cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
BAT AGN Spectroscopic Survey II: X-ray Emission and High Ionization Optical Emission Lines
Creators: name: Berney, Simon
name: Koss, Michael
name: Trakhtenbrot, Benny
name: Ricci, Claudio
name: Lamperti, Isabella
name: Schawinski, Kevin
name: Balokovic, Mislav
name: Crenshaw, D. Michael
name: Fischer, Travis
name: Gehrels, Neil
name: Harrison, Fiona
name: Hashimoto, Yasuhiro
name: Ichikawa, Kohei
name: Mushotzky, Richard
name: Oh, Kyuseok
name: Stern, Daniel
name: Treister, Ezequiel
name: Ueda, Yoshihiro
name: Veilleux, Sylvain
name: Winter, Lisa
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the relationship between X-ray and optical line emission in 340 nearby AGN selected above 10 keV using Swift BAT. We find a weak correlation between the extinction corrected [O III] and hard X-ray luminosity (14-195 keV) with a [OIII] large scatter (R_Pear = 0.64, sigma = 0.62 dex) and a similarly large scatter with the intrinsic 2-10 keV to [O III] luminosities (RPear=0.63, sigma = 0.63 dex). Correlations of the hard X-ray fluxes with the fluxes of high-ionization narrow lines ([O III], He II, [Ne III] and [Ne V]) are not significantly better than with the low ionization lines (Halpha, [SII]). Factors like obscuration or physical slit size are not found to be a significant part of the large scatter. In contrast, the optical emission lines show much better correlations with each other (sigma = 0.3 dex) than with the X-ray flux. The inherent large scatter questions the common usage of narrow emission lines as AGN bolometric luminosity indicators and suggests that other issues such as geometrical differences in the scattering of the ionized gas or long term AGN variability are important.
description: About to be accepted in MNRAS upon minor grammar changes
Relativistic bulk viscous fluids of Burgers type and their presence in neutron stars
Creators: name: Gavassino, Lorenzo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Theory (nucl-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: It is well known that a mixture of two chemical components undergoing one chemical reaction is a bulk viscous fluid, where the bulk stress evolves according to the Israel-Stewart theory. Here, we show that a mixture of three independent chemical components undergoing two distinct chemical reactions can also be viewed as a bulk viscous fluid, whose bulk stress now is governed by a second-order differential equation which reproduces the Burgers model for viscoelasticity. This is a rigorous and physically motivated example of a fluid model where the viscous stress does not undergo simple Maxwell-Cattaneo relaxation, and can actually overshoot the Navier-Stokes stress. We show that, if one accounts for muons, neutron star matter is indeed a bulk viscous fluid of Burgers type.
description: 10 pages, 1 figure, published on CQG, see https://iopscience.iop.org/article/10.1088/1361-6382/ace587
Sequential sharing of two-qudit entanglement based on the entropic uncertainty relation
Creators: name: Hu, Ming-Liang
name: Fan, Heng
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Entanglement and uncertainty relation are two focuses of quantum theory. We relate entanglement sharing to the entropic uncertainty relation in a $(d\times d)$-dimensional system via weak measurements with different pointers. We consider both the scenarios of one-sided sequential measurements in which the entangled pair is distributed to multiple Alices and one Bob and two-sided sequential measurements in which the entangled pair is distributed to multiple Alices and Bobs. It is found that the maximum number of observers sharing the entanglement strongly depends on the measurement scenarios, the pointer states of the apparatus, and the local dimension $d$ of each subsystem, while the required minimum measurement precision to achieve entanglement sharing decreases to its asymptotic value with the increase of $d$. The maximum number of observers remain unaltered even when the state is not maximally entangled but has strong-enough entanglement.
description: 11 pages, 6 figures; Final version published in Phys. Rev. A
The Correlation Between Blood Biomarker and Intracranial Pathologies in Mild Acute Traumatic Brain Injury: a Systematic Review
Creators: name: Siahaan, Andre
name: Fernando, Eric
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Medicine and Health Sciences
subject: Medical Specialties
subject: Trauma
subject: Neurology
subject: Biomarker
subject: CT scan
subject: mild traumatic brain injury
subject: MRI
subject: mTBI
subject: Systematic review

description: Systematic Review
Wormhole and Entanglement (Non-)Detection in the ER=EPR Correspondence
Creators: name: Bao, Ning
name: Pollack, Jason
name: Remmen, Grant N.
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The recently proposed ER=EPR correspondence postulates the existence of wormholes (Einstein-Rosen bridges) between entangled states (such as EPR pairs). Entanglement is famously known to be unobservable in quantum mechanics, in that there exists no observable (or, equivalently, projector) that can accurately pick out whether a generic state is entangled. Many features of the geometry of spacetime, however, are observables, so one might worry that the presence or absence of a wormhole could identify an entangled state in ER=EPR, violating quantum mechanics, specifically, the property of state-independence of observables. In this note, we establish that this cannot occur: there is no measurement in general relativity that unambiguously detects the presence of a generic wormhole geometry. This statement is the ER=EPR dual of the undetectability of entanglement.
description: 14 pages, 4 figures
title: The natural course of computed tomography progression in diffuse idiopathic skeletal hyperostosis: preliminary results
Creators: name: Yaniv, Gal
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Musculoskeletal spine
subject: Musculoskeletal joint
subject: CT
subject: Structured reporting
subject: Tissue characterisation

