cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Laboratory Space Physics: Investigating the Physics of Space Plasmas in the Laboratory
Creators: name: Howes, Gregory G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Space Physics (physics.space-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Laboratory experiments provide a valuable complement to explore the fundamental physics of space plasmas without the limitations inherent to spacecraft measurements. Specifically, experiments overcome the restriction that spacecraft measurements are made at only one (or a few) points in space, enable greater control of the plasma conditions and applied perturbations, can be reproducible, and are orders of magnitude less expensive than launching spacecraft. Here I highlight key open questions about the physics of space plasmas and identify the aspects of these problems that can potentially be tackled in laboratory experiments. Several past successes in laboratory space physics provide concrete examples of how complementary experiments can contribute to our understanding of physical processes at play in the solar corona, solar wind, planetary magnetospheres, and outer boundary of the heliosphere. I present developments on the horizon of laboratory space physics, identifying velocity space as a key new frontier, highlighting new and enhanced experimental facilities, and showcasing anticipated developments to produce improved diagnostics and innovative analysis methods. A strategy for future laboratory space physics investigations will be outlined, with explicit connections to specific fundamental plasma phenomena of interest.
description: Invited paper from APS DPP 2017 Plenary Review Talk, 30 pages, 489 references
Additional file 7: of Structural and functional characterization of protein–lipid interactions of the Salmonella typhimurium melibiose transporter MelB
Creators: name: Hariharan, Parameswaran
name: Tikhonova, Elena
name: Medeiros-Silva, João
name: Jeucken, Aike
name: Bogdanov, Mikhail
name: Dowhan, William
name: Brouwers, Jos
name: Weingarth, Markus
name: Guan, Lan
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: 60506 Virology
subject: FOS: Biological sciences

description: Figure S7. Lipid analyses by TLC. Lipids were extracted from purified MelBSt proteins before (100 μg) and after delipidation treatment (400 μg) as described in Methods. 70 μg of E. coli Extract Polar (Avanti Polar lipids INC) and 20 μg of individual lipids in CHCl3 were used as standards and directly spotted on the pre-treated TLC plates. Samples were run using an alkaline solvent system [CHCl3:MeOH: 28% NH4OH:H2O (45:35:1.6:8, v/v/v/v)]. (PDF 714 kb)
Implications of non-universality of soft terms in supersymmetric grand unified theories
Creators: name: Matalliotakis, D.
name: Nilles, H. P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Most discussions of supersymmetric grand unified theories assume universality of the soft supersymmetry breaking terms at the grand scale. We point out that the behaviour of these theories might change significantly in the presence of non--universal soft terms. Particularly in SO(10)--like models with a large value of tan$β$ we observe a decisive change of predictions, allowing the presence of relatively light gauginos as well as small supersymmetric corrections to the b--quark mass. Some results remain rather stable, including the $μ$--$M_{1/2}$ correlation. Models with small tan$β$ seem to be less affected by non--universality which mainly leads to the new possibility of small $m_{0}$ (i.e. the squark and slepton soft mass parameter), excluded in the universal case.
description: 15 pages (Latex) plus 5 figures (uuencoded postscript file). TUM-HEP 201/94
Carebara vidua Sm.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1913
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Carebara
Carebara vidua

description: Carebara vidua Sm. [[male]] (= Carebara dux Sm. [[queen]]).
— J'ai recu « in copula » le C. vidua [[male]]. La [[queen]] est absolument comme dux, le gastre noir, et le [[male]] a le sien ochrace et repond a la description de Smith. Comme les deux fourmis de Smith sont de la meme localite, je crois bien qu'il ne s'agit que d'une seule espece de Carebara.
description: Published as part of Santschi, F., 1913, Glanure de fourmis africaines., pp. 302-314 in Annales de la Societe Entomologique de Belgique 57 on page 5
Additional file 1: of Barrettâ s oESophagus trial 3 (BEST3): study protocol for a randomised controlled trial comparing the Cytosponge-TFF3 test with usual care to facilitate the diagnosis of oesophageal pre-cancer in primary care patients with chronic acid reflux
Creators: name: Offman, Judith
name: Muldrew, Beth
name: OâDonovan, Maria
name: Debiram-Beecham, Irene
name: Pesola, Francesca
name: Kaimi, Irene
name: Smith, Samuel
name: Wilson, Ashley
name: Zohrah Khan
name: Lao-Sirieix, Pierre
name: Benoit Aigret
name: Walter, Fiona
name: Rubin, Greg
name: Morris, Steve
name: Jackson, Christopher
name: Sasieni, Peter
name: Fitzgerald, Rebecca
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Figure S1. Cytospongeâ ˘ information leaflet. This leaflet was designed based on the findings from a qualitative study investigating the acceptability of and information preferences on this test among patients with GERD. A combination of text and visual illustrations was used to provide easily accessible information on the Cytosponge-TFF3 procedure, the link between GERD, BE and EAC, and BEST3. (PDF 669 kb).
