cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Fontanes Medien
Creators: name: Trilcke, Peer
name: Parr, Rolf
name: D’Aprile, Iwan-Michelangelo
name: Kraus, Hans-Christof
name: Blomqvist, Clarissa
name: McGillen, Petra S.
name: Aus der Au, Carmen
name: Phillips, Alexander Robert
name: Helmer, Debora
name: Singer, Rüdiger
name: Görner, Rüdiger
name: Berbig, Roland
name: Rose, Dirk
name: Wilhelms, Kerstin
name: Krause, Marcus
name: Hehle, Christine
name: Gretz, Daniela
name: Gfrereis, Heike
name: Lepp, Nicola
name: Morlok, Franziska
name: Haut, Gideon
name: Brechenmacher, Thomas
name: Stauffer, Isabelle
name: Lyon, John B.
name: Bachmann, Vera
name: Ewert, Michael
name: Immer, Nikolas
name: Vedder, Ulrike
name: Fischer, Hubertus
name: Becker, Sabina
name: Wegmann, Christoph
name: Möller, Klaus-Peter
name: Schneider, Ulrike
name: Waszynski, Alexander
name: Wedel, Michael
name: Brehm, David
name: Wolpert, Georg
Publisher: name: Universität Potsdam
Year: 2023

description: Theodor Fontane war, im durchaus modernen Sinne, ein Medienarbeiter: Als Presse-Agent in London lernte er die innovativste Presselandschaft seiner Zeit kennen; als Redakteur in Berlin leistete er journalistische Kärrnerarbeit; er schrieb Kritiken über das Theater, die bildende Kunst und die Literatur – und auch seine Romane wie seine Reisebücher sind stets Medienprodukte, als Serien in in Zeitungen und Zeitschriften platziert, bevor sie auf dem Buchmarkt erschienen. Der vorliegende Band dokumentiert die Ergebnisse eines internationalen Kongresses, veranstaltet 2019 vom Theodor-Fontane-Archiv in Potsdam. Die ebenso rasante wie umfassende Medialisierung und Vernetzung der Gesellschaft im Laufe des 19. Jahrhunderts wird dabei als produktive Voraussetzung der schriftstellerischen Tätigkeit Fontanes begriffen. Eingebettet in ein weit verzweigtes Netz der Korrespondenz und der postalischen Textzirkulation, vertraut mit den Routinen und Publika der periodischen Massenpresse, für die er sein Leben lang schrieb, und auf vielfältige Weise geprägt von der visuellen Kultur seiner Zeit wird Theodor Fontane als gleichermaßen journalistisch versierter wie ästhetisch sensibler Grenzgänger erkennbar.
description: Zweitveröffentlichungen der Universität Potsdam : Philosophische Reihe; 178
Letter from Kathleen Raine to Herbert Read, August 29, [1949?-1965?]
Creators: name: Raine, Kathleen, 1908-2003
Publisher: name: University of Victoria Libraries
Year: 2023
Subjects: subject: Scholars
valueUri: http://id.worldcat.org/fast/1106878
subject: Authors
valueUri: http://id.worldcat.org/fast/821688
subject: Poets, English
valueUri: http://id.worldcat.org/fast/1067870
subject: Modernism (Literature)
valueUri: http://id.worldcat.org/fast/1024455
subject: Raine, Kathleen, 1908-2003
valueUri: http://id.worldcat.org/fast/52672
subject: Read, Herbert, 1893-1968
valueUri: http://id.worldcat.org/fast/1754386
subject: Anarchists
valueUri: http://id.worldcat.org/fast/808401
subject: Critics
valueUri: http://id.worldcat.org/fast/883769
subject: Philosophers, Modern
valueUri: http://id.worldcat.org/fast/1060765
subject: Art historians
valueUri: http://id.worldcat.org/fast/815554
subject: Authors, English--Correspondence
valueUri: http://id.worldcat.org/fast/821953
subject: Authors, English
valueUri: http://id.worldcat.org/fast/821945
subject: Literature, Modern
valueUri: http://id.worldcat.org/fast/1000172
subject: Philosophers
valueUri: http://id.worldcat.org/fast/1060746
subject: Poets
valueUri: http://id.worldcat.org/fast/1067778

description: Part of a collection of correspondence from Kathleen Raine to Herbert Read. Raine was a British scholar and poet who was awarded the Queen’s Gold Medal for Poetry in 1992. The correspondence here follows Raine’s work on a book about William Blake’s mythology. Other topics include discussion of philosophical and metaphysical subjects, and references to acquaintances in literary and arts circles. In this letter Raine gives an update on her Blake manuscript, sharing that she has written two chapters in Scotland, focusing on Blake's mythology.
Letter from Kathleen Raine to Herbert Read, October 22, [1949?-1965?]
