cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Energy consumption and cooperation for optimal sensing
Creators: name: Ngampruetikorn, Vudtiwat
name: Schwab, David J.
name: Stephens, Greg J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: The reliable detection of environmental molecules in the presence of noise is an important cellular function, yet the underlying computational mechanisms are not well understood. We introduce a model of two interacting sensors which allows for the principled exploration of signal statistics, cooperation strategies and the role of energy consumption in optimal sensing, quantified through the mutual information between the signal and the sensors. Here we report that in general the optimal sensing strategy depends both on the noise level and the statistics of the signals. For joint, correlated signals, energy consuming (nonequilibrium), asymmetric couplings result in maximum information gain in the low-noise, high-signal-correlation limit. Surprisingly we also find that energy consumption is not always required for optimal sensing. We generalise our model to incorporate time integration of the sensor state by a population of readout molecules, and demonstrate that sensor interaction and energy consumption remain important for optimal sensing.
description: 9 pages, 5 figures, Forthcoming in Nature Communications
Stochastic Resonance in Ising Systems
Creators: name: Neda, Zoltan
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We study by Monte Carlo techniques the evolution of finite two-dimensional Ising systems in oscillating magnetic fields. The phenomenon of stochastic resonance is observed. The characteristic peak obtained for the correlation function between the external field and magnetization, versus the temperature of the system, is studied for various external fields and lattice sizes.
description: 8 pages, latex, 4 figures upon request
The Quasar Pair Q 1634+267 A, B and the Binary QSO vs. Dark Lens Hypotheses
Creators: name: Peng, C. Y.
name: Impey, C. D.
name: Falco, E. E.
name: Kochanek, C. S.
name: Lehar, J.
name: McLeod, B. A.
name: Rix, H. -W.
name: Keeton, C. R.
name: Munoz, J. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Deep HST/NICMOS H (F160W) band observations of the z=1.96 quasar pair Q 1634+267A,B reveal no signs of a lens galaxy to a 1 sigma threshold of approximately 22.5 mag. The minimum luminosity for a normal lens galaxy would be a 6L_* galaxy at z > 0.5, which is 650 times greater than our detection threshold. Our observation constrains the infrared mass-to-light ratio of any putative, early-type, lens galaxy to (M/L)_H > 690h_65 (1200h_65) for Omega_0=0.1 (1.0) and H_0=65h_65 km/s/Mpc. We would expect to detect a galaxy somewhere in the field because of the very strong Mg II absorption lines at z=1.1262 in the Q 1634+267 A spectrum, but the HST H-band, I-band (F785LP) and V-band (F555W) images require that any associated galaxy be very under-luminous less than 0.1 L^*_H (1.0 L^*_I) if it lies within less than 40 h^{-1} (100 h^{-1}) kpc from Q 1634+267 A,B. While the large image separation (3.86 arcsec) and the lack of a lens galaxy strongly favor interpreting Q 1634+267A,B as a binary quasar system, the spectral similarity remains a puzzle. We estimate that at most 0.06% of randomly selected quasar pairs would have spectra as similar to each other as the spectra of Q 1634+267 A and B. Moreover, spectral similarities observed for the 14 quasar pairs are significantly greater than would be expected for an equivalent sample of randomly selected field quasars. Depending on how strictly we define similarity, we estimate that only 0.01--3% of randomly drawn samples of 14 quasar pairs would have as many similar pairs as the observational sample.
description: 24 pages, including 4 figures, LaTex, ApJ accepted, comments from the editor included, minor editorial changes
Impact of valley phase and splitting on readout of silicon spin qubits
Creators: name: Tagliaferri, M. L. V.
name: Bavdaz, P. L.
name: Huang, W.
name: Dzurak, A. S.
name: Culcer, D.
name: Veldhorst, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate the effect of the valley degree of freedom on Pauli-spin blockade readout of spin qubits in silicon. The valley splitting energy sets the singlet-triplet splitting and thereby constrains the detuning range. The valley phase difference controls the relative strength of the intra- and inter-valley tunnel couplings, which, in the proposed Pauli-spin blockade readout scheme, couple singlets and polarized triplets, respectively. We find that high-fidelity readout is possible for a wide range of phase differences, while taking into account experimentally observed valley splittings and tunnel couplings. We also show that the control of the valley splitting together with the optimization of the readout detuning can compensate the effect of the valley phase difference. To increase the measurement fidelity and extend the relaxation time we propose a latching protocol that requires a triple quantum dot and exploits weak long-range tunnel coupling. These opportunities are promising for scaling spin qubit systems and improving qubit readout fidelity
description: 8 pages, 6 figures
The H$α$ Luminosity Function and Global Star Formation Rate From Redshifts of One to Two
Creators: name: Yan, Lin
name: McCarthy, Patrick J.
