cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el
Creators: name: Krisciunas, Kevin
name: Suntzeff, Nicholas B.
name: Candia, Pablo
name: Arenas, Jose
name: Espinoza, Juan
name: Gonzalez, David
name: Gonzalez, Sergio
name: Hoeflich, Peter A.
name: Landolt, Arlo U.
name: Phillips, Mark M.
name: Pizarro, Sergio
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present well sampled optical (UBVRI) and infrared (JHK) light curves of the nearby (~18.0 Mpc) Type Ia supernova SN 2001el, from 11 days before to 142 days after the time of B-band maximum. The data represent one of the best sets of optical and infrared photometry ever obtained for a Type Ia supernova. Based on synthetic photometry using optical spectra of SN 2001el and optical and infrared spectra of SN 1999ee, we were able to devise filter corrections for the BVJHK photometry of SN 2001el which to some extent resolve systematic differences between SN 2001el datasets obtained with different telescope/filter/instrument combinations. We also calculated V minus infrared color curves on the basis of a delayed detonation model and showed that the theoretical color curves match the unreddened loci for Type Ia SNe with mid-range decline rates to within 0.2 mag. Given the completeness of the light curves and the elimination of filter-oriented systematic errors to some degree, the data presented here will be useful for the construction of photometric templates, especially in the infrared. On the whole the photometric behavior of SN 2001el was quite normal. The second H-band maximum being brighter than the first H-band maximum is in accord with the prediction of Krisciunas et al. (2000) for Type Ia SNe with mid-range decline rates. The photometry exhibits non-zero host extinction, with total A_V = 0.57 +/- 0.05 mag along the line of sight. NGC 1448, the host of SN 2001el, would be an excellent target for a distance determination using Cepheids.
description: 45 pages, 13 figures, accepted 14 October 2002 for publication in the January, 2003, issue of the Astronomical Journal, latest revision includes minor changes at page proof correction stage
title: Numerical Study on Vortex- Induced Vibration of Hexagonal Cylinders
Creators: name: Piran, Asghar
Publisher: name: Griffith University
Year: 2018
Subjects: subject: Vortex-induced vibration (VIV)
subject: Wind flow
subject: Computational fluid dynamics (CFD)
subject: Circular cylinder
subject: Hexagonal cylinders

description: Vortex-Induced Vibration (VIV) is a major concern in design of slender structures exposed to the wind flow, such as high-rise buildings and bridges, or water currents, such as offshore structures, marine risers, mooring elements and free spanning pipelines. Many researchers have investigated VIV of circular and rectangular crosssections. However, flow characteristics and VIV of hexagonal cylinders have received limited attention so far. Vortex-induced vibration of infinitely long hexagonal cylinders with corner and face orientations are investigated herein using two-dimensional Computational Fluid Dynamics (CFD). The numerical model is based on the solution of two-dimensional Reynolds-Averaged Navier–Stokes (RANS) equations in ANSYS Fluent. The RANS equations are solved in a moving mesh system using the Arbitrary- Lagrangian–Eulerian (ALE) approach, which allows the cylinder to move as a rigid body in the cross-flow direction. Turbulence is incorporated using the Shear Stress Transport (𝑆𝑆𝑇) 𝑘– 𝜔 model. The numerical model and results are validated against published experimental and numerical results on VIV of a circular cylinder for a Reynolds number (𝑅𝑒) of 1000. Using the validated model, VIV of hexagonal cylinders with corner and face oriented configurations are studied at reduced velocities (𝑉𝑟) between 2 and 12. In all models the non-dimensional mass ratio (𝑚∗) of 2, and 𝑅𝑒 of 1000 are adopted. Results are presented in the form of drag and lift forces, vortex shedding patterns, flow velocities, pressure distributions around the cylinders, frequency of vibrations, Strouhal numbers and amplitude of vibrations. Results show that, the cross-flow amplitudes of vibration of both corner and face-oriented hexagonal cylinders are much lower than that of a circular cylinder of the same diameter. The vortex shedding frequencies of the hexagonal cylinders are smaller than the circular cylinder.
Kinetic energy properties and weak equivalence principle in a space with GUP
Creators: name: Gnatenko, Kh. P.
name: Tkachuk, V. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A space with deformed commutation relations for coordinates and momenta leading to generalized uncertainty principle (GUP) is studied. We show that GUP causes great violation of the weak equivalence principle for macroscopic bodies, violation of additivity property of the kinetic energy, dependence of the kinetic energy on composition, great corrections to the kinetic energy of macroscopic bodies. We find that all these problems can be solved in the case of arbitrary deformation function depending on momentum if parameter of deformation is proportional inversely to squared mass.
Surrogate models for precessing binary black hole simulations with unequal masses
Creators: name: Varma, Vijay
name: Field, Scott E.
name: Scheel, Mark A.
name: Blackman, Jonathan
name: Gerosa, Davide
name: Stein, Leo C.
name: Kidder, Lawrence E.
name: Pfeiffer, Harald P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Only numerical relativity simulations can capture the full complexities of binary black hole mergers. These simulations, however, are prohibitively expensive for direct data analysis applications such as parameter estimation. We present two new fast and accurate surrogate models for the outputs of these simulations: the first model, NRSur7dq4, predicts the gravitational waveform and the second model, \RemnantModel, predicts the properties of the remnant black hole. These models extend previous 7-dimensional, non-eccentric precessing models to higher mass ratios, and have been trained against 1528 simulations with mass ratios $q\leq4$ and spin magnitudes $χ_1,χ_2 \leq 0.8$, with generic spin directions. The waveform model, NRSur7dq4, which begins about 20 orbits before merger, includes all $\ell \leq 4$ spin-weighted spherical harmonic modes, as well as the precession frame dynamics and spin evolution of the black holes. The final black hole model, \RemnantModel, models the mass, spin, and recoil kick velocity of the remnant black hole. In their training parameter range, both models are shown to be more accurate than existing models by at least an order of magnitude, with errors comparable to the estimated errors in the numerical relativity simulations. We also show that the surrogate models work well even when extrapolated outside their training parameter space range, up to mass ratios $q=6$.
description: Matches published version. Models publicly available at https://zenodo.org/record/3455886#.XZ9s1-dKjBI and https://pypi.org/project/surfinBH
MOESM6 of Microsporidian infections in the species complex Gammarus roeselii (Amphipoda) over its geographical range: evidence for both host–parasite co-diversification and recent host shifts
Creators: name: Quiles, Adrien
name: Bacela-Spychalska, Karolina
name: Teixeira, Maria
name: Lambin, Nicolas
name: Grabowski, Michal
name: Rigaud, Thierry
name: Wattier, Rémi
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology

description: Additional file 6: Data S3. Sequences under 200 bp for which no GenBank number can be attributed.
The X-ray afterglow of GRB 020322
Creators: name: Watson, D.
name: Reeves, J. N.
name: Osborne, J. P.
name: Tedds, J. A.
name: O'Brien, P. T.
name: Tomas, L.
name: Ehle, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The spectrum of the afterglow of GRB 020322 is the highest-quality X-ray spectrum of a GRB afterglow available to date. It was detected by XMM-Newton in an observation starting fifteen hours after the GRB with a mean 0.2--10.0 keV observed flux of 3.5+/-0.2x10^-13 erg cm^-2 s^-1, making it the brightest X-ray afterglow observed so far with XMM-Newton. The source faded; its lightcurve was well fit by a power-law with a decay index of 1.26+/-0.23. The spectrum is adequately fit with a power-law absorbed with neutral or ionised gas significantly in excess of the foreground Galactic column, at redshift 1.8_{-1.1}^{+1.0} or with low metal abundances. No spectral line or edge features are detected at high significance, in particular, a thermal emission model fits the data poorly, the upper limit on its contribution to the spectrum is 3.7x10^-14 erg cm^-2 s^-1, or at most ~10% of the total flux. No spectral variability is observed.
description: 5 pages, 3 figures, accepted for publication in A&A Letters
Oberea pagana HAROLD 1880
Creators: name: Adlbauer, K.
name: Ayalew, Amare
name: Beck, R.
name: Drumont, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Oberea
Oberea pagana

description: Oberea pagana HAROLD 1880
M a t e r i a l 7 Arba Minch, 1300-1500 m, 24.V.-4.VI.1999, 16.IV.-3.V.2001 und 21.- 30.X.2003, R. Beck leg.
V: Äthiopien, Kenya (ADLBAUER 2000a).
description: Published as part of Adlbauer, K., Ayalew, Amare, Beck, R. & Drumont, A., 2008, Cerambyciden aus Äthiopien (Coleoptera, Cerambycidae), pp. 1153-1191 in Linzer biologische Beiträge 40 (2) on page 1184, DOI: 10.5281/zenodo.5430603
Large-Scale Structure in the NIR-Selected MUNICS Survey
Creators: name: Botzler, C. S.
name: Snigula, J.
name: Bender, R.
name: Drory, N.
name: Feulner, G.
name: Hill, G. J.
name: Hopp, U.
name: Maraston, C.
name: de Oliveira, C. Mendes
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Munich Near-IR Cluster Survey (MUNICS) is a wide-area, medium-deep, photometric survey selected in the K' band. The project's main scientific aims are the identification of galaxy clusters up to redshifts of unity and the selection of a large sample of field early-type galaxies up to z < 1.5 for evolutionary studies. We created a Large Scale Structure catalog, using a new structure finding technique specialized for photometric datasets, that we developed on the basis of a friends-of-friends algorithm. We tested the plausibility of the resulting galaxy group and cluster catalog with the help of Color-Magnitude Diagrams (CMD), as well as a likelihood- and Voronoi-approach.
description: 4 pages, to appear in "The Evolution of Galaxies III. From Simple Approaches to Self-Consistent Models", proceedings of the 3rd EuroConference on the evolution of galaxies, held in Kiel, Germany, July 16-20, 2002
Chemistry and Dynamics in Pre-Protostellar Cores
Creators: name: Lee, Jeong-Eun
name: Evans, Neal J.
name: Shirley, Yancy L.
name: Tatematsu, Ken'ichi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have compared molecular line emission to dust continuum emission and modeled molecular lines using Monte Carlo simulations in order to study the depletion of molecules and the ionization fraction in three preprotostellar cores, L1512, L1544, and L1689B. L1512 is much less dense than L1544 and L1689B, which have similar density structures. L1689B has a different environment from those of L1512 and L1544. We used density and temperature profiles, calculated by modeling dust continuum emission in the submillimeter, for modeling molecular line profiles. In addition, we have used molecular line profiles and maps observed in several different molecules toward the three cores. We find a considerable diversity in chemical state among the three cores. The molecules include those sensitive to different timescales of chemical evolution such as CCS, the isotopes of CO and HCO+, DCO+, and N2H+. The CO molecule is significantly depleted in L1512 and L1544, but not in L1689B. CCS may be in the second enhancement of its abundance in L1512 and L1544 because of the significant depletion of CO molecules. N2H+ might already start to be depleted in L1512, but it traces very well the distribution of dust emission in L1544. On the other hand, L1689B may be so young that N2H+ has not reached its maximum yet. The ionization fraction has been calculated using H13CO+ and DCO+. This study suggests that chemical evolution depends on the absolute timescale during which a core stays in a given environment as well as its density structure.
description: 33 pages, 12 figures, accepted to ApJ
Additional file 2 of Plant super-barcode: a case study on genome-based identification for closely related species of Fritillaria
Creators: name: Wu, Lan
name: Wu, Mingli
name: Cui, Ning
name: Xiang, Li
name: Li, Ying
name: Li, Xiwen
name: Chen, Shilin
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Table S2. Specific primers used for validation in assembly.
Spelobia pseudonivalis
Creators: name: Roháček, Jindřich
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sphaeroceridae
Spelobia
Spelobia pseudonivalis

