cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
4C +12.50: A Superluminal Precessing Jet in the Recent Merger System IRAS 13451+1232
Creators: name: Lister, M. L.
name: Kellermann, K. I.
name: Vermeulen, R. C.
name: Cohen, M. H.
name: Zensus, J. A.
name: Ros, E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a multi-epoch VLBA study of the powerful radio source 4C +12.50 (PKS 1345+125) at a wavelength of 2 cm. This compact radio source is associated with a hidden quasar whose host galaxy shows signs of a recent merger. It has been classified as a compact symmetric source (CSO) due to its small overall size (~220 pc) and twin-jet morphology, although it also has faint extended emission that may be a relic of previous activity. We report the detection of exceedingly high linear fractional polarization in isolated features of the southern jet (up to 60%), which is highly unusual for a CSO. Given the large amount of gas present in the host galaxy, we would expect significant Faraday depolarization across the whole source, unless the depolarizing gas is fairly clumpy. The southern jet also contains two features that are moving outward from the core at apparent speeds of v/c = 1.0 +/- 0.3 and 1.2 +/- 0.3. These represent the first positive detections of superluminal motion in a CSO, and taken together with the jet to counter-jet flux ratio, suggest an intrinsic flow speed of v/c = 0.84 +/- 0.12. The apparent ridgeline of the jet and counter-jet are consistent with a conical helix of wavelength 280 pc that is the result of Kelvin-Helmholtz instabilities driven by a slow precession of the jet nozzle. A fit to the data implies that the nozzle is precessing around a cone with half-angle 23 degrees, whose axis lies at an angle of 82 degrees to the line of sight. We suggest that the "S"-shaped jet morphologies commonly seen in recent AGN outflows such as 4C +12.50 may simply reflect the fact that their black hole spin axes are still precessing, and have not had sufficient time to align with their accretion disks.
description: 15 pages including 6 figures. Uses emulateapj.sty. Accepted for publication in the Astrophysical Journal
Astenus (Astenus) bimaculatus
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Astenus
Astenus bimaculatus

description: Astenus (Astenus) bimaculatus (ERICHSON 1840)
 Sunius bimaculatus ERICHSON 1840: 641.
 T y p e m a t e r i a l e x a m i n e d: Lectotype, present designation: "7165 / bimaculatus Er., Sardin. Gené / Syntypus Sunius bimaculatus Erichson, 1840, labelled by MNHUB 2008 / Lectotypus Sunius bimaculatus Erichson, desig. V. Assing 2008 / Astenus bimaculatus (Erichson), det. V. Assing 2008" (MNHUB). Paralectotypes: 2, 1, 1 sex? [abdomen missing]: same data as lectotype (MNHUB).
C o m m e n t: The original description is based on an unspecified number of syntypes from " Sardinia " collected by "Dom. Prof. Gené" (ERICHSON 1840). Five of them were located in the historical collection at the MNHUB. One of the males is designated as the lectotype.
description: Published as part of Assing, V., 2008, On the taxonomy and zoogeography of some Palaearctic Paederinae and Xantholinini (Coleoptera: Staphylinidae), pp. 1237-1294 in Linzer biologische Beiträge 40 (2) on page 1243, DOI: 10.5281/zenodo.5430627
Identification of 13 Cepheids and 333 Other Variables in M31
Creators: name: Joshi, Y. C.
name: Pandey, A. K.
name: Narasimha, D.
name: Sagar, R.
name: Giraud-Hiraud, Y.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Cousins $R$ and $I$ band photometry of variable stars in a $\sim13'\times 13'$ region in the disk of M31 galaxy, obtained during 141 nights. Of the 26 Cepheid variables present in the region, two are newly discovered, 11 are classified as Cepheids for the first time and 13 are confirmed as Cepheids. The extensive photometry of these Cepheids enabled us to determine precise phase and amplitude of pulsation which ranges from 0.11 to 0.48 mag in $R$ band. The period of variability ranges from $\sim$7.5 to 56 days. The period-luminosity diagram is used to derive a distance modulus of 24.49$\pm$0.11 mag for M31 galaxy. We also report variability in 333 other stars, of them, 115 stars appear to be long period variables, 2 suspected eclipsing binaries and remaining 216 are irregular variables.
description: Accepted for publication in A&A, 9 figures, the paper and figures with better resolution can be downloaded from http://cdfinfo.in2p3.fr/Downloads/cosmobs/yogesh/paper/
Order parameter dynamics of the non-linear sigma model in the large $N$ limit
Creators: name: Gemsheim, Sebastian
name: Mandal, Ipsita
name: Sengupta, Krishnendu
name: Wang, Zhiqiang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study non-equilibrium order parameter dynamics of the non-linear sigma model in the large $N$ limit, using Keldysh formalism. We provide a scheme for obtaining stable numerical solutions of the Keldysh saddle point equations, and use them to study the order parameter dynamics of the model either following a ramp, or in the presence of a periodic drive. We find that the transient dynamics of the order parameter in the presence of a periodic drive is controlled by the drive frequency displaying the phenomenon of synchronization. We also study the approach of the order parameter to its steady state value following a ramp and find out the effective temperature of the steady state. We chart out the steady state temperature of the ordered phase as a function of ramp time and amplitude, and discuss the relation of our results to experimentally realizable spin models.
description: typos corrected; published version
Prionus (Trichoprionus) aureopilosus Fragoso and Monne 1982
Creators: name: Lingafelter, Steven W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Prionus
Prionus aureopilosus

