cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Low temperatures typical of winter cage-site conditions in Atlantic Canada impact the growth, physiology, health and welfare of Atlantic salmon (Salmo salar)
Creators: name: Vadboncoeur, Émile
Publisher: name: Memorial University of Newfoundland
Year: 2023

description: Limited research has been conducted on the physiology of Atlantic salmon (Salmo salar) at cold temperatures despite significant mortalities during the winter at sea-cages in Atlantic Canada. Thus, in this thesis, I exposed post-smolt cultured Atlantic salmon to a seasonal decline in temperature from 8 to 1°C (at 1°C week-1), and a ‘cold-shock’ from 3 to 0°C for 4 or 24 hours. During the seasonal decline in temperature, feeding decreased starting at 6°C (and ceased by 1-2°C), osmoregulatory changes and increases in heat shock protein expression began at 4-5°C, and at 1°C elevated plasma cortisol levels indicative of mild stress were measured. The ‘cold-shocks’ resulted in a relatively small stress response (i.e., increases in plasma cortisol and glucose), but no other adverse effects or mortalities. Nonetheless, a number of mortalities/moribund fish were noted when various groups of Atlantic salmon were held for long periods at < 8°C. Moribund fish were lethargic and swam erratically, had enlarged livers and plasma enzymes suggestive of liver damage, and developed ulcers to the head/jaw. The former symptoms are indicative of ‘Winter Syndrome’ described in gilthead sea bream (Sparus aurata) aquaculture, and these ulcers have previously been observed in Norway and associated with tenacibaculosis.
Additional file 1 of The challenges of pig farming in Hong Kong: a study of farmers’ perceptions and attitudes towards a pig health and production management service
Creators: name: Rosanowski, Sarah M.
name: Magouras, Ioannis
name: Ho, Wing-Chung
name: Yiu, Wing Chi Jacqueline
name: Pfeiffer, Dirk U.
name: Zeeh, Friederike
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy

description: Additional file 1: Supplementary Table 1. Additional categorical and continuous demographic characteristics of eight participants and their farms included in the study. The data were collected during an interview conducted between August and September 2019 with Hong Kong pig farmers.
Freezing of a two dimensional fluid in to a crystalline phase : Density functional approach
Creators: name: Jaiswal, Anubha
name: Singh, Swarn L.
name: Singh, Yashwant
Publisher: name: arXiv
Year: 2012
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: A free-energy functional for a crystal proposed by Singh and Singh (Europhys. Lett. {\bf {88}}, 16005 (2009)) and which contains both the symmetry conserved and symmetry broken parts of the direct pair correlation function has been used to investigate the crystallization of a two-dimensional fluid. The results found for fluids interacting via the inverse power potential $ u(r)= ε(σ/{r})^{n} $ for n= 3, 6 and 12 are in good agreement with experimental and simulation results. The contribution made by the symmetry broken part to the grand thermodynamic potential at the freezing point is found to increase with the softness of the potential. Our results explain why the Ramakrishnan-Yussouff (Phys. Rev. B {\bf 19}, 2775 (1979)) free-energy functional gave good account of freezing transitions of hard-core potentials but failed for potentials that have soft core and/or attractive tail.
description: 21 pages, 6 figures
Electronic Structures of Graphene Layers on Metal Foil: Effect of Point Defects
Creators: name: Yan, Hui
name: Liu, Cheng-Cheng
name: Bai, Ke-Ke
name: Wang, Xuejiao
name: Liu, Mengxi
name: Yan, Wei
name: Meng, Lan
name: Zhang, Yanfeng
name: Liu, Zhongfan
name: Nie, Jia-Cai
name: Yao, Yugui
name: He, Lin
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Here we report a facile method to generate a high density of point defects in graphene on metal foil and show how the point defects affect the electronic structures of graphene layers. Our scanning tunneling microscopy (STM) measurements, complemented by first principle calculations, reveal that the point defects result in both the intervalley and intravalley scattering of graphene. The Fermi velocity is reduced in the vicinity area of the defect due to the enhanced scattering. Additionally, our analysis further points out that periodic point defects can tailor the electronic properties of graphene by introducing a significant bandgap, which opens an avenue towards all-graphene electronics.
description: 4 figures
Additional file 2 of The challenges of pig farming in Hong Kong: a study of farmers’ perceptions and attitudes towards a pig health and production management service
Creators: name: Rosanowski, Sarah M.
name: Magouras, Ioannis
name: Ho, Wing-Chung
name: Yiu, Wing Chi Jacqueline
name: Pfeiffer, Dirk U.
name: Zeeh, Friederike
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy

description: Additional file 2: Supplementary Table 2. Topics and questions included in semi-structured interviews conducted with Hong Kong pig farmers to identify the barriers in pig industry and expectations from a pig health and production management service in autumn 2019.
Ramsey spectroscopy of high-contrast CPT resonances with push-pull optical pumping in Cs vapor
Creators: name: Liu, Xiaochi
name: Mérolla, Jean-Marc
name: Guérandel, Stéphane
name: de Clercq, Emeric
name: Boudot, Rodolphe
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We report the detection of high-contrast and narrow Coherent Population Trapping (CPT) Ramsey fringes in a Cs vapor cell using a simple-architecture laser system. The latter allows the combination of push-pull optical pumping (PPOP) and a temporal Ramsey-like pulsed interrogation. An originality of the optics package is the use of a single Mach-Zehnder electro-optic modulator (MZ EOM) both for optical sidebands generation and light switch for pulsed interaction. Typical Ramsey fringes with a linewidth of 166 Hz and a contrast of 33 % are detected in a cm-scale buffer-gas filled Cs vapor cell. This technique could be interesting for the development of high-performance and low power consumption compact vapor cell clocks based on CPT.
description: 9 pages, 8 figures
Transits and starspots in the WASP-19 planetary system
Creators: name: Tregloan-Reed, Jeremy
name: Southworth, John
name: Tappert, C.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have developed a new model for analysing light curves of planetary transits when there are starspots on the stellar disc. Because the parameter space contains a profusion of local minima we developed a new optimisation algorithm which combines the global minimisation power of a genetic algorithm and the Bayesian statistical analysis of the Markov chain. With these tools we modelled three transit light curves of WASP-19. Two light curves were obtained on consecutive nights and contain anomalies which we confirm as being due to the same spot. Using these data we measure the star's rotation period and velocity to be $11.76 \pm 0.09$ d and $3.88 \pm 0.15$\kms, respectively, at a latitude of 65$^\circ$. We find that the sky-projected angle between the stellar spin axis and the planetary orbital axis is $λ= 1.0^{\circ} \pm 1.2^{\circ}$, indicating axial alignment. Our results are consistent with and more precise than published spectroscopic measurements of the Rossiter-McLaughlin effect.
description: 9 pages, 6 figures, 5 tables
Additional file 1 of Why healthcare providers are not vaccinated? A qualitative study during the COVID-19 pandemic in Iran
Creators: name: Kokabisaghi, Fatemeh
name: Akhtar, Fatemeh
name: Taghipour, Ali
name: Javan-Noughabi, Javad
name: Moghri, Javad
name: Tabatabaee, Seyed Saeed
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy

description: Supplementary Material 1
Higgs Precision (Higgcision) Era begins
Creators: name: Cheung, Kingman
name: Lee, Jae Sik
name: Tseng, Po-Yan
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: After the discovery of the Higgs boson at the LHC, it is natural to start the research program on the precision study of the Higgs-boson couplings to various standard model (SM) particles. We provide a generic framework for the deviations of the couplings from their SM values by introducing a number of parameters. We show that a large number of models beyond the SM can be covered, including two-Higgs-doublet models, supersymmetric models, little-Higgs models, extended Higgs sectors with singlets, and fourth generation models. We perform global fits to the most updated data from CMS, ATLAS, and Tevatron under various initial conditions of the parameter set. In particular, we have made explicit comparisons between the fitting results BEFORE and AFTER the Moriond 2013 meetings. Highlights of the results include: (i) the nonstandard decay branching ratio of the Higgs boson is less than 22%; (ii) the most efficient way to achieve the best fit for the data before the Moriond update is to introduce additional particle contributions to the triangular-loop functions of Hγγand Hgg vertices; (iii) the 1σallowed range of the relative coupling of HVV is 1.01 +0.13 -0.14, which means that the electroweak-symmetry breaking contribution from the observed Higgs boson leaves only a small room for other Higgs bosons; (iv) the current data do not rule out pseudoscalar couplings nor pseudoscalar contributions to the Hγγand Hgg vertices; and (v) the SM Higgs boson provides the best fit to all the current Higgs data.
description: 48 pages, including 7 tables and 11 figures; in this revision we have updated the analysis using the most updated Higgs data after Moriond 2013; because of the change in CMS diphoton data, the fits change dramatically; we show the fits BEFORE and AFTER the Moriond update; references added
Additional file 1 of How to collaborate for health throughout the project timeline – a longitudinal study reflecting on implemented strategies in three projects for a healthy living environment
Creators: name: Vooren, N. J. E. van
name: Janssen, L. M. S.
name: Drewes, H. W.
name: Baan, C. A.
name: Bongers, I. M. B.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 1. Interviewed partners per project.
Confusion limited surveys: using WISE to quantify the rarity of warm dust around Kepler stars
Creators: name: Kennedy, G. M.
name: Wyatt, M. C.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We describe a search for infra-red excess emission from dusty circumstellar material around 180,000 stars observed by the Kepler and WISE missions. This study is motivated by i) the potential to find bright warm disks around planet host stars, ii) a need to characterise the distribution of rare warm disks, and iii) the possible identification of candidates for discovering transiting dust concentrations. We find about 8,000 stars that have excess emission, mostly at 12um. The positions of these stars correlate with the 100um background level so most of the flux measurements associated with these excesses are spurious. We identify 271 stars with plausible excesses by making a 5MJy/sr cut in the IRAS 100um emission. The number counts of these excesses, at both 12 and 22um, have the same distribution as extra-Galactic number counts. Thus, although some excesses may be circumstellar, most can be explained as chance alignments with background galaxies. The one exception is a 22um excess associated with a relatively nearby A-type star that we were able to confirm because the disk occurrence rate is independent of stellar distance. Despite our low detection rate, these results place valuable upper limits on the distribution of large mid-infrared excesses; e.g. fewer than 1:1000 stars have 12um excesses (F_ obs/F_star) larger than a factor of five. In contrast to previous studies, we find no evidence for disks around 1790 stars with candidate planets (we attribute one significant 12um excess to a background galaxy), and no evidence that the disk distribution around planet hosts is different to the bulk population. Higher resolution imaging of stars with excesses is the best way to rule out galaxy confusion and identify more reliable disk candidates among Kepler stars. A similar survey to ours that focusses on nearby stars would be well suited to finding the distribution of rare warm disks.
description: accepted to MNRAS
Additional file 2 of How to collaborate for health throughout the project timeline – a longitudinal study reflecting on implemented strategies in three projects for a healthy living environment
Creators: name: Vooren, N. J. E. van
name: Janssen, L. M. S.
name: Drewes, H. W.
name: Baan, C. A.
name: Bongers, I. M. B.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 2. Themes for addressing cross-sector collaboration according to van Vooren et al. (2020).
Discovery of a Kiloparsec Scale X-ray/Radio Jet in the z=4.72 Quasar GB 1428+4217
Creators: name: Cheung, C. C.
name: Stawarz, L.
name: Siemiginowska, A.
name: Gobeille, D.
name: Wardle, J. F. C.
name: Harris, D. E.
name: Schwartz, D. A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report the discovery of a one-sided 3.6" (24 kpc, projected) long jet in the high-redshift, z=4.72, quasar GB 1428+4217 in new Chandra X-ray and VLA radio observations. This is the highest redshift kiloparsec-scale X-ray/radio jet known. Analysis of archival VLBI 2.3 and 8.6 GHz data reveal a faint one-sided jet extending out to ~200 parsecs and aligned to within ~30 deg of the Chandra/VLA emission. The 3.6" distant knot is not detected in an archival HST image, and its broad-band spectral energy distribution is consistent with an origin from inverse Compton scattering of cosmic microwave background photons for the X-rays. Assuming also equipartition between the radiating particles and magnetic field, the implied jet Lorentz factor is ~5. This is similar to the other two known z ~ 4 kpc-scale X-ray jet cases and smaller than typically inferred in lower-redshift cases. Although there are still but a few such very high-redshift quasar X-ray jets known, for an inverse Compton origin, the present data suggest that they are less relativistic on large-scales than their lower-redshift counterparts.
description: ApJL, accepted, 5 pages, 3 figures
The DuBois-Reymond Fundamental Lemma of the Fractional Calculus of Variations and an Euler-Lagrange Equation Involving only Derivatives of Caputo
Creators: name: Lazo, Matheus J.
name: Torres, Delfim F. M.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Optimization and Control (math.OC)
subject: Mathematical Physics (math-ph)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 49K05, 26A33, 34A08

