cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unconventional and Powerful Ion Sources for Solid-State Ion Exchange, Cu2SO4 and Cu3PO4: Exemplified by Synthesis of Metastable β-CuGaO2 from Stable β-LiGaO2
Creators: name: Suzuki, Issei
name: Washizu, Kako
name: Motai, Daiki
name: Kita, Masao
name: Omata, Takahisa
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: This study introduces a new method for synthesizing Cu+-containing metastable phases through ion exchange. Traditionally, CuCl has been used as a Cu+ ion source for solid-state ion exchanges; however, its thermodynamic driving force is often insufficient for complete ion exchange with Li+-containing precursors. First-principles calculations have identified Cu2SO4 and Cu3PO4 as more powerful alternatives, providing a higher driving force than CuCl. It has been experimentally demon-strated that these ion sources can open up new reaction pathways through experimental ion exchanges, such as from β-LiGaO2 to β-CuGaO2, which were previously unattainable. An important perspective provided by this study is that the poten-tial of such basic compounds to act as powerful ion sources has been overlooked, and that they were identified through straightforward first-principles calculations. This work presents the initial strategic design of an ion exchange reaction by exploring suitable ion sources, thereby expanding the potential for synthesizing metastable materials.
description: 17 pages, 8 figures
Tylospira glomerata Darragh 1991
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Struthiolariidae
Tylospira
Tylospira glomerata

description: Tylospira glomerata Darragh, 1991
Tylospira glomerata Darragh, 1991: 154, Figs 1B, C, H–J.
Distribution. Bass Basin: Fossil Bluff Sandstone (type). Age: early Miocene.
description: Published as part of Darragh, Thomas A., 2024, A checklist of Australian marine Cenozoic Mollusca, pp. 37-206 in Memoirs of Museum Victoria 83 on page 69, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
Gas Dynamics in the Central Molecular Zone and its connection with the Galactic Bar
Creators: name: Chaves-Velasquez, Leonardo
name: Gómez, Gilberto C.
name: Pérez-Villegas, Ángeles
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The innermost region of the Milky Way harbors the central molecular zone (CMZ). This region contains a large amount of molecular gas but a poor star formation rate considering the densities achieved by the gas in this region. We used the arepo code to perform a hydrodynamic and star formation simulation of the Galaxy, where a Ferrers bar was adiabatically introduced. During the stage of bar imposition, the bar strength excites density waves close to the inner Lindblad resonance guiding material toward the inner Galaxy, driving the formation of a ring that we qualitatively associate with the CMZ. During the simulation, we identified that the ring passes three main phases, namely: formation, instability, and quasi-stationary stages. During the whole evolution, and particularly in the quasi-stationary stage, we observe that the ring is associated with the x2 family of periodic orbits. Additionally, we found that most of the star formation occurs during the ring formation stage, while it drastically decreases in the instability stage. Finally, we found that when the gas has settled in a stable x2 orbit, the star formation takes place mostly after the dense gas passes the apocenter, triggering the conveyor-belt mechanism described in previous studies.
description: Accepted for publication in PASA
Atherigona kirkspriggsi Muller 2015
Creators: name: Magoai, Mokome M. J.
name: Muller, Burgert S.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Atherigona
Atherigona kirkspriggsi

description: Atherigona kirkspriggsi Muller, 2015
Fig. 7
Atherigona kirkspriggsi Muller, 2015: 875, fig. 33.
Material examined.
Lesotho • 17 ♂; Leribe District, Motebong Lodge, Katse Dam area; 29 ° 6.060 ' S, 28 ° 30.084 ' E; 2063 m; 10–13 Dec. 2021; J. M. Midgley, B. Muller leg.; Malaise trap, Garden entertainment area; (BMSA (D) 130773, 130775, 130776, 130777, 130778, 130779, 130783, 130809, 130810, 130826, 130844, 130848, (NMSA - DIP 213809, 213810, 213812, 213813, 213814)) • 1 ♂; Quting, Mphaki Farmers Training Centre; 30 ° 11.598 ' S, 28 ° 7.831 ' E; 2046 m; 01–27 Nov. – Dec. 2022; K. Jordaens, J. Midgley, B. Muller and G. Theron leg.; Malaise trap, Lesotho Highland Basalt Grassland, Garden; BMSA (D) 134687.
Diagnosis.
This species is similar to Atherigona lineata torrida Deeming, 1971. However, it differs from it by having a tridentate hypopygial prominence (Fig. 7) and infuscated mid and hind leg tarsi, compared to the bifurcated hypopygial prominence and brown tarsi in Atherigona lineata lineata (Adams, 1905).
Distribution.
Lesotho (new record), South Africa.
description: Published as part of Magoai, Mokome M. J. & Muller, Burgert S., 2024, The first record of Atherigona from Lesotho (Diptera, Muscidae), with description of a new species, pp. 49-60 in African Invertebrates 65 (2) on pages 49-60, DOI: 10.3897/afrinvertebr.65.131744
The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
Creators: name: Ahlborn, F.
name: Bellinger, E. P.
name: Hekker, S.
name: Basu, S.
name: Mokrytska, D.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Rotation is an important, yet poorly-modelled phenomenon of stellar structure and evolution. Accurate estimates of internal rotation rates are therefore valuable for constraining stellar evolution models. We aim to assess the accuracy of asteroseismic estimates of internal rotation rates and how these depend on the fundamental stellar parameters. We apply the recently-developed method called extended-MOLA inversions to infer localised estimates of internal rotation rates of synthetic observations of red giants. We search for suitable reference stellar models following a grid-based approach, and assess the robustness of the resulting inferences to the choice of reference model. We find that matching the mixed mode pattern between the observation and the reference model is an important criterion to select suitable reference models. We propose to i) select a set of reference models based on the correlation between the observed rotational splittings and the mode-trapping parameter ii) compute rotation rates for all these models iii) use the mean value obtained across the whole set as the estimate of the internal rotation rates. We find that the effect of a near surface perturbation in the synthetic observations on the rotation rates estimated based on the correlation between the observed rotational splittings and the mode-trapping parameter is negligible. We conclude that when using an ensemble of reference models, constructed based on matching the mixed mode pattern, the input rotation rates can be recovered across a range of fundamental stellar parameters like mass, mixing-length parameter and composition. Further, red-giant rotation rates determined in this way are also independent of a near surface perturbation of stellar structure.
description: 23 pages, 16 figures, Accepted for publication in Astronomy and Astrophysics
title: Rapport de voyage, Flandre (1952) : Ligne de New York, 1958, voyage n°7
Creators: name: Bothorel, Robert
name: Joubert, Roger
name: Robichon, Yves
name: Vincelet, Louis
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Compagnie Générale Transatlantique
subject: Transports maritimes - Histoire
subject: Marine marchande
subject: Journaux de bord

