cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Anthoscopus caroli subsp. winterbottomi C. M. N. White 1946
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Remizidae
Anthoscopus
Anthoscopus caroli
Anthoscopus caroli winterbottomi c.m.n. white

description: Anthoscopus caroli winterbottomi C.M.N. White
 Anthoscopus caroli winterbottomi C.M.N. White, 1946: 101 (Mwinilunga).
 Now Anthoscopus caroli winterbottomi C.M.N. White, 1946. See Snow, 1967b: 67, Fry et al., 2000: 112–115, and Madge, 2008: 72–73.
 HOLOTYPE: AMNH 704561, male, collected east of Mwinilunga, 11.44S, 24.24E (Times Atlas), Zambia, on 31 October 1939, by Charles M.N. White.
 COMMENTS: In the original description, White noted that the type, then in his collection, was a male collected on 31 October, 1939 at Mwinilunga and that he had a type series of seven specimens. In 1953, White gave AMNH six of his seven specimens, including the holotype bearing his red type label on which he had written ‘‘Type of Anthoscopus caroli winterbottomi.’’ The five paratypes in AMNH are: Mwinilunga, AMNH 704556, unsexed, 31 October 1939; AMNH 704557, male, 15 July 1946; AMNH 704558, female, 22 December [year not noted]; AMNH 704559, female, 16 April 1944; Lusaka, AMNH 704560, female, 27 July [year not noted]. Snow (1967b: 67) considered winterbottomi a synonym of A. c. robertsi, but it was recognized as valid by Fry et al. (2000: 112–115) and Madge (2008: 72–73).
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on page 64
BaRT gene annotation on Golden Promise reference assembly by association
Creators: name: Schreiber
Publisher: name: figshare
Year: 2019
Subjects: Computational Biology

description: Gene annotation by associationBaRT (Rapazote-Flores et al., 2019) gene annotation mapped onto Golden Promise assembly using Gmap (version 2018-03-25; parameters: -f 2 -n 1 --min-trimmed-coverage=0.8 --min-identity=0.9).
The Stellar CME-flare relation: What do historic observations reveal?
Creators: name: Moschou, Sofia-Paraskevi
name: Drake, Jeremy J.
name: Cohen, Ofer
name: Alvarado-Gómez, Julián D.
name: Garraffo, Cecilia
name: Fraschetti, Federico
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Solar CMEs and flares have a statistically well defined relation, with more energetic X-ray flares corresponding to faster and more massive CMEs. How this relation extends to more magnetically active stars is a subject of open research. Here, we study the most probable stellar CME candidates associated with flares captured in the literature to date, all of which were observed on magnetically active stars. We use a simple CME model to derive masses and kinetic energies from observed quantities, and transform associated flare data to the GOES 1--8~Å band. Derived CME masses range from $\sim 10^{15}$ to $10^{22}$~g. Associated flare X-ray energies range from $10^{31}$ to $10^{37}$~erg. Stellar CME masses as a function of associated flare energy generally lie along or below the extrapolated mean for solar events. In contrast, CME kinetic energies lie below the analogous solar extrapolation by roughly two orders of magnitude, indicating approximate parity between flare X-ray and CME kinetic energies. These results suggest that the CMEs associated with very energetic flares on active stars are more limited in terms of the ejecta velocity than the ejecta mass, possibly because of the restraining influence of strong overlying magnetic fields and stellar wind drag. Lower CME kinetic energies and velocities present a more optimistic scenario for the effects of CME impacts on exoplanets in close proximity to active stellar hosts.
description: 23 pages, 3 tables, 4 figures, accepted by ApJ
Anthoscopus sharpei Hartert
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Remizidae
Anthoscopus
Anthoscopus sharpei

