cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ozone Application in COVID-19 Triage Areas and Its Efficiency of Microbial Decontamination
Creators: name: De Souza, Hilária M.
name: Geovana D. Savi
name: Thauan Gomes
name: Cardoso, Willian A.
name: Maykon Cargnin
name: Angioletto, Elidio
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: This study aimed to conduct an ozone application within a triage area that receives patients with suspected cases of COVID-19. The ozone application was carried out for 10 min to disinfect the air and surfaces of different rooms within the triage area. A 3D model for ozone spread in the doctor’s office was developed. Higher counts of bacteria (3.3 × 102 CFU · m−3) and fungi (1.3 × 103 CFU · m−3) before ozone treatment were observed in the administrative room, which experienced greater circulation by healthcare workers. In this room, ozone was highly effective in reducing bacterial (95%; P P P
Nonperturbative Renormalization for Domain Wall Fermions and the Chiral Condensate
Creators: name: Yamaguchi, Azusa
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We study the chiral condensate, $$, and various quark bilinear vertex functions for domain wall fermions at different lattice scales, with both the Wilson and DBW2 gauge actions, in both quenched and dynamical fermion simulations. We use the vertex functions to calculate renormalization factors within a non-perturbative scheme.
description: 3 pages 4 figures: Lattice2003(chiral)
Microwave magnetoabsorption in R0.6Sr0.4MnO3 (R = Pr and Nd)
Creators: name: Chanda, A.
name: Chaudhuri, U.
name: Mahendiran, R.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report microwave magnetoabsorption (P) at room temperature in R0.6Sr0.4MnO3 (R = Pr and Nd) samples. P as a function of dc magnetic field (-2.5 kOe to +2.5 kOe) was measured for a broad frequency range (f = 0.1 - 4 GHz) of microwave magnetic field using a vector network analyzer and a copper strip coil which encloses one of the above samples. As the external dc magnetic field decreased from the maximum field, P initially increases and shows a maximum for a critical field and then decreases as the field approaches zero. The critical field increases with increasing frequency of the microwave signal. Line shape analysis of the obtained spectra suggests that the observed features in P are caused by ferromagnetic resonance (FMR) in R = Pr and electron paramagnetic resonance (ESR) in R = Nd samples, which were confirmed using a coplanar waveguide-based broadband magnetic resonance spectrometer.
description: 23 pages, 6 figures
Equivalence of Grandfather and Information Antinomy Under Intervention
Creators: name: Baumeler, Ämin
name: Tselentis, Eleftherios
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Causal loops, e.g., in time travel, come with two main problems. Most prominently, the grandfather antinomy describes the potentiality to inconsistencies: a problem of logical nature. The other problem is called information antinomy and is lesser known. Yet, it describes a variant of the former: There are not too few consistent solutions -- namely none -- but too many. At a first glance, the information antinomy does not seem as problematic as the grandfather antinomy, because there is no apparent logical contradiction. In this work we show that, however, both problems are equivalent under interventions: If parties can intervene in such a way that the information antinomy arises, then they can also intervene to generate a contradiction, and vice versa.
description: In Proceedings QPL 2020, arXiv:2109.01534
Tensor Network Rewriting Strategies for Satisfiability and Counting
Creators: name: de Beaudrap, Niel
name: Kissinger, Aleks
name: Meichanetzidis, Konstantinos
Publisher: name: arXiv
Year: 2020
Subjects: subject: Computational Complexity (cs.CC)
subject: Quantum Physics (quant-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We provide a graphical treatment of SAT and #SAT on equal footing. Instances of #SAT can be represented as tensor networks in a standard way. These tensor networks are interpreted by diagrams of the ZH-calculus: a system to reason about tensors over C in terms of diagrams built from simple generators, in which computation may be carried out by transformations of diagrams alone. In general, nodes of ZH diagrams take parameters over C which determine the tensor coefficients; for the standard representation of #SAT instances, the coefficients take the value 0 or 1. Then, by choosing the coefficients of a diagram to range over B, we represent the corresponding instance of SAT. Thus, by interpreting a diagram either over the boolean semiring or the complex numbers, we instantiate either the decision or counting version of the problem. We find that for classes known to be in P, such as 2SAT and #XORSAT, the existence of appropriate rewrite rules allows for efficient simplification of the diagram, producing the solution in polynomial time. In contrast, for classes known to be NP-complete, such as 3SAT, or #P-complete, such as #2SAT, the corresponding rewrite rules introduce hyperedges to the diagrams, in numbers which are not easily bounded above by a polynomial. This diagrammatic approach unifies the diagnosis of the complexity of CSPs and #CSPs and shows promise in aiding tensor network contraction-based algorithms.
description: In Proceedings QPL 2020, arXiv:2109.01534
A Multiwavelength study of NLS1s galaxies from the Second Byurakan Survey
Creators: name: Stepanian, J. A.
name: Benitez, E.
name: Krongold, Y.
name: Cruz-Gonzalez, I.
name: de Diego, J. A.
name: Chavushyan, V.
name: Mujica, R.
name: Dultzin-Hacyan, D.
name: Verdugo, T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this work we present a multiwavelength study of narrow-line Seyfert 1 galaxies (NLS1s) discovered in the Second Byurakan Survey (SBS). The sample consists of 26 objects, which have $M_{B}\ge -23.0$, or $-19.9 > M_{B} > -23.0$, $0.0243 < z < 0.317$ and $15.2 < B < 19.0$. For these objects, we present accurate coordinates, magnitudes, redshifts and the identification of optical objects with X-ray, IR and radio sources. Several galaxies are identified as X-ray or radio sources for the first time. We also report spectroscopic and photometric data, the spectral energy distribution, $α_{ox}$ indices and other data. Our study shows that SBS NLS1s are strong or moderately strong soft X-ray sources with $ \log L_{x}= 42.8-45.4$. Soft X-ray luminous sources in our sample do not tend to be luminous in the infrared. All SBS NLS1s are radio quiet objects ($ \log L_{R}<40.0$), and 52% of them are strong FeII emitters (FeII$\lambda4570/Hβ>1$). The traditional linear correlation $L_x$ and $L_{op}$, which seems to hold for AGN in general, is found for SBS NLS1s. An anticorrelation between FWHM of ${Hβ}$ and the ratio of FeII$\lambda4570/Hβ$ is also observed. A weak correlation is found between $α_{ox}$ slope and $L_{op}$. One of our main findings is that almost all SBS NLS1s may not have a FIR bump. Their SED suggest that they may also possess a BBB. The absence of IR bump in most of SBS NLS1s and the weakness of X-ray radiation in some of them, may argue against the presence of a BLR. The surface density of SBS NLS1s is $
description: 44 pages, 8 figures, published ApJ May 2003
Additional file 4 of A sense of place: transcriptomics identifies environmental signatures in Cabernet Sauvignon berry skins in the late stages of ripening
Creators: name: Cramer, Grant
name: Cochetel, Noé
name: Ghan, Ryan
name: Destrac-Irvine, Agnès
name: Delrot, Serge
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Computational Biology

