cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Orientation Parameters of the Cepheid System in the Galaxy
Creators: name: Bobylev, Vadim
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Based on the distribution of long-period Cepheids, we have redetermined the orientation parameters of their principal plane in the Galaxy. Based on 299 Cepheids with heliocentric distances $r<20$ kpc and pulsation periods $P\geq5^d$, we have found the directions of the three principal axes of the position ellipsoid: $L_1=281.0\pm0.1^\circ,$ $B_1=-1.9\pm0.1^\circ,$ $L_2= 11.0\pm0.7^\circ,$ $B_2=0.2\pm0.1^\circ$ and $L_3=275.9\pm0.7^\circ,$ $B_3=88.1\pm0.1^\circ$. Thus, the line of nodes $l_Ω=L_3+90^\circ=5.9^\circ$ is very close to the direction to the Galactic center; the Cepheid symmetry plane is inclined to the Galactic plane approximately by $-2^\circ$ in the direction of the first axis ($L_1$). The direction of the line of nodes found from old Cepheids ($P<5^d$) differs significantly and is $l_Ω=298^\circ$. The elevation of the Sun above the Galactic plane has been estimated from 365 closer stars ($r<4$ kpc) without any constraint on the pulsation period to be $h_\odot=23\pm5$ pc.
description: 10 pages, 3 figures
Agrilactobacillus Zheng & Wittouck & Salvetti & Franz & Harris & Mattarelli & O'Toole & Pot & Vandamme & Walter & Watanabe & Wuyts & Felis & Gänzle & Lebeer 2020, GEN. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Agrilactobacillus

description: DESCRIPTIONOF AGRILACTOBACILLUS GEN. NOV.
Agrilactobacillus (A.gri.lac.to.ba.cil’lus. L. adj.masc. n. ager, a field; N.L. masc. n. Lactobacillus, a bacterial genus; Agrilactobacillus, a lactobacillus from fields or soil).
Gram positive, rod-shaped, catalase negative, homofermentative and aerotolerant. The genome size ranges from 2.33 to 3.47 Mbp; the mol% G+C content of DNA ranges from 42.1 to 44.0. Origin, physiological properties and genome characteristics suggest a free-living lifestyle of the genus. Isolated from compost that included shochu mash and from vegetables (mustard) in Indonesia and China.
The type species of the genus is A. composti.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on pages 2809-2810, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Dendromus kivu Thomas 1916
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Dendromus
Dendromus kivu

description: Dendromus kivu Thomas, 1916. Ann. Mag. Nat. Hist., ser. 8, 18:242. TYPE LOCALITY: Zaire, near Lake Kivu, Buhamba, 2000 m. DISTRIBUTION: A possible montane Western Rift endemic; recorded from the west and east slopes of the Ruwenzoris in E Zaire and W Uganda (Osgood, 1936, and specimens in the Field Museum of Natural History) and the Kivu region in E Zaire (samples in the American Museum of Natural History and the British Museum of Natural History). SYNONYMS: lunaris. COMMENTS: Osgood (1936:236) discussed two series of Dendromus collected at the same time and place on the western slope of Mt. Ruwenzori. He described one as D. lunaris, based on two examples, and identified the other as D. insignis, a conclustion we verified from study of his specimens. The two species are also sympatric in the Kivu Region (series in American Museum of Natural History). Thomas originally described kivu as a subspecies of D. insignis, but our study of the holotype reveals it to be the same as Osgood's lunaris, which it predates. Both kivu and insignis have been included in D. mesomelas (Bohmann, 1942; Misonne, 1974). It is the smallerbodied kivu that is morphologically similar to D. mesomelas and the nature of the relationship between the two will have to be revealed by systematic revision of the mesomelas group.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 542, DOI: 10.5281/zenodo.7353098
description: {"references": ["Osgood, W. H. 1936. New and imperfectly known small mammals from Africa. Field Museum of Natural History, Zoological Series, 20: 217 - 256.", "Bohmann, L., von. 1942. Die Gattung Dendromus A. Smith. Versuch einer naturlichen Gruppierung (Ergebnisse der Ostafrika-Reise 1937 Uthmoller-Bohmann. VIII). Zoologischer Anzeiger, 139: 33 - 53.", "Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Instantons on Young diagrams with matters
Creators: name: Chen, Yanyan
name: Jiang, Jiaqun
name: Nawata, Satoshi
name: Shao, Yilu
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present the unrefined instanton partition functions of various 5d gauge theories with matter beyond the fundamental representation as sums over Young diagrams. By using these explicit expressions, we verify a range of identities among the instanton partition functions predicted by Higgsing procedures of fivebrane web diagrams and representation theory.
description: 32 pages, Mathematica file is attached: v2, typos corrected, JHEP version
Estimation of high-resolution dust column density maps: Empirical model fits
Creators: name: Juvela, M.
