cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The 2dF QSO Redshift Survey - V. The 10k catalogue
Creators: name: Croom, S. M.
name: Smith, R. J.
name: Boyle, B. J.
name: Shanks, T.
name: Loaring, N. S.
name: Miller, L.
name: Lewis, I. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a catalogue comprising over 10000 QSOs covering an effective area of 289.6 sq. degrees, based on spectroscopic observations with the 2-degree Field instrument at the Anglo-Australian Telescope. This catalogue forms the first release of the 2-degree Field QSO Redshift Survey. QSO candidates with 18.25
description: 9 pages including 8 figures to be published in the April 21 issue of MNRAS, vol. 322, L29. Access to the catalogue and spectra is available at http://www.2dfquasar.org/
Ochthephilum egregium
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Ochthephilum
Ochthephilum egregium

description: Ochthephilum egregium (REITTER 1884) (Figs 8-10, 20-21, Map 2)
 Cryptobium egregium REITTER 1884: 83 f.
 T y p e m a t e r i a l e x a m i n e d Lectotype 3, present designation: " Kaukas Leder / Elisabetpol [= Gyandzha, = Kirovabad (Azerbaijan)] / coll. Reitter / Paratypus 1884, Cryptobium egregium Reitter [curator label] / Lectotypus 3 Cryptobium egregium Reitter, desig. V. Assing 2008 / Ochthephilum egregium (Reitter) det. V. Assing " (HNHM). Paralectotypes: 533, 1♀: same data as lectotype [♀ with the curator label " Holotypus..."]; 13: same data, but " Ochthephilum turkestanicum (Korge) det. V. Assing " (HNHM); 13: " Caucasus Leder. Reitter / Elisabetpol / coll. Reitter / Paratypus 1884, Cryptobium egregium Reitter [curator label] / Ochthephilum turkestanicum (Korge) det. V. Assing " (HNHM).
A d d i t i n a l m a t e r i a l e x a m i n e d: Azerbaijan:333, Xanlar ["Helenendorf"], leg. Reitter (HNHM, cAss). Locality not specified: 13, "Caspi" (HNHM); 11 exs., "Kaukas. Leder" (NHMW, cAss).
 C o m m e n t: The original description is based on an unspecified number of syntypes from "Elisabethpol" (REITTER 1884). An examination of the type series in the Reitter collection at the HNHM, which comprises eight males and one female, revealed that they belong to two species, so that a lectotype designation is mandatory in the interest of the stability of nomenclature. Two males are conspecific with O. turkestanicum (KORGE). One of the males that are not conspecific with O. turkestanicum is designated as the lectotype. The interpretation of O. egregium by ZANETTI (1980) and HOZMAN (1985) refers to an undescribed species, which is described as O. permutatum below.
 Ochthephilum egregium is readily distinguished from O. collare and other similar congeners by the distinctly smaller aedeagus and the shape of its internal structures (Figs 8- 10, 20-21). The forebody of all examined specimens is of more or less uniformly brownish coloration.
D i s t r i b u t i o n: Confirmed records are known only from Azerbaijan (Map 2).
description: Published as part of Assing, V., 2009, On the Western Palaearctic and Middle Asian species of Ochthephilum STEPHENS, with notes on Cryptobium koltzei EPPELSHEIM (Coleoptera: Staphylinidae: Paederinae: Cryptobiina), pp. 397-426 in Linzer biologische Beiträge 41 (1) on pages 403-404, DOI: 10.5281/zenodo.5276149
Paulianidia janaki Lecoq 2008, n. sp.
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia janaki

description: Paulianidia janaki n. sp.
(Fig. 4A)
HOLOTYPE. — Madagascar Est, massif Anjanaharibe nord, 750-850 m, sentier Ambodihasina-Ambalarombe, env. riv. Andramonta, tamisage en forêt humide, 28.II.1996, J. Janák, P. Moravec, 1 ♂ (MNHUB).
PARATYPES. — Mêmes données que pour l’holotype, 1 ♂ (coll. Janák); 1 ♂ (MNHN).
Madagascar Nord, Antsiranana, 6,5 km SSW Befingotra, rés. Anjanaharibe sud, 875 m, 14°45’S, 49°30’E, 19.X.1994, forêt pluviale, litière tamisée (feuilles et bois pourris), B. L. Fisher, 9 ♂♂, 6 ♀♀ (FMNH); 5 ♂♂, 3 ♀♀ (MNHN). — Madagascar Nord, 5 km E Andapa, Lembonibona, 1265 m, forêt dégradée, tamisages, 2.III.1996, J. Janák, P. Moravec, 1 ♂ (MNHN).
 ÉTYMOLOGIE. — Cette espèce est dédiée à mon collègue tchèque, Jiri Janák, remarquable récolteur qui a rapporté de nombreux staphylins de Madagascar et m’a confié l’étude de ses Paulianidia.
DESCRIPTION
Longueur: 5 mm. Ailé. Avant-corps et élytres brun sombre. Pièces buccales et pattes ferrugineux sombres. Antennes assombries sauf le dernier article un peu plus clair.
