cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Presolar Silicon Carbide Grains of Types Y and Z: Their Molybdenum Isotopic Compositions and Stellar Origins
Creators: name: Liu, Nan
name: Stephan, Thomas
name: Cristallo, Sergio
name: Gallino, Roberto
name: Boehnke, Patrick
name: Nittler, Larry R.
name: Alexander, Conel M. O. 'D.
name: Davis, Andrew M.
name: Trappitsch, Reto
name: Pellin, Michael J.
name: Dillmann, Iris
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report Mo isotopic compositions of 37 presolar SiC grains of types Y (19) and Z (18), rare types commonly argued to have formed in lower-than-solar metallicity asymptotic giant branch (AGB) stars. Direct comparison of the Y and Z grain data with data for mainstream grains from AGB stars of close-to-solar metallicity demonstrates that the three types of grains have indistinguishable Mo isotopic compositions. We show that the Mo isotope data can be used to constrain the maximum stellar temperatures (TMAX) during thermal pulses in AGB stars. Comparison of FRUITY Torino AGB nucleosynthesis model calculations with the grain data for Mo isotopes points to an origin from low-mass (~1.5-3 Msun) rather than intermediate-mass (>3-~9 Msun) AGB stars. Because of the low efficiency of 22Ne(α,n)25Mg at the low TMAX values attained in low-mass AGB stars, model calculations cannot explain the large 30Si excesses of Z grains as arising from neutron capture, so these excesses remain a puzzle at the moment.
description: The Astrophysical Journal (Accepted)
Cavitas concava Uan 2001, sp. nov.
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Cavitas
Cavitas concava

description: Cavitas concava sp. nov.
(gures 1–5, 33–42)
 Female. Body (gures 5, 33) length 1.5 mm. H ead and thorax dark green, gaster brown; antennae yellow; hind coxae concolorous with thorax, fore and mid legs brown excepting tibia yellow.
 Head (gures 1–3) in front view subtriangle; clypeus small and lower margin emarginate, gena strongly converging to mouth; scrobe very deep, cavity-like (gure 34); scape completely encased in scrobe, vertex slightly convex and lateral area outside of scrobe in upper face with conspicuous projection (gures 2, 5, 35). Antennal (gures 36, 37) insertion below ventral line of eyes; scape not reaching the median ocellus; pedicellus about 1.3 times as long as broad, much longer than rst funicular segment; each funicular segment broader than long; clava as long as the last three funicular segments together; agellum plus pedicellus shorter than the head width. Relative measurements: head width 34, height 26, length 20, eye space 21, eye height 11, malar space 14, POL 5 OOL as 11 5 4.
Thorax convex (gures 5, 39), with weak reticulations. Pronotum narrower than mesoscutum, collar not margined. Notauli shallow and complete. Frenum with large and conspicuous areolations (gurs 39, 40). Propodeum with short median carina, nucha distinct (gure 38). Fore wing about 2.2 times as long as broad; basal cell bare and lower margin open; basal vein without hairs. Fore leg (gures 41, 42) short, tibia with one spur which is shorter than basitarsus; basitarsus with setae in serrate series and literally with three clavate pegs (gure 51). Gaster sessile, ovate, rst gastral tergite half length of gaster (gure 33). Relative measurements: pronotum length 4, mesoscutum length 15, scutellum 17 long, 24 wide, length of propodeum 5, marginal vein 13, postmarginal 2.5, stigmal vein 3 (gure 4); gaster width 33, length 40.
 Male. Body smaller than female; others very similar to female except antennae: funicular segments yellow and rst two or three subquadrate, last one slightly broader than long (gure 38), clava brown, distinctly shorter than last three funicular segments together; head in dorsal view with weak reticulation.
HOLOTYPE female, China, Hainan, Danxian (Nada), 24 May 1964, from coccids on litchi (Chen Tai-Lu).
PARATYPE, 1 1, same as holotype; China: Hainan, Danxian (Nada), 1 May 1964, 12 2, from coccids (Chen Tai-Lu); Hainan, Danxian (Nada), 14 May 1964, 1, from coccids (Chen Tai-Lu), Hainan, Qiongshan, 18 May 1964, 3 1, from coccids on litchi (Chen Tai-Lu).
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on pages 1589-1591
Open Source Real Time Operating Systems Overview
Creators: name: Straumann, Till
Publisher: name: arXiv
Year: 2001
Subjects: subject: Operating Systems (cs.OS)
subject: FOS: Computer and information sciences
subject: D.4

description: Modern control systems applications are often built on top of a real time operating system (RTOS) which provides the necessary hardware abstraction as well as scheduling, networking and other services. Several open source RTOS solutions are publicly available, which is very attractive, both from an economic (no licensing fees) as well as from a technical (control over the source code) point of view. This contribution gives an overview of the RTLinux and RTEMS systems (architecture, development environment, API etc.). Both systems feature most popular CPUs, several APIs (including Posix), networking, portability and optional commercial support. Some performance figures are presented, focusing on interrupt latency and context switching delay.
description: Talk at ICALEPCS 2001 Conference, Nov 2001, San Jose, USA, (WEBT001), 3 pages, LaTex
Quadratic Matrix Inequality Approach to Robust Adaptive Beamforming for General-Rank Signal Model
Creators: name: Huang, Yongwei
name: Vorobyov, Sergiy A.
name: Luo, Zhi-Quan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: The worst-case robust adaptive beamforming problem for general-rank signal model is considered. This is a nonconvex problem, and an approximate version of it (obtained by introducing a matrix decomposition on the presumed covariance matrix of the desired signal) has been well studied in the literature. Different from the existing literature, herein however the original beamforming problem is tackled. Resorting to the strong duality of linear conic programming, the robust adaptive beamforming problem for general-rank signal model is reformulated into an equivalent quadratic matrix inequality (QMI) problem. By employing a linear matrix inequality (LMI) relaxation technique, the QMI problem is turned into a convex semidefinite programming problem. Using the fact that there is often a positive gap between the QMI problem and its LMI relaxation, an approximate algorithm is proposed to solve the robust adaptive beamforming in the QMI form. Besides, several sufficient optimality conditions for the nonconvex QMI problem are built. To validate our results, simulation examples are presented, which also demonstrate the improved performance of the new robust beamformer in terms of the output signal-to-interference-plus-noise ratio.
