cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Rethinking Conceptions of Borders in the Greater Mekong Subregion: An Interview With Chayan Vaddhanabhuti (RCSD)
Creators: name: Kittisenee, Napakadol
Publisher: name: Austrian Journal of South-East Asian Studies
Year: 2011

description: Dr. Chayan Vaddhanabhuti is Director of the Regional Centre for Social Science and Sustainable Development (RCSD), Thailand. The RCSD was established in 1998 at the Faculty of Social Sciences, Chiang Mai University, in response to the need for integration of social science and natural science knowledge in order to gain a better understanding of sustainable development in upper Mainland South-East Asia. Chayan Vaddhanabhuti has long been dedicated to the fi eld of social sciences, development issues, and engaged himself extensively with ethnic groups both within Thailand and beyond. In this interview he introduces the work of RSCD and discusses the changing perceptions of the concept of ‘border’ in the context of Thailand and the Greater Mekong Subregion.
description: Austrian Journal of South-East Asian Studies, Vol 4 No 2 (2011): Borderlands & Border Studies
Ritorno alle cose, amore per le cose. Lo spazio etico della letteratura
Creators: name: Menzio, Pino
Publisher: name: Università degli Studi di Milano
Year: 2014
Subjects: Filosofia della letteratura; etica della letteratura; pietas; nuovo realismo

description: Di recente si è registrato, in ambito filosofico, un ritorno di interesse per l’oggettività. Le sue manifestazioni più significative si richiamano a due nuclei teorici fondamentali: l’attenzione per l’esperienza artistica e letteraria, e la convinzione che da essa derivi una precisa posizione etica. Ciò non accade nelle riprese del pensiero di Searle note come «nuovo realismo», il cui rapporto con la letteratura è particolarmente problematico.
description: ENTHYMEMA, No 10 (2014)
Additional file 1 of Exploring relationships between drought and epidemic cholera in Africa using generalised linear models
Creators: name: Charnley, Gina E. C.
name: Kelman, Ilan
name: Green, Nathan
name: Hinsley, Wes
name: Gaythorpe, Katy A. M.
name: Murray, Kris A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences

description: Additional file 1. Additional details about the data and models used here.
Microscopic origin of the excellent thermoelectric performance in n-doped SnSe
Creators: name: Chaves, Anderson S.
name: Larson, Daniel T.
name: Kaxiras, Efthimios
name: Antonelli, Alex
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Excellent thermoelectric performance in the out-of-layer n-doped SnSe has been observed experimentally (Chang et al., Science 360, 778-783 (2018)). However, a first-principles investigation of the dominant scattering mechanisms governing all thermoelectric transport properties is lacking. In the present work, by applying extensive first-principles calculations of electron-phonon coupling associated with the calculation of the scattering by ionized impurities, we investigate the reasons behind the superior figure of merit as well as the enhancement of zT above 600 K in n-doped out-of-layer SnSe, as compared to p-doped SnSe with similar carrier densities. For the n-doped case, the relaxation time is dominated by ionized impurity scattering and increases with temperature, a feature that maintains the power factor at high values at higher temperatures and simultaneously causes the carrier thermal conductivity at zero electric current (k_el) to decrease faster for higher temperatures, leading to an ultrahigh-zT = 3.1 at 807 K. We rationalize the roles played by k_el and k^0 (the thermal conductivity due to carrier transport under isoelectrochemical conditions) in the determination of zT. Our results show the ratio between k^0 and the lattice thermal conductivity indeed corresponds to the upper limit for zT, whereas the difference between calculated zT and the upper limit is proportional to k_el.
description: 12 pages, 5 figures
A Universal Decline Law of Classical Novae. III. GQ Mus 1983
Creators: name: Hachisu, Izumi
name: Kato, Mariko
name: Cassatella, Angelo
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a unified model of infrared (IR), optical, ultraviolet (UV), and X-ray light curves for the 1983 outburst of GQ Muscae (Nova Muscae 1983) and estimate its white dwarf (WD) mass. Based on an optically thick wind model of nova outbursts, we model the optical and IR light curves with free-free emission, and the UV 1455 Åand supersoft X-ray light curves with blackbody emission. The best fit model that reproduces simultaneously the IR, optical, UV 1455 Å, and supersoft X-ray observations is a 0.7 \pm 0.05 M_\sun WD for an assumed chemical composition of the envelope, X=0.35-0.55, X_{CNO} =0.2-0.35, and Z = 0.02, by mass weight. The mass lost by the wind is estimated to be ΔM_{wind} \sim 2 \times 10^{-5} M_\sun. We provide a new determination of the reddening, E(B-V) = 0.55 \pm 0.05, and of the distance, \sim 5 kpc. Finally, we discuss the strong UV flash that took place on JD 2,445,499 (151 days after the outburst).
description: to appear in ApJ, 17 pages including 20 figures
Depth estimation of the Large and Small Magellanic Clouds
Creators: name: Subramanian, Smitha
name: Subramaniam, Annapurni
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We used the red clump stars from the photometric data of the Optical Gravitational Lensing Experiment(OGLE II) survey and the Magellanic Cloud Photometric Survey (MCPS) for both the Clouds to estimate the depth.The observed dispersion in the magnitude and colour distribution of red clump stars is used to estimate the depth, after correcting for population effects, internal reddening within the Clouds and photometric errors.The observed dispersion due to the line of sight depth ranges from 0.023 mag to 0.45 mag (a depth of 500 pc to 10.4 kpc) for LMC and from 0.025 to 0.34 magnitude(a depth of 670 pc to 9.53 kpc).The depth profile of the LMC bar indicates that it is flared.The average depth in the bar region is 4.0$\pm$1.4 kpc. The northern disk is found to have depth(4.17$\pm$0.97 kpc)larger than the southern part of the disk (2.63$\pm$0.8kpc).There is no indication of depth variation between the eastern and the western disk.The average depth for the disk is 3.44$\pm$ 1.16 kpc.In the case of SMC, the bar depth(4.90$\pm$1.23 kpc)and the disk depth (4.23$\pm$1.48kpc)are found to be within the standard deviations.A prominent feature in the SMC is the increase in depth near the optical center.The large dispersions estimated for the LMC bar and the northern disk suggest that the LMC either has large depth and/or different stellar populations in these regions.The halo of the LMC(using RR Lyrae stars)is found to have larger depth compared to the disk/bar,which supports the existence of an inner halo for the LMC.On the other hand, the estimated depths for the halo(RR Lyrae stars)and disk are found to be similar,for the SMC bar region. Thus,increased depth and enhanced stellar as well as HI density near the optical center suggests that the SMC may have a bulge.
description: revised version, Accepted in Astronomy & Astrophysics (Section 5 included, modified discussion section, 16 pages 18 figures)
Observation of time correlation function of multimode two-photon pairs on a rubidium D$_2$ line
Creators: name: Wang, Fu-Yuan
name: Shi, Bao-Sen
name: Guo, Guang-Can
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report the generation of a type-I multimode two-photon state on a rubidium D$_2$ line (780 nm) using periodically poled KTiOPO$_4$ crystals. With a degenerate optical parametric oscillator far below threshold, we observe an oscillatory correlation function, the cross-correlation between two photons shows a cavity bandwidth of about 7.8 MHz. We also use a Fabry-P$\acute{\rm{e}}$rot etalon to filter its most longitudinal modes and observe its time correlation function. The experimental data are well fitted to theoretical curves. This system could be utilized for demonstrating storage and retrieval of narrowband photons in Rb atomic ensembles, which is important for long-distance quantum communication.
description: 4 pages, 3 figures, submitted for publication on 29 April 2008
Comment on "Reversible superconducting-normal phase transition in a magnetic field and the existence of topologically protected loop currents that appear and disappear without Joule heating" by Hiroyasu Koizumi
Creators: name: Nikulov, A. V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: This comment is written on the article by Hiroyasu Koizumi, in which an alternative theory of superconductivity is proposed. No Joule heating is predicted in this theory unlike the conventional BCS-London theory of superconductivity. The theory is based on the author's opinion that the kinetic energy for the supercurrent is converted into the energy of the magnetic field during the transition of a bulk superconductor into the normal state in the presence of a magnetic field. The Comment indicates that this opinion cannot be correct, since the kinetic energy is much less than the energy of the magnetic field and both of these energies decrease during the transition to the normal state, according to the generally accepted point of view. It is briefly explained how a reversible thermodynamic process differs from an irreversible process.
description: 2 pages
Entwicklungs- und Gesundheitsarbeit des Österreichischen Roten Kreuzes in Südostasien: Im Gespräch mit Max Santner und Gerlinde Astleithner
Creators: name: Tomancok, Anna-Sophie
Publisher: name: Austrian Journal of South-East Asian Studies
Year: 2012

description: Max Santner leitet den Bereich Internationale Hilfe (Humanitäre Hilfe und Entwicklungszusammenarbeit) im Generalsekretariat des Österreichischen Roten Kreuzes (ÖRK) in Wien. Gerlinde Astleithner ist als Asien-Länderreferentin des ÖRK unter anderem für die Zusammenarbeit in Südostasien (vor allem Laos und Myanmar sowie an Rande auch für Osttimor) verantwortlich. Im vorliegenden Gespräch bieten sie einen Überblick zur gegenwärtigen Lage der Entwicklungs- und Gesundheitsarbeit der internationalen Rotkreuzbewegung in Südostasien. Das Interview wurde am 19. März 2012 in Wien durchgeführt.
description: Austrian Journal of South-East Asian Studies, Vol 5 No 1 (2012): Health
BIRINCHI DARAJALI BIR NOMA'LUMLI TAQQOSLAMALARNI YECHISH USULLARIGA DOIR MISOL VA MASALALAR YECHISH
Creators: name: Zahiriddinova, Shahlo
name: Cho'lliyeva, Mehriniso
Publisher: name: Zenodo
Year: 2025

