cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: [Humaniores]. (1r) Catalogus Humaniorum Ordine alphabetico. (93r) Humaniores secundum series; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
Spermophilus adocetus
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
Spermophilus
Spermophilus adocetus

description: Spermophilus adocetus (Merriam, 1903). Proc. Biol. Soc. Wash., 16:79. TYPE LOCALITY: Mexico, Michoacan, La Salada, 40 mi. (64 km) S. Uruapan. DISTRIBUTION: E. Jalisco, Michoacan, and N. Guerrero (W.C. Mexico). COMMENT: Subgenus Otospermophilus; see Hall, 1981:399. Gromov et al., 1965: 145, considered Otospermophilus a distinct genus. Includes infernatus; see Alvarez and Ramirez-Pulido, 1968, Rev. Soc. Mex. Hist. Nat., 29: 181-190. ISIS NUMBER: 5301410002032001001.
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 366, 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.", "Gromov, I. M., D. I. Bibikov, N. I. Kalabukhov, and M. N. N. Meier. 1965. Fauna SSSR, Mlekopitayushchie, tom. 3, vyp. 2 [Fauna of the U. S. S. R. Mammals. vol. 3, No. 2]. Nazemnye belich'e [Ground Squirrels]. Nauka, Moscow-Leningrad, 467 pp. (in Russian)."]}
Encapsulated formulation of the Selective Frequency Damping method
Creators: name: Jordi, Bastien E.
name: Cotter, C. J.
name: Sherwin, Spencer J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Optimization and Control (math.OC)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We present an alternative "encapsulated" formulation of the Selective Frequency Damping method for finding unstable equilibria of dynamical systems, which is particularly useful when analysing the stability of fluid flows. The formulation makes use of splitting methods, which means that it can be wrapped around an existing time-stepping code as a "black box". The method is first applied to a scalar problem in order to analyse its stability and highlight the roles of the control coefficient $χ$ and the filter width $Δ$ in the convergence (or not) towards the steady-state. Then the steady-state of the incompressible flow past a two-dimensional cylinder at $Re=100$, obtained with a code which implements the spectral/hp element method, is presented.
QU Vul: An Integral Field Spectroscopy Case Study of a Nova Shell
Creators: name: Santamaría, E.
name: Guerrero, M. A.
name: Toalá, J. A.
name: Ramos-Larios, G.
name: Sabin, L.
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 present GTC MEGARA high-dispersion integral field spectroscopic observations of the nova remnant QU\,Vul, which provide a comprehensive 3D view of this nova shell. The tomographic analysis of the H$α$ emission reveals a complex physical structure characterized by an inhomogeneous and clumpy distribution of the material within this shell. The overall structure can be described as a prolate ellipsoid with an axial ratio of 1.4$\pm$0.2, a major axis inclination with the line of sight of $12^{\circ}\pm6^{\circ}$, and polar and equatorial expansion velocities $\approx$560 km~s$^{-1}$ and 400$\pm$60 km s$^{-1}$, respectively. The comparison of the expansion velocity on the plane of the sky with the angular expansion implies a distance of 1.43$\pm$0.23 kpc. The ionized mass is found to be $\approx 2\times 10^{-4}$ M$_\odot$, noting that the information on the 3D distribution of material within the nova shell has allowed us to reduce the uncertainty on its filling factor. The nova shell is still in its free expansion phase, which can be expected as the ejecta mass is much larger than the swept-up circumstellar medium mass. The 3D distribution and radial velocity of material within the nova shell provide an interpretation of the so-called "castellated" line profiles observed in early optical spectra of nova shells, which can be attributed to knots and clumps moving radially along different directions.
description: 10 pages, 6 figures
Rapid and reliable thickness identification of two-dimensional nanosheets using optical microscopy
Creators: name: Li, Hai
name: Wu, Jumiati
name: Huang, Xiao
name: Lu, Gang
name: Yang, Jian
name: Lu, Xin
name: Xiong, Qihua
name: Zhang, Hua
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The physical and electronic properties of ultrathin two-dimensional (2D) layered nanomaterials are highly related to their thickness. Therefore, the rapid and accurate identification of single- and few- to multi-layer nanosheets is essential to their fundamental study and practical applications. Here, a universal optical method has been developed for simple, rapid and reliable identification of single- to quindecuple-layer (1L-15L) 2D nanosheets, including graphene, MoS2, WSe2 and TaS2, on Si substrates coated with 90 nm or 300 nm SiO2. The optical contrast differences between the substrates and 2D nanosheets with different layer numbers were collected and tabulated, serving as a standard reference, from which the layer number of a given nanosheet can be readily and reliably determined without using complex calculation nor expensive instrument. Our general optical identification method will facilitate the thickness-dependent study of various 2D nanomaterials, and expedite their research toward practical applications.