No-go theorem for topological insulators and sure-fire recipe for Chern insulators
Creators: name: Alexandradinata, A.
name: Höller, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: For any symmorphic magnetic space group $G$, it is proven that topological band insulators with vanishing first Chern numbers cannot have a groundstate composed of a single, energetically-isolated band. This no-go statement implies that the minimal dimension of tight-binding Hamiltonians for such topological insulators is four if the groundstate is stable to addition of trivial bands, and three if the groundstate is unstable. A sure-fire recipe is provided to design models for Chern and unstable topological insulators by splitting elementary band representations; this recipe, combined with recently-constructed Bilbao tables on such representations, can be systematized for mass identification of topological materials. All results follow from our theorem which applies to any single, isolated energy band of a $G$-symmetric Schrödinger-type or tight-binding Hamiltonian: for such bands, being topologically trivial is equivalent to being a band representation of $G$.
description: 8 pages main text + 3 pages appendix, 1 figure
LifeLearner: Hardware-Aware Meta Continual Learning System for Embedded Computing Platforms
Creators: name: Kwon, YD
name: Chauhan, J
name: Jia, H
name: Venieris, SI
name: Mascolo, C
Publisher: name: ACM
Year: 2023
Subjects: Continual Learning
Edge Computing
Latent Replay
Meta Learning
Microcontrollers
On-device Training
Product Quantization

description: Continual Learning (CL) allows applications such as user personalization and household robots to learn on the fly and adapt to context. This is an important feature when context, actions, and users change. However, enabling CL on resource-constrained embedded systems is challenging due to the limited labeled data, memory, and computing capacity. In this paper, we propose LifeLearner, a hardware-aware meta continual learning system that drastically optimizes system resources (lower memory, latency, energy consumption) while ensuring high accuracy. Specifically, we (1) exploit meta-learning and rehearsal strategies to explicitly cope with data scarcity issues and ensure high accuracy, (2) effectively combine lossless and lossy compression to significantly reduce the resource requirements of CL and rehearsal samples, and (3) developed hardware-aware system on embedded and IoT platforms considering the hardware characteristics. As a result, LifeLearner achieves near-optimal CL performance, falling short by only 2.8% on accuracy compared to an Oracle baseline. With respect to the state-of-the-art (SOTA) Meta CL method, LifeLearner drastically reduces the memory footprint (by 178.7x), end-to-end latency by 80.8-94.2%, and energy consumption by 80.9-94.2%. In addition, we successfully deployed LifeLearner on two edge devices and a microcontroller unit, thereby enabling efficient CL on resource-constrained platforms where it would be impractical to run SOTA methods and the far-reaching deployment of adaptable CL in a ubiquitous manner. Code is available at https://github.com/theyoungkwon/LifeLearner
title: ADCO, Cart. 186 (11 H 71), f. 0021v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

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. 0021v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-
project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 1 of Mitochondrial impairment and downregulation of Drp1 phosphorylation underlie the antiproliferative and proapoptotic effects of alantolactone on oral squamous cell carcinoma cells
Creators: name: Zhang, Yafei
name: Yang, Bingqian
name: Tu, Chengwei
name: Ping, Yifan
name: Chen, Shuhong
name: Wu, Tong
name: Zhao, Zheyu
name: Mao, Yixin
name: Yang, Zhan
name: Cao, Zelin
name: Li, Jianmin
name: Huang, Kate
name: Ding, Xi
name: Wu, Gang
name: Zou, Peng
name: Deng, Zhennan
name: Sun, Xiaoyu
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Figure S1. Statistical analysis of the level of mitochondrial proteins in OSCC cancer tissues.The corresponding statistical analysis of P-Drp1/GAPDH.The statistical analysis of Drp1/GAPDH.The statistical analysis of P-Drp1/Drp1.The statistical analysis of TOM20/GAPDH.The statistical analysis of VDAC1/GAPDH.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1010051
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Châtelet
subject: registre
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1010051
Quantum Phenomenology for the Disoriented Chiral Condensate
Creators: name: Amado, R. D.
name: Kogan, Ian I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the quantum state describing theDisoriented Chiral Condensate (DCC), which may be produced in high energy collisions. We show how a mean field treatment of the quantum equations corresponding to the classical linear sigma model leads to a squeezed state description of the pions emerging from the DCC. We examine various squeezed and coherent state descriptions of those pions with particular attention to charge and number fluctuations. We also study the phenomenology of multiple DCC domains.