description: Chapitrage : Rapport d'inspecteurs - Rapport général / du capitaine - Rapport du commissaire - Rapport du second - Rapport de l'officier de sécurité - Rapport de l'officier de navigation - Rapport du médecin - Rapport contentieux
description: Source: French Lines & Compagnies, 1997 004 4990-38
description: Coverage: 1958-07-11/1958-07-26
Latin Majuscule Writing with semicursive hand in Herculaneum papyri
Creators: name: Marichal, Robert
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015

description: vue 166
description: "Study of the following Latin papyri: P.Herc. 206, 215, 218, 394, 457, 502, 514, 902, 804, 1254, 1257, 1557, 1774. All papyri are listed on the cover page of the main folder, and sometimes they are accompanied by brief bibliographical notes. The indication 'Vu 54 - fini - Revue 58' is written at the end of the list. The study related to each papyrus is enclosed in one folder with the number of the papyrus written on the upper right corner; in one case the sheets related to two papyri are inserted in one single folder, and one of the two numbers is written in a different ink"
description: Source: 4MAR_9_2_5-15
description: created: n.d., 1957
Croton maranonensis Martín-Muñoz & Silva & Gonzáles & Muñoz-Sánchez & Cumbicus & Goodwin & Meira & Riina 2024
Creators: name: Martín-Muñoz, Juan
name: Silva, Elienai Cândida e
name: Gonzáles, Paúl
name: Muñoz-Sánchez, Álvaro
name: Cumbicus, Nixon
name: Goodwin, Zoë
name: Meira, Renata Maria Strozi Alves
name: Riina, Ricarda
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton maranonensis

description: C. maranonensis sp. nov.
[1]; Ecuador, Loja; Cumbicus & Camacho 1924 (MA); OR622592 *.
description: Published as part of Martín-Muñoz, Juan, Silva, Elienai Cândida e, Gonzáles, Paúl, Muñoz-Sánchez, Álvaro, Cumbicus, Nixon, Goodwin, Zoë, Meira, Renata Maria Strozi Alves & Riina, Ricarda, 2024, Croton maranonensis: a new species of Euphorbiaceae from the tropical inter-Andean dry valleys, pp. 289-308 in European Journal of Taxonomy 947 on page 308, DOI: 10.5852/ejt.2024.947.2639, http://zenodo.org/record/13465689
„Am Tisch des Wortes" — „Kommentar zum Meßbuch"
Creators: name: Jockwig, Klemens
Publisher: name: Ordenskorrespondenz
Year: 1970

description: Ordenskorrespondenz, Bd. 7 (1966): Ordenskorrespondenz: Zeitschrift für Fragen des Ordenslebens, Band 7
title: Activité du port de Saint-Malo – 1767 – Bayonne
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: produits de la mer
subject: poissons
subject: matériaux de construction

description: Cette fiche est issue de l’enquête menée par Jean Delumeau sur l’activité du port de Saint-Malo au 17e et 18e siècle. Cette fiche correspond à l’activité de l’année 1767 avec le port "Bayonne"
description: Marchandises au départ de Saint-Malo : morues sèches
description: Catégories de marchandises au départ de Saint-Malo : produits de la mer ; poissons
description: Marchandises arrivées à Saint-Malo : brai ; goudron ; résine
description: Catégories de marchandises arrivées à Saint-Malo : matériaux de construction
description: Coverage: Grand cabotage
description: Bibliographic citation: BRY, Colette. Le Trafic du port de Saint-Malo (1765-1766-1767). DES : Histoire : Rennes : s.d. (Bibliothèque François-Lebrun, MH 1054)
description: date: Date de numérisation : 2021 à 2023
description: created: Années 1950-1960
Intermediate mass T Tauri disk masses and a comparison to their Herbig disk descendants
Creators: name: Stapper, L. M.
name: Hogerheijde, M. R.
name: van Dishoeck, E. F.
name: Vioque, M.
name: Williams, J. P.
name: Ginski, C.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The precursors of Herbig stars are called Intermediate Mass T Tauri (IMTT) stars, which have spectral types later than F, but stellar masses between 1.5 and 5 M_\odot, and will eventually become Herbig stars with spectral types of A and B. ALMA Band 6 and 7 archival data are obtained for 34 IMTT disks with continuum observations, 32 of which have at least 12CO, 13CO, or C18O observations although most of them at quite shallow integrations. The disk integrated flux together with a stellar luminosity scaled disk temperature are used to obtain a total disk dust mass by assuming optically thin emission. Using thermochemical Dust And LInes (DALI) models from previous work, we additionally obtain gas masses of 10/35 of the IMTT disks based on the CO isotopologues. The IMTT disks in this study have the same dust mass and radius distributions as Herbig disks. The dust mass of the IMTT disks is higher compared to that of the T Tauri disks, as is also found for the Herbig disks. No differences in dust mass are found for group I versus group II disks, in contrast to Herbig disks. The disks for which a gas mass could be determined show similar high mass disks as for the Herbig disks. Comparing the disk dust and gas mass distributions to the mass distribution of exoplanets shows that there also is not enough dust mass in disks around intermediate mass stars to form the massive exoplanets. On the other hand there is more than enough gas to form the atmospheres of exoplanets. We conclude that the sampled IMTT disk population is almost indistinguishable compared to Herbig disks, as their disk masses are the same, even though these are younger objects. Based on this, we conclude that planet formation is already well on its way in these objects, and thus planet formation should start early on in the lifetime of Herbig disks.
description: Accepted for publication in Astronomy and Astrophysics. 16 pages, 12 figures, plus appendices
Oecomys concolor
Creators: name: Don E. Wilson
name: Russell A. Mittermeier
name: Thomas E. Lacher, Jr
Publisher: name: Lynx Edicions
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Cricetidae
Oecomys
Oecomys concolor