description: 49 pages, 20 figures ACS Nano, 2013
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: Mathematici. (1r) Mathematici in Ordine Alphabeti. (70v) Anonymi. (74r) Mathematici in Ordine serierum; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
Jet dynamics. Recollimation shocks and helical patterns
Creators: name: Perucho, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The dynamics and stability of extragalactic jets may be strongly influenced by small (and probable) differences in pressure between the jet and the ambient and within the jet itself. The former give rise to expansion and recollimation of the jet. This occurs in the form of conical shocks, or Mach disks, if the pressure difference is large enough. Pressure asymmetries within the jet may trigger the development of helical patterns via coupling to kink current-driven instability, or to helical Kelvin-Helmholtz instability, depending on the physical conditions in the jet. I summarize here the evidence collected during the last years on the presence of recollimation shocks and waves in jets. In the jet of CTA 102 evidence has been found for (traveling)shock-(standing)shock interaction in the core-region (0.1 mas from the core), using information from the light-curve of the source combined with VLBI data. The conclusions derived have been confirmed by numerical simulations combined with emission calculations that have allowed to study the spectral evolution of the perturbed jet. Helical structures can also be identified in radio-jets. The ridge-line of emission of the jet of S5~0836+710 has been identified as a physical structure corresponding to a wave developing in the jet flow. I review here the evidence that has allowed to reach this conclusion, along with an associated caveat. Current data do not allow to distinguish between magnetic or hydrodynamical instabilities. I finally discuss the importance of these linear and non-linear waves for jet evolution.
description: 11 pages. Proceedings of the conference: The innermost regions of relativistic jets and their magnetic fields. Corrected typos and added references
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: Juristae. (1r) Juristae in Ordine Alphabeti. (57r) Anonymi. (69r) Juristae in Ordine serierum; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
Searching for young runaways across the sky
Creators: name: Kounkel, Marina
name: McBride, Aidan
name: Stassun, Keivan G.
name: Leigh, Nathan
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 present a catalog of 3354 candidate young stars within 500 pc that appear to have been ejected from their parent associations with relative speeds of >5 km/s. These candidates have been homogeneously selected through performing a 2d spherical traceback of previously identified pre-main sequence candidates to various star forming regions, ensuring that the traceback age as well as the estimated age of a star is consistent with the age of the population, and excluding contaminants from the nearby moving groups that follow the dominant velocity currents in the field. Among the identified candidates we identify a number of pairs that appear to have interacted in the process of the ejection, these pairs have similar traceback time, and their trajectory appears to be diametrically opposite from each other, or they have formed a wide binary in the process. As the selection of these candidates is performed solely in 2d, spectral follow-up is necessary for their eventual confirmation. Unfortunately, recently released Gaia DR3 radial velocities appear to be unsuitable for characterizing the kinematics of low mass stars with ages <100 Myr, as the accretion, activity, and a variety of other spectral features that make them distinct from the more evolved stars do not appear to have been accurately accounted for in the data, resulting in significant artificially inflated scatter in their RV distribution.
description: 12 pages, 11 figures, accepted to MNRAS
title: Fish aggregating devices (FADs) as conservation tools: understanding community dynamics at pelagic moored FADs
Creators: name: Schneider, Eric Vaughn Captain
Publisher: name: University of Glasgow
Year: 2023

description: The pelagic ocean covers the majority of the planet and is the largest ecosystem by volume. It is estimated to harbor considerable biodiversity, and a few select species support some of the largest fisheries in existence. The expanse of the open ocean provides important resources and services to humans, and also poses challenges to understanding the biology and ecology of its resident species. Focusing effort, both fishing and research, on hotspots or other aggregation sites increases the feasibility of interacting with these often patchily-distributed animals. Fish aggregating devices (FADs) have become a widespread fishing tool in many of the world’s oceans. Leveraging the natural behavior of many fish species to aggregate around floating or submerged structures, FADs are used to increase the capture efficiency in a range of marine fisheries and the scale of their use has raised concerns around potential effects these artificial structures have on the ecosystems in which they are used. Research efforts have focused on understanding these impacts by taking advantage of the fisheries-related opportunities and data made available by these fishing tools and the fleets that use them. However, this may potentially bias studies towards fishing hotspots and larger, commercially important species. Here, we discuss how subsurface FADs, purpose-built and discretely deployed, can act as useful research platforms to address important pelagic ecology questions and conservation topics. We describe the colonization of new FADs and the aggregation fluctuations through long-term video and visual surveys, provide evidence for invertebrate micronekton aggregation as a potential mechanism behind fish attraction to FADs, and detail a new acoustic telemetry array design that can provide previously unavailable position metrics of tagged fish in the open ocean, a notably challenging habitat to study. These new data and scientific tools will allow for the continued and enhanced study of the pelagic ecosystem and the diversity of species that inhabit it.
