cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Optical Gravitational Lensing Experiment. Gaia South Ecliptic Pole Field as Seen by OGLE-IV
Creators: name: Soszynski, I.
name: Udalski, A.
name: Poleski, R.
name: Kozlowski, S.
name: Wyrzykowski, L.
name: Pietrukowicz, P.
name: Szymanski, M. K.
name: Kubiak, M.
name: Pietrzynski, G.
name: Ulaczyk, K.
name: Skowron, J.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a comprehensive analysis of the Gaia South Ecliptic Pole (GSEP) field, 5.3 square degrees area around the South Ecliptic Pole on the outskirts of the LMC, based on the data collected during the fourth phase of the Optical Gravitational Lensing Experiment, OGLE-IV. The GSEP field will be observed during the commissioning phase of the ESA Gaia space mission for testing and calibrating the Gaia instruments. We provide the photometric maps of the GSEP region containing the mean VI photometry of all detected stellar objects and their equatorial coordinates. We show the quality and completeness of the OGLE-IV photometry and color-magnitude diagrams of this region. We conducted an extensive search for variable stars in the GSEP field leading to the discovery of 6789 variable stars. In this sample we found 132 classical Cepheids, 686 RR Lyr type stars, 2819 long-period, and 1377 eclipsing variables. Several objects deserving special attention were also selected, including a new classical Cepheid in a binary eclipsing system. To provide empirical data for the Gaia Science Alert system we also conducted a search for optical transients. We discovered two firm type Ia supernovae and nine additional supernova candidates. To facilitate future Gaia supernovae detections we prepared a list of more than 1900 galaxies to redshift about 0.1 located in the GSEP field. Finally, we present the results of astrometric study of the GSEP field. With the 26 months time base of the presented here OGLE-IV data, proper motions of stars could be detected with the accuracy reaching 2 mas/yr. Astrometry allowed to distinguish galactic foreground variable stars detected in the GSEP field from LMC objects and to discover about 50 high proper motion stars (proper motion >100 mas/yr). Among them three new nearby white dwarfs were found.
description: 27 pages, color figures
From Clermont to Jerusalem. The Crusades and Crusader Societies 1095–1500. Selected Proceedings of the International Medieval Congress, University of Leeds 10–13 July 1995, ed. by A. V. Murray, 1998
Creators: name: Vones, L.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 1 (2001)
Probing primordial non-Gaussianity: The 3D Bispectrum of Ly-alpha forest and the redshifted 21-cm signal from the post reionization epoch
Creators: name: Sarkar, Tapomoy Guha
name: Hazra, Dhiraj Kumar
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We explore possibility of using the three dimensional bispectra of the Ly-alpha forest and the redshifted 21-cm signal from the post-reionization epoch to constrain primordial non-Gaussianity. Both these fields map out the large scale distribution of neutral hydrogen and maybe treated as tracers of the underlying dark matter field. We first present the general formalism for the auto and cross bispectrum of two arbitrary three dimensional biased tracers and then apply it to the specific case. We have modeled the 3D Ly-alpha transmitted flux field as a continuous tracer sampled along 1D skewers which corresponds to quasars sight lines. For the post reionization 21-cm signal we have used a linear bias model. We use a Fisher matrix analysis to present the first prediction for bounds on f_{NL} and the other bias parameters using the three dimensional 21-cm bispectrum and other cross bispectra. The bounds on f_{NL} depend on the survey volume, and the various observational noises. We have considered a BOSS like Ly-alpha survey where the average number density of quasars \bar{n} = 10^{-3} Mpc^{-2} and the spectra are measured at a 2-sigma level. For the 21-cm signal we have considered a 4000 hrs observation with a futuristic SKA like radio array. We find that bounds on f_{NL} obtained in our analysis (6 < Δf_{NL} < 65) is competitive with CMBR and galaxy surveys. We also find that by combining the various cross-bispectrum estimators it is possible to constrain f_{NL} at a level Δf_{NL} ~ 4.7. For the equilateral and orthogonal template we obtain Δf_{NL}^{equ}~17 and Δf_{NL}^{orth}~13 respectively for the combined estimator. This shall be important in the quest towards understanding the mechanism behind the generation of primordial perturbations.
description: v1: 7 pages, 2 figures and 1 table; v2: 15 pages, 2 figures and 3 tables, matches JCAP Published version
(ϕ,Γ)-modules over noncommutative overconvergent and Robba rings
Creators: name: Zábrádi, Gergely
Publisher: name: arXiv
Year: 2012
Subjects: subject: Representation Theory (math.RT)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11F70, 20G25

description: We construct noncommutative multidimensional versions of overconvergent power series rings and Robba rings. We show that the category of étale $(φ,Γ)$-modules over certain completions of these rings are equivalent to the category of étale $(φ,Γ)$-modules over the corresponding classical overconvergent, resp. Robba rings (hence also to the category of $p$-adic Galois representations of $\mathbb{Q}_p$). Moreover, in the case of Robba rings, the assumption of étaleness is not necessary, so there exists a notion of trianguline objects in this sense.
