cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Zero-field dissipationless chiral edge transport and the nature of dissipation in the quantum anomalous Hall state
Creators: name: Chang, Cui-Zu
name: Zhao, Weiwei
name: Kim, Duk Y.
name: Wei, Peng
name: Jain, J. K.
name: Liu, Chaoxing
name: Chan, Moses H. W.
name: Moodera, Jagadeesh S.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The quantum anomalous Hall (QAH) effect is predicted to possess, at zero magnetic field, chiral edge channels that conduct spin polarized current without dissipation. While edge channels have been observed in previous experimental studies of the QAH effect, their dissipationless nature at a zero magnetic field has not been convincingly demonstrated. By a comprehensive experimental study of the gate and temperature dependences of local and nonlocal magnetoresistance, we unambiguously establish the dissipationless edge transport. By studying the onset of dissipation, we also identify the origin of dissipative channels and clarify the surprising observation that the critical temperature of the QAH effect is two orders of magnitude smaller than the Curie temperature of ferromagnetism.
description: main text+supporting materials. This is the accepted version for PRL. Comments are welcome
Methods File 1 from Genomic variation underlying complex life-history traits revealed by genome sequencing in Chinook salmon.
Creators: name: Narum, Shawn R.
name: Genova, Alex Di
name: Micheletti, Steven J.
name: Maass, Alejandro
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60408 Genomics

description: Method details for genome assembly and bioinformatics.
TYPE Iax SUPERNOVAE: A NEW CLASS OF STELLAR EXPLOSION
Creators: name: Jha, S. W.
name: Challis, P. J.
name: Reichart, D. E.
name: Silverman, J. M.
name: Chornock, R.
name: Filippenko, A. V.
name: Marion, G. H.
name: Anderson, J. P.
name: Pignata, G.
name: Kirshner, R. P.
name: Ganeshalingam, M.
name: Li, W.
name: Morrell, N. I.
name: Foley, Ryan J.
name: Phillips, M. M.
name: Stritzinger, M. D.
name: Hamuy, M.
name: Persson, S. E.
name: Wang, X.
name: Soderberg, A. M.
name: Freedman, W. L.
name: McCully, C.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2013

description: We describe observed properties of the Type Iax class of supernovae (SNe Iax), consisting of SNe observationally similar to its prototypical member, SN 2002cx. The class currently has 25 members, and we present optical photometry and/ or optical spectroscopy for most of them. SNe Iax are spectroscopically similar to SNe Ia, but have lower maximum-light velocities (2000 less than or similar to broken vertical bar v broken vertical bar less than or similar to 8000 km s(-1)), typically lower peak magnitudes (-14.2 >= M-V,M-peak greater than or similar to -18.9 mag), and most have hot photospheres. Relative to SNe Ia, SNe Iax have low luminosities for their light-curve shape. There is a correlation between luminosity and light-curve shape, similar to that of SNe Ia, but offset from that of SNe Ia and with larger scatter. Despite a host-galaxy morphology distribution that is highly skewed to late-type galaxies without any SNe Iax discovered in elliptical galaxies, there are several indications that the progenitor stars are white dwarfs (WDs): evidence of C/ O burning in their maximum-light spectra, low (typically similar to 0.5 M-circle dot) ejecta masses, strong Fe lines in their late-time spectra, a lack of X-ray detections, and deep limits on massive stars and star formation at the SN sites. However, two SNe Iax show strong He lines in their spectra. The progenitor system and explosion model that best fits all of the data is a binary system of a C/ O WD that accretes matter from a He star and has a deflagration. At least some of the time, this explosion will not disrupt the WD. The small number of SNe in this class prohibit a detailed analysis of the homogeneity and heterogeneity of the entire class. We estimate that in a given volume there are 31(-13)(+17) SNe Iax for every 100 SNe Ia, and for every 1M(circle dot) of iron generated by SNe Ia at z = 0, SNe Iax generate similar to 0.036M(circle dot). Being the largest class of peculiar SNe, thousands of SNe Iax will be discovered by LSST. Future detailed observations of SNe Iax should further our understanding of both their progenitor systems and explosions as well as those of SNe Ia.
Crossing boundaries between research and practitioner communities: The role of research use and cross-community journal authorship
Creators: name: Taylor, Joseph A.
name: Bowen, G. Michael
name: Kubsch, Marcus
name: Summers, Ryan
name: Sezen-Barrie, Asli
name: Patrick, Patricia
name: Lachapelle, Cathy
name: Warfa, Abdirizak
name: Guzey, S. Selcen
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: academic research impact
subject: citation analysis
subject: knowledge mobilization
subject: research mobilization
subject: researcher–practitioner partnerships
subject: 300 Sozialwissenschaften::370 Bildung und Erziehung::370 Bildung und Erziehung