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Diffuse idiopathic skeletal hyperostosis (DISH) is a common disease characterized by ossification of paravertebral ligaments and peripheral entheses [1]. Although DISH can be present anywhere in the spine, it is most prevalent at the thoracic...
Field observables near a fluctuating boundary
Creators: name: Armata, Federico
name: Butera, Salvatore
name: Montalbano, Federico
name: Passante, Roberto
name: Rizzuto, Lucia
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We review several aspects related to the confinement of a massless scalar field in a cavity with a movable conducting wall of finite mass, free to move around its equilibrium position to which it is bound by a harmonic potential, and whose mechanical degrees of freedom are described quantum mechanically. This system, for small displacements of the movable wall from its equilibrium position, can be described by an effective interaction Hamiltonian between the field and the mirror, quadratic in the field operators and linear in the mirror operators. In the interacting, i.e. dressed, ground state, we first consider local field observables such as the field energy density: we evaluate changes of the field energy density in the cavity with the movable wall with respect to the case of a fixed wall, and corrections to the usual Casimir forces between the two walls. We then investigate the case of two one-dimensional cavities separated by a movable wall of finite mass, with two massless scalar fields defined in the two cavities. We show that in this case correlations between the squared fields in the two cavities exist, mediated by the movable wall, at variance with the fixed-wall case.
description: 7 pages, Proceedings of the DICE 2022 Conference, Castiglioncello, Italy
Formation, disruption and energy output of Population III X-ray binaries
Creators: name: Ryu, Taeho
name: Tanaka, Takamitsu L.
name: Perna, Rosalba
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The first astrophysical objects shaped the cosmic environment by reionizing and heating the intergalactic medium (IGM). In particular, X-rays are very efficient at heating the IGM before it became completely ionized, an effect that can be measured through the 21 cm line of neutral hydrogen. High-mass X-ray binaries (HMXBs), known to be prolific X-ray sources in star-forming galaxies at lower redshifts, are prime candidates for driving the thermal evolution of the IGM at redshifts $z > 20$. Despite their importance, the formation efficiency of HMXBs from the first stellar populations is not well understood---as such, their collective X-ray emission and the subsequent imprint on the 21 cm signature are usually evaluated using free parameters. Using $N$-body simulations, we estimate the rate of HMXB formation via mutual gravitational interactions of nascent, small groups of the first stars (Pop III stars). We run two sets of calculations: one in which stars form in small groups of five in nearly Keplerian initial orbits, and another in which two such groups collide (expected from mergers of host protogalaxies). We find that HMXBs form at a rate of one per $~10^{4}~{\rm M}_{\odot}$ in newly born stars, and that they emit with a power of $\sim 10^{41} ~{\rm erg}~{\rm s} ^{-1}$ in the $2-10$ keV band per solar mass per year of star formation. This value is a factor $\sim 10^{2}$ larger than what is observed in star forming galaxies at lower redshifts; the X-ray production from early HMXBs would have been even more copious, if they also formed $in$ $situ$ or via migration in protostellar disks. Combining our results with earlier studies suggests that early HMXBs were highly effective at heating the IGM and leaving a strong 21 cm signature. We discuss broader implications of our results, such as the rate of long GRBs from PopIII stars and the direct collapse black hole formation.
description: 16 pages, 12 figures, 4 tables; submitted to MNRAS
Aspekt: Wesen, Grundlagen und Auftreten
Creators: name: Schwerteck, Hans
Publisher: name: Universität Tübingen
Year: 2017
Subjects: subject: Kategorie
subject: 400

description: Im Gegensatz zu der bisher in der Sprachwissenschaft üblichen Auffassung wird die Kategorie Aspekt nicht in Funktion von Zeit , sondern in Funktion des Verhältnisses von Subjekt und Prädikat gesehen.
Sample Size Justifications in Gait & Posture
Creators: name: McCrum, Christopher
name: van Beek, Jorg
name: Van Hooren, Bas
name: Janssen, Sanne
name: Schumacher, Charlotte
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Sports Sciences
subject: Kinesiology
subject: Biomechanics
subject: Medicine and Health Sciences
subject: Life Sciences
subject: Rehabilitation and Therapy
subject: gait
subject: metascience
subject: posture
subject: power analysis
subject: sample size
subject: statistical power

description: This study makes an initial evaluation of sample size justifications in the Gait & Posture field by screening samples of articles from Gait & Posture, including both the the most recent volumes, and the latest volumes before the inclusion of a guideline requiring authors to justify their sample size. We will also determine the frequency of various types of sample size justifications based on the recent article “Sample Size Justifications” by Lakens (2021).
Sprache der Nähe - Sprache der Distanz: Mündlichkeit und Schriftlichkeit im Spannungsfeld von Sprachtheorie und Sprachgeschichte
Creators: name: Koch, Peter
name: Oesterreicher, Wulf
Publisher: name: Universität Tübingen
Year: 1986
Subjects: subject: Linguistik
subject: 400

