cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Photo-electrochemical reactors with hematite hoto-anodes for water and hydrogen sulfide splitting
Creators: name: Bedoya Lora, Franky Esteban
Publisher: name: Imperial College London
Year: 2017

description: The impact of CO₂ emissions on climate change, human health and local environments are driving the search for more benign sources of energy. The sun is the earth’s ultimate energy source, though subject to diurnal and seasonal intermittency. This calls for a technology to effectively store the harvested solar energy, and make it readily available when needed. ‘Solar fuels’, such as hydrogen, have been proposed as suitable energy carriers. However, due to high costs involved in the production of hydrogen using renewable sources, coupling its production to other processes, such as waste treatment, would be advantageous. Hydrogen sulfide is a toxic and highly corrosive gas which is produced by hydrodesulfurisation processes in petroleum refineries for removal of sulfur from gas and petroleum products. Hence, hydrogen sulfide, which is thermodynamically predicted to be easier to oxidise than water, can be treated while simultaneously producing hydrogen via photo-assisted electrolysis. The performances of tin(IV)-doped hematite photo-anodes were assessed for hydrogen production using photo-assisted electrolysis of water and hydrogen sulfide in photo-electrochemical reactors. Initially, photo-electrochemical, optical and morphological properties were measured as a function of post-deposition annealing. Using these parameters, a semi-empirical model was developed for the prediction of photocurrent densities and the performance of bench-scale (< 0.1 dm³) and up-scaled (0.8 dm³) reactors for water splitting. The model was also implemented to predict optimised geometric properties of photo-anodes with the aim to decrease (H₂-O₂) cross-over losses and minimise inhomogeneities in current density distributions. Lastly, a comparison between conventional water splitting and hydrogen sulfide splitting indicated that interfacial electron-hole recombination rates are diminished effectively in presence of hydrogen sulfide ions, and the photo-anode potentials could be decreased by ca. 0.5 V. Charge yields for hydrogen and polysulfide ions were also estimated, typically as 0.9 and 1.0, respectively. A customised UV/vis absorption technique was required for in situ quantification of polysulfide ions at low concentrations in hydrogen sulfide alkaline solution. A mechanism was proposed for hydrogen sulfide oxidation to polysulfide ions on tin(IV)-doped hematite photo-anodes, on which electrodeposition of elemental sulfur occurred and polysulfide ions accumulated; this needs to be considered when selecting operating conditions for hydrogen production via photo-assisted hydrogen sulfide splitting.
Diffraction of a partial temporal coherent beam from a single-slit and a circular aperture
Creators: name: Koushki, E.
name: Alavi, S. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We generalize the notion of the Franhoufer diffraction from a single slit and a circular aperture to the case of partially temporal coherent and quasimonochromatic light. The problem is studied analytically and the effect of coherence length on the diffraction pattern is investigated. In this case the far-field distribution of the irradiance depends on the newly introduced parameter(decoherence parameter) which governs the deviation of the diffraction pattern from the usual one. The corrections due to temporal decoherency on the irradiance distribution in the far field is obtained. Numerical study of the effect of decoherence parameter on the Far-field diffraction pattern is performed. In the case of a single slit, there is no noticeable deviation in the central peak, but in the higher orders of diffraction, deviation become apparent. For circular apertures, as long as the decoherence parameter is greater than one , the beam decoherency affects the distribution profile and the first order diffraction pattern decreases and by increasing the decoherence parameter, the first order of diffraction pattern gradually disappears.
