cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Choosing a library housekeeping system: criteria for selection with specific reference to the system's functionality and user interface
Creators: name: Jonatan, Esterina M.
Publisher: name: Loughborough University
Year: 2021
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Choosing a library housekeeping system: criteria for selection with specific reference to the system's functionality and user interface
The Flattened, Rotating Molecular Gas Core of Protostellar Jet HH 212
Creators: name: Wiseman, Jennifer
name: Wootten, Alwyn
name: Zinnecker, Hans
name: McCaughrean, Mark
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recently discovered protostellar jet known as HH212 is beautifully symmetric, with a series of paired shock knots and bow shocks on either side of the exciting source region, IRAS 05413-0104 (Zinnecker et al. 1998). We present VLA ammonia maps of the IRAS 05413-0104 molecular gas envelope in which the protostellar jet source is embedded. We find that the envelope, with mass of 0.2 M(sun) detected by the interferometer, is flattened perpendicular to the jet axis with a FWHM diameter of 12000 AU and an axis ratio of 2:1, as seen in NH3 (1,1) emission. There is a velocity gradient of about 4-5 km sec^-1 pc^-1 across the flattened disk-like core, suggestive of rotation around an axis aligned with the jet. Flux-weighted mean velocities increase smoothly with radius with a roughly constant velocity gradient. In young (Class 0) systems such as HH212, a significant amount of material is still distributed in a large surrounding envelope, and thus the observable kinematics of the system may reflect the less centrally condensed, youthful state of the source and obscuration of central dynamics. The angular momentum of this envelope material may be released from infalling gas through rotation in the HH212 jet, as recent observations suggest (Davis et al. 2000). A blue-shifted wisp or bowl of emitting gas appears to be swept up along the blue side of the outflow, possibly lining the cavity of a wider angle wind around the more collimated shock jet axis. Our ammonia (2,2)/(1,1) ratio map indicates that this very cold core is heated to 14 Kelvin degrees in a centrally condensed area surrounding the jet source. This edge-on core and jet system appears to be young and deeply embedded. This environment, however, is apparently not disrupting the pristine symmetry and collimation of the jet.
description: 12 pages, including figures. Pages 11 and 12 are both Figure 2; Page 12 is a color version and the gradients in it do not print correctly on black-and-white printers. Thus ignore page 12 if printing or viewing in black-and-white
Zygosiphon Calman 1907
Creators: name: Haye, Pilar A.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Cumacea
Bodotriidae
Zygosiphon

description: ZYGOSIPHON CALMAN, 1907 A
 Type species: Zygosiphon mortenseni Calman, 1907a
 Body: Carapace shorter than abdomen and similar in length to peraeon; abdomen longer than carapace and peraeon together.
 Cephalothorax: From dorsal view the carapace appears laterally compressed in the medial portion. Carapace with mid-dorsal ridge. Pseudorostral lappets extend beyond frontal lobe; meet in midline or partially meet leaving a suture between them. Antennal notch as a subacute or acute incision. Anterolateral corner with subacute or acute tooth. Branchial siphons long, extending much beyond pseudorostrum and not fused in the midline. Frontal lobe 1/4–1/3 of carapace length; wider than long; with anterior margin notched; with ocular pigment and eye lenses.
Antenna 1 with basal article of the peduncle straight; as long as the other two articles together. Main flagellum bi-articulated; with two aesthetascs in distal-most article. Accessory flagellum uniarticulated. Antenna 2 in males reaching end of pleon; with sensory setae on anterior margin of article four. Antenna 2 in females with one article.
Maxilliped 3 basis geniculate; extended dorsodistally over ischium beyond the articulation of the ischium and merus. Ischium longer than merus. Merus extended dorso-distally over carpus. Carpus equal to or shorter than propodus and dactylus together.
 Peraeon: Peraeonite 2 may have ventrolateral expansion, and when present the expansion does not override other somites. Peraeonite 3 extended backwards overriding peraeonite 4. Peraeonite 4 with ventrolateral expansion overriding peraeonite 5.
Peraeopod 1 with basis arcuate; inner apical angle extended to form a convex process; carpus shorter than propodus. Peraeopod 2 with ischium; dactylus longer than propodus. Peraeopod 4 with ischium.
 Pleon: Articular pegs may be present. Pleonite 5 as long or longer than pleonite 6. Pleonite 6 longer than wide; shorter than peduncle of uropod. Wide portion of distal end of pleonite 6 well extended between the bases of the uropods; with rounded apex. Anal plates extend posteriorly beyond distal margin of pleonite 6.
Uropod endopod bi-articulated; proximal article longer than distal one. Uropod exopod with proximal article shorter than distal article. Peduncle of uropods longer than rami; exopod longer than endopod. Males with five pairs of pleopods.
 Species included:
 1. Z. mortenseni Calman, 1907a
 Distribution: Indo-West Pacific from 7 to 22 m.
description: Published as part of Haye, Pilar A., 2007, Systematics of the genera of Bodotriidae (Crustacea: Cumacea), pp. 1-58 in Zoological Journal of the Linnean Society 151 (1) on pages 22-23, DOI: 10.1111/j.1096-3642.2007.00322.x, http://zenodo.org/record/5428051
On the gauge fixing in the Hamiltonian analysis of general teleparallel theories
Creators: name: Blixt, Daniel
name: Hohmann, Manuel
name: Pfeifer, Christian
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences
subject: 83D05

