cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Fermat, Alpha, and the Intellectual Bankruptcy of Science
Creators: name: Smith, John
Publisher: name: figshare
Year: 2017
Subjects: subject: 10101 Algebra and Number Theory
subject: FOS: Mathematics
subject: 20203 Particle Physics
subject: FOS: Physical sciences

description: The world -under the sway of the religion called "science" is in a very sorry state. There is an accumulation of data, an accumulation that says nothing more nor less than that everything is running toward eternal death, but no one knows why. All science can do is can say is "that's just the way it is". This is due to the neglect by science of the basis and the reason for scientific laws/mathematical principles. Feynman described the scientific enterprise best when he analogized scientific inquiry to the study of a gigantic natural chess game where the scientist tries to work out what the rules of the game are. But if and when he or she is able to do this, the question remains as to why the rules are as they are. Science has it backwards. Once one knows the rules governing the empirically discernible rules -once one knows the deep rules- it is a relatively easy matter to work out what the shallow rules are and why, but it is impossible to discover the deep rules from the shallow ones, i.e. the scientific quest is a walk down the proverbial garden path. The shallow philosophy encapsulated by Feynman has given us proofs of Fermat's Last Theorem, and the Poincare Conjecture, in the form of more or less incomprehensible and arbitrary numerical facts, and it has given us the Standard Model of Particle Physics in which all of the free parameters are set from experiment, i.e. science would have us believe that these values are arbitrarily chosen. Science presents us with a world whose evident, encroaching, and irreversible bleakness makes no sense...
Кардиометаболические факторы риск и колоректальный рак.2016.Систематический обзор.pdf
Creators: name: Doe, Jonn
Publisher: name: figshare
Year: 2017
Subjects: subject: 111299 Oncology and Carcinogenesis not elsewhere classified
subject: FOS: Clinical medicine

description: Кардиометаболические факторы риск и колоректальный рак.2016.Систематический обзор проблемы.pdf
Supporting information from Predators indirectly induce stronger prey through a trophic cascade
Creators: name: Spyksma, Arie J. P.
name: Shears, Nick T.
name: Taylor, Richard B.
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Structural Biology

description: Supporting information figure legend and figures S1 - S3
Кардиометаболические факторы риск и колоректальный рак.Систематический обзор.2016.pdf
Creators: name: Doe, Jonn
Publisher: name: figshare
Year: 2017
Subjects: subject: 111299 Oncology and Carcinogenesis not elsewhere classified
subject: FOS: Clinical medicine

description: Кардиометаболические факторы риск и колоректальный рак.2016.Систематический обзор проблемы.pdf
Effect of surface H$_2$ on molecular hydrogen formation on interstellar grains
Creators: name: Zhao, Gang
name: Chang, Qiang
name: Zhang, Xia
name: Quan, Donghui
name: Zhang, Yong
name: Li, Xiao-Hu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate how the existence of hydrogen molecules on grain surfaces may affect H$_2$ formation efficiency in diffuse and translucent clouds. Hydrogen molecules are able to reduce the desorption energy of H atoms on grain surfaces in models. The detailed microscopic Monte Carlo method is used to perform model simulations. We found that the impact of the existence of H$_2$ on H$_2$ formation efficiency strongly depends on the diffusion barriers of H$_2$ on grain surfaces. Diffuse cloud models that do not consider surface H$_2$ predict that H atom recombination efficiency is above 0.5 over a grain temperature (T) range 10 K and 14 K. The adopted H$_2$ diffusion barriers in diffuse cloud models that consider surface H$_2$ are 80$\%$ H$_2$ desorption energies so that H$_2$ can be trapped in stronger binding sites. Depending on model parameters, these diffuse cloud models predict that the recombination efficiency is between nearly 0 and 0.5 at 10 K $\leq$ T $\leq$ 14 K. Translucent cloud model results show that H$_2$ formation efficiency is not affected by the existence of surface H$_2$ if the adopted average H$_2$ diffusion barrier on grain surfaces is low (194 K) so that H$_2$ can diffuse rapidly on grain surfaces. However, the recombination efficiency can drop to below 0.002 at T $\geq$ 10 K if higher average H$_2$ diffusion barrier is used (255 K) in translucent cloud models.
description: accepted for publication in MNRAS
An APEX search for carbon emission from NGC 1977 proplyds
Creators: name: Haworth, Thomas J.
name: Kim, Jinyoung S.
name: Qiao, Lin
name: Winter, Andrew J.
name: Williams, Jonathan P.
name: Clarke, Cathie J.
name: Owen, James E.
name: Facchini, Stefano
name: Ansdell, Megan
name: Kama, Mikhel
name: Ballabio, Giulia
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We used the Atacama Pathfinder Experiment (APEX) telescope to search for CI 1-0 (492.16GHz) emission towards 8 proplyds in NGC 1977, which is an FUV radiation environment two orders of magnitude weaker than that irradiating the Orion Nebular Cluster (ONC) proplyds. CI is expected to enable us to probe the wind launching region of externally photoevaporating discs. Of the 8 targets observed, no 3$σ$ detections of the CI line were made despite reaching sensitivities deeper than the anticipated requirement for detection from prior APEX CI observations of nearby discs and models of external photoevaporation of quite massive discs. By comparing both the proplyd mass loss rates and CI flux constraints with a large grid of external photoevaporation simulations, we determine that the non-detections are in fact fully consistent with the models if the proplyd discs are very low mass. Deeper observations in CI and probes of the disc mass with other tracers (e.g. in the continuum and CO) can test this. If such a test finds higher masses, this would imply carbon depletion in the outer disc, as has been proposed for other discs with surprisingly low CI fluxes, though more massive discs would also be incompatible with models that can explain the observed mass loss rates and CI non-detections. The expected remaining lifetimes of the proplyds are estimated to be similar to those of proplyds in the ONC at 0.1Myr. Rapid destruction of discs is therefore also a feature of common, intermediate UV environments.
description: 10 pages. Accepted for publication in MNRAS
mmhmm
Creators: name: Valls, Ricardo
Publisher: name: OSF Registries
Year: 2021
Subjects: Aseguramniento de Calidad
Control de Calidad
Geología
QA&QC
Sistemática del trabajo en geología
cienciasgeológicas
geochemistry
trainingcourses
vallsgeoconsultant

