cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Microplastic fibres affect soil fungal communities depending on drought conditions with consequences for ecosystem functions
Creators: name: Lozano, Yudi M.
name: Dueñas, Juan F.
name: Zordick, Catrin
name: Rillig, Matthias C.
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: fehlen
subject: 500 Naturwissenschaften und Mathematik::570 Biowissenschaften; Biologie::570 Biowissenschaften; Biologie

description: Microplastics affect soil functions depending on drought conditions. However, how their combined effect influences soil fungi and their linkages with ecosystem functions is still unknown. To address this, we used rhizosphere soil from a previous experiment in which we employed microplastic fibres addition and drought in a factorial design, and evaluated their effects on soil fungal communities. Microplastics decreased soil fungal richness under well-watered conditions, likely linked to microplastics leaching toxic substances into the soil, and microplastic effects on root fineness. Under drought, by contrast, microplastics increased pathogen and total fungal richness, likely related to microplastic positive effects on soil properties, such as water holding capacity, porosity or aggregation. Soil fungal richness was the attribute most affected by microplastics and drought. Microplastics altered the relationships between soil fungi and ecosystem functions to the point that many of them flipped from positive to negative or disappeared. The combined effect of microplastics and drought on fungal richness mitigated their individual negative effect (antagonism), suggesting that changes in soil water conditions may alter the action mode of microplastics in soil. Microplastic leaching of harmful substances can be mitigated under drought, while the improvement of soil properties by microplastics may alleviate such drought conditions.
Additional file 1 of Withholding and withdrawal of life-sustaining treatments in intensive care units in Lebanon: a cross-sectional survey of intensivists and interviews of professional societies, legal and religious leaders
Creators: name: Jawiche, Rita El
name: Hallit, Souheil
name: Tarabey, Lubna
name: Abou-Mrad, Fadi
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 1. Appendix 1. This file includes the questionnaire used for this study.
Precise seismology with TESS CVZ data
Creators: name: Vrard, Mathieu
name: Pinsonneault, Marc
name: Hon, Marc
name: Kuszlewicz, James
name: Li, Yaguang
name: Hekker, Saskia
name: Mathur, Savita
name: Stello, Dennis
Publisher: name: Zenodo
Year: 2021
Subjects: Stellar Astrophysics
Asteroseismology
Stars: evolution

description: The release of TESS light-curves gives us the opportunity to perform all-sky seismology for a lot of stars. Among them, the higher quality data that was obtained from the longer light-curves of the South Continuous Viewing Zone (SCVZ) correspond to the best opportunity to conduct precise seismology. In this work we present the first attempt to measure precisely the evolutionary status of a large number red giants stars with TESS data in order to assess the potentiality of those data to perform precise seimsology.
description: {"references": ["Hon et al. (2017). Decouple software associated to arXiv:1705.06405", "Hon et al. (2018). Decouple software associated to arXiv:1804.07495", "Kuszlewicz et al. (2020). Decouple software associated to arXiv:2007.10921", "Mackereth et al. (2021). Decouple software associated to arXiv:2012.00140", "Vrard et al. (2016). Decouple software associated to arXiv:1602.04940"]}
Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation
Creators: name: Schlaufman, Kevin C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Celestial bodies with a mass of M ~ 10 M_Jup have been found orbiting nearby stars. It is unknown whether these objects formed like gas-giant planets through core accretion or like stars through gravitational instability. I show that objects with M ~ 10 M_Jup do not share this property. This transition is coincident with a minimum in the occurrence rate of such objects, suggesting that the maximum mass of a celestial body formed through core accretion like a planet is less than 10 M_Jup. Consequently, objects with M >~ 10 M_Jup orbiting solar-type dwarf stars likely formed through gravitational instability and should not be thought of as planets. Theoretical models of giant planet formation in scaled minimum-mass solar nebula Shakura--Sunyaev disks with standard parameters tuned to produce giant planets predict a maximum mass nearly an order of magnitude larger. To prevent newly formed giant planets from growing larger than 10 M_Jup, protoplanetary disks must therefore be significantly less viscous or of lower mass than typically assumed during the runaway gas accretion stage of giant planet formation. Either effect would act to slow the Type I/II migration of planetary embryos/giant planets and promote their survival. These inferences are insensitive to the host star mass, planet formation location, or characteristic disk dissipation time.