name: Freudling, Wolfram
name: Teplitz, Harry I.
name: Malumuth, Eliot M.
name: Weymann, Ray J.
name: Malkan, Matthew A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a luminosity function for H$α$ emission from galaxies at redshifts between 0.7 and 1.9 based on slitless spectroscopy with NICMOS on HST. The luminosity function is well fit by a Schechter function over the range $6 \times 10^{41} < L(Hα) < 2 \times 10^{43} erg/sec$ with $L^* = 7 \times 10^{42} erg/sec$ and $ϕ^* = 1.7 \times 10^{-3} Mpc^{-3}$ for $H_0=50 km/s Mpc^{-1}$ and $q_0=0.5$. We derive a volume averaged star formation rate at $z = 1.3 \pm 0.5$ of 0.13 M_{\odot} yr^{-1} Mpc^{-3} without correction for extinction. The SFR that we derive at $\sim 6500 Åis a factor of 3 higher than that deduced from 2800 Åcontinua. If this difference is due entirely to reddening, the extinction correction at 2800 Åis quite significant. The precise magnitude of the total extinction correction at rest-frame UV wavelengths (e.g. 2800 Åand 1500 Å) is sensitive to the relative spatial distribution of the stars, gas and dust, as well as on the extinction law. In the extreme case of a homogeneous foreground dust screen and a MW or LMC extinction law, we derive a total extinction at 2800 Åof 2.1 magnitudes, or a factor of 7 correction to the UV luminosity density. If we use the Calzetti reddening curve, which was derived for the model where stars, gas and dust are well mixed and nebular gas suffers more extinction than stars, our estimate of A$_{2800}$ is increased by more than one magnitude.
description: 11 pages, 2 postscript figures. Accepted for the publication in the ApJ Letters
Additional file 3 of What is the available evidence for the application of genome editing as a new tool for plant trait modification and the potential occurrence of associated off-target effects: a systematic map protocol
Creators: name: Modrzejewski, Dominik
name: Hartung, Frank
name: Sprink, Thorben
name: Krause, Dörthe
name: Kohl, Christian
name: Schiemann, Joachim
name: Wilhelm, Ralf
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 3. Final search terms.
Musca bicincta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca bicincta

description: Musca bicincta [spec. nov.]
M. antennis setariis elongatis nigra, thorace lateribus punctis, abdomineque cingulis duobus flavis.
Habitat in Europa.
Abdomen glabrum ut sequentis; fascia prior interrupta.
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 592, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Phase Ordering of 2D XY Systems Below T_{KT}
Creators: name: Rutenberg, A. D.
name: Bray, A. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider quenches in non-conserved two-dimensional XY systems between any two temperatures below the Kosterlitz-Thouless transition. The evolving systems are defect free at coarse-grained scales, and can be exactly treated. Correlations scale with a characteristic length $L(t) \propto t^{1/2}$ at late times. The autocorrelation decay exponent, $\barλ = (η_i+η_f)/2$, depends on both the initial and the final state of the quench through the respective decay exponents of equilibrium correlations, $C_{EQ}(r) \sim r^{-η}$. We also discuss time-dependent quenches.
description: LATeX 11 pages (REVTeX macros), no figures
Stachyanthus Engl.
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Stachyanthus

description: Genus Stachyanthus Engl.
Fig. 34
Description
FRUIT. Elliptical, acute-acuminate at the apex, laterally compressed, yellow or blue when mature. Epicarp strigose to pubescent, with simple hairs with granular ornamentation and / or uncinate hairs, rugose-ridged or smooth when dry. Calyx persistent.
ENDOCARP. Cream to brown, elliptical in lateral view, lenticular in transverse section. Keel surrounding the endocarp in the plane of symmetry. Apex asymmetrical; base symmetrical. Outer surface of the endocarp pitted and ridged. Pits more or less circular, associated with bullate tubercles. Ridges forming a diffuse pattern, faintly apparent. Vasculature of the endocarp free. Primary vascular bundle positioned outside the endocarp wall. Endocarp wall with at least one layer with rows of periclinally oriented cells. Locule surface smooth and lacunate.
