cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lyomyces albofarinaceus Y. F. Dai & C. L. Zhao 2025, sp. nov.
Creators: name: Dai, Yunfei
name: Yuan, Qi
name: Yang, Xin
name: Liu, Rui
name: Liu, Defu
name: Yuan, Haisheng
name: Zhao, Changlin
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Fungi
Basidiomycota
Agaricomycetes
Hymenochaetales
Corticiaceae
Lyomyces
Lyomyces albofarinaceus

description: Lyomyces albofarinaceus Y. F. Dai & C. L. Zhao sp. nov.
Figs 8, 9
Holotype.
China • Yunnan Province, Zhaotong, Wumengshan National Nature Reserve, GPS coordinates 28°05′N, 104°20′E, evel. 1600 m a. s. l., on a fallen branch of angiosperm, leg. C. L. Zhao, 20 September 2023, CLZhao 33479 (SWFC).
Etymology.
albofarinaceus (Lat.), refers to the white and pruinose hymenophore surface.
Basidiomata.
Annual, resupinate, adnate, without odor or taste when fresh, up to 8 cm long, 3.5 cm wide, and 150 µm thick. Hymenial surface pruinose, smooth, white when fresh, to white to cream upon drying. Sterile margin narrow, white, up to 1 mm wide.
Hyphal system.
Monomitic, generative hyphae with clamp connections, colorless, thin to slightly thick-walled, frequently branched, interwoven, 2.0–3.0 µm in diameter, IKI –, CB –; tissues unchanged in KOH, subhymenial hyphae densely covered by crystals.
Hymenium.
Cystidia of two types: (1) tapering, thin-walled, smooth to be covered by crystals, 11.5–44.0 × 4.5–7.5 µm; (2) capitate, thin-walled, smooth to be covered by crystals, slightly constricted at the neck, with a globose tip, 23.5–40.0 × 3.5–5.5 µm; cystidioles absent. Basidia clavate, colorless, thin-walled, with four sterigmata, 15.0–27.0 × 5.0–9.5 µm; basidioles in shape similar to basidia, but slightly smaller.
Basidiospores.
Broadly ellipsoid, colorless, thin-walled, smooth, with one guttate, IKI –, CB –, (5.5 –) 6.0–7.0 (– 7.5) × (4.5 –) 5.0–6.0 (– 6.5) µm, L = 6.46 µm, W = 5.62 µm, Q = 1.07–1.15 (n = 60 / 2).
Additional specimens examined (Paratype).
China • Yunnan Province, Qujing, Qilin District, Cuishan Forestry Park, on a fallen angiosperm branch, 5 November 2022, CLZhao 26661 (SWFC).
description: Published as part of Dai, Yunfei, Yuan, Qi, Yang, Xin, Liu, Rui, Liu, Defu, Yuan, Haisheng & Zhao, Changlin, 2025, Morphological characteristics and phylogenetic analyses reveal five new species of Hymenochaetales (Agaricomycetes, Basidiomycota) from southwestern China, pp. 133-175 in MycoKeys 114 on pages 133-175, DOI: 10.3897/mycokeys.114.143851
Additional file 1 of SKP alleviates the ferroptosis in diabetic kidney disease through suppression of HIF-1α/HO-1 pathway based on network pharmacology analysis and experimental validation
Creators: name: Yan, Yangtian
name: Yuan, Ningning
name: Chen, Yuchi
name: Ma, Yun
name: Chen, Ali
name: Wang, Fujing
name: Yan, Shihua
name: He, Zhuo’en
name: He, Jinyue
name: Zhang, Chi
name: Wang, Hao
name: Wang, Mingqing
name: Diao, Jianxin
name: Xiao, Wei
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Marine Biology

description: Additional file 1: Table S1. Specific information on compounds in The Herb-ingredient-targets gene network.
A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy
Creators: name: Burke-Spolaor, Sarah
name: Gultekin, Kayhan
name: Postman, Marc
name: Lauer, Tod R.
name: Taylor, Joanna M.
name: Lazio, T. Joseph W.
name: Moustakas, Leonidas A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present VLA images and HST/STIS spectra of sources within the center of the brightest cluster galaxy (BCG) in Abell 2261. These observations were obtained to test the hypothesis that its extremely large, flat core reflects the ejection of its supermassive black hole. Spectra of three of the four most luminous "knots" embedded in the core were taken to test whether one may represent stars bound to a displaced massive black hole. The three knots have radial velocity offsets dV < ~150 km/s from the BCG. Knots 2 and 3 show kinematics, colors, and stellar masses consistent with infalling low-mass galaxies or larger stripped cluster members. Large errors in the stellar velocity dispersion of Knot 1, however, mean that we cannot rule out the hypothesis that it hosts a high-mass black hole. A2261-BCG has a compact, relic radio-source offset by 6.5 kpc (projected) from the optical core's center, but no active radio core that would pinpoint the galaxy's central black hole to a tight 10 GHz flux limit <3.6 uJy. Its spectrum and morphology are suggestive of an active galactic nucleus that switched off >48 Myr ago, with an equipartition condition magnetic field of 15 uG. These observations are still consistent with the hypothesis that the nuclear black hole has been ejected from its core, but the critical task of locating the supermassive black hole or demonstrating that A2261-BCG lacks one remains to be done.
