cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The PBD-Closure of Constant-Composition Codes
Creators: name: Chee, Yeow Meng
name: Ling, Alan C. H.
name: Ling, San
name: Shen, Hao
Publisher: name: arXiv
Year: 2007
Subjects: subject: Information Theory (cs.IT)
subject: Discrete Mathematics (cs.DM)
subject: Combinatorics (math.CO)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: We show an interesting PBD-closure result for the set of lengths of constant-composition codes whose distance and size meet certain conditions. A consequence of this PBD-closure result is that the size of optimal constant-composition codes can be determined for infinite families of parameter sets from just a single example of an optimal code. As an application, the size of several infinite families of optimal constant-composition codes are derived. In particular, the problem of determining the size of optimal constant-composition codes having distance four and weight three is solved for all lengths sufficiently large. This problem was previously unresolved for odd lengths, except for lengths seven and eleven.
description: 8 pages
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0302
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/2012
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: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0302, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0302, 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
Constructions for Difference Triangle Sets
Creators: name: Chee, Yeow Meng
name: Colbourn, Charles J.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Information Theory (cs.IT)
subject: Discrete Mathematics (cs.DM)
subject: Combinatorics (math.CO)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: E.4

description: Difference triangle sets are useful in many practical problems of information transmission. This correspondence studies combinatorial and computational constructions for difference triangle sets having small scopes. Our algorithms have been used to produce difference triangle sets whose scopes are the best currently known.
description: 4 pages
title: A massive protocluster of galaxies at a redshift of z ≈ 5.3
Creators: name: Capak, PL
name: Riechers, D
name: Scoville, NZ
name: Carilli, C
name: Cox, P
name: Neri, R
name: Robertson, B
name: Savato, M
name: Schinnerer, E
name: Yan, L
name: Wilson, GW
name: Yun, Min
name: Civano, F
name: Elvis, M
name: Karim, A
name: Mobasher, B
name: Staguhn, JG
Publisher: name: University of Massachusetts Amherst
Year: 2011
Subjects: subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://www.nature.com/nature/journal/v470/n7333/full/nature09681.html
description: Massive clusters of galaxies have been found that date from as early as 3.9 billion years1 (3.9 Gyr; z = 1.62) after the Big Bang, containing stars that formed at even earlier epochs2, 3. Cosmological simulations using the current cold dark matter model predict that these systems should descend from ‘protoclusters’—early overdensities of massive galaxies that merge hierarchically to form a cluster4, 5. These protocluster regions themselves are built up hierarchically and so are expected to contain extremely massive galaxies that can be observed as luminous quasars and starbursts4, 5, 6. Observational evidence for this picture, however, is sparse because high-redshift protoclusters are rare and difficult to observe6, 7. Here we report a protocluster region that dates from 1 Gyr (z = 5.3) after the Big Bang. This cluster of massive galaxies extends over more than 13 megaparsecs and contains a luminous quasar as well as a system rich in molecular gas8. These massive galaxies place a lower limit of more than 4 × 1011 solar masses of dark and luminous matter in this region, consistent with that expected from cosmological simulations for the earliest galaxy clusters4, 5, 7.
Dark matter Axion search with riNg Cavity Experiment DANCE: Design and development of auxiliary cavity for simultaneous resonance of linear polarizations
Creators: name: Fujimoto, Hiroki
name: Oshima, Yuka
name: Ando, Masaki
name: Fujita, Tomohiro
name: Michimura, Yuta
name: Nagano, Koji
name: Obata, Ippei
Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Axion-like particles (ALPs) are undiscovered pseudo-scalar particles that are candidates for ultralight dark matter. ALPs interact with photons slightly and cause the rotational oscillation of linearly polarized light. Dark matter Axion search with riNg Cavity Experiment (DANCE) searches for ALP dark matter by amplifying the rotational oscillation with a bow-tie ring cavity. Simultaneous resonance of linear polarizations is necessary to amplify both the carrier field and the ALP signal, and to achieve the design sensitivity. The sensitivity of the current prototype experiment DANCE Act-1 is less than expectation by around three orders of magnitude due to the resonant frequency difference between s- and p-polarization in the bow-tie ring cavity. In order to tune the resonant frequency difference, the method of introducing an auxiliary cavity was proposed. We designed an auxiliary cavity that can cancel out the resonant frequency difference and realize simultaneous resonance, considering optical loss. We also confirmed that the sensitivity of DANCE Act-1 with the auxiliary cavity can reach the original sensitivity.