description: The covariant formulation of teleparallel gravity theories must include the spin connection, which has 6 degrees of freedom. One can, however, always choose a gauge such that the spin connection is put to zero. In principle this gauge may affect counting of degrees of freedom in the Hamiltonian analysis. We show for general teleparallel theories of gravity, that fixing the gauge such that the spin connection vanishes in fact does not affect the counting of degrees of freedom. This manifests in the fact that the momenta of the Lorentz transformations which generate the spin connection are fully determined by the momenta of the tetrads.
description: 8 pages, no figures, Contribution to the proceedings of the conference "Teleparallel Universes" in Salamanca
Additional file 2: of Adipose tissue protects against sepsis-induced muscle weakness in mice: from lipolysis to ketones
Creators: name: Chloë Goossens
name: Weckx, Ruben
name: Derde, Sarah
name: Dufour, Thomas
name: Perre, Sarah Vander
name: Pauwels, Lies
name: Thiessen, Steven
name: Veldhoven, Paul Van
name: Berghe, Greet Van Den
name: Langouche, Lies
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Hematology
subject: 60506 Virology
subject: Computational Biology

description: Figure S2. Plasma insulin. Plasma insulin concentrations after 5 days of sepsis in (a) lean (Ln) and overweight/obese (Ob) mice and (b) in Ln mice receiving either standard mixed parenteral nutrition (PN), or a lipid-rich PN (Lipid). (a) Healthy control (Ctrl): Ln n = 17, Ob n = 15; d5 Sepsis: Ln n = 15, Ob n = 15. (b): Ln Ctrl n = 24; Ln Sepsis: PN n = 23, Lipid n = 23. Data are means ± SEM. p values determined through Wilcoxon or Student’s t test [Wilcoxon p values: (a) p = 0.1, (b) p = 0.01]. § p ≤ 0.05, §§ p ≤ 0.01, §§§ p ≤ 0.001 between Ctrl and Sepsis, * p ≤ 0.05, ** p ≤ 0.01, ***p ≤ 0.001 between sepsis groups. (DOCX 40 kb)
Additional file 1: of Adipose tissue protects against sepsis-induced muscle weakness in mice: from lipolysis to ketones
Creators: name: Chloë Goossens
name: Weckx, Ruben
name: Derde, Sarah
name: Dufour, Thomas
name: Perre, Sarah Vander
name: Pauwels, Lies
name: Thiessen, Steven
name: Veldhoven, Paul Van
name: Berghe, Greet Van Den
name: Langouche, Lies
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology
subject: Hematology
subject: Computational Biology

description: Figure S1. Plasma lipid profile and markers of fatty acid oxidation in lean and overweight/obese mice. The plasma lipid profile and gene expression markers of fatty acid oxidation were assessed in lean (Ln) and overweight/obese (Ob) mice after 1 (d1) or 5 days (d5) of sepsis. (a) Plasma free fatty acid (FFA), (b) triglyceride (TG), (c) LDL-cholesterol, and (d) HDL-cholesterol concentrations. (e) Relative mRNA expression of genes involved in fatty acid oxidation in the muscle. (f) Relative mRNA expression of genes involved in hepatic fatty acid oxidation. Gene expression data are normalized to Rn18s or Hprt and shown relative to the mean of Ln healthy controls (Ctrl). For all panels: d1 Ctrl: Ln n = 15, Ob n = 10; d1 Sepsis: Ln n = 15, Ob n = 15; d5 Ctrl: Ln n = 17, Ob n = 15; d5 Sepsis: Ln n = 15, Ob n = 15. Data are mean ± SEM. p values determined through Wilcoxon or Student’s t tests [Wilcoxon p values: (a) d1 p = 0.01, d5 p = 0.6, (b) d1 p = 0.5, d5 p = 0.5, (e) d1 Acadl p = 0.07, d1 Hadha p = 0.2, d5 Hadha p = 0.05, (f) d1 Ppara p = 0.7, d5 Ppara p
Higher‐order modular regulation of the human proteome
Creators: name: Kustatscher, Georg
name: Hödl, Martina
name: Rullmann, Edward
name: Grabowski, Piotr
name: Fiagbedzi, Emmanuel
name: Groth, Anja
name: Rappsilber, Juri
Publisher: name: Springer Science and Business Media LLC
Year: 2023
Subjects: subject: 500 Naturwissenschaften und Mathematik::570 Biowissenschaften; Biologie::570 Biowissenschaften; Biologie
subject: DNA replication
subject: machine-learning
subject: mRNA coexpression
subject: proteinco-regulation
subject: quantitative proteomics

