cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 2 of One-year outcomes in sepsis: a prospective multicenter cohort study in Japan
Creators: name: Liu, Keibun
name: Watanabe, Shinichi
name: Nakamura, Kensuke
name: Nakano, Hidehiko
name: Motoki, Maiko
name: Kamijo, Hiroshi
name: Ayaka, Matsuoka
name: Ishii, Kenzo
name: Morita, Yasunari
name: Hongo, Takashi
name: Shimojo, Nobutake
name: Tanaka, Yukiko
name: Hanazawa, Manabu
name: Hamagami, Tomohiro
name: Oike, Kenji
name: Kasugai, Daisuke
name: Sakuda, Yutaka
name: Irie, Yuhei
name: Nitta, Masakazu
name: Akieda, Kazuki
name: Shimakura, Daigo
name: Katsukawa, Hajime
name: Kotani, Toru
name: McWilliams, David
name: Nydahl, Peter
name: Schaller, Stefan J.
name: Ogura, Takayuki
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Additional file 2. Table 1: Follow-up loss rate at each time point. Table 2. Association of PICS at a follow-up with its prior follow-up in the multivariable analysis with the minimum variable. Table 3. Association of PICS at a follow-up with its prior follow-up in the multivariable analysis with a few variables. Table 4. Risk factors for the incidence of physical dysfunction at the time of each follow-up. Table 5. Risk factors for the incidence of cognitive dysfunction at the time of each follow-up. Table 6. Risk factors for the incidence of mental disorders at the time of each follow-up. Table 7. Differences in patient characteristics from past papers
The Steady Spin Down Rate of 4U 1907+09
Creators: name: Baykal, A.
name: Inam, C.
name: Alpar, M. A.
name: Zand, J. in't
name: Strohmayer, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using X-ray data from the Rossi X-Ray Timing Explorer (RXTE), we report the pulse timing results of the accretion powered high mass X-ray binary (HMXRB) pulsar 4U 1907+09 covering a time span of almost two years. We measured three new pulse periods in addition to the previously measured four pulse periods. We are able to connect pulse arrival times in phase for more than a year. The source has been spinning down almost at a constant rate with a spin down rate of \dot ν= (-3.54 \pm 0.02) \times 10^{-14} Hz s ^{-1} for more than 15 years. Residuals of pulse arrival times yield a very low level of random walk noise strengths \sim 2 \times 10^{-20} rad ^{2} sec ^{-3} on a time scale of 383 days, which is four decades lower than that of the HMXRB pulsar Vela X-1. The noise strength is only a factor of 5 greater than that of the low mass X-ray binary pulsar (LMXRB) 4U 1626-67. The low level of the timing noise and the very stable spin down rate of 4U 1907+09 makes this source unique among the HMXRBs, providing another example, in addition to 4U 1626-67, of long term quiet spin down from an accreting source. These examples show that the extended quiet spin down episodes observed in the anomalous X-ray pulsars (AXPs) pulsars 1RXS J170849.0-400910 and 1E 2259+586 do not necessarly imply that these sources are not accreting pulsars.
description: Submitted to MNRAS
Mechatronics design instruction 2017
Creators: name: Mokgohloa, Tlou Tressure
Publisher: name: T. Mokgohloa
Year: 2017
Subjects: subject: Mechatronics
subject: Automation
subject: Production economics

description: The Mechatronics design instruction was originally created for the Worldskills national competition in 2017, held in Durban, South Africa. The competition was recorded and the video has since been uploaded online, garnering over 4k views. https://www.youtube.com/watch?v=Kti1mSn0GhU
Additional file 1 of Microbial degradation and community structure analysis of hydroxyl-terminated polybutadiene (HTPB)
Creators: name: Zhang, Ying
name: Zou, Min
name: Lodhi, Adil Farooq
name: Deng, Yu-lin
Publisher: name: figshare
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Science Policy

description: Additional file 1: Table S1. PCR amplification system.
A Non-Cooperative Power Control Game in Delay-Constrained Multiple-Access Networks
Creators: name: Meshkati, Farhad
name: Poor, H. Vincent
name: Schwartz, Stuart C.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: A game-theoretic approach for studying power control in multiple-access networks with transmission delay constraints is proposed. A non-cooperative power control game is considered in which each user seeks to choose a transmit power that maximizes its own utility while satisfying the user's delay requirements. The utility function measures the number of reliable bits transmitted per joule of energy and the user's delay constraint is modeled as an upper bound on the delay outage probability. The Nash equilibrium for the proposed game is derived, and its existence and uniqueness are proved. Using a large-system analysis, explicit expressions for the utilities achieved at equilibrium are obtained for the matched filter, decorrelating and minimum mean square error multiuser detectors. The effects of delay constraints on the users' utilities (in bits/Joule) and network capacity (i.e., the maximum number of users that can be supported) are quantified.
description: To apprear in the proceedings of the 2005 IEEE International Symposium on Information Theory, Adelaide, Australia, September 4-9, 2005
Additional file 1: of Muscle mass and muscle strength are associated with pre- and post-hospitalization falls in older male inpatients: a longitudinal cohort study
Creators: name: Ancum, Jeanine Van
name: Pijnappels, Mirjam
name: Jonkman, Nini
name: Scheerman, Kira
name: Verlaan, Sjors
name: Meskers, Carel
name: Maier, Andrea
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 60506 Virology

