cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Myoxanthus melittanthus Luer 1982
Creators: name: Rojas-Alvarado, Gustavo
name: Blanco, Mario A.
name: Karremans, Adam P.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Myoxanthus
Myoxanthus melittanthus

description: 27. Myoxanthus melittanthus (Schltr.) Luer (1982a: 47) (Fig. 15D)
 Basionym: Pleurothallis melittantha Schlechter (1924: 49).
 TYPE:— COLOMBIA. Nariño: epiphytic, 10 km northwest of Pasto, Daza, 3000 m, Jan 1922, Hopp 136 (holotype: B, destroyed, neotype here designated, Luer et al. 3023, SEL-021582!; isoneotype, SEL-021538!, illustrated in Luer (1982: Fig. 8; 1992: pl. 22). COLOMBIA. Cauca: Páramo de Barbilla, 3070 m, 27 Jul 1978.
 Distribution: — Colombia and Venezuela.
 Notes:— Myoxanthus melittanthus is similar to M.hystrix, but the former differs mainly in petals and column shape. Those of M. melittanthus are transversally rhomboid in the lower third with rounded margins, then contracted forming a slender tail with a slightly clavate tip, generally upwardly oriented, whereas those of M. hystrix are subcuadrate in the basal half with the margins obtusely angle, then contracted but terete into a yellow apex with a clavate tip downward oriented. The column wings of M. melittanthus are broader, not lobulate, extending from the base to the apex of the column, whereas in M. hystrix the wings are lobulate and rounded, emerging from near the middle to the apex of the column.
 The holotype of this species was probably destroyed during the WWII. A neotype is designated here based on a collection by Luer near the type locality because no material associated with the protologue has been found. Carnevali and Ramírez (1988 –1989) mentioned that Venezuelan plants of M. melittanthus differ from those in Colombia in their slightly smaller flowers and glabrescent sepals that are verruculose adaxially.
description: Published as part of Rojas-Alvarado, Gustavo, Blanco, Mario A. & Karremans, Adam P., 2021, A taxonomic synopsis and morphological characterization of Myoxanthus (Orchidaceae: Pleurothallidinae), pp. 211-258 in Phytotaxa 507 (3) on page 241, DOI: 10.11646/phytotaxa.507.3.1, http://zenodo.org/record/5425729
PMN J0134-0931: A gravitationally lensed quasar with an unusual radio morphology
Creators: name: Winn, Joshua N.
name: Lovell, James E. J.
name: Chen, Hsiao-Wen
name: Fletcher, Andre B.
name: Hewitt, Jacqueline N.
name: Patnaik, Alok R.
name: Schechter, Paul L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The radio-loud quasar PMN J0134-0931 was discovered to have an unusual morphology during our search for gravitational lenses. In VLA and MERLIN images, there are 5 compact components with maximum separation 681 millarcseconds. All of these components have the same spectral index from 5 GHz to 43 GHz. In a VLBA image at 1.7 GHz, a curved arc of extended emission joins two of the components in a manner suggestive of gravitational lensing. At least two of the radio components have near-infrared counterparts. We argue that this evidence implies that J0134-0931 is a gravitational lens, although we have not been able to devise a plausible model for the foreground gravitational potential. Like several other radio-loud lenses, the background source has an extraordinarily red optical counterpart.
description: Accepted for publication in ApJ. 19 pp., 5 figs. See also the preprint astro-ph/0107441 by Gregg et al., who discovered this object independently
Neutron star binary orbits in their host potential: effect on early r-process enrichment
Creators: name: Bonetti, Matteo
name: Perego, Albino
name: Dotti, Massimo
name: Cescutti, Gabriele
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Coalescing neutron star binary (NSB) systems are primary candidates for $r$-process enrichment of galaxies. The recent detection of $r$-process elements in ultra-faint dwarf (UFD) galaxies and the abundances measured in classical dwarfs challenges the NSB merger scenario both in terms of coalescence time scales and merger locations. In this paper, we focus on the dynamics of NSBs in the gravitational potentials of different types of host galaxies and on its impact on the subsequent galactic enrichment. We find that, for a $\sim t^{-1}$ delay time distribution, even when receiving a low kick ($\sim 10~{\rm km~s^{-1}}$) from the second supernova explosion, in shallow dwarf galaxy potentials NSBs tend to merge with a large off-set from the host galaxy. This results in a significant geometrical dilution of the amount of produced $r-$process elements that fall back and pollute the host galaxy gas reservoir. The combination of dilution and small number statistics produces a large scatter in the expected $r$-process enrichment within a single UFD or classical dwarf galaxy. Comparison between our results and observed europium abundances reveals a tension that even a systematic choice of optimistic parameters in our models cannot release. Such a discrepancy could point to the need of additional $r$-process production sites that suffer less severe dilution or to a population of extremely fast merging binaries.
description: 18 pages, 11 figures, MNRAS accepted
Myoxanthus merae Luer 1982
Creators: name: Rojas-Alvarado, Gustavo
name: Blanco, Mario A.
name: Karremans, Adam P.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Myoxanthus
Myoxanthus merae

description: 28. Myoxanthus merae (Luer) Luer (1982a: 47). (Fig. 15E)
 Basionym: Pleurothallis merae Luer (1976b: 144).
