cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Piotr Górecki, A Local Society in Transition. The Henryków Book and Related Documents
Creators: name: Mühle, Eduard
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2010

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 59 Nr. 4 (2010): 1989 als mediales Ereignis
People, Facts, Figures
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Freya von Moltke, Erinnerungen an Kreisau 1930—1945
Creators: name: Winterhager, Wilhelm Ernst
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 1999

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 48 Nr. 1 (1999)
The enigma of the oldest `nova': the central star and nebula of CK Vul
Creators: name: Hajduk, M.
name: Zijlstra, Albert A.
name: van Hoof, P. A. M.
name: Lopez, J. A.
name: Drew, J. E.
name: Evans, A.
name: Eyres, S. P. S.
name: Gesicki, K.
name: Greimel, R.
name: Kerber, F.
name: Kimeswenger, S.
name: Richer, M. G.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: CK Vul is classified as, amongst others, the slowest known nova, a hibernating nova, or a very late thermal pulse object. Following its eruption in AD 1670, the star remained visible for 2 years. A 15-arcsec nebula was discovered in the 1980's, but the star itself has not been detected since the eruption. We here present radio images which reveal an 0.1-arcsec radio source with a flux of 1.5 mJy at 5 GHz. Deep Halpha images show a bipolar nebula with a longest extension of 70 arcsec, with the previously known compact nebula at its waist. The emission-line ratios show that the gas is shock-ionized, at velocities >100 km/s. Dust emission yields an envelope mass of ~0.05 Msun. Echelle spectra indicate outflow velocities up to 360 km/s. From a comparison of images obtained in 1991 and 2004 we find evidence for expansion of the nebula, consistent with an origin in the 1670 explosion; the measured expansion is centred on the radio source. No optical or infrared counterpart is found at the position of the radio source. The radio emission is interpreted as thermal free-free emission from gas with Tel ~ 10000 K. The radio source may be due to a remnant circumbinary disk, similar to those seen in some binary post-AGB stars. We discuss possible classifications of this unique outburst, including that of a sub-Chandrasekhar mass supernova, a nova eruption on a cool, low-mass white dwarf, or a thermal pulse induced by accretion from a circumbinary disk.
description: 11 pages, 8 figures, published in MNRAS
Workshop: Hands-on IIIF – how to install, configure and prepare simple IIIF services
Creators: name: Seige, Leander
Publisher: name: Zenodo
Year: 2019
Subjects: IIIF

description: Slides for a hands-on workshop on installing a IIIF Image API server, IIIF presentation files and Mirador3 for a group of participants to later interact with each other's server. Time: 2.5 hrs.
TOI-1749: an M dwarf with a Trio of Planets including a Near-Resonant Pair
Creators: name: Fukui, A.
name: Korth, J.
name: Livingston, J. H.
name: Twicken, J. D.
name: Osorio, M. R. Zapatero
name: Jenkins, J. M.
name: Mori, M.
name: Murgas, F.
name: Ogihara, M.
name: Narita, N.
name: Pallé, E.
name: Stassun, K. G.
name: Nowak, G.
name: Ciardi, D. R.
name: Alvarez-Hernandez, L.
name: Béjar, V. J. S.
name: Casasayas-Barris, N.
name: Crouzet, N.
name: de Leon, J. P.
name: Esparza-Borges, E.
name: Soto, D. Hidalgo
name: Isogai, K.
name: Kawauchi, K.
name: Klagyivik, P.
name: Kodama, T.
name: Kurita, S.
name: Kusakabe, N.
name: Luque, R.
name: Madrigal-Aguado, A.
name: Rodriguez, P. Montanes
name: Morello, G.
name: Nishiumi, T.
name: Orell-Miquel, J.
name: Oshagh, M.
name: Parviainen, H.
name: Sánchez-Benavente, M.
name: Stangret, M.
name: Watanabe, N.
name: Chen, G.
name: Tamura, M.
name: Bosch-Cabot, P.
name: Bowen, M.
name: Eastridge, K.
name: Freour, L.
name: Gonzales, E.
name: Guerra, P.
name: Jundiyeh, Y.
name: Kim, T. K.
name: Kroer, L. V.
name: Levine, A. M.
name: Morgan, E. H.
name: Reefe, M.
name: Tronsgaard, R.
name: Wedderkopp, C. K.
name: Wittrock, J.
name: Collins, K. A.
name: Hesse, K.
name: Latham, D. W.
name: Ricker, G. R.
name: Seager, S.
name: Vanderspek, R.
name: Winn, J.
name: Bachelet, E.
name: Bowman, M.
name: McCully, C.
name: Daily, M.
name: Harbeck, D.
name: Volgenau, N. H.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report the discovery of one super-Earth- (TOI-1749b) and two sub-Neptune-sized planets (TOI-1749c and TOI-1749d) transiting an early M dwarf at a distance of 100~pc, which were first identified as planetary candidates using data from the TESS photometric survey. We have followed up this system from the ground by means of multiband transit photometry, adaptive-optics imaging, and low-resolution spectroscopy, from which we have validated the planetary nature of the candidates. We find that TOI-1749b, c, and d have orbital periods of 2.39, 4.49, and 9.05 days, and radii of 1.4, 2.1, and 2.5 $R_\oplus$, respectively. We also place 95\% confidence upper limits on the masses of 57, 14, and 15 $M_\oplus$ for TOI-1749b, c, and d, respectively, from transit timing variations. The periods, sizes, and tentative masses of these planets are in line with a scenario in which all three planets initially had a hydrogen envelope on top of a rocky core, and only the envelope of the innermost planet has been stripped away by photoevaporation and/or core-powered mass loss mechanisms. These planets are similar to other planetary trios found around M dwarfs, such as TOI-175b,c,d and TOI-270b,c,d, in the sense that the outer pair has a period ratio within 1\% of 2. Such a characteristic orbital configuration, in which an additional planet is located interior to a near 2:1 period-ratio pair, is relatively rare around FGK dwarfs.
description: 30 pages, 19 figures, published in AJ
Niemcy i Polska w trudnych latach 1933-1990. Nowe spojrzenie na dawne konflikty. Deutschland und Polen in schweren Zeiten 1933-1990. Alte Konflikte - Neue Sichtweisen
Creators: name: Kessler, Wolfgang
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2005