description: Additional file 4. Image of the top 25 connected GO categories in the topGO network of the DEGs in Additional file 3.
Detrital zircon populations of the South Qiangtang terrane, central Tibetan Plateau, and their implications for Tethyan evolution
Creators: name: Xu, Wang
name: Zhang, Wen
name: Liu, Fulai
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Physical Sciences not elsewhere classified
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Detrital zircon populations of the South Qiangtang terrane (SQT) provide vital information for reconstructing the Tethyan evolution of the Tibetan Plateau but are obscured by the undefined affiliation of detrital zircon samples and the superimposition of multiple Tethyan tectonothermal events. We outlined the SQT based on geological mapping and collated Cambrian-Triassic detrital zircon samples to investigate representative detrital zircon populations. Although diachronous strata have distinctive detrital zircon age distributions, the Cambrian-Permian strata record similar ca. 2.50 Ga, 950 Ma, 800 Ma, and 550 Ma populations, which can be used in future detrital zircon studies as Palaeozoic indicators for the SQT. We analyse the above detrital zircon data and compare them to those from adjacent microcontinents (e.g. North Qiangtang terrane, NQT). We note that (1) the Cambrian-Late Ordovician detrital zircons from Upper Triassic strata yield positive εHf(t) values, suggesting juvenile arc-related magmatism in the NQT, and (2) the late Palaeozoic strata in the SQT and NQT both contain Late Devonian-early Carboniferous detrital zircons but have different detrital zircon populations. Together with previous studies on Tethyan evolution, we support that the southward subduction of the Proto-Tethys oceanic plate opened two diachronous back-arc basins between the NQT and SQT during the late Cambrian-Ordovician and Late Devonian-early Carboniferous. The former closed during the late Silurian; the latter evolved into the Palaeo-Tethys Ocean. Subsequently, the northward subduction of the Palaeo-Tethys oceanic plate produced early-middle Permian arc magmatism in the NQT, and the slab pull force from the subducting oceanic plate caused middle-late Permian intraplate magmatism on the opposite passive margin.
Feshbach resonances in $p$-wave three-body recombination within Fermi-Fermi mixtures of open-shell $^6$Li and closed-shell $^{173}$Yb atoms
Creators: name: Green, Alaina
name: Li, Hui
name: Toh, Jun Hui See
name: Tang, Xinxin
name: McCormick, Katherine
name: Li, Ming
name: Tiesinga, Eite
name: Kotochigova, Svetlana
name: Gupta, Subhadeep
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We report on observations and modeling of interspecies magnetic Feshbach resonances in dilute ultracold mixtures of open-shell alkali-metal $^6$Li and closed-shell $^{173}$Yb atoms with temperatures just above quantum degeneracy for both fermionic species. Resonances are located by detecting magnetic-field-dependent atom loss due to three-body recombination. We resolve closely-located resonances that originate from a weak separation-dependent hyperfine coupling between the electronic spin of $^6$Li and the nuclear spin of $^{173}$Yb, and confirm their magnetic field spacing by ab initio electronic-structure calculations. Through quantitative comparisons of theoretical atom-loss profiles and experimental data at various temperatures between 1 $μ$K and 20 $μ$K, we show that three-body recombination in fermionic mixtures has a $p$-wave Wigner threshold behavior leading to characteristic asymmetric loss profiles. Such resonances can be applied towards the formation of ultracold doublet ground-state molecules and quantum simulation of superfluid $p$-wave pairing.
description: 13 pages, 7 figures, 3 tables
Isotomiella barivierai Deharveng 1989
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Isotomiella
Isotomiella barivierai