description: Table S1. Z-scores of muscle parameters at admission and pre- and post-hospitalization falls, stratified by sex. Adjusted models of the standardized measures of HGS, SMM, SMI and RMM stratified for sex by z-scores. (DOCX 17Â kb)
Analysis of the Determinants of Capital Adequacy Ratio: The Case of Full-Fledged Islamic Banks in the Gulf Cooperation Council (GCC)
Creators: name: Ali, Abdilatif Mao
Publisher: name: European Journal of Islamic Finance
Year: 2019
Subjects: Capital adequacy ratio; full-fledged Islamic banks; Gulf Cooperation Council.

description: This study empirically analyzes bank-level and macroeconomic factors that have impact on the capital adequacy ratio (CAR) of the full-fledged Islamic banks in the Gulf Cooperation Council (GCC) and how they influence the banks’ capitalization decisions. This study covers a six years period ranging from 2013 to 2018. CAR ratio is a key stability indicator that measures the capability of banks to absorb unforeseen losses. To conduct the analysis, secondary data gathered from the annual financial reports of the banks as well from international economic database are used. Using multiple linear regression model, the effect of return on assets (ROA), return on equity (ROE), financing to deposit ratio (FDR), operating expense to operating income (OEOI), bank size (SIZE), non-performing financing (NPF) as bank-specific explanatory variables and economic growth (GDP) and inflation (INF) as a proxy for macroeconomic explanatory variables on the CAR of the banks are studied. Due to multicollinearity issues, ROA is dropped. As a result of the regression analysis, OEO and FDR are observed to positively and strongly impact CAR of the examined banks while SIZE is found to have negative and significant effect. ROE, NPF, GDP and INF demonstrated insignificant influences on the banks’ CAR. This study reveals varying and significant under and over regulatory capitalization decisions across the banks. Additionally, extreme expenditures and financial losses suffered by some banks are also discovered.
description: European Journal of Islamic Finance, No 14 (2019): EJIF - European Journal of Islamic Finance, 14, 2019
Shocks and Spatially Offset Active Galactic Nuclei Produce Velocity Offsets in Emission Lines
Creators: name: Comerford, Julia M.
name: Barrows, R. Scott
name: Greene, Jenny E.
name: Pooley, David
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: While 2% of active galactic nuclei (AGNs) exhibit narrow emission lines with line-of-sight velocities that are significantly offset from the velocity of the host galaxy's stars, the nature of these velocity offsets is unknown. We investigate this question with Chandra/ACIS and Hubble Space Telescope/Wide Field Camera 3 observations of seven velocity-offset AGNs at z<0.12, and all seven galaxies have a central AGN but a peak in emission that is spatially offset by < kpc from the host galaxy's stellar centroid. These spatial offsets are responsible for the observed velocity offsets and are due to shocks, either from AGN outflows (in four galaxies) or gas inflowing along a bar (in three galaxies). We compare our results to a velocity-offset AGN whose velocity offset originates from a spatially offset AGN in a galaxy merger. The optical line flux ratios of the offset AGN are consistent with pure photoionization, while the optical line flux ratios of our sample are consistent with contributions from photoionization and shocks. We conclude that these optical line flux ratios could be efficient for separating velocity-offset AGNs into subgroups of offset AGNs -- which are important for studies of AGN fueling in galaxy mergers -- and central AGNs with shocks -- where the outflows are biased towards the most energetic outflows that are the strongest drivers of feedback.
description: 12 pages, 4 figures, published in ApJ
THE PROGRESS TO ALLOW FULLY FLEDGED INTEREST FREE BANKING BUSINESS IN ETHIOPIA
Creators: name: Ahmed, Mohammed Ibrahim
Publisher: name: European Journal of Islamic Finance
Year: 2019

