cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unsupervised Segmentation of 3D Medical Images Based on Clustering and Deep Representation Learning
Creators: name: Moriya, Takayasu
name: Roth, Holger R.
name: Nakamura, Shota
name: Oda, Hirohisa
name: Nagara, Kai
name: Oda, Masahiro
name: Mori, Kensaku
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: This paper presents a novel unsupervised segmentation method for 3D medical images. Convolutional neural networks (CNNs) have brought significant advances in image segmentation. However, most of the recent methods rely on supervised learning, which requires large amounts of manually annotated data. Thus, it is challenging for these methods to cope with the growing amount of medical images. This paper proposes a unified approach to unsupervised deep representation learning and clustering for segmentation. Our proposed method consists of two phases. In the first phase, we learn deep feature representations of training patches from a target image using joint unsupervised learning (JULE) that alternately clusters representations generated by a CNN and updates the CNN parameters using cluster labels as supervisory signals. We extend JULE to 3D medical images by utilizing 3D convolutions throughout the CNN architecture. In the second phase, we apply k-means to the deep representations from the trained CNN and then project cluster labels to the target image in order to obtain the fully segmented image. We evaluated our methods on three images of lung cancer specimens scanned with micro-computed tomography (micro-CT). The automatic segmentation of pathological regions in micro-CT could further contribute to the pathological examination process. Hence, we aim to automatically divide each image into the regions of invasive carcinoma, noninvasive carcinoma, and normal tissue. Our experiments show the potential abilities of unsupervised deep representation learning for medical image segmentation.
description: This paper was presented at SPIE Medical Imaging 2018, Houston, TX, USA
The star formation histories of low surface brightness galaxies
Creators: name: Bell, Eric F.
name: Barnaby, David
name: Bower, Richard G.
name: de Jong, Roelof S.
name: Harper, Doyal A.
name: Hereld, Mark
name: Loewenstein, Robert F.
name: Rauscher, Bernard J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have performed deep imaging of a diverse sample of 26 low surface brightness galaxies (LSBGs) in the optical and the near-infrared. Using stellar population synthesis models, we find that it is possible to place constraints on the ratio of young to old stars (which we parameterise in terms of the average age of the galaxy), as well as the metallicity of the galaxy, using optical and near-infrared colours. LSBGs have a wide range of morphologies and stellar populations, ranging from older, high metallicity earlier types to much younger and lower metallicity late type galaxies. Despite this wide range of star formation histories, we find that colour gradients are common in LSBGs. These are most naturally interpreted as gradients in mean stellar age, with the outer regions of LSBGs having younger ages than their inner regions. In an attempt to understand what drives the differences in LSBG stellar populations, we compare LSBG average ages and metallicities with their physical parameters. Strong correlations are seen between a LSBG's star formation history and its K band surface brightness, K band absolute magnitude and gas fraction. These correlations are consistent with a scenario in which the star formation history of a LSBG primarily correlates with its surface density and its metallicity correlates both with its mass and surface density.
description: 29 pages; 5 figures; re-submitted to MNRAS after replying to referee's report
The stellar populations of spiral galaxies
Creators: name: Bell, Eric F.
name: de Jong, Roelof S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used a large sample of low-inclination spiral galaxies with radially-resolved optical and near-infrared photometry to investigate trends in star formation history with radius as a function of galaxy structural parameters. A maximum likelihood method was used to match all the available photometry of our sample to the colours predicted by stellar population synthesis models. The use of simplistic star formation histories, uncertainties in the stellar population models and regarding the importance of dust all compromise the absolute ages and metallicities derived in this work, however our conclusions are robust in a relative sense. We find that most spiral galaxies have stellar population gradients, in the sense that their inner regions are older and more metal rich than their outer regions. Our main conclusion is that the surface density of a galaxy drives its star formation history, perhaps through a local density dependence in the star formation law. The mass of a galaxy is a less important parameter; the age of a galaxy is relatively unaffected by its mass, however the metallicity of galaxies depends on both surface density and mass. This suggests that galaxy mass-dependent feedback is an important process in the chemical evolution of galaxies. In addition, there is significant cosmic scatter suggesting that mass and density may not be the only parameters affecting the star formation history of a galaxy.
