cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: College Enhancement Strategies and Socioeconomic Inequality
Creators: name: Wolniak, Gregory C.
name: Wells, Ryan S.
name: Engberg, Mark E.
name: Manly, Catherine A.
Publisher: name: University of Massachusetts Amherst
Year: 2016
Subjects: subject: Higher Education

description: For published version, please consult: Wolniak, G. C., Wells, R. S., Engberg, M. E., & Manly, C. A. (2016). College enhancement strategies and socioeconomic inequality. Research in Higher Education, 57(3), 310-334. Retrieved from https://doi.org/10.1007/s11162-015-9389-4
description: The study provides new information on the relationships between students’ socioeconomic backgrounds, utilization of college enhancement strategies, and subsequent 4-year college enrollment. Enhancement strategies represent student behaviors used to bolster the competitiveness of a college application, such as Advanced Placement exams and a variety of extracurricular activities. By drawing on two national datasets that span the 1990s (NELS) and the 2000s (ELS), the study uncovers how these relationships have changed during a period marked by escalating demand for college and growing class inequality. The findings provide partial evidence of class adaptation (Alon in Am Soc Rev 74:731–755, 2009) based on the combination of increased use of multiple enhancement strategies (“high overall use”) among higher SES students and increased influence of high overall enhancement strategy use in predicting college enrollment, particularly selective college enrollment. Implications are discussed in terms of the higher education system and pervasive social inequality.
Surveys of Economic Results in Agriculture: Demand and Prices
Creators: name: Foote, Richard J.
Publisher: name: Unknown
Year: 1954
Subjects: Demand and Price Analysis
Research Methods/ Statistical Methods

description: Further Experiments with the Simultaneous-equations Approach --- Introduction of Dynamic Elements into Least-square Analyses --- Analyses Based on Data from Consumer Panels or Sales from Retail Stores --- Use of Spatial-Equilibrium Analyses to Study Export Demand --- Demand and Price Structure Research in AMS.
Google matrix of Bitcoin network
Creators: name: Ermann, Leonardo
name: Frahm, Klaus M.
name: Shepelyansky, Dima L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Social and Information Networks (cs.SI)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We construct and study the Google matrix of Bitcoin transactions during the time period from the very beginning in 2009 till April 2013. The Bitcoin network has up to a few millions of bitcoin users and we present its main characteristics including the PageRank and CheiRank probability distributions, the spectrum of eigenvalues of Google matrix and related eigenvectors. We find that the spectrum has an unusual circle-type structure which we attribute to existing hidden communities of nodes linked between their members. We show that the Gini coefficient of the transactions for the whole period is close to unity showing that the main part of wealth of the network is captured by a small fraction of users.
description: 12 pages, 15 figures
title: ADCO, Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Cart. 176 (11 H 8), f. 0099
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/2017
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: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0099, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0099, 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 The impact of HCV co-infection status on healthcare-related utilization among people living with HIV in British Columbia, Canada: a retrospective cohort study
Creators: name: Huiting Ma
name: Villalobos, Conrado
name: St-Jean, Martin
name: Oghenowede Eyawo
name: Lavergne, Miriam
name: Lianping Ti
name: Hull, Mark
name: Yip, Benita
name: Wu, Lang
name: Hogg, Robert
name: Barrios, Rolando
name: Shoveller, Jean
name: Montaner, Julio
name: Lima, Viviane
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Supplementary information detailing the data linkage within the STOP HIV/AIDS cohort, the ascertainment of comorbidities based on the Charlson Comorbidity Index, and the number of healthcare-related visits recorded. (DOCX 35 kb)
GRB 050509B: Constraints on short gamma-ray burst models
Creators: name: Hjorth, J.
name: Sollerman, J.
name: Gorosabel, J.
name: Granot, J.
name: Klose, S.
name: Kouveliotou, C.
name: Melinder, J.
name: Ramirez-Ruiz, E.
name: Starling, R.
name: Thomsen, B.
name: Andersen, M. I.
name: Fynbo, J. P. U.
name: Jensen, B. L.
name: Vreeswijk, P. M.
name: Cerón, J. M. Castro
name: Jakobsson, P.
name: Levan, A.
name: Pedersen, K.
name: Rhoads, J. E.
name: Tanvir, N. R.
name: Watson, D.
name: Wijers, R. A. M. J.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained deep optical images with the Very Large Telescope at ESO of the first well-localized short-duration gamma-ray burst, GRB 050509B. From V and R imaging, initiated ~2 days after the GRB trigger and lasting up to three weeks, we detect no variable object inside the small Swift/XRT X-ray error circle down to 2sigma limits of V = 26.5 and R = 25.1. The X-ray error circle includes a giant elliptical galaxy at z = 0.225, which has been proposed as the likely host of this GRB. Our limits indicate that if the GRB originated at z = 0.225, any supernova-like event accompanying the GRB would have to be over 100 times fainter than normal Type Ia SNe or Type Ic hypernovae, 5 times fainter than the faintest known Ia or Ic SNe, and fainter than the faintest known Type II SNe. Moreover, we use the optical limits to constrain the energetics of the GRB outflow. Simple models indicate that, unless the intrinsic energy in the outflow from GRB 050509B was << 10^51 erg, there was very little radioactive material with efficient decay timescales for generating a large luminosity. These limits strongly constrain progenitor models for this short GRB.
