cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Diphyllodes magnificus subsp. intermedius Hartert
Creators: name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paradisaeidae
Diphyllodes
Diphyllodes magnificus
Diphyllodes magnificus intermedius hartert

description: Diphyllodes magnificus intermedius Hartert
Diphyllodes magnificus intermedius Hartert, 1930: 36 (Snow Mountains, 2,500 feet).
Now Cicinnurus magnificus chrysopterus Elliot, 1873. See Mayr, 1962d: 198; Gilliard, 1969: 201–210; Diamond, 1972: 310–311, 317; Coates, 1990: 496–507; Cracraft, 1992: 32–34; Frith and Beehler, 1998: 391–400; and Frith and Frith, 2009b: 483.
HOLOTYPE: AMNH 678407, adult male, collected in the Pegunungan Maoke (= Snow Mountains), 2500 ft, 04.00, 138.00E (USBGN, 1982), Papua Province, Indonesia, on 13 August 1910, by Albert S. Meek (no. 4604). From the Rothschild Collection.
COMMENTS: Hartert cited Meek’s field number in the original description and gave his type series as three males and two females as well as ‘‘half a dozen fully adult males from the Kapare, Waitakwa, Utakwa valleys.’’ Meek collected three males and three females (Rothschild and Hartert, 1913: 521) on the Setekwa River, 04.54S, 137. 19E (USBGN, 1982), a tributary of the Otakwa (= Utakwa) River, in the lower reaches of the Snow Moutains (Rothschild and Hartert, 1913: 473; LeCroy and Jansen, 2011: 182). I have considered the five specimens in addition to the type to be paratypes of interme- dius: AMNH 678408 (Meek no. 4552), adult male, 29 July 1910; AMNH 678409 (4712), immature male, 4 September 1910; AMNH 678410–678412 (4716, 4642, 4919), three females, 26 August–29 October 1910. The ‘‘half dozen fully adult males’’ may have been borrowed from the Dutch and comparisons made with Meek’s material.
Diamond (1972: 310–311, 317) suggested combining Diphyllodes and Cicinnurus in Cicinnurus and this has been followed by Coates (1990: 496), Frith and Beehler (1998: 392–393), and Frith and Frith (2009b: 483). The last two references also included intermedius as a synonym of chrysopterus, as did Cracraft (1992: 33).
description: Published as part of Lecroy, Mary, 2014, Type Specimens Of Birds In The American Museum Of Natural History Part 12. Passeriformes: Ploceidae, Sturnidae, Buphagidae, Oriolidae, Dicruridae, Callaeidae, Grallinidae, Corcoracidae, Artamidae, Cracticidae, Ptilonorhynchidae, Cnemophilidae, Paradisaeidae, And Corvidae, pp. 1-165 in Bulletin of the American Museum of Natural History 2014 (393) on pages 106-107, DOI: 10.1206/885.1, http://zenodo.org/record/4629954
Nucleon spin-flavor structure in SU(3) breaking chiral quark model
Creators: name: Song, X.
name: McCarthy, J. S.
name: Weber, H. J.
Publisher: name: arXiv
Year: 1997
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The SU(3) symmetric chiral quark model, which describes interactions between quarks, gluons and the Goldstone bosons, explains reasonably well many aspects of the flavor and spin structure of the proton, except for the values of $f_3/f_8$ and $Δ_3/Δ_8$. Introducing the SU(3)-breaking effect suggested by the mass difference between the strange and nonstrange quarks, we find that this discrepancy can be removed and better overall agreement obtained.
description: 18 pages, Latex, 4 tables. Phys. Rev. D (in press, submitted/revised in June/Nov 1996)
Improved Representation of Ocean Heat Content in Energy Balance Models
Creators: name: Nadiga, Balasubramanya T.
name: Urban, Nathan M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: Anomaly-diffusing energy balance models (AD-EBM) are routinely employed to analyze and emulate the warming response of both observed and simulated Earth systems. We demonstrate a deficiency in common multi-layer as well as continuous-diffusion AD-EBM variants: They are unable to, simultaneously, properly represent surface warming and the vertical distribution of heat uptake. We show that this inability is due to the diffusion approximation. On the other hand, it is well understood that transport of water from the surface mixed layer into the ocean interior is achieved, in large part, by the process of ventilation---a process associated with outcropping isopycnals. We, therefore, start from a configuration of outcropping isopycnals and demonstrate how an AD-EBM can be modified to include the effect of ventilation on ocean uptake of anomalous radiative forcing. The resulting EBM is able to successfully represent both surface warming and the vertical distribution of heat uptake, and indeed, a simple four layer model suffices. The simplicity of the models notwithstanding, the analysis presented and the necessity of the modification highlight the role played by processes related to the down-welling branch of global ocean circulation in shaping the vertical distribution of ocean heat uptake.
description: 26 pages with 17 figures. Climatic Change (2018)
High-mass star formation at sub-50AU scales
Creators: name: Beuther, H.
name: Mottram, A. Ahmadi. J. C.
name: Linz, H.
name: Maud, L. T.
name: Henning, Th.
name: Kuiper, R.
name: Walsh, A. J.
name: Johnston, K. G.