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 54 Nr. 1 (2005)
Spatiotemporal dynamics of free and bound excitons in CVD-grown MoS$_2$ monolayer
Creators: name: Akmaev, M. A.
name: Glazov, M. M.
name: Kochiev, M. V.
name: Vinokurov, P. V.
name: Smagulova, S. A.
name: Belykh, V. V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study photoluminescence (PL) spectra and exciton dynamics of MoS$_2$ monolayer (ML) grown by the chemical vapor deposition technique. In addition to the usual direct A-exciton line we observe a low-energy line of bound excitons dominating the PL spectra at low temperatures. This line shows unusually strong redshift with increase in the temperature and submicrosecond time dynamics suggesting indirect nature of the corresponding transition. By monitoring temporal dynamics of exciton PL distribution in the ML plane we observe diffusive transport of A-excitons and measure the diffusion coefficient up to $40$~cm$^2$/s at elevated excitation powers. The bound exciton spatial distribution spreads over tens of microns in $\sim 1$ $μ$s. However this spread is subdiffusive, characterized by a significant slowing down with time. The experimental findings are interpreted as a result of the interplay between the diffusion and Auger recombination of excitons.
Impressions of the Institute history: 1951–2010
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Since its foundation in 1951, the Swiss Institute for Art Research (nowadays abbreviated to SIK-ISEA) has evolved from modest beginnings as a private initiative into an internationally acknowledged centre of competence in the fields of art technology and the documentation and study of art in Switzerland. In 1981 the Federal Council, Switzerland’s government, recognised it as a research establishment as defined by the University Development Act. Later, from 1992, it was embraced by the Federal Research Act. By acquiring its recent status in 2008 as an Institute for Advanced Study, SIK-ISEA has become a valued partner in the Swiss landscape of higher education. The renewal and transformation experienced by the Institute during these 60 years provide good reasons to look back at this history and trace the thread of continuity that has sustained it throughout all these changes, which are described in detail in the richly illustrated volume recently published.
description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Digital Photography at SIK-ISEA
Creators: name: Oberli, Matthias
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: In future, all the photography and image processing at SIK-ISEA will be digital. It is a fitting time, therefore, to look back at the era of analogue photography at our Institute and to look forward to prospects and challenges for the new technology.
description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
MicroLux: high-precision timing of high-speed photometric observations
Creators: name: Hormuth, Felix
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: MicroLux is a GPS-based high precision and high speed timing add-on to the Calar Alto Lucky Imaging camera AstraLux. It allows timestamping of individual CCD exposures at frame rates of more than 1 kHz with an accuracy better than one microsecond with respect to the UTC timeframe. The system was successfully used for high speed observations of the optical pulse profile of the Crab pulsar in January and November 2007. I present the technical design concept of MicroLux as well as first results from these observations, in particular the reconstructed pulse profile of the pulsar.
description: 8 pages, 6 figures, to appear in "Ground-based and Airborne Instrumentation for Astronomy II" SPIE conference, Marseille, 23-28 June 2008
Stanisława Lewandowska, Życie codzienne Wilna w latach II wojny światowej
Creators: name: Chiari, Bernhard
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 1999

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 48 Nr. 1 (1999)
Pericartaptera incrustata Heiss 2009
Creators: name: Heiss, Ernst
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Pericartaptera
Pericartaptera incrustata

description: Pericartaptera incrustata Heiss, 2009
Pericartaptera incrustata Heiss, 2009: 232. HT 3: Madagascar (Maromizah S Andasibe); CEHI Distr.: Madagascar
Ref.: Heiss, 2009 (fig.)
description: Published as part of Heiss, Ernst, 2012, Annotated catalogue of the flat bug family Aradidae Brullé, 1836 of Madagascar and adjacent islands (Hemiptera: Heteroptera), pp. 45-63 in Zootaxa 3426 (1) on page 58, DOI: 10.11646/zootaxa.3426.1.3, http://zenodo.org/record/214110
Martin Zückert, Zwischen Nationsidee und staatlicher Realität. Die tschechoslowakische Armee und ihre Nationalitätenpolitik 1918-1938
Creators: name: Boysen, Jens
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2008

