cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
ERSFQ 8-bit Parallel Binary Shifter for Energy-Efficient Superconducting CPU
Creators: name: Kirichenko, A. F.
name: Kamkar, M. Y.
name: Walter, J.
name: Vernik, I. V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Hardware Architecture (cs.AR)
subject: FOS: Computer and information sciences

description: We have designed and tested a parallel 8-bit ERSFQ binary shifter that is one of the essential circuits in the design of the energy-efficient superconducting CPU. The binary shifter performs a bi-directional SHIFT instruction of an 8-bit argument. It consists of a bi-direction triple-port shift register controlled by two (left and right) shift pulse generators asynchronously generating a set number of shift pulses. At first clock cycle, an 8-bit word is loaded into the binary shifter and a 3-bit shift argument is loaded into the desired shift-pulse generator. Next, the generator produces the required number of shift SFQ pulses (from 0 to 7) asynchronously, with a repetition rate set by the internal generator delay of ~ 30 ps. These SFQ pulses are applied to the left (positive) or the right (negative) input of the binary shifter. Finally, after the shift operation is completed, the resulting 8-bit word goes to the parallel output. The complete 8-bit ERSFQ binary shifter, consisting of 820 Josephson junctions, was simulated and optimized using PSCAN2. It was fabricated in MIT Lincoln Lab 10-kA/cm2 SFQ5ee fabrication process with a high-kinetic inductance layer. We have successfully tested the binary shifter at both the LSB-to-MSB and MSB-to-LSB propagation regimes for all eight shift arguments. A single shift operation on a single input word demonstrated operational margins of +/-16% of the dc bias current. The correct functionality of the 8-bit ERSFQ binary shifter with the large, exhaustive data pattern was observed within +/-10% margins of the dc bias current. In this paper, we describe the design and present the test results for the ERSFQ 8-bit parallel binary shifter.
description: 4 pages, 6 figures, 22 references. Presented at Applied Superconductivity Conference 2018 (ASC 2018), Oct. 28 - Nov. 2, 2018, Seattle, WA, USA. Paper 1EOr1C-07
Eumerus uncipes Rondani 1850
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Eumerus
Eumerus uncipes

description: Eumerus uncipes Rondani, 1850. (Carron et al. 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 Perceived discrimination among older adults living in urban and rural areas in Brazil: a national study (ELSI-Brazil)
Creators: name: Braga, Luciana
name: Waleska Caiaffa
name: Ceolin, Ana
name: FabĂ­Ola Andrade
name: Lima-Costa, Maria
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Principal component analysis (PCA) on health status. A composite measure of the health status was obtained, based on PCA. The selected variables included self-rated health, number of the last 30â days spent in poor mental and/or physical health, and history of medical diagnosis from a list of 12 prevalent chronic diseases/conditions, such as hypertension, diabetes, depression and arthritis. The resulting health status score was divided into tertiles, representing individual with few health problems, some health problems and many health problems. (PDF 163 kb)
Photometric and kinematic studies of open star clusters. III. NGC 4103, NGC 5281, and NGC 4755
Creators: name: Sanner, Joerg
name: Brunzendorf, Jens
name: Will, Jean-Marie
name: Geffert, Michael
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present CCD photometry and proper motion studies of the three open star clusters NGC 4103, NGC 5281, and NGC 4755 (kappa Cru). By fitting isochrones to the colour magnitude diagrams, we found that all three objects are young open star clusters with ages of at most t=45 Myr. They are located at distances from approx. 1600 pc to 2200 pc, derived from distance moduli (m-M)_0 ranging from 11 mag to 12 mag. We combined membership determinations based on proper motions and statistical field star subtraction to derive the initial mass function (IMF) of the clusters. The shape of the IMFs could be represented by power laws with exponents of Gamma=-1.46 +/- 0.22 for NGC 4103, Gamma=-1.60 +/- 0.50 for NGC 5281, and Gamma=-1.68 +/- 0.14 for NGC 4755, when - as a reference - Salpeter's (1955) value would be Gamma=-1.35. These results agree well with other IMF studies of open star clusters.
description: 16 pages, 14 figures, accepted for publication in Astronomy & Astrophysics
Giant thermoemf in multiterminal superconductor/normal metal mesoscopic structures
Creators: name: Seviour, R.