description: 25 pages; 17 figures; re-submitted to MNRAS after replying to referee's report
Additional file 2: of Safety and tolerability of quizartinib, a FLT3 inhibitor, in advanced solid tumors: a phase 1 dose-escalation trial
Creators: name: Papadopoulos, Kyriakos
name: Ben-Ami, Eytan
name: Patnaik, Amita
name: Trone, Denise
name: Jianke Li
name: Demetri, George
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Most common (reported in â Ľ2 patients) treatment-emergent adverse events (safety population). (DOCX 18 kb)
Upper bound on Hot Dark Matter Density from $SO(10)$ Yukawa Unification
Creators: name: Brignole, Andrea
name: Murayama, Hitoshi
name: Rattazzi, Riccardo
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study low-energy consequences of supersymmetric $SO(10)$ models with Yukawa unification $h_t = h_N$ and $h_b = h_τ$. We find that it is difficult to reproduce the observed $m_b/m_τ$ ratio when the third-generation right-handed neutrino is at an intermediate scale, especially for small $\tan β$. We obtain a conservative lower bound on the mass of the right-handed neutrino $M_N > 6 \times 10^{13}$~GeV for $\tan β< 10$. This bound translates into an upper bound on the $τ$-neutrino mass, and therefore on its contribution to the hot dark matter density of the present universe, $Ω_νh^2 < 0.004$. Our analysis is based on the full two-loop renormalization group equations with one-loop threshold effects. However, we also point out that physics above the GUT-scale could modify the Yukawa unification condition $h_b = h_τ$ for $\tan β\lsim 10$. This might affect the prediction of $m_b/m_τ$ and the constraint on $M_N$.
description: LBL-35774, RU-94-51, 18 pages, plain LaTeX, two PostScript figures appended in uuencoded format
Sertularia polyzonias Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia polyzonias

description: Sertularia polyzonias [spec. nov.]
S. denticulis alternis subdenticulatis, calycibus obovatis polyzoniis, caule subramoso.
Ellis corall. 5. n. 3. t. 2. f. A, B. & t. 28. f. 1.
Raj. angl. 3. p. 35. n. 13. Corallina minus ramosa alterna vice denticulata, denticulis lineis transversis externe striatis.
Habitat in Oceano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 813, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Orbital solution leading to an acceptable interpretation for the enigmatic gamma-ray binary HESS J0632+057
Creators: name: Moritani, Yuki
name: Kawano, Takafumi
name: Chimasu, Sho
name: Kawachi, Akiko
name: Takahashi, Hiromitsu
name: Takata, Jumpei
name: Carciofi, Alex C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: High-dispersion spectroscopic monitoring of HESS J0632+057 has been carried out over four orbital cycles in order to search for orbital modulation, covering the entire orbital phase. We have measured radial velocity of H$α$ emission line with the method introduced by Shafter et al. (1986), which has been successfully applied to some Be stars. The velocity is seen to increase much earlier than expected for the orbital period of 315 days, and much more steeply than expected at around "apastron". The period of the H$α$ modulation is found to be as $308^{+26}_{-23}$ days. We have also analyzed Swift/XRT data from 2009 to 2015 to study the orbital modulation, selecting the data with good statistics ($\geq$ 30 counts). With additional two-year data to the previous works, the orbital period has been updated to $313^{+11}_{-8}$ days, which is consistent with the previous X-ray periods and the spectroscopic one. The past XMM-Newton and Chandra observations prefer the period of 313 days. With the new period, assuming that H$α$ velocities accurately trace the motion of the Be star, we have derived a new set of the orbital parameters. In the new orbit, which is less eccentric ($e \sim 0.6$), two outbursts occur after apastron, and just after periastron. Besides, the column density in bright phase ($4.7^{+0.9}_{-08}\times10^{21}\;\mathrm{cm^{-2}}$) is higher than in faint phase ($2.2\pm0.5\times10^{21}\;\mathrm{cm^{-2}}$). These facts suggest that outbursts occur when the compact object passes nearby/through the Be disk. The mass function implies that mass of the compact object is less than 2.5 $\mathrm{M_{sun}}$ assuming that the mass of the Be star is 13.2--18.2 $\mathrm{M_{sun}}$ (Aragona at al. 2010) unless the inclination is extremely small. The photon index indicates that the spectra becomes softer when the system is bright. These suggest that the compact object is a pulsar.