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 57 Nr. 1 (2008): Freiheitskonzepte im östlichen Europa des Mittelalters und der Frühneuzeit - Klaus Zernack zum 75. Geburtstag
The nature of hypervelocity stars as inferred from their galactic trajectories
Creators: name: Svensson, Karl M.
name: Church, Ross P.
name: Davies, Melvyn B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have computed the galactic trajectories of twelve hypervelocity stars (HVSs) under the assumption that they originated in the Galactic Centre. We show that eight of these twelve stars are bound to the Galaxy. We consider the subsequent trajectories of the bound stars to compute their characteristic orbital period, which is 2 Gyr. All eight bound stars are moving away from the centre of the Galaxy, which implies that the stars' lifetimes are less than 2 Gyr. We thus infer that the observed HVSs are massive main sequence stars, rather than blue horizontal branch stars. The observations suggest that blue HVSs are ejected from the Galactic Centre roughly every 15 Myr. This is consistent with the observed population of blue stars in extremely tight orbits round the central super-massive black hole (SMBH), the so-called S-stars, if we assume that the HVSs are produced by the breakup of binaries. One of the stars in such a binary is ejected at high velocities to form a HVS; the other remains bound to the SMBH as an S-star. We further show that the one high-velocity system observed to be moving towards the Galactic Centre, SDSS J172226.55+594155.9, could not have originated in the Galactic Centre; rather, we identify it as a halo object.
description: 5 pages, 3 figures, accepted to MNRAS letters
Reconfigurable 3D magnonic crystal: tunable and localized spin-wave excitations in CoFeB meander-shaped film
Creators: name: Sadovnikov, A. V.
name: Talmelli, G.
name: Gubbiotti, G.
name: Beginin, E. N.
name: Sheshukova, S.
name: Nikitov, S. A.
name: Adelmann, C.
name: Ciubotaru, F.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this work, we study experimentally by broadband ferromagnetic resonance measurements, the dependence of the spin-wave excitation spectra on the magnetic applied field in CoFeB meander-shaped films. Two different orientations of the external magnetic field were explored, namely parallel or perpendicular to the lattice cores. The interpretation of the field dependence of the frequency and spatial profiles of major spin-wave modes were obtained by micromagnetic simulations. We show that the vertical segments lead to the easy-axis type of magnetic anisotropy and support the in-phase and out-of-phase spin-wave precession amplitude in the vertical segments. The latter could potentially be used for the design of tunable metasurfaces or in magnetic memories based on meandering 3D magnetic films.
description: This project has received funding from the European Union's Horizon 2020 research and innovation program under grant agreement No. 801055 "Spin Wave Computing for Ultimately-Scaled Hybrid Low-Power Electronics" CHIRON
Discussion of: Statistical analysis of an archeological find
Creators: name: Höfling, Holger
name: Wasserman, Larry
Publisher: name: arXiv
Year: 2008
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: Discussion of ``Statistical analysis of an archeological find'' by Andrey Feuerverger [arXiv:0804.0079]
description: Published in at http://dx.doi.org/10.1214/08-AOAS99C the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Loss of mass and stability of galaxies in MOND
Creators: name: Wu, Xufen
name: Zhao, HongSheng
name: Famaey, Benoit
name: Gentile, G.
name: Tiret, O.
name: Combes, F.
name: Angus, G. W.
name: Robin, A. C.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The self-binding energy and stability of a galaxy in MOND-based gravity are curiously decreasing functions of its center of mass acceleration towards neighbouring mass concentrations. A tentative indication of this breaking of the Strong Equivalence Principle in field galaxies is the RAVE-observed escape speed in the Milky Way. Another consequence is that satellites of field galaxies will move on nearly Keplerian orbits at large radii (100 - 500 kpc), with a declining speed below the asymptotically constant naive MOND prediction. But consequences of an environment-sensitive gravity are even more severe in clusters, where member galaxies accelerate fast: no more Dark-Halo-like potential is present to support galaxies, meaning that extended axisymmetric disks of gas and stars are likely unstable. These predicted reappearance of asymptotic Keplerian velocity curves and disappearance of "stereotypic galaxies" in clusters are falsifiable with targeted surveys.
description: 4 pages, 2 figures, ApJ Letters
TrajMap.py
Creators: name: Kožić, Matej
Publisher: name: figshare
Year: 2023
Subjects: classificationCode: 310201
subject: Bioinformatic methods development
classificationCode: 310299
subject: Bioinformatics and computational biology not elsewhere classified
classificationCode: 310112
subject: Structural biology (incl. macromolecular modelling)
classificationCode: 310199
subject: Biochemistry and cell biology not elsewhere classified
classificationCode: 349999
subject: Other chemical sciences not elsewhere classified
classificationCode: 340799
subject: Theoretical and computational chemistry not elsewhere classified
classificationCode: 340701
subject: Computational chemistry

description: Content of a GitHub repo of TrajMap.py, a Python software for performing analysis of protein MD simulations using trajectory maps, a novel approach developed by this publication.
Wanda Kononowicz, Wrocław. Kierunki rozwoju urbanistycznego w okresie międzywojennym
Creators: name: Störtkuhl, Beate
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 1999