description: 41 pages, revised
The Spin Effect on Planetary Radial Velocimetry of Exoplanets
Creators: name: Kawahara, Hajime
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We consider the effect of planetary spin on the planetary radial velocity (PRV) in dayside spectra of exoplanets. To understand the spin effect qualitatively, we derive an analytic formula of the intensity-weighted radial velocity from planetary surface on the following assumptions: 1) constant and solid rotation without precession, 2) stable and uniform distribution of molecules/atoms, 3) emission models from dayside hemisphere, and 4) a circular orbit. On these assumptions, we find that the curve of the PRV is distorted by the planetary spin and this anomaly is characterized by spin radial velocity at equator and a projected angle on a celestial plane between the spin axis and the axis of orbital motion λ_p in a manner analogous to the Rossiter-McLaughlin effect. The latter can constrain the planetary obliquity. Creating mock PRV data with 3 km/s accuracy, we demonstrate how λ_p and the spin radial velocity at equator are estimated. We find that the stringent constraint of eccentricity is crucial to detect the spin effect. Though our formula is still qualitative, we conclude that the PRV in the dayside spectra will be a powerful means for constraining the planetary spin.
description: Accepted for publication in ApJL, 6 pages, 4 figures. Discussion on the effect of the eccentricity uncertainty has been added
Investigation of X-ray induced radiation damage at the Si-SiO2 interface of silicon sensors for the European XFEL
Creators: name: Zhang, Jiaguo
name: Fretwurst, Eckhart
name: Klanner, Robert
name: Pintilie, Ioana
name: Schwandt, Joern
name: Turcato, Monica
Publisher: name: arXiv
Year: 2012
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Experiments at the European X-ray Free Electron Laser (XFEL) require silicon pixel sensors which can withstand X-ray doses up to 1 GGy. For the investigation of X-ray radiation damage up to these high doses, MOS capacitors and gate-controlled diodes built on high resistivity n-doped silicon with crystal orientations <100> and <111> produced by two vendors, CiS and Hamamatsu, have been irradiated with 12 keV X-rays at the DESY DORIS III synchrotron light source. Using capacitance/conductance-voltage, current-voltage and thermal dielectric relaxation current measurements, the surface densities of oxide charges and interface traps at the Si-SiO2 interface, and the surface-current densities have been determined as function of dose. Results indicate that the dose dependence of the surface density of oxide charges and the surface-current density depend on the crystal orientation and producer. In addition, the influence of the voltage applied to the gates of the MOS capacitor and the gate-controlled diode during X-ray irradiation on the surface density of oxide charges and the surface-current density has been investigated at doses of 100 kGy and 100 MGy. It is found that both strongly depend on the gate voltage if the electric field in the oxide points from the surface of the SiO2 to the Si-SiO2 interface. Finally, annealing studies have been performed at 60 and 80 degree C on MOS capacitors and gate-controlled diodes irradiated to 5 MGy and the annealing kinetics of oxide charges and surface current determined.
description: 10 pages, 6 figures, 3 tables
Decorrelation of the static and dynamic length scales in hard-sphere glass-formers
Creators: name: Charbonneau, Patrick
name: Tarjus, Gilles
Publisher: name: arXiv
Year: 2012
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We show that in the equilibrium phase of glass-forming hard-sphere fluids in three dimensions, the static length scales tentatively associated with the dynamical slowdown and the dynamical length characterizing spatial heterogeneities in the dynamics unambiguously decorrelate. The former grow at a much slower rate than the latter when density increases. This observation is valid for the dynamical range that is accessible to computer simulations, which roughly corresponds to that of colloidal experiments. We also find that in this same range, no one-to-one correspondence between relaxation time and point-to-set correlation length exists. These results point to the coexistence of several relaxation mechanisms in the accessible dynamical regime of three-dimensional hard-sphere glass formers.
description: 8 pages, 7 figures
P. Desportes (avec la collaboration de P. Bony, É. Bouyé, P. Demouy, C. Jeudy, B. Kurmann-Schwarz, H. Millet, P. Montaubin, H. Müller, V. Tabbagh), Fasti Ecclesiae Gallicanae: Répertoire prosopographique des évêques, dignitaires et chanoines des diocèses de france de 1200 a 1500. T. III: Diocèse de Reims, 1998
Creators: name: Falkenstein, L.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 1 (2001)
Hidden breakpoints in genome alignments
Creators: name: Kehr, Birte
name: Reinert, Knut
name: Darling, Aaron E.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Genomics (q-bio.GN)
subject: FOS: Biological sciences

description: During the course of evolution, an organism's genome can undergo changes that affect the large-scale structure of the genome. These changes include gene gain, loss, duplication, chromosome fusion, fission, and rearrangement. When gene gain and loss occurs in addition to other types of rearrangement, breakpoints of rearrangement can exist that are only detectable by comparison of three or more genomes. An arbitrarily large number of these "hidden" breakpoints can exist among genomes that exhibit no rearrangements in pairwise comparisons. We present an extension of the multichromosomal breakpoint median problem to genomes that have undergone gene gain and loss. We then demonstrate that the median distance among three genomes can be used to calculate a lower bound on the number of hidden breakpoints present. We provide an implementation of this calculation including the median distance, along with some practical improvements on the time complexity of the underlying algorithm. We apply our approach to measure the abundance of hidden breakpoints in simulated data sets under a wide range of evolutionary scenarios. We demonstrate that in simulations the hidden breakpoint counts depend strongly on relative rates of inversion and gene gain/loss. Finally we apply current multiple genome aligners to the simulated genomes, and show that all aligners introduce a high degree of error in hidden breakpoint counts, and that this error grows with evolutionary distance in the simulation. Our results suggest that hidden breakpoint error may be pervasive in genome alignments.