description: 13 pages, 2 figures, ApJL, in press
title: Coin Recovery II
Creators: name: Lofthouse, Carly
Publisher: name: Utah State University
Year: 2020

description: Western Metals Recycling (WMR), a subsidiary of NUCOR Steel, is a metals recycling company with a location in Plymouth, Utah. At Plymouth, a 50 NT/hr. non-ferrous recovery plant uses eddy current technology to generate a non-ferrous product called zorba. Zorba is a mix of aluminum, copper, brass, zinc, printed circuit boards, coins, lead, and the like. (Figure 1) The market value of zorba varies but generally ranges from $0.30 to $0.50 per pound. The value of the coins (not including pennies) is much higher than zorba price. The team's objective is to upgrade and optimize the existing trommel equipment to sort the zorba into coin-sized denominations with greater than 90% accuracy.
MOESM3 of Quality of observational studies in prestigious journals of occupational medicine and health based on Strengthening the Reporting of Observational Studies in Epidemiology (STROBE) Statement: a cross-sectional study
Creators: name: Aghazadeh-Attari, Javad
name: Kazhal Mobaraki
name: Ahmadzadeh, Jamal
name: Mansorian, Behnam
name: Mohebbi, Iraj
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 3: Figure S1. Percentages of adequately reported STROBE sub-items in articles published in the top four occupational medicine and health journals.
Lettre de Jean-François Séguier à Gian Franco Maffei (minute), 1778-05-13 (avant)
Creators: name: Séguier, Jean-François
name: Jean-François Séguier
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022
Subjects: Recommandation

description: [fol. 72r] Sig.e Marchese mio Signore

Il Signore Carlo Scipione Le Cointe, gentilissimo Signore e garbatissimo cavaliere di questa città, amico mio carissimo, se ne parte per andare in giro per l’Italia. Non mancherà di portarsi in Verona ; non ho volsuto lasciarlo partire senza una delle mie lettere, e demandarle delle nuove sue e di quelle della signora Marchese alla quale prego di presentare i miei ossequj. Questo signore è molto dilettante di Musica, di vedere le gallerie di quadri e monumenti antichi, avrà sicuramente di che soddisfare il suo gusto nella bell’ Italia che di tante rarità di questo genere è adorna. La supplico dunque di procurargli in Verona il mezzo di vedere le gallerie Bevilaqua e Moscardi ed introdurlo presso il Signore conte Emili ed altri dilettanti di musica, comme anche in casa Sagramoso dove si radunono.
Con questa occasiona le mando alcune carte manoscrite del Signore suo zio mio padrone, di cui servo una gratissima memoria. Queste debbono serbarsi presso di V. S. Ill.ma, quando avrò altre occasioni ne manderò delle altre. Ma bisognerebbe che avessi un ricapito sicuro [fol. 72v] in Torino, per farvi passare poco a poco, tutto quanto desidero ritorni in Verona, afine che queste carte non si smariscono dopo la mia morte. Essendomi piu facile di valermi delle occasioni di Torino, che d’ogni altra città d’Italia.
Quest’anno sono stato molto travagliato di dolori reumatici, e non ne sono ancora esente. Mia dia la prego delle sue nuove delle quali son privo da tanto tempo, e mi creda con pienissimo ossequio 
Del sig. marchese mio Signore.


Devotissimo ed obligatissimo servitore vero
G. Francesco Seguier

[souscription de Séguier au bas du fol. 72 : Au mois de mai (vers le 12 ou 13) 1778, Mr Lecointe laissa le paquet pour Mr Maffei, al sig. Antonio Vitalis negoziante, con ordine di serbarlo presso di se finche avesse avuto avviso dal Maffei al quale il Lecointe ne avea dato avviso.]
description: Source: [établissement de conservation] Nîmes, Bibliothèque Carré d'Art [cote] ms. 303, fol. 72
Observing the linked depletion of dust and CO gas at 0.1-10 au in disks of intermediate-mass stars
Creators: name: Banzatti, A.
name: Garufi, A.
name: Kama, M.
name: Benisty, M.
name: Brittain, S.
name: Pontoppidan, K. M.
name: Rayner, J. T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report on the discovery of correlations between dust and CO gas tracers of the 0.1-10 au region in planet-forming disks around young intermediate-mass stars. The abundance of refractory elements on stellar photospheres decreases as the location of hot CO gas emission recedes to larger disk radii, and as the near-infrared excess emission from hot dust in the inner disk decreases. The linked behavior between these observables demonstrates that the recession of infrared CO emission to larger disk radii traces an inner disk region where dust is being depleted. We also find that Herbig disk cavities have either low (~ 5-10 %) or high (~ 20-35 %) near-infrared excess, a dichotomy that has not been captured by the classic definition of "pre-transitional" disks.
