cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Bayesian parameter-estimation of Galactic binaries in LISA data with Gaussian Process Regression
Creators: name: Strub, Stefan H.
name: Ferraioli, Luigi
name: Schmelzbach, Cedric
name: Stähler, Simon C.
name: Giardini, Domenico
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: The Laser Interferometer Space Antenna (LISA), which is currently under construction, is designed to measure gravitational wave signals in the milli-Hertz frequency band. It is expected that tens of millions of Galactic binaries will be the dominant sources of observed gravitational waves. The Galactic binaries producing signals at mHz frequency range emit quasi monochromatic gravitational waves, which will be constantly measured by LISA. To resolve as many Galactic binaries as possible is a central challenge of the upcoming LISA data set analysis. Although it is estimated that tens of thousands of these overlapping gravitational wave signals are resolvable, and the rest blurs into a galactic foreground noise; extracting tens of thousands of signals using Bayesian approaches is still computationally expensive. We developed a new end-to-end pipeline using Gaussian Process Regression to model the log-likelihood function in order to rapidly compute Bayesian posterior distributions. Using the pipeline we are able to solve the Lisa Data Challenge (LDC) 1-3 consisting of noisy data as well as additional challenges with overlapping signals and particularly faint signals.
description: 13 pages, 10 figures
First Principles explanation of the positive Seebeck coefficient of lithium
Creators: name: Xu, Bin
name: Verstraete, Matthieu J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Lithium is one of the simplest metals, with negative charge carriers and a close reproduction of free electron dispersion. Experimentally, however, Li is one of a handful of elemental solids (along with Cu, Ag, Au etc.) where the sign of the Seebeck coefficient (S) is opposite to that of the carrier. This counterintuitive behavior still lacks a satisfactory interpretation. We calculate S fully from first-principles, within the framework of P.B. Allen's formulation of Boltzmann transport theory. Here it is crucial to avoid the constant relaxation time approximation, which gives a sign for S which is necessarily that of the carriers. Our calculated S are in excellent agreement with experimental data, up to the melting point. In comparison with another alkali metal Na, we demonstrate that within the simplest non-trivial model for the energy dependency of the electron lifetimes, the rapidly increasing density of states (DOS) across the Fermi energy is related to the sign of S in Li. The exceptional energy dependence of the DOS is beyond the free-electron model, as the dispersion is distorted by the Brillouin Zone edge, a stronger effect in Li than other Aliki metals. The electron lifetime dependency on energy is central, but the details of the electron-phonon interaction are found to be less important, contrary to what has been believed for several decades. Band engineering combined with the mechanism exposed here may open the door to new "ambipolar" thermoelectric materials, with a tunable sign for the thermopower even if either n- or p-type doping is impossible.
description: 5 pages 4 figures
Supplementary Results and Discussion (including Table S1 and S2) from The African mosquito-borne diseasosome: geographical patterns, range expansion and future disease emergence
Creators: name: Lehmann, Tovi
name: Kouam, Cedric
name: Woo, Joshua
name: Diallo, Mawlouth
name: Wilkerson, Richard
name: Linton, Yvonne-Marie
Publisher: name: The Royal Society
Year: 2023
Subjects: classificationCode: 310399
subject: Ecology not elsewhere classified
classificationCode: 419999
subject: Other environmental sciences not elsewhere classified
classificationCode: 420299
subject: Epidemiology not elsewhere classified

description: Additional figures based on complementary analyses are provided to strengthen the main paper and suggest additional future analytical approaches. Table S1 lists genera and subgenera of mosquitoes in continental Africa and Table S2 lists the African countries included in this analysis (area and centroid coordinates).
S. D. N. Pavli Divina Providentia PP. III. Bulla. Novae Prorogationis Sacrosancti Generalis Concilij; 1538
Creators: name: Paul III., Papst
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2008