description: Abstract-Islamic banking refers to banking business in which mobilizing or advancing funds is undertaken in a manner consistent with Islamic Sharia Law. Different literature shows the rapid growth of this Islamic banking as alternative to the conventional banking. Economic globalization, among other things, has led to the flourishment of Islamic banking both in Muslim and non-Muslim countries. There has been increasingly strong public demand for interest free banking products in Ethiopia. As a response to this demand, the Ethiopian government introduced interest free banking business under Banking Business Proclamation No. 592/2008. Following this, the application to establish Fully Fledged Interest Free Banking Business was submitted to National Bank of Ethiopia. However, the prohibition by National Bank of Ethiopia for the same, following the enactment of “Directive to Authorize the Business of Interest Free Banking No.SBB/ 51/2011”, forced the withdrawal of the application. Now Ethiopia is being one of the largest Muslim populations in the Horn of Africa, however, has no Fully Fledged Interest Free Banking Business to provide service to the Muslim community. The enactment of Directive to License and Authorize Interest Free Banking Business No. SBB/72/2019, however, seems changed the situation. This directive allowed the establishment of Fully Fledged Interest Free Banking Business and following this directive, different banks of the same applied for the formation. Hence, the purpose of this Article is to analyze the evolution of Fully Fledged Interest Free Banking Business; to analyze the problem related with allowing Fully Fledged Interest Free Banking Business and to analyze the short coming of legal provision relating to Fully Fledged Interest Free Banking Business in Ethiopia. The outcome of the analysis shows that the legal provision relating to Fully Fledged Interest Free Banking Business is not enough to deal with the same. It calls for the amendment of Banking Business Proclamation No. 592/2008 and the Directive to License and Authorize Interest Free Banking Business No. SBB/72/2019.The outcome also shows that the Authorization of more than one bank of the same at this early stage may bring failure both on the same and other conventional banks. Hence it calls to limit the number of Authorization for Fully Fledged Interest Free Banking Business at this early stage to not more than one. Keyword: Islamic banking, interest free banking, Islamic banking in Ethiopia.
description: European Journal of Islamic Finance, No 14 (2019): EJIF - European Journal of Islamic Finance, 14, 2019
Gravitating BPS Dyons witout a Dilaton
Creators: name: Lee, Choonkyu
name: Park, Q-Han
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We describe curved-space BPS dyon solutions, the ADM mass of which saturates the gravitational version of the Bogomol'nyi bound. This generalizes self-gravitating BPS monopole solutions of Gibbons et al. when there is no dilaton.
description: 10 pages
Additional file 7: of A comparison of methods for estimating substitution rates from ancient DNA sequence data
Creators: name: K. Tong
name: Duchêne, David
name: Duchêne, Sebastián
name: Geoghegan, Jemma
name: Ho, Simon
Publisher: name: figshare
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Plant Biology
subject: Computational Biology

description: Figure S6. Relationships between phylogenetic stemminess and error in median posterior estimates using Bayesian inference in BEAST for 12 simulation treatments. Dashed lines indicate half an order of magnitude above or below the rates used for simulation. Light grey lines indicate lines of best fit for the estimates. (PDF 643 kb)
Front propagation in lattices with on-site bistable non-degenerate potential: multiplicity, bifurcations and route to chaos
Creators: name: Shiroky, I. B.
name: Gendelman, O. V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Other Condensed Matter (cond-mat.other)
subject: Dynamical Systems (math.DS)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Propagation of transition fronts in models of coupled oscillators with non-degenerate on-site potential is usually considered in terms of travelling waves. We show that the system dynamics can be reformulated as an implicit map structure, and the travelling waves correspond to stable fixed points. Therefore, the loss of stability of such waves should follow well-known generic bifurcation scenarios. Then, one can expect a plethora of qualitatively different propagating-front solutions - multistable, multi-periodic, quasiperiodic and chaotic.
title: ADCO, Cart. 186 (11 H 71), f. 0179v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0179v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-
project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
title: {001}-textured Pb(Zr, Ti)O₃ thin films on stainless steel by pulsed laser deposition
Creators: name: Cardoletti, Juliette
name: Komissinskiy, Philipp
name: Bruder, Enrico
name: Morandi, Carl
name: Alff, Lambert
Publisher: name: AIP Publishing
Year: 2024