Creators: name: Raine, Kathleen, 1908-2003
Publisher: name: University of Victoria Libraries
Year: 2023
Subjects: subject: Anarchists
valueUri: http://id.worldcat.org/fast/808401
subject: Authors, English--Correspondence
valueUri: http://id.worldcat.org/fast/821953
subject: Critics
valueUri: http://id.worldcat.org/fast/883769
subject: Scholars
valueUri: http://id.worldcat.org/fast/1106878
subject: Literature, Modern
valueUri: http://id.worldcat.org/fast/1000172
subject: Authors
valueUri: http://id.worldcat.org/fast/821688
subject: Authors, English
valueUri: http://id.worldcat.org/fast/821945
subject: Read, Herbert, 1893-1968
valueUri: http://id.worldcat.org/fast/1754386
subject: Philosophers
valueUri: http://id.worldcat.org/fast/1060746
subject: Art historians
valueUri: http://id.worldcat.org/fast/815554
subject: Raine, Kathleen, 1908-2003
valueUri: http://id.worldcat.org/fast/52672
subject: Poets, English
valueUri: http://id.worldcat.org/fast/1067870
subject: Poets
valueUri: http://id.worldcat.org/fast/1067778
subject: Modernism (Literature)
valueUri: http://id.worldcat.org/fast/1024455
subject: Philosophers, Modern
valueUri: http://id.worldcat.org/fast/1060765

description: Part of a collection of correspondence from Kathleen Raine to Herbert Read. Raine was a British scholar and poet who was awarded the Queen’s Gold Medal for Poetry in 1992. The correspondence here follows Raine’s work on a book about William Blake’s mythology. Other topics include discussion of philosophical and metaphysical subjects, and references to acquaintances in literary and arts circles. In this letter, Raine declines Read's offer to send her to a Jungian analyst, saying that she is feeling slightly better and that financial concerns had added to her desolation. Raine also asks if Read might plead her case to get an extension for her William Blake manuscript.
Versatile electronic properties and exotic edge states in single-layer tetragonal silicon carbides
Creators: name: Yang, Chao
name: Xie, Yuee
name: Liu, Li-Min
name: Chen, Yuanping
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Three single-layer tetragonal silicon carbides (SiC), termed as T1,T2 and T3, are proposed by density functional theory (DFT) computations. Although the three structures have the same topological geometry, they show versatile electronic properties from semiconductor (T1), semimetal (T2) to metal (T3).The versatile properties are originated from the rich bonds between Si and C atoms. The nanoribbons of the three SiC also show interesting electronic properties. Especially, T1 nanoribbons possess exotic edge states, where electrons only distribute on one edge's silicon or carbon atoms. The band gaps of the T1 nanoribbons are constant because of no interaction between the edge states.
Emergence of massless Dirac quasiparticles in correlated hydrogenated graphene with broken sublattice symmetry
Creators: name: Seki, Kazuhiro
name: Shirakawa, Tomonori
name: Zhang, Qinfang
name: Li, Tao
name: Yunoki, Seiji
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Using the variational cluster approximation (VCA) and the cluster perturbation theory, we study the finite temperature phase diagram of a half-depleted periodic Anderson model on the honeycomb lattice at half filling for a model of graphone, i.e., single-side hydrogenated graphene. The ground state of this model is found to be ferromagnetic (FM) semi-metal. The spin wave dispersion in the FM state is linear in momentum at zero temperature but becomes quadratic at finite temperatures, implying that the FM state is fragile against thermal fluctuations. Indeed, our VCA calculations find that the paramagnetic (PM) state dominates the finite temperature phase diagram. More surprisingly, we find that massless Dirac quasiparticles with the linear energy dispersion emerge at the Fermi energy upon introducing the electron correlation $U$ at the impurity sites in the PM phase. The Dirac Fermi velocity is found to be highly correlated to the quasiparticle weight of the emergent massless Dirac quasiparticles at the Fermi energy and monotonically increases with $U$. These unexpected massless Dirac quasiparticles are also examined with the Hubbard-I approximation and the origin is discussed in terms of the spectral weight redistribution involving a large energy scale of $U$. Considering an effective quasiparticle Hamiltonian which reproduces the single-particle excitations obtained by the Hubbard-I approximation, we argue that the massless Dirac quasiparticles are protected by the electron correlation. Our finding is therefore the first example of the emergence of massless Dirac quasiparticles due to dynamical electron correlations without breaking any spatial symmetry. The experimental implications of our results for graphone as well as a graphene sheet on transition metal substrates are also briefly discussed.
description: 28 pages, 21 figures, to be published in Phys. Rev. B
Effect of Lipid Composition on the Atheroprotective Properties of HDL-Mimicking Micelles
Creators: name: Hong, K
name: Yu, M
name: Crowther, J
name: Mei, L
name: Olsen, K
name: Luo, Y
name: Chen, YE
name: Guo, Y
name: Schwendeman, A
Publisher: name: MDPI
Year: 2022
Subjects: atherosclerosis
high-density lipoproteins
lipid composition
micelle
nanoparticle

description: Atherosclerosis progression is driven by an imbalance of cholesterol and unresolved local inflammation in the arteries. The administration of recombinant apolipoprotein A-I (ApoA-I)-based high-density lipoprotein (HDL) nanoparticles has been used to reduce the size of atheroma and rescue inflammatory response in clinical studies. Because of the difficulty in producing large quantities of recombinant ApoA-I, here, we describe the preparation of phospholipid-based, ApoA-I-free micelles that structurally and functionally resemble HDL nanoparticles. Micelles were prepared using various phosphatidylcholine (PC) lipids combined with 1,2-distearoyl-sn-glycero-3-phosphoethanolamine-N-[azido(polyethylene glycol)-2000] (DSPE-PEG2k) to form nanoparticles of 15–30 nm in diameter. The impacts of PC composition and PEGylation on the anti-inflammatory activity, cholesterol efflux capacity, and cholesterol crystal dissolution potential of micelles were investigated in vitro. The effects of micelle composition on pharmacokinetics and cholesterol mobilization ability were evaluated in vivo in Sprague Dawley rats. The study shows that the composition of HDL-mimicking micelles impacts their overall atheroprotective properties and supports further investigation of micelles as a therapeutic for the treatment of atherosclerosis.
