cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ferromagnetic ground state of an orbital degenerate electronic model for transition-metal oxides: exact solution and physical mechanism
Creators: name: Shen, Shun-Qing
name: Wang, Z. D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present an exact ground state solution of a one-dimensional electronic model for transition-metal oxides in the strong coupling limit. The model contains doubly degenerated orbit for itinerant electrons and the Hund coupling between the itinerant electrons and localized spins. The ground state is proven to be a full ferromagnet for any density of electrons. Our model provides a rigorous example for metallic ferromagnetism in narrow band systems. The physical mechanism for ferromagnetism and its relevance to high-dimensional systems, like R$_{1-x}$X$_x$MnO$_3$, are discussed. Due to the orbital degeneracy of itinerant electrons, the superexchange coupling can be ferromagnetic rather than antiferromagnetic in the one-band case.
description: 4 page, no figure To appear in Phys. Rev. B, (January 1, 1999)
MOESM2 of The Y-linked proto-oncogene TSPY contributes to poor prognosis of the male hepatocellular carcinoma patients by promoting the pro-oncogenic and suppressing the anti-oncogenic gene expression
Creators: name: Kido, Tatsuo
name: Yun-Fai Lau
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Figure S1. Results of Ingenuity Pathway Analysis (IPA) using a stringent cutoff on expression level of DEGs.
Fast Zonal Field Dynamo in Collisionless Kinetic Alfven Wave Turbulence
Creators: name: Gruzinov, I.
name: Das, A.
name: Diamond, P. H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The possibility of fast dynamo action by collisionless kinetic Alfven Wave turbulence is demonstrated. The irreversibility necessary to lock in the generated field is provided by electron Landau damping, so the induced electric field does not vanish with resistivity. Mechanisms for self-regulation of the system and the relation of these results to the theory of alpha quenching are discussed. The dynamo-generated fields have symmetry like to that of zonal flows, and thus are termed zonal fields.
The Physics of the Accelerating Universe Camera
Creators: name: Padilla, Cristobal
name: Castander, Francisco J.
name: Alarcon, Alex
name: Aleksic, Jelena
name: Ballester, Otger
name: Cabayol, Laura
name: Cardiel-Sas, Laia
name: Carretero, Jorge
name: Casas, Ricard
name: Castilla, Javier
name: Crocce, Martin
name: Delfino, Manuel
name: Diaz, Carlos
name: Eriksen, Martin
name: Fernandez, Enrique
name: Fosalba, Pablo
name: Garcia-Bellido, Juan
name: Gaztanaga, Enrique
name: Gaweda, Javier
name: Granena, Ferran
name: Illa, Jose Maria
name: Jimenez, Jorge
name: Lopez, Luis
name: Marti, Pol
name: Miquel, Ramon
name: Neissner, Christian
name: Pio, Cristobal
name: Sanchez, Eusebio
name: Serrano, Santiago
name: Sevilla-Noarbe, Ignacio
name: Tallada, Pau
name: Tonello, Nadia
name: de Vicente, Juan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The PAU (Physics of the Accelerating Universe) Survey goal is to obtain photometric redshifts (photo-z) and Spectral Energy Distribution (SED) of astronomical objects with a resolution roughly one order of magnitude better than current broad band photometric surveys. To accomplish this, a new large field of view camera (PAUCam) has been designed, built, commissioned and is now operated at the William Herschel Telescope (WHT). With the current WHT Prime Focus corrector, the camera covers ~1-degree diameter Field of View (FoV), of which, only the inner ~40 arcmin diameter are unvignetted. The focal plane consists of a mosaic of 18 2k$x4k Hamamatsu fully depleted CCDs, with high quantum efficiency up to 1 micrometers in wavelength. To maximize the detector coverage within the FoV, filters are placed in front of the CCDs inside the camera cryostat (made out of carbon fiber) using a challenging movable tray system. The camera uses a set of 40 narrow band filters ranging from ~4500 to ~8500 Angstroms complemented with six standard broad-band filters, ugrizY. The PAU Survey aims to cover roughly 100 square degrees over fields with existing deep photometry and galaxy shapes to obtain accurate photometric redshifts for galaxies down to i_AB~22.5, detecting also galaxies down to i_AB~24 with less precision in redshift. With this data set we will be able to measure intrinsic alignments, galaxy clustering and perform galaxy evolution studies in a new range of densities and redshifts. Here, we describe the PAU camera, its first commissioning results and performance.
description: 34 pages, 55 figures
Additional file 2 of Assessing taxonomic metagenome profilers with OPAL
Creators: name: Meyer, Fernando
name: Bremges, Andreas
name: Belmann, Peter
name: Janssen, Stefan
name: McHardy, Alice
name: Koslicki, David
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology

description: Instructions for reproducing the comparisons of taxonomic profilers. (PDF 79 kb)
Microdontinae Rondani 1845
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy

description: Microdontinae
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Atomic micromotion and geometric forces in a triaxial magnetic trap
Creators: name: Müller, J. H.
name: Morsch, O.
name: Ciampini, D.
name: Anderlini, M.
name: Mannella, R.
name: Arimondo, E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Non-adiabatic motion of Bose-Einstein condensates of rubidium atoms arising from the dynamical nature of a time-orbiting-potential (TOP) trap was observed experimentally. The orbital micromotion of the condensate in velocity space at the frequency of the rotating bias field of the TOP was detected by a time-of-flight method. A dependence of the equilibrium position of the atoms on the sense of rotation of the bias field was observed. We have compared our experimental findings with numerical simulations. The nonadiabatic following of the atomic spin in the trap rotating magnetic field produces geometric forces acting on the trapped atoms.
description: 4 pages, 4 figures
Microdon myrmicae Schonrogge 2002
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Scrophulariaceae
Microdon
Microdon myrmicae

description: Microdon myrmicae Schönrogge et al., 2002. (Speight & Sommaggio 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Additional file 1: of The Epstein-Barr virus EBNA1 protein modulates the alternative splicing of cellular genes
Creators: name: Boudreault, Simon
name: Armero, Victoria
name: Scott, Michelle
name: Perreault, Jean-Pierre
name: Bisaillon, Martin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The following are available online at www.mdpi.com/xxx/s1 , Table S1 List of gene names and their respective official full names Table S2 AS-PCR primers used to analyze the AS of potential ASEs bound by EBNA1 Table S3 List of the 51 peaks identified in EBNA1 RIP-Seq Figure S1 Supplemental electrophoregrams of genes that have their splicing modulated upon EBNA1 expression, Figure S2 Effect of transient MSCV-N transfection on cellular AS. Figure S3 Flowchart summarizing the RIP-Seq protocol and controls used, Figure S4 Western-Blotting of immunoprecipitation of EBNA1, Figure S5 Quality assessment of input RNA and immunoprecipitated RNA for the RIP-Seq experiment, Figure S6 Quality assessment of control and EBNA1 RIP following ribo-depletion, Figure S7 Quality assessment of library for the RIP-Seq, Figure S8 Read distribution on the EBNA1 coding sequence in the EBNA1 RIP-Seq and qPCR measurement of immunoprecipitatedEBNA1 mRNA. (PDF 2818 kb)
Resting-state ASL : Toward an optimal sequence duration
Creators: name: Isabelle, Corouge
name: Vallée, Corentin
name: Maurel, Pierre
name: Corouge, Isabelle
name: Barillot, Christian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Biological sciences

description: Resting-state functional Arterial Spin Labeling (rs-fASL) in clinical daily practice and academic research stay discreet compared to resting-state BOLD. However, by giving direct access to cerebral blood flow maps, rs-fASL leads to significant clinical subject scaled application as CBF can be considered as a biomarker in common neuropathology. Our work here focuses on the link between overall quality of rs-fASL and duration of acquisition. To this end, we consider subject self-Default Mode Network (DMN), and assess DMN quality depletion compared to a gold standard DMN depending on the duration of acquisition.
Additional file 1 of Assessing taxonomic metagenome profilers with OPAL
Creators: name: Meyer, Fernando
name: Bremges, Andreas
name: Belmann, Peter
name: Janssen, Stefan
name: McHardy, Alice
name: Koslicki, David
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Supplementary tables and figures. (PDF 2601 kb)
Brachyopa grunewaldensis Kassebeer 2000
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Brachyopa
Brachyopa grunewaldensis

