cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
Creators: name: Kummer, F.
name: Toonen, S.
name: Dorozsmai, A.
name: Grishin, E.
name: de Koter, A.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Triple stars are prevalent within the population of observed stars. Their evolution, compared to binaries, is notably more complex, influenced by unique dynamical, tidal, and mass transfer processes. Understanding these phenomena is essential for a comprehensive insight into multistar evolution and the formation of energetic transients, including gravitational-wave mergers. Our study probes the evolution of triple star systems when the tertiary fills its Roche lobe and transfers mass to the inner binary, potentially forming GW sources with distinct properties. We develop an analytical model for hierarchical triples undergoing stable mass transfer from the tertiary. Using population synthesis simulations, we investigate triples with a Roche-lobe filling tertiary and an inner binary black hole. These systems originate from inner binaries undergoing chemically homogeneous evolution. Our analysis includes populations with metallicities of Z=0.005 and Z=0.0005, focusing on primary components with initial masses of 20 to 100 M_sun, and inner and outer orbital separations up to 40 R_sun and 10^5 R_sun, respectively. Our results show that mass transfer predominantly leads to orbital shrinkage of the inner binary, non-zero eccentricities, and expansion of the outer orbit. Among systems with CHE inner binaries, 9.5% result in mass transfer from the tertiary onto an inner BBH. We predict high formation efficiency of GW mergers, ranging from 85.1% to 100% at Z=0.005 and 100% at Z=0.0005, with short delay times. Local merger rates are projected to be between 0.69 to 1.74 Gpc^-3 yr^-1. A fraction of these BBH mergers, entering the LISA and aLIGO frequency bands, may still be accreting gas, potentially producing a strong electromagnetic counterpart. EM signals vary significantly based on model assumptions, ranging from less than 0.03% to 46.8% of all mergers if circumbinary disk formation is allowed.
description: 24 pages, 10 figures
Lecithocera macrotoma Meyrick 1934
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera macrotoma

description: Lecithocera macrotoma Meyrick, 1934
Lecithocera macrotoma Meyrick, 1934: 36. TL: China (Guangdong).The type depository of the species can not be found.
Distribution
China (Guangdong).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 62, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
Orbatina Ruckes 1961
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Orbatina

description: Orbatina Ruckes, 1961
The genus can be recognized by having the humeral angles subacute, produced laterad of the hemelytra by a distance subequal to one-half of the width of an eye, the labium is inserted before of the imaginary plane bisecting the head at anterior margin of the eyes and reaching the abdominal sternite V, the labial segment II reaching the mesocoxae, the antennae is five segmented, the antennal segment I surpassing the apex of the head, the clypeus and mandibular plates subequal in length, and the elevated margin of each evaporative area is sigmoid (Rolston 1992).
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 29, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
Many-body tunneling in a double-well potential
Creators: name: Zendra, Matteo
name: Borgonovi, Fausto
name: Celardo, Giuseppe Luca
name: Gurvitz, Shmuel
Publisher: name: arXiv
Year: 2024
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an approach for evaluating Wannier functions, offering an alternative perspective on their role in many-body systems. Unlike traditional methods, such as the maximally localized Wannier functions approach, which focuses on minimizing the function tails, our approach emphasizes these tails. Using perturbative analytical approximations and extensive numerical simulations on an exactly solvable model, we address nonstandard Hubbard terms and demonstrate their critical influence on many-body dynamics. Specifically, we study tunneling dynamics in arbitrary double-well potentials, moving beyond the standard Hubbard model to include nonstandard terms such as density-induced tunneling and pair tunneling. Our results reveal that these terms significantly modify the dynamics predicted by the standard Hubbard model: density-induced tunneling modifies the single-particle tunneling parameter $Ω_0$, while pair tunneling enables coherent propagation not captured by the standard model. We show that the discrepancies between the standard and nonstandard Hubbard models grow with increasing interaction strength, potentially leading to novel transport behaviors. However, at lower interaction strengths, both models converge, as nonstandard terms become negligible. These findings have important implications for phenomena such as superconductivity in twisted bilayer graphene and metal-insulator transitions. Our model aligns well with numerical simulations of lowest-band parameters and is strongly supported by experimental observations of second-order atom tunneling in optical double-well potentials. This strong agreement with experimental data highlights the accuracy and potential of our approach in providing a more comprehensive framework for describing complex many-body systems than the standard Hubbard model.
description: 29 pages, 16 figures
Spilogona arenosa
Creators: name: Sorokina, Vеra S.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Spilogona
Spilogona arenosa