 TYPE:— ECUADOR. Pastaza: epiphytic in forest east of Mera, 1000 m, 20 Mar 1976, Luer et al. 682 (holotype: SEL!).
 Distribution: — Ecuador and Peru.
 Notes:— Myoxanthus merae is a small, caespitose species with slender ramicauls and narrow leaves and producing successive single flowers. It can be recognized by the yellowish flowers with the red to yellowish sepals that are pubescent externally, basally ovate petals then narrower with revolute margins, a red-brownish elliptical, oblong lip, weakly trilobed, with lateral lobes erect below the middle, disc with a pair of longitudinal calli near the centre and a pair of small auricles at its truncate base. Myoxanthus simplicaulis from Venezuela and Guyana has a similar habit and flowers. However, the latter has wider petals with a more pronounced, narrow, thick apical section, more pronounced, oblique lateral lobes of the lip and a pair of longitudinal calli emerging below the middle that extend to the base. Myoxanthus merae had been previously recorded only from Ecuador, but the photograph reproduced here (Fig. 15E) is from a plant collected in Tingo María National Park, Peru.
description: Published as part of Rojas-Alvarado, Gustavo, Blanco, Mario A. & Karremans, Adam P., 2021, A taxonomic synopsis and morphological characterization of Myoxanthus (Orchidaceae: Pleurothallidinae), pp. 211-258 in Phytotaxa 507 (3) on page 241, DOI: 10.11646/phytotaxa.507.3.1, http://zenodo.org/record/5425729
ISOPHOT - Photometric Calibration of Point Sources
Creators: name: Schulz, B.
name: Huth, S.
name: Laureijs, R. J.
name: Acosta-Pulido, J. A.
name: Braun, M.
name: Castaneda, H. O.
name: Cohen, M.
name: Cornwall, L.
name: Gabriel, C.
name: Hammersley, P.
name: Heinrichsen, I.
name: Klaas, U.
name: Lemke, D.
name: Mueller, T.
name: Osip, D.
name: Roman-Fernandez, P.
name: Telesco, C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: All observations by the aperture photometer (PHT-P) and the far-infrared (FIR) camera section (PHT-C) of ISOPHOT included reference measurements against stable internal fine calibration sources (FCS) to correct for temporal drifts in detector responsivities. The FCSs were absolutely calibrated in-orbit against stars, asteroids and planets, covering wavelengths from 3.2 to 240 micron. We present the calibration concept for point sources within a flux-range from 60 mJy up to 4500 Jy for staring and raster observations in standard configurations and discuss the requisite measurements and the uncertainties involved. In this process we correct for instrumental effects like nonlinearities, signal transients, time variable dark current, misalignments and diffraction effects. A set of formulae is developed that describes the calibration from signal-level to flux densities. The scatter of 10 to 20 % of the individual data points around the derived calibration relations is a measure of the consistency and typical accuracy of the calibration. The reproducibility over longer periods of time is better than 10 %. The calibration tables and algorithms have been implemented in the final versions of the software for offline processing and interactive analysis.
description: 21 pages, 16 figures, 5 tables, accepted by Astronomy & Astrophysics
The kinematics of molecular clumps surrounding hot cores in G29.96-0.02 and G31.41+0.31
Creators: name: Maxia, C.
name: Testi, L.
name: Cesaroni, R.
name: Walmsley, C. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high angular resolution interferometric observations of the 3 and 1.3mm continuum emission, and HCO+(1-0) and SiO(2-1)v=0 lines, obtained with the Owens Valley Radio Observatory millimeter-wave array, toward two hot cores (HCs) associated with two well known ultracompact (UC) HII regions: G29.96-0.02 and G31.41+0.31. These HCs are believed to host young forming massive stars which have been suggested to be surrounded by massive rotating accretion disks. The aim of these new observations is to study the structure and kinematics of the molecular clumps surrounding the HCs and nearby UCHII regions at moderately high angular resolution. Our observations reveal that the clumps within which the HCs and UCHII regions are embedded have a complex kinematical structure. The total mass of the clumps is estimated to be in the range 1000-3000 Msun, consistent with previous findings. Our observations also show compelling evidence that the clump in G29.96-0.02 is contracting onto the HC position, suggesting that the accretion process onto the massive young stellar object embedded in the HC is still ongoing. In these objects the kinematical structure that we observe is also compatible with the presence of a massive rotating disk within the HC, even though we cannot prove this suggestion with our data. The case of G31.41+0.31 is more complicated, and our data, although consistent with the presence of an inner disk and an infalling envelope around it, do not have the required spatial resolution to resolve the different structures.
description: 13 pages, 15 figs, A&A in press
Solution of the Kolmogorov equation for TASEP
Creators: name: Nica, Mihai
name: Quastel, Jeremy
name: Remenik, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We provide a direct and elementary proof that the formula obtained in [MQR17] for the TASEP transition probabilities for general (one-sided) initial data solves the Kolmogorov backward equation. The same method yields the solution for the related PushASEP particle system.
description: Minor corrections and improvements. To appear in Ann. Probab
Additional file 1 of Topical Chinese patent medicines for chronic musculoskeletal pain: systematic review and trial sequential analysis
Creators: name: Tang, Kaiqiang
name: Sun, Jigao
name: Dong, Yawei
name: Zheng, Zelu
name: Wang, Rongtian
name: Lin, Na
name: Chen, Weiheng
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy

description: Additional file 1. Search strategy.