name: Montillaud, J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Sub-millimetre dust emission is an important tracer of density N of dense interstellar clouds. One has to combine surface brightness information at different spatial resolutions, and specific methods are needed to derive N at a resolution higher than the lowest resolution of the observations. Some methods have been discussed in the literature, including a method (in the following, method B) that constructs the N estimate in stages, where the smallest spatial scales being derived only use the shortest wavelength maps. We propose simple model fitting as a flexible way to estimate high-resolution column density maps. Our goal is to evaluate the accuracy of this procedure and to determine whether it is a viable alternative for making these maps. The new method consists of model maps of column density (or intensity at a reference wavelength) and colour temperature. The model is fitted using Markov chain Monte Carlo (MCMC) methods, comparing model predictions with observations at their native resolution. We analyse simulated surface brightness maps and compare its accuracy with method B and the results that would be obtained using high-resolution observations without noise. The new method is able to produce reliable column density estimates at a resolution significantly higher than the lowest resolution of the input maps. Compared to method B, it is relatively resilient against the effects of noise. The method is computationally more demanding, but is feasible even in the analysis of large Herschel maps. The proposed empirical modelling method E is demonstrated to be a good alternative for calculating high-resolution column density maps, even with considerable super-resolution. Both methods E and B include the potential for further improvements, e.g., in the form of better a priori constraints.
description: Accepted to A&A
Control of magnetic response in curved stripes by tailoring cross-section
Creators: name: Yershov, Kostiantyn V.
name: Sheka, Denis D.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Curved magnetic architectures are key enablers of the prospective magnetic devices with respect to size, functionality and speed. By exploring geometry-governed magnetic interactions, curvilinear magnetism offers a number of intriguing effects in curved magnetic wires and curved magnetic films. The applicability of the current micromagnetic theory requires that the sample has constant width and thickness, which does not correspond in many cases to specificity of experimental sample preparation. Here, we put forth a self-consistent micromagnetic framework of curvilinear magnetism of nanowires and narrow stripes with spatially inhomogeneous cross-section. The influence of the varying cross-section is exploited and illustrated by an example of the simplest topological texture, which is a transversal head-to-head (tail-to-tail) domain wall. The cross-section gradient becomes a source of domain wall pinning which competes the curvature gradient. Eigenfrequencies of the domain wall free oscillations at the pinning potential are determined by both curvature and cross-section gradients. Prospects for curvilinear magnonics and spintronics are discussed.
Dendromus lovati de Winton 1900
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Dendromus
Dendromus lovati

description: Dendromus lovati de Winton, 1900. Proc. Zool. Soc. Lond., 1899:986 [1900]. TYPE LOCALITY: Ethiopia, Managasha, near Addis Ababa. DISTRIBUTION: Endemic to Ethiopian Plateau where it is recorded from 2500-3550 m (Rupp, 1980; Yalden et al., 1976). COMMENTS: A grassland species differing from other members of Dendromus in its apparently strictly terrestrial habits (Yalden et al., 1976; Yalden, 1988).
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 542, DOI: 10.5281/zenodo.7353098
description: {"references": ["Rupp, H. 1980. Beitrage zur Systematik, Verbreitung und Okologie athiopischer Nagetiere. Ergebnisse mehrerer Forschungsreisen. Saugetierkundliche Mitteilungen, 28 (2): 81 - 123.", "Yalden, D. W., M. J. Largen, and D. Kock. 1976. Catalogue of the mammals of Ethiopia. 2. Insectivora and Rodentia. Monitore Zoologico Italiano, Supplemento 8 (1): 1 - 118.", "Yalden, D. W. 1988. Small mammals of the Bale Mountains, Ethiopia. African Journal of Ecology, 26: 281 - 294."]}
Dihadron Production in DIS at Small $x$ at Next to Leading Order: Transverse Photons
Creators: name: Bergabo, Filip
name: Jalilian-Marian, Jamal
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the next to leading order corrections to dihadron production in Deep Inelastic Scattering (DIS) at small x using the Color Glass Condensate formalism for the case when the virtual photon is transverse polarized. Similar to the case of longitudinal photon exchange all UV and soft singularities cancel while the collinear divergences are absorbed into quark and antiquarkhadron fragmentation functions. Rapidity divergences lead to JIMWLK evolution of dipoles and quadrupoles which describe multiple-scatterings of the quark antiquark dipole on the target proton/ nucleus and contain all the QCD dynamics of the target leading to a finite final result for the dihadron production cross section.