description: This study pursued two major objectives. The first was to use bibliometric techniques to examine bidirectionality in the relationship between teachers and researchers, as indicated by collaborative authorship among these communities. The second was to explore more deeply knowledge mobilization to classrooms by documenting the extent to which research is cited in science education practitioner journals (SEPJ). Specifically, we examined: (a) the frequency of collaboration between researchers and practitioners in the writing of journal articles for both practitioner-focused and academic journals in science education, and (b) the extent to which authors of articles in practitioner-focused journals drew on academic research to support their advocacy for and/or description of science education programs, policies, or practices. Findings indicate that writing collaborations among academic researchers and practitioners are relatively infrequent, even on practitioner-focused articles. Also, articles in SEPJs more often cite books and other resources over academic journals, even those academic journals focused on informing science education teaching and learning. Recommendations include providing open access to published research, development of research summaries for lay audiences, and incentivizing practitioners to engage in research and writing. This study explores only one mechanism by which knowledge can be mobilized to classrooms and only one type of dissemination product (i.e., journal articles) upon which researchers and practitioners can collaborate. Additional limitations are noted including the applicability of the findings only to the specific journals and timeframes analyzed.
(2087) John Carr
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
Infrared galaxies detected by the Atacama Cosmology Telescope
Creators: name: Kilerci, Ece
name: Hashimoto, Tetsuya
name: Goto, Tomotsugu
name: Göğüş, Ersin
name: Kim, Seong Jin
name: Ho, Simon C. -C.
name: Wong, Yi Hang Valerie
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report on 167 infrared (IR) galaxies selected by AKARI and IRAS and detected in the Atacama Cosmology Telescope (ACT) Data Release 5 (DR5) sky maps at the 98, 150 and 220 GHz frequency bands. Of these detections, 134 (80%) of the millimeter counterparts are first-time identifications with ACT. We expand the previous ACT extragalactic source catalogs, by including new 98 GHz detections and measurements from ACT DR5. We also report flux density measurements at the 98, 150, and 220 GHz frequency bands. We compute $α_{98-150}$, $α_{98-220}$, and $α_{150-220}$ millimeter-wave spectral indices and far-IR to millimeter-wave spectral indices between 90 micron and 98, 150, and 220 GHz. We specify the galaxy type, based on $α_{150-220}$. We combine publicly available multiwavelength data-including ultraviolet, optical, near-IR, mid-IR, far-IR, and the millimeter measurements obtained in this work-and perform spectral energy distribution (SED) fitting with CIGALE. With the radio emission decomposition advantage of CIGALE V2022.0, we identify the origins of the millimeter emissions for 69 galaxies in our sample. Our analysis also shows that millimeter data alone indicates the need for a radio synchrotron component in the SEDs that are produced by active galactic nuclei (AGNs) and/or star formation. We present SEDs and measured physical properties of these galaxies, such as the dust luminosity, AGN luminosity, the total IR luminosity, and the ratio of the IR and radio luminosity. We quantify the relationships between the total IR luminosity and the millimeter-band luminosities, which can be used in the absence of SED analysis.
description: 29 pages, 6 tables, 11 figures, 1 appendix with 1 further figure. Accepted for publication in ApJS
(2088) John Carr Nicholson
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
CHARACTERIZATION OF THE ATMOSPHERE OF THE HOT JUPITER HAT-P-32Ab AND THE M-DWARF COMPANION HAT-P-32B
Creators: name: Fulton, Benjamin J.
name: Riddle, Reed
name: Ngo, Henry
name: Burrows, Adam
name: Zhao, Ming
name: Burruss, Rick
name: Wright, Jason T.
name: Law, Nicholas M.
name: Knutson, Heather A.
name: Muirhead, Philip S.
name: O'Rourke, Joseph G.
name: Curtis, Jason
name: Baranec, Christoph
name: Showman, Adam P.
name: Hinkley, Sasha
name: Fortney, Johnathan
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: We report secondary eclipse photometry of the hot Jupiter HAT-P-32Ab, taken with Hale/WIRC in H and Ks bands and with Spitzer/IRAC at 3.6 and 4.5 micron. We carried out adaptive optics imaging of the planet host star HAT-P-32A and its companion HAT-P-32B in the near-IR and the visible. We clearly resolve the two stars from each other and find a separation of 2.923" +/- 0. 004" and a position angle 110.64 deg +/- 0.12 deg. We measure the flux ratios of the binary in g' r' i' z' and H & Ks bands, and determine Teff = 3565 +/- 82 K for the companion star, corresponding to an M1.5 dwarf. We use PHOENIX stellar atmosphere models to correct the dilution of the secondary eclipse depths of the hot Jupiter due to the presence of the M1.5 companion. We also improve the secondary eclipse photometry by accounting for the non-classical, flux-dependent nonlinearity of the WIRC IR detector in the H band. We measure planet-to-star flux ratios of 0.090 +/- 0.033%, 0.178 +/- 0.057%, 0.364 +/- 0.016%, and 0.438 +/- 0.020% in the H, Ks, 3.6 and 4.5 micron bands, respectively. We compare these with planetary atmospheric models, and find they prefer an atmosphere with a temperature inversion and inefficient heat redistribution. However, we also find that the data are equally well-described by a blackbody model for the planet with Tp = 2042 +/- 50 K. Finally, we measure a secondary eclipse timing offset of 0.3 +/- 1.3 min from the predicted mid-eclipse time, which constrains e = 0.0072 +0.0700/-0.0064 when combined with RV data and is more consistent with a circular orbit.
title: Electoral reform in the former USSR and Russian Federation, 1989-1993: Continuity, contradiction and departure
Creators: name: Lentini, Peter
Publisher: name: University of Glasgow
Year: 1996
Subjects: subject: Russian history, Political science