Plain language summary for the manuscript: An Insight into Patients’ Perspectives of Ulcerative Colitis Flares via Analysis of Online Public Forum Posts
Creators: name: Rubin, DT
name: Torres, J
name: Dotan, I
name: Xu, LT
name: Modesto, I
name: Woolcott, JC
name: Gardiner, S
name: Sands, BE
Publisher: name: Pfizer
Year: 2023
Subjects: classificationCode: 320209
subject: Gastroenterology and hepatology

description: This is a plain language summary (PLS) of an article published in a peer-reviewed scientific journal. This PLS is not peer-reviewed. The publisher of the original manuscript was not involved in the preparation of this PLS and has neither reviewed nor approved its content.
Spermophilus alashanicus Buchner 1888
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
Spermophilus
Spermophilus alashanicus

description: Spermophilus alashanicus Buchner, 1888. Wiss. Res. Przewalski Cent. Asien Zool. Th. I: Saugeth., p. 11. TYPE LOCALITY: N. China, S. Alashan Desert. DISTRIBUTION: S.C. Mongolia; Alashan and E. Nan Shan (N. China). COMMENT: Subgenus Spermophilus; see Gromov et al., 1965:208. Placed by Corbet, 1978, in dauricus; Orlov and Davaa, 1975, pp. 8-9, in [Systematics and cytogenetics of mammals], Orlov, ed., "Nauka," Moscow, provided evidence of specific distinctness.
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 366, DOI: 10.5281/zenodo.7353023
description: {"references": ["Gromov, I. M., D. I. Bibikov, N. I. Kalabukhov, and M. N. N. Meier. 1965. Fauna SSSR, Mlekopitayushchie, tom. 3, vyp. 2 [Fauna of the U. S. S. R. Mammals. vol. 3, No. 2]. Nazemnye belich'e [Ground Squirrels]. Nauka, Moscow-Leningrad, 467 pp. (in Russian).", "Orlov, V. N., and N. Davaa. 1975. O systematicheskom polozhenii Alashanskovo suslika Citellus alashanicus Buch. (Sciuridae, Rodentia) [On the systematic position of the Alashan ground squirrel ...]. Pp. 8 - 9, in Sistematika i tsitogenetica mlekopitayushchikh [Systematics and cytogenetics of mammals] (V. N. Orlov, ed.). Nauka, Moscow, 60 pp. (in Russian)."]}
Recent results from the ANTARES neutrino telescope
Creators: name: Van Elewyck, V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The ANTARES neutrino telescope is currently the largest operating water Cherenkov detector and the largest neutrino detector in the Northern Hemisphere. Its main scientific target is the detection of high-energy (TeV and beyond) neutrinos from cosmic accelerators, as predicted by hadronic interaction models, and the measurement of the diffuse neutrino flux. Its location allows for surveying a large part of the Galactic Plane, including the Galactic Centre. In addition to the standalone searches for point-like and diffuse high-energy neutrino signals, ANTARES has developed a range of multi-messenger strategies to exploit the close connection between neutrinos and other cosmic messengers such as gamma-rays, charged cosmic rays and gravitational waves. This contribution provides an overview of the recently conducted analyses, including a search for neutrinos from the Fermi bubbles region, searches for optical counterparts with the TAToO program, and searches for neutrinos in correlation with gamma-ray bursts, blazars, and microquasars. Further topics of investigation, covering e.g. the search for neutrinos from dark matter annihilation, searches for exotic particles and the measurement of neutrino oscillations, are also reviewed.
description: 8 pages, 9 figures. Prepared for the Proceedings of RICAP-13 Roma International Conference on Astroparticle Physics (Rome, 22-24 May 2013); to appear in Nucl. Instr. Meth. A Procs. Suppl
Drazin spectra of Banach space operators and Banach algebra elements
Creators: name: Boasso, Enrico
Publisher: name: arXiv
Year: 2013
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: Primary 47A10, Secondary 46H05, 47A05

description: Given a Banach Algebra $A$ and $a\in A$, several relations among the Drazin spectrum of $a$ and the Drazin spectra of the multiplication operators $L_a$ and $R_a$ will be stated. The Banach space operator case will be also examined. Furthermore, a characterization of the Drazin spectrum will be considered.
description: 16 pages; original research article
The Stability of Prendergast Magnetic Fields
Creators: name: Kaufman, Emma
name: Lecoanet, Daniel
name: Anders, Evan H.
name: Brown, Benjamin P.
name: Vasil, Geoffrey M.
name: Oishi, Jeffrey S.
