cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Psammodes ventricosus Fahraeus 1870
Creators: name: Schoeman, Colin S.
name: Toussaint, Dawn Cory
name: Tshililo, Precious
name: Foord, Stefan H.
name: Hamer, Michelle
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Psammodes
Psammodes ventricosus

description: Psammodes cf. ventricosus Fåhraeus, 1870
Fig. 3T,
MAS
description: Published as part of Schoeman, Colin S., Toussaint, Dawn Cory, Tshililo, Precious, Foord, Stefan H. & Hamer, Michelle, 2020, Checklist of the pimeliine darkling beetles of the Vhembe Biosphere Reserve, South Africa (Coleoptera: Tenebrionidae: Pimeliinae), pp. 1-9 in Bothalia (a 8) (a 8) 50 (1) on page 7, DOI: 10.38201/btha.abc.v50.i1.8, http://zenodo.org/record/10515087
Podalonia atrocyanea
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Podalonia
Podalonia atrocyanea

description: Podalonia atrocyanea (Eversmann, 1849)
(Map 25)
Psammophila atrocyanea Eversmann, 1849. Bulletin de la Société Impériale des Naturalistes de Moscou, 22: 365.
Ammophila (Psammophila) atrocyanea: Kohl, 1906: 270 (Medenine).
Psammophila atrocyanea: Roth, 1928: 171 (Sfax).
Podalonia atrocyanea masinissa: Roth, 1928: 171 (Tunis).
Podalonia atrocyanea: Dollfuss, 2010a: 542 (Gabes).
General distribution. Algeria, China, Central Asia, Egypt, Mongolia, Russia, Tunisia (Dollfuss 2010b).
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 309, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
Crosseola princeps
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Conradiidae
Crosseola
Crosseola princeps

description: Crosseola princeps (Tate, 1890)
Crossea princeps Tate, 1890: 220; Tate, 1892, pl. 8, figs 6a, b. Crosseola princeps (Tate, 1890).— Darragh, 2017: 40, Fig. 1.36.
Distribution. Eucla Basin: Pallinup Formation. St Vincent Basin: Blanche Point Formation (type). Murray Basin: Cadell Marl. Otway Basin: Muddy Creek Formation. Age: late Eocene–middle 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 48, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
How "mixing" affects propagation and structure of intensely turbulent, lean, hydrogen-air premixed flames
Creators: name: Yuvraj
name: Im, Hong G.
name: Chaudhuri, Swetaprovo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Understanding how intrinsically fast hydrogen-air premixed flames can be rendered much faster in turbulence is crucial for systematically developing hydrogen-based gas turbines and spark ignition engines. Here, we present fundamental insights into the variation of flame displacement speeds by investigating how the disrupted flame structure affects speed and vice-versa. Three DNS cases of lean hydrogen-air mixtures with $Le$ from 0.5 to 1 and $Ka$ from 100 to 1000 are analyzed. Suitable comparisons are made with the closest canonical laminar flame configurations at same mixture conditions and their suitability and limitations in expounding turbulent flame properties are elucidated. Since near zero-curvature surface locations are most probable and representative of the average flame geometry in such large $Ka$ flames, this study focuses on the statistical variation of flame displacement speed and the concomitant change in flame structure at those locations. Relevant flame properties are averaged normal to the zero-curvature isotherm regions to obtain the conditional mean flame structures. In the smallest $Le$ case, downstream of the most probable zero-curvature regions, the temperature exceeds that of the standard laminar flame, leading to enhanced local thermal gradient and flame speed. This is due to increased heat-release rate contribution by differential diffusion in positive curvatures downstream of the zero-curvature locations. Furthermore, locally, the flame structure is broadened for all cases due to a reversal in the direction of the flame speed gradient. This reversal is caused by cylindrical flame-flame interactions upstream of the zero-curvature regions, resulting in localized scalar mixing within the flame structure. These non-local effects, in combination, define the mean flame structure and the associated variation in local flame speed in turbulent premixed flames.
Foliaro nº 9 (Sovetio nº5) (p. 27)
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: P.N. 1974. Kial mi obstiniĝis en Kazan ?
Complexity is not Enough for Randomness
Creators: name: Guo, Shiyong
name: Sasieta, Martin
name: Swingle, Brian
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the dynamical generation of randomness in Brownian systems as a function of the degree of locality of the Hamiltonian. We first express the trace distance to a unitary design for these systems in terms of an effective equilibrium thermal partition function, and provide a set of conditions that guarantee a linear time to design. We relate the trace distance to design to spectral properties of the time-evolution operator. We apply these considerations to the Brownian $p$-SYK model as a function of the degree of locality $p$. We show that the time to design is linear, with a slope proportional to $1/p$. We corroborate that when $p$ is of order the system size this reproduces the behavior of a completely non-local Brownian model of random matrices. For the random matrix model, we reinterpret these results from the point of view of classical Brownian motion in the unitary manifold. Therefore, we find that the generation of randomness typically persists for exponentially long times in the system size, even for systems governed by highly non-local time-dependent Hamiltonians. We conjecture this to be a general property: there is no efficient way to generate approximate Haar random unitaries dynamically, unless a large degree of fine-tuning is present in the ensemble of time-dependent Hamiltonians. We contrast the slow generation of randomness to the growth of quantum complexity of the time-evolution operator. Using known bounds on circuit complexity for unitary designs, we obtain a lower bound determining that complexity grows at least linearly in time for Brownian systems. We argue that these bounds on circuit complexity are far from tight and that complexity grows at a much faster rate, at least for non-local systems.
description: 40 pages + appendices. v3: added references
Towards Integrating Emerging AI Applications in SE Education
Creators: name: Vierhauser, Michael
name: Groher, Iris
name: Antensteiner, Tobias
name: Sauerwein, Clemens
Publisher: name: arXiv
Year: 2024
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Artificial Intelligence (AI) approaches have been incorporated into modern learning environments and software engineering (SE) courses and curricula for several years. However, with the significant rise in popularity of large language models (LLMs) in general, and OpenAI's LLM-powered chatbot ChatGPT in particular in the last year, educators are faced with rapidly changing classroom environments and disrupted teaching principles. Examples range from programming assignment solutions that are fully generated via ChatGPT, to various forms of cheating during exams. However, despite these negative aspects and emerging challenges, AI tools in general, and LLM applications in particular, can also provide significant opportunities in a wide variety of SE courses, supporting both students and educators in meaningful ways. In this early research paper, we present preliminary results of a systematic analysis of current trends in the area of AI, and how they can be integrated into university-level SE curricula, guidelines, and approaches to support both instructors and learners. We collected both teaching and research papers and analyzed their potential usage in SE education, using the ACM Computer Science Curriculum Guidelines CS2023. As an initial outcome, we discuss a series of opportunities for AI applications and further research areas.
description: Accepted for publication at the 36th Conference on Software Engineering Education and Training (CSEE&T)
Neusticomys ferreirai Percequillo, Carmignotto & M. J. J. Silva 2005
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
Neusticomys
Neusticomys ferreirai

