cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Focal Conic Flower Textures at Curved Interfaces
Creators: name: Beller, Daniel A.
name: Gharbi, Mohamed A.
name: Honglawan, Apiradee
name: Stebe, Kathleen J.
name: Yang, Shu
name: Kamien, Randall D.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Focal conic domains (FCDs) in smectic-A liquid crystals have drawn much attention both for their exquisitely structured internal form and for their ability to direct the assembly of micro- and nanomaterials in a variety of patterns. A key to directing FCD assembly is control over the eccentricity of the domain. Here, we demonstrate a new paradigm for creating spatially varying FCD eccentricity by confining a hybrid-aligned smectic with curved interfaces. In particular, we manipulate interface behavior with colloidal particles in order to experimentally produce two examples of what has recently been dubbed the flower texture, where the focal hyperbolae diverge radially outward from the center of the texture, rather than inward as in the canonical eventail or fan texture. We explain how this unconventional assembly can arise from appropriately curved interfaces. Finally, we present a model for this system that applies the law of corresponding cones, showing how FCDs may be embedded smoothly within a "background texture" of large FCDs and concentric spherical layers, in a manner consistent with the qualitative features of the smectic flower. Such understanding could potentially lead to disruptive liquid crystal technologies beyond displays, including patterning, smart surfaces, microlens arrays, sensors and nanomanufacturing.
Room Temperature In-plane <100> Magnetic Easy Axis for Fe3O4/SrTiO3(001):Nb Grown by Infrared PLD
Creators: name: Monti, Matteo
name: Sanz, Mikel
name: Oujja, Mohamed
name: Rebollar, Esther
name: Castillejo, Marta
name: Castillejo, Marta
name: Bollero, Alberto
name: Camarero, Julio
name: Cuñado, Jose Luis F.
name: Nemes, Norbert M.
name: Mompean, Federico J.
name: Garcia-Hernández, Mar
name: Nie, Shu
name: McCarty, Kevin F.
name: N'Diaye, Alpha T.
name: Chen, Gong
name: Schmid, Andreas K.
name: Marco, José F.
name: de la Figuera, Juan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We examine the magnetic easy-axis directions of stoichiometric magnetite films grown on SrTiO3:Nb by infrared pulsed-laser deposition. Spin-polarized low-energy electron microscopy reveals that the individual magnetic domains are magnetized along the in-plane <100> film directions. Magneto-optical Kerr effect measurements show that the maxima of the remanence and coercivity are also along in-plane <100> film directions. This easy-axis orientation differs from bulk magnetite and films prepared by other techniques, establishing that the magnetic anisotropy can be tuned by film growth.
description: 3 pages, 3 figures
Microsciurus J. A. Allen 1895
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Microsciurus

description: Microsciurus J. A. Allen, 1895. Bull. Am. Mus. Nat. Hist., 7:332. ISIS NUMBER: 5301410002018000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
Large-gap quantum anomalous Hall states induced by functionalizing buckled Bi-III monolayer/Al$_{2}$O$_{3}$
Creators: name: Jin, Suhua
name: Xia, Yunyouyou
name: Shi, Wujun
name: Hu, Jiayu
name: Claessen, Ralph
name: Hanke, Werner
name: Thomale, Ronny
name: Li, Gang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Chiral edge modes inherent to the topological quantum anomalous Hall (QAH) effect are a pivotal topic of contemporary condensed matter research aiming at future quantum technology and application in spintronics. A large topological gap is vital to protecting against thermal fluctuations and thus enabling a higher operating temperature. From first-principle calculations, we propose Al$_{2}$O$_{3}$ as an ideal substrate for atomic monolayers consisting of Bi and group-III elements, in which a large-gap quantum spin Hall effect can be realized. Additional half-passivation with nitrogen then suggests a topological phase transition to a large-gap QAH insulator. By effective tight-binding modelling, we demonstrate that Bi-III monolayer/Al$_{2}$O$_{3}$ is dominated by $p_{x}, p_{y}$ orbitals, with subdominant $p_z$ orbital contributions. The topological phase transition into the QAH is induced by Zeeman splitting, where the off-diagonal spin exchange does not play a significant role. The effective model analysis promises utility far beyond Bi-III monolayer/Al$_{2}$O$_{3}$, as it should generically apply to systems dominated by $p_{x}, p_{y}$ orbitals with a band inversion at $Γ$.
description: 9 pages with 4 figures
Microsciurus alfari
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Microsciurus
Microsciurus alfari