name: Burns, Keaton J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Convection in massive main sequence stars generates large scale magnetic fields in their cores which persists as they evolve up the red giant branch. The remnants of these fields may take the form of the Prendergast magnetic field, a combination of poloidal and toroidal field components which are expected to stabilize each other. Previous analytic and numerical calculations did not find any evidence for instability of the Prendergast field over short timescales. In this paper, we present numerical simulations which show a long timescale, linear instability of this magnetic field. We find the instability to be robust to changes in boundary conditions and it is not stabilized by strong stable stratification. The instability is a resistive instability, and the growth rate has a power-law dependence on the resistivity, in which the growth rate decreases as the resistivity decreases. We estimate the growth rate of the instability in stars by extrapolating this power-law to stellar values of the resistivity. The instability is sufficiently rapid to destabilize the magnetic field on timescales shorter than the stellar evolution timescale, indicating that the Prendergast field is not a good model to use in studies of magnetic fields in stars.
description: 9 pages, 8 figures
SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
Creators: name: Xi, Gaobo
name: Wang, Xiaofeng
name: Li, Wenxiong
name: Mo, Jun
name: Zhang, Jujia
name: Liu, Jialian
name: Chen, Zhihao
name: Filippenko, Alexei V.
name: Zheng, Weikang
name: Brink, Thomas G.
name: Zhang, Xinghan
name: Sai, Hanna
name: Ehgamberdiev, Shuhrat A.
name: Mirzaqulov, Davron
name: Zhang, Jicheng
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present extensive optical photometric and spectroscopic observations for the nearby Type Ia supernova (SN Ia) 2019ein, spanning the phases from $\sim 3$ days to $\sim 330$ days after the explosion. This SN Ia is characterized by extremely fast expansion at early times, with initial velocities of Si II and Ca II being above ~ 25,000--30,000 km/s. After experiencing an unusually rapid velocity decay, the ejecta velocity dropped to ~ 13,000 km/s around maximum light. Photometrically, SN 2019ein has a moderate post-peak decline rate ($Δm_{15}(B) = 1.35 \pm 0.01$ mag), while being fainter than normal SNe Ia by about 40% (with $M^{\rm max}_{B} \approx -18.71 \pm 0.15$ mag). The nickel mass synthesized in the explosion is estimated to be 0.27--0.31 $M_{\odot}$ from the bolometric light curve. Given such a low nickel mass and a relatively high photospheric velocity, we propose that SN 2019ein likely had a sub-Chandrasekhar-mass white dwarf (WD) progenitor, $M_{\rm WD} \lesssim 1.22 M_{\odot}$. In this case, the explosion could have been triggered by a double-detonation mechanism, for which 1- and 2-dimensional models with WD mass $M_{\rm WD} \approx 1 M_\odot$ and a helium shell of 0.01 $M_{\odot}$ can reasonably produce the observed bolometric light curve and spectra. The predicted asymmetry as a result of double detonation is also favored by the redshifted Fe II and Ni II lines observed in the nebular-phase spectrum. Possible diversity in origin of high velocity SNe Ia is also discussed.
description: 34 pages, 16 figures, accepted for publication in MNRAS
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: Concilia et Canonistae. (1r) Concilia et Canonistae secundum Ordinem Alphabeti. (43r) Concilia et Canonistae in Ordine serierum; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
Supp data 1: U–Pb ages from felsic rocks of the External Ligurian sedimentary mélange (Northern Apennine, Italy): tracing the pre-Jurassic history of the hyperextended Adria continental margin
Creators: name: Di Rosa, Maria
name: Farina, Federico
name: Marroni, Michele
name: Jeon, Heejin
name: Pandolfi, Luca
Publisher: name: Geological Society of London
Year: 2023
Subjects: classificationCode: 3705
subject: Geology
subject: FOS: Earth and related environmental sciences

description: Supplementary dataset: related to the U–Pb and δ18O analysis.
CoVPN COVID-19 Vaccine Efficacy Trial Immune Correlates SAP
Creators: name: CoVPN Biostatistics Team
name: Gilbert, Peter
name: Youyi Fong
name: Benkeser, David
name: Andriesen, Jessica
name: Bhavesh Borate
name: Carone, Marco
name: Carpp, Lindsay N.
name: Diaz, Ivan
name: Fay, Mike
name: Follmann, Dean
name: Hejazi, Nima
name: Huang, Ying
name: Yunda Huang
name: Hyrien, Ollivier
name: Janes, Holly
name: Juraska, Michal
name: Li, Kendrick
name: Luedtke, Alex
name: Nason, Martha
name: Randhawa, April
name: Laan, Lars Van Der
name: Williamson, Brian
name: Wenbo Zhang
Publisher: name: figshare
Year: 2020
Subjects: subject: 10402 Biostatistics
subject: FOS: Mathematics
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Medicine
subject: 110399 Clinical Sciences not elsewhere classified
subject: Diseases

description: This Statistical Analysis Plan (SAP) describes the statistical analysis of antibody markers measured at a key time point post last vaccination as correlates of risk and as various types of correlates of protection against primary and secondary endpoints in COVID-19 Prevention Network (CoVPN) COVID-19 vaccine efficacy (VE) trials.