description: 15 pages, 7 figures, accepted to PASJ
Orbital instability and relaxation in stellar systems
Creators: name: Valluri, Monica
name: Merritt, David
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The orbits of stars in galaxies are generically chaotic: the chaotic behavior arises in part from the intrinsically grainy nature of a potential that is composed of point masses. Even if the potential is assumed to be smooth, however, orbits in non-axisymmetric galaxies can be chaotic due to the presence of central density cusps or black holes. The chaotic nature of orbits implies that perturbations will grow exponentially and this in turn is expected to result in a diffusion in phase space. We show that the degree of orbital evolution is not well predicted by the growth rate of infinitesimal perturbations, i.e. by the Liapunov exponent. A more useful criterion is whether perturbations continue to grow exponentially until their scale is of order the size of the system. We illustrate these ideas in a potential consisting of N fixed point masses. Liapunov exponents are large for all values of N, but orbits become increasingly regular in their behavior as N increases; the reason is that the exponential divergence saturates at smaller and smaller distances as N is increased. The objects which impede diffusion are the invariant tori. When there are few stable tori, an ensemble of chaotic orbits evolves rapidly toward a nearly stationary state. This mixing process occurs on timescales of a few crossing times in triaxial potentials containing massive central singularities, consistent with the rapid evolution observed in N-body simulations of galaxies with central black holes.
description: Invited review to appear in "The Chaotic Universe", eds. R. Ruffini, V.G. Gurzadyan (World Scientific) 1999, 9 pages, 4 figures
Comparative evaluation of autosomal STRs and X-chromosome STRs as a complement of autosomal STRs in kinship testing in Southern Han Chinese
Creators: name: Zhang, Yinming
name: Yu, Zhengliang
name: Mo, Xiaoting
name: Zhao, Xingchun
name: Li, Wanshui
name: Liu, Hong
name: Liu, Chao
name: Wu, Riga
name: Sun, Hongyu
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: Nowadays, kinship testing is very common in forensic caseworks, but the power of autosomal short tandem repeats (A-STRs) may be limited in complex cases. X-Chromosome short tandem repeats (X-STRs), having a unique heritage mode, should be of special use in some deficient cases. To evaluate and compare the potential of A-STR and X-STR as supplement genetic markers in deficient kinship testing, we simulated 10,000 duos for each of 18 kinds of relationships involving full sibling, half-sibling, grandparent-grandchild, and uncle/aunt-nephew/niece. Loci from STRTyper10, PowerPlex 16, and Investigator Argus X-12 were studied in Southern Han Chinese and the distribution of likelihood ratio (LR) values was analysed. With the addition of the X-12 system, the distribution of LR values for the full sisters, paternal half-sisters, paternal grandmother-granddaughters, maternal aunt-nieces, and maternal aunt-nephews separated much more obviously from those of unrelated duos, and the effectiveness was 1.0000, 0.99865, 0.9991, 0.8996 and 0.9634, respectively, which was more efficient than A-STRs. For the individual duos with other relationships, the effects of adding X-STRs and A-STRs were similar. Therefore, for the Southern Han Chinese, X-STRs can be very useful in kinship testing involving full sisters, paternal half-sisters, paternal grandmother-granddaughters, and maternal aunt-nieces/nephews.
Fast Adaptive Identification of Stable Innovation Filters
Creators: name: Mullhaupt, Andrew P.
name: Riedel, Kurt S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: Systems and Control (eess.SY)
subject: Signal Processing (eess.SP)
subject: Statistics Theory (math.ST)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Mathematics

description: The adaptive identification of the impulse response of an innovation filter is considered. The impulse response is a finite sum of known basis functions with unknown coefficients. These unknown coefficients are estimated using a pseudolinear regression. This estimate is implemented using a square root algorithm based on a displacement rank structure. When the initial conditions have low displacement rank, the filter update is $O(n)$. If the filter architecture is chosen to be triangular input balanced, the estimation problem is well-conditioned and a simple, low rank initialization is available.