description: Accepted for publication in A&A Letters; v2 includes language edits as in the A&A publication
Supplementary document for Photocurrent generation following long range propagation of organic exciton-polaritons - 5793149.pdf
Creators: name: Liu, Bin
name: Huang, Xinjing
name: Hou, Shaocong
name: Fan, Dejiu
name: Forrest, Stephen
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: Data for control devices and distance dependence
Results on the Coherent Interaction of High Energy Electrons and Photons in Oriented Single Crystals
Creators: name: NA59 Collaboration
name: Apyan, A.
name: Avakian, R. O.
name: Badelek, B.
name: Ballestrero, S.
name: Biino, C.
name: Birol, I.
name: Cenci, P.
name: Connell, S. H.
name: Eichblatt, S.
name: Fonseca, T.
name: Freund, A.
name: Gorini, B.
name: Groess, R.
name: Ispirian, K.
name: Ketel, T. J.
name: Kononets, Yu. V.
name: Lopez, A.
name: Mangiarotti, A.
name: van Rens, B.
name: Sellschop, J. P. F.
name: Shieh, M.
name: Sona, P.
name: Strakhovenko, V.
name: Uggerhoj, E.
name: Uggerhoj, U. I.
name: Unel, G.
name: Velasco, M.
name: Vilakazi, Z. Z.
name: Wessely, O.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The CERN-NA-59 experiment examined a wide range of electromagnetic processes for multi-GeV electrons and photons interacting with oriented single crystals. The various types of crystals and their orientations were used for producing photon beams and for converting and measuring their polarisation. The radiation emitted by 178 GeV unpolarised electrons incident on a 1.5 cm thick Si crystal oriented in the Coherent Bremsstrahlung (CB) and the String-of-Strings (SOS) modes was used to obtain multi-GeV linearly polarised photon beams. A new crystal polarimetry technique was established for measuring the linear polarisation of the photon beam. The polarimeter is based on the dependence of the Coherent Pair Production (CPP) cross section in oriented single crystals on the direction of the photon polarisation with respect to the crystal plane. Both a 1 mm thick single crystal of Germanium and a 4 mm thick multi-tile set of synthetic Diamond crystals were used as analyzers of the linear polarisation. A birefringence phenomenon, the conversion of the linear polarisation of the photon beam into circular polarisation, was observed. This was achieved by letting the linearly polarised photon beam pass through a 10 cm thick Silicon single crystal that acted as a "quarter wave plate" (QWP) as suggested by N. Cabibbo et al.
description: Presented at International workshop "Relativistic Channeling and Related Coherent Phenomena", Frascati (Rome) 23-26 March 2004
Accuracy and Safety of Novel Designs for Phase I Drug-Combination Oncology Trials
Creators: name: Liu, Rong
name: Yuan, Ying
name: Sen, Suman
name: Yang, Xin
name: Jiang, Qi
name: Li, Xiaoyun
name: Lu, Chengxing
name: Gönen, Mithat
name: Tian, Hong
name: Zhou, Heng
name: Lin, Ruitao
name: Marchenko, Olga
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Science Policy

description: Despite numerous innovative designs having been published for phase I drug-combination dose finding trials, their use in real applications is rather limited. As a working group under the American Statistical Association Biopharmaceutical Section, our goal is to identify the unique challenges associated with drug combination, share industry’s experiences with combination trials, and investigate the pros and cons of the existing designs. Toward this goal, we review seven existing designs and distinguish them based on the criterion of whether their primary objectives are to find a single maximum tolerated dose (MTD) or the MTD contour (i.e., multiple MTDs). Numerical studies, based on either industry-specified fixed scenarios or randomly generated scenarios, are performed to assess their relative accuracy, safety, and ease of implementation. We show that the algorithm-based 3 + 3 design has poor performance and often fails to find the MTD. The performance of model-based combination trial designs is mixed: some demonstrate high accuracy of finding the MTD but poor safety, while others are safe but with compromised identification accuracy. In comparison, the model-assisted designs, such as BOIN and waterfall designs, have competitive and balanced performance in the accuracy of MTD identification and patient safety, and are also simple to implement, thus offering an attractive approach to designing phase I drug-combination trials. By taking into consideration the design’s operating characteristics, ease of implementation and regulation, the need for advanced infrastructures, as well as the risk of regulatory acceptance, our article offers practical guidance on the selection of a suitable dose-finding approach for designing future combination trials.
title: Renaud Persiaux, "ARV : Leibowitch pilote l'allègement !"