description: Brachyopa grunewaldensis Kassebeer, 2000. (Haenni 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
On Turbulent Reconnection
Creators: name: Kim, Eun-Jin
name: Diamond, P. H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We examine the dynamics of turbulent reconnection in 2D and 3D reduced MHD by calculating the effective dissipation due to coupling between small-scale fluctuations and large-scale magnetic fields. Sweet-Parker type balance relations are then used to calculate the global reconnection rate. Two approaches are employed -- quasi-linear closure and an eddy-damped fluid model. Results indicate that despite the presence of turbulence, the reconnection rate remains inversely proportional to $\sqrt{R_m}$, as in the Sweet-Parker analysis. In 2D, the global reconnection rate is shown to be enhanced over the Sweet-Parker result by a factor of magnetic Mach number. These results are the consequences of the constraint imposed on the global reconnection rate by the requirement of mean square magnetic potential balance. The incompatibility of turbulent fluid-magnetic energy equipartition and stationarity of mean square magnetic potential is demonstrated.
description: 37 pages, 2 figures
Spectral function of one hole in several one-dimensional spin arrangements
Creators: name: Hayn, R.
name: Kuzian, R. O.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The spectral function of one hole in different magnetic states of the one-dimensional t-J model including three-site term and frustration $J^{\prime}$ is studied. In the strong coupling limit $J \to 0$ (corresponding to $U \to \infty$ of the Hubbard-model) a set of eigenoperators of the Liouvillian is found which allows to derive an exact expression for the one-particle Green's function that is also applicable at finite temperature and in an arbitrary magnetic state. The spinon dispersion of the pure t-J model with the ground-state of the Heisenberg model can be obtained by treating the corrections due to a small exchange term by means of the projection method. The spectral function for the special frustration $J^{\prime}=J/2$ with the Majumdar-Ghosh wave function is discussed in detail. Besides the projection method, a variational ansatz with the set of eigenoperators of the $t$-term is used. We find a symmetric spinon dispersion around the momentum $k=π/(2a)$ and a strong damping of the holon branch. Below the continuum a bound state is obtained with finite spectral weight and a very small separation from the continuum. Furthermore, the spectral function of the ideal paramagnetic case at a temperature $k_B T \gg J$ is discussed.
description: 15 pages, 6 figures
Observing the gas component of circumplanetary disks around wide-orbit planet-mass companions in the (sub)mm regime
Creators: name: Rab, Ch.
name: Kamp, I.
name: Ginski, C.
name: Oberg, N.
name: Muro-Arena, G. A.
name: Dominik, C.
name: Waters, L. B. F. M.
name: Thi, W. -F.
name: Woitke, P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Several detections of wide-orbit planet-mass/sub-stellar companions around young solar-like stars were reported in the last decade. The origin of those possible planets is still unclear but accretion tracers and VLT/SPHERE observations indicate that they are surrounded by circumplanetary material or even a circumplanetary disk. We want to investigate if the gas component of disks around wide-orbit companions is detectable with current and future (sub)mm telescopes and what constraints such gas observations can provide on the nature of the circumplanetary material and on the mass of the companion. We applied the radiation thermo-chemical disk code ProDiMo to model the dust and gas component of passive circumplanetary disks and produced realistic synthetic observables. We considered different companion properties, disk parameters and radiative environments and compared the resulting synthetic observables to telescope sensitivities and to existing dust observations. The main criterion for a successful detection is the size of the circumplanetary disk. At a distance of about 150 pc, a circumplanetary disk with an outer radius of about 10 au is detectable with ALMA in about 6 hours in optically thick CO lines. Other aspects such as the companion's luminosity, disk inclination and background radiation fields are also relevant and should be considered to optimize the observing strategy for detection experiments. For most of the known wide-orbit planet-mass companions, their maximum theoretical disk size of one third of the Hill radius would be sufficient to allow detection of CO lines. It is therefore feasible to detect their gas disks and constrain the mass of the companion through the kinematic signature. Even in the case of non-detections such observations will provide stringent constraints on disk size and gas mass, information crucial for formation theories.
description: 13 pages, 11 figures, accepted for publication in A&A
MOESM2 of Identification of an immune signature predicting prognosis risk of patients in lung adenocarcinoma
Creators: name: Song, Qian
name: Shang, Jun
name: Zuyi Yang
name: Lanlin Zhang
name: Chufan Zhang
name: Jianing Chen
name: Xianghua Wu
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Computational Biology