description: Materiales usados para preparar la presentación usando mmhmm
Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries
Creators: name: Barker, Adrian J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Tidal dissipation is responsible for circularizing the orbits and synchronizing the spins of solar-type close binary stars, but the mechanisms responsible are not fully understood. Previous work has indicated that significant enhancements to the theoretically-predicted tidal dissipation rates are required to explain the observed circularization periods ($P_\mathrm{circ}$) in various stellar populations, and their evolution with age. This was based partly on the common belief that the dominant mechanism of tidal dissipation in solar-type stars is turbulent viscosity acting on equilibrium tides in convective envelopes. In this paper we study tidal dissipation in both convection and radiation zones of rotating solar-type stars following their evolution. We study equilibrium tide dissipation, incorporating a frequency-dependent effective viscosity motivated by the latest hydrodynamical simulations, and inertial wave (dynamical tide) dissipation, adopting a frequency-averaged formalism that accounts for the realistic structure of the star. We demonstrate that the observed binary circularization periods can be explained by inertial wave (dynamical tide) dissipation in convective envelopes. This mechanism is particularly efficient during pre-main sequence phases, but it also operates on the main sequence if the spin is close to synchronism. The predicted $P_\mathrm{circ}$ due to this mechanism increases with main-sequence age in accord with observations. We also demonstrate that both equilibrium tide and internal gravity wave dissipation are unlikely to explain the observed $P_\mathrm{circ}$, even during the pre-main sequence, based on our best current understanding of these mechanisms. Finally, we advocate more realistic dynamical studies of stellar populations that employ tidal dissipation due to inertial waves.
description: Accepted for publication in The Astrophysical Journal Letters on 7th March 2022
Analysis of a JWST NIRSpec Lab Time Series: Characterizing Systematics, Recovering Exoplanet Transit Spectroscopy, and Constraining a Noise Floor
Creators: name: Rustamkulov, Zafar
name: Sing, David
name: Liu, Rongrong
name: Wang, Ashley
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences
subject: 85A20

