cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Equilibrium Structure of Cosmological Halos
Creators: name: Iliev, Ilian T.
name: Shapiro, Paul R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have derived an analytical model for the postcollapse equilibrium structure of cosmological halos as nonsingular truncated isothermal spheres (TIS) and compared this model with observations and simulations of cosmological halos on all scales. Our model is in good agreement with the observations of the internal structure of dark-matter-dominated halos from dwarf galaxies to X-ray clusters. It reproduces many of the average properties of halos in CDM simulations to good accuracy, including the density profiles outside the central region, while avoiding the possible discrepancy at small radii between observed galaxy and cluster density profiles and the singular density profiles predicted by N-body simulations of the CDM model. While much attention has been focused lately on this possible discrepancy, we show that the observed galaxy rotation curves and correlations of halo properties nevertheless contain valuable additional information with which to test the theory, despite this uncertainty at small radii. The available data allows us to constrain the fundamental cosmological parameters and also to put a unique constraint on the primordial density fluctuation power spectrum at large wavenumbers (i.e. small mass scale).
description: To appear in "The 20th Texas Symposium on Relativistic Astrophysics", eds. H. Martel and J. C. Wheeler, AIP, in press (2001) (3 pages, 1 figure)
Chenanisuchus lateroculi
Creators: name: Hill, Robert V.
name: Mccartney, Jacob A.
name: Roberts, Eric
name: Bouaré, Mohamed
name: Sissoko, Famory
name: O'leary, Maureen A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Crocodylia
Dyrosauridae
Chenanisuchus
Chenanisuchus lateroculi

description: CHENANISUCHUS LATEROCULI Jouve et al., 2005a
HOLOTYPE: OCP DEK-GE 262 (Jouve et al., 2005a).
NEW REFERRED SPECIMEN: CNRST SUNY 280.
LOCALITY: Mali-8; Maastrichtian phosphate conglomerate.
DESCRIPTION: CNRST SUNY 280 consists of the frontoparietal portion of the skull roof with portions of the articulated prefrontals and supraoccipital elements (fig. 6A). The specimen is identified as a dyrosaurid based on the presence of otic capsules that closely approach one another medially, and an occipital exposure of the parietal. Although the lateral margins of the supratemporal fenestrae are not preserved, they can be confidently reconstructed as rostrocaudally elongate, based on the size of the preserved supraoccipital (fig. 6B). In addition, the supraoccipital contributes to the bases of occipital tuberosities, although their full extent is not known.
 The specimen compares most closely with the description of Chenanisuchus lateroculi (Jouve, 2005a). The skull roof is flat and ornamented with moderately deep pits separated by rounded ridges. The ornamentation is most pronounced at the centers of the frontal and parietal, but diminishes in the vicinity of the frontoparietal and frontonasal sutures. The ornamentation extends fully to the straight caudal margin of the parietal, differing slightly from the condition in the holotype of C. lateroculi, in which ornamentation is lacking in this region.
 The interfenestral bar is relatively wide, and does not form a peaked sagittal crest as in Rhabdognathus and Hyposaurus. Instead, the dorsal surface slightly overhangs the base of the bar, forming a broad, T-shaped cross section as in Chenanisuchus lateroculi. The suture between the frontal and prefrontal elements is not L-shaped, as in other specimens of Chenanisuchus, but instead is straight and diagonal, as in all other dyrosaurids in which it is known, forming an angle of about 50 degrees with the long axis of the skull. We do not consider this character to represent an interspecific variation, and accordingly refer this specimen to C. lateroculi.
description: Published as part of Hill, Robert V., Mccartney, Jacob A., Roberts, Eric, Bouaré, Mohamed, Sissoko, Famory & O'leary, Maureen A., 2008, Dyrosaurid (Crocodyliformes: Mesoeucrocodylia) Fossils from the Upper Cretaceous and Paleogene of Mali: Implications for Phylogeny and Survivorship across the K / T Boundary, pp. 1-20 in American Museum Novitates 3631 (1) on page 10, DOI: 10.1206/598.1, http://zenodo.org/record/5390099
Nonlinear Schrodinger equations with repulsive harmonic potential and applications
Creators: name: Carles, Remi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 35Q55; 35B05; 35B40; 35P25