description: Microsciurus alfari (J. A. Allen, 1895). Bull. Am. Mus. Nat. Hist., 7: 333. TYPE LOCALITY: Costa Rica, Jimenez. DISTRIBUTION: S. Central America; perhaps in N. South America. COMMENT: Apparently included in flaviventer by Cabrera, 1961:355; but see Hall, 1981:439-440. ISIS NUMBER: 5301410002018001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
MPEC 2024-C40 : DAILY ORBIT UPDATE (2024 February 4)
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Multi-centered black holes with a negative cosmological constant
Creators: name: Chimento, Samuele
name: Klemm, Dietmar
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present a recipe that allows to construct multi-centered black holes embedded in an arbitrary FLRW universe. These solutions are completely determined by a function satisfying the conformal Laplace equation on the spatial slices $\text{E}^3$, $\text{S}^3$ or $\text{H}^3$. Since anti-de Sitter space can be written in FLRW coordinates, this includes as a special case multi-centered black holes in AdS, in the sense that, far away from the black holes, the energy density and the pressure approach the values given by a negative cosmological constant. We study in some detail the physical properties of the single-centered asymptotically AdS case, which does not coincide with the usual Reissner-Nordström-AdS black hole, but is highly dynamical. In particular, we determine the curvature singularities and trapping horizons of this solution, compute the surface gravity of the trapping horizons, and show that the generalized first law of black hole dynamics proposed by Hayward holds in this case. It turns out that the spurious big bang/big crunch singularities that appear when one writes AdS in FLRW form, become real in presence of these dynamical black holes. This implies that actually only one point of the usual conformal boundary of AdS survives in the solutions that we construct. Finally, a generalization to arbitary dimension is also presented.
description: 17 pages, 5 figures
Antidotarius animae; 30.03.1499
Creators: name: Nicolaus De Saliceto
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: Goff S44; HR 14171; Pell Ms 10324 (10095); IGI 8522; IBP 4848; Madsen 3578; GW M39513
The Hipparcos Pleiades parallax error is also a proper motion error
Creators: name: Makarov, Valeri V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The mean parallax of the Pleiades open cluster from the Hipparcos catalog is larger than the true value by approximately 1 mas. The origin of this error, as well as a possible algorithm of correcting it, was proposed by Makarov (2002). The problem is reassessed using the more accurate Gaia data with a focus on the predicted correction to the Pleiades proper motions. The accurately determined differences Gaia - Hipparcos for 52 common stars are close to these estimates within the formal uncertainties for all three parameters, which strongly suggests that the proposed interpretation was correct. With adjustments for the systematic vector field fitted with 126 vector spherical harmonics to degree 7, these differences amount to $(+0.39,\,-0.74)$ mas yr$^{-1}$. The implications of small-scale proper motion and position errors in Hipparcos for present day astrometry are briefly discussed.
description: Accepted in RevMexAA. In this version, the Abstract in the pdf file is expanded above the publication limit
Microsciurus flaviventer
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Microsciurus
Microsciurus flaviventer

description: Microsciurus flaviventer (Gray, 1867). Ann. Mag. Nat. Hist., ser. 20, 3:432. TYPE LOCALITY: Brazil. DISTRIBUTION: Upper Amazon River Basin, from the Rio Negro to Peru, the Andes of Peru, Ecuador and Colombia. COMMENT: Formerly included alfari and mimulus; see comments under those species. ISIS NUMBER: 5301410002018003001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
Efficient and improved prediction of the band offsets at semiconductor heterojunctions from meta-GGA density functionals
Creators: name: Ghosh, Arghya
name: Jana, Subrata
name: Rauch, Tomáš
name: Tran, Fabien
name: Marques, Miguel A. L.
name: Botti, Silvana
name: Constantin, Lucian A.
name: Niranjan, Manish K.
name: Samal, Prasanjit
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Accurate theoretical prediction of the band offsets at interfaces of semiconductor heterostructures can often be quite challenging. Although density functional theory has been reasonably successful to carry out such calculations and efficient and accurate semilocal functionals are desirable to reduce the computational cost. In general, the semilocal functionals based on the generalized gradient approximation (GGA) significantly underestimate the bulk band gaps. This, in turn, results in inaccurate estimates of the band offsets at the heterointerfaces. In this paper, we investigate the performance of several advanced meta-GGA functionals in the computational prediction of band offsets at semiconductor heterojunctions. In particular, we investigate the performance of r2SCAN (revised strongly-constrained and appropriately-normed functional), rMGGAC (revised semilocal functional based on cuspless hydrogen model and Pauli kinetic energy density functional), mTASK (modified Aschebrock and Kümmel meta-GGA functional), and LMBJ (local modified Becke-Johnson) exchange-correlation functionals. Our results strongly suggest that these meta-GGA functionals for supercell calculations perform quite well, especially, when compared to computationally more demanding GW calculations. We also present band offsets calculated using ionization potentials and electron affinities, as well as band alignment via the branch point energies. Overall, our study shows that the aforementioned meta-GGA functionals can be used within the DFT framework to estimate the band offsets in semiconductor heterostructures with predictive accuracy.
MIRECLE: Science Yield for a Mid-IR Explorer-Class Mission to Study Non-Transiting Rocky Planets Orbiting the Nearest M-Stars Using Planetary Infrared Excess
Creators: name: Mandell, Avi M.
name: Lustig-Yaeger, Jacob
name: Stevenson, Kevin
name: Staguhn, Johannes
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