Creators: name: Persiaux, Renaud
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Extrait du site http://www.seronet.info.
description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111232830363
description: created: start=2010;end=2017
Thermal entanglement in the two-qubit Heisenberg XYZ model
Creators: name: Rigolin, G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the entanglement of a two-qubit one dimensional XYZ Heisenberg chain in thermal equilibrium at temperature T. We obtain an analytical expression for the entanglement of formation for this system in terms of the parameters of the Hamiltonian and T. We show that depending on the relation among the coupling constants it is possible to increase the amount of entanglement of the system increasing its anisotropy. We also show numerically that for all sets of the coupling constants entanglement is a monotonically decreasing function of the temperature T, proving that we must have at least an external magnetic field in the z-direction to obtain a behavior where entanglement increases with T.
description: 13 pages, 10 figures, Published version
Natural Inflation from Polymer Quantization
Creators: name: Ali, Masooma
name: Seahra, Sanjeev S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the polymer quantization of a homogeneous massive scalar field in the early universe using a prescription inequivalent to those previously appearing in the literature. Specifically, we assume a Hilbert space for which the scalar field momentum is well defined but its amplitude is not. This is closer in spirit to the quantization scheme of loop quantum gravity, in which no unique configuration operator exists. We show that in the semi-classical approximation, the main effect of this polymer quantization scheme is to compactify the phase space of chaotic inflation in the field amplitude direction. This gives rise to an effective scalar potential closely resembling that of hybrid natural inflation. Unlike polymer schemes in which the scalar field amplitude is well-defined, the semi-classical dynamics involves a past cosmological singularity; i.e., this approach does not mitigate the big bang.
description: 9 pages, 4 figures, references added
Radial distribution and strong lensing statistics of satellite galaxies and substructure using high resolution LCDM hydrodynamical simulations
Creators: name: Maccio', Andrea V.
name: Moore, Ben
name: Stadel, Joachim
name: Diemand, Juerg
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyse the number density and radial distribution of substructures and satellite galaxies using cosmological simulations that follow the gas dynamics of a baryonic component, including shock heating, radiative cooling and star formation within the hierarchical concordance LCDM model. We find that the dissipation of the baryons greatly enhances the survival of subhaloes, expecially in the galaxy core, resulting in a radial distribution of satellite galaxies that closely follows the overall mass distribution in the inner part of the halo. Hydrodynamical simulations are necessary to resolve the adiabatic contraction and dense cores of galaxies, resulting in a total number of satellites a factor of two larger than found in pure dark matter simulation, in good agreement with the observed spatial distribution of satellite galaxies within galaxies and clusters. Convergence tests show that the cored distribution found by previous authors in pure N-body simulations was due to physical overmerging of dark matter only structures. We proceed to use a ray-shooting technique in order to study the impact of these additional substructures on the number of violations of the cusp caustic magnification relation. We develop a new approach to try to disentangle the effect of substructures from the intrinsic discreteness of N-Body simulations. Even with the increased number of substructures in the centres of galaxies, we are not able to reproduce the observed high numbers of discrepancies observed in the flux ratios of multiply lensed quasars.
description: 11 pages, 15 figures, comparison with previous works updated, one more plot added, minor changes to match the accepted version by MNRAS
Cool by Nature: Exploring Passive Cooling in Earthen Homes
Creators: name: V, Giri Prasath
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 430107
subject: Historical archaeology (incl. industrial archaeology)

description: In a world increasingly facing the challenges of rising temperatures and energy demands, passive cooling in mud architecture presents a time-tested, sustainable solution. Drawing on centuries-old techniques, this approach leverages the natural insulating properties of earth to maintain thermal comfort without relying on mechanical systems. Mud walls act as thermal mass-absorbing heat during the day and releasing it slowly at night-thereby regulating indoor temperatures. Features such as thick walls, high ceilings, shaded courtyards, and minimal yet strategic openings further enhance airflow and cooling. This eco-friendly design not only reduces energy consumption but also promotes comfort in hot climates, making it a valuable model for sustainable construction today. Passive Cooling in Mud Architecture One of the most impressive features of traditional mud houses is their natural ability to keep interiors cool, even in extremely hot climates. Unlike modern concrete buildings, which trap heat, earthen walls have high thermal mass. This means they can absorb heat during the day and release it slowly at night, maintaining a comfortable indoor temperature without air conditioning. In places like Rajasthan, India, and parts of Sub-Saharan Africa, people have used thick mud walls and small windows to manage sunlight and airflow for centuries.
Optical Signatures of Spin-Orbit Exciton in Bandwidth Controlled Sr$_2$IrO$_4$ Epitaxial Films via High-Concentration Ca and Ba Doping
Creators: name: Souri, M.
name: Kim, B. H.
name: Gruenewald, J. H.
name: Connell, J. G.
name: Thompson, J.
name: Nichols, J.
name: Terzic, J.
name: Min, B. I.
name: Cao, G.
name: Brill, J. W.