description: 340.
Ferreira’s Fish-eating Rat
Neusticomys ferreirai
French: Ichthyomys de Ferreira / German: Ferreira-Fischratte / Spanish: Rata pescadora de Ferreira
Other common names: Ferreira’s Ichthyomyine
Taxonomy. Neusticomys ferreirai Percequillo, Carmignotto & M. J. J. Silva, 2005, 20 km W of the left bank of the Rio Juruena, in the municipality ofJuruena, Mato Grosso, Brazil.
This species is monotypic.
Distribution. Scattered Amazonian lowland localities in NC Brazil S of Amazon River.
Descriptive notes. Head-body 106-114 mm, tail 75-95 mm, ear 8:5-12 mm, hindfoot 21-23 mm; weight 31-36 g. Ferreira’s Fish-eating Rat is a small species of Neuticomys. Dorsum is glossy brown, grizzled with orange; dorsal part of head is colored like body; cheeks predominantly orange; and venter is grayish orange buffy, indistinctly paler than dorsal pelage, harsher, and shorter. Eyes are small. Ears are small, rounded, conspicuous above fur of head and well-covered with short,stiff, dark brown hairs. Mystacial vibrissae are sparse and short, not surpassing ears when laid back alongside head. Dorsal surface of manus and pes are covered with short dark brown hairs; hindfeet have natatory fringe weakly developed on lateral metatarsal and tarsal margins; and short webbing occurs between pedal second, third, and fourth digits. Tail is short and unicolored, densely covered with long dark brown hairs. The few known specimens consistently have very small M?; M, are sometimes absent.
Habitat. Terra firma forests near small, slow-moving, clear-water, sandy-bottomed streams surrounded by primary forest with 25-30m high canopy bearing various epiphytes; subcanopy open with regularly spaced dicotyledonous trees and palms and abundant lianas (woody vines).
Food and Feeding. Arthropod remains (Crustacea) were found in a stomach of one Ferreira’s Fish-eating Rat.
Breeding. A pregnant Ferreira’s Fish-eating Rat with five large embryos was recorded in middle of dry season (June).
Activity patterns. Ferreira’s Fish-eating Rat is semi-aquatic.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Data Deficient on The IUCN Red List. Ferreira’s Fish-eating Rat was only recently discovered, and there is very little information on its extent of occurrence, status, and ecological requirements.
Bibliography. Braga & Duda (2017), Miranda et al. (2012), Percequillo & Weksler (2008a), Percequillo et al. (2005), Voss (2015b).
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 pages 405-406, DOI: 10.5281/zenodo.6707142
Podalonia ebenina
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Podalonia
Podalonia ebenina