description: 12 pages, 9 figures, submitted to ApJ
Universality of Egoless Behavior of Software Engineering Students
Creators: name: Waychal, Pradeep
name: Capretz, Luiz Fernando
Publisher: name: arXiv
Year: 2017
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Software organizations have relied on process and technology initiatives to compete in a highly globalized world. Unfortunately, that has led to little or no success. We propose that the organizations start working on people initiatives, such as inspiring egoless behavior among software developers. This paper proposes a multi-stage approach to develop egoless behavior and discusses the universality of the egoless behavior by studying cohorts from three different countries, i.e., Japan, India, and Canada. The three stages in the approach are self-assessment, peer validation, and action plan development. The paper covers the first stage of self-assssment using an instrument based on Lamont Adams Ten commandments (factors) of egoless programming, seven of the factors are general, whereas three are related to coding behavior. We found traces of universality in the egoless behavior among the three cohorts such as there was no difference in egoless behaviours between Indian and Canadian cohorts and both Indian and Japanese cohorts had difficulties in behaving in egoless manner in coding activities than in general activities.
Technosignatures with TESS: The Search for Hidden Stellar Occulters
Creators: name: Giles, Daniel
Publisher: name: Zenodo
Year: 2021

description: Stellar brightness fluctuations encode a diverse range of phenomena from exoplanetary transits. If there are advanced civilizations in the galaxy, we may also be able to detect certain technosignatures in these fluctuations. In particular, artificial structures around a host star may produce pronounced and characteristic fading events in light curves. This possibility was recently brought to the forefront with the analysis of Boyajian’s Star (KIC 8462852), which displayed erratic brightness dips. While no theory provides a perfect explanation for the fading events seen in Boyajian's star, the large volume of imaging data emerging from the TESS mission is now enabling a new search for similar behavior in additional objects. Our team has created light curves for a set of 50 million relatively bright stars across the sky from the TESS Full Frame Images. We are using a combination of supervised and unsupervised machine learning to discover and classify rare fading events. We will follow up on the most unusual objects with ground-based optical and radio observatories to determine the origin of such variability.
description: The 2021 Assembly of the Order of the Octopus - Participant Talks - Session IV: Stars & Megastructures
Additional file 2: of mRNA-seq whole transcriptome profiling of fresh frozen versus archived fixed tissues
Creators: name: Ben-Moshe, Noa Bossel
name: Gilad, Shlomit
name: Perry, Gili
name: Benjamin, Sima
name: Balint-Lahat, Nora
name: Pavlovsky, Anya
name: Halperin, Sharon
name: Markus, Barak
name: Yosepovich, Ady
name: Barshack, Iris
name: Gal-Yam, Einav
name: Domany, Eytan
name: Kaufman, Bella
name: Dadiani, Maya
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Table S2. Number of exonic and intronic reads. (PDF 167Â kb)
Spontaneous antiferromagnetic order and strain effect on electronic properties of $α$-graphyne
Creators: name: Dong, Baojuan
name: Guo, Huaihong
name: Liu, Zhiyong
name: Yang, Teng
name: Tao, Peng
name: Tang, Sufang
name: Saito, Riichiro
name: Zhang, Zhidong
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Using hybrid exchange-correlation functional in ab initio density functional theory calculations, we study magnetic properties and strain effect on the electronic properties of $α$-graphyne monolayer. We find that a spontaneous antiferromagnetic (AF) ordering occurs with energy band gap ($\sim$ 0.5 eV) in the equilibrated $α$-graphyne. Bi-axial tensile strain enhances the stability of AF state as well as the staggered spin moment and value of the energy gap. The antiferromagnetic semiconductor phase is quite robust against moderate carrier filling with threshold carrier density up to 1.7$\times$10$^{14}$ electrons/cm$^2$ to destabilize the phase. The spontaneous AF ordering and strain effect in $α$-graphyne can be well described by the framework of the Hubbard model. Our study shows that it is essential to consider the electronic correlation effect properly in $α$-graphyne and may pave an avenue for exploring magnetic ordering in other carbon allotropes with mixed hybridization of s and p orbitals.
description: 6 pages, 5 figures
title: Methodik zur Erweiterung von Lernfabriken um das Thema Ressourceneffizienz
Creators: name: Weyand, Astrid
Publisher: name: UNSPECIFIED
Year: 2024

description: Im Zuge des Klimawandels und der globalen Bestrebungen für ein nachhaltiges Leben auf der Erde gerät auch die Ressourceneffizienz, also der effiziente Umgang mit vorhandenen Ressourcen, zunehmend in den Fokus der Industrie. Dafür ist die Vermittlung von Kompetenzen von Nöten, wofür sich sogenannte Lernfabriken bewährt haben. Dennoch ist Ressourceneffizienz in Lernfabriken nach wie vor weniger verbreitet als etwa Themen der Digitalisierung oder Lean Production. Die vorliegende Arbeit verfolgt das Ziel, systematisch zu erarbeiten, wie bestehende Lernfabriken um das Thema Ressourceneffizienz erweitert werden können.
