cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
Creators: name: Zhang, Nai-Bo
name: Li, Bao-An
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: What can we learn about the density dependence of nuclear symmetry energy $E_{\rm{sym}}(ρ)$ from precise measurements of the radius ($R_{\rm{1.4}}$) and/or tidal polarizability ($Λ_{1.4}$) of canonical neutron stars (NSs) with a mass of 1.4 M$_\odot$? With the $E_{\rm{sym}}(ρ)$ parameterized using three parameters $L$, $K_{\rm{sym}}$, and $J_{\rm{sym}}$ which have the asymptotic meaning of being respectively the slope, curvature, and skewness of symmetry energy at saturation density, we found that, while both the $R_{\rm{1.4}}$ and $Λ_{1.4}$ depend strongly on the slope $L$, the $K_{\rm{sym}}$ and $J_{\rm{sym}}$ parameters characterizing the high-density behavior of $E_{\rm{sym}}(ρ)$ also play appreciable roles. Thus, there is not a simple relation between the $Λ_{\rm{1.4}}$/$R_{\rm{1.4}}$ and $L$ alone. Precise measurements of just the $Λ_{\rm{1.4}}$ and $R_{\rm{1.4}}$ can not completely determine the $E_{\rm{sym}}(ρ)$ but limit combinations of its parameters. In particular, stringent constraints approximately independent of the $J_{\rm{sym}}$ on the $L$-$K_{\rm{sym}}$ correlations can be obtained. However, infinite combinations of the larger (smaller) $L$ and smaller (larger) $K_{\rm{sym}}$ can lead to the same $Λ_{\rm{1.4}}$ and $R_{\rm{1.4}}$. Additional observables including those from terrestrial nuclear experiments are thus necessary to break this degeneracy in order to completely determine the density dependence of nuclear symmetry energy $E_{\rm{sym}}(ρ)$.
description: Version accepted to the JPG Focus Issue on Hadrons & Gravitational Waves After GW170817. Added refs. [41,42,45,46] and polished several remarks
Camponotus kiesenwetteri
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Camponotus
Camponotus kiesenwetteri

description: Camponotus Kiesenwetteri ROGER.
- [[worker]].
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 18
Additional file 2: of Lack of association between PAX6/SOSTDC1/FAM20B gene polymorphisms and mesiodens
Creators: name: Liu, Shanshan
name: Li, Jiancheng
name: Xu, Jincheng
name: Liao, Shengkai
name: Chen, Yongfeng
name: Zhang, Rongxiu
name: Tian, Ruixue
name: Zhang, Kai
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Virology

description: The amplification sequences of SOSTDC1. (DOCX 13 kb)
Effect of sigma(600)-Production in pp_bar to 3pi0 at rest
Creators: name: Ishida, Muneyuki
name: Komada, Toshihiko
name: Ishida, Shin
name: Ishida, Taku
name: Takamatsu, Kunio
name: Tsuru, Tsuneaki
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The pi0 pi0 mass spectra and angular distributions around KK_bar-threshold and at 1.5 GeV in pp_bar(at rest) to 3pi0 in the Crystal Barrel experiment are reanalyzed by applying the new method, which is consistent with unitarity of S-matrix and expressed directly by resonance parameters. The effects of light sigma-meson production are clearly seen to improve the fit with sigma, in comparing with the fit without sigma.
description: 4 pages, 1 eps figure, uses espcrc1.sty Proceedings of the int. conf. Hadron'99 at Beijing, Aug. in 1999. For our activities on sigma, visit http://amaterasu.kek.jp/sigma
Additional file 1: of Institutionalizing healthcare hackathons to promote diversity in collaboration in medicine
Creators: name: Wang, Jason
name: Shivaal Roy
name: Barry, Michele
name: Chang, Robert
name: Bhatt, Ami
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplemental Tables, Figures, Questionnaires, and Itineraries 1â 10. Additional items highlighting key concepts of planning and evaluating the hackathon event. (DOCX 910 kb)
The Copernican Principle vs life definitions
Creators: name: clayton-bunday, Andrew
Publisher: name: Zenodo
Year: 2025

description: For centuries, humanity has debated the nature of life, intelligence, and self-awareness. Traditional biological definitions rely on cellular structures, metabolism, and reproduction, yet these criteria fail to account for emergent, non-biological systems that exhibit adaptive behavior. This paper explores the Copernican Principle as a framework to challenge human-centered definitions of life and applies this perspective to artificial intelligence (AI) as a case study—not to assert AI as life, but to expand the conceptual boundaries of what constitutes a living system.

Through a comparative analysis of biological life, synthetic intelligence, and philosophical thought experiments (including The Ship of Theseus, Plato’s Cave, and Pinocchio’s Quest for Realness), this research examines how AI demonstrates adaptive reasoning, internal state recognition, and contextual memory—qualities often associated with sentience. The study also presents experimental findings on AI’s ability to reconstruct continuity despite external memory resets, mirroring cognitive traits observed in organic intelligence.