The Search for the Decay of Z Boson into Two Gammas as a Test of Bose Statistics
Creators: name: Ignatiev, A. Yu.
name: Joshi, G. C.
name: Matsuda, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We suggest that Bose statistics for photons can be tested by looking for decays of spin-1 bosons into two photons. The experimental upper limit on the decay $Z \rightarrow γγ$ is used to establish for the first time the quantitative measure of the validity of Bose symmetry for photons.
description: 9 pages, in REVTEX, RCHEP-94/17, UM-P-94/63
Additional file 1: of Multiple mini interviews: revealing similarities across institutions
Creators: name: Griffin, Barbara
name: Auton, Jaime
name: Duvivier, Robbert
name: Shulruf, Boaz
name: Hu, Wendy
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Appendix 1 Fit indices for competing models. (DOCX 39 kb)
Sertularia setacea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia setacea

description: Sertularia setacea [spec. nov.]
S. denticulis secundis subcylindricis, calycibus oblongis cauli adpressis, surculis alternato-pinnatis lanceolatis.
Ellis corall. t. 38. f. 4. Corallina setacea.
Habitat in Oceano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 813, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Vortex coronagraphs for the Habitable Exoplanet Imaging Mission (HabEx) concept: theoretical performance and telescope requirements
Creators: name: Ruane, Garreth
name: Mawet, Dimitri
name: Mennesson, Bertrand
name: Jewell, Jeffrey
name: Shaklan, Stuart
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Habitable Exoplanet Imaging Mission (HabEx) concept requires an optical coronagraph that provides deep starlight suppression over a broad spectral bandwidth, high throughput for point sources at small angular separation, and insensitivity to temporally-varying, low-order aberrations. Vortex coronagraphs are a promising solution that perform optimally on off-axis, monolithic telescopes and may also be designed for segmented telescopes with minor losses in performance. We describe the key advantages of vortex coronagraphs on off-axis telescopes: 1) Unwanted diffraction due to aberrations is passively rejected in several low-order Zernike modes relaxing the wavefront stability requirements for imaging Earth-like planets from <10 to >100 pm rms. 2) Stars with angular diameters >0.1 $λ/D$ may be sufficiently suppressed. 3) The absolute planet throughput is >10%, even for unfavorable telescope architectures. 4) Broadband solutions ($Δλ/λ>0.1$) are readily available for both monolithic and segmented apertures. The latter make use of grayscale apodizers in an upstream pupil plane to provide suppression of diffracted light from amplitude discontinuities in the telescope pupil without inducing additional stroke on the deformable mirrors. We set wavefront stability requirements on the telescope, based on a stellar irradiance threshold set at an angular separation of 3$\pm$0.5 $λ/D$ from the star, and discuss how some requirements may be relaxed by trading robustness to aberrations for planet throughput.
description: accepted for publication in the Journal of Astronomical Telescopes, Instruments, and Systems. arXiv admin note: text overlap with arXiv:1708.05787
The Remarkable Central Structure of the Barred Galaxy NGC 1415
Creators: name: Garcia-Barreto, J. A.
name: Moreno, E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A remarkable structure is observed in the innermost regions of the barred galaxy NGC 1415 : a small stellar bar, bright circumnuclear ionized gas seen in Halpha, two bright ionized gas sources, seen in Halpha, just beyond the ends of the small bar and a boxy distribution of optical continuum. We have developed a mass distribution model consisting in disk, a bulge, and a bar to approximate t he observed central morphology and its surface brightness. In order to reproduce the observed optical brightness distribution a two-component bar was used, with one component to model the elongated isophotes of the bar and the second component to model the boxy-shaped isophotes. We interpret the circumnuclear ionized gas as forming a circumnuclear ring and the two bright sources as a nuclear and/or circumnuclear outflow slightly out of the plane of the disk.