description: We study the Cauchy problem for Schrodinger equations with repulsive quadratic potential and power-like nonlinearity. The local problem is well-posed in the same space as that used when a confining harmonic potential is involved. For a defocusing nonlinearity, it is globally well-posed, and a scattering theory is available, with no long range effect for any superlinear nonlinearity. When the nonlinearity is focusing, we prove that choosing the harmonic potential sufficiently strong prevents blow-up in finite time. Thanks to quadratic potentials, we provide a method to anticipate, delay, or prevent wave collapse; this mechanism is explicit for critical nonlinearity.
description: Final version, to appear in SIAM J. Math. Anal
Improving Grounded Natural Language Understanding through Human-Robot Dialog
Creators: name: Thomason, Jesse
name: Padmakumar, Aishwarya
name: Sinapov, Jivko
name: Walker, Nick
name: Jiang, Yuqian
name: Yedidsion, Harel
name: Hart, Justin
name: Stone, Peter
name: Mooney, Raymond J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Natural language understanding for robotics can require substantial domain- and platform-specific engineering. For example, for mobile robots to pick-and-place objects in an environment to satisfy human commands, we can specify the language humans use to issue such commands, and connect concept words like red can to physical object properties. One way to alleviate this engineering for a new domain is to enable robots in human environments to adapt dynamically---continually learning new language constructions and perceptual concepts. In this work, we present an end-to-end pipeline for translating natural language commands to discrete robot actions, and use clarification dialogs to jointly improve language parsing and concept grounding. We train and evaluate this agent in a virtual setting on Amazon Mechanical Turk, and we transfer the learned agent to a physical robot platform to demonstrate it in the real world.
Cooling Flows of Self-Gravitating, Rotating, Viscous Systems
Creators: name: Shadmehri, Mohsen
name: Ghanbari, Jamshid
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We obtain self-similar solutions that describe the dynamics of a self-gravitating, rotating, viscous system. We use simplifying assumptions; but explicitly include viscosity and the cooling due to the dissipation of energy. By assuming that the turbulent dissipation of energy is as power law of the density and the speed v_{rms} and for a power-law dependence of viscosity on the density, pressure, and rotational velocity, we investigate turbulent cooling flows. It has been shown that for the cylindrically and the spherically cooling flows the similarity indices are the same, and they depend only on the exponents of the dissipation rate and the viscosity model. Depending on the values of the exponents, which the mechanisms of the dissipation and viscosity determine them, we may have solutions with different general physical properties. The conservation of the total mass and the angular momentum of the system strongly depends on the mechanisms of energy dissipation and the viscosity model.
description: 19 pages, 5 figures, To appear in ApJ (scheduled for the v574, July 20, 2002)
Classification of Close Binary Stars Using Recurrence Networks
Creators: name: George, Sandip V.
name: Misra, R.
name: Ambika, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Close binary stars are binary stars where the component stars are close enough such that they can exchange mass and/or energy. They are subdivided into semi-detached, overcontact or ellipsoidal binary stars. A challenging problem in the context of close binary stars, is their classification into these subclasses, based solely on their light curves. Conventionally, this is done by observing subtle features in the light curves like the depths of adjacent minima, which is tedious when dealing with large datasets. In this work we suggest the use of machine learning algorithms applied to measures of recurrence networks and nonlinear time series analysis to differentiate between classes of close binary stars. We show that overcontact binary stars occupy a region different from semi-detached and ellipsoidal binary stars in a plane of characteristic path length(CPL) and average clustering coefficient(CC), computed from their recurrence networks. We use standard clustering algorithms and report that the clusters formed corresponds to the standard classes with a high degree of accuracy.
description: 7 pages, 8 figures, submitted to Chaos: An Interdisciplinary Journal of Nonlinear Science: Focus issue
Chandra X-ray Observations of the X-ray Faint Elliptical Galaxy NGC 4697
Creators: name: Sarazin, Craig L.
name: Irwin, Jimmy A.
name: Bregman, Joel N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) A Chandra ACIS S3 observation of the X-ray faint elliptical galaxy NGC 4697 resolves much of the X-ray emission (61% of the counts from within one effective radius) into 90 point sources, of which ~80 are low mass X-ray binaries (LMXBs) associated with this galaxy. The dominance of LMXBs indicates that X-ray faint early-type galaxies have lost much of their interstellar gas. On the other hand, a modest portion of the X-ray emission from NGC 4697 is due to hot gas. The X-ray emitting gas in NGC 4697 has a rather low temperature (kT = 0.29 keV). The emission from the gas is very extended, with a much flatter surface brightness profile than the optical light, and has an irregular, L-shaped morphology. X-ray spectra of the resolved sources and diffuse emission show that the soft X-ray spectral component, found in this and other X-ray faint ellipticals with {\it ROSAT}, is due to interstellar gas. The cumulative LMXB spectrum is well-fit by thermal bremsstrahlung at kT = 8.1 keV, without a significant soft component. Three of the resolved sources in NGC 4697 are supersoft sources. In the outer regions of NGC 4697, seven of the LMXBs (about 20%) are coincident with candidate globular clusters, which indicates that globulars have a high probability of containing X-ray binaries compared to the normal stellar population. The luminosity function of the LMXBs has a ``knee'' at 3.2 x 10^38 ergs/s, which is approximately the Eddington luminosity of a 1.4 Msun neutron star (NS). This knee appears to be a characteristic feature of the LMXB population of early-type galaxies, and we argue that it separates black hole and NS binaries. This characteristic luminosity could be used as a distance estimator.
description: Astrophysical Journal, in press. 21 pages in emulateapj5 style with 10 embedded Postscript figures
Scutellista caerulea
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Scutellista
Scutellista caerulea