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 48 Nr. 1 (1999)
Recent advances in the three flavor Larkin-Ovchinnikov-Fulde-Ferrel phase of QCD
Creators: name: Anglani, R.
name: Ciminale, M.
name: Ippolito, N. D.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a summary of the recent advances achieved in the study of three flavor Larkin-Ovchinnikov-Fulde-Ferrell (LOFF)phase of QCD. We have explored, using a Ginzburg-Landau expansion of the free energy, the LOFF phase with three flavors, in the simplest single plane wave structure, using the NJL four-fermion coupling. We have found that this phase does not suffer the chromo-magnetic instability problem. A preliminary study of astrophysical effects of quark matter in the aforementioned phase has been done and we have evaluated self-consistently the strange quark mass extending the pairing ansatz to the CubeX and 2Cube45z structure. Finally we have investigated the possibility of Goldstone bosons condensation in the favored cubic structures of LOFF phase.
description: 5 pages, 6 figures,Contributed to International Workshop on Quantum Chromodynamics: QCD@Work 2007, Martina Franca, Valle d'Itria, Italy, 16-20 Jun 2007,reference added, typo corrected
Jiří Vykoukal, Visegrád. Možnosti a meze středoevropské spolupráce
Creators: name: Mrázková, Marie
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2005

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 54 Nr. 1 (2005)
Detectability of Exoplanetary Transits from Radial Velocity Surveys
Creators: name: Kane, Stephen R.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Of the known transiting extra-solar planets, a few have been detected through photometric follow-up observations of radial velocity planets. Perhaps the best known of these is the transiting exoplanet HD 209458b. For hot Jupiters (periods less than ~5 days), the a priori information that 10% of these planets will transit their parent star due to the geometric transit probability leads to an estimate of the expected transit yields from radial velocity surveys. The radial velocity information can be used to construct an effective photometric follow-up strategy which will provide optimal detection of possible transits. Since the planet-harbouring stars are already known in this case, one is only limited by the photometric precision achieveable by the chosen telescope/instrument. The radial velocity modelling code presented here automatically produces a transit ephemeris for each planet dataset fitted by the program. Since the transit duration is brief compared with the fitted period, we calculate the maximum window for obtaining photometric transit observations after the radial velocity data have been obtained, generalising for eccentric orbits. We discuss a typically employed survey strategy which may contribute to a possible radial velocity bias against detection of the very hot Jupiters which have dominated the transit discoveries. Finally, we describe how these methods can be applied to current and future radial velocity surveys.
description: 11 pages, 8 figures, accepted for publication in MNRAS, minor correction
Discussion of: Statistical analysis of an archaeological find
Creators: name: Ingermanson, Randall
Publisher: name: arXiv
Year: 2008
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: We critique the analysis by A. Feuerverger of an archaeological find [arXiv:0804.0079] that has been alleged by some to be the tomb of Jesus of Nazareth. We show that his analysis rests on six faulty assumptions that have been severely criticized by historians, archaeologists, and scholars in related disciplines. We summarize the results of an alternative computation using Bayes' theorem that estimates a probability of less than 2% that the Talpiot tomb belongs to Jesus of Nazareth.
description: Published in at http://dx.doi.org/10.1214/08-AOAS99G the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Andrzej Groth, Warenumschlag am Frischen Haff. Eine Handelsstatistik der kleinen Seehäfen (1581-1712)
Creators: name: Riemer, Robert
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2010

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 59 Nr. 4 (2010): 1989 als mediales Ereignis
Willy Cohn, Kein Recht, nirgends. Tagebuch vom Untergang des Breslauer Judentums 1933-1941
Creators: name: Reinke, Andreas
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2008

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 57 Nr. 1 (2008): Freiheitskonzepte im östlichen Europa des Mittelalters und der Frühneuzeit - Klaus Zernack zum 75. Geburtstag
L'influence de l'intelligence artificielle sur l'efficacité de l'audit financier : Tendances, défis et opportunités
Creators: name: EL BOUZAIDI CHIKHI, Dounia
name: RAMDANI, Bouchra
Publisher: name: Zenodo
Year: 2023
Subjects: « Intelligence artificielle » ; « Audit financier » ; « Analyse des données financières » ; « Risque d'audit » ; « Gestion des données » ; « Réglementation financière».

description: Le paysage de l'audit financier évolue rapidement sous l'influence de la mondialisation, de l'innovation technologique et de la croissance des données financières. Les méthodes traditionnelles d'audit peinent à suivre cette complexité croissante, suscitant le besoin d'une approche plus efficace et précise. L'intelligence artificielle (IA) joue un rôle crucial dans cette réflexion. Cette analyse explore l'impact varié de l'IA sur l'audit financier, mettant en lumière les tendances, les défis et les opportunités.

En examinant des études universitaires, des recherches empiriques et des cas concrets, cet article révèle les transformations significatives induites par l'IA dans l'audit financier. Son intégration ne remplace pas simplement l'expertise humaine, mais offre une collaboration synergique. L'IA permet aux auditeurs d'extraire des informations approfondies des données financières, mettant en évidence les risques et favorisant la transparence des organisations.