description: Additional file 2: Table S2. The coefficient value of 30 immune related risk genes.
The interstellar medium of dwarf galaxies: new insights from Machine Learning analysis of emission line spectra
Creators: name: Ucci, Graziano
name: Ferrara, Andrea
name: Gallerani, Simona
name: Pallottini, Andrea
name: Cresci, Giovanni
name: Kehrig, Carolina
name: Hunt, Leslie K.
name: Vilchez, José M.
name: Vanzi, Leonardo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Dwarf galaxies are ideal laboratories to study the physics of the interstellar medium (ISM). Emission lines have been widely used to this aim. Retrieving the full information encoded in the spectra is therefore essential. This can be efficiently and reliably done using Machine Learning (ML) algorithms. Here, we apply the ML code GAME to MUSE (Multi Unit Spectroscopic Explorer) and PMAS (Potsdam Multi Aperture Spectrophotometer) Integral Field Unit (IFU) observations of two nearby Blue Compact Galaxies (BCGs): Henize 2-10 and IZw18. We derive spatially resolved maps of several key ISM physical properties. We find that both galaxies show a remarkably uniform metallicity distribution. Henize 2-10 is a star forming dominated galaxy, with a Star Formation Rate (SFR) of about 1.2 M$_{\odot}$ yr$^{-1}$. Henize 2-10 features dense and dusty ($A_V$ up to 5-7 mag) star forming central sites. We find IZw18 to be very metal-poor ($Z$= 1/20 $Z_{\odot}$). IZw18 has a strong interstellar radiation field, with a large ionization parameter. We also use models of PopIII stars spectral energy distribution as a possible ionizing source for the HeII $λ$4686 emission detected in the IZw18 NW component. We find that PopIII stars could provide a significant contribution to the line intensity. The upper limit to the PopIII star formation is 52% of the total IZw18 SFR.
description: 21 pages, 21 figures. Accepted for publication in MNRAS
Tests of Conformal Invariance in Randomness Induced Second-Order Phase Transitions
Creators: name: Chatelain, Christophe
name: Berche, Bertrand
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: The conformal covariance of correlation functions is checked in the second-order transition induced by random bonds in the two-dimensional 8-state Potts model. The decay of correlations is obtained {\it via} transfer matrix calculations in a cylinder geometry, and large-scale Monte Carlo simulations give access to the correlations and the profiles inside a square with free or fixed boundary conditions, respectively. In both geometries, conformal transformations constrain the form of the spatial dependence, leading to accurate determinations of the order parameter scaling index in good agreement with previous independent determinations obtained through standard techniques. The energy density exponent is also computed.
description: LaTeX file with Revtex, 4 pages, 4 eps figures, to appear in Phys. Rev. E, minor corrections
High latitude Galactic dust emission in the BOOMERanG maps
Creators: name: Masi, S.
name: Ade, P. A. R.
name: Bock, J. J
name: Boscaleri, A.
name: Crill, B. P.
name: de Bernardis, P.
name: Giacometti, M.
name: Hivon, E.
name: Hristov, V. V.
name: Lange, A. E.
name: Mauskopf, P. D.
name: Montroy, T.
name: Netterfield, C. B.
name: Pascale, E.
name: Piacentini, F.
name: Prunet, S.
name: Ruhl, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present mm-wave observations obtained by the BOOMERanG experiment of Galactic emission at intermediate and high (b < -20 deg) Galactic latitudes. We find that this emission is well correlated with extrapolation of the IRAS-DIRBE maps, and is spectrally consistent with thermal emission from interstellar dust (ISD). The ISD brightness in the 410 GHz map has an angular power spectrum c_l = A l^{-beta} with 2 < beta < 3. At 150 GHz and at multipoles ell \sim 200 the angular power spectrum of the IRAS-correlated dust signal is estimated to be l(l+1)c_l/2 pi = (3.7 \pm 2.9) uK^2. This is negligible with respect to the CMB signal measured by the same experiment l(l+1)c_l/2 pi = (4700 \pm 540) uK^2. For the uncorrelated dust signal we set an upper limit to the contribution to the CMB power at 150GHz and l \sim 200 of l(l+1)c_l/2 pi < 3 uK^2 at 95% C.L. .
Brachypalpus laphriformis
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Brachypalpus
Brachypalpus laphriformis

description: Brachypalpus laphriformis (Fallén, 1816).
 (Merz 2001, Haenni 2010). [Vorher als Synonym von B. valgus (Panzer, [1798]) betrachtet (Maibach et al. 1992)].
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Shedding Light on Vehicular Communication: A Review of the Latest Vehicular Visible Light Communication Channel Models - Materials & Methods
Creators: name: Dotreppe, Guillaume
Publisher: name: Zenodo
Year: 2025
Subjects: V-VLC
Channel Modelling
Luminous Intensity Distribution
V2V
ITS