description: 4 pages, 4 figures, Proceedings for the 17th International Conference on Topics in Astroparticle and Underground Physics, online, August 26 - September 3, 2021
Shell Crossing Singularities in Quasi-Spherical Szekeres Models
Creators: name: Chakraborty, Subenoy
name: Debnath, Ujjal
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate the occurrence of shell crossing singularities in quasi-spherical Szekeres dust models with or without a cosmological constant. We study the conditions for shell crossing singularity both from physical and geometrical point of view and they are in agreement.
description: 10 latex pages, RevTex style, no figures
Applicability of colour index calibrations to T Tauri stars
Creators: name: Schöning, Torsten
name: Ammler, Matthias
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the applicability of effective temperature scales of several broad band colours to T Tauri stars (TTS). We take into account different colour systems as well as stellar parameters like metallicity and surface gravity which influence the conversion from colour indices or spectral type to effective temperature. For a large sample of TTS, we derive temperatures from broad band colour indices and check if they are consistent in a statistical sense with temperatures inferred from spectral types. There are some scales (for V-H, V-K, I-J, J-H, and J-K) which indeed predict the same temperatures as the spectral types and therefore can be at least used to confirm effective temperatures. Furthermore, we examine whether TTS with dynamically derived masses can be used for a test of evolutionary models and effective temperature calibrations. We compare the observed parameters of the eclipsing T Tauri binary V1642 Ori A to the predictions of evolutionary models in both the H-R and the Kiel diagram using temperatures derived with several colour index scales. We check whether the evolutionary models and the colour index scales are consistent with coevality and the dynamical masses of the binary components. It turns out that the Kiel diagram offers a stricter test than the H-R diagram. Only the evolutionary models of Baraffe et al. (1998) with mixing length parameter 1.9 and of D'Antona & Mazzitelli (1994, 1997) show consistent results in the Kiel diagram in combination with some conversion scales of Houdashelt et al. (2000) and of Kenyon & Hartmann (1995).
description: 13 pages, 4 tables, 6 figures, accepted for publication in AN
Strong-field control of x-ray absorption
Creators: name: Santra, Robin
name: Buth, Christian
name: Peterson, Emily R.
name: Dunford, Robert W.
name: Kanter, Elliot P.
name: Krässig, Bertold
name: Southworth, Stephen H.
name: Young, Linda
Publisher: name: arXiv
Year: 2007
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Strong optical laser fields modify the way x rays interact with matter. This allows us to use x rays to gain deeper insight into strong-field processes. Alternatively, optical lasers may be utilized to control the propagation of x rays through a medium. Gas-phase systems are particularly suitable for illustrating the basic principles underlying combined x-ray and laser interactions. Topics addressed include the impact of spin-orbit interaction on the alignment of atomic ions produced in a strong laser field, electromagnetically induced transparency in the x-ray regime, and laser-induced alignment of molecules.
description: 8 pages, 5 figures, 1 table, LaTeX
Additional file 3: of Heparan sulfate proteoglycans undergo differential expression alterations in left sided colorectal cancer, depending on their metastatic character
Creators: name: Crespo, Ainara
name: García-Suárez, Olivia
name: Fernández-Vega, Iván
name: Solis-Hernandez, María Pilar
name: García, Beatriz
name: Castañón, Sonia
name: Quirós, Luis
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: Figure S3. Overall survival in genes displaying statistically significant differences. Only genes with statistical differences are included in this figure. NDST1 underexpression provided a better outcome with an 18-month benefit. The magnitude of the benefit was even higher when CHST12 was downregulated, in more than 50-month. This difference was maintained regardless of lymph node involvement. GCP6 and HS6ST1 underexpression also presented better outcomes, but this magnitude did not reach statistical difference when stratified by node status. (PDF 260 kb)
A Theory For Particle Settling and Shear-Induced Migration in Thin Film Flow
Creators: name: Cook, Benjamin P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Experiments of particle-laden inclined film flow [Zhou, Dupuy, Bertozzi, and Hosoi, Phys. Rev. Lett. 94 (2005)] have displayed different settling behaviors depending on the particle concentration $ϕ$ and angle of inclination $θ$, in which particles accumulate on the substrate or near the advancing contact line, or remain mixed. Zhou et al. presented a lubrication model that captures the qualitative behavior of the high-$ϕ$, high-$θ$ regime, characterized by a particle-rich ridge near the contact line, but cannot explain the other observed settling behaviors. This work presents a model in which $ϕ$ varies through the film depth, unlike Zhou et al.'s model. Average velocities for the liquid and particulate phases are computed, and the implications for phase separation are discussed. It is found that the equilibrium depth profile of $ϕ$ is more important than gravitational settling in the down-slope direction in determining phase separation. The predicted settling behavior is directly compared with Zhou et al.'s experimental data.