name: Volkov, A. F.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We considered a mesoscopic superconductor/normal metal (S/N) structure in which the N reservoirs are maintained at different temperatures. It is shown that in the absence of current between the N reservoirs a voltage difference $V_{T}$ arises between the superconducting and normal conductors. The voltage $V_{T}$ oscillates with increasing phase difference $ϕ$ between the superconductors, and its magnitude does not depend on the small parameter $(T/ε_{F}).$
description: Resubmited, some changes to Text and Figures
Additional file 6: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: CFIR constructs represented within the different reviews. (DOCX 33 kb)
Fast and accurate object detection in high resolution 4K and 8K video using GPUs
Creators: name: Růžička, Vít
name: Franchetti, Franz
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Machine learning has celebrated a lot of achievements on computer vision tasks such as object detection, but the traditionally used models work with relatively low resolution images. The resolution of recording devices is gradually increasing and there is a rising need for new methods of processing high resolution data. We propose an attention pipeline method which uses two staged evaluation of each image or video frame under rough and refined resolution to limit the total number of necessary evaluations. For both stages, we make use of the fast object detection model YOLO v2. We have implemented our model in code, which distributes the work across GPUs. We maintain high accuracy while reaching the average performance of 3-6 fps on 4K video and 2 fps on 8K video.
description: 6 pages, 12 figures, Best Paper Finalist at IEEE High Performance Extreme Computing Conference (HPEC) 2018; copyright 2018 IEEE; (DOI will be filled when known)
Pipizella speighti Verlinden 1999
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Pipizella
Pipizella speighti

description: Pipizella speighti Verlinden, 1999. (van Steenis & Lucas 2011).
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
A geometric Morse-Novikov complex with infinite series coefficients
Creators: name: Laudenbach, François
name: Ferrandiz, Carlos Moraga
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: Let M be a closed n-dimensional manifold, n > 2, whose first real cohomology group H 1 (M ; R) is non-zero. We present a general method for constructing a Morse 1-form $α$ on M , closed but non-exact, and a pseudo-gradient X such that the differential $\partial$ X of the Novikov complex of the pair ($α$, X) has at least one incidence coefficient which is an infinite series. This is an application of our previous study of the homoclinic bifurcation of pseudo-gradients of multivalued Morse functions.
Epistrophe olgae Mutin 1999
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Epistrophe
Epistrophe olgae

description: Epistrophe olgae Mutin, 1999. (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
Additional file 2: of Personalized medicine with IgGAM compared with standard of care for treatment of peritonitis after infectious source control (the PEPPER trial): study protocol for a randomized controlled trial
Creators: name: Kalvelage, Christina
name: Zacharowski, Kai
name: Bauhofer, Artur
name: Gockel, Ulrich
name: Adamzik, Michael
name: Nierhaus, Axel
name: Kujath, Peter
name: Eckmann, Christian
name: Pletz, Mathias
name: Bracht, Hendrik
name: Tim-Philipp Simon
name: Winkler, Michael
name: Kindgen-Milles, Detlef
name: Albertsmeier, Markus
name: Weigand, Markus
name: BjĂśrn Ellger
name: Ragaller, Maximilian
name: Ullrich, Roman
name: Marx, Gernot
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: SPIRIT checklist (2013 version). (DOCX 48 kb)
ERSFQ 8-bit Parallel Arithmetic Logic Unit
Creators: name: Kirichenko, A. F.
name: Vernik, I. V.
name: Kamkar, M. Y.
name: Walter, J.
name: Miller, M.
name: Albu, L. R.
name: Mukhanov, O. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Hardware Architecture (cs.AR)
subject: FOS: Computer and information sciences

description: We have designed and tested a parallel 8-bit ERSFQ arithmetic logic unit (ALU). The ALU design employs wave-pipelined instruction execution and features modular bit-slice architecture that is easily extendable to any number of bits and adaptable to current recycling. A carry signal synchronized with an asynchronous instruction propagation provides the wave-pipeline operation of the ALU. The ALU instruction set consists of 14 arithmetical and logical instructions. It has been designed and simulated for operation up to a 10 GHz clock rate at the 10-kA/cm2 fabrication process. The ALU is embedded into a shift-register-based high-frequency testbed with on-chip clock generator to allow for comprehensive high frequency testing for all possible operands. The 8-bit ERSFQ ALU, comprising 6840 Josephson junctions, has been fabricated with MIT Lincoln Lab 10-kA/cm2 SFQ5ee fabrication process featuring eight Nb wiring layers and a high-kinetic inductance layer needed for ERSFQ technology. We evaluated the bias margins for all instructions and various operands at both low and high frequency clock. At low frequency, clock and all instruction propagation through ALU were observed with bias margins of +/-11% and +/-9%, respectively. Also at low speed, the ALU exhibited correct functionality for all arithmetical and logical instructions with +/-6% bias margins. We tested the 8-bit ALU for all instructions up to 2.8 GHz clock frequency.