description: Anthoscopus sharpei Hartert
 Anthoscopus sharpei Hartert, 1905b: 75 (Usambiro).
 Now Anthoscopus caroli sharpei Hartert, 1905. See Snow, 1967b: 67, Fry et al., 2000: 112–115, and Madge, 2008: 72–73.
 HOLOTYPE: AMNH 683337, female, collected at Usambiro, ca. 03.05S, 32.40E (Polhill, 1988), Tanzania, on 8 September 1889, by Emin Pasha (no. 336). From the Rothschild Collection.
 COMMENTS: The holotype is the only specimen of this form collected by Emin now in AMNH, and its data agree with those given by Hartert for his type. Hartert (1920a: 441) confirmed its type status by giving Emin’s field number. Snow (1967b: 67) considered sharpei a synonym of the monotypic species Anthoscopus sylviella; Fry et al. (2000: 112–115) and Madge (2008: 72–73) recognized it as a valid subspecies of A. caroli.
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on page 64
Better Paracoherent Answer Sets with Less Resources
Creators: name: Amendola, Giovanni
name: Dodaro, Carmine
name: Ricca, Francesco
Publisher: name: arXiv
Year: 2019
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Answer Set Programming (ASP) is a well-established formalism for logic programming. Problem solving in ASP requires to write an ASP program whose answers sets correspond to solutions. Albeit the non-existence of answer sets for some ASP programs can be considered as a modeling feature, it turns out to be a weakness in many other cases, and especially for query answering. Paracoherent answer set semantics extend the classical semantics of ASP to draw meaningful conclusions also from incoherent programs, with the result of increasing the range of applications of ASP. State of the art implementations of paracoherent ASP adopt the semi-equilibrium semantics, but cannot be lifted straightforwardly to compute efficiently the (better) split semi-equilibrium semantics that discards undesirable semi-equilibrium models. In this paper an efficient evaluation technique for computing a split semi-equilibrium model is presented. An experiment on hard benchmarks shows that better paracoherent answer sets can be computed consuming less computational resources than existing methods. Under consideration for acceptance in TPLP.
description: Paper presented at the 35th International Conference on Logic Programming (ICLP 2019), Las Cruces, New Mexico, USA, 20-25 September 2019, 15 pages
Spatial correlations in hexagons generated via a Kerr nonlinearity
Creators: name: Gatti, Alessandra
name: Mancini, Stefano
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider the hexagonal pattern forming in the cross-section of an optical beam produced by a Kerr cavity, and we study the quantum correlations characterizing this structure. By using arguments related to the symmetry broken by the pattern formation, we identify a complete scenario of six-mode entanglement. Five independent phase quadratures combinations, connecting the hexagonal modes, are shown to exhibit sub-shot-noise fluctuations. By means of a non-linear quantum calculation technique, quantum correlations among the mode photon numbers are demonstrated and calculated.
description: ReVTeX file, 20 pages, 7 eps figures
title: Selèction: UNICAmagazine n.2/2025
Creators: name: Università degli Studi di Cagliari
Publisher: name: UNICApress
Year: 2025

description: "La ricerca produce conoscenza, insegna saperi moderni, accultura il territorio, genera trasferimento tecnologico. UniCa riconosce la ricerca come ragione costitutiva dell’Università e, tenacemente fedele al proprio profilo generalista, la promuove libera e aperta in tutti gli ambiti delle scienze umanistiche e sociali, naturali e ingegneristiche, bio-mediche."

Dall'editoriale del Prorettore delegato per la ricerca dell’Università degli Studi di Cagliari, Prof. Luciano Colombo

"La scelta del percorso postdiploma più adatto alle attitudini ed aspirazioni di ogni persona è un processo lungo e articolato che UniCA cerca di facilitare mettendo a disposizione molteplici servizi di supporto alla scelta informata e consapevole.
Il servizio di tutorato di orientamento tramite sei esperte di orientamento è sempre attivo per fornire informazioni sui corsi di studio, sulle modalità di accesso e di iscrizione, nonché sulla prosecuzione degli studi dopo la laurea."

Dall'editoriale della Prorettrice delegata per l'orientamento e Alumni dell’Università degli Studi di Cagliari, Prof.ssa Valentina Onnis
[Enveloppes de correspondance]
Creators: name: Plusieurs Auteurs
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2025
Subjects: Correspondance

description: Destinataire : Tejera, Nivaria
description: Ensemble d’enveloppes, de dates et d’auteurs différents, n’ayant pu être liées à des lettres indexées dans le fonds d’archives Nivaria Tejera.
description: Conjunto de sobres, de fechas y autores diferentes, que no pudieron vincularse a cartas indexadas en el fondo de archivos Nivaria Tejera
description: Source: NT-AB-0000-000
description: Source: Localisation du document : Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
description: created: inconnue
No ghost state of Gauss-Bonnet interaction in warped backgrounds
Creators: name: Cho, Y. M.
name: Neupane, Ishwaree P.
name: Wesson, P. S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A general solution to the Einstein field equations with Gauss-Bonnet(GB) term in the $AdS_5$ bulk background implies that the GB coupling $α$ can take either sign (+ or -), though a positive $α$ will be more meaningful. By considering linearized gravity with the GB term in the Randall-Sundrum(RS) a singular 3-brane model, we study the gravitational interactions between matter sources localized on the brane. With a correctly defined boundary condition on the brane, we find a smooth behavior of graviton propagator and hence the zero-mode solution as a 4d massless graviton localized on the brane with correct momentum and tensor structures. The coupling $α$ modifies the graviton propagators both on the brane and in the bulk. The issue on ghost state of the GB term is resolved, and we find that there is no real ghost (negative norm) state of the GB term in the RS single brane picture. The latter condition leads to a consistency in the coupling between the brane matter and the bulk gravity. We also elucidate about the possibilities for behavior of a test particle on the brane and in the bulk.
description: 24 pages, LaTex, minor correction to discussion, replaced with NPB version
Emergence of localized persistent weakly-evanescent cortical brain wave loops
Creators: name: Galinsky, Vitaly L.
name: Frank, Lawrence R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: An inhomogeneous anisotropic physical model of the brain cortex is presented that predicts the emergence of non--evanescent (weakly damped) wave--like modes propagating in the thin cortex layers transverse to both the mean neural fiber direction and to the cortex spatial gradient. Although the amplitude of these modes stays below the typically observed axon spiking potential, the lifetime of these modes may significantly exceed the spiking potential inverse decay constant. Full brain numerical simulations based on parameters extracted from diffusion and structural MRI confirm the existence and extended duration of these wave modes. Contrary to the commonly agreed paradigm that the neural fibers determine the pathways for signal propagation in the brain, the signal propagation due to the cortex wave modes in the highly folded areas will exhibit no apparent correlation with the fiber directions. The results are consistent with numerous recent experimental animal and human brain studies demonstrating the existence electrostatic field activity in the form of traveling waves (including studies where neuronal connections were severed) and with wave loop induced peaks observed in EEG spectra. The localization and persistence of these cortical wave modes has significant implications in particular for neuroimaging methods that detect electromagnetic physiological activity, such as EEG and MEG, and for the understanding of brain activity in general, including mechanisms of memory.
[Queridos amigos: Cómo me alegra su entusiasmo.]
Creators: name: Luis, Marré
name: Marré, Luis
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2025
Subjects: Littérature
Études
Droits Diplomatiques