description: Bibliogr. Nachweis: EDIT16 CNCE 14658
Revealing giant exciton fine-structure splitting in 2D perovskites using van der Waals passivation
Creators: name: Canet-Albiach, Rodolfo
name: Krecmarova, Marie
name: Bailach, José Bosch
name: Gualdrón-Reyes, Andrés F.
name: Rodríguez-Romero, Jesús
name: Gorji, Setatira
name: Pashaei-Adl, Hamid
name: Mora-Seró, Iván
name: Pastor, Juan Martínez
name: Sánchez-Royo, Juan Francisco
name: Matutano, Guillermo Muñoz
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The study of two-dimensional (2D) van der Waals materials has been an active field of research in the development of new optoelectronics and photonic applications over the last decade. Organic-inorganic layered perovskites are currently some of the most promising 2D van der Waals materials, due to their exceptional optical brightness and enhanced excitonic effects. However, low crystal quality and spectral diffusion usually broaden the exciton linewidth, obscuring the fine structure of the exciton in conventional photoluminescence experiments. Here, we propose a mechanical approach for reducing the effect of spectral diffusion by means of hBN-capping on layered perovskites with different thicknesses, revealing the exciton fine structure. We used a stochastic model to link the reduction of the spectral linewidth with the population of active charge fluctuation centres present in the organic spacer taking part in the dynamical Stark shift. Active fluctuation centres are reduced by a factor of 3.7 to 7.1 when we include hBN-capping according to our direct spectral measurements. This rate is in good agreement with the analysis of the overlap between the squared perovskite lattice and the hexagonal hBN lattice. Van der Waals forces between both lattices cause the partial clamping of the perovskite organic spacer molecules, and hence, the amplitude of the dynamical Stark shift characteristic of the spectral diffusion effect is reduced. Our work provides an easy and low-cost solution to the problem of accessing important fine-structure excitonic state information, along with an explanation of the important carrier dynamics present in the organic spacer that affect the quality of the optical emission.
Macaca thibetana
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Macaca
Macaca thibetana

description: Macaca thibetana (Milne-Edwards, 1870). C. R. Acad. Sci. Paris, 70:341. TYPE LOCALITY: China, Szechwan, Moupin. DISTRIBUTION: E. Tibet; Szechwan to Kwangtung (China). COMMENT: Includes esau; see Fooden, 1966, Folia Primatol., 5: 160. PROTECTED STATUS: CITES - Appendix II as Order Primates. ISIS NUMBER: 5301406008003013001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 236, DOI: 10.5281/zenodo.7353017
Carmen Christophori Hege[n]dorffini Lipsici de disputatione Lipsensi, inter p[rae]stantissimos theologie p[ro]fessores Joannem Eckiu[m] Karolstadium, et Martinum Lutherum; 1519
Creators: name: Hegendorph, Christoph
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2011

description: Bibliogr. Nachweis: VD16 H 1121. - Vorlageform des Erscheinungsvermerks im Kolophon: Lipsiae excussit Vuolffgangus Monacensis. 1519.
On the consistency of MPS
Creators: name: Souto-Iglesias, Antonio
name: Macià, Fabricio
name: González, Leo M.
name: Cercos-Pita, Jose L.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: The consistency of Moving Particle Semi-implicit (MPS) method in reproducing the gradient, divergence and Laplacian differential operators is discussed in the present paper. Its relation to the Smoothed Particle Hydrodynamics (SPH) method is rigorously established. The application of the MPS method to solve the Navier-Stokes equations using a fractional step approach is treated, unveiling inconsistency problems when solving the Poisson equation for the pressure. A new corrected MPS method incorporating boundary terms is proposed. Applications to one dimensional boundary value Dirichlet and mixed Neumann-Dirichlet problems and to two-dimensional free-surface flows are presented.
description: 36 pages
Macaca tonkeana
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Macaca
Macaca tonkeana

description: Macaca tonkeana (Meyer, 1899). Abh. Zool. Anthrop.-Ethnology. Mus. Dresden, 7 (7):3. TYPE LOCALITY: Indonesia, Sulawesi Tengah, Tonkean. DISTRIBUTION: C. Sulawesi, south to Latimojong, northeast to Gorontolo; Togean Isis. COMMENT: Includes hecki; see Groves, 1980; but see also Fooden, 1969, Bibi. Primatol., No. 10, p. 1 -9. Formerly included in Cynopithecus; see Fooden, 1969, Bibi. Primatol, 10: 106- 115. PROTECTED STATUS: CITES - Appendix II as Order Primates.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 237, DOI: 10.5281/zenodo.7353017
description: {"references": ["Fooden, J. 1969. Taxonomy and evolution of the monkeys of Celebes (Primates: Cercopithecidae). Bibliotheca Primatologica, 10: 1 - 148."]}
Eyn wunderbarlich geschichte, wye die Marckischen Jüdenn das hochwirtigst Sacrament gekaufft, vnd czu Martern sich vnterstanden; 1510
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2010