description: 13 pages, 2 figures. arXiv admin note: substantial text overlap with arXiv:2207.03606
Exclusive charmonium production from $e^+ e^-$ annihilation round the $Z^0$ peak
Creators: name: Chen, Gu
name: Wu, Xing-Gang
name: Sun, Zhan
name: Wang, Sheng-Quan
name: Shen, Jian-Ming
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We make a comparative and comprehensive study on the charmonium exclusive productions at the $e^+e^-$ collider with the collision energy either round the $Z^0$-boson mass for a super $Z$ factory or equals to 10.6 GeV for the $B$ factories as Belle and BABAR. We study the total cross sections for the charmonium production via the exclusive processes $e^+e^- \to γ^*/Z^0 \to H_{1}+H_{2}$ and $e^+e^- \to γ^*/Z^0 \to H_{1} +γ$, where $H_{1}$ and $H_{2}$ represent the dominant color-singlet $S$-wave and $P$-wave charmonium states respectively. Total cross sections versus the $e^+e^-$ collision energy $\sqrt{s}$, together with their uncertainties, are presented, which clearly show the relative importance of these channels. At the $B$ factory, the production channels via the virtual $γ^*$ propagator are dominant over the channels via the $Z^0$ propagator by about four orders. While, at the super $Z$ factory, due to the $Z^0$-boson resonance effect, the $Z^0$ boson channels shall provide sizable or even dominant contributions in comparison to the channels via the $γ^*$ propagator. Sizable exclusive charmonium events can be produced at the super $Z$ factory with high luminocity up to $10^{36}{\rm cm}^{-2}{\rm s}^{-1}$, especially for the channel of $e^+e^- \to Z^0 \to H_{1} +γ$, e.g. by taking $m_c=1.50\pm0.20$ GeV, we shall have $(5.0^{+0.8}_{-0.6})\times10^4$ $J/ψ$, $(7.5^{+1.1}_{-0.9})\times10^3$ $η_c$, $(6.2^{+3.3}_{-1.9})\times10^3$ $h_{c}$, $(3.1^{+1.7}_{-0.9})\times10^2$ $χ_{c0}$, $(2.2^{+1.0}_{-0.4})\times10^3$ $χ_{c1}$, and $(7.7^{+4.1}_{-2.4})\times10^2$ $χ_{c2}$ events by one operation year. Thus, in addition to the $B$ factories as BABAR and Belle, such a super $Z$ factory shall provide another useful platform for studying the heavy quarkonium properties and for testing QCD theories.
description: 19 pages, 9 figures. References and discussions updated. To be published in Phys.Rev.D
The use of action research to address vegetation management on beef properties in Central Queensland
Creators: name: Gray, Andrea J
Publisher: name: CQUniversity
Year: 2023

description: Project explores the use of action research processes which were developed and implemented to work with two groups of beef producers in relation to vegetation management. The study implemented an innovative action research/action learning framework for extension education involving two groups of beef industry producers in central Queensland on the topic of vegetation management. The researcher acted as group facilitator for group meetings over the course of seven months in 1994, using a framework of Participatory Problem Solving (Clark 1993). The findings of the study are presented under the headings of participants, vegetation management and action research techniques, with action research as a form of extension education being seen as the main area of learning arising from the project. Data about producer participants is important, since little is recorded in extension education literature and the processes used to gain this knowledge may be extrapolated from this study to other studies using a similar approach. Specialist researchers in vegetation management provided both direct material for group discussion and gave feedback to producers on their vegetation management practice. While the participants themselves did not change their vegetation management practice during the course of the project, they have made a commitment to continue their meetings independently. There are thus grounds for anticipating that the process if continued would see some form of change in this area. The techniques used in the group meetings, and participants evaluation of these techniques is thoroughly documented, using qualitative methods of meeting notes, interviews and questionnaires. The study concludes with a reflection on the action research processes used and suggests that while generalisations are not possible from one extension education situation to another, that some of the techniques and their sequencing could be adapted for use in other settings and that the Participatory Problem Solving cycle, if completed, provides an important contribution to extension education. Future extension models have yet to be developed as a widespread practice in extension. Many remain at the conceptual level, with little literature exploring their significance in practice. This thesis adds to this small but growing literature on alternative extension practices.
Dendromus melanotis Smith 1834
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Dendromus
Dendromus melanotis

description: Dendromus melanotis Smith, 1834. S. Afr. Quart. J., 2: 158. TYPE LOCALITY: South Africa, near Port Natal (Durban). DISTRIBUTION: From South Africa (see map in Skinner and Smithers, 1990:306) north to Uganda, and west through Nigeria to Mt-Nimba in Guinea; also from Ethiopia (# 8119 in American Museum of Natural History), but published records might be D. mystacalis (Yalden et al., 1976). Limits of range unresolved. SYNONYMS: arenarius, basuticus, capensis, carteri, chiversi, concinnus, exoneratus, insignis (Shortridge and Carter, 1938, not Thomas, 1903), leucostomus, nigrifrons, pallidus, pretoriae, shortridgei, spectabilis, subtilis, thorntoni, vulturnus.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 542-543, DOI: 10.5281/zenodo.7353098
description: {"references": ["Skinner, J. D., and R. H. N. Smithers. 1990. The mammals of the southern African subregion. Second ed. University of Pretoria, Republic of South Africa, 771 pp.", "Yalden, D. W., M. J. Largen, and D. Kock. 1976. Catalogue of the mammals of Ethiopia. 2. Insectivora and Rodentia. Monitore Zoologico Italiano, Supplemento 8 (1): 1 - 118.", "Shortridge, G. C., and T. D. Carter. 1938. A new genus and new species and subspecies of mammals from Little Namaqualand and the north-west Cape Province; and a new subspecies of Gerbillus paeba from the eastern Cape Province. Annals of the South African Museum, 3 (2): 281 - 291.", "Thomas, O. 1903. Notes on Neotropical mammals of the genera Felis, Hapale, Oryzomys, Akodon, and Ctenomys, with descriptions of new species. Annals and Magazine of Natural History, ser. 7, 12: 234 - 243."]}
Low-order wavefront control using a Zernike sensor through Lyot coronagraphs for exoplanet imaging: II. Concurrent operation with stroke minimization
Creators: name: Pourcelot, R.