description: 24 pages, PUPT-1483
Long-distance near-field energy transport via propagating surface waves
Creators: name: Dong, Jian
name: Zhao, Junming
name: Liu, Linhua
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Near-field radiative heat transfer (RHT) between two bodies can significantly exceed the far-field limit set by Planck's law due to the evanescent wave tunneling, which typically can only occur when the two bodies are separated at subwavelength distances. We show that the RHT between two SiC nanoparticles with separation distances much larger than the thermal wavelength can still exceed the far-field limit when the particles are located within a subwavelength distance away from a SiC substrate. In this configuration, the localized surface phonon polariton (SPhP) of the particles couples to the propagating SPhP of the substrate which then provides a new channel for the near-field energy transport and enhances the RHT by orders of magnitude at large distances. The enhancement is also demonstrated to appear in a chain of closely spaced SiC nanoparticles located in the near field of a SiC substrate. The findings provide a new way for the long-distance transport of near-field energy.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000781
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Châtelet
subject: registre
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000781
Phenomenology of the Minimal Supergravity SU(5) Model
Creators: name: Drees, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The minimal grand unified supergravity model is discussed. Requiring radiative breaking of the electroweak gauge symmetry, the unification of b and tau Yukawa couplings, a sufficiently stable nucleon, and not too large a relic density of neutralinos produced in the Big Bang constrains the parameter space significantly. In particular, the soft breaking parameter m_1/2 has to be less than about 130 GeV, and the top quark Yukawa coupling has to be near its (quasi) fixed point. The former condition implies m_gluino < 400 GeV and hence very large production rates for gluino pairs at the LHC, while the latter constraint implies that the lighter stop and sbottom eigenstates are significantly lighter than the other squarks, leading to characteristic signatures for gluino pair events.
description: based on a talk presented at the 3rd Workshop on High Energy Particle Physics, Madras, India, January 1994; 23 pages in LaTeX with EQUATION.STY, 3 figures not included (available on request); MAD/PH/843
Carebara ampla Santschi
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1913
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Carebara
Carebara ampla

description: Carebara ampla Santschi.
— Differe de junodi Forel par la couleur du gastre qui est brun fonce chez junodi et jaune ocre assez- clair chez ampla. La tete et le thorax de cette derniere sont bien plus larges que chez junodi. C'est probablement une simple race, mais il faudrait connaitre la [[worker]] de ampla et comparer l'armure genitale des [[male]]. Je ne connais pas encore celui de junodi.
description: Published as part of Santschi, F., 1913, Glanure de fourmis africaines., pp. 302-314 in Annales de la Societe Entomologique de Belgique 57 on page 6
General Non-Commutative Locally Compact Locally Hausdorff Stone Duality
Creators: name: Bice, Tristan
name: Starling, Charles
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: General Topology (math.GN)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics
subject: 03C65, 06E15, 06E75, 06B35, 54D45, 54D70, 54D80

description: We extend the classical Stone duality between zero dimensional compact Hausdorff spaces and Boolean algebras. Specifically, we simultaneously remove the zero dimensionality restriction and extend to étale groupoids, obtaining a duality with an elementary class of inverse semigroups.
description: minor corrections/modifications
Additional file 1 of The role of angiotensin I-converting enzyme gene polymorphism and global DNA methylation in the negative associations between urine di-(2-ethylhexyl) phthalate metabolites and serum adiponectin in a young Taiwanese population
Creators: name: Lin, Chien-Yu
name: Lee, Hui-Ling
name: Chen, Ching-Way
name: Wang, Chikang
name: Sung, Fung-Chang
name: Su, Ta-Chen
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Additional file 1. Materials and Methods and Tables.
Additional file 1: of Serum metabolomic profiling predicts synovial gene expression in rheumatoid arthritis
Creators: name: Narasimhan, Rekha
name: Coras, Roxana
name: Rosenthal, Sara
name: Sweeney, Shannon
name: Lodi, Alessia
name: Tiziani, Stefano
name: Boyle, David
name: Kavanaugh, Arthur
name: Guma, Monica
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine

description: Table S1. Baseline clinical characteristics of patients with rheumatoid arthritis. Table S2. Mean and standard deviation (SD) of synovial biomarker expression. Table S3. Mean and standard deviation (SD) of serum metabolites detected by 1H-NMR (ÎźM). Reference values are from the Human Metabolome Database (HMDB) and were collected via NMR, unless otherwise noted. 1GC/MS; 2HPLC; 3HPLC-fluoroescence; 4ion-exchange chromatography; 5DFI/MS/MS 6unknown. ND, no data available. Metabolites that were upregulated by at least 20% compared to reference values are in green. Metabolites that were downregulated by more than 20% compared to reference values are in red. (DOCX 26 kb)
Are superflares on solar analogues caused by extra-solar planets?