name: Longmore, S. N.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Methods: We observed the high-mass hot core region G351.77-0.54 with ALMA and more than 16km baselines. Results: At a spatial resolution of 18/40au (depending on the distance), we identify twelve sub-structures within the inner few thousand au of the region. The brightness temperatures are high, reaching values greater 1000K, signposting high optical depth toward the peak positions. Core separations vary between sub-100au to several 100 and 1000au. The core separations and approximate masses are largely consistent with thermal Jeans fragmentation of a dense gas core. Due to the high continuum optical depth, most spectral lines are seen in absorption. However, a few exceptional emission lines are found that most likely stem from transitions with excitation conditions above1000K. Toward the main continuum source, these emission lines exhibit a velocity gradient across scales of 100-200au aligned with the molecular outflow and perpendicular to the previously inferred disk orientation. While we cannot exclude that these observational features stem from an inner hot accretion disk, the alignment with the outflow rather suggests that it stems from the inner jet and outflow region. The highest-velocity features are found toward the peak position, and no Hubble-like velocity structure can be identified. Therefore, these data are consistent with steady-state turbulent entrainment of the hot molecular gas via Kelvin-Helmholtz instabilities at the interface between the jet and the outflow. Conclusions: Resolving this high-mass star-forming region at sub-50au scales indicates that the hierarchical fragmentation process in the framework of thermal Jeans fragmentation can continue down to the smallest accessible spatial scales. Velocity gradients on these small scales have to be treated cautiously and do not necessarily stem from disks, but may be better explained with outflow emission.
description: Accepted by Astronomy & Astrophysics, high-resolution version available at http://www.mpia.de/homes/beuther/papers.html
Tracking the connection between disorder and energy landscape in glasses using geologically hyperaged amber
Creators: name: Pogna, E. A. A.
name: Chumakov, A. I.
name: Ferrante, C.
name: Ramos, M. A.
name: Scopigno, T.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Fossil amber offers the unique opportunity of investigating an amorphous material which has been exploring its energy landscape for more than 110 Myears of natural aging. By applying different x-ray scattering methods to amber before and after annealing the sample to erase its thermal history, we identify a link between the potential energy landscape and the structural and vibrational properties of glasses. We find that hyperaging induces a depletion of the vibrational density of states in the THz region, also ruling the sound dispersion and attenuation properties of the corresponding acoustic waves. Critically, this is accompanied by a densification with structural implications different in nature from that caused by hydrostatic compression. Our results, rationalized within the framework of fluctuating elasticity theory, reveal how upon approaching the bottom of the potential energy landscape (9% decrease in the fictive temperature $T_f$) the elastic matrix becomes increasingly less disordered (6%) and longer-range correlated (22%).
description: 9 pages, 10 figures
Additional file 1 of Analysis of association between common variants of uncoupling proteins genes and diabetic retinopathy in a Chinese population
Creators: name: Jin, Peiyao
name: Li, Zhiqiang
name: Xu, Xian
name: He, Jiangnan
name: Chen, Jianhua
name: Xu, Xun
name: Du, Xuan
name: Bai, Xuelin
name: Zhang, Bo
name: He, Xiangui
name: Lu, Lina
name: Zhu, Jianfeng
name: Shi, Yongyong
name: Zou, Haidong
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1: Table S1. The characteristics of 18 single nucleotide polymorphisms of the uncoupling proteins genes.
Additional file 2 of Analysis of association between common variants of uncoupling proteins genes and diabetic retinopathy in a Chinese population
Creators: name: Jin, Peiyao
name: Li, Zhiqiang
name: Xu, Xian
name: He, Jiangnan
name: Chen, Jianhua
name: Xu, Xun
name: Du, Xuan
name: Bai, Xuelin
name: Zhang, Bo
name: He, Xiangui
name: Lu, Lina
name: Zhu, Jianfeng
name: Shi, Yongyong
name: Zou, Haidong
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Additional file 2: Table S2. The association of uncoupling proteins genotypes and sight threatening diabetic retinopathy.
Paradisea apoda var. novae guineae
Creators: name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paradisaeidae
Paradisea
Paradisea apoda
Paradisea apoda (var.) novae guineae d'Albertis and salvadori

description: Paradisea apoda (Var.) novae guineae
D’Albertis and Salvadori
Paradisea apoda (Var.) novae guineae D’Albertis and Salvadori, 1879: 96 (Fiume Fly).
Now Paradisaea apoda novaeguineae D’Albertis and Salvadori, 1879. See Salvadori, 1881: 609– 612; Rothschild and Hartert, 1903a: 80; Mayr, 1962d: 199; Gilliard, 1969: 214–222; Coates, 1990: 517–519; Cracraft 1992: 34; Frith and Beehler, 1998: 448–456; and Frith and Frith, 2009b: 487–488.
PROBABLE SYNTYPE: AMNH 678778, adult male, SYNTYPE: AMNH 678779, immature male, both collected on the Fly River, 400 m, 08.00S, 142.00E (Frith and Beehler, 1998: 567), Western Province, Papua New Guinea, on 23 July 1877, by L.M. D’Albertis (nos. 355 and 335, respectively). From the Rothschild Collection.
COMMENTS: In the original description, D’Albertis and Salvadori did not designate a type, therefore the 40 (not 41) specimens collected in 1877 that they listed, giving D’Albertis’ field numbers, are all syntypes. Rothschild received two specimens from Salvadori. The immature male, AMNH 678779, is a definite syntype, listed by D’Albertis and Salvadori (1879: 97) and by Salvadori (1881: 611), where he enumerated all the specimens of novaeguineae again and in the same order as they were given in the original description. The adult male, AMNH 678778, is a bit more problematic, as it was apparently listed as ‘‘no. 365’’ in the original description, but the number was corrected to ‘‘no. 355’’ in Salvadori (1881: 610) without comment. Three additional numbers were also corrected by Salvadori (1881: 610–611): nos. 303 to 382, 203 to 293, and 714 to 614. It seems likely that D’Albertis’ number of this specimen was a misprint in the original description, but I do not know the whereabouts of all the syntypes. Arbucco et al. (1979: 248) listed 15 syntypes as held in MSNG, but without giving D’Albertis’ numbers.