description: Recent investigations have demonstrated the potential for utilizing a new observational and data analysis technique for studying the atmospheres of non-transiting exoplanets with combined light that relies on acquiring simultaneous, broad-wavelength spectra and resolving planetary infrared emission from the stellar spectrum through simultaneous fitting of the stellar and planetary spectral signatures. This new data analysis technique, called Planetary Infrared Excess (PIE), holds the potential to open up the opportunity for measuring MIR phase curves of non-transiting rocky planets around the nearest stars with a relatively modest telescope aperture. We present simulations of the performance and science yield for a mission and instrument concept that we call the MIR Exoplanet CLimate Explorer (MIRECLE), a concept for a moderately-sized cryogenic telescope with broad wavelength coverage (1 - 18 um) and a low-resolution (R ~ 50) spectrograph designed for the simultaneous wavelength coverage and extreme flux measurement precision necessary to detect the emission from cool rocky planets with PIE. We present exploratory simulations of the potential science yield for PIE measurements of the nearby planet Proxima Cen b, showing the potential to measure the composition and structure of an Earth-like atmosphere with a relatively modest observing time. We also present overall science yields for several mission architecture and performance metrics, and discuss the technical performance requirements and potential telescope and instrument technologies that could meet these requirements.
description: Accepted to Astronomical Journal
On the nature of reconnection at a solar coronal null point above a separatrix dome
Creators: name: Pontin, D. I.
name: Priest, E. R.
name: Galsgaard, K.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Three-dimensional magnetic null points are ubiquitous in the solar corona, and in any generic mixed-polarity magnetic field. We consider magnetic reconnection at an isolated coronal null point, whose fan field lines form a dome structure. We demonstrate using analytical and computational models several features of spine-fan reconnection at such a null, including the fact that substantial magnetic flux transfer from one region of field line connectivity to another can occur. The flux transfer occurs across the current sheet that forms around the null point during spine-fan reconnection, and there is no separator present. Also, flipping of magnetic field lines takes place in a manner similar to that observed in quasi-separatrix layer or slip-running reconnection.
description: Accepted for publication in the Astrophysical Journal
The Making of a Maker Space - A case study
Creators: name: Murphy, Ingrid
Publisher: name: figshare
Year: 2020
Subjects: subject: Design
subject: 139999 Education not elsewhere classified
subject: FOS: Educational sciences

description: A case study exploring design of maker spaces with interactive resources including RFID enabled Materials Library and AR Tool board published in Reframing Space for LearningExcellence and innovation in university teachingAuthor/Editor(s): Bilham, T. Hamsbire, C., Hartog M. &, Doolan , M.A.ISBN: 9781782772460 Published: 15 Jul 2019 UCL IOE Press
Sermones ad heremitas; 1500
Creators: name: Augustinus, Aurelius
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: Goff A1320; TFS 1903oo; Pell 1516; Arnoult 167; IGI 1039; IBP 676; Polain (B) 405; Sallander 2061; Madsen 453; Walsh 3736, S1-3736b; Bod-inc A-599; Sheppard 6550; Pr 8410; BMC VIII 223; GW 3008 (Pseudo-Augustinus)
Beyond galaxy bimodality: the complex interplay between kinematic morphology and star formation in the local Universe
Creators: name: Fraser-McKelvie, A.
name: Cortese, L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: It is generally assumed that galaxies are a bimodal population in both star formation and structure: star-forming galaxies are disks, while passive galaxies host large bulges or are entirely spheroidal. Here, we test this scenario by presenting a full census of the kinematic morphologies of a volume-limited sample of galaxies in the local Universe extracted from the MaNGA galaxy survey. We measure the integrated stellar line-of-sight velocity to velocity dispersion ratio ($V/σ$) for 4574 galaxies in the stellar mass range $9.75 < \log M_{\star}[\rm{M}_{\odot}] < 11.75$. We show that at fixed stellar mass, the distribution of $V/σ$ is not bimodal, and that a simple separation between fast and slow rotators is over-simplistic. Fast rotators are a mixture of at least two populations, referred to here as dynamically-cold disks and intermediate systems, with disks dominating in both total stellar mass and number. When considering star-forming and passive galaxies separately, the star-forming population is almost entirely made up of disks, while the passive population is mixed, implying an array of quenching mechanisms. Passive disks represent $\sim$30% (both in number and mass) of passive galaxies, nearly a factor of two higher than that of slow rotators, reiterating that these are an important population for understanding galaxy quenching. These results paint a picture of a local Universe dominated by disky galaxies, most of which become somewhat less rotation-supported upon or after quenching. While spheroids are present to a degree, they are certainly not the evolutionary end-point for the majority of galaxies.
description: 17 pages (incl. 5 of appendix), accepted for publication in ApJ
(Mirabilia Romae vel potius) Historia et descriptio urbis Romae. Add.: Indulgentiae ecclesiarum principalium urbis Romae; 18.01.1492
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: H 11196; R (Suppl.) p. 79; Sander 4545; Schudt 5; IGI 6449; GW M23570
Microsciurus mimulus
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Microsciurus
Microsciurus mimulus