description: 4 figures, 4 pages
Oscillatory surface rheotaxis of swimming E. coli bacteria
Creators: name: Mathijssen, Arnold
name: Figueroa-Morales, Nuris
name: Junot, Gaspard
name: Clement, Eric
name: Lindner, Anke
name: Zöttl, Andreas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Bacterial contamination of biological conducts, catheters or water resources is a major threat to public health and can be amplified by the ability of bacteria to swim upstream. The mechanisms of this rheotaxis, the reorientation with respect to flow gradients, often in complex and confined environments, are still poorly understood. Here, we follow individual E. coli bacteria swimming at surfaces under shear flow with two complementary experimental assays, based on 3D Lagrangian tracking and fluorescent flagellar labelling and we develop a theoretical model for their rheotactic motion. Three transitions are identified with increasing shear rate: Above a first critical shear rate, bacteria shift to swimming upstream. After a second threshold, we report the discovery of an oscillatory rheotaxis. Beyond a third transition, we further observe coexistence of rheotaxis along the positive and negative vorticity directions. A full theoretical analysis explains these regimes and predicts the corresponding critical shear rates. The predicted transitions as well as the oscillation dynamics are in good agreement with experimental observations. Our results shed new light on bacterial transport and reveal new strategies for contamination prevention.
description: 12 pages, 5 figures
MOBIL ILOVA YARATISHNI VIRTUAL O'RGATISHDA GLOBAL AXBOROT TIZIMLARI VA TEXNOLOGIYALARI
Creators: name: Axmedova, Zulxumor
Publisher: name: Zenodo
Year: 2024

description: O’zbekiston Respublikasi Prezidentining axborot-kommunikatsion va zamonaviy pedagogik texnologiyalarni ta’lim tizimiga joriy etishga bag’ishlangan Qaror, farmon va nutqlaridan kelib chiqib bugungi kunda ilg’or pedagogik texnologiyalar, ma’lumotlar bazasi  resurslari hamda dasturiy vositalarga bo’lgan ehtiyojning ortishi uni ishlab chiqarish va ta’limda qo’llash masalasi dolzarbligini ko’rsatadi Ushbu maqola  “Respublika o’quv markazlari monitoring olib boruvchi mobil ilova platformasi” ni yaratish mavzusi asosida tayyorlandi.
Product groups acting on manifolds
Creators: name: Furman, Alex
name: Monod, Nicolas
Publisher: name: arXiv
Year: 2007
Subjects: subject: Group Theory (math.GR)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics

description: We analyse volume-preserving actions of product groups on Riemannian manifolds. To this end, we establish a new superrigidity theorem for ergodic cocycles of product groups ranging in linear groups. There are no a priori assumptions on the acting groups, except a spectral gap assumption on their action. Our main application to manifolds concerns irreducible actions of Kazhdan product groups. We prove the following dichotomy: Either the action is infinitesimally linear, which means that the derivative cocycle arises from unbounded linear representations of all factors. Otherwise, the action is measurably isometric, in which case there are at most two factors in the product group. As a first application, this provides lower bounds on the dimension of the manifold in terms of the number of factors in the acting group. Another application is a strong restriction for actions of non-linear groups.
description: To appear in the Duke Mathematical Journal; 32 pages. Minor revisions, including the addition of a variation on Theorem A
A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
Creators: name: Kuznetsova, N.
name: Barbary, K.
name: Connolly, B.
name: Kim, A. G.
name: Pain, R.
name: Roe, N. A.
name: Aldering, G.
name: Amanullah, R.
name: Dawson, K.
name: Doi, M.
name: Fadeyev, V.
name: Fruchter, A. S.
name: Gibbons, R.
name: Goldhaber, G.
name: Goobar, A.
name: Gude, A.
name: Knop, R. A.
name: Kowalski, M.
name: Lidman, C.
name: Morokuma, T.
name: Meyers, J.
name: Perlmutter, S.
name: Rubin, D.
name: Schlegel, D. J.
name: Spadafora, A. L.
name: Stanishev, V.
name: Strovink, M.
name: Suzuki, N.
name: Wang, L.
name: Yasuda, N.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST dataset covering the North GOODS field collected in 2004. We employ a novel technique that does not require spectroscopic data for identifying Type Ia supernovae (although spectroscopic measurements of redshifts are used for over half the sample); instead we employ a Bayesian approach using only photometric data to calculate the probability that an object is a Type Ia supernova. This Bayesian technique can easily be modified to incorporate improved priors on supernova properties, and it is well-suited for future high-statistics supernovae searches in which spectroscopic follow up of all candidates will be impractical. Here, the method is validated on both ground- and space-based supernova data having some spectroscopic follow up. We combine our volumetric rate measurements with low redshift supernova data, and fit to a number of possible models for the evolution of the Type Ia supernova rate as a function of redshift. The data do not distinguish between a flat rate at redshift > 0.5 and a previously proposed model, in which the Type Ia rate peaks at redshift >1 due to a significant delay from star-formation to the supernova explosion. Except for the highest redshifts, where the signal to noise ratio is generally too low to apply this technique, this approach yields smaller or comparable uncertainties than previous work.