description: Bibliographischer Nachweis: Nicht VD 16 W 4593 ; Panzer 696
Ab-initio calculation of the effective on-site Coulomb interaction parameters for half-metallic magnets
Creators: name: Sasioglu, Ersoy
name: Galanakis, Iosif
name: Friedrich, Christoph
name: Blügel, Stefan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Correlation effects play an important role in the electronic structure of half-metallic (HM) magnets. In particular, they give rise to non-quasiparticle states above (or below) the Fermi energy at finite temperatures that reduce the spin polarization and, as a consequence, the efficiency of spintronics devices. Employing the constrained random-phase approximation (cRPA) within the full-potential linearized augmented-plane-wave (FLAPW) method using maximally localized Wannier functions, we calculate the strength of the effective on-site Coulomb interaction (Hubbard $U$ and Hund exchange $J$) between localized electrons in different classes of HM magnets considering: (i) \emph{sp}-electron ferromagnets in rock-salt structure, (ii) zincblende 3\emph{d} binary ferromagnets, as well as (iii) ferromagnetic and ferrimagnetic semi- and full-Heusler compounds.
description: 11 pages, 3 figures, 4 tables; accepted for publication in Phys Rev B
Folding lattice proteins with quantum annealing
Creators: name: Irbäck, Anders
name: Knuthson, Lucas
name: Mohanty, Sandipan
name: Peterson, Carsten
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Chemical Physics (physics.chem-ph)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Quantum annealing is a promising approach for obtaining good approximate solutions to difficult optimization problems. Folding a protein sequence into its minimum-energy structure represents such a problem. For testing new algorithms and technologies for this task, the minimal lattice-based HP model is well suited, as it represents a considerable challenge despite its simplicity. The HP model has favorable interactions between adjacent, not directly bound hydrophobic residues. Here, we develop a novel spin representation for lattice protein folding tailored for quantum annealing. With a distributed encoding onto the lattice, it differs from earlier attempts to fold lattice proteins on quantum annealers, which were based upon chain growth techniques. With our encoding, the Hamiltonian by design has the quadratic structure required for calculations on an Ising-type annealer, without having to introduce any auxiliary spin variables. This property greatly facilitates the study of long chains. The approach is robust to changes in the parameters required to constrain the spin system to chain-like configurations, and performs very well in terms of solution quality. The results are evaluated against existing exact results for HP chains with up to $N=30$ beads with 100% hit rate, thereby also outperforming classical simulated annealing. In addition, the method allows us to recover the lowest known energies for $N=48$ and $N=64$ HP chains, with similar hit rates. These results are obtained by the commonly used hybrid quantum-classical approach. For pure quantum annealing, our method successfully folds an $N=14$ HP chain. The calculations were performed on a D-Wave Advantage quantum annealer.
Prevalence of Earth-size planets orbiting Sun-like stars
Creators: name: Petigura, Erik A.
name: Howard, Andrew W.
name: Marcy, Geoffrey W.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Determining whether Earth-like planets are common or rare looms as a touchstone in the question of life in the universe. We searched for Earth-size planets that cross in front of their host stars by examining the brightness measurements of 42,000 stars from National Aeronautics and Space Administration's Kepler mission. We found 603 planets, including 10 that are Earth size (1-2 Earth-radii) and receive comparable levels of stellar energy to that of Earth (within a factor of four). We account for Kepler's imperfect detectability of such planets by injecting synthetic planet-caused dimmings into the Kepler brightness measurements and recording the fraction detected. We find that $11\pm4%$ of Sun-like stars harbor an Earth-size planet receiving between one and four times the stellar intensity as Earth. We also find that the occurrence of Earth-size planets is constant with increasing orbital period (P), within equal intervals of logP up to $\sim200$ d. Extrapolating, one finds $5.7^{+1.7}_{-2.2}%$ of Sun-like stars harbor an Earth-size planet with orbital periods of 200-400 d.
description: Main text: 6 pages, 5 figures, 1 table. Supporting information: 54 pages, 17 pages, 3 tables. Published in the Proceedings of the National Academy of Sciences available at http://www.pnas.org/cgi/doi/10.1073/pnas.1319909110
Von der säligen Bruederschafft der heilige[n] junckfrawen vnnd martererin sant katherinen; [1512]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Bibliographischer Nachweis: VD16 V 2634 und Schottenloher: Schobser, 44 A. - Im Unterschied zur Beschreibung bei Schottenloher "säligen" und "martererin", Textbeginn Bl. 1b. - Erscheinungsvermerk nach der Zuweisung des VD16. - Titelblatt in Rotdruck
Nasalis E. Geoffroy 1812
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Nasalis