description: The James Webb Space Telescope's NIRSpec instrument will unveil the nature of exoplanet atmospheres across the wealth of planet types, from temperate terrestrial worlds to ultrahot Jupiters. In particular, the 0.6-5.3 micron PRISM mode is especially well-suited for efficient spectroscopic exoplanet observations spanning a number of important spectral features. We analyze a lab-measured NIRSpec PRISM mode Bright Object Time Series (BOTS) observation from the perspective of a JWST user to understand the instrument performance and detector properties. We create two realistic transiting exoplanet time series observations by performing injection-recovery tests on the lab-measured data to quantify the effects of real instrument jitter, drift, intrapixel sensitivity variations, and 1/$f$ noise on measured transmission spectra. By fitting the time series systematics simultaneously with the injected transit, we can obtain more realistic transit depth uncertainties that take into account noise sources that are currently not modeled by traditional exposure time calculators. We find that sources of systematic noise related to intrapixel sensitivity variations and PSF motions are apparent in the data at the level of a few hundred ppm, but can be effectively detrended using a low-order polynomial with detector position. We recover the injected spectral features of GJ 436 b and TRAPPIST-1 d, and place a 3-sigma upper limit on the detector noise floor of 14 ppm. We find that the noise floor is consistent with <10 ppm at the 1.7-sigma level, which bodes well for future observations of challenging targets with faint atmospheric signatures.
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0149
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0149, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0149, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
title: 20_F_GUILLARD_CoupsDeTrique_FR_GAD
Creators: name: Guillard, J
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: PuppetPlays
subject: Horizon 2020
subject: Plassard, Didier
subject: Guignol (personnage fictif)

description: MAM - Musée des Arts de la Marionnette (Musée Gadagne). Fonds de la compagnie EMMA. N°88bis
Cahier manuscrit. Du 25 février au 25 mars 1950, 14 séances, 4 semaines.

Numérisé dans le cadre du projet ERC PuppetPlays, financé par le Programme de recherche et d'innovation Horizon 2020 de l'Union Européenne (Grant Agreement 835193).
description: Digitized by the ERC project PuppetPlays, receiving funding from the European Union's Horizon 2020 research and innovation programme under Grant Agreement ERC 835193.
Follow the Water: Finding Water, Snow and Clouds on Terrestrial Exoplanets with Photometry and Machine Learning
Creators: name: Pham, Dang
name: Kaltenegger, Lisa
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: All life on Earth needs water. NASA's quest to follow the water links water to the search for life in the cosmos. Telescopes like JWST and mission concepts like HabEx, LUVOIR and Origins are designed to characterise rocky exoplanets spectroscopically. However, spectroscopy remains time-intensive and therefore, initial characterisation is critical to prioritisation of targets. Here, we study machine learning as a tool to assess water's existence through broadband-filter reflected photometric flux on Earth-like exoplanets in three forms: seawater, water-clouds and snow; based on 53,130 spectra of cold, Earth-like planets with 6 major surfaces. XGBoost, a well-known machine learning algorithm, achieves over 90\% balanced accuracy in detecting the existence of snow or clouds for S/N$\gtrsim 20$, and 70\% for liquid seawater for S/N $\gtrsim 30$. Finally, we perform mock Bayesian analysis with Markov-chain Monte Carlo with five filters identified to derive exact surface compositions to test for retrieval feasibility. The results show that the use of machine learning to identify water on the surface of exoplanets from broadband-filter photometry provides a promising initial characterisation tool of water in different forms. Planned small and large telescope missions could use this to aid their prioritisation of targets for time-intense follow-up observations.
description: 6 pages, 5 figures. Accepted for publications in MNRAS Letters
title: Indirect methods of estimating adult mortality levels
Creators: name: Hill, KH
Publisher: name: London School of Hygiene & Tropical Medicine
Year: 1975

description: Many countries, particularly in the developing world, have inadequate vital registration systems, and data collected by population censuses in these countries often contain serious and predictable biases. Direct methods of measuring mortality are useless in such situations, so indirect methods have been developed instead. The two best known indirect methods, namely estimating childhood mortality from the proportion dead among children ever borne by women of known age, and estimating adult mortality from reports of orphanhood by age, are discussed. Various shortcomings of the orphanhood method are noted, particularly in its application to estimating adult male mortality. To avoid these, two different approaches are suggested, developed and tested. One is to limit the analysis of orphanhood to reports of the eldest surviving child of each parent only, and the other is to analyse proportions widowed of first spouse. It is not difficult to develop a method of analysis for estimating mortality from reports of firstborn children, but using reports of eldest surviving children is more complicated. Allowance has to be made for deaths among firstborn children, and their replacement by second or higher order children. A simple model was developed to work out the birth order composition of eldest surviving children at various ages. The method of analysis so developed has certain advantages over the original orphanhood method, but is found to be very sensitive to changes in the level and age pattern of mortality. The method of analysis developed for widowhood data is much simpler. The only complication is the need for two marriage distributions, male and female, the one to calculate the probability of being widowed for a given exposure to risk, and the other to work out the exposure to risk of a particular age group of respondents. The method proves to be robust to changes in mortality and to deviations from the other crucial assumptions on which it is based. Both methods are applied to suitable data collected by a sample survey in Honduras. The data and the results are critically examined to assess both the possibility of collecting the required data and the success of the methods themselves. The conclusion is drawn that the widowhood method is promising, but the orphanhood of eldest surviving children method is disappointing. More applications are needed, though, to establish whether either or both of these methods are worthy of a place amongst the standard techniques for estimating population parameters in countries having defective or incomplete data.
Supplementary material for 'Nonlinear mode interaction in equal-leg angle struts susceptible to cellular buckling': A simplified linear model for the buckling of equal-leg angle struts
Creators: name: L. Bai
name: F. Wang
name: M. A. Wadee
name: J. Yang
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: 90506 Structural Engineering
subject: FOS: Civil engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: 10299 Applied Mathematics not elsewhere classified
subject: FOS: Mathematics