description: Accepted for publication in ApJ
Cycle time of stochastic max-plus linear systems
Creators: name: Merlet, Glenn
Publisher: name: arXiv
Year: 2007
Subjects: subject: Probability (math.PR)
subject: Discrete Mathematics (cs.DM)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 60F15, 90B15, 93C65, 93E15

description: We analyze the asymptotic behavior of sequences of random variables defined by an initial condition, a stationary and ergodic sequence of random matrices, and an induction formula involving multiplication is the so-called max-plus algebra. This type of recursive sequences are frequently used in applied probability as they model many systems as some queueing networks, train and computer networks, and production systems. We give a necessary condition for the recursive sequences to satisfy a strong law of large numbers, which proves to be sufficient when the matrices are i.i.d. Moreover, we construct a new example, in which the sequence of matrices is strongly mixing, that condition is satisfied, but the recursive sequence do not converges almost surely.
description: This article has been published by IMS in Electronic Journal of Probability at http://www.math.washington.edu/~ejpecp/viewarticle.php?id=1781
High-flux 100-kHz attosecond pulse source driven by a high average power annular laser beam
Creators: name: Ye, Peng
name: Oldal, Lénárd Gulyás
name: Csizmadia, Tamás
name: Filus, Zoltán
name: Grósz, Tímea
name: Jójárt, Péter
name: Seres, Imre
name: Bengery, Zsolt
name: Gilicze, Barnabás
name: Kahaly, Subhendu
name: Varjú, Katalin
name: Major, Balázs
Publisher: name: arXiv
Year: 2021
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: High-repetition-rate attosecond pulse sources are indispensable tools of time-resolved studies of electron dynamics, such as coincidence spectroscopy and experiments with high demands on statistics or signal-to-noise ratio, especially in case of solid and big molecule samples in chemistry and biology. Although with the high-repetition-rate lasers such attosecond pulses in a pump-probe configuration are possible to achieve, until now only a few such light sources have been demonstrated. Here, by shaping the driving laser to an annular beam, a 100-kHz attosecond pulse train (APT) is reported with the highest energy so far (51 pJ/shot) on target (269 pJ at generation) among the high-repetition-rate systems (> 10 kHz) in which the attosecond pulses were temporally characterized. The on-target pulse energy is maximized by reducing the losses from the reflections and filtering of the high harmonics, and an unprecedented 19% transmission rate from the generation point to the target position is achieved. At the same time, the probe beam is also annular, and low loss of this beam is reached by using another holey mirror to combine with the APT. The advantages of using an annular beam to generate attosecond pulses with a high average power laser is demonstrated experimentally and theoretically. The effect of nonlinear propagation in the generation medium on the annular-beam generation concept is also analyzed in detail.
description: 19 pages, 7 figures, after peer review
MOESM4 of Prevalence of human pathogenic Yersinia enterocolitica in Swedish pig farms
Creators: name: Råsbäck, Therese
name: Rosendal, Thomas
name: Stampe, Michael
name: Sannö, Axel
name: Aspán, Anna
name: Järnevi, Katarina
name: Lahti, Elina
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 4: Appendix Table S1. The proportion of herds positive for Yersinia enterocolitica for each of the categorical variable levels recorded in the questionnaire. The P-values and associated odds ratios for the association of each variable with pen level Y. enterocolitica status, tested by logistic regression controlling for repeated pen measurements within herd by a random effect.
Additional file 13: of Comparative analysis of binding patterns of MADS-domain proteins in Arabidopsis thaliana
Creators: name: Aerts, Niels
name: Bruijn, Suzanne De
name: Mourik, Hilda Van
name: Angenent, Gerco
name: Dijk, Aalt Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Figure S7. Central enrichment of G-boxes and TCP class I and II. Kernel density plot showing positions in peak centers relative to the peak summit of matches to the G-box (CACGTG) and the motifs for TCP class I (GGNCCCAC) and class II (GGGNCC(A/G)C) in (A) AG; (B) AP1; (C) AP3; (D) FLC; (E) PI; (F) SEP3; (G) SOC1 and (H) SVP. (PDF 232 kb)
Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters
Creators: name: Adam, R.
name: Hahn, O.
name: Ruppin, F.