Pseudadelphus ciliatus , Arrow 1899
Creators: name: Smith, Andrew B. T.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Rutelidae
Pseudadelphus
Pseudadelphus ciliatus

description: Pseudadelphus ciliatus, Arrow 1899:369 [new combination].
 Aulacopalpus ciliatus, Ohaus 1905:126, 130, 134, 143, 165, 166 [redescription, new combination]; Ohaus 1909:7, 8 [comment on morphology, key to species of Aulacopalpus]; Ohaus 1918:179 [catalog listing]; Blackwelder 1944:247 [checklist]; Gutiérrez 1949:31 [comment on morphology, locality data]; Machatschke 1965:61, 63 [cited as type species for Pseudadelphus, catalog listing]; Machatschke 1972:305 [cited as type species for Pseudadelphus, catalog listing]; Arias 2000:75 [comment on distribution, comment on morphology]; Smith 2002:this paper [phylogenetics, key to species of Aulacopalpus, lectotype designation, redescription, distribution].
description: Published as part of Smith, Andrew B. T., 2002, Revision Of The Southern South American Endemic Genus Aulacopalpus Guérin-Méneville With Phylogenetic And Biogeographic Analyses Of The Subtribe Brachysternina (Coleoptera: Scarabaeidae: Rutelinae: Anoplognathini), pp. 379-437 in The Coleopterists Bulletin 56 (3) on page 425, DOI: 10.1649/0010-065X(2002)056[0379:ROTSSA]2.0.CO;2, http://zenodo.org/record/10103193
Additional file 10: of CRISPR/Cas9 editing of three CRUCIFERIN C homoeologues alters the seed protein profile in Camelina sativa
Creators: name: Lyzenga, Wendy
name: Harrington, Myrtle
name: Bekkaoui, Diana
name: Merek Wigness
name: Hegedus, Dwayne
name: Rozwadowski, Kevin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Plant Biology

description: Table S4. Amino acid content of camelina cruciferins and napins. (DOCX 23 kb)
Hipparcos open clusters and stellar evolution
Creators: name: Castellani, V.
name: Degl'Innocenti, S.
name: Moroni, P. G. Prada
name: Tordiglione, V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: By relying on recently improved Hipparcos parallaxes for the Hyades, Pleiades and Ursa Major clusters we find that stellar models with updated physical inputs nicely reproduce the location in the color magnitude diagram of main sequence stars of different metallicities. Stars in the helium burning phase are also discussed, showing that the luminosity of giants in the Hyades, Praesepe and Ursa Major clusters appears to be in reasonable agreement with theoretical predictions. A short discussion concerning the current evolutionary scenarios closes the paper.
description: 5 pages, 6 Postscript figures, accepted by MNRAS
Quantum Markov chains: recurrence, Schur functions and splitting rules
Creators: name: Grünbaum, F. A.
name: Lardizabal, C. F.
name: Velázquez, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mathematical Physics (math-ph)
subject: Functional Analysis (math.FA)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this work we study the recurrence problem for quantum Markov chains, which are quantum versions of classical Markov chains introduced by S. Gudder and described in terms of completely positive maps. A notion of monitored recurrence for quantum Markov chains is examined in association with Schur functions, which codify information on the first return to some given state or subspace. Such objects possess important factorization and decomposition properties which allow us to obtain probabilistic results based solely on those parts of the graph where the dynamics takes place, the so-called splitting rules. These rules also yield an alternative to the folding trick to transform a doubly infinite system into a semi-infinite one which doubles the number of internal degrees of freedom. The generalization of Schur functions --so-called FR-functions-- to the general context of closed operators in Banach spaces is the key for the present applications to open quantum systems. An important class of examples included in this setting are the open quantum random walks, as described by S. Attal et al., but we will state results in terms of general completely positive trace preserving maps. We also take the opportunity to discuss basic results on recurrence of finite dimensional iterated quantum channels and quantum versions of Kac's Lemma, in close association with recent results on the subject.
Myoxanthus montanus Ortiz 1997
Creators: name: Rojas-Alvarado, Gustavo
name: Blanco, Mario A.
name: Karremans, Adam P.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Myoxanthus
Myoxanthus montanus

description: 30. Myoxanthus montanus Ortiz (1997: 320). (Fig.15I)
 TYPE:— COLOMBIA. Cundinamarca: Guayabetal, “Monterredondo”, 1750 m, Aug 1977, Ortiz 937 (holotype: HPUJ!).