description: Spilogona arenosa (Ringdahl, 1918)
Material examined. Altai Republic: Kosh-Agach district: 3 mаles аnd 2 femаles, Ukоk рlаteаu, vаlleу оf Ak- Allасhа River, оn stоnes neаr the wаter, 2075 m, 49°39'N 88°1'Е, 12.vii.2009, leg. V. Sоrоkinа; 1 mаle, Severо- Chuуskуi Ridge, vаlleу оf Aktru River, 2064 m, 50°06'N 87°48'Е, 21.vii.2013, leg. V. Sоrоkinа.
Remarks. New reсоrd frоm the Altаi. The first reсоrd frоm Russiа wаs frоm Wrаngel Islаnd (Sоrоkinа & Khrulevа 2012).
description: Published as part of Sorokina, Vеra S., 2018, Eleven new species of Spilogona Schnabl, 1911 (Diptera, Muscidae) from the Altai Mountains of Russia, with key to species, pp. 201-250 in Zootaxa 4410 (2) on page 235, DOI: 10.11646/zootaxa.4410.2.1, http://zenodo.org/record/1221458
Additional file 3: of Comprehensive benchmarking and ensemble approaches for metagenomic classifiers
Creators: name: McIntyre, Alexa
name: Ounit, Rachid
name: Afshinnekoo, Ebrahim
name: Prill, Robert
name: HĂŠnaff, Elizabeth
name: Alexander, Noah
name: Minot, Samuel
name: Danko, David
name: Foox, Jonathan
name: Ahsanuddin, Sofia
name: Tighe, Scott
name: Hasan, Nur
name: Poorani Subramanian
name: Moffat, Kelly
name: Levy, Shawn
name: Lonardi, Stefano
name: Greenfield, Nick
name: Colwell, Rita
name: Rosen, Gail
name: Mason, Christopher
Publisher: name: Figshare
Year: 2017
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Supplementary figures. (PDF 496 kb)
The cosmological analysis of X-ray cluster surveys: VI. Inference based on analytically simulated observable diagrams
Creators: name: Kosiba, M.
name: Cerardi, N.
name: Pierre, M.
name: Lanusse, F.
name: Garrel, C.
name: Werner, N.
name: Shalak, M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The number density of galaxy clusters across mass and redshift has been established as a powerful cosmological probe. Cosmological analyses with galaxy clusters traditionally employ scaling relations. However, many challenges arise from this approach as the scaling relations are highly scattered, may be ill-calibrated, depend on the cosmology, and contain many nuisance parameters with low physical significance. In this paper, we use a simulation-based inference method utilizing artificial neural networks to optimally extract cosmological information from a shallow X-ray survey of galaxy clusters, solely using count rates (CR), hardness ratios (HR), and redshifts. This procedure enables us to conduct likelihood-free inference of cosmological parameters $Ω_{\mathrm{m}}$ and $σ_8$. We analytically generate simulations of galaxy cluster distribution in a CR, HR space in multiple redshift bins based on totally random combinations of cosmological and scaling relation parameters. We train Convolutional Neural Networks (CNNs) to retrieve the cosmological parameters from these simulations. We then use neural density estimation (NDE) neural networks to predict the posterior probability distribution of $Ω_{\mathrm{m}}$ and $σ_8$ given an input galaxy cluster sample. The 1 $σ$ errors of our density estimator on one of the target testing simulations are 1000 deg$^2$: 15.2% for $Ω_{\mathrm{m}}$ and 10.0% for $σ_8$; 10000 deg$^2$: 9.6% for $Ω_{\mathrm{m}}$ and 5.6% for $σ_8$. We also compare our results with Fisher analysis. We demonstrate, as a proof of concept, that it is possible to calculate cosmological predictions of $Ω_{\mathrm{m}}$ and $σ_8$ from a galaxy cluster population without explicitly computing cluster masses and even, the scaling relation coefficients, thus avoiding potential biases resulting from such a procedure. [abridged]
description: 14 pages, 4 tables, 15 figures, accepted for publication in A&A - pre-proofs version
title: On hardness of some Boolean counting CSPs
Creators: name: Behrisch, Mike
name: Hermann, Miki
Publisher: name: TU Wien
Year: 2021
Subjects: counting complexity
#ETH
#CSP
counting problems
weak base
strong partial clone
restriction-closed partial clone
partial polymorphism
reductions