description: 9. Prionus (Trichoprionus) aureopilosus Fragoso and Monné, 1982  (Figs. 2c, d, 14b)
 Discussion. This is a rarely collected Hispaniolan species, with only about four specimens known since the original description by Fragoso and Monné (1982). That paper included the male holotype, two male paratypes, and one female paratype that was collected in February (the male specimens had no date on their labels). An additional, very rare female specimen was collected in March, making only two known for that gender (MNRJ and WIBF).
Males of this species are distinctive by their strongly appendiculate antennae (particularly antennomeres 3–8) and densely golden pubescent elytra. Females are very different from males, being larger, all black, mostly glabrous, and having weakly serrate antennae. The pronotum of both sexes has three lateral spines (positioned anteriorly, postmedially, and posteriorly).
 Hispaniolan Localities. D O M I N I C A N REPUBLIC: La Vega Province (Yaquecillo, Constanza [holotype male, MNRJ]; near Constanza, 5,000’, Casalito, 1,200 m [paratype males, female, MNRJ]; no specific data [1 male, USNM]); Santiago Province (Parque Nacional Armando Bermúdez, near Cerro Prieto, 13 March 1999, A. Del Monte [1 female, WIBF]).
description: Published as part of Lingafelter, Steven W., 2015, The Prioninae (Coleoptera: Cerambycidae) of Hispaniola, with Diagnoses, Descriptions of New Species, Distribution Records, and a Key for Identification, pp. 353-388 in The Coleopterists Bulletin 69 (3) on page 358, DOI: 10.1649/0010-065x-69.3.353, http://zenodo.org/record/10105002
Additional file 1: of Preoperative malnutrition with mild hypoalbuminemia associated with postoperative mortality and morbidity of colorectal cancer: a propensity score matching study
Creators: name: Wan-Hsiang Hu
name: Eisenstein, Samuel
name: Parry, Lisa
name: Ramamoorthy, Sonia
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: ICD-9 code and CPT code. (DOCX 50 kb)
title: Assessment of Schistosomiasis Induced Morbidity in the Philippines
Creators: name: Olveda, David Brian Uy
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Schistosomiasis
subject: Schistosomiasis japonica
subject: Philippine National Schistosomiasis Control Program
subject: Water-borne tropical disease
subject: Hepatic fibrosis
subject: Schistosomiasis-induced liver fibrosis

description: Schistosomiasis is a water-borne tropical disease plaguing approximately 240 million people worldwide. Approximately 3-70 million disability-adjusted life years are lost due to the disease. In the Philippines, schistosomiasis japonica is currently endemic in 28 provinces, 190 municipalities, and 2230 barangays (villages). Approximately 12 million residents of these endemic areas are vulnerable to infection. Preventive chemotherapy with praziquantel has been the cornerstone for schistosomiasis control in the country. The current national control program comprises annual free mass drug administration (MDA) (40 mg/kg PZQ) in all schistosomiasis-endemic communities with a prevalence of >10%. The Philippine National Schistosomiasis Control Program has recently reported that human prevalence has declined to less than 3% nationally. However, contradictory reports claim the national program is faltering. Poor drug coverage, poor drug compliance, infrequent monitoring and evaluation, and high reinfection rates daunt control efforts. Zoonotic transmission further complicates control efforts. Furthermore, advanced disease cases and schistosomiasis-related deaths are currently being reported in endemic areas throughout the country.
Review of October 14th Concert at Young Vic, London. Bertram Turetzky, with Nancy Turetzky and Barry Guy.
Creators: name: Cowie, Leroy
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: -
description: Contact: A Journal for Contemporary Music (1971-1988), No 7 (1974): Contact: A Journal for Contemporary Music
Cantaberella TRONQUET 1998
Creators: name: Assing, V.
name: Tronquet, M.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Cantaberella