description: Microsciurus mimulus (Thomas, 1898). Ann. Mag. Nat. Hist., ser. 7, 2:266. TYPE LOCALITY: Ecuador, Esmeraldas, Cachavi, 665 ft. (203 m). DISTRIBUTION: N. W. Ecuador, W. Colombia, and Panama. COMMENT: Includes boquetensis and isthmius; see Handley, 1966, in Wenzel and Tipton, Ectoparasites of Panama, p. 777. Cabrera, 1961:356, included mimulus in flaviventer; but see Hall, 1981:440. ISIS NUMBER: 5301410002018002001 as M. boquetensis. 5301410002018004001 as M. isthmius.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
Hilbert Space Methods for Reduced-Rank Gaussian Process Regression
Creators: name: Solin, Arno
name: Särkkä, Simo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: This paper proposes a novel scheme for reduced-rank Gaussian process regression. The method is based on an approximate series expansion of the covariance function in terms of an eigenfunction expansion of the Laplace operator in a compact subset of $\mathbb{R}^d$. On this approximate eigenbasis the eigenvalues of the covariance function can be expressed as simple functions of the spectral density of the Gaussian process, which allows the GP inference to be solved under a computational cost scaling as $\mathcal{O}(nm^2)$ (initial) and $\mathcal{O}(m^3)$ (hyperparameter learning) with $m$ basis functions and $n$ data points. Furthermore, the basis functions are independent of the parameters of the covariance function, which allows for very fast hyperparameter learning. The approach also allows for rigorous error analysis with Hilbert space theory, and we show that the approximation becomes exact when the size of the compact subset and the number of eigenfunctions go to infinity. We also show that the convergence rate of the truncation error is independent of the input dimensionality provided that the differentiability order of the covariance function is increases appropriately, and for the squared exponential covariance function it is always bounded by ${\sim}1/m$ regardless of the input dimensionality. The expansion generalizes to Hilbert spaces with an inner product which is defined as an integral over a specified input density. The method is compared to previously proposed methods theoretically and through empirical tests with simulated and real data.
Spin-motive force and orbital-motive force: from magnon BEC to chiral Weyl superfluids
Creators: name: Volovik, G. E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Spin-motive geometric force acting on electrons in metallic ferromagnets is extended to spin-motive force in magnon BEC, which is represented by phase-coherent precession of magnetization, and to the orbital-motive force in superfluid 3He-A. In 3He-A there are two contributions to the orbital-motive force. One of them comes from the chiral nature of this liquid. Another one originates from chiral Weyl fermions living in the vicinity of the topologically protected Weyl points, and is related to the phenomenon of chiral anomaly.
description: 4 pages, JETP Letters style, no figures, references added, version submitted to JETP Letters
Sermones et tractatus diversi. (1r) [Systematisches Inhaltsverzeichnis]. (2r) Johannes Gerson: Tractatus de praeparatione ad missam post pollutionem nocturnam. (6r) Sermones diversi praecipue de poenitentia et de tempore. (22ra) [Franciscus de Mayronis: Sermones de tempore]. (22rb) Sermones de tempore. (80r) [Franciscus de Mayronis: De sancto Matthaeo]. (86r) [Materialsammlung]. (99r) Sermones diversi. (113r) [Bernardinus Senensis: Quadragesimale de evangelio aeterno. Sermo XVI]. (119r) Sermones de diversis praecipue de confessione. (154v) Sermones de sancta Clara. (158r) Sermones et tractatus de diversis. (169r) Sermones de poenitentia. (182r) De VII itineribus aeternitatis. (184r) [Notiz]. (185r) De tribus zelis. (188v) [Robertus Caracciolus de Licio:] Sermo de cathenis daemonum. (194r) Sermo de nativitate B.M.V. (196r) De XII malis quae veniunt a concupiscentia. (199r) Sermones de B.M.V. (203r) [De misericordia]. (206r) Sermones de sanctis. (220r) Franciscus de Mayronis: Sermones de sanctis. (234r) Sermones diversi. (241v) Bernardinus. (249r) Notae de vanitate, de flagellis dei et de oratione. (252r) [Engelbertus de Colonia:] Sermo de purificatione B.M.V. (258r) [Johannes Herolt:] Sermo in die resurrectionis domini. (260r) Nota de peccato mortali. (261r) Sermones de angelis. (270r) Johannes Herolt: Sermones communes.; [um 1450]
Creators: name: Gerson, Jean
name: Franciscus De Maironis
name: Bernardinus Senensis
name: Caracciolo, Roberto
name: Engelbertus Admontensis
name: Herolt, Johannes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2019