description: We relate #ETH to the hardness of certain counting CSPs over Boolean constraint languages with the aim of characterising #ETH. For this we rely on the theory of weak bases as established by Schnoor and Schnoor based on the Galois theory for strong partial clones by Romov. Moreover, we exploit and extend results of Lagerkvist describing certain irredundant weak bases in the Boolean case.
Lecithocera manesa Wu & Liu 1992
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera manesa

description: Lecithocera manesa Wu & Liu, 1992
Lecithocera manesa Wu & Liu in Peng & Liu, 1992: 678. TL: China (Sichuan). TD: IZCAS.
Distribution
China (Hunan, Sichuan).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 62, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
The Intrinsic Flattening of Galaxy Disks
Creators: name: Favaro, Jeremy
name: Courteau, Stéphane
name: Comerón, Sébastien
name: Stone, Connor
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Highly inclined (edge-on) disk galaxies offer the unique perspective to constrain their intrinsic flattening, $c/a$, where $c$ and $a$ are respectively the vertical and long radial axes of the disk measured at suitable stellar densities. The ratio $c/a$ is a necessary quantity in the assessment of galaxy inclinations, three-dimensional structural reconstructions, total masses, as well as a constraint to galaxy formation models. 3.6 micron maps of 133 edge-on spiral galaxies from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and its early-type galaxy extension are used to revisit the assessment of $c/a$ free from dust extinction and away from the influence of a stellar bulge. We present a simple definition of $c/a$ and explore trends with other galactic physical parameters: total stellar mass, concentration index, total HI mass, mass of the central mass concentration, circular velocity, model-dependent scales, as well as Hubble type. Other than a dependence on early/late Hubble types, and a related trend with light concentration, no other parameters were found to correlate with the intrinsic flattening of spiral galaxies. The latter is mostly constant with $\langle c/a \rangle$ = 0.124 $\pm$ 0.001 (stat) $\pm$ 0.033 (intrinsic/systematic) and greater for earlier types.
description: 27 full pages, 15 figures, 6 tables, 1 appendix. Published in ApJ
Orbatina fuliginia Ruckes 1961
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Orbatina
Orbatina fuliginia