name: Seo, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have investigated the electronic and optical properties of (Sr$_{1-x}$Ca$_{x}$)$_2$IrO$_4$ (x= 0 - 0.375) and (Sr$_{1-y}$Ba$_y$)$_2$IrO$_4$ (y= 0 - 0.375) epitaxial thin-films, in which the bandwidth is systematically tuned via chemical substitutions of Sr ions by Ca and Ba. Transport measurements indicate that the thin-film series exhibits insulating behavior, similar to the J$_{eff}$= 1/2 spin-orbit Mott insulator Sr$_2$IrO$_4$. As the average A-site ionic radius increases from (Sr$_{1-x}$Ca$_{x}$)$_2$IrO$_4$ to (Sr$_{1-y}$Ba$_y$)$_2$IrO$_4$, optical conductivity spectra in the near-infrared region shift to lower energies, which cannot be explained by the simple picture of well-separated J$_{eff}$= 1/2 and J$_{eff}$= 3/2 bands. We suggest that the two-peak-like optical conductivity spectra of the layered iridates originates from the overlap between the optically-forbidden spin-orbit exciton and the inter-site optical transitions within the J$_{eff}$= 1/2 band. Our experimental results are consistent with this interpretation as implemented by a multi-orbital Hubbard model calculation: namely, incorporating a strong Fano-like coupling between the spin-orbit exciton and inter-site d-d transitions within the J$_{eff}$= 1/2 band.
description: 5 figures
Additional file 2: of Two versus five days of antibiotics after appendectomy for complex acute appendicitis (APPIC): study protocol for a randomized controlled trial
Creators: name: Boom, Anne Loes Van Den
name: Wijkerslooth, Elisabeth De
name: Rosmalen, Joost Van
name: FrĂŠdĂŠrique Beverdam
name: Evert-Jan Boerma
name: Boermeester, Marja
name: Bosmans, Joanna
name: Burghgraef, Thijs
name: Consten, Esther
name: Imro Dawson
name: Dekker, Jan Willem
name: Emous, Marloes
name: Geloven, Anna Van
name: Go, Peter
name: Heijnen, Luc
name: Huisman, Sander
name: Pierre, Dayanara Jean
name: Jonge, Joske De
name: Kloeze, Jurian
name: Koopmanschap, Marc
name: Langeveld, Hester
name: Luyer, Misha
name: Melles, Damian
name: Mouton, Johan
name: Ploeg, Augustinus Van Der
name: Poelmann, Floris
name: Ponten, Jeroen
name: Rossem, Charles Van
name: Schreurs, Wilhelmina
name: JoĂŤl Shapiro
name: Steenvoorde, Pascal
name: Toorenvliet, Boudewijn
name: Verhelst, Joost
name: Hendt Versteegh
name: Wijnen, Rene
name: Wijnhoven, Bas
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology

description: Subject information and consent form (in Dutch). (PDF 231Â kb)
Supplementary document for Self-injection-locked microcomb-based coherent oscillator - 6851201.pdf
Creators: name: Lei, Fuchuan
name: Sun, Yi
name: Helgason, Óskar
name: Ye, Zhichao
name: Gao, Yan
name: Karlsson, Magnus
name: Andrekson, Peter
name: Company, Victor Torres
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Numerical simulation details
Light reflection upon a movable mirror as a paradigm for continuous variable teleportation network
Creators: name: Pirandola, Stefano
name: Mancini, Stefano
name: Vitali, David
name: Tombesi, Paolo
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an optomechanical system as a paradigm of three-mode teleportation network. Quantum state transfer among optical and vibrational modes becomes possible by exploiting correlations established by radiation pressure.
description: 7 pages, 5 figures, to be published in the special issue of J. Mod. Opt. edited by R. Bonifacio, B.G. Englert and M.G.A. Paris, devoted to the 2003 Garda Lake Workshop on "Mysteries, Puzzles and Paradoxes in Quantum Mechanics"
Accuracy and Safety of Novel Designs for Phase I Drug-Combination Oncology Trials*
Creators: name: Liu, Rong
name: Yuan, Ying
name: Sen, Suman
name: Yang, Xin
name: Jiang, Qi
name: Li, Xiaoyun
name: Lu, Chengxing
name: Göneng, Mithat
name: Tian, Hong
name: Zhou, Heng
name: Lin, Ruitao
name: Marchenko, Olga
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Science Policy

description: Despite numerous innovative designs having been published for phase I drug-combination dose finding trials, their use in real applications is rather limited. As a working group under the American Statistical Association Biopharmaceutical Section, our goal is to identify the unique challenges associated with drug combination, share industry’s experiences with combination trials, and investigate the pros and cons of the existing designs. Toward this goal, we review seven existing designs and distinguish them based on the criterion of whether their primary objectives are to find a single maximum tolerated dose (MTD) or the MTD contour (i.e., multiple MTDs). Numerical studies, based on either industry-specified fixed scenarios or randomly generated scenarios, are performed to assess their relative accuracy, safety, and ease of implementation. We show that the algorithm-based 3 + 3 design has poor performance and often fails to find the MTD. The performance of model-based combination trial designs is mixed: some demonstrate high accuracy of finding the MTD but poor safety, while others are safe but with compromised identification accuracy. In comparison, the model-assisted designs, such as BOIN and waterfall designs, have competitive and balanced performance in the accuracy of MTD identification and patient safety, and are also simple to implement, thus offering an attractive approach to designing phase I drug-combination trials. By taking into consideration the design’s operating characteristics, ease of implementation and regulation, the need for advanced infrastructures, as well as the risk of regulatory acceptance, our paper offers practical guidance on the selection of a suitable dose-finding approach for designing future combination trials.