 Tête un peu plus longue que large au niveau des yeux (R = 1,08). Les tempes plus de deux fois plus longues que les yeux, en courbe régulière peu accentuée, presque fuyantes, l’angle postérieur inexistant. Ponctuation analogue à celle de P.itremo n. sp.: forte, nette et dense sur tout le pourtour, plus clairsemée au centre du disque.Tégument lisse et brillant. Articles antennaires analogues à ceux de P. itremo n. sp.
Pronotum un peu plus long que large, aussi large que la tête au niveau des yeux. Les angles antérieurs à peine indiqués, les postérieurs très émoussés. Ponctuation forte et dense, analogue à celle des bords de la tête; une bande médiane imponctuée interrompue avant la base et bordée vers l’arrière de deux petites dépressions. Écusson ponctué.
Élytres rectangulaires, un peu plus longs que larges (R = 1,12), plus larges que le pronotum (R = 1,20). Ponctuation analogue à celle du pronotum en force et densité.
Tergites abdominaux à ponctuation fine et peu dense, plus forte dans la dépression basale des premiers segments. Tégument très finement et superficiellement réticulé en travers sur les premiers tergites.
Mâle: bordure postérieure du sternite du pygidium découpée en arc de cercle sur toute sa largeur.
Édéage: paramères larges, plaqués sur le lobe médian, aussi longs que celui-ci et comme sectionnés à l’extrémité; celle-ci avec une dent en crochet dirigée vers le lobe médian.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on pages 592-593, DOI: 10.5281/zenodo.5390906
Using MCA tools for evaluating community-managed forests from a green economy perspective: lessons from Nepal
Creators: name: S. Baral
name: C. Khadka
name: H. Vacik
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Nepal is in the process of formulating its forest policies at the provincial level . Various community-managed forests have been designed in the past by the Nepal government to decentralize the forest for its sustainable management practice. This study facilitates the process of identifying appropriate forest management options in two of the provinces, namely Provinces Three and Gandaki. Four forest management options – passive, active, scientific and multiple – were identified following the existing management practices. For the evaluation of the overall performance of the options, a framework with three criteria, 10 indicators and 28 verifiers were designed. The framework followed the green economy perspective considering the improvement of the forest conditions, economic and social well-being, and low carbon emission. The Analytical Hierarchy Process was used to prioritize the best management option and analyse trade-offs to guide future decision-making and reduce the risk of unwanted consequences. Our results show that the elicitation of preferences for the evaluation criteria varied by stakeholder groups. Their preference was largely guided by improving the forest resource condition and economic well-being. Foresters prefer scientific and active forest management, policymakers prefer multiple-use forest management and scientific management, whereas community forest user groups prefer active forest management. We argue that a scientific management approach may contribute better to economic aspects, although it may often compromise the other aspects. The multiple forest management option seems to be the best for green economy considering ecological, economic and social consequences.
Cordalia vestita
Creators: name: Assing, V.
name: J, Cordalia
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Cordalia
Cordalia vestita

description: Cordalia vestita (BOHEMAN 1858)
M a t e r i a l e x a m i n e d: India: 4 exs., Assam, Nameri N. P., 27.V.2006, leg. de Rougemont (cAss, cRou).
C o m m e n t: This species has frequently been misidentified and/or misinterpreted, so that most literature records prior to 2002 are unreliable. A redescription was provided by ASSING (2002), who also designated a lectotype.
description: Published as part of Assing, V. & J, Cordalia, 2009, New species and additional records of Palaearctic Falagriini (Coleoptera: Staphylinidae: Aleocharinae), pp. 471-480 in Linzer biologische Beiträge 41 (1) on page 474, DOI: 10.5281/zenodo.5276207
Time delays in ultracold atomic and molecular collisions
Creators: name: Frye, Matthew D.
name: Hutson, Jeremy M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We study the behavior of the Eisenbud-Wigner collisional time delay around Feshbach resonances in cold and ultracold atomic and molecular collisions. We carry out coupled-channels scattering calculations on ultracold Rb and Cs collisions. In the low-energy limit, the time delay is proportional to the scattering length, so exhibits a pole as a function of applied field. At high energy, it exhibits a Lorentzian peak as a function of either energy or field. For narrow resonances, the crossover between these two regimes occurs at an energy proportional to the square of the resonance strength parameter $s_\textrm{res}$. For wider resonances, the behavior is more complicated and we present an analysis in terms of multichannel quantum defect theory.
Far Ultraviolet Spectroscopy of the Intergalactic and Interstellar Absorption Toward 3C 273
Creators: name: Sembach, K. R.
name: Howk, J. C.
name: Savage, B. D.
name: Shull, J. M.