description: Destinataire : Jamís, Fayad / Tejera, Nivaria
description: L’auteur évoque : une nouvelle de Pedro de Oraá, ‘’El Aposento Oculto’’, Francisco Antigua, Eduardo, Pepe, ses études, la sortie de ‘’El Ciclón’’, ‘’Sala de Sueños’’, Sigismundo, Federico García Lorca, Antonio Machado, André Breton, Ernest Hemingway...
description: El autor menciona: un cuento de Pedro de Oraá, ''El Aposento Oculto'', Francisco Antigua, Eduardo, Pepe, sus estudios, el estreno de ''El Ciclón'', ''Sala de Sueños'' , Sigismundo, Federico García Lorca, Antonio Machado, André Breton, Ernest Hemingway…
description: Note : Lettre avec son enveloppe.
description: Source: NT-AB-1955-03-15
description: Source: Localisation du document : Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
Supplementary material.docx
Creators: name: Flores, Carlos
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: In order to verify that cases and controls from the discovery stage were similar in terms of genetic admixtures, we first run a model-based analysis including data from reference populations from EUR, NAF and SSA. At the best fitting number of ancestry partitions (k=4)1, reference African populations showed two distinct ancestry clusters that reached maximum values in NAF or in SSA (Figure S2). The other two ancestry clusters had their maximum values among the EUR references. Based on our profound previous assessments (Guillen-Guio et al., 2018), these clusters can be considered as precise estimates of NAF (20% in cases, 22% in controls), SSA (4% in cases, 3% in controls) and EUR (76% in cases, 75% in controls) ancestry components in the study sample (Figure S2). In fact, differences in their averages were subtle, strongly supporting of an effective ancestry matching among samples. This also occurs in samples from the replication stage.
Tritex gene annotation on Golden Promise reference assembly by association
Creators: name: Schreiber
Publisher: name: figshare
Year: 2020
Subjects: Computational Biology

description: Gene annotation by association
Tritex (Monat et al., 2019) gene annotation mapped onto Golden Promise assembly using Gmap (version 2018-03-25; parameters: -f 2 -n 1 --min-trimmed-coverage=0.8 --min-identity=0.9)
Surface Brightness Profiles and Structural Parameters for Globular Clusters in the Fornax and Sagittarius Dwarf Spheroidal Galaxies
Creators: name: Mackey, A. D.
name: Gilmore, G. F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present radial surface brightness profiles for all five globular clusters in the Fornax dwarf spheroidal galaxy, and for the four present members of the Sagittarius dwarf spheroidal galaxy. These profiles are derived from archival Hubble Space Telescope observations, and have been calculated using the same techniques with which we measured profiles in our previous studies of LMC and SMC clusters (astro-ph/0209031 and astro-ph/0209046 respectively), apart from some small modifications. From the surface brightness profiles, we have determined structural parameters for each cluster, including core radii and luminosity and mass estimates. We also provide a brief summary of literature measurements of other parameters for these clusters, including their ages, metallicities and distances. Our core radius measurements are mostly in good agreement with those from previous lower resolution studies, although for several clusters our new values are significantly different. The profile for Fornax cluster 5 does not appear to be well fit by a King-type model and we suggest that it is a post core-collapse candidate. We examine the distribution of cluster core radii in each of the two dwarf galaxy systems, and compare these with the distribution of core radii for old LMC clusters. The three distributions match within the limits of measurement errors and the small sample sizes. We discuss the implications of this in the context of the radius-age trend we have previously highlighted for the Magellanic Cloud clusters.
description: 16 pages, 6 figures. Accepted for publication in MNRAS. We recommend that the interested reader visit http://www.ast.cam.ac.uk/STELLARPOPS/dSph_clusters/ for on-line data and the full resolution paper
Mesochorus atriventris Cresson 1872
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Mesochorus
Mesochorus atriventris