description: 7. Spelobia pseudonivalis (Dahl, 1909)
(Figs. 31–34)
 Material examined. 29 specimens (9 JJ 20 ♀♀, with 1 ♀ macropterous, 1 J 2 ♀♀ submacropterous, others brachypterous) from Germany, Czech Republic and Slovakia – localities listed by ROHÁČEK (1975a, 1980, 1983, 1999, 2009a) and ROHÁČEK et al. (2005).
 The species was originally described as brachypterous (for typical wing see Fig. 33). The first longer-winged specimens (Fig. 31) were recorded by ROHÁČEK (1980) and its wing polymorphism was discussed by ROHÁČEK (1983). Unfortunately, the relatively small number of specimens available for study makes it impossible to study the phenomenon in S. pseudonivalis more thoroughly. It seems to be of a similar type to Puncticorpus cribratum but perhaps without geographical dependence and with a much rarer (sub)macropterous form. Among the brachypterous specimens a mutant female with strongly reduced wing and venation (dm-cu lost) was found (Fig. 34) and recently a fully winged female was recorded from Poľana Mts. in Slovakia (ROHÁČEK 2009a). Except for Spelobia manicata, S. pseudonivalis is the only microcavernicolous wing polymorphic species in Europe. It lives in burrows of small mammals, particularly in nests of moles (ROHÁČEK 1983).
description: Published as part of Roháček, Jindřich, 2012, Wing polymorphism in European species of Sphaeroceridae (Diptera), pp. 535-558 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 548, DOI: 10.5281/zenodo.5332511
Resonant optical second harmonic generation in graphene-based heterostructures
Creators: name: Vandelli, M.
name: Katsnelson, M. I.
name: Stepanov, E. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: An optical Second-Harmonic Generation (SHG) allows to probe various structural and symmetry-related properties of materials, since it is sensitive to the inversion symmetry breaking in the system. Here, we investigate the SHG response from a single layer of graphene disposed on an insulating hexagonal Boron Nitride (hBN) and Silicon Carbide (SiC) substrates. The considered systems are described by a non-interacting tight-binding model with a mass term, which describes a non-equivalence of two sublattices of graphene when the latter is placed on a substrate. The resulting SHG signal linearly depends on the degree of the inversion symmetry breaking (value of the mass term) and reveals several resonances associated with the band gap, van Hove singularity, and band width. The difficulty in distinguishing between SHG signals coming from the considered heterostrusture and environment (insulating substrate) can be avoided applying a homogeneous magnetic field. The latter creates Landau levels in the energy spectrum and leads to multiple resonances in the SHG spectrum. Position of these resonances explicitly depends on the value of the mass term. We show that at energies below the band-gap of the substrate the SHG signal from the massive graphene becomes resonant at physically relevant values of the applied magnetic field, while the SHG response from the environment stays off-resonant.
Letter from Alice R. Appenzeller to William Elliot Griffis, April 24, 1913
Creators: name: Appenzeller, Alice R.
Publisher: name: No Publisher Supplied
Year: 1913

description: Updates on the Appenzeller family; Ida elected president of the Christian Association, Mary happy, Henry arranging trip to Bryn Mawr. Discusses Miss Merrill's stay with the family. Discusses her own life, schoolwork, a trip to Wellesley, and future family plans (go to Berlin).
PORA OLISH BERISHDA VOSITACHILIK QILISH JINOYTAI JAVOBGARLIGI YUZASIDAN XALQARO STANDARTLAR
Creators: name: Raxmatov, Rustambek
Publisher: name: Zenodo
Year: 2024