description: Bir noma'lumli birinchi darajali tengsizliklarni yechish algebraik ifodalarni tahlil qilish va noma'lum qiymatni aniqlashga asoslanadi. Ushbu maqolada tengsizliklarni yechishning asosiy usullari – tengsizlikni soddalashtirish, algebraik amallar bajarish va yechimni tekshirish jarayonlari yoritiladi. Misollar yordamida asosiy qoidalar va amaliy yechim usullari tushuntiriladi.
DIAGNOSTICS AND SURGICAL TACTICS IN TRAUMATIC INJURIES OF THE SPLEEN.
Creators: name: Xakimov, M.Sh.
name: Jumanazarov, A.U.
name: Ismailova, U.A.
name: Aripov, Sh.Sh.
Publisher: name: Zenodo
Year: 2025

description: Traumatic injuries of the spleen account for 15 to 35% of all injuries to abdominal organs. Methods of treating the spleen are still controversial, since the important role of this organ in the body's immunological defense has been proven recently. There are reports of severe infectious diseases, often with a fulminant course, in patients who have previously undergone splenectomy.
Experiments in character recognition using linear and quadratic filters
Creators: name: DeMarco, John Francis
Publisher: name: University of British Columbia
Year: 2010

description: This thesis describes the simulation of a character recognition system using rive filter designs based on probabilistic models of character patterns. Four of the designs yield linear filters. Of these, three are based on variations of a Gaussian model. The fourth is based on the assumption of independent binary-valued features. The latter design is shown to produce higher recognition rates than any of the others when tested on Munson's multi-author hand-printed characters. This filter design is also tested on two subsets of the Cornell machine-printed data base. The fifth filter design is a special case of a quadratic filter, based on a Gaussian model in which spatially stationary covariance statistics are assumed. This assumption results in a filter structure consisting of a linear operation on the pattern vector plus a linear operation on the autocorrelation vector of the pattern. This filter design is found to achieve lower performance than the best linear filter design when tested on Munson's characters, and nearly equal performance on the Cornell characters. However, there are indications that a filter of this structure could achieve higher performance for some choice of filter coefficients.
Additional file 1 of Sleep quality and emergence delirium in children undergoing strabismus surgery: a comparison between preschool- and school-age patients
Creators: name: Do, Wangseok
name: Kim, Hyo-Sung
name: Kim, Seung Ha
name: Kang, Hyunjong
name: Lee, Dowon
name: Baik, Jiseok
name: Lee, Hyeon Jeong
name: Hong, Jeong-Min
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1 : Supplementary Table 1. Pediatric anesthesia emergence delirium scale. Supplementary Table 2. Watcha scale.
Accretion bursts in young stars driven by cluster environment
Creators: name: Pfalzner, S.
name: Tackenberg, J.
name: Steinhausen, M.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The standard picture of accretion is a steady flow of matter from the disc onto the young star - a concept which assumes the star-disc system to be completely isolated. However, in a dense cluster environment star-disc systems do interact gravitationally. The aim here is to estimate the encounter-induced accretion rate in an ONC-like environment. Combining simulations of the cluster dynamics with simulations of the effect of encounters on star-disc systems we determine the likelihood and degree of encounter-triggered accretion processes. We show that accretion bursts triggered by encounters of star-disc systems are common in young dense clusters like the ONC leading in the outburst phase to typical accretion rates of 10^(-7)-10^(-4) M(sun)/yr. Up to a third of stars presently in the Trapezium region accreted at least 1% of their disc mass via this mechanism in the last 1Myr. Accretion of over 6-7% of the disc material can occur in a single encounter. Despite losing their discs quickly, the total percentage of disc matter accreted per star is largest for the massive stars. Supplementing the steady accretion flow there exist episodic periods of high accretion in dense cluster environments. Due to their high accretion rate these processes should be observable even now in some of the low-mass stars in the ONC.
description: 4+2 pages, 3+1 figures, accepted for publication in A&A
Südostasienforschung in Österreich: Die Sammlung Insulares Südostasien des Museums für Völkerkunde Wien
Creators: name: Kuhnt-Saptodewo, Sri Tjahjani
Publisher: name: Austrian Journal of South-East Asian Studies
Year: 2012