description: Scutellista caerulea (Fonscolombe)
(gures 31, 32)
 Encyrtus caerulea Forscolombe, 1832: 304. Synonymized with S. cyanea by G raham, 1969: 76. Scutellista cyanea M otschulsky, 1859: 172–173. Synonymized by BoucÏek, 1988: 351. Aspidocoris cyaneus Costa, 1863: 24–26.
 Scutellista caerulea (Fonscolomb e); BoucÏek, 1988: 351.
 Material examined. Turkey: Bornova-Izmit, 4 September 1974, 2, ex. Ceroplastes rusci, Oncuer, India: Maharashtra, Rahuri, 12 December 1977, 1 1, CIE A10037, ex. Scale. Oman: Saham, 18 January 1989, 1 on M ango, CIE A20674, det. LaSalle, 1989. Trinidad: Curepe, February 1977, 1, ex. Saissetia coOEeae on Leucophyllum taxanum (F. D. Bennett), D et. N oyes, 1977.
 Biology. The parasite attacks Ceroplastes X oridensis Comstock, Ceroplastes rusci (L.), Parasaissetia nigra, Saissetia hemisphaerica (Targioni), Saissetta oleae (Bernard) and Saissetia coOEeae (Walker) (data from Noyes, 1988).
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on page 1603
Additional file 3 of Causal relationships between genetically determined metabolites and human intelligence: a Mendelian randomization study
Creators: name: Yang, Jian
name: Zhao, Binbin
name: Qian, Li
name: Gao, Fengjie
name: Fan, Yanjuan
name: He, Xiaoyan
name: Ma, Qingyan
name: Yang, Lihong
name: Yan, Bin
name: Wang, Wei
name: Ma, Xiancang
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: Additional file 3: Fig. S3. Mendelian randomizationassociations of p-acetamidophenylglucuronide on other intelligence-relatedoutcomes from other data sources.
Additional file 2: of Clinical and immunological control of experimental autoimmune encephalomyelitis by tolerogenic dendritic cells loaded with MOG-encoding mRNA
Creators: name: Derdelinckx, Judith
name: Mansilla, María
name: Laere, Maxime De
name: Wai-Ping Lee
name: Navarro-Barriuso, Juan
name: Wens, Inez
name: Nkansah, Irene
name: Daans, Jasmijn
name: Reu, Hans De
name: Keliris, Aneta Jolanta
name: Audekerke, Johan Van
name: Vanreusel, Verdi
name: Pieters, Zoë
name: Linden, Annemie Van Der
name: Verhoye, Marleen
name: Molenberghs, Geert
name: Niel Hens
name: Goossens, Herman
name: Willekens, Barbara
name: Cras, Patrick
name: Ponsaerts, Peter
name: Zwi Berneman
name: Martínez-Cáceres, Eva
name: Cools, Nathalie
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Hematology

description: Figure S2. Graphical overview of the protein structure of murine MOG. (PDF 357 kb)
A needle in a haystack: transient porosity in a closed pore square lattice coordination network
Creators: name: Koupepidou, Kyriaki
name: Eaby, Alan
name: Sensharma, Debobroto
name: Javan Nikkhah, Sousa
name: He, Tao
name: Lusi, Matteo
name: Vandichel, Matthias
name: J. Barbour, Leonard
name: Mukherjee, Soumya
name: Zaworotko, Michael
Publisher: name: University of Limerick
Year: 2025
Subjects: classificationCode: 34
subject: Chemical sciences
subject: FOS: Chemical sciences

description: Guest transport through discrete voids (closed pores) in crystalline solids is poorly understood. Herein, we report the gas sorption properties of a nonporous coordination network, {[Co(bib)2Cl2] ⋅ 2MeOH}n (sql-bib-Co-Cl-α), featuring square lattice (sql) topology and the bent linker 1,3-bis(1H-imidazol-1-yl)benzene (bib). The as-synthesized sql-bib-Co-Cl-α has 11.3 % (313 Å3) of its unit cell volume in closed pores occupied by methanol (MeOH). Upon desolvation and air exposure, sql-bib-Co-Cl-α underwent a single-crystal to single-crystal (SC-SC) phase transformation to sql-bib-Co-Cl-β′, wherein MeOH was replaced by water. Activation (vacuum or N2 flow) resulted in dehydration and retention of the closed pores, affording sql-bib-Co-Cl-β with 7.7 % (194 Å3) guest-accessible space. sql-bib-Co-Cl-β was found to preferentially adsorb C2H2 (at 265 K) over CO2 (at 195 K) through gate-opening mechanisms, at gate-opening pressures of 59.8 and 27.7 kPa, respectively, while other C2 gases were excluded. PXRD was used to monitor transformations between the three phases of sql-bib-Co-Cl, while in situ DSC, in situ SCXRD under CO2 pressure, and computational studies provided insight into the guest transport mechanism, which we attribute to the angular, flexible nature of the bib ligand. Further, the preferential adsorption of C2H2 over CO2 and other C2 gases suggests that transiently porous sorbents might have utility in separations.
Ena Turton 1831
Creators: name: Hausdorf, B
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Stylommatophora
Enidae
Ena