description: Korrupsiyaga oid jinoyatlar tahdidining kuchayishi poraxo'rlik uchun yangi, yuqori samarali jinoiy-huquqiy vositalarni izlash, har bir mamlakatda korrupsiyaga qarshi kurashning normativ-huquqiy va tashkiliy-amaliy mexanizmlarini yaratishga universal yondashuvlarni ishlab chiqish zarurligini taqozo etadi. Ushbu ilmiy maqolada xalqaro standartlar asosida poraxo'rlik, xususan, “Pora olish – berishda vositachilik” uchun maqbul jinoiy-huquqiy model va javobgarlikni takomillashtirish nuqtai nazaridan xalqaro standartlar qiyosiy huquqiy o'rganilgan.
Spin-dependent conductance statistics in systems with spin-orbit coupling
Creators: name: de Queiroz, S. L. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Spin-dependent partial conductances are evaluated in a tight-binding description of electron transport in the presence of spin-orbit (SO) couplings, using transfer-matrix methods. As the magnitude of SO interactions increases, the separation of spin-switching channels from non-spin-switching ones is gradually erased. Spin-polarised incident beams are produced by including a Zeeman-like term in the Hamiltonian. The exiting polarisation is shown to exhibit a maximum as a function of the intensity of SO couplings. For moderate site disorder, and both weak and strong SO interactions, no evidence is found for a decay of exiting polarisation against increasing system length. With very low site disorder and weak SO couplings a spin-filter effect takes place, as polarisation {\em increases} with increasing system length.
description: 7 pages, 8 figures (published version)
Terrilimosina corrivalis
Creators: name: Roháček, Jindřich
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sphaeroceridae
Terrilimosina
Terrilimosina corrivalis

description: 8. Terrilimosina corrivalis (Villeneuve, 1918)
(Figs. 35–37)
 Material examined. 80 specimens (44 JJ 36 ♀♀, with only l J macropterous, 2 JJ 2 ♀♀ submacropterous, others slightly to strongly brachypterous) from Czech Republic, Slovakia, Ukraine – localities listed by ROHÁČEK (1975c, 1983, 1984, 1994b, 1995) and ROHÁČEK & BARTÁK (2001) – all as Limosina or Terrilimosina sudetica and by ROHÁČEK (2001, 2009a). Additional localities: CZECH REPUBLIC: MORAVIA: Hrubý Jeseník Mts.– Velká kotlina glacial cirque (V. Kavalcová leg.). SLOVAKIA: Velká Fatra Mts. – Rakša res., Malá Fatra Mts. – Šútovská dolina, Nízke Tatry Mts. – Donovaly 3 km E, Vysoké Tatry Mts – Popradské pleso (J. Roháček leg.). ROMANIA: Banat, Sfânta Elena – Kulhavá skála rock, at Vranovec cave, sifting decayed leaves by stream, 1.vi.2008, 1 J (f. macroptera) (J. Roháček leg.).
 A rather poorly known species. Originally described as slightly to distinctly brachypterous (VILLENEUVE 1918; ROHÁČEK 1975c – under the synonymous name Limosina sudetica Roháček, 1975), later the submacropterous form was recorded (ROHÁČEK 1983, as T. sudetica) and recently more strongly brachypterous (Fig. 37) and almost fully winged specimens (Fig. 35) were found. Thus, its wing polymorphism with prevailing brachypterous form and continual transition to rare macropterous form seems to be similar to that of Spelobia pseudonivalis. Venal mutants seem to be rather rare in the brachypterous form of T. corrivalis – only two specimens (1J 1 ♀) with posterior cross-vein lost were found in the Hrubý Jeseník Mts. (Czech Republic). Terrilimosina corrivalis is a terricolous species associated with leaf-litter, moss and other decayed vegetation in mountain forests of Central Europe; hitherto it has only been recorded from Switzerland, Germany, Czech Republic, Slovakia, and Western Ukraine (ROHÁČEK et al. 2001). It is newly recorded from Romania (new southernmost distribution limit).
description: Published as part of Roháček, Jindřich, 2012, Wing polymorphism in European species of Sphaeroceridae (Diptera), pp. 535-558 in Acta Entomologica Musei Nationalis Pragae 52 (2) on pages 548-549, DOI: 10.5281/zenodo.5332511
The Imprint of the Cosmic Dark Ages on the Near Infrared Background
Creators: name: Salvaterra, R.
name: Ferrara, A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The redshifted light of the first (Pop III) stars might substantially contribute to the near infrared background (NIRB). By fitting recent data with models including up-to-date Pop III stellar spectra, we find that such stars can indeed account for the whole NIRB residual (i.e. after `normal' galaxy contribution subtraction) if the high redshift star formation efficiency is f = 10%-50%, depending on the IMF (the top-heaviest requiring lowest efficiency) and on the unknown galaxy contribution in the L band (our models, however, suggest it to be negligible). Such epoch of Pop III star formation ends in all models by z_end ~ 8.8, with a hard limit z_end < 9 set by J band observations. To prevent an associated IGM over-enrichment with heavy elements compared to observed levels in the IGM, pair-instability supernovae must be the dominant heavy element sources. Alternative explanations must break the light-metal production link by advocating very massive stars (M > 260 M_sun) locking their nucleosynthetic products in the compact remnant or by postulating an extremely inhomogeneous metal enrichment of the Ly alpha forest. We discuss these possibilities in detail along with the uncertainties related to the adopted zodiacal light model.
description: 11 pages, 7 figures, submitted to MNRAS
Kantorovich's Mass Transport Problem for Capacities
Creators: name: Gal, Sorin G.
name: Niculescu, Constantin P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics

description: The aim of the present paper is to extend Kantorovich's mass transport problem to the framework of upper/lower continuous capacities and to prove the cyclic monotonicity of the supports of optimal supermodular plans. As in the probabilistic case, this easily yields the corresponding extension of the Kantorovich duality.
description: This is the final version, as it is published in the journal. With respect to the previous version, on page 4 it was modified the definition of Choquet integral on a set A
The afterglow of GRB 021004: surfing on density waves
Creators: name: Lazzati, D.
name: Rossi, E.
name: Covino, S.
name: Ghisellini, G.
name: Malesani, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a model for the early optical afterglow of GRB 021004. This burst had one of the earliest detected optical afterglows, allowing a dense optical sampling. The lightcurve was peculiar, since bright bumps were superimposed to the regular power-law decay observed in many other events. We show that, given their time scale and shape, the bumps are due to the interaction of the fireball with moderate enhancements in the ambient medium density. The enhancements have a density contrast of order 10, modifying only slightly the dynamics of the fireball, which therefore surfs on them rather than colliding onto them. A relativistic reverse shock does not develop. Since the interaction takes place when the fireball is still hyper-relativistic it is not possible to understand if the overdensities are localized in clumps or are spherically symmetric around the GRB progenitor. The monotonic decrease of the contrast of successive rebrightenings suggests however the presence of clumps in an average uniform environment. Such an interpretation, complemented by the detection of several high velocity absorption systems in the optical spectrum, strongly suggests that GRB 021004 exploded within the remnant of a previous explosion.
description: 5 pages, 2 postscript figures, A&A reference added
Colomboniscus VANDEL 1972
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Colomboniscus

description: COLOMBONISCUS VANDEL, 1972
 Type species: Colomboniscus regressus Vandel, 1972 (by monotypy).
 Diagnosis
Endoantennal conglobation. Very small: maximum 3.5 mm. Integument smooth, with very fine and short ‘hairs’. Eye reduced, represented only by a spot of pigment without lens, or entirely absent. Cephalothorax rounded, without any rectangular corner. Pleotelson rounded, with straight sides. Flagellum of second antenna three-jointed, and very slender. All coxal plates simple. Noduli laterales small, on the hind margins of the tergites.
 Remark
Vandel (1972) defined this genus by its ‘numerous regressive traits’.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on page 22, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080
MOESM5 of Microsporidian infections in the species complex Gammarus roeselii (Amphipoda) over its geographical range: evidence for both host–parasite co-diversification and recent host shifts
Creators: name: Quiles, Adrien
name: Bacela-Spychalska, Karolina
name: Teixeira, Maria
name: Lambin, Nicolas
name: Grabowski, Michal
name: Rigaud, Thierry
name: Wattier, Rémi
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
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: Additional file 5: Data S2. Alignments based on SSU rDNA sequences, used for trees in Figs. 2, 3, 4, 5 and Additional file 1: Figure S1.
Delta hottentotum subsp. elegans
Creators: name: Dvo, L.
name: M, J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Delta
Delta hottentotum
Delta hottentotum elegans (de saussure 1852)

description: Delta hottentotum elegans (DE SAUSSURE 1852)
M a t e r i a l: Wadi Dahr, NW San'a', N=15°26’, E=44°08’, 2199 m, 5.10.2005, 2.
Recently reported from Yemen by WAHIS (2000) and GUSENLEITNER (2007).
description: Published as part of Dvo, L. & M, J., 2010, New records of vespid wasps from Yemen with synonymy in Belonogaster (Hymenoptera: Vespidae: Polistinae and Eumeninae), pp. 561-563 in Linzer biologische Beiträge 42 (1) on page 561, DOI: 10.5281/zenodo.5332555
title: Shedding Light on the Maelstrom of Atomic Images
Creators: name: Richter, Steffi
Publisher: name: Fachinformationsdienst (FID) Asien
Year: 2024
Subjects: subject: nuclear situation
subject: genbaku / genpatsu dichotomy
subject: nuclear village
subject: censorship Japan
subject: pikadon
subject: maruki gallery
subject: Hiroshima murals
subject: hibakusha
subject: Nuclear Power Plant Worker
subject: NPP Gipsy
subject: Japan
subject: Kollektives Gedächtnis
subject: Atombombenabwurf
subject: Kernenergie
subject: 952

description: Fissures: Nuclear Post-War Japan, p. 288
Delta dimidiatipenne
Creators: name: Dvo, L.
name: M, J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Delta
Delta dimidiatipenne

