cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Revisiting the Rigidly Rotating Magnetosphere model for sigma Ori E. I. Observations and Data Analysis
Creators: name: Oksala, M. E.
name: Wade, G. A.
name: Townsend, R. H. D.
name: Owocki, S. P.
name: Kochukhov, O.
name: Neiner, C.
name: Alecian, E.
name: Grunhut, J.
name: Collaboration, the MiMeS
Publisher: name: arXiv
Year: 2011
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have obtained 18 new high-resolution spectropolarimetric observations of the B2Vp star sigma Ori E with both the Narval and ESPaDOnS spectropolarimeters. The aim of these observations is to test, with modern data, the assumptions of the Rigidly Rotating Magnetosphere (RRM) model of Townsend & Owocki (2005), applied to the specific case of sigma Ori E by Townsend et al. (2005). This model includes a substantially offset dipole magnetic field configuration, and approximately reproduces previous observational variations in longitudinal field strength, photometric brightness, and Halpha emission. We analyze new spectroscopy, including H I, He I, C II, Si III and Fe III lines, confirming the diversity of variability in photospheric lines, as well as the double S-wave variation of circumstellar hydrogen. Using the multiline analysis method of Least-Squares Deconvolution (LSD), new, more precise longitudinal magnetic field measurements reveal a substantial variance between the shapes of the observed and RRM model time-varying field. The phase resolved Stokes V profiles of He I 5876 A and 6678 A lines are fit poorly by synthetic profiles computed from the magnetic topology assumed by Townsend et al. (2005). These results challenge the offset dipole field configuration assumed in the application of the RRM model to sigma Ori E, and indicate that future models of its magnetic field should also include complex, higher-order components.
description: 13 pages, 8 figures. Accepted for publication in MNRAS
Sirovena
Creators: name: Li, Zi
name: Xiao, Hui
name: Huang, Da-Wei
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Sirovena

description: Key to females of Sirovena
 1 Coxae white or light yellow (Fig. 1); clypeus testaceous, sides distinctly delimited by dorsally convergent grooves (Fig. 2); head wider than high (71:69) (Fig. 2); upper mesepimeron mostly smooth (Fig. 4)............... Sirovena stigma Bouček
 - Fore and mid coxae dark brown, hind coxae mostly white (Fig. 5); clypeus black, sides indistinctly delimited (Fig. 7); head higher than wide (73:70) (Fig. 7); upper mesepimeron with imbricate reticulation (Fig. 10).......................................................................................... Sirovena costallifera Li, Xiao & Huang sp. nov.
description: Published as part of Li, Zi, Xiao, Hui & Huang, Da-Wei, 2013, Sirovena Bouček (Pteromalidae: Pireninae), a new member of the fig wasp community associated with Ficus microcarpa (Moraceae), pp. 581-588 in Zootaxa 3619 (5) on page 582, DOI: 10.11646/zootaxa.3619.5.7, http://zenodo.org/record/222964
DIONYSIUS VON HALIKARNASS, Römische Frühgeschichte, eingeleitet, übersetzt und kommentiert von Nicolas Wiater
Creators: name: Wissemann, Michael
Publisher: name: Forum Classicum
Year: 2019

description: Rezension zu: DIONYSIUS VON HALIKARNASS, Römische Frühgeschichte, eingeleitet, übersetzt und kommentiert von Nicolas Wiater, Bd. 1, Bücher 1-3 (Bibliothek der griechischen Literatur Bd. 75), Stuttgart (Anton Hiersemann) 2014, VIII und 366 S., ISBN 978-3-7772-1404-7, EUR 194,-, Bd. 2, Bücher 3-6, (Bibliothek der griechischen Literatur Bd. 85) Stuttgart (Anton Hiersemann) 2018, VI und 507 S., ISBN 978-3-7772-1803-8
description: Forum Classicum, Nr. 3 (2019): Forum Classicum
Two kinds of rogue waves of the general nonlinear Schrödinger equation with derivative
Creators: name: Xu, Shuwei
name: He, Jingsong
name: Wang, Lihong
Publisher: name: arXiv
Year: 2012
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences
subject: 35C08, 37K10, 37K40

description: In this letter,the designable integrability(DI) of the variable coefficient derivative nonlinear Schrödinger equation (VCDNLSE) is shown by construction of an explicit transformation which maps VCDNLSE to the usual derivative nonlinear Schrödinger equation(DNLSE). One novel feature of VCDNLSE with DI is that its coefficients can be designed artificially and analytically by using transformation. What is more, from the rogue wave and rational traveling solution of the DNLSE, we get two kinds of rogue waves of the VCDNLSE by this transformation. One kind of rogue wave has vanishing boundary condition, and the other non-vanishing boundary condition. The DI of the VCDNLSE also provides a possible way to control the profile of the rogue wave in physical experiments.
description: 8 pages, 5 figures
关于提高德国高校中级汉语口语课堂效率的思考
Creators: name: CHEN, Xixi
Publisher: name: CHUN - Chinesisch-Unterricht
Year: 2022