description: 391.
Unicolored Arboreal Rice Rat
Oecomys concolor
French: Oecomys de Wagner / German: Einfarb-Baumreisratte / Spanish: Rata arrocera arboricola unicolor
Other common names: Natterer's Oecomys, Unicolored Oecomys
Taxonomy. Hesperomys concolor Wagner, 1845, “Flusse Curicuriari im nordwestlichen Brasilien.” Interpreted by P. Hershkovitz in 1960 as “Rio Curicuriari, an affluent [= tributary] of the upper Rio Negro, entering from the right below Sao Gabriel [da Cachoeira], Amazonas, Brazil.” This species is monotypic.
Distribution. E Colombia, S Venezuela (S Orinoco River), and NW Brazil (N of Amazonas River).
Descriptive notes. Head—body 115-141 mm, tail 137-160 mm, ear 15-20 mm, hindfoot 26-29 mm; weight 41-80 g. The Unicolored Arboreal Rice Rat is medium-to-large, with relatively long tail (c.118% of head-body length) and short pelage (5-7 mm over mid-rump). Dorsum varies from dull fulvous brown to brighter ocherous tawny, especially over shoulders and cheeks. Venter is wholly dull white in most specimens, with strong overwash of buff-tipped to ocherous tipped hairs in other specimens, or with small to broad expanses of gray over mid-abdomen in others; dorsal and ventral pelage contrasts weakly in the last two venter color types. Pinnae are dark brown, usually contrasting with adjacent upperparts. Tail is brown to dark brown all around for most of its length, mottled beneath near base; short caudal hairs expose scale rows for most of tail length, without formation of terminal pencil.
Habitat. Lowland rainforest at elevations above 400 m.
Food and Feeding. No information.
Breeding. No information.
Activity patterns. No information.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Least Concern on The IUCN Red List.
Bibliography. Carleton & Musser (2015), Carleton et al. (2009), Costa et al. (2016), Hershkovitz (1960), Wagner (1845).
description: Published as part of Don E. Wilson, Russell A. Mittermeier & Thomas E. Lacher, Jr, 2017, Cricetidae, pp. 204-535 in Handbook of the Mammals of the World – Volume 7 Rodents II, Barcelona :Lynx Edicions on page 421, DOI: 10.5281/zenodo.6707142
Atherigona laevigata
Creators: name: Magoai, Mokome M. J.
name: Muller, Burgert S.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Atherigona
Atherigona laevigata

description: Atherigona laevigata (Loew, 1852)
Fig. 8
Coenosia laevigata Loew, 1852: 660.
Atherigona laevigata: Van Emden 1940: 113, figs 6, 56; Deeming 1971: 148, figs 13–18; Pont 1991: 341; Muller 2015: 877, fig. 7, Muller and Mostovski 2018: 350, fig. 6, Deeming 2022: 127.
Atherigona scutellaris Stein in Becker 1903: 110.
Atherigona minuta Schnabl & Dziedzicki, 1911: 183.
Material examined.
Lesotho • 1 ♂; Mamathes [Masupha], Basutoland; [29 ° 8.000 ' S, 27 ° 51.000 ' E]; 16 May 1948; C. Jacot Guillarmod leg.
Other material examined.
South Africa • 1 ♂; Free State, Brandfort, Florisbad Research Station; 28 ° 46.039 ' S, 26 ° 04.234 ' E; 4–6 Apr. 2009; A. H. Kirk-Spriggs leg.; Malaise traps, Acacia, Savanna; BMSA (D) 05529 • 1 ♂; KwaZulu-Natal, Ndumo Game Reserve, Shokwe area at: 26 ° 52.125 ' S, 32 ° 13.731 ' E; 30 Nov. – 4 Dec. 2009; A. H. Kirk-Spriggs leg.; Malaise traps, Ficus forest; BMSA (D) 15826.
Diagnosis.
This species can be distinguished from other Afrotropical species by its glossy frontal plate and infuscated frontal vitta with apical third yellow in combination with a knoblike hypopygial prominence (Fig. 8).
Distribution.
AFROTROPICAL – Angola, Comoros, Democratic Republic of Congo, Ethiopia, Kenya, Lesotho (new record), Madagascar, Mali, Mauritius, Mozambique, Namibia, Nigeria, Rwanda, Seychelles, South Africa, Tanzania, Uganda, Zambia, Zimbabwe. PALAEARCTIC – Cyprus, Egypt, Iraq, Israel, Jordan, Saudi Arabia, UAE, Yemen.
description: Published as part of Magoai, Mokome M. J. & Muller, Burgert S., 2024, The first record of Atherigona from Lesotho (Diptera, Muscidae), with description of a new species, pp. 49-60 in African Invertebrates 65 (2) on pages 49-60, DOI: 10.3897/afrinvertebr.65.131744
Croton maranonensis Martín-Muñoz & Silva & Gonzáles & Muñoz-Sánchez & Cumbicus & Goodwin & Meira & Riina 2024
Creators: name: Martín-Muñoz, Juan
name: Silva, Elienai Cândida e
name: Gonzáles, Paúl
name: Muñoz-Sánchez, Álvaro
name: Cumbicus, Nixon
name: Goodwin, Zoë
name: Meira, Renata Maria Strozi Alves
name: Riina, Ricarda
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton maranonensis