Dafür werden zunächst relevante Begrifflichkeiten abgegrenzt und in einer systematischen Literaturanalyse ermittelt, welche Kompetenzen im Kontext Ressourceneffizienz in der Industrie zu vermitteln sind. Diese Kompetenzen werden anschließend mit typischen Vorgehensweisen zur Steigerung von Ressourceneffizienz abgeglichen und in Bezug zu den Vorteilen von Lernfabriken gesetzt. Daraus ergeben sich drei Aspekte, die bei der entwickelten Methodik im Fokus stehen. Zum einen ist das die Vermittlung von Methodenkompetenz hinsichtlich sogenannter Hotspotanalysemethoden. Mit diesen können kritische Stellen (Hotspots) im Produktionsprozess identifiziert werden. Im Anschluss können als zweiter Aspekt Ressourceneffizienzmaßnahmen für diese Stellhebel gesucht und in der Lernfabrik veranschaulicht werden. Und zum dritten werden die Teilaspekte in einem ganzheitlichen Vorgehen zusammengeführt.
Die resultierende Methodik beinhaltet insgesamt fünf Schritte. Zunächst müssen Randbedingungen wie das vorhandene Budget für die Erweiterung oder die bereits vorhandene Infrastruktur analysiert werden, wobei ein entsprechender Fragebogen unterstützen kann. Im nächsten Schritt wird passend zu diesen Randbedingungen ermittelt, welche Hotspotanalysemethode oder auch -methoden geschult werden sollen. Dafür wurde ein adaptierbares Vergleichstool entwickelt. Analog gilt dies auch für den dritten Schritt; die Auswahl der Ressourceneffizienzmaßnahmen, die in der Lernfabrik gezeigt werden sollen. Auch hierfür wurde im Rahmen der Arbeit ein Maßnahmentool entwickelt, welches knapp 120 Ressourceneffizienzmaßnahmen systematisch kategorisiert und dabei auch lernfabrik-spezifische Kriterien wie den Umbauaufwand berücksichtigt. Im vierten Schritt werden basierend auf den zuvor getroffenen Entscheidungen Kompetenzen und die für die Vermittlung notwendige Infrastruktur abgeleitet. Im fünften Schritt erfolgt dann parallel die Umsetzung der Kompetenzen in entsprechenden Lernmodulen und, nach Abgleich mit der vorhandenen Infrastruktur, die Umsetzung der technischen Anforderungen. Die entwickelte Methodik konnte in zwei Lernfabriken in Darmstadt sowie in einer Lernfabrik in Aachen angewendet und evaluiert werden. Die Evaluationsergebnisse konnten die Erfüllung der zuvor aufgestellten Anforderungen belegen und Anhaltspunkte für zukünftige Arbeiten aufzeigen.
On the origin of the O and B-type stars with high velocities II Runaway stars and pulsars ejected from the nearby young stellar groups
Creators: name: Hoogerwerf, R.
name: de Bruijne, J. H. J.
name: de Zeeuw, P. T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use milli-arcsecond accuracy astrometry (proper motions and parallaxes) from Hipparcos and from radio observations to retrace the orbits of 56 runaway stars and nine compact objects with distances less than 700 pc, to identify the parent stellar group. It is possible to deduce the specific formation scenario with near certainty for two cases. (i) We find that the runaway star zeta Ophiuchi and the pulsar PSR J1932+1059 originated about 1 Myr ago in a supernova explosion in a binary in the Upper Scorpius subgroup of the Sco OB2 association. The pulsar received a kick velocity of about 350 km/s in this event, which dissociated the binary, and gave zeta Oph its large space velocity. (ii) Blaauw & Morgan and Gies & Bolton already postulated a common origin for the runaway-pair AE Aur and mu Col, possibly involving the massive highly-eccentric binary iota Ori, based on their equal and opposite velocities. We demonstrate that these three objects indeed occupied a very small volume \sim 2.5Myr ago, and show that they were ejected from the nascent Trapezium cluster. We identify the parent group for two more pulsars: both likely originate in the 50 Myr old association Per OB3, which contains the open cluster alpha Persei. At least 21 of the 56 runaway stars in our sample can be linked to the nearby associations and young open clusters. These include the classical runaways 53 Arietis (Ori OB1), xi Persei (Per OB2), and lambda Cephei (Cep OB3), and fifteen new identifications, amongst which a pair of stars running away in opposite directions from the region containing the lambda Ori cluster. Other currently nearby runaways and pulsars originated beyond 700 pc, where our knowledge of the parent groups is very incomplete.
description: Accepted for publication in the A&A. 29 pages, 19 figures
Evolutionary and Observational Consequences of Dyson Sphere Feedback
Creators: name: Huston, Macy
Publisher: name: Zenodo
Year: 2021

description: The search for signs of extraterrestrial technology, or technosignatures, includes the search for objects which collect starlight for some technological use, such as those composing a Dyson sphere. These searches typically account for a star’s light and some blackbody temperature for the surrounding structure. However, such a structure inevitably returns some light back to the surface of its star, either from direct reflection or thermal re-emission. In this work, we explore how this feedback may affect the structure and evolution of stars, and when such feedback may affect observations. We find that in general this returned light can cause stars to expand and cool. Our MESA models show that this energy is only transported toward a star’s core effectively by convection, so low mass stars are strongly affected, while higher mass sta s with radiative exteriors are not. Ultimately, the effect only has significant observational consequences for spheres with very high temperatures and/or high specular reflectivity. Lastly, we produce color-magnitude diagrams of combined star-Dyson sphere systems for a wide array of possible configurations.