$ϕN$ photoproduction coupled with the $KΛ^*$ channel
Creators: name: Kim, Hyun-Chul
name: Ryu, Hui-Young
name: Titov, Alexander
name: Hosaka, Atsushi
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present in this talk a recent investigation on $ϕ$ photoproduction, emphasizing the rescattering effects of the $KΛ^*$ channel near the threshold region. We discuss the results of the differential cross section and the angular distributions.
description: 4 pages, 3 figures. A talk presented at The 22nd European Conference on Few-Body Problems in Physics (EFB22) held in Krakow, Poland, 9 - 13 September 2013
Common Envelope Shaping of Planetary Nebulae. IV. From Proto-planetary to Planetary Nebula
Creators: name: García-Segura, Guillermo
name: Taam, Ronald E.
name: Ricker, Paul M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present 2D hydrodynamical simulations of the transition of a proto-planetary nebula to a planetary nebula for central stars in binary systems that have undergone a common envelope event. After 1,000 yr of magnetically driven dynamics (proto-planetary nebula phase), a line-driven stellar wind is introduced into the computational domain and the expansion of the nebula is simulated for another 10,000 yr, including the effects of stellar photoionization. In this study we consider central stars with main sequence (final) masses of 1 (0.569) and 2.5 (0.677) \Mo, together with a 0.6 \Mo ma in sequence companion. Extremely bipolar, narrow-waisted proto-planetary nebulae result in bipolar planetary nebulae, while the rest of the shapes mainly evolve into elliptical planetary nebulae. The initial magnetic field's effects on the collimated structures, such as jets, tend to disappear in most of the cases, leaving behind the remnants of those features in only a few cases. Equatorial zones fragmented mainly by photoionization ( 1 \Mo progenitors), result in ``necklace'' structures made of cometary clumps aligned with the radiation field. On the other hand, fragmentation by photoionization and shocked wind ( 2.5 \Mo progenitors) give rise to the formation of multiple clumps in the latitudinal direction, which remain within the lobes, close to the center, which are immersed and surrounded by hot shocked gas, not necessarily aligned with the radiation field. These results reveal that the fragmentation process has a dependence on the stellar mass progenitor. This fragmentation is made possible by the distribution of gas in the previous post-common envelope proto-planetary nebula as sculpted by the action of the jets.
description: 12 pages, 7 figures, accepted by MNRAS
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: Polemici. (2r) Polemici in Ordine Alphabeti. (249v) Anonymi; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
Topological Flat Band Models and Fractional Chern Insulators
Creators: name: Bergholtz, Emil J.
name: Liu, Zhao
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Topological insulators and their intriguing edge states can be understood in a single-particle picture and can as such be exhaustively classified. Interactions significantly complicate this picture and can lead to entirely new insulating phases, with an altogether much richer and less explored phenomenology. Most saliently, lattice generalizations of fractional quantum Hall states, dubbed fractional Chern insulators, have recently been predicted to be stabilized by interactions within nearly dispersionless bands with non-zero Chern number, $C$. Contrary to their continuum analogues, these states do not require an external magnetic field and may potentially persist even at room temperature, which make these systems very attractive for possible applications such as topological quantum computation. This review recapitulates the basics of tight-binding models hosting nearly flat bands with non-trivial topology, $C\neq 0$, and summarizes the present understanding of interactions and strongly correlated phases within these bands. Emphasis is made on microscopic models, highlighting the analogy with continuum Landau level physics, as well as qualitatively new, lattice specific, aspects including Berry curvature fluctuations, competing instabilities as well as novel collective states of matter emerging in bands with $|C|>1$. Possible experimental realizations, including oxide interfaces and cold atom implementations as well as generalizations to flat bands characterized by other topological invariants are also discussed.
description: Invited review. 46 pages, many illustrations and references. V2: final version with minor improvements and added references
Spermophilus annulatus Audubon and Bachman 1842
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
Spermophilus
Spermophilus annulatus

description: Spermophilus annulatus Audubon and Bachman, 1842. J. Acad. Nat. Sci. Phila., 8:319. TYPE LOCALITY: Mexico, Colima, Manzanillo. DISTRIBUTION: Nayarit to N. Guerrero (Mexico). COMMENT: Subgenus Otospermophilus; see Hall, 1981:403. Gromov et al., 1965:145, considered Otospermophilus a distinct genus. Type locality designated by Howell, 1938, N. Am. Fauna, 56: 163. ISIS NUMBER: 5301410002032002001.