description: -
description: Austrian Journal of South-East Asian Studies, Vol 5 No 1 (2012): Health
Discovery of two cyano derivatives of acenaphthylene (C$_{12}$H$_8$) in TMC-1 with the QUIJOTE line survey
Creators: name: Cernicharo, J.
name: Cabezas, C.
name: Fuentetaja, R.
name: Agúndez, M.
name: Tercero, B.
name: Janeiro, J.
name: Juanes, M.
name: Kaiser, R. I.
name: Endo, Y.
name: Steber, A. L.
name: Pérez, D.
name: Pérez, C.
name: Lesarri, A.
name: Marcelino, N.
name: de Vicente, P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery in TMC-1 of two cyano derivatives of the PAH acenaphthylene (C$_{12}$H$_8$). We have found two series of lines with the QUIJOTE line survey that we assign to 1-C$_{12}$H$_7$CN and 5-C$_{12}$H$_7$CN. For the 1-isomer, we have detected and assigned 173 rotational transitions with $J$ up to 46 and $K_a$ up to 9, corresponding to 107 independent frequencies. For the 5-isomer, the identification is based on 56 individual lines, corresponding to 117 rotational transitions with $J$ up to 40 and $K_a$ up to 8. Identification of the carriers was achieved through a careful analysis of the derived rotational constants, which permit us to focus on molecules larger than naphthalene but smaller than anthracene and phenanthrene. Moreover, the derived rotational constants indicate that the species are planar; this allows us to discard derivatives of fluorene and acenaphthene, which are non-planar species. Quantum chemical calculations and subsequent chemical synthesis of these molecules, as well as the observation of their rotational transitions in the laboratory, unequivocally support our identifications. We also confirm, via a robust line-by-line detection, the previous claimed detection of 1- and 2- cyanonaphthalene, which were obtained through statistical stacking techniques. The column densities of 1- and 5-cyanoacenaphthylene are (9.5\,$\pm$\,0.9)$\,\times$\,10$^{11}$ cm$^{-2}$, while those of 1- and 2-cyanonapthalene are (5.5\,$\pm$\,0.5)$\,\times$\,10$^{11}$ cm$^{-2}$. Hence, it seems that acenaphthylene could be a factor of 1.7 more abundant than naphthalene. These results support a scenario in which PAHs grow in cold dark clouds based on fused five- and six-membered carbon rings.
description: Accepted as a Letter to the Editor in Astronomy and Astrophysics on 18th September 2024
Non-perturbative renormalization-group approach to lattice models
Creators: name: Dupuis, N.
name: Sengupta, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The non-perturbative renormalization-group approach is extended to lattice models, considering as an example a $ϕ^4$ theory defined on a $d$-dimensional hypercubic lattice. Within a simple approximation for the effective action, we solve the flow equations and obtain the renormalized dispersion $\eps(\q)$ over the whole Brillouin zone of the reciprocal lattice. In the long-distance limit, where the lattice does not matter any more, we reproduce the usual flow equations of the continuum model. We show how the numerical solution of the flow equations can be simplified by expanding the dispersion in a finite number of circular harmonics.
description: v1) 8 pages, 7 figures, v2) includes a discussion of the Ginzburg scale vs. the lattice scale
Operator theoretic methods for the eigenvalue counting function in spectral gaps
Creators: name: Pushnitski, Alexander
Publisher: name: arXiv
Year: 2008
Subjects: subject: Spectral Theory (math.SP)
subject: FOS: Mathematics
subject: 35P20; 47B25, 47F05

description: Using the notion of spectral flow, we suggest a simple approach to various asymptotic problems involving eigenvalues in the gaps of the essential spectrum of self-adjoint operators. Our approach uses some elements of the spectral shift function theory. Using this approach, we provide generalisations and streamlined proofs of two results in this area already existing in the literature. We also give a new proof of the generalised Birman-Schwinger principle.
description: Latex, 25 pages
Additional file 2 of Decomposition of outpatient health care spending by disease - a novel approach using insurance claims data
Creators: name: Stucki, Michael
name: Nemitz, Janina
name: Trottmann, Maria
name: Wieser, Simon
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 2. Additional results not shown in the article.
Alle origini del romanzo aziendale. Lessico e narrazione in La morte in banca di Giuseppe Pontiggia
Creators: name: Ceteroni, Alessandro
Publisher: name: Università degli Studi di Milano
Year: 2014
Subjects: Pontiggia; Carabba; La morte in banca; identità narrativa; conoscenza incarnata; utopia

description: L’articolo sviluppa un’analisi testuale del primo romanzo di Giuseppe Pontiggia, La morte in ban- ca, sfruttando la teoria degli schema e degli script per ricostruire i processi della fruizione narrativa del lettore, e la teoria della conoscenza incarnata per l’analisi dell’identità narrativa del protago- nista Carabba. Si propone un’interpretazione complessiva del testo incentrata sul tema dell’utopia, che consente di cogliere la profonda attualità di questo romanzo.
description: ENTHYMEMA, No 10 (2014)
Additional file 3 of Decomposition of outpatient health care spending by disease - a novel approach using insurance claims data
Creators: name: Stucki, Michael
name: Nemitz, Janina
name: Trottmann, Maria
name: Wieser, Simon
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 3. Regression results.
Michael Silk, Ingo Gildenhard, Rosemary Barrow, The Classical Tradition: Art, Literature, Thought
Creators: name: Veglia, Andrea
Publisher: name: Università degli Studi di Milano
Year: 2014
Subjects: reception; tradition; antiquity; influence

description: A review of Michael Silk, Ingo Gildenhard, Rosemary Barrow (eds), The Classical Tradition: Art, Literature, Thought. Oxford: Wiley-Blackwell, 2014. Print.
description: ENTHYMEMA, No 10 (2014)
Additional file 1 of Split it up and see: using proxies to highlight divergent inter-populational performances in aquaculture standardised conditions
Creators: name: Toomey, Lola
name: Dellicour, Simon
name: Kapusta, Andrzej
name: Żarski, Daniel
name: Buhrke, Frederik
name: Milla, Sylvain
name: Fontaine, Pascal
name: Lecocq, Thomas
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Principal component analysis biplot representing environmental variables (in blue) and populations (dots in grey) using the first two axes. Populations: BAL: Balaton, VAL : Valkea-Müstajärvi, ISO: Iso-Valkjärvi, KIE: Kierzlinskie, GEN: Geneva, BOU: Bourget, HOH: Hohen Sprenzer. BIO1 to BIO19 correspond to the bioclimatic variables from Worldclim. Vap, wind, and srad correspond to water vapor pressure, wind speed, and solar radiation, respectively.
A Generalized Model for Multidimensional Intransitivity
Creators: name: Duan, Jiuding
name: Li, Jiyi
name: Baba, Yukino
name: Kashima, Hisashi
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: Computation and Language (cs.CL)
subject: Computer Science and Game Theory (cs.GT)
subject: General Economics (econ.GN)
subject: FOS: Computer and information sciences
subject: FOS: Economics and business