description: Zweitveröffentlichung
title: МНОГОЛЕТНИЕ ИССЛЕДОВАНИЯ ЯПОНСКИХ УЧЕНЫХ В ОБЛАСТИ РАЗРАБОТКИ ИСКУССТВЕННОГО РАЦИОНА  ТУТОВОГО ШЕЛКОПРЯДА (ОБЗОР)
Creators: name: Евлагина, Е.Г.
name: Евлагин, Е.В.
name: Лейнвебер, Е.Ф.
name: Юматов, Е.Н.
name: Аветисян, С.В.
Publisher: name: Федеральное государственное бюджетное научное учреждение «Северо-Кавказский федеральный научный аграрный центр»
Year: 2024
Subjects: тутовый шелкопряд (Bombyx mori L.), шелковица, искусственная питательная среда, рацион, диета, корм, выкормка.
silkworm (Bombyx mori L.), mulberry, artificial nutrient medium, ration, diet, feed, feeding.

description: В статье рассмотрены вопросы использования различных искусственных питательных сред при выращивании гусениц тутового шелкопряда, обобщены результаты исследований, проведенных японскими учеными, за период 1960-2020 гг. Представленный анализ научных работ, посвященных более чем двадцати различным рецептурам искусственных питательных сред и результатам выкормки на искусственном рационе, позволяет выявить преимущества и недостатки компонентов диеты и их количественного соотношения, а также определить дальнейшие направления изучения и совершенствования, в частности необходимости детальных исследований адаптивной способности различных пород, гибридов тутового шелкопряда к искусственному рациону и методах их подбора.
description: The article discusses the use of various artificial nutrient media in the cultivation of silkworm caterpillars, summarizes the results of research conducted by Japanese scientists for the period 1960-2020. The presented analysis of scientific papers devoted to more than twenty different recipes of artificial nutrient media and results of feeding on an artificial diet allows us to identify the advantages and disadvantages of diet components and their quantitative ratio, as well as to determine further directions of study and improvement, in particular the need for detailed studies of the adaptive ability of various breeds, silkworm hybrids to artificial diet and methods their selection.
Testing electroweak scale seesaw models at $e^{-} γ$ and $γγ$ colliders
Creators: name: Das, Arindam
name: Mandal, Sanjoy
name: Shil, Sujay
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We investigate the possibilities of probing the electroweak scale seesaw scenarios such as type-I, type-II and type-III seesaw at $e^-γ$ and $γγ$ colliders. For the case of type-I seesaw, the heavy neutrinos can be produced at $e^{-}γ$ colliders in association with a $W$ boson. We study a variety of final states in this case including single and multilepton modes in association with jets to estimate bounds on the light-heavy neutrino mixing angle. In case of type-II seesaw, doubly charged multiplets of the SU$(2)_L$ triplet scalar can be produced in pair at $γγ$ collider. We study the multi-leptonic decay modes coming from this pair production of doubly charged Higgs and show how one can probe neutrino mass hierarchy. We also study same sign $W$ boson production from the doubly charged Higgs to study multilepton modes in association with missing energy. From the type-III seesaw, we study same sign dilepton+jets and trilepton+jets modes at $e^-γ$ collider which are coming from the neutral and charged component of the triplet fermion in association with a $W$ boson and $Z$ boson, respectively. Due to the existing limits on the triplet fermions from the LHC we choose heavier mass so that the gauge boson originated from the decay of a neutral multiplet can be sufficiently boosted producing a fat-jet signature in association with same sign dilepton and trilepton. Finally we estimate bounds on the light neutrino-heavy triplet fermion mixing angle and compare with the existing bounds.
description: 53 pages, 30 figures
Book of Abstracts of the 1st Colloquium for Bioinformatics Learning, Education, and Training
Creators: name: Fatima, Ayesha
name: Khan, Mohammad Asif
Publisher: name: F1000 Research Limited
Year: 2023

description: The publication contains abstracts submitted to the 1st Colloquium on Bioinformatics Learning, Education and Training in the categories of oral presentations, poster presentations, keynote speeches and training workshops.
title: Contrast Enhanced Ultrasound, revision of our 50 first patients
Creators: name: CASADO MORAGON Luis Martín, Luiis Martin
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Tissue characterisation
subject: Diagnostic procedure
subject: Ultrasound
subject: Abdomen

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: To evaluate the contribution of the contrast-enhanced ultrasound to the basal ultrasound study in liver and abdominal...
Performance Measurement Data for Speeding Up Lagrangian Fluid-Flow Particle Simulations in Python  via Dynamic Collections
Publisher: name: Utrecht University
Year: 2021
Subjects: subject: Natural Sciences - Earth and related environmental sciences (1.5)
subject: Scientific Computing
subject: Scientific Python
subject: Dynamic Data Structures
subject: Python
subject: Performance Measurement
subject: Performance Profiling

description: This data repository contains the raw measurement for the scientific computing-article of speeding up lagrangian fluid-flow simulations in Python (within the parcels-framework), called:

Kehl, C., van Sebille, E. and Gibson, A. "Speeding up Python-based Lagrangian Fluid-Flow Particle Simulations via Dynamic Collection Data Structures", 2021, to be submitted to SIAM Journal of Scientific Computing