description: Podalonia ebenina (Spinola, 1839)
Ammophila ebenina Spinola, 1839: Annales de la Société Entomologique de France, 7: 464.
Ammophila (Psammophila) ebenina: Roth, 1928: 175 (Tunisia: no specific locality).
General distribution. Arabia Saudi, Central Asia, Mediterranean Region (Dollfuss 2010b).
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 309, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
КОММУНИКАТИВНАЯ КОМПЕТЕНТНОСТЬ В ОБУЧЕНИИ ИНОСТРАННОМУ ЯЗЫКУ
Creators: name: Тлеумуратова, А.Б.
Publisher: name: Zenodo
Year: 2024

description: Статья посвящена исследованию роли коммуникативной компетентности в обучении иностранным языкам. В ней рассматривается понятие коммуникативной компетентности как совокупности знаний, навыков и умений, необходимых для успешного общения на иностранном языке в различных социальных и культурных контекстах. Особое внимание уделяется четырем основным компонентам коммуникативной компетентности: грамматической, социолингвистической, дискурсивной и стратегической компетенции. В статье подчеркивается важность интеграции этих аспектов в процесс обучения, а также роль преподавателя в создании эффективных коммуникативных ситуаций, способствующих развитию у студентов навыков аудирования, говорения, чтения и письма. Ожидается, что развитие коммуникативной компетентности у учащихся повысит их способность к межкультурному взаимодействию и обеспечит успешную адаптацию в разных языковых и культурных средах.
Psammodes vialis
Creators: name: Schoeman, Colin S.
name: Toussaint, Dawn Cory
name: Tshililo, Precious
name: Foord, Stefan H.
name: Hamer, Michelle
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Psammodes
Psammodes vialis

description: Psammodes vialis (Burcell, 1822)
BLN, GON, GOR
description: Published as part of Schoeman, Colin S., Toussaint, Dawn Cory, Tshililo, Precious, Foord, Stefan H. & Hamer, Michelle, 2020, Checklist of the pimeliine darkling beetles of the Vhembe Biosphere Reserve, South Africa (Coleoptera: Tenebrionidae: Pimeliinae), pp. 1-9 in Bothalia (a 8) (a 8) 50 (1) on page 7, DOI: 10.38201/btha.abc.v50.i1.8, http://zenodo.org/record/10515087
Signatures of gravitational wave memory in the radiative process of entangled quantum probes
Creators: name: Barman, Subhajit
name: Chakraborty, Indranil
name: Mukherjee, Sajal
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this article, we examine entangled quantum probes in geodesic trajectories in a flat background with a gravitational wave (GW) burst. In particular, these quantum probes are prepared initially either in the symmetric or anti-symmetric Bell's states, and we study the radiative process as the GW burst passes. We split a generic GW burst into two profiles with and without memory. GW burst with (without) memory profiles have different (similar) asymptotic strains between early and late times. We observe that for eternal switching, there is a finite change in the collective atomic transition rate due to the memory part of the GW burst, while the contribution from the without memory counterpart vanishes. We also consider finite Gaussian switching and observe characteristic differences in the radiative process between the GW backgrounds with and without memory. Notably, if the Gaussian switching is peaked much later compared to the passing of GW, only the memory part contributes to the radiative process. Thus, although examined in a simplified set-up, our findings suggest the potential to distinguish bursts with and without GW memory based on the radiative process of entangled detectors.
description: Sections IV and V have been revised to include necessary clarifications and corrections, with some omissions. The current version matches with the published article in Physical Review D
Bolma anacanthos Beu and Ponder 1979
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Bolma
Bolma anacanthos

description: Bolma anacanthos Beu and Ponder, 1979
Bolma anacanthos Beu and Ponder, 1979: 17, Figs 3j–l.
Distribution. Port Phillip Basin: Jan Juc Formation (type). Age: late Oligocene.
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 49, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
Psammophanes undefined-A
Creators: name: Schoeman, Colin S.
name: Toussaint, Dawn Cory
name: Tshililo, Precious
name: Foord, Stefan H.
name: Hamer, Michelle
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Psammophanes
Psammophanes undefined-A

description: Psammophanes sp. A
Fig. 3U,
RM, LM
description: Published as part of Schoeman, Colin S., Toussaint, Dawn Cory, Tshililo, Precious, Foord, Stefan H. & Hamer, Michelle, 2020, Checklist of the pimeliine darkling beetles of the Vhembe Biosphere Reserve, South Africa (Coleoptera: Tenebrionidae: Pimeliinae), pp. 1-9 in Bothalia (a 8) (a 8) 50 (1) on page 7, DOI: 10.38201/btha.abc.v50.i1.8, http://zenodo.org/record/10515087
Podalonia flavida
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Podalonia
Podalonia flavida

description: Podalonia flavida (Kohl, 1901)
(Map 26)
Ammophila flavida Kohl, 1901. Annalen des kaiserlich-königlichen naturhistorischen Hofmuseums. Wien, 16: 163.
Podalonia rothi: Dollfuss, 2010a: 556 (Medenine, Tozeur).
General distribution. Morocco, Spain, Tunisia, Turkey (Dollfuss 2010b).
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 309, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
On minimal presentations of numerical monoids
Creators: name: Moscariello, Alessio
name: Sammartano, Alessio
Publisher: name: arXiv
Year: 2024
Subjects: subject: Combinatorics (math.CO)
subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 20M14, 05E40, 13D02, 13F55, 13F65