description: Nasalis E. Geoffroy, 1812. Ann. Mus. Hist. Nat. Paris, 19:89. REVIEWED BY: D. K. Candland (DKC); R. Fontaine (RF). COMMENT: Includes Simias; see Groves, 1970:639. Szalay and Delson, 1979; and Delson, 1975, Contrib. Primatol., 5:217, considered Simias a subgenus; but also see Krumbiegel, 1978, Saugetierk. Mitt., 26:59-75. ISIS NUMBER: 5301406008007000000 as Nasalis. 5301406008012000000 as Simias.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 237, DOI: 10.5281/zenodo.7353017
description: {"references": ["Groves, C. P. 1970. The forgotten leaf-eaters, and the phylogeny of the Colobinae. Pp. 555 - 587, in Old World Monkeys: Evolution, systematics and behavior (J. R. Napier and P. H. Napier, eds.). Academic Press, London, 660 pp.", "Szalay, F. S., and E. Delson. 1979. Evolutionary history of the primates. Academic Press, New York, 580 pp.", "Krumbiegel, I. 1978. Die Kurzschwanz-Stumpfnase, Simias concolor (Miller, 1903), und die ubrigen Nasenaffen. Saugetierkundliche Mitteilungen, 26: 59 - 75."]}
Vermerckt die Begencknuß des kunig philips vo[n] Castilia, Gehalten durch die kuniglichen maiestat zu Costentz des reichstag, Anno Tausent Funffhundert und siben iare; [1507]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2010

description: Bibliogr. Nachweis: VD16 V 811
MPEC 2023-V132 : 2023 VX3
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 VX3

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.
Nasalis concolor Miller 1903
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Nasalis
Nasalis concolor

description: Nasalis concolor Miller, 1903. Smithson. Mise. Coll., 45:67. TYPE LOCALITY: Indonesia, W. Sumatra, S. Pagai Isl. DISTRIBUTION: Mentawi Isis. COMMENT: Type species of Simias (Miller, 1903) which was considered a subgenus by Delson, 1975, Contrib. Primatol., 5: 217. PROTECTED STATUS: CITES - Appendix I as Simias concolor and U.S. ESA - Endangered as Nasalis (= Simias) concolor. ISIS NUMBER: 5301406008012001001 as Simias concolor.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 237, DOI: 10.5281/zenodo.7353017
title: Argentinensium Episcoporu[m] Cathalogus; 1508
title: cu[m] eorundem vita at[que] certis historijs: rebus[que] gestis: & illustratione totius fere Episcopatus Argẽn. Castigationibus Ioanne Adelpho Mülingo Argentinesi. & Geruasio Souphero brisgoico
titleType: Subtitle
Creators: name: Wimpfeling, Jakob
name: Adelphus, Johannes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliogr. Nachweis: VD16 W 3344. - Verfasser nicht auf der Haupttitelseite genannt. - Conclusio: Ioannes Grieninger: Ciuis Argentinensis: formis excussit Anno natalium christianorum: millesimo supra quingentesimu[m]: octauo. Die vero vndetrigesima Mensis Augusti
Accurate Evaluations of Strain and Stress in Atomistic Simulations of Crystalline Solids
Creators: name: Yang, Jerry Zhijian
name: Wu, Xiaojie
name: Li, Xiantao
Publisher: name: arXiv
Year: 2013
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In this paper, we study the accuracy of Irving-Kirkwood type of formulas for the approximation of continuum quantities from atomistic simulations. Such formulas are derived by expressing the displacement, deformation gradient and stress in terms of certain kernel functions. We propose two criteria for choosing the kernel functions to significantly improve the sampling accuracy. We present a simple procedure to construct kernel functions that meet these criteria. Further, numerical tests on homogeneous and non-homogeneous systems provide validations for our analysis.
description: 16 pages, 8 figures
Nanoscopic friction under electrochemical control
Creators: name: de Wijn, A. S.
name: Fasolino, A.
name: Filippov, A.
name: Urbakh, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We propose a theoretical model of friction under electrochemical conditions focusing on the interaction of a force microscope tip with adsorbed polar molecules of which the orientation depends on the applied electric field. We demonstrate that the dependence of friction force on the electric field is determined by the interplay of two channels of energy dissipation: (i) the rotation of dipoles and (ii) slips of the tip over potential barriers. We suggest a promising strategy to achieve a strong dependence of nanoscopic friction on the external field based on the competition between long range electrostatic interactions and short range chemical interactions between tip and adsorbed polar molecules.
description: 5 pages, 5 figures
Multi-scale comparative spectral analysis of satellite total solar irradiance measurements from 2003 to 2013 reveals a planetary modulation of solar activity and its non-linear dependence on the 11-year solar cycle
Creators: name: Scafetta, Nicola
name: Willson, Richard C.
Publisher: name: arXiv
Year: 2013
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Herein we adopt a multi-scale dynamical spectral analysis technique to compare and study the dynamical evolution of the harmonic components of the overlapping ACRIMSAT/ACRIM3, SOHO/VIRGO and SORCE/TIM total solar irradiance (TSI) records during 2003.15 to 2013.16 in solar cycles 23 and 24. The three TSI time series present highly correlated patterns. Significant power spectral peaks are common to these records and are observed at the following periods: 0.070 year, 0.097 year, 0.20 year, 0.25 year, 0.30-0.34 year, 0.39 year. Less certain spectral peaks occur at about 0.55 year, 0.60-0.65 year and 0.7-0.9 year. Four main frequency periods at 24.8 days (0.068 year), 27.3 days (0.075 year), at 34-35 days (0.093-0.096 year) and 36-38 days (0.099-0.104 year) characterize the solar rotation cycle. The amplitude of these oscillations, in particular of those with periods larger than 0.5 year, appears to be modulated by the 11-year solar cycle. Similar harmonics have been found in other solar indices. The observed periodicities are found highly coherent with the spring, orbital and synodic periods of Mercury, Venus, Earth and Jupiter. We conclude that solar activity is likely modulated by planetary gravitational and electromagnetic forces acting on the sun. The strength of the sun's response to planetary forcing depends non-linearly on the state of internal solar dynamics: planetary-sun coupling effects are enhanced during solar activity maxima and attenuated during minima.
description: 18 pages, 10 figures, 3 tables
Jn hoc libello co[n]tinent[ur] Reliquiae cu[m] indulge[n]cijs Monasterij S. Maximini Co[n]fessoris & Archiepiscopi Treuirorum :-; [1515]
Creators: name: Scheckmann, Johann
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliogr. Nachweis: VD16 S 2392. - Verf. ermittelt
MPEC 2023-V133 : 2023 VY3
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 VY3