Alors que le monde financier évolue vers le numérique, le partenariat entre les auditeurs humains et l'IA promet de remodeler profondément l'avenir de l'audit financier.
$\cos 2 ϕ$ asymmetries in unpolarized semi-inclusive DIS
Creators: name: Zhang, Bing
name: Lu, Zhun
name: Ma, Bo-Qiang
name: Schmidt, Ivan
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use the Boer-Mulders functions parameterized from unpolarized $p+D$ Drell-Yan data by the FNAL E866/NuSea Collaboration combined with recently extracted Collins functions to calculate the $\cos 2 ϕ$ asymmetries in unpolarized semi-inclusive deeply inelastic scattering (SIDIS) processes both for ZEUS at Hadron Electron Ring Accelerator (HERA) and Jefferson Lab experiments (JLab), and to compare our results with their data. We also give predictions for the $\cos 2 ϕ$ asymmetries of SIDIS in the kinematical regime of HERMES Collaboration, and the forthcoming JLab experiments. We predict that the $\cos 2 ϕ$ asymmetries of semi-inclusive $π^-$ production are somewhat larger than that of $π^+$ production. We suggest to measure these two processes separately, which will provide more detail information on the Boer-Mulders functions as well as on the Collins functions.
description: 9 latex pages, 18 figures, to appear in PRD
Sozialgeschichtliche Kommunismusforschung. Tschechoslowakei, Polen, Ungarn, DDR 1945-1968
Creators: name: Behrends, Jan C.
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2005

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 54 Nr. 1 (2005)
Contenance Principle. Taking Leave of Hans-Jörg Heusser
Creators: name: Beyer, Andreas
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
A coverage independent method to analyze large scale anisotropies
Creators: name: Billoir, Pierre
name: Letessier-Selvon, Antoine
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The arrival time distribution of cosmic ray events is well suited to extract information regarding sky anisotropies. For an experiment with nearly constant exposure, the frequency resolution one can achieve is given by the inverse of the time $T$ during which the data was recorded. For $T$ larger than one calendar year the resolution becomes sufficient to resolve the sidereal and diurnal frequencies. Using a Fourier expansion on a modified time parameter, we show in this note that one can accurately extract sidereal modulations without knowledge of the experimental coverage. This procedure also gives the full frequency pattern of the event sample under studies which contains important information about possible systematics entering in the sidereal analysis. We also show how this method allows to correct for those systematics. Finally, we show that a two dimensional analysis, in the form of the spherical harmonic ($Y_l^m$) decomposition, can be performed under the same conditions for all $m\ne 0$.
description: 8 pages, 6 figures
Sabine Jagodzinski, Die illustrierte Apokalypse Heinrichs von Hesler im Deutschen Orden
Creators: name: Jähnig, Bernhart
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2010

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 59 Nr. 4 (2010): 1989 als mediales Ereignis
Michał Kaczmarek, Mateusz Goliński, Teresa Kulak, Włodzimierz Suleja, Wrocław. Dziedzictwo wieków
Creators: name: Wünsch, Thomas
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 1999

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 48 Nr. 1 (1999)
Kristine Wohlfart, Der Rigaer Letten Verein und die lettische Nationalbewegung von 1868 bis 1905
Creators: name: Hroch, Miroslav
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2008

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 57 Nr. 1 (2008): Freiheitskonzepte im östlichen Europa des Mittelalters und der Frühneuzeit - Klaus Zernack zum 75. Geburtstag
Design and Implementation of the New D0 Level-1 Calorimeter Trigger
Creators: name: Abolins, M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Increasing luminosity at the Fermilab Tevatron collider has led the D0 collaboration to make improvements to its detector beyond those already in place for Run IIa, which began in March 2001. One of the cornerstones of this Run IIb upgrade is a completely redesigned level-1 calorimeter trigger system. The new system employs novel architecture and algorithms to retain high efficiency for interesting events while substantially increasing rejection of background. We describe the design and implementation of the new level-1 calorimeter trigger hardware and discuss its performance during Run IIb data taking. In addition to strengthening the physics capabilities of D0, this trigger system will provide valuable insight into the operation of analogous devices to be used at LHC experiments.
description: 43 pages, 20 figures, version published in Nucl. Instrum. and Methods A
ความเป็นพิษร่วมกันของเอ็นโดซัลแฟน-ซัลเฟตและเฮปตาคลอร์ต่อการเจริญเติบโตในระยะต้นกล้าของพืชชนิดต่างๆ
Creators: name: ขนิษฐา สมตระกูล
name: สุนันทา ประทุมมา
Publisher: name: มหาวิทยาลัยมหาสารคาม
Year: 2012
Subjects: ความเป็นพิษต่อพืช,เอ็นโดซัลแฟน-ซัลเฟต,เฮปตาคลอร์

