cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 19 of Phylogenetic signal from rearrangements in 18 Anopheles species by joint scaffolding extant and ancestral genomes
Creators: name: Anselmetti, Yoann
name: Duchemin, Wandrille
name: Tannier, Eric
name: Chauve, Cedric
name: Sèverine Bérard
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Plant Biology
subject: Computational Biology

description: Table S3. Assembly statistics at various stages of the gene annotation step of validation protocol of ADseq (step 4 of Additional file 8: Figure S7). For each species and annotation step, table gives different assembly statistics (column2): the number of contigs in the assembly, the size of the assembly in bp and in gene number, the N50 statistics of the assembly in bp and in gene number (if available) and gene trees number corresponding to gene present in the assembly (for the two last columns). Column 3 (Initial assembly) corresponds to the assembly statistics of reference genomes. Columns 4-8 of upper and lower table corresponds to Minia assembly statistics at different filtering step respectively with 50% reads sampling and without reads sampling. Column “initial” corresponds to assembly in output of Minia algorithm assembly. Minia contigs are then mapped on reference genome to annotate gene of reference assembly on Minia contigs. Assembly statistics after filter1 corresponds to Minia contigs that have been mapped on reference assembly with an identity and a coverage >=90%. Filter2 consists to keep only contig with an unique optimal alignment (to avoid uncertainty in gene annotation). Column 7 corresponds to Minia assembly statistics after merging of Minia contigs overlapping a same gene (simulating RNA-seq scaffolding). Then last column corresponds to statistics after filter3 that consists to discard gene families of genes that have not been mapped on Minia contigs. (PDF 51 kb)
Radiative corrections to Higgs couplings with weak gauge bosons in custodial multi-Higgs models
Creators: name: Chiang, Cheng-Wei
name: Kuo, An-Li
name: Yagyu, Kei
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate 1-loop radiative corrections to the $hZZ$ and $hWW$ couplings in models with next--to--simplest Higgs sectors satisfying the electroweak $ρ$ parameter equal to 1 at tree level: the Higgs singlet model, the two-Higgs doublet models, and the Georgi-Machacek model. Under theoretical and current experimental constraints, the three models have different correlations between the deviations in the $hZZ$ and $hWW$ couplings from the standard model predictions. In particular, we find for each model predictions with no overlap with the other two models.
description: 5 pages, 1 figure
Probing the Metal Enrichment of the Intergalactic Medium at $z=5-6$ Using the Hubble Space Telescope
Creators: name: Cai, Zheng
name: Fan, Xiaohui
name: Dave, Romeel
name: Finlator, Kristian
name: Oppenheimer, Ben
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We test the galactic outflow model by probing associated galaxies of four strong intergalactic CIV absorbers at $z=5$--6 using the Hubble Space Telescope (HST) ACS ramp narrowband filters. The four strong CIV absorbers reside at $z=5.74$, $5.52$, $4.95$, and $4.87$, with column densities ranging from $N_{\rm{CIV}}=10^{13.8}$ cm$^{-2}$ to $10^{14.8}$ cm$^{-2}$. At $z=5.74$, we detect an i-dropout Ly$α$ emitter (LAE) candidate with a projected impact parameter of 42 physical kpc from the CIV absorber. This LAE candidate has a Ly$α$-based star formation rate (SFR$_{\rm{Lyα}}$) of 2 $M_\odot$ yr$^{-1}$ and a UV-based SFR of 4 $M_\odot$ yr$^{-1}$. Although we cannot completely rule out that this $i$-dropout emitter may be an [OII] interloper, its measured properties are consistent with the CIV powering galaxy at $z=5.74$. For CIV absorbers at $z=4.95$ and $z=4.87$, although we detect two LAE candidates with impact parameters of 160 kpc and 200 kpc, such distances are larger than that predicted from the simulations. Therefore we treat them as non-detections. For the system at $z=5.52$, we do not detect LAE candidates, placing a 3-$σ$ upper limit of SFR$_{\rm{Lyα}}\approx 1.5\ M_\odot$ yr$^{-1}$. In summary, in these four cases, we only detect one plausible CIV source at $z=5.74$. Combining the modest SFR of the one detection and the three non-detections, our HST observations strongly support that smaller galaxies (SFR$_{\rm{Lyα}} \lesssim 2\ M_\odot$ yr$^{-1}$) are main sources of intergalactic CIV absorbers, and such small galaxies play a major role in the metal enrichment of the intergalactic medium at $z\gtrsim5$.
description: Accepted for Publications in ApJL
Anion Exchange in II-VI Semiconducting Nanostructures via Atomic Templating
Creators: name: Agarwal, Rahul
name: Krook, Nadia M.
name: Ren, Ming-Liang
name: Tan, Liang Z.
name: Liu, Wenjing
name: Rappe, Andrew M.
name: Agarwal, Ritesh
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Controlled chemical transformation of nanostructures is a promising technique to obtain precisely designed novel materials which are difficult to synthesize otherwise. We report high-temperature vapor phase anion exchange reactions to chemically transform II-VI semiconductor nanostructures (100-300 nm length scale) while retaining the single crystallinity, crystal structure, morphology and even defect distribution of the parent material via atomic templating. The concept of atomic templating is employed to obtain kinetically controlled, thermodynamically metastable structural phases such as zincblende CdSe and CdS from zincblende CdTe upon complete chemical replacement of Te with Se or S. The underlying transformation mechanisms are explained through first-principles density functional theory calculations. Atomic templating is a unique path to independently tune materials phase and composition at the nanoscale allowing synthesis of novel materials.
Additional file 1: of Use of an electronic Partograph: feasibility and acceptability study in Zanzibar, Tanzania
Creators: name: Litwin, Lindsay Elizabeth
name: Maly, Christina
name: Khamis, Asma
name: Hiner, Cyndi
name: JĂŠrĂŠmie Zoungrana
name: Mohamed, Khadija
name: Drake, Mary
name: Machaku, Michael
name: Njozi, Mustafa
name: Salhiya Muhsin
name: Yusuph Kulindwa
name: Gomez, Patricia
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: ePartogram Development Process. Detailed information on the design process to develop the ePartogram from 2012 to 2015 (DOCX 22Â kb)
Self-Force in the Radiation Reaction Formula -- Adiabatic Approximation of a Metric Perturbation and an Orbit --
Creators: name: Mino, Yasushi