description: Through an examination of the elections of the USSR Congress of People's Deputies and the elections to the Russian Federal Assembly and their deputy compositions, this dissertation argues that the elections held in the former Soviet Union and the contemporary Russian Federation from 1989-1993 have demonstrated elements of continuity, contradiction and departure compared to those elections held before Mikhail Gorbachev's tenure as General Secretary of the Communist Party of the Soviet Union (CPSU). There has been a continuity of a central, powerful institution interfering and designing the electoral system and largely influencing, encouraging and restricting their outcomes. This continuity can be interpreted as a contradiction between the regime's intention to implement democratic changes and its reform efforts. Notwithstanding these factors, with each successive election there have been numerous innovations, greater scope for candidate competition and subsequently public choice, improved possibilities for civic involvement in all stages of the election campaigns and the opportunity for civil society to become actively involved in political affairs. Therefore, this accumulation of these electoral reform measures has resulted in significant departures from the previous electoral system that existed in the USSR from 1937-late 1980s. These developments have changed the Soviet electoral system from a series of plebiscites in which there was no choice among candidates to elections in which citizens were offered a choice among candidates to, ultimately, multiparty elections.
Fractional order logistic map; Numerical approach
Creators: name: Danca, Marius-F.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Numerical Analysis (math.NA)
subject: Dynamical Systems (math.DS)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: In this paper the fractional order logistic map in the sense of Caputo's fractional differences is numerically approached. It is shown that the necessary iterations number to avoid transients must be of order of thousand, not of order of hundreds as commonly used in several works. Also, it is revealed an interesting phenomenon according to which for every initial condition it correspond a different bifurcation diagram. This phenomenon seems to appear also in other FO difference systems, fact which could represent an obstacle for the numerical analysis. A short Matlab code is used to obtain the results.
description: accepted
Dispersionless propagation of electron wavepackets in single-walled carbon nanotubes
Creators: name: Rosati, Roberto
name: Dolcini, Fabrizio
name: Rossi, Fausto
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate the propagation of electron wavepackets in single-walled carbon nanotubes via a Lindblad-based density-matrix approach that enables us to account for both dissipation and decoherence effects induced by various phonon modes. We show that, while in semiconducting nanotubes the wavepacket experiences the typical dispersion of conventional materials, in metallic nanotubes its shape remains essentially unaltered, even in the presence of the electron-phonon coupling, up to micron distances at room temperature.
description: 4 pages, 2 figures, accepted by Appl. Phys. Lett
Martin et al. 2018 Supplementary Methods from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range.
Creators: name: Martin, Morgan J.
name: Gridley, Tess
name: Elwen, Simon H.
name: Jensen, Frants H.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60801 Animal Behaviour

description: Supplementary Methods include detail on the statistical analyses conducted for classifying the pulsed signal types of Heaviside's dolphins. Also, these methods contain the relevant information, steps and figures used in the acoustic modelling of the detection range and active space of a NBHF click compared to a lower-frequency burst-pulse click.
Remote Sensing Image Super-resolution and Object Detection: Benchmark and State of the Art
Creators: name: Wang, Yi
name: Bashir, Syed Muhammad Arsalan
name: Khan, Mahrukh
name: Ullah, Qudrat
name: Wang, Rui
name: Song, Yilin
name: Guo, Zhe
name: Niu, Yilong
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: For the past two decades, there have been significant efforts to develop methods for object detection in Remote Sensing (RS) images. In most cases, the datasets for small object detection in remote sensing images are inadequate. Many researchers used scene classification datasets for object detection, which has its limitations; for example, the large-sized objects outnumber the small objects in object categories. Thus, they lack diversity; this further affects the detection performance of small object detectors in RS images. This paper reviews current datasets and object detection methods (deep learning-based) for remote sensing images. We also propose a large-scale, publicly available benchmark Remote Sensing Super-resolution Object Detection (RSSOD) dataset. The RSSOD dataset consists of 1,759 hand-annotated images with 22,091 instances of very high resolution (VHR) images with a spatial resolution of ~0.05 m. There are five classes with varying frequencies of labels per class. The image patches are extracted from satellite images, including real image distortions such as tangential scale distortion and skew distortion. We also propose a novel Multi-class Cyclic super-resolution Generative adversarial network with Residual feature aggregation (MCGR) and auxiliary YOLOv5 detector to benchmark image super-resolution-based object detection and compare with the existing state-of-the-art methods based on image super-resolution (SR). The proposed MCGR achieved state-of-the-art performance for image SR with an improvement of 1.2dB PSNR compared to the current state-of-the-art NLSN method. MCGR achieved best object detection mAPs of 0.758, 0.881, 0.841, and 0.983, respectively, for five-class, four-class, two-class, and single classes, respectively surpassing the performance of the state-of-the-art object detectors YOLOv5, EfficientDet, Faster RCNN, SSD, and RetinaNet.
description: 39 pages, 15 figures, 5 tables. Submitted to Elsevier journal for review
FINGERING CONVECTION INDUCED BY ATOMIC DIFFUSION IN STARS: 3D NUMERICAL COMPUTATIONS AND APPLICATIONS TO STELLAR MODELS
Creators: name: Zemskova, Varvara
name: Deal, Morgan
name: Vauclair, Sylvie
name: Garaud, Pascale
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: Iron-rich layers are known to form in the stellar subsurface through a combination of gravitational settling and radiative levitation. Their presence, nature and detailed structure can affect the excitation process of various stellar pulsation modes, and must therefore be modeled carefully in order to better interpret Kepler asteroseismic data. In this paper, we study the interplay between atomic diffusion and fingering convection in A-type stars, and its role in the establishment and evolution of iron accumulation layers. To do so, we use a combination of three-dimensional idealized numerical simulations of fingering convection, and one-dimensional realistic stellar models. Using the three-dimensional simulations, we first validate the mixing prescription for fingering convection recently proposed by Brown et al. (2013), and identify what system parameters (total mass of iron, iron diffusivity, thermal diffusivity, etc.) play a role in the overall evolution of the layer. We then implement the Brown et al. (2013) prescription in the Toulouse-Geneva Evolution code to study the evolution of the iron abundance profile beneath the stellar surface. We find, as first discussed by Th\'eado et al. (2009), that when the concurrent settling of helium is ignored, this accumulation rapidly causes an inversion in the mean molecular weight profile, which then drives fingering convection. The latter mixes iron with the surrounding material very efficiently, and the resulting iron layer is very weak. However, taking helium settling into account partially stabilizes the iron profile against fingering convection, and a large iron overabundance can accumulate. The opacity also increases significantly as a result, and in some cases ultimately triggers dynamical convection.
Methods File 1 from Genomic variation underlying complex life-history traits revealed by genome sequencing in Chinook salmon
Creators: name: Narum, Shawn R.
name: Genova, Alex Di
name: Micheletti, Steven J.
name: Maass, Alejandro
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60408 Genomics