description: A simplified and linearized system is presented for the equal-leg angle strut. This demonstrates that, when linearized, the current variational model reproduces classical work.
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1239
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1239, 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. 1239, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
title: AN, Registre des écrous du Châtelet, Y5266, f. p1010040
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. p1010040
Supplementary Tables and Figures from Identification of a molecular pH sensor in coral
Creators: name: Barott, Katie L.
name: Barron, Megan E.
name: Tresguerres, Martin
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Environmental Science

description: Included in the file
The evolution of protoplanetary discs in star formation and feedback simulations
Creators: name: Qiao, Lin
name: Haworth, Thomas J.
name: Sellek, Andrew D.
name: Ali, Ahmad A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We couple star cluster formation and feedback simulations of a Carina-like star forming region with 1D disc evolutionary models to study the impact of external photoevaporation on disc populations in massive star forming regions. To investigate the effect of shielding of young stellar objects by star forming material, we track the FUV field history at each star in the cluster with two methods: i) Monte Carlo radiative transfer accounting for the shielding of stars from the FUV by the star forming cloud ii) Geometric dilution of the radiation from other stars which ignores shielding effects. We found that significant shielding only occurs for a small fraction of discs and offers protection from external photoevaporation for < 0.5 Myr. However, this initial protection can prevent significant early gas/dust mass loss and disc radius reduction due to external photoevaporation. Particularly, shielding for 0.5 Myr is sufficient for much of the solid reservoir to evolve to larger sizes where it will not be entrained in an external wind. Shielding is therefore potentially significant for terrestrial planet formation in retaining the solid mass budget, but the continued stripping of gas when shielding ends could still impact migration and the gas reservoir for giant planet atmospheres. Our models highlight issues with treating all discs in a cluster with a single characteristic age, since shielded objects are typically only the youngest. Our model predicts that the majority of discs in a 2 Myr Carina-like environment are subject to strong external photoevaporation.
description: 18 pages, 9 figure, resubmitted to MNRAS with minor revisions
Adaptative Perturbation Patterns: Realistic Adversarial Learning for Robust Intrusion Detection
Creators: name: Vitorino, João
name: Oliveira, Nuno
name: Praça, Isabel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cryptography and Security (cs.CR)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Adversarial attacks pose a major threat to machine learning and to the systems that rely on it. In the cybersecurity domain, adversarial cyber-attack examples capable of evading detection are especially concerning. Nonetheless, an example generated for a domain with tabular data must be realistic within that domain. This work establishes the fundamental constraint levels required to achieve realism and introduces the Adaptative Perturbation Pattern Method (A2PM) to fulfill these constraints in a gray-box setting. A2PM relies on pattern sequences that are independently adapted to the characteristics of each class to create valid and coherent data perturbations. The proposed method was evaluated in a cybersecurity case study with two scenarios: Enterprise and Internet of Things (IoT) networks. Multilayer Perceptron (MLP) and Random Forest (RF) classifiers were created with regular and adversarial training, using the CIC-IDS2017 and IoT-23 datasets. In each scenario, targeted and untargeted attacks were performed against the classifiers, and the generated examples were compared with the original network traffic flows to assess their realism. The obtained results demonstrate that A2PM provides a scalable generation of realistic adversarial examples, which can be advantageous for both adversarial training and attacks.
description: 18 pages, 6 tables, 10 figures, Future Internet journal
Early dynamical evolution of rotating star clusters in a tidal field
Creators: name: Tiongco, Maria
name: Vesperini, Enrico
name: Varri, Anna Lisa
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In order to explore how the early internal rotational properties of star clusters are affected by the external potential of their host galaxies, we have run a suite of $N$-body simulations following the early dynamical evolution and violent relaxation of rotating star clusters embedded in a tidal field. Our study focuses on models for which the cluster's rotation axis has a generic orientation relative to the torque of the tidal field. The interaction between the violent relaxation process, angular momentum of the cluster, and the external torque creates a complex kinematic structure within the cluster, most prominently a radial variation in the position of the rotation axis along both the polar and azimuthal directions. We also examine the cluster's velocity dispersion anisotropy and show that the projected anisotropy may be affected by the variation of the rotation axis directions within the cluster; the combination of projection effects and the complex kinematical features may result in the measurement of tangential anisotropy in the cluster's inner regions. We also characterize the structural properties of our clusters as a function of their initial rotation and virial ratio and find that clusters may develop a triaxial morphology and a radial variation of the minor axis not necessarily aligned with the rotation axis. Finally, we examine the long-term evolution of these complex kinematic features.
description: 15 pages, 12 figures, accepted by MNRAS
title: ADCO, Ordre cistercien : comptes (1499-1515) (11 H 1162), f. 00059
Creators: name: de la Côte-d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162), f. 00059, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Supporting information - Figure S4 from Predators indirectly induce stronger prey through a trophic cascade
Creators: name: Spyksma, Arie J. P.
name: Shears, Nick T.
name: Taylor, Richard B.
Publisher: name: The Royal Society
Year: 2017
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Structural Biology