description: Entstehungsort:. [Süddeutschland] - Entstehungszeit: [um 1450]
Azimuthal dynamo wave in spherical shell convection
Creators: name: Cole, Elizabeth
name: Käpylä, Petri J.
name: Mantere, Maarit J.
name: Brandenburg, Axel
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the finding of an azimuthal dynamo wave of a low-order (m=1) mode in direct numerical simulations (DNS) of turbulent convection in spherical shells. Such waves are predicted by mean field dynamo theory and have been obtained previously in mean-field models. Observational results both from photometry and Doppler imaging have revealed persistent drifts of spots for several rapidly rotating stars, but, although an azimuthal dynamo wave has been proposed as a possible mechanism responsible for this behavior, it has been judged as unlikely, as practical evidence for such waves from DNS has been lacking. The large-scale magnetic field in our DNS, which is due to self-consistent dynamo action, is dominated by a retrograde m=1 mode. Its pattern speed is nearly independent of latitude and does not reflect the speed of the differential rotation at any depth. The extrema of magnetic m=1 structures coincide reasonably with the maxima of m=2 structures of the temperature. These results provide direct support for the observed drifts being due to an azimuthal dynamo wave.
description: 6 pages, 4 figures, submitted to ApJL
The relation between quasars' optical spectra and variability
Creators: name: Nagoshi, Shumpei
name: Iwamuro, Fumihide
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: This work aimed to find the relationship between quasars' optical variability and spectral features to reveal the regularity behind the random variation. It is known that quasar's FeII/Hbeta flux ratio and equivalent width of [OIII]5007 are negatively correlated, called Eigenvector 1. In this work, we visualized the relationship between the position on this Eigenvector 1 (EV1) plane and how they had changed their brightness after ~10 years. We conducted three analyses using different quasar samples each. The first analysis showed the relation between their distributions on the EV1 plane and how much they had changed brightness, using 13,438 Sloan Digital Sky Survey quasars. This result shows how brightness changes later are clearly related to the position on the EV1 plane. In the second analysis, we plotted the sources reported as Changing-Look(State) Quasars on the EV1 plane. This result shows that the position on the EV1 plane corresponds activity level of each source, the bright or dim state of them are distributed on the opposite sides divided by the typical quasar distribution. In the third analysis, we examined the transition vectors on the EV1 plane using sources with multiple-epoch spectra. This result shows that the brightening and dimming sources move on the similar path and they turn into the position corresponding to the opposite activity level. We also found this trend is opposite to the empirical rule that RFeII positively correlated with the Eddington ratio, which has been proposed based on the trends of a large number of quasars. From all these analyses, it is indicated that quasars tend to oscillate between both sides of the distribution ridge on the EV1 plane; each of them corresponds to a dim state and a bright state. This trend in optical variation suggests that significant brightness changes, such as Changing-Look quasars, are expected to repeat.
description: 12 pages, 4 figures, 1 table. Accepted for publication in PASJ
Microsciurus santanderensis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Microsciurus
Microsciurus santanderensis

description: Microsciurus santanderensis (Hernandez-Camacho, 1957). An. Soc. Biol. Bogota, 7:219. TYPE LOCALITY: Colombia, Santander Dept., Meseta de los Caballeros, N.E. of La Albania. DISTRIBUTION: Colombia, between the Magdalena River and the Cordillera Oriental. COMMENT: Originally described as a subspecies of Sciurus pucheranii; see HernandezCamacho, 1960, Caldasia, 8:359-368.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
Vinylphosphonites for Staudinger-induced chemoselective peptide cyclization and functionalization
Creators: name: Kasper, Marc-André
name: Glanz, Maria
name: Oder, Andreas
name: Schmieder, Peter
name: Von Kries, Jens Peter
name: Hackenberger, Christian
Publisher: name: Humboldt-Universität zu Berlin
Year: 2019
Subjects: subject: 540 Chemie und zugeordnete Wissenschaften

description: In this paper, we introduce vinylphosphonites for chemoselective Staudinger-phosphonite reactions (SPhR) with azides to form vinylphosphonamidates for the subsequent modification of cysteine residues in peptides and proteins. An electron-rich alkene is turned into an electron-deficient vinylphosphonamidate, thereby inducing electrophilic reactivity for a following thiol addition. We show that by varying the phosphonamidate ester substituent we can fine-tune the reactivity of the thiol addition and even control the functional properties of the final conjugate. Furthermore, we observed a drastic increase in thiol addition efficiency when the SPhR is carried out in the presence of a thiol substrate in a one-pot reaction. Hence, we utilize vinylphosphonites for the chemoselective intramolecular cyclization of peptides carrying an azide-containing amino acid and a cysteine in high yields. Our concept was demonstrated for the stapling of a cell-permeable peptidic inhibitor for protein–protein interaction (PPI) between BCL9 and beta-catenin, which is known to create a transcription factor complex playing a role in embryonic development and cancer origin, and for macrocyclization of cell-penetrating peptides (CPPs) to enhance the cellular uptake of proteins.
ASSESSMENT OF ALCOHOL USE AND RISKY SEXUAL BEHAVIORS AMONG LOCAL DRINK SELLERS IN ADDIS KETEMA SUB-CITY, ADDIS ABABA
Creators: name: IBRAHIM KEDIR
Publisher: name: Zenodo
Year: 2011