description: Delta dimidiatipenne (DE SAUSSURE 1852)
M a t e r i a l: Wadi Daw'an, NW Al Mukalla, N=15°09’, E=48°26’, 946 m, 3.4.2007, 1.
Recently reported from Yemen by GUSENLEITNER (2007).
description: Published as part of Dvo, L. & M, J., 2010, New records of vespid wasps from Yemen with synonymy in Belonogaster (Hymenoptera: Vespidae: Polistinae and Eumeninae), pp. 561-563 in Linzer biologische Beiträge 42 (1) on page 562, DOI: 10.5281/zenodo.5332555
SySTEM 2020 Impact Assessment Report
Creators: name: Perry, Sophie
name: Hurley, Mairéad
Publisher: name: Zenodo
Year: 2021
Subjects: Science Education
STEM
STEAM
Non-formal education
Impact

description: The SySTEM 2020 project has researched science learning outside the classroom in 19 countries across Europe and Isreal. The project explores the ways in which science learning, attitudes and aptitudes, are influenced by learners’ physical, emotional, social and cultural contexts. Across research and practice, SySTEM 2020 explores equity in relation to science learning, which is considered crucial in exploring who is able to engage with science, how and why. This report summarises the findings of the project and aims to assess their impact on learners, non-formal science learning organisations, and the wider science learning community.
The radial velocities and physical parameters of HD 553
Creators: name: Duemmler, R.
name: Iliev, I. Kh.
name: Iliev, L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: HD 553 was discovered as an eclipsing binary by Hipparcos. Here, we present the first radial velocity curve for this system. It is found that HD 553 is a double-lined spectroscopic binary. Despite the large luminosity difference, the two components of the system are of very simmilar mass. The primary, a K0-giant, fills a large fraction of its Roche-lobe. The secondary is, despite its very similar mass, still a late-type dwarf. The radial velocity curve allows to constrain several stellar and system parameters.
description: 6 pages, 3 Postscript figures, accepted in Astronomy and Astrophysics
Parsec Scale Properties of Radio Sources
Creators: name: Giovannini, G.
name: Giroletti, M.
name: Taylor, G. B.
name: Cotton, W. D.
name: Lara, L.
name: Venturi, T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new complete sample of radio sources selected from the B2 and 3CR catalogues, with no bias respect to the jet velocity and orientation. Using preliminary data we investigate the parsec scale properties of radio sources with different radio power and kpc scale morphology. We stress the evidence for high velocity pc scale jets in all sources and conclude that the properties of parsec scale jets are similar regardless of the source total power and large scale morphology. Moreover we show two epoch images of two nearby radio galaxies: a low power compact source and a CSO. The comparison of the two epoch images suggests that in both sources the size is increasing with time. We derive a possible advance speed and estimate their dynamic age.
description: 4 pages, 5 figures. Contributed paper to the 6th European VLBI Network Symposium held on June 25th-28th in Bonn (D)
The Life Cycle of the Central Molecular Zone. I: Inflow, Star Formation, and Winds
Creators: name: Armillotta, L.
name: Krumholz, M. R.
name: Di Teodoro, E. M.
name: McClure-Griffiths, N. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of the gas cycle and star formation history in the central 500 pc of the Milky Way, known as Central Molecular Zone (CMZ). Through hydrodynamical simulations of the inner 4.5 kpc of our Galaxy, we follow the gas cycle in a completely self-consistent way, starting from gas radial inflow due to the Galactic bar, the channelling of this gas into a dense, star-forming ring/stream at ~ 200 - 300 pc from the Galactic centre, and the launching of galactic outflows powered by stellar feedback. We find that star formation activity in the CMZ goes through oscillatory burst/quench cycles, with a period of tens to hundreds of Myr, characterised by roughly constant gas mass but order-of-magnitude level variations in the star formation rate. Comparison with the observed present-day star formation rate of the CMZ suggests that we are currently near a minimum of this cycle. Stellar feedback drives a mainly two-phase wind off the Galactic disc. The warm phase dominates the mass flux, and carries 100 - 200 % of the gas mass converted into stars. However, most of this gas goes into a fountain and falls back onto the disc rather than escaping the Galaxy. The hot phase carries most of the energy, with a time-averaged energy outflow rate of 10 - 20 % of the supernova energy budget.
description: 20 pages, 15 figures, accepted for publication in MNRAS
Brief Study on Application of New Indoor Lawn in Northern Areas of China
Creators: name: LUO, Yinghua
name: QU, Shanmin
name: LIU, Xiangping
name: JIN, Chenghao
name: LUO, Yinghua
name: QU, Shanmin
name: LIU, Xiangping
name: JIN, Chenghao
Publisher: name: Unknown
Year: 2019
Subjects: subject: Agribusiness
subject: Northern areas of China, Indoor lawn, Environmental protection

description: At present, the development and function research of lawn has become diversified, and the application of lawn has been extended from outdoor to indoor environment. The indoor lawn has functions of absorbing toxic and harmful gases, releasing oxygen, increasing air humidity and regulating temperature. It can effectively improve the indoor air quality of northern areas, purify and beautify the home environment. This paper elaborated the purpose and significance of the application of new indoor lawn, the establishment methods of the indoor lawn, and the application design of the indoor lawn landscape.
Additional file 1: of Long-term outcome after mitral valve replacement using biological versus mechanical valves
Creators: name: Ayse Cetinkaya
name: Poggenpohl, Julia
name: Bramlage, Karin
name: Hein, Stefan
name: Doss, Mirko
name: Bramlage, Peter
name: Schรถnburg, Markus
name: Richter, Manfred
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified

description: Table S1. Major complications (embolism/stroke and bleeding) and their localisation. Legend: Values are patients applicable/patients with available information with the percentage in brackets. MI, myocardial infarction. (DOCX 12 kb)
The Cool ISM in S0 Galaxies. I. A Survey of Molecular Gas
Creators: name: Welch, Gary A.
name: Sage, Leslie J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Lenticular galaxies remain remarkably mysterious as a class. Observations to date have not led to any broad consensus about their origins, properties and evolution, though they are often thought to have formed in one big burst of star formation early in the history of the Universe, and to have evolved relatively passively since then. In that picture, current theory predicts that stellar evolution returns substantial quantities of gas to the interstellar medium; most is ejected from the galaxy, but significant amounts of cool gas might be retained. Past searches for that material, though, have provided unclear results. We present results from a survey of molecular gas in a volume-limited sample of field S0 galaxies, selected from the Nearby Galaxies Catalog. CO emission is detected from 78 percent of the sample galaxies. We find that the molecular gas is almost always located inside the central few kiloparses of a lenticular galaxy, meaning that in general it is more centrally concentrated than in spirals. We combine our data with HI observations from the literature to determine the total masses of cool and cold gas. Curiously, we find that, across a wide range of luminosity, the most gas rich galaxies have about 10 percent of the total amount of gas ever returned by their stars. That result is difficult to understand within the context of either monolithic or hierarchical models of evolution of the interstellar medium.
description: 26 pages of text, 15 pages of tables, 10 figures. Accepted for publication in the Astrophysical Journal
Coupling nuclear reaction rates with temperature in explosive conditions
Creators: name: Garcia-Senz, Domingo
name: Gomez, Ruben M. Cabezon
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a straightforward integration method to compute the abundance and temperature evolution in explosive scenarios. In this approach the thermal equation is implicitely coupled with chemical equations in order to avoid instabilities and ensure a gentle transition from the normal combustion regime to the quasi (QSE) and complete nuclear statistical equilibrium (NSE). Two nuclear networks, with 14 nuclei (alpha-network) and 86 nuclei (including protons and neutrons) respectively, have been considered. The scheme is suitable to cope with a variety of explosive burning regimes.
description: 3 pages, 1 figure, proceedings "Nuclei in the Cosmos VII" 2002. To appear in Nucl. Phys. A
Engineering Effects of Vacuum Fluctuations on Two-dimensional Semiconductors
Creators: name: Horng, Jason
name: Chou, Yu-Hsun
name: Chang, Tsu-chi
name: Hsu, Chu-Yuan
name: Lu, Tien-chang
name: Deng, Hui
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The resonance energy and the transition rate of atoms, molecules and solids were understood as their intrinsic properties in classical electromagnetism. With the development of quantum electrodynamics, it is realized that these quantities are linked to the coupling of the transition dipole and the quantum vacuum. Such effects can be greatly amplified in macroscopic many-body systems from virtual photon exchange between dipoles, but are often masked by inhomogeneity and pure dephasing, especially in solids. Here, we observe an exceptionally large renormalization of exciton resonance and radiative decay rate in transition metal dichalcogenides monolayers due to interactions with the vacuum in both absorption and emission spectroscopy. Tuning the vacuum energy density near the monolayer, we demonstrate control of cooperative Lamb shift, radiative decay, and valley polarization as well as control of the charged exciton emission. Our work establishes a simple and robust experimental system for vacuum engineering of cooperative matter-light interactions.
description: 13 pages, 4 figures
Delta fenestrale
Creators: name: Dvo, L.
name: M, J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Delta
Delta fenestrale