description: 13 pages, 4 figures
E. Pibiri, Sous la férule du maître. Les écoles d'Yverdon (14e–16e siècles). Avec une étude de P. Dubuis, »Les écoles en Suisse romande à la fin du Moyen Âge: quelques jalons«, 1998
Creators: name: Angers, D.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 1 (2001)
Quantum and classical dissipation of charged particles
Creators: name: Ibarra-Sierra, V. G.
name: Anzaldo-Meneses, A.
name: Cardoso, J. L.
name: Hernández-Saldaña, H.
name: Kunold, A.
name: Roa-Neri, J. A. E.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A Hamiltonian approach is presented to study the two dimensional motion of damped electric charges in time dependent electromagnetic fields. The classical and the corresponding quantum mechanical problems are solved for particular cases using canonical transformations applied to Hamiltonians for a particle with variable mass. The Green's function is constructed and, from it, the motion of a Gaussian wave packet is studied in detail.
description: 14 pages, 4 figures, misprints and figures corrected
A semi-adelic Kuznetsov formula over number fields
Creators: name: Maga, Péter
Publisher: name: arXiv
Year: 2012
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11F30

description: In these notes, we prove a semi-adelic version of the Kuznetsov formula over arbitrary number fields. The extent is the set of those automorphic vectors which are not necessarily spherical in the archimedean aspect and a class of weight functions which is important for applications.
description: 23 pages
Neoperla coosa Smith & Stark
Creators: name: DeWalt, R. Edward
name: Grubbs, Scott A.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperla
Neoperla coosa

description: Neoperla coosa Smith & Stark. This species was described from central Alabama and has subsequently been collected from Tennessee (DeWalt & Heinold 2005) and North Carolina (Lenat et al. 2009). We present a single record from southern Indiana. IN, Harrison Co., Blue River, 1 mi E White Cloud, [38.229, -86.226], 8/23/1973, A.V. Provonsha, K. Black, 5♀ (BYU).
description: Published as part of DeWalt, R. Edward & Grubbs, Scott A., 2011, Updates To The Stonefly Fauna Of Illinois And Indiana, pp. 31-50 in Illiesia 7 (3) on page 43, DOI: 10.5281/zenodo.4760399
description: {"references": ["Lenat, D., R. E. Zuellig, B. C. Kondratieff, & S. R. Beaty. 2009. Distribution of Neoperla (Plecoptera: Perlidae) in North Carolina, with new state records for three species. Illiesia, 5: 164 - 168."]}
Do intergalactic magnetic fields imply an open universe?
Creators: name: Barrow, J. D.
name: Tsagas, C. G.
name: Yamamoto, K.
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The detection of magnetic fields at high redshifts, and in empty intergalactic space, support the idea that cosmic magnetism has a primordial origin. Assuming that Maxwellian electromagnetism and general relativity hold, and without introducing any `new' physics, we show how the observed magnetic fields can easily survive cosmological evolution from the inflationary era in a marginally open Friedmann universe but fail to do so, by a very wide margin, in a flat or a marginally closed universe. Magnetic fields evolve very differently in open and closed Friedmann models. The existence of significant magnetic fields in the universe today, that require primordial seeding, may therefore provide strong evidence that the universe is marginally open rather than marginally closed.
description: Minor changes, published version
V. Lind, Selbstmord in der Frühen Neuzeit. Diskurs, Lebenswelt und kultureller Wandel am Beispiel der Herzogtümer Schleswig-Holstein, 1999
Creators: name: Frijhoff, W.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 2 (2001)
Electrometry Using Coherent Exchange Oscillations in a Singlet-Triplet-Qubit
Creators: name: Dial, O. E.
name: Shulman, M. D.
name: Harvey, S. P.
name: Bluhm, H.
name: Umansky, V.
name: Yacoby, A.
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: Two level systems that can be reliably controlled and measured hold promise in both metrology and as qubits for quantum information science (QIS). When prepared in a superposition of two states and allowed to evolve freely, the state of the system precesses with a frequency proportional to the splitting between the states. In QIS,this precession forms the basis for universal control of the qubit,and in metrology the frequency of the precession provides a sensitive measurement of the splitting. However, on a timescale of the coherence time, $T_2$, the qubit loses its quantum information due to interactions with its noisy environment, causing qubit oscillations to decay and setting a limit on the fidelity of quantum control and the precision of qubit-based measurements. Understanding how the qubit couples to its environment and the dynamics of the noise in the environment are therefore key to effective QIS experiments and metrology. Here we show measurements of the level splitting and dephasing due to voltage noise of a GaAs singlet-triplet qubit during exchange oscillations. Using free evolution and Hahn echo experiments we probe the low frequency and high frequency environmental fluctuations, respectively. The measured fluctuations at high frequencies are small, allowing the qubit to be used as a charge sensor with a sensitivity of $2 \times 10^{-8} e/\sqrt{\mathrm{Hz}}$, two orders of magnitude better than the quantum limit for an RF single electron transistor (RF-SET). We find that the dephasing is due to non-Markovian voltage fluctuations in both regimes and exhibits an unexpected temperature dependence. Based on these measurements we provide recommendations for improving $T_2$ in future experiments, allowing for higher fidelity operations and improved charge sensitivity.