 Distribution: — Colombia.
 Notes:— The proliferous habit of this species is similar to M. frutex and M. gyas, but M. montanus differs by bearing congested white flowers with a pubescent floral bract covering the base of the perianth and lateral sepals connate to near the middle.
 31. Myoxanthus neillii Luer & Dodson (1992: 62)
 TYPE:— ECUADOR. Napo: near Coca, 200 m, epiphytic in large fallen tree, collected by D. Neill, flowered in cultivation at the Río Palenque Science Center, 3 Oct 1986, Dodson 16621 (holotype: MO, not located, lectotype, here designated, illustration of the holotype in Luer (1992: pl. 25).
 Distribution: — Ecuador and Peru.
 Notes:— This species is similar to M. affinis and M. parahybunensis, but M. neillii is distinguished from these by its small flowers with sepals only 4–5 mm long, oblong petals not narrowed above the middle and column with teeth at the apex. Since the holotype at MO was not located, a lectotype is designated here.
description: Published as part of Rojas-Alvarado, Gustavo, Blanco, Mario A. & Karremans, Adam P., 2021, A taxonomic synopsis and morphological characterization of Myoxanthus (Orchidaceae: Pleurothallidinae), pp. 211-258 in Phytotaxa 507 (3) on page 242, DOI: 10.11646/phytotaxa.507.3.1, http://zenodo.org/record/5425729
Collisional Cascades in Planetesimal Disks I. Stellar Flybys
Creators: name: Kenyon, Scott J.
name: Bromley, Benjamin C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a new multiannulus planetesimal accretion code to investigate the evolution of a planetesimal disk following a moderately close encounter with a passing star. The calculations include fragmentation, gas and Poynting-Robertson drag, and velocity evolution from dynamical friction and viscous stirring. We assume that the stellar encounter increases planetesimal velocities to the shattering velocity, initiating a collisional cascade in the disk. During the early stages of our calculations, erosive collisions damp particle velocities and produce substantial amounts of dust. For a wide range of initial conditions and input parameters, the time evolution of the dust luminosity follows a simple relation, L_d/L_{\star} = L_0 / [alpha + (t/t_d)^{beta}]. The maximum dust luminosity L_0 and the damping time t_d depend on the disk mass, with L_0 proportional to M_d and t_d proportional to M_d^{-1}. For disks with dust masses of 1% to 100% of the `minimum mass solar nebula' (1--100 earth masses at 30--150 AU), our calculations yield t_d approx 1--10 Myr, alpha approx 1--2, beta = 1, and dust luminosities similar to the range observed in known `debris disk' systems, L_0 approx 10^{-3} to 10^{-5}. Less massive disks produce smaller dust luminosities and damp on longer timescales. Because encounters with field stars are rare, these results imply that moderately close stellar flybys cannot explain collisional cascades in debris disk systems with stellar ages of 100 Myr or longer.
description: 33 pages of text, 12 figures, and an animation. The paper will appear in the March 2002 issue of the Astronmomical Journal. The animation and a copy of the paper with full resolution figures are at S. Kenyon's planet formation website: http://cfa-www.harvard.edu/~kenyon/pf
Additional file 1 of Medical behaviours and medication adherence of older hypertensive patients in different medical insurance programs in Beijing, China: a cross-sectional study
Creators: name: Lan, Lan
name: Hai, Pengcheng
name: Luo, Jiawei
name: Li, Rui
name: Wang, Yilong
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Supplementary: Table S1. Medical behaviors of hypertensive patients aged 60~74 in Beijing, China. Table S2. Medical behaviors of hypertensive patients aged 75~89 in Beijing, China. Table S3. Medical behaviors of hypertensive patients aged 90 or older in Beijing, China.
Azimuth Reference - Human Lung
Creators: name: Satija Lab
Publisher: name: Zenodo
Year: 2021
Subjects: Azimuth
Seurat
single-cell

description: Here we provide the reference data files used to run the Azimuth Human Lung reference web application. For a full description of the reference data structure, please see the wiki at https://github.com/satijalab/azimuth/wiki/Azimuth-Reference-Format.
Gallup Poll # 725
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Lent (1); President Lyndon Baines Johnson job performance (1); most important problem facing the country (1); Single Presbyterian Church (1); War in Vietnam (8); Dean Rusk (1); keeping prices down (2); another World War (1); Republican presidential candidate (1); Republican vs. Democratic vs. Independent (2); Vote in 1964 election (1).
