linguistic anthropology and applied linguistics, and recasts them and reassesses them in such a way, that their relevance to post-globalized scenarios is brought out. It also merges them with our theories and approaches in the field of linguistics, and brings them in line with our philosophy of the ‘Globalization of science’. Thus, the approach and emphasis of this paper is quite different from other vital publications in this field.
Meta-analysis of randomized controlled trials on calcium supplements and dairy products for changes in body weight and obesity indices
Creators: name: Hong, Jee Yeon
name: Lee, Ji Seon
name: Woo, Hye Won
name: Son, Ae
name: Kwock, Chang Keun
name: Kim, Mi Kyung
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: This meta-analysis was performed to investigate whether calcium supplements and dairy products change obesity indices including fat mass. Original articles published in English between July 2009 and August 2019 were identified. Ten and 14 randomised controlled trials (RCTs) with ≥ 12 weeks interventions of calcium supplements and dairy products among overweight or obese adults aged ≥18 were critically reviewed. Mean difference (MD) or standardised mean difference (SMD) with 95% confidence interval (CI) were obtained using a random effect meta-analysis. Dairy products significantly changed fat mass (SMD, 95% CI; −0.40 [−0.77, −0.02]) and BMI (MD, 95% CI: −0.46 kg/m2 [−0.67, −0.26]), and calcium supplements also showed changes in fat mass (SMD, 95% CI; −0.15[−0.28, −0.02]). However, in the analysis of RCTs with low risk of bias scores, the significant changes remained only in the dairy-products intervention. Our findings suggest that dairy products without distinction of fat percentage may help reduce fat mass and BMI, but calcium supplements may not.
On the Significance of the Electroweak Precision Data
Creators: name: Dittmaier, S.
name: Schildknecht, D.
name: Kolodziej, K.
name: Kuroda, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We elaborate on a recently suggested effective Lagrangian for charged-current and neutral-current electroweak interactions which in comparison with the standard electroweak theory contains three free parameters $Δx, Δy$, $\varepsilon$ which quantify different sources for violations of $SU(2)$ symmetry. Within the standard $SU(2)_I \times U(1)_Y$ electroweak theory, we present both exact and very much refined approximate analytical one-loop expressions for these parameters in terms of the canonical input, $G_μ, \MZ$, $\alpz$, the top-quark mass, $\Mt$, and the Higgs-boson mass, $\MH$. We reemphase the importance of discriminating between the {\it empirically well-known purely fermionic} (vacuum polarization) contributions to $Δx, Δy$, $\varepsilon$ and the {\it empirically unknown bosonic} ones with respect to present and future electroweak precision tests. The parameters $Δx$ and $\varepsilon$ are hardly affected by standard bosonic corrections, while the full one-loop results for $Δy$ differ appreciably from the ones obtained by taking into account fermion loops only. A detailed comparison with the experimental data on $\MWpm/\MZ$, $\bar\sw^2$, $Γ_l$ shows that these data start to become accurate enough to be sensitive to standard (bosonic) contributions to $Δy$ beyond fermion loops.
description: 23 pages LATEX, 6 figures appended in uuencoded form; Bielefeld preprint BI-TP 94/09
Cosmic Star Formation History and the Brightness of the Night Sky
Creators: name: Madau, Piero
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I review the constraints imposed by the observed extragalactic background light (EBL) on the history of the stellar birthrate in galaxies. At faint magnitudes, the logarithmic slope of the galaxy counts is flatter than 0.4 in all seven UBVIJHK optical bandpasses of the Hubble Deep Field-South imaging survey. The integration of the number counts provides a lower limit to the surface brightness of the optical extragalactic sky of 15 nW/m2/sr, comparable to the intensity of the far-IR background from COBE data. If the initial mass function has a Salpeter slope with a lower mass cutoff consistent with observations of M subdwarf disk stars, a lower limit of Omega_*>0.005 (at Hubble constant 50 km/s/Mpc) is derived for the visible (processed gas + stars) mass density needed to generate an extragalactic background light (EBL) at a level of 50 nW/m2/sr. The current `best-guess' estimate to Omega_* is 0.012, about 16% of the nucleosynthetic baryon density. The contribution of quasar activity to the observed EBL is unlikely to exceed 20%.