description: Figure S4
The Hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium
Creators: name: Seidel, J. V.
name: Cegla, H. M.
name: Doyle, L.
name: Lafarga, M.
name: Brogi, M.
name: Gandhi, S.
name: Anderson, D. R.
name: Allart, R.
name: Buchschacher, N.
name: Lovis, C.
name: Sosnowska, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The hot Neptune desert, a distinct lack of highly irradiated planets in the size range of Neptune, remains one of the most intriguing results of exoplanet population studies. A deeper understanding of the atmosphere of exoplanets sitting at the edge or even within the Neptune desert will allow us to better understand if planetary formation or evolution processes are at the origin of the desert. A detection of sodium in WASP-166b was presented previously with tentative line broadening at the 3.4 sigma with the HARPS spectrograph. We update this result with two transits observed with the ESPRESSO spectrograph, confirming the detection in each night and the broadened character of the line. This result marks the first confirmed resolved sodium detection within the Neptune desert. In this work, we additionally highlight the importance of treating low-SNR spectral regions, particularly where absorption lines of stellar sodium and planetary sodium overlap at mid-transit - an important caveat for future observations of the system.
description: Letter, re-submitted to MNRAS after minor referee report; comments welcome
An introductory discussion on mudrās – Ācārya Dr. Sthaneshwar Timalsina
Creators: name: Timalsina, Staneshwar
Publisher: name: Zenodo
Year: 2022
Subjects: Guhyakālī
Kubjika
amnaya
Kaula
timalsina
Divine Mother
consciousness
krama
Kula
Īśāna
shakta upāya
Saundaryalahari
Mālinīvijayottaratantra
Chandi
advaita vedanta
sthaneshwar timalsina
vimarsha-foundation
Sarvamnaya
Abhinavagupta
vedanta
Kali
Devi Mahatmya
trika
Spanda
Shiva Sutra
Tantra
mahadeva
saivadvaita
shakti
sarvamnaya-oral-tradition-archive
Vasugupta
Tripura Rahasya
sarvamnaya
anava upaya
agama
Sadāśiva
Camunda
Shiva
Bhairava
yantra
Mahakali
tripura
Tantric philosophy
Shaiva
tantraloka
Durga
shambhava
Kashmir Shaivism
Tripurasundari

description: In this talk given by Śaivācārya Prof. Sthaneshwar Timalsina at Harvard University, the topic of discussion is the importance of gestures and mudrās regarding tantric practice. These gestures not only convey meaning, but also are powerful tools to evoke certain states of mind to transform that mental reality of the practitioner. Like a spectacle in a theater, emotional states (rasa) are also present during the practice, and the body and speech become mediators between the sādhaka and the deity. It is important to notice that in non-dual tantra, these gestures and practices of visualisation seek to remove the sense of difference between the practitioner and the Deity.