description: Derivatives and integrals of non-integer order were introduced more than three centuries ago, but only recently gained more attention due to their application on nonlocal phenomena. In this context, the Caputo derivatives are the most popular approach to fractional calculus among physicists, since differential equations involving Caputo derivatives require regular boundary conditions. Motivated by several applications in physics and other sciences, the fractional calculus of variations is currently in fast development. However, all current formulations for the fractional variational calculus fail to give an Euler-Lagrange equation with only Caputo derivatives. In this work, we propose a new approach to the fractional calculus of variations by generalizing the DuBois-Reymond lemma and showing how Euler-Lagrange equations involving only Caputo derivatives can be obtained.
description: This is a preprint of a paper whose final and definite form will appear in Journal of Optimization Theory and Applications (JOTA). Paper submitted 26-July-2012; revised 12-Sept-2012 and 22-Sept-2012; accepted for publication 02-Oct-2012. arXiv admin note: text overlap with arXiv:1203.2102 by other authors
Additional file 3 of How to collaborate for health throughout the project timeline – a longitudinal study reflecting on implemented strategies in three projects for a healthy living environment
Creators: name: Vooren, N. J. E. van
name: Janssen, L. M. S.
name: Drewes, H. W.
name: Baan, C. A.
name: Bongers, I. M. B.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 3. Examples of Strategy-Context-Mechanism-Outcome configurations for the three overall insights.
Noise-resistant control for a spin qubit array
Creators: name: Kestner, J. P.
name: Wang, Xin
name: Bishop, Lev S.
name: Barnes, Edwin
name: Sarma, S. Das
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We develop a systematic method of performing corrected gate operations on an array of exchange-coupled singlet-triplet qubits in the presence of both fluctuating nuclear Overhauser field gradients and charge noise. The single-qubit control sequences we present have a simple form, are relatively short, and form the building blocks of a corrected CNOT gate when also implemented on the inter-qubit exchange link. This is a key step towards enabling large-scale quantum computation in a semiconductor-based architecture by facilitating error reduction below the quantum error correction threshold for both single-qubit and multi-qubit gate operations.
description: 5 pages + 4 pages supplementary material
Inhomogeneous and interacting vacuum energy
Creators: name: De-Santiago, Josue
name: Wands, David
name: Wang, Yuting
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Vacuum energy is a simple model for dark energy driving an accelerated expansion of the universe. If the vacuum energy is inhomogeneous in spacetime then it must be interacting. We present the general equations for a spacetime-dependent vacuum energy in cosmology, including inhomogeneous perturbations. We show how any dark energy cosmology can be described by an interacting vacuum+matter. Different models for the interaction can lead to different behaviour (e.g., sound speed for dark energy perturbations) and hence could be distinguished by cosmological observations. As an example we present the cosmic microwave microwave background anisotropies and the matter power spectrum for two different versions of a generalised Chaplygin gas cosmology.
description: 10 pages, 5 figures; to appear in the proceedings of IV International Meeting on Gravitation and Cosmology, Guadalajara, May 2012
Giant X-ray Bump in GRB 121027A: Evidence for Fall-back Disk Accretion
Creators: name: Wu, Xue-Feng
name: Hou, Shu-Jin
name: Lei, Wei-Hua
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A particularly interesting discovery in observations of GRB 121027A is that of a giant X-ray bump detected by the Swift/X-Ray Telescope. The X-ray afterglow re-brightens sharply at about 1000 s after the trigger by more than two orders of magnitude in less than 200 s. This X-ray bump lasts for more than 10 ks. It is quite different from typical X-ray flares. In this Letter we propose a fall-back accretion model to interpret this X-ray bump within the context of the collapse of a massive star for a long-duration gamma-ray burst. The required fall-back radius of about 3.5e10 cm and mass of about 0.9-2.6 solar masses imply that a significant part of the helium envelope should survive through the mass loss during the last stage of the massive progenitor of GRB 121027A.
description: 5 pages, 3 figures, 2013, ApJL, 767:L36
How Levins' dynamics emerges from a Ricker metapopulation model on the brink of extinction
Creators: name: Wolff, F. Elias
name: Eriksson, A.
name: Manica, A.
name: Mehlig, B.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: Understanding the dynamics of metapopulations close to extinction is of vital importance for management. Levins-like models, in which local patches are treated as either occupied or empty, have been used extensively for this purpose, but they ignore the important role of local population dynamics. In this paper, we consider a stochastic metapopulation model where local populations follow a Ricker dynamics, and use this framework to investigate the behaviour of the metapopulation at the brink of extinction. As long as dispersal rates are not too large, the system is shown to have a time evolution consistent with Levins' dynamics. We derive analytical expressions for the colonisation and extinction rates (c and e) in Levins-type models in terms of reproduction, survival, and dispersal parameters of the local populations, providing an avenue to parameterising Levins-like models from the type of information on local demography that is available for a number of species. To facilitate applying our results, we provide a numerical implementation for computing c and e.