description: Mesochorus atriventris Cresson, 1872, syn. sylvarum auct. non CURTIS
M a t e r i a l: H 1: 2♀♀ 1♂ 15-25. VI, 1♀ 25.VI-5.VII; H 4: 1♀ 25.V-4. VI; H 6: 1♀ 23.V-13. VI.
D i s t r i b u t i o n: Holarctic and Oriental regions, new for Georgia and the Caucasus region.
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1483, DOI: 10.5281/zenodo.5275090
Anthoscopus rothschildi Neumann
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Remizidae
Anthoscopus
Anthoscopus rothschildi

description: Anthoscopus rothschildi Neumann
 Anthoscopus rothschildi Neumann, 1907a: 597 (Simba).
 Now Anthoscopus caroli sylviella Reichenow, 1904. See Fry et al., 2000: 112–115, and Madge, 2008: 72–73.
 HOLOTYPE: AMNH 683335, female, collected at Simba, 3350 ft, 02.09S, 37.36E (Polhill, 1988), Kenya, on 18 January 1906, by C.F. Camburn (no. 55). From the Rothschild Collection.
COMMENTS: Neumann had the single specimen. The name of the collector, indicated on the original label as ‘‘C.F.C.,’’ has been transcribed erroneously onto the Rothschild type label as ‘‘F.C. Coburn.’’ The original label is printed ‘‘Collection Maurice de Rothschild.’’ J.P. Chapin’s collector’s cards in the archives of the Department of Ornithology note that Camburn collected in Congo (Kinshasa) in 1906, but under whose auspices is not mentioned. Maurice de Rothschild’s expedition to Africa was earlier, 1904–1905, but he apparently purchased specimens collected later by Camburn.
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on page 64
Solutions of the boundary Yang-Baxter equation for arbitrary spin
Creators: name: Delius, G. W.
name: Nepomechie, Rafael I.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We use boundary quantum group symmetry to obtain recursion formulas which determine nondiagonal solutions of the boundary Yang-Baxter equation (reflection equation) of the XXZ type for any spin j.
description: 10 pages, LaTeX, no figures
Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST
Creators: name: Mardini, Mohammad K.
name: Li, Haining
name: Placco, Vinicius M.
name: Alexeeva, Sofya
name: Carollo, Daniela
name: Taani, Ali
name: Ablimit, Iminhaji
name: Wang, Liang
name: Zhao, Gang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report on the discovery of five carbon-enhanced metal-poor (CEMP) stars in the metallicity range of $-3.3
Pseudo-Hermiticity of Hamiltonians under imaginary shift of the co-ordinate : real spectrum of complex potentials
Creators: name: Ahmed, Zafar
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose that the real spectrum and the orthogonality of the states for several known complex potentials of both types, PT-symmetric and non-PT-symmetric can be understood in terms of currently proposed $η$-pseudo-Hermiticity (Mostafazadeh, quant-ph/0107001) of a Hamiltonian, provided the Hermitian linear automorphism, $η$, is introduced as $e^{-θp}$ which affects an imaginary shift of the co-ordinate : $e^{-θp} x e^{θp} = x+iθ$.
description: 7 pages, no figure, eq.5 is changed, eqs.6a-e added, submitted to Phys. Lett. A
Conirostrum ornatum Lawrence
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Thraupidae
Conirostrum
Conirostrum ornatum