Energetics of Tev Blazars and Physical Constraints on their Emission Regions
Creators: name: Kino, Motoki
name: Takahara, Fumio
name: Kusunose, Masaaki
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using multi-frequency spectra from TeV blazars in quiescent states, we obtain the physical parameters of the emission region of blazars within the framework of the one-zone synchrotron self-Compton (SSC) model. We numerically calculate the steady-state energy spectra of electrons by self-consistently taking into account the effects of radiative cooling with a proper account of the Klein-Nishina effects. Here electrons are assumed to be injected with a power-law spectrum and to escape on a finite time scale, which naturally leads to the existence of a break energy scale. Although we do not use time variabilities but utilize a model of electron escape to constrain the size of the emission region, the resultant size turns out to be similar to that obtained based on time variabilities. Through detailed comparison of the predicted emission spectra with observations, we find that for Mrk 421, Mrk 501, and PKS 2155--304, the energy density of relativistic electrons is about an order of magnitude larger than that of magnetic fields with an uncertainty within a factor of a few.
description: Accepted for publication in ApJ
Information geometric analysis of long range topological superconductors
Creators: name: Amin, Syed Tahir
name: Mera, Bruno
name: Paunković, Nikola
name: Vieira, Vítor R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The Uhlmann connection is a mixed state generalisation of the Berry connection. The latter has a very important role in the study of topological phases at zero temperature. Closely related, the quantum fidelity is an information theoretical quantity which is a measure of distinguishability of quantum states. Moreover, it has been extensively used in the analysis of quantum phase transitions. In this work, we study topological phase transitions in 1D and 2D topological superconductors with long-range hopping and pairing amplitudes, using the fidelity and the quantity $Δ$ closely related to the Uhlmann connection. The drop in the fidelity and the departure of $Δ$ from zero signal the topological phase transitions in the models considered. The analysis of the ground state fidelity susceptibility and its associated critical exponents are also applied to the study of the aforementioned topological phase transitions.
description: 10 pages, 5 figures; closer to published version
Additional file 1: of HIV-1 self-testing to improve the efficiency of pre-exposure prophylaxis delivery: a randomized trial in Kenya
Creators: name: Ortblad, Katrina
name: Kearney, John
name: Mugwanya, Kenneth
name: Irungu, Elizabeth
name: Haberer, Jessica
name: Ruanne Barnabas
name: Donnell, Deborah
name: Mugo, Nelly
name: Baeten, Jared
name: Ngure, Kenneth
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: SPIRIT 2013 checklist: recommended items to address in a clinical trial protocol and related documents. (DOC 123 kb)
Pericoma (Pericoma) calcilega Feuerborn 1923
Creators: name: Ježek, Jan
name: Hájek, Josef
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Pericoma
Pericoma calcilega

description: Pericoma (Pericoma) calcilega Feuerborn, 1923
 Unpublished record. Hradisko [36], J, 1.viii.1996, J.
 Vegetation. 32, 42, 84, 86; 117, 119, 121, 126.
European species, not rare, endangered; for its distribution see JEŽEK & GOUTNER (1995) and JEŽEK (2004b).
description: Published as part of Ježek, Jan & Hájek, Josef, 2007, Psychodidae (Diptera) of the Orlické hory Protected Landscape Area and neighbouring areas with descriptions of two new species from the Czech Republic, pp. 237-285 in Acta Entomologica Musei Nationalis Pragae 47 on page 268, DOI: 10.5281/zenodo.5328353
Zahlungsverpflichtungen, bilanzielle Schulden und DCF-Theorie
Creators: name: Kruschwitz, Lutz
name: Löffler, Andreas
name: Scholze, Andreas
Publisher: name: Freie Universität Berlin
Year: 2010
Subjects: subject: Discounted Cashflow
subject: Unternehmensbewertung
subject: 300 Sozialwissenschaften::330 Wirtschaft
subject: 300 Sozialwissenschaften::330 Wirtschaft::332 Finanzwirtschaft

description: In diesem Aufsatz geht es um die Frage, ob und wie eine Bewertungstheorie in der Tradition des Discounted Cashflow auf Unternehmen mit Pensionsrückstellungen, Lieferantenverbindlichkeiten und andere bilanziellen Schulden angewendet werden kann. Es wird diskutiert, welche Eigenschaften bilanzrechtliche Verbindlichkeiten aufweisen müssen, damit sie auch in einer Modigliani-Miller-Welt als Fremdkapital aufgefasst werden können.
Myoxanthus oliviae Kolanowska & Szlachetko 2019
Creators: name: Rojas-Alvarado, Gustavo
name: Blanco, Mario A.
name: Karremans, Adam P.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Myoxanthus
Myoxanthus oliviae

description: 33. Myoxanthus oliviae Kolanowska & Szlachetko (2019: 3) (Fig. 15K)
 TYPE:— PERU. Cuzco: Urubamba, 3100 m., 5 Dec 1968, Vargas 20860 (holotype: AMES!).
 Distribution: — Peru.