name: Por, E. H.
name: N'Diaye, M.
name: Benard, H.
name: Brady, G.
name: Canas, L.
name: Carbillet, M.
name: Dohlen, K.
name: Laginja, I.
name: Lugten, J.
name: Noss, J.
name: Perrin, M. D.
name: Petrone, P.
name: Pueyo, L.
name: Redmond, S. F.
name: Sahoo, A.
name: Vigan, A.
name: Will, S. D.
name: Soummer, R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Wavefront sensing and control (WFSC) will play a key role in improving the stability of future large segmented space telescopes while relaxing the thermo-mechanical constraints on the observatory structure. Coupled with a coronagraph to reject the light of an observed bright star, WFSC enables the generation and stabilisation of a dark hole (DH) in the star image to perform planet observations. While WFSC traditionally relies on a single wavefront sensor (WFS) input to measure wavefront errors, the next generation of instruments will require several WFSs to address aberrations with different sets of spatial and temporal frequency contents. The multiple measurements produced in such a way will then have to be combined and converted to commands for deformable mirrors (DMs) to modify the wavefront subsequently. We asynchronously operate a loop controlling the high-order modes digging a DH and a control loop that uses the rejected light by a Lyot coronagraph with a Zernike wavefront sensor to stabilize the low-order aberrations. Using the HiCAT testbed with a segmented telescope aperture, we implement concurrent operations and quantify the expected cross-talk between the two controllers. We then present experiments that alternate high-order and low-order control loops to identify and estimate their respective contributions. We show an efficient combination of the high-order and low-order control loops, keeping a DH contrast better than 5 x 10-8 over a 30 min experiment and stability improvement by a factor of 1.5. In particular, we show a contrast gain of 1.5 at separations close to the DH inner working angle, thanks to the low-order controller contribution. Concurrently digging a DH and using the light rejected by a Lyot coronagraph to stabilize the wavefront is a promising path towards exoplanet imaging and spectroscopy with future large space observatories.
Cepheid Kinematics and the Galactic Warp
Creators: name: Bobylev, Vadim
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The space velocities of 200 long-period ($P>5$ days) classical Cepheids with known proper motions and line-of-sight velocities whose distances were estimated from the period--luminosity relation have been analyzed. The linear Ogorodnikov-Milne model has been applied, with the Galactic rotation having been excluded from the observed velocities in advance. Two significant gradients have been found in the Cepheid velocities, $\partial W/\partial Y=-2.1\pm0.7$ km s$^{-1}$ kpc$^{-1}$ and $\partial V/\partial Z= 27\pm10 $ km s$^{-1}$ kpc$^{-1}$. In such a case, the angular velocity of solid-body rotation around the Galactic $X$ axis directed to the Galactic center is $-15\pm5$ km s$^{-1}$ kpc$^{-1}$.
description: 9 pages, 3 figures, 1 table
Multiclass classification utilising an estimated algorithmic probability prior
Creators: name: Dingle, Kamaludin
name: Batlle, Pau
name: Owhadi, Houman
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Probability (math.PR)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: Methods of pattern recognition and machine learning are applied extensively in science, technology, and society. Hence, any advances in related theory may translate into large-scale impact. Here we explore how algorithmic information theory, especially algorithmic probability, may aid in a machine learning task. We study a multiclass supervised classification problem, namely learning the RNA molecule sequence-to-shape map, where the different possible shapes are taken to be the classes. The primary motivation for this work is a proof of concept example, where a concrete, well-motivated machine learning task can be aided by approximations to algorithmic probability. Our approach is based on directly estimating the class (i.e., shape) probabilities from shape complexities, and using the estimated probabilities as a prior in a Gaussian process learning problem. Naturally, with a large amount of training data, the prior has no significant influence on classification accuracy, but in the very small training data regime, we show that using the prior can substantially improve classification accuracy. To our knowledge, this work is one of the first to demonstrate how algorithmic probability can aid in a concrete, real-world, machine learning problem.
Sur le comptage des fibrés de Hitchin nilpotents
Creators: name: Chaudouard, Pierre-Henri
name: Laumon, Gérard
Publisher: name: arXiv
Year: 2013
Subjects: subject: Algebraic Geometry (math.AG)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics

description: This paper is concerned with two problems. One is to count Hitchin bundles on a projective curve and the other is to get an explicit formula for the nilpotent part of the Arthur-Selberg trace formula for a simple test function. The fact that the two problems are in fact related has been noticed in a previous paper. We expand the nilpotent part of the Arthur-Selberg trace formula in a sum of adelic integrals indexed by nilpotent orbits. For "regular by blocks" orbits, we get an explicit formula for these integrals in terms of the zeta function of the curve.
Dendromus mesomelas Brants 1827
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Dendromus
Dendromus mesomelas

description: Dendromus mesomelas Brants, 1827. Het. Geslacht der Muizen, p. 122. TYPE LOCALITY: South Africa, E Cape Prov., Sunday's River, east of Port Elizabeth. DISTRIBUTION: Discontinuous ranges in South Africa (SW Cape Prov. east to Natal and E Transvaal), C Mozambique, extreme NE Zambia, N Botswana (see Map in Skinner and Smithers, 1990:307), extreme NW and NE Zaire (Ansell, 1978), highlands of N and S Malawi (Ansell and Dowsett, 1988), mountains of SW (Rungwe) and EC (Uluguru) Tanzania, and SE Zaire (Marungu); extent of range unresolved. SYNONYMS: ayresi, hintoni, major, nyasae, pumilio, typicus, typus. COMMENTS: We treat some of the names usually included in D. mesomelas (see Misonne, 1974) as distinct species (see accounts of insignis, kivu, oreas, and vernayi). Judged by our study of specimens, samples from SE Zaire and SW Tanzania are morphologically similar to series of D. kivu, and the relationship among these and samples of true mesomelas has to be resolved by critical systematic revision. We include major, which was described as a subspecis of D. mesomelas (see St. Leger, 1930), but its relationships should be reexamined because of its large body size.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 543, DOI: 10.5281/zenodo.7353098
description: {"references": ["Skinner, J. D., and R. H. N. Smithers. 1990. The mammals of the southern African subregion. Second ed. University of Pretoria, Republic of South Africa, 771 pp.", "Ansell, W. F. H. 1978. The mammals of Zambia. National Parks and Wildlife Service, Chilanga, 126 pp.", "Ansell, W. F. H., and R. J. Dowsett. 1988. Mammals of Malawi: An annotated check list and atlas. Trendrine Press, Zennor, St. Ives, United Kingdom, 170 pp.", "Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated.", "St. Leger, J. 1930. On two species of Dendromus. Annals and Magazine of Natural History, ser. 10, 6: 622."]}
CKM benchmarks for electron EDM experiments
Creators: name: Pospelov, Maxim
name: Ritz, Adam
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: All current experiments searching for an electron EDM d_e are performed with atoms and diatomic molecules. Motivated by significant recent progress in searches for an EDM-type signal in diatomic molecules with an uncompensated electron spin, we provide an estimate for the expected signal in the Standard Model due to the CKM phase. We find that the main contribution originates from the effective electron-nucleon operator $\bar{e} iγ_5 e \bar{N}N$, induced by a combination of weak and electromagnetic interactions at $O(G_F^2α^2)$, and not by the CKM-induced electron EDM itself. When the resulting atomic P,T-odd mixing is interpreted as an {\it equivalent} electron EDM, this estimate leads to the benchmark $d_e^{equiv}(CKM) \sim 10^{-38}$ ecm.
description: 7 pages, 4 figures; v2: references added
Agrilactobacillus camposti COMPOSTI 2020, COMB. NOV.
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Agrilactobacillus
Agrilactobacillus camposti

description: DESCRIPTIONOF AGRILACTOBACILLUS COMPOSTI COMB. NOV.
Agrilactobacillus composti (com.pos’ti. N.L. gen. n. composti of compost, the source of the type strain).
Basonym: Lactobacillus composti Endo and Okada 2007, 872 VP
The type strain grows over a relatively wide pH range and in the range of 10–37°C but not at 45 °C [150]. The genome size is 3.47 Mbp and the mol% G+C content of DNAis 44.0.
Isolated from compost from shochu mash solids and from pulque, a Mexican alcoholic beverage [151].
Thetypestrainis NRIC 0689 T =DSM 18527 T =JCM 14202 T.
Genome sequence accession number: AZGA00000000.
16S rRNA gene accession number: AB268118.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2810, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
A "Boosted Fireball" Model for Structured Relativistic Jets
Creators: name: Duffell, Paul C.
name: MacFadyen, Andrew I.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a model for relativistic jets which generates a particular angular distribution of Lorentz factor and energy per solid angle. We consider a fireball with specific internal energy E/M launched with bulk Lorentz factor γ_B. This "boosted fireball" model is motivated by the phenomenology of collapsar jets, but is applicable to a wide variety of relativistic flows. In its center-of-momentum frame the fireball expands isotropically, converting its internal energy into radially expanding flow with asymptotic Lorentz factor η_0 ~ E/M. In the lab frame the flow is beamed, expanding with Lorentz factor Γ= 2 η_0 γ_B in the direction of its initial bulk motion and with characteristic opening angle θ_0 ~ 1/γ_B. The flow is jet-like with Γθ_0 ~ 2 η_0 such that jets with Γ> 1/θ_0 are naturally produced. The choice η_0 ~ γ_B ~ 10 yields a jet with Γ~ 200 on-axis and angular structure characterized by opening angle θ_0 ~ 0.1 of relevance for cosmological GRBs, while γ_B >~ 1 may be relevant for low-luminosity GRBs. The model produces a family of outflows, of relevance for different relativistic phenomena with structures completely determined by η_0 and γ_B. We calculate the energy per unit solid angle for the model and use it to compute light curves for comparison with the widely used top-hat model. The jet break in the boosted fireball light curve is greatly subdued when compared to the top-hat model because the edge of the jet is smoother than for a top-hat. This may explain missing jet breaks in afterglow light curves.
description: ApJ Accepted
On the accuracy of one-way approximate models for nonlinear waves in soft solids
Creators: name: Berjamin, Harold
Publisher: name: arXiv
Year: 2023
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mathematical Physics (math-ph)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences
subject: 74D10, 74J30

description: Simple strain-rate viscoelasticity models of isotropic soft solid are introduced. The constitutive equations account for finite strain, incompressibility, material frame-indifference, nonlinear elasticity, and viscous dissipation. A nonlinear viscous wave equation for the shear strain is obtained exactly, and corresponding one-way Burgers-type equations are derived by making standard approximations. Analysis of the travelling wave solutions shows that these partial differential equations produce distinct solutions, and that deviations are exacerbated when wave amplitudes are not arbitrarily small. In the elastic limit, the one-way approximate wave equation can be linked to simple wave theory and shock wave theory, thus allowing direct error measurements.
title: Η αρχιτεκτονική μέσα από σενάρια δυστοπίας του κινηματογράφου
title: Architecture through dystopia cinema scenarios
Creators: name: Γκοφη Νικολετα
name: Σωτηριου Βασιλικη-Ελενη
Publisher: name: Technical University of Crete
Year: 2023

description: Το κείμενο διερευνά το δίπολο δυστοπία - ουτοπία στον κινηματογράφο. Πιο συγκεκριμένα την αρχιτεκτονική έκφραση των δύο εννοιών σε μελλοντολογικά σενάρια ταινιών σκηνοθεσίας μεταγενέστερης του 2010. Μέσα από την παρουσίαση επιλεγμένων ταινιών, γίνεται ο εντοπισμός αρχιτεκτονικών εκφράσεων και χειρισμών προκειμένου να τονιστεί το σενάριο της δυστοπίας και συνάμα της ουτοπίας καθώς γίνεται αντιληπτό ότι οι δύο καταστάσεις είναι αλληλένδετες. Έπειτα, παραθέτονται τρεις δυστοπικές ταινίες του Κορεάτικου και του Αμερικάνικου κινηματογράφου, το Snowpiercer, το HighRise και το Elysium, με κριτήριο την αρχιτεκτονική κλίμακα του πεδίου δράσης τους. Τα θέματα που αντιμετωπίζονται είναι ο κοινωνικός διαχωρισμός, η ιδιωτικότητα, ο φυσικός και τεχνητός φωτισμός, η κλίμακα του χώρου. Τα συμπεράσματα συνοψίζουν τους αρχιτεκτονικούς χειρισμούς στο πεδίο δράσης των ταινιών μελέτης, οι οποίοι τονίζουν εμφατικά το σενάριο της δυστοπίας που διαπραγματεύεται το σενάριο της κάθε σκηνοθεσίας.
Dendromus messorius Thomas 1903
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Dendromus
Dendromus messorius

description: Dendromus messorius Thomas, 1903. Ann. Mag. Nat. Hist., ser. 7, 12:340. TYPE LOCALITY: Cameroon, Efulen. DISTRIBUTION: Benin, Nigeria to Zaire, Uganda, Kenya, and Sudan; limits not yet resolved. SYNONYMS: haymani, kumasi, ruddi. COMMENTS: Treated as part of D. mystacalis by Misonne (1974), but regarded as a separate species by Hatt (1940a) and Dieterlen (1971), who pointed out its sympatric distribution with D. mystacalis.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 543, DOI: 10.5281/zenodo.7353098
description: {"references": ["Misonne, X. 1974. Order Rodentia. Part 6. Pp. 1 - 39, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.). [issued 10 Sep 1974]. Smithsonian Institution Press, Washington, D. C., not continuously paginated.", "Hatt, R. T. 1940 a. Lagomorpha and Rodentia other than Sciuridae, Anomaluridae and Idiuridae, collected by the American Museum Congo Expedition. Bulletin of the American Museum of Natural History, 76 (9): 457 - 604.", "Dieterlen, F. 1971. Beitrage zur Systematik, Okologie und Biologie der Gattung Dendromus (Dendromurinae, Cricetidae, Rodentia), insbesondere ihrer zentralafrikanischen Formen. Saugetierkundliche Mitteilungen, 19: 97 - 132."]}
Beyond ITER: Neutral beams for DEMO
Creators: name: McAdams, R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: In the development of magnetically confined fusion as an economically sustainable power source, ITER is currently under construction. Beyond ITER is the DEMO programme in which the physics and engineering aspects of a future fusion power plant will be demonstrated. DEMO will produce net electrical power. The DEMO programme will be outlined and the role of neutral beams for heating and current drive will be described. In particular, the importance of the efficiency of neutral beam systems in terms of injected neutral beam power compared to wallplug power will be discussed. Options for improving this efficiency including advanced neutralisers and energy recovery are discussed.
description: 5 pages, 10 figures
An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB
Creators: name: Cook, Amanda M.
name: Bhardwaj, Mohit
name: Gaensler, B. M.
name: Scholz, Paul
name: Eadie, Gwendolyn M.
name: Hill, Alex S.
name: Kaspi, Victoria M.
name: Masui, Kiyoshi W.
name: Curtin, Alice P.
name: Dong, Fengqiu Adam
name: Fonseca, Emmanuel
name: Herrera-Martin, Antonio
name: Kaczmarek, Jane
name: Lanman, Adam E.
name: Lazda, Mattias
name: Leung, Calvin
name: Meyers, Bradley W.
name: Michilli, Daniele
name: Pandhi, Ayush
name: Pearlman, Aaron B.
name: Pleunis, Ziggy
name: Ransom, Scott
name: Rahman, Mubdi
name: Sand, Ketan R.
name: Shin, Kaitlyn
name: Smith, Kendrick
name: Stairs, Ingrid
name: Stenning, David C.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The CHIME/FRB project has detected hundreds of fast radio bursts (FRBs), providing an unparalleled population to probe statistically the foreground media that they illuminate. One such foreground medium is the ionized halo of the Milky Way (MW). We estimate the total Galactic electron column density from FRB dispersion measures (DMs) as a function of Galactic latitude using four different estimators, including ones that assume spherical symmetry of the ionized MW halo and ones that imply more latitudinal-variation in density. Our observation-based constraints of the total Galactic DM contribution for $|b|\geq 30^\circ$, depending on the Galactic latitude and selected model, span 87.8 - 141 pc cm^-3. This constraint implies upper limits on the MW halo DM contribution that range over 52-111 pc cm^-3. We discuss the viability of various gas density profiles for the MW halo that have been used to estimate the halo's contribution to DMs of extragalactic sources. Several models overestimate the DM contribution, especially when assuming higher halo gas masses (~ 3.5 x 10^12 solar masses). Some halo models predict a higher MW halo DM contribution than can be supported by our observations unless the effect of feedback is increased within them, highlighting the impact of feedback processes in galaxy formation.
description: 19 pages, 4 figures. ApJ in press (accepted February 8th, 2023)
"TT_directTT_800_1.dat" of "Search for a scalar partner of the top quark in the jets plus missing transverse momentum final state at $\sqrt{s}$=13 TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: TT_directTT_800_1 SLHA
description: A search for pair production of a scalar partner of the top quark in events with four or more jets plus missing transverse momentum is presented. An analysis of 36.1 fb$^{-1}$ of $\sqrt{s}$=13 TeV proton--proton collisions collected using the ATLAS detector at the LHC yields no significant excess over the expected Standard Model background. To interpret the results a simplified supersymmetric model is used where the top squark is assumed to decay via $\tilde{t}_1 \rightarrow t^{(*)} \tilde\chi^0_1$ and $\tilde{t}_1\rightarrow b\tilde\chi^\pm_1 \rightarrow b W^{(*)} \tilde\chi^0_1$, where $\tilde\chi^0_1$ ($\chi^\pm_1$) denotes the lightest neutralino (chargino). Exclusion limits are placed in terms of the top-squark and neutralino masses. Assuming a branching ratio of 100% to $t \tilde\chi^0_1$, top-squark masses in the range 450--950 GeV are excluded for $\tilde\chi^0_1$ masses below 160 GeV. In the case where $m_{\tilde{t}_1}\sim m_t+m_{\tilde\chi^0_1}$, top-squark masses in the range 235--590 GeV are excluded.
"TT_directTT_600_300.dat" of "Search for a scalar partner of the top quark in the jets plus missing transverse momentum final state at $\sqrt{s}$=13 TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: TT_directTT_600_300 SLHA
description: A search for pair production of a scalar partner of the top quark in events with four or more jets plus missing transverse momentum is presented. An analysis of 36.1 fb$^{-1}$ of $\sqrt{s}$=13 TeV proton--proton collisions collected using the ATLAS detector at the LHC yields no significant excess over the expected Standard Model background. To interpret the results a simplified supersymmetric model is used where the top squark is assumed to decay via $\tilde{t}_1 \rightarrow t^{(*)} \tilde\chi^0_1$ and $\tilde{t}_1\rightarrow b\tilde\chi^\pm_1 \rightarrow b W^{(*)} \tilde\chi^0_1$, where $\tilde\chi^0_1$ ($\chi^\pm_1$) denotes the lightest neutralino (chargino). Exclusion limits are placed in terms of the top-squark and neutralino masses. Assuming a branching ratio of 100% to $t \tilde\chi^0_1$, top-squark masses in the range 450--950 GeV are excluded for $\tilde\chi^0_1$ masses below 160 GeV. In the case where $m_{\tilde{t}_1}\sim m_t+m_{\tilde\chi^0_1}$, top-squark masses in the range 235--590 GeV are excluded.
Galactic Rotation Curve and Spiral Density Wave Parameters from 73 Masers
Creators: name: Bobylev, Vadim
name: Bajkova, Anisa
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Based on kinematic data on masers with known trigonometric parallaxes and measurements of the velocities of HI clouds at tangential points in the inner Galaxy, we have refined the parameters of the Allen-Santillan model Galactic potential and constructed the Galactic rotation curve in a wide range of Galactocentric distances, from 0 to 20 kpc. The circular rotation velocity of the Sun for the adopted Galactocentric distance $R_0=8$ kpc is $V_0=239\pm16$ km s$^{-1}$. We have obtained the series of residual tangential, $ΔV_θ$, and radial, $ΔV_R,$ velocities for 73 masers. Based on these series, we have determined the parameters of the Galactic spiral density wave satisfying the linear Lin.Shu model using the method of periodogram analysis that we proposed previously. The tangential and radial perturbation amplitudes are $f_θ=7.0\pm1.2$ km s$^{-1}$ and $f_R=7.8\pm0.7$ km s$^{-1}$, respectively, the perturbation wavelength is $λ=2.3\pm0.4$ kpc, and the pitch angle of the spiral pattern in a two-armed model is $i=-5.2^\circ\pm0.7^\circ$. The phase of the Sun $χ_\odot$ in the spiral density wave is $-50^\circ\pm15^\circ$ and $-160^\circ\pm15^\circ$ from the residual tangential and radial velocities, respectively.
description: 14 pages, 3 figures, 2 tables
"TT_directTT_250_77.dat" of "Search for a scalar partner of the top quark in the jets plus missing transverse momentum final state at $\sqrt{s}$=13 TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: TT_directTT_250_77 SLHA
description: A search for pair production of a scalar partner of the top quark in events with four or more jets plus missing transverse momentum is presented. An analysis of 36.1 fb$^{-1}$ of $\sqrt{s}$=13 TeV proton--proton collisions collected using the ATLAS detector at the LHC yields no significant excess over the expected Standard Model background. To interpret the results a simplified supersymmetric model is used where the top squark is assumed to decay via $\tilde{t}_1 \rightarrow t^{(*)} \tilde\chi^0_1$ and $\tilde{t}_1\rightarrow b\tilde\chi^\pm_1 \rightarrow b W^{(*)} \tilde\chi^0_1$, where $\tilde\chi^0_1$ ($\chi^\pm_1$) denotes the lightest neutralino (chargino). Exclusion limits are placed in terms of the top-squark and neutralino masses. Assuming a branching ratio of 100% to $t \tilde\chi^0_1$, top-squark masses in the range 450--950 GeV are excluded for $\tilde\chi^0_1$ masses below 160 GeV. In the case where $m_{\tilde{t}_1}\sim m_t+m_{\tilde\chi^0_1}$, top-squark masses in the range 235--590 GeV are excluded.
Evaluating the Transferability of Machine-Learned Force Fields for Material Property Modeling
Creators: name: Mohanty, Shaswat
name: Yoo, Sanghyuk
name: Kang, Keonwook
name: Cai, Wei
Publisher: name: arXiv
Year: 2023
Subjects: subject: Machine Learning (cs.LG)
subject: Numerical Analysis (math.NA)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: Machine-learned force fields have generated significant interest in recent years as a tool for molecular dynamics (MD) simulations, with the aim of developing accurate and efficient models that can replace classical interatomic potentials. However, before these models can be confidently applied to materials simulations, they must be thoroughly tested and validated. The existing tests on the radial distribution function and mean-squared displacements are insufficient in assessing the transferability of these models. Here we present a more comprehensive set of benchmarking tests for evaluating the transferability of machine-learned force fields. We use a graph neural network (GNN)-based force field coupled with the OpenMM package to carry out MD simulations for Argon as a test case. Our tests include computational X-ray photon correlation spectroscopy (XPCS) signals, which capture the density fluctuation at various length scales in the liquid phase, as well as phonon density-of-state in the solid phase and the liquid-solid phase transition behavior. Our results show that the model can accurately capture the behavior of the solid phase only when the configurations from the solid phase are included in the training dataset. This underscores the importance of appropriately selecting the training data set when developing machine-learned force fields. The tests presented in this work provide a necessary foundation for the development and application of machine-learned force fields for materials simulations.
description: 27 pages, 14 figures, under review
PREVALENCE OF CHILDHOOD OVERWEIGHT, OBESITY AND ITS ASSOCIATED FACTORS IN ELEMENTARY SCHOOL CHILDREN IN DIRE DAWA TOWN, EASTERN ETHIOPIA 2016.
Creators: name: ASSEFA DESALEW
Publisher: name: Zenodo
Year: 2016

description: Introduction: The double burden of malnutrition in developing countries is a challenge to people health. Childhood obesity is related to an increased risk of high blood pressure, diabetes, respiratory disease and orthopedic disorders during childhood as well as its adverse effects in adulthood. Obesity in children is increasing worldwide. More than 10 percent children 5 to 17 years of age is obese.

Objective: The overall purpose of this study was to determine the prevalence of childhood overweight, obesity and its associated factors in elementary school children of Dire Dawa town Eastern Ethiopia.

Methods: The study was conducted in Dire Dawa town of Eastern Ethiopia from March 1st to 30th, 2016. School based cross-sectional study design was applied. Participants were selected by multistage sampling. Data was collected using pre-tested self-administered questionnaires, face to face interview and weight and height measurements through trained eight data collectors. Data were coded and entered in epi-data version 3.1 and exported and analyzed using SPSS version 21. Bivariate and multivariate logistic regression models were used to identify factors associated with childhood overweight and obesity. Statistical significance declared at p-value less than 0.05