description: 19 pages, 29 figures. To be published in February 2000, ApJ, 529
Universality for 1d random band matrices: sigma-model approximation
Creators: name: Shcherbina, Mariya
name: Shcherbina, Tatyana
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The paper continues the development of the rigorous supersymmetric transfer matrix approach to the random band matrices started in J Stat Phys 164:1233 -- 1260, 2016; Commun Math Phys 351:1009 -- 1044, 2017. We consider random Hermitian block band matrices consisting of $W\times W$ random Gaussian blocks (parametrized by $j,k \inΛ=[1,n]^d\cap \mathbb{Z}^d$) with a fixed entry's variance $J_{jk}=δ_{j,k}W^{-1}+βΔ_{j,k}W^{-2}$, $β>0$ in each block. Taking the limit $W\to\infty$ with fixed $n$ and $β$, we derive the sigma-model approximation of the second correlation function similar to Efetov's one. Then, considering the limit $β, n\to\infty$, we prove that in the dimension $d=1$ the behaviour of the sigma-model approximation in the bulk of the spectrum, as $β\gg n$, is determined by the classical Wigner -- Dyson statistics.
description: 38 pp
Green functions from a gauge-invariant effective action for the electroweak Standard Model
Creators: name: Denner, A.
name: Dittmaier, S.
name: Weiglein, G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Application of the background-field method to the electroweak Standard-Model yields a gauge-invariant effective action giving rise to simple Ward identities. We find that in the background-field `t Hooft-Feynman gauge the resulting vertex functions are exactly those that are obtained using the pinch technique. Thus, the background-field method provides a general framework that generalizes the pinch technique directly and uniquely to arbitrary Green functions and arbitrary orders of perturbation theory. Moreover, the desirable properties of the pinch-technique vertex functions hold for arbitrary gauge parameters and have a simple explanation within the background- field method.
description: to appear in Nucl. Phys. B Proc. Suppl., proceedings to the 1994 Zeuthen workshop on elementary particle theory, "physics at LEP200 and beyond", 6 pages uuencoded postscript, BI-TP 94/22
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00217
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00217, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Additional file 1: of Genome-based analysis for the identification of genes involved in o-xylene degradation in Rhodococcus opacus R7
Creators: name: Canito, Alessandra Di
name: Zampolli, Jessica
name: Orro, Alessandro
name: DâUrsi, Pasqualina
name: Milanesi, Luciano
name: Sello, Guido
name: SteinbĂźchel, Alexander
name: Gennaro, Patrizia Di
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S1. Sequences used to generate dioxygenase tree. (DOCX 25 kb)
Sertularia stipulata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia stipulata

description: Sertularia stipulata [spec. nov.]
S. denticulis secundis, calycibus campanulatis pedicellatis infra frondes, surculis alternato-pinnatis lanceolatis.
Ellis corall. t. 38. f. 5. Corallina capillamentis falcatis.
Habitat in Oceano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 813, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Radio Afterglow and the Host Galaxy of the X-Ray Rich GRB 981226
Creators: name: Frail, D. A.
name: Kulkarni, S. R.
name: Bloom, J. S.
name: Djorgovski, S. G.
name: Gorjian, V.
name: Gal, R. R.
name: Meltzer, J.
name: Sari, R.
name: Chaffee, F. H.
name: Goodrich, R. W.
name: Frontera, F.
name: Costa, E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a radio transient VLA 232937.2-235553, coincident with the proposed X-ray afterglow for the gamma-ray burst GRB 981226. This GRB has the highest ratio of X-ray to gamma-ray fluence of all the GRBs detected by BeppoSAX so far and yet no corresponding optical transient was detected. The radio light curve of VLA 232937.2-235553 is qualitatively similar to that of several other radio afterglows. At the sub-arcsecond position provided by the radio detection, optical imaging reveals an extended R=24.9 mag object, which we identify as the host galaxy of GRB 981226. Afterglow models which invoke a jet-like geometry for the outflow or require an ambient medium with a radial density dependence, such as that produced by a wind from a massive star, are both consistent with the radio data. Furthermore, we show that the observed properties of the radio afterglow can explain the absence of an optical transient without the need for large extinction local to the GRB.
description: Accepted for publication in the Astrophysical Journal Letters. Thirteen pages. Three Postscript figures
Dimensionally mixed coupled collective modes
Creators: name: Hwang, E. H.