description: 2, 6, วารสารวิชาการและวิจัย มทร.พระนคร
AstraLux - the Calar Alto 2.2-m telescope Lucky Imaging camera
Creators: name: Hormuth, Felix
name: Brandner, Wolfgang
name: Hippler, Stefan
name: Henning, Thomas
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: AstraLux is a Lucky Imaging camera for the Calar Alto 2.2-m telescope, based on an electron-multiplying high speed CCD. By selecting only the best 1-10% of several thousand short exposure frames, AstraLux provides nearly diffraction limited imaging capabilities in the SDSS i' and z' filters over a field of view of 24x24 arcseconds. By choosing commercially available components wherever possible, the instrument could be built in short time and at comparably low cost. We briefly present the instrument design, the data reduction pipeline, and summarise the performance and characteristics
description: 6 pages, 5 figures, to appear in proceedings of "The Universe under the Microscope - Astrophysics at High Angular Resolution", published in the Journal of Physics: Conference Series by Institute of Physics Publishing
Rudolphia Grosso & Peralta, 2009, n. gen.
Creators: name: Grosso, Luis E.
name: Peralta, Marcela
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Plantae
Arthropoda
Malacostraca
Amphipoda
Paraleptamphopidae
Rudolphia

description: Rudolphia n. gen.
Both antennae (=A) long, A1 equal to length of body. A1 inner flagellum scale shaped. Calceoli gammaridtype, in males only. Maxille 1 (=Mx1) asymmetrical. Gnatopod 1 (=Gn1) propodus mitten-like, palmar index= 1.81. Gnatopod 2 (=Gn2) slender and longer than Gn1, palmar index = 2.39. Dactyls of pereopods (=P) very long. Coxal gills of P 2–5 and 7 bilobate; coxal gills P6 ovoid. Pleopods (=Pl) multiarticulate, Pl 2 sexually dimorphic. Uropods (=Ur) biramose, rami uniarticulate, Ur1 and Ur2 exopodites scarcely shorter than endopodites. Ur1 peduncle longer than rami. Ur2 resembling Ur1 but much shorter. Ur3 subequal in
description: Published as part of Grosso, Luis E. & Peralta, Marcela, 2009, A new Paraleptamphopidae (Crustacea Amphipoda) in the burrow of Virilastacus rucapihuelensis (Parastacidae) and surrounding peat bogs. Rudolphia macrodactylus n. gen., n. sp. from southern South America, pp. 40-52 in Zootaxa 2243 on page 41, DOI: 10.5281/zenodo.190647
Maria Paola Funaioli (a cura di), Callimaco. Inno ad Apollo e altre poesie, Novara, Giuliano Landolfi 2012, pp. 82, ISBN 978-88-6644-066-6
Creators: name: Garulli, Valentina
Publisher: name: Annali Online  Lettere - Ferrara
Year: 2013

description: Annali Online  Lettere - Ferrara, VIII 1 (2013)
Non-equilibrium hydrogen ionization in 2D simulations of the solar atmosphere
Creators: name: Leenaarts, J.
name: Carlsson, M.
name: Hansteen, V.
name: Rutten, R. J.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The ionization of hydrogen in the solar chromosphere and transition region does not obey LTE or instantaneous statistical equilibrium because the timescale is long compared with important hydrodynamical timescales, especially of magneto-acoustic shocks. We implement an algorithm to compute non-equilibrium hydrogen ionization and its coupling into the MHD equations within an existing radiation MHD code, and perform a two-dimensional simulation of the solar atmosphere from the convection zone to the corona. Analysis of the simulation results and comparison to a companion simulation assuming LTE shows that: a) Non-equilibrium computation delivers much smaller variations of the chromospheric hydrogen ionization than for LTE. The ionization is smaller within shocks but subsequently remains high in the cool intershock phases. As a result, the chromospheric temperature variations are much larger than for LTE because in non-equilibrium, hydrogen ionization is a less effective internal energy buffer. The actual shock temperatures are therefore higher and the intershock temperatures lower. b) The chromospheric populations of the hydrogen n = 2 level, which governs the opacity of Halpha, are coupled to the ion populations. They are set by the high temperature in shocks and subsequently remain high in the cool intershock phases. c) The temperature structure and the hydrogen level populations differ much between the chromosphere above photospheric magnetic elements and above quiet internetwork. d) The hydrogen n = 2 population and column density are persistently high in dynamic fibrils, suggesting that these obtain their visibility from being optically thick in Halpha also at low temperature.
description: 10 pages, 4 figures
The Scandinavian impact on Irish seafaring technology
Creators: name: Wilson, Garth Stewart
Publisher: name: University of British Columbia
Year: 2010