name: Ade, P.
name: André, P.
name: Arnaud, M.
name: Bartalucci, I.
name: Beelen, A.
name: Benoît, A.
name: Bideaud, A.
name: Billot, N.
name: Bourrion, O.
name: Calvo, M.
name: Catalano, A.
name: Coiffard, G.
name: Comis, B.
name: D'Addabbo, A.
name: Désert, F. -X.
name: Doyle, S.
name: Ferrari, C.
name: Goupy, J.
name: Kramer, C.
name: Lagache, G.
name: Leclercq, S.
name: Lestrade, J. -F.
name: Macías-Pérez, J. F.
name: MartinezAviles, G.
name: Martizzi, D.
name: Maurogordato, S.
name: Mauskopf, P.
name: Mayet, F.
name: Monfardini, A.
name: Pajot, F.
name: Pascale, E.
name: Perotto, L.
name: Pisano, G.
name: Pointecouteau, E.
name: Ponthieu, N.
name: Pratt, G. W.
name: Revéret, V.
name: Ricci, M.
name: Ritacco, A.
name: Rodriguez, L.
name: Romero, C.
name: Roussel, H.
name: Schuster, K.
name: Sievers, A.
name: Triqueneaux, S.
name: Tucker, C.
name: Wu, H. -Y.
name: Zylka, R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Sub-structures in the hot gas of galaxy clusters are related to their formation history and to the astrophysical processes at play in the intracluster medium (ICM). The thermal Sunyaev-Zel'dovich (tSZ) effect is directly sensitive to the line-of-sight integrated ICM pressure, and is thus particularly adapted to study ICM sub-structures. We apply structure-enhancement filtering algorithms to high resolution tSZ observations of distant clusters, in order to search for pressure discontinuities, compressions, as well as secondary peaks in the ICM. The same filters are applied to synthetic tSZ images extracted from RHAPSODY-G hydrodynamic simulations, in order to better interpret the extracted features. We also study the noise propagation trough the filters and quantify the impact of systematic effects, point source residuals being identified as the dominant potential contaminant. In 3 of our 6 NIKA clusters we identify features at high S/N that show clear evidence for merger events. In MACSJ0717 (z=0.55), three strong pressure gradients are observed on the E, SE and W sectors, and two main peaks in the pressure distribution are identified. We observe a lack of tSZ compact structure in the cool-core cluster PSZ1G045.85 (z=0.61), and a tSZ gradient ridge dominates in the SE. In the highest z cluster, CLJ1227 (z=0.89), we detect a ~45" (360 kpc) long ridge pressure gradient associated with a secondary pressure peak in the W region. Our results show that current tSZ facilities have now reached the angular resolution and sensitivity to allow an exploration of the details of pressure sub-structures in clusters, even at high z. This opens the possibility to quantify the impact of the dynamical state on the relation between the tSZ signal and the mass of clusters, which is important when using tSZ clusters to test cosmological models. This work also marks the first NIKA cluster sample data release.
description: Accepted in A&A
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1231
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/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1231, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1231, 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
Latitudinal variation of the solar photospheric intensity
Creators: name: Rast, Mark P.
name: Ortiz, Ada
name: Meisner, Randle W.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have examined images from the Precision Solar Photometric Telescope (PSPT) at the Mauna Loa Solar Observatory (MLSO) in search of latitudinal variation in the solar photospheric intensity. Along with the expected brightening of the solar activity belts, we have found a weak enhancement of the mean continuum intensity at polar latitudes (continuum intensity enhancement $\sim0.1 - 0.2%$ corresponding to a brightness temperature enhancement of $\sim2.5{\rm K}$). This appears to be thermal in origin and not due to a polar accumulation of weak magnetic elements, with both the continuum and CaIIK intensity distributions shifted towards higher values with little change in shape from their mid-latitude distributions. Since the enhancement is of low spatial frequency and of very small amplitude it is difficult to separate from systematic instrumental and processing errors. We provide a thorough discussion of these and conclude that the measurement captures real solar latitudinal intensity variations.