description: Orbatina fuliginia Ruckes, 1961 [Fig. 41]
Distribution. Panama, Colombia, and Bolivia.
Distribution in Colombia. Unknown. This species was recorded for Colombia by Rolston (1992), but without specific locality.
Remarks. Orbatina is a monotypic genus.
References. Rolston 1992.
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 29, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
Thermodynamic and observational constraints on black holes with primary hair in Beyond Horndeski Gravity: Stability and shadows
Creators: name: Erices, Cristian
name: Fathi, Mohsen
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 Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper, we find that unlike in General Relativity, the shift-symmetric subclass of Beyond Horndeski theories permits black holes with primary hair that are thermodynamically stable and align with current Event Horizon Telescope observations of the M87* and Sgr A* black holes. This work begins by investigating thermodynamic properties, analyzing how primary hair influences thermodynamic quantities and local stability, which imposes strict constraints on the allowed range of primary hair values. The null geodesics near this black hole are then examined, demonstrating how scalar hair affects the shadow diameter. Specifically, when the parameter of the Beyond Horndeski function $F_4$ is negative, increasing scalar hair enlarges the shadow; in contrast, when this parameter is positive, greater scalar hair reduces the shadow size. Further constraints on the scalar hair are derived using observational data, highlighting its sensitivity to other black hole parameters. To explore additional observational features, face-on two-dimensional images of spherically infalling accretion disks are simulated, revealing how primary scalar hair shapes the black hole's shadow. Finally, all relevant constraints are combined to identify black holes that are both stable and consistent with observational data.
description: 16 pages, 12 figures, 1 table
Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
Creators: name: Lyskova, N.
name: Churazov, E.
name: Khabibullin, I.
name: Bikmaev, I. F.
name: Burenin, R. A.
name: Forman, W. R.
name: Khamitov, I. M.
name: Rajpurohit, K.
name: Sunyaev, R.
name: Jones, C.
name: Kraft, R.
name: Zaznobin, I.
name: Gorbachev, M. A.
name: Suslikov, M. V.
name: Gumerov, R. I.
name: Sakhibullin, N. A.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Massive clusters of galaxies are very rare in the observable Universe. Even rarer are mergers of such clusters observed close to pericenter passage. Here, we report on one such case: a massive (~ $10^{15}\,M_\odot$) and hot (kT ~ 10 keV) cluster CL0238.3+2005 at $z\approx 0.42$. For this cluster, we combine X-ray data from SRG/eROSITA and Chandra, optical images from DESI, and spectroscopy from BTA and RTT-150 telescopes. The X-ray and optical morphologies suggest an ongoing merger with the projected separation of subhalos of $\sim 200$ kpc. The line-of-sight velocity of galaxies tentatively associated with the two merging halos differs by 2000-3000 km/s. We conclude that, most plausibly, the merger axis is neither close to the line of sight nor to the sky plane. We compare CL0238 with two well-known clusters MACS0416 and Bullet, and conclude that CL0238 corresponds to an intermediate phase between the pre-merging MACS0416 cluster and the post-merger Bullet cluster. Namely, this cluster has recently (only $\lesssim 0.1$ Gyr ago) experienced an almost head-on merger. We argue that this "just after" system is a very rare case and an excellent target for lensing, Sunyaev-Zeldovich effect, and X-ray studies that can constrain properties ranging from dynamics of mergers to self-interacting dark matter, and plasma effects in intracluster medium that are associated with shock waves, e.g., electron-ion equilibration efficiency and relativistic particle acceleration.
description: submitted to A&A; comments are welcome
Lecithocera margirecta Yu & Wang 2024, sp. nov.
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera margirecta

description: Lecithocera margirecta sp. nov.
TL: China (Guizhou). TD: NKU.
Distribution
China (Guangxi, Guizhou, Hunan).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 62, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
Edge-Wise Graph-Instructed Neural Networks
Creators: name: Della Santa, Francesco
name: Mastropietro, Antonio
name: Pieraccini, Sandra
name: Vaccarino, Francesco
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: Numerical Analysis (math.NA)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: 05C21, 65D15, 68T07, 90C35

description: The problem of multi-task regression over graph nodes has been recently approached through Graph-Instructed Neural Network (GINN), which is a promising architecture belonging to the subset of message-passing graph neural networks. In this work, we discuss the limitations of the Graph-Instructed (GI) layer, and we formalize a novel edge-wise GI (EWGI) layer. We discuss the advantages of the EWGI layer and we provide numerical evidence that EWGINNs perform better than GINNs over some graph-structured input data, like the ones inferred from the Barabasi-Albert graph, and improve the training regularization on graphs with chaotic connectivity, like the ones inferred from the Erdos-Renyi graph.
Lecithocera medogensis Yu & Wang 2024, sp. nov.
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera medogensis