A low-surface energy carbon allotrope: the case for bcc-C6
Creators: name: Yin, Wen-Jin
name: Chen, Yuan-Ping
name: Xie, Yue-E.
name: Liu, Li-Min
name: Zhang, S. B.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Graphite may be viewed as a low-surface-energy carbon allotrope with little layer-layer interaction. Other low-surface-energy allotropes but with much stronger layer-layer interaction may also exist. Here, we report a first-principles prediction for one of the known carbon allotropes, bcc-C6 (a body centered carbon allotrope with six atoms per primitive unit) that should have exceptionally low-surface energy and little size dependence down to only a couple layer thickness. This unique property may explain the existence of the relatively-high-energy bcc-C6 during growth. The electronic properties of the bcc-C6thin layers can also be intriguing: the (111), (110), and (001) thin layers havedirect band gap, indirect band gap, and metallic character, respectively. The refrained chemical reactivity of the thin layers does not disappear after cleaving, as lithium-doped (Li-doped) 3-layers (111) has a noticeably increased binding energies of H2 molecules with a maximum storage capacity of 10.8 wt%.
Letter from Emmett L. Bennett Jr. to William B. Dinsmoor, February 22, 1950
Creators: name: Bennett, Emmett L.
Publisher: name: The University of Texas at Austin
Year: 1950
Subjects: Emmett L. Bennett, Jr. Collection
Emmett L. Bennett, Jr. Collection--Correspondence
Emmett L. Bennett, Jr. Collection--Correspondence--William B. Dinsmoor
IBM
Linear A
Linear B

description: Bennett, in response to an earlier letter from Dinsmoor, discusses the potential uses of IBM machines for investigating the Linear A and Linear B scripts , with particular interest on the results of what the IBM computers could reach if they can perform sign substitution within these scripts.
The SLUGGS survey: Exploring the globular cluster systems of the Leo II group and their global relationships
Creators: name: Kartha, Sreeja S.
name: Forbes, Duncan A.
name: Alabi, Adebusola B.
name: Brodie, Jean P.
name: Romanowsky, Aaron J.
name: Strader, Jay
name: Spitler, Lee R.
name: Jennings, Zachary G.
name: Roediger, Joel C.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an investigation of the globular cluster (GC) systems of NGC 3607 and NGC 3608 as part of the ongoing SLUGGS survey. We use wide-field imaging data from the Subaru telescope in the g, r, and i filters to analyse the radial density, colour and azimuthal distributions of both GC systems. With the complementary kinematic data obtained from the Keck II telescope, we measure the radial velocities of a total of 81 GCs. Our results show that the GC systems of NGC 3607 and NGC 3608 have a detectable spatial extent of ~ 15, and 13 galaxy effective radii, respectively. Both GC systems show a clear bimodal colour distribution. We detect a significant radial colour gradient for the GC subpopulations in both galaxies. NGC 3607 exhibits an overabundance of red GCs on the galaxy minor axis and NGC 3608 shows a misalignment in the GC subpopulation position angles with respect to the galaxy stellar component. With the aid of literature data, we discuss several relationships between the properties of GC systems and their host galaxies. A one-to-one relation between the ellipticities of red GCs and the galaxy stellar light emphasises the evolutionary similarities between them. In our sample of four slowly rotating galaxies with kinematically decoupled cores, we observe a higher ellipticity for the blue GC subpopulation than their red counterparts. Also, we notice the flattening of negative colour gradients for the blue GC subpopulations with increasing galaxy stellar mass. Finally, we discuss the formation scenarios associated with the blue GC subpopulation.
description: 25 pages, 20 figures and 8 tables. Accepted for publication in MNRAS
Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
Creators: name: Pürrer, Michael
Publisher: name: arXiv
Year: 2015
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: I provide a frequency domain reduced order model (ROM) for the aligned-spin effective-one-body (EOB) model "SEOBNRv2" for data analysis with second and third generation ground based gravitational wave (GW) detectors. SEOBNRv2 models the dominant mode of the GWs emitted by the coalescence of black hole (BH) binaries. The large physical parameter space (dimensionless spins $-1 \leq χ_i \leq 0.99$ and symmetric mass-ratios $0.01 \leq η\leq 0.25$) requires sophisticated reduced order modeling techniques, including patching in the parameter space and in frequency. I find that the time window over which the inspiral-plunge and the merger-ringdown waveform in SEOBNRv2 are connected is discontinuous when the spin of the deformed Kerr BH $χ=0.8$ or the symmetric mass-ratio $η\sim 0.083$. This discontinuity increases resolution requirements for the ROM. The ROM can be used for compact binary systems with total masses of $2 M_\odot$ or higher for the advanced LIGO (aLIGO) design sensitivity and a $10$ Hz lower cutoff frequency. The ROM has a worst mismatch against SEOBNRv2 of $\sim 1\%$, but in general mismatches are better than $\sim 0.1\%$. The ROM is crucial for key data analysis applications for compact binaries, such as GW searches and parameter estimation carried out within the LIGO Scientific Collaboration (LSC).
description: 14 pages, 14 figures
Letter from Kathleen Raine to Herbert Read, March, [1949?-1965?]