description: Operons are transcriptional modules that allow bacteria to adapt to environmental changes by coordinately expressing the relevant set of genes. In humans, biological pathways and their regulation are more complex. If and how human cells coordinate the expression of entire biological processes is unclear. Here, we capture 31 higher‐order co‐regulation modules, which we term progulons, by help of supervised machine‐learning on proteomics data. Progulons consist of dozens to hundreds of proteins that together mediate core cellular functions. They are not restricted to physical interactions or co‐localisation. Progulon abundance changes are primarily controlled at the level of protein synthesis and degradation. Implemented as a web app at www.proteomehd.net/progulonFinder, our approach enables the targeted search for progulons of specific cellular processes. We use it to identify a DNA replication progulon and reveal multiple new replication factors, validated by extensive phenotyping of siRNA‐induced knockdowns. Progulons provide a new entry point into the molecular understanding of biological processes.
Challenges for Hybrid Water Electrolysis to Replace the Oxygen Evolution Reaction on an Industrial Scale
Creators: name: Kahlstorf, Till
name: Hausmann, J. Niklas
name: Sontheimer, Tobias
name: Menezes, Prashanth W.
Publisher: name: Wiley
Year: 2023
Subjects: subject: 500 Naturwissenschaften und Mathematik::540 Chemie::540 Chemie und zugeordnete Wissenschaften
subject: co-electrolysis
subject: electrooxidation of biomass
subject: hybrid water electrolysis
subject: hybrid water splitting
subject: industrial scale
subject: techno-economic analysis
subject: value-added organic oxidation reaction

description: To enable a future society based on sun and wind energy, transforming electricity into chemical energy in the form of fuels is crucial. This transformation can be achieved in an electrolyzer performing water splitting, where at the anode, water is oxidized to oxygen—oxygen evolution reaction (OER)—to produce protons and electrons that can be combined at the cathode to form hydrogen—hydrogen evolution reaction (HER). While hydrogen is a desired fuel, the obtained oxygen has no economic value. A techno‐economically more suitable alternative is hybrid water electrolysis, where value‐added oxidation reactions of abundant organic feedstocks replace the OER. However, tremendous challenges remain for the industrial‐scale application of hybrid water electrolysis. Herein, these challenges, including the higher kinetic overpotentials of organic oxidation reactions compared to the OER, the small feedstock availably and product demand of these processes compared to the HER (and carbon dioxide reduction), additional purifications costs, and electrocatalytic challenges to meet the industrially required activities, selectivities, and especially long‐term stabilities are critically discussed. It is anticipated that this perspective helps the academic research community to identify industrially relevant research questions concerning hybrid water electrolysis.
Quark-diquark equation of state and compact star structure
Creators: name: Lugones, G.
name: Horvath, J. E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) We construct quark-diquark equations of state using the quark mass density-dependent formalism. A region inside a $2-D$ parameter space in which this matter is absolutely stable is identified. Motivated by the reported compactness of some neutron star candidates we present stellar sequences and show that the quark-diquark EOSs allow a very compact structure, even in the cases in which the diquark itself is not bound.
description: 11 pages, 5 .eps figures. submitted to Int. Jour. Mod. Phys. D
Mimosaceae R.Brown 1814
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Fabales
Mimosaceae

description: Mimosaceae.
Acacia sieberiana DC.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Mesohelophorus Ponomarenko 1977
Creators: name: Fikáček, Martin
name: Prokin, Alexander
name: Angus, Robert B.
name: Pono, Alexander
name: Marenko
name: Yue, Yanli
name: Ren, Dong
name: Prokop, Jakub
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Helophoridae
Mesohelophorus