The two AMNH syntypes were not listed by Hartert in any of his lists of types in the Rothschild Collection and had not been included with the AMNH types until they were called to my attention by Carlo Violani (personal commun.). AMNH type labels have been added.
Most authors have recognized this subspecies, but Cracraft (1992: 34) did not consider it diagnosably distinct from the nominate form.
description: Published as part of Lecroy, Mary, 2014, Type Specimens Of Birds In The American Museum Of Natural History Part 12. Passeriformes: Ploceidae, Sturnidae, Buphagidae, Oriolidae, Dicruridae, Callaeidae, Grallinidae, Corcoracidae, Artamidae, Cracticidae, Ptilonorhynchidae, Cnemophilidae, Paradisaeidae, And Corvidae, pp. 1-165 in Bulletin of the American Museum of Natural History 2014 (393) on page 107, DOI: 10.1206/885.1, http://zenodo.org/record/4629954
Metallic temperature dependence of resistivity in perchlorate doped polyacetylene
Creators: name: Park, Y. W.
name: Choi, E. S.
name: Suh, D. S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We have measured the electrical resistivity ($ρ$) and the thermoelectric power (TEP) of the perchlorate (ClO4^-) doped stretch oriented polyacetylene (PA) film. For the highly conducting samples ($σ_{RT} > 41000 S/cm$), the temperature dependence of the 4-probe resistivity shows positive temperature coefficient of resistivity (TCR) from T=1.5K to 300K. For the less conducting samples, the 4-probe resistivity data show the crossover of TCR with a broad minimum peak at T=T* > 200K. For samples of $σ_{RT}$$>$20000 S/cm, the $ρ(1.5K)/ρ(300K) <1$, i.e., the resistivity at 1.5K is lower than the room temperature resistivity value. The temperature dependence of the TEP shows diffusive linear metallic TEP becoming temperature independent below 40K. Unlike the others who used Cu(ClO_4)_2 for the ClO_4^- doping, the initial doping material we used is anhydrous Fe(ClO_4)_3 which is crucial to obtain the positive TCR from T=1.5K to 300K.
description: 14 pages, 5 figures
Magnetically tunable multi-band near-field radiative heat transfer between two graphene sheets
Creators: name: Ge, Lixin
name: Gong, Ke
name: Cang, Yuping
name: Luo, Yongsong
name: Shi, Xi
name: Wu, Ying
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Near-field radiative heat transfer (NFRHT) is strongly related with many applications such as near-field imaging, thermos-photovoltaics and thermal circuit devices. The active control of NFRHT is of great interest since it provides a degree of tunability by external means. In this work, a magnetically tunable multi-band NFRHT is revealed in a system of two suspended graphene sheets at room temperature. It is found that the single-band spectra for B=0 split into multi-band spectra under an external magnetic field. Dual-band spectra can be realized for a modest magnetic field (e.g., B=4 T). One band is determined by intra-band transitions in the classical regime, which undergoes a blue shift as the chemical potential increases. Meanwhile, the other band is contributed by inter-Landau-level transitions in the quantum regime, which is robust against the change of chemical potentials. For a strong magnetic field (e.g., B=15 T), there is an additional band with the resonant peak appearing at near-zero frequency (microwave regime), stemming from the magneto-plasmon zero modes. The great enhancement of NFRHT at such low frequency has not been found in any previous systems yet. This work may pave a way for multi-band thermal information transfer based on atomically thin graphene sheets.
description: 8 pages, 7 figures
A Dark-Matter Spike at the Galactic Center?
Creators: name: Ullio, Piero
name: Zhao, HongSheng
name: Kamionkowski, Marc
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The past growth of the central black hole (BH) might have enhanced the density of cold dark matter halo particles at the Galactic center. We compute this effect in realistic growth models of the present (2-3)*10**6 solar mass BH from a low-mass seed BH, with special attention to dynamical modeling in a realistic galaxy environment with merger and orbital decay of a seed BH formed generally outside the exact center of the halo. An intriguing ``very-dense spike'' of dark matter has been claimed in models of Gondolo and Silk with density high enough to contradict with experimental upper bounds of neutralino annihilation radiation. This ``spike'' disappears completely or is greatly weakened when we include important dynamical processes neglected in their idealized/restrictive picture with cold particles surrounding an at-the-center zero-seed adiabaticly-growing BH. For the seed BH to spiral in and settle to the center within a Hubble time by dynamical friction, the seed mass must be at least a significant fraction of the present BH. Any subsequent at-the-center growth of the BH and steepening of the central Keplerian potential well can squeeze the halo density distribution only mildly, whether the squeezing happens adiabatically or instantaneously.
description: 11 pages, 6 figures
MPA Europe Deliverable 5.3 Prioritisation analysis based on biodiversity variables
Creators: name: Addamo, Anna Maria
name: Principe, Silas C.
name: Stephenson, Fabrice
name: Zhao, Qianshuo
name: Costello, Mark John
Publisher: name: Zenodo
Year: 2025

description: Disclaimer: This is document is part of a deliverable not yet approved by the European Commission. This report presents results of preliminary prioritisation analysis based on species ranges on the MPA Europe project study area. It uses the species range maps (species distribution models, SDM) developed under the project WP3 (Species and Biogenic habitat Distribution (Principe et al., 2023; OBIS 2024). Through this prioritisation process, optimal MPA networks covering 10% and 30% of European seas will be identified for biodiversity, blue carbon, and their combined benefits.