description: 24 pages, 8 figs, accepted in ApJ
title: A GREEN BANK TELESCOPE SURVEY FOR H I 21 cm ABSORPTION IN THE DISKS AND HALOS OF LOW-REDSHIFT GALAXIES*
Creators: name: Borthakur, S
name: Tripp, TM
name: Yun, Min
name: Bowen, DV
name: Meiring, JD
name: York, DG
name: Momjian, E
Publisher: name: University of Massachusetts Amherst
Year: 2011
Subjects: subject: galaxies: abundances; galaxies: ISM; quasars: absorption lines
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://iopscience.iop.org/0004-637X/727/1/52/
description: We present an H I 21 cm absorption survey with the Green Bank Telescope (GBT) of galaxy-quasar pairs selected by combining galaxy data from the Sloan Digital Sky Survey (SDSS) and radio sources from the Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) survey. Our sample consists of 23 sight lines through 15 low-redshift foreground galaxy-background quasar pairs with impact parameters ranging from 1.7 kpc up to 86.7 kpc. We detected one absorber in the GBT survey from the foreground dwarf galaxy, GQ1042+0747, at an impact parameter of 1.7 kpc and another possible absorber in our follow-up Very Large Array (VLA) imaging of the nearby foreground galaxy UGC 7408. The line widths of both absorbers are narrow (FWHM of 3.6 and 4.8km s–1). The absorbers have sub-damped Lyα column densities, and most likely originate in the disk gas of the foreground galaxies. We also detected H I emission from three foreground galaxies including UGC 7408. Although our sample contains both blue and red galaxies, the two H I absorbers as well as the H I emissions are associated with blue galaxies. We discuss the physical conditions in the 21 cm absorbers and some drawbacks of the large GBT beam for this type of survey.
Contragredient representations over local fields of positive characteristic
Creators: name: Li, Wen-Wei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Representation Theory (math.RT)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 11F70 (Primary) 22E55 (Secondary)

description: It is conjectured by Adams-Vogan and Prasad that under the local Langlands correspondence, the L-parameter of the contragredient representation equals that of the original representation composed with the Chevalley involution of the L-group. We verify a variant of their prediction for all connected reductive groups over local fields of positive characteristic, in terms of the local Langlands parameterization of Genestier-Lafforgue. We deduce this from a global result for cuspidal automorphic representations over function fields, which is in turn based on a description of the transposes of V. Lafforgue's excursion operators.
description: 42 pages. Updated the references
Prediction of flow dynamics using point processes
Creators: name: Hirata, Yoshito
name: Stemler, Thomas
name: Eroglu, Deniz
name: Marwan, Norbert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Describing a time series parsimoniously is the first step to study the underlying dynamics. For a time-discrete system, a generating partition provides a compact description such that a time series and a symbolic sequence are one-to-one. But, for a time-continuous system, such a compact description does not have a solid basis. Here, we propose to describe a time-continuous time series using a local cross section and the times when the orbit crosses the local cross section. We show that if such a series of crossing times and some past observations are given, we can predict the system's dynamics with fine accuracy. This reconstructability neither depends strongly on the size nor the placement of the local cross section if we have a sufficiently long database. We demonstrate the proposed method using the Lorenz model as well as the actual measurement of wind speed.
description: 7 pages, 5 figures
Additional file 1: of Modelling the impact of social protection on tuberculosis: the S-PROTECT project
Creators: name: D. Boccia
name: W. Rudgard
name: S. Shrestha
name: K. LĂśnnroth
name: P. Eckhoff
name: J. Golub
name: M. Sanchez
name: E. Maciel
name: D. Rasella
name: P. Shete
name: D. Pedrazzoli
name: R. Houben
name: S. Chang
name: D. Dowdy
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: Computational Biology

description: Appendix 1. Data review strategy. Appendix 2. Assumptions for pathway #10. Appendix 3. Model parameters affected by Pathway #10. (PDF 461Â kb)
Effective field theories for QCD with rooted staggered fermions
Creators: name: Bernard, Claude
name: Golterman, Maarten
name: Shamir, Yigal
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Even highly improved variants of lattice QCD with staggered fermions show significant violations of taste symmetry at currently accessible lattice spacings. In addition, the "rooting trick" is used in order to simulate with the correct number of light sea quarks, and this makes the lattice theory nonlocal, even though there is good reason to believe that the continuum limit is in the correct universality class. In order to understand scaling violations, it is thus necessary to extend the construction of the Symanzik effective theory to include rooted staggered fermions. We show how this can be done, starting from a generalization of the renormalization-group approach to rooted staggered fermions recently developed by one of us. We then explain how the chiral effective theory follows from the Symanzik action, and show that it leads to "rooted" staggered chiral perturbation theory as the correct chiral theory for QCD with rooted staggered fermions. We thus establish a direct link between the renormalization-group based arguments for the correctness of the continuum limit and the success of rooted staggered chiral perturbation theory in fitting numerical results obtained with the rooting trick. In order to develop our argument, we need to assume the existence of a standard partially-quenched chiral effective theory for any local partially-quenched theory. Other technical, but standard, assumptions are also required.