description: Conirostrum ornatum Lawrence
 Conirostrum ornatum Lawrence, 1851: 112 (no locality given).
 Now Auriparus flaviceps ornatus (Lawrence, 1851). See Webster, 1999: 3, and Madge, 2008: 74.
 SYNTYPE: AMNH 39401, unsexed, collected at Brownsville, 25.54N, 97.30W (Times Atlas), Texas, USA, no date, by Capt. J.P. McCown. From the G.N. Lawrence Collection.
 COMMENTS: No type was designated in the original description, Lawrence only saying that he examined two specimens; the above specimen is the only one in AMNH from the Lawrence Collection that was collected before the publication of ornatum, undoubtedly in 1850 when McCown was stationed at Brownsville (Mearns and Mearns, 1992: 301). It is illustrated in Lawrence (1851: pl. 5, fig. 1). The original label is not with this specimen; on the Lawrence label, the number 300 appears, the significance of which is unknown. The publication date of this form is often given as 1852 (e.g., Snow, 1967b: 69); although it was included in volume 5 of the Annals of the Lycaeum of Natural History of New York, dated 1852, the description of ornatum was in part 3, issued in May 1851 (Foster, 1892: 2, and LeCroy, personal observation).
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on page 65
Additional file 2 of Chest high-resolution computed tomography can make higher accurate stages for thoracic sarcoidosis than X-ray
Creators: name: Zhang, Yuan
name: Du, Shan-shan
name: Zhao, Meng-meng
name: Li, Qiu-hong
name: Zhou, Ying
name: Song, Jia-cui
name: Chen, Tao
name: Shi, Jing-yun
name: Jie, Bing
name: Li, Wei
name: Shen, Li
name: Zhang, Fen
name: Su, Yi-liang
name: Hu, Yang
name: Lower, Elyse E.
name: Baughman, Robert P.
name: Li, Huiping
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 2. Tables S1 and S2. Table S1. Reasons for the inconsistent stage determined according to CXR and HRCT presentations. Table S2. Pleural involvement in the patients.
[Querida Nivaria: Te envío ahora un ejemplar de la miniplaquette]
Creators: name: Emilio Adolfo, Westphalen
name: Westphalen, Emilio Adolfo
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2025
Subjects: Vie personnelle
Vie professionnelle
Exposition

description: Destinataire : Tejera, Nivaria
description: L’auteur évoque : l’envoi d’une plaquette faite par le poète Domingo (?) illustrée par sa femme Judith Westphallen (il donne des détails à ce sujet), son départ de Lisbonne, son état d’esprit, la réception de sa lettre, des préparatifs pour une exposition de Tejera, des affaires à régler à Lima, la publication d’une plaquette avec un texte inédit de César Moro arrangée avec Armando Rojas, les éditions Cátedra en Espagne pour un livre publié par FCE (Fondo de Cultura Económica, Mexico), et sa fille Silvia.
description: El autor menciona: el envío de un folleto hecho por el poeta Domingo ilustrado por su esposa Judith Westphallen (da detalles sobre este tema), su partida de Lisboa, su estado de ánimo, la recepción de su carta, preparativos para una exposición de Tejera, asuntos pendientes en Lima, publicación de un folleto con un texto inédito de César Moro arreglado con Armando Rojas, la editorial Cátedra en España para un libro publicado por FCE (Fondo de Cultura Económica, México), y su hija Silvia.
description: Source: NT-AB-1983-11-25
description: Source: Localisation du document : Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
Additional file 1: of Salicylic acid-induced differential resistance to the Tomato yellow leaf curl virus among resistant and susceptible tomato cultivars
Creators: name: Li, Tong
name: Huang, Ying
name: Xu, Zhi-Sheng
name: Wang, Feng
name: Xiong, Ai-Sheng
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: Ecology
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Figure S1. HPLC chromatogram of ascorbic acid (AsA) in two tomato cultivars at 4 days after infected with TYLCV (a), (e) The standard curve of AsA. (b), (c), (d) The HPLC chromatogram of AsA in salicylic acid (SA), TYLCV, and SA + TYLCV treated plants in ‘Zhefen-702’ at 4 days post inoculated (dpi) with TYLCV. (f), (g), (h) The HPLC chromatogram of AsA in SA, TYLCV, and SA + TYLCV treated plants in ‘Jinpeng-1’ at 4 dpi. Figure S2. Phenotype enlargement of SA + TYLCV and only TYLCV treated plants in ‘Zhefen-702’ during whole experiment period. Figure S3. Phenotype enlargement of SA + TYLCV and only TYLCV treated plants in ‘Jinpeng-1’ during whole experiment period. (DOCX 2033 kb)
Stable Solitons in Field Theory Models for Tachyon Condensation
Creators: name: Jatkar, Dileep P.
name: Vathsan, Radhika
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study soliton solutions in scalar field theory with a variety of unbounded potentials. A subset of these potentials have Gaussian lump solutions and their fluctuation spectrum is governed by the harmonic oscillator problem. These lumps are unstable with one tachyonic mode. Soliton solutions in several other classes of potentials are stable and are of kink type. The problem of the stability of these solutions is related to a supersymmetric quantum mechanics problem. The fluctuation spectrum is not equispaced and does not contain any tachyonic mode. The lowest energy mode is the massless Goldstone mode which restores broken translation invariance.
description: Latex, 13 pages, 3 figures; references updated
The PRIMPing Routine -- Tiling through Proximal Alternating Linearized Minimization
Creators: name: Hess, Sibylle
name: Morik, Katharina
name: Piatkowski, Nico
Publisher: name: arXiv
Year: 2019
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Mining and exploring databases should provide users with knowledge and new insights. Tiles of data strive to unveil true underlying structure and distinguish valuable information from various kinds of noise. We propose a novel Boolean matrix factorization algorithm to solve the tiling problem, based on recent results from optimization theory. In contrast to existing work, the new algorithm minimizes the description length of the resulting factorization. This approach is well known for model selection and data compression, but not for finding suitable factorizations via numerical optimization. We demonstrate the superior robustness of the new approach in the presence of several kinds of noise and types of underlying structure. Moreover, our general framework can work with any cost measure having a suitable real-valued relaxation. Thereby, no convexity assumptions have to be met. The experimental results on synthetic data and image data show that the new method identifies interpretable patterns which explain the data almost always better than the competing algorithms.
Efficient Deep Learning Techniques for Multiphase Flow Simulation in Heterogeneous Porous Media
Creators: name: Wang, Yating
name: Lin, Guang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: We present efficient deep learning techniques for approximating flow and transport equations for both single phase and two-phase flow problems. The proposed methods take advantages of the sparsity structures in the underlying discrete systems and can be served as efficient alternatives to the system solvers at the full order. In particular, for the flow problem, we design a network with convolutional and locally connected layers to perform model reductions. Moreover, we employ a custom loss function to impose local mass conservation constraints. This helps to preserve the physical property of velocity solution which we are interested in learning. For the saturation problem, we propose a residual type of network to approximate the dynamics. Our main contribution here is the design of custom sparsely connected layers which take into account the inherent sparse interaction between the input and output. After training, the approximated feed-forward map can be applied iteratively to predict solutions in the long range. Our trained networks, especially in two-phase flow where the maps are nonlinear, show their great potential in accurately approximating the underlying physical system and improvement in computational efficiency. Some numerical experiments are performed and discussed to demonstrate the performance of our proposed techniques.
Parus subpalustris Brehm
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paridae
Parus
Parus subpalustris