description: C. maranonensis sp. nov.
[2]; Peru, Amazonas; Bagua Grande; Vásquez 27094 (MO); OR622593 *.
description: Published as part of Martín-Muñoz, Juan, Silva, Elienai Cândida e, Gonzáles, Paúl, Muñoz-Sánchez, Álvaro, Cumbicus, Nixon, Goodwin, Zoë, Meira, Renata Maria Strozi Alves & Riina, Ricarda, 2024, Croton maranonensis: a new species of Euphorbiaceae from the tropical inter-Andean dry valleys, pp. 289-308 in European Journal of Taxonomy 947 on page 308, DOI: 10.5852/ejt.2024.947.2639, http://zenodo.org/record/13465689
Dicliptera sumichrastii Lindau
Creators: name: Daniel, Thomas F.
name: García-Morales, Leccinum J.
name: Mora-Olivo, Arturo
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Acanthaceae
Dicliptera
Dicliptera sumichrastii

description: Dicliptera sumichrastii Lindau
PHENOLOGY.— Flowering: February–March, August–September, December; fruiting: March, September.
DISTRIBUTION.— Mexico (Oax., Pue., S.L.P., Tamps., Ver.), Central America.
HABITAT.— Oak woodland, grassland.
ELEVATION.— 270–900 meters.
NOTES.— This represents the first report of this species (Fig. 1L) from Tamaulipas, where it attains the northern extent of its distribution. Plants occurring in the state are part of a species complex consisting of D. brachiata (Pursh) Spreng. from the southern U.S.A. and Nuevo León (Daniel, in press), plants occurring in eastern and southern Mexico and treated as either D. acuminata (Ruiz & Pav.) Juss. var. spicata Nees or D. sumichrastii (the types of both are from Veracruz), plants treated in Central America as D. antidysenterica A. Molina R. (Daniel 2005, 2010), D. acuminata from western South America, and probably other New World taxa as well. Specimens cited below show characteristics somewhat intermediate between extremes of D. brachiata and D. sumichrastii, but conform more closely to the latter species. The taxonomy of these entities remains to be satisfactorily resolved.
REPRESENTATIVE SPECIMENS.— Vic. of El Milagro, Cerro Zamora, H. Bartlett 11152 (DS, US); Mpio. Victoria, Cañón de La Peregrina, ca. 13 km W de Ejido La Libertad, L. García-Morales 4180 (ITCV); Mpio. Villa de Casas, Sierra de Tamaulipas, from Rancho “Las Yucas ” to Santa María de los Nogales and Hac. Acuna, from Cerro de San Juan to Santa María de los Nogales, F. Martinez M. & G. Borja L. F-1982 (TEX); Mpio. Soto la Marina, Cañón del Diablo, H. Puig 4150 (P).
description: Published as part of Daniel, Thomas F., García-Morales, Leccinum J. & Mora-Olivo, Arturo, 2021, Taxonomic and Photographic Guide to the Acanthaceae of Tamaulipas, Mexico, pp. 185-228 in Proceedings of the California Academy of Sciences 67 (6) on page 199, DOI: 10.5281/zenodo.11513051
Latin phonetics
Creators: name: André, Jacques
name: Marichal, Robert
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015

description: vue 28
description: Bibliographical references and list of papyrological and epigraphic sources on various Latin phonetic phenomena.
description: Source: 4MAR_22_4_5
description: Relation: Jacques André, Dag Norberg
description: created: n.d., 1959, 1974
Radon emanation rate measurements using liquid scintillation counting
Creators: name: Sazzad, A. B. M. R.
name: Acharya, P.
name: Back, P.
name: Busenitz, J.
name: Chernyak, D.
name: Meng, Y.
name: Piepke, A.
name: Rhyne, C. A.
name: Tsang, R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: This article describes a radon emanation measurement technique using liquid scintillator counting. A model for radon loading and transport is described, along with its calibration. Detector background and blank have been studied and quantified. The Minimal detectable activity has been determined for the counting setup using a toy Monte Carlo simulation. The measurement technique is validated using a butyl rubber sample previously used for cross-calibration between different radon counting facilities.
description: Typos and articles fixed
Oecomys awyantepui Tate 1939
Creators: name: Don E. Wilson
name: Russell A. Mittermeier
name: Thomas E. Lacher, Jr
Publisher: name: Lynx Edicions
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Cricetidae
Oecomys
Oecomys awyantepui