Creators: name: Rubenstein, Eric P.
name: Schaefer, Bradley E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Stellar flares with ${10^2-10^7}$ times more energy than the largest solar flare have been detected from 9 normal F and G main sequence stars (Schaefer, King & Deliyannis 1999). These superflares have durations of hours to days and are visible from at least x-ray to optical frequencies. The absence of world-spanning aurorae in historical records and of anomalous extinctions in the geological record indicate that our Sun likely does not suffer superflares. In seeking to explain this new phenomenon, we are struck by its similarity to large stellar flares on RS Canum Venaticorum binary systems, which are caused by magnetic reconnection events associated with the tangling of magnetic fields between the two stars. The superflare stars are certainly not of this class, although we propose a similar flare mechanism. That is, superflares are caused by magnetic reconnection between fields of the primary star and a close-in Jovian planet. Thus, by only invoking known planetary properties and reconnection scenarios, we can explain the energies, durations, and spectra of superflares, as well as explain why our Sun does not have such events.
description: 13 pages, Accepted for publication in ApJ
title: 02_0304
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Magnetic Inflation and Stellar Mass II: On the Radii of Single, Rapidly Rotating, Fully Convective M Dwarf Stars
Creators: name: Kesseli, Aurora Y.
name: Muirhead, Philip S.
name: Mann, Andrew W.
name: Mace, Greg
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Main sequence, fully-convective M dwarfs in eclipsing binaries are observed to be larger than stellar evolutionary models predict by as much as $10-15\%$. A proposed explanation for this discrepancy involves effects from strong magnetic fields, induced by rapid-rotation via the dynamo process. Although, a handful of single, slowly-rotating M dwarfs with radius measurements from interferometry also appear to be larger than models predict, suggesting that rotation or binarity specifically may not be the sole cause of the discrepancy. We test whether single, rapidly rotating, fully convective stars are also larger than expected by measuring their $R \sin i$ distribution. We combine photometric rotation periods from the literature with rotational broadening ($v \sin i$) measurements reported in this work for a sample of 88 rapidly rotating M dwarf stars. Using a Bayesian framework, we find that stellar evolutionary models underestimate the radii by $10-15\% \substack{+3 \\ -2.5}$, but that at higher masses ($0.18
description: Accepted to AJ
Additional file 1: of Palliative care for patients with a substance use disorder and multiple problems: a study protocol
Creators: name: Ebenau, Anne
name: Dijkstra, Boukje
name: Stal-Klapwijk, Marianne
name: Huurne, Chantal Ter
name: Blom, Ans
name: Vissers, Kris
name: Groot, Marieke
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Case Study SUD+. (DOC 27 kb)
Maximal $CP$ violation in the Higgs Sector and its Effect on the $ρ$ Parameter
Creators: name: Joshi, Grish C.
name: Matsuda, Masahisa
name: Tanimoto, Morimitsu
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the conditions of maximal $CP$ violation in the neutral Higgs mass matrix of the two Higgs doublet model. We get fixed values of $\tan\b$ and constraints on the Higgs potential parameters. Two neutral Higgs scalars are constrained to be lighter than the charged Higgs scalar and these two Higgs scalars are expected to be almost degenerate due to the smallness of the $h$ parameter, where $h$ is the CP violating coupling constant of the Higgs interaction. The radiative correction of the $ρ$ parameter from the Higgs scalar exchange is rather small and its sign negative for a wide range of Higgs masses. It follows that maximum $CP$ violation in the two Higgs doublet model is safely allowed for the $ρ$ parameter without the custodial symmetry.
description: 13-pages including 2-figures(figures will be sent by fax or postal mail if request), UWThPh-1994-25, AUE-94-04
Additional file 3 of Genome-wide analysis of ATP-binding cassette transporter provides insight to genes related to bioactive metabolite transportation in Salvia miltiorrhiza
Creators: name: Yan, Li
name: Zhang, Jianhong
name: Chen, Hongyu
name: Luo, Hongmei
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Figure S2. qRT-PCR validation of the 18 selected candidate transporter genes involved in bioactive compound transportation in S. miltiorrhiza. SmActin was used as an internal control. Each gene has three biological replicates and three technical replicates
The emission and distribution of dust of the torus of NGC 1068
Creators: name: Lopez-Rodriguez, Enrique
name: Fuller, Lindsay
name: Alonso-Herrero, Almudena
name: Efstathiou, Andreas
name: Ichikawa, Kohei
name: Levenson, Nancy A.