description: Parus subpalustris Brehm
 Parus subpalustris Brehm, 1855: 242 (Deutschland).
 Now Poecile palustris palustris (Linnaeus, 1758). See Hartert, 1918a: 27, Snow, 1967c: 72, and Gosler and Clement, 2007: 711–712.
 SYNTYPES: AMNH 455866, male, and AMNH 455867, female, both collected at Renthendorf, 50.48N, 11.58E (USBGN, 1959), Germany, on 4 January 1851; and AMNH 455868, immature female, collected in the Roda River Valley (5 Rodathal, as on label), Germany, on 1 June 1853. From the Brehm Collection via the Rothschild Collection.
 COMMENTS: Brehm, in the original description, did not indicate a type or give the number of specimens he examined. Hartert (1918a: 27) listed the above pair as the ‘‘types,’’ noting that as all of the specimens were from Renthendorf, that was the ‘‘terra typica.’’ These two specimens are tied together and bear a single Rothschild type label. This does not represent the designation of a lectotype, and I consider all of the Brehm specimens labeled subpaulustris by Brehm and collected before the publication of the name in 1855 to be syntypes. The third syntype in AMNH was not listed by Hartert, but is labeled subpalustris by Brehm. It has been given an AMNH type label and included in the type collection. AMNH 455859–455868 were all cataloged as subpalustris and all except the three listed above were exchanged to ZFMK; if any or all were collected before 1855 and labeled subpalustris by Brehm, they are also syntypes.
 Hartert (1918a: 27) synonymized subpalustris with P. p. communis, which Snow (1967c: 72) considered a synonym of P. p. palustris. Until recently palustris usually has been included in the broad genus Parus, and this is still preferred by some authors. Gill et al. (2005) suggested elevating five subgenera within Parus to generic status to reflect the phylogeny obtained in their study of mitochondrial cytochrome-b in the Paridae, and placed palustris in the genus Poecile. See David and Gosselin (2008: 19) for use of masculine endings with this genus.
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on pages 65-66
Tritex gene annotation on Golden Promise reference assembly by association
Creators: name: Schreiber
Publisher: name: figshare
Year: 2019
Subjects: Computational Biology

description: Gene annotation by association
Tritex (Monat et al., 2019) gene annotation mapped onto Golden Promise assembly using Gmap (version 2018-03-25; parameters: -f 2 -n 1 --min-trimmed-coverage=0.8 --min-identity=0.9)
Perturbation theory for quantum-mechanical observables
Creators: name: Franson, J. D.
name: Donegan, Michelle M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum-mechanical state vector is not directly observable even though it is the fundamental variable that appears in Schrodinger's equation. In conventional time-dependent perturbation theory, the state vector must be calculated before the experimentally-observable expectation values of relevant operators can be computed. We discuss an alternative form of time-dependent perturbation theory in which the observable expectation values are calculated directly and expressed in the form of nested commutators. This result is consistent with the fact that the commutation relations determine the properties of a quantum system, while the commutators often have a form that simplifies the calculation and avoids canceling terms. The usefulness of this method is illustrated using several problems of interest in quantum optics and quantum information processing.
description: Submitted to Phys. Rev. A. 17 pages, 4 figures. Minor changes
[Cher client, Nous avons le plaisir de vous confirmer]
Creators: name: Apple Assistance
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2025
Subjects: Vie personnelle