description: Key to the species of Cantaberella
The references to illustrations in the literature are abbreviated as follows: A00 = ASSING (2000); A03 = ASSING (2003); T98 = TRONQUET (1998).
1 Forebody, including the appendages, yellowish, distinctly paler than the abdomen...........2
- Forebody dark-brown to blackish-brown, as dark as the abdomen or nearly so; antennae brown to dark-brown............................................................................................3
 2: posterior margin of tergite VIII distinctly emarginate in the middle (Fig. A00: 12); posterior margin of sternite VIII strongly convex (Fig. A00: 13); median lobe of aedeagus as in Fig. T98: 2.: posterior margin of sternite VIII more broadly incised in the middle (Fig. A00: 15); spermatheca as in Figs T98: 3-5. Cantabria: Pico de Tres Mares (Map 1)..................................................................................... C. pacei (TRONQUET)
 -: posterior margin of tergite VIII almost truncate, not distinctly emarginate in the middle (Fig. A00: 8); posterior margin of sternite VIII moderately convex (Fig. A00: 9); median lobe of aedeagus as in Figs A00: 4-5.: posterior margin of sternite VIII more narrowly incised in the middle (Fig. A00: 11); spermatheca as in Fig. A00: 7. León: Sierra del Teleno (Map 1)......................................................... C. feldmanni ASSING
 3 Forebody with shallow, but distinct microsculpture and subdued luster. Punctation of pronotum extremely fine, barely visible, and rather sparse. Elytra longer, approximately 0.6 times as long as pronotum (Fig. A03: 3).: sternite VIII strongly convex posteriorly (Fig. A03: 5); median lobe of aedeagus with short and in lateral view subapically angled ventral process (Figs A 03: 7-10).: sternite VIII and spermatheca as in Figs A 03: 6, 11. Cantabria: Picos de Europa (Map 1)........................................................................................................................................... C. tenebrosa ASSING
 - Forebody glossy, microsculpture very shallow, visible only at high magnification. Pronotum with distinct and rather dense punctation. Elytra shorter, approximately 0.5 times as long as pronotum (Fig. 1).: sternite VIII weakly convex, almost truncate posteriorly (Fig. 4); ventral process of aedeagus conspicuously long and in lateral view arched (Figs 5-6).: unknown. Western Pyrenees: Pic d'Orhy (Map 1)........................................................................................................................................... C. pyrenaica nov.sp.
description: Published as part of Assing, V. & Tronquet, M., 2008, The first species of Cantaberella from the western Pyrenees (Coleoptera: Staphylinidae: Aleocharinae), pp. 1295-1299 in Linzer biologische Beiträge 40 (2) on page 1298, DOI: 10.5281/zenodo.5430655
title: Citizen Science on the Ground: Visualising Nuclear Power. The Citizens’ Group Eizō no kai in Murakami
Creators: name: Hopf, Anja
Publisher: name: Fachinformationsdienst (FID) Asien
Year: 2024
Subjects: subject: Citizen Science
subject: Bürgerwissenschaften
subject: nuclear films
subject: Eizō no kai
subject: nuclear documentary
subject: Japan
subject: Film
subject: Dokumentarfilm
subject: Kernenergie
subject: Graswurzelbewegung
subject: grassroot movement
subject: Kashiwazaki-Kariwa
subject: Kuwahara Mie
subject: Murakami City
subject: Maki-machi
subject: 952

description: Fissures: Nuclear Post-War Japan, p. 342
Ultra-light Dark Matter is Incompatible with the Milky Way's Dwarf Satellites
Creators: name: Safarzadeh, Mohammadtaher
name: Spergel, David N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The density profiles of dwarf galaxies are a highly varied set. If the dark matter is an ultra-light particle such as axions, then simulations predict a distinctive and unique profile. If the axion mass is large enough to fit the ultra-faint dwarf (UFD) satellites($m\gtrapprox 10^{-21}$ eV), then the models do not fit the density profile of Fornax and Sculptor and are ruled out by more than $3-σ$ confidence. If the axion mass is in the mass range that can fit mass profiles of Fornax and Sculptor dwarf spheroidals, then its extended profile implies enormous masses ($\approx10^{11}-10^{12}M_{\odot}$) for the UFDs. These large masses for the UFDS are ruled out by more than $3-σ$ confidence by dynamical friction arguments. The tension would increase further considering star formation histories and stellar masses of the UFDs. Unless future ultra-light dark matter (ULDM) simulations with baryonic feedback show a significant change in the density structure of the halos, the current data is incompatible with the ULDM scenario. Relaxing the slope constraint from classical dwarf galaxies would lead to excluding ULDM with mass less than $6\times10^{-22}$ eV.
description: Accepted for publication in ApJ main journal
title: Modeling the Impact of Change on Software Intensive Systems
Creators: name: Wen, Lian
Publisher: name: Griffith University
Year: 2007
Subjects: subject: Software-intensive systems.