description: 20 pages, 4 figures, and 2 tables in aastex61 format; accepted for publication in ApJ
Electronic Synapses Enabled by an Epitaxial SrTiO3-δ / Hf0.5Zr0.5O2 Ferroelectric Field-Effect Memristor Integrated on Silicon
Creators: name: Siannas, Nikitas
name: Zacharaki, Christina
name: Tsipas, Polychronis
name: Kim, Dong Jik
name: Hamouda, Wassim
name: Istrate, Cosmin
name: Pintilie, Lucian
name: Schmidbauer, Martin
name: Dubourdieu, Catherine
name: Dimoulas, Athanasios
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: artificial synapses
subject: epitaxial HZO
subject: ferroelectric field effect memristors
subject: molecular beam epitaxy
subject: neuromorphic computing
subject: 500 Naturwissenschaften und Mathematik::540 Chemie::540 Chemie und zugeordnete Wissenschaften

description: Synapses play a vital role in information processing, learning, and memory formation in the brain. By emulating the behavior of biological synapses, electronic synaptic devices hold the promise of enabling high-performance, energy-efficient, and scalable neuromorphic computing. Ferroelectric memristive devices integrate the characteristics of both ferroelectric and memristive materials and present a far-reaching potential as artificial synapses. Here, it is reported on a new ferroelectric device on silicon, a field-effect memristor, consisting of an epitaxial ultrathin ferroelectric Hf0.5Zr0.5O2 film sandwiched between an epitaxial highly doped oxide semiconductor SrTiO3-δ and a top metal. Upon a low voltage of less than 2 V, the field-effect modulation in the semiconductor enables to access multiple states. The device works in a large time domain ranging from milliseconds down to tens of nanoseconds. By gradually switching the polarization by identical pulses, the ferroelectric diode devices can dynamically adjust the synaptic strength to mimic short- and long-term memory plasticity. Ionic contributions due to redox processes in the oxide semiconductor beneficially influence the device operation and retention.
Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning
Creators: name: Heger, Alexander
name: Cumming, Andrew
name: Galloway, Duncan K.
name: Woosley, Stanford E.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The X-ray burster GS 1826-24 shows extremely regular Type I X-ray bursts whose energetics and recurrence times agree well with thermonuclear ignition models. We present calculations of sequences of burst lightcurves using multizone models which follow the rp-process nucleosynthesis with an extensive nuclear reaction network. The theoretical and observed burst lightcurves show remarkable agreement. The models naturally explain the slow ~5s rise and long ~100s tails of these bursts, as well as their dependence on mass accretion rate. This comparison provides further evidence for solar metallicity in the accreted material in this source, and constrains the distance to the source. The main difference is that the observed lightcurves do not show the distinct two-stage rise of the models. This may reflect the time for burning to spread over the stellar surface, or may indicate that our treatment of heat transport or nuclear physics needs to be revised. The trends in burst properties with accretion rate are well-reproduced by our spherically symmetric models which include chemical and thermal inertia from the ashes of previous bursts. Changes in the covering fraction of the accreted fuel are not required.
description: 5 pages, 4 figures, to appear in ApJ letters
Understanding Network Complexity
Creators: name: Wing, Jeannette M.
Publisher: name: Carnegie Mellon University
Year: 2001
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Our networks have evolved to be extremely complex and we do not understand them. The Internet, for example, is complex. In 1970 we could draw the four‐node DARPAnet on a napkin. Forty years later, due to its scale and dynamic nature, the Internet is too complex to draw, let alone understand, model, or predict its behavior. The Internet is computer science’s gift to society, but ironically we cannot even describe it.
Additional file 1 of Life is different now – impacts of eating disorders on Carers in New Zealand: a qualitative study
Creators: name: Fletcher, Louise
name: Trip, Henrietta
name: Lawson, Rachel
name: Wilson, Nicki
name: Jordan, Jennifer
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. COREQ (COnsolidated criteria for REporting Qualitative research) Checklist.
Additional file 1 of Polymorphisms of brain-derived neurotrophic factor genes are associated with anxiety and body mass index in fibromyalgia syndrome patients
Creators: name: Nugraha, Boya
name: Sumadi Lukman Anwar
name: Gutenbrunner, Christoph
name: Korallus, Christoph
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Figure S1. Pyrograms from individuals with polymorphisms of rs712442 and rs2049046. Representative pyrograms from a HC with AT allele and a FMS patient with AT allele of rs2049046 were shown in panel A and B, respectively. Representative pyrograms from a HC with GA allele and a FMS patient with AA allele of rs712442 were shown in panel C and D, respectively.
Néel temperature and reentrant H-T phase diagram of quasi-2D frustrated magnets
Creators: name: Schmidt, Burkhard
name: Thalmeier, Peter
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In quasi-2D quantum magnets the ratio of Néel temperature $T_\text N$ to Curie-Weiss temperature $Θ_\text{CW}$ is frequently used as an empirical criterion to judge the strength of frustration. In this work we investigate how these quantities are related in the canonical quasi-2D frustrated square or triangular $J_1$-$J_2$ model. Using the self-consistent Tyablikov approach for calculating $T_\text N$ we show their dependence on the frustration control parameter $J_2/J_1$ in the whole Néel and columnar antiferromagnetic phase region. We also discuss approximate analytical results. In addition the field dependence of $T_\text N(H)$ and the associated possible reentrance behavior of the ordered moment due to quantum fluctuations is investigated. These results are directly applicable to a class of quasi-2D oxovanadate antiferromagnets. We give clear criteria to judge under which conditions the empirical frustration ratio $f=Θ_\text{CW}/T_\text N$ may be used as measure of frustration strength in the quasi-2D quantum magnets.