description: 16 pages, 7 figures
Local air-fuel ratio and gas velocity measurements in flames using LIBS
Creators: name: Shi, Zhengjie
Publisher: name: Imperial College London
Year: 2018

description: Turbulent combustion is an important but complex technical process that takes place in many industrial devices, such as internal combustion engines and gas turbines. Laser-based techniques are widely applied to the combustion research, since they are able to provide important information without severe interferences with the process and with high temporal and spatial resolution. Among these techniques, Laser-induced Breakdown Spectroscopy (LIBS) is an experimental technique that can deliver a manifold of information through the laser-induced plasma. In the current work, laser-induced plasma is used to develop novel diagnostic methods for the measurement of the gas composition and velocity in flames. This research firstly evaluated and improved the instantaneous LIBS measurement of local equivalence ratio in methane-air opposed-jet flames. It was found that the increased measurement uncertainty in reacting flows, relative to non-reacting flows, could be counteracted by increasing the laser pulse energy and using a proposed filter method, which resulted in a 10% uncertainty for single-shot measurements in flames. LIBS measurements in binary hydrocarbon mixtures, including CH4, C3H8, CO2 and air, were also investigated. The effects of blends on LIBS spectra were analysed. While limitations exist, it was shown that LIBS results can be used to infer the binary fuel blends and the Wobbe index of the mixture. Further, a novel seeding-free velocimetry technique, Laser-Induced Plasma Image Velocimetry (LIPIV) was proposed and developed, which is based on recording the displacement of plasma as it gets convected by the gas flow field. It was found that the uncertainty of the novel technique is about 1 m/s along the axis perpendicular to the direction of the laser beam and 3.6 m/s along the laser beam axis and its spatial resolution is about 5 mm. This technique was then successfully applied to measure the gas flow in a non-reacting turbulent jet. Finally, local equivalence ratio and velocity measurements were performed in a swirl-stabilised non-premixed burner at an air-fuel ratio of 0.72 (overall equivalence ratio) and Reynolds number of 29,000. It was shown that, although the quenching effects and plasma deformation effects increased the measurement uncertainty, the velocity results still verified the feasibility of applying the LIPIV in reacting flows after applying the proposed methods. In conclusion, combined measurements of composition and velocity using the laser-induced plasma are demonstrated in realistic combustion geometries.
A Tangent Category Alternative to the Faà di Bruno Construction
Creators: name: Lemay, Jean-Simon
Publisher: name: arXiv
Year: 2018
Subjects: subject: Category Theory (math.CT)
subject: FOS: Mathematics

description: The Faà di Bruno construction, introduced by Cockett and Seely, constructs a comonad $\mathsf{Fa{\grave{a}}}$ whose coalgebras are precisely Cartesian differential categories. In other words, for a Cartesian left additive category $\mathbb{X}$, $\mathsf{Fa{\grave{a}}}(\mathbb{X})$ is the cofree Cartesian differential category over $\mathbb{X}$. Composition in these cofree Cartesian differential categories is based on the Faà di Bruno formula, and corresponds to composition of differential forms. This composition, however, is somewhat complex and difficult to work with. In this paper we provide an alternative construction of cofree Cartesian differential categories inspired by tangent categories. In particular, composition defined here is based on the fact that the chain rule for Cartesian differential categories can be expressed using the tangent functor, which simplifies the formulation of the higher order chain rule.
description: Accepted and to be published in Theory and Applications of Categories (Oct 2018)
Macro-prudential policy and asset pricing
Creators: name: Wei, Daren
Publisher: name: Imperial College London
Year: 2017

description: I study questions related to the general equilibrium effects of macro-prudential policy designed to restrict speculation driven by belief dispersion among investors. First, I explore the asset pricing implications of differences in beliefs, and I find that belief dispersion caused by overconfidence can explain the downward sloping equity premium term structure and upward sloping bond yield curve. Second, I investigate the impact of speculation driven by belief dispersion on asset prices, social welfare and the aggregate economy. I find speculation reduces social welfare and creates a negative output gap, creating a role for macro-prudential policy. I conclude by studying a general equilibrium asset pricing model with a macro-prudential policy constraint that dampens the leverage cycle. My results show that macroprudential policy can help to mitigate the externalities caused by speculation, enhance economic growth, and increase social welfare even when policy makers do not know the correct physical distribution of exogenous technology shocks.
Additional file 2 of The prevalence of perceived stigma and self-blame and their associations with depression, emotional well-being and social well-being among advanced cancer patients: evidence from the APPROACH cross-sectional study in Vietnam
Creators: name: Pham, Nguyen Tuong
name: Lee, Jia Jia
name: Pham, Nhu Hiep
name: Phan, Thi Do Quyen
name: Tran, Khoa
name: Dang, Hoai Bao
name: Teo, Irene
name: Malhotra, Chetna
name: Finkelstein, Eric A.
name: Ozdemir, Semra
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Holm’s correction for the p-values
Corvus paradisi Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Corvidae
Corvus
Corvus paradisi

description: Corvus paradisi [spec. nov.]
C. albo nigroque varius, cauda cuneiformi, remigibus intermediis longissimis, capite nigro cristato:
Manucodiota cristata ex albo nigroque variata. Raj. av. 195. t. 2. f. 13.
Avis paradisi. Seb. mus. 1 p. 85. t. 52. f. 3. & t. 30. f. 5.
Pica orientalis, cauda duabus pennis longissimis. Edw. av. 113. t. 113.
Habitat in India.