name: Oegerle, W. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the molecular, neutral atomic, weakly ionized, and highly ionized components of the interstellar and intergalactic material toward the quasar 3C 273. We identify Ly-beta absorption in 8 of the known intergalactic Ly-alpha absorbers along the sight line with rest-frame equivalent widths greater than 50 mA. Refined estimates of the H I column densities and Doppler parameters (b) of the clouds are presented. We find a range of b = 16-46 km/s. We detect multiple H I lines (Ly-beta - Ly-theta) in the 1590 km/s Virgo absorber and estimate log N(H I) = 15.85, ten times more H I than in all of the other absorbers along the sight line combined. The Doppler width of this absorber, b ~ 16 km/s, implies T < 15,000 K. We detect O VI absorption at 1015 km/s at the 2-3 sigma level that may be associated with hot, X-ray emitting gas in the Virgo Cluster. We detect weak C III and O VI absorption in the IGM at z=0.12007; this absorber is predominantly ionized and has N(H+)/N(H I) > 4000/Z, where Z is the metallicity. Strong Galactic interstellar O VI is present between -100 and +100 km/s, with an additional high-velocity wing containing about 13% of the total O VI between +100 and +240 km/s. The broad O VI absorption wing likely traces the expulsion of hot gas out of the Galactic disk into the halo. A limit on the amount of diffuse O VI emission present 3.5 arc minutes off the sight line combined with the observed O VI column density toward 3C 273, implies n_e < 0.02 cm^-3 and P/k < 11,500 cm^-3 K for an assumed temperature of 3x10^5 K. (abbreviated version)
description: 59 pages, 15 figures, aastex condensed format, to appear in the Nov. 10, 2001 issue of the Astrophysical Journal
Paulianidia peyrierasi Lecoq 2008, n. sp.
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia peyrierasi

description: Paulianidia peyrierasi n. sp.
(Fig. 4B)
HOLOTYPE. — Madagascar Est, Périnet, route de la Grande Île, litière, A. Peyrieras, X.1973, 1 ♂ (MNHN).
PARATYPES. — Madagascar Est, massif Anjanaharibe nord, sentier Ambodihasina-Ambalarombe, 750-850 m, env. riv. Andramonta, 28.II.1996, tamisages en forêt humide; même localité, 600-700 m, 24-29.II.1996, J. Janák, P. Moravec, 2 ♂♂ (coll. Janák); 1 ♂, 1 ♀ (MNHN).
ÉTYMOLOGIE. — Je dédie cette espèce à son récolteur, André Peyrieras, qui a tant contribué par ses méthodes de récolte par tamisages et lavages de terre à la connaissance de la microfaune de la Grande Île.
DESCRIPTION
Longueur: 5-5,2 mm. Ailé. Avant-corps et élytres brun foncé, abdomen brun. Pattes et antennes ferrugineuses. Les paratypes sont un peu moins foncés, notamment la tête et le pronotum.
Tête un peu plus longue que large (R = 1,06). Les tempes deux fois plus longues que les yeux. La ponctuation forte et très dense sur toute la tête sauf au centre du disque où elle est seulement un peu moins dense. Tous les articles antennaires plus longs que larges, progressivement moins longs du deuxième au dixième qui est à peine oblong.
Pronotum un peu plus long que large (R = 1,07), presque aussi large que la tête (R = 1,06). Les bords latéraux en courbe régulière sur toute leur longueur. La ponctuation visiblement moins dense que celle de la tête, les points de même taille mais plus superficiels, moins enfoncés, à bords moins marqués, espacés de plus d’un diamètre. La bande médio-sagittale imponctuée, entière. Les dépressions basales de part et d’autre de cette bande, présentes.Tégument lisse et brillant. Écusson avec quelques points.
Élytres d’environ un cinquième plus longs que larges,les épaules bien marquées, d’un tiers plus larges que le pronotum. La ponctuation régulièrement répartie, les points un peu moins gros dans la moitié postérieure, espacés de plus d’un diamètre. Le tégument lisse.
Ponctuation abdominale très fine, espacée, plus grosse et plus serrée à la base des premiers segments. Tégument lisse sans traces de microsculpture.
Mâle: sternite du pygidium avec une échancrure en V ouvert sur le tiers environ de sa longueur.
Édéage: apex du lobe médian terminé par deux excroissances planes à bords arrondis comme deux oreilles plates et symétriques. Paramères étroits sur toute leur longueur, effilés à l’extrémité, à peine plus longs que le lobe médian.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on pages 593-594, DOI: 10.5281/zenodo.5390906
Additional file 1 of Outcomes of severe systemic rheumatic disease patients requiring extracorporeal membrane oxygenation
Creators: name: Bay, Pierre
name: Lebreton, Guillaume
name: Mathian, Alexis
name: Demondion, Pierre
name: Desnos, Cyrielle
name: Chommeloux, Juliette
name: Hékimian, Guillaume
name: Bréchot, Nicolas
name: Nieszkowska, Ania
name: Schmidt, Matthieu
name: Cohen-Aubart, Fleur
name: Leprince, Pascal
name: Luyt, Charles-Edouard
name: Amoura, Zahir
name: Combes, Alain
name: Pineton de Chambrun, Marc
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file1: Table S1. Supplementary characteristics of 90 SRD Patients Given ECMO Support. Table S2. Microbiological Findings for In-ICU–Acquired Infections of the 90 ECMO-Treated SRD Patients. Table S3. In-ICU Characteristics and Outcomes of the 48 VA-ECMO–Treated SRD Patients: Hospital Survivors vs. Nonsurvivors. Table S4. Univariable and Multivariable Analyses of Factors Associated with In-Hospital Mortality for the 48 VA-ECMO–Treated SRD Patients. Table S5. In-ICU Characteristics and Outcomes of the 42 VV-ECMO–Treated SRD Patients: Hospital Survivors vs. Nonsurvivors. Table S6. Univariable and Multivariable Analyses of Factors Associated with In-Hospital Mortality for the 42 VV-ECMO–Treated SRD Patients (DOCX 58 KB)
A central partition of molecular conformational space. I. Basic structures
Creators: name: Gabarro-Arpa, Jacques
Publisher: name: arXiv
Year: 2002
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Biological Physics (physics.bio-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: On the basis of empirical evidence from molecular dynamics simulations, molecular conformational space can be described by means of a partition of central conical regions characterized by the dominance relations between cartesian coordinates. This work presents a geometric and combinatorial description of this structure.