description: Materials & methods employed for the retrieval of relevant literature in the context of a survey on the channel modelling techniques for vehicular visible light communication.
UAV Base Station Location Optimization for Next Generation Wireless Networks: Overview and Future Research Directions
Creators: name: Cicek, Cihan Tugrul
name: Gultekin, Hakan
name: Tavli, Bulent
name: Yanikomeroglu, Halim
Publisher: name: arXiv
Year: 2018
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Unmanned aerial vehicles mounted base stations (UAV-BSs) are expected to become one of the significant components of the Next Generation Wireless Networks (NGWNs). Rapid deployment, mobility, higher chances of unobstructed propagation path, and flexibility features of UAV-BSs have attracted significant attention. Despite, potentially, high gains brought by UAV-BSs in NGWNs, many challenges are also introduced by them. Optimal location assignment to UAV-BSs, arguably, is the most widely investigated problem in the literature on UAV-BSs in NGWNs. This paper presents a comprehensive survey of the literature on the location optimization of UAV-BSs in NGWNs. A generic optimization framework through a universal Mixed Integer Non-Linear Programming (MINLP) formulation is constructed and the specifications of its constituents are elaborated. The generic problem is classified into a novel taxonomy. Due to the highly challenging nature of the optimization problem a range of solutions are adopted in the literature which are also covered under the aforementioned classification. Furthermore, future research directions on UAV-BS location optimization in 5G and beyond non-terrestrial aerial communication systems are discussed.
description: 1st IEEE Unmanned Vehicle Systems (UVS) Conference - Oman Feb.2019
MOESM1 of Identification of an immune signature predicting prognosis risk of patients in lung adenocarcinoma
Creators: name: Song, Qian
name: Shang, Jun
name: Zuyi Yang
name: Lanlin Zhang
name: Chufan Zhang
name: Jianing Chen
name: Xianghua Wu
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 1: Table S1.Â The gene lists of the 10 gene groups.
Trace and antitrace maps for aperiodic sequences, their extensions and applications
Creators: name: Wang, Xiaoguang
name: Grimm, Uwe
name: Schreiber, Michael
Publisher: name: arXiv
Year: 2000
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We study aperiodic systems based on substitution rules by means of a transfer-matrix approach. In addition to the well-known trace map, we investigate the so-called `antitrace' map, which is the corresponding map for the difference of the off-diagonal elements of the 2x2 transfer matrix. The antitrace maps are obtained for various binary, ternary and quaternary aperiodic sequences, such as the Fibonacci, Thue-Morse, period-doubling, Rudin-Shapiro sequences, and certain generalizations. For arbitrary substitution rules, we show that not only trace maps, but also antitrace maps exist. The dimension of the our antitrace map is r(r+1)/2, where r denotes the number of basic letters in the aperiodic sequence. Analogous maps for specific matrix elements of the transfer matrix can also be constructed, but the maps for the off-diagonal elements and for the difference of the diagonal elements coincide with the antitrace map. Thus, from the trace and antitrace map, we can determine any physical quantity related to the global transfer matrix of the system. As examples, we employ these dynamical maps to compute the transmission coefficients for optical multilayers, harmonic chains, and electronic systems.
description: 13 pages, REVTeX, now also includes applications to electronic systems, some references added
MusE GAs FLOw and Wind (MEGAFLOW) II. A study of gas accretion around $z\approx1$ star-forming galaxies with background quasars
Creators: name: Zabl, Johannes
name: Bouché, Nicolas F.
name: Schroetter, Ilane
name: Wendt, Martin
name: Finley, Hayley
name: Schaye, Joop
name: Conseil, Simon
name: Contini, Thierry
name: Marino, Raffaella A.
name: Mitchell, Peter
name: Muzahid, Sowgat
name: Pezzulli, Gabriele
name: Wisotzki, Lutz
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use the MusE GAs FLOw and Wind (MEGAFLOW) survey to study the kinematics of extended disk-like structures of cold gas around $z\approx1$ star-forming galaxies. The combination of VLT/MUSE and VLT/UVES observations allows us to connect the kinematics of the gas measured through MgII quasar absorption spectroscopy to the kinematics and orientation of the associated galaxies constrained through integral field spectroscopy. Confirming previous results, we find that the galaxy-absorber pairs of the MEGAFLOW survey follow a strong bimodal distribution, consistent with a picture of MgII absorption being predominantly present in outflow cones and extended disk-like structures. This allows us to select a bona-fide sample of galaxy-absorber pairs probing these disks for impact parameters of 10-70 kpc. We test the hypothesis that the disk-like gas is co-rotating with the galaxy disks, and find that for 7 out of 9 pairs the absorption velocity shares the sign of the disk velocity, disfavouring random orbits. We further show that the data are roughly consistent with inflow velocities and angular momenta predicted by simulations, and that the corresponding mass accretion rates are sufficient to balance the star formation rates.
description: 22 pages + Supplementary Appendix (15 pages); submitted to MNRAS; version after addressing referee's comments
Absolute Calibration of the DANCE Thermal Neutron Beam using Sodium Activation
Creators: name: Fischer, V.
name: Pagani, L.
name: Pickard, L.
name: Grant, C.
name: He, J.
name: Pantic, E.
name: Svoboda, R.
name: Ullmann, J.
name: Wang, J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The measurement of the neutron capture cross-section as a function of energy in the thermal range requires a precise knowledge of the absolute neutron flux. In this paper a new method of calibrating a thermal neutron beam using the controlled activation of sodium is described. The method is applied to the FP-14 Time Of Flight neutron beam line at the Los Alamos Neutron Science Center to calibrate the beam to a precision of $\pm5$%.
description: 12 pages, 3 figures, v2 is the version accepted for publication in NIM A
Decomposition of flood losses by environmental and economic drivers (FloodDrivers)
Creators: name: Paprotny, Dominik
Publisher: name: FID GEO
Year: 2025
Subjects: subject: Hydrology
subject: Floods
subject: Attribution
subject: Vulnerability
subject: Climate change