description: Genus Ena Turton, 1831
 Ena Turton, 1831: 80. Type species (Herrmannsen, 1847: 421): Bulimus montanus D raparnaud, 1801.
 Diagnosis. A genus of Buliminidae which is characterized by a large, brownish, elongated oval shell without apertural teeth, the palatal insertion of the peristome which does not distinctly approach to the columellar edge, a usually well-developed imperforate penial papilla (which is rudimentary only in Ena dazimonensis sp. n.; see below), a penial appendix, the lack of a penial caecum, a caecum at the middle section of the epiphallus, a more or less short agellum, and a diverticulum to the bursa copulatrix.
description: Published as part of Hausdorf, B, 2001, The genus Ena in Turkey, with remarks on its phylogenetic relationships (Gastropoda: Buliminidae), pp. 1627-1638 in Journal of Natural History 35 on page 1629
Estimation and selection for high-order Markov chains with Bayesian mixture transition distribution models
Creators: name: Heiner, Matthew
name: Kottas, Athanasios
Publisher: name: arXiv
Year: 2019
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: We develop two models for Bayesian estimation and selection in high-order, discrete-state Markov chains. Both are based on the mixture transition distribution, which constructs a transition probability tensor with additive mixing of probabilities from first-order transition matrices. We demonstrate two uses for the proposed models: parsimonious approximation of high-order dynamics by mixing lower-order transition models, and order/lag selection through over-specification and shrinkage via priors for sparse probability vectors. The priors further shrink all models to an identifiable and interpretable parameterization, useful for data analysis. We discuss properties of the models and demonstrate their utility with simulation studies. We further apply the methodology to a data analysis from the high-order Markov chain literature and to a time series of pink salmon abundance in a creek in Alaska, U.S.A.
Additional file 1: of Clinical and immunological control of experimental autoimmune encephalomyelitis by tolerogenic dendritic cells loaded with MOG-encoding mRNA
Creators: name: Derdelinckx, Judith
name: Mansilla, María
name: Laere, Maxime De
name: Wai-Ping Lee
name: Navarro-Barriuso, Juan
name: Wens, Inez
name: Nkansah, Irene
name: Daans, Jasmijn
name: Reu, Hans De
name: Keliris, Aneta Jolanta
name: Audekerke, Johan Van
name: Vanreusel, Verdi
name: Pieters, Zoë
name: Linden, Annemie Van Der
name: Verhoye, Marleen
name: Molenberghs, Geert
name: Niel Hens
name: Goossens, Herman
name: Willekens, Barbara
name: Cras, Patrick
name: Ponsaerts, Peter
name: Zwi Berneman
name: Martínez-Cáceres, Eva
name: Cools, Nathalie
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Hematology

description: Figure S1. Graphical overview of the culture protocol for murine bone marrow-derived dendritic cells. (PDF 271 kb)
Dependence of atomic parity-violation effects on neutron skins and new physics
Creators: name: Viatkina, A. V.
name: Antypas, D.
name: Kozlov, M. G.
name: Budker, D.
name: Flambaum, V. V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We estimate the relative contribution of nuclear structure and new physics couplings to the parity non-conserving spin-independent effects in atomic systems, for both single isotopes and isotopic ratios. General expressions are presented to assess the sensitivity of isotopic ratios to neutron skins and to couplings beyond standard model at tree level. The specific coefficients for these contributions are calculated assuming Fermi distribution for proton and neutron nuclear densities for isotopes of Cs, Ba, Sm, Dy, Yb, Pb, Fr, and Ra. The present work aims to provide a guide to the choice of the best isotopes and pairs of isotopes for conducting atomic PNC measurements.
description: 11 pages, 2 figures, 3 tables
Infall, Outflow, Rotation, and Turbulent Motions of Dense Gas within NGC 1333 IRAS 4
Creators: name: Di Francesco, James
name: Myers, Philip C.
name: Wilner, David J.
name: Ohashi, Nagayoshi
name: Mardones, Diego
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Millimeter wavelength observations are presented of NGC 1333 IRAS 4, a group of highly-embedded young stellar objects in Perseus, that reveal motions of infall, outflow, rotation, and turbulence in the dense gas around its two brightest continuum objects, 4A and 4B. These data have finest angular resolution of approximately 2" (0.0034 pc) and finest velocity resolution of 0.13 km/s. Infall motions are seen from inverse P-Cygni profiles observed in H2CO 3_12-2_11 toward both objects, but also in CS 3-2 and N2H+ 1-0 toward 4A, providing the least ambiguous evidence for such motions toward low-mass protostellar objects. Outflow motions are probed by bright line wings of H2CO 3_12-2_11 and CS 3-2 observed at positions offset from 4A and 4B, likely tracing dense cavity walls. Rotational motions of dense gas are traced by a systematic variation of the N2H+ line velocities, and such variations are found around 4A but not around 4B. Turbulent motions appear reduced with scale, given N2H+ line widths around both 4A and 4B that are narrower by factors of 2 or 3 than those seen from single-dish observations. Minimum observed line widths of approximately 0.2 km/s provide a new low, upper bound to the velocity dispersion of the parent core to IRAS 4, and demonstrate that turbulence within regions of clustered star formation can be reduced significantly. A third continuum object in the region, 4B', shows no detectable line emission in any of the observed molecular species.
description: LateX, 51 pages, 9 figures, accepted by ApJ
Ascocotyle (Ascocotyle) leighi Burton 1956
Creators: name: Scholz, T.
name: Aguirre-Macedo, M. L.
name: Salgado-Maldonado, G.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Platyhelminthes
Trematoda
Plagiorchiida
Heterophyidae
Ascocotyle
Ascocotyle leighi