description: Abstract Most significant software-intensive systems undergo substantive change/evolution during their life time of service. Managing the consequent software changes is a difficult and costly task. In this thesis, we use two different approaches to investigate system change and its impact on the architecture and design of the system. The first approach involves traditional software change impact analysis. We propose a new and different traceability model, which is based on Genetic Software Engineering (GSE). The proposed traceability model exploits some features of GSE to create a number of advanced properties that are rare in other traceability models. For example, once a software change has been fully captured, some other design documents including the component architecture and component behavior can be automatically generated/updated. All the consequent change impacts are presented in a clear way. We have also introduced the concept of evolutionary design documents that show the evolution process of a system’s architecture as well as the design of individual components. Using this proposed traceability model, a practical method to normalize and simplify the component architecture of software intensive systems has been developed. An important result we have proved is that the component architecture of a software system is independent to the functional requirements of the system. We claim that a normalized software system is easier to maintain and change. The second approach starts from a macro view. Rather than exploring the details of the change impacts from individual changes, this approach focuses on the common properties of the architecture evolution of complex systems; it stresses the topological structure from an evolutionary viewpoint. For this investigation we use scale-free networks and hierarchy theory as the major tools. Hierarchy is a natural structure for diverse large and complex systems, and recent studies reveal that many large networks from different domains are scale-free. In this research, we have discovered that the component dependency networks of many software systems are scale-free; we have also found that there is a close connection between the scale-free feature and the optimization of sorting algorithms. These results imply that there are fundamental rules working behind the evolution of large systems including software intensive systems, and that the scale-free property can be used as a possible index for the optimization level of the structure of a system. Software change and software evolution are critical aspects of software engineering. This thesis has used a macroscopic and technical, formal approach to make positive contributions to understanding and accommodating change of software-intensive systems.
Discovery of a Near-Infrared Jet-Like Feature in the Z Canis Majoris System
Creators: name: Millan-Gabet, R.
name: Monnier, J. D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present near-infrared high resolution observations of the young binary system Z Canis Majoris using the adaptive optics system at the Keck-II telescope. Both components are unresolved at 1.25 and 1.65 microns, although high dynamic range images reveal a previously unknown jet-like feature in the circumstellar environment. We argue that this feature probably arises from light scattered off the walls of a jet-blown cavity, and proper motion studies of this feature can probe the dynamics of the bipolar outflow. Potentially, the morphology of the dust-laden cavity walls offers a new probe of the momentum profile and collimation of bipolar winds from young stellar objects. We also derive high precision binary parameters, which when combined with historical data have allowed the first detection of orbital motion. Lastly, our observations confirm the high degree of flux variability in the system; the North-West binary component is dominant at H-band, in contrast to all previous observations.
description: 6 pages 3 figures 1 table
The Impact of Plasma Instabilities on the Spectra of TeV Blazars
Creators: name: Batista, Rafael Alves
name: Saveliev, Andrey
name: Pino, Elisabete M. de Gouveia Dal
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Relativistic jets from blazars are known to be sources of very-high-energy gamma rays (VHEGRs). During their propagation in the intergalactic space, VHEGRs interact with pervasive cosmological photon fields such as the extragalactic background light (EBL) and the cosmic microwave background (CMB), producing electron-positron pairs. These pairs can upscatter CMB/EBL photons to high energies via inverse Compton scattering, thereby continuing the cascade process. This is often used to set limits on intergalactic magnetic fields (IGMFs). However, the picture may change if plasma instabilities, arising due to the interaction of the pairs with the intergalactic medium (IGM), cool down the electrons/positrons faster than inverse Compton scattering. As a consequence, the kinetic energy lost by the pairs to the IGM could cause a hardening in the observed gamma-ray spectrum at energies below $\sim$100 GeV. Here we study several types and models of instabilities and assess their impact for interpreting observations of distant blazars. Our results suggest that plasma instabilities can describe the spectra of some blazars and mimic the effects of IGMFs, depending on parameters such as intrinsic spectrum of the object, the density and temperature of the IGM, and the luminosity of the beam. On the other hand, we find that for our fiducial set of parameters plasma instabilities do not have a major impact on the spectra of some of the blazars studied. Therefore, they may be used for constraining IGMFs.
description: 14 pages, 8 figures; minor changes to match published version
Dwarf Galaxies: Important Clues to Galaxy Formation
Creators: name: Tolstoy, Eline
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The smallest dwarf galaxies are the most straight forward objects in which to study star formation processes on a galactic scale. They are typically single cell star forming entities, and as small potentials in orbit around a much larger one they are unlikely to accrete much (if any) extraneous matter during their lifetime (either intergalactic gas, or galaxies) because they will typically lose the competition with the much larger galaxy. We can utilise observations of stars of a range of ages to measure star formation and enrichment histories back to the earliest epochs. The most ancient objects we have ever observed in the Universe are stars found in and around our Galaxy. Their proximity allows us to extract from their properties detailed information about the time in the early Universe into which they were born. A currently fashionable conjecture is that the earliest star formation in the Universe occurred in the smallest dwarf galaxy sized objects. Here I will review some recent observational highlights in the study of dwarf galaxies in the Local Group and the implications for understanding galaxy formation and evolution.
description: 10 pages, 4 figures, Invited talk in "Galaxy Evolution III: From Simple Approaches to Self-Consistent Models" (Kiel, Germany, July 16-20, 2002) eds. G. Hensler et al., in press
Derancistrus hovorei Lingafelter and Woodley 2007
Creators: name: Lingafelter, Steven W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Derancistrus
Derancistrus hovorei

description: 12. Derancistrus hovorei Lingafelter and Woodley, 2007  (Figs. 2g, 15a)
 Discussion. This endemic Hispaniolan species, described recently by Lingafelter and Woodley (2007), is known from only three specimens, all collected in June and July along the Cabo Rojo road in the extreme southwestern part of the Dominican Republic. No additional material has been collected since its description.
 Derancistrus hovorei, with its vittate elytra, is morphologically similar only to D. elegans and S. vittata. It differs from the latter by its large, spine-like lateral processes on the pronotum and distinctly bilobed posterior margin of the prosternal process. In males, the pronotal margins of S. vittata are nearly parallel and slightly erose; in females, the pronotal margins are crenulate, with the posterolateral margin acutely produced but not as spine-like as in D. hovorei. The posterior margin of the prosternal process is evenly rounded in both sexes of S. vittata. Derancistrus hovorei differs from D. elegans by having obvious coarse punctation on the elytra (nearly impunctate in D. elegans, the tiny punctures not apparent without high magnification) and in having the median lateral spine of the pronotum shorter and less hooked than in D. elegans.
 Hispaniolan Localities. D O M I N I C A N REPUBLIC: Pedernales Province (23–25 km north of Cabo Rojo [USNM, RHTC]).
description: Published as part of Lingafelter, Steven W., 2015, The Prioninae (Coleoptera: Cerambycidae) of Hispaniola, with Diagnoses, Descriptions of New Species, Distribution Records, and a Key for Identification, pp. 353-388 in The Coleopterists Bulletin 69 (3) on page 360, DOI: 10.1649/0010-065x-69.3.353, http://zenodo.org/record/10105002
Additional file 1: of miRkwood: a tool for the reliable identification of microRNAs in plant genomes
Creators: name: Guigon, Isabelle
name: Legrand, Sylvain
name: Jean-Frédéric Berthelot
name: Bini, Sébastien
name: Lanselle, Delphine
name: Mohcen Benmounah
name: Touzet, Hélène
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
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: Developmental Biology
subject: 60506 Virology