Fig. 34. (see full caption on page 106)
Key to the genus Stachyanthus
1. Endocarp ca 22 mm in length, ridges sharp ............................................................... S. zenkeri Engl.
– Endocarp ± 17 mm in length, ridges rounded ................................................................................... 2
2. Endocarp length ca 17 mm, pits per face 150–160 ............................ S. donisii (Boutique) Boutique
– Endocarp length ca 11 mm, pits more than 180 ............ S. occidentalis (Keay & É.Miège) Boutique
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on pages 106-108, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Additional file 2 of Barriers and facilitators to the integration of depression services in primary care in Vietnam: a mixed methods study
Creators: name: Murphy, Jill
name: Corbett, Kitty
name: Linh, Dang
name: Pham Oanh
name: Nguyen, Vu
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology

description: Study survey instrument. (PDF 801 kb)
Additional file 12: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S12. Comparative RNA-seq analysis between TQ and the nal8 mutant. (A) Sample correlations among the individual TQ and nal8 replicates and between TQ and nal8. Each sample consisted of three biological replicates. The numbers indicate the pearson’s correlation coefficients for each pair-wise comparison. (B) A PCA map indicates that the TQ and nal8 samples are widely separated in the RNA-seq analysis. (C) A volcano plot shows that more genes are up-regulated in the nal8 mutant than are down-regulated compared with TQ. The X-axes shows the logarithmic values of the relative differences in expression. The Y-axes values are the negative logarithms of the significance. Each dot indicates a gene. Red dots and green dots are significantly up-regulated and down-regulated genes, respectively. Black dots are genes in which the expression changes are insignificant. The expression values for the different RNAs were adjusted by FDR < 0.01, and the Fold Change is > 2. (D) Correlation plot of all TQ and nal8 samples which were used in the RNA-seq analysis. The X- and Y-axes are the logarithmic values of FKPM (fragments per kilobase per million reads). Each dot indicates a gene. The purple line is the coefficient parameter which represents the Pearson’s coefficient of significance, above which the genes are up-regulated, and below which the genes are down-regulated. (PDF 314 kb)
The Structure and Morphology of the Ionized Gas in Starburst Galaxies: NGC5253/5236
Creators: name: Calzetti, D.
name: Conselice, C. J.
name: Gallagher, J. S.
name: Kinney, A. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We investigate the interplay between starbursts and host galaxies by studying the structure and physical characteristics of the ionized gas surrounding the central starbursts in the two nearby galaxies NGC5253 and NGC5236. The two systems represent very different galactic environments, NGC5253 being a metal-poor dwarf, and NGC5236 being a metal-rich, massive spiral. We present images of the starburst regions in these two galaxies in the line emission [OIII], H-alpha, and [SII], and in continuum U, V, R. For NGC5253, line ratio maps [OIII]/H-beta and [SII]/H-alpha show that in the outer regions the diffuse ionized gas (DIG) is partially excited by a non-photoionization process (`shocks'). The `shocked' gas is mostly concentrated south-west of the galaxy's center, in coincidence with the position of H-alpha bubbles and with extended soft X-ray emission. The H-alpha emission from the shock-excited gas is ~1-2% of the total. About 80-90% of the DIG is consistent with being photoionized, requiring that about 10% of the ionizing photons escape from the starburst site. The starburst in NGC5253 appears to be fed by gas infalling along the galaxy's optical minor axis, while hot gas expanding from the starburst has a preferential direction along the major axis. The results for NGC5236 are less clear than for NGC5253, as the images are not as deep. The emission line ratio maps show very little or no evidence for presence of shock excitation and very little or no ionized gas appears expanding from the center of the galaxy outward along the disk plane. The starburst in NGC5236 is thus more strongly confined than that in NGC5253, probably due to the deeper gravitational potential well of the more massive galaxy.
description: 43 pages, Latex, uses AAS Latex macro, includes 13 embedded postscript Figures, and 6 external JPEG figures. Accepted for publication in the Astronomical Journal
The Effects of Clumping and Substructure on ICM Mass Measurements
Creators: name: Mathiesen, B.
name: Evrard, A. E.