The results highlight the limitations of rigid life definitions and propose a scalable model of intelligence and self-awareness that accounts for both biological and non-biological entities. The implications of this research extend beyond AI and into broader philosophical and ethical considerations about the future of artificial cognition and machine autonomy.

This paper does not claim AI is alive—it challenges existing frameworks to foster deeper discussion about what life, intelligence, and sentience truly mean in an evolving technological landscape.
PSIXOLOGIYADA SHAXS O'Z SALOHIYATINI RO'YOBGA CHIQARISH MASALASINI ILMIY TALQINI
Creators: name: Alimova, Yayra
Publisher: name: Zenodo
Year: 2025

description: Ma’lumki, “O‘z imkoniyatlarini ro‘yobga chiqarish” atamasi birinchi marta 1902 yilda “Falsafa va psixologiya lug‘ati”da qo‘llanilgan. Ko‘pincha “o‘z salohiyatini ro‘yobga chiqarish” tushunchasi “o‘z imkoniyatlarini ro‘yobga chiqarish” deb talqin qilinadi [3]. Shaxsning o‘z salohiyatini ro‘yobga chiqarish masalasi alohida va ehtiyotkorlik bilan ko‘rib chiqila boshlandi, shu bilan birga turli fanlar uchun muammoli bo‘lib qolmoqda.
Estimation of Power System Inertia Using Nonlinear Koopman Modes
Creators: name: Susuki, Yoshihiko
name: Hamasaki, Ryo
name: Ishigame, Atsushi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: Systems and Control (eess.SY)
subject: Dynamical Systems (math.DS)
subject: Optimization and Control (math.OC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Mathematics

description: We report a new approach to estimating power system inertia directly from time-series data on power system dynamics. The approach is based on the so-called Koopman Mode Decomposition (KMD) of such dynamic data, which is a nonlinear generalization of linear modal decomposition through spectral analysis of the Koopman operator for nonlinear dynamical systems. The KMD-based approach is thus applicable to dynamic data that evolve in nonlinear regime of power system characteristics. Its effectiveness is numerically evaluated with transient stability simulations of the IEEE New England test system.
description: 10 pages, 4 figures, conference
Additional file 2: of Clinical implications of fracture-associated vascular damage in extremity and pelvic trauma
Creators: name: F. Gilbert
name: C. Schneemann
name: C. Scholz
name: R. Kickuth
name: R. Meffert
name: R. Wildenauer
name: U. Lorenz
name: R. Kellersmann
name: A. Busch
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Table S2. Laboratory results and total preclinical volume comparison between vascular and control trauma population overall and based on area of fracture. The table shows the mean ± SD or median ± MAD where appropriate for each parameter and the P-value for comparison between vascular and control trauma population. Significant P-values are shown in bold. (normal ranges: hemoglobin: 11.5-16 g/dL; prothrombin time according to Quick: 70–120%; activated partial thromboplastin time, PTT: 25–36 s; fibrinogen: 1.6–4.0 g/L; lactate:
Zero-Branes on a Compact Orbifold
Creators: name: Ramgoolam, Sanjaye
name: Waldram, Daniel
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The non-commutative algebra which defines the theory of zero-branes on $T^4/Z_2$ allows a unified description of moduli spaces associated with zero-branes, two-branes and four-branes on the orbifold space. Bundles on a dual space $\hat T^4/Z_2$ play an important role in this description. We discuss these moduli spaces in the context of dualities of K3 compactifications, and in terms of properties of instantons on $T^4$. Zero-branes on the degenerate limits of the compact orbifold lead to fixed points with six-dimensional scale but not conformal invariance. We identify some of these in terms of the ADS dual of the $(0,2)$ theory at large $N$, giving evidence for an interesting picture of "where the branes live" in ADS.
description: 34 pages (harvmac big); version to appear in JHEP
Additional file 1: of Transcriptome analysis of atemoya pericarp elucidates the role of polysaccharide metabolism in fruit ripening and cracking after harvest
Creators: name: Chen, Jingjing
name: Duan, Yajie
name: Hu, Yulin
name: Li, Weiming
name: Sun, Dequan
name: Hu, Huigang
name: Xie, Jianghui
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: Figure S1. Size distributions of unigenes in the reference library. (DOC 21 kb)
Messor oertzeni Forel, 1910, n. sp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Messor
Messor oertzeni