description: Subgenus † Mesohelophorus Ponomarenko, 1977 stat. nov.
 Mesohelophorus Ponomarenko, 1977b: 113.
 Type species. Mesohelophorus sibiricus Ponomarenko, 1977 (= H. palaeosibiricus nom. nov.) (by original designation).
 Time range. Early Cretaceous, Berriasian – Hauterivian, ca. 146–135 mya.
  Diagnosis. Adult:  Body rather wide; mentum ca. as wide as long; gula constricted, gular sutures joint at a point; maxillary palpomere 4 symmetrical; pronotum with three longitudinal furrows; pronotal intervals bearing very distinct granulation; pronotal flanks narrow; elytron with rather long scutellar stria; alternate elytral intervals not elevated or costate; epipleuron well-developed, wide anteriorly.
 By the rather wide body, strongly granulate pronotum, constricted gula and symmetrical maxillary palpomere 4, Mesohelophorus resembles the species of the modern subgenera Empleurus Hope, 1838, Transithelophorus Angus, 1970, Eutrichelophorus Sharp, 1915 and Kyphohelophorus Kuwert, 1886. It may be easily distinguished from them by the presence of only three pronotal furrows (five in the modern subgenera), elytra without elevated alternate intervals or tubercles (elevated in Empleurus, Transithelophorus and Eutrichelophorus, bearing tubercles in Kyphohelophorus) and wide elytral epipleura (extremely narrow in modern taxa). In addition, it differs from Empleurus by narrow pronotal flanks (very wide in Empleurus). Mesohelophorus also resembles the modern H. (Orphelophorus) arcticus Brown, 1937 by the reduced number of pronotal grooves and strong pronotal granulation, but may be easily distinguished from it by the rather long scutellar stria on the elytron (the scutellary stria is absent, or very rarely consists of one or two punctures only in H. arcticus).
 Taxonomic note. Due to the presence of all diagnostic characters of Helophorus, we downgrade Mesohelophorus to a subgenus of Helophorus which seems to be confined to the early Cretaceous only. Three species of Mesohelophorus have been described till now, of which only M. palaeosibiricus nom. nov. belongs to the subgenus. Mesohelophorus elongatus is synonymised with Helophorus (Mesosperchus) tarsalis above, and Mesohelophorus mongolicus Ponomarenko, 1986 is transferred to the Buprestoidea below.
description: Published as part of Fikáček, Martin, Prokin, Alexander, Angus, Robert B., Pono, Alexander, Marenko, Yue, Yanli, Ren, Dong & Prokop, Jakub, 2012, Revision of Mesozoic fossils of the helophorid lineage of the superfamily Hydrophiloidea (Coleoptera: Polyphaga), pp. 89-127 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 109, DOI: 10.5281/zenodo.5330604
Dark Halos: The Flattening of the Density Cusp by Dynamical Friction
Creators: name: El-Zant, Amr
name: Shlosman, Isaac
name: Hoffman, Yehuda
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: N-body simulations and analytical calculations of the gravitational collapse in an expanding universe predict that halos should form with a diverging inner density profile, the cusp. There are some observational indications that the dark matter distribution in galaxies might be characterized by a finite core. This `core catastrophe' has prompted a search for alternatives to the CDM cosmogony. It is shown here that the discrepancy between theory and observations can be very naturally resolved within the standard CDM model, provided that gas is not initially smoothly distributed in the dark matter halo, but rather is concentrated in clumps of mass $\geq 0.01 %$ the total mass of the system. Dynamical friction acting on these lumps moving in the background of the dark matter particles, dissipates the clumps orbital energy and deposits it in the dark matter. Using Monte-Carlo simulations, it is shown that the dynamical friction provides a strong enough drag, and that with realistic baryonic mass fractions, the available orbital energy of the clumps is sufficient to heat the halo and turn the primordial cusp into a finite, non-diverging core --- overcoming the competing effect of adiabatic contraction due to gravitational influence of the shrinking baryonic component. Depending on the initial conditions, the total density distribution may either become more or less centrally concentrated. Possible consequences of the proposed mechanism for other problems in the CDM model and for the formation and early evolution of the baryonic component of galaxies are also briefly discussed.
description: Version to appear in ApJ (with extra figure and extended discussion)
Rolling with quantum fields
Creators: name: Mukhopadhyay, Mainak
name: Vachaspati, Tanmay
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Other Condensed Matter (cond-mat.other)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the dynamics of a classical scalar field that rolls down a linear potential as it interacts bi-quadratically with a quantum field. We explicitly solve the dynamical problem by using the classical-quantum correspondence (CQC). Rolling solutions on the effective potential are shown to compare very poorly with the full solution. Spatially homogeneous initial conditions maintain their homogeneity and small inhomogeneities in the initial conditions do not grow.
description: 10 pages, 8 figures; updated references; published in PRD with title "Rolling classical scalar field in a linear potential coupled to a quantum field"
Additional file 8 of Identification of long noncoding RNAs reveals the effects of dinotefuran on the brain in Apis mellifera (Hymenopptera: Apidae)
Creators: name: Huang, Minjie
name: Dong, Jie
name: Guo, Haikun
name: Xiao, Minghui
name: Wang, Deqian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 8.
The Formation of Broad Emission Line Regions in Supernova-QSO Wind Interactions
Creators: name: Pittard, J. M.
name: Dyson, J. E.
name: Falle, S. A. E. G.
name: Hartquist, T. W.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that a cooled region of shocked supernova ejecta forms in a type II supernova-QSO wind interaction, and has a density, an ionization parameter, and a column density compatible with those inferred for the high ionization component of the broad emission line regions in QSOs. The calculations are based on the assumption that the ejecta flow is described initially by a similarity solution investigated by Chevalier (1982) and Nadyozhin (1985) and is spherically symmetric. Heating and cooling appropriate for gas irradiated by a nearby powerful continuum source is included in our model, together with reasonable assumptions for the properties of the QSO wind. The model results are also in agreement with observational correlations and imply reasonable supernova rates.
description: 13 pages, 7 figures, to be published in A&A
Chandra deep X-ray observation on the Galactic plane
Creators: name: Ebisawa, K.
name: Bamba, A.
name: Kaneda, H.
name: Maeda, Y.
name: Paizis, A.
name: Sato, G.
name: Yamauchi, S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Chandra ACIS-I instruments, we have carried out the deepest X-ray observation on a typical Galactic plane region at l 28.5 deg, where no discrete X-ray sources have been known previously. We have detected, as well as strong diffuse emission, 275 new point X-ray sources (4 sigma confidence) within two partially overlapping fields (~250 arcmin^2 in total) down to ~3 x 10^{-15} erg s^{-1} cm^{-2} (2 -- 10 keV) or ~ 7 x 10^{-16} erg s^{-1} cm^{-2} (0.5 -- 2 keV). We have studied spectral distribution of these point sources, and found that very soft sources detected only below ~ 3 keV are more numerous than hard sources detected only above ~ 3 keV. Only small number of sources are detected both in the soft and hard bands. Surface density of the hard sources is almost consistent with that at high Galactic regions, thus most of the hard sources are considered to be Active Galactic Nuclei seen through the milky way. On the other hand, some of the bright hard X-ray sources which show extremely flat spectra and iron line or edge features are considered to be Galactic, presumably quiescent dwarf novae. The soft sources show thermal spectra and small interstellar hydrogen column densities, and some of them exhibit X-ray flares. Therefore, most of the soft sources are probably X-ray active nearby late type stars.
description: Contribution to the proceedings of the "New Visions of the X-Ray Universe in the XMM-Newton and Chandra Era" symposium at ESTEC, The Netherlands. 26-30 Nov. 2001
MOESM1 of Diabetes mellitus and its associated factors among human immunodeficiency virus-infected patients on anti-retroviral therapy in Northeast Ethiopia
Creators: name: Temesgen Fiseha
name: Alemu Belete
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 1. Questioner used in the study.
Spin-exchange-induced exotic superfluids in a Bose-Fermi spinor mixture
Creators: name: Zhu, Chuanzhou
name: Chen, Li
name: Hu, Hui
name: Liu, Xia-Ji
name: Pu, Han
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider a mixture of spin-1/2 bosons and fermions, where only the bosons are subjected to the spin-orbit coupling induced by Raman beams. The fermions, although not directly coupled to the Raman lasers, acquire an effective spin-orbit coupling through the spin-exchange interaction between the two species. Our calculation shows that this is a promising way of obtaining spin-orbit coupled Fermi gas without Raman-induced heating, where the long-sought topological Fermi superfluids and topological bands can be realized. Conversely, we find that the presence of fermions not only provides a new way to create the supersolid stripe phase of the bosons, but more strikingly it can also greatly increase the spatial period of the bosonic density stripes, and hence makes this phase directly observable in the experiment. This system provides a new and practical platform to explore the physics of spin-orbit coupling, which possesses a dynamic nature through the interaction between the two species.
description: 6 pages, 3 figures, Published on PRA Rapid Communications, Comments are welcome
SDSS J124602.54+011318.8: A Highly Luminous Optical Transient at z=0.385
Creators: name: Berk, D. E. Vanden
name: Lee, B. C.
name: Wilhite, B. C.
name: Beacom, J. F.
name: Lamb, D. Q.
name: Annis, J.
name: Abazajian, K.
name: McKay, T. A.
name: Kron, R. G.
name: Kent, S.
name: Hurley, K.
name: Kehoe, R.
name: Wren, J.
name: Henden, A.
name: York, D. G.
name: Schneider, D. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a highly luminous optical transient (OT), SDSS J124602.54+011318.8, associated with a galaxy at a redshift of 0.385. In this paper we consider the possibility that the OT may be a GRB afterglow. Three sets of images and two sets of spectra were obtained as part of the normal operations of the Sloan Digital Sky Survey (SDSS). In the first two image sets, observed two nights apart, the object appears as a point source at $r^{*}\approx 17$. The third image set, observed about 410 days later, shows an extended source which is more than 2.5 magnitudes fainter. The spectra were observed about 400 and 670 days after the first two image sets, and both show an apparently normal galaxy at a redshift of 0.385. Associating the OT with the galaxy, the absolute magnitude was $M_{r^*}=-24.8$, which is over 4 magnitudes brighter than the most luminous supernova ever measured. The spectral energy distributions of the galaxy-subtracted OT derived from the first two image sets are well-fit by single power-laws with indices of $β_ν=-0.92$ and -1.29 respectively, similar to most GRB afterglows. Based upon the luminosity of the OT, non-detections in contemporaneous ROTSE-I images, and the change in spectral slope, the OT, if an afterglow, was likely discovered early during a ``plateau'' or slowly-fading phase. The discovery of a GRB afterglow at this stage of the SDSS is consistent with expectations, but only if the optical emission is much less strongly beamed than the gamma-rays. We emphasize that other explanations for the OT cannot be ruled out; a recent follow-up study by [galyam02] provides strong evidence that this source is in fact an unusual AGN.
description: Updated version to appear in ApJ
MOESM1 of SIMLIN: a bioinformatics tool for prediction of S-sulphenylation in theÂ human proteome based on multi-stage ensemble-learning models
Creators: name: Wang, Xiaochuan
name: Li, Chen
name: Li, Fuyi
name: Sharma, Varun
name: Song, Jiangning
name: Webb, Geoffrey
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Computational Biology