name: Packham, Chris
name: Radomski, James
name: Almeida, Cristina Ramos
name: Benford, Dominic J.
name: Berthoud, Marc
name: Hamilton, Ryan
name: Harper, Doyal
name: Kovavcs, Attila
name: Santos, Fabio P.
name: Staguhn, J.
name: Herter, Terry
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present observations of NGC 1068 covering the $19.7-53.0$ $μ$m wavelength range using FORCAST and HAWC+ onboard SOFIA. Using these observations, high-angular resolution infrared (IR) and sub-mm observations, we find an observational turn-over of the torus emission in the $30-40$ $μ$m wavelength range with a characteristic temperature of $70-100$ K. This component is clearly different from the diffuse extended emission in the narrow line and star formation regions at 10-100 $μ$m within the central 700 pc. We compute $2.2-432$ $μ$m 2D images using the best inferred \textsc{clumpy} torus model based on several nuclear spectral energy distribution (SED) coverages. We find that when $1-20$ $μ$m SED is used, the inferred result gives a small torus size ($<4$ pc radius) and a steep radial dust distribution. The computed torus using the $1-432$ $μ$m SED provides comparable torus sizes, $5.1^{+0.4}_{-0.4}$ pc radius, and morphology to the recently resolved 432 $μ$m ALMA observations. This result indicates that the $1-20$ $μ$m wavelength range is not able to probe the full extent of the torus. The characterization of the turn-over emission of the torus using the $30-60$ $μ$m wavelength range is sensitive to the detection of cold dust in the torus. The morphology of the dust emission in our 2D image at 432 $μ$m is spatially coincident with the cloud distribution, while the morphology of the emission in the $1-20$ $μ$m wavelength range shows an elongated morphology perpendicular to the cloud distribution. We find that our 2D \textsc{clumpy} torus image at 12 $μ$m can produce comparable results to those observed using IR interferometry.
description: 12 pages, 7 Figures, Accepted for publication in ApJ
Additional file 1: of Splenic involvement in umbilical cord matrix-derived mesenchymal stromal cell-mediated effects following traumatic spinal cord injury
Creators: name: Badner, Anna
name: Hacker, Justin
name: Hong, James
name: Mirriam Mikhail
name: Reaz Vawda
name: Fehlings, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Computational Biology

description: Figure S1. Spleen weight and length following traumatic SCI. There was no significant difference in spleen weight (A) or length (B) at 1 or 24 h following SCI. Data are expressed as mean ± SEM (n = 4 per group), one-way ANOVA with Tukey’s multiple comparisons test. (PDF 354 kb)
A Cranial-Feature-Based Registration Scheme for Robotic Micromanipulation Using a Microscopic Stereo Camera System
Creators: name: Lin, Xiaofeng
name: Pérez, Saúl Alexis Heredia
name: Harada, Kanako
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Biological specimens exhibit significant variations in size and shape, challenging autonomous robotic manipulation. We focus on the mouse skull window creation task to illustrate these challenges. The study introduces a microscopic stereo camera system (MSCS) enhanced by the linear model for depth perception. Alongside this, a precise registration scheme is developed for the partially exposed mouse cranial surface, employing a CNN-based constrained and colorized registration strategy. These methods are integrated with the MSCS for robotic micromanipulation tasks. The MSCS demonstrated a high precision of 0.10 mm $\pm$ 0.02 mm measured in a step height experiment and real-time performance of 30 FPS in 3D reconstruction. The registration scheme proved its precision, with a translational error of 1.13 mm $\pm$ 0.31 mm and a rotational error of 3.38$^{\circ}$ $\pm$ 0.89$^{\circ}$ tested on 105 continuous frames with an average speed of 1.60 FPS. This study presents the application of a MSCS and a novel registration scheme in enhancing the precision and accuracy of robotic micromanipulation in scientific and surgical settings. The innovations presented here offer automation methodology in handling the challenges of microscopic manipulation, paving the way for more accurate, efficient, and less invasive procedures in various fields of microsurgery and scientific research.
description: Accepted by Advanced Robotics, Vol. 38, Issue 21
Superflares on Ordinary Solar-Type Stars
Creators: name: Schaefer, Bradley E.
name: King, Jeremy R.