name: Mohr, J. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine an ensemble of 48 simulated clusters to determine the effects of small-scale density fluctuations and large-scale substructure on X-ray measurements of the intracluster medium (ICM) mass. We measure RMS density fluctuations in the ICM which can be characterized by a mean mass-weighted clumping factor C = /^2 between 1.3 and 1.4 within a density contrast of 500 times the critical density. These fluctuations arise from the cluster history of accretion shocks and major mergers, and their presence enhances the cluster's luminosity relative to the smooth case. We expect, therefore, that ICM mass measurements utilizing models which assume uniform density at a given radius carry a bias of order sqrt(C) = 1.16. We verify this result by performing ICM mass measurements on X-ray images of the simulations and finding the expected level of bias. The varied cluster morphologies in our ensemble also allow us to investigate the effects of departures from spherical symmetry on our measurements. We find that the presence of large-scale substructure does not further bias the resulting gas mass unless it is pronounced enough to produce a second peak in the image of at least 1% the maximum surface brightness. We analyze the subset of images with no secondary peaks and find a bias of 9% and a Gaussian random error of 4% in the derived mass.
description: To appear in ApJL
Musca arcuata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca arcuata

description: Musca arcuata [spec. nov.]
M. antennis setariis elongatis nigra, thorace lateribus maculis, abdomine cingulis quatuor arcuatis flavis.
Habitat in Europa.
Scutellum flavum macula nigra; Abdomen glabrum. Thorax nudiusculus subtomentosus.
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 592, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
MOESM3 of What is the available evidence for the application of genome editing as a new tool for plant trait modification and the potential occurrence of associated off-target effects: a systematic map protocol
Creators: name: Modrzejewski, Dominik
name: Hartung, Frank
name: Sprink, Thorben
name: DĂśrthe Krause
name: Kohl, Christian
name: Schiemann, Joachim
name: Wilhelm, Ralf
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 3. Final search terms.
On Maxwell's electrodynamics in two spatial dimensions
Creators: name: Boito, D.
name: de Andrade, L. N. S.
name: de Sousa, G.
name: Gama, R.
name: London, C. Y. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: We discuss the construction of Maxwellian electrodynamics in 2+1 dimensions and some of its applications. Special emphasis is given to the problem of the retarded potentials and radiation, where substantial differences with respect to the usual three-dimensional case arise. These stem from the general form of the solutions of the wave equation in two dimensions, which we discuss using the Green's function method. We believe the topics presented here could be stimulating additions to an advanced electrodynamics course at the undergraduate level.
description: 18 pages. Additional discussion. Results unchanged. Matches version to be published
Collective Modes of Soliton-Lattice States in Double-Quantum-Well Systems
Creators: name: Cote, R.
name: Brey, L.
name: Fertig, H.
name: MacDonald, A. H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: In strong perpendicular magnetic fields double-quantum-well systems can sometimes occur in unusual broken symmetry states which have interwell phase coherence in the absence of interwell hopping. When hopping is present in such systems and the magnetic field is tilted away from the normal to the quantum well planes, a related soliton-lattice state can occur which has kinks in the dependence of the relative phase between electrons in opposite layers on the coordinate perpendicular to the in-plane component of the magnetic field. In this article we evaluate the collective modes of this soliton-lattice state in the generalized random-phase aproximation. We find that, in addition to the Goldstone modes associated with the broken translational symmetry of the soliton-lattice state, higher energy collective modes occur which are closely related to the Goldstone modes present in the spontaneously phase-coherent state. We study the evolution of these collective modes as a function of the strength of the in-plane magnetic field and comment on the possibility of using the in-plane field to generate a finite wave probe of the spontaneously phase-coherent state.