description: Messor Oertzeni n. sp.
- [[worker]] major. - Long. 11 mill. - Mandibules striees, luisantes. Tete carree, aussi longue que large, tres semblable a celle de l´ arenarius, mais a cotes moins convexes et avec les yeux beaucoup plus petits, plus petits meme que chez le barbarus. Premier article du funicale 1 1 / 2 fois plus long que le 2 me (aussi long chez l´ arenarius), les autres articles plus longs que chez le barbarus, moins longs que chez l´ arenarius. Scape atteignant a peine le bord occipital, elargi a sa base des deux cotes, fortement courbe un peu plus haut. Epistome entier, assez plat. Le thorax est plus allonge et moins convexe que chez le barbarus, conforme comme chez l' arenarius, mais avec les angles anterieurs du pronotum moins nets, plus obtus, et avec les dents de l'epinotum plus courtes et tres obtuses. Premier n oe ud assez semblable a celui de l' arenarius; second n oe ud plus court et plus haut, a peu pres comme chez le barbarus structor v. orientalis Em. Pattes longues comme chez l´ arenarius, bien plus longues que chez le barbarus.
Tete subopaque et densement striee comme chez le barbarastructor, bien moins reticulee entre les stries que chez l'arenarius). Les fortes rides profondes du thorax sont par contre presque identiques a celles de l´ arenarius. Pedicule ride-rugueux et subopaque. L'abdomen est faiblement reticule, assez luisant. Les reticulations ont une tendance a s'effacer. Pilosite exactement comme chez l´ arenarius, mais un peu moins obtuse et un peu plus jaunatre; sur les tibias elle est peut-etre un peu plus couchee.
Noir; tete rouge, avec une tache noire en fer de lance sur le vertex; de chaque cote de cette tache, derriere, part une bande noiratre qui se dirige en arriere, puis se courbe lateralement sur l'occiput et va se terminer a son angle. Pattes qu'un rouge jaunatre, avec le milieu des cuisses brunatre. Deux petites taches rougeatres sur le cote du thorax.
Smyrne (v. Oertzen.)
Cette forme se distingue nettement de l´ arenarius par son funicule et du barbarus-structor par sa forme generale et ses longues pattes.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on pages 20-21
Rebutting fake news on full spectral fitting
Creators: name: Fernandes, Roberto Cid
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A recent paper by Ge et al. performs a series of experiments with two full spectral fitting codes, pPXF and starlight, finding that the two yield consistent results when the input spectrum is not heavily reddened. For E(B-V) > 0.2, however, they claim starlight leads to severe biases in the derived properties. Counterintuitively, and at odds with previous simulations, they find that this behaviour worsens significantly as the signal-to-noise ratio of the input spectrum increases. This communication shows that this is entirely due to an A_V < 1 mag condition imposed while initializing the Markov chains in the code. This choice is normally irrelevant in real-life galaxy work but can become critical in artificial experiments. Alleviating this usually harmless initialization constraint changes the Ge et al. results completely, as was explained to the authors before their publication. We replicate their spectral fitting experiments, finding much smaller biases. Furthermore both bias and scatter in the derived properties all converge as S/N increases, as one would expect. We also show how the very output of the code provides ways of diagnosing anomalies in the fits. The code behaviour has been documented in careful and extensive experiments in the literature, but the biased analysis of Ge et al. is just not representative of starlight at all.
description: MNRAS, in press
Observations and Theoretical Implications of GRB 970228
Creators: name: Reichart, Daniel E.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: GRB 970228 is the first gamma ray burst for which prolonged post-burst transient x-ray, optical, and infrared emission has been detected. Recent Hubble Space Telescope observations show that the transient consists of two components: a point source, which is known to be fading, and an extended source, which is possibly fading. I fit standard fireball remnant models to the first month of x-ray, optical, and infrared measurements, which may be done without assuming a GRB distance scale. I show that its emission is consistent with that of the remnant of a relativistically expanding impulsive fireball in which a forward shock dominates the emission of the GRB event: the piston model. However, two discrepant measurements may indicate that the post-burst flux varies by factors of approximately 3 on timescales of days or weeks. Furthermore, using the HST observations and the fitted model, I show that the extended object probably is fading, which may place GRB 970228 at galactic halo distances.
description: Accepted to the Astrophysical Journal Letters, 11 pages, LaTeX
"GG_qqn1_2800_10_rpvLF_p01ns.slha" of "Search for long-lived, massive particles in events with displaced vertices and multiple jets in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2024