description: 16 pages, 14 figures, to appear in Physical Review B
On the existence of a luminosity threshold of GRB jets in massive stars
Creators: name: Aloy, Miguel-Ángel
name: Cuesta-Martínez, Carlos F.
name: Obergaulinger, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Motivated by the many associations of $γ$-ray bursts (GRBs) with energetic supernova (SN) explosions, we study the propagation of relativistic jets within the progenitor star in which a SN shock wave may be launched briefly before the jets start to propagate. Based on analytic considerations and verified with an extensive set of 2D axisymmetric relativistic hydrodynamic simulations, we have estimated a threshold intrinsic jet luminosity, $L_{\rm j}^{\rm thr}$, for successfully launching a jet. This threshold depends on the structure of the progenitor and, thus, it is sensible to its mass and to its metallicity. For a prototype host of cosmological long GRBs, a low-metallicity star of 35$\,M_{\odot}$, it is $L_{\rm j}^{\rm thr} \simeq 1.35\times 10^{49}\,$erg$\,$s$^{-1}$. The observed equivalent isotropic $γ$-ray luminosity, $L_{\rm γ,iso,BO} \simeq 4 ε_γL_{\rm j} θ_{\rm BO}^{-2}$, crucially depends on the jet opening angle after breakout, $θ_{\rm BO}$, and on the efficiency for converting the intrinsic jet luminosity into $γ$-radiation, $ε_γ$. Highly energetic jets can produce low-luminosity events if either their opening angle after the breakout is large, which is found in our models, or if the conversion efficiency of kinetic and internal energy into radiation is low enough. Beyond this theoretical analysis, we show how the presence of a SN shock wave may reduce this luminosity threshold by means of numerical simulations. We foresee that the high-energy transients released by jets produced near the luminosity threshold will be more similar to llGRBs or XRFs than to GRBs.
description: 14 pages, 7 color figures. Submitted to MNRAS
Neurological examination of clinically healthy pigeons (Columba livia domestica), mute swans (Cygnus olor), common buzzards (Buteo buteo), common kestrels (Falco tinnunculus) and northern goshawks (Accipiter gentilis)
Creators: name: Feyer, Sina
name: Loderstedt, Shenja
name: Halter-Gölkel, Lesley
name: Merle, Roswitha
name: Zein, Stephanie
name: Müller, Kerstin
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: avian neurological examination
subject: feral pigeons
subject: mute swans
subject: neurology
subject: raptors
subject: 600 Technik, Medizin, angewandte Wissenschaften::630 Landwirtschaft::630 Landwirtschaft und verwandte Bereiche

description: Background A neurological examination is essential for determining the localisation of neurological lesions. However, in avian species, quantitative data regarding the practicability and feasibility of neurological tests are very limited. Therefore, the aim of this study was to establish normative data for the neurological examination of clinically healthy birds of different species. Methods Forty-two domestic and feral pigeons (Columba livia domestica), 42 mute swans (Cygnus olor), 12 common buzzards (Buteo buteo), 24 common kestrels (Falco tinnunculus) and six northern goshawks (Accipiter gentilis) were examined. All birds underwent a predefined neurological examination. Interobserver variations between three examiners were investigated in 11 pigeons and 11 mute swans. Results All postural reaction tests, except for the drop and flap reaction in mute swans, provoked a consistent response in pigeons and mute swans, whereas postural reaction tests of the legs in raptors were often not performable. Cranial nerve tests and most of the spinal reflexes revealed variable responses in all birds. The gastrocnemius reflex was not provokable in any bird. Interobserver agreement was almost perfect (Gwet's AC1 coefficient ≥0.81) for 16 of 21 parameters in the examination in pigeons and for 14 of 21 in mute swans. Limitations The inclusion of free-ranging birds, which were not used to handling and for which limited information regarding age, history of previous diseases, etc. was available, may have influenced the results. Conclusion The normative neurological examination data provided in this study will help improve clinicians' interpretation of neurological examination results in the respective bird species.