description: Method details for genome assembly and bioinformatics.
Additional file 1 of Retrospective study of canine cutaneous tumors submitted to a diagnostic pathology laboratory in Northern Portugal (2014–2020)
Creators: name: Martins, Ana Luísa
name: Canadas-Sousa, Ana
name: Mesquita, João R.
name: Dias-Pereira, Patrícia
name: Amorim, Irina
name: Gärtner, Fátima
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 1: Figure S1. Age distribution according to tumor types
title: Zwischen Humanitarismus und Zivilisierung
title: Eine deutsch-portugiesische kritische Edition von Hugo Genschs „Die Erziehung eines Indianerkindes“ (1908)
titleType: Subtitle
Creators: name: Rinke, Stefan
name: Kriegesmann, Karina
Publisher: name: Freie Universität Berlin
Year: 2024
Subjects: subject: Historamericana
subject: Deutschland
subject: Hugo Gensch
subject: Zivilisierung
subject: Xokleng
subject: Kaingang
subject: Indigene
subject: Genozid
subject: Immigration
subject: Bildung
subject: Ethnologie
subject: Kolonisten
subject: Humanitarismus
subject: Gewalt
subject: Erziehung eines Indianerkindes
subject: 900 Geschichte und Geografie::980 Geschichte Südamerikas::980 Geschichte Südamerikas

description: Hugo Gensch, ein Arzt in der von deutschen Immigrant:innen gegründeten Kolonie Blumenau in Südbrasilien, erläuterte in seiner 1908 veröffentlichten Studie, wie es ihm ungeachtet der Kritik und Zweifel mancher seiner Zeitgenossen gelungen sei, sein Adoptivkind Korikrá, ein junges Xokleng-Mädchen, zu erziehen. Er nahm sie in seine Familie und Gemeinde auf und konnte zudem von ihr lernen und so sein Wissen über verschiedene Ethnien in Brasilien erweitern. Mit dieser im Vergleich zu anderen Kolonist:innen und auch Akademiker:innen verhältnismäßig humanen und überwiegend von wissenschaftlichen Interessen und Engagement geleiteten Einstellung gehörte Gensch zu Beginn des 20. Jahrhunderts zu einem kleinen Kreis von Personen, die sich gegen den blutigen Kampf und die Tötung der Indigenen aussprachen. Dieser Band beinhaltet erstmals eine kritische Edition von Genschs Werk „Die Erziehung eines Indianerkindes: Praktischer Beitrag zur Lösung der südamerikanischen Indianerfrage“ samt einer Übersetzung ins Portugiesische. Er umfasst eine Einführung in die Geschichte der indigenen Bevölkerungsgruppen Südbrasiliens und der transatlantischen Migrationsbewegungen in die Region seit dem 19. Jahrhundert. Darüber hinaus werden die Auseinandersetzungen zwischen den verschiedenen Interessengruppen und die unterschiedlichen Positionen in wissenschaftlichen Kreisen skizziert. Auch werden Genschs Leben, Wirken und Ansichten dargelegt, um seine Ausführungen einordnen zu können. Der Band umfasst die Originalquelle sowie weitere Erläuterungen insbesondere zu zeitgenössischen Begriffen in Form von Endnoten. Ein Quellen- und Literaturverzeichnis, eine Chronologie, ein Register und eine Karte runden die Edition ab.
ROBOTIC LASER ADAPTIVE OPTICS IMAGING OF 715 KEPLER EXOPLANET CANDIDATES USING ROBO-AO
Creators: name: Ravichandran, Ganesh
name: Morton, Tim
name: Johnson, John Asher
name: Bui, Khanh
name: Das, H. K.
name: Punnadi, Sujit
name: Burse, Mahesh P.
name: Baranec, Christoph
name: Ziegler, Carl
name: Ramaprakash, A. N.
name: Tendulkar, Shriharsh P.
name: Dekany, Richard G.
name: Kulkarni, Shrinivas
name: Riddle, Reed
name: Law, Nicholas M.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: The Robo-AO Kepler Planetary Candidate Survey is designed to observe every Kepler planet candidate host star with laser adaptive optics imaging to search for blended nearby stars, which may be physically associated companions and/or responsible for transit false positives. In this paper we present the results from the 2012 observing season, searching for stars close to 715 representative Kepler planet candidate hosts. We find 53 companions, 44 of which are new discoveries. We detail the Robo-AO survey data reduction methods including a method of using the large ensemble of target observations as mutual point-spread-function references, along with a new automated companion-detection algorithm designed for large adaptive optics surveys. Our survey is sensitive to objects from 0.15" to 2.5" separation, with contrast ratios up to delta-m~6. We measure an overall nearby-star-probability for Kepler planet candidates of 7.4% +/- 1.0%, and calculate the effects of each detected nearby star on the Kepler-measured planetary radius. We discuss several KOIs of particular interest, including KOI-191 and KOI-1151, which are both multi-planet systems with detected stellar companions whose unusual planetary system architecture might be best explained if they are "coincident multiple" systems, with several transiting planets shared between the two stars. Finally, we detect 2.6-sigma evidence for <15d-period giant planets being 2-3 times more likely be found in wide stellar binaries than smaller close-in planets and all sizes of further-out planets.
title: Propositions for a Place-Based Practice: Implicating the Designer in Care and Relationality
Creators: name: Chisholm, Catherine Jean
Publisher: name: Emily Carr University of Art and Design
Year: 2020
Subjects: subject: Design
valueUri: http://id.loc.gov/authorities/subjects/sh85037197
subject: Relationism
valueUri: http://id.loc.gov/authorities/subjects/sh85112489
subject: Communities
valueUri: http://id.loc.gov/authorities/subjects/sh85029195