description: 7 pages, 10 figures, 2 tables, 41 references. Presented at Applied Superconductivity Conference 2018 (ASC 2018), Oct. 28 - Nov. 2, 2018, Seattle, WA, USA. Paper 1EOr1C-06
Electronic and optical properties of spinel zinc ferrite: $Ab$ $initio$ hybrid functional calculations
Creators: name: Fritsch, Daniel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Spinel ferrites in general show a rich interplay of structural, electronic, and magnetic properties. Here, we particularly focus on zinc ferrite (ZFO), which has been observed experimentally to crystallise in the cubic $normal$ spinel structure. However, its magnetic ground state is still under dispute. In addition, some unusual magnetic properties in ZFO thin films or nanostructures have been explained by a possible partial cation inversion and a different magnetic interaction between the two cation sublattices of the spinel structure compared to the crystalline bulk material. Here, density functional theory has been applied to investigate the influence of different inversion degrees and magnetic couplings among the cation sublattices on the structural, electronic, magnetic, and optical properties. Effects of exchange and correlation have been modelled using the generalised gradient approximation (GGA) together with the Hubbard `+$U$' parameter, and the more elaborate hybrid functional PBE0. While the GGA+$U$ calculations yield an antiferromagnetically coupled $normal$ spinel structure as the ground state, in the PBE0 calculations the ferromagnetically coupled $normal$ spinel is energetically slightly favoured, and the hybrid functional calculations perform much better with respect to structural, electronic and optical properties.
description: 5 pages, 3 figures, 1 table
X-ray Power Density Spectrum of the Narrow Line Seyfert 1 Galaxy Akn 564
Creators: name: Pounds, Ken
name: Edelson, Rick
name: Markowitz, Alex
name: Vaughan, Simon
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Beginning in 1999 January, the bright, strongly variable Narrow-Line Seyfert 1 (NLS1) galaxy Akn 564 has been observed by RXTE once every ~4.3 days. It was also monitored every ~3.2 hr throughout 2000 July. These evenly-sampled observations have allowed the first quantitative comparison of long and short time-scale X-ray variability in an NLS1 and the derivation of an X-ray Power Density Spectrum (PDS). The variability amplitude in the short time-scale light curve is very similar to that in the long time-scale light curve, in marked contrast to the stronger variability on longer time-scales which is characteristic of "normal" broad-line Seyfert 1s (BLS1s). Furthermore, the Akn 564 PDS power law cuts off at a frequency of 8.7x10^-7 Hz corresponding to a timescale of ~13 d, significantly shorter than that seen in the PDS of NGC 3516, a BLS1 of comparable luminosity. This result is consistent with NLS1s showing faster (as opposed to larger amplitude) variations than BLS1s, providing further evidence that NLS1s harbour lower mass black holes than BLS1s of similar luminosity, accreting at a correspondingly higher relative rate.
description: Accepted for publication in ApJ
Spin and charge excitations in incommensurate spin density waves
Creators: name: Kaneshita, Eiji
name: Ichioka, Masanori
name: Machida, Kazushige
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Collective excitations both for spin- and charge-channels are investigated in incommensurate spin density wave (or stripe) states on two-dimensional Hubbard model. By random phase approximation, the dynamical susceptibility χ(q,ω) is calculated for full range of (q,ω) with including all higher harmonics components. An intricate landscape of the spectra in χ(q,ω) is obtained. We discuss the anisotropy of the dispersion cones for spin wave excitations, and for the phason excitation related to the motion of the stripe line. Inelastic neutron experiments on Cr and its alloys and stripe states of underdoped cuprates are proposed.
Additional file 1: of Personalized medicine with IgGAM compared with standard of care for treatment of peritonitis after infectious source control (the PEPPER trial): study protocol for a randomized controlled trial
Creators: name: Kalvelage, Christina
name: Zacharowski, Kai
name: Bauhofer, Artur
name: Gockel, Ulrich
name: Adamzik, Michael
name: Nierhaus, Axel
name: Kujath, Peter
name: Eckmann, Christian
name: Pletz, Mathias
name: Bracht, Hendrik
name: Tim-Philipp Simon
name: Winkler, Michael
name: Kindgen-Milles, Detlef
name: Albertsmeier, Markus
name: Weigand, Markus
name: BjĂśrn Ellger
name: Ragaller, Maximilian
name: Ullrich, Roman
name: Marx, Gernot
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: MOF score as modified by Lefering et al. [42]. (PDF 101 kb)
Melangyna barbifrons
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Melangyna
Melangyna barbifrons

description: Melangyna barbifrons (Fallén, 1817):
 1 ♀, Bonmont (VD), Sachet, 09.04.2011, leg. H. Boillat (MHNG). Neufund (det. B. Merz).