The repository is structured as follows:
- code_links/ - folder containing a collection of text files with links to GitHub (where the code is stored), and meta-information on version etc.
- measurements/ - contains the OpenOffice / LibreCalc table with the performance measurements of the different data structures in relation to the number of particles (raw data)
- plots/ - original-resolution plots of the *measurements*, as they are found in the publication
Velocity and magnetic fields within 1000 AU from a massive YSO
Creators: name: Sanna, A.
name: Surcis, G.
name: Moscadelli, L.
name: Cesaroni, R.
name: Goddi, C.
name: Vlemmings, W. H. T.
name: Garatti, A. Caratti o
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We want to study the velocity and magnetic field morphology in the vicinity (<1000 AU) of a massive young stellar object (YSO), at very high spatial resolution (10-100 AU). We performed milli-arcsecond polarimetric observations of the strong CH3OH maser emission observed in the vicinity of an O-type YSO, in G023.01-00.41. We have combined this information with the velocity field of the CH3OH masing gas previously measured at the same angular resolution. We analyse the velocity and magnetic fields in the reference system defined by the direction of the molecular outflow and the equatorial plane of the hot molecular core at its base, as recently observed on sub-arcsecond scales. We provide a first detailed picture of the gas dynamics and magnetic field configuration within a radius of 2000 AU from a massive YSO. We have been able to reproduce the magnetic field lines for the outer regions (>600 AU) of the molecular envelope, where the magnetic field orientation shows a smooth change with the maser cloudlets position (0.2 degree/AU). Overall, the velocity field vectors well accommodate with the local, magnetic field direction, but still show an average misalignment of 30 degrees. We interpret this finding as the contribution of a turbulent velocity field of about 3.5 km/s, responsible for braking up the alignment between the velocity and magnetic field vectors. We do resolve different gas flows which develop both along the outflow axis and across the disk plane, with an average speed of 7 km/s. In the direction of the outflow axis, we establish a collimation of the gas flow, at a distance of about 1000 AU from the disk plane. In the disk region, gas appears to stream outward along the disk plane for radii greater than 500-600 AU, and inward for shorter radii.
description: 7 pages, 4 figures, 1 table, accepted by Astronomy & Astrophysics
The hygiene hypothesis and childhood asthma in Orange County, North Carolina
Creators: name: Ward, Ashley R.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2007

description: This thesis examines childhood asthma in Orange County, North Carolina and its relationship to the Hygiene Hypothesis. The Hygiene Hypothesis challenges traditionally held views on hygiene and asserts that decreased exposures to microbes during an infant’s first year of life results in the poor development of the immune system. According to this hypothesis, the lack of development in the immune system is at least partially responsible for the increasing number of autoimmune disorders, asthma being one of them. In addition to the cross-sectional analysis, spatial analysis is used to determine spatial patterning or clustering of childhood asthma cases in the county. A cross-sectional study was conducted including 427 households (1000 children). First and fourth grade households were surveyed via the Orange County School System. Geographic information was voluntarily collected on each household that participated. The results of the survey demonstrate that the primary factors impacting childhood asthma in Orange County are genetics, premature birth, daycare attendance, and urban/suburban living. Spatial analysis reveals areas of high prevalence in the county but clusters of questionable significance.
title: Are the ASAS-OMERACT criteria useful in the diagnosis of sacroiliitis with MR? Our experience
Creators: name: López Menéndez, Carlos
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Inflammation
subject: Oedema
subject: Imaging sequences
subject: MR
subject: Musculoskeletal bone
subject: Musculoskeletal joint

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Sacroiliitis is a diagnostic criterion of spondyloarthropaties (SpA) (1). Magnetic resonance of the sacroiliac joints (MR-SI), detects a group of inflammatory and structural alterations, non pathognomonic, that contribute to the diagnosis...
Distinctive Treatment, Collective Action
Creators: name: Begeny, Christopher
name: van Breen, Jolien
name: Leach, Colin
name: van Zomeren, Martijn
name: Iyer, Aarti
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Social Psychology
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: Experiences of Distinctive Treatment among Racial/Ethnic Minority Ingroup Members: Effects on Individuals’ Perceived Value to the Group and Willingness to Engage in Collective Action
Carter and Gilovich (2012) replication and extension
Creators: name: Feldman, Gilad
name: Chee, Michelle
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Social and Behavioral Sciences
subject: biases
subject: heuristics
subject: judgement and decision making
subject: replication
subject: replication and extension
subject: social psychology

description: Please see pre-registration folder, with main manuscript and supplementary in Registered Reports Stage 1 style, including simulated datasets and R planned data analysis code.
Promoting Online Civility Through Platform Architecture
Creators: name: Kim, Jisu
name: McDonald, Curtis
name: Meosky, Paul
name: Katsaros, Matthew
name: Tyler, Tom R.
Publisher: name: Singapore Institute of Technology
Year: 2023
Subjects: Human-computer interaction
Communication technology and digital media studies