description: Ascocotyle (Ascocotyle) leighi Burton, 1956
 Metacercaria
 Morphology. Sogandares-Bernal and Lumsden (1964) did not describe metacercariae found in Mexico.
 Second intermediate hosts. Belonesox belizanus Kner, Poecilia sphenops Valenciennes in Cuvier and Valenciennes (Poeciliidae).
 Site of infection. Heart.
 Distribution. YucataÂn (Progreso).
 References from Mexico. Sogandares-Bernal and Lumsden (1964).
 Specimens deposited. None.
 Comments. Sogandares-Bernal and Lumsden (1964) found metacercariae of A. (A.) leighi in two poeciliid ®sh from Progreso, YucataÂn, most probably from CheleÂm lagoon. However, the authors did not provide any data on the morphology of metacercariae.
 Metacercariae of A. (A.) leighi are encysted exclusively in the heart and they have been found in poeciliid and cyprinodonti d ®sh in the USA and Mexico (Burton, 1956; Sogandares-Bernal and Bridgman, 1960; Sogandares-Bernal and Lumsden, 1964). They diOEer from those of A. (A.) tenuicollis encysted in the heart as well mainly in the number of circumoral spines (48±52 in total, i.e. 24±26 in each row, in the former taxon versus 32, i.e. 161 16 in A. (A.) tenuicollis) (Burton, 1956, 1958; Scholz et al., 1997a).
 Salgado-Maldonad o and Kennedy (1997), and Salgado-Maldonad o et al. (1997) reported metacercariae of A. (A.) leighi from the gills, mesenteries, heart and kidney of several species of cichlids from southeastern Mexico. Although few reference specimens were preserved and available to the present authors, it is possible to assume that most, if not all, metacercariae previously reported as A. leighi were misidenti®ed and belonged to other species of the Ascocotyle- complex. Metacercariae from internal organs of cichlid, characid and poeciliid ®sh were conspeci®c with A. (P). nana and those encysted in the gills of cichlids with A. (A.) nunezae. Metacercariae encysted in the heart of ®sh of diOEerent families might belong to A. (A.) leighi but all voucher specimens examined were conspeci®c with A. (A.) tenuicollis .
 Adult trematodes of A. (A.) leighi are not known from Mexico because specimens found in the intestine of Casmerodius albus from PaÂtzcuaro Lake (MichoacaÂn), identi®ed by G. PeÂrez Ponce de LeoÂn as A. leighi (Lamothe-Argumedo et al., 1997; CNHE 1532), belonged in fact to A. (A.) tenuicollis (®gure 2).
description: Published as part of Scholz, T., Aguirre-Macedo, M. L. & Salgado-Maldonado, G., 2001, Trematodes of the family Heterophyidae (Digenea) in Mexico: a review of species and new host and geographical records, pp. 1733-1772 in Journal of Natural History 35 (12) on pages 1737-1738, DOI: 10.1080/00222930152667087, http://zenodo.org/record/5275922
On OH line formation and oxygen abundances in metal-poor stars
Creators: name: Asplund, M.
name: Perez, A. E. Garcia
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The formation of the UV OH spectral lines has been investigated for a range of stellar parameters in the light of 3D hydrodynamical model atmospheres. The low atmospheric temperatures encountered at low metallicities compared with the radiative equilibrium values enforced in classical 1D hydrostatic model atmospheres have a profound impact on the OH line strengths. As a consequence, the derived O abundances using 3D models are found to be systematically lower by more than 0.6 dex at [Fe/H]=-3.0 compared with previous 1D analyses, casting doubts on the recent claims for a monotonic increase in [O/Fe] towards lower metallicities. In fact, taken at face value the resulting 3D LTE trend is in rough agreement with the conventional [O/Fe] plateau. Caution must, however, be exercised in view of the remaining assumptions in the 3D calculations. We have verified that the stellar parameters remain essentially unchanged with 3D model atmospheres provided that the infrared flux method, Hipparcos parallaxes and FeII lines are utilised, leaving the 3D O abundances from OH lines largely intact. Greater concern stems from possible departures from LTE in both the line formation and the molecular equilibrium, which, if present, would increase the derived O abundances again. Non-LTE line formation calculations with 1D model atmospheres suggest no significant steepening of the [O/Fe] trend even if the abundance corrections amount to about 0.2 dex for all investigated stellar parameters. We note, however, that the 3D case may not necessarily be as metallicity-independent. The apparent lack of laboratory or theoretical rate coefficients at the relevant temperatures for the involved molecular reactions unfortunately prevents a quantitative discussion on the possible effects of non-equilibrium chemistry.
description: Accepted for A&A
Diploglena capensis Purcell
Creators: name: Platnick, Norman I.
name: Jäger, Peter
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Caponiidae
Diploglena
Diploglena capensis