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We propose a new metric perturbation scheme under a possible constraint of the gauge conditions in which we obtain a physically expected prediction of the orbital evolution caused by the MiSaTaQuWa self-force. In this new scheme of a metric perturbation, an adiabatic approximation is applied to both the metric perturbation and the orbit. As a result, we are able to predict the gravitational evolution of the system in the so-called radiation reaction time scale, which is longer than the dephasing time scale. However, for gravitational wave detection by LISA, this may still be insufficient. We further consider a gauge transformation in this new metric perturbation scheme, and find a special gauge condition with which we can calculate the gravitational waveform of a time scale long enough for gravitational wave detection by LISA.
description: published in Progress of Theoretical Physics Vol.113 No.4 pp.733
Single photon generation by pulsed excitation of a single dipole
Creators: name: Brouri, Rosa
name: Beveratos, Alexios
name: Poizat, Jean-Philippe
name: Grangier, Philippe
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The fluorescence of a single dipole excited by an intense light pulse can lead to the generation of another light pulse containing a single photon. The influence of the duration and energy of the excitation pulse on the number of photons in the fluorescence pulse is studied. The case of a two-level dipole with strongly damped coherences is considered. The presence of a metastable state leading to shelving is also investigated.
description: 17 pages, 4 figures, submitted to PRA
Additional file 4: of Patient-directed self-management of pain (PaDSMaP) compared to treatment as usual following total knee replacement; a randomised controlled trial
Creators: name: Deane, Katherine
name: Gray, Richard
name: Balls, Paula
name: Darrah, Clare
name: Swift, Louise
name: Clark, Alan
name: Barton, Garry
name: Morris, Sophie
name: Butters, Sue
name: Bullough, Angela
name: Flaherty, Helen
name: Talbot, Barbara
name: Sanders, Mark
name: Donell, Simon
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Consent form for Patients in the PaDSMaP Study. (PDF 741 kb)
Additional file 2 of Genetic evidence of tri-genealogy hypothesis on the origin of ethnic minorities in Yunnan
Creators: name: Yang, Zhaoqing
name: Chen, Hao
name: Lu, Yan
name: Gao, Yang
name: Sun, Hao
name: Wang, Jiucun
name: Jin, Li
name: Chu, Jiayou
name: Xu, Shuhua
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2. Introduction of studied ethnic minorities.
Mapping the Cosmic Web with Ly-alpha Emission
Creators: name: Furlanetto, Steven
name: Schaye, Joop
name: Springel, Volker
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a high-resolution cosmological simulation to predict the distribution of HI Ly-alpha emission from the low-redshift (z<0.5) intergalactic medium (IGM). Our simulation can be used to reliably compute the emission from optically thin regions of the IGM but not that of self-shielded gas. We therefore consider several models that bracket the expected emission from self-shielded regions. Most galaxies are surrounded by extended (>10^2 kpc) ``coronae'' of optically thin gas with Ly-alpha surface brightness close to the expected background. Most of these regions contain smaller cores of dense, cool gas. Unless self-shielded gas is able to cool to T<10^4.1 K, these cores are much brighter than the background. The Ly-alpha coronae represent ``cooling flows'' of IGM gas accreting onto galaxies. We also estimate the number of Ly-alpha photons produced through the reprocessing of stellar ionizing radiation in the interstellar medium of galaxies; while this mechanism is responsible for the brightest Ly-alpha emission, it occurs on small physical scales and can be separated using high-resolution observations. In all cases, we find that Ly-alpha emitters are numerous (with a space density ~0.1 h^3 Mpc^-3) and closely trace the filamentary structure of the IGM, providing a new way to map gas inside the cosmic web.
description: 4 pages, 3 figures, accepted by ApJL
Conformally Flat Noncircular Spacetimes
Creators: name: Ayón-Beato, Eloy
name: Campuzano, Cuauhtemoc
name: García, Alberto
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The general metric for conformally flat stationary cyclic symmetric noncircular spacetimes is explicitly given. In spite of the complexity introduced by the inclusion of noncircular contributions, the related metric is derived via the full integration of the conformal flatness constraints. It is also shown that the conditions for the existence of a rotation axis (axisymmetry) are the same ones which restrict the above class of spacetimes to be static. As a consequence, a known theorem by Collinson is just part of a more general result: any conformally flat stationary cyclic symmetric spacetime, even a noncircular one, is additionally axisymmetric if and only if it is also static. Since recent astrophysical motivations point in the direction of considering noncircular configurations to describe magnetized neutron stars, the above results seem to be relevant in this context.
description: 7 pages
Observations of Cyanopolyynes toward Four High-Mass Star-Forming Regions Containing Hot Cores
Creators: name: Taniguchi, Kotomi
name: Saito, Masao
name: Hirota, Tomoya
name: Ozeki, Hiroyuki
name: Miyamoto, Yusuke
name: Kaneko, Hiroyuki
name: Minamidani, Tetsuhiro
name: Shimoikura, Tomomi
name: Nakamura, Fumitaka
name: Dobashi, Kazuhito
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We carried out line survey observations at the 26-30 GHz band toward the four high-mass star-forming regions containing hot cores, G10.30-0.15, G12.89+0.49, G16.86-2.16, and G28.28-0.36, with the Robert C. Byrd Green Bank Telescope. We have detected HC5N from all of the sources, and HC7N from the three sources, except for G10.30-0.15. We further conducted observations of HC5N at the 42-46 GHz and 82-103 GHz bands toward the three sources, G12.89+0.49, G16.86-2.16, and G28.28-0.36, with the Nobeyama 45 m radio telescope. The rotational lines of HC5N with the high excitation energies (Eu/k=63-100 K), which are hardly excited in the cold dark clouds, have been detected from the three sources. The rotational temperatures of HC5N are found to be 13-20 K in the three sources. The detection of the lines with the high excitation energies and the derived rotational temperatures indicate that HC5N exists in the warm gas within 0.07-0.1 pc radii around massive young stellar objects. The column densities of HC5N in the three sources are derived to be (2.0+-2.8)*10^(13) cm-2 . We compare the ratios between N(HC5N) the column density of HC5N and W(CH3OH) the integrated intensity of the thermal CH3OH emission line among the three high-mass star-forming regions. We found a possibility of the chemical differentiation in the three high-mass star-forming regions; G28.28-0.36 shows the largest N (HC5N)/W (CH3OH) ratio of > 8.0*10^(14) in units of (K km s-1 )-1 cm-2 , while G12.89+0.49 and G16.86-2.16 show the smaller values (~2*10^(13) ).
description: Accepted for publication in ApJ, 18 pages, 8 figures, 6 tables
Environmental Justice Matters: designing a WorkShop
Creators: name: Moses, Kevin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Air Pollutants
subject: Health Disparities
subject: Collection_Strategies
subject: High_School
subject: ReImagining_Education