Belief Propagation Reconstruction for Discrete Tomography
Creators: name: Gouillart, Emmanuelle
name: Krzakala, Florent
name: Mezard, Marc
name: Zdeborová, Lenka
Publisher: name: arXiv
Year: 2012
Subjects: subject: Numerical Analysis (math.NA)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Information Theory (cs.IT)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We consider the reconstruction of a two-dimensional discrete image from a set of tomographic measurements corresponding to the Radon projection. Assuming that the image has a structure where neighbouring pixels have a larger probability to take the same value, we follow a Bayesian approach and introduce a fast message-passing reconstruction algorithm based on belief propagation. For numerical results, we specialize to the case of binary tomography. We test the algorithm on binary synthetic images with different length scales and compare our results against a more usual convex optimization approach. We investigate the reconstruction error as a function of the number of tomographic measurements, corresponding to the number of projection angles. The belief propagation algorithm turns out to be more efficient than the convex-optimization algorithm, both in terms of recovery bounds for noise-free projections, and in terms of reconstruction quality when moderate Gaussian noise is added to the projections.
Toolkit briefing (Italian/Italiano)
Creators: name: ySKILLS
Publisher: name: Zenodo
Year: 2023

description: I ricercatori di ySKILLS hanno il piacere di introdurvi a questa risorsa progettata per introdurre a bambini e adolescente il tema delle competenze digitali. Questa raccolta di risorse e attività è il frutto delle ricerche condotte nell'ambito del progetto Horizon ySKILLS. Più informazioni sul progetto sono disponibili sul sito: www.yskills.eu. 
Questo documento contiene un briefing sulle attività e gli aspetti pratici del toolkit.
Three-dimensional Topside Ionospheric Model and GNSS Data from LEO Satellites
Creators: name: Han, Yi
Publisher: name: Zenodo
Year: 2022

description: Here are three-dimensional topside ionospheric models based on machine learning methods and GNSS observations from LEO satellites. The trained models contain two files, including XGBoost-GA and NN-GA. It can provide topside TEC (450-830 km) with the given features. Besides, we also give the access to download GNSS observations from LEO satellites in this repository, and the downloaded data is also displayed in the folder.
Detection of Sugar-Lectin Interactions by Multivalent Dendritic Sugar Functionalized Single-Walled Carbon Nanotubes
Creators: name: Vasu, K. S.
name: Naresh, K.
name: Bagul, R. S.
name: Jayaraman, N.
name: Sood, A. K.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We show that single walled carbon nanotubes (SWNT) decorated with sugar functionalized poly (propyl ether imine) (PETIM) dendrimer is a very sensitive platform to quantitatively detect carbohydrate recognizing proteins, namely, lectins. The changes in electrical conductivity of SWNT in field effect transistor device due to carbohydrate - protein interactions form the basis of present study. The mannose sugar attached PETIM dendrimers undergo charge - transfer interactions with the SWNT. The changes in the conductance of the dendritic sugar functionalized SWNT after addition of lectins in varying concentrations were found to follow the Langmuir type isotherm, giving the concanavalin A (Con A) - mannose affinity constant to be 8.5 x 106 M-1. The increase in the device conductance observed after adding 10 nM of Con A is same as after adding 20 \muM of a non - specific lectin peanut agglutinin, showing the high specificity of the Con A - mannose interactions. The specificity of sugar-lectin interactions was characterized further by observing significant shifts in Raman modes of the SWNT.
description: 12 pages, 3 figures
N. Franz, B.-S. Grewe, M. Knauff (Hg.), Landgemeinden im Übergang zum modernen Staat. Vergleichende Mikrostudien im linksrheinischen Raum, 1999
Creators: name: Boehler, J.-M.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 2 (2001)
Laomenes cornutus
Creators: name: Marin, Ivan
name: Chan, Tin-Yam
name: Okuno, Junji
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Palaemonidae
Laomenes
Laomenes cornutus

description: Laomenes cornutus (Borradaile, 1915) (Figs. 6, 8d) Periclimenes cornutus Borradaile, 1915: 211 [type locality: Malé Atoll, Maldive Islands]. Material examined. 1 male (pcl. 1.8 mm) (NTOU M00954), Philippines, PANGLAO 2004, stn. R38, Pamilacan Island, 9°29.4ʹN, 123°56.0ʹE, scuba diving, 6–37 m, 11 June 2004; 2 juveniles (NTOU M00997), Philippines, PANGLAO 2004, stn. R75, Panglao Island, west of Pontod, 9°32.8ʹN, 123°42.1ʹE, scuba diving, 3–35 m, 3 July 2004. Colouration. Body generally blackish-brown and bearing row of small yellowish-white dots along lateral margin of carapace and abdomen (Fig. 8d). Pereiopods and eyes also with yellowish-white dots. Host. Unknown. Probably associated with dark coloured species feather star of the genus Comanthus (Echinodermata, Crinoidea, Comasteridae). Distribution. The species is known from the Maldive Islands (type locality; Borradaile 1915, 1917; Tchesunov et al. 1989 as “ Periclimenes amboinensis ”; Marin 2009) and now the Philippines (present study). Remarks. The present specimens agree well with the previous descriptions of this rarely collected species (Bruce 1978; Tchesunov et al. 1989, as “ Periclimenes amboinensis ”; Marin, 2009). The distinguishing characters of L. cornutus are relatively smaller body size, short and stout eyestalk, chela of pereiopod II with stout cylindrical palm and characteristic structure of the dactylus of pereiopod III (see Marin 2009).