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 107, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Hydrostatic mass profiles in X-COP galaxy clusters
Creators: name: Ettori, S.
name: Ghirardini, V.
name: Eckert, D.
name: Pointecouteau, E.
name: Gastaldello, F.
name: Sereno, M.
name: Gaspari, M.
name: Ghizzardi, S.
name: Roncarelli, M.
name: Rossetti, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the reconstruction of hydrostatic mass profiles in 13 X-ray luminous galaxy clusters that have been mapped in their X-ray and SZ signal out to $R_{200}$ for the XMM-Newton Cluster Outskirts Project (X-COP). Using profiles of the gas temperature, density and pressure that have been spatially resolved out to (median value) 0.9 $R_{500}$, 1.8 $R_{500}$, and 2.3 $R_{500}$, respectively, we are able to recover the hydrostatic gravitating mass profile with several methods and using different mass models. The hydrostatic masses are recovered with a relative (statistical) median error of 3% at $R_{500}$ and 6% at $R_{200}$. By using several different methods to solve the equation of the hydrostatic equilibrium, we evaluate some of the systematic uncertainties to be of the order of 5% at both $R_{500}$ and $R_{200}$. A Navarro-Frenk-White profile provides the best-fit in nine cases out of 13, with the remaining four cases that do not show a statistically significant tension with it. The distribution of the mass concentration follows the correlations with the total mass predicted from numerical simulations with a scatter of 0.18 dex, with an intrinsic scatter on the hydrostatic masses of 0.15 dex. We compare them with the estimates of the total gravitational mass obtained through X-ray scaling relations applied to $Y_X$, gas fraction and $Y_{SZ}$, and from weak lensing and galaxy dynamics techniques, and measure a substantial agreement with the results from scaling laws, from WL at both $R_{500}$ and $R_{200}$ (with differences below 15%), from cluster velocity dispersions, but a significant tension with the caustic masses that tend to underestimate the hydrostatic masses by 40% at $R_{200}$. We also compare these measurements with predictions from alternative models to the Cold Dark Matter, like the "Emergent Gravity" and MOND scenarios.
description: 14 pages, 8 figures, 4 tables. Updated to match the version accepted for publication in A&A. This is one of the three companion papers (including Ghirardini et al. and Eckert et al.) on the X-COP sample. X-COP data products are available for download on https://www.astro.unige.ch/xcop
A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
Creators: name: Korol, Valeriya
name: Rossi, Elena M.
name: Barausse, Enrico
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The upcoming LISA mission offers the unique opportunity to study the Milky Way through gravitational wave radiation from Galactic binaries. Among the variety of Galactic gravitational wave sources, LISA is expected to individually resolve signals from $\sim 10^5$ ultra-compact double white dwarf (DWD) binaries. DWDs detected by LISA will be distributed across the Galaxy, including regions that are hardly accessible to electromagnetic observations such as the inner part of the Galactic disc, the bulge and beyond. We quantitatively show that the large number of DWD detections will allow us to use these systems as tracers of the Milky Way potential. We demonstrate that density profiles of DWDs detected by LISA may provide constraints on the scale length parameters of the baryonic components that are both accurate and precise, with statistical errors of a few percent to $10$ percent level. Furthermore, the LISA sample is found to be sufficient to disentangle between different (commonly used) disc profiles, by well covering the disc out to sufficiently large radii. Finally, up to $\sim 80$ DWDs can be detected through both electromagnetic and gravitational wave radiation. This enables multi-messenger astronomy with DWD binaries and allows one to extract their physical properties using both probes. We show that fitting the Galactic rotation curve constructed using distances inferred from gravitational waves {\it and} proper motions from optical observations yield a unique and competitive estimate of the bulge mass. Instead robust results for the stellar disc mass are contingent upon knowledge of the Dark Matter content.
Luminosity Distributions within Rich Clusters - II: Demonstration and Verification via Simulation
Creators: name: Driver, Simon P.
name: Couch, Warrick J.
name: Phillipps, Steven
name: Smith, Rodney
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present detailed simulations of long exposure CCD images. The simulations are used to explore the validity of the statistical method for reconstructing the luminosity distribution of galaxies within a rich cluster i.e. by the subtraction of field number-counts from those of a sight-line through the cluster. In particular we use the simulations to establish the reliability of our observational data presented in Paper 3. Based on our intended CCD field-of-view (6.5 by 6.5 arcmins) and a 1-sigma detection limit of 26 mags per sq arcsecond, we conclude that the luminosity distribution can be robustly determined over a wide range of absolute magnitude (-23 < M_{R} < -16) provided: (a) the cluster has an Abell richness 1.5 or greater, (b) the cluster's redshift lies in the range 0.1 < z < 0.3, (c) the seeing is better than FWHM 1.25'' and (d) the photometric zero points are accurate to within Delta m = \pm 0.12. If these conditions are not met then the recovered luminosity distribution is unreliable and potentially grossly miss-leading. Finally although the method clearly has limitations, within these limitations the technique represents an extremely promising probe of galaxy evolution and environmental dependencies.