description: Additional file 1: Table S1. A detailed summary of the selected sequence and structural features using the MDL and mRMR feature selection methods. Table S2. The assigned weights of each node in the final neural network model.
Owner perceptions and management of the adverse behavioural effects of fireworks on companion animals: an update
Creators: name: MC Gates
name: S Zito
name: JK Walker
name: AR Dale
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Aims: To provide updated results on the adverse behavioural effects of fireworks on companion animals in New Zealand, measures that owners use to mitigate these effects, and opinions on a ban on the sale of fireworks. Method: A cross-sectional survey of companion animal owners in New Zealand was conducted between 2 November and 5 December 2016 using an online survey. The survey was modelled after a similar study conducted in 2006. Owners were asked to provide information on the types and severity of behaviours observed in their animals that were frightened by fireworks, what they did for their frightened animals and whether they would support a ban on the sale of fireworks. Results: There were 4,293 respondents who completed the online survey and they owned 15,871 companion animals, of which 11,750 (74.4%) were frightened of fireworks. For the 7,464 fearful animals with individual data available, the most commonly reported adverse behaviours were hiding (5,287; 70.8%), shivering (4,058; 54.3%) and cowering (3,324; 44.5%). Owners reported that 345 animals had been physically injured as the result of fireworks. Of 3,682 owners with frightened animals, 2,649 (71.9%) had not sought help or treatment for their animal. Frightened animals were mostly kept inside (3,479/7,464; 46.%) or comforted (2,112/7,464; 28.2%). Of all 4,325 respondents, 3,631 (84.0%) were supportive of a ban on the private sale of fireworks, with 370 (8.6%) against and 315 (7.3%) undecided. Owners with ≥1 animal that was fearful towards fireworks were more likely to support a ban (3,137/3,412; 91.9%) than owners whose animals were not afraid (466/561; 83.1%) (OR = 2.32; 95% CI = 1.80–2.98). Conclusion and Clinical Relevance: Among respondents to this survey, many owners of companion animals reported that their animals were adversely affected by fireworks, but few of them sought advice about strategies to mitigate the impacts. The majority of respondents supported a ban on the private sale of fireworks. Campaigns to raise public awareness of treatment strategies for managing fear behaviours during anticipated fireworks displays may be beneficial.
The cession of Sarawak to the British Crown in 1946
Creators: name: Reece, Bob H. W.
Publisher: name: The Australian National University
Year: 1977
Subjects: subject: British Malaysia Malaya
subject: Sarawak History