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.
Finite inflation in curved space
Creators: name: Hergt, Lukas T.
name: Agocs, Fruzsina J.
name: Handley, Will J.
name: Hobson, Michael P.
name: Lasenby, Anthony N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate the effects of non-zero spatial curvature on cosmic inflation in the light of cosmic microwave background (CMB) anisotropy measurements from the Planck 2018 legacy release and from the 2015 observing season of BICEP2 and the Keck Array. Even a small percentage of non-zero curvature today would significantly limit the total number of e-folds of the scale factor during inflation, rendering just-enough inflation scenarios with a kinetically dominated or fast-roll stage prior to slow-roll inflation more likely. Finite inflation leads to oscillations and a cutoff towards large scales in the primordial power spectrum and curvature pushes them into the CMB observable window. Using nested sampling, we carry out Bayesian parameter estimations and model comparisons taking into account constraints from reheating and horizon considerations. We confirm the preference of CMB data for closed universes with Bayesian odds of over $100:1$ and with a posterior on the curvature density parameter of $Ω_{K,0}=-0.051\pm0.017$ for a curvature extension of LCDM and $Ω_{K,0}=-0.031\pm0.014$ for Starobinsky inflation. Model comparisons of various inflation models give similar results as for flat universes with the Starobinsky model outperforming most other models.
description: 46 pages, 32 figures, 3 tables, submitted to PRD, from chapter 5 of L. T. Hergt's doctoral thesis at https://www.repository.cam.ac.uk/handle/1810/323129, data available at https://zenodo.org/record/6547872
Nasalis larvatus
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Nasalis
Nasalis larvatus