description: Final report for DFG project „Aufteilung von Hochwasserschäden auf Umwelt- und wirtschaftliche Faktoren" / „Decomposition of flood losses by environmental and economic drivers“ (FloodDrivers), project no. 449175973, reporting period 1 July 2021 - 30 June 2024.
The Nature of Turbulence in the Outer Regions of Protoplanetary Disks
Creators: name: Gole, Daniel A.
name: Simon, Jacob B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We carry out a series of local, shearing box simulations of the outer regions of protoplanetary disks, where ambipolar diffusion is important due to low ionization levels, to better characterize the nature of turbulence and angular momentum transport in these disks. These simulations are divided into two groups, one with far ultraviolet (FUV) ionization included, and one without FUV. In both cases, we explore a large range in diffusivity values. We find that in the simulations without FUV, the properties of the turbulence are similar to the unstratified simulations of Bai & Stone (2011); for a given diffusivity, the MRI can still be present so long as the magnetic field is sufficiently weak. Furthermore, the dynamics of the mid-plane in these simulations are primarily controlled by the MRI. In the FUV simulations on the other hand, the MRI-active FUV layers transport strong toroidal magnetic flux to the mid-plane, which shuts off the MRI. Instead, angular momentum transport at the mid-plane is dominated by laminar magnetic fields, resulting in lower levels of turbulent Maxwell stress compared to the no-FUV simulations. Finally, we perform a temporal correlation analysis on the FUV simulations, confirming our result that the dynamics in the mid-plane region is strongly controlled by the FUV-ionized layers.
description: 12 pages, 13 figures
Cheilosia pedestris Becker 1894
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Cheilosia
Cheilosia pedestris

description: Cheilosia pedestris Becker, 1894. (Claussen & Speight 2007).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Four-dimensional gonihedric gauge spin system
Creators: name: Ambjørn, J.
name: Koutsoumbas, G.
name: Savvidy, G. K.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We perform Monte Carlo simulations of a four-dimensional gauge invariant spin system which describes random surfaces with gonihedric action. We develop the analogy between the flat-crumpled phase transition of the lattice surface model and the liquid-gas phase transition of non-ideal gases, and identify the self-intersection coupling constant $k$ of the surface model with the pressure $P$. As $k$ increases the system moves to a critical point in complete analogy with the situation for non-ideal gases, where the liquid and the gas phases approach each other with increasing $P$. We measure vacuum expectation values of various operators and the corresponding critical indices.
description: 12 pages, Latex
Cheilosia rhodiolae Schmid 2000
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Cheilosia
Cheilosia rhodiolae