Antiferromagnetic skyrmion crystals: generation, topological Hall and topological spin Hall effect
Creators: name: Göbel, Börge
name: Mook, Alexander
name: Henk, Jürgen
name: Mertig, Ingrid
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Skyrmions are topologically nontrivial, magnetic quasi-particles, that are characterized by a topological charge. A regular array of skyrmions - a skyrmion crystal (SkX) - features the topological Hall effect (THE) of electrons, that, in turn, gives rise to the Hall effect of the skyrmions themselves. It is commonly believed that antiferromagnetic skyrmion crystals (AFM-SkXs) lack both effects. In this Rapid Communication, we present a generally applicable method to create stable AFM-SkXs by growing a two sublattice SkX onto a collinear antiferromagnet. As an example we show that both types of skyrmion crystals - conventional and antiferromagnetic - exist in honeycomb lattices. While AFM-SkXs with equivalent lattice sites do not show a THE, they exhibit a topological spin Hall effect. On top of this, AFM-SkXs on inequivalent sublattices exhibit a nonzero THE, which may be utilized in spintronics devices. Our theoretical findings call for experimental realization.
description: 5 pages, 5 figures
Constraints on the Evolution of the Galaxy Stellar Mass Function II: Quenching Timescale of Galaxies and its Implication for their Star Formation Rate
Creators: name: Contini, E.
name: Kang, X.
name: Romeo, A. D.
name: Xia, Q.
name: Yi, S. K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the connection between the observed star formation rate-stellar mass (SFR-$M_*$) relation and the evolution of the stellar mass function (SMF) by means of a subhalo abundance matching technique coupled to merger trees extracted from a N-body simulation. Our approach consist of forcing the model to match the observed SMF at redshift $z \sim 2.3$, and let it evolve down to $z \sim 0.3$ according to a $τ$ model, an exponentially declining functional form which describes the star formation rate decay of both satellite and central galaxies. In this study, we use three different sets of SMFs: ZFOURGE data from Tomczak et al.; UltraVISTA data from Ilbert et al. and COSMOS data from Davidzon et al. We also build a mock survey combining UltraVISTA with ZFOURGE. Our modelling of quenching timescales is consistent with the evolution of the SMF down to $z \sim 0.3$, with different accuracy depending on the particular survey used for calibration. We tested our model against the observed SMFs at low redshift and it predicts residuals (observation versus model) within $1σ$ observed scatter along most of the stellar mass range investigated, and with mean residuals below 0.1 dex in the range $\sim [10^{8.7}-10^{11.7}] M_{\odot}$. We then compare the SFR-$M_*$ relation predicted by the model with the observed one at different redshifts. The predicted SFR-$M_*$ relation underpredicts the median SFR at fixed stellar mass relative to observations at all redshifts. Nevertheless, the shapes are consistent with the observed relations up to intermediate-mass galaxies, followed by a rapid decline for massive galaxies.
description: 16 pages, accepted for publication in ApJ, minor changes after proof
Cosmic gamma-ray background from Type Ia supernovae revisited: Evidence for missing gamma-rays at MeV
Creators: name: Ahn, Kyungjin
name: Komatsu, Eiichiro
name: Hoflich, Peter
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The observed cosmic gamma-ray background at ~ MeV has often been attributed to Type Ia supernovae (SNIa). Since SNIa is close to a standard candle, one can calculate the gamma-ray intensity of SNIa integrated over redshifts fairly accurately, once the evolution of the SNIa rate is known. The latest SNIa rate measured at z < ~1.6 (Dahlen et al. 2004) indicates that the previous calculations of the gamma-ray background consistently overestimated the SNIa rate. With the new rate, we find that the SNIa contribution is an order of magnitude smaller than observed, and thus new population(s) of sources should be invoked.