description: The 2021 Assembly of the Order of the Octopus - Participant Talks - Session IV: Stars & Megastructures
Additional file 1 of The burden of disease in metachromatic leukodystrophy: results of a caregiver survey in the UK and Republic of Ireland
Creators: name: Thomas, Sophie
name: Morrison, Alexandra
name: Morton, Georgina
name: Roberts, Pat
name: Clark, Vivienne
name: Imrie, Jackie
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Lyomyces albomarginatus Y. F. Dai & C. L. Zhao 2025, sp. nov.
Creators: name: Dai, Yunfei
name: Yuan, Qi
name: Yang, Xin
name: Liu, Rui
name: Liu, Defu
name: Yuan, Haisheng
name: Zhao, Changlin
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Fungi
Basidiomycota
Agaricomycetes
Hymenochaetales
Corticiaceae
Lyomyces
Lyomyces albomarginatus

description: Lyomyces albomarginatus Y. F. Dai & C. L. Zhao sp. nov.
Figs 10, 11
Holotype.
China • Yunnan Province, Dali, Weishan County, QinghuaTown, Green Peacock Reserve, Jiangzui Village, GPS coordinates 25°01′N, 100°11′E, evel. 1500 m a. s. l., on a fallen branch of angiosperm, leg. C. L. Zhao, 18 July 2022, CLZhao 22551 (SWFC).
Etymology.
albomarginatus (Lat.), refers to the white margin of the basidiomata.
Basidiomata.
Annual, resupinate, adnate, without odor or taste when fresh, up to 8 cm long, 3 cm wide, and 150 µm thick. Hymenial surface cracked, slightly buff when fresh, turning to buff to slightly yellowish upon drying. Sterile margin slightly buff, up to 3 mm wide.
Hyphal system.
Monomitic, generative hyphae with clamp connections, colorless, thin to slightly thick-walled, rarely branched, interwoven, 2.0–3.5 µm in diameter, IKI –, CB –; tissues unchanged in KOH.
Hymenium.
Cystidia numerous, tapering, thin-walled, smooth, 22.5–30.0 × 2.0–4.0 µm; cystidioles absent. Basidia cylindrical, colorless, thin-walled, with four sterigmata, 15.0–19.0 × 3.5–4.3 µm; basidioles in shape similar to basidia, but slightly smaller.
Basidiospores.
Elliposoid, colorless, thin-walled, smooth, with one guttate, IKI –, CB –, (3.5 –) 4.0–5.5 (– 6.0) × (2.5 –) 2.7–3.5 (– 3.7) µm, L = 4.89 µm, W = 3.13 µm, Q = 1.56 (n = 30 / 1).
description: Published as part of Dai, Yunfei, Yuan, Qi, Yang, Xin, Liu, Rui, Liu, Defu, Yuan, Haisheng & Zhao, Changlin, 2025, Morphological characteristics and phylogenetic analyses reveal five new species of Hymenochaetales (Agaricomycetes, Basidiomycota) from southwestern China, pp. 133-175 in MycoKeys 114 on pages 133-175, DOI: 10.3897/mycokeys.114.143851
All-optical switching, bistability, and slow-light transmission in photonic crystal waveguide-resonator structures
Creators: name: Mingaleev, Sergei F.
name: Miroshnichenko, Andrey E.
name: Kivshar, Yuri S.
name: Busch, Kurt
Publisher: name: arXiv
Year: 2006
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We analyze the resonant linear and nonlinear transmission through a photonic crystal waveguide side-coupled to a Kerr-nonlinear photonic crystal resonator. Firstly, we extend the standard coupled-mode theory analysis to photonic crystal structures and obtain explicit analytical expressions for the bistability thresholds and transmission coefficients which provide the basis for a detailed understanding of the possibilities associated with these structures. Next, we discuss limitations of standard coupled-mode theory and present an alternative analytical approach based on the effective discrete equations derived using a Green's function method. We find that the discrete nature of the photonic crystal waveguides allows a novel, geometry-driven enhancement of nonlinear effects by shifting the resonator location relative to the waveguide, thus providing an additional control of resonant waveguide transmission and Fano resonances. We further demonstrate that this enhancement may result in the lowering of the bistability threshold and switching power of nonlinear devices by several orders of magnitude. Finally, we show that employing such enhancements is of paramount importance for the design of all-optical devices based on slow-light photonic crystal waveguides.
description: 16 pages, 12 figures
Additional file 1 of Delivering medical leadership training through the Healthcare Leadership Academy: a four year analysis
Creators: name: Zarif, Azmaeen
name: Bandyopadhyay, Soham
name: Miller, George
name: Malawana, Johann
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Pharmacology
subject: Geology
subject: FOS: Earth and related environmental sciences
subject: Science Policy

description: Additional file 1.