description: LaTeX, 9 pages, 4 figures, invited review at the VLT Opening Symposium, Antofagasta, Chile 1-4 March 1999
Directional wavelets on $n$-dimensional spheres
Creators: name: Iglewska-Nowak, Ilona
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 42C40, 42B20

description: Directional Poisson wavelets, being directional derivatives of Poisson kernel, are introduced on $n$-dimensional spheres. It is shown that, slightly modified and together with another wavelet family, they are an admissible wavelet pair according to the definition derived from the theory of approximate identities. We investigate some of the properties of directional Poisson wavelets, such as recursive formulae for their Fourier coefficients or explicit representations as functions of spherical variables (for some of the wavelets). We derive also an explicit formula for their Euclidean limits.
description: 30 pages
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000759
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. p1000759
Convective dynamics and disequilibrium chemistry in the atmospheres of giant planets and brown dwarfs
Creators: name: Bordwell, Baylee
name: Brown, Benjamin P.
name: Oishi, Jeffrey S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Disequilibrium chemical processes have a large effect upon the spectra of substellar objects. To study these effects, dynamical disequilibrium has been parameterized using the quench and eddy diffusion approximations, but little work has been done to explore how these approximations perform under realistic planetary conditions in different dynamical regimes. As a first step in addressing this problem, we study the localized, small scale convective dynamics of planetary atmospheres by direct numerical simulation of fully compressible hydrodynamics with reactive tracers using the Dedalus code. Using polytropically-stratified, plane parallel atmospheres in 2- and 3-D, we explore the quenching behavior of different abstract chemical species as a function of the dynamical conditions of the atmosphere as parameterized by the Rayleigh number. We find that in both 2- and 3-D, chemical species quench deeper than would be predicted based on simple mixing length arguments. Instead, it is necessary to employ length scales based on the chemical equilibrium profile of the reacting species in order to predict quench points and perform chemical kinetics modeling in 1-D. Based on the results of our simulations, we provide a new length scale, derived from the chemical scale height, which can be used to perform these calculations. This length scale is simple to calculate from known chemical data and makes reasonable predictions for our dynamical simulations.
description: 12 pages, 9 figures; Published in the Astrophysical Journal
Dissolved Massive Metal-Rich Globular Clusters Can Cause the Range of UV Upturn Strengths Found among Early-type Galaxies
Creators: name: Goudfrooij, Paul
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: I discuss a scenario in which the ultraviolet (UV) upturn of giant early-type galaxies (ETGs) is primarily due to helium-rich stellar populations that formed in massive metal-rich globular clusters (GCs) which subsequently dissolved in the strong tidal field in the central regions of the massive host galaxy. These massive GCs are assumed to show UV upturns similar to those observed recently in M87, the central giant elliptical galaxy in the Virgo cluster of galaxies. Data taken from the literature reveals a strong correlation between the strength of the UV upturn and the specific frequency of metal-rich GCs in ETGs. Adopting a Schechter function parametrization of GC mass functions, simulations of long-term dynamical evolution of GC systems show that the observed correlation between UV upturn strength and GC specific frequency can be explained by variations in the characteristic truncation mass ${\cal{M}}_{\rm c}$ such that ${\cal{M}}_{\rm c}$ increases with ETG luminosity in a way that is consistent with observed GC luminosity functions in ETGs. These findings suggest that the nature of the UV upturn in ETGs and the variation of its strength among ETGs are causally related to that of helium-rich populations in massive GCs, rather than intrinsic properties of field stars in massive galactic spheroids. With this in mind, I predict that future studies will find that [N/Fe] decreases with increasing galactocentric radius in massive ETGs, and that such gradients have the largest amplitudes in ETGs with the strongest UV upturns.