description: 15 pages, 4 figures
Additional file 1 of Evaluation of a digital game for teaching behavioral aspects of clinical communication in dentistry
Creators: name: Lin, Chia-Shu
name: Yang, Cheng-Chieh
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Description and design of the game scenarios. Please note that the scenarios are designed based on the clinical context of a local clinic in Taiwan. Therefore, the treatment procedures, the patient-doctor relationship, and the health-related policies may differ from those in other countries.
Vibron-vibron coupling from ab initio molecular dynamics simulations of a silicon cluster
Creators: name: Han, Peng
name: Vilciauskas, Linas
name: Bester, Gabriel
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the temperature dependent dynamical processes of a Si10H16 cluster and obtain a blue shift of the Si-Si vibrational modes with transverse acoustic character and a red shift of the other vibrational modes with increasing temperature. We link this behavior to the bond length expansion and the varying sign of the Grueneisen parameter. We further present a computational approach able to extract the vibron-vibron coupling strength in clusters or molecules. Our approach is based on ab initio Born-Oppenheimer molecular dynamics and a projection formalism able to deliver the individual vibron occupation numbers. From the Fourier transform of the vibron energy autocorrelation function we obtain the coupling strength of each vibron to the most strongly coupled vibronic states. We find vibron-vibron coupling strength up to 2.5 THz with a moderate increase of about 5 % when increasing the temperature from 50 to 150 K.
description: 14 pages, 8 figures
A magnetic reconnection origin for the soft X-ray excess in AGN
Creators: name: Zhong, Xiaogu
name: Wang, Jiancheng
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a new scenario to explain the soft X-ray excess in Active Galactic Nucleus. The magnetic reconnection could happen in a thin layer on the surface of accretion disk. Electrons are accelerated by shock wave and turbulence triggered by magnetic reconnection, then they take place inverse Compton scattering above accretion disk which contributes soft X-rays. Based on standard disk model, we estimate the magnetic field strength and the energy released by magnetic reconnection along accretion disk, and find that the luminosity caused by magnetic reconnection mainly emits in the inner disk which is dominated by radiation pressure. We then apply the model to fit the spectra of AGNs with strong soft X-ray excess.
description: 22 pages, 7 figures, Accepted by ApJ
The Arecibo Legacy Fast ALFA Survey: The Galaxy Population Detected by ALFALFA
Creators: name: Huang, Shan
name: Haynes, Martha P.
name: Giovanelli, Riccardo
name: Brinchmann, Jarle
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Making use of HI 21 cm line measurements from the ALFALFA survey (alpha.40) and photometry from the Sloan Digital Sky Survey (SDSS) and GALEX, we investigate the global scaling relations and fundamental planes linking stars and gas for a sample of 9417 common galaxies: the alpha.40-SDSS-GALEX sample. In addition to their HI properties derived from the ALFALFA dataset, stellar masses (M_*) and star formation rates (SFRs) are derived from fitting the UV-optical spectral energy distributions. 96% of the alpha.40-SDSS-GALEX galaxies belong to the blue cloud, with the average gas fraction f_HI = M_HI/M_* ~ 1.5. A transition in SF properties is found whereby below M_* ~ 10^9.5 M_sun, the slope of the star forming sequence changes, the dispersion in the specific star formation rate (SSFR) distribution increases and the star formation efficiency (SFE) mildly increases with M_*. The evolutionary track in the SSFR-M_* diagram, as well as that in the color magnitude diagram are linked to the HI content; below this transition mass, the star formation is regulated strongly by the HI. Comparison of HI- and optically-selected samples over the same restricted volume shows that the HI-selected population is less evolved and has overall higher SFR and SSFR at a given stellar mass, but lower SFE and extinction, suggesting either that a bottleneck exists in the HI to H_2 conversion, or that the process of SF in the very HI-dominated galaxies obeys an unusual, low efficiency star formation law. A trend is found that, for a given stellar mass, high gas fraction galaxies reside preferentially in dark matter halos with high spin parameters. Because it represents a full census of HI-bearing galaxies at z~0, the scaling relations and fundamental planes derived for the ALFALFA population can be used to assess the HI detection rate by future blind HI surveys and intensity mapping experiments at higher redshift.
description: 21 pages (2 columns), 14 figures. Accepted for publication in ApJ. Version with full-resolution figures is available at http://egg.astro.cornell.edu/alfalfa/pubs/Huang2012b_120702.pdf
Вопросы устойчивого развития общества,Выпуск 11 2022
Creators: name: ООО "Институт развития образования и консалтинга"
Publisher: name: ООО "Институт развития образования и консалтинга"
Year: 2022