description: Nasalis larvatus (Wurmb, 1787). Verh. Batav. Genootsch., 3:353. TYPE LOCALITY: Indonesia, W. Kalimantan, Pontianak. DISTRIBUTION: Borneo. COMMENT: Subgenus Nasalis; see Delson, 1975, Contrib. Primatol., 5:217. PROTECTED STATUS: CITES - Appendix I and U.S. ESA - Endangered. ISIS NUMBER: 5301406008007001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 237, DOI: 10.5281/zenodo.7353017
Implementation of the left-right symmetric model in FeynRules
Creators: name: Roitgrund, Aviad
name: Eilam, Gad
name: Bar-Shalom, Shaouly
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present an implementation of the manifest left-right symmetric model in FeynRules. The different aspects of the model are briefly described alongside the corresponding elements of the model file. The model file is validated and can be easily translated to matrix element generators such as MadGraph5_aMC@NLO, CalcHEP, Sherpa, etc. The implementation of the left-right symmetric model is a useful step for studying new physics signals with the data generated at the LHC.
description: 59 pages, 3 figures, 9 Tables
Infra posite sacros[an]ct[a]e reliquie in monasterio s[an]cti Mathie aplii extra muros ciuitatis Treuiren[sis] pie cristi fidelium deuotioni ostendi consueuerunt; 1513
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Kolophon: ... Caspar Hochffeder calcographo diligenter impresse Anno d[omin]i. M. quinge[n]tesimotredecimo Jn vigilia ascensionis
R-matrix analysis of elastic scattering, phase shift and radiative capture reaction cross sections in the $α+ α$ system
Creators: name: Chakraborty, Suprita
name: Santra, Rajkumar
name: Roy, Subinit
name: Datar, V. M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The unstable nucleus $^8$Be, with its two $α$-cluster configuration, is the doorway to the formation of heavier $α$-cluster nuclei. Most importantly, its the precursor of the production of $^{12}$C through the Hoyle state, a resonance state of three $α$ clusters, in the helium burning phase of a massive star. The nucleus exhibits a ground state band of rotational states established through $α-α$ scattering experiments. A subsequent precision particle-$γ$ coincidence measurement of the electromagnetic transition between the 4$^+\rightarrow$ 2$^+$ excited states also corroborated the evidence for a highly deformed dumb-bell shaped structure of $^8$Be. A simultaneous phenomenological R-matrix analysis of the measured capture reaction cross sections along with the elastic excitation function and phase shift data has been performed. The resulting reduced transition strength of 21.96$\pm$3.86 $e^2 fm^4$ compares well with the estimated experimental value of 21.0$\pm$2.3 e$^2$ fm$^4$. The R-matrix yield of the B($E2$) value is closer to the prediction of cluster model but about 19$\%$ less than the {\it ab initio} result.
A fully-actuated quadcopter representation using quaternions
Creators: name: Cariño, J.
name: Abaunza, H.
name: Castillo, P.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology

description: Recent advances in practical fields like robotics and the miniaturisation of many sensors and actuators have turned autonomous vehicles into a reality. These systems come in many shapes and forms depending on the medium and their design but can be classified in one of two categories according to their mechanical configuration and number of actuators: fully-actuated and under-actuated vehicles; the second group still poses many challenges for the automatic control and robotics communities. This work introduces an easy methodology, based on quaternions, for designing controllers for a class of under-actuated systems, such as multicopter vehicles. The methodology starts from a fully-actuated representation of the system and adapts it to be implemented in under-actuated systems. In addition, it allows the easy development of controllers without taking care the coupled dynamics of the system. The proposed approach is based on Lyapunov's stability theory and is proven for certain criteria of the system's dynamics. The quadcopter configuration is used to validate the proposed methodology in simulations and in experimental tests. Abbreviations: AGV: autonomous ground vehicle; AUV: autonomous underwatervehicle; DoF: degree(s) of freedom; ESC: energy shaping controller; SFC: statefeedback controller; SSC: separated saturations controller; UAV: unmanned aerialvehicle
title: Ordnung der gantzen Procession, deß Allerheiligsten un[d] Hochwürdigisten Sacraments, wie dieselb in der Fürstlichen Hauptstatt München inn Obern Bayrn, [et]c. auff das Fest Corporis Christi gehalten wirdt; [ca. 1586]
title: Auß dem alten vnd newen Testament genommen, vnnd in Zünfften eingetheylet
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Vorlageform des Erscheinungsvermerks: Getruckt zu München
title: Ordnung der gantzen Procession deß Allerheiligisten vnnd Hochwürdigisten Sacraments, wie dieselb inn der Fürstlichen Hauptstatt München inn Obern Bayrn, [et]c. auff das Fest Corporis Christi gehalten vnnd diß drey vnd neuntzigist Jahr inn grosser perfection angestellt wirdt; 1593
title: Auß dem Alten vnd Newen Testament genommen, vnd in Zünfften eingetheilt
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Vorlageform des Erscheinungsvermerks: Anno M. D. LXXXXIII. - Kolophon: Getruckt zu München, bey Adam Berg
Papio Muller 1773
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Cercopithecidae
Papio