description: 15 pages, 10 figures, 2 tables; LaTeX emulateapj format
Additional file 2 of Differential effects of sound interventions tuned to 432 Hz or 443 Hz on cardiovascular parameters in cancer patients: a randomized cross-over trial
Creators: name: Hohneck, Anna
name: Rodríguez, Ánxelo Maia
name: Weingärtner, Simone
name: Merx, Kirsten
name: Sarodnick, Felicitas
name: von Gagern, Fritjof
name: Mavratzas, Athanasios
name: Burkholder, Iris
name: Schumacher, Gerhard
name: Hofmann, Wolf-Karsten
name: Hofheinz, Ralf-Dieter
Publisher: name: figshare
Year: 2025
Subjects: Medicine
Cell Biology
Neuroscience
Biological Sciences not elsewhere classified
Science Policy
Mental Health

description: Supplementary Material 2
Supplementary document for Single-cell resolution, whole-brain, light-field microscopy - 4840204.pdf
Creators: name: Yoon, Young-Gyu
name: Wang, Zeguan
name: Pak, Nikita
name: Park, Demian
name: Dai, Peilun
name: Kang, JEONG SEUK
name: SUK, HO-JUN
name: Symvoulidis, Panagiotis
name: GUNER-ATAMAN, BURCU
name: Wang, Kai
Publisher: name: Optica Publishing Group
Year: 2020
Subjects: Animal Neurobiology

description: Supplementary Figures
Towards a robust data organization scheme for neuroimaging: the Brain Imaging Data Structure (BIDS)
Creators: name: Poldrack, Russell
name: Gorgolewski, Krzysztof
Publisher: name: figshare
Year: 2018
Subjects: subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Neuroscience

description: Talk presented at Neuroinformatics 2018, Montreal, August 9
Star-disc interaction in galactic nuclei: formation of a central stellar disc
Creators: name: Panamarev, Taras
name: Shukirgaliyev, Bekdaulet
name: Meiron, Yohai
name: Berczik, Peter
name: Just, Andreas
name: Spurzem, Rainer
name: Omarov, Chingis
name: Vilkoviskij, Emmanuil
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We perform high resolution direct $N$-body simulations to study the effect of an accretion disc on stellar dynamics in an active galactic nucleus (AGN). We show that the interaction of the nuclear stellar cluster (NSC) with the gaseous disc (AD) leads to formation of a stellar disc in the central part of the NSC. The accretion of stars from the stellar disc onto the super-massive black hole is balanced by the capture of stars from the NSC into the stellar disc, yielding a stationary density profile. We derive the migration time through the AD to be 3\% of the half-mass relaxation time of the NSC. The mass and size of the stellar disc are 0.7\% of the mass and 5\% of the influence radius of the super-massive black hole. An AD lifetime shorter than the migration time would result in a less massive nuclear stellar disc. The detection of such a stellar disc could point to past activity of the hosting galactic nucleus.
description: submitted to MNRAS after revision
Polarized Narrow-Line Emission from the Nucleus of NGC 4258
Creators: name: Barth, A. J.
name: Tran, H. D.
name: Brotherton, M. S.
name: Filippenko, A. V.
name: Ho, L. C.
name: van Breugel, W.
name: Antonucci, R.
name: Goodrich, R. W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The detection of polarized continuum and line emission from the nucleus of NGC 4258 by Wilkes et al. (1995) provides an intriguing application of the unified model of Seyfert nuclei to a galaxy in which there is known to be an edge-on, rotating disk of molecular gas surrounding the nucleus. Unlike most Seyfert nuclei, however, NGC 4258 has strongly polarized narrow emission lines. To further investigate the origin of the polarized emission, we have obtained spectropolarimetric observations of the NGC 4258 nucleus at the Keck-II telescope. The narrow-line polarizations range from 1.0% for [S II] 6716 to 13.9% for the [O II] 7319,7331 blend, and the position angle of polarization is oriented nearly parallel to the projected plane of the masing disk. A correlation between critical density and degree of polarization is detected for the forbidden lines, indicating that the polarized emission arises from relatively dense (n_e > 10^4 cm^-3) gas. An archival Hubble Space Telescope narrow-band [O III] image shows that the narrow-line region has a compact, nearly unresolved core, implying a FWHM size of <2.5 pc. We discuss the possibility that the polarized emission might arise from the accretion disk itself and become polarized by scattering within the disk atmosphere. A more likely scenario is an obscuring torus or strongly warped disk surrounding the inner portion of a narrow-line region which is strongly stratified in density. The compact size of the narrow-line region implies that the obscuring structure must be smaller than ~2.5 pc in diameter.
description: To appear in the Astronomical Journal. 13 pages, including 1 table and 4 figures. Uses emulateapj.sty
A Transient New Coherent Condition of Matter: The Signal for New Physics in Hadronic Diffractive Scattering
Creators: name: Barshay, S.
name: Heiliger, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We demonstrate the existence of an anomalous structure in the data on the diffractive elastic scattering of hadrons at high energies and small momentum transfer. We analyze five sets of experimental data on $p(\overline{p})-p $ scattering from five different experiments with colliding beams, ranging from the first-- and second--generation experiments at $\sqrt{s} = 53 $ GeV to the most recent experiments at 546 GeV and at 1800 GeV. All of the data sets exhibit a localized anomalous structure in momentum transfer. We represent the anomalous behavior by a phenomenological formula. This is based upon the idea that a transient coherent condition of matter occurs in some of the intermediate inelastic states which give rise, via unitarity, to diffractive elastic scattering. The Fourier--Bessel transform into momentum--transfer space of a spatial oscillatory behavior of matter in the impact--parameter plane results in a small piece of the diffractive amplitude which exhibits a localized anomalous behavior near a definite value of $-t $. In addition, we emphasize possible signals coming directly from such a new condition of matter that may be present in current experiments on inelastic processes.
description: 25 pages, LaTeX (12 figures, not included). A complete postscript file (except figures 1 and 11, which are available upon request) is available via anonymous ftp at ttpux2.physik.uni-karlsruhe.de (129.13.102.139) as /ttp94-03 /ttp94-03.ps, Local preprint# TTP94-03 (March 1994)
Buccinum hecticu Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum hecticu

description: Buccinum hecticu [spec. nov.]