description: Isotomiella barivierai Deharveng, 1989 **
Isotomiella barivierai Deharveng, 1989: 197.
DISTRIBUTION. — Lot. Saint-Jean-de-Laur, gouffredel’Ouleet Espagnac-Sainte-Eulalie, grottede Sainte-Eulalie (Deharveng 1989).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 358, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Complete mitogenome of Uca rosea and Uca paradussumieri, and their implications in evolution history of fiddler crab in Ocypodidae
Creators: name: Ting, Seng Yeat
name: Nyok-Sean Lau
name: Shu-Chien, Alexander Chong
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry

description: We determined the complete mitogenomes of two fiddler crabs Uca rosea (15,643 bp) and Uca paradussumieri (15,614 bp) of Ocypodidae within Brachyura. Both consist of 37 genes (13 protein-coding genes (PCGs), two ribosomal RNA genes, 22 transfer RNA genes and one control region). The mitogenomes composition of U. rosea and U. paradussumieri are highly A + T biased, 70.77% and 71.12%, respectively, and showed positive AT (0.03 and 0.02) and negative GC (−0.29 and −0.24) skews. Phylogenetic analysis showing all the fiddler crabs were under monophyletic group relationship and belong to Ocypodidae; U. rosea has a sister group relationship with U. paradussumieri.
QCD Functional Integrals for Systems with Nonzero Chemical Potential
Creators: name: Cohen, Thomas D.
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: This paper reviews some recent progress on QCD functional integrals at nonzero chemical potentials. One issue discussed is the use of QCD inequalities for this regime. In particular, the positivity of the integrand of particular Euclidean space functional integrals for two-flavor QCD with degenerate quark masses is used to demonstrate that the free energy per unit volume for QCD with a baryon chemical potential $μ_B$ (and zero isospin chemical potential) is necessarily greater than the free energy with isospin chemical potential $μ_I = \frac{2 μ_B}{N_c} $ (and zero baryon chemical potential). This result may be of use in model finite density systems. A corollary to this result is a rigorous {\it ab initio} bound on the nucleon mass. The second major issue addressed is the so-called ``Silver Blaze'' problem: the fact that at zero temperature and chemical potentials less than some critical value the free energy remains as that of the vacuum. This is puzzling in the context of a functional integral since a chemical potential affects the functional determinant of the Dirac operator and any nonzero $μ$ changes every eigenvalue of the Dirac operator compared to the $μ=0$ value. The isospin Silver Blaze problem is solved through the study of the spectrum of the operator $γ_0 (\dslash + m)$. The status of the baryon Silver Blaze problem is briefly discussed.
description: In memory of I. I. Kogan; to appear in the Iam Kogan Memorial volume
GLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy
Creators: name: Benjamin, Robert A.
name: Churchwell, E.
name: Babler, Brian L.
name: Bania, T. M.
name: Clemens, Dan P.
name: Cohen, Martin
name: Dickey, John M.
name: Indebetouw, Remy
name: Jackson, James M.
name: Kobulnicky, Henry A.
name: Lazarian, Alex
name: Marston, A. P.
name: Mathis, John S.
name: Meade, Marilyn R.
name: Seager, Sara
name: Stolovy, S. R.
name: Watson, C.
name: Whitney, Barbara A.
name: Wolff, Michael J.
name: Wolfire, Mark G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: GLIMPSE (Galactic Legacy Infrared Mid-Plane Survey Extraordinaire), a SIRTF Legacy Science Program, will be a fully sampled, confusion-limited infrared survey of the inner two-thirds of the Galactic disk with a pixel resolution of \~1.2" using the Infrared Array Camera (IRAC) at 3.6, 4.5, 5.8, and 8.0 microns. The survey will cover Galactic latitudes |b| <1 degree and longitudes |l|=10 to 65 degrees (both sides of the Galactic center). The survey area contains the outer ends of the Galactic bar, the Galactic molecular ring, and the inner spiral arms. The GLIMPSE team will process these data to produce a point source catalog, a point source data archive, and a set of mosaicked images. We summarize our observing strategy, give details of our data products, and summarize some of the principal science questions that will be addressed using GLIMPSE data. Up-to-date documentation, survey progress, and information on complementary datasets are available on the GLIMPSE web site: www.astro.wisc.edu/glimpse.
description: Description of GLIMPSE, a SIRTF Legacy project (Aug 2003 PASP, in press). Paper with full res.color figures at http://www.astro.wisc.edu/glimpse/glimpsepubs.html
Additional file 5 of Fluorescent amplification for next generation sequencing (FA-NGS) library preparation
Creators: name: Chiniquy, Jennifer
name: Garber, Megan
name: Aindrila Mukhopadhyay
name: Hillson, Nathan
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences

description: Additional file 5: Figure S5. Melting curve analysis of Nextera prepared plasmids: The melting curve plot (temperature vs. negative derivative of fluorescence (âˆ’dF/dT)) of every well from the Nextera library is plotted. From left to right, the plasmids tested are pXMJ19, pskb3-CopR1598, pGEN-292, pms6126
The ZX&-calculus: A complete graphical calculus for classical circuits using spiders
Creators: name: Comfort, Cole
Publisher: name: arXiv
Year: 2020
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Category Theory (math.CT)
subject: Quantum Physics (quant-ph)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We give a complete presentation for the fragment, ZX&, of the ZX-calculus generated by the Z and X spiders (corresponding to copying and addition) along with the not gate and the and gate. To prove completeness, we freely add a unit and counit to the category TOF generated by the Toffoli gate and ancillary bits, showing that this yields the full subcategory of finite ordinals and functions with objects powers of two; and then perform a two way translation between this category and ZX&. A translation to some extension of TOF, as opposed to some fragment of the ZX-calculus, is a natural choice because of the multiplicative nature of the Toffoli gate. To this end, we show that freely adding counits to the semi-Frobenius algebras of a discrete inverse category is the same as constructing the Cartesian completion. In particular, for a discrete inverse category, the category of classical channels, the Cartesian completion and adding counits all produce the same category. Therefore, applying these constructions to TOF produces the full subcategory of finite ordinals and partial maps with objects powers of two. By glueing together the free counit completion and the free unit completion, this yields "qubit multirelations."
description: In Proceedings QPL 2020, arXiv:2109.01534
Hubble Space Telescope Observations of UV Oscillations in WZ Sagittae During the Decline from Outburst
Creators: name: Welsh, W. F.
name: Sion, E. M.
name: Godon, P.
name: Gansicke, B. T.
name: Knigge, C.
name: Long, K. S.
name: Szkody, P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a time series analysis of Hubble Space Telescope observations of WZ Sge obtained in 2001 September, October, November and December as WZ Sge declined from its 2001 July superoutburst. Previous analysis of these data showed the temperature of the white dwarf decreased from ~29,000 K to ~18,000 K. In this study we binned the spectra over wavelength to yield ultraviolet light curves at each epoch that were then analyzed for the presence of the well-known 27.87 s and 28.96 s oscillations. We detect the 29 s periodicity at all four epochs, but the 28 s periodicity is absent. The origin of these oscillations has been debated since their discovery in the 1970s and competing hypotheses are based on either white dwarf non-radial g-mode pulsations or magnetically-channelled accretion onto a rotating white dwarf. By analogy with the ZZ Ceti stars, we argue that the non-radial g-mode pulsation model demands a strong dependence of pulse period on the white dwarf's temperature. However, these observations show the 29 s oscillation is independent of the white dwarf's temperature. Thus we reject the white dwarf non-radial g-mode pulsation hypothesis as the sole origin of the oscillations. It remains unclear if magnetically-funnelled accretion onto a rapidly rotating white dwarf (or belt on the white dwarf) is responsible for producing the oscillations. We also report the detection of a QPO with period ~18 s in the September light curve. The amplitudes of the 29 s oscillation and the QPO vary erratically on short timescales and are not correlated with the mean system brightness nor with each other.
description: 20 pages, 3 figures, 1 table; accepted for publication in ApJ
The Host Galaxy of GRB 031203: Implications of its low metallicity, low redshift, and starburst nature
Creators: name: Prochaska, Jason X.
name: Bloom, Joshua S.
name: Chen, Hsiao-Wen
name: Hurley, Kevin C.
name: Melbourne, Jason
name: Dressler, Alan
name: Graham, James R.
name: Osip, David J.