description: The cession of Sarawak by the third Rajah to the British Crown finally resolved the ambiguous position of a European-ruled Malay state which remained within the British imperial system for 100 years without being a formal part of it. External pressures, principally the Japanese invasion, had made direct British control both necessary and irresistible. The problem of the succession also helped to ensure that the Rajah’s agreement was not difficult to obtain. But it was already apparent in the 1930s that Brooke rule had come to the end of the road and could only look backwards. The Brooke administration’s failure to re-define native interests in the light of economic and social developments had removed the rationale upon which the Raj was avowedly based. The legitimization of cession was a grubby affair undertaken more for the benefit of British domestic opinion than the people of Sarawak. Nevertheless, it provided an issue which fostered the political development of Sarawak from a loose group of communities linked only by a common acceptance of the Rajah’s authority to a multi-racial state with its own nationalist tradition. Sarawak nationalism took the form of a movement to restore Brooke rule but it envisaged the establishment of an independent native state in which power would be shared between the Malays and the Ibans.
Kaon oscillations and baryon asymmetry of the universe
Creators: name: Tan, Wanpeng
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Baryon asymmetry of the universe (BAU) is naturally explained with $K^0-K^{0'}$ oscillations of a newly developed mirror-matter model and new understanding of quantum chromodynamics (QCD) phase transitions. A consistent picture for the origin of both BAU and dark matter is presented with the aid of $n-n'$ oscillations of the new model. The global symmetry breaking transitions in QCD are proposed to be staged depending on condensation temperatures of strange, charm, bottom, and top quarks in the early universe. The long-standing BAU puzzle can then be understood with $K^0-K^{0'}$ oscillations that occur at the stage of strange quark condensation and baryon number violation via a non-perturbative sphaleron-like (coined "quarkiton") process. Similar processes at charm, bottom, and top quark condensation stages are also discussed including an interesting idea for top quark condensation to break both the QCD global $U_t(1)_A$ symmetry and the electroweak gauge symmetry at the same time. Meanwhile, the $U(1)_A$ or strong CP problem of particle physics is simply solved under the same framework.
description: Phys. Rev. D accepted, See arXiv:1902.01837 for dark matter and n-lifetime, arXiv:1906.10262 for CKM and tests, arXiv:1902.03685 for application in stars, arXiv:1903.07474 for UHE cosmic rays, arXiv:1908.11838 for dark energy
Additional file 3 of Accurate long-read de novo assembly evaluation with Inspector
Creators: name: Chen, Yu
name: Zhang, Yixin
name: Wang, Amy Y.
name: Gao, Min
name: Chong, Zechen
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 3. Review history.
Live Reviews Information Document
Creators: name: PREreview
Publisher: name: Zenodo
Year: 2025
Subjects: preprint
preprintreview
livereview
prereview