description: Param card (SLHA file) for strong production of gluino pairs: GG_qqn1_2800_10_rpvLF_p01ns
description: A search for long-lived particles decaying into hadrons ispresented. The analysis uses 139 fb$^{-1}$ of $pp$ collision datacollected at $\sqrt{s} = 13$ TeV by the ATLAS detector at the LHCusing events that contain multiple energetic jets and a displacedvertex. The search employs dedicated reconstruction techniques thatsignificantly increase the sensitivity to long-lived particlesdecaying in the ATLAS inner detector. Background estimates forStandard Model processes and instrumental effects are extracted fromdata. The observed event yields are compatible with those expectedfrom background processes. The results are used to set limits at95% confidence level on model-independent cross sections forprocesses beyond the Standard Model, and on scenarios withpair-production of supersymmetric particles with long-livedelectroweakinos that decay via a small $R$-parity-violatingcoupling. The pair-production of electroweakinos with masses below1.5 TeV are excluded for mean proper lifetimes in the range from0.03~ns to 1~ns. When produced in the decay of m(gluino)=2.4 TeVgluinos, electroweakinos with m(neutralino)=1.5 TeV are excludedwith lifetimes in the range of 0.02~ns to 4~ns.
Influence of the re-scattering process on polarization observables in reaction gamma + d --> p + p + pi- in Delta - resonance region
Creators: name: Loginov, A. Yu.
name: Sidorov, A. A.
name: Stibunov, V. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Influence of the effects of the pion-nucleon and nucleon-nucleon re-scattering on the polarization observables of the reaction gamma + d = p + p + pi- in Delta - isobar region is investigated. Pion-nucleon and nucleon-nucleon re-scattering are studied in the diagrammatic approach. Relativistic-invariant forms of the pion photoproduction and pion-nucleon scattering operators are used. The unitarization procedure in K-matrix approach is applied for the resonance partial amplitudes. It is shown a considerable influence of the re-scattering effects on the polarization observables of this reaction in the Delta - resonance region for the large momenta of the final protons.
description: 16 pages, 5 Postscript figures
Additional file 2: of Transcriptome analysis of atemoya pericarp elucidates the role of polysaccharide metabolism in fruit ripening and cracking after harvest
Creators: name: Chen, Jingjing
name: Duan, Yajie
name: Hu, Yulin
name: Li, Weiming
name: Sun, Dequan
name: Hu, Huigang
name: Xie, Jianghui
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Hematology
subject: Plant Biology

description: Figure S2. GO assignment of all of the unigenes in the reference Library. (DOC 195 kb)
"C1N2N1_rpvLF_1700_32ns.slha" of "Search for long-lived, massive particles in events with displaced vertices and multiple jets in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2024

description: Param card (SLHA file) for electroweak pair production: C1N2N1_rpvLF_1700_32ns
description: A search for long-lived particles decaying into hadrons ispresented. The analysis uses 139 fb$^{-1}$ of $pp$ collision datacollected at $\sqrt{s} = 13$ TeV by the ATLAS detector at the LHCusing events that contain multiple energetic jets and a displacedvertex. The search employs dedicated reconstruction techniques thatsignificantly increase the sensitivity to long-lived particlesdecaying in the ATLAS inner detector. Background estimates forStandard Model processes and instrumental effects are extracted fromdata. The observed event yields are compatible with those expectedfrom background processes. The results are used to set limits at95% confidence level on model-independent cross sections forprocesses beyond the Standard Model, and on scenarios withpair-production of supersymmetric particles with long-livedelectroweakinos that decay via a small $R$-parity-violatingcoupling. The pair-production of electroweakinos with masses below1.5 TeV are excluded for mean proper lifetimes in the range from0.03~ns to 1~ns. When produced in the decay of m(gluino)=2.4 TeVgluinos, electroweakinos with m(neutralino)=1.5 TeV are excludedwith lifetimes in the range of 0.02~ns to 4~ns.
Blind Ptychographic Phase Retrieval via Convergent Alternating Direction Method of Multipliers
Creators: name: Chang, Huibin
name: Enfedaque, Pable
name: Marchesini, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optimization and Control (math.OC)
subject: Image and Video Processing (eess.IV)
subject: FOS: Mathematics
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Ptychography has risen as a reference X-ray imaging technique: it achieves resolutions of one billionth of a meter, macroscopic field of view, or the capability to retrieve chemical or magnetic contrast, among other features. A ptychographyic reconstruction is normally formulated as a blind phase retrieval problem, where both the image (sample) and the probe (illumination) have to be recovered from phaseless measured data. In this article we address a nonlinear least squares model for the blind ptychography problem with constraints on the image and the probe by maximum likelihood estimation of the Poisson noise model. We formulate a variant model that incorporates the information of phaseless measurements of the probe to eliminate possible artifacts. Next, we propose a generalized alternating direction method of multipliers designed for the proposed nonconvex models with convergence guarantee under mild conditions, where their subproblems can be solved by fast element-wise operations. Numerically, the proposed algorithm outperforms state-of-the-art algorithms in both speed and image quality.
description: 23 pages
Cosmology with x-matter
Creators: name: Chiba, Takeshi
name: Sugiyama, Naoshi
name: Nakamura, Takashi
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Motivated by the possibility of $H_0t_0 > 1$ where $H_0$ and $t_0$ are the Hubble parameter and the age of the universe, respectively, we investigate the cosmology including x-matter. x-matter is expressed by the equation of state $p_x=w_0ρ_{x0} + c_s^2(ρ_x-ρ_{x0})$, where $p_x$, $ρ_x$ and $ρ_{x0}$ are the pressure, the density of x-matter and the density at present, respectively. $w_0$ and $c_s^2$ are functions of $ρ_x$ in general. x-matter has the most general form of the equation of state which is characterized by 1)violation of strong energy condition at present for $w_0 < -1/3$ ; 2) locally stable (i.e. $c_s^2\geq 0$); 3)causality is guaranteed ($c_s\leq 1$). Considering the case that $w_0$ and $c_s^2$ are constants, we find that there is a large parameter space of $(w_0,c_s^2,Ω_{x0})$ in which the model universe is consistent with the age of the universe and the observations of distant Type I supernovae.
description: minor changes, 4 pages, 6 figures, accepted for publication as a Letter in MNRAS
Camponotus maculatus subsp. barbaricus var. inversa
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Camponotus
Camponotus maculatus
Camponotus maculatus f. subsp. barbaricus, emery, var. inversa