description: This thesis reflects on the role of the designer within a place-based practice, exploring the implications of being knowingly and intentionally embedded within community and building a design practice rooted in relationality and reciprocity. Propositions for a place-based practice emerged from a methodology of material and collaborative making, as examined through three case studies (two completed, one proposed) within Prince George and Vancouver, Canada.
(2083) John Webster Nicholson
Creators: name: Professions, Victorian
Publisher: name: University of Oxford
Year: 2022
Subjects: subject: 220201 Business and Labour History
subject: FOS: Philosophy, ethics and religion
subject: History
subject: 140203 Economic History
subject: FOS: Economics and business

description: This three-year research project began in January 2014 and investigated whether, during the Victorian period, the professions formed a distinct self-sustaining social group with its own mores and values. The project looked at 16,000 individuals drawn from census data for Alnwick, Brighton, Bristol, Dundee, Greenock, Leeds, Merthyr Tydfil, Morpeth, and Winchester. The research project was funded by the UK Economic & Social Research Council and was based at the Universities of Oxford and Northumbria.
SUPERNOVA 2010as: THE LOWEST-VELOCITY MEMBER OF A FAMILY OF FLAT-VELOCITY TYPE IIb SUPERNOVAE
Creators: name: Nomoto, Ken'Ichi
name: Lacluyze, Aaron P.
name: Folatelli, Gastón
name: Anderson, Joseph P.
name: Olivares Estay, Felipe
name: Greiner, Jochen
name: Prieto, José Luis
name: Hamuy, Mario
name: Kuncarayakti, Hanindyo
name: Altenmüller, Konrad
name: Förster, Francisco
name: Contreras, Carlos
name: Stritzinger, Maximilian
name: Updike, Adria
name: Maeda, Keiichi
name: Moore, Justin P.
name: Pignata, Giuliano
name: Holmbo, Simon
name: Valenti, Stefano
name: Bersten, Melina C.
name: Elliott, Jonny
name: Afonso, Paulo
name: Haislip, Joshua B.
name: Reichart, Daniel E.
name: Phillips, Mark M.
name: Morrell, Nidia
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: We present extensive optical and near-infrared photometric and spectroscopic observations of the stripped-envelope supernova SN 2010as. Spectroscopic peculiarities such as initially weak helium features and low expansion velocities with a nearly flat evolution place this object in the small family of events previously identified as transitional Type Ib/c supernovae (SNe). There is ubiquitous evidence of hydrogen, albeit weak, in this family of SNe, indicating that they are in fact a peculiar kind of Type IIb SNe that we name "flat-velocity Type IIb. The flat-velocity evolution—which occurs at different levels between 6000 and 8000 km s–1 for different SNe—suggests the presence of a dense shell in the ejecta. Despite the spectroscopic similarities, these objects show surprisingly diverse luminosities. We discuss the possible physical or geometrical unification picture for such diversity. Using archival Hubble Space Telescope images, we associate SN 2010as with a massive cluster and derive a progenitor age of ≈6 Myr, assuming a single star-formation burst, which is compatible with a Wolf-Rayet progenitor. Our hydrodynamical modeling, on the contrary, indicates that the pre-explosion mass was relatively low, ≈4 M ☉. The seeming contradiction between a young age and low pre-SN mass may be solved by a massive interacting binary progenitor.
Martin et al. 2018 Supplementary Methods from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range
Creators: name: Martin, Morgan J.
name: Gridley, Tess
name: Elwen, Simon H.
name: Jensen, Frants H.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60801 Animal Behaviour

description: Supplementary Methods include detail on the statistical analyses conducted for classifying the pulsed signal types of Heaviside's dolphins. Also, these methods contain the relevant information, steps and figures used in the acoustic modelling of the detection range and active space of a NBHF click compared to a lower-frequency burst-pulse click.
title: Cytokines in the immunopathogenesis of murine graft-versus-host disease
Creators: name: Williamson, Eilidh
Publisher: name: University of Glasgow
Year: 1997