description: Recording our Submission for a 45-minute WorkShop at Reimagining Education, Summer Institute, The Edmund W. Gordon Institute for Advanced Study 202503201600EST ... Teachers College, Columbia Univ., July 2025

Added version 202503250829EST

Added version 20250330

Our WorkShop Proposal was accepted 20250417.  

Added version 20250427
Kolophone digital - Digital Humanities Tools in der Anwendung
Creators: name: Berns, Nils
name: Christ, Andreas
name: Dahm, Margit
name: Diebel, Richard
name: Klemenz, Arne
Publisher: name: Zenodo
Year: 2024
Subjects: DHd2024
Posterpräsentation
Software
Datenbank
Mediävistik
Kolophon
Ediarum
IIIF
Sammlung
Kollaboration
Manuskript
virtuelle Forschungsumgebungen

description: Das Poster 'Kolophone digital' stellt den digitalen Workflow des DFG-geförderten Kieler Forschungsprojekts 'Kolophone in deutschsprachigen Handschriften des Mittelalters' vor. Auf Basis etablierter DH-Technologien wurde eine virtuelle Arbeitsumgebung implementiert, die den Forschenden eine systematische Erfassung und Erforschung von Kolophonen erlaubt. Im Fokus der Präsentation steht das Zusammenwirken der verschiedenen technischen Komponenten und fachlichen Domänen.
Additional file 18 of Phylogenetic signal from rearrangements in 18 Anopheles species by joint scaffolding extant and ancestral genomes
Creators: name: Anselmetti, Yoann
name: Duchemin, Wandrille
name: Tannier, Eric
name: Chauve, Cedric
name: Sèverine Bérard
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Table S2. Assembly statistics on the 18 Anopheles genomes. Statistics before before processing are displayed in columns 2-7 and after the pipeline to produce input data for the DeCoSTAR algorithm in columns 8-11 (see Additional file 3: Figure S2 for illustration of the data preprocessing step). For initial dataset assembly statistics, columns 2 and 3 present contigs number and N50 statistic in bp for all contigs in genome assemblies. In columns 4-7, only contigs with at least one gene are considered. Column 4 corresponds to contigs number with gene in reference assemblies. Columns 5 & 6 represent N50 statistics respectively in bp and in gene number. Column 7 represent the number of gene in reference genome assemblies. For genome assemblies used as input of DeCoSTAR, all contigs contains at least one gene. Column 8 gives the number of contigs after step 4 of Additional file 3: Figure S2. Columns 9 & 10 represent N50 statistics respectively in bp and in gene number. And column 11 represents the number of gene in genomes taken as input of DeCoSTAR. The input dataset of DeCoSTAR is composed of 14,940 gene trees (see Additional file 4: Figure S3 and Additional file 5: Figure S4 for more information on gene trees) and 68,876 gene adjacencies with sequence support (scaffolding gene adjacencies) (see Additional file 6: Figure S5 and Additional file 7: Figure S6 for more information on scaffolding adjacencies). (PDF 33 kb)
Environmental Justice Matters: designing a WorkShop
Creators: name: Moses, Kevin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Air Pollutants
subject: Health Disparities
subject: Collection_Strategies
subject: High_School
subject: ReImagining_Education

description: Recording our Submission for a 45-minute WorkShop at Reimagining Education, Summer Institute, The Edmund W. Gordon Institute for Advanced Study 202503201600EST ... Teachers College, Columbia Univ., July 2025
Enhanced electron dephasing in three-dimensional topological insulators
Creators: name: Liao, Jian
name: Ou, Yunbo
name: Liu, Haiwen
name: He, Ke
name: Ma, Xucun
name: Xue, Qi-Kun
name: Li, Yongqing
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Study of the dephasing in electronic systems is not only important for probing the nature of their ground states, but also crucial to harnessing the quantum coherence for information processing. In contrast to well-studied conventional metals and semiconductors, it remains unclear which mechanism is mainly responsible for electron dephasing in three-dimensional (3D) topological insulators (TIs). Here, we report on using weak antilocalization effect to measure the dephasing rates in highly tunable (Bi,Sb)$_2$Te$_3$ thin films. As the transport is varied from a bulk-conducting regime to surface-dominant transport, the dephasing rate is observed to evolve from a linear temperature dependence to a sublinear power-law dependence. While the former is consistent with the Nyquist electron-electron interactions commonly seen in ordinary 2D systems, the latter leads to enhanced electron dephasing at low temperatures and is attributed to the coupling between the surface states and the localized charge puddles in the bulk of 3D TIs.
description: 18 pages, 4 figures, supplemental information available upon request or visit the ncomms website
Advances in non-relativistic matter via complex Langevin approaches
Creators: name: Drut, J. E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The recent progress in understanding the mathematics of complex stochastic quantization, as well as its application to quantum chromodynamics in situations that have a complex phase problem (e.g. finite quark density, real time), has opened up an intriguing possibility for non-relativistic many-body physics which has so far remained largely unexplored. In this brief contribution, I review a few specific examples of advances in the characterization of the thermodynamics of non-relativistic matter in a variety of one-dimensional cases affected by the sign problem: repulsive interactions, finite polarization, finite mass imbalance, and projection to finite systems to obtain virial coefficients.
description: 7 pages, 4 figures. Proceedings of RPMBT19, Pohang, South Korea
Loading a continuous-wave atom laser by optical pumping techniques
Creators: name: Bhongale, Satyan
name: Holland, Murray
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Demonstrating that despite loss processes, Bose-Einstein condensates can be formed in steady state is a prerequisite for obtaining a coherent beam of atoms in a continuous-wave atom laser. In this paper we propose a method for loading atoms into the thermal component of a Bose condensed cloud confined in a magnetic trap. This method is aimed at allowing steady state dynamics to be achieved. The proposed scheme involves loading atoms into the conservative magnetic potential using the spontaneous emission of photons. We show that the probability for the reabsorption of these photons may be small .
description: 6 pages, 7 figures
Spin eigen-excitations of the magnetic skyrmion and problem of the effective mass
Creators: name: Kravchuk, Volodymyr P.
name: Sheka, Denis D.
name: Rößler, Ulrich K.
name: Brink, Jeroen van den
name: Gaididei, Yuri
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Properties of magnon modes localized on a ferromagnetic skyrmion are studied. Three types of possible asymptotic behavior of the modes eigenfrequencies are found for the case of large skyrmion radius $R_s$, namely $ω_0\sim R_s^{-2}$ for the breathing mode, $ω_{-|μ|}\sim R_s^{-1}$ and $ω_{|μ|}\sim R_s^{-3}$ for modes with negative and positive azimuthal quantum numbers, respectively. A number of properties of the magnon eigenfunctions are determined. This enables us to demonstrate that the skyrmion dynamics based on the traveling wave model is described by the massless Thiele equation.
description: 11 pages, 4 figures
Environmental Justice Matters: designing a WorkShop
Creators: name: Moses, Kevin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Air Pollutants
subject: Health Disparities
subject: Collection_Strategies
subject: High_School
subject: ReImagining_Education