description: Detailed description of some of the miRkwood steps. (PDF 166 kb)
Rugilus geniculatus
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Rugilus
Rugilus geniculatus

description: Rugilus geniculatus (ERICHSON 1839)
 Stilicus geniculatus ERICHSON 1839a: 522.
 T y p e m a t e r i a l e x a m i n e d Lectotype, present designation: " geniculatus Er., Berol. Er. / Zool. Mus. Berlin, "Hist. Coll." Nr. 6402 / Syntype / Rugilus geniculatus Er., det. M. Schülke 1991 / Lectotypus Stilicus geniculatus Erichson, desig. V. Assing 2008 / Rugilus geniculatus (Erichson), det. V. Assing 2008" (MNHUB). Paralectotypes: 3 exs.: same data as lectotype (MNHUB).
A d d i t i o n a l m a t e r i a l e x a m i n e d: Germany: 1 ex., Niedersachsen, Oldenburg, Pestrup, 3.XI.1945, leg. Kerstens (MNHUB); 1 ex., Niedersachsen, NW Hannover, Helstorf, heathland, sifted, 2.I.1982 (cAss). Poland: 4 exs., Legnica (NHMW, cAss). Spain: 1 ex., Madrid, Sierra de Guadarrama, Navacerrada, 1800 m, 5.IX.2001, leg. Anichtchenko (cAss).
C o m m e n t: The original description is based on an unspecified number of syntypes. The type series in the historical collection of the MNHUB is composed of four specimens. A male in good condition is designated as the lectotype. It is in agreement with the interpretation of LOHSE (1964) and COIFFAIT (1984).
description: Published as part of Assing, V., 2008, On the taxonomy and zoogeography of some Palaearctic Paederinae and Xantholinini (Coleoptera: Staphylinidae), pp. 1237-1294 in Linzer biologische Beiträge 40 (2) on page 1245, DOI: 10.5281/zenodo.5430627
The impact of mass loss on star cluster formation. I. Analytic results
Creators: name: Boily, C. M.
name: Kroupa, P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study analytically the disruptive effect of instantaneous gas removal from a cluster containing O stars. We setup an iterative calculation based on the stellar velocity distribution function to compute the fraction of stars that remain bound once the cluster has ejected the gas and is out of equilibrium. We show that the stellar bound fraction is a function of the initial cluster distribution function as well as the star formation efficiency, $ε$, taken constant throughout the cluster. The case of the Plummer sphere is dealt with in greater details. We find for this case that up to ~ 50% of the stars may remain bound when $ε$ assumes values < 1/2, contrary to expectations derived from the virial theorem. The fraction of bound stars is expressed algebraically for polytropic distribution functions.
description: to appear in MN
Scalable Majorana vortex modes in iron-based superconductors
Creators: name: Chiu, Ching-Kai
name: Machida, T.
name: Huang, Yingyi
name: Hanaguri, T.
name: Zhang, Fu-Chun
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A vortex in an s-wave superconductor with a surface Dirac cone can trap a Majorana bound state with zero energy leading to a zero-bias peak (ZBP) of tunneling conductance. The iron-based superconductor FeTe$_x$Se$_{1-x}$ is one of the material candidates hosting these Majorana vortex modes. It has been observed by recent scanning tunneling spectroscopy measurement that the fraction of vortex cores possessing ZBPs decreases with increasing magnetic field on the surface of this iron-based superconductor. We construct a three-dimensional tight-binding model simulating the physics of over a hundred Majorana vortex modes in FeTe$_x$Se$_{1-x}$ with realistic physical parameters. Our simulation shows that the Majorana hybridization and disordered vortex distribution can explain the decreasing fraction of the ZBPs observed in the experiment. Furthermore, we find the statistics of the energy peaks off zero energy in our simulation with the Majorana physics in agreement with the analyzed peak statistics in the vortex cores from the experiment. This agreement and the explanation of the decreasing ZBP fraction lead to an important indication of scalable Majorana vortex modes in the iron-based superconductor. Thus, FeTe$_x$Se$_{1-x}$ can be one promising platform possessing scalable Majorana qubits for quantum computing. In addition, we further show the interplay of the ZBP presence and the vortex locations qualitatively agrees with our additional experimental observation and predict the universal spin signature of the hybridized multiple Majorana vortex modes.
description: 10 pages, 7 figures, Supplementary Information
title: 原子力平和利用と＜軍事＞の接続: テレビ番組からの考察
Creators: name: Nanasawa, Kiyoshi
Publisher: name: Fachinformationsdienst (FID) Asien
Year: 2024
Subjects: subject: NHK
subject: 原子力の平和利用
subject: 日本放送協会
subject: Japan
subject: Nihon Hōsō Kyōkai
subject: Kernenergie / Friedliche Nutzung
subject: 核保有
subject: 非核三原則
subject: NPT体制
subject: 核燃料サイクル計画
subject: 対テロ軍事社会
subject: 軍事組織
subject: 自衛隊
subject: 952