description: Intransitivity is a critical issue in pairwise preference modeling. It refers to the intransitive pairwise preferences between a group of players or objects that potentially form a cyclic preference chain and has been long discussed in social choice theory in the context of the dominance relationship. However, such multifaceted intransitivity between players and the corresponding player representations in high dimensions is difficult to capture. In this paper, we propose a probabilistic model that jointly learns each player's d-dimensional representation (d>1) and a dataset-specific metric space that systematically captures the distance metric in Rd over the embedding space. Interestingly, by imposing additional constraints in the metric space, our proposed model degenerates to former models used in intransitive representation learning. Moreover, we present an extensive quantitative investigation of the vast existence of intransitive relationships between objects in various real-world benchmark datasets. To our knowledge, this investigation is the first of this type. The predictive performance of our proposed method on different real-world datasets, including social choice, election, and online game datasets, shows that our proposed method outperforms several competing methods in terms of prediction accuracy.
description: 13 pages, 1 figure
A vertex fitting package
Creators: name: Bedeschi, Franco
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Vertex fitting code is commonly found within the analysis packages of several HEP experiments, unfortunately it usually deeply packaged inside their software infrastructure, making it cumbersome to use in the context of external applications. In this paper a totally independent package is described. The only dependencies being the ROOT libraries, making it easy to use in a wide range of applications. The code currently works with track trajectories that are either helices or straight lines, as generated by charged or neutral particles in a constant magnetic field, but is expandable in principle to other type of trajectories or parameterizations.
description: 22 pages
Photon echoes generated by reversing magnetic field gradients in a rubidium vapour
Creators: name: Hétet, G.
name: Hosseini, M.
name: Sparkes, B. M.
name: Oblak, D.
name: Lam, P. K.
name: Buchler, B. C.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose a photon echo quantum memory scheme using detuned Raman coupling to long lived ground states. In contrast to previous 3-level schemes based on controlled reversible inhomogeneous broadening that use sequences of $π$-pulses, the scheme does not require accurate control of the coupling dynamics to the ground states. We present a proof of principle experimental realization of our proposal using rubidium atoms in a warm vapour cell. The Raman resonance line is broadened using a magnetic field that varies linearly along the direction of light propagation. Inverting the magnetic field gradient rephases the atomic dipoles and re-emits the light pulse in the forward direction.
Classical signal detection theory and reconstruction problems in holographic imaging systems
Creators: name: Ghandeharian, Hossein
Publisher: name: University of British Columbia
Year: 2010

description: A new "circuit" model is developed to study non-linear effects in holography. The model links classical signal detection theory to holography, for it clearly shows that the reconstructed images in a thin hologram can be computed from mathematical formulas obtained for the output of non-linear detectors. In preparation for hologram analysis, the results for the (time-) autocorrelation of electrical ʋth-law devices in response to signal plus noise are extended to memoryless non-linear detectors with arbitrary characteristics. Mathematical parallels are next established between holography and the non-linear detection of signals, and these are incorporated in the model. The ready-made formulas for electrical detectors apply directly to give formulas for the (space-)autocorrelation of holograms of diffuse objects. The autocorrelation function predicts distorted multi-pie images, their relative positions, orientations, widths, and strengths. The multiplicity of images is due to the generation of harmonics; the background halo-like noise components added to the faithful images are mainly due to the multiplicity of the first harmonic itself. The analysis is further expanded to include a still more general case in which the reflected light from the object is depolarized. A decrease in signal-to-noise ratio (decrease in fringe visibility); a loss of information, and an augmentation of non-linear distortion could be expected. A simple way of reducing these effects is suggested. Finally, holography with more than one reference beam is studied. An exact formulation is given for double-reference-beam holograms. For multiple-reference-beam holograms, only approximate closed forms are presented. It is shown that the addition of extra reference beams during the recording step of the hologram may amplify the faithful images without increasing their background noise significantly. Experiments confirm the theoretical expectations.
Additional file 2 of Split it up and see: using proxies to highlight divergent inter-populational performances in aquaculture standardised conditions
Creators: name: Toomey, Lola
name: Dellicour, Simon
name: Kapusta, Andrzej
name: Żarski, Daniel
name: Buhrke, Frederik
name: Milla, Sylvain
name: Fontaine, Pascal
name: Lecocq, Thomas
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Figure S2. Barplots representing results obtained for all key traits studied (n = 3 per population, except for activity and inter-individual distances for which n=9). Different letters indicate significant differences between populations (p-value<0.05) using post-hoc tests.
Migrazioni di archetipi: tradizioni e rapimenti
Creators: name: Valsecchi, Giulia
Publisher: name: Università degli Studi di Milano
Year: 2014
Subjects: Archetipo; invariante; plot; inconscio collettivo; tradizione