Sagnac interference in Carbon nanotube loops
Creators: name: Refael, Gil
name: Heo, Jinseong
name: Bockrath, Marc
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In this paper we study electron interference in nanotube loops. The conductance as a function of the applied voltage is shown to oscillate due to interference between electron beams traversing the loop in two opposite directions, with slightly different velocities. The period of these oscillations with respect to the gate voltage, as well as the temperatures required for the effect to appear, are shown to be much larger than those of the related Fabry-Perot interference. This effect is analogous to the Sagnac effect in light interferometers. We calculate the effect of interactions on the period of the oscillations, and show that even though interactions destroy much of the near-degeneracy of velocities in the symmetric spin channel, the slow interference effects survive.
description: 5 pages, 4 figures
MOESM10 of Age-related DNA methylation changes are tissue-specific with ELOVL2 promoter methylation as exception
Creators: name: Slieker, Roderick
name: Relton, Caroline
name: Gaunt, Tom
name: P. Slagboom
name: Heijmans, Bastiaan
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Pharmacology
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 10: Figure S8. A Percentage (top) and odds ratios (bottom) of gain-aDMPs in CGIs, shores and non-CGIs. Blue enriched, red depleted, grey non-significant. B Percentage (top) and odds ratios (bottom) of aDMPs in EZH2 binding sites in the seven tissues plus whole blood (ChIP-seq, any cell type, ENCODE). Blue enriched, red depleted, grey non-significant. C Enrichment of gain-aDMPs in chromatin segmentations expressed in the seven tissues plus whole blood as an odds ratio, grey non-significant. D Percentage (top) and odds ratios (bottom) of loss-aDMPs in CGIs, shores and non-CGIs. Blue enriched, red depleted, grey non-significant. E Enrichment of loss-aDMPs in chromatin segmentations expressed in the seven tissues plus whole blood as an odds ratio, grey non-significant. Abbreviations: TssA, Active TSS; TssAFlnk, Flanking active TSS; TxFlnk, Transcr. at gene 5′ and 3′; Tx, Strong transcription; TxWk, Weak transcription; EnhG, Genic enhancers; Enh, Enhancers; ZNF/Rpts, ZNF genes + repeats; Het, Heterochromatin; TssBiv, Bivalent/Poised TSS; BivFlnk, Flanking bivalent TSS/Enh; EnhBiv, Bivalent enhancer; ReprPC, Repressed Polycomb; ReprPCWk, Weak repressed Polycomb, Quies, Quiescent/low.
Tubulicrinis albobadius Y. F. Dai & C. L. Zhao 2025, sp. nov.
Creators: name: Dai, Yunfei
name: Yuan, Qi
name: Yang, Xin
name: Liu, Rui
name: Liu, Defu
name: Yuan, Haisheng
name: Zhao, Changlin
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Fungi
Basidiomycota
Agaricomycetes
Hymenochaetales
Hymenochaetaceae
Tubulicrinis
Tubulicrinis albobadius

description: Tubulicrinis albobadius Y. F. Dai & C. L. Zhao sp. nov.
Figs 12, 13
Holotype.
China • Yunnan Province, Qujing, Qilin District, Cuishan Forest Park, GPS coordinates 25°32′N, 103°42′E, evel. 2250 m a. s. l., on a fallen branch of angiosperm, leg. C. L. Zhao, 5 Novermber 2022, CLZhao 26202 (SWFC).
Etymology.
albobadius (Lat.), refers to the white basidiomata.
Basidiomata.
Annual, resupinate, thin, adnate, without odor or taste when fresh, up to 8 cm long, 1.5 cm wide, and 150 µm thick. Hymenial surface arachnoid, white when fresh and became white to gray when drying. Sterile margin narrow, white, up to 1 mm.
Hyphal system.
Monomitic, generative hyphae with clamp connections, colorless, thick-walled, branched, interwoven, 2.0–4.0 µm in diameter, IKI –, CB –; tissues unchanged in KOH.
Hymenium.
Cystidia and cystidioles absent. Lyocystidia projecting, thick-walled, with a globose tip, some of the globose tips are thin-walled, 38.0–71.0 × 8.3–10.0 µm. Basidia barred, colorless, thin-walled, with four sterigmata, 9.5–14.0 × 4.0–5.0 µm; basidioles in shape similar to basidia, but slightly smaller.
Basidiospores.
Cylindrical to allantoid, colorless, thin-walled, smooth, with one or two guttate, IKI –, CB –, (3.5 –) 4.0–6.0 (– 6.5) × 1.5–2.2 (– 2.5) µm, L = 5.09 µm, W = 1.89 µm, Q = 2.55–2.77 (n = 60 / 2).
Additional specimens examined (Paratype).