description: Recording our Submission for a 45-minute WorkShop at Reimagining Education, Summer Institute, The Edmund W. Gordon Institute for Advanced Study 202503201600EST ... Teachers College, Columbia Univ., July 2025

Added version 202503250829EST
Paths on a website: research on customers’ online search and purchase behaviours using clickstream data
Creators: name: Guo, Boshuo
Publisher: name: Imperial College London
Year: 2018

description: This dissertation is comprised of three chapters studying customers’ online search and purchase behaviours using clickstream data collected from the context of air travel. The first chapter explores how choice overload effect influences customers’ purchase decisions under different time pressure conditions. Two studies yield two findings. The first finding is that larger choice sets result in purchase deferral, which is consistent with choice overload effects. Time pressure significantly moderates this effect, because more deferrals occur when the purchase deadline is further away. The second finding is that it is not the real, physical time passing per se that creates a sense of time pressure; instead, time pressure appears to be defined by customers’ perception of time limit, which moderates the choice overload effect by shifting customers’ regulatory focus. The second chapter develops the modelling approaches of using path data to predict purchases. We develop the concepts of two types of sequence of browsing behaviours: the sequence of search strategies and the sequence of viewing behaviours. We find that viewing behaviour is a better indicator of purchase tendencies. We develop the modelling approaches of predicting the next viewing behaviour and using this predicted viewing behaviour to predict the purchase probability. Our approach improves current methods of predicting purchases by overcoming two disadvantages: inflexibility in adaption to different websites and missing detailed information of customers’ behaviours. We provide managerial insights on customising information shown to customers according to predicted viewing behaviours in order to improve purchase conversion rates. The third chapter reveals the relationship between customers’ online search strategies and decision strategies. Our first finding is that the search strategy of filtering can be viewed as a decision strategy characterised by Elimination by aspects (EBA) strategy, while flexible searches can be viewed as a decision strategy featured by Satisficing strategy. Our second finding is that the goal-related variable has the predominate effect on choice of decision strategies in the studied context. Customers choose the decision strategy that can enable them to fulfil the goal of finding a good price, instead of the strategy that simplify the choice task.
Paradox of integration - mean field approach
Creators: name: Kulakowski, Krzysztof
name: Gronek, Piotr
name: Borzi, Alfio
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Recently a computational model has been proposed of the social integration, as described in sociological terms by Peter Blau. In this model, actors praise or critique each other, and these actions influence their social status and raise negative or positive emotions. The role of a self-deprecating strategy of actors with high social status has also been discussed there. Here we develop a mean field approach, where the active and passive roles (praising and being praised, etc.) are decoupled. The phase transition from friendly to hostile emotions has been reproduced, similarly to the previously applied purely computational approach. For both phases, we investigate the time dependence of the distribution of social status. There we observe a diffusive spread, which - after some transient time - appears to be limited from below or from above, depending on the phase. As a consequence, the mean status flows.
description: 9 pages, 1 figure
MOESM2 of Husbandâ s involvement with motherâ s awareness and knowledge of newborn danger signs in facility-based childbirth settings: a cross-sectional study from rural Bangladesh
Creators: name: Sojib Zaman
name: Rajat Gupta
name: Kibria, Gulam Al
name: Naznin Hossain
name: Md. Bulbul
name: Dewan Hoque
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2. Participants correctly identified the neonatal danger signs.
Environmental Justice Matters: designing a WorkShop
Creators: name: Moses, Kevin
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Air Pollutants
subject: Health Disparities
subject: Collection_Strategies
subject: High_School
subject: ReImagining_Education

description: Recording our Submission for a 45-minute WorkShop at Reimagining Education, Summer Institute, The Edmund W. Gordon Institute for Advanced Study 202503201600EST ... Teachers College, Columbia Univ., July 2025