name: Deliyannis, Constantine P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Short duration flares are well known to occur on cool main-sequence stars as well as on many types of `exotic' stars. Ordinary main-sequence stars are usually pictured as being static on time scales of millions or billions of years. Our sun has occasional flares involving up to $\sim 10^{31}$ ergs which produce optical brightenings too small in amplitude to be detected in disk-integrated brightness. However, we identify nine cases of superflares involving $10^{33}$ to $10^{38}$ ergs on normal solar-type stars. That is, these stars are on or near the main-sequence, are of spectral class from F8 to G8, are single (or in very wide binaries), are not rapid rotators, and are not exceedingly young in age. This class of stars includes many those recently discovered to have planets as well as our own Sun, and the consequences for any life on surrounding planets could be profound. For the case of the Sun, historical records suggest that no superflares have occurred in the last two millennia.
description: 16 pages, accepted for publication in ApJ
The Maximum Stellar Surface Density Due to the Failure of Stellar Feedback
Creators: name: Grudić, Michael Y.
name: Hopkins, Philip F.
name: Quataert, Eliot
name: Murray, Norman
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A maximum stellar surface density $Σ_{max} \sim 3 \times 10^5\,{\rm M_\odot\,pc^{-2}}$ is observed across all classes of dense stellar systems (e.g. star clusters, galactic nuclei, etc.), spanning $\sim 8$ orders of magnitude in mass. It has been proposed that this characteristic scale is set by some dynamical feedback mechanism preventing collapse beyond a certain surface density. However, simple analytic models and detailed simulations of star formation moderated by feedback from massive stars argue that feedback becomes {\it less} efficient at higher surface densities (with the star formation efficiency increasing as $\sim Σ/Σ_{crit}$). We therefore propose an alternative model wherein stellar feedback becomes ineffective at moderating star formation above some $Σ_{crit}$, so the supply of star-forming gas is rapidly converted to stars before the system can contract to higher surface density. We show that such a model -- with $Σ_{crit}$ taken directly from the theory -- naturally predicts the observed $Σ_{max}$. $Σ_{max}\sim 100Σ_{crit}$ because the gas consumption time is longer than the global freefall time even when feedback is ineffective. Moreover the predicted $Σ_{max}$ is robust to spatial scale and metallicity, and is preserved even if multiple episodes of star formation/gas inflow occur. In this context, the observed $Σ_{max}$ directly tells us where feedback fails.
description: 5 pages, 5 figures. Submitted to MNRAS. Comments welcome!
Cataulacus weissi Santschi, 1913, n. sp.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1913
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Cataulacus
Cataulacus weissi

description: Cataulacus weissi n. sp.
- [[worker]]. Long. 3.1 mill. — Noir. Scape, genoux, tibias et tarses testaces. " ' Mandibules et funicule brunatres. Un peu luisant. Tete lachement ridee reticulee, avec le fond distinctement ponctue (rides plus irregulieres et plus larges que chez C. jeanneli Sants.) Elles sont plus fortes, au contraire, sur le dos du thorax. A partir des deux tiers posterieurs du thorax les rides prennent une direction franchement longitudinals, il en est de meme sur le 2 ° article du pedicule, tandis que sur le 1 er elles deviennent concentriques en arriere. Gastre reticule ponctue comme du reste toute la sculpture fondamentale.
Pilosite dressee assez longue, epaisse et tronquee, abondante partout, presque aussi longue et abondante que chez C. erinaceus Stitz, mais un peu moins redressee.
Tete un sixieme plus longue que large, tres peu retrecie en avant avec le bord posterieur droit et les angles peu arrondis et denticules. Cotes de la tete legerement convexes, denticules en arriere des yeux et bidentes en avant. Yeux aussi larges que l'espace qui les separe de l'angle anterieur de la tete, le bord anterieur des yeux divise par l'arete antennaire de facon que la portion externe regarde en dessous dans le scrobe. Aretes antennaires non echan-crees, faiblement convexes, aussi longues que la largeur de l'epistome. Thorax un peu moins large que la tete, sans sutures, a bord denticule, presque deux fois aussi long que large. Sur le profil il est convexe en avant et legerement concave en arriere. Le mesonotum se retrecit assez fortement. Le pronotum legerement plus etroit en avant qu'en arriere. Epines de l'epinotum horizontales, divergentes et longues comme les deux tiers de l'intervalle de leur extremite. Premier n oe ud un peu plus long que large, plus large en avant, assez arrondi en arriere. Deuxieme n oe ud distinctement plus large que le precedent mais un tiers plus court, bien plus large en avant qu'en arriere, avec les angles anterieurs bien marques. Le dessous des deux n oe uds pourvu d'un processus comprime, assez long, bifide sous le premier article. Gastre assez allonge, bien plus large que le thorax, a cotes legerement convexes, plus largement echancre en avant que la largeur du deuxieme n oe ud.