description: In this work, we report nearly single oriented {001}-textured ferroelectric PbZr0.52Ti0.48O3 thin films grown by pulsed laser deposition onto AISI 304 stainless steel substrates. Pt, Al2O3, and LaNiO3 buffer layers promote the PbZr0.52Ti0.48O3 {001} texture and protect the substrate against oxidation during deposition. The dominant {001} texture of the PbZr0.52Ti0.48O3 layer was confirmed using x-ray and electron backscatter diffraction. Before poling, the films exhibit a permittivity of about 350 at 1 kHz and a dielectric loss below 5%. The films display a remanent polarization of about 16.5 μC cm⁻² and a high coercive field of up to Ec ¼ 135.9 kV cm⁻¹. The properties of these PbZr0.52Ti0.48O3 thin films on stainless steel are promising for various MEMS applications such as transducers or energy harvesters.
Giant cluster arcs as a constraint on the scattering cross-section of dark matter
Creators: name: Meneghetti, Massimo
name: Yoshida, Naoki
name: Bartelmann, Matthias
name: Moscardini, Lauro
name: Springel, Volker
name: Tormen, Giuseppe
name: White, Simon D. M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We carry out ray tracing through five high resolution simulations of a galaxy cluster to study how its ability to produce giant gravitationally lensed arcs is influenced by the collision cross-section of its dark matter. In three cases typical dark matter particles in the cluster core undergo between 1 and 100 collisions per Hubble time; two more explore the long (``collisionless'') and short (``fluid'') mean free path limits. We study the size and shape distributions of arcs and compute the cross-section for producing ``extreme'' arcs of various sizes. Even a few collisions per particle modify the core structure enough to destroy the cluster's ability to produce long, thin arcs. For larger collision frequencies the cluster must be scaled up to unrealistically large masses before it regains the ability to produce giant arcs. None of our models with self-interacting dark matter (except the ``fluid'' limit) is able to produce radial arcs; even the case with the smallest scattering cross-section must be scaled to the upper limit of observed cluster masses before it produces radial arcs. Apparently the elastic collision cross-section of dark matter in clusters must be very small, below 0.1 cm^2 g^-1, to be compatible with the observed ability of clusters to produce both radial arcs and giant arcs.
description: 8 pages, Latex using MN style, accepted version, to appear in MNRAS. Other figures not included in the paper can be found at http://www.mpa-garching.mpg.de/~massimo/SIDMlens.html
The Circumgalactic Medium
Creators: name: Tumlinson, Jason
name: Peeples, Molly S.
name: Werk, Jessica K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The gas surrounding galaxies outside their disks or interstellar medium and inside their virial radii is known as the circumgalactic medium (CGM). In recent years this component of galaxies has assumed an important role in our understanding of galaxy evolution owing to rapid advances in observational access to this diffuse, nearly invisible material. Observations and simulations of this component of galaxies suggest that it is a multiphase medium characterized by rich dynamics and complex ionization states. The CGM is a source for a galaxy's star-forming fuel, the venue for galactic feedback and recycling, and perhaps the key regulator of the galactic gas supply. We review our evolving knowledge of the CGM with emphasis on its mass, dynamical state, and coevolution with galaxies. Observations from all redshifts and from across the electromagnetic spectrum indicate that CGM gas has a key role in galaxy evolution. We summarize the state of this field and pose unanswered questions for future research.
description: 46 pages, 11 figures. Authors' draft version; see http://www.annualreviews.org/doi/10.1146/annurev-astro-091916-055240 for a well-edited final version and fun supplementary figures
Integrable structure in supersymmetric gauge theories with massive hypermultiplets
Creators: name: Ahn, Changhyun
name: Nam, Soonkeon
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the quantum moduli space of vacua of $N=2$ supersymmetric $SU(N_c)$ gauge theories coupled to $N_f$ flavors of quarks in the fundamental representation. We identify the moduli space of the $N_c = 3$ and $N_f=2$ massless case with the full spectral curve obtained from the Lax representation of the Goryachev-Chaplygin top. For the case with {\it massive} quarks, we present an integrable system where the corresponding hyperelliptic curve parametrizing the Laurent solution coincides with that of the moduli space of $N_{c}=3$ with $N_{f}=0, 1, 2$. We discuss possible generalizations of the integrable systems relevant to gauge theories with $N_c \neq 3 $ and general $N_f$.
description: 11 pages, latex, no figures
Additional file 1: of Case report on pathogenetic link between gluten and IgA nephropathy
Creators: name: Costa, Stefano
name: CurrĂ˛, Giovanni
name: Pellegrino, Salvatore
name: Lucanto, Maria
name: Tuccari, Giovanni
name: Ieni, Antonio
name: Visalli, Giuseppina
name: MagazzĂš, Giuseppe
name: Santoro, Domenico
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
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

description: Table S1. Medical history timeline. (PDF 3430Â kb)
The Be/X-ray transient 4U 0115+63/V635 Cas I. A consistent model
Creators: name: Negueruela, I.
name: Okazaki, A. T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present photometry and high SNR spectroscopy in the classification region of V635 Cas, the optical counterpart to the transient X-ray pulsator 4U 0115+63, taken at a time when the circumstellar envelope had disappeared. V635 Cas is classified as a B0.2Ve star at a distance of 7-8 kpc. We use the physical parameters derived from these observations and the orbit derived from X-ray observations to elaborate a model of the system based on the theory of decretion discs around Be stars. We show that the disc surrounding the Be star must be truncated by the tidal/resonant interaction with the neutron star and cannot be in a steady state. This explains many of the observed properties of 4U 0115+63. In particular, because of this effect, under normal circumstances, the neutron star cannot accrete from the disc, which explains the lack of regular Type I outbursts from the source.
description: 10 pages, 6 figures, uses aa.cls. To appear in Astronomy and Astrophysics Main Journal
Additional file 6: of A comparison of methods for estimating substitution rates from ancient DNA sequence data
Creators: name: K. Tong
name: Duchêne, David
name: Duchêne, Sebastián
name: Geoghegan, Jemma
name: Ho, Simon
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Plant Biology