name: Vacca, W. D.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Keck/NIRSPEC near-IR images and Magellan/IMACS optical spectroscopy of the host galaxy of GRB 031203. The host is an actively star-forming galaxy at z=0.1055 +/- 0.0001. This is the lowest redshift GRB to-date, aside from GRB 980425. From the hydrogen Balmer lines, we infer an extinction of A_V = 3.62 +/- 0.25 or a total reddening E_T(B-V) = 1.17 +/- 0.1 toward the sightline to the nebular regions. After correcting for reddening, we perform an emission-line analysis and derive an ISM temperature of T=13400+/-2000K and electron density of n_e = 300 cm^(-3). These imply a metallicity [O/H]=-0.72+/-0.15 dex and a roughly solar abundance pattern for N, Ne, S, and Ar. Integrating Ha, we infer a dust-corrected star formation rate (SFR) of > 11 Msol/yr. These observations have the following implications: (1) the galaxy has a low K'-band luminosity L ~ L^*/5, typical of GRB host galaxies; (2) the low redshift indicates GRB 031203 had an isotropic-equivalent gamma-ray energy release smaller than all previous confirmed GRB events. The burst discovery raises the likelihood of identifying many additional low z, low flux events with Swift; (3) the large SFR, low metallicity, and the inferred hard radiation field is suggestive of massive star formation, supporting the collapsar model; (4) several lines of evidence argue against the identification of GRB 031203 as an X-ray flash event.
description: 8 pages, 3 figures. Uses emulateapj5.sty. Accepted to the Astrophysical Journal on April 20, 2004
Additional file 4 of Fluorescent amplification for next generation sequencing (FA-NGS) library preparation
Creators: name: Chiniquy, Jennifer
name: Garber, Megan
name: Aindrila Mukhopadhyay
name: Hillson, Nathan
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Additional file 4: Figure S4. Distributions of end RFU and transfer volumes of AL libraries: End RFU values (A) and transfer volumes (B) of AL libraries generated with 500 (blue), 250 (red), 125 (yellow), and 62.5 (green) pg of input AL DNA are represented in a histogram. For adjacent histograms, * represents distributions with p-value
Obscured star formation in the central region of the dwarf galaxy NGC5253
Creators: name: Alonso-Herrero, Almudena
name: Takagi, Toshinobu
name: Baker, Andrew J.
name: Rieke, George H.
name: Rieke, Marcia J.
name: Imanishi, Masatoshi
name: Scoville, Nick Z.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present HST/NICMOS observations (1.1-2.2micron) and 1.9-4.1micron spectroscopy of the central region of the dwarf galaxy NGC5253. The HST/NICMOS observations reveal the presence of a nuclear double star cluster separated by 0.3-0.4arcsec or 6-8pc (for a distance d=4.1Mpc). The double star cluster, also a bright double source of Pa-alpha emission, appears to be coincident with the double radio nebula detected at 1.3cm. The eastern near-infrared star cluster (C1) is identified with the youngest optical cluster, whereas the western star cluster (C2), although it is almost completely obscured in the optical, becomes the brightest star cluster in the central region of NGC 5253 at wavelengths longer than 2micron. Both clusters are extremely young with ages of approximately 3.5 million years old. C2 is more massive than C1 by a factor of 6 to 20 (M(C2)= 7.7 x 10^5 - 2.6 x 10^6Msun, for a Salpeter IMF in the mass range 0.1-100Msun). Analysis of the circumnuclear spectrum excluding C1 and C2, as well as of a number of other near-infrared selected clusters with a range of (young) ages, suggests that the star formation was triggered across the central regions of the galaxy. We have also modelled the nuclear UV to mid-infrared spectral energy distribution (SED) of NGC5253 and found that the infrared part is well modelled with a highly obscured (A_V= 17mag) young starburst with a stellar mass consistent with our photometric estimates for C1 and C2. The SED model predicts a moderately bright polycyclic aromatic hydrocarbon (PAH) feature at 3.3micron that is not detected in our nuclear L-band spectrum. NGC5253's low metallicity and a top-heavy IMF likely combine to suppress the 3.3micron PAH emission that is commonly seen in more massive starburst systems.
description: Accepted for publication in ApJ. High quality versions of Figures 1 and 2 are available upon request
Heron: RAS NAM 2019 Poster
Creators: name: Williams, Daniel
name: Gair, Jonathan
name: Heng, Ik Siong
name: Clark, James
name: Khamesra, Bhavesh
Publisher: name: Zenodo
Year: 2019
Subjects: gravitational waves
surrogate models
gaussian process