Cordalia permutata ASSING 2002
Creators: name: Assing, V.
name: J, Cordalia
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Cordalia
Cordalia permutata

description: Cordalia permutata ASSING 2002
M a t e r i a l e x a m i n e d: Nepal: 17 exs., Manaslu, Bara Pokhari, 28°15'N, 84°25'E, 2100 m, 29.IV.2005, leg. Schmidt (NME, cAss); 14 exs., Manaslu, Dudh Pokhari Lekh, upper Dordi Khola, 2300-2600 m, 15.-17.IV.2003, leg. Schmidt (NME, cAss); 2 exs., Manaslu, S Bara Pokhari, 2300 m, 8.IV.2003, leg. Schmidt (NME, cAss); 8 exs., Dhaulagiri, SE-slope, N Dwari village, upper Rahugat Khola, 2500 m, 13.-15.V.2002, leg. Schmidt (NME, cAss).
C o m m e n t: This recently described species is one of the most common representatives of the genus in Nepal and has been recorded also from Taiwan (ASSING 2002, 2006).
description: Published as part of Assing, V. & J, Cordalia, 2009, New species and additional records of Palaearctic Falagriini (Coleoptera: Staphylinidae: Aleocharinae), pp. 471-480 in Linzer biologische Beiträge 41 (1) on page 475, DOI: 10.5281/zenodo.5276207
A connection theoretic approach to sub-Riemannian geometry
Creators: name: Langerock, B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Differential Geometry (math.DG)
subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 53C05, 53C17, 58E25

description: We use the notion of generalized connection over a bundle map in order to present an alternative approach to sub-Riemannian geometry. Known concepts, such as normal and abnormal extremals, will be studied in terms of this new formalism. In particular, some necessary and sufficient conditions for the existence of abnormal extremals will be derived. We also treat the problem of characterizing those curves that verify both the nonholonomic equations and the so-called vakonomic equations for a `free' particle submitted to some kinematical constraints.
description: accepted for publication in J. Geom. Phys
Superconducting fluctuation current in a space with the Kerr metric
Creators: name: Kuratsuji, Hiroshi
name: Tsuchida, Satoshi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study a fluctuation current through a superconducting ring placed in a space with the Kerr metric. This attempt aims at exploring conceptual problem; namely, we are concerned with the question about the condensed state in an extreme space-time. The superconducting ring is supposed to be placed in the space surrounding the Kerr black hole (KBH) such that the rotating axis of the KBH penetrates the center of the ring. The formulation is based on the Landau-Ginzburg free energy functional of linear form. The resultant fluctuation current shows several peculiar features that reflect characteristic aspects of the KBH; that is, the effect of the Kerr metric gives rise to the shift of superconducting transition temperature as well as the scale change of absolute temperature.
description: 6 pages, 2 figures,
A fast, miniaturised in-vitro assay developed for quantification of lipase enzyme activity
Creators: name: Menden, Ariane
name: Davane Hall
name: Paris, Daniel
name: Venkatarian Mathura
name: Crawford, Fiona
name: Mullan, Michael
name: Crynen, Stefan
name: Ghania Ait-Ghezala
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The discovery of allosteric modulators is a multi-disciplinary approach, which is time- and cost-intensive. High-throughput screening combined with novel computational tools can reduce these factors. Thus, we developed an enzyme activity assay, which can be included in the drug discovery work-flow subsequent to the in-silico library screening. While the in-silico screening yields in the identification of potential allosteric modulators, the developed in-vitro assay allows for the characterisation of them. Candida rugosa lipase (CRL), a glyceride hydrolysing enzyme, has been selected for the pilot development. The assay conditions were adjusted to CRL’s properties including pH, temperature and substrate specificity for two different substrates. The optimised assay conditions were validated and were used to characterise Tropolone, which was identified as an allosteric modulator. In conclusion, the assay is a reliable, reproducible, and robust tool, which can be streamlined with in-silico screening and incorporated in an automated high-throughput screening workflow.
Paulianidia vicina Jarrige 1978
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia vicina

description: Paulianidia vicina Jarrige, 1978
 Paulianidia vicina Jarrige, 1978: 270.
HOLOTYPE. — Madagascar Centre, Andringitra sud, Andrianony, cirque Manjarivolo, 1300 m, FDHMA, 4.XI.1970 (mission CNRS, RCP 225), 1 ♀ (MNHN).
DESCRIPTION
Longueur: 5,4 mm. Ailé. Avant-corps et élytres brun rougeâtre, l’abdomen un peu plus clair, ainsi que les pattes, les antennes et les pièces buccales.
Tête subcirculaire, aussi longue que large. Les yeux à peine saillants. Les tempes moitié plus longues que les yeux, convexes.Troisième article antennaire moitié plus long que le précédent; le quatrième aussi long que le deuxième, les suivants jusqu’au huitième tous plus longs que larges. Les 9 et 10 subcarrés. Le dernier oblong, presque deux fois plus long que le précédent.Le disque densément ponctué, les points tangents entre eux au niveau du front, un peu plus espacés au centre du disque.