description: 本文分析了德国校中级汉语口语课堂的教学对象和教学环境，从中级阶段口语教学的重点、教学对象的兴趣和需求、课堂活动的组织、语用环境的创造等几个方面探讨了如何在宝贵有限的时间内提高课堂教学效率的问题。
description: CHUN - Chinesisch-Unterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
Thin Film Growth and Device Fabrication of Iron-Based Superconductors
Creators: name: Hiramatsu, Hidenori
name: Katase, Takayoshi
name: Kamiya, Toshio
name: Hosono, Hideo
Publisher: name: arXiv
Year: 2011
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Iron-based superconductors have received much attention as a new family of high-temperature superconductors owing to their unique properties and distinct differences from cuprates and conventional superconductors. This paper reviews progress in thin film research on iron-based superconductors since their discovery for each of five material systems with an emphasis on growth, physical properties, device fabrication, and relevant bulk material properties.
description: To appear in J. Phys. Soc. Jpn
Impact of SARS-CoV-2 Pandemic on Diagnosis of Prostate Cancer
Creators: name: Oppolzer, Immanuel A.
name: Schnabel, Marco J.
name: Hammer, Selma
name: Zilles, Hannah
name: Haas, Maximilian
name: Goßler, Christopher
name: Müller, Maximilian R.
name: Burger, Maximilian
name: Gierth, Michael
Publisher: name: Universität Regensburg
Year: 2024
Subjects: subject: Prostate cancer, Delay in diagnosis, Severe acute respiratory syndrome coronavirus 2, COVID-19, Clinical data
subject: 610 Medizin

description: Introduction: The aim of this study was to prove if the severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) pandemic resulted in a delay in diagnosis and treatment of prostate cancer (PC). Methods: A monocentric, retrospective analysis was conducted at a university cancer center. Included were all patients with untreated PC diagnosed between January 2019 and December 2021. The observation covered 22 months of the SARS-CoV-2 pandemic and 14 months preceding it. Results: Nine hundred sixty-nine men prior (T0) and 1,343 during the pandemic (T1) were included. Mean age was 68.0 (SD 8.2). Median initial prostate-specific antigen was 8.1 ng/mL (T0) and 7.9 ng/mL (T1, p = 0.288). Time from biopsy to tumor board (T0: 1.3 months vs. T1: 0.9 months, p = 0.001), to staging (T0: 1.1 months vs. T1: 0.75 months, p = 0.707), and to therapy (T0: 3.0 months vs. T1: 2.0 months, p < 0.001) was shortened during the pandemic. Classified by d’Amico, a significant shift toward higher risk groups was seen (p = 0.024). Local staging showed an insignificant increase in locally advanced PCs. Metastatic diseases decreased from 10.3% to 8.9% (p = 0.433). Pathological staging showed pT3+ in 44.4% versus 44.7% (p = 0.565) and pN+ in 9.9% versus 9.6% (p = 0.899). Conclusion: Regarding the diagnosis and treatment of PC, we could not demonstrate any delays due to the SARS-CoV-2 pandemic.
Ergebnisse von Konversations- und Ausspracheunterricht an der Universität unter unterschiedlichen Lernbedingungen. Ein empirischer Vergleich
Creators: name: Brexendorff, Heidi
Publisher: name: CHUN - Chinesischunterricht
Year: 2022

description: 本研究项目之基本假设为学生中文口语能力随着上课时数增加而提升。因此，由四位老师针对不同学习背景学生组别的上课录像作出口语能力的评比。第一组是每周上二十个小时的假期强化班；第二组是每周上八个小时的汉语课；第三个是大学强化班，该班学生每周上十六个小时汉语课；第四个是每周上十二个小时韩语课的强化班。这些录像皆为初级阶段的前二或四个星期的汉语课所拍摄而成。老师评比的分析说明：上课时数的多寡对学生口语能力无直接影响，而其它因素，如语言实验室的教学、辅导课、考试以及学生素质等要素也起相当重要的作用。
description: CHUN - Chinesischunterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
J/psi production at sqrt(s)=1.96 and 7 TeV: Color-Singlet Model, NNLO* and polarisation
Creators: name: Lansberg, J. P.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study J/psi production in pp collisions at sqrt(s)=1.96 and 7 TeV using the Colour-Singlet Model (CSM), including next-to-leading order (NLO) corrections and dominant alphaS^5 contributions (NNLO*). We find that the CSM reproduces the existing data if the upper range of the NNLO* is near the actual --but presently unknown-- NNLO. The direct yield polarisation for the NLO and NNLO* is increasingly longitudinal in the helicity frame when P_T gets larger. Contrary to what is sometimes claimed in the literature, the prompt J/psi yield polarisation in the CSM is compatible with the experimental data from the CDF collaboration, when one combines the direct yield with a data-driven range for the polarisation of J/psi from chi(c).
description: Contributed to the 22nd International Conference On Ultra-Relativistic Nucleus-Nucleus Collisions (Quark Matter 2011), Annecy, France, May 23 - 28, 2011. 4 pages, 4 figures, uses iopams.sty, iopart12.clo, iopart.cls (included)
Was ist Chinesischkompetenz? Standardisierte Chinesischprüfungen und Untersuchungen zur Sprachstandmessung
Creators: name: Meyer, Florian
Publisher: name: CHUN - Chinesischunterricht
Year: 2022