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 367, 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.", "Gromov, I. M., D. I. Bibikov, N. I. Kalabukhov, and M. N. N. Meier. 1965. Fauna SSSR, Mlekopitayushchie, tom. 3, vyp. 2 [Fauna of the U. S. S. R. Mammals. vol. 3, No. 2]. Nazemnye belich'e [Ground Squirrels]. Nauka, Moscow-Leningrad, 467 pp. (in Russian).", "Howell, A. H. 1938. Revision of the North American ground squirrels, with a classification of the North American Sciuridae. North American Fauna, 56: 1 - 256."]}
Doping-dependent band structure of LaAlO$_{3}$/SrTiO$_{3}$ interfaces by soft x-ray polarization-controlled resonant angle-resolved photoemission
Creators: name: Cancellieri, Claudia
name: Reinle-Schmitt, Mathilde L.
name: Kobayashi, Masaki
name: Strocov, Vladimir N.
name: Fontaine, Denis
name: Ghosez, Philippe
name: Filippetti, Alessio
name: Delugas, Pietro
name: Fiorentini, Vincenzo
name: Willmott, Philip R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Polarization-controlled synchrotron radiation was used to map the electronic structure of buried conducting interfaces of LaAlO$_3$/SrTiO$_3$ in a resonant angle-resolved photoemission experiment. A strong dependence on the light polarization of the Fermi surface and band dispersions is demonstrated, highlighting the distinct Ti 3d orbitals involved in 2D conduction. Samples with different 2D doping levels were prepared and measured by photoemission, revealing different band occupancies and Fermi surface shapes. A direct comparison between the photoemission measurements and advanced first-principle calculations carried out for different 3d-band fillings is presented in conjunction with the 2D carrier concentration obtained from transport measurements.
description: Main Text: 12 pages, 4 figures
[Catalogi bibliothecae Jesuitarum confecti circa 1769]: Patres Graeci et Latini in Ordine serierum; [um 1769]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [um 1769]
PROJETO PARA INTERLIGAÇÃO DE REDES CASE DA EMPRESA 2SHOW.IE
Creators: name: Thomas, Guilherme
Publisher: name: figshare
Year: 2023
Subjects: classificationCode: 460908
subject: Information systems organisation and management

description: Solution for the case presented to us of the fictitious company 2SHOW.IE. The company in question has the need to expand its Headquarters and Branch network, so, with the theoretical knowledge acquired in classes, in its written materials, in our indications of extracurricular materials during our academic classes of ‘Fundamentals of Data and Communications Networks'', 'Mathematics for Computing', 'Scientific Methodology', 'Ethics and Professional Legislation' and 'Laboratory of Architecture and Computer Networks' in addition to the student's research capability, we have here presented the solution of the case using VPN solutions, network addressing tuning solutions, confined tuning solutions, and more to meet the 2SHOW.IE company's growth and ensure its scalability.
A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - V. Neutral and Ionised Phase Metallicities
Creators: name: Peroux, Celine
name: Kulkarni, Varsha P.
name: York, Donald G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The gas-phase and stellar metallicities have proven to be important parameters to constrain the star formation history of galaxies. However, HII regions associated with recent star-formation may not have abundances typical for the galaxy as a whole and it is believed that the bulk of the metals may be contained in the neutral gas. It is therefore important to directly probe the metal abundances in the neutral gas, which can be done by using absorption lines imprinted on a background quasar. Recently, we have presented studies of the stellar content of a small sample of such quasar absorbers with HI column densities measured to be in the sub-Damped Lyman-alpha to Damped Lyman-alpha range. Here, we present observations covering 300 nm to 2.5 microns of emission line spectra of three of these absorbing-galaxies using the long-slit spectrograph X-Shooter on the VLT. This allows us to compare the neutral and ionised phase metallicities in the same objects and relates these measures to possible signature of low-metallicity gas accretion or outflows of gas enriched by star formation. Our results suggest that the abundances derived in absorption along the line-of-sight to background quasars are reliable measures of the overall galaxy metallicities. In addition to a comparison of abundances in different phases of the gas, a potential observational consequence of differences in fueling mechanisms for disc galaxies is the internal distribution of their chemical abundances. We present some evidence for small negative metallicity gradients in the three systems. The flat slopes are in line with the differences observed between the two phases of the gas. These results suggest that a comparison of the HI and HII metallicities is a robust indicator of abundance gradients in high-redshift galaxies and do not favour the presence of infall of fresh gas in these objects.
description: 17 pages, 10 figures, accepted for publication in MNRAS
[Catalogi bibliothecae Jesuitarum Ingolstadiensis.] Secundum series: Miscellanei; [nach 1760]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [nach 1760]
Hall Effect in Neutron Star Crusts: Evolution, Endpoint and Dependence on Initial Conditions
Creators: name: Gourgouliatos, K. N.