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
Computer simulations of the two-dimensional melting transition using hard disks
Creators: name: Jaster, Andreas
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present detailed Monte Carlo results for the two-dimensional melting transition of various systems up to N=65536 hard disks. The simulations are performed in the NVT ensemble, using a new updating scheme. In the isotropic phase the bond orientational correlation length xi_6 and the susceptibility chi_6 are measured and compared with the predictions of the Kosterlitz-Thouless-Halperin-Nelson-Young (KTHNY) theory. From the scaling relation of xi_6 and chi_6 we calculate the critical exponent eta_6. In the phase transition region we use finite-size scaling methods to locate the disclination binding transition point and compare the results with the values obtained from the behaviour in the isotropic phase. Additionally, we measure the topological defect density, the pressure and the distribution of the second moment of the local bond orientational order parameter. All results are in good agreement with the KTHNY theory, while a first-order phase transition with small correlation length and a one-stage continuous transition can be ruled out.
description: 18 pages, 12 figures
Additional file 2: of Single- versus double-layer closure of the caesarean (uterine) scar in the prevention of gynaecological symptoms in relation to niche development â the 2Close study: a multicentre randomised controlled trial
Creators: name: S. Stegwee
name: I. Jordans
name: L. Voet
name: M. Bongers
name: C. Groot
name: C. Lambalk
name: R. Leeuw
name: W. Hehenkamp
name: P. Ven
name: J. Bosmans
name: E. Pajkrt
name: E. Bakkum
name: C. Radder
name: M. Hemelaar
name: W. Baal
name: H. Visser
name: J. Laar
name: H. Vliet
name: R. Rijnders
name: M. Sueters
name: C. Janssen
name: W. Hermes
name: A. Feitsma
name: K. Kapiteijn
name: H. Scheepers
name: J. Langenveld
name: K. Boer
name: S. Coppus
name: D. Schippers
name: A. Oei
name: M. Kaplan
name: D. Papatsonis
name: L. Vleeschouwer
name: E. Beek
name: M. Bekker
name: A. Huisjes
name: W. Meijer
name: K. Deurloo
name: E. Boormans
name: H. Eijndhoven
name: J. Huirne
Publisher: name: figshare
Year: 2019
Subjects: subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Text of the online standardised instruction film for double-layer closure of the uterotomy. The spoken text in the online instruction film, which shows a standardised way to perform double-layer closure of the uterotomy, has been translated into English. (DOCX 15 kb)
Hunting for Galaxies and Halos in simulations with VELOCIraptor
Creators: name: Elahi, Pascal J.
name: Cañas, Rodrigo
name: Poulton, Rhys J. J.
name: Tobar, Rodrigo J.
name: Willis, James S.
name: Lagos, Claudia del P.
name: Power, Chris
name: Robotham, Aaron S. G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present VELOCIraptor, a massively parallel galaxy/(sub)halo finder that is also capable of robustly identifying tidally disrupted objects and separate stellar halos from galaxies. The code is written in c++11, use the MPI and OpenMP API's for parallelisation, and includes python tools to read/manipulate the data products produced. We demonstrate the power of the VELOCIraptor (sub)halo finder, showing how it can identify subhalos deep within the host that have negligible density contrasts to their parent halo. We find a subhalo mass-radial distance dependence: large subhalos with mass ratios of $\gtrsim10^{-2}$ are more common in the central regions that smaller subhalos, a result of dynamical friction and low tidal mass loss rates. This dependence is completely absent in (sub)halo finders in common use, which generally search for substructure in configuration space, yet is present in codes that track particles belonging to halos as they fall into other halos, such as HBT+. VELOCIraptor largely reproduces the dependence seen without tracking, finding a similar radial dependence to HBT+ in well resolved halos from our limited resolution fiducial simulation.
description: 22 pages in main text, 33 pages total, 15 figures, 4 tables. Accepted for publication in PASA. Code available from https://www.github/pelahi/VELOCIraptor-STF
Interpreting Debris from Satellite Disruption In External Galaxies
Creators: name: Johnston, Kathryn V.
name: Sackett, Penny D.
name: Bullock, James S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the detectability and interpretation of debris trails caused by satellite disruption in external galaxies using semi-analytic approximations for the dependence of streamer length, width and surface brightness on satellite and primary galaxy characteristics. The semi-analytic method is tested successfully against N-body simulations and then applied to three representative astronomical applications. First, we show how streamer properties can be used to estimate mass-to-light ratios $Υ$ and streamer ages of totally disrupted satellites, and apply the method to the stellar arc in NGC 5907. Second, we discuss how the lack of observed tidal debris around a satellite can provide an upper limit on its mass-loss rate, and, as an example, derive the implied limits on mass-loss rates for M32 and NGC 205 around Andromeda. Finally, we point out that a statistical analysis of streamer properties might be applied to test and refine cosmological models of hierarchical galaxy formation, and use the predicted debris from a standard $Λ$CDM realization to test the feasibility of such a study. Using the Local Group satellites and the few known examples of debris trails in the Galaxy and in external systems, we estimate that the best current techniques could characterize the brightest ($R < 29$ mag/ arcsec$^{2}$) portions of the youngest (3 dynamical periods) debris streamers. If systematics can be controlled, planned large-aperture telescopes such as CELT and OWL may allow fainter trails to be detected routinely and thus used for statistical studies such as those required for tests of galaxy formation.