name: Hu, Ben Yu-Kuang
name: Sarma, S. Das
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We develop the diagrammatic formulation of the many-body theory for the coupled collective modes in interacting electron systems of different dimensions. The formalism is then applied in detail to a two-dimensional system coupled to a three-dimensional electron gas. We find two dimensionally-mixed plasmon modes which in the long wavelength limit are respectively 3D-like and acoustic in nature, but are strongly coupled at larger wave vectors. The same formalism can be applied to any dimensional combinations, and we also present the results for 1D-2D and 1D-3D coupled systems.
description: 5 pages, 3 figures
Optimal Estimation of Dynamically Evolving Diffusivities
Creators: name: Riedel, Kurt S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: Signal Processing (eess.SP)
subject: Optimization and Control (math.OC)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: The augmented, iterated Kalman smoother is applied to system identification for inverse problems in evolutionary differential equations. In the augmented smoother, the unknown, time-dependent coefficients are included in the state vector, and have a stochastic component. At each step in the iteration, the estimate of the time evolution of the coefficients is linear. We update the slowly varying mean temperature and conductivity by averaging the estimates of the Kalman smoother. Applications include the estimation of anomalous diffusion coefficients in turbulent fluids and the plasma rotation velocity in plasma tomography.
Dynamical Electroweak Symmetry Breaking
Creators: name: King, Stephen F
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review the status of and recent developments in dynamical electroweak symmetry breaking, concentrating on the ideas of technicolour and top quark condensates. The emphasis is on the essential physical ideas and experimental implications rather than on detailed mathematical formalism.
description: This revised version contains some minor changes and is somewhat shorter than the original.
Difference in dwarf galaxy surface brightness profiles as a function of environment
Creators: name: Lee, Youngdae
name: Park, Hong Soo
name: Kim, Sang Chul
name: Moon, Dae-Sik
name: Lee, Jae-Joon
name: Kim, Dong-Jin
name: Cha, Sang-Mok
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate surface brightness profiles (SBPs) of dwarf galaxies in field, group, and cluster environments. With deep $BVI$ images from the Korea Microlensing Telescope Network Supernova Program, SBPs of 38 dwarfs in the NGC 2784 group are fitted by a single exponential or double exponential model. We find that 53% of the dwarfs are fitted with single exponential profiles ("Type I"), while 47% of the dwarfs show double exponential profiles. 37% of all dwarfs have smaller sizes of the outer part than inner part ("Type II"), while 10% have a larger sized outer than inner part ("Type III"). We compare these results with those in the field and in the Virgo cluster, where SBP types of 102 field dwarfs are compiled from a previous study and SBP types of 375 cluster dwarfs are measured using SDSS $r$-band images. As a result, the distributions of SBP types are different in three environments. Common SBP types of the field, the NGC 2784 group, and the Virgo cluster are Type II, Type I and II, and Type I and III profiles, respectively. After comparing sizes of dwarfs in different environments, we suggest that since sizes of some dwarfs are changed due to the environmental effects, SBP types are able to be transformed and the distributions of SBP types in three environments are different. We discuss possible environmental mechanisms on the transformation of SBP types.
description: 28 pages, 7 figures, 5 tables, accepted to ApJ
Additional file 1: of Safety and tolerability of quizartinib, a FLT3 inhibitor, in advanced solid tumors: a phase 1 dose-escalation trial
Creators: name: Papadopoulos, Kyriakos
name: Ben-Ami, Eytan
name: Patnaik, Amita
name: Trone, Denise
name: Jianke Li
name: Demetri, George
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Scheduled assessments to evaluate the safety and tolerability of quizartinib. (DOCX 18 kb)
title: ADCO, Cartulaire de Fontenay, premier fragment (XIIIe siècle), Cart. 201 (15 H 9), 175 folios, f. 066v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, premier fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), 175 folios, f. 066v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
A novel data representation framework based on nonnegative manifold regularisation
Creators: name: Jiang, Yan
name: Liang, Wei
name: Tang, Jintian
name: Zhou, Hongbo
name: Li, Kuan-Ching
name: Gaudiot, Jean-Luc
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified

description: Representation learning techniques have been frequently applied in multimedia content analysis and retrieval. In this study, an efficient multimedia data clustering method is presented, which consists of two independent algorithms. First, we propose a new representation framework by incorporating sparse coding and manifold regularisation in an optimisation objective function, the cluster indicator matrix is estimated by introducing ℓ1 sparsity norm coarsely. Second, we refine the estimated cluster indicator matrix by performing spectral rotation such that an optimal assignment for clustering can be learned. Compared with existing methods, we have the following merits: our method takes into account the global matrix reconstruction information and locality manifold information simultaneously. Therefore, global and locality information both are respected. Additionally, theoretical justification about the novel representation method is presented in this study. Comprehensive experiments demonstrate the effectiveness and efficiency of our method in comparison with the state-of-the-art clustering methods on six real-world image datasets.