Creators: name: Raine, Kathleen, 1908-2003
Publisher: name: University of Victoria Libraries
Year: 2023
Subjects: subject: Poets
valueUri: http://id.worldcat.org/fast/1067778
subject: Authors
valueUri: http://id.worldcat.org/fast/821688
subject: Critics
valueUri: http://id.worldcat.org/fast/883769
subject: Scholars
valueUri: http://id.worldcat.org/fast/1106878
subject: Read, Herbert, 1893-1968
valueUri: http://id.worldcat.org/fast/1754386
subject: Authors, English--Correspondence
valueUri: http://id.worldcat.org/fast/821953
subject: Modernism (Literature)
valueUri: http://id.worldcat.org/fast/1024455
subject: Philosophers
valueUri: http://id.worldcat.org/fast/1060746
subject: Philosophers, Modern
valueUri: http://id.worldcat.org/fast/1060765
subject: Anarchists
valueUri: http://id.worldcat.org/fast/808401
subject: Art historians
valueUri: http://id.worldcat.org/fast/815554
subject: Raine, Kathleen, 1908-2003
valueUri: http://id.worldcat.org/fast/52672
subject: Poets, English
valueUri: http://id.worldcat.org/fast/1067870
subject: Literature, Modern
valueUri: http://id.worldcat.org/fast/1000172
subject: Authors, English
valueUri: http://id.worldcat.org/fast/821945

description: Part of a collection of correspondence from Kathleen Raine to Herbert Read. Raine was a British scholar and poet who was awarded the Queen’s Gold Medal for Poetry in 1992. The correspondence here follows Raine’s work on a book about William Blake’s mythology. Other topics include discussion of philosophical and metaphysical subjects, and references to acquaintances in literary and arts circles. In this letter, Raine writes about the poetry of Ned O'Gorman, comparing it to that of Dylan Thomas. She goes on to discuss other contemporary writers and their work.
Effect of GRB spectra on the empirical luminosity correlations and the GRB Hubble diagram
Creators: name: Lin, Hai-Nan
name: Li, Xin
name: Chang, Zhe
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The spectra of gamma-ray bursts (GRBs) in a wide energy range can usually be well described by the Band function, which is a two smoothly jointed power laws cutting at a breaking energy. Below the breaking energy, the Band function reduces to a cut-off power law, while above the breaking energy it is a simple power law. However, for some detectors (such as the Swift-BAT) whose working energy is well below or just near the breaking energy, the observed spectra can be fitted to cut-off power law with enough precision. Besides, since the energy band of Swift-BAT is very narrow, the spectra of most GRBs can be fitted well even using a simple power law. In this paper, with the most up-to-date sample of Swift-BAT GRBs, we study the effect of different spectral models on the empirical luminosity correlations, and further investigate the effect on the reconstruction of GRB Hubble diagram. We mainly focus on two luminosity correlations, i.e., the Amati relation and Yonetoku relation. We calculate these two luminosity correlations on both the case that the GRB spectra are modeled by Band function and cut-off power law. It is found that both luminosity correlations only moderately depend on the choice of GRB spectra. Monte Carlo simulations show that Amati relation is insensitive to the high-energy power-law index of the Band function. As a result, the GRB Hubble diagram calibrated using luminosity correlations is almost independent on the GRB spectra.
description: 13 pages, 7 figures, 5 tables, accepted by MNRAS
Extracting the Kaon Collins function from $e^+e^-$ hadron pair production data
Creators: name: Anselmino, M.
name: Boglione, M.
name: D'Alesio, U.
name: Hernandez, J. O. Gonzalez
name: Melis, S.
name: Murgia, F.
name: Prokudin, A.
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The latest data released by the BaBar Collaboration on azimuthal correlations measured for pion-kaon and kaon-kaon pairs produced in $e^+e^-$ annihilations allow, for the first time, a direct extraction of the kaon Collins functions. These functions are then used to compute the kaon Collins asymmetries in Semi Inclusive Deep Inelastic Scattering processes, which result in good agreement with the measurements performed by the HERMES and COMPASS Collaborations.
description: 11 pages, 6 figures
Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
Creators: name: Soumagnac, M. T.
name: Barkana, R.
name: Sabiu, C. G.
name: Loeb, A.
name: Ross, A. J.
name: Abdalla, F. B.
name: Balan, S. T.
name: Lahav, O.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Baryon Acoustic Oscillations (BAOs) in the early Universe are predicted to leave an as yet undetected signature on the relative clustering of total mass versus luminous matter. A detection of this effect would provide an important confirmation of the standard cosmological paradigm and constrain alternatives to dark matter as well as non-standard fluctuations such as Compensated Isocurvature Perturbations (CIPs). We conduct the first observational search for this effect, by comparing the number-weighted and luminosity-weighted correlation functions, using the SDSS-III BOSS Data Release 10 CMASS sample. When including CIPs in our model, we formally obtain evidence at $3.2σ$ of the relative clustering signature and a limit that matches the existing upper limits on the amplitude of CIPs. However, various tests suggest that these results are not yet robust, perhaps due to systematic biases in the data. The method developed in this Letter, used with more accurate future data such as that from DESI, is likely to confirm or disprove our preliminary evidence.