Pronotum convexe à peine plus étroit que la tête et plus long que large (R = 1,13). Les bords latéraux régulièrement convexes.La ponctuation plus forte et un peu plus espacée que celle de la tête, les points à bord atténué.La bande médiane imponctuée confuse, réduite à une courte élévation lisse antebasale.
Élytres un peu plus longs que larges ensemble (R = 1,07) et d’un tiers plus larges que le pronotum. La ponctuation plus forte et espacée en avant, progressivement plus fine vers le sommet.
Tergites finement et densément ponctués. Le tégument très finement strié en travers.
Mâle inconnu.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on page 594, DOI: 10.5281/zenodo.5390906
Post-AGB Stars in Globular Clusters and Galactic Halos
Creators: name: Bond, Howard E.
name: Alves, David R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss three aspects of post-AGB (PAGB) stars in old populations. (1) HST photometry of the nucleus of the planetary nebula (PN) K 648 in the globular cluster (GC) M15 implies a mass of 0.60 Msun, in contrast to the mean masses of white dwarfs in GCs of ~0.5 Msun. This suggests that K 648 is descended from a merged binary, and we infer that single Pop II stars do not produce visible PNe. (2) Yellow PAGB stars are the visually brightest stars in old populations (Mv ~ -3.3) and are easily recognizable because of their large Balmer jumps; thus they show great promise as a Pop II standard candle. Two yellow PAGB stars in the GC NGC 5986 have the same V magnitudes to within +/-0.05 mag, supporting an expected narrow luminosity function. (3) Using CCD photometry and a u filter lying below the Balmer jump, we have detected yellow PAGB stars in the halo of M31 and in its dwarf elliptical companion NGC 205. With the Milky Way zero point, we reproduce the Cepheid distance to M31, and find that NGC 205 is ~100 kpc further away than M31. The star counts imply a yellow PAGB lifetime of about 25,000 yr, and their luminosities imply masses near 0.53 Msun.
description: 6 pages, 2 figures. To appear in proceedings of Torun, Poland, workshop on "Post-AGB Objects (Proto-Planetary Nebulae) as a Phase of Stellar Evolution," ed. S.K. Gorny
Dielectronic Recombination (via N=2 --> N'=2 Core Excitations) and Radiative Recombination of Fe XX: Laboratory Measurements and Theoretical Calculations
Creators: name: Savin, D. W.
name: Behar, E.
name: Kahn, S. M.
name: Gwinner, G.
name: Saghiri, A. A.
name: Schmitt, M.
name: Grieser, M.
name: Repnow, R.
name: Schwalm, D.
name: Wolf, A.
name: Bartsch, T.
name: Mueller, A.
name: Schippers, S.
name: Badnell, N. R.
name: Chen, M. H.
name: Gorczyca, T. W.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have measured the resonance strengths and energies for dielectronic recombination (DR) of Fe XX forming Fe XIX via N=2 --> N'=2 (Delta_N=0) core excitations. We have also calculated the DR resonance strengths and energies using AUTOSTRUCTURE, HULLAC, MCDF, and R-matrix methods, four different state-of-the-art theoretical techniques. On average the theoretical resonance strengths agree to within ~30% which is significantly larger than the estimated relative experimental uncertainty of ~1 eV, which includes the predicted formation temperatures for Fe XX in an optically thin, low-density photoionized plasma with cosmic abundances, our experimental and theoretical results are in good agreement. We have also used our R-matrix results, topped off using AUTOSTRUCTURE for RR into J>=25 levels, to calculate the rate coefficient for RR of Fe XX. Our RR results are in good agreement with previously published calculations.
description: To be published in ApJS. 65 pages with 4 tables and lots of figures
Paulianidia ikoka Lecoq 2008, n. sp.
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia ikoka

description: Paulianidia ikoka n. sp.
(Fig. 5A)
HOLOTYPE. — Madagascar Est, massif Ambondrombe, env. Ikoka, crête Amboasa, 1300-1400 m, forêt pluviale, bord de ruisseau, 11-12.III.1996, J. Janák, P. Moravec, 1 ♂ (MNHUB).
PARATYPES. — Mêmes données que pour l’holotype, 1 ♀ (coll. Janák); 1 ♀ (MNHN).
ÉTYMOLOGIE. — Espèce récoltée aux environs de la localité d’Ikoka.
DESCRIPTION
Longueur: 5,1 mm. Ailé. Avant-corps et élytres noirs; abdomen à peine moins sombre, pattes, antennes et pièces buccales marron clair.
Tête aussi longue que large au niveau des yeux; les tempes moins de deux fois plus longues que les yeux (R = 1,75) en courbe régulière jusqu’au cou. Ponctuation céphalique dense, les points nontangents, à peine plus espacés au centre du disque. Tégument lisse et brillant entre les points. Articles antennaires tous plus longs que larges, notamment les sept premiers qui décroissent en longueur du troisième au septième.