No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
Creators: name: Fitts, Alex
name: Boylan-Kolchin, Michael
name: Bullock, James S.
name: Weisz, Daniel R.
name: El-Badry, Kareem
name: Wheeler, Coral
name: Faucher-Giguère, Claude-André
name: Quataert, Eliot
name: Hopkins, Philip F.
name: Kereš, Dušan
name: Wetzel, Andrew
name: Hayward, Chris
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the merger histories of isolated dwarf galaxies based on a suite of 15 high-resolution cosmological zoom-in simulations, all with masses of $M_{\rm halo} \approx 10^{10}\,{\rm M}_{\odot}$ (and M$_\star\sim10^5-10^7\,{\rm M}_{\odot}$) at $z=0$, from the Feedback in Realistic Environments (FIRE) project. The stellar populations of these dwarf galaxies at $z=0$ are formed essentially entirely "in situ": over 90$\%$ of the stellar mass is formed in the main progenitor in all but two cases, and all 15 of the galaxies have >70$\%$ of their stellar mass formed in situ. Virtually all galaxy mergers occur prior to $z\sim3$, meaning that accreted stellar populations are ancient. On average, our simulated dwarfs undergo 5 galaxy mergers in their lifetimes, with typical pre-merger galaxy mass ratios that are less than 1:10. This merger frequency is generally comparable to what has been found in dissipationless simulations when coupled with abundance matching. Two of the simulated dwarfs have a luminous satellite companion at $z=0$. These ultra-faint dwarfs lie at or below current detectability thresholds but are intriguing targets for next-generation facilities. The small contribution of accreted stars make it extremely difficult to discern the effects of mergers in the vast majority of dwarfs either photometrically or using resolved-star color-magnitude diagrams (CMDs). The important implication for near-field cosmology is that star formation histories of comparably massive galaxies derived from resolved CMDs should trace the build-up of stellar mass in one main system across cosmic time as opposed to reflecting the contributions of many individual star formation histories of merged dwarfs.
description: 14 pages, 12 figures; submitted to MNRAS on 12/28/17
Adaptive antenna system by ESP32-PICO-D4 and its application to web radio system
Creators: name: Kodera, Toshiro
Publisher: name: arXiv
Year: 2017
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Adaptive antenna technique has an important role in the IoT environment in order to establish reliable and stable wireless communication in high congestion situation. Even if knowing antenna characteristics in advance, electromagnetic wave propagation in the non-line-of-sight environment is very complex and unpredictable, therefore, the adjustment the antenna radiation for the optimum signal reception is important for the better wireless link. This article presents a simple but effective adaptive antenna system for Wi-Fi utilizing the function of a highly integrated component, ESP32-PICO-D4. This chip is a system-in-chip containing all components for Wi-Fi and Bluetooth application except for antenna. Together with SP3T RF switch and dielectric antennas and high-resolution audio DAC, completed web-radio system is made in the size of 50 x 50 mm.
description: This article is submitted for HardwareX
title: Les merdjas du Gharb
title: Les merdjas du Gharb
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: Espace naturel
subject: Merja
subject: Lagunes

description: Cartographie
description: BESM-carto_1935-08-p120_08-08
description: 120
description: 8
description: Bulletin économique et social du Maroc
description: Source: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Source: Bulletin économique et social du Maroc
description: Source: Bulletin économique et social du Maroc (BESM) > BESM (Cartographie)
description: Relation: https://cinumed.mmsh.univ-aix.fr/idurl/1/81615
description: Coverage: Maroc
description: Coverage: Gharb
description: Coverage: XXe siècle
description: Temporal: XXe siècle
description: Bibliographic citation: « Les merdjas du Gharb », In Bulletin économique et social du Maroc (BESM), n° 8, 1935
description: Provenance: Maison méditerranéenne des sciences de l'homme, Cité numérique de la Méditerranée (Cinumed), Bibliothèque nationale du Royaume du Maroc (BNRM)
description: Provenance: https://cinumed.mmsh.univ-aix.fr/
Occultations from an active accretion disk in a 72 day detached post-Algol system detected by K2
Creators: name: Zhou, G.
name: Rappaport, S.
name: Nelson, L.
name: Huang, C. X.
name: Senhadji, A.
name: Rodriguez, J. E.
name: Vanderburg, A.
name: Quinn, S.
name: Johnson, C. I.
name: Latham, D. W.
name: Torres, G.
name: Gary, B. L.
name: Tan, T. G.
name: Johnson, M. C.
name: Burt, J.
name: Kristiansen, M. H.
name: Jacobs, T. L.
name: LaCourse, D.
name: Schwengeler, H. M.
name: Terentev, I.
name: Bieryla, A.
name: Esquerdo, G. A.
name: Berlind, P.
name: Calkins, M. L.
name: Bento, J.
name: Cochran, W. D.
name: Karjalainen, M.
name: Hatzes, A. P.
name: Karjalainen, R.
name: Holden, B.