Articles mentioned during the talk:
1) Can Representation be Transformative? Resemblance,
Suggestion, and Metaphor in Tantric Meditation.
2) Language of Gestures: Mudrā, Mirror, and Meaning in Śākta Philosophy.

https://www.vimarshafoundation.org/articles
https://sdsu.academia.edu/SthaneshwarTimalsina

Original YouTube video: https://www.youtube.com/watch?v=w6f-tAFEQdk

This presentation is part of the Sarvāmnāya Oral Tradition Archive.
Vimarsha Foundation. (2025). The Sarvāmnāya Oral Tradition Archive [Data set]. Zenodo. https://doi.org/10.5281/zenodo.15188107
Do twin spectral peaks of olivine particles in the thermal infrared diagnose their sizes and porosities?
Creators: name: Kimura, Hiroshi
name: Markkanen, Johannes
name: Kolokolova, Ludmilla
name: Hilchenbach, Martin
name: Wada, Koji
name: Kanada, Yasumasa
name: Matsui, Takafumi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: A well-established constraint on the size of non-porous olivine grains or the porosity of aggregates consisting of small olivine grains from prominent narrow peaks in thermal infrared spectra characteristic of crystalline silicates is reexamined. To thoroughly investigate thermal infrared peaks, we make theoretical argument for the absorption and scattering of light by non-porous, non-spherical olivine particles, which is followed by numerical verification. Our study provides perfectly rational explanations of the physics behind the small-particle effect of emission peaks in the framework of classical electrodynamics and convincing evidence of small-particle's emission peaks in the literature. While resonant absorption excited by surface roughness on the order of submicrometer scales can be identified even for non-porous olivine particles with a radius of $10~{\rm μm}$, it makes only a negligible contribution to thermal infrared spectra of the particles. In contrast, the porosity of non-spherical particles has a significant impact on the strength and wavelength of the peaks, while the resonant absorption excited by an ensemble of small grains takes place at a wavelength different than one expects for surface roughness. We finally reaffirm that twin peaks of olivine in thermal infrared spectra of dust particles in astronomical environments are the intrinsic diagnostic characters of submicrometer-sized small grains and their aggregate particles in fluffy and porous configurations.
description: 16 pages, 8 figures, to appear in Icarus
title: The protein composition of infectious bronchitis virus
Creators: name: Lanser, JA
Publisher: name: London School of Hygiene & Tropical Medicine
Year: 1979