description: Poster presented at the UK National Astronomy Meeting 2019. Abstract: Most methods for extracting signals and parameter estimation for gravitational wave signals from compact binary coalescences require prior knowledge of the signal morphology. This prior information is obtained from numerical relativity simulations which are both expensive and time-consuming to produce. Consequently, only a small region of the overall signal parameter space has been probed. We present a method, based on Gaussian process regression informed by numerical relativity waveforms, which is capable of placing a prior probability distribution over the entire precessing binary black hole merger parameter space. This allows us to produce interpolated waveforms with an associated measure of the interpolation uncertainty across the entire parameter space.
Isotomiella paraminor Gisin 1942
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Isotomiella
Isotomiella paraminor

description: Isotomiella paraminor Gisin, 1942 *
Isotomiella paraminor Gisin, 1942: 294.
DISTRIBUTION. — Ariège. Cassagne etal. 2004; forêtde Bethmale (Cassagne et al. 2006). — Près du cirque Campuls, vallée de Bethmale (Luque etal. 2011).
Hautes-Pyrénées. Pyrénéescentrales (Cassagne etal. 2003, 2004).
ÉCOLOGIE. — Cassagne etal. 2003, 2004, 2006; Luque etal. 2011.
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 359, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
DNA barcoding of selected short-horned grasshoppers (Orthoptera: Acrididae) from Indian Himalayan region
Creators: name: Shantanu Kundu
name: Hirdesh Kumar
name: Kaomud Tyagi
name: Chandra, Kailash
name: Kumar, Vikas
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: In the context of Indian zoogeography, the DNA barcode data of short-horned grasshoppers (family Acrididae) are limited in global databases. Hence, the present study was aimed to collect selected Acridid species from the Indian Himalayan regions and generate DNA barcode data to enrich the global database. The estimated K2P genetic distances, Bayesian analysis (BA) topology and multiple species delimitation methods (ABGD, bPTP, and GMYC) clearly discriminate all the studied species. Based on high genetic distance (7.5%), multiple clades, and more than one molecular operational taxonomic unit, the present study elucidates the allopatric speciation and presence of possible cryptic diversity of Oxya japonica within India, China, and Russia. The present study suggests the collection of multiple specimens from different geographical locations and the generation of more DNA barcode data would facilitate the actual diversity of this insect group.
As Audiências Públicas como Instrumentos de Participação Social na Incorporação de Tecnologias em Saúde no SUS: Um Estudo Exploratório
Creators: name: Lopes, Sarah Gomes Pitta
name: Caetano, Rosangela
Publisher: name: Zenodo
Year: 2024
Subjects: portuguese

description: Objetivos:

Examinar a utilização da AP como espaço de participação social nos processos de gestão de tecnologias em saúde desenvolvidos pela Conitec, caracterizando-as em termos de sua distribuição temporal, objeto e quantidade e participantes inscritos e atuantes.
Diluted II-VI Oxide Semiconductors with Multiple Band Gaps
Creators: name: Yu, K. M.
name: Walukiewicz, W.
name: Wu, J.
name: Shan, W.
name: Beeman, J. W.
name: Scarpulla, M. A.
name: Dubon, O. D.
name: Becla, P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the realization of a new multi-band-gap semiconductor. The highly mismatched alloy Zn1-yMnyOxTe1-x has been synthesized using the combination of oxygen ion implantation and pulsed laser melting. Incorporation of small quantities of isovalent oxygen leads to the formation of a narrow, oxygen-derived band of extended states located within the band gap of the Zn1-yMnyTe host. When only 1.3% of Te atoms is replaced with oxygen in a Zn0.88Mn0.12Te crystal (with band gap of 2.32 eV) the resulting band structure consists of two direct band gaps with interband transitions at ~1.77 eV and 2.7 eV. This remarkable modification of the band structure is well described by the band anticrossing model in which the interactions between the oxygen-derived band and the conduction band are considered. With multiple band gaps that fall within the solar energy spectrum, Zn1-yMnyOxTe1-x is a material perfectly satisfying the conditions for single-junction photovoltaics with the potential for power conversion efficiencies surpassing 50%.
description: 12 pages, 4 figures
Observation of ferromagnetism above 900 K in Cr-GaN and Cr-AlN
Creators: name: Liu, H. X.
name: Wu, Stephen Y.
name: Singh, R. K.
name: Gu, Lin
name: Smith, David J.
name: Dilley, N. R.
name: Montes, L.
name: Simmonds, M. B.
name: Newman, N.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the observation of ferromagnetism at over 900K in Cr-GaN and Cr-AlN thin films. The saturation magnetization moments in our best films of Cr-GaN and Cr-AlN at low temperatures are 0.42 and 0.6 u_B/Cr atom, respectively, indicating that 14% and 20%, of the Cr atoms, respectively, are magnetically active. While Cr-AlN is highly resistive, Cr-GaN exhibits thermally activated conduction that follows the exponential law expected for variable range hopping between localized states. Hall measurements on a Cr-GaN sample indicate a mobility of 0.06 cm^2/V.s, which falls in the range characteristic of hopping conduction, and a free carrier density (1.4E20/cm^3), which is similar in magnitude to the measured magnetically-active Cr concentration (4.9E19/cm^3). A large negative magnetoresistance is attributed to scattering from loose spins associated with non-ferromagnetic impurities. The results indicate that ferromagnetism in Cr-GaN and Cr-AlN can be attributed to the double exchange mechanism as a result of hopping between near-midgap substitutional Cr impurity bands.
description: 14 pages, 4 figures, submitted to APL
Additional file 3 of Fluorescent amplification for next generation sequencing (FA-NGS) library preparation
Creators: name: Chiniquy, Jennifer
name: Garber, Megan
name: Aindrila Mukhopadhyay
name: Hillson, Nathan
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Additional file 3: Figure S3. MCA maxima correlates with input titration: Amount of input DNA is correlated with the local maxima of the MCA determined derivative RFU of the input titrations of both Nextera (A) and AL (B) library prepared samples, with R2 equal to 0.807 and 0.842 respectively
Telescopus dhara
Creators: name: Crochet, Pierre-André
name: Rasmussen, Jens B.
name: Wilms, Thomas
name: Geniez, Philippe
name: Trape, Jean-François
name: Böhme, Wolfgang
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Squamata
Colubridae
Telescopus
Telescopus dhara