description: We consider the classical problem of determining the largest possible cardinality of a minimal presentation of a numerical monoid with given embedding dimension and multiplicity. Very few values of this cardinality are known. In addressing this problem, we apply tools from Hilbert functions and free resolutions of artinian standard graded algebras. This approach allows us to solve the problem in many cases and, at the same time, identify subtle difficulties in the remaining cases. As a by-product of our analysis, we deduce results for the corresponding problem for the type of a numerical monoid.
title: Activité du port de Saint-Malo – 1715 – Dieppe
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: produits agroalimentaires
subject: alcool
subject: graines
subject: produits manufacturés

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 1715 avec le port "Dieppe"
description: Marchandises arrivées à Saint-Malo : harengs ; verres ; vin ; houblon
description: Catégories de marchandises arrivées à Saint-Malo : produits de la mer ; poissons ; produits agroalimentaires ; alcool ; graines ; produits manufacturés
description: Coverage: Grand cabotage
description: Bibliographic citation: BOSSARD, Joseph. Le Trafic malouin en 1714 et 1715. DES : Histoire : Rennes, 1964 (Bibliothèque François-Lebrun, MH 1020)
description: Bibliographic citation: VÉRON, Odile. Le Commerce de Saint-Malo dans la Mer du Sud en 1715 (Bibliothèque François-Lebrun, MH 1021)
description: date: Date de numérisation : 2021 à 2023
description: created: Années 1950-1960
HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
Creators: name: Schuldt, Stefan
name: Cañameras, Raoul
name: Andika, Irham T.
name: Bag, Satadru
name: Melo, Alejandra
name: Shu, Yiping
name: Suyu, Sherry H.
name: Taubenberger, Stefan
name: Grillo, Claudio
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We performed a systematic search for strong gravitational lenses using Hyper Suprime-Cam (HSC) data, focusing on galaxy-scale lenses combined with an environment analysis resulting in the identification of lensing clusters. To identify these lens candidates, we exploited our neural network (NN) from HOLISMOKES VI. During our visual grading, we also simultaneously inspected larger stamps (80'' x 80'') to identify large, extended arcs and also classify their overall environment. Here, we also re-inspected our previous lens candidates with i-Kron radii larger than 0.8''. Using the 546 visually identified lens candidates, we further defined various criteria to select the candidates in overdensities. In total, we identified 24 grade A and 138 grade B candidates that exhibit either spatially-resolved multiple images or extended, distorted arcs in the new sample. Furthermore, combining our different techniques to determine overdensities, we identified a total of 231/546 lens candidates by at least one of our three identification methods for overdensities. This new sample contains only 49 group- or cluster-scale re-discoveries, while 43 systems had been identified by all three procedures. Furthermore, we performed a statistical analysis by using the NN from HOLISMOKES IX to model these systems, making this the largest uniformly modeled sample to date. We find a tendency towards larger Einstein radii for galaxy-scale systems in overdense environments. These results demonstrate the feasibility of applying NNs to hundreds of million cutouts, while resulting in a sample size that can be visually inspected by humans. These deep learning pipelines, with false-positive rates of ~0.01%, are very powerful tools to identify such rare galaxy-scale strong lensing systems, while also aiding in the discovery of new strong lensing clusters.
description: 13+12 pages, 6+9 figures, 4+2 Tables, accepted by A&A for publication
Parapsammophila lateritia Taschenberg 1869
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Parapsammophila
Parapsammophila lateritia

description: Parapsammophila lateritia Taschenberg, 1869
Parapsammophila lateritia Taschenberg, 1869. Zeitschrift für die Gesammten Naturwissenschaften, 34: 431. Parapsammophila lateritia: Dollfuss, 2010a: 538 (Tunisia: no specific locality).
General distribution. Iran, Mali, North Africa, Saudi Arabia, Sudan, Western India (Gadallah & Assery 2004; Guichard 1988).
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 309, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
Neusticomys peruviensis
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
Neusticomys
Neusticomys peruviensis