China • Qujing, Qilin District, Cuishan Forest Park, on a fallen angiosperm branch, 5 November 2022, CLZhao 26330 (SWFC).
description: Published as part of Dai, Yunfei, Yuan, Qi, Yang, Xin, Liu, Rui, Liu, Defu, Yuan, Haisheng & Zhao, Changlin, 2025, Morphological characteristics and phylogenetic analyses reveal five new species of Hymenochaetales (Agaricomycetes, Basidiomycota) from southwestern China, pp. 133-175 in MycoKeys 114 on pages 133-175, DOI: 10.3897/mycokeys.114.143851
Boundary triplets, tensor products and point contacts to reservoirs
Creators: name: Boitsev, A. A.
name: Brasche, J. F.
name: Malamud, M. M.
name: Neidhardt, H.
name: Popov, I. Yu.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Functional Analysis (math.FA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We consider symmetric operators of the form $S := A\otimes I_{\mathfrak T} + I_{\mathfrak H} \otimes T$ where $A$ is symmetric and $T = T^*$ is (in general) unbounded. Such operators naturally arise in problems of simulating point contacts to reservoirs. We construct a boundary triplet $Π_S$ for $S^*$ preserving the tensor structure. The corresponding $γ$-field and Weyl function are expressed by means of the $γ$-field and Weyl function corresponding to the boundary triplet $Π_A$ for $A^*$ and the spectral measure of $T$. Applications to 1-D Schrödinger and Dirac operators are given. A model of electron transport through a quantum dot assisted by cavity photons is proposed. In this model the boundary operator is chosen to be the well-known Jaynes-Cumming operator which is regarded as the Hamiltonian of the quantum dot.
Upper limits on the prevalence of Dyson spheres in the Milky Way
Creators: name: Suazo, Matías
Publisher: name: Zenodo
Year: 2021

description: Dyson spheres are hypothetical structures that high-level civilizations may have built up to harvest the energy of their host star. As in any thermodynamic process, the conversion of stellar energy would involve the emission of waste heat that would be emitted as infrared radiation. If we picture a Dyson sphere as a swarm of smaller satellites collecting the energy from its host star, a broad family of partial Dyson spheres with different covering factors seems plausible. At the same time, these partial Dyson spheres would block some of their host stellar light, leading to a drop in their optical fluxes. Nowadays, we count on missions that have mapped the sky in the optical as well as in the mid-infrared, specifically Gaia and WISE. Both together provide magnitude measurements for roughly 10^7 - 10^8 stars in the galaxy and can recover the two signatures mentioned above. Using this data we estimate how many stars are compatible with Dyson spheres based on Dyson sphere models with temperature ranges between 100-1000 K. In this work, we identify four different scenarios: transparent Dyson spheres, Cool Dyson spheres, intermediate states, and perfect cases.
description: The 2021 Assembly of the Order of the Octopus - Participant Talks - Session IV: Stars & Megastructures
A Model of Quantum Space-Time Symmetry in Two Dimensions
Creators: name: Smolinski, Kordian Andrzej
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: An example of a toy model of $D=2$ Minkowski space and Poincaré group with real deformation parameter $q$ is considered. A notion of free motion is defined. The kinematics and phase-space are constructed and the ``uncertainity'' ralations are found.
description: LaTeX (A4), 13pp, KFT UL 6/93
Additional file 1 of Joint association of sedentary behavior and physical activity with pulmonary function
Creators: name: Wang, Yiwen
name: Xie, Yujie
name: Chen, Yan
name: Ding, Guodong
name: Zhang, Yongjun
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Supplementary Material 1.
Xylodon musicola Y. F. Dai & C. L. Zhao 2025, sp. nov.
Creators: name: Dai, Yunfei
name: Yuan, Qi
name: Yang, Xin
name: Liu, Rui
name: Liu, Defu
name: Yuan, Haisheng
name: Zhao, Changlin
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Fungi
Basidiomycota
Agaricomycetes
Hymenochaetales
Schizoporaceae
Xylodon
Xylodon musicola

description: Xylodon musicola Y. F. Dai & C. L. Zhao sp. nov.
Figs 14, 15
Holotype.
China • Yunnan Province, Zhaotong, Yongshan County, Mugan Town, Wumengshan Nature Reserve, GPS coordinates 28°05′N, 103°58′E, evel. 2200 m a. s. l., on a fallen angiosperm branch, leg. C. L. Zhao, 7 November 2023, CLZhao 35567 (SWFC).
Etymology.
musicola (Lat.), refers to the growth on the mosses, which is located Bryophyta.
Basidiomata.
Annual, resupinate, adnate, very difficult to separate from substrate, without odor or taste when fresh, up to 7 cm long, 2 cm wide, and 150 µm thick. Hymenial surface arachnoid, white when fresh and becoming white to cream when drying. Sterile margin narrow, slightly cream, up to 1 mm wide. The basidiomata grow on the surface of muscus.
Hyphal system.
Monomitic, generative hyphae with clamp connections, colorless, thin to slightly thick-walled, rarely branched, interwoven, 2.5–4.0 µm in diam, IKI –, CB –; tissues unchanged in KOH.
Hymenium.
Cystidia capitate, thin-walled, smooth, slightly constricted at the neck, with a globose tip, 12.5–20.0 × 3.5–5.0 µm; cystidioles absent. Basidia clavate, colorless, thin-walled, with four sterigmata, 11.0–15.5 × 3.5–5.0 µm; basidioles in shape similar to basidia, but slightly smaller.
Basidiospores.
Broadly ellipsoid to globe, colorless, thin-walled, smooth, with one guttate, IKI –, CB –, 4.0–5.5 (– 6.0) × 3.5–5.0 (– 5.5) µm, L = 4.77 µm, W = 4.35 µm, Q = 1.07–1.13 (n = 60 / 2).
Additional specimens examined (Paratype).