description: Telescopus dhara (Forsskål, 1775)
 Coluber dhara, Forsskål, 1775, Descriptiones animalium, avium, amphibiorum, piscium, insectorum, vermium, quae in itinere Orientali observavit Petrus Forskal; post mortem auctoris edidit Carsten Niebuhr: adjuncta est materia medica Kahirina atque tabula Maris Rubris geographica: 14. Name-bearing type(s): one specimen described in Forsskål (1775), holotype by monotypy, lost. Type locality: “ Yemen ”, hence probably in present-day Yemen.
 Remarks on name-bearing type(s). According to Forsskål (1775), the description is based on a single specimen (“Unum tantum mihi videre licuit”) which is thus the holotype by monotypy. The type is lost: most of the material from Forsskål’s travel has been lost during the return journey; a few specimens (mostly dry fishes) are still kept in the Zoological Museum in Copenhagen but no snake (M. Andersen, pers. com.).
description: Published as part of Crochet, Pierre-André, Rasmussen, Jens B., Wilms, Thomas, Geniez, Philippe, Trape, Jean-François & Böhme, Wolfgang, 2008, Systematic status and correct nomen of the western North African cat snake: Telescopus tripolitanus (Werner, 1909) (Serpentes: Colubridae), with comments on the other taxa in the dhara-obtusus group, pp. 25-46 in Zootaxa 1703 (1) on page 37, DOI: 10.11646/zootaxa.1703.1.2, http://zenodo.org/record/5107364
The role of Fourier modes in extension theorems of Hartogs-Chirka type
Creators: name: Barrett, David E.
name: Bharali, Gautam
Publisher: name: arXiv
Year: 2004
Subjects: subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 32D15

description: We generalize Chirka's theorem on the extension of functions holomorphic in a neighbourhood of graph(F)\cup(\partial D\times D) -- where D is the open unit disc and graph(F) denotes the graph of a continuous D-valued function F -- to the bidisc. We extend holomorphic functions by applying the Kontinuitaetssatz to certain continuous families of analytic annuli, which is a procedure suited to configurations not covered by Chirka's theorem.
description: 17 pages
Splitting and focusing of neutrino collective states
Creators: name: Marklund, Mattias
name: Shukla, Padma K.
name: Stenflo, Lennart
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It is shown that the collective nonlinear interactions between intense neutrino or anti-neutrino fluxes and a dense neutrino plasma are governed by a multi-dimensional coupled cubic Schrödinger equation in which the interaction potential is positive or negative depending on the neutrino type. The cubic Schrödinger equation describes the splitting and focusing of intense neutrino beams due to the nonlinear excitations associated with the modifications of the individual neutrino energies in a dense neutrino background.
description: 5 pages, 2 figures (colour)
Participação e Características dos Medicamentos de Alto Custo no Contexto da Judicialização no Brasil: Uma Revisão de Escopo
Creators: name: Caetano, Rosangela
name: Osorio-de-Castro, Claudia Garcia Serpa
name: Mattos, Lívia
name: Krauze, Patrícia
name: Oliveira, Ione Ayala Gualandi de
Publisher: name: Zenodo
Year: 2024

description: Medicamentos são uma preocupação crescente dos gestores dos sistemas de saúde, porque seus custos representam um componente importante e em rápida elevação das despesas com cuidados de saúde.No Brasil, esse quadro tem sido agravado pela importante participação dos medicamentos nas demandas judiciais. Muito dessa judicialização de medicamentos tem por foco aqueles pertencentes ao Componente Especializado da Assistência Farmacêutica (CEAF), que inclui a maioria dos medicamentos de alto custo unitário ou agregado, dispensados conforme Protocolos Clínicos e Diretrizes Terapêuticas (PCDT). .Existe uma expressiva produção científica e acadêmica se propondo a descrever e analisar a judicialização em saúde e/ou a judicialização de medicamentos no país. Entretanto, seu enfoque principal não é especificamente sobre os medicamentos de alto custo (MAC), tornando-se importante conhecer essa demanda específica.