description: 6 pages, 2 figures, accepted for publication in PRL
Code Sharing for Reuse and Reproducibility
Creators: name: Specht, Alison
name: Machicao, Jeaneth
name: Ben Abbes, Ali
name: Correa, Pedro
Publisher: name: Zenodo
Year: 2023
Subjects: reproducibiity
replicability
deep learning
experiments
remote sensing
open science

description: This presentation is the PARSEC-based contribution to a Birds of a Feather session at RDA P20 in March 2023. This session aimed to: discuss research software visibility highlight to the audience existing mechanisms to make code visible, and collect community input about other mechanisms and future coordinated actions. Our presentation focussed on the challenges related to achieving reproducibility and replicability of Deep Learning (DL) experiments, drawing on the developed protocol for checking the veracity of a DL paper published by Machicao et al. (2022) doi:10.1029/2022EA002379
description: This research is product of the PARSEC group funded by the Belmont Forum as part of its Collaborative Research Action (CRA) on Science-Driven e-Infrastructures Innovation (SEI), with funding from the Agence Nationale de Research (ANR), France, the Japan Science and Technology Agency (JST), the Sao Paulo Research Foundation (FAPESP) and the US National Science Foundation (NSF) grant number 1929464, with support from the synthesis centre CESAB of the French Foundation for Research on Biodiversity. The link to the session page is here: https://www.rd-alliance.org/coordinating-mechanisms-making-code-visible
The baryon cycle and how to study it
Creators: name: Wijers, Nastasha Anna
Publisher: name: Zenodo
Year: 2023
Subjects: circumgalactic medium
intra-group medium
baryon cycle
theory
simulations
multi-phase
galaxy halo
X-ray spectra
UV spectra

description: The circumgalactic medium and intra-group medium around galaxies with masses similar to or greater than that of our Milky Way, contain warm/hot gas at a temperature roughly predicted by the viral theorem. However, galaxy haloes also contain gas in a range of warm/hot temperatures close to the viral temperature, as well as a cooler and denser gas phase. This means that, in order to understand the content and properties of the halo gas, we need to study the different gas phases, which are typically best observed at different wavelengths. The cool phase has been observed, largely in UV absorption, but the warm/hot phase in haloes less massive than those of galaxy clusters has largely remained elusive in observations. This is because it produces absorption and emission lines primarily in the X-ray band, where instrument sensitivity has been a limiting factor. One consequence of this is that the mass and metal content of the halo gas are highly uncertain. Different cosmological simulations also predict very different halo gas masses. A major factor in these differences is that different prescriptions for supernova and AGN feedback in simulations can be tuned to produce realistic galaxy populations, but they can accomplish this with different effects on the halo gas. Observations of X-ray lines, which can shed more light on the warm/hot phase, will likely become possible with future instruments like the Athena X-IFU.
Parallel hybrid methods for generalized equilibrium problems and asymptotically strictly pseudocontractive mappings
Creators: name: Van Hieu, Dang
Publisher: name: arXiv
Year: 2016
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: In this paper, we propose two novel parallel hybrid methods for finding a common element of the set of solutions of a finite family of generalized equilibrium problems for monotone bifunctions $\left\{f_i\right\}_{i=1}^N$ and $α$ - inverse strongly monotone operators $\left\{A_i\right\}_{i=1}^N$ and the set of common fixed points of a finite family of (asymptotically) $κ$- strictly pseudocontractive mappings $\left\{S_j\right\}_{j=1}^M$ in Hilbert spaces. The strong convergence theorems are established under the standard assumptions imposed on equilibrium bifunctions and operators. A numerical example is presented to illustrate the efficiency of the proposed parallel methods.
description: 18 pages, Journal of Applied Mathematics and Computing (2016), Hybrid method, Equilibrium problem, Strictly pseudocontractive mapping, Parallel computation
"Unusual Rainbow and White Rainbow" A new auroral candidate in oriental historical sources
Creators: name: Hayakawa, Hisashi
name: Isobe, Hiroaki
name: Kawamura, Akito Davis
name: Tamazawa, Harufumi
name: Miyahara, Hiroko
name: Kataoka, Ryuho
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Solar activity has been recorded as auroras or sunspots in various historical sources. These records are of much importance for investigating both long-term solar activities and extremely intense solar flares. In previous studies, they were recorded as "vapor," "cloud," or "light," especially in oriental historical sources; however, the terminology was not discussed adequately and is still quite vague. In this paper, we suggest the possibility of "unusual rainbow" and "white rainbow" as candidates of historical auroras in oriental historical sources and examine if it is probable. This discovery will help us to make more comprehensive historical auroral catalogues and require us to add these terms to auroral candidates in oriental historical sources.