description: Introduction AIDS continues to be a major global health priority. The number of people living with HIV is still growing worldwide reaching an estimated 33.3 million in 2009. Slightly more than half are women. Patterns of alcohol consumption prevail in countries with the most severe HIV epidemics. Hazardous alcohol use is often assumed mainly to affect men, but women are harmed in large numbers by alcohol use: either their own or that of their partner. Women are at risk of alcohol-related sexual risk behavior in several ways. Women who sell alcohol are at increased risk of drinking alcohol themselves, engaging in unprotected sex with their clients, and HIV infection. Objective The objective of this study was to assess the prevalence of alcohol use and its association with risky sexual behaviors among local drink sellers in Addis Ketema sub-city, Addis Ababa. Method A cross sectional study was conducted among 698 women engaged in selling local alcohol drinks in Addis Ketema sub-city Addis Ababa. The sample size was calculated using single population proportion formula and multistage cluster sampling technique was used. The data were collected through standardized questionnaire by trained data collectors. Respondents were assessed by socio demographic variables, type, amount and frequency of alcohol use and also risky sexual behaviors and bivariate and multivariate analysis were used to assess the association between these variables. Logistic regression was used to control confounding variables
Myosciurus Thomas 1909
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Myosciurus

description: Myosciurus Thomas, 1909. Ann. Mag. Nat. Hist., ser. 8, 3:474. ISIS NUMBER: 5301410002019000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 356, DOI: 10.5281/zenodo.7353023
SI.pdf from A predictive model of UV-A-riboflavin crosslinking treatment on porcine corneas
Creators: name: Bonfanti, Alessandra
name: Pandolfi, Anna
Publisher: name: The Royal Society
Year: 2023
Subjects: classificationCode: 400399
subject: Biomedical engineering not elsewhere classified
classificationCode: 460207
subject: Modelling and simulation
classificationCode: 490109
subject: Theoretical and applied mechanics

description: Material data for the layers of cornea
[Theologisch-prophetische Sammelhandschrift]. (1r) Marquard von Lindau: Auslegung der zehn Gebote. (53r) Allegorische Ausdeutung des Kirchengebäudes. (56r) Vom rechten Verhalten in der Kirche. (57v) Die sieben Weihen der Priester, allegorisch ausgedeutet. (59r) Engelstaat und irdische Ordnung. (59v) [Nachtrag]. (60r) Johannes Tortsch: Onus mundi . (86r) Johannes Tortsch: Die drei Feste der heiligen Birgitta. (86v) [Vorrede]. (87r) Weissagungen, Hildegard von Bingen zugeschrieben. (92r) Prophetische Vision. (94v) Anselm von Marsico: Vaticinia 18, 20, 23 . (95v) Priester Siegwalts Prophezeiung des Römischen Reiches und eines neuen Reiches unter Nürnbergs Führung. (96v) Umsturzprophezeiung. (97r) Politische Prophezeiung über die Könige von Böhmen, Frankreich, England, den Kaiser und den Papst. (98r) Prophezeiung von Zwietracht und kirchlicher Erneuerung für 1420-1470. (98v) Prophezeiung des Sieges der Ketzer. (99v) Lateinische Prophezeiung. (99v) Erweiternde deutsche Übersetzung in Reimpaaren mit Prosazusatz. (100r) Prophezeiung des Weltendes. (102v) [Bardellini de Bardellinis: Umsturzprophezeiung]. (103r) Birgitta von Schweden zugeschriebene Prophezeiung. (103v) [Dietrich von Zengg OFM: Umsturzprophezeiung. (106r) Telesforus von Cosenza: Prophezeiung . (109r) Johannes de Rupescissa: Vademecum in tribulatione . (112v) Anton Zipfer: Reformschrift in Visionsform. (117v) 13 Prophezeiungen für 1464, einem Meister Theodorius zugeschrieben. (119v) [Inhaltsregister]. (120r) Prophetische Verse, Legat und Kaiser in den Mund gelegt. (120v) [Gebet- oder Psalmfragment, 16. Jh.]. (121r) [Namenseintrag](unleserlich); 1465
Creators: name: Marquard Von Lindau
name: Tortsch, Johannes
name: Hildegard von Bingen, Heilige
name: Telesphorus De Cusentia
name: Johannes de Rupescissa, OFM
name: Dietrich Von Zengg
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2019