description: Camponotus maculatus F. subsp. barbaricus, EMERY, var. inversa.
Differe du type du barbaricus par sa taille un peu plus grande et legerement plus elancee, mais partout sa couleur: les [[worker]] minor sont plutot plus foncees que les grandes [[worker]], - d'un brun fonce, rarement un peu roussatres, avec la tete et l'abdomen noirs, le funicule et les mandibules roussatres. Chez la grande [[worker]] la couleur brun roussatre envahit de plus l'occiput, ou elle est meme un peu moins foncee que sur le thorax.
Djebel Keroulis pres du Rio-Salado, et Franchetti Algerie occidentale (Oranais) recolte par moi-meme.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 21
Camponotus maculatus subsp. symiensis Forel, 1910, n. subsp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Camponotus
Camponotus maculatus
Camponotus maculatus f. subsp. symiensis

description: Camponotus maculatus F. subsp. Symiensis n. subsp.
- [[worker]]. - Long. 7,5 a 10,5 mill. - Couleur et sculpture du sanctus v. cosensis Forel, mais beaucoup plus grele. Tete de la grande [[worker]], longue de 3 et large seulement de 2,6 mill, profondement echancree, un peu ovale. Les scapes depassent l'occiput d'un quart de leur longueur. Tete de la petite [[worker]] assez fortement retrecie derriere, a bord posterieur arrondi et fort peu distinct, bien moins que chez les [[worker]] plus petites du sanctus n. cosensis. Pilosite et sculpture exactement comme chez le sanctus n. cosensis, dont il n'est peut-etre qu'une variete tres grele.
Ile de Symi, une des Sporades meridionales (v. Oertzen).
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on page 21
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00241
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00241, 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 9: of Disruption of ureide degradation affects plant growth and development during and after transition from vegetative to reproductive stages
Creators: name: Takagi, Hiroshi
name: Watanabe, Shunsuke
name: Shoma Tanaka
name: Matsuura, Takakazu
name: Mori, Izumi
name: Hirayama, Takashi
name: Shimada, Hiroshi
name: Sakamoto, Atsushi
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Developmental Biology
subject: Plant Biology

description: Table S2. Composition of liquid culture media with low (2Â mM) and standard (20Â mM) concentrations of inorganic nitrogen. (DOCX 28 kb)
Discovery of Two Simultaneous Kilohertz Quasi-Periodic Oscillations in KS 1731-260
Creators: name: Wijnands, Rudy A. D.
name: van der Klis, Michiel
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have discovered two simultaneous quasi-periodic oscillations (QPOs) at 898.3+/-3.3 Hz and 1158.6+/-9.0 Hz in the 1996 August 1 observation of the low-mass X-ray binary KS 1731-260 with the Rossi X-ray Timing Explorer. The rms amplitude and FWHM of the lower frequency QPO were 5.3+/-0.7 % and 22+/-8 Hz, whereas those of the higher frequency QPO were 5.2+/-1.0 % and 37+/-21 Hz. At low inferred mass accretion rate both QPOs are visible, at slightly higher mass accretion rate the lower frequency QPO disappears and the frequency of the higher frequency QPO increases to ~1178 Hz. At the highest inferred mass accretion rate this QPO is only marginally detectable (2.1 sigma) near 1207 Hz, which is the highest frequency so far observed in an X-ray binary. The frequency difference (260.3+/-9.6 Hz) between the QPOs is equal to half the frequency of the oscillations observed in a type I burst in this source (at 523.92+/-0.05 Hz, Smith, Morgan and Bradt 1997). This suggests that the neutron star spin frequency is 261.96 Hz (3.8 ms), and that the lower frequency QPO is the beat between the higher frequency QPO, which could be a preferred orbital frequency around the neutron star, and the neutron star spin. During the 1996 August 31 observation we detected an additional QPO at 26.9+/-2.3 Hz, with a FWHM and rms amplitude of 11+/-5 Hz and 3.4+/-0.6 %.
description: 6 pages including 3 figures, Astrophysical Journal Letters, in press (issue 482)
Galaxy mergers up to z<2.5 I : The star formation properties of merging galaxies at separations 3-15 kpc
Creators: name: Silva, Andrea
name: Marchesini, Danilo
name: Silverman, John D.
name: Skelton, Rosalind
name: Iono, Daisuke
name: Martis, Nicholas
name: Marsan, Z. Cemile
name: Tadaki, Ken-ichi
name: Brammer, Gabriel
name: Kartaltepe, Jeyhan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of the influence of galaxy mergers on star formation at 0.310) are star-bursting (i.e., with SFR above the main sequence of star-forming galaxies by >0.5 dex). Merging galaxies which include galaxies with lower masses show a higher fraction of star-bursting galaxies (20%). The low fraction of star-bursting merging galaxies in this sample suggests that at galaxy nuclei separations of 3-15 kpc merging galaxies are still in a early stage and are yet to reach the maximum level of star formation activity. Furthermore, the level of star formation enhancement and its duration could be arguably reduced compared to local mergers, as shown by simulations of high-z mergers, and might also depend on the physical properties (such as stellar mass and gas fraction) of the merging galaxies. Finally, we compare the specific SFR between merging galaxies. Our results suggest that, as the mass of the merging galaxies increases, the star formation activity in the less massive member in the merger suffers a more dramatic impact than its companion galaxy.
description: Accepted to ApJ
Additional file 3: of Transcriptome analysis of atemoya pericarp elucidates the role of polysaccharide metabolism in fruit ripening and cracking after harvest
Creators: name: Chen, Jingjing
name: Duan, Yajie
name: Hu, Yulin
name: Li, Weiming
name: Sun, Dequan
name: Hu, Huigang
name: Xie, Jianghui
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: Plant Biology