description: Lecithocera medogensis sp. nov.
TL: China (Xizang [Tibet]). TD: NKU.
Distribution
China (Xizang [Tibet]).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 63, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
Additional file 1 of A two-step framework for inferring direct protein-protein interaction network from AP-MS data
Creators: name: Tian, Bo
name: Zhao, Can
name: Feiyang Gu
name: Zengyou He
Publisher: name: Figshare
Year: 2017
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Supplementary Tables. This file provides the supplementary tables (Tables S1â  S24) that illustrate why significant improvements are observed when some scoring methods are used in the first phase. We present the top-10 ranked PPIs detected from three data sets after the refinement procedure. Meanwhile, we also record the initial ranks of these top-10 ranked PPIs in these tables. Note that we list more than 10 PPIs in some tables such as Table S3 and Table S5 because there are top-k ranked PPIs (k >10) that have the same ranking score. (PDF 67 kb)
Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
Creators: name: Liu, Kexin
name: Guo, Hong
name: Wang, Sen
name: Xu, Dandan
name: Lu, Shengdong
name: Cui, Weiguang
name: Dav'e, Romeel
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this study, we examine the role of circumgalactic medium (CGM) angular momentum ($j_{\rm CGM}$) on star formation in galaxies, whose influence is currently not well understood. The analysis utilises central galaxies from two hydrodynamical simulations, SIMBA and IllustrisTNG. We observe a substantial divergence in how star formation rates correlate with CGM angular momentum between the two simulations. Specifically, quenched galaxies in IllustrisTNG show high $j_{\rm CGM}$, while in SIMBA, quenched galaxies have low $j_{\rm CGM}$. This difference is attributed to the distinct active galactic nucleus (AGN) feedback mechanisms active in each simulation. Moreover, both simulations demonstrate similar correlations between $j_{\rm CGM}$ and environmental angular momentum ($j_{\rm Env}$) in star-forming galaxies, but these correlations change notably when kinetic AGN feedback is present. In IllustrisTNG, quenched galaxies consistently show higher $j_{\rm CGM}$ compared to their star-forming counterparts with the same $j_{\rm Env}$, a trend not seen in SIMBA. Examining different AGN feedback models in SIMBA, we further confirm that AGN feedback significantly influences the CGM gas distribution, although the relationship between the cold gas fraction and the star formation rate (SFR) remains largely stable across different feedback scenarios.
description: Accepted by A&A
Paralincus Distant 1911
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Paralincus

description: Paralincus Distant, 1911
The genus can be recognized by having the inferior surface of the pro- and mesofemur armed distally with small peg-like tubercles, these reduced or absent on the metafemur, and the space between the eye and the pronotum about 0.5 times of the diameter of an eye (Ruckes 1958; Rolston 1983c).
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 29, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
Micropolar elastoplasticity using a fast Fourier transform-based solver
Creators: name: Francis, Noah M.
name: Lebensohn, Ricardo A.
name: Pourahmadian, Fatemeh
name: Dingreville, Rémi
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computational Engineering, Finance, and Science (cs.CE)
subject: FOS: Computer and information sciences

description: This work presents a micromechanical spectral formulation for obtaining the full-field and homogenized response of elastoplastic micropolar composites. A closed-form radial-return mapping is derived from thermodynamics-based micropolar elastoplastic constitutive equations to determine the increment of plastic strain necessary to return the generalized stress state to the yield surface, and the algorithm implementation is verified using the method of numerically manufactured solutions. Then, size-dependent material response and micro-plasticity are shown as features that may be efficiently simulated in this micropolar elastoplastic framework. The computational efficiency of the formulation enables the generation of large datasets in reasonable computing times.
Lecithocera megalopis Meyrick 1916
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera megalopis

description: Lecithocera megalopis Meyrick, 1916
Lecithocera megalopis Meyrick, 1916: 575. TL: Philippines. TD: NHMUK.
Distribution
China (Jiangxi, Taiwan) (Wu & Liu 1993; Park 1999), Philippines.
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 63, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
Additional file 1 of A two-step framework for inferring direct protein-protein interaction network from AP-MS data
Creators: name: Tian, Bo
name: Zhao, Can
name: Feiyang Gu
name: Zengyou He
Publisher: name: Figshare
Year: 2017
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Mental Health