description: Cheilosia rhodiolae Schmid, 2000. (Schmid 2007).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
High-Resolution X-ray Spectroscopy and Modeling of the Absorbing and Emitting Outflow in NGC 3783
Creators: name: Kaspi, Shai
name: Brandt, W. N.
name: Netzer, Hagai
name: George, Ian M.
name: Chartas, George
name: Behar, Ehud
name: Sambruna, Rita M.
name: Garmire, Gordon P.
name: Nousek, John A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) The high-resolution X-ray spectrum of NGC 3783 shows several dozen absorption lines and a few emission lines from the H-like and He-like ions of O, Ne, Mg, Si, and S as well as from Fe XVII - Fe XXIII L-shell transitions. We have reanalyzed the Chandra HETGS spectrum using better flux and wavelength calibrations along with more robust methods. Combining several lines from each element, we clearly demonstrate the existence of the absorption lines and determine they are blueshifted relative to the systemic velocity by -610+/-130 km/s. We find the Ne absorption lines in the High Energy Grating spectrum to be resolved with FWHM=840{+490}{-360} km/s. We have used regions in the spectrum where no lines are expected to determine the X-ray continuum, and we model the absorption and emission lines using photoionized-plasma calculations. The model consists of two absorption components which have an order of magnitude difference in their ionization parameters. The two components are spherically outflowing from the AGN and thus contribute to both the absorption and the emission via P Cygni profiles. The model also clearly requires O VII and O VIII absorption edges. The low-ionization component of our model can plausibly produce UV absorption lines with equivalent widths consistent with those observed from NGC 3783. However, we note that this result is highly sensitive to the unobservable UV-to-X-ray continuum, and the available UV and X-ray observations cannot firmly establish the relationship between the UV and X-ray absorbers. We find good agreement between the Chandra spectrum and simultaneous ASCA and RXTE observations. We set an upper limit on the FWHM of the narrow Fe Kαemission line of 3250 km/s. This is consistent with this line originating outside the broad line region, possibly from a torus.
description: 17 pages, 9 figures included, Figure 1 in color, LaTeX emulateapj5.sty, accepted for publication by The Astrophysical Journal
Green Computer Science Millennial Students Examination
Creators: name: Abdillah, Leon Andretti
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Smartphones as one of information technology products have been affected higher education in various aspects. This article explains the useness of smartphones in facilitating online examination in information systems and computer science students. The research objective to be achieved by the researchers through the research, are as follows: 1) Utilizing smartphone as a media test online exam for green computing environment, 2) How to use social information technologies in online test, and 3) Explore the facilities or features that could be used for the online exam implementation. The observation was conducted with 100 students as respondents. Researcher used google forms to disseminate questions for online examination. The findings of the research showed that most the college students used Android OS for their online examination. Social technology like google forms has rich features in supporting online examination for computer science students. The use of smartphones, google forms, and facebook can create an atmosphere of modern, green computer science exams, efficient, and environmentally friendly.
description: The Third International Conference on Islamic Education, Information Technology and Media (ICIED2018), Universitas Islam Negeri (UIN) Maulana Malik Ibrahim, Malang
An update on the genetic population structure of the invasive ash dieback pathogen Hymenoscyphus fraxineus
Creators: name: Landa, Blanca B.
name: Pérez-Sierra, Ana
name: Vahideh Rafiei
name: Olivares, Concepción
name: Rees, Helen
name: Linde, Sietse Van Der
name: Keča, Nenad
name: Schwanda, Katharina
name: Venche Talgø
Publisher: name: Zenodo
Year: 2018

description: In this study 11 microsatellite markers (MM) were used to characterize the genetic structure
 and diversity of 111 new isolates obtained from nine locations (five of them with no
 previous MM information in Serbia and the UK) and compare them with a published dataset of
 1377 isolates from a total of 11 European countries, Russia and Japan.
Evidence for charm-bottom tetraquarks and the mass dependence of heavy-light tetraquark states from lattice QCD
Creators: name: Francis, Anthony
name: Hudspith, Renwick J.
name: Lewis, Randy
name: Maltman, Kim
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We continue our study of heavy-light four-quark states and find evidence from lattice QCD for the existence of a strong-interaction-stable $I(J^P)=0(1^+)$ $ud\bar{c}\bar{b}$ tetraquark with mass in the range of 15 to 61 MeV below $\bar{D}B^*$ threshold. Since this range includes the electromagnetic $\bar{D}Bγ$ decay threshold, current uncertainties do not allow us to determine whether such a state would decay electromagnetically, or only weakly. We also perform a study at fixed pion mass, with NRQCD for the heavy quarks, simulating $qq^\prime \bar{b}^\prime \bar{b}$ and $q q^\prime \bar{b}^\prime\bar{b}^\prime$ tetraquarks with $q,\, q^\prime =ud$ or $\ell s$ and variable, unphysical $m_{b^\prime}$ in order to investigate the heavy mass-dependence of such tetraquark states. We find that the dependence of the binding energy follows a phenomenologically-expected form and that, though NRQCD breaks down before $m_{b^\prime}=m_c$ is reached, the results at higher $m_{b^\prime}$ clearly identify the $ud\bar{b}^\prime \bar{b}$ channel as the most likely to support a strong-interaction-stable tetraquark state at $m_{b^\prime}=m_c$. This observation serves to motivate the direct $ud\bar{c}\bar{b}$ simulation. Throughout we use dynamical $n_f=2+1$ ensembles with pion masses $m_π=$415, 299, and 164 MeV reaching down almost to the physical point, a relativistic heavy quark prescription for the charm quark, and NRQCD for the bottom quark(s).
description: 24 pages, 4 figures
Finite-temperature ordering in two-dimensional magnets
Creators: name: Cuccoli, Alessandro
name: Tognetti, Valerio
name: Roscilde, Tommaso
name: Verrucchi, Paola
name: Vaia, Ruggero
Publisher: name: arXiv
Year: 2000
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study the two dimensional quantum Heisenberg antiferromagnet on the square lattice with easy-axis exchange anisotropy. By the semiclassical method called pure-quantum self-consistent harmonic approximation we analyse several thermodynamic quantities and investigate the existence of a finite temperature transition, possibly describing the low-temperature critical behaviour experimentally observed in many layered real compounds. We find that an Ising-like transition characterizes the model even when the anisotropy is of the order of $10^{-2}J$ ($J$ being the intra-layer exchange integral), as in most experimental situations. On the other hand, typical features of the isotropic Heisenberg model are observed for both values of anisotropy considered, one in the {\it quasi}-isotropic limit and the other in a more markedly easy-axis region. The good agreement found between our theoretical results and the experimental data relative to the real compound Rb$_2$MnF$_4$ shows that the insertion of the easy-axis exchange anisotropy, with quantum effects properly taken into account, provides a quantitative description and explanation of the experimental data, thus allowing to recognize in such anisotropy the main agent for the observed onset of finite temperature long-range order.
description: To appear on Phys. Rev. B
Cheilosia urbana
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Cheilosia
Cheilosia urbana