description: Live Reviews are topic-centered, interactive preprint review sessions that are live-streamed via Zoom for open-access scientific manuscripts that have not yet been through editorial peer review. These events are designed to be inclusive by allowing structured and constructive discussions around preprints and encouraging diverse methods of participation. This document provides further information in a condensed, easy-to-share format.
A contest for postwar Malaya : social conflict, August 1945-March 1946
Creators: name: Cheah, Boon Kheng
Publisher: name: The Australian National University
Year: 1978
Subjects: subject: Chinese Malaysia
subject: Malaysia Race relations
subject: Malaysia History

description: The Japanese occupation dramatically altered Malaya’s prewar pattern of race relations and politics. Relations between Malays and Chinese, which previously had been civil , broke down and led lo the two races fighting one another. The Japanese occupation also gave certain political groups an opportunity to come to the forefront. Due to the growing strength of its resistance movement the Malayan Communist Party became a major political force. Japanese plans to grant Indonesia independence raised the hopes of the Kesatuan Melayu Muda to try to achieve its goal of Malay independence within Indonesia Raya (Creater.Indonesia). But the Japanese surrender once again dramatically altered the situation in Malaya. For nineteen days or more, depending on the location, neither the Japanese, the British, nor any Chinese or Malay oriented group could be said to control events. Instead, local resistance units, religious mystics, vengeful and fear-ridden citizens roamed the countryside, swept into the towns and took the law into their own hands. While the arrival of British troops may have brought outward order, the fabric of society had been rent, attitudes permanently altered. This study concentrates on the causes of wartime inter-racial conflicts between Malays and Chinese, the breakdown of authority during the post-surrender interregnum and the confrontation between the Malayan Communist Party, the Malay population and the British during the period of the British Military Administration.
Live Reviews Information Document
Creators: name: PREreview
Publisher: name: Zenodo
Year: 2023
Subjects: preprint
preprintreview
livereview
prereview

description: Live Reviews are topic-centered, interactive preprint review sessions that are live-streamed via Zoom for open-access scientific manuscripts that have not yet been through editorial peer review. These events are designed to be inclusive by allowing structured and constructive discussions around preprints and encouraging diverse methods of participation. This document provides further information in a condensed, easy-to-share format.
The [OII]3727 Luminosity Function of the Local Universe
Creators: name: Gallego, J.
name: Garcia-Dabo, C. E.
name: Zamorano, J.
name: Aragon--Salamanca, A.
name: Rego, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The measurement of the Star Formation Rate density of the Universe is of prime importance in understanding the formation and evolution of galaxies. The [OII]3727 emission line flux, easy to measure up to z~1.4 within deep redshift surveys in the optical and up to z~5.4 in the near infrared, offers a reliable means of characterizing the star formation properties of high-z objects. In order to provide the high-z studies with a local reference, we have measured total [OII]3727 fluxes for the well analyzed local sample of star-forming galaxies from the Universidad Complutense de Madrid Survey. This data is used to derive the [OII]3727 luminosity function for local star-forming galaxies. When compared with similar luminosity densities published for redshift up to z~1, the overall evolution already observed in the star formation activity of the Universe is confirmed.
description: 8 pages, 2 postscript figures, published in ApJL
Daughters of Sina : a study of gender, status and power in Western Samoa
Creators: name: Meleisea, Penelope Schoeffel
Publisher: name: The Australian National University
Year: 1979
Subjects: subject: Samoa Social conditions