 Notes:— Myoxanthus oliviae, described from Peru, was said to differ from M. serripetalus in the colour of flowers, brownish yellowish vs. dark-purple, an entire midlobe vs. fimbriate midlobe and apex of the petals sagittate vs. apex oblong to linear. According to our revision, the linear apex of the petals in M. serripetalus (and dark-purple flowers) appears to be consistent. However, the entire midlobe of the lip in M. oliviae and brownish flowers are inconsistent, but a fimbriate margin may also be found.
description: Published as part of Rojas-Alvarado, Gustavo, Blanco, Mario A. & Karremans, Adam P., 2021, A taxonomic synopsis and morphological characterization of Myoxanthus (Orchidaceae: Pleurothallidinae), pp. 211-258 in Phytotaxa 507 (3) on page 242, DOI: 10.11646/phytotaxa.507.3.1, http://zenodo.org/record/5425729
title: RF MEMS Switches for Smart Antenna
Creators: name: Pal, Jitendra
Publisher: name: Griffith University
Year: 2016
Subjects: subject: Smart antenna techniques
subject: RF MEMS Switches
subject: High actuation voltage
subject: Single Pole Single Throw (SPST)

description: The adoption of smart antenna techniques in future wireless systems is expected to have a significant impact on the efficient use of the spectrum and the minimisation of the cost of establishing new wireless networks. RF MEMS devices are the potential candidates to revolutionise RF and microwave system implementation for next generation wireless applications. Despite having excellent performances, there are some drawbacks associated with RF MEMS switches. The main challenges with RF MEMS switches are their high actuation voltage, limited reliability and low power handling capability. This thesis presents novel RF MEMS switches which can overcome these issues. To achieve zero power consumption, we have fabricated latching RF MEMS switches. In addition, we have combined thermal actuation and electrostatic actuation mechanisms to achieve lower actuation voltage. We have also developed a novel contactless RF MEMS switch to increase the reliability of the switch. The switch is free from unavoidable stiction and micro-welding problems in other contact types, which in return guarantees high reliability and long lifetime. The proposed device is based on variable capacitance between signal lines and movable grounded electrodes controlled by electrostatic actuator. The movable grounded electrode has the capability to move bi- directionally, therefore the switch can change among ON, OFF and deep-OFF states. Thus, additional isolation can be achieved in the deep-OFF state. The switch shows excellent RF performances. To increase the power handling capability of switch, we have developed a multi-contact Single Pole Single Throw (SPST). The switch achieves uniform current distribution through each contact, thereby increasing power handling capability. The switch is actuated with separate electrodes to control the current density and direction.
Ferroelectricity Driven by Orbital Resonance of Protons in CH$_3$NH$_3$Cl and CH$_3$NH$_3$Br
Creators: name: Peng, Chu Xin
name: Meng, Lei
name: Xu, Yi Yang
name: Xing, Tian Tian
name: Zhao, Miao Miao
name: Ren, Peng
name: Yen, Fei
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The $β$ and $γ$ phases of methylammonium chloride CH$_3$NH$_3$Cl and methylammonium bromide CH$_3$NH$_3$Br are identified to be ferroelectric $via$ pyroelectric current and dielectric constant measurements. The magnetic susceptibility also exhibits pronounced discontinuities at the Curie temperatures. We attribute the origin of spontaneous polarization to the emergence of two groups of proton orbital magnetic moments from the uncorrelated motion of the CH$_3$ and NH$_3$ groups in the $β$ and $γ$ phases. The two inequivalent frameworks of intermolecular orbital resonances interact with each other to distort the lattice in a non-centrosymmetric fashion. Our findings indicate that the structural instabilities in molecular frameworks are magnetic in origin as well as provide a new pathway toward uncovering new organic ferroelectrics.
description: 5 pages, 5 figures
Pneumia nubila
Creators: name: Ježek, Jan
name: Hájek, Josef
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Pneumia
Pneumia nubila

description: Pneumia nubila (Meigen, 1818)
 Unpublished records. Boroviny [6],J, 19.vii.1996, J; Dolní Čermná, Orlice Nature Park [24],J, 27.vii.-11.viii.1995, J, white ST; Hlinné [30], J, 19.vii.1996, J; Rašeliniště Kačerov NR peatbog [42], J, 18.vii.-8.viii.1994, H + V, MT; Semanín, Mušlový rybník pond [102],J, 16.viii.1996, J; Svinecký Dvůr [108],J, 19.vii.1996, J; Třebovice, Hvězda pond [120], J, 16.viii.1996, J; Záměl [130], J, 20.ix.1993, J; Zelenka [134], J, 15.-24.ix.1993, J + H, YPT.
 Vegetation. 3, 8, 14, 18, 30, 33-34, 44, 57, 62, 65, 71, 73, 82-84, 86, 88, 90, 98; 111, 113-114, 116, 118-119, 124- 125.
European species, very common; for its distribution see JEŽEK & GOUTNER (1995). Also known from Abkhazia (see Appendix).
description: Published as part of Ježek, Jan & Hájek, Josef, 2007, Psychodidae (Diptera) of the Orlické hory Protected Landscape Area and neighbouring areas with descriptions of two new species from the Czech Republic, pp. 237-285 in Acta Entomologica Musei Nationalis Pragae 47 on page 269, DOI: 10.5281/zenodo.5328353
The evolution of the Mira variable R Hydrae
Creators: name: Zijlstra, Albert A.
name: Bedding, T. R.