description: Murine models of graft-versus-host disease (GvHD) provide important information relevant to clinical bone marrow transplantation (BMT), as well as to other types of T cell-mediated pathology. The nature of the GvHD which develops in (C57BL/6 X DBA/2)F1 (BDF1) mice injected with parental lymphocytes is dependent on whether C57B1/6 (B6) or DBA/2 parental donor cells are used. BDF1 mice injected with B6 donor cells (B6 => BDF1) develop an acute GvHD with early lymphoid hyperplasia and NK cell activation, followed by immunosuppression, activation of anti-host cytotoxic T lymphocytes (CTL), weight loss and early death. In contrast, BDF1 mice given DBA/2 donor cells (DBA/2 => BDF1) exhibit a chronic, stimulatory GvHD, characterised by B cell hyperreactivity, autoantibody production and immune complex-mediated glomerulonephritis (ICGN). Previous studies have shown that the distinct forms of GvHD in BDF1 recipient mice are associated with different patterns of cytokine production. Whereas acute GvHD is characterised by production of high levels of Th1 cytokines, chronic GvHD is associated with a preferential Th2 response. Therefore, it was suggested that the two forms of GvHD may reflect differential activation of distinct subsets of CD4+ T helper (Th) cells. However, when and why such T cell polarisation should occur has remained unclear. A number of recent studies have demonstrated that cytokines produced by cells of the non-specific immune system during the early phase of an immune response can strongly influence the type of specific response which develops subsequently. The main aim of this thesis was to explore the role of these early immune mediators in determining the outcome of the GvHD in BDF1 mice. These studies of the cellular and molecular interactions involved in murine GvHD have implications for understanding the pathogenesis of clinical GvHD and the development of specific therapy following BMT. In addition, they provide an important insight into the regulation of immune responses during other immunologically-mediated diseases.
TESTING MONDian DARK MATTER WITH GALACTIC ROTATION CURVES
Creators: name: Minic, Djordje
name: Takeuchi, Tatsu
name: Farrah, Duncan
name: Edmonds, Doug
name: Ho, Chiu Man
name: Ng, Y. Jack
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: MONDian dark matter (MDM) is a new form of dark matter quantum that naturally accounts for Milgrom's scaling, usually associated with modified Newtonian dynamics (MOND), and theoretically behaves like cold dark matter (CDM) at cluster and cosmic scales. In this paper, we provide the first observational test of MDM by fitting rotation curves to a sample of 30 local spiral galaxies (z approximately 0.003). For comparison, we also fit the galactic rotation curves using MOND, and CDM. We find that all three models fit the data well. The rotation curves predicted by MDM and MOND are virtually indistinguishable over the range of observed radii (~1 to 30 kpc). The best-fit MDM and CDM density profiles are compared. We also compare with MDM the dark matter density profiles arising from MOND if Milgrom's formula is interpreted as Newtonian gravity with an extra source term instead of as a modification of inertia. We find that discrepancies between MDM and MOND will occur near the center of a typical spiral galaxy. In these regions, instead of continuing to rise sharply, the MDM mass density turns over and drops as we approach the center of the galaxy. Our results show that MDM, which restricts the nature of the dark matter quantum by accounting for Milgrom's scaling, accurately reproduces observed rotation curves.
Martin et al. 2018 Appendix S1 from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range.
Creators: name: Martin, Morgan J.
name: Gridley, Tess
name: Elwen, Simon H.
name: Jensen, Frants H.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60801 Animal Behaviour

description: Appendix S1 contains the parameter measurements for all measured Heaviside's dolphin pulsed signals.
Thickness-dependent magnetic properties and strain-induced orbital magnetic moment in SrRuO3 thin films
Creators: name: Ishigami, K.
name: Yoshimatsu, K.
name: Toyota, D.
name: Takizawa, M.
name: Yoshida, T.
name: Shibata, G.
name: Harano, T.
name: Takahashi, Y.
name: Kadono, T.
name: Verma, V. K.
name: Singh, V. R.
name: Takeda, Y.
name: Okane, T.
name: Saitoh, Y.
name: Yamagami, H.
name: Koide, T.
name: Oshima, M.
name: Kumigashira, H.
name: Fujimori, A.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Thin films of the ferromagnetic metal SrRuO3 (SRO) show a varying easy magnetization axis depending on the epitaxial strain and undergo a metal-to-insulator transition with decreasing film thickness. We have investigated the magnetic properties of SRO thin films with varying thicknesses fabricated on SrTiO3(001) substrates by soft x-ray magnetic circular dichroism (XMCD) at the Ru M2,3 edge. Results have shown that, with decreasing film thickness, the film changes from ferromagnetic to non-magnetic around 3monolayer thickness, consistent with previous magnetization and magneto-optical Kerr effect measurements. The orbital magnetic moment perpendicular to the film was found to be ~ 0.1μB/Ru atom, and remained nearly unchanged with decreasing film thickness while the spin magnetic moment decreases. Mechanism for the formation of the orbital magnetic moment is discussed based on the electronic structure of the compressively strained SRO film.
description: 6 pages, 6 figures, Submitted in Phys. Rev. B
title: Συγκόλληση δια τριβής με ανάδευση ανόμοιων υλικών-Ενίσχυση με κεραμικά νανοσωματίδια
title: Dissimilar friction stir welding-reinforcing by ceramic nanoparticles
titleType: AlternativeTitle
Creators: name: Κρανιάς, Βασίλειος
Publisher: name: Πανεπιστήμιο Δυτικής Αττικής
Year: 2024
Subjects: Συγκόλληση δια τριβής με ανάδευση