The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
Creators: name: Pratt, G. W.
name: Arnaud, M.
name: Biviano, A.
name: Eckert, D.
name: Ettori, S.
name: Nagai, D.
name: Okabe, N.
name: Reiprich, T. H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The total mass of a galaxy cluster is one of its most fundamental properties. Together with the redshift, the mass links observation and theory, allowing us to use the cluster population to test models of structure formation and to constrain cosmological parameters. Building on the rich heritage from X-ray surveys, new results from Sunyaev-Zeldovich and optical surveys have stimulated a resurgence of interest in cluster cosmology. These studies have generally found fewer clusters than predicted by the baseline Planck LCDM model, prompting a renewed effort on the part of the community to obtain a definitive measure of the true cluster mass scale. Here we review recent progress on this front. Our theoretical understanding continues to advance, with numerical simulations being the cornerstone of this effort. On the observational side, new, sophisticated techniques are being deployed in individual mass measurements and to account for selection biases in cluster surveys. We summarise the state of the art in cluster mass estimation methods and the systematic uncertainties and biases inherent in each approach, which are now well identified and understood, and explore how current uncertainties propagate into the cosmological parameter analysis. We discuss the prospects for improvements to the measurement of the mass scale using upcoming multi-wavelength data, and the future use of the cluster population as a cosmological probe.
description: arXiv version of review article to appear in Space Science Reviews; 44 pages, 22 figures
The resistance anomaly in the surface layer of Bi$_2$Sr$_2$CaCu$_2$O$_{8+x}$ single crystals under radio-frequency irradiation
Creators: name: Kim, Nam
name: Chang, Hyun-Sik
name: Lee, Hu-Jong
name: Doh, Yong-Joo
Publisher: name: arXiv
Year: 2000
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We observed that radio-frequency (rf) irradiation significantly enhances the $c$-axis resistance near and below the superconducting transition of the CuO$_{2}$ layer in contact with a normal-metal electrode on the surface of Bi$_{2}$Sr$_{2}$CaCu$_{2}$O$_{8+x}$ single crystals. We attribute the resistance anomaly to the rf-induced charge-imbalance nonequilibrium effect in the surface CuO$_{2}$ layer. The relaxation of the charge-imbalance in this highly anisotropic system is impeded by the slow quasiparticle recombination rate, which results in the observed excessive resistance.
description: 8 pages, 5 figures
title: Parental Quality Ratings of Early Child Care Experiences and Subsequent School Adjustment
Creators: name: Collier, Donna Owens
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 1996

description: The purpose of the present study was to investigate differences in the school performances of children with different early child care experiences. The relationship between parental quality ratings of early child care experiences and subsequent school performance was also examined. The subjects in this study were 99 first grade students from two public elementary schools in Chesapeake, Virginia. The parents of these students were asked to assess broad areas of their children's early care. This assessment resulted in four subscores and one overall score of quality. The school performance scores included two measures of academic achievement obtained from the students' kindergarten records and a measure of social-emotional adjustment obtained from the students' teachers. The results of analyses of variance indicated that there were very few differences in the school performance measures among the various early child care settings. Multiple regression analyses and Pearson Product Moment correlations revealed that there was a significant relationship between parental ratings of early child care experience and the three school performance measures. These results support the view that parents should look for desired qualities within a particular setting when making a child care choice.
A monolithic ASIC demonstrator for the Thin Time-of-Flight PET scanner
Creators: name: Valerio, Pierpaolo
name: Cardarelli, Roberto
name: Iacobucci, Giuseppe
name: Paolozzi, Lorenzo
name: Ripiccini, Emanuele
name: Hayakawa, Daiki
name: Bruno, Salvatore
name: Caltabiano, Alessandro
name: Kaynak, Mehmet
name: Rueker, Holger
name: Nessi, Marzio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Time-of-flight measurement is an important advancement in PET scanners to improve image reconstruction with a lower delivered radiation dose. This article describes the monolithic ASIC for the TT-PET project, a novel idea for a high-precision PET scanner for small animals. The chip uses a SiGe Bi-CMOS process for timing measurements, integrating a fully-depleted pixel matrix with a low-power BJT-based front-end per channel, integrated on the same 100 $μ m$ thick die. The target timing resolution is 30 ps RMS for electrons from the conversion of 511 keV photons. A novel synchronization scheme using a patent-pending TDC is used to allow the synchronization of 1.6 million channels across almost 2000 different chips at picosecond-level. A full-featured demonstrator chip with a 3x10 matrix of 500x500 $μ m^{2}$ pixels was produced to validate each block. Its design and experimental results are presented here.
CONCISE HISTORY OF PSYCHOLOGICAL MEASUREMENT INSTRUMENTS
Creators: name: MURILLO DE OLIVEIRA DIAS
Publisher: name: figshare
Year: 2019
Subjects: subject: 150301 Business Information Management (incl. Records, Knowledge and Information Management, and Intelligence)
subject: FOS: Economics and business

description: This paper presents a concise history of psychometrics. It is an important field of Psychology concerned with the psychological measurement. Psychometrics can help, practitioners, students, managers, and other professionals in general, stimulating the reflection on their social and workplace behaviors, in order to deepen their self-awareness and thus provide an opportunity self-learning, behavior changes and development. It encompasses also intelligence, achievement, aptitudes, and the personality traits test. This research addressed the history of such tests, such as social value orientation tests, IQ, 16-PF, Big Five personality traits tests, among others. This literature review is part of my doctoral thesis, and is helpful to managers, practitioners, educators, among others. Discussion and future research recommendations complete the present article.