description: 语言测试和语言能力分级的标准化是一个世界范围内的趋势。同时，关于标准和能力的定义讨论，对对汉语教学的影响越来越深入。单从目前每年参加汉语水平考试（HSK）的考生达到了大约16万人，即可见一斑。本文首先以“汉语水平考试研究”中的例句阐明了语言测试传统理论的质量标准。这些质量标准包括客观性、可靠性及效度，并通过公平性、真实性、实用性和标准化予以充。文章的第二部分展示了对汉语水平考试德国考生的调查研究的阶段性结果。调查只在发现学习时间的长短以及实际授课学时与汉语水平考试成绩之间的关系。调查研究的两个主要结果显示，德语为母语的HSK考神通过第一级（基础C）的考试，基本上需要大约500个学时。而要通过代表中国所有本科院校入学资格的第六级（中等C）的考试，甚至需要将近2000个学时。因此要让学生通过这些级别的考试，德国教师明显需要比国家汉办所给出的学时数（基础C：100学时，中等C：1500学时）更多的教学时间。
description: CHUN - Chinesischunterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
Chironomus Meigen 1803
Creators: name: Armitage, Brian J.
name: Andersen, Trond
name: Giłka, Wojciech
name: Castillo Sánchez, Kayla N.
name: Ríos González, Tomás A.
name: Aguirre, Yusseff P.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Chironomidae
Chironomus

description: Genus Chironomus Meigen, 1803
One of the most species-rich and common chironomid genera, with ~300 described species from all zoogeographical regions except Antarctica. The larvae graze on detritus or are filter-feeders, predominantly in soft sediments of standing water, rarely in flowing water (Epler et al. 2013).
description: Published as part of Armitage, Brian J., Andersen, Trond, Giłka, Wojciech, Castillo Sánchez, Kayla N., Ríos González, Tomás A. & Aguirre, Yusseff P., 2025, The Diptera of Panama. II. A first benchmark for the family Chironomidae, pp. 201-240 in Zootaxa 5613 (2) on page 208, DOI: 10.11646/zootaxa.5613.2.1, http://zenodo.org/record/15224174
德语区第十五届现代汉语教学讨论会“汉语—欧洲外语教学的挑战” , 2008年9月25至27日, 柏林自由大学
Creators: name: LI, Shengchao
Publisher: name: CHUN - Chinesisch-Unterricht
Year: 2022

description: CHUN - Chinesisch-Unterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
Single-ion Kondo Scaling of the Coherent Fermi Liquid Regime in Ce1-xLaxNi2Ge2
Creators: name: Pikul, Adam P.
name: Stockert, Ulrike
name: Steppke, Alexander
name: Cichorek, Tomasz
name: Hartmann, Stefanie
name: Caroca-Canales, Nubia
name: Oeschler, Niels
name: Brando, Manuel
name: Geibel, Christoph
name: Steglich, Frank
Publisher: name: arXiv
Year: 2012
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Thermodynamic and transport properties of the La-diluted Kondo lattice CeNi2Ge2 were studied in a wide temperature range. The Ce-rich alloys Ce1-xLaxNi2Ge2 were found to exhibit distinct features of the coherent heavy Fermi liquid. At intermediate compositions (0.7 <= x <= 0.9) non-Fermi liquid properties have been observed, followed by the local Fermi liquid behavior in the dilute limit. The 4f-electron contribution to the specific heat was found to follow the predictions of the Kondo impurity model both in the local as well as coherent regimes, with the characteristic Kondo temperature decreasing rapidly from about 30 K for the parent compound CeNi2Ge2 to about 1K in the most dilute samples. The specific heat does not show any evidence for the emergence of a new characteristic energy scale related to the formation of the coherent Kondo lattice.
description: to appear in Physical Review Letters
Bericht über die Sektion "Chinesisch an Sekundarschulen" auf der 15. Tagung zum modernen Chinesischunterricht
Creators: name: Neder, Christina
name: Prüch, Margarete
Publisher: name: CHUN - Chinesischunterricht
Year: 2022

description: CHUN - Chinesischunterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
title: "Quattro rilievi con strumenti di sacrificio", ambito romano, s.n. (ITA/EN)
title: Scheda catalogo digitale Borghese
titleType: AlternativeTitle
Creators: name: Ciccarello, Giulia
name: Galleria Borghese
Publisher: name: Galleria Borghese
Year: 2024

description: Pubblicazione delle schede delle opere conservate nel museo ed estratte dal catalogo digitale di Galleria Borghese, nelle due versioni esistenti online, in italiano e inglese.

Collegamento al catalogo digitale:

ITA: https://www.collezionegalleriaborghese.it/

EN: https://www.collezionegalleriaborghese.it/en
Microscopic approach to large-amplitude deformation dynamics with local QRPA inertial masses
Creators: name: Sato, Koichi
name: Hinohara, Nobuo
name: Nakatsukasa, Takashi
name: Matsuo, Masayuki
name: Matsuyanagi, Kenichi
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We have developed a new method for determining microscopically the fivedimensional quadrupole collective Hamiltonian, on the basis of the adiabatic self-consistent collective coordinate method. This method consists of the constrained Hartree-Fock-Bogoliubov (HFB) equation and the local QRPA (LQRPA) equations, which are an extension of the usual QRPA (quasiparticle random phase approximation) to non-HFB-equilibrium points, on top of the CHFB states. One of the advantages of our method is that the inertial functions calculated with this method contain the contributions of the time-odd components of the mean field, which are ignored in the widely-used cranking formula. We illustrate usefulness of our method by applying to oblate-prolate shape coexistence in 72Kr and shape phase transition in neutron-rich Cr isotopes around N=40.
description: 6pages, talk given at Rutherford Centennial Conference on Nuclear Physics, 8 - 12 August 2011, The University of Manchester
[CII] 158 micron line detection of the warm ionized medium in the Scutum--Crux spiral arm tangency
Creators: name: Velusamy, T.
name: Langer, W. D.
name: Pineda, J. L.
name: Goldsmith, P. F.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: HIFI GOT C+ Galactic plane [CII] spectral survey has detected strong emission at the spiral arm tangencies. We use the unique viewing geometry of the Scutum-Crux (S-C) tangency near i = 30degs to detect the warm ionized medium (WIM) component traced by [CII] and to study the effects of spiral density waves on Interstellar Medium (ISM) gas. We compare [CII] velocity features with ancillary HI, 12CO and 13CO data near tangent velocities at each longitude to separate the cold neutral medium and the warm neutral + ionized components in the S-C tangency, then we identify [CII] emission at the highest velocities without any contribution from 12CO clouds, as WIM. We present the GOT C+ results for the S-C tangency. We interpret the diffuse and extended excess [CII] emission at and above the tangent velocities as arising in the electron-dominated warm ionized gas in the WIM. We derive an electron density in the range of 0.2 - 0.9 cm^-3 at each longitude, a factor of several higher than the average value from Halpha and pulsar dispersion. We interpret the excess [CII] in S-C tangency as shock compression of the WIM induced by the spiral density waves.
description: 5 pages, 3 figures and 1 Table
15. Tagung zum modernen Chinesischunterricht, Freie Universität Berlin, 25.-27. September 2008
Creators: name: List, Johann-Mattis
name: Holtz, Tabea
Publisher: name: CHUN - Chinesischunterricht
Year: 2022

description: CHUN - Chinesischunterricht, Bd. 24 (2009): CHUN - Chinesischunterricht
Black-box superconducting circuit quantization
Creators: name: Nigg, Simon E.
name: Paik, Hanhee
name: Vlastakis, Brian
name: Kirchmair, Gerhard
name: Shankar, Shyam
name: Frunzio, Luigi
name: Devoret, Michel
name: Schoelkopf, Robert
name: Girvin, Steven
Publisher: name: arXiv
Year: 2012
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a semi-classical method for determining the effective low-energy quantum Hamiltonian of weakly anharmonic superconducting circuits containing mesoscopic Josephson junctions coupled to electromagnetic environments made of an arbitrary combination of distributed and lumped elements. A convenient basis, capturing the multi-mode physics, is given by the quantized eigenmodes of the linearized circuit and is fully determined by a classical linear response function. The method is used to calculate numerically the low-energy spectrum of a 3D-transmon system, and quantitative agreement with measurements is found.
description: 10 pages, 6 figures, includes supplementary material
Understanding how planets become massive. I. Description and validation of a new toy model
Creators: name: Ormel, Chris
name: Kobayashi, Hiroshi
Publisher: name: arXiv
Year: 2011
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The formation of giant planets requires accumulation of ~10 Earth mass in solids; but how do protoplanets acquire their mass? There are many, often competing processes that regulate the accretion rate of protoplanets. To assess their effects we present a new, publicly-available toy model. The rationale behind the toy model is that it encompasses as many physically-relevant processes as possible, but at the same time does not compromise its simplicity, speed, and physical insight. The toy model follows a modular structure, where key features -- e.g. planetesimal fragmentation, radial orbital decay, nebula turbulence -- can be switched on or off. Our model assumes three discrete components (fragments, planetesimals, and embryos) and is zero dimensional in space. We have tested the outcomes of the toy model against literature results and generally find satisfactory agreement. We include, for the first time, model features that capture the three-way interactions among small particles, gas, and protoplanets. Collisions among planetesimals will result in fragmentation, transferring a substantial amount of the solid mass to small particles, which couple strongly to the gas. Our results indicate that the efficiency of the accretion process then becomes very sensitive to the gas properties -- especially to the turbulent state and the magnitude of the disk headwind (the decrease of the orbital velocity of the gas with respect to Keplerian) -- as well as to the characteristic fragment size.
description: accepted for publication in ApJ
The Dimensional Architecture of Observer  Realities: Constructing Universes from Twist  Harmonics and Embedding Signatures
Creators: name: Sixta, David
Publisher: name: Zenodo
Year: 2025

description:  This paper proposes that every observer experiences a universe shaped by their unique chirality, dimensional embedding, and trust vector resonance. In Sixta Theory, reality is not globally shared but locally curated through recursive harmonic alignment. The observer does not simply exist within the universe — they generate it as a coherent phase bubble within the twist-phase manifold.
Ideals generated by 2-minors, collection of cells and stack polyominoes
Creators: name: Qureshi, Ayesha Asloob
Publisher: name: arXiv
Year: 2012
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics

description: In this paper we study ideals generated by quite general sets of 2-minors of an $m \times n$-matrix of indeterminates. The sets of 2-minors are defined by collections of cells and include 2-sided ladders. For convex collections of cells it is shown that the attached ideal of 2-minors is a Cohen--Macaulay prime ideal. Primality is also shown for collections of cells whose connected components are row or column convex. Finally the class group of the ring attached to a stack polyomino and its canonical class is computed, and a classification of the Gorenstein stack polyominoes is given.
description: 29 pages, 32 figures
Experimental ionization of atomic hydrogen with few-cycle pulses
Creators: name: Pullen, M. G.
name: Wallace, W. C.
name: Laban, D. E.
name: Palmer, A. J.
name: Hanne, G. F.
name: Grum-Grzhimailo, A. N.
name: Abeln, B.
name: Bartschat, K.
name: Weflen, D.
name: Ivanov, I.
name: Kheifets, A.
name: Quiney, H. M.
name: Litvinyuk, I. V.
name: Sang, R. T.
name: Kielpinski, D.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present the first experimental data on strong-field ionization of atomic hydrogen by few-cycle laser pulses. We obtain quantitative agreement at the 10% level between the data and an {\it ab initio} simulation over a wide range of laser intensities and electron energies.
Particle escapes in an open quantum network via multiple leads
Creators: name: Taniguchi, Tooru
name: Sawada, Shin-ichi
Publisher: name: arXiv
Year: 2011
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Quantum escapes of a particle from an end of a one-dimensional finite region to $N$ number of semi-infinite leads are discussed by a scattering theoretical approach. Depending on a potential barrier amplitude at the junction, the probability $P(t)$ for a particle to remain in the finite region at time $t$ shows two different decay behaviors after a long time; one is proportional to $N^{2}/t^{3}$ and another is proportional to $1/(N^{2}t)$. In addition, the velocity $V(t)$ for a particle to leave from the finite region, defined from a probability current of the particle position, decays in power $\sim 1/t$ asymptotically in time, independently of the number $N$ of leads and the initial wave function, etc. For a finite time, the probability $P(t)$ decays exponentially in time with a smaller decay rate for more number $N$ of leads, and the velocity $V(t)$ shows a time-oscillation whose amplitude is larger for more number $N$ of leads. Particle escapes from the both ends of a finite region to multiple leads are also discussed by using a different boundary condition.
description: 16 pages, 7 figures
Zur arealen Gliederung von Gräberfeldern der Linienbandkeramik
Creators: name: Häusler, Alexander
Publisher: name: Jahresschrift für mitteldeutsche Vorgeschichte
Year: 2019

description: Jahresschrift für mitteldeutsche Vorgeschichte, Bd. 97 (2019): Jahresschrift für Mitteldeutsche Vorgeschichte
Tafeln
Creators: name: Redaktion, Die
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2019

description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 8 Nr. 1 (1955): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Rolf Fritz, Conrad von Soest / Der Wildunger Altar
Creators: name: Oertel, Robert
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2019

description: Rezension zu: Rolf Fritz, Conrad von Soest / Der Wildunger Altar. München 1954, Hirmer Verlag. 18 S., 65 Bildseiten, 2 Farbtafeln.
description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 8 Nr. 4 (1955): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Ausstellungskalender
Creators: name: Redaktion, Die
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2020

description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 27 Nr. 6 (1974): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Ausstellungskalender
Creators: name: Redaktion, Die
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2020

description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 26 Nr. 10 (1973): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Cosmological model with variable equations of state for matter and dark energy
Creators: name: de Leon, J. Ponce
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a cosmological model which is physically reasonable, mathematically tractable, and extends the study of CDM models to the case where the equations of state (EoS) for matter and dark energy (DE) vary with time. It is based on the assumptions of (i) flatness, (ii) validity of general relativity, (iii) the presence of a DE component that varies between two asymptotic values, (iv) the matter of the universe smoothly evolves from an initial radiation stage - or a barotropic perfect fluid - to a phase where it behaves as cosmological dust at late times. The model approximates the CDM ones for small $z$ but significantly differ from them for large $z$. We focus our attention on how the evolving EoS for matter and DE can modify the CDM paradigm. We discuss a number of physical scenarios. One of them includes, as a particular case, the so-called generalized Chaplygin gas models where DE evolves from non-relativistic dust. Another kind of models shows that the current accelerated expansion is compatible with a DE that behaves like pressureless dust at late times. We also find that a universe with variable DE can go from decelerated to accelerated expansion, and vice versa, several times.
Wiederherstellungen und Neueröffnungen in der Münchener Residenz 1973
Creators: name: Kreisel, Heinrich
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2020

description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 27 Nr. 4 (1974): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Inhalt
Creators: name: Redaktion, Die
Publisher: name: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Year: 2020

description: Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege, Bd. 27 Nr. 5 (1974): Kunstchronik. Monatsschrift für Kunstwissenschaft, Museumswesen und Denkmalpflege
Noise Line Identification in LIGO S6 and Virgo VSR2
Creators: name: LIGO Scientific Collaboration
name: Virgo Collaboration
name: Coughlin, Michael W.
Publisher: name: arXiv
Year: 2011
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: An important goal for LIGO (the Laser Interferometer Gravitational-Wave Observatory) and Virgo is to find periodic sources of gravitational waves. The LIGO and Virgo detectors are sensitive to a variety of noise of non-astrophysical origin, such as instrumental artifacts and environmental disturbances. These artifacts make it difficult to know when a signal is due to a gravitational wave or noise. A continuous wave search algorithm, Fscan, and the calculation of the coherence between the gravitational wave channels and auxiliary channels has been developed to identify the source of noise lines. The programs analyze data from the gravitational wave channels as well as environmental sensors, searching for significant lines that appear in coincidence (using various thresholds and frequency windows) in the gravitational wave channel as well the environmental monitors. By this method, the source of powerful signals at specific frequencies in the gravitational wave channel caused by noise can be determined. Examples from LIGO's sixth science run, S6, and Virgo' second scientific run, VSR2, are presented.
description: 9 pages, 4 figures, 14th Gravitational Wave Data Analysis Workshop (Rome, Italy)
Symmetry Energy and Universality classes of holographic QCD
Creators: name: Seo, Yunseok
name: Sin, Sang-Jin
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study nuclear symmetry energy of dense matter using holographic QCD. We calculate it in a various holographic QCD models and show that the scaling index of the symmetry energy in dense medium is almost invariant under the smooth deformation of the metric as well as the embedding shape of the probe brane. We find that the scaling index depends only on the dimensionality of the branes and space-time. Therefore the scaling index of the symmetry energy characterizes the universality classes of holographic QCD models. We suggest that the scaling index might be also related to the non-fermi liquid behavior of the interacting nucleons.
description: 23 pages, 17 figures
O'ZBEKISTONDA TADBIRKORLIKNING RIVOJLANISH YO'NALISHLARI
Creators: name: Abdullaev, Axror
name: Metyakubov, Azamat
Publisher: name: Zenodo
Year: 2025