name: Butler, R. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Disks in binary systems can cause exotic eclipsing events. MWC 882 (BD-22 4376, EPIC 225300403) is such a disk-eclipsing system identified from observations during Campaign 11 of the K2 mission. We propose that MWC 882 is a post-Algol system with a B7 donor star of mass $0.542\pm0.053\,M_\odot$ in a 72 day period orbit around an A0 accreting star of mass $3.24\pm0.29\,M_\odot$. The $59.9\pm6.2\,R_\odot$ disk around the accreting star occults the donor star once every orbit, inducing 19 day long, 7% deep eclipses identified by K2, and subsequently found in pre-discovery ASAS and ASAS-SN observations. We coordinated a campaign of photometric and spectroscopic observations for MWC 882 to measure the dynamical masses of the components and to monitor the system during eclipse. We found the photometric eclipse to be gray to $\approx 1$%. We found the primary star exhibits spectroscopic signatures of active accretion, and observed gas absorption features from the disk during eclipse. We suggest MWC 882 initially consisted of a $\approx 3.6\,M_\odot$ donor star transferring mass via Roche lobe overflow to a $\approx 2.1\,M_\odot$ accretor in a $\approx 7$ day initial orbit. Through angular momentum conservation, the donor star is pushed outward during mass transfer to its current orbit of 72 days. The observed state of the system corresponds with the donor star having left the Red Giant Branch ~0.3 Myr ago, terminating active mass transfer. The present disk is expected to be short-lived ($10^2$ years) without an active feeding mechanism, presenting a challenge to this model.
description: 19 pages, accepted for publication in ApJ
Additional file 2 of Attrition, physical integrity and insecticidal activity of long-lasting insecticidal nets in sub-Saharan Africa and modelling of their impact on vectorial capacity
Creators: name: Briet, Olivier
name: Koenker, Hannah
name: Norris, Laura
name: Wiegand, Ryan
name: Eng, Jodi Vanden
name: Thackeray, Alex
name: Williamson, John
name: Gimnig, John E.
name: Fortes, Filomeno
name: Akogbeto, Martin
name: Anges W. Yadouleton
name: Ombok, Maurice
name: M. Nabie Bayoh
name: Themba Mzilahowa
name: Abílio, Ana Paula
name: Mabunda, Samuel
name: Cuamba, Nelson
name: Elhadji Diouf
name: Lassana Konaté
name: Busiku Hamainza
name: Katebe-Sakala, Cecilia
name: León, Gabriel Ponce De
name: Kwame Asamoa
name: Wolkon, Adam
name: Smith, Stephen C.
name: Swamidoss, Isabel
name: Green, Mike
name: Gueye, Salam
name: Mihigo, Jules
name: Morgan, Juliette
name: Dotson, Ellen
name: Craig, Allen S.
name: Tan, Kathrine R.
name: Wirtz, Robert A.
name: Smith, Tom
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Computational Biology

description: Additional file 2: Details of methods and results.
title: ADCO, Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0000-001
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0000-001, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0000-001, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Saint-Seine
description: Provenance: http://www.wikidata.org/entity/Q2820709
Testing the relativistic Doppler boost hypothesis for supermassive black hole binary candidates
Creators: name: Charisi, M.
name: Haiman, Z.
name: Schiminovich, D.
name: D'Orazio, D. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Supermassive black hole binaries (SMBHBs) should be common in galactic nuclei as a result of frequent galaxy mergers. Recently, a large sample of sub-parsec SMBHB candidates was identified as bright periodically variable quasars in optical surveys. If the observed periodicity corresponds to the redshifted binary orbital period, the inferred orbital velocities are relativistic (v/c~0.1). The optical and UV luminosities are expected to arise from gas bound to the individual BHs, and would be modulated by the relativistic Doppler effect. The optical and UV light curves should vary in tandem with relative amplitudes which depend on the respective spectral slopes. We constructed a control sample of 42 quasars with aperiodic variability, to test whether this Doppler colour signature can be distinguished from intrinsic chromatic variability. We found that the Doppler signature can arise by chance in ~20% (~37%) of quasars in the nUV (fUV) band. These probabilities reflect the limited quality of the control sample and represent upper limits on how frequently quasars mimic the Doppler brightness+colour variations. We performed separate tests on the periodic quasar candidates, and found that for the majority, the Doppler boost hypothesis requires an unusually steep UV spectrum or an unexpectedly large BH mass and orbital velocity. We conclude that at most ~1/3rd of these periodic candidates can harbor Doppler-modulated SMBHBs.
description: submitted in MNRAS
Observations of Six Glitches in PSR B1737-30
Creators: name: Zou, W. Z.
name: Wang, N.
name: Manchester, R. N.
name: Urama, J. O.
name: Hobbs, G.
name: Liu, Z. Y.
name: Yuan, J. P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Six glitches have been recently observed in the rotational frequency of the young pulsar PSR B1737-30 (J1740-3015) using the 25-m Nanshan telescope of Urumqi Observatory. With a total of 20 glitches in 20 years, it is one of the most frequently glitching pulsars of the about 1750 known pulsars. Glitch amplitudes are very variable with fractional increases in rotation rate ranging from 10^{-9} to 10^{-6}. Inter-glitch intervals are also very variable, but no relationship is observed between interval and the size of the preceding glitch. There is a persistent increase in |\dotν|, opposite in sign to that expected from slowdown with a positive braking index, which may result from changes in the effective magnetic dipole moment of the star during the glitch.
description: 7 pages, 10 figures
Additional file 1 of Sex differences in adaptation to intermittent post-exercise sauna bathing in trained middle-distance runners
Creators: name: Kirby, Nathalie V.
name: Lucas, Samuel J. E.
name: Cable, Thomas G.
name: Armstrong, Oliver J.
name: Weaver, Samuel R.
name: Lucas, Rebekah A. I.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy
subject: 60506 Virology

description: Additional file 1.