description: Diploglena capensis Purcell   Figures 26–30
 Diploglena capensis Purcell, 1904: 170, figs. 36–38 (three male and four female syntypes from St. Helena Bay, Malmesbury Div., Western Cape Province, South Africa, should be in the South African Museum, not examined).
DIAGNOSIS: With the characters of the genus and genitalia as in figs. 28–30.
MALE: Described by Purcell (1904).
FEMALE: Described by Purcell (1904).
 OTHER MATERIAL EXAMINED: NAMIBIA: Erongo: 10 mi W Okombahe, May 10, 1958, elev. 920 m (E. Ross, R. Leech, CAS), 1♀. SOUTH AFRICA: Northern Cape: 20 km N Concordia, 26 ° 40 9 S, 22 ° 40E, June 2, 1997, from scorpion burrow (A. Harrington, PPRI 98 /291), 13; Garies, Namaqualand, Nov. 14, 1949 (B. Malkin, CAS), 1♀; Henkries, June 2, 1997, in scorpion burrow (A. Harrington, PPRI 98 /292), 13, 2♀; Kweekfontein, June 2, 1997, from burrow of scorpion, Opisthophthalmus crassimanus Purcell (A. Harrington, PPRI 98 /290), 13. Western Cape: Saldanha Bay, Nov. 18, 1949 (B. Malkin, CAS), 1♀; Tierberg, July 25, 1989 (R. Dean, PPRO 91 /40), 13.
 DISTRIBUTION: Known only from the western parts of South Africa and Namibia. Lawrence (1928: 225) described D. capensis major, as a new ‘‘variety’’, based on a female from Kaross, Namibia; collections including males will be needed to help determine whether the Namibian population is conspecific with the specimens from the cape, or belongs to a diagnosable taxon.
description: Published as part of Platnick, Norman I. & Jäger, Peter, 2008, On the First Asian Spiders of the Family Caponiidae (Araneae, Haplogynae), with Notes on the African Genus Diploglena, pp. 1-12 in American Museum Novitates 2008 (3634) on page 10, DOI: 10.1206/624.1, http://zenodo.org/record/5390236
Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
Creators: name: Hartmann, Lee
name: Ballesteros-Paredes, Javier
name: Bergin, Edwin A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of both star-forming regions and young, gas-free stellar associations indicate that most nearby molecular clouds form stars only over a short time span before dispersal; large-scale flows in the diffuse interstellar medium have the potential for forming clouds sufficiently rapidly, and for producing stellar populations with ages much less than the lateral crossing times of their host molecular clouds. We identify four important factors for understanding rapid star formation and short cloud lifetimes. First, much of the accumulation and dispersal of clouds near the solar circle might occur in the atomic phase; only the high-density portion of a cloud's lifecycle is spent in the molecular phase, thus helping to limit molecular cloud ``lifetimes''. Second, once a cloud achieves a high enough column density to form $\h2$ and CO, gravitational forces become larger than typical interstellar pressure forces; thus star formation can follow rapidly upon molecular gas formation and turbulent dissipation in limited areas of each cloud complex. Third, typical magnetic fields are not strong enough to prevent rapid cloud formation and gravitational collapse. Fourth, rapid dispersal of gas by newly-formed stars, and reduction of shielding by a small expansion of the cloud after the first events of star formation, might limit the length of the star formation epoch and the lifetime of a cloud in its molecular state. This picture emphasizes the importance of large-scale boundary conditions for understanding molecular cloud formation, and implies that star formation is a highly dynamic, rather than quasi-static, process.
description: 41 pages, 10 figures, accepted by ApJ
Microcardium , Thiele 1934
Creators: name: Poutiers, Jean-Maurice
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Cardiida
Cardiidae
Microcardium

description: Genus Microcardium Thiele, 1934
 TYPE SPECIES. — Cardium (Fulvia) peramabilis Dall, 1881, by subsequent designation (Keen 1937).
REMARKS
description: Published as part of Poutiers, Jean-Maurice, 2006, Two new species of protocardiine cockles (Mollusca, Bivalvia, Cardiidae) from the tropical Southwest Pacific, pp. 635-654 in Zoosystema 28 (3) on page 643, DOI: 10.5281/zenodo.5390212
Manipulating the transmission matrix of scattering media for nonlinear imaging beyond the memory effect
Creators: name: Hofer, Matthias
name: Brasselet, Sophie
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The measurement of the Transmission Matrix (TM) of a scattering medium is of great interest for imaging. It can be acquired directly by interferometry using an internal reference wavefront. Unfortunately, internal reference fields are scattered by the medium which results in a speckle that makes the TM measurement heterogeneous across the output field of view. We demonstrate how to correct for this effect using the intrinsic properties of the TM. For thin scattering media, we exploit the memory effect of the medium and the reference speckle to create a corrected TM. For highly scattering media where the memory effect is negligible, we use complementary reference speckles to compose a new TM, not compromised by the speckled reference anymore. Using this correction, we demonstrate large field of view second harmonic generation imaging through thick biological media.
Preheating in the Universe Suppressing High Energy Gamma-rays from Structure Formation
Creators: name: Totani, Tomonori
name: Inoue, Susumu
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Structure formation in the universe can produce high energy gamma-rays from shock-accelerated electrons, and this process may be the origin of the extragalactic gamma-ray background (EGRB) as well as a part of the unidentified sources detected by EGRET in the GeV band, if about 5% of the kinetic energy of the shock is going into electron acceleration. However, we point out that the production of gamma-rays may be severely suppressed if the collapsing matter has been preheated by external entropy sources at the time of gravitational collapse, as can be inferred from the luminosity-temperature (LT) relation of galaxy clusters and groups. We also make a rough estimate of this effect by a simple model, showing that the EGRB flux may be suppressed by a factor of about 30. Hence structure formation is difficult to be the dominant origin of EGRB if preheating is actually responsible for the observed anomary in the LT relation. The detectable number of gamma-ray clusters is also reduced, but about 5-10 forming clusters should still be detectable by EGRET all sky, and this number is similar to that of the steady and high-latitude unidentified sources in the EGRET catalog. The future GLAST mission should detect 10^2-10^3 gamma-ray clusters of galaxies even if the intergalactic medium has been preheated.
description: References added for relevant work. 5 pages, 4 figures, accepted in Astroparticle Physics
Stochastic Transition between Turbulent Branch and Thermodynamic Branch of an Inhomogeneous Plasma
Creators: name: Kawasaki, Mitsuhiro
name: Itoh, Sanae-I.
name: Yagi, Masatoshi
name: Itoh, Kimitaka
Publisher: name: arXiv
Year: 2002
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Transition phenomena between thermodynamic branch and turbulent branch in submarginal turbulent plasma are analyzed with statistical theory. Time-development of turbulent fluctuation is obtained by numerical simulations of Langevin equation which contains submarginal characteristics. Probability density functions and transition rates between two states are analyzed. Transition from turbulent branch to thermodynamic branch occurs in almost entire region between subcritical bifurcation point and linear stability boundary.
description: 10 pages, 8 figures, to be published in J. Phys. Soc. Jpn
Finite-Range Coulomb Gas Models I: Some Analytical Results
Creators: name: Pandey, Akhilesh
name: Kumar, Avanish
name: Puri, Sanjay
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Dyson has shown an equivalence between infinite-range Coulomb gas models and classical random matrix ensembles for the study of eigenvalue statistics. In this paper, we introduce finite-range Coulomb gas (FRCG) models as a generalization of the Dyson models with a finite range of eigenvalue interactions. As the range of interaction increases, there is a transition from Poisson statistics to classical random matrix statistics. These models yield new universality classes of random matrix ensembles. They also provide a theoretical framework to study banded random matrices, and dynamical systems whose matrix representation can be written in the form of banded matrices.
Elamenopsis A. Milne Edwards 1873
Creators: name: Rahayu, Dwi Listyo
name: Ng, Peter K. L.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Hymenosomatidae
Elamenopsis