description: Published as part of Marin, Ivan, Chan, Tin-Yam & Okuno, Junji, 2012, Crinoid-associated pontoniine shrimps of the genus Laomenes Clark, 1919 (Decapoda, Caridea, Palaemonidae) from PANGLAO 2004 and KUMEJIMA 2009 Expeditions, with description of two new species, pp. 103-114 in Zootaxa 3367 (1) on page 111, DOI: 10.11646/zootaxa.3367.1.10, http://zenodo.org/record/5251928
description: {"references": ["Borradaile, L. A. (1915) Notes on Carides. Annals and Magazine of Natural History, ser. 8, 15, 205 - 213.", "Borradaile, L. A. (1917) On the Pontoniinae. The Percy Sladen Trust Expedition to the Indian Ocean in 1905, under the leadership of Mr. J. Stanley Gardiner. Transactions of the Linnean Society of London, Zoology, 17 (2), 323 - 396.", "Tchesunov, A. V., Britayev, T. A., Larionov, V. V., Khodkina, I. V. & Tzetlin, A. B. (1989) Notes on commensals of some crinoids from Maldives coral reefs. In: Sveshnikov, V. A. (ed.), Symbiosis in Marine Animals. Moscow, pp. 166 - 191.", "Marin, I. (2009) Crinoid-associated shrimps of the genus Laomenes A. H. Clark, 1919 (Caridea: Palaemonidae: Pontoniinae): new species and probable diversity. Zootaxa, 1971, 1 - 49."]}
The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
Creators: name: Kang, Xi
name: Macciò, Andrea V.
name: Dutton, Aaron A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this paper we combine high resolution N-body simulations with a semi analytical model of galaxy formation to study the effects of a possible Warm Dark Matter (WDM) component on the observable properties of galaxies. We compare three WDM models with a dark matter mass of 0.5, 0.75 and 2.0 keV, with the standard Cold Dark Matter case. For a fixed set of parameters describing the baryonic physics the WDM models predict less galaxies at low (stellar) masses, as expected due to the suppression of power on small scales, while no substantial difference is found at the high mass end. However these differences in the stellar mass function, vanish when different set of parameters are used to describe the (largely unknown) galaxy formation processes. We show that is possible to break this degeneracy between DM properties and the parameterization of baryonic physics by combining observations on the stellar mass function with the Tully-Fisher relation (the relation between stellar mass and the rotation velocity at large galactic radii as probed by resolved HI rotation curves). WDM models with a too warm candidate (m<0.75 keV) cannot simultaneously reproduce the stellar mass function and the Tully-Fisher relation. We conclude that accurate measurements of the galaxy stellar mass function and the link between galaxies and dark matter haloes down to the very low-mass end can give very tight constraints on the nature of DM candidates.
description: 8 pages, 5 figures, minor changes, accepted for publication on ApJ
J. Ojala, Tehokasta liiketoimintaa Pohjanwaan pikkukaupungeissa Purjemerenkulun kannattavuus ja tuottavuus 1700-1800-luvulla. [Efficient business activity in small Ostrobothnian towns Profitability and productivity of Shipping by Sail during the Eighteenth and Nineteenth Century]. Suomen Historiallinen Seura, 1999
Creators: name: Burger, P.-F.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 28 Nr. 2 (2001)
Opening the Open: Role of Article Processing Charges and Publication Fee in Opening Knowledge from Sub-Sahara Africa
Creators: name: Hamisu Abdu, Alkasim
Publisher: name: Zenodo
Year: 2023

description: Alkasim Hamisu Abdu presented "Opening the Open: Role of Article Processing Charges and Publication Fee in Opening Knowledge from Sub-Sahara Africa" during the 2023 Annual Forum for Open Research online.
Répertoire des cartulaires français. Provinces ecclésiastiques d'Aix, Arles, Embrun, Vienne. Diocèse de Tarentaise, publié par Isabelle Vérité, Anne-Marie Legras, Caroline Bourlet, Anne Dufour avec la collaboration d'Olivier Guyotjeannin, Anne-Marie Hayez
Creators: name: Weiss, S.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 32 Nr. 1 (2005)
Laomenes holthuisi Marin & Okuno 2010
Creators: name: Marin, Ivan
name: Chan, Tin-Yam
name: Okuno, Junji
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Palaemonidae
Laomenes
Laomenes holthuisi

description: Laomenes holthuisi Marin & Okuno, 2010 (Figs. 7, 8c) Laomenes holthuisi Marin & Okuno, 2010: 462, figs. 1–6 [type locality: Izu Islands, southern Japan]. Material examined. 1 ovigerous female (pcl 2.7 mm), 1 male (pcl 2.2 mm) (NTOU M00998), Pacific Ocean, Japan, Ryukyu Islands, Kume Island, KUMEJIMA 2009 Expedition, stn. Dive 12, Torishima Islet, 26°19.683ʹN, 126°44.625ʹE, scuba diving, <20 m, 12 November 2009. Colouration. Body blackish and distributed with large irregular yellowish white patches (Fig. 8c). Host. The present specimens were collected from an unidentified comatulid feather star. Laomenes holthuisi is known as a symbiont of yellow-black-green comasterid feather stars of the genus Comanthina A.H. Clark, 1909 (Echinodermata, Crinoidea, Comasteridae) such as C. nobilis (Carpenter, 1884) and C. schlegelii (Carpenter, 1881) (see Marin & Okuno 2010). Distribution. This species is known only from Japan in the Izu Islands (type locality; Marin & Okuno 2010) and the Ryukyu Islands, Japan (present study). Remarks. The present specimens agree well with the original description of the species provided by Marin & Okuno (2010).