description: Το πρώτο κεφάλαιο αναφέρεται στη σημασία της νανοτεχνολογίας, εξετάζοντας τον χειρισμό της ύλης στη νανοκλίμακα. Δίνονται βασικές πληροφορίες για τους διάφορους τύπους και τις ταξινομήσεις των νανοσωματιδίων (ΝΡs). Επίσης, γίνεται αναφορά στις μοναδικές φυσικοχημικές ιδιότητές των νανοσωματιδίων, συμπεριλαμβανομένων των μηχανικών, θερμικών και μαγνητικών χαρακτηριστικών τους. Ακόμη, γίνεται αναφορά στην αναγκαιότητα της νανοτεχνολογίας, ιδιαίτερα στον τομέα της ναυτιλίας. Το δεύτερο κεφάλαιο περιγράφει τη συγκόλληση δια τριβής με ανάδευση (FSW), μια τεχνική με προοπτικές περαιτέρω εφαρμογής στη ναυπηγική βιομηχανία, παρέχοντας μια ολοκληρωμένη επισκόπηση της ιστορικής της εξέλιξης, των βασικών αρχών, της διαδικασίας και του εξοπλισμού της. Το κεφάλαιο αυτό εξετάζει επίσης τα ελαττώματα που μπορεί να εμφανιστούν κατά τη διάρκεια της FSW και τις μεθόδους ανίχνευσής τους. Κλείνοντας, γίνεται παρουσίαση των πλεονεκτημάτων και των μειονεκτημάτω της FSW, καθώς πιθανές εφαρμογές της στη ναυπηγική βιομηχανία. Στο τρίτο κεφάλαιο, περιγράφονται οι βασικές αρχές της ενίσχυσης της συγκόλλησης με κεραμικά νανοσωματίδια με τη μέθοδο της FSW. Περιγράφοντας λεπτομερώς τη διαδικασία, αναλύονται οι μηχανικές ιδιότητες των συγκολλήσεων που προκύπτουν και παρουσιάζονται μελέτες περιπτώσεων συγκόλλησης FSW μεταξύ συγκεκριμένων ναυπηγικών κραμάτων αλουμινίου ενισχυμένων με νανοσωματίδια TiC και SiC. Στην ενότητα αυτή παρέχεται μια ολοκληρωμένη περιγραφή της πειραματικής διαδικασίας, των αποτελεσμάτων, των συμπερασμάτων και των παρατηρήσεων που προέκυψαν από τη μελέτη. Το τέταρτο κεφάλαιο αναφέρεται στις εφαρμογές, στη ναυπηγική βιομηχανία, της συγκόλλησης FSW ανόμοιων υλικών. Επιπλέον, εξετάζεται η συμπεριφορά κόπωσης των συγκολλήσεων FSW για χάλυβα υψηλής αντοχής μέσω δοκιμών κόπωσης. Στο πέμπτο κεφάλαιο διερευνώνται οι πρόσφατες εξελίξεις στην FSW, σε σχέση με την τρισδιάστατη εκτύπωση και την υβριδική συγκόλληση FSW (ΗFSW). Μελέτες περιπτώσεων, όπως η εφαρμογή της ΗFSW σε κράματα αλουμινίου και χάλυβα, αναλύονται ως προς τα επιφανειακά και μηχανικά χαρακτηριστικά τους. Τέλος, το έκτο κεφάλαιο παρουσιάζει τις προκλήσεις και τις μελλοντικές προοπτικές στην ναυτιλία, περιγράφοντας την τρέχουσα κατάσταση και των πιθανών εξελίξεων στις συγκολλήσεις FSW για τη ναυπηγική βιομηχανία.
THE FACTORY AND THE BEEHIVE. II. ACTIVITY AND ROTATION IN PRAESEPE AND THE HYADES
Creators: name: Kraus, A.
name: Cargile, P. A.
name: Law, N. M.
name: Arce, H. G.
name: Agüeros, M. A.
name: Douglas, S. T.
name: Fierroz, D. F.
name: Bochanski, J. J.
name: Bowsher, E. C.
name: Lemonias, J. J.
name: Kundert, A.
name: Covey, K. R.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: Open clusters are collections of stars with a single, well-determined age, and can be used to investigate the connections between angular-momentum evolution and magnetic activity over a star's lifetime. We present the results of a comparative study of the relationship between stellar rotation and activity in two benchmark open clusters: Praesepe and the Hyades. As they have the same age and roughly solar metallicity, these clusters serve as an ideal laboratory for testing the agreement between theoretical and empirical rotation-activity relations at approximate to 600 Myr. We have compiled a sample of 720 spectra-more than half of which are new observations-for 516 high-confidence members of Praesepe; we have also obtained 139 new spectra for 130 high-confidence Hyads. We have also collected rotation periods (P-rot) for 135 Praesepe members and 87 Hyads. To compare H alpha emission, an indicator of chromospheric activity, as a function of color, mass, and Rossby number R-o, we first calculate an expanded set of chi values, with which we can obtain the H alpha to bolometric luminosity ratio, L-H alpha/L-bol, even when spectra are not flux-calibrated and/or stars lack reliable distances. Our. values cover a broader range of stellar masses and colors (roughly equivalent to spectral types from K0 to M9), and exhibit better agreement between independent calculations, than existing values. Unlike previous authors, we find no difference between the two clusters in their H alpha equivalent width or L-H alpha/L-bol distributions, and therefore take the merged H alpha and Prot data to be representative of 600 Myr old stars. Our analysis shows that H alpha activity in these stars is saturated for R-o <= 0.11(-0.03)(+0.02) Above that value activity declines as a power-law with slope beta = -0.73(-0.12,)(+0.06) before dropping off rapidly at Ro approximate to 0.4. These data provide a useful anchor for calibrating the age-activity-rotation relation beyond 600 Myr.
Additional file 2 of Retrospective study of canine cutaneous tumors submitted to a diagnostic pathology laboratory in Northern Portugal (2014–2020)
Creators: name: Martins, Ana Luísa
name: Canadas-Sousa, Ana
name: Mesquita, João R.
name: Dias-Pereira, Patrícia
name: Amorim, Irina
name: Gärtner, Fátima
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 2: Table S1. Number (n) and frequency (%) of the breeds from the Canine population in the database, 2014-2020 used in the calculations for occurrence within breed. Table S2. Binary logistic regression analysis showing the association of cutaneous tumors development with age. sex. and specific breed
THE TYPE IIP SUPERNOVA 2012aw IN M95: HYDRODYNAMICAL MODELING OF THE PHOTOSPHERIC PHASE FROM ACCURATE SPECTROPHOTOMETRIC MONITORING
Creators: name: Fraser, M.
name: Cappellaro, E.
name: Iijima, T.
name: Benitez, S.
name: Phillips, M. M.
name: Pritchard, T. A.
name: Harutyunyan, A.
name: Zampieri, L.
name: Sollerman, J.
name: Della Valle, M.
name: Kankare, E.
name: Patat, F.
name: Howell, D. A.
name: Siviero, A.
name: Ochner, P.
name: Inserra, C.
name: Taubenberger, S.
name: Benetti, S.
name: Tomasella, L.
name: Hsiao, E. Y.
name: Pignata, G.
name: Haislip, J. B.
name: Roming, P. W.A.
name: Maund, J. R.
name: Elias-Rosa, N.
name: Bayless, A. J.
name: Valenti, S.
name: Munari, U.
name: Kotak, R.
name: Bufano, F.
name: Taddia, F.
name: Smartt, S. J.
name: Wright, D.
name: Botticella, M. T.
name: Reichart, D.
name: Pastorello, A.
name: Kuin, P.
name: Morales-Garoffolo, A.
name: Morrell, N.
name: Pumo, M. L.
name: Dall'Ora, M.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2014