description: Minor changes, few references added; RevTeX, 35 pages
Additional file 2 of Symptoms awareness, emergency medical service utilization and hospital transfer delay in myocardial infarction
Creators: name: CĂŠzar Mesas
name: Rodrigues, Ricardo
name: Mesas, Arthur
name: FeijĂł, Vivian
name: Paraiso, Lucas
name: Bragatto, Gabriela
name: Moron, Viviane
name: Bergonso, Marcos
name: Laercio Uemura
name: Grion, Cintia
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified

description: Response to Symptoms Questionnaire (Portuguese version). Version of symptons questionnaire modified by Dracup K and Moser DK. Beyond sociodemographics: Factors influencing the decision to seek treatment for symptoms of acute myocardial infarction. (DOCX 15 kb)
title: Solutions naturopathie
title: une approche globale de la santé entre science et tradition
titleType: Subtitle
title: Solutions naturopathie
titleType: AlternativeTitle
Creators: name: PureSanté Editions SA
Publisher: name: PureSanté Editions SA
Year: 2021

description: Avant 2021, l'éditeur n'exerçait pas dans le canton de Vaud.
Oscillatory Modes of a Prominence-PCTR-Corona Slab Model
Creators: name: Soler, R.
name: Oliver, R.
name: Ballester, J. L.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Oscillations of magnetic structures in the solar corona have often been interpreted in terms of magnetohydrodynamic waves. We study the adiabatic magnetoacoustic modes of a prominence plasma slab with a uniform longitudinal magnetic field, surrounded by a prominence-corona transition region (PCTR) and a coronal medium. Considering linear small-amplitude oscillations, the dispersion relation for the magnetoacoustic slow and fast modes is deduced assuming evanescent-like perturbations in the coronal medium. In the system without PCTR, a classification of the oscillatory modes according to the polarisation of their eigenfunctions is made in order to distinguish modes with fast-like or slow-like properties. Internal and external slow modes are governed by the prominence and coronal properties respectively, and fast modes are mostly dominated by prominence conditions for the observed wavelengths. In addition, the inclusion of an isothermal PCTR does not substantially influence the mode frequencies, but new solutions (PCTR slow modes) are present.
description: Accepted for publication in Solar Physics
The Monge-Ampère-Kantorovich approach to reconstruction in cosmology
Creators: name: Mohayaee, Roya
name: Sobolevskii, Andrei
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Motion of a continuous fluid can be decomposed into an "incompressible" rearrangement, which preserves the volume of each infinitesimal fluid element, and a gradient map that transfers fluid elements in a way unaffected by any pressure or elasticity (the polar decomposition of Y. Brenier). The Euler equation describes a system whose kinematics is dominated by the incompressible rearrangement. The opposite limit, in which the incompressible component is negligible, corresponds to the Zel'dovich approximation, a model of motion of self-gravitating fluid in cosmology. We present a method of approximate reconstruction of the large-scale proper motions of matter in the Universe from the present-day mass density field. The method is based on recovering the corresponding gradient transfer map. We discuss its algorithmics, tests of the method against mock cosmological catalogues, and its application to observational data, which result in tight constraints on the mean mass density Omega_m and age of the Universe.
description: 6 pages, 2 figures; based on an invited lecture at the conference "Euler's Equations: 250 Years On" (see http://www.obs-nice.fr/etc7/EE250/); to be published in a special issue of Physica D containing the proceedings of that conference
Generalised Potential Functions in Differential Geometry and Information Geometry
Creators: name: Ciaglia, Florio M.
name: Marmo, Giuseppe
name: Pérez-Pardo, Juan Manuel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C99, 53Z05, 53A40

description: Potential functions can be used as generating potentials of relevant geometric structures for a Riemannian manifold such as the Riemannian metric and affine connections. We study wether this procedure can also be applied to tensors of rank four and find a negative answer. We study this from the perspective of solving the inverse problem and also from an intrinsic point of view.
description: 16 pages
Design and testing of an sTGC ASIC interface board for the ATLAS New Small Wheel upgrade
Creators: name: Wang, Xu
name: Guan, Liang
name: Sun, Siyuan
name: Zhou, Bing
name: Zhu, Junjie
name: Jin, Ge
Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The ATLAS experiment will replace the present Small Wheel (SW) detector with a New Small Wheel detector (NSW) aiming to improve the performance of muon triggering and precision tracking in the endcap region at the High-Luminosity LHC. Small-strip Thin Gap Chamber (sTGC) is one of the two new detector technologies used in this upgrade. A few custom-designed ASICs are needed for the sTGC detector. We designed an sTGC ASIC interface board to test ASIC-to-ASIC communication and validate the functionality of the entire system. A test platform with the final readout system is set up and the whole sTGC readout chain is demonstrated for the first time. Key parameters in the readout chain are discussed and the results are shown.
description: 11 pages, 7 figures
Strobe Checklist for (Prescribing Pattern of Antidiabetic Drugs and its adherence to ADA guidelines in patients of Type 2 with and without co-morbidities in Rural Tertiary Care Hospital in Central India)
Creators: name: AMIN, DR. SHANTANU
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 321402
subject: Clinical pharmacology and therapeutics

description: Strobe Checklist for (Prescribing Pattern of Antidiabetic Drugs and its adherence to ADA guidelines in patients of Type 2 with and without co-morbidities in Rural Tertiary Care Hospital in Central India).