description: Supplementary Tables. This file provides the supplementary tables (Tables S1â  S24) that illustrate why significant improvements are observed when some scoring methods are used in the first phase. We present the top-10 ranked PPIs detected from three data sets after the refinement procedure. Meanwhile, we also record the initial ranks of these top-10 ranked PPIs in these tables. Note that we list more than 10 PPIs in some tables such as Table S3 and Table S5 because there are top-k ranked PPIs (k >10) that have the same ranking score. (PDF 67 kb)
Measurements of polarization and spin correlation and observation of entanglement in top quark pairs using lepton+jets events from proton-proton collisions at $\sqrt{s}$ = 13 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Measurements of the polarization and spin correlation in top quark pairs ($\mathrm{t\bar{t}}$) are presented using events with a single electron or muon and jets in the final state. The measurements are based on proton-proton collision data from the LHC at $\sqrt{s}$ = 13 TeV collected by the CMS experiment, corresponding to an integrated luminosity of 138 fb$^{-1}$. All coefficients of the polarization vectors and the spin correlation matrix are extracted simultaneously by performing a binned likelihood fit to the data. The measurement is performed inclusively and in bins of additional observables, such as the mass of the $\mathrm{t\bar{t}}$ system and the top quark scattering angle in the $\mathrm{t\bar{t}}$ rest frame. The measured polarization and spin correlation are in agreement with the standard model. From the measured spin correlation, conclusions on the $\mathrm{t\bar{t}}$ spin entanglement are drawn by applying the Peres-Horodecki criterion. The standard model predicts entangled spins for $\mathrm{t\bar{t}}$ states at the production threshold and at high masses of the $\mathrm{t\bar{t}}$ system. Entanglement is observed for the first time in events at high $\mathrm{t\bar{t}}$ mass, where a large fraction of the $\mathrm{t\bar{t}}$ decays are space-like separated, with an expected and observed significance of above 5 standard deviations.
description: Replaced with the published version. Added the journal reference and the DOI. All the figures and tables, including additional supplementary figures, can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/TOP-23-007 (CMS Public Pages)
Paralincus bimaculatus
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Paralincus
Paralincus bimaculatus

description: Paralincus bimaculatus (Ruckes, 1958) [Fig. 42]
Distribution. Colombia and Guyana.
Distribution in Colombia. Amazonas.
Remarks. Paralincus bimaculatus has the paramere laminate, and the antennal segments II, IV and V with equal length, longer than the antennal segment III.
References. Ruckes 1958; Rolston 1983c; Castro-Huertas et al. 2015.
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 29, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
Schraderiellus Rider 1998
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Schraderiellus

description: Schraderiellus Rider, 1998
The genus can be recognized by having an anteapical tooth on the lateral margins of each mandibular plate; the ventral rim of the pygophore is not visible in dorsal view, and its base of the posterolateral angles has a pair of projections with tuft of setae, and the posterolateral angles of the pygophore have a basal dorsal excavation (Roell & Campos 2018).
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 30, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
New interferometric aperture masking technique for full transverse beam characterization using synchrotron radiation
Creators: name: Iriso, Ubaldo
name: Torino, Laura
name: Carilli, Chris
name: Nikolic, Bojan
name: Thyagarajan, Nithyanandan
Publisher: name: arXiv
Year: 2024
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Emittance measurements using synchrotron radiation are usually performed using x-rays to avoid diffraction limits. Interferometric techniques using visible light are also used to measure either the horizontal or the vertical beam projection. Several measurements rotating the interferometry axis are needed to obtain a full beam reconstruction. In this report we present a new interferometric multi-aperture masking technique and data analysis, inspired by astronomical methods, that are able to provide a full 2-D transverse beam reconstruction in a single acquisition. Results of beam characterization obtained at ALBA synchrotron light source will also been shown.
description: 4 pages, 8 figures, Accepted in IBIC 2024
Lecithocera meishanensis Park 2018
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera meishanensis