description: This study tests whether the architecture of a social media platform can encourage conversations among users to be more civil. It was conducted in collaboration with Nextdoor, a networking platform for neighbors within a defined geographic area. The study involved: (1) prompting users to move popular posts from the neighborhood-wide feed to new groups dedicated to the topic and (2) an experiment that randomized the announcement of community guidelines to members who join those newly formed groups. We examined the impact of each intervention on the level of civility, moral values reflected in user comments, and user’s submitted reports of inappropriate content. In a large quantitative analysis of comments posted to Nextdoor, the results indicate that platform architecture can shape the civility of conversations. Comments within groups were more civil and less frequently reported to Nextdoor moderators than the comments on the neighborhood-wide posts. In addition, comments in groups where new members were shown guidelines were less likely to be reported to moderators and were expressed in a more morally virtuous tone than comments in groups where new members were not presented with guidelines. This research demonstrates the importance of considering the design, structure, and affordance of the online environment when online platforms seek to promote civility and other pro-social behaviors.
A catalog of visual-like morphologies in the 5 CANDELS fields using deep-learning
Creators: name: Huertas-Company, M.
name: Gravet, R.
name: Cabrera-Vives, G.
name: Pérez-González, P. G.
name: Kartaltepe, J. S.
name: Barro, G.
name: Bernardi, M.
name: Mei, S.
name: Shankar, F.
name: Dimauro, P.
name: Bell, E. F.
name: Kocevski, D.
name: Koo, D. C.
name: Faber, S. M.
name: Mcintosh, D. H.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a catalog of visual like H-band morphologies of $\sim50.000$ galaxies ($H_{f160w}<24.5$) in the 5 CANDELS fields (GOODS-N, GOODS-S, UDS, EGS and COSMOS). Morphologies are estimated with Convolutional Neural Networks (ConvNets). The median redshift of the sample is $\sim1.25$. The algorithm is trained on GOODS-S for which visual classifications are publicly available and then applied to the other 4 fields. Following the CANDELS main morphology classification scheme, our model retrieves the probabilities for each galaxy of having a spheroid, a disk, presenting an irregularity, being compact or point source and being unclassifiable. ConvNets are able to predict the fractions of votes given a galaxy image with zero bias and $\sim10\%$ scatter. The fraction of miss-classifications is less than $1\%$. Our classification scheme represents a major improvement with respect to CAS (Concentration-Asymmetry-Smoothness)-based methods, which hit a $20-30\%$ contamination limit at high z. The catalog is released with the present paper via the $\href{http://rainbowx.fis.ucm.es/Rainbow_navigator_public}{Rainbow\,database}$
description: Accepted for publication in ApjS. Figure 10 summarizes the excellent agreement between our classification and a pure visual one. Table 3 shows the content of the catalogs. The catalogs are available from the Rainbow database (http://rainbowx.fis.ucm.es/Rainbow_navigator_public) based on the selections from the CANDELS team and cross-matched with 3D-HST v4.1 catalogs
title: Long term results of percutaneous drainage and ethanol sclerotherapy in simple renal cysts with a different type of catheter
Creators: name: Özkan, Mehmet
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Interventional non-vascular
subject: Kidney
subject: Percutaneous
subject: Ablation procedures
subject: Cysts

description: Learning objectives Background Imaging findings OR Procedure details Conclusion References Personal Information
description: Learning objectives: Renal cysts are the most common benign lesions of the kidney .Usually they don't need treatment .Unless pain and related symptoms are occured due to obstruction ,the cysts are required for the treatment.Nowadays the first choice for the cyst...
Agenda Setters, Responders, or Both? Organized Interests and Congressional Agendas
Creators: name: Sykes, Jennifer E.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2009

description: At what point organized interests become involved in the policy process is a matter of debate for scholars. On one side are the interest groups scholars who argue that groups set the agenda and members of Congress respond; at the other end of the spectrum are Congressionalists who give credit to those with power over the formal agenda and relegate organized interests to a responsive position. The compromise approach promoted by some is that both are involved in a muddied process to shape the agenda. By looking at activity both before and after arrival on the formal agenda, I test to see which comes first -- the group, the member, or both? Using three different tests for agenda-setting activity, I discern that both members of Congress and organized interests play a role in agenda-setting, but organized interests play the larger part.
title: ÜBER 20 JAHRE ARIADNE
title: DIE FRAUENSPEZIFISCHE INFORMATION UND DOKUMENTATION AN DER ÖSTERREICHISCHEN NATIONALBIBLIOTHEK
titleType: Subtitle
Creators: name: Jammernegg, Lydia
Publisher: name: Humboldt-Universität zu Berlin
Year: 2016
Subjects: subject: Feminismus
subject: Frauenbewegung
subject: Digitalisierung
subject: 020 Bibliotheks- und Informationswissenschaften
subject: Fraueninformations- und -dokumentationsstelle
subject: Neue Frauenbewegung
subject: Historische Frauenbewegung
subject: feministische Bibliotheksarbeit
subject: Österreichische Nationalbibliothek
subject: Dokumentation
subject: Webportal
subject: Informations- und Dokumentationswissenschaft
subject: Frauenbibliothek