Added version 202503250829EST

Added version 20250330
NIR Observations of the QSO 3C 48 Host Galaxy
Creators: name: Zuther, J.
name: Eckart, A.
name: Scharwaechter, J.
name: Krips, M.
name: Straubmeier, C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we present new near infrared (NIR) imaging and spectroscopic data of the quasar 3C 48 and its host galaxy. The data were obtained with the ESO-VLT camera ISAAC.We report the first detection of the apparent second nucleus 3C 48A about 100NE of the bright QSO nucleus in the NIR bands J, H, and Ks. 3C 48A is highly reddened with respect to the host, which could be due to warm dust, heated by enhanced star formation or by interstellar material intercepting the radio jet. In fact, all colors on the host galaxy are reddened by several magnitudes of visual extinction. Imaging and initial spectroscopy also reveal a stellar content of about 30% to the overall QSO-light in the NIR. These results are important input parameters for future models of the stellar populations by taking extinction into account.
description: 8 pages, 8 figures, accepted by A&A
Combining Aspects of Genetic Algorithms with Weighted Recommender Hybridization
Creators: name: Mueller, Juergen
Publisher: name: arXiv
Year: 2017
Subjects: subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Recommender systems are established means to inspire users to watch interesting movies, discover baby names, or read books. The recommendation quality further improves by combining the results of multiple recommendation algorithms using hybridization methods. In this paper, we focus on the task of combining unscored recommendations into a single ensemble. Our proposed method is inspired by genetic algorithms. It repeatedly selects items from the recommendations to create a population of items that will be used for the final ensemble. We compare our method with a weighted voting method and test the performance of both in a movie- and name-recommendation scenario. We were able to outperform the weighted method on both datasets by 20.3 % and 31.1 % and decreased the overall execution time by up to 19.9 %. Our results do not only propose a new kind of hybridization method, but introduce the field of recommender hybridization to further work with genetic algorithms.
description: 10 pages, 6 figures, 2 tables, iiWAS '17, December 4-6, 2017, Salzburg, Austria
Additional file 3: of Patient-directed self-management of pain (PaDSMaP) compared to treatment as usual following total knee replacement; a randomised controlled trial
Creators: name: Deane, Katherine
name: Gray, Richard
name: Balls, Paula
name: Darrah, Clare
name: Swift, Louise
name: Clark, Alan
name: Barton, Garry
name: Morris, Sophie
name: Butters, Sue
name: Bullough, Angela
name: Flaherty, Helen
name: Talbot, Barbara
name: Sanders, Mark
name: Donell, Simon
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Information Sheet for Patients in the PaDSMaP Study. (PDF 800 kb)
Experimental realization of a highly structured search algorithm
Creators: name: Zhu, Xiwen
name: Fang, Ximing
name: Feng, Mang
name: Du, Fei
name: Gao, Kelin
name: Mao, Xi'an
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The highly structured search algorithm proposed by Hogg[Phys.Rev.Lett. 80,2473(1998)] is implemented experimentally for the 1-SAT problem in a single search step by using nuclear magnetic resonance technique with two-qubit sample. It is the first demonstration of the Hogg's algorithm, and can be readily extended to solving 1-SAT problem for more qubits in one step if the appropriate samples possessing more qubits are experimentally feasible.
description: RevTex, 11 pages + 3 pages of figures
High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
Creators: name: Bromley, J. M.
name: Somerville, R. S.
name: Fabian, A. C.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the constraints on models of supermassive black hole (SMBH) and quasar formation obtainable from two recent observational developments: the discovery of luminous quasars at z~6, and estimates of the local mass density of SMBHs. If ~90 per cent of this mass was accreted at redshifts z<3, as suggested by the observed quasar luminosity functions, these joint constraints pose a challenge for models, which must account for the observed luminous quasar population at z~6 within a very limited `mass budget'. We investigate a class of models based within the hierarchical structure formation scenario, in which major mergers lead to black hole formation and fuelling, and the resulting quasars shine at their Eddington-limited rate until their fuel is exhausted. We show that the simplest such model, in which a constant fraction of the gas within the halo is accreted in each major