description: 341.
Peruvian Fish-eating Rat
Neusticomys peruviensis
French: Ichthyomys du Pérou / German: Peru-Fischratte / Spanish: Rata pescadora de Peru
Other common names: Peruvian Ichthyomyine
Taxonomy. Daptomys peruviensis Musser & Gardner, 1974, “Balta (10° 08’ S, 17° 13’ W), at the point where the streams known to the local Cashinahua Indians as the Inuya and the Xumuya enter the Rio Curanja, elevation 300 meters, Departamento de Loreto, Peru.” This species is monotypic.
Distribution. Currently known from only a few localities in Amazonian lowlands of E Peru.
Descriptive notes. Head—body 114-133 mm, tail 90-110 mm, ear 11-4-12 mm, hindfoot 24-30 mm; weight 37 g. The Peruvian Fish-eating Rat has a bright yellowish brown coat. Tail is densely covered with blackish brown hair and is shorter than head-body length. Eyes and ears are small, and ears are clearly visible above head fur. Dorsum is velvety yellowish brown, venteris yellowish gray, and legs and ears are creamy.
Habitat. Primary evergreen lowland forest.
Food and Feeding. The Peruvian Fish-eating Rat eat aquatic insects and perhaps crabs.
Breeding. No information.
Activity patterns. One Peruvian Fish-eating Rat was captured in a pitfall trap after heavy rain, suggesting terrestrial displacement can occur during this kind of weather.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Least Concern on The IUCN Red List.
Bibliography. Medina et al. (2015), Musser & Gardner (1974), Pacheco & Vivar (1996), Vivar & Zeballos (2016), Voss (1988, 2015b).
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 406, DOI: 10.5281/zenodo.6707142
Bolma austroconica Beu and Ponder 1979
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Bolma
Bolma austroconica

description: Bolma austroconica Beu and Ponder, 1979
Bolma austroconica Beu and Ponder, 1979: 18, Figs 3a, b.
Distribution. Port Phillip Basin: Jan Juc Formation (type). Age: late Oligocene.
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 49, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
Comprehensive analysis of the Apertif Fast Radio Burst sample: similarities with young, energetic neutron stars
Creators: name: Pastor-Marazuela, Inés
name: van Leeuwen, Joeri
name: Bilous, Anna
name: Connor, Liam
name: Maan, Yogesh
name: Oostrum, Leon
name: Petroff, Emily
name: Vohl, Dany
name: Hess, Kelley M.
name: Orrù, Emanuela
name: Sclocco, Alessio
name: Wang, Yuyang
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Understanding the origin of fast radio bursts (FRBs) has become the main science driver of recent dedicated FRB surveys. Between July 2019 and February 2022, we carried out ALERT, an FRB survey at 1370 MHz using the Apertif instrument installed at the Westerbork Synthesis Radio Telescope (WSRT). Here we report the detection of 18 new FRBs, and we study the properties of the entire 24 burst sample detected during the survey. For five bursts, we identify host galaxy candidates with >50% probability association. We observe an average linear polarisation fraction of $\sim$43% and an average circular polarisation fraction consistent with 0%. A third of the FRBs display multiple components. The sample next reveals a population of highly scattered bursts, which is most likely to have been produced in the immediate circumburst environment. Furthermore, two FRBs show evidence for high rotation measures, reaching |RM|>$10^3$ rad m$^{-2}$ in the source reference frames. Together, the scattering and rotation measures ALERT finds prove that a large fraction of FRBs are embedded in complex media such as star forming regions or supernova remnants. Through the discovery of the third most dispersed FRB so far, we show that one-off FRBs can emit at frequencies in excess of 6 GHz. Finally, we determine an FRB all-sky rate of $459^{+208}_{-155}$ sky$^{-1}$ day$^{-1}$ above a fluence limit of 4.1 Jy ms, and a fluence cumulative distribution with a power law index $γ=-1.23\pm0.06\pm0.2$, which is roughly consistent with the Euclidean Universe predictions. Through the high resolution in time, frequency, polarisation and localisation that ALERT featured, we were able to determine the morphological complexity, polarisation, local scattering and magnetic environment, and high-frequency luminosity of FRBs. We find all these strongly resemble those seen in young, energetic, highly magnetised neutron stars.
description: 40 pages (including 11 of appendix), 37 figures, 5 tables. Accepted for publication in A&A
Podalonia hirsuta
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Podalonia
Podalonia hirsuta

description: Podalonia hirsuta (Scopoli, 1763)
(Map 27)
Sphex hirsutus Scopoli, 1763. Entomologia Carniolica exhibens Insecta Carnioliae indigena et distributa in ordines, genera, species, varietates. Methodo Linnaeano. Typis loannis, Thomae, Trattner, Vindobonae: 292.
Psammophila hirsuta: Smits van Burgst, 1913: 319 (Tunisia: no specific locality).
Ammophila hirsuta: Graeffe, 1906: 455 (Tunis).
Ammophila (Psammophila) hirsuta: Roth, 1928: 172 (Gafsa, Kairouan).
New records (Total 3 ♂, 9 ♀). Gabes, 1 ♀ (A. Weiss Collection, MNHN); Medenine, 3 ♂ (J. de Gaulle Collection, MNHN), 6 ♀ (Vachal Collection, MNHN); Tozeur, 1 ♀ (Dumont Collection, MNHN); Tunisia: no specific locality, 1 ♀ (J. de Gaulle Collection, MNHN).
General distribution. Palearctic region (Dollfuss 2010b).
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 309, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
Relativistic interacting fluids in cosmology
Creators: name: Iosifidis, Damianos
name: Jensko, Erik
name: Koivisto, Tomi S.
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Motivated by cosmological applications for interacting matters, an extension of the action functional for relativistic fluids is proposed to incorporate the physics of non-adiabatic processes and chemical reactions. The former are characterised by entropy growth, while the latter violate particle number conservation. The relevance of these physics is demonstrated in the contexts of self-interacting fluids, fluids interacting with scalar fields, and hyperhydrodynamical interactions with geometry. The possible cosmological applications range from early-universe phase transitions to astrophysical phenomena, and from matter creation inflationary alternatives to interacting dark sector alternatives to the $Λ$CDM model that aim to address its tensions. As an example of the latter, a single fluid model of a unified dark sector is presented. The simple action of the model features one field and one parameter, yet it can both reproduce the $Λ$CDM cosmology and predict new phenomenology.
description: 15 pages, 1 figure. V2: added references and minor clarifications
Chibchanomys trichotis
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
Chibchanomys
Chibchanomys trichotis