description: 24 pages, 8 figures accepted for publication in MNRAS also available from http://star-www.st-and.ac.uk/~spd3/bib.html
High-Efficiency Multilevel Phase Lenses with Nanostructures on Polyimide Membranes
Creators: name: Howe, Leslie
name: Rajapaksha, Tharindu D.
name: Ellepola, Kalani H.
name: Ho, Vinh X.
name: Aycock, Zachary
name: Nguyen, Minh L. P.
name: Leckey, John P.
name: Macdonnell, Dave G.
name: Kim, Hyun Jung
name: Vinh, Nguyen Q.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Optics (physics.optics)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The emergence of planar meta-lenses on flexible materials has profoundly impacted the long-standing perception of diffractive optics. Despite their advantages, these lenses still face challenges in design and fabrication to obtain high focusing efficiency and resolving power. A nanofabrication technique is demonstrated based on photolithography and polyimide casting for realizing membrane-based multilevel phase-type Fresnel zone plates (FZPs) with high focusing efficiency. By employing advantageous techniques, these lenses with nanostructures are directly patterned into thin polyimide membranes. The computational and experimental results have indicated that the focusing efficiency of these nanostructures at the primary focus increases significantly with increasing the number of phase levels. Specifically, 16-level phase lenses on a polyimide membrane can achieve a focusing efficiency of more than 91.6% of the input signal (9.5 times better than that of a conventional amplitude-type FZP) and focus light into a diffraction-limited spot together with very weak side-lobes. Furthermore, these lenses exhibit considerably reduced unwanted diffraction orders and produce extremely low background signals. The potential impact of these lenses extends across various applications and techniques including microscopy, imaging, micro-diffraction, remote sensing, and space flight instruments which require lightweight and flexible configurations.
description: 27 pages, 7 figures with supporting information
Additional file 3 of The prevalence of perceived stigma and self-blame and their associations with depression, emotional well-being and social well-being among advanced cancer patients: evidence from the APPROACH cross-sectional study in Vietnam
Creators: name: Pham, Nguyen Tuong
name: Lee, Jia Jia
name: Pham, Nhu Hiep
name: Phan, Thi Do Quyen
name: Tran, Khoa
name: Dang, Hoai Bao
name: Teo, Irene
name: Malhotra, Chetna
name: Finkelstein, Eric A.
name: Ozdemir, Semra
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3. Full list of estimates
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0065r
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: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0065r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0065r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Text-mining and ontologies: new approaches to knowledge discovery of microbial diversity
Creators: name: Nédellec, Claire
name: Bossy, Robert
name: Chaix, Estelle
name: Deléger, Louise
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantitative Methods (q-bio.QM)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Biological sciences
subject: FOS: Computer and information sciences

description: Microbiology research has access to a very large amount of public information on the habitats of microorganisms. Many areas of microbiology research uses this information, primarily in biodiversity studies. However the habitat information is expressed in unstructured natural language form, which hinders its exploitation at large-scale. It is very common for similar habitats to be described by different terms, which makes them hard to compare automatically, e.g. intestine and gut. The use of a common reference to standardize these habitat descriptions as claimed by (Ivana et al., 2010) is a necessity. We propose the ontology called OntoBiotope that we have been developing since 2010. The OntoBiotope ontology is in a formal machine-readable representation that enables indexing of information as well as conceptualization and reasoning.
description: 5 pages
Super-efficient temporal solitons in mutually coupled optical cavities
Creators: name: Xue, Xiaoxiao
name: Zheng, Xiaoping
name: Zhou, Bingkun
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: A coherently driven Kerr optical cavity is able to convert a continuous-wave laser to a sequence of ultrashort soliton pulses, enabling the generation of broadband and mode-locked frequency combs. Kerr cavity solitons are balanced through an energy exchange with the driving pump field. Improving the energy conversion efficiency from the pump to the soliton is of great significance for practical applications, but remains an outstanding challenge due to a limited temporal overlap between the soliton and the pump. Here, we report the discovery of temporal Kerr solitons in mutually coupled cavities instead of a traditional single cavity. We propose a strategy for breaking the limitation of pump-to-soliton energy conversion, and connect the underlying mechanism to impedance matching in radiofrequency electronic circuits. With macro optical fiber ring cavities which share the same physical model as miniature optical microresonators, we demonstrate nearly one-order improvement of the efficiency. The results pave the way towards super-efficient soliton microcombs based on optical microresonators with ultra-high quality factors.