description: Entstehungsort: [Süddeutschland]. - Entstehungszeit: 1465
(Mirabilia Romae vel potius) Historia et descriptio urbis Romae; 14.03.1496
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: Goff M601; HR 11198; MirR p. 25, (7); Sander 4549; IGI 6455; IDL 3233; Oates 1524, 1525; GW M23581
Wave-Front Reconstruction via Single-Pixel Homodyne Imaging
Creators: name: Cuozzo, Savannah L.
name: Gabaldon, Charris
name: Barge, Pratik J.
name: Niu, Ziqi
name: Lee, Hwang
name: Cohen, Lior
name: Novikova, Irina
name: Mikhailov, Eugeniy E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We combine single-pixel imaging and homodyne detection to perform full object recovery (phase and amplitude). Our method does not require any prior information about the object or the illuminating fields. As a demonstration, we reconstruct the optical properties of several semi-transparent objects and find that the reconstructed complex transmission has a phase precision of 0.02 radians and a relative amplitude precision of 0.01.
Disappearance of a narrow Mg II absorption system with a measured velocity up to $\rm 166,000 km s^{-1}$
Creators: name: Chen, Zhi-Fu
name: Qin, Yi-Ping
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Quasar J152645.61+193006.7 ($z_{\rm e}=2.5771$) was observed by the Sloan Digital Sky Survey (SDSS) on 2006 May 31, and again on 2011 April 9. The time interval of the SDSS two observations is 497.4 days at the quasar rest frame. From the spectra of this quasar, we detect a phenomenon of disappearance of a narrow $\rm Mg II λ\lambda2796,2803$ absorption system with a velocity up to $\rm 166,129 km s^{-1}$ with respect to the quasar. This disappearance event can be caused by changes in the ionization state of absorbing gas or by the bulk motion of the absorbing gas across the quasar sightline. The coverage fraction analysis shows that this absorber partially covers the background emission sources with an effective coverage fraction of $C_{\rm f}=0.40\pm0.06$. The time variation analysis and the coverage fraction analysis imply that this absorber might be intrinsic to the quasar. However, the scenario of a cosmologically separated foreground object located at $z=0.9170$ accounting for the phenomenon cannot be ruled out according to current available data.
Analysis of eight magnetic chemically peculiar stars with rotational modulation
Creators: name: Kobzar, O.
name: Khalack, V.
name: Bohlender, D.
name: Mathys, G.
name: Shultz, M. E.
name: Bowman, D. M.
name: Paunzen, E.
name: Lovekin, C.
name: David-Uraz, A.
name: Sikora, J.
name: Lampens, P.
name: Richard, O.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar photometry to the astronomical community. We have used TESS data to study rotational modulation in the light curves of a sample of chemically peculiar stars with measured large-scale magnetic fields (mCP stars). In general, mCP stars show inhomogeneous distributions of elements in their atmospheres that lead to spectroscopic (line profile) and photometric (light curve) variations commensurate with the rotational period. We analyzed the available TESS data from 50 sectors for eight targets after post-processing them in order to minimize systematic instrumental trends. Analysis of the light curves allowed us to determine rotational periods for all eight of our targets. For each star, we provide a phase diagram calculated using the derived period from the light curves and from the available measurements of the disk-averaged longitudinal magnetic field $\langle B_{\rm z}\rangle$. In most cases, the phased light curve and $\langle B_{\rm z}\rangle$ measurements show consistent variability. Using our rotation periods, and global stellar parameters derived from fitting Balmer line profiles, and from Geneva and Strömgren-Crawford photometry, we determined the equatorial rotational velocities and calculated the respective critical rotational fractions $v_{\rm eq}/v_{\rm crit}$. We have shown from our sample that the critical rotational fraction decreases with stellar age, at a rate consistent with the magnetic braking observed in the larger population of mCP stars.
A unified framework for linear thermo-visco-elastic wave propagation including the effects of stress-relaxation
Creators: name: Neefjes, Erik García
name: Nigro, David
name: Gower, Artur L.
name: Assier, Raphaël C.
name: Pinfield, Valerie J.
name: Parnell, William J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences
subject: 74J05, 74J25, 74B10, 74B15, 74B02

description: We present a unified framework for the study of wave propagation in homogeneous linear thermo-visco-elastic (TVE) continua, starting from conservation laws. In free-space such media admit two thermo-compressional modes and a shear mode. We provide asymptotic approximations to the corresponding wavenumbers which facilitate the understanding of dispersion of these modes, and consider common solids and fluids as well as soft materials where creep compliance and stress relaxation are important. We further illustrate how commonly used simpler acoustic/elastic dissipative theories can be derived via particular limits of this framework. Consequently, our framework allows us to: i) simultaneously model interfaces involving both fluids and solids, and ii) easily quantify the influence of thermal or viscous losses in a given configuration of interest. As an example, the general framework is applied to the canonical problem of scattering from an interface between two TVE half spaces in perfect contact. To illustrate, we provide results for fluid-solid interfaces involving air, water, steel and rubber, paying particular attention to the effects of stress relaxation.
description: Accepted in Proceedings of the Royal Society A
Myosciurus pumilio
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Myosciurus
Myosciurus pumilio