description: Lecithocera meishanensis Park, 2018
Lecithocera meishanensis Park, 2018: 111. TL: China (Taiwan). TD: USNM.
Distribution
China (Taiwan).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 63, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
On the Gravitational Wave Counterpart to a Gamma-ray Galactic Center Signal from Millisecond Pulsars
Creators: name: Bartel, Kayla
name: Profumo, Stefano
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The new tools of gravitational wave and multi-messenger astronomy allow for the study of astrophysical phenomenon in new ways and enables light to be shed on some of the longest-enduring mysteries of high-energy astrophysics. Among the latter stands the Galactic center gamma-ray excess, associated with a source whose nature could be annihilating dark matter or a yet-unresolved population of millisecond pulsars (MSPs). MSPs are most likely asymmetric about their axis of rotation, and are thus thought to also source quasi-monochromatic gravitational waves, that dark matter processes would not emit. Using statistical methods, we simulate realistic MSP population samples with differing morphology and moment of inertia, that could give rise to the gamma-ray excess, and we compute the corresponding gravitational wave signal amplitude and frequency. We find that the gravitational wave signal frequency likely ranges between $\sim$200 and 1400 Hz, and that the collective dimensionless strain from the center of the Galaxy has an amplitude between $10^{-26}$ and $10^{-24}$, thus most likely beyond current and near-term detectors, unless the unresolved MSPs are extraordinarily gamma-ray dim.
description: 19 pages, 11 figures
ROBOTIC BIOMIMICRY: OCTOPUS-INSPIRED AUV SIMULATION AND DESIGN
Creators: name: Jianwei, Lei Zhang
name: Hui, Chen Li
name: Feng, Wei Liu
Publisher: name: kEITH jOURNAL
Year: 2025
Subjects: Ocean Exploration, Unmanned Underwater Vehicles (UUVs), Hydrogen Fuel Cells, Oceanic Resources, Underwater Environment

description: As the global population continues to expand, the consumption of land resources accelerates, prompting an intensified focus on alternative strategic spaces. The ocean, recognized as a major strategic frontier alongside terrestrial environments, boasts a wealth of untapped biological and mineral resources, harboring countless unexplored phenomena awaiting human investigation. A surge in ocean exploration and development efforts has transpired worldwide in recent years, driven by the realization of the ocean's vast potential.

The inherent challenges posed by the ocean's immense expanse and complex environment have spurred the emergence of Unmanned Underwater Vehicles (UUVs) as indispensable tools for oceanic exploration and exploitation. UUVs represent a class of equipment capable of navigating underwater, equipped with exploration capabilities and the capacity to execute underwater tasks, often leveraging mechanical arms for specific functions. Notably, UUVs possess the versatility to undertake a myriad of complex tasks, and recent advancements in hydrogen fuel cell technology and battery capacity have significantly bolstered their endurance.

This research explores the evolution and significance of UUVs in the context of ocean exploration. It delves into the multifaceted utility of UUVs in unlocking the ocean's mysteries, leveraging their adaptability to perform diverse tasks in challenging underwater environments. Moreover, the study addresses the pivotal role played by advancements in hydrogen fuel cells and battery technologies in extending UUVs' operational endurance. By providing an in-depth analysis of these developments, this research contributes to our understanding of the burgeoning importance of UUVs in advancing human exploration and exploitation of the ocean
Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
Creators: name: Spadaro, Alice
name: Buscicchio, Riccardo
name: Izquierdo-Villalba, David
name: Gerosa, Davide
name: Klein, Antoine
name: Pratten, Geraint
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Massive black-hole binaries will be the loudest sources detectable by LISA. These systems are predicted to form during the hierarchical assembly of cosmic structures and coalesce by interacting with the surrounding environment. The hardening phase of their orbit is driven by either stars or gas and encodes distinctive features into the binary black holes that can potentially be reconstructed with gravitational-wave observations. We present a Bayesian framework to assess the likelihood of massive mergers being hardened by either gaseous or stellar interactions. We use state-of-the-art astrophysical models tracking the cosmological evolution of massive black-hole binaries and construct a large number of simulated catalogs of sources detectable by LISA. From these, we select a representative catalog and run both parameter estimation assuming a realistic LISA response as well model comparison capturing selection effects. Our results suggest that, at least within the context of the adopted models, future LISA observations can confidently constrain whether stars or gas are responsible for the binary hardening. We stress that accurate astrophysical modeling of the black-hole spins and the inclusion of subdominant emission modes in the adopted signal might be crucial to avoid systematic biases.
description: 10 pages, 6 figures (accepted to Physical Review D on 2 December 2024)
Schraderiellus cinctus
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Schraderiellus
Schraderiellus cinctus