Polypodium adianthoides Burm. f.
Creators: name: Mazumdar, Jaideep
name: Callmander, Martin W.
name: Fumeaux, Nicolas
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Polypodiaceae
Polypodium
Polypodium adianthoides

description: Polypodium adianthoides Burm. f., Fl. Ind.: 234. 1768.
 Lectotypus (designated here): INDONESIA: sine loco, s.d., Pryon s.n. (G-PREL [G00800154]!) (Fig. 4).
 Notes. – In the protologue, BURMAN (1768) cited an illustration (PETIVER, 1712: 67 (sphalm. “69”), tab. 2, fig. 9) and a Pryon collection. The single specimen representing original material is a Pryon specimen with no clear origin. MERRILL (1921: 337) mentioned a probable origin from Java. Pryon left on the 7 th December 1756 as head surgeon for the Dutch East India Company (VOC: Vereenigde Oostindische Compagnie) on board the Vrouwe Petronella Maria vessel to Batavia [Jakarta] (FLORIJN, 1987). The vessel arrived in Batavia on the 21 st July 1757 (BRUIJN et al., 1979). Before his definitive settlement in Java in 1760, Pryon served on two vessels in the region between 1757 and 1760 (FLORIJN, 1987). It is clear that Pryon also collected outside Java. He must have collected in other VOC settlements, elsewhere in Indonesia and possibly in India. Correspondence between Pryon and N.L. Burman kept in the archives of the University of Amsterdam (see STEENIS-KRUSEMAN, 1958) dated 1764 give no further information on Pryon’s itinerary (A. Stork, pers. comm.).
 The Pryon specimen in G-PREL (Fig. 4) clearly represents a species of the genus Rumohra Raddi. It corresponds to Rumohra adiantiformis (G. Forst.) Ching, showing similar frond morphology, leathery lamina, and free veins. BURMAN (1768) ’s Polypodium adianthoides predates FORSTER (1786) ’s P. adiantiforme G. Forst. In order to allow the further use of a well-known and widely used fern name (A. Smith, pers. comm.) and to avoid disadvantageous nomenclatural changes entailed by the strict application of the ICN rules (TURLAND et al., 2018: Art. 14.1), a proposal to conserve Forster’s name over Burman’s is in preparation.
 Rumohra adiantiformis is widely distributed in the neotropics (South and Central America and the West Indies), the paleotropics (Southern Africa, Madagascar, the Mascarenes, New Guinea), Australia and New Zealand. It is also widely cultivated and known as the “leatherleaf fern”. The type locality is unknown but it has been most probably collected from a cultivated specimen somewhere in Asia or Southeast Asia, and not in its natural range in the Cape region.
 A recent molecular phylogeny showed that the species represents a polyphyletic taxon and includes six lineages in distinct geographical regions (BAURET et al., 2017). Rumohra adiantiformis may therefore represent several cryptic species.
description: Published as part of Mazumdar, Jaideep, Callmander, Martin W. & Fumeaux, Nicolas, 2019, Typification and nomenclature of the ferns described in N. L. Burman's Flora Indica, pp. 93-109 in Candollea 74 (1) on pages 98-100, DOI: 10.15553/c2019v741a10, http://zenodo.org/record/5684532
Additional file 1 of A rapid advice guideline for the diagnosis and treatment of 2019 novel coronavirus (2019-nCoV) infected pneumonia (standard version)
Creators: name: Jin, Ying-Hui
name: Cai, Lin
name: Cheng, Zhen-Shun
name: Cheng, Hong
name: Deng, Tong
name: Fan, Yi-Pin
name: Fang, Cheng
name: Huang, Di
name: Huang, Lu-Qi
name: Huang, Qiao
name: Han, Yong
name: Hu, Bo
name: Hu, Fen
name: Li, Bing-Hui
name: Li, Yi-Rong
name: Liang, Ke
name: Lin, Li-Kai
name: Luo, Li-Sha
name: Ma, Jing
name: Ma, Lin-Lu
name: Peng, Zhi-Yong
name: Pan, Yun-Bao
name: Pan, Zhen-Yu
name: Ren, Xue-Qun
name: Sun, Hui-Min
name: Wang, Ying
name: Wang, Yun-Yun
name: Weng, Hong
name: Wei, Chao-Jie
name: Wu, Dong-Fang
name: Xia, Jian
name: Xiong, Yong
name: Xu, Hai-Bo
name: Yao, Xiao-Mei
name: Yuan, Yu-Feng
name: Ye, Tai-Sheng
name: Zhang, Xiao-Chun
name: Zhang, Ying-Wen
name: Zhang, Yin-Gao
name: Zhang, Hua-Min
name: Zhao, Yan
name: Zhao, Ming-Juan
name: Zi, Hao
name: Zeng, Xian-Tao
name: Wang, Yong-Yan
name: Wang, Xing-Huan
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. A successful treatment case of the severe 2019-nCoV infected pneumonia patient.
Paradisaea apoda subsp. salvadorii Mayr and Rand
Creators: name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paradisaeidae
Paradisaea
Paradisaea apoda
Paradisaea apoda salvadorii mayr and rand

description: Paradisaea apoda salvadorii Mayr and Rand
Paradisaea apoda salvadorii Mayr and Rand, 1935: 11 (Vanumai, Central Division, Territory of Papua).