ASCA X-ray observations of the disk wind in the dwarf nova Z Camelopardalis
Creators: name: Baskill, D. S.
name: Wheatley, P. J.
name: Osborne, J. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ASCA observations of the dwarf nova Z Camelopardalis during outburst and during a transition from quiescence to another outburst. At the beginning of the transition the X-ray count rate was an order of magnitude higher and the spectrum much harder than during the outburst. As the transition progressed, the spectrum remained hard as the X-ray flux decreased by a factor of 3, with no spectral softening. Spectral modelling reveals an optically-thin, high-temperature component (kT$\approx$10 keV) which dominates the transition observation and is also observed during outburst. This is expected from material accreting onto the white dwarf surface. The outburst spectra require additional emission at lower temperatures, either through an additional discrete temperature component, or a combination of a cooling flow model and an ionised absorber. Fits to both observations show large amounts of absorption ($N_H=8-9\times10^{21}$cm$^{-2}$), two orders of magnitude greater than the measured interstellar value, and consistent with UV measurements of the outburst. This suggests that a disk wind is present even in the earliest stages of outburst, possibly before the outburst heating wave has reached the boundary layer.
description: 9 pages, 9 figures, MNRAS Accepted
Moranila californica
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Moranila
Moranila californica

description: Moranila californica (H owa rd)
(gures 12–14)
 Tomocera californica H oward, 1881: 352, 368–369.
 Moranila testaceipes Cameron, 1883: 188–189. Synonymized by Howard, 1896: 165.
 Tomocera ceroplastis Perkins, 1906: 75. Synonymized by Burks, 1978: 783.
 Tomocera glabriventris Girault, 1915: 208. Synonymized by Burks, 1978: 783.
 Tomocera X aviceps Girault, 1915: 208. Synonymized by Burks, 1978: 783.
 Eunotomyi a festiva M asi, 1917: 195–197. Synonymized by BoucÏek, 1988: 357.
 Moranila californica (H oward); Burks, in K rombein, 1958: 75. G raham, 1969: 70–71. M ani, 1989: 550–551. Berry, 1995: 33–35.
 Material examined. China: Hainan, 22 May 1964, 2 3, from coccids on oak tree (Quercus ?) (Liao Ding-Xi); Hainan, 2 April 1964, 10, on Engelhardtia colebrookiana Lindl, ex. Wall (Liao Ding-Xi); Hainan, 8 May 1964, 9, on oak tree (Quercus ?) (Liao Ding-Xi); Hainan, Jianfengling, 28 July 1964, 1 3 (Liao Ding-Xi); Hebei, Xinglong, 30 M arch 1964, 3 3, from Coccus sp. (Liao Ding-Xi); Hebei, Xinglong, 31 March 1964, 1, from Rosanococcus sp. (Liao Ding-Xi); Yunnan, Jingdong, 4 May 1974, 1 (Liao Ding-Xi); Zhejiang, Hangzhou, 3 7, from Eriococcus sp. (Liao Ding-Xi); Anhui, 26 September 1965, 3 (Chen Tai-Lu).
 Biology. This species is mainly a parasitoid of scale insects, particularly Coccidae, and rarely as a hyperparasitoid through encyrtids. In China, this species was reared from coccids on oak tree and Rosanococcus sp. The known hosts are listed as follows: Asterolecaniidae: Asterolecanium pustulans (Cockerell); Coccidae: Ceroplastes ceriferus (F.), C. X oridensis (Comstock), C. rubens Maskell, C. rusci (L.); Coccus hesperidum L., Parasaissetia nigra Takahashi, Saissetia coOEeae (Walker), S. hemisphaerica (Targioni-Tozzetti), S. oleae (Olivier); Pseudococcidae: Antonina bambusae (M askell).
 Distribution. Cosmopolitan. China (Hainan, Yunnan, Zhejiang, Anhui and H ebei).
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on pages 1594-1596
High-resolution Near-Infrared Images and Models of the Circumstellar Disk in HH 30
Creators: name: Cotera, A. S.
name: Whitney, B. A.
name: Young, E.
name: Wolff, M. J.
name: Wood, K.
name: Povich, M.
name: Schneider, G.
name: Rieke, M.
name: Thompson, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Hubble Space Telescope (HST) Near-Infrared Camera and Multi-object Spectrometer (NICMOS) observations of the reflection nebulosity associated with the T Tauri star HH 30. The images show the scattered light pattern characteristic of a highly inclined, optically thick disk with a prominent dustlane whose width decreases with increasing wavelength. The reflected nebulosity exhibits a lateral asymmetry in the upper lobe on the opposite side to that reported in previously published Wide Field Planetary Camera 2 (WFPC2) images. The radiation transfer model which most closely reproduces the data has a flared accretion disk with dust grains larger than standard interstellar medium grains by a factor of approximately 2.1. A single hotspot on the stellar surface provides the necessary asymmetry to fit the images and is consistent with previous modeling of the light curve and images. Photometric analysis results in an estimated extinction of Av>~80; however, since the photometry measures only scattered light rather than direct stellar flux, this a lower limit. The radiative transfer models require an extinction of Av = 7,900.