Pronotum aussi long que la tête, très légèrement plus long que large, presque aussi large que la tête. Les bords latéraux en courbe très régulière, les angles inexistants.Ponctuation un peu moins forte que celle de la tête mais visiblement moins dense, les points séparés d’au moins un diamètre. La bande médiane étroite, irrégulière. Élytres rectangulaires, plus longs que larges (R = 1,14), nettement plus larges que le pronotum (R = 1,31). Épaules bien marquées; les bords latéraux à peine convexes. Ponctuation du tiers basal plus forte que celle du pronotum, les points séparés d’au moins un diamètre, progressivement moins forte jusqu’à l’apex.
Tergites finement et densément ponctués. Le tégument très finement strié en travers à l’exception du tergite du pygidium. Pubescence fine couchée vers l’arrière.
Mâle: bordure postérieure du sternite du pygidium avec une échancrure médiane en V à bords sinués. Bord postérieur du sternite du propygidium avec une large échancrure en U encadrée de deux petits prolongements membraneux.
Édéage: l’apex du lobe médian présente deux prolongements latéraux, chacun avec une petite dent retournée à la base. Paramères étroits et régulièrement rétrécis jusqu’à l’apex.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on pages 596-597, DOI: 10.5281/zenodo.5390906
Magnetic field of superconductive in-vacuo undulators in comparison with permanent magnet undulators
Creators: name: Moser, H. O.
name: Rossmanith, R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: During the last few years superconductive undulators with a period length of 3.8 mm and 14 mm have been built. In this paper scaling laws for these novel insertion devices are presented: a simple analytic formula is derived which describes the achievable magnetic field of a superconcuctive undulator as a function of gap-width and period length.
description: Accepted for publication in Nuclear Instruments and Methods in Physics Research, Section A
Falagrioma sherpa
Creators: name: Assing, V.
name: J, Cordalia
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Falagrioma
Falagrioma sherpa

description: Falagrioma sherpa (PACE 1986)
M a t e r i a l e x a m i n e d: Nepal: 6 exs., Kathmandu, Shivapuri Lekh, slope west of Bagmati river, 2000-2300 m, 22.-23.V.2005, leg. Schmidt (NME, cAss).
C o m m e n t: This species has become known only from Nepal (PACE 1986, 1991).
description: Published as part of Assing, V. & J, Cordalia, 2009, New species and additional records of Palaearctic Falagriini (Coleoptera: Staphylinidae: Aleocharinae), pp. 471-480 in Linzer biologische Beiträge 41 (1) on page 479, DOI: 10.5281/zenodo.5276207
Masses of ground-state mesons and baryons, including those with heavy quarks
Creators: name: Yin, Pei-Lin
name: Chen, Chen
name: Krein, Gastao
name: Roberts, Craig D.
name: Segovia, Jorge
name: Xu, Shu-Sheng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using a confining, symmetry-preserving regularisation of a vector$\times$vector contact interaction, we compute the spectra of ground-state pseudoscalar and vector $(f\bar g)$ mesons, scalar and axial-vector $(fg)$ diquarks, and $J^P=1/2^+, 3/2^+$ $(fgh)$ baryons, where $f,g,h \in \{u,d,s,c,b\}$. The diquark correlations are essentially dynamical and play a key role in formulating and solving the three-valence-quark baryon problems. The baryon spectrum obtained from this largely-algebraic approach reproduces the 22 known experimental masses with an accuracy of $2.9(2.4)$%. It also possesses the richness of states typical of constituent-quark models, predicting many heavy-quark baryons not yet observed. This study indicates that diquark correlations are an important component of all baryons; and owing to the dynamical character of the diquarks, it is typically the lightest allowed diquark correlation which defines the most important component of a baryon's Faddeev amplitude.
description: 18 pages, 5 figures, 5 tables
Interplay between Intra- and Intermolecular Charge Transfer in the Optical Excitations of J-Aggregates
Creators: name: Guerrini, Michele
name: Cocchi, Caterina
name: Calzolari, Arrigo
name: Varsano, Daniele
name: Corni, Stefano
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: In a first-principles study based on density functional theory and many-body perturbation theory, we address the interplay between intra- and intermolecular interactions in a J-aggregate formed by push-pull organic dyes by investigating its electronic and optical properties. We find that the most intense excitation dominating the spectral onset of the aggregate, i.e., the J-band, exhibits a combination of intramolecular charge transfer, coming from the push-pull character of the constituting dyes, and intermolecular charge transfer, due to the dense molecular packing. We also show the presence of a pure intermolecular charge-transfer excitation within the J-band, which is expected to play a relevant role in the emission properties of the J-aggregate. Our results shed light on the microscopic character of optical excitations of J-aggregates and offer new perspectives to further understand the nature of collective excitations in organic semiconductors.
description: published under ACS Authorchoice license
Carcinocephalus BERNHAUER 1903
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Carcinocephalus

description: Carcinocephalus BERNHAUER 1903
 Astacops BERNHAUER 1902: 61; preoccupied.
 Carcinocephalus BERNAUUER 1903: 592; replacement name.
 Scribaia LUZE 1906: 546; nov.syn.
 C o m m e n t: According to SCHEERPELTZ (1934) and ZANETTI (1987), the subgenus Scribaia LUZE 1906 (type species: Omalium blandum LUZE 1906) is distinguished from Carcinocephalus (type species: Omalium merkli EPPELSHEIM 1883) primarily by longer and more slender legs and antennae. These differences may be interpreted as adaptations to different habitats and are most certainly evidence of interspecific differentiation. However, in view of the criteria and standards commonly applied in the systematics of Staphylinidae, they are insufficient to justify a distinction at the subgeneric level. Moreover, from a practical viewpoint, a conservation of Scribaia would seem unnecessary, since both subgenera would be monotypical (see below and remark in introduction). Therefore, Scribaia is formally placed in synonymy with Carcinocephalus.
description: Published as part of Assing, V., 2009, On the Western Palaearctic species of Carcinocephalus (Coleoptera: Staphylinidae: Omaliinae), pp. 463-469 in Linzer biologische Beiträge 41 (1) on page 464, DOI: 10.5281/zenodo.5276201
Algebraic surfaces with quotient singularities - including some discussion on automorphisms and fundamental groups
Creators: name: Keum, J.
name: Zhang, D. -Q.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14J17, 14J50, 14F35

description: We survey some recent progress in the study of algebraic varieties X with log terminal singularities, especially, the uni-ruledness of the smooth locus X^0 of X, the fundamental group of X^0 and the automorphisms group on (smooth or singular) X when dim X = 2. The full automorphism groups of a few interesting types of K3 surfaces are described, mainly by Keum-Kondo. We conjecture that when X is Q-Fano then X^0 has a finite fundamental group, which had been proved if either dim X < 3 or the Fano index is bigger than dim X - 2. We also conjecture that when X is a log Enriques (e.g. a normal K3 or a normal Enriques) surface then either pi_1(X^0) is finite or X has an abelian surface as its quasi-etale cover, which has been proved by Catanese-Keum-Oguiso under some extra conditions.
description: 26 pages, Proc. Alg. Geom. in East Asia, Kyoto, 3-10 Aug 2001, A. Ohbuchi et al (eds), to appear
The Substellar Mass Function in sigma Orionis
Creators: name: Bejar, V. J. S.
name: Martin, E. L.
name: Osorio, M. R. Zapatero
name: Rebolo, R.
name: Navascues, D. Barrado y
name: Bailer-Jones, C. A. L.
name: Mundt, R.
name: Baraffe, I.
name: Chabrier, G.
name: Allard, F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We combine results from imaging searches for substellar objects in the sigma Orionis cluster and follow-up photometric and spectroscopic observations to derive a census of the brown dwarf population in a region of 847 arcmin^2. We identify 64 very low-mass cluster member candidates in this region. We have available three color (IZJ) photometry for all of them, spectra for 9 objects, and K photometry for 27% of our sample. These data provide a well defined sequence in the I vs I-J, I-K color magnitude diagrams, and indicate that the cluster is affected by little reddening despite its young age (~5 Myr). Using state-of-the-art evolutionary models, we derive a mass function from the low-mass stars (0.2 Msol) across the complete brown dwarf domain (0.075 Msol to 0.013 Msol), and into the realm of free-floating planetary-mass objects (<0.013 Msol). We find that the mass spectrum (dN/dm ~ m^{-alpha}) increases toward lower masses with an exponent alpha = 0.8+/-0.4. Our results suggest that planetary-mass isolated objects could be as common as brown dwarfs; both kinds of objects together would be as numerous as stars in the cluster. If the distribution of stellar and substellar masses in sigma Orionis is representative of the Galactic disk, older and much lower luminosity free-floating planetary-mass objects with masses down to about 0.005 Msol should be abundant in the solar vicinity, with a density similar to M-type stars.
description: Accepted for publication in ApJ. 19 pages, 3 figures included
Additional file 2 of Repetitive transcranial magnetic stimulation treatment for peripartum depression: systematic review & meta-analysis
Creators: name: Lee, Hyune June
name: Kim, Sung Min
name: Kwon, Ji Yean
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Science Policy
Mental Health

description: Additional file 2: Appendix 2. Risk assessment of selected literature.
Atheta (Microdota) detruncata ASSING 2006
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Atheta
Atheta detruncata

description: Atheta (Microdota) detruncata ASSING 2006
M a t e r i a l e x a m i n e d China: 1♀, Yunnan, Nujiang Lisu Aut. Pref., Gaoligong Shan, valley 18 km W Gongshan, 27°48'N, 98°30'E, 3020 m, mixed forest, litter, wood, and moss sifted, 7.VI.2007, leg. Wrase (cSch).
C o m m e n t: The original description of this recently described species is based on three females (ASSING 2006a). The above locality is not far from the type locality.
description: Published as part of Assing, V., 2009, New species and additional records of Homalotini, Athetini, Pygostenini, and Lomechusini from Yunnan, China (Coleoptera: Staphylinidae: Aleocharinae), pp. 485-507 in Linzer biologische Beiträge 41 (1) on page 491, DOI: 10.5281/zenodo.5276225
Paulianidia hova Lecoq 2008, n. sp.
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia hova

description: Paulianidia hova n. sp.
(Fig. 3C)
HOLOTYPE. — Madagascar Est, prov. Fianarantsoa, 7 km W Ranomafana, 1100 m, 22-31.X.1988, piège d’interception avec assiette jaune, piège Malaise en clairière, forêt pluviale de montagne, W. E. Steiner, 1 ♂ (USNM).