description: The Massachusetts strain of avian infectious bronchitis virus was purified from embryonated hens' eggs by polyethylene glycol 6,000 precipitation and isopycnic centrifugation through Metrizamide gradients. Four major polypeptides of apparent molecular weight 90,000, 52,000, 29,000 and 26,000 were resolved by SDS-polyacrylamide gel electrophoresis. Omission of reducing agent failed to resolve the 29,000 molecular weight component and increased the mobility of the 90,000 molecular weight polypeptide. Labelling of acrylamide gels with 125 I-concanavalin A indicated that polypeptides of molecular weignt 90,000, 29,000 and 26,000 were glycosylated, and in the absence of reducing agent that the 29,000 glycopeptide migrated as a dimer in the 50,000 molecular weight region. Purified IBV radioiodinated with Bolton and Hunter reagent, which banded as a single peak of radioactivity in Metrizamide gradients, was found to contain bands of radioactivity when analysed by SDS-PAGE corresponding to the polypeptides of molecular weight 90,000, 52,000 and 29.000 resolved in stained gels. Disruption of IBV particles in Triton X-100 released two subviral particles; a 16 nm spike which was comprised of polypeptides with molecular weights of 90,000, 52.000 and 29,000; and another denser spherical particle 25-45 mm in diameter which contained nucleic acid and the 52,000 and 26,000 polypeptides. A model for the structure of IBV is presented.
Multiply charged naphthalene and its C10H8 isomers: bonding, spectroscopy and implications in AGN environments
Creators: name: Santos, Julia C.
name: Fantuzzi, Felipe
name: Quitián-Lara, Heidy M.
name: Martins-Franco, Yanna
name: Menéndez-Delmestre, Karín
name: Boechat-Roberty, Heloisa M.
name: Oliveira, Ricardo R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Naphthalene (C10H8) is the simplest polycyclic aromatic hydrocarbon (PAH) and an important component in a series of astrochemical reactions involving hydrocarbons. Its molecular charge state affects the stability of its isomeric structures, which is specially relevant in ionised astrophysical environments. We thus perform an extensive computational search for low-energy molecular structures of neutral, singly, and multiply charged naphthalene and its isomers with charge states +q = 0-4 and investigate their geometric properties and bonding situations. We find that isomerisation reactions should be frequent for higher charged states and that open chains dominate their low-energy structures. We compute both the scaled-harmonic and anharmonic infrared spectra of selected low-energy species and provide the calculated scaling factors for the naphthalene neutral, cation, and dication global minima. All simulated spectra reproduce satisfactorily the experimental data and, thus, are adequate for aiding observations. Moreover, the potential presence of these species in the emission spectra of the circumnuclear regions of active galactic nuclei (AGNs), with high energetic X-ray photon fluxes, is explored using the experimental value of the naphthalene photodissociation cross-section, σ_{ph-d}, to determine its half-life, t_{1/2}, at a photon energy of 2.5 keV in a set of relevant sources. Finally, we show that the computed IR bands of the triply and quadruply charged species are able to reproduce some features of the selected AGN sources.
description: Accepted for publication in the Monthly Notices of the Royal Astronomical Society. 15 pages, 7 pages, supplementary information available online
Self-consistent dynamical models with a finite extent -- I. The uniform density sphere
Creators: name: Baes, Maarten
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The standard method to generate dynamical models with a finite extent is to apply a truncation in binding energy to the distribution function. This approach has the disadvantages that one cannot choose the density to start with, that the important dynamical quantities cannot be calculated analytically, and that a fraction of the possible bound orbits are excluded a priori. We explore another route and start from a truncation in radius rather than a truncation in binding energy. We focus on the simplest truncated density profile, the uniform density sphere. We explore the most common inversion techniques to generate distribution functions for the uniform density sphere, corresponding to a large range of possible anisotropy profiles. We find that the uniform density sphere cannot be supported by the standard isotropic, constant anisotropy or Osipkov-Merritt models, as all these models are characterised by negative distribution functions. We generalise the Cuddeford inversion method to models with a tangential anisotropy and present a one-parameter family of dynamical models for the uniform density sphere. Each member of this family is characterised by an anisotropy profile that smoothly decreases from an arbitrary value $β_0\leqslant0$ at the centre to completely tangential at the outer radius. All models have a positive distribution function over the entire phase space, and a nonzero occupancy of all possible bound orbits. This shows that one can generate nontrivial self-consistent dynamical models based on preset density profile with a finite extent.
description: Accepted for publication in MNRAS
Explosive instability of dust settling in a protoplanetary disc
Creators: name: Zhuravlev, V. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: It is shown that gas-dust perturbations in a disc with dust settling to the disc midplane exhibit the non-linear three-wave resonant interactions between streaming dust wave (SDW) and two inertial waves (IW). In the particular case considered in this paper, SDW at the wavenumber $k^\bullet = 2κ/ (g_z t_s)$, where $κ$, $g_z$ and $t_s$ are, respectively, epicyclic frequency, vertical gravitational acceleration and particle's stopping time, interacts with two IW at the lower wavenumbers $k^\prime$ and $k^{\prime\prime}$ such that $k^\prime < k_{\rm DSI} < k^{\prime\prime} < k^\bullet$, where $k_{\rm DSI} = κ/ (g_z t_s)$ is the wavenumber of the linear resonance between SDW and IW associated with the previously discovered linear dust settling instability. The problem is solved analytically in the limit of the small dust fraction. As soon as the dynamical dust back reaction on gas is taken into account, ${\bf k}^\bullet$, ${\bf k}^\prime$ and ${\bf k}^{\prime\prime}$ become slightly non-collinear and the emerging interaction of waves leads to simultaneous explosive growth of their amplitudes. This growth is explained by the conservative exchange with energy between the waves. The amplitudes of all three waves grow because the negative energy SDW transfers its energy to the positive energy IW. The product of the dimensionless amplitude of initially dominant wave and the time of explosion can be less than Keplerian time in a disc. It is shown that, generally, the three-wave resonance of an explosive type exists in a wide range of wavenumbers $0 < k^\bullet \leq 2κ/ (g_z t_s)$. An explosive instability of gas-dust mixture may facilitate the dust clumping and the subsequent formation of planetesimals in young protoplanetary discs.
description: 19 pages, 5 figures, accepted for publication in MNRAS
Cytological study of Allium cepa and Allium sativum
Creators: name: Awe, Emmanuel
Publisher: name: figshare
Year: 2017
Subjects: subject: Cell Biology
subject: Botany
subject: 60310 Plant Systematics and Taxonomy
subject: FOS: Biological sciences
subject: Toxicology