description: Genus Elamenopsis A. Milne Edwards, 1873
 Elamenopsis lineata A. Milne Edwards, 1873 Elamenopsis lineatus A. Milne Edwards, 1873: 324, pl. 18 fig. 4. — Kemp 1917: 250. — Tesch 1918: 26, pl. 1 figs 5, 5a-c. — Serène & Umali 1970: 58, pl. 5 fig. 11.
 Elamenopsis lineata – Lucas 1980: 192, figs 3j, 5j, 8e, 10j. — Chuang & Ng 1994: 87. — Ng & Chuang 1996: 40, figs 15, 16. — Ng & Richer de Forges 1996: 263, fig. 1. — Guinot & Richer de Forges 1997: 468, figs 4J-L, 7B.
 MATERIAL EXAMINED. — Indonesia. Kamora, intertidal, mud substrate in mangrove area, 10.VII.2001, coll. A. Pratiwi, 1 2.7 × 2.1 mm, 1 3.5 × 2.7 mm (RCO); 22.IX.2001, 1 2.8 × 2.4 mm, 2 4.9 × 3.2 mm, 3.4 × 2.7 mm (RCO).
Mawati, 4°58’S, 137°7’E, sandy mud, 3 m, estuary, 4.VIII.1999, coll. A. Haris, 2 2.3 × 1.7 mm, 2.3 × 1.6 mm, 2 2.4 × 1.7 mm, 2.1 × 1.5 mm (MNHN); 9.VIII.1999, 2 2.3 × 1.7 mm, 2.5 × 1.9 mm (MNHN).
Otakwa, 4°58’S, 137°12’E, sandy mud, 5 m, estuary, 6.VIII.1999, coll. A. Haris, 2 2.7 × 1.8 mm, 2.9 × 2.1 mm, 5 2.5 × 2 mm, 2.2 × 1.6 mm, 2.2 × 1.6 mm, 3.23 × 2.3 mm, 2.9 × 2.0 mm (MZB); 28.VIII.1999, 4 2.4 × 1.7 mm, 2.7 × 1.9 mm, 2.6 × 1.9 mm, 2.5 × 2.0 mm, 2 2.4 × 1.6 mm (ZRC 2002.604).
REMARKS
 This species has previously been reported from New Caledonia (type locality), Queensland (Australia) and Sulawesi (Indonesia) (Ng & Chuang 1996). Its presence in Irian Jaya is thus not at all surprising. In nearby Ambon, a related species, E. comosa Ng & Chuang, 1996, is present.
description: Published as part of Rahayu, Dwi Listyo & Ng, Peter K. L., 2004, The Hymenosomatidae (Crustacea, Decapoda, Brachyura) of Timika (Irian Jaya, Indonesia), pp. 87-94 in Zoosystema 26 (1) on page 88, DOI: 10.5281/zenodo.5390317
Variable Stars in Galactic Globular Clusters
Creators: name: Clement, Christine M.
name: Muzzin, Adam
name: Dufton, Quentin
name: Ponnampalam, Thivya
name: Wang, John
name: Burford, Jay
name: Richardson, Alan
name: Rosebery, Tara
name: Rowe, Jason
name: Hogg, Helen Sawyer
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Based on a search of the literature up to May 2001, the number of known variable stars in Galactic globular clusters is approximately 3000. Of these, more than 2200 have known periods and the majority (approximately 1800) are of the RR Lyrae type. In addition to the RR Lyrae population, there are approximately 100 eclipsing binaries, 120 SX Phe variables, 60 Cepheids (including population II Cepheids, anomalous Cepheids and RV Tauri) and 120 SR/red variables. The mean period of the fundamental mode RR Lyrae variables is 0.585, for the overtone variables it is 0.342 (0.349 for the first-overtone pulsators and 0.296 for the second-overtone pulsators) and approximately 30% are overtone pulsators. These numbers indicate that about 65% of RR Lyrae variables in Galactic globular clusters belong to Oosterhoff type I systems. The mean period of the RR Lyrae variables in the Oosterhoff type I clusters seems to be correlated with metal abundance in the sense that the periods are longer in the more metal poor clusters. Such a correlation does not exist for the Oosterhoff type II clusters. Most of the Cepheids are in clusters with blue horizontal branches.
description: 45 pages, 10 figures, to be published in AJ November 2001
CHALLENGES AND DEVELOPMENT TRENDS IN CLOUD-NATIVE APPLICATIONS: A COMPREHENSIVE SURVEY
Creators: name: Sandeep K Guduru
Publisher: name: Zenodo
Year: 2024