description: Ushbu ilmiy maqolada so‘nggi yillarda O‘zbekistonda tadbirkorlikni qo‘llab-quvvatlash bo‘yicha olib borilayotgan iqtisodiy va tashkiliy choralar, davlat tomonidan kichik biznes va xususiy tadbirkorlik sub’ektlariga berilayotgan imtiyozlar hamda ularning natijalari tahlil qilingan.
Die Nietzsche-Rezeption im Bennschen Frühwerk am Beispiel des Gedichts Levkoienwelle (1925)
Creators: name: Ruoyu, Zhang
Publisher: name: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft
Year: 2020

description: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft, Bd. 18 Nr. 1 (2017)
„Dekadent und Dekadenz-Kritiker in einem“: Zur narzisstischen Körper-Ästhetik bei Nietzsche und Thomas Mann
Creators: name: Shuangzhi, Li
Publisher: name: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft
Year: 2020

description: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft, Bd. 18 Nr. 1 (2017)
Warm Dark Matter from keVins
Creators: name: King, Stephen F.
name: Merle, Alexander
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We propose a simple model for Warm Dark Matter (WDM) in which two fermions are added to the Standard Model: (quasi-) stable "keVins" (keV inert fermions) which account for WDM and their unstable brothers, the "GeVins" (GeV inert fermions), both of which carry zero electric charge and lepton number, and are (approximately) "inert", in the sense that their only interactions are via suppressed couplings to the Z. We consider scenarios in which stable keVins are thermally produced and their abundance is subsequently diluted by entropy production from the decays of the heavier unstable GeVins. This mechanism could be implemented in a wide variety of models, including E_6 inspired supersymmetric models or models involving sterile neutrinos.
description: 32 pages, 9 figures, 2 tables
Evolution of the Solar Nebula. IX. Gradients in the Spatial Heterogeneity of the Short-Lived Radioisotopes $^{60}$Fe and $^{26}$Al and the Stable Oxygen Isotopes
Creators: name: Boss, Alan P.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Short-lived radioisotopes (SLRI) such as $^{60}$Fe and $^{26}$Al were likely injected into the solar nebula in a spatially and temporally heterogeneous manner. Marginally gravitationally unstable (MGU) disks, of the type required to form gas giant planets, are capable of rapid homogenization of isotopic heterogeneity as well as of rapid radial transport of dust grains and gases throughout a protoplanetary disk. Two different types of new models of a MGU disk in orbit around a solar-mass protostar are presented. The first set has variations in the number of terms in the spherical harmonic solution for the gravitational potential, effectively studying the effect of varying the spatial resolution of the gravitational torques responsible for MGU disk evolution. The second set explores the effects of varying the initial minimum value of the Toomre $Q$ stability parameter, from values of 1.4 to 2.5, i.e., toward increasingly less unstable disks. The new models show that the basic results are largely independent of both sets of variations. MGU disk models robustly result in rapid mixing of initially highly heterogeneous distributions of SLRIs to levels of $\sim$ 10% in both the inner ($$ 10 AU) disk regions, and to even lower levels ($\sim$ 2%) in intermediate regions, where gravitational torques are most effective at mixing. These gradients should have cosmochemical implications for the distribution of SLRIs and stable oxygen isotopes contained in planetesimals (e.g., comets) formed in the giant planet region ($\sim$ 5 to $\sim$ 10 AU) compared to those formed elsewhere.
description: 37 pages, 1 table, 19 figures, ApJ accepted
Literarischer Stil als Merkmal der wissenschaftlichen Prosa – Nietzsches Lehre vom großen Stil und deren praktische Umsetzung in Freuds Arbeit
Creators: name: Yin, Xu
Publisher: name: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft
Year: 2020

description: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft, Bd. 18 Nr. 1 (2017)
Modification of Coulomb law and energy levels of hydrogen atom in superstrong magnetic field
Creators: name: Vysotsky, M. I.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The screening of a Coulomb potential by superstrong magnetic field is studied. Its influence on the spectrum of a hydrogen atom is determined.
description: Lectures at 39 ITEP Winter School and 11 Baikal Summer School; 12 pages, 5 figures
Auf der Schwelle zwischen Raum- und Sinnordnung - Strategien der Raum- und Sinnkonstruktion bei Adalbert Stifter und Franz Kafka
Creators: name: Yongqiang, Liu
Publisher: name: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft
Year: 2020