description: Figure S5. Relationships between phylogenetic stemminess and error in rate estimates using least-squares dating in LSD for 12 simulation treatments. Dashed lines indicate half an order of magnitude above or below the rates used for simulation. Light grey lines indicate lines of best fit for the estimates. (PDF 634 kb)
Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
Creators: name: Jones, Mackenzie L.
name: Hickox, Ryan C.
name: Mutch, Simon J.
name: Croton, Darren J.
name: Ptak, Andrew F.
name: DiPompeo, Michael A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In studies of the connection between active galactic nuclei (AGN) and their host galaxies there is widespread disagreement on some key aspects stemming largely from a lack of understanding of the nature of the full underlying AGN population. Recent attempts to probe this connection utilize both observations and simulations to correct for a missed population, but presently are limited by intrinsic biases and complicated models. We take a simple simulation for galaxy evolution and add a new prescription for AGN activity to connect galaxy growth to dark matter halo properties and AGN activity to star formation. We explicitly model selection effects to produce an "observed" AGN population for comparison with observations and empirically motivated models of the local universe. This allows us to bypass the difficulties inherent in many models which attempt to infer the AGN population by inverting selection effects. We investigate the impact of selecting AGN based on thresholds in luminosity or Eddington ratio on the "observed" AGN population. By limiting our model AGN sample in luminosity, we are able to recreate the observed local AGN luminosity function and specific star formation-stellar mass distribution, and show that using an Eddington ratio threshold introduces less bias into the sample by selecting the full range of growing black holes, despite the challenge of selecting low mass black holes. We find that selecting AGN using these various thresholds yield samples with different AGN host galaxy properties.
description: 8 pages, 4 figures. Accepted for publication in ApJ
Pest control in German forests: General patterns of biodiversity and possible impacts of Btk, diflubenzuron and lambda-Cyhalothrin on non-target arthropods, birds and bats – a literature review
Creators: name: Brunk, Ingo
name: Sobczyk, Thomas
name: Roth, Mechthild
Publisher: name: Journal of Forest and Landscape Research
Year: 2019

description: This review focuses on direct and indirect impacts of three insecticides (Bacillus thuringiensis kurstaki, Diflubenzuron, lambda-Cyhalothrin) on arthropods, bats and birds. General patterns of ecology, diversity, distribution and aspects of nature conservation of these three non-target animal taxa in Germany were examined, as well as their specific exposure and possible direct and indirect effects of the insecticides after application. We conclude, that a) the knowledge of direct and indirect effects of the above mentioned insecticides is still very scarce, b) there is an urgent need for more in detail studies in field in general, especially on indirect effects on vertebrates (including amphibians and reptilians), and for further ecotoxicological laboratory studies especially on sublethal effects on vertebrates.
description: Journal of Forest and Landscape Research, Vol 4 No 1 (2019)
Additional file 2 of Non-invasive investigation of early kidney damage in streptozotocin-induced diabetic rats by intravoxel incoherent motion diffusion-weighted (IVIM) MRI
Creators: name: Feng, You-Zhen
name: Chen, Xiao-Qiao
name: Cheng, Zhong-Yuan
name: Lin, Qi-Ting
name: Chen, Ping-Kang
name: Si-Tu, Ding-Kun
name: Cao, Rui
name: Qian, Long
name: Heng, Baoli
name: Cai, Xiang-Ran
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified

description: Additional file 2: Supplemental Table. Expression of Collagen IV in renal tissue of the two groups of rats
Photometric redshifts for the next generation of deep radio continuum surveys - I: Template fitting
Creators: name: Duncan, Kenneth J
name: Brown, Michael J. I.
name: Williams, Wendy L.
name: Best, Philip N.
name: Buat, Veronique
name: Burgarella, Denis
name: Jarvis, Matt J.
name: Malek, Katarzyna
name: Oliver, S. J.
name: Rottgering, Huub J. A.
name: Smith, Daniel J. B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of photometric redshift performance for galaxies and active galactic nuclei detected in deep radio continuum surveys. Using two multi-wavelength datasets, over the NOAO Deep Wide Field Survey Boötes and COSMOS fields, we assess photometric redshift (photo-z) performance for a sample of $\sim 4,500$ radio continuum sources with spectroscopic redshifts relative to those of $\sim 63,000$ non radio-detected sources in the same fields. We investigate the performance of three photometric redshift template sets as a function of redshift, radio luminosity and infrared/X-ray properties. We find that no single template library is able to provide the best performance across all subsets of the radio detected population, with variation in the optimum template set both between subsets and between fields. Through a hierarchical Bayesian combination of the photo-z estimates from all three template sets, we are able to produce a consensus photo-z estimate which equals or improves upon the performance of any individual template set.
description: 20 pages, 17 figures. Accepted for publication in MNRAS
T-duality invariance in random lattice strings
Creators: name: Siegel, W.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Preserving the T-duality invariance of the continuum string in its random lattice regularization uniquely determines the random matrix model potential. For D=0 the duality transformation can be performed explicitly on the matrix action, and replaces color with flavor; invariance thus requires that the color and flavor groups be the same.
description: 8 pg., plain tex, other formats available at http://insti.physics.sunysb.edu/~siegel/preprints/ or at ftp://max.physics.sunysb.edu/preprints/siegel
Latest CMS results on Higgs boson production in association with top quarks ($\mathrm{t\bar{t}H}$)
Creators: name: Ghosh, Saranya
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The searches for Higgs boson production in association with a pair of top quarks at the Compact Muon Solenoid (CMS) experiment using data collected during proton-proton collisions at a center of mass energy of 13 TeV in 2016 are presented. The decay modes of the Higgs boson that are discussed here correspond to the $H \rightarrow ZZ^{*}$, $H \rightarrow WW^{*}$, $H \rightarrow ττ$ and $H \rightarrow γγ$ channels.
description: 7 pages, 10 figures, for the proceedings of the European Physical Society conference on High Energy Physics (EPS-HEP) 2017
A mass conserved reaction-diffusion system captures properties of cell polarity
Creators: name: Otsuji, Mikiya
name: Ishihara, Shuji
name: Co, Carl
name: Kaibuchi, Kozo
name: Mochizuki, Atsushi
name: Kuroda, Shinya
Publisher: name: arXiv
Year: 2006
Subjects: subject: Cell Behavior (q-bio.CB)
subject: FOS: Biological sciences

description: Various molecules exclusively accumulate at the front or back of migrating eukaryotic cells in response to a shallow gradient of extracellular signals. Directional sensing and signal amplification highlight the essential properties in the migrating cells, known as cell polarity. In addition to these, such properties of cell polarity involve unique determination of migrating direction (uniqueness of axis) and localized gradient sensing at the front edge (localization of sensitivity), both of which may be required for smooth migration. Here we provide the mass conservation system based on the reaction-diffusion system with two components, where the mass of the two components is always conserved. Using two models belonging to this mass conservation system, we demonstrate through both numerical simulation and analytical approximations that the spatial pattern with a single peak (uniqueness of axis) can be generally observed and that the existent peak senses a gradient of parameters at the peak position, which guides the movement of the peak. We extended this system with multiple components, and we developed a multiple-component model in which cross-talk between members of the Rho family of small GTPases is involved. This model also exhibits the essential properties of the two models with two components. Thus, the mass conservation system shows properties similar to those of cell polarity, such as uniqueness of axis and localization of sensitivity, in addition to directional sensing and signal amplification.
description: PDF only
Imaging the water snowline in protostellar envelopes
Creators: name: Hoff, Merel L. R. van 't
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Determining the locations of the major snowlines in protostellar environments is crucial to fully understand the planet formation process and its outcome. Despite being located far enough from the central star to be spatially resolved with ALMA, the CO snowline remains difficult to detect directly in protoplanetary disks. Instead, its location can be derived from N$_2$H$^+$ emission, when chemical effects like photodissociation of CO and N$_2$ are taken into account. The water snowline is even harder to observe than that for CO, because in disks it is located only a few AU from the protostar, and from the ground only the less abundant isotopologue H$_2^{18}$O can be observed. Therefore, using an indirect chemical tracer, as done for CO, may be the best way to locate the water snowline. A good candidate tracer is HCO$^+$, which is expected to be particularly abundant when its main destructor, H$_2$O, is frozen out. Comparison of H$_2^{18}$O and H$^{13}$CO$^+$ emission toward the envelope of the Class 0 protostar IRAS2A shows that the emission from both molecules is spatially anticorrelated, providing a proof of concept that H$^{13}$CO$^+$ can indeed be used to trace the water snowline in systems where it cannot be imaged directly.
description: To appear in "Astrochemistry VII -- Through the Cosmos from Galaxies to Planets", proceedings of the IAU Symposium No. 332, 2017, Puerto Varas, Chile. M. Cunningham, T. Millar and Y. Aikawa, eds. (7 pages, 5 figures)
Covariant path integral for chiral p-forms
Creators: name: Devecchi, Fernando P.
name: Henneaux, Marc
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The covariant path integral for chiral bosons obtained by McClain, Wu and Yu is generalized to chiral p-forms. In order to handle the reducibility of the gauge transformations associated with the chiral p-forms and with the new variables (in infinite number) that must be added to eliminate the second class constraints, the field-antifield formalism is used.
description: revtex, 9 pages, submitted to Physical Review D
Additional file 1 of Lactate induces oxidative stress by HIF1α stabilization and circadian clock disturbance in mammary gland of dairy cows
Creators: name: Feng, Juan
name: Zhu, Lei
name: He, Cunman
name: Xiang, Ruidong
name: Liu, Jianxin
name: Cai, Jie
name: Wang, Diming
Publisher: name: figshare
Year: 2025
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Additional file 1: Fig. S1. Protein sequence alignment of Bos taurus BMAL1 and Bos taurus HIF1β (ARNT).
MOESM1 of Development and validation of a new tumor-based gene signature predicting prognosis of HBV/HCV-included resected hepatocellular carcinoma patients
Creators: name: Zhu, Gui-Qi
name: Yang, Yi
name: Chen, Er-Bao
name: Wang, Biao
name: Xiao, Kun
name: Shi, Shi-Ming
name: Zhou, Zheng-Jun
name: Zhou, Shao-Lai
name: Wang, Zheng
name: Shi, Ying-Hong
name: Fan, Jia
name: Zhou, Jian
name: Liu, Tian-Shu
name: Dai, Zhi
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 1: Table S1. Name list of the genes tested by Nanostring in our study for further analysis.
Additional file 1 of Immunogenicity and duration of antibodies after vaccination with a two-dose series of the nine-valent human papillomavirus vaccine among Alaska Native children: a prospective cohort study
Creators: name: Steinberg, Jonathan
name: Panicker, Gitika
name: Unger, Elizabeth R.
name: Blake, Ian
name: Lewis, Rayleen M.
name: Geis, Jesse
name: Bruden, Dana
name: Fischer, Marc
name: Markowitz, Lauri E.
name: Bruce, Michael G.
Publisher: name: figshare
Year: 2025
Subjects: subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology
subject: Cardiology