description: 30 pages, 13 figures; updated with experimental results
Modification of hyperon masses in nuclear matter
Creators: name: Hong, Ki-Hoon
name: Yakhshiev, Ulugbek
name: Kim, Hyun-Chul
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss the properties of baryons within the framework of the in-medium modified SU(3) Skyrme model. The modification is performed by a minimal way, the medium functionals in the SU(2) sector being introduced. These functionals are then related to nuclear matter properties near the saturation point. The modifications in the SU(3) sector are performed with the additional changes of kaon properties in nuclear matter. The results show that the properties of baryons in the strange sector are sensitive to the in-medium modifications of the kaon properties. The consistency of the in-medium modifications of hadron properties in the present approach with other model approaches and phenomenological indications is also discussed.
description: 11 pages, 7 figures
Shaped Pulses for Energy Efficient High-Field NMR at the Nanoscale
Creators: name: Casanova, J.
name: Wang, Z. -Y.
name: Schwartz, I.
name: Plenio, M. B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The realisation of optically detected magnetic resonance via nitrogen vacancy centers in diamond faces challenges at high magnetic fields which include growing energy consumption of control pulses as well as decreasing sensitivities. Here we address these challenges with the design of shaped pulses in microwave control sequences that achieve orders magnitude reductions in energy consumption and concomitant increases in sensitivity when compared to standard top-hat microwave pulses. The method proposed here is general and can be applied to any quantum sensor subjected to pulsed control sequences.
description: 7 pages, 4 figures
The tilt of the Fundamental Plane of Early-type galaxies: wavelength dependence
Creators: name: Scodeggio, M.
name: Gavazzi, G.
name: Belsole, E.
name: Pierini, D.
name: Boselli, A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The photometric parameters R_e and mu_e of 74 early-type (E+S0+S0a) galaxies in the Coma cluster are derived for the first time in the near IR H band. These are used, coupled with measurements of the central velocity dispersion found in the literature, to determine the H band Fundamental Plane (FP) relation of this cluster. The same procedure is applied to previously available photometric data in the B, V, r, I, and K bands, to perform a multi-wavelength study of the FP. Because systematic uncertainties in the value of the FP parameters are introduced both by the choice of the fitting algorithm, and by the presence of statistical biases connected with the sample selection procedure, we emphasize the importance of deriving the FP parameters in the six photometric bands using an identical fitting algorithm, and appropriate corrections to eliminate the effects of sample incompleteness. We find that the FP mu_e coefficient is stable with wavelength, while the sigma coefficient increases significantly with increasing wavelength, in agreement with an earlier result presented by Pahre & Djorgovski. The slope of the FP relation, although changing with wavelength, never approaches the virial theorem expectation. We also find that the magnitude of the slope change can be entirely explained by the presence of the well known relation between color and magnitude among early-type galaxies. We conclude that the tilt of the Fundamental Plane is significant, and must be due to some form of broken homology among early-type galaxies, while its wavelength dependence derives from whatever mechanism (currently the preferred one is the existence of a mass-metal content sequence) produces the color-magnitude relation in those galaxies.
description: 8 pages, 7 figures, 6 tables; table 3 should be printed in landscape mode, and inserted into the text. Accepted for publication in MNRAS
Orbital magneto-optical response of periodic insulators from first principles
Creators: name: Lebedeva, Irina V.
name: Strubbe, David A.
name: Tokatly, Ilya V.
name: Rubio, Angel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Magneto-optical response, i.e. optical response in the presence of a magnetic field, is commonly used for characterization of materials and in optical communications. However, quantum mechanical description of electric and magnetic fields in crystals is not straightforward as the position operator is ill defined. We present a reformulation of the density matrix perturbation theory for time-dependent electromagnetic fields under periodic boundary conditions, which allows us to treat the orbital magneto-optical response of solids at the \textit{ab initio} level. The efficiency of the computational scheme proposed is comparable to standard linear-response calculations of absorption spectra and the results of tests for molecules and solids agree with the available experimental data. A clear signature of the valley Zeeman effect is revealed in the continuum magneto-optical spectrum of a single layer of hexagonal boron nitride. The present formalism opens the path towards the study of magneto-optical effects in strongly driven low-dimensional systems.