description: Accepted for publication in Ap.J
Construction of anti-de Sitter-like spacetimes using the metric conformal Einstein field equations: the tracefree matter case
Creators: name: Carranza, Diego A.
name: Kroon, Juan A. Valiente
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Using a metric conformal formulation of the Einstein equations, we develop a construction of 4-dimensional anti-de Sitter-like spacetimes coupled to tracefree matter models. Our strategy relies on the formulation of an initial-boundary problem for a system of quasilinear wave equations for various conformal fields by exploiting the conformal and coordinate gauges. By analysing the conformal constraints we show a systematic procedure to prescribe initial and boundary data. This analysis is complemented by the propagation of the constraints, showing that a solution to the wave equations implies a solution to the Einstein field equations. In addition, we study three explicit tracefree matter models: the conformally invariant scalar field, the Maxwell field and the Yang-Mills field. For each one of these we identify the basic data required to couple them to the system of wave equations. As our main result, we establish the local existence and uniqueness of solutions for the evolution system in a neighbourhood around the corner, provided compatibility conditions for the initial and boundary data are imposed up to a certain order.
description: 25 pages
Additional file 1 of Sensitivity to thyroid hormone indices are associated with papillary thyroid carcinoma in Chinese patients with thyroid nodules
Creators: name: Sun, Jie
name: Liu, Jie
name: Wu, Ting-ting
name: Gu, Zhi-yuan
name: Zhang, Xiao-wen
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1.
Operads, deformation theory and F-manifolds
Creators: name: Merkulov, S. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: It is shown that every algebra over the chain operad of the little disks operad gives naturally rise to a Hertling-Manin's F-manifold, that is a smooth manifold equipped with an integrable graded commutative associative product on the tangent sheaf. In particular, moduli spaces of extended deformations of complex/symplectic structures are shown to have a canonical structure of F-manifold. With the help of the $G_\infty$-operad a strong homotopy version of the notion of F-manifold is constructed. Among natural examples of $F_\infty$-manifolds one finds formal manifolds associated with the Hochschild cohomology of an associative algebra and with the singular cohomology of an arbitrary compact topological space.
description: LaTeX, 39 pages; citations added
Data Access - Experiences Implementing an Object Oriented Library on Various Platforms
Creators: name: Lange, R.
name: Hill, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Software Engineering (cs.SE)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences
subject: D.1.5; D.2.13

description: Data Access will be the next generation data abstraction layer for EPICS. Its implementation in C++ brought up a number of issues that are related to object oriented technology's impact on CPU and memory usage. What is gained by the new abstract interface? What is the price that has to be paid for these gains? What compromises seem applicable and affordable? This paper discusses tests that have been made about performance and memory usage as well as the different measures that have been taken to optimize the situation.
description: Poster paper submitted to ICALEPCS'01, San Jose, Nov. 2001, PSN# THAP015, 3 pages, PDF (source: M$ Office 2000)
The Quiescent Spectrum of the AM CVn star CP Eri
Creators: name: Groot, Paul J.
name: Nelemans, Gijs
name: Steeghs, Danny
name: Marsh, Tom
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We used the 6.5m MMT to obtain a spectrum of the AM CVn star CP Eri in quiescence. The spectrum is dominated by He I emission lines, which are clearly double peaked with a peak-to-peak separation of ~1900 km/s. The spectrum is similar to that of the longer period AM CVn systems GP Com and CE 315, linking the short and the long period AM CVn systems. In contrast with GP Com and CE 315, the spectrum of CP Eri does not show a central 'spike' in the line profiles, but it does show lines of SiII in emission. The presence of these lines indicates that the material being transferred is of higher metallicity than in GP Com and CE 315, which, combined with the low proper motion of the system, probably excludes a halo origin of the progenitor of CP Eri. We constrain the primary mass to M_1>0.27 M_sun and the orbital inclination to 33 degr < i < 80 degr. The presence of the He I lines in emission opens up the possibility for phase resolved spectroscopic studies which allows a determination of the system parameters and a detailed study of helium accretion disks under highly varying circumstances.
description: 12 pages, 2 figures, accepted for publication in ApJ Letters
Additional file 3: of Clinical and immunological control of experimental autoimmune encephalomyelitis by tolerogenic dendritic cells loaded with MOG-encoding mRNA
Creators: name: Derdelinckx, Judith
name: Mansilla, María
name: Laere, Maxime De
name: Wai-Ping Lee
name: Navarro-Barriuso, Juan
name: Wens, Inez
name: Nkansah, Irene
name: Daans, Jasmijn
name: Reu, Hans De
name: Keliris, Aneta Jolanta
name: Audekerke, Johan Van
name: Vanreusel, Verdi
name: Pieters, Zoë
name: Linden, Annemie Van Der
name: Verhoye, Marleen
name: Molenberghs, Geert
name: Niel Hens
name: Goossens, Herman
name: Willekens, Barbara
name: Cras, Patrick
name: Ponsaerts, Peter
name: Zwi Berneman
name: Martínez-Cáceres, Eva
name: Cools, Nathalie
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology

description: Figure S3. Nucleotide sequence of the Sig-full length MOG-LAMP-3 and Sig-extracellular MOG-LAMP-3 constructs. (PDF 385 kb)
Decorosa aladecoris Opitz 2008, new species
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Decorosa
Decorosa aladecoris

description: Decorosa aladecoris, new species   Figures 1, 34, 39, 42, 46
HOLOTYPE: Female. DOMINIC. REP.: La Vega, Constanza, 1160 m, 30AUG1988, beating in secondary pine guava forest, M. A. Ivie, T. K. Philips & K. A. Johnson (USNM). (Specimen mounted on on minuten pin in neoprene block; gender label and metathoracic wing mounted on support card; locality label; holotype label).