description: 342.
Northern Andean Water Mouse
Chibchanomys trichotis
French: Ichthyomys chibchan / German: Nordliche Andenwassermaus / Spanish: Raton de agua septentrional
Other common names: Chibchan Ichthyomyine, Chibchan Water Mouse
Taxonomy. Ichthyomys trichotis Thomas, 1897, “W. Cundinamarca, in low country near to Magdalena R[iver, Colombia].”
Chibchanomys trichotis 1s the type species of the genus. Monotypic.
Distribution. E Andes Range in extreme SW Venezuela and NC Colombia.
Descriptive notes. Head-body 113-125 mm, tail 115-133 mm, ear 6-10 mm, hindfoot 30-33 mm; weight 35-50 g. Dorsum of the Northern Andean Water Mouse is dull gray or black, contrasting pale gray venter. Tail is longer than headbody length. There are no supraorbital vibrissae, and pinnae are hidden in fur of head. Manus has five separate plantar pads. Pes has well-developed fringe of stiff, silvery hair, and claw of pedalfifth digit extends beyond first interphalangeal joint of fourth digit.
Habitat. Small mountain streams bordered by cloud forest at of 2400-2900 m.
Food and Feeding. The Northern Andean Water Mouse eats aquatic insects, including larval beetles (Scirtidae = Helodidae), larval crane flies (Tipulidae), larval caddisflies (Leptoceridae), and nymphs of mayflies (Leptophlebiidae and Tricorythidae) and stoneflies (Perlidae).
Breeding. An adult Northern Andean Water Mouse trapped in middle of dry season (January) had a single near-term embryo.
Activity patterns. The Northern Andean Water Mouse is semi-aquatic and probably nocturnal.
Movements, Home range and Social organization. No information.
Status and Conservation. Classified as Data Deficient on The IUCN Red List. This classification 1s due to lack of recent information on extent of occurrence, threats, status, and ecological requirements of the Northern Andean Water Mouse.
Bibliography. Gbmez-Laverde et al. (2008), Jenkins & Barnett (1997), Thomas (1897b), Voss (1988, 2015b).
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 406, DOI: 10.5281/zenodo.6707142
Podalonia marismortui
Creators: name: Khedher, Hassib Ben
name: Yildirim, Erol
name: Braham, Mohamed
name: Ljubomirov, Toshko
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Sphecidae
Podalonia
Podalonia marismortui

description: Podalonia marismortui (Bytinski-Salz, 1955)
(Map 28)
Ammophila maris-mortui Bytinski-Salz in de Beaumont and Bytinski-Salz, 1955. The Bulletin of the Research Council of Israel. Section B: Zoology 5: 33.
Ammophila hirsuta sp. gen.: Roth, 1928: 175 (Gafsa, Medenine).
Ammophila (Podalonia) maris mortui: de Beaumont, 1968: 145 (Medenine).
General distribution. Canary Islands, Egypt, Iraq, Israel, Oman (Dollfuss 2010b).
Remark. Roth, 1928 mentioned that the Tunisian specimens from Medenine and Gafsa have affinity to Podalonia hirsuta and then de Beaumont 1968 studied 1 female from Medenine and assigned it as Podalonia marismortui.
description: Published as part of Khedher, Hassib Ben, Yildirim, Erol, Braham, Mohamed & Ljubomirov, Toshko, 2020, First checklist of Tunisian sphecid wasps (Hymenoptera: Sphecidae) with new and additional records, pp. 301-327 in Zootaxa 4801 (2) on page 310, DOI: 10.11646/zootaxa.4801.2.6, http://zenodo.org/record/3900484
Somaticus Hope 1840
Creators: name: Schoeman, Colin S.
name: Toussaint, Dawn Cory
name: Tshililo, Precious
name: Foord, Stefan H.
name: Hamer, Michelle
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Somaticus