description: 33 pages, 8 figures. Revised version, accepted for publication in ApJ
Quantum suppression of shot noise in atom-size metallic contacts
Creators: name: Brom, H. E. van den
name: van Ruitenbeek, J. M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The transmission of conductance modes in atom-size gold contacts is investigated by simultaneously measuring conductance and shot noise. The results give unambiguous evidence that the current in the smallest gold contacts is mostly carried by nearly fully transmitted modes. In particular, for a single-atom contact the contribution of additional modes is only a few percent. In contrast, the trivalent metal aluminum does not show this property.
description: Fig. 2 replaced, small errors corrected
Dark energy and the epoch of galaxy formation
Creators: name: Alcaniz, J. S.
name: Lima, J. A. S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The influence of a dark component on the first epoch of galaxy formation is analysed by using the ages of the three oldest high-redshift galaxies known in the literature. Our results, based on a spatially flat accelerated Universe driven by a "quintessence" component ($p_x = ωρ_x$), show that if the inferred ages of these objects are correct the first formation era is pushed back to extremely high redshifts. For the present best-fit quintessence model ($Ω_{x}= 0.7$, $ω< -0.6$), we find a lower bound of $z_f \geq 7.7$, whereas in the extreme case of $Λ$CDM model ($ω= -1$) the limit is slightly smaller ($z_f \geq 5.8$). The case for open cold dark matter models (OCDM) has also been discussed. For $Ω_m \simeq 0.3$, the formation redshift is restricted by $z_f \geq 18$. As a general result, if $Ω_m \geq 0.37$, these galaxies are not formed in FRW cosmologies with no dark energy since for all these cases $z_f \to \infty$.
description: 17 pages, 3 figures, Accepted for publication in Astrophysical Journal Letters
Scaling laws and vortex profiles in 2D decaying turbulence
Creators: name: Laval, Jean-Philippe
name: Chavanis, Pierre-Henri
name: Dubrulle, Bérengère
name: Sire, Clément
Publisher: name: arXiv
Year: 2000
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We use high resolution numerical simulations over several hundred of turnover times to study the influence of small scale dissipation onto vortex statistics in 2D decaying turbulence. A self-similar scaling regime is detected when the scaling laws are expressed in units of mean vorticity and integral scale, as predicted by Carnevale et al., and it is observed that viscous effects spoil this scaling regime. This scaling regime shows some trends toward that of the Kirchhoff model, for which a recent theory predicts a decay exponent $ξ=1$. In terms of scaled variables, the vortices have a similar profile close to a Fermi-Dirac distribution.
description: 4 Latex pages and 4 figures. Submitted to Phys. Rev. Lett
Xanthogramma dives
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Xanthogramma
Xanthogramma dives

description: Xanthogramma dives (Rondani, 1857). (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 5: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Computational Biology

description: Full presentation of constructs and subconstructs. (DOCX 536 kb)
Revealing environmental dependence of molecular gas content in a distant X-ray cluster at z=2.51
Creators: name: Wang, Tao
name: Elbaz, David
name: Daddi, Emanuele
name: Liu, Daizhong
name: Kodama, Tadayuki
name: Tanaka, Ichi
name: Schreiber, Corentin
name: Zanella, Anita
name: Valentino, Francesco
name: Sargent, Mark
name: Kohno, Kotaro
name: Xiao, Mengyuan
name: Pannella, Maurilio
name: Ciesla, Laure
name: Gobat, Raphael
name: Koyama, Yusei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a census of the molecular gas properties of galaxies in the most distant known X-ray cluster, CLJ1001, at z=2.51, using deep observations of CO(1-0) with JVLA. In total 14 cluster members with $M_{*} > 10^{10.5} M_{\odot}$ are detected, including all the massive star-forming members within the virial radius, providing the largest galaxy sample in a single cluster at $z > 2$ with CO(1-0) measurements. We find a large variety in the gas content of these cluster galaxies, which is correlated with their relative positions (or accretion states), with those closer to the cluster core being increasingly gas-poor. Moreover, despite their low gas content, the galaxies in the cluster center exhibit an elevated star formation efficiency (SFE=SFR/$M_{\rm gas}$) compared to field galaxies, suggesting that the suppression on the SFR is likely delayed compared to that on the gas content. Their gas depletion time is around $t_{\rm dep} \sim 400$ Myrs, comparable to the cluster dynamical time. This implies that they will likely consume all their gas within a single orbit around the cluster center, and form a passive cluster core by $z\sim2$. This result is one of the first direct pieces of evidence for the influence of environment on the gas reservoirs and SFE of $z > 2$ cluster galaxies, thereby providing new insights into the rapid formation and quenching of the most massive galaxies in the early universe.
description: accepted for publication in ApJ Letters
Spatial Diffusion of X-ray Emission Lines in the M87 Cooling Flow; Evidence for Absorption
Creators: name: Mathews, William G.
name: Buote, David A.