description: Quel che resta di una trasmissione orale o scritta sono tracce multiple e mai estinte. I segni e i simboli che la rinnovano, secondo influsso e revisione dei confini di tradizione, traduzione o plagio, sono oggetto del volume collettaneo Archetypes in Literatures and Cultures – Cultural and Re- gional Studies a cura di Rahilya Geybullayeva (Baki Slavian Universiteti, Azerbaijan). Un’analisi a più voci degli attraversamenti identitari per migrazioni di archetipi nello spazio-tempo delle lettera- ture ed epopee.
description: ENTHYMEMA, No 10 (2014)
Measurement of CP asymmetries in $B^0 \to K^0π^0$ decays
Creators: name: Fujikawa, M.
name: Yusa, Y.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report measurements of CP violation parameters in $B^0 \to K^0 π^0$ decays based on a data sample of $657 \times 10^6 B\bar{B}$ pairs collected with the Belle detector at the KEKB $e^+ e^-$ asymmetric-energy collider. We use $B^0 \to K^0_S π^0$ decays for both mixing-induced and direct $CP$ violating asymmetry measurements and $B^0 \to K^0_L π^0$ decays for the direct CP violation measurement. The CP violation parameters obtained are $\sin 2 ϕ_1^{\rm eff} = +0.67 \pm 0.31{(stat)} \pm 0.08 {(syst)}$ and $\mathcal{A}_{K^0 π^0} = +0.14 \pm 0.13{(stat)} \pm 0.06 {(syst)}$. The branching fraction of $B^0 \to K^0 π^0$ decay is measured to be $\mathcal{B}(B^0 \to K^0 π^0) = (8.7\pm0.5 (\rm{stat.})\pm0.6 (\rm{syst.}))\times 10^{-6}$. The observed $\mathcal{A}_{K^0 π^0}$ value differs by 1.9 standard deviations from the value expected from an isospin sum rule.
description: 6 pages, 3 figures
Quantum computing with trapped ions
Creators: name: Haeffner, H.
name: Roos, C. F.
name: Blatt, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum computers hold the promise to solve certain computational task much more efficiently than classical computers. We review the recent experimental advancements towards a quantum computer with trapped ions. In particular, various implementations of qubits, quantum gates and some key experiments are discussed. Furthermore, we review some implementations of quantum algorithms such as a deterministic teleportation of quantum information and an error correction scheme.
description: Review article, accepted for publication in Physics Reports, 99pages, 38 Figures, ~2 MByte
The magnetic field of the proto-planetary nebula candidate IRAS 19296+2227
Creators: name: Vlemmings, W. H. T.
name: van Langevelde, H. J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Context: Magnetic fields are thought to be one of the possible mechanisms responsible for shaping the generally spherical outflow of evolved stars into often aspherical planetary nebulae. However, direct measurements of magnetic fields during the transition to the planetary nebula phase are rare. Aims: The aim of this project is to expand the number of magnetic field measurements of stars in the (proto-)planetary nebula phase and find if the magnetic field strength is sufficient to affect the stellar outflow. Methods: We used Very Long Baseline Array observations to measure the circular polarization due to the Zeeman splitting of 22 GHz water masers in the envelope of the proto-planetary nebula candidate star IRAS 19296+2227 and the planetary nebula K3-35. Results: A strong magnetic field of B||=-135+-28 is detected in the water maser region of the proto-planetary nebula candidate IRAS 19296+2227. The water masers of K3-35 are too weak to detect circular polarization although we do present the measurements of weak linear polarization in those masers. Conclusions: The field measured in the masers of IRAS 19296+2227 is dynamically important and, if it is representative of the large scale field, is an important factor in driving the stellar mass loss and shaping the stellar outflow.
description: 5 pages, 3 figures; A&A accepted
Additional file 3 of Split it up and see: using proxies to highlight divergent inter-populational performances in aquaculture standardised conditions
Creators: name: Toomey, Lola
name: Dellicour, Simon
name: Kapusta, Andrzej
name: Żarski, Daniel
name: Buhrke, Frederik
name: Milla, Sylvain
name: Fontaine, Pascal
name: Lecocq, Thomas
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S1. Correlation results between proxy-based (geographic, hydrologic, genetic, and habitat proxies) and KTA-based distance matrices with r the Mantel correlation value and its associated p-value (significant r (p-value<0.05) are indicated in bold).
Evolution of newly formed dust in Population III supernova remnants and its impact on the elemental composition of Population II.5 stars
Creators: name: Nozawa, Takaya
name: Kozasa, Takashi
name: Habe, Asao
name: Dwek, Eli
name: Umeda, Hideyuki
name: Tominaga, Nozomu
name: Maeda, Keiichi
name: Nomoto, Ken'ichi
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the evolution of dust formed in Population III supernovae (SNe) by considering its transport and processing by sputtering within the SN remnants (SNRs). We find that the fates of dust grains within SNRs heavily depend on their initial radii $a_{\rm ini}$. For Type II SNRs expanding into the ambient medium with density of $n_{\rm H,0} = 1$ cm$^{-3}$, grains of $a_{\rm ini} < 0.05$ $μ$m are detained in the shocked hot gas and are completely destroyed, while grains of $a_{\rm ini} > 0.2$ $μ$m are injected into the surrounding medium without being destroyed significantly. Grains with $a_{\rm ini}$ = 0.05-0.2 $μ$m are finally trapped in the dense shell behind the forward shock. We show that the grains piled up in the dense shell enrich the gas up to 10$^{-6}-10^{-4}$ $Z_\odot$, high enough to form low-mass stars with 0.1-1 $M_\odot$. In addition, [Fe/H] in the dense shell ranges from -6 to -4.5, which is in good agreement with the ultra-metal-poor stars with [Fe/H] < -4. We suggest that newly formed dust in a Population III SN can have great impacts on the stellar mass and elemental composition of Population II.5 stars formed in the shell of the SNR.
description: 5 pages, 3 figures and 1 table. To appear in the proceedings of IAU Symposium 255 "Low-Metallicity Star Formation: From the First Stars to Dwarf Galaxies", Rapallo, June 2008, eds. L.K. Hunt, S. Madden, & R. Schneider (Cambridge Univ. Press)
Health and Environmental Risk Communication in Thailand: An Analysis of Agency Staff’ Perspectives on Risk Communication With External Stakeholders
Creators: name: Tuler, Seth
name: Langkulsen, Uma
name: Chess, Caron
name: Vichit-Vadakan, Nuntavarn
Publisher: name: Austrian Journal of South-East Asian Studies
Year: 2012