description: Papio Muller, 1773. Des Ritters... Linne...Vollständiges Natursyst. REVIEWED BY: D. K. Candland (DKC); R. Fontaine (RF). COMMENT: Includes Mandrillus; see Dandelot, 1974, Part 3:9. CAH and PG consider Mandrillus a distinct genus. In view of intergradation data, it might be preferable to combine most of the species in this genus (except leucophaeus and sphinx); see Thorington and Groves, 1970:639 (CPG). Includes Chaeropithecus as a subgenus; see Szalay and Delson, 1979:403. Van Gelder, 1977, Am. Mus. Novit., 2635:8 included Papio in Cercopithecus. For authorship of generic name, see Delson and Napier, 1976, Bull. Zool. Nomenci., 33:46. ISIS NUMBER: 5301406008004000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Primates, pp. 216-243 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 237, DOI: 10.5281/zenodo.7353017
description: {"references": ["Dandelot, P. 1974. Order Primates. Part 3. Pp. 1 - 45, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated.", "Thorington, R. W., Jr., and C. P. Groves. 1970. An annotated classification of the Cercopithecoidea. Pp. 629 - 647, in Old World Monkeys (J. R. Napier and P. H. Napier, eds.). Academic Press, London, 660 pp.", "Szalay, F. S., and E. Delson. 1979. Evolutionary history of the primates. Academic Press, New York, 580 pp.", "Delson, E., and P. H. Napier. 1976. Request for determination of the generic names of the baboon and the mandrill (Mammalia: Primates, Cercopithecidae) Z. N. (S.) 2093. Bulletin of Zoological Nomenclature, 33 (1): 46 - 60."]}
The blue sky of GJ3470b: the atmosphere of a low-mass planet unveiled by ground-based photometry
Creators: name: Nascimbeni, V.
name: Piotto, G.
name: Pagano, I.
name: Scandariato, G.
name: Sani, E.
name: Fumana, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: GJ3470b is a rare example of a "hot Uranus" transiting exoplanet orbiting a nearby M1.5 dwarf. It is of crucial interest for atmospheric studies because it is one of the most inflated low-mass planets known, bridging the boundary between "super-Earths" and Neptunian planets. We present two new ground-based light curves of GJ3470b gathered by the LBC camera at the Large Binocular Telescope. Simultaneous photometry in the ultraviolet (lambda_c = 357.5 nm) and optical infrared (lambda_c = 963.5 nm) allowed us to detect a significant change of the effective radius of GJ3470b as a function of wavelength. This can be interpreted as a signature of scattering processes occurring in the planetary atmosphere, which should be cloud-free and with a low mean molecular weight. The unprecedented accuracy of our measurements demonstrates that the photometric detection of Earth-sized planets around M dwarfs is achievable using 8-10m size ground-based telescopes. We provide updated planetary parameters, and a greatly improved orbital ephemeris for any forthcoming study of this planet.
description: 8 pages, 6 figures, 1 table; accepted for publication in A&A
A vindication of the RR Lyrae Fourier light curve decomposition for the calculation of metallicity and distance in globular clusters
Creators: name: Ferro, A. Arellano
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: We report the mean metallicity and absolute magnitude of RR Lyrae stars in a sample of 37 globular clusters, calculated via the Fourier decomposition of their light curves and ad hoc semiempirical calibrations, in an unprecedented homogeneous approach. This enabled a new discussion of the metallicity dependence of the horizontal branch (HB) luminosity, as a fundamental distance indicator. The calibration for the RRab and RRc stars should be treated separately. For the RRab the dispersion is larger and non-linear. For the RRc stars the correlation is less steep, very tight and linear. The relevance of the HB structural parameter L, is highlighted and offer a non-linear calibration of the form MV ([Fe/H],L). Excellent agreement is found between values of [Fe/H] and MV from the light curve decomposition with spectroscopic values and distances obtained via Gaia-DR3 and HST. The variable stars census in 35 clusters includes 326 stars found by our program.
description: 17 pages, 4 figures, 3 tables. arXiv admin note: text overlap with arXiv:1701.02719
title: Thuntenhausen vnnser lieben frawe[n] gotzhauß; 1544
title: in des Durchleüchtigen hochgebornen Fürsten vnd herrn, herrn Wilhelms vnd Ludwigs gebrüeder Pfallntzgrauen bey Rhein, Herzogen in Obern vnnd Nidern Bair[e]n [et]c. Land, Freysinger bistumb gelege[n]: Etlich mercklich genaden so Got der Almechtig durch verdiennen vnnd fürpit Marie seiner werd[e]n můter. Nemlich im yetzigen der mindern zal. xliiij. Jar vil menschen beweist hat ... So ... herr Lucas Brobst zů Beyherting, Als Obrister Pfarrer genennten Gotzhauss zedruckhen vergönnt hat
titleType: Subtitle
Creators: name: Wagner, Lucas
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Vorlageform des Erscheinungsvermerks: Anno domini 1544.
Zero-phase angle asteroid taxonomy classification using unsupervised machine learning algorithms
Creators: name: Colazo, M.
name: Alvarez-Candal, A.
name: Duffard, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We are in an era of large catalogs and, thus, statistical analysis tools for large data sets, such as machine learning, play a fundamental role. One example of such a survey is the Sloan Moving Object Catalog (MOC), which lists the astrometric and photometric information of all moving objects captured by the Sloan field of view. One great advantage of this telescope is represented by its set of five filters, allowing for taxonomic analysis of asteroids by studying their colors. However, until now, the color variation produced by the change of phase angle of the object has not been taken into account. In this paper, we address this issue by using absolute magnitudes for classification. We aim to produce a new taxonomic classification of asteroids based on their magnitudes that is unaffected by variations caused by the change in phase angle. We selected 9481 asteroids with absolute magnitudes of Hg, Hi and Hz, computed from the Sloan Moving Objects Catalog using the HG12 system. We calculated the absolute colors with them. To perform the taxonomic classification, we applied a unsupervised machine learning algorithm known as fuzzy C-means. This is a useful soft clustering tool for working with {data sets where the different groups are not completely separated and there are regions of overlap between them. We have chosen to work with the four main taxonomic complexes, C, S, X, and V, as they comprise most of the known spectral characteristics. We classified a total of 6329 asteroids with more than 60% probability of belonging to the assigned taxonomic class, with 162 of these objects having been characterized by an ambiguous classification in the past. By analyzing the sample obtained in the plane Semimajor axis versus inclination, we identified 15 new V-type asteroid candidates outside the Vesta family region.
A Fully-Actuated Quadcopter Representation using Quaternions
Creators: name: no, J. Cari
name: Abaunza, H.
name: Castillo, P.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Computational Biology