China • Yunnan Province, Zhaotong, Yongshan County, Mugan Town, Wumengshan Nature Reserve, on a fallen angiosperm branch, 7 November 2023, CLZhao 40298 (SWFC).
description: Published as part of Dai, Yunfei, Yuan, Qi, Yang, Xin, Liu, Rui, Liu, Defu, Yuan, Haisheng & Zhao, Changlin, 2025, Morphological characteristics and phylogenetic analyses reveal five new species of Hymenochaetales (Agaricomycetes, Basidiomycota) from southwestern China, pp. 133-175 in MycoKeys 114 on pages 133-175, DOI: 10.3897/mycokeys.114.143851
Algebraic Heun operator and band-time limiting
Creators: name: Grünbaum, F. Alberto
name: Vinet, Luc
name: Zhedanov, Alexei
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 33C45, 47E99, 65R20, 94A11

description: We introduce the algebraic Heun operator associated to any bispectral pair of operators. We show that these operators are natural generalizations of the ordinary Heun operator. This leads to a simple construction of the operators commuting with the projection operators in problems of band-time limiting and it gives a way to adapt a construction first used by Perline in a purely finite setup to quite a few other situations. We also extend his algebraic construction to cover some purely finite cases where his proposal fails to give a useful commuting operator.
description: 27 pages
Levitated droplet dye laser
Creators: name: Azzouz, H.
name: Alkhafadiji, L.
name: Balslev, S.
name: Johansson, J.
name: Mortensen, N. A.
name: Nilsson, S.
name: Kristensen, A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present the first observation, to our knowledge, of lasing from a levitated, dye droplet. The levitated droplets are created by computer controlled pico-liter dispensing into one of the nodes of a standing ultrasonic wave (100 kHz), where the droplet is trapped. The free hanging droplet forms a high quality optical resonator. Our 750 nL lasing droplets consist of Rhodamine 6G dissolved in ethylene glycol, at a concentration of 0.02 M. The droplets are optically pumped at 532 nm light from a pulsed, frequency doubled Nd:YAG laser, and the dye laser emission is analyzed by a fixed grating spectrometer. With this setup we have achieved reproducible lasing spectra in the visible wavelength range from 610 nm to 650 nm. The levitated droplet technique has previously successfully been applied for a variety of bio-analytical applications at single cell level. In combination with the lasing droplets, the capability of this high precision setup has potential applications within highly sensitive intra-cavity absorbance detection.
description: 6 pages including 3 figures
Observations of Lyman-alpha Absorption in a Triple Quasar System
Creators: name: Young, P. A.
name: Impey, C. D.
name: Foltz, C. B.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained follow-up observations of the quasar pair LBQS 0107-025A,B and new observations of the nearby quasar LBQS 0107-0232 with the Hubble Space Telescope Faint Object Spectrograph. Extended wavelength coverage of LBQS 0107-025A and B using the G270H grating was also obtained. This triple system is unique in providing sensitivity to coherent Ly-alpha absorption on transverse scales of approximately 1 Mpc at z < 1. Monte Carlo simulations were used to establish the confidence level for matches between absorption features in different lines of sight as a function of velocity separation. Pairwise, there are 8, 9, and 12 lines that match between spectra. Three instances of matches between all three lines of sight were found with velocity separations of less than 550 kms^-1. Two of the pairings have coincident lines within |Delta v| < 200 kms^-1 that would occur with less than 10% probability by chance. Taking into account the equivalent widths of the lines, one of these triple coincidences is significant at the 99.99% confidence level, based on Monte Carlo simulations with random line placements. Matches with strong lines preferentially have small velocity separations. These same simulations are used to demonstrate that the distribution of matches for a population of absorbers randomly distributed in velocity space is peaked toward |Delta v| = 0, which has implications for the statistical significance of matches. One of the triple coincidences appears to be a strong absorber with a sheet-like, but inhomogeneous, geometry and a coherence length approaching or exceeding 1 Mpc.
description: 23 pages, 9 figures, accepted for publication in the Astrophysical Journal
Additional file 1: of mRNA-seq whole transcriptome profiling of fresh frozen versus archived fixed tissues
Creators: name: Ben-Moshe, Noa Bossel
name: Gilad, Shlomit
name: Perry, Gili
name: Benjamin, Sima
name: Balint-Lahat, Nora
name: Pavlovsky, Anya
name: Halperin, Sharon
name: Markus, Barak
name: Yosepovich, Ady
name: Barshack, Iris
name: Gal-Yam, Einav
name: Domany, Eytan
name: Kaufman, Bella
name: Dadiani, Maya
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Table S1. RNA integrity number for all samples. (PDF 212Â kb)
The Future May Be Sooner Than You Think
Creators: name: Ajeya Cotra
Publisher: name: Zenodo
Year: 2021

description: A lot of people picture a distant future that looks like Star Trek -- after hundreds of years of further scientific and technological R&D, humanity may have better health and life spans of well over a century, and may have spread across the solar system or perhaps to other stars by the 23rd century. But I think there are actually good reasons to think a spacefaring future could be both a lot sooner and a lot wilder than Star Trek implies, because I think there's a good chance that we could automate the process of science enough to fit centuries of R&D into decades instead.