description: Health and environmental agencies are routinely called upon to provide risk-related information to the public-at-large and to more narrowly defi ned audiences, such as children, pregnant women, or labourers. While a large body of guidance is available, it is often general and transferability to new contexts is not well understood. In particular, the relevance of this guidance for South-East Asia is not clear. This paper reports the results of a study, using Q method, that aimed to develop a better understanding of offi cers’ and staff ’s perspectives on health and environmental risk communication within a single regulatory agency in Thailand, the Pollution Control Department. The results demonstrate that there are multiple perspectives, and they are unrelated to roles or experience. This study contributes to a deeper understanding of the ways that offi cers and staff within a national agency with important responsibilities for health and environmental risk communication in Thailand think about these responsibilities and how to achieve them.
description: Austrian Journal of South-East Asian Studies, Vol 5 No 1 (2012): Health
An optical view of the filament region of Abell 85
Creators: name: Boué, G.
name: Durret, F.
name: Adami, C.
name: Mamon, G. A.
name: Ilbert, O.
name: Cayatte, V.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the distribution of optically and Halpha (Ha) selected galaxies in the Southern half of the nearby Abell 85 (A85) cluster with the recently discovered X-ray filament (XRF). We search for galaxies where star formation (SF) may have been triggered by interactions with intracluster gas or tidal pressure due to the cluster potential when entering the cluster. Our analysis is based on images obtained with CFHT MegaPrime/MegaCam (1x1 deg2 field) in four bands (ugri) and ESO 2.2mWFI (38'x36' field) in a narrow band filter corresponding to the redshifted Halpha (Ha) line and in a broad R-band filter. The LFs are estimated by statistically subtracting a reference field. Background contamination is minimized by cutting out galaxies redder than the observed red sequence in the g-i vs. i colour-magnitude diagram. The galaxy distribution shows a significantly flattened cluster, whose principal axis is slightly offset from the XRF. The analysis of the broad band LFs shows that the filament region is well populated. The filament is also independently detected as a gravitationally bound structure by the Serna & Gerbal hierarchical method. 101 galaxies are detected in Ha, among which 23 have spectroscopic redshifts in the cluster, 2 have spectroscopic redshifts higher than the cluster and 58 have photometric redshifts that tend to indicate that they are background objects.The 23 galaxies with spectroscopic redshifts in the cluster are mostly concentrated in the South part of the cluster and along the filament. We find a number of galaxies showing evidence for SF in the XRF, and all our results are consistent with the previous hypothesis that the XRF in A85 is a gravitationally bound structure made of groups falling on to the main cluster.
description: Accepted in A&A. 39 pages, 107 figures. Full resolution images available at ftp://ftp.iap.fr/pub/from_users/gam/A85/
Do supernovae indicate an accelerating universe?
Creators: name: Mohayaee, Roya
name: Rameez, Mohamed
name: Sarkar, Subir
Publisher: name: arXiv
Year: 2021
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: FOS: Physical sciences