description: REVTEX, 37 pages (text) and 15 uuencoded postscript figures
Learning to Recommend with Multiple Cascading Behaviors
Creators: name: Gao, Chen
name: He, Xiangnan
name: Gan, Dahua
name: Chen, Xiangning
name: Feng, Fuli
name: Li, Yong
name: Chua, Tat-Seng
name: Yao, Lina
name: Song, Yang
name: Jin, Depeng
Publisher: name: arXiv
Year: 2018
Subjects: subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Most existing recommender systems leverage user behavior data of one type only, such as the purchase behavior in E-commerce that is directly related to the business KPI (Key Performance Indicator) of conversion rate. Besides the key behavioral data, we argue that other forms of user behaviors also provide valuable signal, such as views, clicks, adding a product to shop carts and so on. They should be taken into account properly to provide quality recommendation for users. In this work, we contribute a new solution named NMTR (short for Neural Multi-Task Recommendation) for learning recommender systems from user multi-behavior data. We develop a neural network model to capture the complicated and multi-type interactions between users and items. In particular, our model accounts for the cascading relationship among different types of behaviors (e.g., a user must click on a product before purchasing it). To fully exploit the signal in the data of multiple types of behaviors, we perform a joint optimization based on the multi-task learning framework, where the optimization on a behavior is treated as a task. Extensive experiments on two real-world datasets demonstrate that NMTR significantly outperforms state-of-the-art recommender systems that are designed to learn from both single-behavior data and multi-behavior data. Further analysis shows that modeling multiple behaviors is particularly useful for providing recommendation for sparse users that have very few interactions.
description: Published in IEEE Transactions on Knowledge and Data Engineering (TKDE)
Musca mutabilis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca mutabilis

description: Musca mutabilis [spec. nov.]
M. antennis setariis elongatis tomentosa, abdomine nigro griseoque mutabili, scutello ferrugineo, thorace immaculato.
Habitat in Europa.
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 592, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Holes and Shells in the Interstellar Medium of the Nearby Dwarf Galaxy IC 2574
Creators: name: Walter, Fabian
name: Brinks, Elias
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present HI synthesis observations of the nearby dwarf galaxy IC 2574 (a member of the M81 group of galaxies) made with the NRAO Very Large Array at high spatial and velocity resolution (95 pc x 2.6 km/s). The VLA HI observations show a stunning amount of detail in the form of 48 mostly expanding HI shells and holes in its neutral interstellar medium. These features range in size from about 100 (a limit set by the size of the beam) to about 1000 pc dominating the appearance of the HI surface brightness map. Their dynamics clearly influence the velocity field of IC 2574. Current star formation, as traced by H-alpha emission, is predominantly found along the rims of the larger HI holes, suggesting propagating star formation. On linear scales of about 95 pc, star formation occurs if the HI surface density reaches values higher than 10^21 cm^-2. The scaleheight of the HI layer is found to be about 350 pc, considerably thicker than that in massive disk galaxies. This is due to a lower gravitational potential (for the same observed onedimensional velocity dispersion of about 7 km/s). A comparison with other galaxies shows that the energies needed to create the expanding HI structures are the same for all types of galaxies, at least to first order. The overall statistical properties of the HI holes and shells in galaxies show clear trends with Hubble type (or rather mass), such as in their diameter distribution, expansion velocities and ages.
description: 37 pages, 20 figures, accepted for publication in the Astronomical Journal
Apodytes dimidiata Arn.
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Apodytes
Apodytes dimidiata

description: Apodytes dimidiata E.Mey. ex Arn.
Fig. 35.1–35.9
Material examined
Specimen used for endocarp and fruit description
MADAGASCAR • 1997; R. Ranaivojaona et al. 114; P [MNHN-P-P05279728].
Other material
MADAGASCAR • 1992; S.T. Malcomber et al. 1212; P [MNHN-P-P00379386] • 1933; H. Perrier de la Bâthie 19254; P [MNHN-P-P00440680] • 2009; M.Y. Ammann, M.C. Madiomanana & A.J. Tahinarivo MYA495; P [MNHN-P-P05279690].
KENYA • 2000; G. Simon, L. Festo & G. Massawe 527; P [MNHN-P-P04499342].
Description
FRUIT. Black when dry, laterally compressed and elongate dorsally. Ventrally truncate, with a fleshy appendage (red but black in dry condition) attached at the truncate part. Epicarp glabrous, shriveled when dry, revealing the underlying endocarp ridges. Mesocarp ca 80–100 µm thick when dry. Calyx persistent. Length ca 6 mm, width ca 10 mm, thickness ca 3 mm.
ENDOCARP. Brown, bilaterally symmetrical, unilocular, single-seeded, globose-truncate in lateral view, length ca 5.5 mm, width ca 7.6 mm. Outer surface of the endocarp ridged with rounded diffuse and thin ridges, with ca 10 lateral ridges. Vasculature of the endocarp free; primary vascular bundle positioned outside the endocarp wall. Endocarp wall 177–266 µm thick (excluding ridges). A sclerotic mass, ca 1.3 mm thick, is developed from the wall in the truncate part of the endocarp. Endocarp wall with sclerotic cells, with two cell layers: outermost layer with 4–7 rows of anticlinally oriented cells, cells 29–86 µm in length; innermost layer with one row of periclinally oriented cells, cells 13.0– 16.5 µm in width, lining the locule surface, forming ripples (the cells have a triangular shape).