description: 392.
Guianan Arboreal Rice Rat
Oecomys awyantepui
French: Oecomys de I'Auyantepui / German: Guyana-Baumreisratte / Spanish: Rata arrocera arboricola de Guayana
Other common names: Guianan Oecomys
Taxonomy. Oecomys auyantepui Tate, 1939, “south slopes of Mt. Auyan-tepui, Caroni River [Bolivar], Venezuela, 3500 feet [= 1069 m].”
Taxonomy of O. awyantepui is poorly explored. Monotypic.
Distribution. E Venezuela, The Guianas, and NC Brazil.
Descriptive notes. Head-body 101-121 mm, tail 108-128 mm, ear 14-18 mm, hindfoot 23-25 mm; weight 30-48 g. The Guianan Arboreal Rice Rat is small, with luxuriant, soft, dense, and long (10-12 mm over mid-rump) pelage and sharp demarcation between dorsal and ventral pelage. Dorsum is rich ocherous tawny (nearly orange brown) in most specimens but darker— brownish tawny—in others; tops of hindfeet are dark brown to tip of digits. Venter is typically grayish white (hairs with gray bases and white tips) or uncommonly with rich ocherous overwash of gray bases; in some specimens, chin and throat are pure white, in others white strip extends along midline from throat to groin. Tail ¢.106% of head-body length and dark brown on all surfaces; caudal hairs are long, typically obscuring distal scale rows and forming conspicuous tuft at tip (c¢.6-10 mm long). Recent cytogenetic studies revealed sympatric occurrence of two different chromosomal complements: 2n = 64, FNa = 110 and 2n = 66, FNa = 114.
Habitat. Humid forest (Venezuela) and primary lowland forest on well-drained sites and in creekside or swampy settings (Guianan subregion of Amazonia), from sea level up to elevations of ¢.1100 m.
Food and Feeding. No information.
Breeding. No information.
Activity patterns. Guianan Arboreal Rice Rats are arboreal, with most specimens trapped in canopies.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Least Concern on The [UCN Red List.
Bibliography. Carleton & Musser (2015), Gomes et al. (2016), Rosa (2015), Tate (1939), Voss et al. (2001), Weksler & Bonvicino (2016b).
description: Published as part of Don E. Wilson, Russell A. Mittermeier & Thomas E. Lacher, Jr, 2017, Cricetidae, pp. 204-535 in Handbook of the Mammals of the World – Volume 7 Rodents II, Barcelona :Lynx Edicions on page 421, DOI: 10.5281/zenodo.6707142
Tylospira clathrata
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Struthiolariidae
Tylospira
Tylospira clathrata

description: Tylospira clathrata (Tate, 1885)
Pelicaria clathrata Tate, 1885a: 2; Tate, 1889: 170, pl. 10, fig. 9.
Tylospira clathrata (Tate, 1885).—Darragh, 1991: 155, Figs 1A, D, E–G, K.
Distribution. Gippsland Basin: Rose Hill Marl (type). Age: late Miocene.
description: Published as part of Darragh, Thomas A., 2024, A checklist of Australian marine Cenozoic Mollusca, pp. 37-206 in Memoirs of Museum Victoria 83 on page 70, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
Überlegungen zur Erziehung und Persönlichkeitsbildung der Ordenskleriker nach dem II. Vatikanischen Konzil
Creators: name: Stenger, Hermann
Publisher: name: Ordenskorrespondenz
Year: 1970

description: Ordenskorrespondenz, Bd. 7 (1966): Ordenskorrespondenz: Zeitschrift für Fragen des Ordenslebens, Band 7
Atherigona londti Muller 2015
Creators: name: Magoai, Mokome M. J.
name: Muller, Burgert S.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Atherigona
Atherigona londti

description: Atherigona londti Muller, 2015
Fig. 10 a – e
Atherigona londti Muller, 2015: 882, fig. 48.
Material examined.
Lesotho • 2 ♂; Leribe, Motebong Lodge, Katse Dam area; 29 ° 6.060 ' S, 28 ° 30.084 ' E; 2063 m; 10–13 Dec. 2021; J. M. Midgley and B. Muller leg.; Malaise trap, Garden entertainment area; (BMSA (D) 130774, NMSA - DIP 213800). 3 ♂; Maseru, Roma Trading Post Lodge; 29 ° 26.592 ' S, 27 ° 42.224 ' E; 1640 m; 24–27 Nov. 2022; K. Jordaens, J. Midgley, B. Muller and G. Theron leg.; Malaise trap, Basotho Montane Shrubland, Garden; (BMSA (D) 134689, 134691, 134690).
Diagnosis.
This species’ scutellum is similar to Atherigona flavifinis Muller, 2015 (fig. 16 in Muller 2015) and Atherigona latibasilaris Muller, 2015 (fig. 40 in Muller 2015) in having the apex of the scutellum yellow. However, the trifoliate process and hypopygial prominence differ greatly. It keys close to Atherigona hyalinipennis van Emden, 1959 and Atherigona s ecrecauda Séguy, 1938 using the keys provided by Deeming (1971) and Dike (1989) but the trifoliate process (Fig. 10) of A. londti does not have the wing-like projections of the hood present as in A. secrecauda, nor does it have the cordiform median piece of A. hyalinipennis.
Distribution.
Lesotho (new record), South Africa.
description: Published as part of Magoai, Mokome M. J. & Muller, Burgert S., 2024, The first record of Atherigona from Lesotho (Diptera, Muscidae), with description of a new species, pp. 49-60 in African Invertebrates 65 (2) on pages 49-60, DOI: 10.3897/afrinvertebr.65.131744
Misbinding Raw Public Keys to Identities in TLS
Creators: name: Moustafa, Mariam
name: Sethi, Mohit
name: Aura, Tuomas
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: The adoption of security protocols such as Transport Layer Security (TLS) has significantly improved the state of traffic encryption and integrity protection on the Internet. Despite rigorous analysis, vulnerabilities continue to emerge, sometimes due to fundamental flaws in the protocol specification. This paper examines the security of TLS when using Raw Public Key (RPK) authentication. This mode has not been as extensively studied as X.509 certificates and Pre-Shared Keys (PSK). We develop a formal model of TLS RPK using applied pi calculus and the ProVerif verification tool, revealing that the RPK mode is susceptible to identity misbinding attacks. Our contributions include formal models of TLS RPK with several mechanisms for binding the endpoint identity to its public key, verification results, practical scenarios demonstrating the misbinding attack, and recommendations for mitigating such vulnerabilities. These findings highlight the need for improved security measures in TLS RPK.
Oecomys rex Thomas 1910
Creators: name: Don E. Wilson
name: Russell A. Mittermeier
name: Thomas E. Lacher, Jr
Publisher: name: Lynx Edicions
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Cricetidae
Oecomys
Oecomys rex