Now Paradisaea raggiana raggiana Sclater, 1873. See Mayr, 1962d: 199; Gilliard, 1969: 222–229; Coates, 1990: 508–516; Cracraft, 1992: 34–35; Frith and Beehler, 1998: 456–469; and Frith and Frith, 2009b: 488.
HOLOTYPE: AMNH 330366, adult male, collected at Vanuamai (= Vanumai), 08.47S, 146.38E (Frith and Beehler, 1998: 571), Central Province, Papua New Guinea (formerly Central Division, Territory of Papua), on 11 June 1929, by Hannibal Hamlin on the Whitney South Sea Expedition (no. 37296).
COMMENTS: Mayr and Rand cited the AMNH catalog number of the holotype in the original description and listed their type series. Paratypes of salvadorii: Veimauri, Galley Reach, AMNH 295732, male immature, 17 August 1920, collected by J.T. Zimmer (no. 1765); Cloudy Bay, AMNH 295734, male immature, 6 January 1921, collected by J.T. Zimmer (2035); Vanuamai, AMNH 330367, 330368, adult males, both 13 June 1929, collected by Hannibal Hamlin (37297, 37295); Deva Deva, AMNH 330377, adult male, 25 May 1929, collected by Hannibal Hamlin (–); Wuroi, Oriomo River, AMNH 422205–422208, two adult males, one immature male, one female, 18 January–4 February 1934, collected by R. Archbold and A.L. Rand on the 1933–1934 Archbold Expedition. Most authors have recognized salvadorii, but Cracraft (1992: 34) synonymized salvadorii with raggiana, saying that ‘‘differences vary, probably clinally, over a large geographic area.’’ This appears to be correct.
Hannibal Hamlin collected these specimens while waiting for repairs to be made to the Whitney Expedition ship, France. The ornithological results of the Archbold Expedition were published by Mayr and Rand (1937) and included mention of the Hamlin and Zimmer collections on pages 1 and 2. A summary of the 1933–1934 expedition was provided by Archbold and Rand (1935).
description: Published as part of Lecroy, Mary, 2014, Type Specimens Of Birds In The American Museum Of Natural History Part 12. Passeriformes: Ploceidae, Sturnidae, Buphagidae, Oriolidae, Dicruridae, Callaeidae, Grallinidae, Corcoracidae, Artamidae, Cracticidae, Ptilonorhynchidae, Cnemophilidae, Paradisaeidae, And Corvidae, pp. 1-165 in Bulletin of the American Museum of Natural History 2014 (393) on pages 107-108, DOI: 10.1206/885.1, http://zenodo.org/record/4629954
Valley engineering by strain in Kekulé-distorted graphene
Creators: name: Andrade, Elias
name: Carrillo-Bastos, Ramon
name: Naumis, Gerardo G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A Kekulé bond texture in graphene modifies the electronic band structure by folding the Brillouin zone and bringing the two inequivalent Dirac points to the center. This can result, in the opening of a gap (Kek-O) or the locking of the valley degree of freedom with the direction of motion (Kek-Y). We analyze the effects of uniaxial strain on the band structure of Kekulé-distorted graphene for both textures. Using a tight-binding approach, we introduce strain by considering the hopping renormalization and corresponding geometrical modifications of the Brillouin zone. We numerically evaluate the dispersion relation and present analytical expressions for the low-energy limit. Our results indicate the emergence of a Zeeman-like term due to the coupling of the pseudospin with the pseudomagnetic strain potential which separates the valleys by moving them in opposite directions away from the center of the Brillouin zone. For the Kek-O phase, this results in a competition between the Kekulé parameter that opens a gap and the magnitude of strain which closes it. While for the Kek-Y phase, in a superposition of two shifted Dirac cones. As the Dirac cones are much closer in the supperlattice reciprocal space that in pristine graphene, we propose strain as a control parameter for intervalley scattering.
description: 8 pages, 3 figures
$Wγγ$ Production at the Fermilab Tevatron Collider: Gauge Invariance and Radiation Amplitude Zero
Creators: name: Baur, U.
name: Han, T.
name: Kauer, N.
name: Sobey, R.
name: Zeppenfeld, D.
Publisher: name: arXiv
Year: 1997
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The electroweak process $p\bar p \to \ell^\pmνγγ$ is calculated at tree level, including finite W width effects. In order to obtain a gauge invariant amplitude, the imaginary parts of $WWγ$ triangle graphs and $WWγγ$ box diagrams have to be included, in addition to resumming the imaginary contributions to the W polarization. We demonstrate the existence of a radiation amplitude zero in $p\bar p \to W^\pm γγ\to \ell^\pmνγγ$, and discuss how it may be observed in correlations of the $γγ$ and lepton rapidities at the Fermilab Tevatron.
description: 37 pages,12 figures, postscript file also available via anonymous ftp at ftp://ucdhep.ucdavis.edu/han/vvv/Wgmgm.ps
Colimit-Dense Subcategories
Creators: name: Adámek, J.
name: Brooke-Taylor, A.
name: Campion, T.
name: Positselski, L.
name: Rosický, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Category Theory (math.CT)
subject: FOS: Mathematics

description: Among cocomplete categories, the locally presentable ones can be defined as those with a strong generator consisting of presentable objects. Assuming Vop{ě}nka's Principle, we prove that a cocomplete category is locally presentable iff it has a colimit dense subcategory and a generator consisting of presentable objects. We further show that a $3$-element set is colimit-dense in $\Set^{\op}$, and spaces of countable dimension are colimit-dense in $\Vec^{op}$.