Gehlen, Andreas von: Parteiendemokratien – Zur Legitimation der EU-Mitgliedstaaten durch politische Parteien, De Gruyter, Oldenbourg 2017
Creators: name: Roßner, Sebastian
Publisher: name: Zeitschrift für Parteienwissenschaften
Year: 2018

description: Zeitschrift für Parteienwissenschaften, Nr. 1 (2018): Mitteilungen des Instituts für Deutsches und Internationales Parteienrecht und Parteienforschung
Combined application of up to ten pesticides decreases key soil processes
Creators: name: Meidl, Peter
name: Lehmann, Anika
name: Bi, Mohan
name: Breitenreiter, Carla
name: Benkrama, Jasmina
name: Li, Erqin
name: Riedo, Judith
name: Rillig, Matthias C.
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: Agriculture
subject: Currently used pesticides
subject: Litter decomposition
subject: Rate of change
subject: Soil processes
subject: Water stable aggregates
subject: 500 Naturwissenschaften und Mathematik::570 Biowissenschaften; Biologie::570 Biowissenschaften; Biologie

description: Natural systems are under increasing pressure by a range of anthropogenic global change factors. Pesticides represent a nearly ubiquitously occurring global change factor and have the potential to affect soil functions. Currently the use of synthetic pesticides is at an all-time high with over 400 active ingredients being utilized in the EU alone, with dozens of these pesticides occurring concurrently in soil. However, we presently do not understand the impacts of the potential interaction of multiple pesticides when applied simultaneously. Using soil collected from a local grassland, we utilize soil microcosms to examine the role of both rate of change and number of a selection of ten currently used pesticides on soil processes, including litter decomposition, water stable aggregates, aggregate size, soil pH, and EC. Additionally, we used null models to enrich our analyses to examine potential patterns caused by interactions between pesticide treatments. We find that both gradual and abrupt pesticide application have negative consequences for soil processes. Notably, pesticide number plays a significant role in affecting soil health. Null models also reveal potential synergistic behavior between pesticides which can further their consequences on soil processes. Our research highlights the complex impacts of pesticides, and the need for environmental policy to address the threats posed by pesticides.
Spin Dynamics at the Mott Transition and in the Metallic State of the Cs_{3}C_{60} Superconducting Phases
Creators: name: Ihara, Y.
name: Alloul, H.
name: Wzietek, P.
name: Pontiroli, D.
name: Mazzani, M.
name: Riccò, M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We present here ^{13}C and ^{133}Cs NMR spin lattice relaxation T_{1} data in the A15 and fcc-Cs_{3}C_{60} phases for increasing hydrostatic pressure through the transition at p_{c} from a Mott insulator to a superconductor. We evidence that for p>> p_{c} the (T_{1}T)^{-1} data above T_{c} display metallic like Korringa constant values which match quantitatively previous data taken on other A_{3}C_{60} compounds. However below the pressure for which T_{c} goes through a maximum, (T_{1}T)^{-1} is markedly increased with respect to the Korringa values expected in a simple BCS scenario. This points out the importance of electronic correlations near the Mott transition. For p > p_{c} singular T dependences of (T_{1}T)^{-1} are detected for T >> T_{c}. It will be shown that they can be ascribed to a large variation with temperature of the Mott transition pressure p_{c} towards a liquid-gas like critical point, as found at high T for usual Mott transitions.
description: 6 pages, 6 figures, submitted to EPL
Optical, near-IR and sub-mm IFU Observations of the nearby dual AGN Mrk 463
Creators: name: Treister, E.
name: Privon, G. C.
name: Sartori, L. F.
name: Nagar, N.
name: Bauer, F. E.
name: Schawinski, K.
name: Messias, H.
name: Ricci, C.
name: U, V.
name: Casey, C.
name: Comerford, J. M.
name: Muller-Sanchez, F.
name: Evans, A. S.
name: Finlez, C.
name: Koss, M.
name: Sanders, D. B.