description: In the Middle Ages mariners from both Ireland and Scandinavia sailed the North Atlantic, but in different types of ships and for very different reasons. The Irish sailors appear to have favoured skin-covered ships called curraghs as the means by which they sought out remote islands on which to establish monastic retreats. The Norsemen, however, travelled the northern seas in clinker-built wooden vessels seeking plunder, land and trade. When at the end of the eighth century the Vikings invaded Ireland, these two distinct seafaring traditions came into contact with one another. This thesis is an analysis of the impact that the arrival of Scandinavian seafaring technology had upon that of the indigenous Irish. Although this issue has been largely neglected by scholars, the little that has been done has tended to promote the conclusion that Viking seafaring technology displaced the vigorous but inferior curragh technology of the Irish. This thesis argues that rather than replacing the Irish tradition, the Scandinavians supplemented it. While ultimately unsuccessful in their bid for political sovereignty in Erinn, the Norsemen established a series of port: cities along Ireland's coast, cities which became important links in the chain of Viking trading centres in Europe. Overseas commerce of this magnitude was new to the Irish who were then largely a pastoral and parochial people. Moreover, their shipbuilding and seafaring heritage had not developed in response to the range of military, political and economic needs that encouraged the high sea ventures of the Vikings. Instead, Irish seafaring was almost exclusively the concern of a select sector of Irish society: the anchorite monks. Admittedly, the seafaring technology of these churchmen was sufficient to allow for journeys to as distant a place as Iceland. In addition, their skills as mariners and religious devotion inspired a rich body of literature from which much of what is currently known about early Irish shipbuilding and navigation is derived. Nevertheless, the seafaring heritage of the Irish was simply not capable of dealing with the volume or variety of traffic which accompanied the Viking invasions. When the naval technologies of medieval Ireland and Scandinavia are viewed within the context of the functions they served in their respective societies, their relative merits can be more accurately judged. From this perspective, the arrival of Viking ships in Ireland can be seen as not so much a challenge, to the indigenous seafaring tradition, as an addition to it.
Association pour la promotion de SIK-ISEA
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Andrzej Kopiczko, Kościół Warminski a polityka wyznaniowa po II wojnie światowej
Creators: name: Hartmann, Stefan
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 1999

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 48 Nr. 1 (1999)
Verein zur Förderung von SIK-ISEA
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Cladonia chlorophaea Spreng.
Creators: name: Farkas, Edit
name: Lőkös, László
name: Veres, Katalin
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Lecanoromycetes
Lecanorales
Cladoniaceae
Cladonia
Cladonia chlorophaea

description: Cladonia chlorophaea (Flörke ex Sommerf.) Spreng.
(Fig. 11)
NOTES
It contains fumarprotocetraric acid (itself or with related compound protocetraric acid – not analysed separately).
Their colour is pale greenish brown, the margin of the scyphi is dentate and becoming broken and denuded with age, the base
of the podetia is not melanotic (Ahti et al. 2013). The soredia are granulose and thus measured as relatively larger (34-138µm) than in other species in Hungary. It has relatively tall (3.6-20.8 mm) and broad (1.1-7.9 mm) scyphi with short stalk. Differences were found from C. asahinae in several characters (CH, CW, PH, PHCW, sor, SW), from C. cryptochlorophaea in height of cup and podetium, from C. grayi in the height of podetium, from C. merochlorophaea in the length of squamules and from C. novochlorophaea in the height of the podetium (Table 1).
It is the most frequent and most widely spread species in Hungary among the C. chlorophaea s.l. species. C. chlorophaea is found on calcareous soil, in deciduous and coniferous forests, at the basis of various tree species (e.g. Alnus glutinosa (L.) Gaertn., Betula pendula Roth, Fagus sylvatica L., Quercus spp., Robinia pseudoacacia L.), sometimes on stumps on lignum or thatched roof and almost equally frequent in the Hungarian Great Plain (70-200 m a.s.l.) and in hilly regions (up to c. 1000 m a.s.l.) in Hungary. However, specimens from hilly regions were mostly recognised as other C. chlorophaea s.l. species during our revision.
description: Published as part of Farkas, Edit, Lőkös, László & Veres, Katalin, 2023, Analysis of lichen secondary metabolites and morphometrics in the Cladonia chlorophaea species group (Cladoniaceae, lichenized Ascomycota) in Hungary, pp. 61-82 in Cryptogamie, Mycologie 20 (5) on page 70, DOI: 10.5252/cryptogamie-mycologie2023v44a5, http://zenodo.org/record/8055982
Using nodal coordinates as variables for the dimensional synthesis of mechanisms
Creators: name: Garcia-Marina, V.
name: de Bustos, I. Fernandez
name: Urkullu, G.
name: Abasolo, M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Dynamical Systems (math.DS)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: The method of the lower deformation energy has been successfully used for the synthesis of mechanisms for quite a while. It has shown to be a versatile, yet powerful method for assisting in the design of mechanisms. Until now, most of the implementations of this method used the dimensions of the mechanism as the synthesis variables, which has some advantages and some drawbacks. For example, the assembly configuration is not taken into account in the optimization process, and this means that the same initial configuration is used when computing the deformed positions in each synthesis point. This translates into a reduction of the total search space. A possible solution to this problem is the use of a set of initial coordinates as variables for the synthesis, which has been successfully applied to other methods. This also has some additional advantages, such as the fact that any generated mechanism can be assembled. Another advantage is that the fixed joint locations are also included in the optimization at no additional cost. But the change from dimensions to initial coordinates means a reformulation of the optimization problem when using derivatives if one wants them to be analytically derived. This paper tackles this reformulation, along with a proper comparison of the use of both alternatives using sequential quadratic programming methods. In order to do so, some examples are developed and studied.
On the nature of QPO in the tail of SGR giant flares
Creators: name: Timokhin, A. N.
name: Eichler, D.
name: Lyubarsky, Yu.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A model is presented for the quasiperiodic component of magnetar emission during the tail phase of giant flares. The model invokes modulation of the particle number density in the magnetosphere. The magnetospheric currents are modulated by torsional motion of the surface and we calculate that the amplitude of neutron star surface oscillation should be ~1% of the NS radius in order to produce the observed features in the power spectrum. Using an axisymmetric analytical model for structure of the magnetosphere of an oscillating NS, we calculate the angular distribution of the optical depth to the resonant Compton scattering. The anisotropy of the optical depth may be why QPO are observed only at particular rotational phases.
description: 7 pages, 4 figures, emulateapj style
Discussion of: Statistical analysis of an archeological find
Creators: name: Mortera, J.
name: Vicard, P.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: Discussion of ``Statistical analysis of an archeological find'' by Andrey Feuerverger [arXiv:0804.0079]
description: Published in at http://dx.doi.org/10.1214/08-AOAS99F the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
The Homogeneous Approximation Property and the Comparison Theorem for Coherent Frames
Creators: name: Gröchenig, Karlheinz
Publisher: name: arXiv
Year: 2007
Subjects: subject: Functional Analysis (math.FA)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 42C40