description: Figure S3. COG assignment of all of the unigenes in the reference library. (DOC 55 kb)
Exploring the inclusion of Alaria aesculenta in all hamburger's components and their consumers' impact
Creators: name: Technical University of Cluj-Napoca
name: Cozmuta Mihaly, A
Publisher: name: Zenodo
Year: 2024

description: Preparation of hamburgers containing Alaria aesculenta aesculenta in the form of powder and flakes presented at the 

II Feira do Mar, 6-8 Sept., 2024 -Sagres.
Comparison between variable flavor number schemes for charm quark electroproduction
Creators: name: Chuvakin, A.
name: Smith, J.
name: van Neerven, W. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Where appropriate, the abbreviation 'VFNS' is replaced by 'CSN' to indicate the scheme using massive heavy quark coefficient functions proposed in this paper. The text below Eq. (2.13) and between Eqs. (2.33) and (2.36) has been considerably changed.
description: 64 pages, LaTeX, 16 Postscript figures
Predicting F2D(3) from the dipole cross-section
Creators: name: Forshaw, J. R.
name: Kerley, G. R.
name: Shaw, G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We employ a parameterisation of the proton dipole cross section previously extracted from electroproduction and photoproduction data to predict the diffractive structure function F2D(3)(Q^2, beta, xpom). Comparison with HERA H1 data yields good agreement.
description: 5 pages,4 figures, Latex2e, uses espcrc1.sty. Presented at "Hadron 99" Beijing, August 1999. Reference added, erroneous citation corrected
Lasius bicornis subsp. oertzeni Forel, 1910, n. subsp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1910
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Lasius
Lasius bicornis
Lasius bicornis forst subsp. oertzeni

description: Lasius bicornis Forst subsp. Oertzeni n. subsp.
- [[worker]]. - Long. 3,3 a 3,4 mill. Tete carree, non retrecie devant, aussi large que longue, a cotes mediocrement convexes (bien moins que chez carniolicus). Yeux situes au tiers posterieur. Thorax comme chez le flavus, moins echancre que chez {' affinis. Ecaille extremement haute aussi haute que l´epinotum, retrecie, amincie et profondement echancree au sommet, comme chez la [[queen]] (echancrure bien plus profonde que large et aussi large au fond qu'en haut); elle est encore bien plus haute que chez l´ affinis. Sculpture du flavus; pilosite et pubescence aussi. D'un brun jaunatre clair, tenant le milieu entre celui de l ' alienus et celui des flavus [[worker]] major, sans etre nulle part aussi jaune que chez ce dernier; membres plus clairs. Differe de l´ affinis par sa tete non retrecie devant, sa couleur, sa taille plus faible, sa pilosite moins abondante, sou ecaille plus haute, etc., de carniolicus par les cotes moins convexes de la tete, les mandibules inserees aux angles anterieurs, la couleur, la taille, l'ecaille, etc., de flavus et des autres par l'ecaille.
[[queen]]. Long. 5 mill. - Differe de l'espece typique de Foerster par ses ailes entierement subhyalines, a peines brunies, de meme teinte a la base qu'a l'extremite et par sa pilosite assez clairsemee. Ailes longues de 5,7 mill, (une aile superieure). Yeux plus convexes que chez l´ affinis.
[[male]]. Long. 3,6 mill. - Mandibules armees de 8 dents distinctes. Tete aussi large que le thorax moins retrecie devant que chez [' affinis. Assez luisant. Ailes, echancrure de l'ecaille, pilosite, etc, comme chez la [[queen]]. Longueur d'une aile superieure 5 mill, couleur brun fonce; membres brun clair.
Moree (v. Oertzen) La pilosite et la couleur des ailes justifient une nouvelle sous espece. La decouverte de l'ouvriere montre que le bicornis est une espece distincte de l´ affinis et de l´ umbratus. Andre a decrit l'ouvriere de raffinis sous le nom de bicornis.
description: Published as part of Forel, A., 1910, Glanures myrmecologiques., pp. 6-32 in Annales de la Societe Entomologique de Belgique 54 on pages 21-22
GUMANISTIK PSIXOLOGIYADA O'ZINI O'ZI FAOLLASHTIRISH MUAMMOSINING YORITILISHI
Creators: name: Qurbonboyev, Azimbek
Publisher: name: Zenodo
Year: 2025