description: The dyadic structure of Samoan society is based upon a concept of power comprising two complementary aspects; sacred and secular. These divisions operate as fundamental ordering principles in society. Power, in the sense of the ability to exert moral suasion and authority, is perceived as the combination of secular action and sacred legitimation. This duality derives from beliefs about the origin of society; that sacred power originated through matrilineal descent lines from the creater deity to dignify secular power, and is maintained through a predomiiifenly patrilineal mode of inheritance. Thus the focal dyad is the kinship of a sister and brother, and a number of other important dyadic relationships are metaphorically derived from it. The division of power into two aspects does not focus, symbolically or otherwise, upon male and female, but upon an opposition of qualities ascribed to particular statuses. Samoan females have two distinct statuses which are usually held similtaneously but exercised in different contexts. As sisters this status is sacred relative to the secular status of their brothers. -is wives their status is secular relative to the sacred status of their husband's descent group and is also derived from the status of their husband in that descent group. Similarly the designation of male statuses as sacred or secular is contextually defined, according to the rank and status of a title or descent group, and by categories of kinship with respect to a descent group on the basis of ancestral cross-sex siblingship. Since 1830, Christianity has eroded aspects of Samoan social structure and, together with the new «venues for acquiring wealth and prestige, has blurred many of the fundamental distinctions on which the complementarity of secular and secular power rest. Despite change and modification, the traditional concept of power is still reflected in kinship and village institutions. One of the most interesting manifestations of change and continuity is the introduction of village womens committees since the 1920s. These have adopted a tripartite structure which maintains distinctions between the wives of titled and untitled men, but more importantly, maintains the distinction between sisters and wives in the context of the local community. This distinction supports a complementarity between sacred and secular aspects of power, as exercised collectively by the two female status groups within a institutional framework. The persistance of patterns of belief, action and social institutions, even after the ancient religious ideology which justified them has been formally abandoned, is illustrated by the way in which an innovation such as the Western Samoan village womens committee has developed. This evidence has particularly significant implications for planned change and economic development in small-scale societies.
description: appendix pp.81-98
Caste and ritual in a Malwa village
Creators: name: Mathur, Kripa Shanker
Publisher: name: The Australian National University
Year: 1960

description: Caste is of fundamental importance to Hindus and to students of Hindu society and culture. Caste constitutes the basic element of Hindu social structure. It channelises, to a large extent, the activities, relations and incentives of the people. India is widely known as the classic land of castes, and the word "caste" is universally associated with India and her people. Even non-Hindus, it is said, have not scapted infection, and a number of scholars have drawn our attention to the fact that Muslims and Christians in India are divided into caste-like groups.
The politics of the Anti-Japanese United Front (1935-45) : Ch'en Shao-yü versus Mao Tse-tung
Creators: name: Shum, Kui-Kwong
Publisher: name: The Australian National University
Year: 1979
Subjects: subject: Mao, Zedong, 1893-1976
subject: Wang, Ming, 1904-1974
subject: Zhongguo gong chan dang History
subject: China History 1937-1945

description: In late 1934, the Chinese Communists were forced to evacuate the Kiangsi Soviet by the Nationalists' Fifth Encirclement Campaign. The defeat, as the Chinese Communists perceived, was not due to the failure of the land revolution in capturing the support of the peasant masses, but to their isolation from the bourgeois strata in the nation at large. Consequently, in the summer of 1935 Ch'en Shao-yli put forward the anti-imperialist united front tactics at the Seventh Comintern Congress, shifting the relative emphasis of the Party from the land revolution to the anti-imperialist struggle. The new tactics called for a relaxation of the struggle against rich peasants, small landlords and the national bourgeoisie, so as to facilitate the united front "from above" with other political groups and armies against Japan and Chiang Kai-shek. Ch'en's proposals were adopted by the CCP's Wayaopao Conference of December 1935. From 1936 onwards, both the Comintern and the CCP gradually realized the desirability of bringing Chiang Kai-shek into the alliance, and repeated overtures were made to Chiang. The CCP's peace efforts, however, obtained no results until the Sian Incident of December 1936. In the ensuing negotiation with the KMT, the CCP agreed to cease confiscating the landlords' land as a condition for the formation of the Anti-Japanese United Front. Following the outbreak of the Sino-Japanese War in July 1937, Conflicts developed between Ch'en Shao-yü and Mao over the proper strategies for the expansion of the Party. Ch'en's approach was based on Lenin's formula of the united front, which stressed the utilization of legal and democratic channels for the expansion of the Party's influence amongst the masses. Mao's strategy was premised on the construction of rural guerrilla bases under the protection of the united front. For a brief period, Ch'en's strategy gained notable successes but the KMT reacted by clamping down the CCP's mass organizations in Wuhan. At the Sixth Plenum of October 1938, Mao privately discredited Ch'en's approach as inappropriate for China. With the rapid deterioration in KMT-CCP relations and the changes in the international situation which demanded the CCP to rely exclusively on its own effort to sustain the Resistance, Mao’s rural strategy gained ascendancy in the Party. Nevertheless, Mao retained the united front policy for the purposes of forestalling full-scale Nationalist attack on the CCP and of securing the cooperation of the landlord-capitalist elites, so as to stabilize the Communist base areas and isolate the KMT. This dualistic approach remained the CCP’s policy even after the New Fourth Army Incident of 1941, and laid the foundation of the CCP’s ultimate victory which was based on the support of the lower masses as well as the national and petty bourgeoisie.