 PARATYPES: Three specimens: Dominican Republic: La Vega: Estación Cabanito, 20- VII-1996, R. Turnbow (RHTC, 1); Cordillera Central, 4.1 km SW El Convento, 18 ° 50 9 N 70 ° 42 9 W, 31-IV-2003, 1729 m, disturbed evergreen forest with pine canopy trap, J. Rawlins, R. Davidson, C. Young, C. Nuñez, P. Acevedo (CMNH, 1); Loma Casablito, 16.0 km NW Bonao, 19 ° 02 ° N 70 ° 31 9 W, 28-IV- 2003. 1487 m, evergreen cloud forest at summit, canopy trap, J. Rawlins, R. Davidson, C. Young, C. Nuñez, P. Acevedo (WOPC, 1).
DIAGNOSIS: From congeners these beetles are distinguished by the uniform dark brown coloration of the cranium and pronotum, and by the color pattern on the elytral disc (fig, 1).
 DESCRIPTION: Size: Length 4.0 mm; width 1.2 mm. Integumental Color: Cranium and pronotum dark brown; antennae yellow; elytra as in figure 1; legs yellow; venter dark brown. Vestiture: Cranium and pronotum densely vested with pale decumbent setae. Head: Vertex much wider than width of eye (27:13); ratio of head width to pronotal width 1.05 (62:59); antennal form similar to antenna depicted in figure 4. Thorax: Pronotum only slightly longer than broad (60:58); pronotal lateral tubercle obtuse; anterior margin conspicuously wider than posterior margin (58:50); apical region of protibial anterior margin with 3 spines; seventh row of elytral punctations begins slightly anterior to elytral middle. Abdomen: Aedeagus as in figure 34.
VARIATION: There is some variation in the extent of dark and light coloration in the most distal region of the elytral disc.
NATURAL HISTORY: Specimens were collected during May, July, and August, one by beating secondary vegetation in a pine/guava forest at 1160 m. Two specimens were captured in canopy traps, one in disturbed evergreen forest with pine at 1729 m, the other at the summit of an evergreen cloud forest at 1487 m.
DISTRIBUTION (fig. 46): Known only from the highlands of the La Vega Province of the Dominican Republic.
 ETYMOLOGY: The specific epithet is a Latin compound name that stems from the noun ala (‘‘wing’’) and decoris (‘‘adorned’’). I refer to the ornate markings on the elytral disc.
description: Published as part of Opitz, Weston, 2008, Classification, Natural History, and Evolution of Epiphloeinae (Coleoptera: Cleridae). Part V. Decorosa Opitz, a New Genus of Checkered Beetles from Hispaniola with Description of Its Four New Species, pp. 1-20 in American Museum Novitates 3628 (1) on page 6, DOI: 10.1206/599.1, http://zenodo.org/record/5389946
An extended catalog of galaxy-galaxy strong gravitational lenses discovered in DES using convolutional neural networks
Creators: name: Jacobs, C.
name: Collett, T.
name: Glazebrook, K.
name: Buckley-Geer, E.
name: Diehl, H. T.
name: Lin, H.
name: McCarthy, C.
name: Qin, A. K.
name: Odden, C.
name: Escudero, M. Caso
name: Dial, P.
name: Yung, V. J.
name: Gaitsch, S.
name: Pellico, A.
name: Lindgren, K. A.
name: Abbott, T. M. C.
name: Annis, J.
name: Avila, S.
name: Brooks, D.
name: Burke, D. L.
name: Rosell, A. Carnero
name: Kind, M. Carrasco
name: Carretero, J.
name: da Costa, L. N.
name: De Vicente, J.
name: Fosalba, P.
name: Frieman, J.
name: Garcia-Bellido, J.
name: Gaztanaga, E.
name: Goldstein, D. A.
name: Gruen, D.
name: Gruendl, R. A.
name: Gschwend, J.
name: Hollowood, D. L.
name: Honscheid, K.
name: Hoyle, B.
name: James, D. J.
name: Krause, E.
name: Kuropatkin, N.
name: Lahav, O.
name: Lima, M.
name: Maia, M. A. G.
name: Marshall, J. L.
name: Miquel, R.
name: Plazas, A. A.
name: Roodman, A.
name: Sanchez, E.
name: Scarpine, V.
name: Serrano, S.
name: Sevilla-Noarbe, I.
name: Smith, M.
name: Sobreira, F.
name: Suchyta, E.
name: Swanson, M. E. C.
name: Tarle, G.
name: Vikram, V.
name: Walker, A. R.
name: Zhang, Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We search Dark Energy Survey (DES) Year 3 imaging for galaxy-galaxy strong gravitational lenses using convolutional neural networks, extending previous work with new training sets and covering a wider range of redshifts and colors. We train two neural networks using images of simulated lenses, then use them to score postage stamp images of 7.9 million sources from the Dark Energy Survey chosen to have plausible lens colors based on simulations. We examine 1175 of the highest-scored candidates and identify 152 probable or definite lenses. Examining an additional 20,000 images with lower scores, we identify a further 247 probable or definite candidates. After including 86 candidates discovered in earlier searches using neural networks and 26 candidates discovered through visual inspection of blue-near-red objects in the DES catalog, we present a catalog of 511 lens candidates.
description: Accepted for publication in ApJ Supplement Series
Eunotus aequalivena Uan 2001, sp. nov.