merger, cannot satisfy both constraints simultaneously. When this model is normalized to reproduce the number density of luminous quasars at z~6, the mass budget is grossly exceeded due to an overabundance of lower mass SMBHs. We explore a range of modifications to the simple model designed to overcome this problem. We show that both constraints can be satisfied if the gas accretion fraction scales as a function of the halo virial velocity. Similar scalings have been proposed in order to reproduce the local M-sigma relation. Successful models can also be constructed by restricting the formation of seed black holes to redshifts above z~11.5 or to haloes above a velocity threshold ~55 km/s, or assuming that only a fraction of major mergers result in formation of a seed SMBH. (abridged)
description: 19 pages, 6 figures, 1 table. v2: Corrected references. v3: Extended Section 5.1, corrected Section 3.2, various other corrections and additions suggested by referee. Accepted by MNRAS in this form
Additional file 17 of Phylogenetic signal from rearrangements in 18 Anopheles species by joint scaffolding extant and ancestral genomes
Creators: name: Anselmetti, Yoann
name: Duchemin, Wandrille
name: Tannier, Eric
name: Chauve, Cedric
name: Sèverine Bérard
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Table S1. Summary of genome assemblies and sequencing data information. 16 on the 18 Anopheles species have been sequenced in [4] and data are available on the SRA database of the NCBI (see column 4 and 6 for BioProject and SRA ID). FASTQ files of paired sequencing data have been obtained with SRA-toolkit. After mapping of paired reads on reference genome assemblies (column 2), median insert size of libraries have been determined with package “CollectInsertSizeMetrics” of Picard Tools (v1.61) (column 7). Column “Library name” give information on the sequencing strategies employed in [4]. Where ’fragment’ library corresponds to a Paired-End library with an expected insert size of 180bp and FR orientation (→←). ’jump’ library corresponds to a Mate-Pair library with an insert size of 1.5kbp and RF orientation (←→). And ’fosill’ corresponds to a library generated from a pool of hundred mosquitoes to improve the scaffolding with an expected insert size around 38kbp and FR orientation (→←). Column 3 gives the ID of gene set used in this study. (PDF 38 kb)
Could There Be A Hole In Type Ia Supernovae?
Creators: name: Kasen, Daniel
name: Nugent, Peter
name: Thomas, R. C.
name: Wang, Lifan
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In the favored progenitor scenario, Type Ia supernovae arise from a white dwarf accreting material from a non-degenerate companion star. Soon after the white dwarf explodes, the ejected supernova material engulfs the companion star; two-dimensional hydrodynamical simulations by Marietta et. al. show that, in the interaction, the companion star carves out a conical hole of opening angle 30-40 degrees in the supernova ejecta. In this paper we use multi-dimensional Monte Carlo radiative transfer calculations to explore the observable consequences of an ejecta-hole asymmetry. We calculate the variation of the spectrum, luminosity, and polarization with viewing angle for the aspherical supernova near maximum light. We find that the supernova looks normal from almost all viewing angles except when one looks almost directly down the hole. In the latter case, one sees into the deeper, hotter layers of ejecta. The supernova is relatively brighter and has a peculiar spectrum characterized by more highly ionized species, weaker absorption features, and lower absorption velocities. The spectrum viewed down the hole is comparable to the class of SN 1991T-like supernovae. We consider how the ejecta-hole asymmetry may explain the current spectropolarimetric observations of SNe Ia, and suggest a few observational signatures of the geometry. Finally, we discuss the variety currently seen in observed SNe Ia and how an ejecta-hole asymmetry may fit in as one of several possible sources of diversity.
description: 11 pages, 9 figures, submitted to ApJ
MOESM1 of Husbandâ s involvement with motherâ s awareness and knowledge of newborn danger signs in facility-based childbirth settings: a cross-sectional study from rural Bangladesh
Creators: name: Sojib Zaman
name: Rajat Gupta
name: Kibria, Gulam Al
name: Naznin Hossain
name: Md. Bulbul
name: Dewan Hoque
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. Data collection tool and procedure.
НОВАЦИОННОЕ РАЗВИТИЕ И ПЕРСПЕКТИВЫ ЧЕЛОВЕКА В КНИГЕ «CОВА МИНЕРВЫ ВЫЛЕТАЕТ В СУМЕРКИ» В.А. КУТЫРЁВА
Creators: name: Алексей Станиславович Тимощук
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: традиция
субъективность
человек
феноменология почвы