description: Accepted by Publ. Astron. Soc. Japan
The QWERTY effect on the web: How typing shapes the meaning of words in online human-computer interaction
Creators: name: Garcia, David
name: Strohmaier, Markus
Publisher: name: arXiv
Year: 2016
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: The QWERTY effect postulates that the keyboard layout influences word meanings by linking positivity to the use of the right hand and negativity to the use of the left hand. For example, previous research has established that words with more right hand letters are rated more positively than words with more left hand letters by human subjects in small scale experiments. In this paper, we perform large scale investigations of the QWERTY effect on the web. Using data from eleven web platforms related to products, movies, books, and videos, we conduct observational tests whether a hand-meaning relationship can be found in decoding text on the web. Furthermore, we investigate whether encoding text on the web exhibits the QWERTY effect as well, by analyzing the relationship between the text of online reviews and their star ratings in four additional datasets. Overall, we find robust evidence for the QWERTY effect both at the point of text interpretation (decoding) and at the point of text creation (encoding). We also find under which conditions the effect might not hold. Our findings have implications for any algorithmic method aiming to evaluate the meaning of words on the web, including for example semantic or sentiment analysis, and show the existence of "dactilar onomatopoeias" that shape the dynamics of word-meaning associations. To the best of our knowledge, this is the first work to reveal the extent to which the QWERTY effect exists in large scale human-computer interaction on the web.
description: In International WWW Conference, 2016. April 11-15, 2016, Montreal, Quebec, Canada. 978-1-4503-4143-1/16/04
Atomic structure and electronic properties of folded graphene nanoribbons: a first-principles study
Creators: name: Yin, Wenjin
name: Xie, Yuee
name: Liu, Li-Min
name: Chen, Yuanping
name: Wang, Ru-Zhi
name: Wei, Xiao-Lin
name: Lau, Leo
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The atomic structure, stacking sequences and electronic structure of folded graphene nanoribbons (FGNRs) are investigated by first-principles calculations. It reveals that the common configurations of all FGNRs are racket-like structures including a nanotube-like edge and two flat nanoribbons. Interestingly, the two flat nanoribbons can form new stacking styles instead of the most stable AB-stacking sequences for bilayer nanoribbons. The stability of the FGNRs are associated with several factors of initial structures, such as interlayer distance of two nanoribbons, stacking sequences, edge styles, and width of nanoribbons. These folded nanoribbons can only be thermodynamically stable when the width reaches about 61 Å and 95 Å for the zigzag and armchair nanoribbons, respectively. In addition, the band gap of the folded zigzag graphene nanoribbons becomes about 0.17 eV, which provides a new way to open the band gap.
Size evolution of star-forming galaxies with $2
Creators: name: Ribeiro, B.
name: Fèvre, O. Le
name: Tasca, L. A. M.
name: Lemaux, B. C.
name: Cassata, P.
name: Garilli, B.
name: Maccagni, D.
name: Zamorani, G.
name: Zucca, E.
name: Amorín, R.
name: Bardelli, S.
name: Fontana, A.
name: Giavalisco, M.
name: Hathi, N. P.
name: Koekemoer, A.
name: Pforr, J.
name: Tresse, L.
name: Dunlop, J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We measure galaxy sizes on a sample of $\sim1200$ galaxies with confirmed spectroscopic redshifts $2 \leq z_{spec} \leq 4.5$ in the VIMOS Ultra Deep Survey (VUDS), representative of star-forming galaxies with $i_\mathrm{AB} \leq 25$. We first derive galaxy sizes applying a classical parametric profile fitting method using GALFIT. We then measure the total pixel area covered by a galaxy above a given surface brightness threshold, which overcomes the difficulty of measuring sizes of galaxies with irregular shapes. We then compare the results obtained for the equivalent circularized radius enclosing 100\% of the measured galaxy light $r_T^{100}$ to those obtained with the effective radius $r_{e,\mathrm{circ}}$ measured with GALFIT. We find that the sizes of galaxies computed with our non-parametric approach span a large range but remain roughly constant on average with a median value $r_T^{100}\sim2.2$ kpc for galaxies with $2
description: 22 pages, 20 figures (+3 in appendix), submitted to A&A
Physical Resources for Quantum-enhanced Phase Estimation
Creators: name: Sahota, Jaspreet
name: Quesada, Nicolás
name: James, Daniel F. V.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the role of quantum entanglement (particle entanglement and mode entanglement) in optical phase estimation by employing the first and second quantization formalisms of quantum mechanics. The quantum Fisher information (QFI) is expressed as a function of the first and second order optical coherence functions. The resulting form of the QFI elucidates the deriving metrological resources for quantum phase estimation: field intensity and photon detection correlations. In addition, our analysis confirms that mode entanglement is not required for quantum-enhanced interferometry, whereas particle entanglement is a necessary requirement.
description: 8 pages, 2 figures, 2 tables
Contact Induced Spin Relaxation in Graphene Spin Valves with Al2O3 and MgO Tunnel Barriers
Creators: name: Amamou, Walid
name: Lin, Zhisheng
name: van Baren, Jeremiah
name: Turkyilmaz, Serol
name: Shi, Jing
name: Kawakami, Roland K.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate spin relaxation in graphene by systematically comparing the roles of spin absorption, other contact-induced effects (e.g. fringe fields, etc.), and bulk spin relaxation for graphene spin valves with MgO barriers, Al2O3 barriers, and transparent contacts. We obtain effective spin lifetimes by fitting the Hanle spin precession data with two models that include or exclude the effect of spin absorption. Results indicate that additional contact-induced spin relaxation other than spin absorption dominates the contact effect. For tunneling contacts, we find reasonable agreement between the two models with median discrepancy of ~20% for MgO and ~10% for Al2O3.
description: 21 pages, 4 figures
The extended epoch of galaxy formation: age dating of ~3600 galaxies with 2
Creators: name: Thomas, R.