description: Destinataire : Tejera, Nivaria
description: Confirmation d’accès à un service d’assistance téléphonique.
description: Confirmación de acceso a un servicio de asistencia telefónica.
description: Note : Papier à en-tête : Centre Apple Assistance. 91975, Les Ulis.
description: Source: NT-AB-1996-08-16
description: Source: Localisation du document : Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
Sulfur-Bearing Species Tracing the Disk/Envelope System in the Class I Protostellar Source Elias 29
Creators: name: Oya, Yoko
name: López-Sepulcre, Ana
name: Sakai, Nami
name: Watanabe, Yoshimasa
name: Higuchi, Aya E.
name: Hirota, Tomoya
name: Aikawa, Yuri
name: Sakai, Takeshi
name: Ceccarelli, Cecilia
name: Lefloch, Bertrand
name: Caux, Emmanuel
name: Vastel, Charlotte
name: Kahane, Claudine
name: Yamamoto, Satoshi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have observed the Class I protostellar source Elias 29 with Atacama Large Millimeter/submillimeter Array (ALMA). We have detected CS, SO, $^{34}$SO, SO$_2$, and SiO line emissions in a compact component concentrated near the protostar and a ridge component separated from the protostar by 4\arcsec\ ($\sim 500$ au). The former component is found to be abundant in SO and SO$_2$ but deficient in CS. The abundance ratio SO/CS is as high as $3^{+13}_{-2} \times 10^2$ at the protostar, which is even higher than that in the outflow-shocked region of L1157 B1. However, organic molecules (HCOOCH$_3$, CH$_3$OCH$_3$, CCH, and c-C$_3$H$_2$) are deficient in Elias 29. We attribute the deficiency in organic molecules and richness in SO and SO$_2$ to the evolved nature of the source or the relatively high dust temperature (\protect\raisebox{-0.7ex}{$\:\stackrel{\textstyle >}{\sim}\:$} 20 K) in the parent cloud of Elias 29. The SO and SO$_2$ emissions trace rotation around the protostar. Assuming a highly inclined configuration ($i \geq 65$\degr; 0\degr\ for a face-on configuration) and Keplerian motion for simplicity, the protostellar mass is estimated to be (0.8 -- 1.0) \Msun. The $^{34}$SO and SO$_2$ emissions are asymmetric in their spectra; the blue-shifted components are weaker than the red-shifted ones. Although this may be attributed to the asymmetric molecular distribution, other possibilities are also discussed.
The Common Agricultural Policy post-2020: Views and recommendations from scientists to improve performance for biodiversity : Volume 2 - Annexes
Creators: name: Pe'er, Guy
name: Birkenstock, Maren
name: Lakner, Sebastian
name: Röder, Norbert
name: Pe'er, Guy
name: Birkenstock, Maren
name: Lakner, Sebastian
name: Röder, Norbert
Publisher: name: Unknown
Year: 2021
Subjects: subject: Agribusiness
subject: Agricultural and Food Policy
subject: Land Economics/Use
subject: CAP
subject: Common Agricultural Policy
subject: AECM
subject: eco-schemes
subject: European Union
subject: biodiversity