description: The core value that cloud-native applications (CNAs) deliver through modern software development depends upon cloud computing's natural scalability, adaptability, and automated systems. The paper dives deeply into CNAs while analyzing their foundational concepts that combine service-based designs, API management, and infrastructure code automation for expedited implementation and resilient dynamic operations. The growth of CNAs tracks from original cloud computing models through modern artificial intelligence systems that include edge computing and multi-cloud implementations. An examination of new trends in microservices serverless computing and containerization and DevSecOps details how they contribute to system scalability and operational efficiency while improving security. Cloud-native applications continue to evolve, but professionals encounter complexity alongside interoperability issues and implementation lock-ins that need innovative approaches. The research investigates sustainability effects alongside cost optimization practices in cloud-native environments to offer practical guidance for companies working on their cloud-native architecture improvement. The analysis provides comprehensive insights into Cloud Native Applications to empower developers and decision-makers in achieving cloud computing success through understanding complex trends and current challenges.
ทัศนคติของผู้ใช้บริการที่มีต่อมาตรฐานอาชีพของผู้ปฏิบัติงานแผนกอาหารและเครื่องดื่มในธุรกิจโรงแรม จังหวัดกระบี่
Creators: name: ปนิตา ปัญญาพิจัย
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: ทัศนคติ
ผู้ใช้บริการ
มาตรฐานอาชีพ
ผู้ปฏิบัติงานแผนกอาหารและเครื่องดื่ม

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 66-73
A BeppoSAX view of transient black hole candidates in quiescence
Creators: name: Campana, S.
name: Parmar, A. N.
name: Stella, L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on BeppoSAX observations of five transient black hole candidates during their quiescent phase. We confirm these sources are X-ray faint, improving on and complementing existing upper limits. We derive 1-10 keV upper limits for GRO J0422+32, GRS 1009-45, 4U 1630-47 and XTE J1748-288, which range from 2x10^32 erg/s to 5x10^34 erg/s. We positively detect GS 2023+338. Its X-ray spectrum can be fit by a power law (photon index Gamma=1.9) or a thermal bremsstrahlung (with kT= 7$ keV), converting in both cases to a 1-10 keV unabsorbed luminosity of ~10^33 erg/s. These values are comparable to the ones derived during an ASCA observation in 1994, indicating that the source remains stable over a ~5 yr baseline.
description: 4 pages, 1 figure. Accepted for publication on A&A (including new A&A macro)
MOESM2 of Molecular detection of drug resistant malaria in Southern Thailand
Creators: name: Chaturong Noisang
name: Prosser, Christiane
name: Meyer, Wieland
name: Waenurama Chemoh
name: Ellis, John
name: Nongyao Sawangjaroen
name: Lee, Rogan
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 2: Table S2. PCR primers used in study.
title: Промышленная и экономическая безопасность. Курс лекций
Creators: name: ELS IPR BOOKS
Publisher: name: Ай Пи Ар Медиа
Year: 2025

description: Курс лекций посвящен основам промышленной и экономической безопасности организации. Первый раздел учебного пособия рассматривает вопросы обеспечения промышленной безопасности организации: раскрывается ее суть и содержание, дана характеристика системы менеджмента промышленной безопасности, определены особенности стандартизации в этой сфере, описаны технологии формирования системы промышленной безопасности современной организации. Второй раздел учебного пособия посвящен экономической безопасности организации. В частности, дан краткий обзор современных угроз экономической безопасности, определены юридические аспекты функционирования службы экономической безопасности организации, выявлена специфика и методы сбора информации, представлена характеристика основных официальных и неофициальных источников информации, определены информационно-технологические и финансовые аспекты обеспечения экономической безопасности и пр. Подготовлено с учетом требований Федерального государственного образовательного стандарта высшего образования. Учебное пособие предназначено для студентов укрупненной группы направлений подготовки «Экономика», изучающих дисциплину «Экономическая и промышленная безопасность предприятия».
On the compactification of hyperconcave ends and the theorems of Siu-Yau and Nadel
Creators: name: Marinescu, George
name: Dinh, Tien-Cuong
Publisher: name: arXiv
Year: 2002
Subjects: subject: Complex Variables (math.CV)
subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 32J05 (Primary), 32C22, 53C55 (Secondary)

description: We show that the pseudoconcave holes of some naturally arising class of manifolds, called hyperconcave ends, can be filled in, including the case of complex dimension 2 . As a consequence we obtain a stronger version of the compactification theorem of Siu-Yau and extend Nadel's theorems to dimension 2.
description: 13 pages, AMSLaTeX, short version accepted for publication in Inventiones Math
Ascocotyle (Phagicola) macrostoma
Creators: name: Scholz, T.
name: Aguirre-Macedo, M. L.
name: Salgado-Maldonado, G.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Platyhelminthes
Trematoda
Plagiorchiida
Heterophyidae
Ascocotyle
Ascocotyle macrostoma

description: Ascocotyle (Phagicola) macrostoma (Robinson, 1956)
 Metacercaria
 Morphology. To date, no data on metacercarial morphology exist.
 Second intermediate host. Poecilia velifera (Poeciliidae).
description: Published as part of Scholz, T., Aguirre-Macedo, M. L. & Salgado-Maldonado, G., 2001, Trematodes of the family Heterophyidae (Digenea) in Mexico: a review of species and new host and geographical records, pp. 1733-1772 in Journal of Natural History 35 (12) on page 1752, DOI: 10.1080/00222930152667087, http://zenodo.org/record/5275922