description: Вопросы устойчивого развития общества,Выпуск 11 2022
Additional file 1 of A systematic comparison of different composite measures (DAS 28, CDAI, SDAI, and Boolean approach) for determining treatment effects on low disease activity and remission in rheumatoid arthritis
Creators: name: Janke, Kirsten
name: Kiefer, Corinna
name: McGauran, Natalie
name: Richter, Bernd
name: Krause, Dietmar
name: Wieseler, Beate
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 1. Details on statistical methods, supplementary tables and figures
Detection of fast transients with radio interferometric arrays
Creators: name: Bhat, N. D. R.
name: Chengalur, J. N.
name: Cox, P. J.
name: Gupta, Y.
name: Prasad, J.
name: Roy, J.
name: Bailes, M.
name: Burke-Spolaor, S.
name: Kudale, S. S.
name: van Straten, W.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Next-generation radio arrays, including the Square Kilometre Array (SKA) and its pathfinders, will open up new avenues for exciting transient science at radio wavelengths. Their innovative designs, comprising a large number of small elements, pose several challenges in digital processing and optimal observing strategies. The Giant Metrewave Radio Telescope (GMRT) presents an excellent test-bed for developing and validating suitable observing modes and strategies for transient experiments with future arrays. Here we describe the first phase of the ongoing development of a transient detection system for GMRT that is planned to eventually function in a commensal mode with other observing programs. It capitalizes on the GMRT's interferometric and sub-array capabilities, and the versatility of a new software backend. We outline considerations in the plan and design of transient exploration programs with interferometric arrays, and describe a pilot survey that was undertaken to aid in the development of algorithms and associated analysis software. This survey was conducted at 325 and 610 MHz, and covered 360 deg$^2$ of the sky with short dwell times. It provides large volumes of real data that can be used to test the efficacies of various algorithms and observing strategies applicable for transient detection. We present examples that illustrate the methodologies of detecting short-duration transients, including the use of sub-arrays for higher resilience to spurious events of terrestrial origin, localization of candidate events via imaging and the use of a phased array for improved signal detection and confirmation. In addition to demonstrating applications of interferometric arrays for fast transient exploration, our efforts mark important steps in the roadmap toward SKA-era science.
description: With improved figures; 25 Pages, 18 Figures, 1 Table; Accepted for publication in the Astrophysical Journal
MPEC 2023-M04 : 2020 FM4
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Computing integral points on X_ns^+(p)
Creators: name: Bajolet, Aurélien
name: Bilu, Yuri
name: Matschke, Benjamin
Publisher: name: arXiv
Year: 2012
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: We describe an algorithm for computing integral points on the modular curve of prime level p associated to the normalizer of a non-split Cartan subgroup of GL_2(F_p). Using our method, we show that for 7
description: To appear in Algebra and Number Theory
Fundamentos e tendências da Inteligência Artificial na Academia
Creators: name: De Sá Ferreira, Arthur
Publisher: name: OSF
Year: 2024