description: Despite significant efforts, investments and some local successes, the EU’s Common Agricultural Policy (CAP) has not succeeded in halting the loss of farmland biodiversity. To address this (and other) weaknesses, the CAP post-2020 proposes a new “Green Architecture” comprising (inter alia) compulsory elements (enhanced conditionality through Good Agricultural and Environmental Conditions - GAEC), voluntary Agri-Environment-Climate Measures (AECMs), and a new instrument called “Eco-schemes”. Will this new Green Architecture, combined with a result-based orientation of the CAP, help address the biodiversity crisis? To provide science-based feedback on this proposal, more than 300 scientists from 22 Member States (MSs) have provided their expertise through 13 workshops that took place between October and December 2020, and a follow up online survey. The results are published in Thünen Working Reports with 3 volumes. The Thünen Working Paper 175 – Volume 1 contains all results of the workshops with experts' assessment. The present Thünen Working Paper 175 – Volume 2 contains all reports of the Member-State-Workshops as well as an overview of the experts' opinions on the Flagship-Eco-schemes proposed by the EU Commission. In addition, a policy brief on the results was published in Thünen Working Paper 175 – Volume 3.
description: DOI:10.3220/WP1620647428000
On a Formation Scenario of Star Clusters
Creators: name: Theis, Christian
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Most formation scenarios of globular clusters assume a molecular cloud as the progenitor of the stellar system. However, it is still unclear, how this cloud is transformed into a star cluster, i.e. how the destructive processes related to gas removal or low star formation efficiency can be avoided. Here a scheme of supernova (SN) induced cluster formation is studied. According to this scenario an expanding SN shell accumulates the mass of the cloud. This is accompanied by fragmentation resulting in star formation in the shell. Provided the stellar shell expands sufficiently slow, its self-gravity stops the expansion and the shell recollapses, by this forming a stellar system. I present N-body simulations of collapsing shells which move in a galactic potential on circular and elliptic orbits. It is shown that typical shells (10^5 Msun, 30 pc) evolve to twin clusters over a large range of galactocentric distances. Outside this range single stellar systems are formed, whereas at small galactocentric distances the shells are tidally disrupted. In that case many small fragments formed during the collapse survive as single bound entities. About 1/3 of the twin cluster systems formed on circular orbits merge within 400 Myr. On elliptic orbits the merger rate reduces to less than 4%. Thus, there could be a significant number of twin clusters even in our Galaxy, which, however, might be undetected as twins due to a large phase shift on their common orbit.
description: 4 pages, 2 figures, to be published in "The Evolution of Galaxies. II. Basic Building Blocks", ed. M. Sauvage et al
Parus stagnatilis Brehm
Creators: name: Pachycephalidae
name: Aegithalidae
name: Remizidae
name: Paridae
name: Sittidae
name: Neosittidae
name: Certhiidae
name: Rhabdornithidae
name: Climacteridae
name: Dicaeidae
name: Pardalotidae
name: Nectariniidae, And
name: Lecroy, Mary
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Paridae
Parus
Parus stagnatilis

description: Parus stagnatilis Brehm
 Parus stagnatilis Brehm, 1855: 242 (in Galizien).
 Now Poecile palustris stagnatilis Brehm, 1855. See Hartert, 1918a: 27, and Gosler and Clement, 2007: 711–712.
 LECTOTYPE: AMNH 455853 (Kleinschmidt no. 1), adult male, collected in Poland or the Ukraine (5 Galizia), on 3 January 1853, by Count Wodzicki. From the C.L. Brehm Collection via the Rothschild Collection.
 COMMENTS: In the original description, Brehm noted that this form was from Galicia. Kleinschmidt (1897: 70) listed three Brehm specimens as syntypes, two from Galicia (Kleinschmidt nos. 1 and 2) and one from Dniester River (no. 3), and added his numbers on the reverse of the Brehm labels. Hartert (1918a: 27) listed the male specimen collected on 3 January 1853 as the type, thereby designating it the lectotype. The AMNH catalog number had been written incorrectly on this specimen as 455803; an AMNH type label has been added to correct this error. The other two syntypes listed by Kleinschmidt also came to AMNH. AMNH 455854 (no. 2), also from Galicia, and collected on 12 March, year not given in AMNH catalog, was exchanged to ZFMK. If it is labeled stagnatilis by Brehm and was collected early enough, it is a paralectotype. AMNH 455855 collected on the Dniester River, on 1 February 1851, the third syntype listed by Kleinschmidt, is a paralectotype.
description: Published as part of Pachycephalidae, Aegithalidae, Remizidae, Paridae, Sittidae, Neosittidae, Certhiidae, Rhabdornithidae, Climacteridae, Dicaeidae, Pardalotidae, Nectariniidae, And & Lecroy, Mary, 2010, Type Specimens Of Birds In The American Museum Of Natural History Part 8. Passeriformes:, pp. 1-178 in Bulletin of the American Museum of Natural History 2010 (333) on page 66
Orbital dynamics in realistic galaxy models: NGC 3726, NGC 3877 and NGC 4010
Creators: name: Dubeibe, F. L.
name: Martínez-Sicacha, Sandra M.
name: González, Guillermo A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: In the present paper, using a generalization of the Miyamoto and Nagai potential we adjusted the observed rotation curves of three specific spiral galaxies to the analytical circular velocities. The observational data have been taken from a 21 cm-line synthesis imaging survey using the Westerbork Synthesis Radio Telescope, for three particular galaxies in the Ursa Major cluster: NGC 3726, NGC 3877 and NGC 4010. Accordingly, the dynamics of the system is analyzed in terms of the Poincaré sections method, finding that for larger values of the angular momentum of the test particle or lower values its total energy the dynamics is mainly regular, while on the opposite cases, the dynamics is mainly chaotic. Our toy model opens the possibility to find chaotic bounded orbits for stars in those particular galaxies.
description: 7 pages, 9 figures
Mesochorus bipartitus SCHWENKE 1999
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Mesochorus
Mesochorus bipartitus

description: Mesochorus bipartitus SCHWENKE, 1999
M a t e r i a l: H 4-5: 1♀ 15-25.VI.
D i s t r i b u t i o n: Europe, new for Georgia and the Caucasus region.
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1483, DOI: 10.5281/zenodo.5275090