Objetivos:

Mapear perfil e representatividade da participação dos medicamentos de alto custo entre os medicamentos citados na produção científica e acadêmica nacional que versa sobre a judicialização em saúde, descrevendo suas principais características no período 2005 a 2022.
Nonlinear supersymmetry: from classical to quantum mechanics
Creators: name: Plyushchay, Mikhail
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantization of the nonlinear supersymmetry faces a problem of a quantum anomaly. For some classes of superpotentials, the integrals of motion admit the corrections guaranteeing the preservation of the nonlinear supersymmetry at the quantum level. With an example of the system realizing the nonlinear superconformal symmetry, we discuss the nature of such corrections and speculate on their possible general origin.
description: 11 pages
Additional file 2 of Fluorescent amplification for next generation sequencing (FA-NGS) library preparation
Creators: name: Chiniquy, Jennifer
name: Garber, Megan
name: Aindrila Mukhopadhyay
name: Hillson, Nathan
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Marine Biology

description: Additional file 2: Figure S2. Input titration of Nextera library prepared plasmid monitored with FA: DNA diluted 4-fold starting at 100â€‰pg per Nextera tagmentation reaction was amplified with SYBR green and monitored by continuous fluorescence (A), and melting curve analysis (B)
Telescopus gezirae Broadley 1994
Creators: name: Crochet, Pierre-André
name: Rasmussen, Jens B.
name: Wilms, Thomas
name: Geniez, Philippe
name: Trape, Jean-François
name: Böhme, Wolfgang
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Reptilia
Squamata
Colubridae
Telescopus
Telescopus gezirae

description: Telescopus gezirae Broadley, 1994
 Telescopus gezirae Broadley, 1994, Journal of African Zoology 108: 205. Name-bearing type(s): Natural History Museum of Zimbabwe NMZB 11807, holotype by original designation. Type locality: Blue Nile 30 km north of Sennar (Sudan).
 Diagnosis. Only two preserved specimens are currently known so morphological variation is still inadequately documented. Coloration in life unknown. A north-African species of Telescopus most similar to T. tripolitanus, sharing with that species a low number of supralabials (9) of which only two (4th and 5th) enter the eye and a low number of ventrals. Head broad, not as well separated from body as in dhara, obtusus or somalicus due to deeper body, short as in tripolitanus, with square snout; head pale, like pale ground colour of body, with uniform pileus and no dark longitudinal line along head side; supralabials pale with darker suffusion along upper edge; body grey-brown with 28 and 37 subrectangular dark brown dorsal blotches, plus 6–8 and 11 dark spots on tail, blotches widely separated (2–3 scale rows and 3–6 scale rows); flanks uniform, same colour as ground colour of dorsum; belly pale with dark blotches. Mid-body scale rows 21 in both specimens; ventral scales 195 and 207; subcaudal scales paired, 49 and 52 pairs; anal divided in the holotype; both specimens with 9 upper labials, of which two (4–5) touch the eye.
 Distribution. The species is currently known only from the Blue Nile valley in eastern central Sudan.
 Specimens examined. SUDAN: 85: BMNH 1927.8.18.2, Wad Medani (= Wad Madani) [14.40°N / 33.35°E], received from the Sudan Government Museum; 86: NMZB 11807, Blue Nile 30 km of Sennar [13.81°N / 33.54°E], collected by G. R. C. Van Someren in late 1966.
description: Published as part of Crochet, Pierre-André, Rasmussen, Jens B., Wilms, Thomas, Geniez, Philippe, Trape, Jean-François & Böhme, Wolfgang, 2008, Systematic status and correct nomen of the western North African cat snake: Telescopus tripolitanus (Werner, 1909) (Serpentes: Colubridae), with comments on the other taxa in the dhara-obtusus group, pp. 25-46 in Zootaxa 1703 (1) on page 41, DOI: 10.11646/zootaxa.1703.1.2, http://zenodo.org/record/5107364
The spinning-top Be star Achernar from VLTI-VINCI
Creators: name: de Souza, A. Domiciano
name: Kervella, P.
name: Jankov, S.
name: Abe, L.
name: Vakili, F.
name: di Folco, E.
name: Paresce, F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report here the first observations of a rapidly rotating Be star, $α$ Eridani, using Earth-rotation synthesis on the Very Large Telescope (VLT) Interferometer. Our measures correspond to a $2a/2b = 1.56\pm0.05$ apparent oblate star, $2a$ and $2b$ being the equivalent uniform disc angular diameters in the equatorial and polar direction. Considering the presence of a circumstellar envelope (CSE) we argue that our measurement corresponds to a truly distorted star since $α$ Eridani exhibited negligible H$α$ emission during the interferometric observations. In this framework we conclude that the commonly adopted Roche approximation (uniform rotation and centrally condensed mass) should not apply to $α$ Eridani. This result opens new perspectives to basic astrophysical problems, such as rotationally enhanced mass loss and internal angular momentum distribution. In addition to its intimate relation with magnetism and pulsation, rapid rotation thus provides a key to the Be phenomenon: one of the outstanding non-resolved problems in stellar physics.
description: 5 pages, 3 figures, Accepted for Publication in A&A Letter