description: 12 pages, 3 figures
title: ADCO, Cart. 186 (11 H 71), f. 0118r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/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: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0118r, 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
Inflationary stochastic anomalies
Creators: name: Pinol, Lucas
name: Renaux-Petel, Sébastien
name: Tada, Yuichiro
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The stochastic approach aims at describing the long-wavelength part of quantum fields during inflation by a classical stochastic theory. It is usually formulated in terms of Langevin equations, giving rise to a Fokker-Planck equation for the probability distribution function of the fields, and possibly their momenta. The link between these two descriptions is ambiguous in general, as it depends on an implicit discretisation procedure, the two prominent ones being the Itô and Stratonovich prescriptions. Here we show that the requirement of general covariance under field redefinitions is verified only in the latter case, however at the expense of introducing spurious `frame' dependences. This stochastic anomaly disappears when there is only one source of stochasticity, like in slow-roll single-field inflation, but manifests itself when taking into account the full phase space, or in the presence of multiple fields. Despite these difficulties, we use physical arguments to write down a covariant Fokker-Planck equation that describes the diffusion of light scalar fields in non-linear sigma models in the overdamped limit. We apply it to test scalar fields in de Sitter space and show that some statistical properties of a class of two-field models with derivative interactions can be reproduced by using a correspondence with a single-field model endowed with an effective potential. We also present explicit results in a simple extension of the single-field $λϕ^4$ theory to a hyperbolic field space geometry. The difficulties we describe seem to be the stochastic counterparts of the notoriously difficult problem of maintaining general covariance in quantum theories, and the related choices of operator ordering and path-integral constructions. Our work thus opens new avenues of research at the crossroad between cosmology, statistical physics, and quantum field theory.
description: 9 pages, 2 figures, additional numerical results, version published as a Letter in Classical and Quantum Gravity
Dorylaimus vestibulifer Micoletzky 1921
Creators: name: Thorne, Gerald
Publisher: name: Zenodo
Year: 1929
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Chromadorea
Rhabditida
Criconematidae
Dorylaimus
Dorylaimus vestibulifer

description: Dorylaimus vestibulifer Micoletzky, 1921.
Micoletzky gave this species the speciﬁc name because of the deep vestibule forming the pharynx. The slightly set off head bears two circlets of large papillae. The posterior half of the esophagus is enlarged by a rather sudden expansion. The cardia is pyriform and as long as the width of the base of the esophagus. The symmetrical ovaries are reﬂexed one-half their length the front being on the left, the rear on the right, side of the body. The prerectum is about twice as long as the rectum.
The male tail bears a pair of supplementary organs just in front of the anus and beginning at a distance about one anal body-diameter in front of this pair is a series of ventral supplementary organs varying in number from eleven to twenty-one. Four pairs of pores are located on the tail.
Several dozen specimens in the collection. Fig. 5 a-e.
description: Published as part of Thorne, Gerald, 1929, Nematodes from the Summit of Long's Peak, Colorado, pp. 181 in Transactions of the American Microscopical Society 48 (2) on pages 185-186, DOI: 10.2307/3222211, http://zenodo.org/record/10797374
Obscured AGB stars in the Magellanic Clouds II. Near-infrared and mid-infrared counterparts
Creators: name: Zijlstra, Albert A.
name: Loup, Cecile
name: Waters, L. B. F. M.
name: Whitelock, P. A.
name: van Loon, Jacco Th.
name: Guglielmo, F.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have carried out an infrared search for obscured AGB stars in the Magellanic Clouds. The survey uncovered a number of obscured AGB stars as well as some supergiants with infrared excess. We present photometry of the sources and discuss the colour diagrams and bolometric luminosities. Most of the AGB stars are luminous, often close to the classical limit of $M_{\rm bol}=-7.1$. To determine whether the stars are oxygen-rich or carbon-rich, we have acquired narrow-band mid-infrared photometry with the ESO TIMMI camera for several sources. All but one are found to show the silicate feature and therefore to have oxygen-rich dust: the colours of the remaining source are consistent with either an oxygen-rich or a carbon-rich nature. A method to distinguish carbon and oxygen stars based on H$-$K versus K$-$[12] colours is presented. We discuss several methods of calculating the mass-loss rate: for the AGB stars the mass-loss rates vary between approximately 5 times 10**-4 and 5 times 10**-6 solar masses per year, depending on assumed dust-to-gas mass ratio. We present a new way to calculate mass-loss rates from the OH-maser emission. We find no evidence for a correlation of the mass-loss rates with luminosity in these obscured stars. Neither do the mass-loss rates for the LMC and SMC stars differ in any clear systematic way from each other. Expansion velocities appear to be slightly lower in the LMC than in the Galaxy. Period determinations are discussed for two sources: the periods are comparable to those of the longer-period galactic OH/IR stars. All of the luminous stars for which periods are available, have significantly higher luminosities than predicted from the period--luminosity relations.
description: 22 pages, uuencoded postscript. 14 figures available on request from Albert Zijlstra (azijlstr@eso.org). Accepted for publication in MNRAS
Perceptual analysis of concatenated moving window (Ehrlich et al., 2018)
Creators: name: Ehrlich, Benjamin
name: Liyu Lin
name: Jiang, Jack
Publisher: name: ASHA journals
Year: 2018
Subjects: subject: 170112 Sensory Processes, Perception and Performance
subject: FOS: Psychology

description: Purpose: The purpose of this study is to develop a program to concatenate acoustic vowel segments that were selected with the moving window technique, a previously developed technique used to segment and select the least perturbed segment from a sustained vowel segment. The concatenated acoustic segments were compared with the nonconcatenated, short, individual acoustic segments for their ability to differentiate normal and pathological voices. The concatenation process sometimes created a clicking noise or beat, which was also analyzed to determine any confounding effects.Method: A program was developed to concatenate the moving window segments. Listeners with no previous rating experience were trained and, then, rated 20 normal and 20 pathological voice segments, both concatenated (2 s) and short (0.2 s) for a total of 80 segments. Listeners evaluated these segments on both the Grade, Roughness, Breathiness, Asthenia, and Strain scale (GRBAS; 8 listeners) and the Consensus Auditory-Perceptual Evaluation of Voice (Kempster, Gerratt, Abbott, Barkmeier-Kraemer, & Hillman, 2009) scale (7 listeners). The sensitivity and specificity of these ratings were analyzed using a receiver-operating characteristic curve. To evaluate if there were increases in particular criteria due to the beat, differences between beat and nonbeat ratings were compared using a 2-tailed analysis of variance.Results: Concatenated segments had a higher sensitivity and specificity for distinguishing pathological and normal voices than short segments. Compared with nonbeat segments, the beat had statistically similar increases for all criteria across Consensus Auditory-Perceptual Evaluation of Voice and GRBAS scales, except pitch and loudness.Conclusions: The concatenated moving window method showed improved sensitivity and specificity for detecting voice disorders using auditory-perceptual analysis, compared with the short moving window segment. It is a helpful tool for perceptual analytic protocols, allowing for voice evaluation using standardized and automated voice-segmenting procedures.
Supplemental Material S1. Introduction and tutorial for using the Grade, Roughness, Breathiness, Asthenia, and Strain (GRBAS) and Consensus Auditory-Perceptual Evaluation of Voice (CAPE-V) scales and an explanation of how auditory-perceptual evaluation can aid in diagnosis and how various vocal fold pathologies can affect speech.
Ehrlich, B., Lin, L., & Jiang, J. (2018). Concatenation of the moving window technique for auditory-perceptual analysis of voice quality. American Journal of Speech-Language Pathology. Advance online publication. https://doi.org/10.1044/2018_AJSLP-17-0103
Preliminary Spectral Analysis of SN 1994I
Creators: name: Baron, E.
name: Hauschildt, P. H.
name: Branch, D.
name: Kirshner, R. P.
name: Filippenko, A. V.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical spectra of the Type Ic supernova 1994I in M51 and preliminary non-LTE analysis of the spectra. Our models are not inconsistent with the explosions of C+O cores of massive stars. While we find no direct evidence for helium in the optical spectra, our models cannot rule out small amounts of helium. More than 0.1~\msol\ of helium seems unlikely.
description: LaTeX, MN style, psfig, and natbib substyles, 7 pages, 4 figures, to appear in MNRAS. Postscript file available from http://www.nhn.uoknor.edu/~baron
VeriPlan: Integrating Formal Verification and LLMs into End-User Planning
Creators: name: Lee, Christine
name: Porfirio, David
name: Wang, Xinyu Jessica
name: Zhao, Kevin
name: Mutlu, Bilge
Publisher: name: arXiv
Year: 2025
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences
subject: I.2.1; I.2.5; I.2.2; I.2.7

description: Automated planning is traditionally the domain of experts, utilized in fields like manufacturing and healthcare with the aid of expert planning tools. Recent advancements in LLMs have made planning more accessible to everyday users due to their potential to assist users with complex planning tasks. However, LLMs face several application challenges within end-user planning, including consistency, accuracy, and user trust issues. This paper introduces VeriPlan, a system that applies formal verification techniques, specifically model checking, to enhance the reliability and flexibility of LLMs for end-user planning. In addition to the LLM planner, VeriPlan includes three additional core features -- a rule translator, flexibility sliders, and a model checker -- that engage users in the verification process. Through a user study (n=12), we evaluate VeriPlan, demonstrating improvements in the perceived quality, usability, and user satisfaction of LLMs. Our work shows the effective integration of formal verification and user-control features with LLMs for end-user planning tasks.