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Eunotus
Eunotus aequalivena

description: Eunotus aequalivena sp. nov.
(gures 20, 21)
 Female. Body length 2.1 mm. Body black; antenna brown, excepting scape and pedicellus deep yellow; coxae, legs, tibiae reddish brown.
 Head in front view, clypeal margin emarginate, gena strongly exceeding mouth. Antennal insertion above clypeal margin; antenna (gure 20) with scape not reaching the median ocellus; pedicellus about twice as long as broad, and longer than rst funicular segment; rst funicular segment much shorter than the second; the second quadrate, the fth transverse; clava about 1.8 times as long as broad; agellum plus pedicellus shorter than head width. Relative measurements: head width 52, height 37, length 21, eyes height 18, scape 18, POL 5 OOL as 16 5 5.
Thorax convex; pronotum narrower than mesoscutum, collar not margined; notauli deep and complete; scutellum without frenal line; propodeum with slightly tooth-like median carina, nucha distinct. Fore wing (gure 21) densely hairy, without speculum. G aster sessile, ovate, rst gastral tergite about three- fths length of gaster. Relative measurements: pronotum length 5, mesoscutum length 23, scutellum 31 long and 29 wide, fore wing length 110, width 48, marginal vein 10, postmarginal 11, stigmal vein 10; gaster width 55, length 71.
 Male. Unknown.
 E. aequalivena is very similar to E. strenus except for the marginal vein as long as the stigmal (gure 21); POL 5 OOL as 3 5 1. E. strenus with marginal vein about 1.5 times as long as the stigmal (gure 19); POL 5 OOL as 4 5 1.
HOLOTYPE female, China, Xinjiang, Korla, from coccids, July 1956 (Zhang Xui-Z u).
PARATYPE, 1, same as holotype.
 Biology. Reared from coccids.
 Distribution. China (Xianjiang).
 Eunotus cretaceus Walker (gures 22, 23) Eunotus cretaceus Walker, 1834: 298.
 Eunotus festucae Masi, 1928: 128.
 Eunotus cretaceus Walker; M asi, 1931: 426–428.
 Eunotus (Eunotus) cretaceus Walker; G raham, 1969: 72.
 Eunotus cretaceus Walker, BoucÏek, 1972: 281–282.
Material examined: China: Gansu, Gulang, August 1980, 3 1 (Guo Yu-Ling); N ei M ongol, 2 September 1981, 1 (Liao D ing-Xi).
 Biology. According to BoucÏek (1972), this species develops as predator on the eggs of the following coccids on grasses: Eriopeltis festucae (Fonscolombe), (Masi, 1928, 1931), E. agropyri Borchsenius, E. strelkovi Borchsenius (Graham, 1969), Scythia festuceti (S Ï ulc).
 Distribution. Europe and Palearctic region, including China (Gansu, Nei M ongo l), Austria, F rance, G eorgia, G ermany, H ungary, Italy, M oldova, R ussia, U kraine, Sweden and U K.
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on pages 1598-1599
Radio Emission and the Timing Properties of the Hard X-ray State of GRS 1915+105
Creators: name: Muno, M. P.
name: Remillard, R. A.
name: Morgan, E. H.
name: Waltman, E. B.
name: Dhawan, V.
name: Hjellming, R. M.
name: Pooley, G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We combine a complete sample of 113 pointed observations taken with the Rossi X-ray Timing Explorer between 1996-1999, monitoring observations taken with the Ryle telescope and the Green Bank Interferometer, and selected observations with the Very Large Array to study the radio and X-ray properties of GRS 1915+105 when its X-ray emission is hard and steady. We establish that radio emission always accompanies the hard-steady state of GRS 1915+105, but that the radio flux density at 15.2 GHz and the X-ray flux between 2-200 keV are not correlated. Therefore we study the X-ray spectral and timing properties of GRS 1915+105 using three approaches: first, by describing in detail the properties of three characteristic observations, then by displaying the time evolution of the timing properties during periods of both faint and bright radio emission, and lastly by plotting the timing properties as a function of the the radio flux density. We find that as the radio emission becomes brighter and more optically thick, 1) the frequency of a ubiquitous 0.5-10 Hz QPO decreases, 2) the Fourier phase lags between hard (11.5-60 keV) and soft (2-4.3 keV) in the frequency range of 0.01-10 Hz change sign from negative to positive, 3) the coherence between hard and soft photons at low frequencies decreases, and 4) the relative amount of low frequency power in hard photons compared to soft photons decreases. We discuss how these results reflect upon basic models from the literature describing the accretion flow around black holes and the possible connection between Comptonizing electrons and compact radio jets.
description: 22 pages with 8 figures and 2 tables in emulateapj style. Submitted to ApJ
Additional file 4 of Genetically determined blood pressure, antihypertensive medications, and risk of Alzheimer’s disease: a Mendelian randomization study
Creators: name: Ou, Ya-Nan
name: Yang, Yu-Xiang
name: Shen, Xue-Ning
name: Ma, Ya-Hui
name: Chen, Shi-Dong
name: Dong, Qiang
name: Tan, Lan
name: Yu, Jin-Tai
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4. Genome-wide significant and independent SNPs that were used as instruments for DBP.