description: Fissures: Nuclear Post-War Japan, p. 167
Additional file 1: of Outcome measurement in mental health services: insights from symptom networks
Creators: name: Barbalat, Guillaume
name: Bergh, Don
name: Kossakowski, Jolanda
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Glossary for HoNOS Score Sheet. (PDF 353 kb)
Structure of multiplicative simple Hom-Jordan algebras
Creators: name: Yao, Chenrui
name: Ma, Yao
name: Chen, Liangyun
Publisher: name: arXiv
Year: 2019
Subjects: subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 17C10, 17C20, 17C50, 17B10, 17A30

description: In this paper, we mainly study structure of multiplicative simple Hom-Jordan algebras. We talk about equivalent conditions for multiplicative Hom-Jordan algebras being solvable, simple and semi-simple. As an application, we give a theorem about classification of multiplicative simple Hom-Jordan algebras. Moreover, some propositions about bimodules of multiplicative Hom-Jordan algebras are also displayed.
description: 19pages
Difficulties with Recovering The Masses of Supermassive Black Holes from Stellar Kinematical Data
Creators: name: Valluri, Monica
name: Merritt, David
name: Emsellem, Eric
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the ability of three-integral, axisymmetric, orbit-based modeling algorithms to recover the parameters defining the gravitational potential (M/L ratio and black hole mass Mh) in spheroidal stellar systems using stellar kinematical data. We show that the potential estimation problem is generically under-determined when applied to long-slit kinematical data of the kind used in most black hole mass determinations to date. A range of parameters (M/L, Mh) can provide equally good fits to the data, making it impossible to assign best-fit values. We illustrate the indeterminacy using a variety of data sets derived from realistic models as well as published observations of the galaxy M32. In the case of M32, our reanalysis demonstrates that data published prior to 2000 are equally consistent with Mh in the range 1.5x10^6-5x10^6 solar masses, with no preferred value in that range. While the HST/STIS data for this galaxy may overcome the degeneracy in Mh, HST data for most galaxies do not resolve the black hole's sphere of influence and in these galaxies the degree of degeneracy allowed by the data may be substantial. We investigate the effect on the degeneracy of enforcing smoothness (regularization) constraints. However we find no indication that the true potential can be recovered simply by enforcing smoothness. For a given smoothing level, all solutions in the minimum-chisquare valley exhibit similar levels of noise. These experiments affirm that the indeterminacy is real and not an artifact associated with non-smooth solutions. (Abridged)
description: Accepted for publication in The Astrophysical Journal. Changes include discussion of regularization
Astenus (Astenus) serpentinus
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Astenus
Astenus serpentinus

description: Astenus (Astenus) serpentinus (MOTSCHULSKY 1858)
 Sunius subditus MULSANT & REY 1878: 278.
 T y p e m a t e r i a l e x a m i n e d: Lectotype, present designation: " / Lyon / Rey / subditus Rey / ex auctore / Cotypus Astenus subditus Rey / ex coll. Skalitzky / ex coll. Scheerpeltz / Lectotypus Sunius subditus Mulsant & Rey, desig. V. Assing 2008 / Astenus serpentinus (Motschulsky), det. V. Assing 2008" (NHMW). Paralectotypes: 2: same data as lectotype (NHMW).
 C o m m e n t: The original description of Sunius subditus is based on an unspecified number of syntypes from "les environs de Lyon et dans le Beaujolais" (MULSANT & REY 1878). Three syntypes, a male and two females were located in the collections of the NHMW; the male is designated as the lectotype.
description: Published as part of Assing, V., 2008, On the taxonomy and zoogeography of some Palaearctic Paederinae and Xantholinini (Coleoptera: Staphylinidae), pp. 1237-1294 in Linzer biologische Beiträge 40 (2) on page 1243, DOI: 10.5281/zenodo.5430627
Experimental Music Catalogue: Robert Ashley: Fancy Free or It's There; Complete with Heat. David Jackman: Untitled Prose Collection.
Creators: name: Jones, David
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: -
description: Contact: A Journal for Contemporary Music (1971-1988), No 8 (1974): Contact: A Journal for Contemporary Music
MEDIA MAKONDA MANIPULYATSIYANING NAZARIY METODOLOGIK TAHLILI
Creators: name: Marifjonov, Abrorjon
Publisher: name: Zenodo
Year: 2024

description: Inson psixologiyasi nihoyatda murakkab, uning muhim qismini xayolot olami tashkil qiladi. Shunday ekan, odam bir vaqting o‘zida ikki parallel olamda yashaydi: real hayotda va tasavvurlar dunyosida. Shunisi qiziqki, insonning aynan xayoliy dunyosiga tashqaridan osonlikcha ta’sir ko‘rsatish mumkin. Muhimi shundaki, bu ta’sir doim yashirin xarakterga ega bo‘lib, insonning o‘zi buni ko‘pincha payqamaydi. Bu jarayonni manipulyasiya mexanizmi boshqaradi. Shu jihatdan mavzuda manipulyasiya mexanizmi haqida ma'lumot berishga harakat qilingan.
Rugilus rufipes
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Rugilus
Rugilus rufipes