description: Delta fenestrale (DE SAUSSURE 1852)
M a t e r i a l: Jabal Bura', NEE Al Hudaydah, N=14°53’, E=43°26’, 557 m, 19.- 21.3.2007, 1. Najd an Nashaman, S Ta'izz, N=13°20’, E=44°05’, 1433 m, 24.10.2005, 1. 20 km S Ta'izz, N=13°30’, E=43°57’, 1289 m, 24.10.2005, 1.
Recently reported from Yemen by WAHIS (2000) and GUSENLEITNER (2007).
description: Published as part of Dvo, L. & M, J., 2010, New records of vespid wasps from Yemen with synonymy in Belonogaster (Hymenoptera: Vespidae: Polistinae and Eumeninae), pp. 561-563 in Linzer biologische Beiträge 42 (1) on page 562, DOI: 10.5281/zenodo.5332555
A Trio of Massive Black Holes Caught in the Act of Merging
Creators: name: Liu, Xin
name: Hou, Meicun
name: Li, Zhiyuan
name: Nyland, Kristina
name: Guo, Hengxiao
name: Kong, Minzhi
name: Shen, Yue
name: Wrobel, Joan M.
name: Peng, Sijia
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report the discovery of SDSS J0849+1114 as the first known triple Type 2 Seyfert nucleus. It represents three active black holes that are identified from new spatially resolved optical slit spectroscopy using the Dual Imaging Spectrograph on the 3.5 m telescope at the Apache Point Observatory. We also present new complementary observations including the Hubble Space Telescope Wide Field Camera 3 U- and Y-band imaging, Chandra Advanced CCD Imaging Spectrometer S-array X-ray 0.5--8 keV imaging spectroscopy, and NSF Karl G. Jansky Very Large Array radio 9.0 GHz imaging in its most extended A configuration. These comprehensive multiwavelength observations, when combined together, strongly suggest that all three nuclei are active galactic nuclei. While they are now still at kiloparsec-scale separations, where the host-galaxy gravitational potential dominates, the black holes may evolve into a bound triple system in $\lesssim$2 Gyr. These triple merger systems may explain the overly massive stellar cores that have been observed in some elliptical galaxies such as M87, which are expected to be unique gravitational wave sources. Similar systems may be more common in the early universe, when galaxy mergers are thought to have been more frequent.
description: 19 pages, 8 figures, 6 tables; ApJ published version
MOESM3 of Microsporidian infections in the species complex Gammarus roeselii (Amphipoda) over its geographical range: evidence for both host–parasite co-diversification and recent host shifts
Creators: name: Quiles, Adrien
name: Bacela-Spychalska, Karolina
name: Teixeira, Maria
name: Lambin, Nicolas
name: Grabowski, Michal
name: Rigaud, Thierry
name: Wattier, Rémi
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
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: Additional file 3: Data S1. Alignments based on SSU rDNA sequences, used for Additional file 2: Table S2.
Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae
Creators: name: Garcia-Senz, Domingo
name: Bravo, Eduardo
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The explosion of a white dwarf of mass 1.36 M$_\odot$ has been simulated in three dimensions with the aid of a SPH code. The explosion follows the delayed detonation paradigma. In this case the deflagration-detonation transition is induced by the large corrugation of the flame front resulting from Rayleigh-Taylor instability and turbulence. The nucleosynthetic yields have been calculated, showing that some neutronized isotopes such as 54^Fe or 58^Ni are not overproduced with respect to the solar system ratios. The distribution of intermediate-mass elements is also compatible with the spectra of normal SNIa. The excepcion is, however, the abundance of carbon and oxygen, which are overproduced.
description: 3 pages, 2 figures. Proceedings "Nuclei in the Cosmos VII" 2002. To appear in Nucl. Phys. A
Caecopactes Schmidt 2007
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Caecopactes

description: CAECOPACTES GEN NOV.
 Diagnosis
Very small, eyeless and unpigmented specimens. Endoantennal (?) conglobation ability. Frons of cephalothorax concave. First coxal plate with schisma on hind corner. Second antenna with two-jointed flagellum and strong proximal articles. Fourth and fifth articles triangular, with one corner projecting ventrally.
 Type species: Caecopactes minimus sp. nov.
 Derivation of the name caecus (Latin) (blind) and pactes derived from the name Scleropactes.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on page 25, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080
ИНДЕКС МАССЫ ТЕЛА И КОМПЛАЕНТНОСТЬ У БОЛЬНЫХ ИШЕМИЧЕСКОЙ БОЛЕЗНЬЮ СЕРДЦА КОМОРБИДНЫХ С САХАРНЫМ ДИАБЕТОМ
Creators: name: Юлдошев, Н.П.
name: Санакулов, Ж.M
name: Юлдошева, Х.А.
name: Холикулов, С.Ш.
name: Пирманов, Ш.В.
Publisher: name: Zenodo
Year: 2024

description: оценить взаимосвязь индекса массы тела и комплаености у больных ИБС коморбидных с сахарным диабетом.
title: Exploring the Calorie Dimension in Nutrition Transition and Measuring Household Welfare: Evidence from Sri Lanka
Creators: name: Rathu Manannalage, Kalyani M
Publisher: name: Griffith University
Year: 2023
Subjects: subject: Sri Lanka
subject: calorie consumption
subject: household welfare
subject: nutrition transition

description: Household food consumption patterns in many developing countries are currently undergoing rapid changes. This ‘nutrition transition’ is characterised by a shift from a traditional, less processed, plant-based diet to one that features more meat, sweets, and oils. The extant literature on nutrition transition has used indirect approaches to characterise changes in dietary transition with a strong emphasis on the associated drivers of this change. However, the literature has thus far ignored the use of a more direct approach in exploring the nutrition transition process and its implications for measuring household welfare. Therefore, this thesis developed a calorie-based approach to explore nutrition transition and its implications for measuring poverty using household-level data from Sri Lanka. The thesis examines the most important drivers behind this nutrition transition, such as calorie satiation and education, and develops a novel approach for measuring household poverty. Overall, the thesis emphasises it is crucial to develop a calorie-based approach when modelling nutrition transition and devising effective poverty reduction strategies to improve the standard of living for poor and vulnerable households, particularly in developing countries.
Troglopactes Schmidt 2007, GEN. NOV.
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Troglopactes

description: TROGLOPACTES GEN. NOV.   Type species: Scleropactes botosaneanui Vandel, 1973.
 Diagnosis
Exoantennal conglobation. Cephalothorax with two longitudinal furrows, and without transverse furrow behind the frontal shield. Eyes and pigment absent. All coxal plates simple. Noduli laterales distinct, much larger than the other dorsal sensilla. Second antenna with three-jointed flagellum.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on page 26, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080