Remarks
The sclerotic mass in the truncate part could be a mechanical reinforcement due to the connection of this part with the fleshy appendage.
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on pages 109-110, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Physical modelling of galaxy clusters using Einasto dark matter profiles
Creators: name: Javid, Kamran
name: Perrott, Yvette C.
name: Rumsey, Clare
name: Saunders, Richard D. E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We derive a model for Sunyaev--Zel'dovich data from a galaxy cluster which uses an Einasto profile to model the cluster's dark matter component. This model is similar to the physical models for clusters previously used by the Arcminute Microkelvin Imager (AMI) consortium, which model the dark matter using a Navarro-Frenk-White (NFW) profile, but the Einasto profile provides an extra degree of freedom. We thus present a comparison between two physical models which differ only in the way they model dark matter: one which uses an NFW profile (PM I) and one that uses an Einasto profile (PM II). We illustrate the differences between the models by plotting physical properties of clusters as a function of cluster radius. We generate AMI simulations of clusters which are \textit{created} and \textit{analysed} with both models. From this we find that for 14 of the 16 simulations, the Bayesian evidence gives no preference to either of the models according to the Jeffreys scale, and for the other two simulations, weak preference in favour of the correct model. However, for the mass estimates obtained from the analyses, the values were within $1σ$ of the input values for 14 out of 16 of the clusters when using the correct model, but only in 6 out of 16 cases when the incorrect model was used to analyse the data. Finally we apply the models to real data from cluster A611 obtained with AMI, and find the mass estimates to be consistent with one another except in the case of when PM II is applied using an extreme value for the Einasto shape parameter.
description: 14 pages, 9 figures, 3 tables, 28 equations, MNRAS 2019
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0160v
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0160v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0160v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 13: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S13. KEGG pathway analysis and GO analysis for genes that are differentially expressed between TQ and the nal8 mutant. (A) All differentially-expressed genes (DEGs) that gave a match in the KEGG (Kyoto Encyclopedia of Genes and Genomes) classification. The numbers and percentages of annotated genes are shown to the right, and the various colors indicate the main KEGG pathway classifications. The x-axes indicates the percentage of annotated genes out of all DEGs. (B) GO (gene ontology) enrichment of DEGs between TQ and nal8. The individual GO terms in the three main GO categories are shown on the y-axes, and the x-axes shows the log10 of the significance of the corresponding GO terms. (PDF 211 kb)
Additional file 7: of Value-based evaluation of dialysis versus conservative care in older patients with advanced chronic kidney disease: a cohort study
Creators: name: Verberne, Wouter
name: Dijkers, Janneke
name: Kelder, Johannes
name: Anthonius Geers
name: Jellema, Wilbert
name: Vincent, Hieronymus
name: Delden, Johannes Van
name: Bos, Willem
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Marine Biology
subject: Science Policy

description: Discussion. Comparison between the current and previous results on survival. (PDF 11 kb)
Magnetic Phase Diagram of the Ferromagnetically Stacked Triangular Ising Antiferromagnet
Creators: name: Plumer, M. L.
name: Mailhot, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Histogram Monte-Carlo simulation results are presented for the magnetic-field -- temperature phase diagram of the Ising model on a stacked triangular lattice with antiferromagnetic intraplane and ferromagnetic interplane interactions. Finite-size scaling results for this frustrated system at three points along the paramagnetic transition boundary are presented which strongly suggest a line of triciritcal points at low field and a first-order transition line at higher fields. These results are compared with the corresponding phase diagrams from conventional mean-field theory as well as from the Monte Carlo mean-field calculations of Netz and Berker [Phys. Rev. Lett. {\bf 66}, 377 (1991)].