description: 393.
King Arboreal Rice Rat
Oecomys rex
French: Oecomys roi / German: Konigsbaumreisratte / Spanish: Rata arrocera arboricola real
Other common names: Regal Oecomys
Taxonomy. Oecomys rex Thomas, 1910, “R. Supinaam [= Supenaam], Lower Essequibo, Demerara [= Georgetown],” Demerara-Mahaica, Guyana.
This species is monotypic.
Distribution. E Venezuela (Bolivar State), the Guianas, and NC Brazil (Amapa, Roraima, and Amazonas states).
Descriptive notes. Head-body 121-135 mm, tail 142-168 mm, ear 17-18 mm, hindfoot 27-29 mm; weight 47-71 g. The King Arboreal Rice Rat is large and easily identified. Dorsal pelage is thick and long (10-12 mm), with very fine and luxurious texture. Upperparts are generally dark in tone, ranging from dull ocherous brown to deep chestnut, finely intermixed with black-tipped hairs over mid-dorsum and grading to brighter on flanks. Venter is uniformly dark grayish white (hairs with gray bases and white tips) in most specimens, although some have overwash of buff to ocherous on belly and dingy white on gular and inguinal regions. Tail is brown all around, and caudal hairs are short and inconspicuous without terminal pencil or tuft. Tops of forefeet and hindfeet are fuscous brown, becoming dingy white over digits.
Habitat. Humid evergreen forests in Guiana subregion of Amazonia.
Food and Feeding. No information.
Breeding. No information.
Activity patterns. King Arboreal Rice Rats are terrestrial.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Least Concern on The IUCN Red List.
Bibliography. Carleton & Musser (2015), Catzeflis & Percequillo (2016), Ochoa et al. (1993).
description: Published as part of Don E. Wilson, Russell A. Mittermeier & Thomas E. Lacher, Jr, 2017, Cricetidae, pp. 204-535 in Handbook of the Mammals of the World – Volume 7 Rodents II, Barcelona :Lynx Edicions on page 422, DOI: 10.5281/zenodo.6707142
Constraint on the equation of state of strange quark star: Perturbative QCD along with a density-dependent bag constant
Creators: name: Sedaghat, J.
name: Bordbar, G. H.
name: Zebarjad, S. M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This study investigates the structural properties of strange quark stars (SQS) using a Quantum Chromodynamics (QCD) perturbative model combined with the latest Particle Data Group dataset. Given the energy scale present in compact stars, QCD perturbation theory alone may not fully explain their structure. To account for non-perturbative contributions, we incorporate a density-dependent effective bag parameter, $B$, and derive the equation of state (EOS) for strange quark matter (SQM). We start by demonstrating the limitations of EOSs with a constant $B$ in describing massive objects with $ M_{TOV}> 2M_{\odot} $. Subsequently, we show that considering $B$ as a density-dependent function significantly changes the results. Our definition of $B$ includes two parameters determined by both theoretical and observational constraints. We demonstrate that incorporating a density-dependent $B$ into the perturbative EOS can yield SQSs with masses exceeding $2M_{\odot}$, while complying with gravitational wave constraints such as tidal deformability, and thermodynamic considerations, including stability conditions and speed of sound behavior. Specifically, we show that massive compact objects like PSR J0952-0607, PSR J2215+5135, PSR J0740+6620, and the secondary mass of GW190814 can be SQSs. Additionally, we compare our EOS with the EOS of the authors who use a generalized polytropic form with adjustable parameters and obtain an interesting result.
description: 15 pages, 18 figures, 3 tables, Annals of Physics (2024) accepted for publication
Sycophancy in Large Language Models: Causes and Mitigations
Creators: name: Malmqvist, Lars
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Large language models (LLMs) have demonstrated remarkable capabilities across a wide range of natural language processing tasks. However, their tendency to exhibit sycophantic behavior - excessively agreeing with or flattering users - poses significant risks to their reliability and ethical deployment. This paper provides a technical survey of sycophancy in LLMs, analyzing its causes, impacts, and potential mitigation strategies. We review recent work on measuring and quantifying sycophantic tendencies, examine the relationship between sycophancy and other challenges like hallucination and bias, and evaluate promising techniques for reducing sycophancy while maintaining model performance. Key approaches explored include improved training data, novel fine-tuning methods, post-deployment control mechanisms, and decoding strategies. We also discuss the broader implications of sycophancy for AI alignment and propose directions for future research. Our analysis suggests that mitigating sycophancy is crucial for developing more robust, reliable, and ethically-aligned language models.
Croton maranonensis Martín-Muñoz & Silva & Gonzáles & Muñoz-Sánchez & Cumbicus & Goodwin & Meira & Riina 2024
Creators: name: Martín-Muñoz, Juan
name: Silva, Elienai Cândida e
name: Gonzáles, Paúl
name: Muñoz-Sánchez, Álvaro
name: Cumbicus, Nixon
name: Goodwin, Zoë
name: Meira, Renata Maria Strozi Alves
name: Riina, Ricarda
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton maranonensis