Additional file 2: of Analysis of the genetically tractable crustacean Parhyale hawaiensis reveals the organisation of a sensory system for low-resolution vision
Creators: name: Ramos, Ana
name: Gustafsson, Ola
name: Labert, Nicolas
name: Salecker, Iris
name: Dan-Eric Nilsson
name: Averof, Michalis
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Trimmed alignment of opsin sequences. (DOCX 46 kb)
On the Nature of the NGC 1275 System
Creators: name: Conselice, Christopher J.
name: Gallagher, John S.
name: Wyse, Rosemary F. G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Sub-arcsecond images, taken in B, R, and H-Alpha filters, and area spectroscopy obtained with the WIYN 3.5-m telescope provide the basis for an investigation of the unusual structures in the stellar body and ionized gas in and around the Perseus cluster central galaxy, NGC 1275. Our H-Alpha filter is tuned to gas at the velocity of NGC 1275, revealing complex, probably unresolved, small-scale features in the extended ionized gas, located up to 50/h kpc from NGC 1275. The mean H-Alpha surface brightness varies little along the outer filaments; this, together with the complex excitation state demonstrated by spectra, imply that the filaments are likely to be tubes, or ribbons, of gas. The morphology, location and inferred physical parameters of the gas in the filaments are consistent with a model whereby the filaments form through compression of the intracluster gas by relativistic plasma emitted from the active nucleus of NGC 1275. Imaging spectroscopy with the Densepak fiber array on WIYN suggests partial rotational support of the inner component of low velocity ionized gas. We confirm and extend evidence for features in the stellar body of NGC 1275, and identify outer stellar regions containing very blue, probably very young, star clusters. We interpret these as evidence for recent accretion of a gas-rich system, with subsequent star formation. We suggest that two main processes, which may be causally connected, are responsible for the rich phenomenology of the NGC 1275 system -- NGC 1275 experienced a recent merger/interaction with a group of gas-rich galaxies, and recent outflows from its AGN have compressed the intracluster gas, and perhaps the gas in the infalling galaxies, to produce a complex web of filaments. (Abridged)
description: AJ, accepted; a recommended full resolution version is available at http://www.astro.wisc.edu/~chris/pera.ps
Eunotus applanatus Uan 2001, sp. nov.
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Eunotus
Eunotus applanatus

description: Eunotus applanatus sp. nov.
(gures 24, 43–50)
 Female. Body length 2.0–2.2 mm. Body black; antenna black; legs cocolorous with body except tarsi yellow.
 Head (gure 43) in front view, clypeal margin emarginate, genae strongly exceeding mouth. Antennal insertion above clypeal margin; antenna (gures 44–46) with a very small anellus; scape not reaching the median ocellus; pendicellus about twice as long as broad, and longer than rst funicular segment; rst funicular segment slightly shorter than the second, and without sensilla; the second to the fth quadrate or sub-subquadrate, and with a row of large sensilla; clava very swollen, about 1.8 times as long as broad; agellum plus pedicellus shorter than head width. R elative measurements: head width 40, height 29, length 20, eyes height 16, scape 16, agellum plus pedicellus 30, POL 5 OOL as 12.5 5 2.5.
Thorax at, reticulate and with hairs (gure 47); pronotum narrower than mesoscutum, collar not margined; notauli deep and complete; scutellum without frenal line; propodeum (gure 48) with slightly tooth-like median carina, plica complete, nucha distinct. Fore wing densely hairy. Gaster sessile, ovate, rst gastral tergite near four- fth the length of the gaster. Relative measurements: pronotum 5 long and 32 wide, mesoscutum 17 long and 35 wide, scutellum 20 long and 20 wide, fore wing 88 long and 40 wide, marginal vein 15, postmarginal 7.5, stigmal vein 5; gaster width 43, length 50.
 Male. Unknown.
 Eunotus applanatus diOEers from all described species by having one anellus and ve funicular segments (gure 44).
HOLOTYPE female, China, Beijing, Tiantan Park, April 1997 (Zhu Chao-Dong).
PARATYPE, 9, same as holotype.
 Biology. Host unknown.
 Distribution. China (Beijing).
 Eunotus acutus Kurdjumov (gure 25) Eunotus acutus K urdjumov, 1912: 330–331.
 Eunotus acutus K urdjumov; M asi, 1931: 430–431.
 Eunotus (Eunotus) acutus K urdjumov; G raham, 1969: 73–74.
 Eunotus acutus K urdjumov; BoucÏek, 1972: 285–286.
 Material examined. China, Beijing, 22 June 1955, 8 (Zhang Dai-Xiang); Shandong, Pingyi, 9 October 1958, 2 (Liao Ding-Xi).
 Biology. The recorded hosts are listed as following coccids: Eriococcus agropyri, E. Greeni and Greenisca placida.
 Distribution. Palearctic region, including China (Beijing, Shandong), Czechoslovakia, Poland, R ussia, U kraine.