description: Published as part of Marin, Ivan, Chan, Tin-Yam & Okuno, Junji, 2012, Crinoid-associated pontoniine shrimps of the genus Laomenes Clark, 1919 (Decapoda, Caridea, Palaemonidae) from PANGLAO 2004 and KUMEJIMA 2009 Expeditions, with description of two new species, pp. 103-114 in Zootaxa 3367 (1) on page 114, DOI: 10.11646/zootaxa.3367.1.10, http://zenodo.org/record/5251928
description: {"references": ["Marin, I. & Okuno, J. (2010) Laomenes holthuisi, sp. nov., a new crinoid-associated pontoniine shrimp from Izu Islands, Japan, with some remarks on Japanese species of the genus Laomenes Clark, 1915. In: Fransen, C., De Grave, S. & Ng, P. K. L. (eds.), Studies on Malacostraca: Lipke Bijdeley Holthuis Memorial Volume. Crustaceana Monographs, 14, 461 - 472."]}
The Extragalactic Background Light and the Gamma-ray Opacity of the Universe
Creators: name: Dwek, Eli
name: Krennrich, Frank
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The extragalactic background light (EBL) is one of the fundamental observational quantities in cosmology. All energy releases from resolved and unresolved extragalactic sources, and the light from any truly diffuse background, excluding the cosmic microwave background (CMB), contribute to its intensity and spectral energy distribution. It therefore plays a crucial role in cosmological tests for the formation and evolution of stellar objects and galaxies, and for setting limits on exotic energy releases in the universe. The EBL also plays an important role in the propagation of very high energy gamma-rays which are attenuated en route to Earth by pair producing gamma-gamma interactions with the EBL and CMB. The EBL affects the spectrum of the sources, predominantly blazars, in the ~10 GeV to 10 TeV energy regime. Knowledge of the EBL intensity and spectrum will allow the determination of the intrinsic blazar spectrum in a crucial energy regime that can be used to test particle acceleration mechanisms and VHE gamma-ray production models. Conversely, knowledge of the intrinsic gamma-ray spectrum and the detection of blazars at increasingly higher redshifts will set strong limits on the EBL and its evolution. This paper reviews the latest developments in the determination of the EBL and its impact on the current understanding of the origin and production mechanisms of gamma-rays in blazars, and on energy releases in the universe. The review concludes with a summary and future directions in Cherenkov Telescope Array techniques and in infrared ground-based and space observatories that will greatly improve our knowledge of the EBL and the origin and production of very high energy gamma-rays.
description: To be published in the special Cherenkov Telescope Array issue of Astroparticle Physics. 55 pages including 15 figures (excluding 42 pages of references)
Gate-induced carrier density modulation in bulk graphene: Theories and electrostatic simulation using Matlab pdetool
Creators: name: Liu, Ming-Hao
Publisher: name: arXiv
Year: 2012
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: This article aims at providing a self-contained introduction to theoretical modeling of gate-induced carrier density in graphene sheets. For this, relevant theories are introduced, namely, classical capacitance model (CCM), self-consistent Poisson-Dirac method (PDM), and quantum capacitance model (QCM). The usage of Matlab pdetool is also briefly introduced, pointing out the least knowledge required for using this tool to solve the present electrostatic problem. Results based on the three approaches are compared, showing that the quantum correction, which is not considered by the CCM but by the other two, plays a role only when the metal gate is exceedingly close to the graphene sheet, and that the exactly solvable QCM works equally well as the self-consistent PDM. Practical examples corresponding to realistic experimental conditions for generating graphene pnp junctions and superlattices, as well as how a background potential linear in position can be achieved in graphene, are shown to illustrate the applicability of the introduced methods. Furthermore, by treating metal contacts in the same way, the last example shows that the PDM and the QCM are able to resolve the contact-induced doping and screening potential, well agreeing with the previous first-principles studies.
description: 15 pages, 8 figures, significant revision with section 4.5 about contact doping newly added
Neoperla gaufini Stark & Baumann
Creators: name: DeWalt, R. Edward
name: Grubbs, Scott A.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperla
Neoperla gaufini

description: Neoperla gaufini Stark & Baumann. This species has a very limited distribution in Indiana, Kentucky, and Ohio (Stark & Baumann 1978; Stark 2004). Grubbs (2004) listed it from four southern Indiana counties. We present three new records. IN, Brown Co., Yellowwood Lake, Yellowwood State Forest, [39.18118, -86.35254], 6/20/1946, E. Mockford, 2♀ (CNC); Perry Co. Poison Creek, 5 mi NW Derby, [38.04836, -86.60128], 8/1/1975, A.V. Provonsha, M. Minno, ♀ (PERC); Switzerland Co., Indian Creek, 2 mi W Mt. Sterling, [38.79751, -85.09323], 7/18/1972, A.V. Provonsha, E. Levine, ♂ (PERC).