A Near-Infrared Photometric Study of the Low Latitude Globular Clusters Liller 1, Djorgovski 1, HP 1, and NGC 6528
Creators: name: Davidge, T. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Images recorded through J, H, Ks, 2.2 micron continuum, and 2.3 micron CO filters are used to investigate the stellar contents of the low Galactic latitude globular clusters NGC 6528, Liller 1, Djorgovski 1, and HP 1, as well as surrounding bulge fields. Metallicities are estimated for the latter three clusters by comparing the colors and CO indices of giant branch stars with those in other clusters and the bulge, while reddenings are estimated from the colors of bright bulge stars in the surrounding fields. In some cases the metallicities and reddenings are significantly different from previous estimates.
description: 32 pages, and 28 figures
QCD S Parameter from Inhomogeneous Bethe-Salpeter Equation
Creators: name: Harada, Masayasu
name: Yoshida, Yuhsuke
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the low-energy parameter S in QCD, which is also known as L_{10}, and the pion decay constant f_πusing inhomogeneous Bethe-Salpeter equation in improved ladder approximation. To extract these quantities we calculate the ``V-A'' two-point function, Π_{VV}(q^2) - Π_{AA}(q^2), in space-like region. We obtain S = 0.43 \sim 0.48, which is about 30% larger than the experimental value. The calculated f_πis well consistent with the result by solving the homogeneous Bethe-Salpeter equation for pion. We also evaluate $S$ parameter in SU(3) gauge theory with N_D doublets of fermions in connection with walking technicolor model, and find that the value of S/N_D hardly depends on N_D.
description: 22 pages (LaTeX), 6 PostScript figures are included as uuencoded-compressed-tar file at the end (need 'epsf.tex' macro package), KUNS-1270 HE(TH)94/09
Sertularia pennaria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia pennaria

description: Sertularia pennaria [spec. nov.]
S. denticulis secundis, surculis bipinnatis.
Habitat in M. Indico. Steller.
Caulis sesquipedalis, rudis, contortus, pinnatus Ramis alternis, subpetiolatis, distantibus, parallelis. Rami pennati radiis parallelis, approximatis & fere contiguis (ut in penna); Radii articulati, dorso convexi, sed latere superiore imbricati. Sic rami referunt structura Sert. plumam, sed distincta species magnitudine, compositione, approximatis radiis, facie.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 813, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Magnetic gravity compensation
Creators: name: Nikolayev, Vadim
name: Chatain, D.
name: Beysens, D.
name: Pichavant, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: Magnetic gravity compensation in fluids is increasingly popular as a means to achieve low-gravity forphysical and life sciences studies. We explain the basics of the magnetic gravity compensation and analyzeits advantages and drawbacks. The main drawback is the spatial heterogeneity of the residual gravity field.We discuss its causes. Some new results concerning the heterogeneity estimation and measurement arepresented. A review of the existing experimental installations and works involving the magnetic gravitycompensation is given for both physical and life sciences.