description: We present an extensive optical and near-infrared photometric and spectroscopic campaign of the Type IIP supernova SN 2012aw. The data set densely covers the evolution of SN 2012aw shortly after th ...
Martin et al. 2018 Appendix S1 from Heaviside's dolphins (Cephalorhynchus heavisidii) relax acoustic crypsis to increase communication range
Creators: name: Martin, Morgan J.
name: Gridley, Tess
name: Elwen, Simon H.
name: Jensen, Frants H.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60801 Animal Behaviour

description: Appendix S1 contains the parameter measurements for all measured Heaviside's dolphin pulsed signals.
A SURVEY OF THE HIGH ORDER MULTIPLICITY OF NEARBY SOLAR-TYPE BINARY STARS WITH Robo-AO
Creators: name: Mason, Brian D.
name: Tokovinin, Andrei
name: Burse, Mahesh P.
name: Dekany, Richard G.
name: Hartkopf, William I.
name: Das, H. K.
name: Kulkarni, Shrinivas
name: Law, Nicholas M.
name: Tendulkar, Shriharsh P.
name: Punnadi, Sujit
name: Bui, Khanh
name: Riddle, Reed L.
name: Ramaprakash, A. N.
name: Baranec, Christoph
name: Roberts, Lewis C.
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2015

description: We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive optics instrument, we collected high angular resolution images with deep and well-defined detection limits in the SDSS $i'$ band. A total of 695 components belonging to 595 systems were observed. We prioritized observations of faint secondary components with separations over $10''$ to quantify the still poorly constrained frequency of their sub-systems. Of the 214 secondaries observed, 39 contain such subsystems; 19 of those were discovered with Robo-AO. The selection-corrected frequency of secondary sub-systems with periods from $10^{3.5}$ to $10^5$ days is 0.12$\pm$0.03, the same as the frequency of such companions to the primary. Half of the secondary pairs belong to quadruple systems where the primary is also a close pair, showing that the presence of sub-systems in both components of the outer binary is correlated. The relatively large abundance of 2+2 quadruple systems is a new finding, and will require more exploration of the formation mechanism of multiple star systems. We also targeted close binaries with periods less than 100~yr, searching for their distant tertiary components, and discovered 17 certain and 2 potential new triples. In a sub-sample of 241 close binaries, 71 have additional outer companions. The overall frequency of tertiary components is not enhanced, compared to all (non-binary) targets, but in the range of outer periods from $10^6$ to $10^{7.5}$ days (separations on the order of 500~AU), the frequency of tertiary components is 0.16$\pm$0.03, exceeding by almost a factor of two the frequency of similar systems among all targets (0.09).