Supplementary Data 1 for "Digital phenotyping by consumer wearables identifies sleep-associated markers of cardiovascular disease risk and biological aging"
Creators: name: Teo, Jing Xian
name: Davila, Sonia
name: Chengxi Yang
name: Pua, Chee Jian
name: Yap, Jonathan
name: Swee Yaw Tan
name: Sahlén, Anders
name: Chin, Calvin Woon-Loong
name: Teh, Bin Tean
name: Rozen, Steven G.
name: Cook, Stuart Alexander
name: Khung Keong Yeo
name: Tan, Patrick
name: Weng Khong Lim
Publisher: name: figshare
Year: 2019
Subjects: subject: 80702 Health Informatics
subject: FOS: Media and communications
subject: 111712 Health Promotion
subject: FOS: Health sciences
subject: 119999 Medical and Health Sciences not elsewhere classified
subject: FOS: Other medical sciences
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Biotechnology

description: Characteristics of study participants.
Polypodium glabrum Burm. f.
Creators: name: Mazumdar, Jaideep
name: Callmander, Martin W.
name: Fumeaux, Nicolas
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Polypodiaceae
Polypodium
Polypodium glabrum

description: Polypodium glabrum Burm. f., Fl. Ind.: 235. 1768.
 Lectotypus (designated by MERRILL, 1921: 337): INDONESIA. Java: s.d., Pryon s.n. (G-PREL [G00800126]!) (Fig. 5).
 Notes. – Asingle specimen of original material, collected by Pryon in Java, is present in G-PREL [G00800126] (Fig. 5). Afurther Javanese specimen mentioned by Burman as (unnamed) variety could not be traced.
 The Pryon specimen was cited by MERRILL (1921: 337) as type. This is regarded as a valid implicit lectotypification.
 The Pryon specimen in G-PREL (Fig. 5) clearly represents a species of the genus Nephrolepis Schott. It corresponds to Nephrolepis biserrata (Sw.) Schott, showing glabrous lamina, pinnate fronds, entire margin, pinnae articulate to rachis, hydathodes at vein endings. BURMAN (1768) ’s Polypodium glabrum predates SWARTZ (1801) ’s Aspidium biserratum Sw. In order to allow the further use of a well-known and widely used fern name (A. Smith, pers. comm.) and to avoid disadvantageous nomenclatural changes entailed by the strict application of the ICN rules (TURLAND et al., 2018: Art. 14.1), a proposal to conserve Swartz’s name over Burman’s is in preparation.
description: Published as part of Mazumdar, Jaideep, Callmander, Martin W. & Fumeaux, Nicolas, 2019, Typification and nomenclature of the ferns described in N. L. Burman's Flora Indica, pp. 93-109 in Candollea 74 (1) on page 100, DOI: 10.15553/c2019v741a10, http://zenodo.org/record/5684532
Detection of Cosmic-Ray Ensembles with CREDO
Creators: name: Woźniak, Krzysztof W.
name: Almeida-Cheminant, Kevin
name: Bratek, Łukasz
name: Castillo, David Edwin Alvarez
name: Dhital, Niraj
name: Duffy, Alan R.
name: Góra, Dariusz
name: Hnatyk, Bohdan
name: Homola, Piotr
name: Jagoda, Paweł
name: Jałocha-Bratek, Joanna
name: Kasztelan, Marcin
name: Lemański, Dawid
name: Kovács, Peter
name: Nazari, Vahab
name: Niedźwiecki, Michał
name: Smelcerz, Katarzyna
name: Smolek, Karel
name: Stasielak, Jarosław
name: Stuglik, Sławomir
name: Sushchov, Oleksandr
name: Zamora-Saá, Jilberto
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: One of the main objectives of cosmic-ray studies are precise measurements of energy and chemical composition of particles with extreme energies. Large and sophisticated detectors are used to find events seen as showers starting in the Earth's atmosphere with recorded energies larger than 100 EeV. However, a Cosmic-Ray Ensemble (CRE) developing before reaching the Earth as a bunch of correlated particles may spread over larger areas and requires an extended set of detectors to be discovered. The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a solution to find such phenomena. Even simple detectors measuring the particle arrival time only are useful in this approach, as they are sufficient both to provide candidate CRE events and to determine the direction from which they are arriving.
description: 20th International Symposium on Very High Energy Cosmic Ray Interactions, May 21-15, 2018, Nagoya, Japan
Optical Investigations of La_{7/8}Sr_{1/8}MnO_3
Creators: name: Jung, J. H.
name: Kim, K. H.
name: Lee, H. J.
name: Ahn, J. S.
name: Hur, N. J.
name: Noh, T. W.
name: Kim, M. S.
name: Park, J. -G.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigated temperature dependent optical conductivity spectra of La_{7/8}Sr_{1/8}MnO_3. Its phonon bending mode starts to be splitted near a structural phase transition temperature. With further cooling, strength of a mid-infrared small polaron peak, which is located at 0.4 eV, becomes increased. These temperature dependent changes in the phonon spectra and the polaron absorption peaks were explained by a phase separation and a percolation-type transition.
description: Revtex 12 pages, 5 figures, Submitted to Phys. Rev. B
CP-Violating Phases in SUSY, Electric Dipole Moments, and Linear Colliders
Creators: name: Barger, V.
name: Falk, T.
name: Han, T.
name: Jiang, J.
name: Li, T.