B. testa turrita, anfractibus margine superiore com- presso-attenuato.
Gvalt. test. t. 56. f. C.
Habitat in O. Africano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 741, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2 of Dual effects of targeting S100A11 on suppressing cellular metastatic properties and sensitizing drug response in gastric cancer
Creators: name: Cui, Yuxin
name: Li, Liting
name: Li, Zhilei
name: Yin, Jie
name: Lane, Jane
name: Ji, Jiafu
name: Jiang, Wen G.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Figure S2. Hierarchical Clustering on Principal Components (HCPC) multivariate analysis of the human S100 family member genes in gastric cancer.
Additional file 1 of Utilization, satisfaction, and barriers to antenatal care among pregnant women in Gadarif State during the Sudan war: a cross-sectional study
Creators: name: Ali, Eithar M.
name: M. Ahmed, Ahmed Balla
name: Ahmed, Muhannad Bushra Masaad
name: Omer, Alaa T.
name: Ahmedtaha, Elshaima Ibrahim Mohamedelhassan
name: Khalil, Khadija A.
name: Ibrahim, Logien Abuelgasim Ahmad
name: Abdallah, Maab Hassan Ahmed
name: Abdelrahim, Mohamed Osman Mohamed
name: Abdallah, Sakhr Hassan Ahmed
name: Ahmed, Sohaib Mohammed Mokhtar
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Ages for exoplanet host stars
Creators: name: Christensen-Dalsgaard, Joergen
name: Aguirre, Victor Silva
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Age is an important characteristic of a planetary system, but also one that is difficult to determine. Assuming that the host star and the planets are formed at the same time, the challenge is to determine the stellar age. Asteroseismology provides precise age determination, but in many cases the required detailed pulsation observations are not available. Here we concentrate on other techniques, which may have broader applicability but also serious limitations. Further development of this area requires improvements in our understanding of the evolution of stars and their age-dependent characteristics, combined with observations that allow reliable calibration of the various techniques.
description: To appear in "Handbook of Exoplanets", eds. Deeg, H.J. & Belmonte, J.A, Springer (2018)
Supplementary Materials from Evolutionary and food supply implications of ongoing maize domestication by Mexican campesinos
Creators: name: Bellon, Mauricio R.
name: Mastretta-Yanes, Alicia
name: Ponce, Alejandro
name: María, Daniel Ortiz Santa
name: Galindo, Oswaldo Oliveros
name: Perales, Hugo
name: Acevedo, Francisca
name: Sarukhán, José
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Science

description: Supplementary figures, tables and information on methods
Early GRB Afterglows from Relativistic Blast Waves in General Radiative Regimes
Creators: name: Boettcher, M.
name: Dermer, C. D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present simple analytical expressions for the predicted spectral and temporal behavior of the early afterglow radiation from gamma-ray bursts in radiative regimes intermediate between the adiabatic and the fully radiative solutions of the blastwave hydrodynamic equations. Our expressions are valid as long as the relativistic electrons responsible for the observed synchrotron emission are in the fast cooling regime and the blast wave is relativistic. We show that even a slight deviation from a perfectly adiabatic evolution results in significant changes of the temporal characteristics of the afterglow emission.
description: Now accepted for publication in ApJ, part I (originally submitted to ApJ Letters). Extended discussion w.r.t. original version. Includes 4 figures, using epsf.sty, rotate.sty
Semi-Empirical Bound on the Chlorinr-37 Solar Neutrino Experiment
Creators: name: Kwong, Waikwok
name: Rosen, S. P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Kamiokande measurement of energetic Boron-8 neutrinos from the sun is used to set a lower bound on the contribution of the same neutrinos to the signal in the \Chlorine\ experiment. Implications for Beryllium-7 neutrinos are discussed.
description: Latex, 6 pages + 1 postscript figure (included). UTAPHY-HEP-9
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1371
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1371, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1371, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q15945019
description: Provenance: abbaye Saint-Étienne de Dijon