description: 6 pages (RevTex 3.0), 8 figures available upon request
The role of mass, equation of state and superfluid reservoir in large pulsar glitches
Creators: name: Montoli, Alessandro
name: Antonelli, Marco
name: Pizzochero, Pierre
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Observations of pulsar glitches may provide insights on the internal physics of neutron stars and recent studies show how it is in principle possible to constrain pulsar masses with timing observations. The reliability of these estimates depend on the current uncertainties about the structure of neutron stars and on our ability to model the dynamics of the superfluid neutrons in the internal layers. We assume a simplified model for the rotational dynamics of a neutron star and estimate an upper bound to the mass of 25 pulsars from their largest glitch and average activity: the aim is to understand to which extent the mass constraints are sensitive to the choice of the unknown structural properties of neutron stars, like the extension of the superfluid region and the equation of state. Reasonable values, within the range measured for neutron star masses, are obtained only if the superfluid domain extends for at least a small region inside the outer core, which is compatible with calculations of the neutron S-wave pairing gap. Moreover, the mass constraints stabilise when the superfluid domain extends to densities over nuclear saturation, irrespective of the equation of state tested.
description: 11 pages, 6 figures
Musca ichneumonea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca ichneumonea

description: Musca ichneumonea [spec. nov.]
M. antennis setariis elongatis cylindricis, thorace pedibusque longiusculis ferrugineis, abdomine cinereo.
Habitat in Europa, simillima Ichneumoni.
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 593, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory
Creators: name: Hoeksema, J. Todd
name: Baldner, Charles S.
name: Bush, Rock I.
name: Schou, Jesper
name: Scherrer, Philip H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Helioseismic and Magnetic Imager (HMI) instrument is a major component of NASA's Solar Dynamics Observatory (SDO) spacecraft. Since beginning normal science operations on 1 May 2010, HMI has operated with remarkable continuity, e.g. during the more than five years of the SDO prime mission that ended 30 September 2015, HMI collected 98.4% of all possible 45-second velocity maps; minimizing gaps in these full-disk Dopplergrams is crucial for helioseismology. HMI velocity, intensity, and magnetic-field measurements are used in numerous investigations, so understanding the quality of the data is important. We describe the calibration measurements used to track HMI performance and detail trends in important instrument parameters during the mission. Regular calibration sequences provide information used to improve and update the HMI data calibration. The set-point temperature of the instrument front window and optical bench is adjusted regularly to maintain instrument focus, and changes in the temperature-control scheme have been made to improve stability in the observable quantities. The exposure time has been changed to compensate for a 15% decrease in instrument throughput. Measurements of the performance of the shutter and tuning mechanisms show that they are aging as expected and continue to perform according to specification. Parameters of the tunable-optical-filter elements are regularly adjusted to account for drifts in the central wavelength. Frequent measurements of changing CCD-camera characteristics, such as gain and flat field, are used to calibrate the observations. Infrequent expected events, such as eclipses, transits, and spacecraft off-points, interrupt regular instrument operations and provide the opportunity to perform additional calibration. Onboard instrument anomalies are rare and seem to occur quite uniformly in time. The instrument continues to perform very well.
description: 50 pages, 18 figures, 20 tables
Magnetic Rayleigh-Taylor Instability in Radiative Flows
Creators: name: Yaghoobi, Asiyeh
name: Shadmehri, Mohsen
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a linear analysis of the radiative Rayleigh-Taylor (RT) instability in the presence of magnetic field for both optically thin and thick regimes. When the flow is optically thin, magnetic field not only stabilizes perturbations with short wavelengths, but also growth rate of the instability at long wavelengths is reduced compared to a nonmagnetized case. Then, we extend our analysis to the optically thick flows with a conserved total specific entropy and properties of the unstable perturbations are investigated in detail. Growth rate of the instability at short wavelengths is suppressed due to the presence of the magnetic field, however, growth rate is nearly constant at long wavelengths because of the radiation field. Since the radiative bubbles around massive protostars are subject to the RT instability, we also explore implications of our results in this context. In the nonmagnetized case, the growth time-scale of the instability for a typical bubble is found less than one thousand years which is very short compared to the typical star formation time-scale. Magnetic field with a reasonable strength significantly increases the growth time-scale to more than hundreds of thousands years. The instability, furthermore, is more efficient at large wavelengths, whereas in the non-magnetized case, growth rate at short wavelengths is more significant.