description: 1992 wurde Ariadne als Fraueninformations- und -dokumentationsstelle an der Österreichischen Nationalbibliothek (ÖNB) eingerichtet und arbeitet seitdem sowohl an der dokumentarischen Aufarbeitung des aktuellen frauen-, geschlechterrelevanten und feministischen Literaturbestandes als auch an der Sichtbarmachung des historischen Bestandes der ÖNB zu diesem Themenbereich. In diesem Beitrag geht es darum, die Position von Ariadne im Fraueninformations- und -dokumentationswesen, als Teil der ÖNB, an der Schnittstelle zur Frauenszene, Frauenbewegung, feministischen Szene und zur Frauen- und Geschlechterforschung einer Reflexion zu unterziehen. Nach einer mehr als 20-jährigen Tätigkeit soll ein Rückblick in die Geschichte zeigen, was Ariadne geleistet hat und wo Grenzen liegen, welche Ansprüche und Anliegen Ausgangspunkte für die Arbeit waren und wofür es heute noch frauenspezifische Informations- und Dokumentationseinrichtungen wie Ariadne braucht.
TraceMyFish D3.2 Analysis methodology and performance
Creators: name: Lytou, Anastasia
name: Nychas, George
name: Lemonia-Christina Fengou
name: Aske Schultz Carstensen
name: Genio, Alessia Del
name: Carstensen, Jens Michael
name: Schultz, Nette
name: Lerfall, Jørgen
name: Jakobsen, Anita
name: Kobbenes, Sine Marie Moen
name: Hansen, Marcus Hoff
name: Guðjónsdóttir, Maria
name: Sveinsdóttir, Hildur Inga
Publisher: name: Zenodo
Year: 2023

description: In this Deliverable, the VIDEOMETER spectral imaging technology and data analysis methodology developed in the TMF project is presented. More specifically, descriptions of the two mobile Videometer instruments are provided, including information about the capabilities of the Videometer software and the Videometer workspace. Moreover, different applications are presented by the pilot partners, including the estimation of microbiological quality, changes in fisheye, gills, texture etc., while methodologies on data pre-processing and analysis of acquired images based on a specific problem/task are presented as well.
 More specifically, NTNU partners examined two different analytical approaches for the estimation of salmon fillets color including direct analysis of the fish fillet and analysis of parts of the fillets with specific dimensions placed in a petri dish. In addition to that, the comparison of the performance of the two different Videometer instruments was tested.
 UoI partners focused on the detection of parasites, along with texture, chemical and microbiological measurements.
 AUA partners worked on the assessment of 1. the microbiological quality and freshness 2. Texture profile, 3. Any changes on fish head/eyes using the two imaging analysis instruments. Certain analytical methodologies are presented while a part of the analyses is still in progress.
 The overall results will be presented in the final deliverables of WP6 at the end of the project.
Labeled pupils in the wild: A dataset for studying pupil detection in unconstrained environments
Creators: name: Tonsen, Marc
name: Zhang, Xucong
name: Sugano, Yusuke
name: Bulling, Andreas
Publisher: name: arXiv
Year: 2015
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: We present labelled pupils in the wild (LPW), a novel dataset of 66 high-quality, high-speed eye region videos for the development and evaluation of pupil detection algorithms. The videos in our dataset were recorded from 22 participants in everyday locations at about 95 FPS using a state-of-the-art dark-pupil head-mounted eye tracker. They cover people with different ethnicities, a diverse set of everyday indoor and outdoor illumination environments, as well as natural gaze direction distributions. The dataset also includes participants wearing glasses, contact lenses, as well as make-up. We benchmark five state-of-the-art pupil detection algorithms on our dataset with respect to robustness and accuracy. We further study the influence of image resolution, vision aids, as well as recording location (indoor, outdoor) on pupil detection performance. Our evaluations provide valuable insights into the general pupil detection problem and allow us to identify key challenges for robust pupil detection on head-mounted eye trackers.
title: Lesion conspicuity and image quality of cerebral MDCT scans: comparison of filtered back projection and sinogram affirmed iterative reconstruction
Creators: name: Zizka, Jan
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Technology assessment
subject: Technical aspects
subject: Radiation effects
subject: Image manipulation / Reconstruction
subject: CT
subject: Radioprotection / Radiation dose
subject: Computer applications
subject: CNS
subject: Quality assurance
subject: Biological effects

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Iterative reconstruction (IR) of CT image offers significant image noise reduction when compared to filtered back projection (FBP), thus allowing CT acquisitions of comparable image quality with lower radiation dose. The advantages of iterative...
Continental Distribution of Published Dentistry Citations
Creators: name: Leehacharoenkul, Ron R.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2006