name: Brighenti, Fabrizio
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent XMM-Newton observations of the cooling flow gas in M87 indicate sharply decreasing oxygen, iron and silicon abundances within $\sim 5$ kpc of the galactic center. This result is unexpected since stellar mass loss and Type Ia supernovae are expected to produce pronounced central abundance maxima for all three elements. However, it has been suggested that many of the strong X-ray lines are optically thick and diffuse to larger radii in the cooling flow before escaping, falsifying the central abundances. We verify with radiation transfer calculations that this effect does indeed occur in the M87 cooling flow, but that it is insufficient to account for the M87 observations. We suggest that some source of continuous opacity is required to reduce the central X-ray line emission, perhaps by warm gas at $T \sim 10^5 - 10^6$ K. The radial surface brightness profiles of X-ray resonance lines are also sensitive to turbulence in cooling flows which reduces the line center optical depths considerably. Turbulence may provide sufficient energy to continuously heat the warm absorbing gas.
description: 4 pages (emulateapj5) with 2 figures; accepted by Astrophysical Journal Letters
Additional file 1: of Single- versus double-layer closure of the caesarean (uterine) scar in the prevention of gynaecological symptoms in relation to niche development â the 2Close study: a multicentre randomised controlled trial
Creators: name: S. Stegwee
name: I. Jordans
name: L. Voet
name: M. Bongers
name: C. Groot
name: C. Lambalk
name: R. Leeuw
name: W. Hehenkamp
name: P. Ven
name: J. Bosmans
name: E. Pajkrt
name: E. Bakkum
name: C. Radder
name: M. Hemelaar
name: W. Baal
name: H. Visser
name: J. Laar
name: H. Vliet
name: R. Rijnders
name: M. Sueters
name: C. Janssen
name: W. Hermes
name: A. Feitsma
name: K. Kapiteijn
name: H. Scheepers
name: J. Langenveld
name: K. Boer
name: S. Coppus
name: D. Schippers
name: A. Oei
name: M. Kaplan
name: D. Papatsonis
name: L. Vleeschouwer
name: E. Beek
name: M. Bekker
name: A. Huisjes
name: W. Meijer
name: K. Deurloo
name: E. Boormans
name: H. Eijndhoven
name: J. Huirne
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Affiliations of all 32 participating hospitals in the Netherlands that granted approval. The board of the hospitals granted approval to participate and to start recruiting patients. (DOCX 15 kb)
title: Finding fundamental operations in language acquisition: Formal features as triggers
Creators: name: Roeper, Thomas
Publisher: name: University of Massachusetts Amherst
Year: 1999

description: Roeper, T. (1999). Finding fundamental operations in language acquisition: Formal features as triggers. In B. Hollebrandse (Ed.), New perspectives on language acquisition (pp. 197-214). University of Massachusetts Occasional Papers (UMOP) 22. Amherst, MA: GLSA.
Xanthogramma stackelbergi Violovitsh 1975
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Syrphidae
Xanthogramma
Xanthogramma stackelbergi

description: Xanthogramma stackelbergi Violovitsh, 1975. (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 4: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Hematology

description: Full quality assessment results. (DOCX 83 kb)
Self-organized Beating and Swimming of Internally Driven Filaments
Creators: name: Camalet, S.
name: Julicher, F.
name: Prost, J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: We study a simple two-dimensional model for motion of an elastic filament subject to internally generated stresses and show that wave-like propagating shapes which can propel the filament can be induced by a self-organized mechanism via a dynamic instability. The resulting patterns of motion do not depend on the microscopic mechanism of the instability but only of the filament rigidity and hydrodynamic friction. Our results suggest that simplified systems, consisting only of molecular motors and filaments could be able to show beating motion and self-propulsion.
description: 8 pages, 2 figures, REVTeX
NSV 1440: First WZ Sge-type Object in AM CVn stars and candidates
Creators: name: Isogai, Keisuke
name: Kato, Taichi
name: Monard, Berto
name: Hambsch, Franz-Josef
name: Myers, Gordon
name: Starr, Peter
name: Cook, Lewis M.
name: Nogami, Daisaku
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In 2015 and 2017, the AM CVn candidate NSV 1440 showed superoutbursts having the characteristic features of WZ Sge-type dwarf novae (DNe). By analogy with hydrogen-rich cataclysmic variables (CVs), we can interpret these outbursts as `double superoutbursts' which are composed of the first superoutburst with early superhumps and the second superoutburst with ordinary superhumps. The object also showed multiple rebrightenings after the main superoutbursts. Early superhumps had been never observed in AM CVn stars and candidates, thus NSV 1440 is the first confirmed WZ Sge-type AM CVn candidate. We obtained the early superhump period of 0.0252329(49) d and the growing (stage A) superhumps period of 0.025679(20) d from the 2015 superoutburst. We regarded the early superhump period as the orbital one. By using these periods we estimated the mass ratio $q = $0.045(2). This value suggests that NSV 1440 is indeed an AM CVn star and that the secondary is a semi-degenerate star.