PARATYPES. — Madagascar Est, Fianarantsoa, R. N. Ranomafana, 1100-1200 m, Vohiparara, 21-24.I.1993, J. Janák, 3 ♂♂, 2 ♀♀ (coll. Janák); 2 ♂♂ (MNHN). — P. N. Ranomafana, Ambodiamontana, 850-1000 m, 26-27.I.1993, J. Janák, 1 ♀ (coll. Janák).
ÉTYMOLOGIE. — Du nom d’une caste malgache.
DESCRIPTION
Longueur: 5,5 mm. Ailé. Avant-corps et élytres noirs, abdomen brun foncé.Pattes et pièces buccales roux châtain. Antennes sombres, les derniers articles un peu éclaircis.
Tête un peu plus longue que large au niveau des yeux (R = 1,10). Tempes deux fois plus longues que les yeux, subrectilignes au départ des yeux puis s’arrondissant en arc jusqu’au cou.Ponctuation forte et dense, s’espaçant sur le disque où les points sont distants d’un peu moins d’un diamètre. Tégument lisse et brillant. Premier article antennaire aussi long que les deux suivants ensemble. Les 4-7 oblongs, les 8-10 subcarrés, le dernier en ogive aiguë.
Pronotum plus long que large (R = 1,13), aussi large que la tête; ses bords latéraux en courbe régulière, les angles antérieurs inexistants. Ponctuation forte mais moins dense que celle de la tête, les points distants d’au moins un diamètre. Une bande médiane imponctuée va du bord antérieur au bord postérieur avec de chaque côté une impression ante-basale. Écusson ponctué.
Élytres rectangulaires, un peu plus longs que larges et d’un cinquième plus larges que le pronotum. Ponctuation progressivement moins forte de la base à l’apex; les points séparés d’au moins un diamètre à la base.
Tergites à ponctuation fine, moyennement dense sur un tégument lisse et brillant sans trace de microréticulation.
Mâle: la bordure postérieure du sternite du pygidium est échancrée en forme de V largement ouvert à fond arrondi.
Édéage: paramères aussi longs que le lobe médian, effilés à l’extrémité.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on pages 590-592, DOI: 10.5281/zenodo.5390906
Far Ultraviolet Spectroscopic Explorer Observations of a Supernova Remnant in the Line of Sight to HD 5980 in the Small Magellanic Cloud
Creators: name: Hoopes, Charles G.
name: Sembach, Kenneth R.
name: Howk, J. Christopher
name: Blair, William P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report a detection of far ultraviolet absorption from the supernova remnant SNR 0057 - 7226 in the Small Magellanic Cloud (SMC). The absorption is seen in the Far Ultraviolet Spectroscopic Explorer (FUSE) spectrum of the LBV/WR star HD 5980. Absorption from O VI 1032 and C III 977 is seen at a velocity of +300 km/s with respect to the Galactic absorption lines, +170 km/s with respect to the SMC absorption. The O VI 1038 line is contaminated by H_2 absorption, but is present. These lines are not seen in the FUSE spectrum of Sk80, only ~1' (~17 pc) away from HD 5980. No blue-shifted O VI 1032 absorption from the SNR is seen in the FUSE spectrum. The O VI 1032 line in the SNR is well described by a Gaussian with FWHM=75 km/s. We find log N(O VI)=14.33-14.43, which is roughly 50% of the rest of the O VI column in the SMC (excluding the SNR) and greater than the O VI column in the Milky Way halo along this sight line. The N(C IV)/N(O VI) ratio for the SNR absorption is in the range of 0.12-0.17, similar to the value seen in the Milky Way disk, and lower than the halo value, supporting models in which SNRs produce the highly ionized gas close to the plane of the Galaxy, while other mechanisms occur in the halo. The N(C IV)/N(O VI) ratio is also lower than the SMC ratio along this sight line, suggesting that other mechanisms contribute to the creation of the global hot ionized medium in the SMC. The O VI, C IV, and Si IV apparent column density profiles suggest the presence of a multi-phase shell followed by a region of higher temperature gas.
description: 7 pages, 3 figures, 2 tables, uses emulateapj5.sty. Accepted for publication in ApJ Letters
Atom-in-jellium equations of state in the high energy density regime
Creators: name: Swift, Damian C.
name: Lockard, Thomas
name: Kraus, Richard G.
name: Benedict, Lorin X.
name: Sterne, Philip A.
name: Bethkenhagen, Mandy
name: Hamel, Sebastien
name: Bennett, Bard I.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent path-integral Monte Carlo and quantum molecular dynamics simulations have shown that computationally efficient average-atom models can predict thermodynamic states in warm dense matter to within a few percent. One such atom-in-jellium model has typically been used to predict the electron-thermal behavior only, although it was previously developed to predict the entire equation of state (EOS). We report completely atom-in-jellium EOS calculations for Be, Al, Si, Fe, and Mo, as elements representative of a range of atomic number and low-pressure electronic structure. Comparing the more recent method of pseudo-atom molecular dynamics, atom-in-jellium results were similar: sometimes less accurate, sometimes more. All these techniques exhibited pronounced effects of electronic shell structure in the shock Hugoniot which are not captured by Thomas-Fermi based EOS. These results demonstrate the value of a hierarchical approach to EOS construction, using average-atom techniques with shell structure to populate a wide-range EOS surface efficiently, complemented by more rigorous 3D multi-atom calculations to validate and adjust the EOS.