description: Supplementary Material 1.
MOESM1 of Observational study of coagulation activation in early breast cancer: development of a prognostic model based on data from the real world setting
Creators: name: Mandoj, Chiara
name: Pizzuti, Laura
name: Sergi, Domenico
name: Sperduti, Isabella
name: Mazzotta, Marco
name: Lauro, Luigi
name: Amodio, Antonella
name: Carpano, Silvia
name: Benedetto, Anna
name: Botti, Claudio
name: Ferranti, Francesca
name: Antenucci, Anna
name: DâAlessandro, Maria
name: Marchetti, Paolo
name: Tomao, Silverio
name: Sanguineti, Giuseppe
name: Giordano, Antonio
name: Maugeri-SaccĂ, Marcello
name: Ciliberto, Gennaro
name: Conti, Laura
name: Vici, Patrizia
name: Barba, Maddalena
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Table S1. Multivariate analysis for disease-free survival in a subset of 62 breast cancer patients.
Does the 1/f frequency-scaling of brain signals reflect self-organized critical states?
Creators: name: Bedard, Claude
name: Kroeger, Helmut
name: Destexhe, Alain
Publisher: name: arXiv
Year: 2006
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: Many complex systems display self-organized critical states characterized by 1/f frequency scaling of power spectra. Global variables such as the electroencephalogram, scale as 1/f, which could be the sign of self-organized critical states in neuronal activity. By analyzing simultaneous recordings of global and neuronal activities, we confirm the 1/f scaling of global variables for selected frequency bands, but show that neuronal activity is not consistent with critical states. We propose a model of 1/f scaling which does not rely on critical states, and which is testable experimentally.
description: 3 figures, 6 pages
TENDENCIAS DE INNOVACIÓN EDUCATIVA ¿POR QUÉ PARECEN TAN ALEJADAS DEL AULA?
Creators: name: Fidalgo-Blanco, Ángel
Publisher: name: Zenodo
Year: 2019
Subjects: Innovación Eductiva, Tendencias, Impacto, Sobre expectativas, Post Científico