name: Urry, C. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present optical and near-IR Integral Field Unit (IFU) and ALMA band 6 observations of the nearby dual Active Galactic Nuclei (AGN) Mrk 463. At a distance of 210 Mpc, and a nuclear separation of $\sim$4 kpc, Mrk 463 is an excellent laboratory to study the gas dynamics, star formation processes and supermassive black hole (SMBH) accretion in a late-stage gas-rich major galaxy merger. The IFU observations reveal a complex morphology, including tidal tails, star-forming clumps, and emission line regions. The optical data, which map the full extent of the merger, show evidence for a biconical outflow and material outflowing at $>$600 km s$^{-1}$, both associated with the Mrk 463E nucleus, together with large scale gradients likely related to the ongoing galaxy merger. We further find an emission line region $\sim$11 kpc south of Mrk 463E that is consistent with being photoionized by an AGN. Compared to the current AGN luminosity, the energy budget of the cloud implies a luminosity drop in Mrk 463E by a factor 3-20 over the last 40,000 years. The ALMA observations of $^{12}$CO(2-1) and adjacent 1mm continuum reveal the presence of $\sim$10$^{9}$M$_\odot$ in molecular gas in the system. The molecular gas shows velocity gradients of $\sim$800 km/s and $\sim$400 km/s around the Mrk 463E and 463W nuclei, respectively. We conclude that in this system the infall of $\sim$100s $M_\odot$/yr of molecular gas is in rough balance with the removal of ionized gas by a biconical outflow being fueled by a relatively small, $
description: Accepted by The Astrophysical Journal, 23 pages, 19 figures
"Gravitational mass" of information?
Creators: name: Kish, Laszlo B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We hypothesize possible new types of forces that would be the result of new types of interactions, static and a slow transient, between objects with related information contents (pattern). Such mechanism could make material composition dependence claimed by Fishbach, et al in Eotvos type experiments plausible. We carried out experiments by using a high-resolution scale with the following memories: USB-2 flash drives (1-16GB), DVD and CD disks to determine if such an interaction exist/detectable with a scale resolution of 10 microgram with these test objects. We applied zero information, white noise and 1/f noise type data. Writing or deleting the information in any of these devices causes peculiar negative weight transients, up to milligrams (mass fraction around 10^-5), which is followed by various types of relaxation processes. These relaxations have significantly different dynamics compared to transients observed during cooling after stationary external heating. Interestingly, a USB-1 MP3 player has also developed comparable transient mass loss during playing music. A classical interpretation of the negative weight transients could be absorbed water in hygroscopic components however comparison of relaxation time constants with air humidity data does not support an obvious explanation. Another classical interpretation with certain contribution is the lifting Bernoulli force caused by the circulation due to convection of the warm air. However, in this case all observed time constants with a device should have been the same unless some hidden parameter causes the observed variations. Further studies are warranted to clarify if there is indeed a new force, which is showing up as negative mass at weight measurement when high-density structural information is changed or read out (measured).
description: Final language corrections based on the galley proof of the published paper
Evolutionary Dynamics in a Simple Model of Self-Assembly
Creators: name: Johnston, Iain G.
name: Ahnert, Sebastian A.
name: Doye, Jonathan P. K.
name: Louis, Ard A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: We investigate the evolutionary dynamics of an idealised model for the robust self-assembly of two-dimensional structures called polyominoes. The model includes rules that encode interactions between sets of square tiles that drive the self-assembly process. The relationship between the model's rule set and its resulting self-assembled structure can be viewed as a genotype-phenotype map and incorporated into a genetic algorithm. The rule sets evolve under selection for specified target structures. The corresponding, complex fitness landscape generates rich evolutionary dynamics as a function of parameters such as the population size, search space size, mutation rate, and method of recombination. Furthermore, these systems are simple enough that in some cases the associated model genome space can be completely characterised, shedding light on how the evolutionary dynamics depends on the detailed structure of the fitness landscape. Finally, we apply the model to study the emergence of the preference for dihedral over cyclic symmetry observed for homomeric protein tetramers.
Photo-responsive hydrogels based on a ruthenium complex: synthesis and degradation
Creators: name: Tavakkoli Fard, Sara
name: Thongrom, Boonya
name: Achazi, Katharina
name: Ma, Guoxin
name: Haag, Rainer
name: Tzschucke, C. Christoph
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: Photo-responsive
subject: hydrogel
subject: ruthenium complex
subject: 500 Naturwissenschaften und Mathematik::540 Chemie::540 Chemie und zugeordnete Wissenschaften

description: We report the synthesis of a photo responsive metallo-hydrogel based on a ruthenium(II) complex as a functional cross-linker. This metal complex contains reactive 4AAMP (= 4-(acrylamidomethyl)pyridine) ligands, which can be cleaved by light-induced ligand substitution. Ru[(bpy)2(4AAMP)2] cross-links 4-arm-PEG-SH macromonomers by thia-Michael-addition to the photocleavable 4AAMP ligand for the preparation of the hydrogel. Irradiation with green light at 529 nm leads to photodegradation of the metallo-hydrogel due to the ligand dissociation, which can be adjusted by adjusting the Ru[(bpy)2(4AAMP)2] concentration. The ligand substitution forming [Ru(bpy)2(L)2]2+ (L = H2O and CH3CN) can be monitored by 1H NMR spectroscopy and UV-visible absorption. The control of degradation by light irradiation plays a significant role in modulating the elasticity and stiffness of the light sensitive metallo-hydrogel network. The photo-responsive hydrogel is a viable substrate for cell cultures.