description: Somaticus cf. (Trichotrichus) metropolis Koch, 1955
RM
description: Published as part of Schoeman, Colin S., Toussaint, Dawn Cory, Tshililo, Precious, Foord, Stefan H. & Hamer, Michelle, 2020, Checklist of the pimeliine darkling beetles of the Vhembe Biosphere Reserve, South Africa (Coleoptera: Tenebrionidae: Pimeliinae), pp. 1-9 in Bothalia (a 8) (a 8) 50 (1) on page 7, DOI: 10.38201/btha.abc.v50.i1.8, http://zenodo.org/record/10515087
Machine learning Hubbard parameters with equivariant neural networks
Creators: name: Uhrin, Martin
name: Zadoks, Austin
name: Binci, Luca
name: Marzari, Nicola
name: Timrov, Iurii
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Machine Learning (cs.LG)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Density-functional theory with extended Hubbard functionals (DFT+$U$+$V$) provides a robust framework to accurately describe complex materials containing transition-metal or rare-earth elements. It does so by mitigating self-interaction errors inherent to semi-local functionals which are particularly pronounced in systems with partially-filled d and f electronic states. However, achieving accuracy in this approach hinges upon the accurate determination of the on-site $U$ and inter-site $V$ Hubbard parameters. In practice, these are obtained either by semi-empirical tuning, requiring prior knowledge, or, more correctly, by using predictive but expensive first-principles calculations. Here, we present a machine learning model based on equivariant neural networks which uses atomic occupation matrices as descriptors, directly capturing the electronic structure, local chemical environment, and oxidation states of the system at hand. We target here the prediction of Hubbard parameters computed self-consistently with iterative linear-response calculations, as implemented in density-functional perturbation theory (DFPT), and structural relaxations. Remarkably, when trained on data from 12 materials spanning various crystal structures and compositions, our model achieves mean absolute relative errors of 3% and 5% for Hubbard $U$ and $V$ parameters, respectively. By circumventing computationally expensive DFT or DFPT self-consistent protocols, our model significantly expedites the prediction of Hubbard parameters with negligible computational overhead, while approaching the accuracy of DFPT. Moreover, owing to its robust transferability, the model facilitates accelerated materials discovery and design via high-throughput calculations, with relevance for various technological applications.
A field-level emulator for modified gravity
Creators: name: Saadeh, Daniela
name: Koyama, Kazuya
name: Morice-Atkinson, Xan
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Stage IV surveys like LSST and Euclid present a unique opportunity to shed light on the nature of dark energy. However, their full constraining power cannot be unlocked unless accurate predictions are available at all observable scales. Currently, only the linear regime is well understood in models beyond $Λ$CDM: on the nonlinear scales, expensive numerical simulations become necessary, whose direct use is impractical in the analyses of large datasets. Recently, machine learning techniques have shown the potential to break this impasse: by training emulators, we can predict complex data fields in a fraction of the time it takes to produce them.
 In this work, we present a field-level emulator capable of turning a $Λ$CDM N-body simulation into one evolved under $f(R)$ gravity. To achieve this, we build on the map2map neural network, using the strength of modified gravity $|f_{R_0}|$ as style parameter. We find that our emulator correctly estimates the changes it needs to apply to the positions and velocities of the input N-body particles to produce the target simulation.
 We test the performance of our network against several summary statistics, finding $1\%$ agreement in the power spectrum up to $k \sim 1$ $h/$Mpc, and $1.5\%$ agreement against the independent boost emulator eMantis. Although the algorithm is trained on fixed cosmological parameters, we find it can extrapolate to models it was not trained on. Coupled with available field-level emulators and simulation suites for $Λ$CDM, our algorithm can be used to constrain modified gravity in the large-scale structure using full information available at the field level.
description: 17 pages, 11 figures; version accepted on MNRAS
The Lyman Alpha Reference Sample XV. Relating Ionised Gas Kinematics with Lyman-$α$ observables
Creators: name: Herenz, E. C.
name: Schaible, A.
name: Laursen, P.
name: Runnholm, A.
name: Melinder, J.
name: Reste, A. Le
name: Hayes, M. J.
name: Östlin, G.
name: Cannon, J.
name: Micheva, G.
name: Roth, M.
name: Saha, K.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Gas kinematics affect the radiative transfer and escape of hydrogen Lyman-$α$ (Ly$α$) emission from galaxies. We investigate this interplay empirically by relating the ionised gas kinematics of 42 galaxies in the extended Ly$α$ Reference Sample with their Ly$α$ escape fractions, $f_\rm{esc}$, Ly$α$ equivalent widths, $\rm{EW}_\rm{Lyα}$, and Ly$α$ luminosities, $L_\rm{Lyα}$. To this aim we use PMAS integral-field spectroscopic observations of the Balmer-$α$ line. We calculate shearing velocities, $v_\rm{shear}$, and intrinsic velocity dispersions, $σ_0^\rm{obs}$ (empirically corrected for beam-smearing effects), as global kinematical measures for each galaxy. The sample is characterised by highly turbulent motions and more than half of the sample shows dispersion dominated kinematics. We uncover clear trends between Ly$α$ observables and global kinematical statistics. We discuss statistically the importance of $v_\rm{shear}$, $σ_0^\rm{obs}$, and $v_\rm{shear}/σ_0^\rm{obs}$ for regulating the Ly$α$ observables in comparison to other galaxy parameters. It emerges that $σ_0^\rm{obs}$ is the dominating parameter for $\rm{EW}_\rm{Lyα}$ and that is as important as nebular extinction, gas covering fraction, and ionising photon production efficiency in regulating $f_\rm{esc}$. A simple scenario where the starburst age is simultaneously regulating turbulence, $\rm{EW}_\rm{Lyα}$, and $f_\rm{esc}$ does not find support by our observations. However, we show that the small scale distribution of dust appears to be influenced by turbulence in some galaxies. In support of our observational result we discuss how turbulence is theoretically expected to play a significant role in modulating $f_\rm{esc}$.
 (abridged)
description: Accepted version for publication in A&A
Bolma flindersi subsp. flindersi
Creators: name: Darragh, Thomas A.
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Trochida
Turbinidae
Bolma
Bolma flindersi
Bolma flindersi flindersi (tenison woods, 1877)