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on pages 1599-1601
Explosions and Outflows during Galaxy Formation
Creators: name: Martel, Hugo
name: Shapiro, Paul R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider an explosion at the center of a halo which forms at the intersection of filaments inside a cosmological pancake, a convenient test-bed model for galaxy formation. ASPH/P3M simulations reveal that such explosions are anisotropic. The energy and metals are channeled into the low density regions, away from the pancake. The pancake remains essentially undisturbed, even if the explosion is strong enough to blow away all the gas located inside the halo and reheat the IGM surrounding the pancake. Infall quickly replenishes this ejected gas and gradually restores the gas fraction as the halo continues to grow. Estimates of the collapse epoch and SN energy-release for galaxies of different mass in the CDM model can relate these results to scale-dependent questions of blow-out and blow-away and their implication for early IGM heating and metal enrichment and the creation of gas-poor dwarf galaxies.
description: To appear in "The 20th Texas Symposium on Relativistic Astrophysics", eds. H. Martel and J.C. Wheeler, AIP, in press (2001) (3 pages, 2 figures)
Numerical estimation of entropy loss on dimerization: improved prediction of the quaternary structure of the GCN4 leucine zipper
Creators: name: Vinals, Jorge
name: Kolinski, Andrzej
name: Skolnick, Jeffrey
Publisher: name: arXiv
Year: 2002
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: A lattice based model of a protein is used to study the dimerization equilibrium of the GCN4 leucine zipper. Replica exchange Monte Carlo is used to determine the free energy of both the monomeric and dimeric forms as a function of temperature. The method of coincidences is then introduced to explicitly calculate the entropy loss associated with dimerization, and from it the free energy difference between monomer and dimer, as well as the corresponding equilibrium reaction constant. We find that the entropy loss of dimerization is a strong function of energy (or temperature), and that it is much larger than previously estimated, especially for high energy states. The results confirm that it is possible to study the dimerization equilibrium of GCN4 at physiological concentrations within the reduced representation of the protein employed.
Determining the Transport of Magnetic Helicity and Free Energy in the Sun's Atmosphere
Creators: name: Schuck, Peter W.
name: Antiochos, Spiro K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The most important factors determining solar coronal activity are believed to be the availability of magnetic free energy and the constraint of magnetic helicity conservation. Direct measurements of the helicity and magnetic free energy in the coronal volume are difficult, but their values may be estimated from measurements of the helicity and free energy transport rates through the photosphere. We examine these transport rates for a topologically open system such as the corona, in which the magnetic fields have a nonzero normal component at the boundaries, and derive a new formula for the helicity transport rate at the boundaries. In addition, we derive new expressions for helicity transport due to flux emergence/submergence versus photospheric horizontal motions. The key feature of our formulas is that they are manifestly gauge invariant. Our results are somewhat counterintuitive in that only the lamellar electric field produced by the surface potential transports helicity across boundaries, and the solenoidal electric field produced by a surface stream function does not contribute to the helicity transport. We discuss the physical interpretation of this result. Furthermore, we derive an expression for the free energy transport rate and show that a necessary condition for free energy transport across a boundary is the presence of a closed magnetic field at the surface, indicating that there are current systems within the volume. We discuss the implications of these results for using photospheric vector magnetic and velocity field measurements to derive the solar coronal helicity and magnetic free energy, which can then be used to constrain and drive models for coronal activity.
description: 35 pages, 3 figures, Accepted for Publication in the Astrophysical Journal
Electroteleia Brues 1940
Creators: name: Johnson, Norman F.
name: Masner, Lubomír
name: Musetti, Luciana
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Scelionidae
Electroteleia

description: Electroteleia Brues   Figures 1–6
description: Published as part of Johnson, Norman F., Masner, Lubomír & Musetti, Luciana, 2008, Review of Genera of the Tribe Sparasionini (Hymenoptera: Platygastroidea, Scelionidae), and Description of Two New Genera from the New World, pp. 1-24 in American Museum Novitates 3629 (1) on page 4, DOI: 10.1206/578.1, http://zenodo.org/record/5390053
Descartes' rule of signs and moduli of roots
Creators: name: Kostov, Vladimir Petrov
Publisher: name: arXiv
Year: 2019
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics

description: A hyperbolic polynomial (HP) is a real univariate polynomial with all roots real. By Descartes' rule of signs a HP with all coefficients nonvanishing has exactly $c$ positive and exactly $p$ negative roots counted with multiplicity, where $c$ and $p$ are the numbers of sign changes and sign preservations in the sequence of its coefficients. For $c=1$ and $2$, we discuss the question: When the moduli of all the roots of a HP are arranged in the increasing order on the real half-line, at which positions can be the moduli of its positive roots depending on the positions of the sign changes in the sequence of coefficients?
Additional file 1: of Analysis of the genetically tractable crustacean Parhyale hawaiensis reveals the organisation of a sensory system for low-resolution vision
Creators: name: Ramos, Ana
name: Gustafsson, Ola
name: Labert, Nicolas
name: Salecker, Iris
name: Dan-Eric Nilsson
name: Averof, Michalis
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Opsin sequence accession numbers and spectral information. (PDF 65 kb)
Cephaleta brunniventris Motschulsky 1859
Creators: name: Uan, H Ui Xiao D A-Wei H
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Cephaleta
Cephaleta brunniventris

description: Cephaleta brunniventris M otschulsky
(gures 29, 30)
 Cephaleta purpureiventris Motschulsky, 1859: 173.
 Cephaleta brunniventris Motschulsky, 1859: 174.
 Pteromalus magniceps Walker, 1860: 369. Synonymized by BoucÏek, Subba R ao and F arooqi, 1979: 439.
 Encyrtus obstructus Walker, 1860: 359. Synonymized by BoucÏek, Subba Rao and Farooqi, 1979: 439.
 Cardiogaster fusciventris Motschulksy, 1863: 72, 73. Synonymized by BoucÏek, 1965: 547.