description: Oficina de capacitação docente do Programa de Pós-Graduação em Fisioterapia da UFTM (Universidade Federal do Triângulo Mineiro) e da UFU (Universidade Federal de Uberlândia)
Supplementary materials for 'Long-term weight change and its temporal relation to later-life dementia in the Health and Retirement Study'
Creators: name: Shen, Jie
name: Chen, Hui
name: Zhou, Tianjing
name: Zhang, Simei
name: Huang, Liyan
name: Lv, Xiaozhen
name: Ma, Yuan
name: Zheng, Yan
name: Yuan, Changzheng
Publisher: name: figshare
Year: 2022
Subjects: classificationCode: 320905
subject: Neurology and neuromuscular diseases

description: Supplementary materials for 'Long-term weight change and its temporal relation to later-life dementia in the Health and Retirement Study'Corresponding authors: Changzheng Yuan, School of Public Health, Zhejiang University
School of Medicine, Hangzhou, China, 310058, Email: chy478@zju.edu.cn, ORCID: 0000-
0002-2389-8752. Yan Zheng, Human Phenome Institute, School of Life Sciences, Fudan
University, Shanghai, China, 200043, Email: yan_zheng@fudan.edu.cn
Moments of net-charge multiplicity distribution in Au+Au collisions measured by the PHENIX experiment at RHIC
Creators: name: Garg, P.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Beam Energy Scan (BES) program at RHIC is important to search for the existence of the critical point in the QCD phase diagram. Lattice QCD have shown that the predictions of the susceptibility of the medium formed in heavy-ion collisions can be sensitive to the various moments (mean ($μ$) =${}$, variance ($σ^2$) = ${}$, skewness (S) = $\frac{}{σ^3}$ and kurtosis ($κ$) =$\frac{}{σ^4} -3$) of conserved quantities like net-baryon number ($Δ$B), net-electric charge ($Δ$Q) and net-strangeness ($Δ$S). Any non-monotonic behavior of the higher moments would confirm the existence of the QCD critical point. The recent results of the higher moments of net-charge multiplicity distributions for Au+Au collisions at $\sqrt{s}_{NN}$ varying from 7.7 GeV to 200 GeV from the PHENIX experiment at RHIC are presented. The energy and centrality dependence of the higher moments and their products (S$σ$ and $κσ^{2}$) are shown for the net-charge multiplicity distributions. Furthermore, the results are compared with the values obtained from the heavy-ion collision models, where there is no QCD phase transition and critical point.
description: Talk presented at "Critical Point and the Onset of Deconfinement", Napa, CA, March 2013
Kinetic operator effects in B-> X_c l nu at O(alpha_s)
Creators: name: Alberti, Andrea
name: Ewerth, Thorsten
name: Gambino, Paolo
name: Nandi, Soumitra
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We compute the O(alpha_s) corrections to the Wilson coefficient of the kinetic operator in inclusive semileptonic B decays. Our analytic calculation agrees with reparameterization invariance and with previous numerical results and paves the way to the calculation of analogous corrections to other power-suppressed coefficients.
description: 16 pages, v2: typos in eqs. 5.1 and A.5 fixed, results unchanged
Pseudospin-Resolved Transport Spectroscopy of the Kondo Effect in a Double Quantum Dot
Creators: name: Amasha, S.
name: Keller, A. J.
name: Rau, I. G.
name: Carmi, A.
name: Katine, J. A.
name: Shtrikman, H.
name: Oreg, Y.
name: Goldhaber-Gordon, D.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report measurements of the Kondo effect in a double quantum dot (DQD), where the orbital states act as pseudospin states whose degeneracy contributes to Kondo screening. Standard transport spectroscopy as a function of the bias voltage on both dots shows a zero-bias peak in conductance, analogous to that observed for spin Kondo in single dots. Breaking the orbital degeneracy splits the Kondo resonance in the tunneling density of states above and below the Fermi energy of the leads, with the resonances having different pseudospin character. Using pseudospin-resolved spectroscopy, we demonstrate the pseudospin character by observing a Kondo peak at only one sign of the bias voltage. We show that even when the pseudospin states have very different tunnel rates to the leads, a Kondo temperature can be consistently defined for the DQD system.
description: Text and supplementary information. Text: 4 pages, 5 figures. Supplementary information: 4 pages, 4 figures
Additional file 1 of 3D hESC exosomes enriched with miR-6766-3p ameliorates liver fibrosis by attenuating activated stellate cells through targeting the TGFβRII-SMADS pathway
Creators: name: Wang, Ning
name: Li, Xiajing
name: Zhong, Zhiyong
name: Qiu, Yaqi
name: Liu, Shoupei
name: Wu, Haibin
name: Tang, Xianglian
name: Chen, Chuxin
name: Fu, Yingjie
name: Chen, Qicong
name: Guo, Tingting
name: Li, Jinsong
name: Zhang, Shuai
name: Zern, Mark A.
name: Ma, Keqiang
name: Wang, Bailin
name: Ou, Yimeng
name: Gu, Weili
name: Cao, Jie
name: Chen, Honglin
name: Duan, Yuyou
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 1. Extra materials and methods, additional figures and antibodies used in this study shown.
Additional file 1 of Surface electroencephalographic neurofeedback improves sustained attention in ADHD: a meta-analysis of randomized controlled trials
Creators: name: Chiu, Hsien‐Jane
name: Sun, Cheuk-Kwan
name: Fan, Hsin-Yi
name: Tzang, Ruu‐Fen
name: Wang, Ming-Yu
name: Cheng, Ying-Chih
name: Cheng, Yu-Shian
name: Yeh, Pin-Yang
name: Chung, Weilun
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Science Policy