description: In CHI Conference on Human Factors in Computing Systems (CHI '25), April 26-May 1, 2025, Yokohama, Japan. ACM, New York, NY, USA, 19 pages
Statistical Connections Between the Properties of Type Ia Supernovae and the B--V Colors of Their Parent Galaxies, and the Value of H$_0$
Creators: name: Branch, David
name: Romanishin, W.
name: Baron, E.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Statistical connections between the properties of Type Ia supernovae (SNe Ia) and the B--V colors of their parent galaxies are established. Compared to SNe Ia in blue galaxies [B-V$\la$0.75], SNe Ia in redder galaxies have (1) a wider dispersion in the blueshifts of their Si II $λ$6355 absorption features, ten days after maximum light; (2) more rapidly declining light curves; and (3) lower luminosities. Even when the spectroscopically peculiar, very subluminous SNe Ia such as SN 1991bg are disregarded, SNe Ia in red galaxies are less luminous than those in blue galaxies by about 0.3 magnitudes. When SNe Ia that are thought to have been significantly extinguished by dust in their parent galaxies are disregarded, those in blue galaxies have observational absolute--magnitude dispersions of only $σ_{obs}(M_B)$=0.20 and $σ_{obs}(M_V)$=0.17, which implies that their intrinsic absolute--magnitude dispersions are very small. We use six SNe Ia whose absolute magnitudes have been calibrated by means of Cepheids, which also indicate that the intrinsic absolute--magnitude dispersions of SNe Ia in blue galaxies are very small, to calibrate SNe Ia in blue galaxies and obtain $\rm H_0=57\pm4\ km\ s^{-1}\ Mpc^{-1}$. This value is in excellent agreement with that obtained by Saha et al. (1995b), in spite of the fact that they do not take into account any dependence of SN Ia absolute magnitude on the nature of the parent galaxy. Some implications of the statistical connections between SNe Ia and the colors of their parent galaxies, for identifying the progenitor binary systems of SNe Ia and for using high--redshift SNe Ia to measure q$_0$, are briefly discussed.
description: LaTeX file, AASTeX4 style, 2 Tables and 4 Figures included separately. Postscript file available from http://www.nhn.uoknor.edu/~baron/
Corvus infaustus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Corvidae
Corvus
Corvus infaustus

description: Corvus infaustus [spec. nov.]
C. dorso cinereo, rectricibus rufis: intermediis duabus cinereis, fascia nigricante.
Turdus rectricibus rufis: duabus intermediis cinereis fascia nigricante; proximis apice cinereis. Fn. svec. 187.
Merula saxatilis. Will. orn. 145. t. 36. Raj. av. 65. Alb. av. 3. p. 51. t. 55.
Habitat in Europae alpinis sylvis.
Avis proterva, saepe carnivora.
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 107, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quantum Measurement Cooling
Creators: name: Buffoni, Lorenzo
name: Solfanelli, Andrea
name: Verrucchi, Paola
name: Cuccoli, Alessandro
name: Campisi, Michele
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Invasiveness of quantum measurements is a genuinely quantum mechanical feature that is not necessarily detrimental: Here we show how quantum measurements can be used to fuel a cooling engine. We illustrate quantum measurement cooling (QMC) by means of a prototypical two-stroke two-qubit engine which interacts with a measurement apparatus and two heat reservoirs at different temperatures. We show that feedback control is not necessary for operation while entanglement must be present in the measurement projectors. We quantify the probability that QMC occurs when the measurement basis is chosen randomly, and find that it can be very large as compared to the probability of extracting energy (heat engine operation), while remaining always smaller than the most useless operation, namely dumping heat in both baths. These results show that QMC can be very robust to experimental noise. A possible low-temperature solid-state implementation that integrates circuit QED technology with circuit quantum thermodynamics technology is presented.
description: 18 pages, 4 figures
Науково-методичні засади економічної діяльності об’єктів природно-заповідного фонду України
Creators: name: Henyk, Oksana
Publisher: name: figshare
Year: 2018
Subjects: Economics

description: Геник О. В. Науково-методичні засади економічної діяльності об’єктів природно-заповідного фонду України: автореф. дис... канд. екон. наук: 08.00.06 / О. В. Геник; Нац. лісотехн. ун-т України. – Л., 2009. – 20 c.