Differe de pygmaeus Andre par sa tete plus longue et sa taille plus grande et de Jeanneli Santschi par sa sculpture et sa pilosite.
Congo francais: Brazaville (A. Weis 1907). J'avais confondu cette forme avec la pygmaeus.
description: Published as part of Santschi, F., 1913, Glanure de fourmis africaines., pp. 302-314 in Annales de la Societe Entomologique de Belgique 57 on pages 9-10
Additional file 6: of Structural and functional characterization of proteinâ lipid interactions of the Salmonella typhimurium melibiose transporter MelB
Creators: name: Hariharan, Parameswaran
name: Tikhonova, Elena
name: JoĂŁo Medeiros-Silva
name: Jeucken, Aike
name: Bogdanov, Mikhail
name: Dowhan, William
name: Brouwers, Jos
name: Weingarth, Markus
name: Guan, Lan
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology

description: Figure S6. Identification of lipid species associated with purified MelBSt by HPLC-MS. Lipids extraction for HPLC-MS analyses and MelBSt delipidation treatment were carried out as described in Methods. (a). A typical base peak chromatogram of the separation of phospholipids co-purified with MelBSt protein. PG, CL, and PE peaks, as well as detergent UDM, are indicated. (b and c). PE and PG spectra before and after delipidation of MelBSt. (PDF 990 kb)
The Spin Structure of the Proton in a Non-relativistic Quark Model
Creators: name: Keppler, J.
name: Hofmann, H. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The spin structure of the proton is investigated in the framework of an extended quark potential model which in addition to the conventional $3q$--structure also takes into account $(3q)(q\bar q)$--admixtures in the proton wave function. For reasons of parity such admixtures contain an odd orbital angular momentum thus allowing the proton spin to be shared among quark spins and orbital angular momenta. We show that only certain admixtures are suited for a significant reduction of the quark spin content of the proton as suggested by the EMC--result. Within a Hamiltonian model quark spin contributions to the proton spin down to $0.5$ can be reproduced easily.
description: email: keppler@faupt31.physik.uni-erlangen.de, 9 pages REVTEX, 1 figure added as PostScript-file which should be stripped off before texing
The PSCz catalogue
Creators: name: Saunders, Will
name: Oliver, Seb
name: Keeble, Oliver
name: Rowan-Robinson, Michael
name: Maddox, Steve
name: McMahon, Richard
name: Efstathiou, George
name: Sutherland, Will
name: Tadros, Helen
name: White, Simon
name: Frenk, Carlos
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the catalogue and redshift data for the PSCz survey of 15,000 IRAS galaxies over 84% of the sky. The uniformity, completeness and data quality are assessed, and guidelines and caveats for its use are given.
description: 4 pages, 1 figure. To be published in 'Towards an Understanding of Cosmic Flows of Large-Scale Structure', Victoria, July 1999, eds Courteau,S., Strauss,M., Willick,J., PASP
Additional file 1 of Analysis of enterovirus genotypes in the cerebrospinal fluid of children associated with aseptic meningitis in Liaocheng, China, from 2018 to 2019
Creators: name: Wang, Jing
name: Meng, Min
name: Xu, Huan
name: Wang, Ting
name: Liu, Ying
name: Yan, Han
name: Liu, Peiman
name: Qin, Daogang
name: Yang, Qiaozhi
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. The sequences of EVs in this study.
On Quantum Nature of Black-Hole Spacetime: A Possible New Source of Intense Radiation
Creators: name: Ahluwalia, D. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Atoms and the planets acquire their stability from the quantum mechanical incompatibility of the position and momentum measurements. This incompatibility is expressed by the fundamental commutator [x, p_x]=i hbar, or equivalently, via the Heisenberg's uncertainty principle Delta x Delta p_x sim hbar. A further stability-related phenomenon where the quantum realm plays a dramatic role is the collapse of certain stars into white dwarfs and neutron stars. Here, an intervention of the Pauli exclusion principle, via the fermionic degenerate pressure, stops the gravitational collapse. However, by the neutron-star stage the standard quantum realm runs dry. One is left with the problematic collapse of a black hole. This essay is devoted to a concrete argument on why the black-hole spacetime itself should exhibit a quantum nature. The proposed quantum aspect of spacetime is shown to prevent the general-relativistic dictated problematic collapse. The quantum nature of black-hole spacetime is deciphered from a recent result on the universal equal-area spacing [=lambda_P^2 4 ln(3)] for black holes. In one interpretation of the emergent picture, an astrophysical black hole can fluctuate to sqrt{pi/ln(3)} approx 1.7 times its classical size, and thus allow radiation and matter to escape to the outside observers. These fluctuations I conjecture provide a new source, perhaps beyond Hawking radiation, of intense radiation from astrophysical black holes and may be the primary source of observed radiation from those galactic cores what carry black hole(s). The presented interpretation may be used as a criterion to choose black holes from black hole candidates.
description: This essay received an "honorable mention" in the 1999 Essay Competition of the Gravity Research Foundation - Ed. Int. J. Mod. Phys. D (1999, in press). For Joseph Knecht
Dicroapsis emeryi For.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1913
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Dicroapsis
Dicroapsis emeryi

description: Dicroapsis emeryi For.