description: Es posible que se haya preguntado la razón por la que las tendencias en innovación educativa (eso de lo que todo el mundo dice que va a cambiar el modelo educativo) parecen inalcanzables, lejanas e inviables para aplicarlas de forma inmediata en el aula. Pues si se lo ha preguntado, no es la única persona. De hecho, es una realidad que una parte de las tendencias en innovación educativa no se puedan aplicar de forma eficaz en el aula. Tampoco ayuda comprobar que lo que hace años se decía que iba a revolucionar la educación (las tendencias) al final ni se han implantado en el aula, ni han tenido el impacto esperado. Y esto ¿por qué ocurre? ¿Están las tendencias alejadas del aula? ¿Son caras, complejas o poco fiables? Hay tres razones fundamentales para explicar esta aparente lejanía: Las propias características de las tendencias. La rápida y variada evolución. No saber diferenciar el tipo de tendencia (cada tipo tiene un comportamiento distinto). En esta ocasión nos centraremos en la primera razón: las características asociadas a las tendencias de la innovación educativa; como su ciclo de vida.
Additional file 5: of A cross-sectional investigation of the health needs of asylum seekers in a refugee clinic in Germany
Creators: name: Goodman, Laura
name: Jensen, Guy
name: Galante, Joseph
name: Farmer, Diana
name: TachĂŠ, Stephanie
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Science Policy

description: Figure S4. Countries of origin of asylum seekers in Saxony 2015. Countries of origin are plotted with percentage of total asylum seekers who arrived in Saxony between 1 January and 31 December 2015. The data is from Landesdirektion Sachsen, or the State Directorate of Saxony [11]. (DOCX 77Â kb)
Unsupervised and Semi-supervised Anomaly Detection with LSTM Neural Networks
Creators: name: Ergen, Tolga
name: Mirza, Ali Hassan
name: Kozat, Suleyman Serdar
Publisher: name: arXiv
Year: 2017
Subjects: subject: Signal Processing (eess.SP)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: We investigate anomaly detection in an unsupervised framework and introduce Long Short Term Memory (LSTM) neural network based algorithms. In particular, given variable length data sequences, we first pass these sequences through our LSTM based structure and obtain fixed length sequences. We then find a decision function for our anomaly detectors based on the One Class Support Vector Machines (OC-SVM) and Support Vector Data Description (SVDD) algorithms. As the first time in the literature, we jointly train and optimize the parameters of the LSTM architecture and the OC-SVM (or SVDD) algorithm using highly effective gradient and quadratic programming based training methods. To apply the gradient based training method, we modify the original objective criteria of the OC-SVM and SVDD algorithms, where we prove the convergence of the modified objective criteria to the original criteria. We also provide extensions of our unsupervised formulation to the semi-supervised and fully supervised frameworks. Thus, we obtain anomaly detection algorithms that can process variable length data sequences while providing high performance, especially for time series data. Our approach is generic so that we also apply this approach to the Gated Recurrent Unit (GRU) architecture by directly replacing our LSTM based structure with the GRU based structure. In our experiments, we illustrate significant performance gains achieved by our algorithms with respect to the conventional methods.
N=1 Heterotic/M-theory Duality and Joyce Manifolds
Creators: name: Acharya, B. S.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present an ansatz which enables us to construct heterotic/M-theory dual pairs in four dimensions. It is checked that this ansatz reproduces previous results and that the massless spectra of the proposed dual pairs agree. The new dual pairs consist of M-theory compactifications on Joyce manifolds of $G_2$ holonomy and Calabi-Yau compactifications of heterotic strings. These results are further evidence that M-theory is consistent on orbifolds. Finally, we interpret these results in terms of M-theory geometries which are K3 fibrations and heterotic geometries which are conjectured to be $T^3$ fibrations. Even though the new dual pairs are constructed as non-freely acting orbifolds of existing dual pairs, the adiabatic argument is apparently not violated.
description: 25 pages, Latex
Unveiling the physical and chemical conditions in the young disk around L1527
Creators: name: Hoff, Merel L. R. van 't
name: Tobin, John J.
name: Harsono, Daniel
name: van Dishoeck, Ewine F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Planets form in disks around young stars. The planet formation process may start when the protostar and disk are still deeply embedded within their infalling envelope. However, unlike more evolved protoplanetary disks, the physical and chemical structure of these young embedded disks are still poorly constrained. We have analyzed ALMA data for $^{13}$CO, C$^{18}$O and N$_2$D$^+$ to constrain the temperature structure, one of the critical unknowns, in the disk around L1527. The spatial distribution of $^{13}$CO and C$^{18}$O, together with the kinetic temperature derived from the optically thick $^{13}$CO emission and the non-detection of N$_2$D$^+$, suggest that this disk is warm enough ($\gtrsim$ 20 K) to prevent CO freeze-out.
description: To appear in "Astrochemistry VII -- Through the Cosmos from Galaxies to Planets", proceedings of the IAU Symposium No. 332, 2017, Puerto Varas, Chile. M. Cunningham, T. Millar and Y. Aikawa, eds. (3 pages, 2 figures)