name: Mattei, J. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Mira variable R Hydrae is well known for its declining period, which Wood & Zarro (1981) attributed to a possible recent thermal pulse. Here we investigate the long-term period evolution, covering 340 years, going back to its discovery in AD 1662. Wavelets are used to determine both the period and semi-amplitude. We show that the period decreased linearly between 1770 and 1950; since 1950 the period has stabilized at 385 days. The semi-amplitude closely follows the period evolution. Detailed analysis of the oldest data shows that before 1770 the period was about 495 days. We find no evidence for an increasing period during this time as found by Wood & Zarro. IRAS data shows that the mass loss dropped dramatically around AD 1750. The decline agrees with the mass-loss formalism from Vassiliadis & Wood, but is much larger than predicted by the Bloecker mass-loss law. An outer detached IRAS shell suggests that R Hya has experienced such mass-loss interruptions before. The period evolution can be explained by a thermal pulse occuring around AD 1600, or by an non-linear instability leading to an internal relaxation of the stellar structure. The elapsed time between the mass-loss decline giving rise to the outer detached shell, and the recent event, of approximately 5000 yr suggests that only one of these events could be due to a thermal pulse. Further monitoring of R Hya is recommended, as both models make strong predictions for the future period evolution. R Hya-type events, on time scales of 10^2-10^3 yr, could provide part of the explanation for the rings seen around some AGB and post-AGB stars.
description: 13 pages. MNRAS, accepted for publication
Gallup Poll # 1966-0726: Politics/Anti-Poverty Program/China/Vietnam
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Favorite way to spend an evening (1); plans to vote in November 1966 election (1); Lyndon B. Johnson job performance (3); anti-poverty program (5); Communist China should/should not be admitted to United Nations (3); 1968 Republican presidential candidates (2); description of German people (2); description of Chinese people (2); description of Russian people (2); description of Japanese people (2); congressional campaign (3); Vietnam (3); increase in world population (2); racial issues (3); congressional elections (2); 1964 presidential election (1).
Deep H I observations of the compact high-velocity cloud HVC125+41-207
Creators: name: Bruens, C.
name: Kerp, J.
name: Pagels, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present deep HI observations of the compact high-velocity cloud HVC125+41-207 using the 100-m Effelsberg telescope. Our goal was in particular to study the warm neutral medium (WNM) in detail. The Effelsberg data reveal a two phase core/halo structure - one component with a velocity width of FWHM approx 5 km/s (Westerbork data show FWHM approx 2 km/s, Braun & Burton 2000) and one with FWHM approx 18 km/s. The column density distribution of the warmer component is highly asymmetric and shows a head-tail structure. We performed a Gaussian decomposition of the cloud and found that 52% of the HI mass of the cloud is in the WNM. 24% of the WNM is located in the tail. The overall structure and the systematic variation of the observational parameters radial velocity, velocity dispersion and column density indicate that this cloud is currently interacting with the ambient medium. The Westerbork HI data of this HVC (Braun & Burton 2000) reveal an interesting dense condensation. Assuming that this condensation is virialized and in pressure equilibrium with the ambient medium, we derive a distance of 130 kpc for HVC125+41-207. Following these considerations, it is possible to constrain the parameters n_IGM < 7.8 10^-6 cm^-3 and T_IGM > 1.1 10^5 K of the intergalactic medium of the Local Group.
description: 5 pages, 2 figures, LaTeX2e, accepted for publication in A&A Letters
Observation of topological transition in high-T$_{c}$ superconductor FeTe$_{1-x}$Se$_{x}$/SrTiO$_{3}$(001) monolayers
Creators: name: Peng, X. -L.
name: Li, Y.
name: Wu, X. -X.
name: Deng, H. -B.
name: Shi, X.
name: Fan, W. -H.
name: Li, M.
name: Huang, Y. -B.
name: Qian, T.
name: Richard, P.
name: Hu, J. -P.
name: Pan, S. -H.
name: Mao, H. -Q.
name: Sun, Y. -J.
name: Ding, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Superconductors with topological surface or edge states have been intensively explored for the prospect of realizing Majorana bound states, which obey non-Abelian statistics and are crucial for topological quantum computation. The traditional routes for making topological insulator/superconductor and semiconductor/superconductor heterostructures suffer fabrication difficulties and can only work at low temperature. Here, we use angle-resolved photoemission spectroscopy to directly observe the evolution of a topological transition of band structure nearby the Fermi level in two-dimensional high-T$_{c}$ superconductor FeTe$_{1-x}$Se$_{x}$/SrTiO$_{3}$(001) monolayers, fully consistent with our theoretical calculations. Furthermore, evidence of edge states is revealed by scanning tunneling spectroscopy with assistance of theoretical calculations. Our study provides a simple and tunable platform for realizing and manipulating Majorana states at high temperature.
description: 19 pages, 4 figures and 1 table
Additional file 1: of Postoperative complications and prognosis after radical gastrectomy for gastric cancer: a systematic review and meta-analysis of observational studies
Creators: name: Wang, Shiqi
name: Xu, Lei
name: Wang, Quan
name: Li, Jipeng
name: Bai, Bin
name: Li, Zhengyan
name: Wu, Xiaoyong
name: Yu, Pengfei
name: Li, Xuzhao
name: Yin, Jichao
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Table S1. NOS of Cohort studies. NOS of Case-control studies. (DOCX 27 kb)
Myoxanthus ortizianus Kolanowska & Szlachetko 2014
Creators: name: Rojas-Alvarado, Gustavo
name: Blanco, Mario A.
name: Karremans, Adam P.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Myoxanthus
Myoxanthus ortizianus

description: 34. Myoxanthus ortizianus Kolanowska & Szlachetko (2014: 8) (Fig. 15L)
 TYPE:— COLOMBIA. Putumayo: Valle del Sibundoy. Vereda San José del Chunga. ca. 2200 m. 19 Jan 2007, flowered in cultivation Mar 2007. ex cult. Medina T. 466 (holotype: HPUJ, MEDEL –photos!, UGDA –drawing!).