Fusion of Correlated Decisions Using Regular Vine Copulas
Creators: name: Zhang, Shan
name: Theagarajan, Lakshmi Narasimhan
name: Choi, Sora
name: Varshney, Pramod K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In this paper, we propose a regular vine copula based methodology for the fusion of correlated decisions. Regular vine copula is an extremely flexible and powerful graphical model to characterize complex dependence among multiple modalities. It can express a multivariate copula by using a cascade of bivariate copulas, the so-called pair copulas. Assuming that local detectors are single threshold binary quantizers and taking complex dependence among sensor decisions into account, we design an optimal fusion rule using a regular vine copula under the Neyman-Pearson framework. In order to reduce the computational complexity resulting from the complex dependence, we propose an efficient and computationally light regular vine copula based optimal fusion algorithm. Numerical experiments are conducted to demonstrate the effectiveness of our approach.
Untitled Item strobe checklist for (analysis of prescription pattern and adverse drug reactions of drugs used in Urinary Tract Infection in reproductive age group (15-44 years) women in a Tertiary Care Hospital in Central India - An observational retrospective study)
Creators: name: patil, gayatri
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 321402
subject: Clinical pharmacology and therapeutics

description: strobe checklist for (analysis of prescription pattern and adverse drug reactions of drugs used in Urinary Tract Infection in reproductive age group (15-44 years) women in a Tertiary Care Hospital in Central India - An observational retrospective study)
The 2+1 flavor topological susceptibility from the asqtad action at 0.06 fm
Creators: name: Bernard, C.
name: Billeter, B.
name: DeTar, C.
name: Levkova, L.
name: Gottlieb, Steven
name: Heller, U. M.
name: Hetrick, J. E.
name: Osborn, J.
name: Renner, D. B.
name: Toussaint, D.
name: Sugar, R.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We report new data for the topological susceptibility computed on 2+1 flavor dynamical configurations with lattice spacing 0.06 fm, generated with the asqtad action. The topological susceptibility is computed by HYP smearing and compared with rooted staggered chiral perturbation theory as the pion mass goes to zero. At 0.06 fm, the raw data is already quite close to the continuum extrapolated values obtained from coarser lattices. These results provide a further test of the asqtad action with rooted staggered flavors.
description: 7 pages, 5 figures, talk presented at the XXV International Symposium on Lattice Field Theory, July 30 - August 4, 2007, Regensburg, Germany
MOESM3 of Transcranial magnetic stimulation and amyloid markers in mild cognitive impairment: impact on diagnostic confidence and diagnostic accuracy
Creators: name: Padovani, Alessandro
name: Benussi, Alberto
name: Cotelli, Maria
name: Ferrari, Clarissa
name: Cantoni, Valentina
name: Dell’Era, Valentina
name: Turrone, Rosanna
name: Paghera, Barbara
name: Borroni, Barbara
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Cell Biology
Neuroscience

description: Additional file 3: Table S1. Cerebrospinal fluid markers, amyloid PET imaging and TMS parameters in MCI subtypes according to “gold standard” diagnosis.
MatchNAS: Optimizing Edge AI in Sparse-Label Data Contexts via Automating Deep Neural Network Porting for Mobile Deployment
Creators: name: Huang, Hongtao
name: Chang, Xiaojun
name: Hu, Wen
name: Yao, Lina
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: Recent years have seen the explosion of edge intelligence with powerful Deep Neural Networks (DNNs). One popular scheme is training DNNs on powerful cloud servers and subsequently porting them to mobile devices after being lightweight. Conventional approaches manually specialized DNNs for various edge platforms and retrain them with real-world data. However, as the number of platforms increases, these approaches become labour-intensive and computationally prohibitive. Additionally, real-world data tends to be sparse-label, further increasing the difficulty of lightweight models. In this paper, we propose MatchNAS, a novel scheme for porting DNNs to mobile devices. Specifically, we simultaneously optimise a large network family using both labelled and unlabelled data and then automatically search for tailored networks for different hardware platforms. MatchNAS acts as an intermediary that bridges the gap between cloud-based DNNs and edge-based DNNs.