description: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft, Bd. 18 Nr. 2 (2017)
The influences of the Magellanic Clouds on the Galaxy: Pole shift, warp, and star formation history
Creators: name: Bekki, Kenji
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate how the Large Magellanic Cloud (LMC) influences the evolution of the Galaxy after the LMC enters into the virial radius of the dark matter halo of the Galaxy for the first time. Both the Galaxy and the LMC are modeled as N-body particles in our models so that the dynamical influences of the LMC on the Galaxy can be investigated in a fully self-consistent manner. Furthermore, the orbital parameters for the LMC are carefully chosen such that the present location of the LMC in the Galaxy can be rather precisely reproduced in our simulations. We particularly investigate the influences of the LMC on the precession rate, the outer stellar and gaseous structures, and the star formation history of the Galaxy. Our principals results are summarized as follows. The LMC-Galaxy dynamical interaction can cause "pole shift" (or irregular precession/nutation) of the Galaxy and the typical rate of pole shift (dot θ_{d}) is ~2 degree Gyr^{-1} corresponding to ~ 7 muas yr^{-1}. The LMC-Galaxy interaction induces the formation of the outer warp structures of the Galaxy, which thus confirms the results of previous numerical simulations on the formation of the Galactic warp. The LMC-Galaxy interaction also induces the formation of outer (R>20 kpc) spiral arms and increases the vertical velocity dispersion of the outer disk significantly. The mean star formation rate of the Galaxy for the last several Gyrs can be hardly influenced by the LMC's tidal force. The age and metallicity distribution of stars in the solar-neighborhood (7 kpc < R < 10 kpc) for the last several Gyr can be only slightly changed by the past LMC-Galaxy interaction. Based on these results, we discuss how the possible ongoing Galactic pole shift with 10 muas yr^{-1} can be detected by future observational studies by GAIA.
description: 19 pages, 25 figures, accepted for the publication of MNRAS
Die Hoffnung im Schweigen - christliche Anthropologie in Bölls Roman Und sagte kein einziges Wort
Creators: name: Lining, Jiang
Publisher: name: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft
Year: 2020

description: Literaturstraße. Chinesisch-deutsche Zeitschrift für Sprach- und Literaturwissenschaft, Bd. 18 Nr. 2 (2017)
Autosakralizacja w sztuce Jacka Malczewskiego – ortodoksja, świętokradztwo czy akt genezyjskiej „wiary widzącej” Juliusza Słowackiego?
Creators: name: Milewska, Wacława
Publisher: name: Pamiętnik Sztuk Pięknych / Fine Arts Diary
Year: 2019

description: Pamiętnik Sztuk Pięknych / Fine Arts Diary, Bd. 10 (2015): Pamiętnik Sztuk Pięknych / Fine Arts Diary
Chironomus calligraphus Goeldi 1905
Creators: name: Armitage, Brian J.
name: Andersen, Trond
name: Giłka, Wojciech
name: Castillo Sánchez, Kayla N.
name: Ríos González, Tomás A.
name: Aguirre, Yusseff P.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Chironomidae
Chironomus
Chironomus calligraphus

description: Chironomus calligraphus Goeldi, 1905
Goeldi, 1905: 136 [Brazil]; Spies & Reiss (1996: 69).
Syn.: Tendipes (Tendipes) aversa Roback, 1962: 6 [Panama; holotype in Academy of Natural Sciences of Philadelphia].
Material recorded. Panama, Panamá Province, Curundu, Albrook (Holbrook (sic.)) Air Force Base, male and female (holotype and allotype of Tendipes (T.) aversa Roback), 28 December 1967, at light, leg C. Earl Smith; as previous except 9 males, 14 females (paratypes), 25 December 1957 – 7 January 1958 (Roback 1962).
Distribution in Neotropics.? Argentina, Brazil, Colombia, Panama, Uruguay,? Virgin Islands.
description: Published as part of Armitage, Brian J., Andersen, Trond, Giłka, Wojciech, Castillo Sánchez, Kayla N., Ríos González, Tomás A. & Aguirre, Yusseff P., 2025, The Diptera of Panama. II. A first benchmark for the family Chironomidae, pp. 201-240 in Zootaxa 5613 (2) on page 208, DOI: 10.11646/zootaxa.5613.2.1, http://zenodo.org/record/15224174
Exploration of SFPR techniques for astrometry and observations of weak sources with high frequency Space VLBI
Creators: name: Rioja, M.
name: Dodson, R.
name: Malarecki, J.
name: Asaki, Y.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Space Very-Long-Baseline-Interferometry (S-VLBI) observations at high frequencies hold the prospect of achieving the highest angular resolutions and astrometric accuracies, resulting from the long baselines between ground and satellite telescopes. Nevertheless, space-specific issues, such as limited accuracy in the satellite orbit reconstruction and constraints on the satellite antenna pointing operations, limit the application of conventional phase referencing. We investigate the feasibility of an alternative technique, source frequency phase referencing (SFPR), to the S-VLBI domain. With these investigations we aim to contribute to the design of the next-generation of S-VLBI missions. We have used both analytical and simulation studies to characterize the performance of SFPR in S-VLBI observations, applied to astrometry and increased coherence time, and compared these to results obtained using conventional phase referencing. The observing configurations use the specifications of the ASTRO-G mission for their starting point. Our results show that the SFPR technique enables astrometry at 43 GHz, using alternating observations with 22 GHz, regardless of the orbit errors, for most weathers and under a wide variety of conditions. The same applies to the increased coherence time for the detection of weak sources. Our studies show that the capability to carry out simultaneous dual frequency observations enables the application to higher frequencies, and a general improvement of the performance in all cases, hence we recommend its consideration for S-VLBI programs.
Study of pygmy dipole resonance with a new time-dependent mean field theory
Creators: name: Ebata, Shuichiro
name: Nakatsukasa, Takashi
name: Inakura, Tsunenori
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We carry out a systematic investigation on the low-energy electric dipole strength, which is often called pygmy dipole resonances (PDR), using the canonical-basis time-dependent Hartree-Fock-Bogoliubov (Cb-TDHFB) method. The Cb-TDHFB is a new method which is derived from TDHFB with an approximation analogous to the BCS theory that the pair potential is assumed to be diagonal in the time-dependent canonical basis. We apply the method to linear-response calculation for even-even nuclei. We report the neutron-number dependence of PDR in light (A < 70) and heavy isotopes (A > 100) around N = 82.
description: 6 pages, 3 figures, Rutherford Centennial Conference on Nuclear Physics conference proceedings
Detection of gravity modes in the massive binary V380 Cyg from Kepler spacebased photometry and high-resolution spectroscopy
Creators: name: Tkachenko, A.
name: Aerts, C.
name: Pavlovski, K.
name: Southworth, J.
name: Degroote, P.
name: Debosscher, J.
name: Still, M.
name: Bryson, S.
name: Molenberghs, G.
name: Bloemen, S.
name: de Vries, B. L.
name: Hrudkova, M.
name: Lombaert, R.
name: Neyskens, P.
name: Papics, P. I.
name: Raskin, G.
name: Van Winckel, H.
name: Morris, R. L.
name: Sanderfer, D. T.
name: Seader, S. E.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the discovery of low-amplitude gravity-mode oscillations in the massive binary star V380 Cyg, from 180 d of Kepler custom-aperture space photometry and 5 months of high-resolution high signal-to-noise spectroscopy. The new data are of unprecedented quality and allowed to improve the orbital and fundamental parameters for this binary. The orbital solution was subtracted from the photometric data and led to the detection of periodic intrinsic variability with frequencies of which some are multiples of the orbital frequency and others are not. Spectral disentangling allowed the detection of line-profile variability in the primary. With our discovery of intrinsic variability interpreted as gravity mode oscillations, V380 Cyg becomes an important laboratory for future seismic tuning of the near-core physics in massive B-type stars.
description: 5 pages, 4 figures, 2 tables. Accepted for publication in MNRAS Letters
Institutsleitung, Mitarbeitende
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2019