description: Rugilus rufipes (GERMAR 1836)
 Stilicus nematideus GISTEL 1857: 19; nov syn.
 C o m m e n t: The nomen dubium Stilicus nematideus GISTEL was made available in a widely neglected paper containing more than 800 non-informative descriptions of miscellaneous animals. With few exceptions, Gistel´s type material, which according to HORN et al (1990) is deposited in the Zoologische Staatssammlung München, is lost (BAEHR pers. comm.).
 The original description of S. nematideus best fits Rugilus rufipes ("Dunkelbraun,..., Kopf viereckig,..., Brustschild eiförmig,.... Zu Paederus scabricollis gyl."). Hence the synonymy proposed above.
description: Published as part of Assing, V., 2008, On the taxonomy and zoogeography of some Palaearctic Paederinae and Xantholinini (Coleoptera: Staphylinidae), pp. 1237-1294 in Linzer biologische Beiträge 40 (2) on page 1246, DOI: 10.5281/zenodo.5430627
Exploiting Faraday Rotation to Jam Quantum Key Distribution via Polarized Photons
Creators: name: Daschner, Maximilian
name: Kaiser, David I.
name: Formaggio, Joseph A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum key distribution (QKD) involving polarized photons could be vulnerable to a jamming (or denial-of-service) attack, in which a third party applies an external magnetic field to rotate the plane of polarization of photons headed toward one of the two intended recipients. Sufficiently large Faraday rotation of one of the polarized beams would prevent Alice and Bob from establishing a secure quantum channel. We investigate requirements to induce such rotation both for free-space transmission and for transmission via optical fiber, and find reasonable ranges of parameters in which a jamming attack could be successful against fiber-based QKD, even for systems that implement automated recalibration for polarization-frame alignment. The jamming attack could be applied selectively and indefinitely by an adversary without revealing her presence, and could be further combined with various eavesdropping attacks to yield unauthorized information.
description: 8 pages, 1 figure. References added and further discussion included of how the jamming attack could be combined with various eavesdropping attacks
Elateropsis sericeiventris Chevrolat 1862
Creators: name: Lingafelter, Steven W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Elateropsis
Elateropsis sericeiventris

description: 17. Elateropsis sericeiventris Chevrolat, 1862  (Figs. 3d, 16a)
 Discussion. This species was previously known only from Cuba (Monné 2015). Two male specimens from the Dominican Republic (USNM, MNDR) were examined, representing a new island and new country records, along with a female from Galbis, Cuba (USNM).
 The key of Galileo and Martins (1994) works well for these specimens and identifies them as E. sericeiventris on the basis of the pronotum having dense pubescence at the sides but not the posterior margin, the prosternum lacking a ventral projection (a weak projection is present in females), the prosternal intercoxal process being pronounced and deeply bilobed, and having long pubescence present on the mesal surface of the profemora and throughout the venter except along the middle of the sternites.
 Elateropsis sericeiventris is part of the complex of similar species including E. trimarginatus and E. quinquenotatus. Both of those species differ in having dense pubescence along the posterior margin of the pronotum. Both the Dominican male and Cuban female specimens of E. sericeiventris in the USNM have mostly ferruginous elytra, legs, and antennae which is very similar to the holotype in BMNH, while the MNDR specimen is mostly piceous to black except for a ferruginous apical margin of the elytra. In E. quinquenotatus, the elytra are all black and the proportions are broader and less elongate. In E. trimarginatus the elytra are mostly ferruginous but, like E. quinquenotatus, the dimensions are broader and less elongate than in E. sericeiventris.
 Zayas (1957: plate 13) has a photograph of a Cuban specimen from the USNM (not found) identified as E. sericeiventris. However, this specimen is either a variant of E. trimarginatus with incomplete pronotal pubescence along the posterior margin and a pronounced prosternal process that extends beyond hind margins of the procoxae or an undescribed species.
 Hispaniolan Localities. D O M I N I C A N REPUBLIC: Santo Domingo (no further data [USNM]); Elías Piña Province (Cerro de San Francisco, El Tabacal, Pedro Santana [MNDR]).
description: Published as part of Lingafelter, Steven W., 2015, The Prioninae (Coleoptera: Cerambycidae) of Hispaniola, with Diagnoses, Descriptions of New Species, Distribution Records, and a Key for Identification, pp. 353-388 in The Coleopterists Bulletin 69 (3) on page 363, DOI: 10.1649/0010-065x-69.3.353, http://zenodo.org/record/10105002
title: Darstellung von Kernenergie im Japan der 1950er Jahre: Am Beispiel des Manga Astro Boy von Tezuka Osamu
Creators: name: Yamamoto, Akihiro
Publisher: name: Fachinformationsdienst (FID) Asien
Year: 2024
Subjects: subject: Tetsuwan Atomu
subject: Astro Boy
subject: Japan
subject: Tezuka, Osamu
subject: Manga
subject: Kernenergie
subject: 952