description: 4 pages, 2 figures; Accepted for publication in Physical Review D
Additional file 1 of SWISS: multiplexed orthogonal genome editing in plants with a Cas9 nickase and engineered CRISPR RNA scaffolds
Creators: name: Li, Chao
name: Zong, Yuan
name: Jin, Shuai
name: Zhu, Haocheng
name: Lin, Dexing
name: Li, Shengnan
name: Qiu, Jin-Long
name: Wang, Yanpeng
name: Gao, Caixia
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 1: Figure S1. Flow cytometry of BFP-to-GFP conversion induced by PBE and the five PBEcs in rice protoplasts. Figure S2. Engineering the secondary structures of CRISPR RNA scaffolds. Figure S3. Flow cytometry of BFP-to-GFP conversion induced by various scRNAs and their cognate PBEcs in rice protoplasts. Figure S4. Frequencies of base editing of endogenous genes by different scRNAs and cognate PBEcs in rice protoplasts. Figure S5. Activities of esgRNA-2×MS2, esgRNA-3×MS2, sgRNA4.0, and esgRNA-2×com with cognate PBEcs in rice protoplasts. Figure S6. C-to-T editing frequencies generated by scaffold RNA-recruited APOBEC1 narrow-window variants in rice protoplasts. Figure S7. Flow cytometry of mGFP-to-GFP conversion induced by PABE and the three PABEcs in rice protoplasts. Figure S8. Flow cytometry of mGFP-to-GFP conversion induced by various scRNAs and their cognate PABEcs in rice protoplasts. Figure S9. Activities of the selected scaffold RNAs with their cognate PABEcs in rice protoplasts. Figure S10. Schematic of multiple sgRNAs assembly for SWISSv1.1 and SWISSv1.2. Figure S11. The distributions of deletion reads among the indel sequencing reads for SWISSv1.1, SWISSv1.2, and SWISSv3. Figure S12. Schematic of multiple sgRNAs assembly for SWISSv2 and SWISSv3. Figure S13. Comparison of the editing efficiencies between the SWISS systems and the individual genome editing tools (PBE, PBEc4, PABE-2, PABEc5, and paired nCas9). Figure S14. Simultaneous CBE, ABE, and DSB formation in rice plants. Table S1. The sgRNA sequences used to compare the activities of PBEcs and PABEcs. Table S2. The sgRNA sequences used for SWISSv1.1, SWISSv1.2, SWISSv2, and SWISSv3 editing in rice protoplasts. Table S3. Potential off-target sites analyzed for OsALS-T2, OsACC-T2, OsBADH2-Indels-sgL, and OsBADH2-Indels-sgR triple mutants. Table S4. Statistics of whole genome sequencing analysis. Table S5. Primer sequences used in this study.
The Hercules stream as seen by APOGEE-2 South
Creators: name: Hunt, Jason A. S.
name: Bovy, Jo
name: Pérez-Villegas, Angeles
name: Holtzman, Jon A.
name: Sobeck, Jennifer
name: Chojnowski, Drew
name: Santana, Felipe A.
name: Palicio, Pedro A.
name: Wegg, Christopher
name: Gerhard, Ortwin
name: Almeida, Andrés
name: Bizyaev, Dmitry
name: Fernandez-Trincado, Jose G.
name: Lane, Richard R.
name: Longa-Peña, Penélope
name: Majewski, Steven R.
name: Pan, Kaike
name: Roman-Lopes, Alexandre
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Hercules stream is a group of co-moving stars in the Solar neighbourhood, which can potentially be explained as a signature of either the outer Lindblad resonance (OLR) of a fast Galactic bar or the corotation resonance of a slower bar. In either case, the feature should be present over a large area of the disc. With the recent commissioning of the APOGEE-2 Southern spectrograph we can search for the Hercules stream at $(l,b)=(270^\circ,0)$, a direction in which the Hercules stream, if caused by the bar's OLR, would be strong enough to be detected using only the line-of-sight velocities. We clearly detect a narrow, Hercules-like feature in the data that can be traced from the solar neighbourhood to a distance of about 4 kpc. The detected feature matches well the line-of-sight velocity distribution from the fast-bar (OLR) model. Confronting the data with a model where the Hercules stream is caused by the corotation resonance of a slower bar leads to a poorer match, as the corotation model does not predict clearly separated modes, possibly because the slow-bar model is too hot.
description: 7 pages, 5 figures; Submitted to MNRAS 8th September 2017, accepted October 23rd
Additional file 1: of Inflammation functions as a key mediator in the link between ACPA and erosion development: an association study in Clinically Suspect Arthralgia
Creators: name: R. Ten Brinck
name: R. Toes
name: A. Van Der HelmâVan Mil
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology

description: Methods. MRI scanning and scoring. Figure S1. Median erosion scores in patients with Clinically Suspect Arthralgia comparing ACPA-positive and ACPA-negative patients in relation to the concomitant presence of any inflammation. Figure S2. Median erosion scores of ACPA-positive patients with Clinically Suspect Arthralgia according to tertiles of ACPA levels. (DOCX 133 kb)
Absolute Branching Fraction Measurements of Exclusive D^0 Semileptonic Decays
Creators: name: Coan, T. E.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: With the first data sample collected by the CLEO-c detector at the psi(3770) resonance we have studied four exclusive semileptonic decays of the D0 meson. Our results include the first observation and absolute branching fraction measurement for D0 --> rho- e+ nu_e and improved measurements of the absolute branching fractions for D0 decays to K- e+ nu_e, pi- e+ nu_e, and K*- e+ nu_e.
description: 9 pages postscript,also available through http://www.lns.cornell.edu/public/CLNS/2005/, submitted to PRL
The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament
Creators: name: Pattle, Kate
name: Ward-Thompson, Derek
name: Berry, David
name: Hatchell, Jennifer
name: Chen, Huei-Ru
name: Pon, Andy
name: Koch, Patrick M.
name: Kwon, Woojin
name: Kim, Jongsoo
name: Bastien, Pierre
name: Cho, Jungyeon
name: Coudé, Simon
name: Di Francesco, James
name: Fuller, Gary
name: Furuya, Ray S.