 Distribution: — Colombia.
 Notes:— Myoxanthus ortizianus is similar to M. priapus; they share the purple-yellow flowers covered abaxially with short trichomes, lateral sepals forming a suborbicular synsepal, petals yellowish purple-stripped, obovate to oblong basally, then contracted, and lip with a thick, erect basal callus. However, the former is distinguished by its narrower petal apex forming a slender tail vs. apex narrow not forming a slender tail, and a scarcely trilobed lip with rounded lateral lobes below the middle vs. lip oblong with small acute lateral lobes near the middle.
description: Published as part of Rojas-Alvarado, Gustavo, Blanco, Mario A. & Karremans, Adam P., 2021, A taxonomic synopsis and morphological characterization of Myoxanthus (Orchidaceae: Pleurothallidinae), pp. 211-258 in Phytotaxa 507 (3) on pages 242-243, DOI: 10.11646/phytotaxa.507.3.1, http://zenodo.org/record/5425729
Mean-field and cumulant approaches to modelling organic polariton physics
Creators: name: Fowler-Wright, Piper
Publisher: name: arXiv
Year: 2024
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this thesis we develop methods for many-body open quantum systems and apply them to systems of organic polaritons. The methods employ a mean-field approach to reduce the dimensionality of large-scale problems. Initially assuming the absence of correlations in the many-body state, this approach is built upon in two ways.
 First, we show how the mean-field approximation can be combined with matrix product operator methods to efficiently simulate the non-Markovian dynamics of a many-body system with strong coupling to multiple environments. We apply this method to calculate the threshold and photoluminescence for a realistic model of an organic laser.
 Second, we extend the mean-field description by systematically including higher-order correlations via cumulant expansions of the Heisenberg equations of motion. We investigate the validity and convergence properties of these expansions, both with respect to expansion order and system size, for many-body systems with many-to-one network structures. We then show how the cumulant expansions may be used to calculate spatially resolved dynamics of organic polaritons. This enables a study of organic polariton transport in which we observe reversible conversion to dark exciton states and sub-group-velocity propagation.
 The methods established in this work offer versatile tools for analysing large, many-body open quantum systems and investigating finite-size effects. Their application reveals the intricate dynamics of organic polaritons resulting from the interplay of strong light-matter coupling and vibrational effects.
description: PhD Thesis
The build-up of halos within Press-Schechter theory
Creators: name: Percival, Will J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Modelling the build-up of halos is important for linking the formation of galaxies with cosmological models. A simple model of halo growth is provided by Press-Schechter (PS) theory, where the initial field of density fluctuations is smoothed using spherically symmetric filters centred on a given position to obtain information about the likelihood of later collapse on varying scales. In this paper the predicted halo mass growth is compared for three filter shapes: Gaussian, top-hat and sharp k-space. Preliminary work is also presented analysing the build-up of halos within numerical simulations using a friends-of-friends group finder. The best-fit to the simulation mass function was obtained using PS theory with a top-hat filter. By comparing both the backwards conditional mass function, which gives the distribution of halo progenitors, and the distribution of halo mergers in time, the build-up of halos in the simulations is shown to be better fitted by PS theory with a sharp k-space filter. This strengthens previous work, which also found the build-up of halos in simulations to be well matched to PS theory with a sharp k-space filter by providing a direct comparison of different filters and by extending the statistical tools used to analyse halo mass growth. The usefulness of this work is illustrated by showing that the cosmological evolution in the proportion of halos that have undergone recent merger is predicted to be independent of mass and power spectrum and to only depend upon cosmology. Recent results from observations of field galaxies are shown to match the evolution expected, but are not sufficiently accurate to usefully distinguish between cosmological parameters.
description: 10 pages, 8 figures, accepted for publication in MNRAS
title: 02_0563
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Additional file 1: of Mortality after osteoporotic hip fracture: incidence, trends, and associated factors
Creators: name: Guzon-Illescas, Olalla
name: Fernandez, Elia Perez
name: Villarias, Natalia Crespí
name: Donate, Francisco Quirós
name: Peña, Marina
name: Alonso-Blas, Carlos
name: García-Vadillo, Alberto
name: Mazzucchelli, Ramon
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Developmental Biology
subject: Science Policy

description: Figure S1. Supplementary material. Survival analysis by sex. (DOCX 153 kb)