description: Additional file 1: Table S1. Applied keyword and the search result in each database.
SPIDER VII - Revealing the Stellar Population Content of Massive Early-type Galaxies out to 8Re
Creators: name: La Barbera, F.
name: Ferreras, I.
name: de Carvalho, R. R.
name: Bruzual, G.
name: Charlot, S.
name: Pasquali, A.
name: Merlin, E.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Radial trends of stellar populations in galaxies provide a valuable tool to understand the mechanisms of galaxy growth. In this paper, we present the first comprehensive analysis of optical-optical and optical-NIR colours, as a function of galaxy mass, out to the halo region (8Re) of early-type galaxies (ETGs). We select a sample of 674 massive ETGs (M*>3x10^10MSun) from the SDSS-based SPIDER survey. By comparing with a large range of population synthesis models, we derive robust constraints on the radial trends in age and metallicity. Metallicity is unambiguously found to decrease outwards, with a measurable steepening of the slope in the outer regions (Re10^11MSun). Furthermore, when segregating with respect to large scale environment, the age gradient is more significant in ETGs residing in higher density regions. These results shed light on the processes leading from the formation of the central core to the growth of the stellar envelope of massive galaxies. The fact that the populations in the outer regions are older and more metal-poor than in the core suggests a process whereby the envelope of massive galaxies is made up of accreted small satellites (i.e. minor mergers) whose stars were born during the first stages of galaxy formation.
description: 20 pages, 13 figures, 10 tables. Accepted for publication in MNRAS
Interatomic potentials, electric properties, and spectroscopy of the ground and excited states of the Rb_2 molecule: Ab initio calculations and effect of a non-resonant field
Creators: name: Tomza, Michał
name: Skomorowski, Wojciech
name: Musiał, Monika
name: González-Férez, Rosario
name: Koch, Christiane P.
name: Moszynski, Robert
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We formulate the theory for a diatomic molecule in a spatially degenerate electronic state interacting with a non-resonant laser field and investigate its rovibrational structure in the presence of the field. We report on \textit{ab initio} calculations employing the double electron attachment intermediate Hamiltonian Fock space coupled cluster method restricted to single and double excitations for all electronic states of the Rb$_2$ molecule up to $5s+5d$ dissociation limit of about 26.000$\,$cm$^{-1}$. In order to correctly predict the spectroscopic behavior of Rb$_2$, we have also calculated the electric transition dipole moments, non-adiabatic coupling and spin-orbit coupling matrix elements, and static dipole polarizabilities, using the multireference configuration interaction method. When a molecule is exposed to strong non-resonant light, its rovibrational levels get hybridized. We study the spectroscopic signatures of this effect for transitions between the X$^1Σ_g^+$ electronic ground state and the A$^1Σ_u^+$ and b$^3Π_u$ excited state manifold. The latter is characterized by strong perturbations due to the spin-orbit interaction. We find that for non-resonant field strengths of the order $10^9$W/cm$^2$, the spin-orbit interaction and coupling to the non-resonant field become comparable. The non-resonant field can then be used to control the singlet-triplet character of a rovibrational level.
description: 28 pages, 14 figures, 5 tables
Additional file 1 of Patients’ experience of accessing hepatitis C treatment through the Myanmar national hepatitis C treatment program: a qualitative evaluation
Creators: name: Draper, Bridget
name: Yee, Win Lei
name: Bowring, Anna
name: Naing, Win
name: Kyi, Khin Pyone
name: Htay, Hla
name: Howell, Jessica
name: Hellard, Margaret
name: Pedrana, Alisa
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Supplementary Material 1
Additional file 2 of Surface electroencephalographic neurofeedback improves sustained attention in ADHD: a meta-analysis of randomized controlled trials
Creators: name: Chiu, Hsien‐Jane
name: Sun, Cheuk-Kwan
name: Fan, Hsin-Yi
name: Tzang, Ruu‐Fen
name: Wang, Ming-Yu
name: Cheng, Ying-Chih
name: Cheng, Yu-Shian
name: Yeh, Pin-Yang
name: Chung, Weilun
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Science Policy

description: Additional file 2: Table S2. PRISMA checklist of the present meta-analysis.
How to tell a data story
Creators: name: Wildisen-Münch, Cristina
name: Görlich, Nico
name: Mähr, Moritz
Publisher: name: Zenodo
Year: 2022
Subjects: data story
digital storytelling
digital humanities
digital history
public history

description: At Stadt.Geschichte.Basel, more than 70 historians research the history of Basel from the Celts to the present. The focus is on current and little-researched topics such as the industrial and commercial history of the 19th and 20th centuries or the history of migration. The city's history is not viewed in isolation, but is interwoven regionally and internationally at the economic, political and cultural levels. It is published in 10 printed volumes. In addition, selected historical aspects are presented in the form of data stories.

 To facilitate this process, the Stadt.Geschichte.Basel research data management team has developed a guide. It walks through the questions that led to the development, production and publication of the data story.
Classification of Polynomial Mappings Between Commutative Groups
Creators: name: Schauz, Uwe
Publisher: name: arXiv
Year: 2012
Subjects: subject: Commutative Algebra (math.AC)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05E99, 13F20, 41A05

description: Some polynomials $P$ with rational coefficients give rise to well defined maps between cyclic groups, $\Z_q\longrightarrow\Z_r$, $x+q\Z\longmapsto P(x)+r\Z$. More generally, there are polynomials in several variables with tuples of rational numbers as coefficients that induce maps between commutative groups. We characterize the polynomials with this property, and classify all maps between two given finite commutative groups that arise in this way. We also provide interpolation formulas and a Taylor-type theorem for the calculation of polynomials that describe given maps.
description: 27 pages
Obstacle avoidance and line following autonomous unmanned ground vehicle.
Creators: name: Khaffaf, Thulfiqar
Publisher: name: figshare
Year: 2022
Subjects: Mechanical engineering not elsewhere classified

description: White paper about Planning and implementation of obstacle avoidance and line following autonomous unmanned ground vehicle,detailed information about the vehicle's design, capabilities, and performance and vehicle employment plan for multiple tasks .
Schrifttum der Burgenkunde. Buchbesprechungen und Schrifttums-Nachweisungen
Creators: name: Redaktion, Die
Publisher: name: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Year: 2017

description: -
description: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege, Bd. 4, Nr. 1 (1963): Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege