cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
Creators: name: Guo, A. Q.
name: Wu, L. H.
name: Wang, L. L.
name: Mitchell, R. E.
name: Amoroso, A.
name: Ferroli, R. Baldini
name: Balossino, I.
name: Bertani, M.
name: Bettoni, D.
name: Bianchi, F.
name: Bortone, A.
name: Cibinetto, G.
name: Ramusino, A. Cotta
name: Cossio, F.
name: Dong, M. Y.
name: Rolo, M. Da Rocha
name: De Mori, F.
name: Destefanis, M.
name: Dong, J.
name: Evangelisti, F.
name: Farinelli, R.
name: Fava, L.
name: Felici, G.
name: Garzia, I.
name: Gatta, M.
name: Giraudo, G.
name: Gramigna, S.
name: Garbolino, S.
name: Greco, M.
name: Huang, Z.
name: Hou, Y. R.
name: Imoehl, W.
name: Lavezzi, L.
name: Lu, X. L.
name: Maggiora, M.
name: Melendi, F. M.
name: Malaguti, R.
name: Mangoni, A.
name: Marcello, S.
name: Melchiorri, M.
name: Mezzadri, G.
name: Ouyang, Q.
name: Pacetti, S.
name: Patteri, P.
name: Rivetti, A.
name: Shi, R. S.
name: Scodeggio, M.
name: Sosio, S.
name: Spataro, S.
name: Wang, B. L.
name: Wang, H. P.
name: Zhao, J. Y.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The Beijing Electron Spectrometer III (BESIII) is a multipurpose detector operating on the Beijing Electron Positron Collider II (BEPCII). After more than ten year's operation, the efficiency of the inner layers of the Main Drift Chamber (MDC) decreased significantly. To solve this issue, the BESIII collaboration is planning to replace the inner part of the MDC with three layers of Cylindrical triple Gas Electron Multipliers (CGEM). The transverse plane spatial resolution of CGEM is required to be 120 $μ$m or better. To meet this goal, a careful calibration of the detector is necessary to fully exploit the potential of the CGEM detector. In all the calibrations, the detector alignment plays an important role to improve the detector precision. The track-based alignment for the CGEM detector with the Millepede algorithm is implemented to reduce the uncertainties of the hit position measurement. Using the cosmic-ray data taken in 2020 with the two layers setup, the displacement and rotation of the outer layer with respect to the inner layer is determined by a simultaneous fit applied to more than 160000 tracks. A good alignment precision has been achieved that guarantees the design request could be satisfied in the future. A further alignment is going to be performed using the combined information of tracks from cosmic-ray and collisions after the CGEM is installed into the BESIII detector.
Phenacomys ungava Merriam 1889
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Phenacomys
Phenacomys ungava

description: Phenacomys ungava Merriam, 1889. N. Am. Fauna, 2:35. TYPE LOCALITY: Canada, Quebec Prov., Fort Chimo, near Ungava Bay. DISTRIBUTION: S Yukon across much of Canada to E Labrador; as far south as S Alberta, along the northern Great Lakes and St. Lawrence River. SYNONYMS: celatus, crassus, latimanus, mackenzii, soperi. COMMENTS: See remarks under P. intermedius and McAllister and Hoffmann (1988) on proper usage of ungava for this form.
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 533, DOI: 10.5281/zenodo.7353098
description: {"references": ["McAllister, J. A., and R. S. Hoffmann. 1988. Phenacomys intermedius. Mammalian Species, 305: 1 - 8."]}
$L^p$ $(p\geq 1)$ solutions of multidimensional BSDEs with monotone generators in general time intervals
Creators: name: Xiao, Lishun
name: Fan, Shengjun
name: Xu, Na
Publisher: name: arXiv
Year: 2013
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60H10

description: In this paper, we are interested in solving general time interval multidimensional backward stochastic differential equations in $L^p$ $(p\geq 1)$. We first study the existence and uniqueness for $L^p$ $(p>1)$ solutions by the method of convolution and weak convergence when the generator is monotonic in $y$ and Lipschitz continuous in $z$ both non-uniformly with respect to $t$. Then we obtain the existence and uniqueness for $L^1$ solutions with an additional assumption that the generator has a sublinear growth in $z$ non-uniformly with respect to $t$.
description: 23 pages
"slhaTab15.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2019

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 38
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
Creators: name: Damour, Thibault
name: Rettegno, Piero
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compare numerical relativity (NR) data on the scattering of equal-mass, non-spinning binary black holes to various analytical predictions based on post-Minkowskian (PM) results. While the usual sequence of PM-expanded scattering angles shows a rather poor convergence towards NR data, we find that a reformulation of PM information in terms of Effective-One-Body radial potentials leads to remarkable agreement with NR data, especially when using the radiation-reacted 4PM information. Using Firsov's inversion formula we directly extract, for the first time, from NR simulations a (radiation-reacted) gravitational potential describing the scattering of equal-mass, non-spinning binary black holes. We urge the NR community to compute more sequences of scattering simulations, so as to extend this knowledge to a wider region of parameter space.
description: 16 pages, 7 figures, 2 tables
Proedromys Thomas 1911
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Proedromys

description: Proedromys Thomas, 1911. Abstr. Proc. Zool. Soc. London, 1911 (90):4. TYPE SPECIES: Proedromys bedfordi Thomas, 1911. COMMENTS: Tribe Arvicolini. Ellerman and Morrison-Scott (1951) and Corbet (1978c) included this taxon in Microtus, but it is kept separate by Allen (1940), Wang et al. (1966), and Gromov and Polyakov (1977).
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 533, DOI: 10.5281/zenodo.7353098
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Wang Y. - C., Y. - C. Tu, and Wang Sung. 1966. Notes on some small mammals from Szechuan Province with description of a new subspecies. Acta Zootaxonomica Sinica, 3: 89 - 90 (in English and Chinese).", "Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian)."]}
Criteria and requirements for Incubator project (NFDI4Earth MS1.2.1)
Creators: name: Busch, Steffen
Publisher: name: NFDI4Earth Community on Zenodo
Year: 2024
Subjects: NFDI
NFDI4Earth
NFDI4Earth Milestone
NFDI4Earth Task Area 1
NFDI4Earth 2Participate
NFDI4Earth Incubator

description: This document outlines the expectations, the criteria, as well as the call and the review of incubator projects.
description: This work has been funded by the German Research Foundation (DFG) through the project NFDI4Earth (DFG project no.460036893, https://www.nfdi4earth.de/) within the German National Research Data Infrastructure (NFDI, https://www.nfdi.de/).
Flashlights: An Off-Caustic Lensed Star at Redshift $z$ = 1.26 in Abell 370
Creators: name: Meena, Ashish Kumar
name: Chen, Wenlei
name: Zitrin, Adi
name: Kelly, Patrick L.
name: Golubchik, Miriam
name: Zhou, Rui
name: Alfred, Amruth
name: Broadhurst, Tom
name: Diego, Jose M.
name: Oguri, Masamune
name: Williams, Liliya L. R.
name: Filippenko, Alexei V.
name: Li, Sung Kei
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report the discovery of a transient seen in a strongly lensed arc at redshift $z_{\rm s}=1.2567$ in \emph{Hubble Space Telescope} imaging of the Abell 370 galaxy cluster. The transient is detected at $29.51\pm0.14$ AB mag in a WFC3/UVIS F200LP difference image made using observations from two different epochs, obtained in the framework of the \emph{Flashlights} program, and is also visible in the F350LP band ($m_{\rm F350LP} \approx 30.53\pm0.76$ AB mag). The transient is observed on the negative-parity side of the critical curve at a distance of $\sim 0.6"$ from it, greater than previous examples of lensed stars. The large distance from the critical curve yields a significantly smaller macromagnification, but our simulations show that bright, O/B-type supergiants can reach sufficiently high magnifications to be seen at the observed position and magnitude. In addition, the observed transient image is a trailing image with an observer-frame time delay of $\sim+0.8$ days from its expected counterpart, so that any transient lasting for longer than that should have also been seen on the minima side and is thus excluded. This, together with the blue colour we measure for the transient ($m_{\rm F200LP} - m_{\rm F350LP} \approx [-0.3,-1.6]$ AB), rules out most other transient candidates such as (kilo)novae, for example, and makes a lensed star the prime candidate. Assuming the transient is indeed a lensed star as suggested, many more such events should be detected in the near future in cluster surveys with the \emph{Hubble Space Telescope} and \emph{James Webb Space Telescope}.
description: 9 pages. 5 figures. Accepted in MNRAS
"slhaTab16.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2019

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 39
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Algebra of the spinor invariants and the relativistic hydrogen atom
Creators: name: Eremko, A. A.
name: Brizhik, L. S.
name: Loktev, V. M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences
subject: 81Q05, 81Q37

description: It is shown that the Dirac equation with the Coulomb potential can be solved using the algebra of the three spinor invariants of the Dirac equation without the involvement of the methods of supersymmetric quantum mechanics. The Dirac Hamiltonian is invariant with respect to the rotation transformation, which indicates the dynamical (hidden) symmetry $ SU(2) $ of the Dirac equation. The total symmetry of the Dirac equation is the symmetry $ SO(3) \otimes SU(2) $. The generator of the $ SO(3) $ symmetry group is given by the total momentum operator, and the generator of $ SU(2) $ group is given by the rotation of the vector-states in the spinor space, determined by the Dirac, Johnson-Lippmann, and the new spinor invariants. It is shown that using algebraic approach to the Dirac problem allows one to calculate the eigenstates and eigenenergies of the relativistic hydrogen atom and reveals the fundamental role of the principal quantum number as an independent number, even though it is represented as the combination of other quantum numbers.
description: 16 pages, no figures
"slhaTab17.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2019

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 40
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Dark matter production through a non-thermal flavon portal
Creators: name: Cheek, Andrew
name: Osiński, Jacek K.
name: Roszkowski, Leszek
name: Trojanowski, Sebastian
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The Froggatt-Nielsen (FN) mechanism provides an attractive way of generating the determined fermion mass hierarchy and quark mixing matrix elements in the Standard Model (SM). Here we extend it by coupling the FN field, the flavon, to a dark sector containing one or more dark matter particles which are produced non-thermally sequentially through flavon production. Non-thermal flavon production occurs efficiently via freeze-in and through field oscillations. We explore this in the regime of high-scale breaking $Λ$ of the global $U(1)_{\textrm{FN}}$ group and at the reheating temperature $T_R\ll Λ$ where the flavon remains out of equilibrium at all times. We identify phenomenologically acceptable regions of $T_R$ and the flavon mass where the relic abundance of dark matter and other cosmological constraints are satisfied. In the case of one-component dark matter we find an effective upper limit on the FN charges at high $Λ$, i.e. $Q_{\rm FN}^{\rm DM}\leq13$. In the multi-component dark sector scenario the dark matter can be the heaviest dark particle that can be effectively stable at cosmological timescales, alternatively it can be produced sequentially by decays of the heavier ones. For scenarios where dark decays occur at intermediate timescales, i.e. $t\sim 0.1- 10^{28}\,{\rm s}$, we find that existing searches can effectively probe interesting regions of parameter space. These searches include indirect probes on decays such as $γ$-ray and neutrino telescopes as well as analyses of the Cosmic Microwave Background, as well as constraints on small scale structure formation from the Lyman-$α$ forest. We comment on the future prospects of such probes, place projected sensitivities, and discuss how this scenario could accommodate the cosmological $S_8$ tension.
description: 21 pages, 4 figures. Additional appendices and discussion. Matches published version
Studying a Chaotic Spiking Neural Model
Creators: name: Alhawarat, Mohammad
name: Nazih, Waleed
name: Eldesouki, Mohammad
Publisher: name: arXiv
Year: 2013
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Neural and Evolutionary Computing (cs.NE)
subject: FOS: Computer and information sciences

description: Dynamics of a chaotic spiking neuron model are being studied mathematically and experimentally. The Nonlinear Dynamic State neuron (NDS) is analysed to further understand the model and improve it. Chaos has many interesting properties such as sensitivity to initial conditions, space filling, control and synchronization. As suggested by biologists, these properties may be exploited and play vital role in carrying out computational tasks in human brain. The NDS model has some limitations; in thus paper the model is investigated to overcome some of these limitations in order to enhance the model. Therefore, the models parameters are tuned and the resulted dynamics are studied. Also, the discretization method of the model is considered. Moreover, a mathematical analysis is carried out to reveal the underlying dynamics of the model after tuning of its parameters. The results of the aforementioned methods revealed some facts regarding the NDS attractor and suggest the stabilization of a large number of unstable periodic orbits (UPOs) which might correspond to memories in phase space.
description: Journal, 13 pages
Supernova remnants: Types and evolution
Creators: name: Bamba, Aya
name: Williams, Brian J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Although only a small fraction of stars end their lives as supernovae, all supernovae leave behind a supernova remnant (SNR), an expanding shock wave that interacts with the surrounding medium, heating the gas and seeding the cosmos with elements forged in the progenitor In this chapter, we introduce the basic properties of galactic and extragalactic SNRs (Section 2). We summarize how SNRs evolve throughout their life cycles over the course of ~10^6 yrs (Section 3). We discuss the various morphological types of SNRs and discuss the emission processes at various wavelengths.(Section 4).
description: 13 pages, 8 figures, To appear in "Handbook of X-ray and Gamma-ray Astrophysics" by Springer - Editors in chief: C. Bambi and A. Santangelo
Tunneling current between graphene layers
Creators: name: Poklonski, Nikolai A.
name: Siahlo, Andrei I.
name: Vyrko, Sergey A.
name: Popov, Andrey M.
name: Lozovik, Yurii E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The physical model that allows to calculate the values of the tunneling current be-tween graphene layers is proposed. The tunneling current according to the pro-posed model is proportional to the area of tunneling transition. The calculated value of tunneling conductivity is in qualitative agreement with experimental data.
description: 4 pages
Companilactobacillus kimchiensis KIMCHIENSIS 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
Companilactobacillus
Companilactobacillus kimchiensis

description: DESCRIPTIONOF COMPANILACTOBACILLUS KIMCHIENSIS COMB. NOV.
Companilactobacillus kimchiensis (kim.chi.en’sis. N.L. gen. n. kimchiensis from kimchi, a Korean fermented-vegetable food).
Basonym: Lactobacillus kimchiensis Kim et al. 2013, 1358 VP.
Hexoses and disaccharides but not pentoses are fermented; growthis observed at 15–37 °C [133]. The genome size is 2.70 Mbp. The mol% G+C content of DNAis 35.5.
Isolatedfrom kimchi.
Thetypestrainis L133 T =DSM 24716 T =JCM 17702 T =KACC 15533 T.
Genome sequence accession number: JQCF00000000.
16S RNA gene sequence accession number: HQ906500.
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 2806, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Cosmicflows-2: The Data
Creators: name: Tully, R. Brent
name: Courtois, Helene M.
name: Dolphin, Andrew E.
name: Fisher, J. Richard
name: Heraudeau, Philippe
name: Jacobs, Bradley A.
name: Karachentsev, Igor D.
name: Makarov, Dmitry
name: Makarova, Lidia
name: Mitronova, Sofia
name: Rizzi, Luca
name: Shaya, Edward J.
name: Sorce, Jenny G.
name: Wu, Po-Feng
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cosmicflows-2 is a compilation of distances and peculiar velocities for over 8000 galaxies. Numerically the largest contributions come from the luminosity-linewidth correlation for spirals, the TFR, and the related Fundamental Plane relation for E/S0 systems, but over 1000 distances are contributed by methods that provide more accurate individual distances: Cepheid, Tip of the Red Giant Branch, Surface Brightness Fluctuation, SNIa, and several miscellaneous but accurate procedures. Our collaboration is making important contributions to two of these inputs: Tip of the Red Giant Branch and TFR. A large body of new distance material is presented. In addition, an effort is made to assure that all the contributions, our own and those from the literature, are on the same scale. Overall, the distances are found to be compatible with a Hubble Constant H_0 = 74.4 +-3.0 km/s/Mpc. The great interest going forward with this data set will be with velocity field studies. Cosmicflows-2 is characterized by a great density and high accuracy of distance measures locally, falling to sparse and coarse sampling extending to z=0.1.
description: To be published in Astronomical Journal. Two extensive tables to be available on-line. Table 1 available at http://edd.ifa.hawaii.edu select catalog `Cosmicflows-2 Distances'
title: Alte und neue Perspektivierungen auf die Arzneimittelforschung. Aus den Studien zur Praxis der Arzneimittelerprobung an Heimkindern und Anstaltsbewohner:innen von 1945 bis 1975
Creators: name: Hulverscheidt, Marion
Publisher: name: Universität Kassel
Year: 2024
Subjects: subject: 360
subject: Arzneimittelforschung
subject: Kind
subject: Heimkind
subject: Heimerziehung

description: Gefördert im Rahmen des Projekts DEAL
Generalized Lawson tori and Klein bottles
Creators: name: Penskoi, Alexei V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Differential Geometry (math.DG)
subject: Spectral Theory (math.SP)
subject: FOS: Mathematics
subject: 58E11, 58J50, 49Q05

description: Using Takahashi theorem we propose an approach to extend known families of minimal tori in spheres. As an example, the well-known two-parametric family of Lawson tau-surfaces including tori and Klein bottles is extended to a three-parametric family of tori and Klein bottles minimally immersed in spheres. Extremal spectral properties of the metrics on these surfaces are investigated. These metrics include i) both metrics extremal for the first non-trivial eigenvalue on the torus, i.e. the metric on the Clifford torus and the metric on the equilateral torus and ii) the metric maximal for the first non-trivial eigenvalue on the Klein bottle.
description: 17 pages, v.2: minor corrections
Proedromys bedfordi Thomas 1911
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Proedromys
Proedromys bedfordi

description: Proedromys bedfordi Thomas, 1911. Abstr. Proc. Zool. Soc. London, 1911(90):4. TYPE LOCALITY: China, Gansu (Kansu), 60 mi SE Minchow. DISTRIBUTION: Recorded from Gansu and Sichuan, China. COMMENTS: This is the only extant species in the genus. The Sichuan record is reported by Wang et al (1966). Pleistocene fragments from Shanxi, Hebei, and Shandong have been referred to P. cf. bedfordi (Zheng and Li, 1990).
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 533, DOI: 10.5281/zenodo.7353098
description: {"references": ["Wang Y. - C., Y. - C. Tu, and Wang Sung. 1966. Notes on some small mammals from Szechuan Province with description of a new subspecies. Acta Zootaxonomica Sinica, 3: 89 - 90 (in English and Chinese).", "Zheng, S., and Li Chuan-kwei. 1990. Comments on fossil arvicolids of China. Pp. 431 - 442, in International symposium evolution, phylogeny and biostratigraphy of arvicolids (Rodentia, Mammalia) (O. Fejfar and W. - D. Heinrich, eds.). Geological Survey, Prague, 448 pp."]}
Relativistic resistive magneto-hydrodynamics code for high-energy heavy-ion collisions
Creators: name: Nakamura, Kouki
name: Miyoshi, Takahiro
name: Nonaka, Chiho
name: Takahashi, Hiroyuki R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We construct a relativistic resistive magneto-hydrodynamic (RRMHD) numerical simulation code for high-energy heavy-ion collisions. We split the system of differential equations into two parts, a non-stiff and a stiff part. For the non-stiff part, we evaluate the numerical flux using HLL approximated Riemann solver and execute the time integration by the second-order of Runge-Kutta algorithm. For the stiff part, which appears in Ampere's law, we integrate the equations using semi-analytic solutions of the electric field. We employ the generalized Lagrange multiplier method to ensure the divergence-free constraint for the magnetic field and Gauss's law. We confirm that our code reproduces well the results of standard RRMHD tests in the Cartesian coordinates. In the Milne coordinates, the code with high conductivity is validated against relativistic ideal MHD tests. We also verify the semi-analytic solutions of the accelerating longitudinal expansion of relativistic resistive magneto-hydrodynamics in high-energy heavy-ion collisions in a comparison with our numerical result. Our numerical code reproduces these solutions.
description: 16 pages, 14 figures
GHRSST Data Discovery and Cataloguing Service : A federated access to all sea surface temperature data
Creators: name: Piollé, Jean-François
name: Armstrong, Edward M.
name: Briand, Dominque
Publisher: name: Zenodo
Year: 2023

description: This presentation was presented at the 2023 IGARSS Meeting held on July 19, 2023 in Pasadena, California. Ed Armstrong, GHRSST Science Team member, held this presentation during the "SST Applications and GHRSST" session (WE1.R16).
List decoding - random coding exponents and expurgated exponents
Creators: name: Merhav, Neri
Publisher: name: arXiv
Year: 2013
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: Some new results are derived concerning random coding error exponents and expurgated exponents for list decoding with a deterministic list size $L$. Two asymptotic regimes are considered, the fixed list-size regime, where $L$ is fixed independently of the block length $n$, and the exponential list-size, where $L$ grows exponentially with $n$. We first derive a general upper bound on the list-decoding average error probability, which is suitable for both regimes. This bound leads to more specific bounds in the two regimes. In the fixed list-size regime, the bound is related to known bounds and we establish its exponential tightness. In the exponential list-size regime, we establish the achievability of the well known sphere packing lower bound. Relations to guessing exponents are also provided. An immediate byproduct of our analysis in both regimes is the universality of the maximum mutual information (MMI) list decoder in the error exponent sense. Finally, we consider expurgated bounds at low rates, both using Gallager's approach and the Csiszár-Körner-Marton approach, which is, in general better (at least for $L=1$). The latter expurgated bound, which involves the notion of {\it multi-information}, is also modified to apply to continuous alphabet channels, and in particular, to the Gaussian memoryless channel, where the expression of the expurgated bound becomes quite explicit.
description: 28 pages; submitted to the IEEE Trans. on Information Theory
Cloud based EPC: A Design Approach
Creators: name: Mwangama, Joyce
name: Jarvis, Keagan
name: Ventura, Neco
Publisher: name: University of Cape Town
Year: 2024
Subjects: classificationCode: 400602
subject: Data communications

description: In this paper, we present a design of a cloud based Evolved Packet Core (EPC) utilizing Software Defined Networks (SDN) and Network Function Virtualisation (NFV) techniques. The ability of SDN to separate the control plane from the user plane such that it can then be moved onto a cloud based service is discussed as well as its relevance. The EPC is a Third Generation Partnership Project (3GPP) defined mobile aggregation network for the deployment of 4G and broadband services while also allowing for the interoperability of legacy technologies such as 3G. The decline in profitability of Mobile Network Operators (MNOs) is the driving force behind this research area and this design attempts to lower the Capital Expenditure (CAPEX) and Operating Expenditure (OPEX) involved in creating and managing such a Core infrastructure. The system is also designed to be highly flexible and scalable to cope with the increasing amounts of data that users are requesting from their MNOs.
Renormalized Perturbation Theory for Fast Evaluation of Feynman Diagrams on the Real Frequency Axis
Creators: name: Burke, M. D.
name: Grandadam, Maxence
name: LeBlanc, J. P. F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a method to accelerate the numerical evaluation of spatial integrals of Feynman diagrams when expressed on the real frequency axis. This can be realized through use of a renormalized perturbation expansion with a constant but complex renormalization shift. The complex shift acts as a regularization parameter for the numerical integration of otherwise sharp functions. This results in an exponential speed up of stochastic numerical integration at the expense of evaluating additional counter-term diagrams. We provide proof of concept calculations within a difficult limit of the half-filled 2D Hubbard model on a square lattice.
Prometheomys Satunin 1901
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Prometheomys

description: Prometheomys Satunin, 1901. Zool. Anz., 24:572. TYPE SPECIES: Prometheomys schaposchnikowi Satunin, 1901. COMMENTS: The only extant member of an archaic line of the arvicoline radiation, which most specialists isolate as the tribe Prometheomyini within Arvicolinae (Gromov and Polyakov, 1977; Hooper and Hart, 1962; Kretzoi, 1969; Pavlinov and Rossolimo, 1987; Zagorodnyuk, 1990). Repenning et al. (1990), however, aligned Prometheomys with another presumed relic, Ellobius, in the subfamily Prometheomyinae.
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 534, DOI: 10.5281/zenodo.7353098
description: {"references": ["Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian).", "Hooper, E. T., and B. S. Hart. 1962. A synopsis of Recent North American microtine rodents. Miscellaneous Publications, Museum of Zoology, University of Michigan, 120: 1 - 68.", "Kretzoi, M. 1969. Skizze einer Arvicoliden-Phylogenie. Vertebrata Hungarica (Budapest), 11: 155 - 193.", "Pavlinov, I. Ya., and O. L. Rossolimo. 1987. Sistematika mlekopitayushchikh SSSR [Systematics of the mammals of the USSR.]. Moscow University Press, Moscow, 282 pp. (in Russian).", "Zagorodnyuk, I. V. 1990. Kariotipicheskaya izmenchivost' i sistematika serykh polevok (Rodentia, Arvicolini). Soobshchenie 1. Vidovoi sostav i khromosomnye chisla [Karyotypic variability and systematics of the gray voles (Rodentia, Arvicolini). Communication 1. Species composition and chromosomal numbers]. Vestnik Zoologii, 2: 26 - 37 (in Russian).", "Repenning, C. A., O. Fejfar, and W. - D. Heinrich. 1990. Arvicolid rodent biochronology of the Northern Hemisphere. Pp. 385 - 417, in International symposium evolution, phylogeny and biostratigraphy of arvicolids (Rodentia, Mammalia) (O. Fejfar and W. - D. Heinrich, eds.). Geological Survey, Prague, 448 pp."]}
"slhaTab18.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2019

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 41
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
"slhaTab19.dat" of "Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb$^{-1}$ of $\sqrt{s}=13$ TeV $pp$ collision data with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2019

description: SLHA file listing the superpartner masses and decay channels for the signal scenario figured in Table 42
description: CERN-LHC. A search for strongly produced supersymmetric particles using signatures involving multiple energetic jets and either two isolated same-sign leptons (electrons or muons), or at least three isolated leptons, is presented. The analysis relies on b-tagged jets and missing transverse momentum, to achieve good sensitivity. A data sample of proton-proton collisions at $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider in 2015 and 2016, corresponding to a total integrated luminosity of 36.1 fb$^{-1}$, is used for the search. No significant excess over the Standard Model prediction is observed. The results are interpreted in several simplified supersymmetric models featuring R-parity conservation and R-parity violation, extending the exclusion limits from previous searches. In models considering gluino pair production, gluino masses are excluded up to 1.87 TeV at 95% confidence level. When bottom squarks are pair-produced and decay to a chargino and a top quark, models with bottom squark masses below 700 GeV and light neutralinos are excluded at 95% confidence level. In addition, model-independent limits are set on a possible contribution of new phenomena to the signal region yields.
Polarity Reversed Robust Carrier Mobility in Monolayer MoS2 Nanoribbons
Creators: name: Cai, Yongqing
name: Zhang, Gang
name: Zhang, Yong-Wei
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Using first-principles calculations and deformation potential theory, we investigate the intrinsic carrier mobility (μ) of monolayer MoS2 sheet and nanoribbons. In contrast to the dramatic three orders of magnitude of deterioration of μ in graphene upon forming nanoribbons, the magnitude of μ in armchair MoS2 nanoribbons is comparable to that in monolayer MoS2 sheet, albeit oscillating with width. Surprisingly, a room-temperature transport polarity reversal is observed with μ of hole (h) and electron (e) being 200.52 (h) and 72.16 (e) cm2V-1s-1 in sheet, and 49.72 (h) and 190.89 (e) cm2V-1s-1 in 4 nm-wide nanoribbon. The robust magnitudes of μ and polarity reversal are attributable to the different characteristics of edge states inherent in MoS2 nanoribbons. Our study suggests that width-reduction together with edge engineering provide a promising route for improving the transport properties of MoS2 nanostructures.
CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results
Creators: name: Bagley, Micaela B.
name: Finkelstein, Steven L.
name: Koekemoer, Anton M.
name: Ferguson, Henry C.
name: Haro, Pablo Arrabal
name: Dickinson, Mark
name: Kartaltepe, Jeyhan S.
name: Papovich, Casey
name: Pérez-González, Pablo G.
name: Pirzkal, Nor
name: Somerville, Rachel S.
name: Willmer, Christopher N. A.
name: Yang, Guang
name: Yung, L. Y. Aaron
name: Fontana, Adriano
name: Grazian, Andrea
name: Grogin, Norman A.
name: Hirschmann, Michaela
name: Kewley, Lisa J.
name: Kirkpatrick, Allison
name: Kocevski, Dale D.
name: Lotz, Jennifer M.
name: Medrano, Aubrey
name: Morales, Alexa M.
name: Pentericci, Laura
name: Ravindranath, Swara
name: Trump, Jonathan R.
name: Wilkins, Stephen M.
name: Calabrò, Antonello
name: Cooper, M. C.
name: Costantin, Luca
name: de la Vega, Alexander
name: Hutchison, Taylor A.
name: Lucas, Ray A.
name: McGrath, Elizabeth J.
name: Wang, Xin
name: Wuyts, Stijn
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations (Yang et al. in prep). We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known pre-launch issues such as 1/f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with pre-launch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated dataset in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public datasets released from the Directors Discretionary Early Release Science (DD-ERS) program.
description: 27 pages, 14 figures, submitted to ApJ. Accompanying CEERS public Data Release 0.5 available at ceers.github.io/releases.html
Prometheomys schaposchnikowi Satunin 1901
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Prometheomys
Prometheomys schaposchnikowi