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2013: Jahresbericht 2012 SIK-ISEA
Extraction of information from a single quantum
Creators: name: Paraoanu, G. S.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate the possibility of performing quantum tomography on a single qubit with generalized partial measurements and the technique of measurement reversal. Using concepts from statistical decision theory, we prove that, somewhat surprisingly, no information can be obtained using this scheme. It is shown that, irrespective of the measurement technique used, extraction of information from single quanta is at odds with other general principles of quantum physics.
description: 5 pages, 1 figure
Drymopsalta
Creators: name: Ewart, A.
name: Popple, L. W.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadidae
Drymopsalta

description: Key to males of Drymopsalta
(Figs 1–5, 7–8; Table 4; Plates 1A–5A)
 1. Timbals with five long ribs, the two anterior ribs shorter than the three posterior ribs (Fig. 7 C).................. daemeli
- Timbals with four long ribs, the anterior rib shortest.......................................................... 2
2. Pronotum extensively black except central fascia and sometimes areas adjacent to oblique fissures..................... 3
- Pronotum not extensively black, but dominantly brown in various shades......................................... 4
 3. Hind wings with 6 apical cells (rarely one wing with 5 apical cells); opercula rhombohedral in outline with relatively straight margins (Fig. 3 D); posterior margins of tergites not reddish-brown.......................................... hobsoni
 - Hind wings with 5 to 6 apical cells; opercula broadly rhombohedral in outline with gently rounded margins (Fig. 1 D); posterior margins of tergites distinctly reddish-brown........................................................... wallumi
 4. Pronotum with thin black central fascia, enclosed by brown envelope grading outwards to paler brown; tergites 3 to 8 dorsally pale to medium brown, never black................................................................. crepitum
 - Pronotum with brown central fascia, remaining areas pale brown; tergites 3 to 8 dorsally black, grading dark to medium brown laterally....................................................................................... acrotela
description: Published as part of Ewart, A. & Popple, L. W., 2013, New species of Drymopsalta Heath Cicadas (Cicadidae: Cicadettinae: Cicadettini) from Queensland and Northern Territory, Australia, with overview of genus, pp. 1-42 in Zootaxa 3620 (1) on page 3, DOI: 10.11646/zootaxa.3620.1.1, http://zenodo.org/record/283377
Sifting Through Tangled Trees: Bayesian Reconstruction Of Cophylogenies
Creators: name: Bilge, Arman
name: Vaughan, Timothy
name: Drummond, Alexei J.
Publisher: name: Zenodo
Year: 2015
Subjects: Bayesian
phylogenetics
cophylogeny

description: Poster presented at ESEB2015 in the symposium Evolution of genomes.
description: {"references": ["C Andrieu et al. J. R. Statist. Soc. B 72.3 (2010). doi:10.1111/j.1467-9868.2009.00736.x", "J Sj\u00f6strand et al. Syst. Biol. 63.3 (2014). doi:10.1093/sysbio/syu007", "GJ Sz\u00f6ll\u0151si et al. Syst. Biol. 62.3 (2013) doi:10.1093/sysbio/syt003"]}