description: The objectives were to (1) determine if article-first-authors (afa) in 8 journals published in 1998 and 2002 affiliated with North America (NA), Europe (EU), Oceania (OC= SE Asia), or other regions cited references with first authors (rfa) with differing frequencies and (2) contrast the influence of journal geographic origin (NA= JDR, JPD, OD, AJD; EU= EJOS, DM, CR, JD) on these patterns. Articles (n=653) and references (excluding case reports, reviews and non-research items) were classified (using ISI and PubMed databases) by first author geographic affiliation. Results for both years (1998, 2002) were identical. Articles from NA and EU cited reference-first-authors from their own continent-of-origin more frequently (p<0.001). Pooled journals (NA versus EU) showed geographic differences. Geographic bias may affect reader impressions of the pertinent literature and distort key indexes of citations such as scientific impact factors.
An extensible lattice Boltzmann method for viscoelastic flows: complex and moving boundaries in Oldroyd-B fluids
Publisher: name: Utrecht University
Year: 2020
Subjects: subject: Natural Sciences - Physical sciences (1.3)
subject: hydrodynamic models
subject: viscoelasticity
subject: lattice-Boltzmann method
subject: microswimmers
subject: numerical techniques

description: This data package contains the outcome of a study to develop a new method for the simulation of colloids suspended in viscoelatic fluids. This includes the implementation itself, scripts for running the validation simulations, and high-resolution data produced during this validation process. This data could serve as a reliable reference for future investigations, and the simulations scripts can easily be customized to study similar systems at parameters and resolutions of interest. The results of the analysis are reported on in the associated publication with the same title https://doi.org/10.1140/epje/s10189-020-00005-6. This data set contains all information necessary to reproduce the graphs in the paper and can be broken down into three categories. The first category (code_data.zip) contains all scripts necessary for graph reproduction using post-processed data. This subset comprises latex, python, and gnuplot scripts. It also contains the C++ source code (for 3-dimensional simulations) and Python scripts (for 2-dimensional simulations) to generate unprocessed data; and the scripts that lead to the post-processed data from which the figures can be generated. The unprocessed data from the two-dimensional simulations is also included. The second category (dataLB.tar.gz) contains the unprocessed data from the three-dimensional simulations. At the top level, a full description is given in the form of a README.md file that details the manner in which the provided scripts may be used to recreate the figures in the paper.

# code_data.zip

* [python-code] Python scripts to discretize Oldroyd-B and to perform the calculations for sections 4.1, 4.2 and 4.3
* [sphere-code] Python scripts and C++ code that perform simulations and analyze them to produce the results for figure 10
* [plots/data] Data as presented in the paper
* everything else: Gnuplot scripts and LaTeX source for the paper and its figures

# dataLB.tar.gz

* LB: Data from the LB simulations

# Software versions used

* Python 3.8.5
* NumPy 1.19.1
* SciPy 1.5.2
* SymPy 1.6.2
* pystencils git hash: 2d75846228efb147b3f1f9af819baf28ba168dc5
* lbmpy git hash: 956c5c44011340e0ea026ddf1035614c507fdc98
* waLBerla git hash: ffe98bd7754c80e53a5507037eb5b00b7e125cca
* gnuplot 5.2 patchlevel 8
* TeX Live 2020
title: Percutaneous irreversible electroporation (IRE) of hepatic malignant tumours: contrast-enhanced ultrasound (CEUS) ﬁndings
Creators: name: Wiggermann, Philipp
Publisher: name: European Congress of Radiology
Year: 2013
Subjects: subject: Liver
subject: MR
subject: CT
subject: Percutaneous
subject: Ablation procedures

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Irreversible electroporation (IRE) is novel non-thermal ablation technique. This technique has shown promise for tissue ablation in the preclinical setting (1,2). Only very limited data exists regarding image findings after ablation (3,4). To the...
Autonomously probing viscoelasticity in disordered suspensions
Publisher: name: Utrecht University
Year: 2020
Subjects: subject: Natural Sciences - Physical sciences (1.3)
subject: Colloidal glass
subject: Microrheology
subject: Microswimmers
subject: Viscoelasticity
subject: Friction

description: Data package for the publication with above title [Phys. Rev. Lett. 125, 258002 (2020); https://link.aps.org/doi/10.1103/PhysRevLett.125.258002]. It contains the full latex directory for compiling the paper, plus the data required to reproduce the graphs for the simulations, as well as the simulation source code and analysis scripts required to process the raw simulation output. In the top-level directory (and various subdirectories) there are readme_use.txt files that describe the content and use of the elements contained therein, e.g., how to run various scripts to obtain the raw simulation data and figures in the paper.