description: Myosciurus pumilio (Le Conte, 1857). Proc. Acad. Nat. Sci. Phila., 9: 11. TYPE LOCALITY: Gabon. DISTRIBUTION: S.E. Nigeria; Cameroun; Gabon; Bioko. ISIS NUMBER: 5301410002019001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 357, DOI: 10.5281/zenodo.7353023
title: Quartierspiegel Leimbach 2024
Creators: name: (:Unkn) Unknown
Publisher: name: Zentralbibliothek Zürich
Year: 2024
Subjects: subject: 314 Allgemeine Statistiken zu Europa
subject: 710 Städtebau, Raumplanung, Landschaftsgestaltung
subject: 949 Geschichte anderer Teile Europas
subject: Zürich-Leimbach
subject: Zürich / Kreis 2
subject: Quartier
subject: Amtliche Statistik
subject: Bevölkerungsstatistik

description: Eingefasst von Uetliberg und Entlisberg, hat Leimbach seinen Vorort-Charakter nie ganz verloren. Geprägt wurde das südlichste Quartier der Stadt von jeher durch seine genossenschaftlichen Siedlungen. Dank zahlreichen unbebauten Flächen ist Leimbach in den letzten Jahren immer attraktiver geworden: Viele neue Wohnungen sind auf Familien ausgerichtet.
Indian Ceramics Triennial Exhibition/Symposium Catalogue & Reviews
Creators: name: Murphy, Ingrid
Publisher: name: figshare
Year: 2020
Subjects: subject: 190501 Crafts
subject: FOS: Arts (arts, history of arts, performing arts, music)
subject: 190502 Fine Arts (incl. Sculpture and Painting)

description: Catalogue/Symposium and reviews of work created for the inaugural Indian Ceramics Triennial. The Jawahar Kala Kendra (JKK), in collaboration with the Contemporary Clay Foundation, Breaking Ground, held the 1st Indian Ceramic Triennale, from August 31 to November 18, 2018. The event involved projects from 37 Indian and 13 international artist projects, and a 2 day symposium. Artists were invited to explore themes of scale, site specificity and/or concept through installation, interaction, technology and performance. The Indian artists were selected through a nationwide open call and foreign artists through invitation from the ICT selection committee, comprised of 6 curators.
Causal dynamical triangulation for non-critical open-closed string field theory
Creators: name: Kawabe, Hiroshi
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We extend the 2 dimensional Causal Dynamical Triangulation (CDT) model from the usual model of closed string to the one of open-closed string. The matrix-vector model describing the loop gas model is modified so as to possess the nature of the CDT, i.e. the time foliation structure. Stochastic quantization method produces interactions of loop and line variables similar to those in the non-critical open-closed string field theories. By taking an appropriate scaling, we realize an extended model of the generalized CDT (GCDT), which keeps the causality in a broad sense.
description: 15pages, 22figures, typos corrected
Postilla super Epistolas et Evangelia quadragesimalia (cum Quaestionibus Antonii Betontini et Alexandri de Ales); 13.12.1494
Creators: name: Nicolaus De Lyra
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: Goff N119; HR 10390; Pestail-Lota 2; Polain (B) 4600; IBE 2287; IGI 6828; IBP 3953; IBPort 1279; Kotvan 882; Mendes 896; Martín Abad N-19; Walsh 2235; Oates 2043; BMC V 426; GW M26590
Vita S. Alberti de Drepano; [1499]
Creators: name: Poluciis, Johannes Maria de
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Bibliografischer Nachweis: Goff P906; C 4809; R 1846; Essling 1305; Sander 168; IBE 4713; IGI 7977; IBP 4537; Walsh 2760; Hunt 3060; BMC V 591; GW M34814
Anomaly inflow for local boundary conditions
Creators: name: Ivanov, A. V.
name: Vassilevich, D. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study the $η$-invariant of a Dirac operator on a manifold with boundary subject to local boundary conditions with the help of heat kernel methods. In even dimensions, we relate this invariant to $η$-invariants of a boundary Dirac operator, while in odd dimension, it is expressed through the index of boundary operators. We stress the necessity of the strong ellipticity condition for the applicability of our methods. We show that the Witten--Yonekura boundary conditions are not strongly elliptic, though they are very close to strongly elliptic ones.
description: 19 pages, V2: misprints corrected, comments added
title: Quartierspiegel Enge 2024
Creators: name: (:Unkn) Unknown
Publisher: name: Zentralbibliothek Zürich
Year: 2024
Subjects: subject: 314 Allgemeine Statistiken zu Europa
subject: 710 Städtebau, Raumplanung, Landschaftsgestaltung
subject: 949 Geschichte anderer Teile Europas
subject: Zürich-Enge
subject: Zürich / Kreis 2
subject: Quartier
subject: Amtliche Statistik
subject: Bevölkerungsstatistik

description: Dem Engpass zwischen Sihl und unterem Seebecken verdankt das Quartier Enge seinen Namen. Alles andere als eng sind dagegen die Seepromenade und der Rieterpark mit dem darin liegenden Museum Rietberg. Diese Orte der Erholung verleihen der Gegend ebenso ihren Charakter wie die zahlreiche Villen oder die beiden Kulturzentren Tonhalle und Kongresshaus.