name: Cumming, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present new simulations of the evolution of axially symmetric magnetic fields in neutron star crusts under the influence of the Hall effect and subdominant Ohmic dissipation. In the Hall effect, differential rotation of the electron fluid generates toroidal field by winding of the poloidal field. For this reason, we focus on the influence of the initial choice of the electron angular velocity profile on the subsequent and long term magnetic evolution. Whereas previous simulations have generally chosen angular velocities increasing outwards, corresponding to the lowest order Ohmic mode in the crust, a more realistic choice is an angular velocity decreasing outwards, corresponding to the MHD equilibrium field that is likely present at the time of crust formation. We find that the evolution passes through three basic phases. The early evolution is a response to the initial conditions. During the second phase the field consists of poloidal and toroidal components which eventually relax to an isorotation state in which the angular velocity of the electrons becomes constant along poloidal magnetic field lines, causing Hall evolution to saturate. In the third phase the field dissipates slowly while maintaining isorotation. We discuss the implications for the long term field structure and observable properties of isolated neutron stars.
description: 13 pages, 8 figures, Accepted by MNRAS
Spermophilus armatus Kennicott 1863
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
Spermophilus
Spermophilus armatus

description: Spermophilus armatus Kennicott, 1863. Proc. Acad. Nat. Sci. Phila., 15: 158. TYPE LOCALITY: U.S.A., Wyoming, Uinta Co., foothills of Uinta Mtns., near Fort Bridger. DISTRIBUTION: S.C. Utah to S. Montana, S.E. Idaho to W. Wyoming (U.S.A.). COMMENT: Subgenus Spermophilus; see Hall, 1981:386. ISIS NUMBER: 5301410002032003001.
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 367, 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."]}
[Catalogi bibliothecae Jesuitarum Ingolstadiensis.] Secundum series: Poetae; [nach 1760]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [nach 1760]
Coloring 2-intersecting hypergraphs
Creators: name: Colucci, Lucas
name: Gyárfás, András
Publisher: name: arXiv
Year: 2013
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C15, 05C65

description: A hypergraph is 2-intersecting if any two edges intersect in at least two vertices. Blais, Weinstein and Yoshida asked (as a first step to a more general problem) whether every 2-intersecting hypergraph has a vertex coloring with a constant number of colors so that each hyperedge e has at least min{|e|,3} colors. We show that there is such a coloring with at most 5 colors (which is best possible).
Influence of the enclosed fluid on the flow over a microstructured surface in the Cassie state
Creators: name: Schönecker, Clarissa
name: Baier, Tobias
name: Hardt, Steffen
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Analytical expressions for the flow field as well as for the effective slip length of a shear flow over a surface with periodic rectangular grooves are derived. The primary fluid is in the Cassie state with the grooves being filled with a secondary immiscible fluid. The coupling of both fluids is reflected in a locally varying slip distribution along the fluid-fluid interface, which models the effect of the secondary fluid on the outer flow. The obtained closed-form analytical expressions for the flow field and effective slip length of the primary fluid explicitly contain the influence of the viscosities of the two fluids as well as the magnitude of the local slip, which is a function of the surface geometry. They agree well with results from numerical computations of the full geometry. The analytical expressions allow investigating the influence of the viscous stresses inside the secondary fluid for arbitrary geometries of the rectangular grooves. For classic superhydrophobic surfaces, the deviations in the effective slip length compared to the case of inviscid gas flow are are pointed out. Another important finding with respect to an accurate modeling of flow over microstructured surfaces is that the local slip length of a grooved surface is anisotropic.
description: submitted to the Journal of Fluid Mechanics
[Catalogi bibliothecae Jesuitarum Ingolstadiensis.] Secundum series: Mathematici; [nach 1760]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [nach 1760]
Spermophilus atricapillus W. E. Bryant 1889
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
Spermophilus
Spermophilus atricapillus

description: Spermophilus atricapillus W. E. Bryant, 1889. Proc. Calif. Acad. Sci., ser. 2, 2: 26. TYPE LOCALITY: Mexico, Baja California Sur, Comondu. DISTRIBUTION: Baja California (Mexico). COMMENT: Subgenus Otospermophilus; see Hall, 1981:402. Gromov et al., 1965:145, considered Otospermophilus a distinct genus. ISIS NUMBER: 5301410002032004001.