In brief, the data packages contains C++ code for the generation of the passive and active systems [simulations]. Using this source code, passive glassy background systems can be produced, for which the Brownian colloidal particles interact via the Weeks-Chandler-Anderson potential. The active systems contain a single self-propelled probe particle, that additionally interacts with the passive neighbors through a friction criterion. This enables the probe to experience enhanced rotational diffusion, which spikes at a second-order type transition in neighbor contacts. The directory [analysis] contains a mix of C++ codes, Mathematica (10.3), and GNUplot scripts (5.2 patchlevel 2) for the analysis of the data generated using the simulation, such that self-intermediate scattering functions, mean-squared displacements, viscosities, etc. can be obtained from the raw particle coordinates.  Lastly, the directory [data] provides the processed data (ASCII files) and scripts (GNUplot, PowerPoint, and bash) to generate the figures in the main text and supplement.
The 2010 Eruption of the Recurrent Nova U Scorpii: The Multi-Wavelength Light Curve
Creators: name: Pagnotta, Ashley
name: Schaefer, Bradley E.
name: Clem, James L.
name: Landolt, Arlo U.
name: Handler, Gerald
name: Page, Kim L.
name: Osborne, Julian P.
name: Schlegel, Eric M.
name: Hoffman, Douglas I.
name: Kiyota, Seiichiro
name: Maehara, Hiroyuki
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The recurrent nova U Scorpii most recently erupted in 2010. Our collaboration observed the eruption in bands ranging from the Swift XRT and UVOT w2 (193 nm) to K-band (2200 nm), with a few serendipitous observations stretching down to WISE W2 (4600 nm). Considering the time and wavelength coverage, this is the most comprehensively observed nova eruption to date. We present here the resulting multi-wavelength light curve covering the two months of the eruption as well as a few months into quiescence. For the first time, a U Sco eruption has been followed all the way back to quiescence, leading to the discovery of new features in the light curve, including a second, as-yet-unexplained, plateau in the optical and near-infrared. Using this light curve we show that U Sco nearly fits the broken power law decline predicted by Hachisu & Kato, with decline indices of -1.71 +/- 0.02 and -3.36 +/- 0.14. With our unprecedented multi-wavelength coverage, we construct daily spectral energy distributions and then calculate the total radiated energy of the eruption, E_rad=6.99 (+0.83)(-0.57) * 10^44 erg. From that, we estimate the total amount of mass ejected by the eruption to be m_ej=2.10 (+0.24)(-0.17) * 10^-6 M_solar. We compare this to the total amount of mass accreted by U Sco before the eruption, to determine whether the white dwarf undergoes a net mass loss or gain, but find that the values for the amount of mass accreted are not precise enough to make a useful comparison.
description: 10 figures, 5 tables, Published in ApJ
Search for a new heavy gauge boson resonance decaying into a lepton and missing transverse momentum in 36 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} =$ 13 TeV with the ATLAS experiment
Creators: name: ATLAS Collaboration
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2017
Subjects: p p: scattering
p p: colliding beams
gauge boson: resonance
gauge boson: heavy
W': leptonic decay
W': coupling
W': mass: lower limit
transverse momentum: missing-energy
ATLAS
channel cross section: branching ratio: upper limit
CERN LHC Coll
lepton: final state
electron: particle identification
muon: particle identification
experimental results
13000 GeV-cms

description: The results of a search for new heavy $W^\prime$ bosons decaying to an electron or muon and a neutrino using proton-proton collision data at a centre-of-mass energy of $\sqrt{s} = 13$ TeV are presented. The dataset was collected in 2015 and 2016 by the ATLAS experiment at the Large Hadron Collider and corresponds to an integrated luminosity of 36.1 fb$^{-1}$. As no excess of events above the Standard Model prediction is observed, the results are used to set upper limits on the $W^\prime$ boson cross-section times branching ratio to an electron or muon and a neutrino as a function of the $W^\prime$ mass. Assuming a $W^\prime$ boson with the same couplings as the Standard Model $W$ boson, $W^\prime$ masses below 5.1 TeV are excluded at the 95% confidence level.
Period change and stellar evolution of $β$ Cephei stars
Creators: name: Neilson, Hilding R.
name: Ignace, Richard
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The $β$ Cephei stars represent an important class of massive star pulsators probing the evolution of B-type stars and the transition from main sequence to hydrogen-shell burning evolution. By understanding $β$ Cep stars, we gain insights into the detailed physics of massive star evolution such as rotational mixing, convective core overshooting, magnetic fields and stellar winds, all of which play important roles. Similarly, modeling their pulsation provides additional information into their interior structures. Furthermore, measurements of the rate of change of pulsation period offer a direct measure of $β$ Cephei stellar evolution. In this work, we compute state-of-the-art stellar evolution models assuming different amounts of initial rotation and convective core overshoot and measure theoretical rates of period change for which we compare to rates previously measured for a sample of $β$ Cephei stars. The results of this comparison are mixed. For three stars, the rates are too small to infer any information from stellar evolution models, whereas for three other stars the rates are too large. We infer stellar parameters, such as mass and age, for two $β$ Cephei stars: $ξ^1$ CMa and $δ$ Cet, that agree well with independent measurements. We explore ideas for why models may not predict the larger rates of period change. In particular, period drifts in $β$ Cep stars can artificially lead to overestimated rates of secular period change.
description: 6 pages, 2 figures 2 tables, accepted to A&A
More than meets the eye: three African-American women activists in North Carolina
Creators: name: White, Tiffany N.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2009

description: African American women have a rich history as community leaders and activists during slavery, the women's movement and the civil rights movement, but despite their centrality within the black community during these eras, they have received little regard from the mass media. In three articles, this master's thesis examines the activism of three black female activists who work within smaller communities than those typically associated with more well-known activists. These articles represent areas of work historically connected to black women's activism and significance in the black community. The first article looks at a woman's fight for quality housing and her efforts to help others do the same. The second story focuses on an activist's work to create awareness among local Carolinians about Africa. The final story follows the work of a woman who is a trainer in a program that confronts racism and oppression. The thesis aims to provide an in-depth look into the lives of North Carolina's black female activists while simultaneously connecting their activism with efforts of the past.