— [[queen]] Long. 3 mill. — Couleur et sculpture de l´[[worker]]. Les poils en massue sont plus allonges sur le gastre et plus redresses sur le dos du thorax. Sous la tete se voient des poils ordinaires. Le scutellum, du double plus large que long, surplombe en arriere le devant de l'epinotum. La face basale est distinctement plus courte que la face declive. Les n oe uds plus larges que chez l'ouvriere, le 1 er presque trois fois aussi large que long. Le gastre plus long que chez l'ouvriere.
[[queen]] [[worker]] Abyssinie: Harrar. Recues de M. Reichensperger.
description: Published as part of Santschi, F., 1913, Glanure de fourmis africaines., pp. 302-314 in Annales de la Societe Entomologique de Belgique 57 on page 10
A high-efficiency gas target setup for underground experiments, and redetermination of the branching ratio of the 189.5 keV $\mathbf{^{22}Ne(p,γ)^{23}Na}$ resonance
Creators: name: Ferraro, F.
name: Takács, M. P.
name: Piatti, D.
name: Mossa, V.
name: Aliotta, M.
name: Bemmerer, D.
name: Best, A.
name: Boeltzig, A.
name: Broggini, C.
name: Bruno, C. G.
name: Caciolli, A.
name: Cavanna, F.
name: Chillery, T.
name: Ciani, G. F.
name: Corvisiero, P.
name: Csedreki, L.
name: Davinson, T.
name: Depalo, R.
name: D'Erasmo, G.
name: Di Leva, A.
name: Elekes, Z.
name: Fiore, E. M.
name: Formicola, A.
name: Fülöp, Zs.
name: Gervino, G.
name: Guglielmetti, A.
name: Gustavino, C.
name: Gyürky, Gy.
name: Imbriani, G.
name: Junker, M.
name: Kochanek, I.
name: Lugaro, M.
name: Marcucci, L. E.
name: Marigo, P.
name: Menegazzo, R.
name: Pantaleo, F. R.
name: Paticchio, V.
name: Perrino, R.
name: Prati, P.
name: Schiavulli, L.
name: Stöckel, K.
name: Straniero, O.
name: Szücs, T.
name: Trezzi, D.
name: Zavatarelli, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The experimental study of nuclear reactions of astrophysical interest is greatly facilitated by a low-background, high-luminosity setup. The Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator offers ultra-low cosmic-ray induced background due to its location deep underground in the Gran Sasso National Laboratory (INFN-LNGS), Italy, and high intensity, 250-500 $μ$A, proton and $α$ ion beams. In order to fully exploit these features, a high-purity, recirculating gas target system for isotopically enriched gases is coupled to a high-efficiency, six-fold optically segmented bismuth germanate (BGO) $γ$-ray detector. The beam intensity is measured with a beam calorimeter with constant temperature gradient. Pressure and temperature measurements have been carried out at several positions along the beam path, and the resultant gas density profile has been determined. Calibrated $γ$-intensity standards and the well-known $E_p$ = 278 keV $\mathrm{^{14}N(p,γ)^{15}O}$ resonance were used to determine the $γ$-ray detection efficiency and to validate the simulation of the target and detector setup. As an example, the recently measured resonance at $E_p$ = 189.5 keV in the $^{22}$Ne(p,$γ$)$^{23}$Na reaction has been investigated with high statistics, and the $γ$-decay branching ratios of the resonance have been determined.
description: 11 pages, 11 figures, accepted in Eur. Phys. Journal A
Phenomenology of a non-standard top quark Yukawa coupling
Creators: name: Zhang, X.
name: Lee, S. K.
name: Whisnant, K.
name: Young, B. -L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: There are theoretical speculations that the top quark may have different properties from that predicted by the standard model. We use an effective Lagrangian technique to model such a non-standard top quark scenario and study its effects on the electroweak baryogenesis, low and high energy physics.
description: (TeX file, Figures available by request) AMES-HET 94-05, June 1994