description: C. maranonensis sp. nov.
[3]; Peru, Amazonas; Dexter 5935 (E); OR622594 *.
description: Published as part of Martín-Muñoz, Juan, Silva, Elienai Cândida e, Gonzáles, Paúl, Muñoz-Sánchez, Álvaro, Cumbicus, Nixon, Goodwin, Zoë, Meira, Renata Maria Strozi Alves & Riina, Ricarda, 2024, Croton maranonensis: a new species of Euphorbiaceae from the tropical inter-Andean dry valleys, pp. 289-308 in European Journal of Taxonomy 947 on page 308, DOI: 10.5852/ejt.2024.947.2639, http://zenodo.org/record/13465689
Chemical enrichment in LINERs from MaNGA. I. Tracing Oxygen and Nitrogen Nuclear Abundances in LINERs with Varied Ionizing Sources
Creators: name: Pérez-Díaz, Borja
name: Pérez-Montero, Enrique
name: Zinchenko, Igor A.
name: Vílchez, José M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The chemical enrichment in low-ionization nuclear emission-line regions (LINERs) is still an issue with spatial resolution spectroscopic data due to the lack of studies and the uncertainties in the nature of their ionizing source, despite being the most abundant type of active galaxies in the nearby Universe. Considering different scenarios for the ionizing source (hot old stellar populations, active galactic nuclei (AGN) or inefficient accretion disks), we analyze the implications of these assumptions to constrain the chemical content of the gas-phase interstellar medium (ISM). We used a sample of 105 galaxies from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, whose nuclear central spaxels show LINER-like emission. For each scenario considered, we built a grid of photoionization models (4928 models for each considered ionizing source) which are later used in the open-source code HII-CHI-Mistry, allowing us to estimate chemical abundance ratios such as 12+log(O/H) or log(N/O) and constrain the ionization parameter that characterize the ionized ISM in those galaxies. We obtain that oxygen abundances in the nuclear region of LINER-like galaxies spread over a wide range 8.08 < 12+log(O/H) < 8.89, with a median solar value (in agreement with previous studies) if AGN models are considered. Nevertheless, the derived nitrogen-to-oxygen ratio is much less affected by the assumptions on the ionizing source, and point towards suprasolar values (log(N/O) = -0.69). By comparing the different analyzed scenarios, we show that if hot old stellar populations were responsible of the ionization of the ISM a complex picture (such as outflows and/or inflows scaling with galaxy chemical abundance) would be needed to explain the chemical enrichment history, whereas the assumption of AGN activity is compatible with the standard scenario found in most galaxies.
description: Revised version after language edition. 24 pages, 13 figures, 9 tables (5 as supplemented material). Accepted for publication in A&A
Croton michauxii var. elliptica B. W. van Ee & P. E. Berry
Creators: name: Martín-Muñoz, Juan
name: Silva, Elienai Cândida e
name: Gonzáles, Paúl
name: Muñoz-Sánchez, Álvaro
name: Cumbicus, Nixon
name: Goodwin, Zoë
name: Meira, Renata Maria Strozi Alves
name: Riina, Ricarda
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton michauxii
C. michauxii g.l.webster var. elliptica (willd.) b.w.van ee & p.e.berry

description: C. michauxii G.L.Webster var. elliptica (Willd.) B.W.van Ee & P.E.Berry;
U.S.A., Missouri; Archer 40 (MO); EU478004.
description: Published as part of Martín-Muñoz, Juan, Silva, Elienai Cândida e, Gonzáles, Paúl, Muñoz-Sánchez, Álvaro, Cumbicus, Nixon, Goodwin, Zoë, Meira, Renata Maria Strozi Alves & Riina, Ricarda, 2024, Croton maranonensis: a new species of Euphorbiaceae from the tropical inter-Andean dry valleys, pp. 289-308 in European Journal of Taxonomy 947 on page 308, DOI: 10.5852/ejt.2024.947.2639, http://zenodo.org/record/13465689
legal research- Asylum in the United States of America.pdf
Creators: name: wadid, Bassem
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 489999
subject: Other law and legal studies not elsewhere classified

description: This research provides an in-depth analysis of the U.S. asylum system, focusing on its legal foundations, processes, and challenges. It explores the five primary grounds for asylum claims—race, religion, nationality, political opinion, and membership in a particular social group—as defined under the Immigration and Nationality Act (INA) and influenced by landmark judicial decisions. By examining legal precedents such as INS v. Cardoza-Fonseca and Matter of Acosta, the study highlights the evolving interpretation of asylum eligibility and procedural requirements. The research also identifies systemic challenges, including procedural delays and inconsistencies, and proposes reforms to enhance efficiency and fairness in asylum adjudication. Key recommendations include the introduction of centralized case management systems, improved access to legal representation, and the application of trauma-informed practices during asylum interviews. This study underscores the critical role of the U.S. asylum system in safeguarding human rights and offers practical solutions to address the complexities faced by applicants and adjudicators.
Non-linear saturation and energy transport in global simulations of magneto-thermal turbulence in the stratified intracluster medium
Creators: name: Kempf, Jean M.
name: Rincon, François
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. The magneto-thermal instability (MTI) is one of many possible drivers of stratified turbulence in the intracluster medium (ICM) outskirts of galaxy clusters, where the background temperature gradient is aligned with the gravity. This instability occurs because of the fast anisotropic conduction of heat along magnetic field lines; but to what extent it impacts the ICM dynamics, energetics and overall equilibrium is still a matter of debate. Aims. This work aims at understanding MTI turbulence in an astrophysically stratified ICM atmosphere, its saturation mechanism, and its ability to carry energy and to provide non-thermal pressure support. Methods. We perform a series of 2D and 3D numerical simulations of the MTI in global spherical models of stratified ICM, thanks to the finite-volume code IDEFIX, using Braginskii-magnetohydrodynamics. We use volume-, shell-averaged and spectral diagnostics to study the saturation mechanism of the MTI, and its radial transport energy budget. Results. The MTI is found to saturate through a dominant balance between injection and dissipation of available potential energy, which amounts to marginalising the Braginskii heat flux but not the background temperature gradient itself. Accordingly, the strength and injection length of MTI-driven turbulence exhibit clear dependencies on the thermal diffusivity. The MTI drives cluster-size motions with Mach numbers up to $\mathcal{M} \sim 0.3$, even in presence of strong stable entropy stratification. We show that such mildly compressible flows can provide about $\sim 15\%$ of non-thermal pressure support in the outermost ICM regions, and that the convective transport itself is much less efficient than conduction at radially transporting energy. Finally, we show that the MTI saturation can be described by a diffusive mixing-length theory, shedding light on the diffusive buoyant nature of the instability.
description: 20 pages, 8 figures, accepted for publication in A&A, arXiv abstract slightly shortened
Dyschoriste crenulata Kobuski
Creators: name: Daniel, Thomas F.
name: García-Morales, Leccinum J.
name: Mora-Olivo, Arturo
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Acanthaceae
Dyschoriste
Dyschoriste crenulata