description: Чем опасно умножение миров? Куда может завести преследование новых горизонтов инновационизма? Может ли контингентная фактичность заменить необходимость? Предмет исследования – монография В.А. Кутырёва «Cова Минервы вылетает в сумерки», вышедшая в 2018 г. Философия Кутырёва представлена как реактуализация узкого пути между агностициз-мом и технократизмом, реизмом и структурализмом. Выводы книги, как и всегда, – спасение Человека. Разница в деталях, если в прошлых работах нас спасали от техники, от пустоты, от прогресса, здесь он спасает от самоапокалипсиса, эсхатологической рукотворной трагедии. В статье даётся обзор основных сюжетов творчества автора: борьба естественного и искусст-венного, открытое vs. устойчивое общество, саморазвитие технонауки, угрозы гипермодерниз-ма и трансгуманизма, проблемы биотехнического конструирования постчеловека, перспективы консервативного философствования, оправдание бытия. Основу монографии составляют сле-дующие глубокие идеи: бытие есть благо; самоутверждение есть сущность каждого живого существа; вечное возвращение есть прочная платформа вместо прогрессивизма. В книге нашло отражение примордиальное понимание Хайдеггера как почвенника, по отношению к которому Гуссерль противопоставляется как умозрительный схоластик. Низовая традиционная поэзия сопротивляется абстрактному логоцентризму, где фактичность конкурирует с контингетно-стью. Кутырёв берёт реванш за Жан Жореса и Карл Маркса, Ф.М. Достоевского и Христа, пы-таясь противостоять холокосту традиционной предметной реальности и соответствующей ей метафизической философии. Человечество лепит образ хаоса, не обращая внимания на то, что образ мыслей намагничивает образ действий и фатализм телесно-предметного тем ближе, чем больше статей по спекулятивно-телесной нигитологии. Выводы: 1) хочешь понять Хайдег-гера – читай Кутырёва; 2) бытие есть благо, 3) вечное возвращение есть более прочная плат-форма вместо безрассудного прогрессивизма.
Distribution-Free One-Pass Learning
Creators: name: Zhao, Peng
name: Zhou, Zhi-Hua
Publisher: name: arXiv
Year: 2017
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: In many large-scale machine learning applications, data are accumulated with time, and thus, an appropriate model should be able to update in an online paradigm. Moreover, as the whole data volume is unknown when constructing the model, it is desired to scan each data item only once with a storage independent with the data volume. It is also noteworthy that the distribution underlying may change during the data accumulation procedure. To handle such tasks, in this paper we propose DFOP, a distribution-free one-pass learning approach. This approach works well when distribution change occurs during data accumulation, without requiring prior knowledge about the change. Every data item can be discarded once it has been scanned. Besides, theoretical guarantee shows that the estimate error, under a mild assumption, decreases until convergence with high probability. The performance of DFOP for both regression and classification are validated in experiments.
Factsheet 8 | The Socio-Economic Dimension of Responsible Robotics
Creators: name: Civita
name: LOBA - Customer Experience Design
name: Laboratoire National de Métrologie et d'Essais
name: Robotex
name: DBT
name: AFL
name: NTNU
Publisher: name: Zenodo
Year: 2024