 Eurycephalus alcocki Ashmead, 1903: 61. Synonymized by BoucÏek, Subba R ao and Farooqi, 1979: 439.
 Eurycranium saissetiae Ashmead, 1905: 405.
 Anysis saissetiae (Ashmead); BoucÏek, 1965: 547. Liao et al., 1987: 94–95.
 Cephaleta brunniventris M otschulsky; BoucÏek, Subb a R ao and F arooqi, 1979: 438. F arooqi, 1983: 187–188. M ani, 1989: 555–557.
 Material examined. China: Hainan, 17 May 1964, 10 8 (Chen Tai-Lu); 23/ 24 May 1964, 4 1, ex. Saissetia sp. (Liao Ding-Xi); 19 May 1964, 9 3, ex. Ceroplastes rubens Maskell (Liao Ding-Xi); Hainan, Zhanxian, 5 November 1980, 7 (Liao D ing-Xi); 10 August 1979, 1, ex. Saissetia sp. (Luo Yong-M ing); 23 M ay 1964, 1, 19 M ay 1964, 2 (Liao D ing-Xi); G uandong, G urangzhou, 26/27 M ay 1964, 3, ex. Pseudococcus sp. (Liao Ding-Xi); 22 June 1963, 2 4 (Liao Ding-Xi); 30 M arch 1957, 2 (Liao D ing-X i); F ujian, Shaxian, 1980, 3 (H uang Jian); F ujian, Sanming, October 1994, 1 5, ex. Ceroplastes sp. (Liang Wei-G uang); Hebei, Xinglong, 1 April 1964, 1, ex. Coccus sp. (Liao Ding-Xi); Nei Mongol, Hailar, 17 May 1964, 1, ex. Coccus sp. (Liao Ding-Xi).
 Biology. Host records found in China are as follows: Saissetia sp., Ceroplastes rubens Maskell, Coccus sp., Pseudococcus sp. Hosts from other countries: Asterolecanium sp., Cerococcus hibisci (Green), Ceroplastes pseudoceriferus (Green), Ceroplastodes chiton (Green), Saissetia coOEeae (Walker), Pulvinaria psidii Maskell.
 Distribution. Oriental species, has been recorded from China (Guangdong, H ainan, F ujian and H ebei, N ei M ongol, Taiwan); India, Sri Lanka, Philippines.
description: Published as part of Uan, H Ui Xiao D A-Wei H, 2001, A review of Eunotinae (Hymenoptera: Chalcidoidea: Pteromalidae) from China, pp. 1587-1605 in Journal of Natural History 35 on pages 1602-1603
Listron bilaminatum Johnson & Masner & Musetti 2008, new species
Creators: name: Johnson, Norman F.
name: Masner, Lubomír
name: Musetti, Luciana
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Scelionidae
Listron
Listron bilaminatum

description: Listron bilaminatum Masner, new species   Figures 10–12
DESCRIPTION: Holotype male: Femora yellow; frons with two well-developed transverse ledges (figs. 11, 12); occiput transversely striate (fig. 10); penultimate maxillary palpomere expanded apically; middle lobe of mesoscutum with distinct umbilicate setigerous punctures on rugulose background (fig. 10); upper portion of mesopleuron microreticulate; T1 – T4 longitudinally rugulose.
 MATERIAL EXAMINED: Holotype male: CHILE, Region IV, Elqui Prov., Quebrada El Arrayán, 10 km S La Villa; malaise in dry wash; 400 m; 16.XII. 2003 / 3.I. 2004; ME Irwin, FD Parker, 30 ° 04.26 9 S 71 ° 00.04 9 W; OSUC 174168 (MEUC).
description: Published as part of Johnson, Norman F., Masner, Lubomír & Musetti, Luciana, 2008, Review of Genera of the Tribe Sparasionini (Hymenoptera: Platygastroidea, Scelionidae), and Description of Two New Genera from the New World, pp. 1-24 in American Museum Novitates 3629 (1) on pages 9-10, DOI: 10.1206/578.1, http://zenodo.org/record/5390053
COSMOSOMAS: A Circular Scanning Instrument to Map the Sky at Centimetric Wavelengths
Creators: name: Gallegos, J. E.
name: Macias-Perez, J. F.
name: Gutierrez, C. M.
name: Rebolo, R.
name: Watson, R. A.
name: Hoyland, R. J.
name: Fernandez-Cerezo, S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the first instrument of a Cosmic Microwave Background experiment for mapping cosmological structures on medium angular scales (the COSMOSOMAS experiment) and diffuse Galactic emission. The instrument is located at Teide Observatory (Tenerife) and is based on a circular scanning sky strategy. It consists of a 1 Hz spinning flat mirror directing the sky radiation into a 1.8 m off-axis paraboloidal antenna which focuses it on to a cryogenically cooled HEMT-based receiver operating in the frequency range 12--18 GHz. The signal is split by a set of three filters, allowing simultaneous observations at 13, 15 and 17 GHz, each with a 1 GHz bandpass. A 1-5 degree resolution sky map complete in RA and covering 20 degrees in declination is obtained each day at these frequencies. The observations presented here correspond to the first months of operation, which have provided a map of ~9000 square degrees on the sky centred at DEC = +31 degrees with sensitivities of 140, 150 and 250 microK per beam area in the channels at 13, 15 and 17 GHz respectively. We discuss the design and performance of the instrument, the atmospheric effects, the reliability of the data obtained and prospects of achieving a sensitivity of 30 microK per beam in two years of operation.
description: Accepted for publication in MNRAS, 7 pages, 9 figures