description: Dyschoriste crenulata Kobuski
PHENOLOGY.— Flowering: February–July, October; fruiting: July, October.
DISTRIBUTION.— U.S.A. (Tex.), Mexico (Coah., Tamps.).
HABITAT.— Thornscrub, disturbed sites, sometimes on limestone.
ELEVATION.— 120–350 meters.
NOTES.— Henrickson (1999) provided a description, discussed the taxonomy, and mapped the distribution of this species (Fig. 2A). The type of D. crenulata (Nelson 6604) is from Tamaulipas.
REPRESENTATIVE SPECIMENS.— Sierra de San Carlos, La Tamaulipeca, vic. of San Miguel, H. Bartlett 10646 (F); along Hwy. 81 between González and Hwy. 85, 38.1 mi SE of jct. Hwy. 85, T. Daniel & B. Bartholomew 5084 (CAS); between Victoria and Antiguo, G. Happ 37 (MO); Mpio. Abasolo, Carr. 80, KM 232 Tampico–Matamoros, tramo Soto la Marina a La Coma, Ejido Los Morales, “La Labor,” 7 km NE de Los Morales, 24°23ʹ08ʺN, 098°21ʹ02ʺW, M. González G. 213 (MEXU); 48 mi from Reynosa on San Fernando rd., 27 mi from Matamoros–San Fernando hwy. turnoff, M. Johnston & J. Graham 4382 (TEX, US); San Fernando to Jiménez [Santander Jiménez], E. Nelson 6604 (holotype: GH-image!; isotype: US-image!); 20 mi W of Reynosa, J. Painter & F. Barkley 14393 (MO, TEX); 3 mi N of Santander Jiménez on Rte. 101, R. Wilbur 35266 (MEXU-image).
description: Published as part of Daniel, Thomas F., García-Morales, Leccinum J. & Mora-Olivo, Arturo, 2021, Taxonomic and Photographic Guide to the Acanthaceae of Tamaulipas, Mexico, pp. 185-228 in Proceedings of the California Academy of Sciences 67 (6) on page 200, DOI: 10.5281/zenodo.11513051
Manifold nº 17 (Chine nº 3) (p. 12)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: Mausolées de l’Empereur Min
Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops
Creators: name: Ram, B.
name: Chitta, L. P.
name: Mandal, S.
name: Peter, H.
name: Plaschke, F.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Coronal loops generally trace magnetic lines of force in the upper solar atmosphere. Understanding the loop morphology and its temporal evolution has implications for coronal heating models that rely on plasma heating due to reconnection at current sheets. Simultaneous observations of coronal loops from multiple vantage points are best suited for this purpose. Here, we report a stereoscopic analysis of coronal loops in an active region based on observations from the Extreme Ultraviolet Imager on board the Solar Orbiter Spacecraft and the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. Our stereoscopic analysis reveals that coronal loops have nearly circular cross-sectional widths and that they exhibit temporally coherent intensity variations along their lengths on timescales of around 30\,minutes. Results suggest that coronal loops can be best represented as three-dimensional monolithic or coherent plasma bundles that outline magnetic field lines. Therefore, at least on the scales resolved by Solar Orbiter, it is unlikely that coronal loops are manifestations of emission from the randomly aligned wrinkles in two-dimensional plasma sheets along the line-of-sight as proposed in the `coronal veil' hypothesis.
Tylospira coronata
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Struthiolariidae
Tylospira
Tylospira coronata

description: Tylospira coronata (Tate, 1885)
Pelicaria coronata Tate, 1885a: 2.— Tate, 1889: 171, pl. 10, figs 6, 13.
Struthiolaria (Pelicaria) coronata (Tate, 1885).— Cossmann, 1904: 106, pl. 8, figs 5, 6.
Tylospira coronata (Tate, 1885).— Harris, 1897: 222, pl. 6, figs 9a, b; Marwick, 1924b, 166, fig. 8a; Marwick, 1960: 43; Ludbrook, 1969b: fig. 96. 11; Ludbrook, 1973: pl. 27, fig. 85; Darragh, 1991: 156, Figs 2A–K.
Distribution. Murray Basin: Bookpurnong Formation. Otway Basin: Grange Burn Formation (type). Port Phillip Basin: Sandringham Sandstone. Gippsland Basin: Jemmys Point Formation. Bass Basin: Cameron Inlet Formation. Age: middle Miocene–late Pliocene.
description: Published as part of Darragh, Thomas A., 2024, A checklist of Australian marine Cenozoic Mollusca, pp. 37-206 in Memoirs of Museum Victoria 83 on page 70, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472