name: Fèvre, O. Le
name: Scodeggio, M.
name: Cassata, P.
name: Garilli, B.
name: Brun, V. Le
name: Lemaux, B. C.
name: Maccagni, D.
name: Pforr, J.
name: Tasca, L. A. M.
name: Zamorani, G.
name: Bardelli, S.
name: Hathi, N. P.
name: Tresse, L.
name: Zucca, E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We aim at improving constraints on the epoch of galaxy formation by measuring the ages of 3597 galaxies with spectroscopic redshifts 22 the joint analysis of spectroscopy and photometry combined with restricted age possibilities when taking into account the age of the Universe substantially reduces systematic uncertainties and degeneracies in the age derivation. We find galaxy ages ranging from very young with a few tens of million years to substantially evolved with ages up to ~1.5-2 Gyr. The formation redshifts z_f derived from the measured ages indicate that galaxies may have started forming stars as early as z_f~15. We produce the formation redshift function (FzF), the number of galaxies per unit volume formed at a redshift z_f, and compare the FzF in increasing redshift bins finding a remarkably constant 'universal' FzF. The FzF is parametrized with (1+z)^ζ, with ζ~0.58+/-0.06, indicating a smooth 2 dex increase from z~15 to z~2. Remarkably this observed increase is of the same order as the observed rise in the star formation rate density (SFRD). The ratio of the SFRD with the FzF gives an average SFR per galaxy of ~7-17Msun/yr at z~4-6, in agreement with the measured SFR for galaxies at these redshifts. From the smooth rise in the FzF we infer that the period of galaxy formation extends from the highest possible redshifts that we can probe at z~15 down to redshifts z~2. This indicates that galaxy formation is a continuous process over cosmic time, with a higher number of galaxies forming at the peak in SFRD at z~2 than at earlier epochs. (Abridged)
description: Submitted to A&A, 24 pages
Optimal scan strategies for future CMB satellite experiments
Creators: name: Wallis, Christopher G. R.
name: Brown, Michael L.
name: Battye, Richard A.
name: Delabrouille, Jacques
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The B-mode polarisation power spectrum in the Cosmic Microwave Background (CMB) is about four orders of magnitude fainter than the CMB temperature power spectrum. Any instrumental imperfections that couple temperature fluctuations to B-mode polarisation must therefore be carefully controlled and/or removed. We investigate the role that a scan strategy can have in mitigating certain common systematics by averaging systematic errors down with many crossing angles. We present approximate analytic forms for the error on the recovered B-mode power spectrum that would result from differential gain, differential pointing and differential ellipticity for the case where two detector pairs are used in a polarisation experiment. We use these analytic predictions to search the parameter space of common satellite scan strategies in order to identify those features of a scan strategy that have most impact in mitigating systematic effects. As an example we go on to identify a scan strategy suitable for the CMB satellite proposed for the ESA M5 call. considering the practical considerations of fuel requirement, data rate and the relative orientation of the telescope to the earth. Having chosen a scan strategy we then go on to investigate the suitability of the scan strategy.
description: 21 pages, 11 figures, Comments welcome
Investigating the impact of differential facial emotion displays on dominance ratings in minimal acquaintance dynamic video material.
Creators: name: Störkel, Lisa
name: Valeriia Didushok
name: Langenstein, Michelle
name: Niedtfeld, Inga
Publisher: name: Open Science Framework
Year: 2024
Subjects: subject: Clinical Psychology
subject: Social and Behavioral Sciences
subject: Personality and Social Contexts
subject: Psychology
subject: FOS: Psychology
subject: Impression formation, minimal acquaintance, personality disorder, PID-5, assertiveness, dominance, emotional facial expression, social interaction, video material, thin slices paradigm

description: In this associated master thesis project on impression formation in a clinical sample with varying personality disorder (PD) severity, I want to investigate the effect of targets’ different facial emotion displays (anger, disgust, sadness, fear, happiness), quantified with an emotion recognition software, on dominance rated by unknown others in a minimal acquaintance digital meeting format, representing short social interactions. Moreover, the aim is to study first impressions of dominance with regard to pathological personality traits, and test in an exploratory manner whether differential emotion displays mediate the association between self-reported pathological personality traits of the target, more specifically the facet submissiveness, and dominance evaluations by unknown raters.
R-graphyne: a new two-dimension carbon allotrope with versatile Dirac-like point in nanoribbons
Creators: name: Yin, Wen-Jin
name: Xie, Yue-E
name: Liu, Li-Min
name: Wang, Ru-Zhi
name: Lau, Leo
name: Zhong, Jian-Xin
name: Chen, Yuan-Ping
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A novel two-dimensional carbon allotrope, rectangular graphyne (R-graphyne) with tetra-rings and acetylenic linkages, is proposed by first-principles calculations. Although the bulk R-graphyne exhibits metallic property, the nanoribbons of R-graphyne show distinct electronic structures from the bulk. The most intriguing feature is that band gaps of R-graphene nanoribbons oscillate between semiconductor and metal as a function of width. Particularly, the zigzag edge nanoribbons with half-integer repeating unit cell exhibits unexpected Dirac-like fermions in the band structures. The Dirac-like fermions of the R-graphyne nanoribbons originate from the central symmetry and two sub-lattices. The extraordinary properties of R-graphene nanoribbons greatly expand our understanding on the origin of Dirac-like point. Such findings uncover a novel fascinating property of nanoribbons, which may have broad potential applications for carbon-based nano-size electronic devices.