description: Published as part of DeWalt, R. Edward & Grubbs, Scott A., 2011, Updates To The Stonefly Fauna Of Illinois And Indiana, pp. 31-50 in Illiesia 7 (3) on page 43, DOI: 10.5281/zenodo.4760399
description: {"references": ["Stark, B. P. 2004. Perlidae (The Stones). Pages 61 - 148. In: Stark, B. P. & B. J. Armitage (editors). The stoneflies (Plecoptera) of eastern North America. Volume II. Chloroperlidae, Perlidae, and Perlodidae (Perlodinae). Bulletin of the Ohio Biological Survey, New Series, Volume 14. Ohio Biological Society, Columbus, Ohio. 192 pp.", "Grubbs, S. A. 2004. Studies on Indiana stoneflies (Plecoptera), with an annotated and revised state checklist. Proceedings of the Entomological Society of Washington, 106: 865 - 876."]}
Constraints on the Universe as a Numerical Simulation
Creators: name: Beane, Silas R.
name: Davoudi, Zohreh
name: Savage, Martin J.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Observable consequences of the hypothesis that the observed universe is a numerical simulation performed on a cubic space-time lattice or grid are explored. The simulation scenario is first motivated by extrapolating current trends in computational resource requirements for lattice QCD into the future. Using the historical development of lattice gauge theory technology as a guide, we assume that our universe is an early numerical simulation with unimproved Wilson fermion discretization and investigate potentially-observable consequences. Among the observables that are considered are the muon g-2 and the current differences between determinations of alpha, but the most stringent bound on the inverse lattice spacing of the universe, b^(-1) >~ 10^(11) GeV, is derived from the high-energy cut off of the cosmic ray spectrum. The numerical simulation scenario could reveal itself in the distributions of the highest energy cosmic rays exhibiting a degree of rotational symmetry breaking that reflects the structure of the underlying lattice.
description: 14 pages, 3 figures
The Rossiter-McLaughlin effect for exomoons or binary planets
Creators: name: Zhuang, Quntao
name: Gao, Xun
name: Yu, Qingjuan
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper we study possible signatures of binary planets or exomoons on the Rossiter-McLaughlin (R-M) effect. Our analyses show that the R-M effect for a binary planet or exomoon during its complete transit phase can be divided into two parts. The first is the conventional one similar to the R-M effect from the transit of a single planet, of which the mass and the projected area are the combinations of the binary components; and the second is caused by the orbital rotation of the binary components, which may add a sine- or linear-mode deviation to the stellar radial velocity curve. We find that the latter effect can be up to several or several ten m/s. By doing numerical simulations as well as analytical analyses, we illustrate that the distribution and dispersion of the latter effects obtained from multiple transit events can be used to constrain the dynamical configuration of the binary planet, such as, how the inner orbit of the binary planet is inclined to its orbit rotating around the central star. We find that the signatures caused by the orbital rotation of the binary components are more likely to be revealed if the two components of binary planet have different masses and mass densities, especially if the heavy one has a high mass density and the light one has a low density. Similar signature on the R-M effect may also be revealed in a hierarchical triple star system containing a dark compact binary and a tertiary star.
description: 30 pages, 9 figures
E. Hlawitschka, Konradiner-Genealogie, unstatthafte Verwandtenehen und spätottonisch-frühsalische Thronbesetzungspraxis. Ein Rückblick auf 25 Jahre Forschungsdisput, 2003
Creators: name: Jackman, D. C.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 32 Nr. 1 (2005)
Strongly Interacting Two-Dimensional Bose Gases
Creators: name: Ha, Li-Chung
name: Hung, Chen-Lung
name: Zhang, Xibo
name: Eismann, Ulrich
name: Tung, Shih-Kuang
name: Chin, Cheng
Publisher: name: arXiv
Year: 2012
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We prepare and study strongly interacting two-dimensional Bose gases in the superfluid, the classical Berezinskii-Kosterlitz-Thouless (BKT) transition, and the vacuum-to-superfluid quantum critical regimes. A wide range of the two-body interaction strength 0.05 < g < 3 is covered by tuning the scattering length and by loading the sample into an optical lattice. Based on the equations of state measurements, we extract the coupling constants as well as critical thermodynamic quantities in different regimes. In the superfluid and the BKT transition regimes, the extracted coupling constants show significant down-shifts from the mean-field and perturbation calculations when g approaches or exceeds one. In the BKT and the quantum critical regimes, all measured thermodynamic quantities show logarithmic dependence on the interaction strength, a tendency confirmed by the extended classical-field and renormalization calculations.
description: 5 pages, 4 figures
Das Necrolog des Klosters Michelsberg in Bamberg, hg. von J. Nospickel, mit Beiträgen von D. Geuenich, E. Hochholzer und J. Wollasch, 2004
Creators: name: Lemaitre, J.-L.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 32 Nr. 1 (2005)
A multiparameter Garsia-Rodemich-Rumsey inequality and some applications
Creators: name: Hu, Yaozhong
name: Le, Khoa
Publisher: name: arXiv
Year: 2012
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: We extend the classical Garsia-Rodemich-Rumsey inequality to the multiparameter situation. The new inequality is applied to obtain some joint Hölder continuity along the rectangles for fractional Brownian fields $W(t, x)$ and for the solution $u(t, y)$ of stochastic heat equation with additive white noise.