description: Cheilosia urbana (Meigen, 1822). (Claussen & Speight 1999).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Modèles de jeux sérieux collaboratifs et mobiles
Creators: name: Marfisi-Schottman, Iza
name: George, Sébastien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics Education (physics.ed-ph)
subject: FOS: Physical sciences

description: Mobile Collaborative Learning Games combine all the ingredients necessary to attract students' attention and engage them in learning activities. However, designing a coherent game scenario that combines mobility, game mechanics and collaborative learning is quite a challenge. In this article, we propose three game patterns that naturally integrate these mechanics in order to support educational goals.
description: in French
Soft modes, Gaps and Magnetization Plateaus in 1D Spin-1/2 Antiferromagnetic Heisenberg Models
Creators: name: Fledderjohann, A.
name: Gerhardt, C.
name: Karbach, M.
name: Mütter, K. -H.
name: Wießner, R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the one-dimensional spin-1/2 model with nearest and next-to-nearest-neighbor couplings exposed to a homogeneous magnetic field $h_{3}$ and a dimer field with period $q$ and strength $δ$. The latter generates a magnetization plateau at $M=(1-q/π)/2$, which evolves with strength $δ$ of the perturbation as $δ^ε$, where $ε=ε(h_{3},α)$ is related to the $η$-exponent which describes the critical behavior of the dimer structure factor, if the perturbation is switched of ($δ=0$). We also discuss the appearance of magnetization plateaus in ladder systems with $l$ legs.
description: to be published in Phys. Rev. B
Semi-supervised learning with Bidirectional GANs
Creators: name: Zamorski, Maciej
name: Zięba, Maciej
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Information Retrieval (cs.IR)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: In this work we introduce a novel approach to train Bidirectional Generative Adversarial Model (BiGAN) in a semi-supervised manner. The presented method utilizes triplet loss function as an additional component of the objective function used to train discriminative data representation in the latent space of the BiGAN model. This representation can be further used as a seed for generating artificial images, but also as a good feature embedding for classification and image retrieval tasks. We evaluate the quality of the proposed method in the two mentioned challenging tasks using two benchmark datasets: CIFAR10 and SVHN.
description: 12 pages, 3 figures
Criorhina pachymera
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Criorhina
Criorhina pachymera

description: Criorhina pachymera (Egger, 1858). (Dirickx & Obrecht 2007).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Additional file 1: of Psychosocial factors that mediate the association between mode of birth and maternal postnatal adjustment: findings from a population-based survey
Creators: name: Alderdice, Fiona
name: Henderson, Jane
name: Opondo, Charles
name: Lobel, Marci
name: Quigley, Maria
name: Redshaw, Maggie
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Developmental Biology
subject: Cancer

description: Table S1. a: Mediation by Perceived control of the association between mode of delivery and maternal adjustment. b: Mediation by Expectations of the association between mode of delivery and maternal adjustment. c: Mediation by Holding baby of the association between mode of delivery and maternal adjustment. d: Mediation by HCP support of the association between mode of delivery and maternal adjustment. (DOCX 28 kb)