description: We show that the homogeneous approximation property and the comparison theorem hold for arbitrary coherent frames. This observation answers some questions about the density of frames that are not covered by the theory of Balan, Casazza, Heil, and Landau. The proofs are a variation of the method developed by Ramanathan and Steger.
Isabel Heinemann, "Rasse, Siedlung, deutsches Blut". Das Rasse- und Siedlungshauptamt der SS und die rassenpolitische Neuordnung Europas
Creators: name: Tönsmeyer, Tatjana
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2005

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 54 Nr. 1 (2005)
Personnes, chiffres, faits
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Kurland. Vom polnisch-litauischen Lehnsherzogtum zur russischen Provinz. Dokumente zur Verfassungsgeschichte 1561-1795
Creators: name: Hartmann, Stefan
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2008

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 57 Nr. 1 (2008): Freiheitskonzepte im östlichen Europa des Mittelalters und der Frühneuzeit - Klaus Zernack zum 75. Geburtstag
Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
Creators: name: Li, Yuexing
name: Hopkins, Philip F.
name: Hernquist, Lars
name: Finkbeiner, Douglas P.
name: Cox, Thomas J.
name: Springel, Volker
name: Jiang, Linhua
name: Fan, Xiaohui
name: Yoshida, Naoki
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The detection of large quantities of dust in z ~ 6 quasars by infrared and radio surveys presents puzzles for the formation and evolution of dust in these early systems. Previously (Li et al. 2007), we showed that luminous quasars at z > 6 can form through hierarchical mergers of gas-rich galaxies. Here, we calculate the dust properties of simulated quasars and their progenitors using a three-dimensional Monte Carlo radiative transfer code, ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree. ART^2 incorporates a radiative equilibrium algorithm for dust emission, an adaptive grid for inhomogeneous density, a multiphase model for the ISM, and a supernova-origin dust model. We reproduce the SED and dust properties of SDSS J1148+5251, and find that the infrared emission are closely associated with the formation and evolution of the quasar host. The system evolves from a cold to a warm ULIRG owing to heating and feedback from stars and AGN. Furthermore, the AGN has significant implications for the interpretation of observation of the hosts. Our results suggest that vigorous star formation in merging progenitors is necessary to reproduce the observed dust properties of z~6 quasars, supporting a merger-driven origin for luminous quasars at high redshifts and the starburst-to-quasar evolutionary hypothesis. (Abridged)
description: 26 pages, 22 figures, accepted by ApJ. Version with full resolution images is available at http://www.cfa.harvard.edu/~yxli/ARTDUST/astroph0706.3706.pdf
Simon Helms, Luther von Braunschweig. Der Deutsche Orden in Preußen zwischen Krise und Stabilisierung und das Wirken eines Fürsten in der ersten Hälfte des 14. Jahrhunderts
Creators: name: Jähnig, Bernhart
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2010

description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 59 Nr. 4 (2010): 1989 als mediales Ereignis
Personen, Zahlen, Fakten
Creators: name: Redaktion, Die
Publisher: name: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft
Year: 2022

description: Jahresbericht SIK-ISEA / Schweizerisches Institut für Kunstwissenschaft, 2011: Jahresbericht 2010 SIK-ISEA
Pictinus Stal 1973
Creators: name: Heiss, Ernst
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Pictinus

description: Genus Pictinus Stål, 1973
Pictinus Stål, 1873: 140. Type species. Pictinus cinctipes Stål, 1873 (Colombia). Pictinus Usinger & Matsuda, 1987: 358 (redescription, new status)
description: Published as part of Heiss, Ernst, 2012, Annotated catalogue of the flat bug family Aradidae Brullé, 1836 of Madagascar and adjacent islands (Hemiptera: Heteroptera), pp. 45-63 in Zootaxa 3426 (1) on page 58, DOI: 10.11646/zootaxa.3426.1.3, http://zenodo.org/record/214110