description: 24 pages, 6 figures, accepted for publication in PASJ
The European Large Area ISO Survey V: a BeppoSAX hard X-ray survey of the S1 region
Creators: name: Alexander, D. M.
name: La Franca, F.
name: Fiore, F.
name: Barcons, X.
name: Ciliegi, P.
name: Danese, L.
name: Della Ceca, R.
name: Franceschini, A.
name: Gruppioni, C.
name: Matt, G.
name: Matute, I.
name: Oliver, S.
name: Pompilio, F.
name: Wolter, A.
name: Efstathiou, A.
name: Heraudeau, P.
name: Perola, G. C.
name: Perri, M.
name: Rigopoulou, D.
name: Rowan-Robinson, M.
name: Serjeant, S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present BeppoSAX observations of the Southern S1 region in the European Large Area ISO Survey (ELAIS). These observations cover an area of ~1.7 sq. deg. and reach an on-axis (~0.7 sq. deg) 2-10 keV (HX) sensitivity of ~10E-13 cgs. This is the first HX analysis of an ISOCAM survey. We detect 9 sources with a signal to noise ratio SNR_HX>3, 4 additional sources with a 1.3 to 10 keV (T) SNR_T>3 and 2 additional sources which appear to be associated with QSOs with SNR_T>2.9. The number densities of the SNR_HX>3 sources are consistent with the ASCA and BeppoSAX logN-logS functions. Six BeppoSAX sources have reliable ISOCAM 15 micron counterparts within ~60 arcsec. All these ISOCAM sources have optical counterparts of R<20 mags. Five of these sources have been previously optically classified giving 4 QSOs and 1 BALQSO at z=2.2. The remaining unclassified source has X-ray and photometric properties consistent with that of a nearby Seyfert galaxy. One further HX source has a 2.6sigma ISOCAM counterpart associated with a galaxy at z=0.325. If this ISOCAM source is real, the HX/MIR properties suggest either an unusual QSO or a cD cluster galaxy. We have constructed MIR and HX spectral energy distributions to compute the expected HX/MIR ratios for these classes of objects up to z=3.2 and assess the HX/MIR survey depth. The BALQSO has an observed X-ray softness ratio and HX/MIR flux ratio similar to QSOs but different to those found for low redshift BALQSOs. This difference can be explained in terms of absorption, and suggests that high redshift BALQSOs should be comparatively easy to detect in the HX band, allowing their true fraction in the high redshift QSO population to be determined (ABRIDGED).
description: 27 pages (draft format), 10 figures, ApJ, in press (May 20 edition)
The Effects of Gravity on the Climate and Circulation of a Terrestrial Planet
Creators: name: Thomson, Stephen I.
name: Vallis, Geoffrey K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The climate and circulation of a terrestrial planet are governed by, among other things, the distance to its host star, its size, rotation rate, obliquity, atmospheric composition and gravity. Here we explore the effects of the last of these, the Newtonian gravitational acceleration, on its atmosphere and climate. We first demonstrate that if the atmosphere obeys the hydrostatic primitive equations, which are a very good approximation for most terrestrial atmospheres, and if the radiative forcing is unaltered, changes in gravity have no effect at all on the circulation except for a vertical rescaling. That is to say, the effects of gravity may be completely scaled away and the circulation is unaltered. However, if the atmosphere contains a dilute condensible that is radiatively active, such as water or methane, then an increase in gravity will generally lead to a cooling of the planet because the total path length of the condensible will be reduced as gravity increases, leading to a reduction in the greenhouse effect. Furthermore, the specific humidity will decrease, leading to changes in the moist adiabatic lapse rate, in the equator-to-pole heat transport, and in the surface energy balance because of changes in the sensible and latent fluxes. These effects are all demonstrated both by theoretical arguments and by numerical simulations with moist and dry general circulation models.
description: 17 pages, 9 figures. Submitted to QJRMS on 23/01/19
The Structure of a Quantized Vortex in a Bose-Einstein Condensate
Creators: name: Tang, Jian-Ming
Publisher: name: arXiv
Year: 2000
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The structure of a quantized vortex in a Bose-Einstein Condensate is investigated using the projection method developed by Peierls, Yoccoz, and Thouless. This method was invented to describe the collective motion of a many-body system beyond the mean-field approximation. The quantum fluctuation has been properly built into the variational wave function, and a vortex is described by a linear combination of Feynman wave functions weighted by a Gaussian distribution in their positions. In contrast to the solution of the Gross-Pitaevskii equation, the particle density is finite at the vortex axis and the vorticity is distributed in the core region.