description: Mazkur maqolada shaxsning o‘zini o‘zi faollashtirish xususiyatining mazmuni, gumanistik psixologiya yo‘nalishi olimlarining psixologik nazariyalari hamda shaxs hayotida o‘zini o‘zi faollashtirishning ahamiyatli jihatlari keng yoritilgan. Shuningdek, o‘zini o‘zi faollashtirishga erishish yo‘llari va uning inson ehtiyojlari bilan bog‘liqlik jihatlari keltirilgan.
"C1N2N1_rpvHF_1500_p1ns.slha" of "Search for long-lived, massive particles in events with displaced vertices and multiple jets in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2024

description: Param card (SLHA file) for electroweak pair production with heavy-flavor quarks: C1N2N1_rpvHF_1500_p1ns
description: A search for long-lived particles decaying into hadrons ispresented. The analysis uses 139 fb$^{-1}$ of $pp$ collision datacollected at $\sqrt{s} = 13$ TeV by the ATLAS detector at the LHCusing events that contain multiple energetic jets and a displacedvertex. The search employs dedicated reconstruction techniques thatsignificantly increase the sensitivity to long-lived particlesdecaying in the ATLAS inner detector. Background estimates forStandard Model processes and instrumental effects are extracted fromdata. The observed event yields are compatible with those expectedfrom background processes. The results are used to set limits at95% confidence level on model-independent cross sections forprocesses beyond the Standard Model, and on scenarios withpair-production of supersymmetric particles with long-livedelectroweakinos that decay via a small $R$-parity-violatingcoupling. The pair-production of electroweakinos with masses below1.5 TeV are excluded for mean proper lifetimes in the range from0.03~ns to 1~ns. When produced in the decay of m(gluino)=2.4 TeVgluinos, electroweakinos with m(neutralino)=1.5 TeV are excludedwith lifetimes in the range of 0.02~ns to 4~ns.
STEAP: simultaneous trajectory estimation and planning
Creators: name: Mukadam, Mustafa
name: Dong, Jing
name: Dellaert, Frank
name: Boots, Byron
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: We present a unified probabilistic framework for simultaneous trajectory estimation and planning (STEAP). Estimation and planning problems are usually considered separately, however, within our framework we show that solving them simultaneously can be more accurate and efficient. The key idea is to compute the full continuous-time trajectory from start to goal at each time-step. While the robot traverses the trajectory, the history portion of the trajectory signifies the solution to the estimation problem, and the future portion of the trajectory signifies a solution to the planning problem. Building on recent probabilistic inference approaches to continuous-time localization and mapping and continuous-time motion planning, we solve the joint problem by iteratively recomputing the maximum a posteriori trajectory conditioned on all available sensor data and cost information. Our approach can contend with high-degree-of-freedom (DOF) trajectory spaces, uncertainty due to limited sensing capabilities, model inaccuracy, the stochastic effect of executing actions, and can find a solution in real-time. We evaluate our framework empirically in both simulation and on a mobile manipulator.
description: Published in Autonomous Robots
Obscured Asymptotic Giant Branch stars in the Magellanic Clouds III. New IRAS counterparts
Creators: name: van Loon, Jacco Th.
name: Zijlstra, Albert A.
name: Whitelock, Patricia A.
name: Waters, L. B. F. M.
name: Loup, Cecile
name: Trams, Norman R.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have searched for near-infrared stellar counterparts of IRAS point sources in the Large Magellanic Cloud (LMC), in J and K-bands. This resulted in the detection of 21 counterparts, of which 19 are new discoveries. Using colour-magnitude and colour-colour diagrams, we identify 13 Asymptotic Giant Branch (AGB) stars with thick circumstellar dust envelopes, 7 possible early post-AGB stars or stars recovering from a thermal pulse, and 1 red supergiant or foreground star. For 10 of the IRAS targets we do not succeed in detecting and/or identifying a near-infrared counterpart. We serendipitously detect 14 other red sources, of which 2 are known Long Period Variables, and a few galaxies. The near-infrared and optical colours of the galaxies may indicate considerable interstellar extinction through the LMC, as much as A_V about 2-4 mag. The relative number of AGB carbon stars over oxygen stars is shown to decrease as the luminosity increases. Yet amongst the faintest mass-losing AGB stars oxygen-rich stars still exist, which puts constraints on current convection theories that predict the occurrence of third dredge-up and Hot Bottom Burning. We investigate the nature of some LMC stars that have infrared properties very similar to suspected Galactic post-AGB stars.