Additional file 1 of An exploratory assessment of the applicability of direct-to-consumer genetic testing to translational research in Japan
Creators: name: Inoue, Masahiro
name: Arichi, Shota
name: Hachiya, Tsuyoshi
name: Ohtera, Anna
name: Kim, Seok-Won
name: Yu, Eric
name: Nishimura, Masatoshi
name: Shiosakai, Kazuhito
name: Ohira, Takeshi
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Method details for this study and supplementary Table 1, 2, 3 and 4, and supporting figure S1, S2, S3 and S4.
Kolleck, Alma: Politische Diskurse online. Einflussfaktoren auf die Qualität der kollektiven Meinungsbildung in internetgestützten Beteiligungsverfahren, Nomos, Baden-Baden 2017
Creators: name: Witt, Theresa
Publisher: name: Zeitschrift für Parteienwissenschaften
Year: 2018

description: Zeitschrift für Parteienwissenschaften, Nr. 1 (2018): Mitteilungen des Instituts für Deutsches und Internationales Parteienrecht und Parteienforschung
Prospects of cold dark matter searches with an ultra-low-energy germanium detector
Creators: name: Wong, H. T.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The report describes the research program on the development of ultra-low-energy germanium detectors, with emphasis on WIMP dark matter searches. A threshold of 100 eV is achieved with a 20 g detector array, providing a unique probe to the low-mas WIMP. Present data at a surface laboratory is expected to give rise to comparable sensitivities with the existing limits at the $\rm{5 - 10 GeV}$ WIMP-mass range. The projected parameter space to be probed with a full-scale, kilogram mass-range experiment is presented. Such a detector would also allow the studies of neutrino-nucleus coherent scattering and neutrino magnetic moments.
description: 3 pages, 4 figures, Proceedings of TAUP-2007 Conference
Kepler Object of Interest Network I. First results combining ground and space-based observations of Kepler systems with transit timing variations
Creators: name: von Essen, C.
name: Ofir, A.
name: Dreizler, S.
name: Agol, E.
name: Freudenthal, J.
name: Hernandez, J.
name: Wedemeyer, S.
name: Parkash, V.
name: Deeg, H. J.
name: Hoyer, S.
name: Morris, B. M.
name: Becker, A. C.
name: Sun, L.
name: Gu, S. H.
name: Herrero, E.
name: Tal-Or, L.
name: Poppenhaeger, K.
name: Mallonn, M.
name: Albrecht, S.
name: Khalafinejad, S.
name: Boumis, P.
name: Delgado-Correal, C.
name: Fabrycky, D. C.
name: Janulis, R.
name: Lalitha, S.
name: Liakos, A.
name: Mikolaitis, S.
name: D'Angelo, M. L. Moyano
name: Sokov, E.
name: Pakstiene, E.
name: Popov, A.
name: Krushinsky, V.
name: Ribas, I.
name: S., M. M. Rodriguez
name: Rusov, S.
name: Sokova, I.
name: Tautvaisiene, G.
name: Wang, X.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: During its four years of photometric observations, the Kepler space telescope detected thousands of exoplanets and exoplanet candidates. One of Kepler's greatest heritages has been the confirmation and characterization of hundreds of multi-planet systems via Transit Timing Variations (TTVs). However, there are many interesting candidate systems displaying TTVs on such long time scales that the existing Kepler observations are of insufficient length to confirm and characterize them by means of this technique. To continue with Kepler's unique work we have organized the "Kepler Object of Interest Network" (KOINet). The goals of KOINet are, among others, to complete the TTV curves of systems where Kepler did not cover the interaction timescales well. KOINet has been operational since March, 2014. Here we show some promising first results obtained from analyzing seven primary transits of KOI-0410.01, KOI-0525.01, KOI-0760.01, and KOI-0902.01 in addition to Kepler data, acquired during the first and second observing seasons of KOINet. While carefully choosing the targets we set demanding constraints about timing precision (at least 1 minute) and photometric precision (as good as 1 part per thousand) that were achieved by means of our observing strategies and data analysis techniques. For KOI-0410.01, new transit data revealed a turn-over of its TTVs. We carried out an in-depth study of the system, that is identified in the NASA's Data Validation Report as false positive. Among others, we investigated a gravitationally-bound hierarchical triple star system, and a planet-star system. While the simultaneous transit fitting of ground and space-based data allowed for a planet solution, we could not fully reject the three-star scenario. New data, already scheduled in the upcoming 2018 observing season, will set tighter constraints on the nature of the system.
description: 22 figures
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0529
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: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0529, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0529, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q15945019
description: Provenance: abbaye Saint-Étienne de Dijon