description: LaTeX (JLTP style), 6 pages, 2 EPS figures, Procceding of International Symposium on Quantum Fluids and Solids 2000
Integration of Renewable Energy Resources into the Turkish Electricity System
Creators: name: Bulut, Mehmet
Publisher: name: Zenodo
Year: 2021
Subjects: Yenilenebilir Enerji Kaynakları, Türkiye, Elektrik Sistemi, Entegrasyon

description: Yenilenebilir Enerji Kaynaklarının Türkiye Elektrik Sistemine Entegrasyonu Dr. Mehmet BULUT In Book: MÜHENDİSLİK ALANINDA AKADEMİK ARAŞTIRMA ve DERLEMELER Chapter #5 Türkiye’nin birincil enerji tüketiminin en büyük payı yüzde 70 ile ithal petrol ve doğalgaza bağımlı bulunmaktadır. Bu dışa bağımlılıktan kurtulmak için yenilenebilir enerji kaynaklarına yönelik eğilim giderek artmaktadır. 2020 yılı sonu itibarıyla Türkiye’nin toplam kurulu gücü yaklaşık 96.270 MW değerine ulaşmıştır. Bu kapasitenin %27’si doğalgaz santralleri, %32’si hidroelektrik santralleri ve %9.3’ü ithal kömür santralları olmak üzere %21 linyit santrallerinden oluşmaktadır. Baraj tipi hidrolik dahil olmak üzere rüzgar, güneş, jeotermal ve biyokütle enerjine dayalı yenilenebilir enerji kaynaklarının kurulu güç kapasiteleri toplamda 49.577 MW olup bu oran toplam kurulu gücün %51,5’una denk gelmektedir. Bu durumda yenilenebilir enerji kaynaklarının payı toplam toplam kurulu gücün yarısından fazlasını oluşturmaktadır. Üretimde ise 2020 yılı geçici rakamlarına göre 129,5 milyar kWh elektrik enerjisi yenilenebilir enerji kaynaklarından elde edilmiş olup bu değer toplam 305,4 milyar kWh brüt üretimin yaklaşık %42,4’üne denk gelmektedir. Türkiye’nin elektrik talep projeksiyonlarına göre, talebi karşılamak için 2030 yılına kadar mevcut kurulu güce ek olarak yaklaşık 37.000 MW güç kapasitesine ihtiyaç vardır. Bu miktar mevcut kapasitenin %40’ına karşılık gelmektedir. Dolayısıyla güneş ve rüzgar enerjisinden beklenen gücün elde edilmesi hem yerli kaynakların değerlendirilmesine hem de emisyonların azaltılmasına büyük katkı sağlayacaktır. Bu çalışmada, özellikle hidroelektrik, güneş, rüzgar v.b yenilenebilir enerji kaynaklarının gelişimi incelenerek, Türkiye’nin elektrik şebekesine bağlanacak yenilenebilir enerji kaynaklarının entegrasyonuna ilişkin bir analiz yapılmıştır. Yenilenebilir elektrik üretim teknolojilerinin kurulu kapasitesindeki artış, özellikle rüzgar ve güneş enerjisinin artan payı Türkiye’nin elektrik sistemindeki durumu incelenmiştir. Önümüzdeki yıllarda Türkiye’nin elektrik kurulu gücünün ne kadarının yenilenebilir enerji kaynaklarından karşılanabileceği sorusuna cevap bulmak için bir analiz çalışması yapılmıştır.
description: Citation/Alıntı : Bulut M., (2021), Yenilenebilir Enerji Kaynaklarının Türkiye Elektrik Sistemine Entegrasyonu, Mühendislik Alanında Akademik Araştırma ve Derlemeler, Editör: Prof. Dr. Servet Soygüder, Sayfa: 71-91, Mayıs 2021, Duvar Yayınları, İzmir, Türkiye. ISBN: 978-625-7680-60-8
Additional file 2: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Hematology

description: Consolidated Framework for Implementation Research construct descriptions. (DOCX 21 kb)
Eudorylas pannonicus
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Pipunculidae
Eudorylas
Eudorylas pannonicus

description: Eudorylas pannonicus (Becker, 1897). (Dirickx & Merz 2012).
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
Multimodal Polynomial Fusion for Detecting Driver Distraction
Creators: name: Du, Yulun
name: Raman, Chirag
name: Black, Alan W
name: Morency, Louis-Philippe
name: Eskenazi, Maxine
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Distracted driving is deadly, claiming 3,477 lives in the U.S. in 2015 alone. Although there has been a considerable amount of research on modeling the distracted behavior of drivers under various conditions, accurate automatic detection using multiple modalities and especially the contribution of using the speech modality to improve accuracy has received little attention. This paper introduces a new multimodal dataset for distracted driving behavior and discusses automatic distraction detection using features from three modalities: facial expression, speech and car signals. Detailed multimodal feature analysis shows that adding more modalities monotonically increases the predictive accuracy of the model. Finally, a simple and effective multimodal fusion technique using a polynomial fusion layer shows superior distraction detection results compared to the baseline SVM and neural network models.
description: INTERSPEECH 2018