description: This document introduces the findings on socio-economic issues and solutions gathered as a part of Robotics4EU project activities in 2021-2023 in support of understanding how to support the more widespread adoption of robots in households and workplaces.
Optimal distillation of a GHZ state
Creators: name: Acin, A.
name: Jane, E.
name: Dur, W.
name: Vidal, G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present the optimal local protocol to distill a Greenberger-Horne-Zeilinger (GHZ) state from a single copy of any pure state of three qubits.
description: RevTex, 4 pages, 2 figures. Published version, some references added
ДЕСТРУКЦИЯ ИСТОРИЧЕСКОГО ВРЕМЕНИ В СОВРЕМЕННОМ ГОРОДЕ
Creators: name: Надежда Дмитриевна Асташова
Publisher: name: Революция и эволюция: модели развития в науке, культуре, обществе
Year: 2019
Subjects: развитие технологий
городское пространство
историческое время
современная мораль

description: Статья посвящена анализу представлений об историческом времени в современном го-роде эпохи техногенной цивилизации XXI века. Ставится цель проанализировать изменения восприятия исторического времени в зависимости от представлений о пространстве в связи с бурным развитием современных технологий. Актуальной задачей исследования является выяв-ление изменений в восприятии социальной среды современного города, а также их последст-вий для общественного сознания. Рассматривается мозаичный, фрагментарный коллаж город-ской реальности, который не самым лучшим образом сказывается на состоянии человека: живший раньше в условиях структурированного пространства и времени, в разорванном на куски, пестром пространстве современного города индивид испытывает страх, смятение от по-тери целостного восприятия действительности. Делаются выводы о том, что в сознании совре-менного человека произошла деконструкция исторического времени и исторической памяти, культурное прошлое города потерялось в бурном потоке современных технологий. Все это сформировало не просто специфическое отношение к историческому времени и пространству, но привело к изменениям общественной морали, не признающей важности для жизни человека связи поколений.
Extreme Mass Ratio Binary: Radiation reaction and gravitational waveform
Creators: name: Mino, Yasushi
Publisher: name: arXiv
Year: 2005
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: For a successful detection of gravitational waves by LISA, it is essential to construct theoretical waveforms in a reliable manner. We discuss gravitational waves from an extreme mass ratio binary system which is expected to be a promising target of the LISA project. The extreme mass ratio binary is a binary system of a supermassive black hole and a stellar mass compact object. As the supermassive black hole dominates the gravitational field of the system, we suppose that the system might be well approximated by a metric perturbation of a Kerr black hole. We discuss a recent theoretical progress in calculating the waveforms from such a system.
description: Classical and Quantum Gravity 22 (2005) S375-S379, Proceedings for 5th International LISA Symposium
Pinching parameters for open (super) strings
Creators: name: Playle, Sam
name: Sciuto, Stefano
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present an approach to the parametrization of (super) Schottky space obtained by sewing together three-punctured discs with strips. Different cubic ribbon graphs classify distinct sets of pinching parameters; we show how they are mapped onto each other. The parametrization is particularly well-suited to describing the region within (super) moduli space where open bosonic or Neveu-Schwarz string propagators become very long and thin, which dominates the IR behaviour of string theories. We show how worldsheet objects such as the Green's function converge to graph theoretic objects such as the Symanzik polynomials in the $α' \to 0$ limit, allowing us to see how string theory reproduces the sum over Feynman graphs. The (super) string measure takes on a simple and elegant form when expressed in terms of these parameters.
description: 68 pages, 31 figures