description: The 2021 Assembly of the Order of the Octopus - Invited Talk
title: 02_1102
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Finding an Effective Classification Technique to Develop a Software Team Composition Model
Creators: name: Gilal, Abdul Rehman
name: Jaafar, Jafreezal
name: Capretz, Luiz Fernando
name: Omar, Mazni
name: Aziz, Izzatdin Abdul
Publisher: name: arXiv
Year: 2017
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Ineffective software team composition has become recognized as a prominent aspect of software project failures. Reports from results extracted from different theoretical personality models have produced contradicting fits, validity challenges, and missing guidance during software development personnel selection. It is also believed that the technique/s used while developing a model can impact the overall results. Thus, this study aims to: 1) discover an effective classification technique to solve the problem, and 2) develop a model for composition of the software development team. The model developed was composed of three predictors: team role, personality types, and gender variables; it also contained one outcome: team performance variable. The techniques used for model development were logistic regression, decision tree, and Rough Sets Theory (RST). Higher prediction accuracy and reduced pattern complexity were the two parameters for selecting the effective technique. Based on the results, the Johnson Algorithm (JA) of RST appeared to be an effective technique for a team composition model. The study has proposed a set of 24 decision rules for finding effective team members. These rules involve gender classification to highlight the appropriate personality profile for software developers. In the end, this study concludes that selecting an appropriate classification technique is one of the most important factors in developing effective models.
description: 12 pages
Dynamics of a broad-band Quantum Cascade Laser. From chaos to coherent dynamics and mode-locking
Creators: name: Columbo, L. L.
name: Barbieri, S.
name: Sirtori, C.
name: Brambilla, M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The dynamics of a multimode Quantum Cascade Laser, is studied in a model based on effective semiconductor Maxwell-Bloch equations, encompassing key features for the radiationmedium interaction such as an asymmetric, frequency dependent, gain and refractive index as well as the phase-amplitude coupling provided by the Henry factor. By considering the role of the free spectral range and Henry factor, we develop criteria suitable to identify the conditions which allow to destabilize, close to threshold, the traveling wave emitted by the laser and lead to chaotic or regular multimode dynamics. In the latter case our simulations show that the field oscillations are associated to self-confined structures which travel along the laser cavity, bridging mode-locking and solitary wave propagation. In addition, we show how a RF modulation of the bias current leads to active mode-locking yielding high-contrast, picosecond pulses. Our results compare well with recent experiments on broad-band THz-QCLs and may help understanding the conditions for the generation of ultrashort pulses and comb operation in Mid-IR and THz spectral regions
Perturbation of the Ground Varieties of C = 1 String Theory
Creators: name: Ghoshal, Debashis
name: Lakdawala, Porus
name: Mukhi, Sunil
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the effect of perturbations on the ground rings of $c=1$ string theory at the various compactification radii defining the $A_N$ points of the moduli space. We argue that perturbations by plus-type moduli define ground varieties which are equivalent to the unperturbed ones under redefinitions of the coordinates and hence cannot smoothen the singularity. Perturbations by the minus-type moduli, on the other hand, lead to semi-universal deformations of the singular varieties that can smoothen the singularity under certain conditions. To first order, the cosmological perturbation by itself can remove the singularity only at the self-dual ($A_1$) point.}
description: 15 pages, TIFR/TH/93-36, phyzzx macro.(A clarification added in Introduction, and a few references added)
Additional file 3: of Mental models of audit and feedback in primary care settings
Creators: name: Hysong, Sylvia
name: Smitham, Kristen
name: SoRelle, Richard
name: Amspoker, Amber
name: Hughes, Ashley
name: Haidet, Paul
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Example site summary. (DOCX 19Â kb)
Stellar Gravitational Lens Engineering for Interstellar Communication and Artifact SETI
Creators: name: Kerby, Steve
Publisher: name: Zenodo
Year: 2021

description: Several recent works have proposed "stellar relay" transmission system over interstellar distances, in which a transmitting spacecraft at the focus of a star’s gravitational lens achieves dramatic boosts in the gain of the outgoing beam. We examine some of the engineering requirements of a stellar relay system, evaluate the long-term sustainability of a gravitational relay, and describe the perturbations and drifts that must be actively countered to maintain a relay-star-target alignment. Our analysis is applicable to many of the myriad uses of a stellar gravitational lens, several of which have artifact SETI applications. We discuss at length the prospects for an artifact SETI search to observe stellar relays placed around the Sun by an extraterrestrial intelligence, and we suggest certain nearby stars that are relatively unperturbed by planetary systems as favorable nodes for such a stellar relay communications system.
description: The 2021 Assembly of the Order of the Octopus - Participant Talks - Session III: Communication SETI
Pathways of activated escape in periodically modulated systems
Creators: name: Ryvkine, D.
name: Dykman, M. I.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate dynamics of activated escape in periodically modulated systems. The trajectories followed in escape form diffusion broadened tubes, which are periodically repeated in time. We show that these tubes can be directly observed and find their shape. Quantitatively, the tubes are characterized by the distribution of trajectories that, after escape, pass through a given point in phase space for a given modulation phase. This distribution may display several peaks separated by the modulation period. Analytical results agree with the results of simulations of a model Brownian particle in a modulated potential.