description: Recent advances in practical fields like robotics and the miniaturization of many sensors and actuators have turned autonomous vehicles into a reality. These systems come in many shapes and forms depending on the medium and their design, but can be classified in one of two categories according to their mechanical configuration and number of actuators: fully actuated and under actuated vehicles, the second group still poses many challenges for the automatic control and robotics communities. This work introduces an easy methodology, based on quaternions, for designing controllers for a class of under-actuated systems, such as multicopter vehicles. The methodology starts from a fully actuated representation of the system and adapts it to be implemented in under actuated systems. In addition, it allows the easy development of controllers without take on care the coupled dynamics of the system. The proposed approach is based on Lyapunov's stability theory and is proven for certain criteria of the system's dynamics. The quadcopter configuration is used to validate the proposed methodology in simulations and in experimental tests.
Supplemental Figures S1-S10 & Supplemental Tables S1 & S2 from Innovation-facilitating networks create inequality
Creators: name: Moser, Cody
name: Smaldino, Paul E.
Publisher: name: The Royal Society
Year: 2023
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310901
subject: Animal behaviour

description: Supplemental figures and tables for Innovation-Facilitating Networks Create Inequality
Finite-size effects on the ferroelectricity in rhombohedral HfO$_2$
Creators: name: Delodovici, Francesco
name: Barone, Paolo
name: Picozzi, Silvia
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this work we analyze the finite-size effects on the structural properties and on the polarization of the rhombohedral phase of HfO$_2$ subjected to a biaxial compressive strain. We show how the presence of surface charges affects the polarization, leading to a strong reduction with respect to its bulk value. This reduction can be ascribed to two mechanisms: the coupling between compressive strain and the phase-transition order parameter; the changes in the ferroelectric distortion. We give two alternative explanations of this phenomenon: from an atomistic point of view, analyzing the evolution of the bond lengths, and from a symmetry-analysis point of view, considering the changes in the amplitude of the symmetry-allowed distortions, when a slab configuration is considered. These results are independent on the slab-thickness in the considered range, suggesting the absence of a critical thickness for ferroelectricity in HfO$_2$, in agreement with the proposed improper nature of hafnia ferroelectricity.
Low-Resolution Spectrum of the Diffuse Galactic Light and 3.3 um PAH emission with AKARI InfraRed Camera
Creators: name: Tsumura, Kohji
name: Matsumoto, Toshio
name: Matsuura, Shuji
name: Sakon, Itsuki
name: Tanaka, Masahiro
name: Wada, Takehiko
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We first obtained the spectrum of the diffuse Galactic light (DGL) at general interstellar space in 1.8-5.3 um wavelength region with the low-resolution prism spectroscopy mode of the AKARI Infra-Red Camera (IRC) NIR channel. The 3.3 um PAH band is detected in the DGL spectrum at Galactic latitude |b| < 15 deg, and its correlations with the Galactic dust and gas are confirmed. The correlation between the 3.3 um PAH band and the thermal emission from the Galactic dust is expressed not by a simple linear correlation but by a relation with extinction. Using this correlation, the spectral shape of DGL at optically thin region (5 deg < |b| < 15 deg) was derived as a template spectrum. Assuming that the spectral shape of this template spectrum is uniform at any position, DGL spectrum can be estimated by scaling this template spectrum using the correlation between the 3.3 um PAH band and the thermal emission from the Galactic dust.
description: 7 pages, 5 figures, accepted by Publications of the Astronomical Society of Japan (PASJ)