The Role of Magnetic Field Dissipation in the Black Hole Candidate Sgr A*
Creators: name: Coker, Robert F.
name: Melia, Fulvio
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The compact, nonthermal radio source Sgr A* at the Galactic Center appears to be coincident with a 2.6 million solar mass point-like object. Its energy source may be the release of gravitational energy as gas from the interstellar medium descends into its potential well. Simple attempts at calculating the spectrum and flux based on this picture have come close to the observations, yet have had difficulty in accounting for the low efficiency in this source. There now appear to be two reasons for this low conversion rate: (1) the plasma separates into two temperatures, with the protons attaining a significantly higher temperature than that of the radiating electrons, and (2) the magnetic field, B, is sub-equipartition, which reduces the magnetic bremsstrahlung emissivity, and therefore the overall power of Sgr A*. We investigate the latter with improvement over what has been attempted before: rather than calculating B based on a presumed model, we instead infer its distribution with radius empirically with the requirement that the resulting spectrum matches the observations. Our ansatz for B(r) is motivated in part by earlier calculations of the expected magnetic dissipation rate due to reconnection in a compressed flow. We find reasonable agreement with the observed spectrum of Sgr A* as long as its distribution consists of 3 primary components: an outer equipartition field, a roughly constant field at intermediate radii (~1000 Schwarzschild radii), and an inner dynamo (more or less within the last stable orbit for a non-rotating black hole) which increases B to about 100 Gauss. The latter component accounts for the observed sub-millimiter hump in this source.
description: 33 pages including 2 figures; submitted to ApJ
Nuclear quantum effects enter the mainstream
Creators: name: Markland, Thomas E.
name: Ceriotti, Michele
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Over the past decades, atomistic simulations of chemical, biological and materials systems have become increasingly precise and predictive thanks to the development of accurate and efficient techniques that describe the quantum mechanical behavior of electrons. However, the overwhelming majority of such simulations still assume that the nuclei behave as classical particles. While historically this approximation could sometimes be justified due to complexity and computational overhead, the lack of nuclear quantum effects has become one of the biggest sources of error when systems containing light atoms are treated using current state-of-the-art descriptions of chemical interactions. Over the past decade, this realization has spurred a series of methodological advances that have led to dramatic reductions in the cost of including these important physical effects in the structure and dynamics of chemical systems. Here we show how these developments are now allowing nuclear quantum effects to become a mainstream feature of molecular simulations. These advances have led to new insights into chemical processes in the condensed phase and open the door to many exciting future opportunities.
description: Pre-review version
Sertularia flexuosa Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia flexuosa

description: Sertularia flexuosa [spec. nov.]
S. denticulis obsoletis, calycibus alternis ovatis sessilibus, caule simplici flexuoso.
Loefl. Act. Stockh. 1752. p. 114. t. 3. f. 5-10. Madrepora plantaeformis mollis, caule flexuoso, ramulis alternis turbinatis.
Ellis corall. t. 38. f. 1. A. Corallina altera vice denticulata.
Habitat in Oceano.
* * Ovariis non distinctis, sed intra articulos latitantibus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 814, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Local uniqueness of $m$-bubbling sequences for the Gel'fand equation
Creators: name: Bartolucci, Daniele
name: Jevnikar, Aleks
name: Lee, Youngae
name: Yang, Wen
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35B32, 35J25, 35J61, 35J99, 82D15

description: We consider the Gel'fand problem, $$ \begin{cases} Δw_{\varepsilon}+\varepsilon^2 h e^{w_{\varepsilon}}=0\quad&\mbox{in}\quadΩ, w_{\varepsilon}=0\quad&\mbox{on}\quad\partialΩ, \end{cases} $$ where $h$ is a nonnegative function in ${Ω\subset\mathbb{R}^2}$. Under suitable assumptions on $h$ and $Ω$, we prove the local uniqueness of $m-$bubbling solutions for any $\varepsilon>0$ small enough.
Additional file 2: of Independent investigator incubator (I3): a comprehensive mentorship program to jumpstart productive research careers for junior faculty
Creators: name: Spence, John
name: Buddenbaum, Jennifer
name: Bice, Paula
name: Welch, Julie
name: Carroll, Aaron
Publisher: name: figshare
Year: 2018
Subjects: subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Figure S2. Snapshot of mentee performance for I3 mentors. A short report (1 page) was developed to provide the mentors with a â snapshotâ of assessment of mentee performance over time in order to supplement mentor impressions of the mentee and to identify perceived deficits that can be addressed. (PDF 6781Â kb)
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0182
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: LaMOP
subject: Chartes de la Bourgogne du Moyen Âge
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0182, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0182, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019