name: Plehn, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We reexamine large CP-violating phases in the general Minimal Supersymmetric Standard Model, as well as more restricted models. We perform a detailed scan over parameter space to find solutions which satisfy the current experimental limits on the electric dipole moments of the electron, neutron and $^{199}$Hg atom, exploring the allowed configurations of phases and masses, and we attempt to quantify the level of tuning of the parameters necessary to populate the regions of cancellations. We then consider the measurement of CP-violating phases at a future linear collider. We find that measurements of chargino and neutralino masses and production cross-sections allow for a determination of $ϕ_1$(the phase of $M_1$) to a precision of $π/30$, while the EDM constraints require that $θ_μ$ be too small to be measured. Using the EDM constraints we find that the CP-even model parameters and the phase $ϕ_1$ can be determined at a Linear Collider with $400 \gev$ c.m. energy. As long as some information on the size of $|μ|$ is included in the observables, a measurement of $ϕ_1$ is guaranteed for $ϕ_1 > π/10$. To unambiguously identify CP violation, we construct CP-odd kinematical variables at a linear collider. However, the CP asymmetries are rather small, typically about $0.1-1.5%$, and it will be challenging to experimentally observe the predicted asymmetries.
description: 29 pages, version accepted by PRD, Figure 8 changed, minor changes in wording
Additional file 1 of Thunder-fire moxibustion for cervical spondylotic radiculopathy: Study protocol for a randomized controlled trial
Creators: name: Huang, Yunxuan
name: Zhang, Jiabi
name: Xiong, Buhui
name: Huang, Ruina
name: Zhao, Wenjing
name: Zhou, Mengxue
name: Chen, Qi
name: Xu, Danghan
name: Chen, Xinghua
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 1. SPIRIT 2013 Checklist: Recommended items to address in a clinical trial protocol and related documents.
Paradisea apoda subsp. subintermedia Rothschild
Creators: name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paradisaeidae
Paradisea
Paradisea apoda
Paradisea apoda subintermedia rothschild

description: Paradisea apoda subintermedia Rothschild
Paradisea apoda subintermedia Rothschild, 1921c: 138 (probably inland of Traitors’ and Hercules bays).
Now considered an intergrade between P. raggiana augustaevictoriae and P. r. intermedia. See Hartert, 1928: 190; Mayr, 1962d: 200; Gilliard, 1969: 222–229; Coates, 1990: 508–516; Frith and Beehler, 1998: 456–469; and Frith and Frith, 2009b: 488.
LECTOTYPE: AMNH 678862, [adult male], trade skin smuggled into England in 1921, no indication of collecting locality. From the Rothschild Collection.
COMMENTS: When Rothschild described this form he did not designate a type, but said that he had nine males and thought that they came from inland of Huon Gulf. Only seven of these specimens came to AMNH, and Hartert (1928: 190) had tied the Rothschild type label on the specimen that became AMNH 678862 without otherwise distinguishing it from other trade skins obtained by Rothschild at the same time. This number was cited by Frith and Beehler (1998: 459), and perhaps others, as the type, not realizing that it had not been so designated. I hereby designate AMNH 678862 the lectotype of P. a. subintermedia in order to validate the specimen that has always been considered the type. The six paralectotypes in AMNH are: AMNH 678857–678861, 678863.
Both P. a. granti and P. a. subintermedia are based on trade skins without exact locality, but they seem to have come from around Huon Gulf. Most authors agree that these two forms comprise a population intergrading between P. raggiana augustaevictoriae and P. r. intermedia; of the two names, granti is the older.
description: Published as part of Lecroy, Mary, 2014, Type Specimens Of Birds In The American Museum Of Natural History Part 12. Passeriformes: Ploceidae, Sturnidae, Buphagidae, Oriolidae, Dicruridae, Callaeidae, Grallinidae, Corcoracidae, Artamidae, Cracticidae, Ptilonorhynchidae, Cnemophilidae, Paradisaeidae, And Corvidae, pp. 1-165 in Bulletin of the American Museum of Natural History 2014 (393) on page 109, DOI: 10.1206/885.1, http://zenodo.org/record/4629954
Green Bank Telescope Observations of 3He+: HII Regions
Creators: name: Balser, Dana S.
name: Bania, T. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: During the era of primordial nucleosynthesis the light elements 2H, 3He, 4He, and 7Li were produced in significant amounts and these abundances have since been modified primarily by stars. Observations of 3He+ in HII regions located throughout the Milky Way disk reveal very little variation in the 3He/H abundance ratio---the "3He Plateau"---indicating that the net effect of 3He production in stars is negligible. This is in contrast to much higher 3He/H abundance ratios found in some planetary nebulae. This discrepancy is known as the "3He Problem". Stellar evolution models that include thermohaline mixing can resolve the 3He Problem by drastically reducing the net 3He production in most stars. These models predict a small negative 3He/H abundance gradient across the Galactic disk. Here we use the Green Bank Telescope to observe 3He+ in five HII regions with high accuracy to confirm the predictions of stellar and Galactic chemical evolution models that include thermohaline mixing. We detect 3He+ in all the sources and derive the 3He+/H+ abundance ratio using model HII regions and the numerical radiative transfer code NEBULA. The over 35 radio recombination lines (RRLs) that are simultaneously observed, together with the 3He+ transition provide stringent constraints for these models. We apply an ionization correction using observations of 4He RRLs. We determine a 3He/H abundance gradient as a function of Galactocentric radius of -0.116 +/- 0.022 x 10-5, consistent with stellar evolution models including thermohaline mixing that predict a small net contribution of 3He from solar mass stars.
description: Accepted for publication in AJ