description: Prometheomys schaposchnikowi Satunin, 1901. Zool. Anz., 24:572. TYPE LOCALITY: Georgia (Gruzinskaya), Caucasus Mtns, Gudaur, S of Krestovyi Pass, 6500 ft (as given by Ognev, 19636). DISTRIBUTION: Alpine zone of Caucasus Mtns, Georgia, and extreme NE Turkey. COMMENTS: Reviewed by Gromov and Polyakov (1977) and Corbet (1978c); cranial and dental morphology detailed by Hinton (1926); chromosomal data summarized by Zima and Krâl (1984a).
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 534, DOI: 10.5281/zenodo.7353098
description: {"references": ["Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian).", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Zima, J., and B. Kral. 1984 a. Karyotypes of European mammals. II. Acta Scientiarum Naturalium, Academiae Scientarium Bohemoslovacae (Brno), 18 (8): 1 - 62."]}
W40 region in the Gould Belt : An embedded cluster and H II region at the junction of filaments
Creators: name: Mallick, K. K.
name: Kumar, M. S. N.
name: Ojha, D. K.
name: Bachiller, Rafael
name: Samal, M. R.
name: Pirogov, L.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a multiwavelength study of W40 star-forming region using IR observations in UKIRT JHK bands, Spitzer IRAC bands & Herschel PACS bands; 2.12 micron H2 narrow-band imaging; & radio observations from GMRT (610 & 1280 MHz), in a FoV of ~34'x40'. Spitzer observations along with NIR observations are used to identify 1162 Class II/III & 40 Class I sources in the FoV. The NN stellar surface density analysis shows that majority of these YSOs constitute the embedded cluster centered on the source IRS1A South. Some YSOs, predominantly younger population, are distributed along & trace the filamentary structures at lower stellar surface density. The cluster radius is obtained as 0.44pc - matching well with the extent of radio emission - with a peak density of 650pc^-2. The JHK data is used to map the extinction which is subsequently used to compute the cloud mass. It has resulted in 126 Msun & 71 Msun for the central cluster & the northern IRS5 region, respectively. H2 narrow-band imaging displays significant emission, which prominently resembles fluorescent emission arising at the borders of dense regions. Radio analysis shows this region as having blister morphology, with the radio peak coinciding with a protostellar source. Free-free emission SED analysis is used to obtain physical parameters of the overall region & the IRS5 sub-region. This multiwavelength scenario is suggestive of star formation having resulted from merging of multiple filaments to form a hub. Star formation seems to have taken place in two successive epochs, with the first epoch traced by the central cluster & the high-mass star(s) - followed by a second epoch which is spreading into the filaments as uncovered by the Class I sources & even younger protostellar sources along the filaments. The IRS5 HII region displays indications of swept-up material which has possibly led to the formation of protostars.
description: 17 pages, 12 figures, 2 tables. Accepted for publication in The Astrophysical Journal