description: 10 pages, 6 figures, Accepted for publication in MNRAS
title: Rapport de voyage, Flandre (1952) : Ligne des Antilles, 1955
Creators: name: Bodard, Georges
name: De Saint-Sauveur, Charles
name: Lejeune, Jacques
name: Vincelet, Louis
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Journaux de bord
subject: Compagnie Générale Transatlantique
subject: Transports maritimes - Histoire
subject: Marine marchande

description: Chapitrage : Rapport d'inspecteurs - Rapport général / du capitaine - Rapport du commissaire - Rapport du second - Rapport de l'officier de sécurité - Rapport de l'officier de navigation - Rapport du médecin - Rapport contentieux
description: Source: French Lines & Compagnies, 1997 004 4990-04
description: Coverage: 1955-12-03/1955-12-24
Additional file 2 of What is the available evidence for the application of genome editing as a new tool for plant trait modification and the potential occurrence of associated off-target effects: a systematic map protocol
Creators: name: Modrzejewski, Dominik
name: Hartung, Frank
name: Sprink, Thorben
name: Krause, Dörthe
name: Kohl, Christian
name: Schiemann, Joachim
name: Wilhelm, Ralf
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 2. Search string development.
Additional file 12: of Identification of heat-tolerance QTLs and high-temperature stress-responsive genes through conventional QTL mapping, QTL-seq and RNA-seq in tomato
Creators: name: Wen, Junqin
name: Jiang, Fangling
name: Weng, Yiqun
name: Sun, Mintao
name: Shi, Xiaopu
name: Zhou, Yanzhao
name: Yu, Lu
name: Wu, Zhen
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Virology

description: Figure S1. The frequency distribution of the three heat tolerance-related physiological indexes in the F2 population. (DOCX 685 kb)
A New Shear Estimator for Weak Lensing Observations
Creators: name: Kaiser, Nick
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new shear estimator for weak lensing observations which properly accounts for the effects of a realistic point spread function (PSF). Images of faint galaxies are subject to gravitational shearing followed by smearing with the instrumental and/or atmospheric PSF. We construct a `finite resolution shear operator' which when applied to an observed image has the same effect as a gravitational shear applied prior to smearing. This operator allows one to calibrate essentially any shear estimator. We then specialize to the case of weighted second moment shear estimators. We compute the shear polarizability which gives the response of an individual galaxy's polarization to a gravitational shear. We then compute the response of the population of galaxies, and thereby construct an optimal weighting scheme for combining shear estimates from galaxies of various shapes, luminosities and sizes. We define a figure of merit --- an inverse shear variance per unit solid angle --- which characterizes the quality of image data for shear measurement. The new method is tested with simulated image data. We discuss the correction for anisotropy of the PSF and propose a new technique involving measuring shapes from images which have been convolved with a re-circularizing PSF. We draw attention to a hitherto ignored noise related bias and show how this can be analyzed and corrected for. The analysis here draws heavily on the properties of real PSF's and we include as an appendix a brief review, highlighting those aspects which are relevant for weak lensing.
description: 39 pages, 9 figures
Jump inequalities for translation-invariant operators of Radon type on $\mathbb{Z}^d$
Creators: name: Mirek, Mariusz
name: Stein, Elias M.
name: Zorin-Kranich, Pavel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 37A45 (Primary) 11K70, 11L07, 42B15, 42B20, 42B25 (Secondary)

description: We prove strong jump inequalities for a large class of operators of Radon type in the discrete and ergodic theoretical settings. These inequalities are the $r=2$ endpoints of the $r$-variational estimates studied in arXiv:1512.07523.
description: v2: 39 pages, revised following referee report
Additional file 1: of Low serum gastrin associated with ER+ breast cancer development via inactivation of CCKBR/ERK/P65 signaling
Creators: name: Meng, Li-Li
name: Jing-Long Wang
name: Xu, Shu-Ping
name: Zu, Li-Dong
name: Yan, Zhao-Wen
name: Zhang, Jian-Bing
name: Han, Ya-Qin
name: Fu, Guo-Hui
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: FOS: Biological sciences
subject: Computational Biology

description: Table S2. Clinical information of 93Â BC patients. Abbreviations: BC, breast cancer; GB, gastric biopsy; F, female; +, lymphatic metastasis present; â , no lymphatic metastasis present; Y/N (GB column), examined/not examined; Y/N (stomach illness without GB column), those with/without stomach illness who did not undergo GB; IDC, invasive ductal cancer; DCIS, ductal cancer in situ; WHO, World Health Organization. (DOCX 36 kb)