description: he large number of species in the Allium genus has necessitated comparative analysis of related species which hasalways been used in many cases to describe patterns and directions of chromosomal evolution within a group. Thisstudy was carried out to cytologically analyse two species of Allium- Allium cepa and Allium sativum. All the fourstages of cell division were observed in both species, although well spread metaphase chromosomes could not beobserved in A. sativum which limited the extent to which we could cytologically evaluate the species. Allium cepa inthis study show cell with a complement of sixteen chromosomes. A total chromosome length of 577.5 µm was observedin the best c-metaphase spread with the longest chromosome being 43.4µm and the shortest 27.9 µm.
SPLASH: The Southern Parkes Large-Area Survey in Hydroxyl -- Data Description & Release
Creators: name: Dawson, J. R.
name: Jones, P. A.
name: Purcell, C.
name: Walsh, A. J.
name: Breen, S. L.
name: Brown, C.
name: Carretti, E.
name: Cunningham, M. R.
name: Dickey, J. M.
name: Ellingsen, S. P.
name: Gibson, S. J.
name: Gomez, J. F.
name: Green, J. A.
name: Imai, H.
name: Krishnan, V.
name: Lo, N.
name: Lowe, V.
name: Marquarding, M.
name: McClure-Griffiths, N. M.
name: .
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the full data release for the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH), a sensitive, unbiased single-dish survey of the Southern Galactic Plane in all four ground-state transitions of the OH radical at 1612, 1665, 1667 and 1720 MHz. The survey covers the inner Galactic Plane, Central Molecular Zone and Galactic Centre over the range $|b|
description: Main paper: 22 pages, 15 figures. Online-only material (appended to ArXiv PDF): 11 pages, 3 figure sets. Accepted to MNRAS. Survey data is available from: https://docs.datacentral.org.au/splash/
Biological dose and complication probabilities for the rectum and bladder based on linear energy transfer distributions in spot scanning proton therapy of prostate cancer
Creators: name: Pedersen, Jesper
name: Petersen, Jørgen B. B.
name: Stokkevåg, Camilla H.
name: Ytre-Hauge, Kristian S.
name: Flampouri, Stella
name: Zuofeng Li
name: Mendenhall, Nancy
name: Muren, Ludvig P.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 60506 Virology
subject: Computational Biology

description: Background: The increased linear energy transfer (LET) at the end of the Bragg peak causes concern for an elevated and spatially varying relative biological effectiveness (RBE) of proton therapy (PT), often in or close to dose-limiting normal tissues. In this study, we investigated dose-averaged LET (LETd) distributions for spot scanning PT of prostate cancer patients using different beam angle configurations. In addition, we derived RBE-weighted (RBEw) dose distributions and related normal tissue complication probabilities (NTCPs) for the rectum and bladder. Material and methods: A total of 21 spot scanning proton plans were created for each of six patients using a prescription dose of 78 Gy(RBE1.1), with each plan using two ‘mirrored’ beams with gantry angles from 110°/250° to 70°/290°, in steps of 2°. Physical dose and LETd distributions were calculated as well as RBEw dose distributions using either RBE = 1.1 or three different variable RBE models. The resulting biological dose distributions were used as input to NTCP models for the rectum and bladder. Results: For anterior oblique (AO) configurations, the rectum LETd volume and RBEw dose increased with increasing angles off the lateral opposing axis, with the RBEw rectum dose being higher than for all posterior oblique (PO) configurations. For PO configurations, the corresponding trend was seen for the bladder. Using variable RBE models, the rectum NTCPs were highest for the AO configurations with up to 3% for the 80°/280° configuration while the bladder NTCPs were highest for the PO configurations with up to 32% for the 100°/260°. The rectum D1cm3 constraint was fulfilled for most patients/configurations when using uniform RBE but not for any patient/configuration with variable RBE models. Conclusions: Compared to using constant RBE, the variable RBE models predicted increased biological doses to the rectum, bladder and prostate, which in turn lead to substantially higher estimated rectum and bladder NTCPs.
Choose a fighter: Preregistration
Creators: name: Třebický, Vít
name: Tureček, Petr
Publisher: name: OSF Registries
Year: 2022
Subjects: Bayesian inference
Counterfactual plots
Face perception
MMA
Stan
attractiveness
forced choice test
formidability
reaction time
rethinking
sexual selection

description: Analysis plan and scripts demonstrating the future analysis on the empirical data