The VIMOS Ultra Deep Survey First Data Release: spectra and spectroscopic redshifts of 698 objects up to z~6 in CANDELS
Creators: name: Tasca, L. A. M.
name: Fevre, O. Le
name: Ribeiro, B.
name: Thomas, R.
name: Moreau, C.
name: Cassata, P.
name: Garilli, B.
name: Brun, V. Le
name: Lemaux, B. C.
name: Maccagni, D.
name: Pentericci, L.
name: Schaerer, D.
name: Vanzella, E.
name: Zamorani, G.
name: Zucca, E.
name: Amorin, R.
name: Bardelli, S.
name: Cassara, L. P.
name: Castellano, M.
name: Cimatti, A.
name: Cucciati, O.
name: Durkalec, A.
name: Fontana, A.
name: Giavalisco, M.
name: Grazian, A.
name: Hathi, N. P.
name: Ilbert, O.
name: Paltani, S.
name: Pforr, J.
name: Scodeggio, M.
name: Sommariva, V.
name: Talia, M.
name: Tresse, L.
name: Vergani, D.
name: Capak, P.
name: Charlot, S.
name: Contini, T.
name: de la Torre, S.
name: Dunlop, J.
name: Fotopoulou, S.
name: Guaita, L.
name: Koekemoer, A.
name: Lopez-Sanjuan, C.
name: Mellier, Y.
name: Salvato, M.
name: Scoville, N.
name: Taniguchi, Y.
name: Wang, P. W.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This paper describes the first data release (DR1) of the VIMOS Ultra Deep Survey (VUDS). The DR1 includes all low-resolution spectroscopic data obtained in 276.9 arcmin2 of the CANDELS-COSMOS and CANDELS-ECFDS survey areas, including accurate spectroscopic redshifts z_spec and individual spectra obtained with VIMOS on the ESO-VLT. A total of 698 objects have a measured redshift, with 677 galaxies, two type-I AGN and a small number of 19 contaminating stars. The targets of the spectroscopic survey are selected primarily on the basis of their photometric redshifts to ensure a broad population coverage. About 500 galaxies have z_spec>2, 48 with z_spec>4, and the highest reliable redshifts reach beyond z_spec=6. This dataset approximately doubles the number of galaxies with spectroscopic redshifts at z>3 in these fields. We discuss the general properties of the sample in terms of the spectroscopic redshift distribution, the distribution of Lyman-alpha equivalent widths, and physical properties including stellar masses M_star and star formation rates (SFR) derived from spectral energy distribution fitting with the knowledge of z_spec. We highlight the properties of the most massive star-forming galaxies, noting the large range in spectral properties, with Lyman-alpha in emission or in absorption, and in imaging properties with compact, multi-component or pair morphologies. We present the catalogue database and data products. All data are publicly available and can be retrieved from a dedicated query-based database available at http://cesam.lam.fr/vuds.
description: 11 pages, 6 figures, submitted to A&A
A new insight into neutrino energy loss by electron capture of iron group nuclei in magnetars surface
Creators: name: Liu, Jing-Jing
name: Gu, Wei-Min
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Based on the relativistic mean-field effective interactions theory, and Lai dong model \citep{b37, b38, b39}, we discuss the influences of superstrong magnetic fields (SMFs) on electron Fermi energy, nuclear blinding energy, and single-particle level structure in magnetars surface. By using the method of Shell-Model Monte Carlo (SMMC), and the Random Phase Approximation (RPA) theory, we detailed analyze the neutrino energy loss rates(NELRs) by electron capture (EC) for iron group nuclei in SMFs.
description: 22 pages, 8 figures, accepted for publication in ApJS. arXiv admin note: text overlap with arXiv:astro-ph/0606674, arXiv:nucl-th/9707052, arXiv:nucl-th/9801012, arXiv:1505.07304 by other authors
Converse theorems: from the Riemann zeta function to the Selberg class
Creators: name: Perelli, Alberto
Publisher: name: arXiv
Year: 2016
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11F66, 11M41

description: This is an expanded version of the author's lecture at the XX Congresso U.M.I., held in Siena in September 2015. After a brief review of L-functions, we turn to the classical converse theorems of H.Hamburger, E.Hecke and A.Weil, and to some later developments. Finally we present several results on converse theorems in the framework of the Selberg class of L-functions.
description: 24 pages
Resonant splitting in periodic T-shape photonic waveguides
Creators: name: Yin, Wenjin
name: Yang, Kaike
name: Xie, Yuee
name: Ouyang, Tao
name: Chen, Yuanping
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Resonant splitting phenomena of photons in periodic T-shape waveguide structure are investigated by the Green's function method. It is found that, except for the (n-1)-fold resonant splitting in the low frequency region, (n-2)-fold resonant splitting occurs in the high frequency region of the transmission spectra. The (n-2)-fold resonant splitting peaks are induced by the high quasi-bound states where the photons are mainly localized in the constrictions rather than in the stubs. To this kind of quasi-bound state, the stub acts as a potential barrier rather than a well, which is the inverse of the case of the low quasi-bound states corresponding to the (n-1)-fold splitting peaks. These resonant peaks can be modulated by adjusting the periodic number and geometry of the waveguide structures.