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 367, 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.", "Gromov, I. M., D. I. Bibikov, N. I. Kalabukhov, and M. N. N. Meier. 1965. Fauna SSSR, Mlekopitayushchie, tom. 3, vyp. 2 [Fauna of the U. S. S. R. Mammals. vol. 3, No. 2]. Nazemnye belich'e [Ground Squirrels]. Nauka, Moscow-Leningrad, 467 pp. (in Russian)."]}
Ram Pressure Stripping and ISM disc Truncation : Prediction vs. Observation
Creators: name: Lee, Seona
name: Sheen, Yun-Kyeong
name: Yoon, Hyein
name: Jaffé, Yara
name: Chung, Aeree
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Ram pressure stripping (RPS) is known to be a key environmental effect that can remove interstellar gas from galaxies in a cluster. The RPS process is commonly described as a competition between the ram pressure by the intracluster medium (ICM) and the anchoring pressure on the interstellar medium (ISM) by the gravitational potential of a galaxy. However, the actual gas stripping process can be more complicated due to the complexity of gas physics such as compression and geometrical self-shielding as well as cooling and heating. In order to verify how well the observed signatures of the RPS process can be understood as simple momentum transfer, we compare the stripping radii of Virgo cluster galaxies in different stages of RPS measured from the HI observation with the predicted gas truncation radii for the given conditions. For the sample undergoing active RPS, we generally find good agreements between predictions and observations within a measurement uncertainty. On the other hand, galaxies likely in the early or later RPS stage and/or the ones with signs of environmental impacts other than RPS such as tidal interaction or starvation, show some discrepancies. Our results imply that the conventional RPS relation works reasonably well in a broad sense when RPS is the most dominant process and the galaxy is located where the surrounding environment can be well defined. Otherwise, more careful inspections on the second mechanism and local environment are required to assess the impact of RPS on the target.
description: 13 pages, 11 figures, accepted for publication in MNRAS
Novel Scintillating Materials Based on Phenyl-Polysiloxane for Neutron Detection and Monitoring
Creators: name: Degerlier, M.
name: Carturan, S.
name: Gramegna, F.
name: Marchi, T.
name: Palma, M. Dalla
name: Cinausero, M.
name: Maggioni, G.
name: Quaranta, A.
name: Collazuol, G.
name: Bermudez, J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Neutron detectors are extensively used at many nuclear research facilities across Europe. Their application range covers many topics in basic and applied nuclear research: in nuclear structure and reaction dynamics (reaction reconstruction and decay studies); in nuclear astrophysics (neutron emission probabilities); in nuclear technology (nuclear data measurements and in-core/off-core monitors); in nuclear medicine (radiation monitors, dosimeters); in materials science (neutron imaging techniques); in homeland security applications (fissile materials investigation and cargo inspection). Liquid scintillators, widely used at present, have however some drawbacks given by toxicity, flammability, volatility and sensitivity to oxygen that limit their duration and quality. Even plastic scintillators are not satisfactory because they have low radiation hardness and low thermal stability. Moreover organic solvents may affect their optical properties due to crazing. In order to overcome these problems, phenyl-polysiloxane based scintillators have been recently developed at Legnaro National Laboratory. This new solution showed very good chemical and thermal stability and high radiation hardness. The results on the different samples performance will be presented, paying special attention to a characterization comparison between synthesized phenyl containing polysiloxane resins where a Pt catalyst has been used and a scintillating material obtained by condensation reaction, where tin based compounds are used as catalysts. Different structural arrangements as a result of different substituents on the main chain have been investigated by High Resolution X-Ray Diffraction, while the effect of improved optical transmittance on the scintillation yield has been elucidated by a combination of excitation/fluorescence measurements and scintillation yield under exposure to alpha and γ-rays.
description: InterM 2013 - International Multidisciplinary Microscopy Congress
[Catalogi bibliothecae Jesuitarum Ingolstadiensis.] Secundum series: Medici; [nach 1760]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [nach 1760]
[Catalogi bibliothecae Jesuitarum Ingolstadiensis.] Secundum series: Canonistae; [nach 1760]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Ingolstadt]. - Entstehungszeit: [nach 1760]
Parametric Studies on the Fatigue Life Improvement of Passenger Rail Vehicle Axlebox House
Creators: name: Behaylu, Alem
Publisher: name: Zenodo
Year: 2015

description: Failure of passenger rail axlebox house is mainly due to fatigue caused by repeated cyclic loading which cause catastrophic mechanical failure on axleboxes house and bearing assemblies. The general objective of this thesis is to improve the fatigue life of passenger rail vehicle axlebox house by studding influential geometry and fatigue strength factor parameters on the fatigue life of the axlebox house. Primary data such as bogie type and application, axle load, axle journal size, bearing type and size are selected and analysed for modelling the geometry. In addition to primary data, secondary data such as material data, boundary condition, loading data are required for the input of ANSYSI software analysis. Four geometry types are modelled with SolidWorks based on the axlebox house design principles then all models are analysed with FEM ANSYS Workbench 14 fatigue tools under the same non-proportional loading, equivalent dimension and the same material property to investigate which model has a longer fatigue life