W. Harms, A. Messerli (Hg.), in Verbindung mit Frieder von Ammon und Nikola von Merveldt, Wahrnehmungsgeschichte und Wissensdiskurs im illustrierten Flugblatt der Frühen Neuzeit (1450–1700), 2002
Creators: name: Genton, F.
Publisher: name: Francia
Year: 2019

description: Francia, Bd. 32 Nr. 2 (2005)
Curvature Perturbations from a Massive Vector Curvaton
Creators: name: Namba, Ryo
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study a ghost-free model of massive vector curvaton proposed in the literature, where the quick decrease of the vector background expectation value is avoided by a suitable choice of kinetic and mass functions. The curvaton perturbations of this model have been so far computed assuming that these functions are external classical quantities, and it was found that some special time evolution of these functions leads to scale invariant and statistically isotropic perturbations of the vector curvaton. However, external functions should be understood as originating from the expectation value of some additional field. Since these functions need to present a non-trivial evolution during inflation, the field cannot be trivially integrated out, and, in particular, its perturbations need to be included in the computation. We do so in a minimal implementation of the mechanism, where the additional field is identified with the inflaton. We show that, except for a narrow window of model parameters, the interaction with this field generally causes the curvature perturbations to violate statistical isotropy beyond the observational limit.
description: 23 pages, 5 figures, references added and sorted, a footnote added
The eNanoMapper Ontology v9.0: Semi-automated and Community-based Ontology Development
Creators: name: Acosta, Javier Millán
name: Willighagen, Egon
Publisher: name: Zenodo
Year: 2023
Subjects: nanosafety
ontology
nanomaterial safety

description: The release of version 9.0 marks the transition of the ontology build to a GitHub Actions-based system. Since the build actions can be (programmatically) monitored, the new development cycle allows downstream users, like other NanoSafety cluster projects, to quickly react to new releases and integrate them into their own workflows.With the continuous discussion on domain terminology and knowledge representation ever changing together with our understanding of the chemistry and biology of NanoSafety, the eNanoMapper ontology will keep being supported and expanded with new community requested classes and properties in future releases to serve as a data curation completeness standard in the domain.
description: {"references": ["Hastings, J., Jeliazkova, N., Owen, G., Tsiliki, G., Munteanu, C. R., Steinbeck, C., & Willighagen, E. (2015). eNanoMapper: Harnessing ontologies to enable data integration for nanomaterial risk assessment. Journal of Biomedical Semantics, 6(1). https://doi.org/10.1186/s13326-015-0005-5", "Hastings, J., Jeliazkova, N., Owen, G., Tsiliki, G., Munteanu, C. R., Steinbeck, C., & Willighagen, E. & Millan Acosta, J. (2023). eNanoMapper 9.0 (9.0). Zenodo. https://doi.org/10.5281/zenodo.7503729", "https://github.com/enanomapper/ontologies", "Matentzoglu, N., Goutte-Gattat, D., Tan, S. Z. K., Balhoff, J. P., Carbon, S., Caron, A. R., Duncan, W. D., Flack, J. E., Haendel, M., Harris, N. L., Hogan, W. R., Hoyt, C. T., Jackson, R. C., Kim, H., Kir, H., Larralde, M., McMurry, J. A., Overton, J. A., Peters, B., ... Osumi-Sutherland, D. (2022). Ontology Development Kit: A toolkit for building, maintaining and standardizing biomedical ontologies. Database, 2022, baac087. https://doi.org/10.1093/database/baac087", "Jackson, R.C., Balhoff, J.P., Douglass, E. et al. ROBOT: A Tool for Automating Ontology Workflows. BMC Bioinformatics 20, 407 (2019). https://doi.org/10.1186/s12859- 019-3002-3"]}
Vertical loop nodes in iron-based superconductors
Creators: name: Khodas, M.
name: Chubukov, A. V.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider Fe-based superconductors with s^{+-} gap with accidental nodes on electron pockets. We analyze how the gap structure changes if we include into the consideration the hybridization between the two electron pockets (the inter-pocket hopping term with momentum (pi,pi,pi). We derive the hybridization term and relate it to the absence of inversion symmetry in the Fe-plane because of two non-equivalent locations of pnictogen (chalcogen) above and below the plane. We find that the hybridization tends to eliminate the nodes -- as it increases, the pairs of neighboring nodes approach each other, merge and disappear once the hybridization exceeds a certain threshold. The nodes disappear first around k_z =pi/2, and vertical line nodes split into two vertical loops centered at k_z =0 and k_z = pi. We also show that the hybridization moves the nodes along the loops away from the normal state Fermi surfaces. This creates a subset of k-points at which the peak in the spectral function does not shift as the system enters into a superconducting state ("no-shift" lines). These "no-shift" lines evolve with increasing hybridization in highly non-trivial manner and eventually form horizontal loops in (k_x, k_y) plane, surrounding the nodes. Both vertical line nodes and horizontal "no-shift" loops surrounding them should be detectable in photoemission experiments.
description: 16 pages, 13 figures. References reordered, typos corrected