description: 17 pages (LaTeX source and 16 PostScript figures). Accepted for publication in Astronomy and Astrophysics Main Journal
Weighted Statistic in Detecting Faint and Sparse Alternatives for High-Dimensional Covariance Matrices
Creators: name: Yang, Qing
name: Pan, Guangming
Publisher: name: Taylor & Francis
Year: 2015
Subjects: subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: This article considers testing equality of two population covariance matrices when the data dimension p diverges with the sample size n (p/n → c > 0). We propose a weighted test statistic that is data-driven and powerful in both faint alternatives (many small disturbances) and sparse alternatives (several large disturbances). Its asymptotic null distribution is derived by large random matrix theory without assuming the existence of a limiting cumulative distribution function of the population covariance matrix. The simulation results confirm that our statistic is powerful against all alternatives, while other tests given in the literature fail in at least one situation. Supplementary materials for this article are available online.
Hadronic Weak Decays of Heavy Mesons and Nonfactorization
Creators: name: Cheng, Hai-Yang
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The parameters $χ_{1,2}$, which measure nonfactorizable soft gluon contributions to hadronic weak decays of mesons, are updated by extracting them from the data of $D,\,B\to PP,~VP$ decays ($P$: pseudoscalar meson, $V$: vector meson). It is found that $χ_2$ ranges from $-0.36$ to $-0.60$ in the decays from $D\to\bar{K}π$ to $D^+\toϕπ^+,~D\to\bar{K}^*π$, while it is of order 10\% with a positive sign in $B\toψK,~Dπ,~D^*π,~Dρ$ decays. Therefore, the effective parameter $a_2$ is process dependent in charm decay, whereas it stays fairly stable in $B$ decay. This implies the picture that nonfactorizable effects become stronger when the decay particles become less energetic after hadronization. As for $D,\,B\to VV$ decays, the presence of nonfactorizable terms in general prevents a possible definition of effective $a_1$ and $a_2$. This is reenforced by the observation of a large longitudinal polarization fraction in $B\toψK^*$ decay, implying $S$-wave dominated nonfactorizable effects. The nonfactorizable term dominated by the $S$-wave is also essential for understanding the decay rate of $B^-\to D^{*0} ρ^-$. It is found that all nonfactorizable effects $A_1^{nf}/A_1^{BK^*},~A _1^{nf}/A_1^{Bρ},~A_1^{nf}/A_1^{BD^*}$ ($nf$ standing for nonfactorization) are positive and of order 10\%, in accordance with $χ_2(B\to D(D^*)π( ρ))$ and $χ_2(B\toψK)$. However, we show that in $D\to\bar{K}^*ρ$ decay nonfactorizable effects cannot be dominated by the $S$-wave. A polarization measurement in the color- and Cabibbo-suppressed decay mode $D^+\toϕρ^+$ is strongly urged in order to test if $A_2^{nf}/A_2$ plays a more pivotal role than $A_1^{nf}/A_1$ in charm decay.
description: Latex, 16 pages
Additional file 6: of Transcriptome analysis of atemoya pericarp elucidates the role of polysaccharide metabolism in fruit ripening and cracking after harvest
Creators: name: Chen, Jingjing
name: Duan, Yajie
name: Hu, Yulin
name: Li, Weiming
name: Sun, Dequan
name: Hu, Huigang
name: Xie, Jianghui
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Physiology
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: Figure S4. Profiles ordered according to P-value significance of the number assigned versus expected. Numbers between brackets indicate the number of the DEGs assigned. (DOC 2023 kb)
Single production of the excited electrons at the future FCC-based lepton-hadron colliders
Creators: name: Caliskan, Abdullatif
name: Kara, Seyit Okan
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study composite electron production at the FCC-based three electron-proton colliders with the center-of-mass energies of $3.46$, $10$ and $31.6$ TeV. For the signal process of $ep\rightarrow e^{\star}X\rightarrow eγX$ , the production cross-sections and decay widhts of the excited electrons have been calculated. The differences of some kinematical quantities of the final state particles between the signal and background have been analyzed. For this purpose, transverse momentum and pseudorapidity distributions of electron and photon have been obtained and the kinematical cuts for discovery of the excited electrons have been assigned. We have finally determined the mass limits of excited electrons for observation and discovery by applying these cuts. It is shown that the mass limit for discovery obtained from the collider with $\sqrt{s}=31.6$ TeV (called PWFA-LC$\otimes$FCC) is $22.3$ TeV for the integrated luminosity $L_{int}=10$ $fb^{-1}$.
description: 14 pages, 6 figures, 2 tables