description: In the late 1990's, observations of 93 Type Ia supernovae were analysed in the framework of the FLRW cosmology assuming these to be `standard(isable) candles'. It was thus inferred that the Hubble expansion rate is accelerating as if driven by a positive Cosmological Constant $Λ$. This is still the only direct evidence for the `dark energy' that is the dominant component of the standard $Λ$CDM cosmological model. Other data such as BAO, CMB anisotropies, stellar ages, the rate of structure growth, etc are all `concordant' with this model but do not provide independent evidence for accelerated expansion. Analysis of a larger sample of 740 SNe Ia shows that these are not quite standard candles, and highlights the "corrections" applied to analyse the data in the FLRW framework. The latter holds in the reference frame in which the CMB is isotropic, whereas observations are made in our heliocentric frame in which the CMB has a large dipole anisotropy. This is assumed to be of kinematic origin i.e. due to our non-Hubble motion driven by local inhomogeneity in the matter distribution. The $Λ$CDM model predicts how this peculiar velocity should fall off as the averaging scale is raised and the universe becomes sensibly homogeneous. However observations of the local `bulk flow' are inconsistent with this expectation and convergence to the CMB frame is not seen. Moreover the kinematic interpretation implies a corresponding dipole in the sky distribution of high redshift quasars, which is rejected by observations at 4.9$σ$. The acceleration of the Hubble expansion rate is also anisotropic at 3.9$σ$ and aligned with the bulk flow. Thus dark energy may be an artefact of analysing data assuming that we are idealised observers in an FLRW universe, when in fact the real universe is inhomogeneous and anisotropic out to distances large enough to impact on cosmological analyses.
description: 14 pages, 4 figures, 4 tables
Additional file 1 of A systems approach to the exploration of research activity and relationships within a local authority
Creators: name: Fynn, Judith F.
name: Jones, John
name: Jones, Andy
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 1. Themes and questions for Interviews and Focus Groups.
On the Edge of Crisis: Contending Perspectives on Development, Tourism and Community Participation on Rote Island, Indonesia
Creators: name: Wright, Cassandra
name: Lewis, Belinda
Publisher: name: Austrian Journal of South-East Asian Studies
Year: 2012

description: The eastern Indonesian province of Nusa Tenggara Timur (NTT) is struggling to overcome the burden of widespread poverty, illness, and illiteracy. Within the context of globalisation and Indonesia’s ongoing transitions in governance, people on Rote Island, NTT, are experiencing rapid socio-cultural change. The increasing arrival of tourists and foreign business interests add further complexity to these processes of transition. The direction forward for Rote is a topic of considerable debate amongst community members, development workers, businesses, and other stakeholders. This qualitative pilot study explores key community stakeholders’ perspectives on development, tourism, and community sustainability in Delha, Rote. It has revealed confl icting perspectives about future development and tourism on Rote, with particular concern regarding social, cultural, and environmental impacts, and loss of autonomy and community control. Important ‘dynamics of exclusion’ between stakeholders are identifi ed. More equitable participation in planning and decision-making is needed to ensure that the benefi ts of tourism and development are not concentrated with a privileged few.
description: Austrian Journal of South-East Asian Studies, Vol 5 No 1 (2012): Health
Additional file 2 of A systems approach to the exploration of research activity and relationships within a local authority
Creators: name: Fynn, Judith F.
name: Jones, John
name: Jones, Andy
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 2. Case studies of differing approaches and models of research activity within different local authority teams or departments.
Additional file 1 of Survival impact of additional chemotherapy after adjuvant concurrent chemoradiation in patients with early cervical cancer who underwent radical hysterectomy
Creators: name: Kim, Se Ik
name: Kim, Jeong Yun
name: Wee, Chan Woo
name: Lee, Maria
name: Kim, Hee Seung
name: Chung, Hyun Hoon
name: Lee, Taek Sang
name: Jeon, Hye Won
name: Park, Noh Hyun
name: Song, Yong Sang
name: Kim, Tae Hun
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer

description: Additional file 1.
The Devil Is in the Details: An Efficient Convolutional Neural Network for Transport Mode Detection
Creators: name: Moreau, Hugues
name: Vassilev, Andréa
name: Chen, Liming
Publisher: name: arXiv
Year: 2021
Subjects: subject: Signal Processing (eess.SP)
subject: Machine Learning (cs.LG)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Transport mode detection is a classification problem aiming to design an algorithm that can infer the transport mode of a user given multimodal signals (GPS and/or inertial sensors). It has many applications, such as carbon footprint tracking, mobility behaviour analysis, or real-time door-to-door smart planning. Most current approaches rely on a classification step using Machine Learning techniques, and, like in many other classification problems, deep learning approaches usually achieve better results than traditional machine learning ones using handcrafted features. Deep models, however, have a notable downside: they are usually heavy, both in terms of memory space and processing cost. We show that a small, optimized model can perform as well as a current deep model. During our experiments on the GeoLife and SHL 2018 datasets, we obtain models with tens of thousands of parameters, that is, 10 to 1,000 times less parameters and operations than networks from the state of the art, which still reach a comparable performance. We also show, using the aforementioned datasets, that the current preprocessing used to deal with signals of different lengths is suboptimal, and we provide better replacements. Finally, we introduce a way to use signals with different lengths with the lighter Convolutional neural networks, without using the heavier Recurrent Neural Networks.
description: 13 pages, 5 figures, 6 tables. Published in IEEE Transactions on Intelligent Transportation Systems