description: Bolma flindersi flindersi (Tenison Woods, 1877)
Astralium (Calcar) flindersii Tenison Woods, 1877: 95.— May 1919: 71, pl. 10, fig. 11.
Bolma flindersi flindersi (Tenison Woods, 1877).— Beu and Ponder, 1979: 21, Figs 4d–j.
Distribution. Bass Basin: Freestone Cove 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 49, DOI: 10.24199/j.mmv.2024.83.02, http://zenodo.org/record/14704472
Kaius Gómez, 2024, nom. nov.
Creators: name: Gómez, Samuel
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Copepoda
Harpacticoida
Argestidae
Kaius

description: Genus Kaius nom. nov.
urn:lsid:zoobank.org:act: 4AEC9D7A-292B-4B0F-801A-4458B6133FB4
Georgus Gómez, 2018 [J. Nat. Hist., 52(41–42): 2615–2616] (Crustacea: Copepoda: Harpacticoida: Argestidae) preoccupied by Georgus Thiele, 1893 [Geb. Sch. Beg. natür. Class., 2: 366] (Mollusca: Polyplacophora: Chitonida: Chitonidae), syn. Rhyssoplax Thiele, 1893 [Geb. Sch. Beg. natür. Class., 2: 368] (Mollusca: Polyplacophora: Chitonida: Chitonidae).
Remarks. Thiele (1893: 367–368) proposed the genus Georgus for two species formerly placed in the genus Chiton Linnaeus, 1758 (Polyplacophora: Chitonida), G. rusticus (Deshayes, 1863) and G. nigrovirescens (Blainville, 1825). Some years later, Thiele (1909) synonymised these two species with C. angusticostatus Quoy & Gaimard, 1835 which was subsequently synonymised with C. mauritianus Quoy & Gaimard, 1835 by Dupuis (1918). Van Belle (1983) regarded the genus Rhyssoplax proposed by Thiele (1893), as a subgenus of Chiton, but O’Neill (1989) gave Rhyssoplax full genus status. Bullock (1988a) noted that many chitonid species from the Old World placed in the genus Chiton probably belong in Rhyssoplax, and Bullock (1988b) reallocated C. nigrovirescens into Radsia Gray 1847. At present, C. mauritianus (= G. rusticus) is accepted as R. mauritiana (Quoy & Gaimard, 1835), and the chitonid genus Georgus is currently regarded as a junior subjective synonym of Rhyssoplax (MolluscaBase eds. 2024). Despite its status, the chitonid genus Georgus remains available irrespective of its invalidity as a junior synonym (ICZN 1999, Art. 10.6).
Gómez (2018) proposed the genus name Georgus for Bodinia peterrumi George, 2004 (Crustacea: Copepoda: Harpacticoida: Argestidae) and entered homonymy with the chitonid genus name Georgus. Since the chitonid genus name Georgus (Polyplacophora) remains available (see above), a new replacement name for the argestid genus name Georgus (Copepoda) is required.
Here I propose the new replacement name, Kaius nom. nov., as intentionally new for Georgus Gómez, 2018 (Copepoda: Harpacticoida: Argestidae) (ICZN 1999, Art. 16.1).
The prior nominal taxon, Georgus Gómez, 2018 and the new replacement name Kaius nom. nov., proposed herein, have the same type species, Bodinia peterrumi George, 2004) [= Georgus peterrumi (George, 2004)] (ICZN 1999, Art. 67.8), and should be referred to as Kaius peterrumi (George, 2004) comb. nov. The generic diagnosis of Kaius nom. nov. is the same as for the prior nominal taxon, Georgus Gómez, 2018, and is as in Gómez (2018: 2615–2616) (ICZN 1999, Art. 13.3).
Etymology. The new replacement name, Kaius nom. nov., is dedicated to Dr Kai Horst George for his contribution to the knowledge of the Argestidae.
description: Published as part of Gómez, Samuel, 2024, Proposal of a new replacement name for Georgus Gómez, 2018 (Copepoda, Harpacticoida, Argestidae), pp. 399-400 in Zootaxa 5523 (3) on page 399, DOI: 10.11646/zootaxa.5523.3.9, http://zenodo.org/record/13949589