description: Fissures: Nuclear Post-War Japan, p. 183
Measurements of streaming motions of the Galactic bar with Red Clump Giants
Creators: name: Sumi, T.
name: Eyer, L.
name: Wozniak, P. R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report a measurement of the streaming motion of the stars in the Galactic bar with the Red Clump Giants (RCGs) using the data of the Optical Gravitational Lensing Experiment II (OGLE-II). We measure the proper motion of 46,961 stars and divide RCGs into bright and faint sub-samples which on average will be closer to the near and far side of the bar, respectively. We find that the far-side RCGs (4,979 stars) have a proper motion of Δ ~ 1.5 +- 0.11 mas yr^{-1} toward the negative l relative to the near-side RCGs (3,610 stars). This result can be explained by stars in the bar rotating around the Galactic center in the same direction as the Sun with v_b ~ 100 km s^{-1}. In the Disc Star (DS) and Red Giant (RG) samples, we do not find significant difference between bright and faint sub-samples. For those samples Δ \~ 0.3 +- 0.14 mas yr^{-1} and ~ 0.03 +- 0.14 mas yr^{-1}, respectively. It is likely that the average proper motion of RG stars is the same as that of the Galactic center. The proper motion of DSs with respect to RGs is ~ 3.3 mas yr^{-1} toward positive l. This value is consistent with the expectations for a flat rotation curve and Solar motion with respect to local standard of rest. RGs have proper motion approzimately equal to the average of bright and faint RCGs, which implies that they are on average near the center of the bar. This pilot project demonstrates that OGLE-II data may be used to study streaming motions of stars in the Galactic bar. We intend to extend this work to all 49 OGLE-II fields in the Galactic bulge region.
description: 7 pages, 9 figures, submitted to MNRAS
A new infrared band in the Interstellar and Circumstellar Clouds: C_4 or C_4H?
Creators: name: Cernicharo, J.
name: Goicoechea, J. R.
name: Benilan, Y.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the detection with the Infrared Space Observatory (ISO) of a molecular band at 57.5 microns (174 cm^{-1}) in carbon-rich evolved stars and in Sgr B2. Taking into account the chemistry of these objects the most likelihood carrier is a carbon chain. We tentatively assign the band to the nu_5 bending mode of C_4 for which a wavenumber of 170-172.4 cm^{-1} has been derived in matrix experiments (Withey et al. 1991). An alternate carrier might be C_4H, although the frequency of its lowest energy vibrational bending mode, nu_7, is poorly known (130-226 cm^{-1}). If the carrier is C_4, the derived maximum abundance is nearly similar to that found for C_3 in the interstellar and circumstellar media by Cernicharo, Goicoechea & Caux (2000). Hence, tetra-atomic carbon could be one of the most abundant carbon chain molecules in these media.
description: 11 pages, 1 figure, accepted in ApJ Letters
Rugilus orbiculatus
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Rugilus
Rugilus orbiculatus

description: Rugilus orbiculatus (PAYKULL 1796)
 Rugilus exiguus HEER 1839: 233; nov syn.
 C o m m e n t: The nomen dubium Rugilus exiguus HEER (SMETANA 2004) is based on type material from "Zürichberg..., Genf " (HEER 1839). The original description best fits Rugilus orbiculatus ("Caput subobiculare, latitudine fere elytrorum,... pronot. suborbiculatum,... elytra opaca, nigra, apice picea"), with which the name is synonymised.
description: Published as part of Assing, V., 2008, On the taxonomy and zoogeography of some Palaearctic Paederinae and Xantholinini (Coleoptera: Staphylinidae), pp. 1237-1294 in Linzer biologische Beiträge 40 (2) on page 1246, DOI: 10.5281/zenodo.5430627
Strange metal behavior in a pure ferromagnetic Kondo lattice
Creators: name: Shen, Bin
name: Zhang, Yongjun
name: Komijani, Yashar
name: Nicklas, Michael
name: Borth, Robert
name: Wang, An
name: Chen, Ye
name: Nie, Zhiyong
name: Li, Rui
name: Lu, Xin
name: Lee, Hanoh
name: Smidman, Michael
name: Steglich, Frank
name: Coleman, Piers
name: Yuan, Huiqiu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The strange metal phases found to develop in a wide range of materials near a quantum critical point (QCP), have posed a long-standing mystery. The frequent association of strange metals with unconventional superconductivity and antiferromagnetic QCPs has led to a belief that they are highly entangled quantum states. Ferromagnets, by contrast are regarded as an unlikely setting for strange metals, for they are weakly entangled and their QCPs are often interrupted by competing phases or first order phase transitions. Here, we provide compelling evidence that the stoichiometric heavy fermion ferromagnet CeRh$_6$Ge$_4$ becomes a strange metal at a pressure-induced QCP: specific heat and resistivity measurements demonstrate that the FM transition is continuously suppressed to zero temperature revealing a strange metal phase. We argue that strong magnetic anisotropy plays a key role in this process,injecting entanglement, in the form of triplet resonating valence bonds (tRVBs) into the ordered ferromagnet. We show that the singular transformation from tRVBs into Kondo singlets that occurs at the QCP causes a jump in the Fermi surface volume: a key driver of strange metallic behavior. Our results open up a new direction for research into FM quantum criticality, while also establishing an important new setting for the strange metal problem. Most importantly, strange metallic behavior at a FM quantum critical point suggests that it is quantum entanglement rather than the destruction of antiferromagnetism that is the common driver of the many varied examples of strange metallic behavior.
description: 15 pages, 3 figures, Supplementary Information available upon request. The manuscript is the original submitted version, the revised version is accepted by Nature