name: Graves, Sarah F.
name: Johnstone, Doug
name: Kirk, Jason
name: Kwon, Jungmi
name: Lee, Chang Won
name: Matthews, Brenda C.
name: Mottram, Joseph C.
name: Parsons, Harriet
name: Sadavoy, Sarah
name: Shinnaga, Hiroko
name: Soam, Archana
name: Hasegawa, Tetsuo
name: Lai, Shih-Ping
name: Qiu, Keping
name: Friberg, Per
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We determine the magnetic field strength in the OMC 1 region of the Orion A filament via a new implementation of the Chandrasekhar-Fermi method using observations performed as part of the James Clerk Maxwell Telescope (JCMT) B-Fields In Star-Forming Region Observations (BISTRO) survey with the POL-2 instrument. We combine BISTRO data with archival SCUBA-2 and HARP observations to find a plane-of-sky magnetic field strength in OMC 1 of $B_{\rm pos}=6.6\pm4.7$ mG, where $δB_{\rm pos}=4.7$ mG represents a predominantly systematic uncertainty. We develop a new method for measuring angular dispersion, analogous to unsharp masking. We find a magnetic energy density of $\sim1.7\times 10^{-7}$ Jm$^{-3}$ in OMC 1, comparable both to the gravitational potential energy density of OMC 1 ($\sim 10^{-7}$ Jm$^{-3}$), and to the energy density in the Orion BN/KL outflow ($\sim 10^{-7}$ Jm$^{-3}$). We find that neither the Alfvén velocity in OMC 1 nor the velocity of the super-Alfvénic outflow ejecta is sufficiently large for the BN/KL outflow to have caused large-scale distortion of the local magnetic field in the $\sim$500-year lifetime of the outflow. Hence, we propose that the hour-glass field morphology in OMC 1 is caused by the distortion of a primordial cylindrically-symmetric magnetic field by the gravitational fragmentation of the filament and/or the gravitational interaction of the BN/KL and S clumps. We find that OMC 1 is currently in or near magnetically-supported equilibrium, and that the current large-scale morphology of the BN/KL outflow is regulated by the geometry of the magnetic field in OMC 1, and not vice versa.
description: 23 pages, 14 figures, 2 tables. Accepted for publication in ApJ
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0667
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/2012
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: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0667, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0667, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Experimental Hamiltonian identification for controlled two-level systems
Creators: name: Schirmer, SG
name: Kolli, A
name: Oi, DKL
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a strategy to empirically determine the internal and control Hamiltonians for an unknown two-level system (black box) subject to various (piecewise constant) control fields when direct readout by measurement is limited to a single, fixed observable.
description: approx 4 pages, 5 figures, RevTeX, minor corrections/notational changes
Additional file 2 of SWISS: multiplexed orthogonal genome editing in plants with a Cas9 nickase and engineered CRISPR RNA scaffolds
Creators: name: Li, Chao
name: Zong, Yuan
name: Jin, Shuai
name: Zhu, Haocheng
name: Lin, Dexing
name: Li, Shengnan
name: Qiu, Jin-Long
name: Wang, Yanpeng
name: Gao, Caixia
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 2: Sequences S1. DNA sequences of the OsU3 and TaU6 promoters used in this study. Sequences S2. DNA sequences of sgRNA, esgRNA, and scRNAs used in this study. Sequences S3. DNA sequences of the modules composed of PBEcs and PABEcs used in this study. Sequences S4. DNA sequences of templates for assemble multiple sgRNAs used in this study. Sequences S5. DNA sequences of SWISSv2/v3 and SWISSv2/v3-NG used in this study.
Sparse reduced-order modeling : Sensor-based dynamics to full-state estimation
Creators: name: Loiseau, Jean-Christophe
name: Noack, Bernd R.
name: Brunton, Steven L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We propose a general dynamic reduced-order modeling framework for typical experimental data: time-resolved sensor data and optional non-time-resolved PIV snapshots. This framework contains four steps. First, the sensor signals are lifted to a dynamic feature space. Second, we identify a sparse human-interpretable nonlinear dynamical system for the feature state based on the sparse identification of nonlinear dynamics (SINDy). Third, if PIV snapshots are available, a local linear mapping from the feature state to velocity fields is shown to be orders of magnitudes more accurate than optimal modal expansions of the same order. Fourth, a generalized feature-based modal decomposition identifies coherent structures that are most dynamically correlated with the linear and nonlinear interaction terms in the sparse model, adding interpretability. Steps 1 and 2 define a black-box model. Optional steps 3 and 4 lift the black-box dynamics to a 'gray-box' model of the coherent structures, if non-time-resolved full-state data is available. This gray-box modeling strategy is successfully applied to the transient and post-transient laminar cylinder wake, and compares favorably with a POD model. We foresee numerous applications of this highly flexible modeling strategy, including estimation, prediction and control. Moreover, the feature space may be based on intrinsic coordinates, which are unaffected by a key challenge of modal expansion: the slow change of low-dimensional coherent structures with changing geometry and varying parameters.