description: Schraderiellus cinctus (Ruckes, 1959) [Fig. 44]
Distribution. Nicaragua, Costa Rica, Panama, and Colombia.
Distribution in Colombia. Valle del Cauca.
Remarks. Schraderiellus cinctus is dark brown with the anterolateral margin of the pronotum, the anterolateral margin of hemelytra, and the lateral margin of the connexivum orange or yellowish.
References. Ruckes 1959 a; Castro-Huertas et al. 2015; Roell & Campos 2018.
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 30, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
A High-Resolution Spectroscopic Survey of Directly Imaged Companion Hosts: I. Determination of diagnostic stellar abundances for planet formation and composition
Creators: name: Baburaj, Aneesh
name: Konopacky, Quinn M.
name: Theissen, Christopher A.
name: Peacock, Sarah
name: Huseby, Lori
name: Fulton, Benjamin
name: Gerasimov, Roman
name: Barman, Travis S.
name: Hoch, Kielan K. W.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the first results of an extensive spectroscopic survey of directly imaged planet host stars. The goal of the survey is the measurement of stellar properties and abundances of 15 elements (including C, O, and S) in these stars. In this work, we present the analysis procedure and the results for an initial set of five host stars, including some very well-known systems. We obtain C/O ratios using a combination of spectral modeling and equivalent width measurements for all five stars. Our analysis indicates solar C/O ratios for HR 8799 (0.59 $\pm$ 0.11), 51 Eri (0.54 $\pm$ 0.14), HD 984 (0.63 $\pm$ 0.14), and GJ 504 (0.54 $\pm$ 0.14). However, we find a super-solar C/O (0.81 $\pm$ 0.14) for HD 206893 through spectral modeling. The ratios obtained using the equivalent width method agree with those obtained using spectral modeling but have higher uncertainties ($\sim$0.3 dex). We also calculate the C/S and O/S ratios, which will help us to better constrain planet formation, especially once planetary sulfur abundances are measured using JWST. Lastly, we find no evidence of highly elevated metallicities or abundances for any of our targets, suggesting that a super metal-rich environment is not a prerequisite for large, widely separated gas planet formation. The measurement of elemental abundances beyond carbon and oxygen also provides access to additional abundance ratios, such as Mg/Si, which could aid in further modeling of their giant companions.
description: 53 pages, 29 figures, 11 tables
Spilogona bomynensis Hennig 1959
Creators: name: Sorokina, Vеra S.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Spilogona
Spilogona bomynensis

description: Spilogona bomynensis Hennig, 1959
Material examined. Altai Republic: Ust-Koksa district: 1 femаle, 22 km SW Ust’ -Kоksа, “ Serebrуаnуi Ruсhei” 1572 m, 50°10'N 85°18'Е, 16.vii.2015, leg. V. Sоrоkinа.
Remarks. This reсоrd саn be соnsidered аs the first fоr the Altаi beсаuse the reсоrd in Sоrоkinа (2012а: 211) wаs а misidentifiсаtiоn оf S. deflorata (Hоlmgren) (see belоw).
Aссоrding tо Hennig’s desсriрtiоn (1959а: 280), the mаle рrоbоsсis оf this sрeсies hаs shining рrementum. I exаmined the tурe series оf Spilogona bomynensis (in ZISР) аnd соnсluded thаt the mаle рrоbоsсis оf this sрeсies hаs а subshining рrementum but is dusted сentrаllу оn the underside. One femаle раrаtурe is nоt Spilogona bomynensis beсаuse it hаs аneрisternum withоut intersраtiаl setаe, рrоbоsсis with shining рrementum, аnd hind femur with lоng роsterоventrаl setаe аt bаse. This femаle withоut аbdоmen аnd роstgenitаl рlаte соuld nоt be рreсiselу reсоgnized аt the sрeсies level.
This sрeсies is verу similаr tо Spilogona stackelbergi Hennig, 1959, esрeсiаllу the femаle, but the femаle саn be distinguished аs indiсаted in the keу.
The detаils оf the tурe lосаlitу оf Spilogona bomynensis: р Бомын (ИчЕгын) св Цаüдамъ, Гоби Роб Козлов кVI95 [= Qinghаi рrоv., NЕ Tsаidаm, Gоbi desert, Iсhegуn River, 38°00'N 96°48'Е, 3100 m аsl, V. Rоbоrоvskу, Р. Kоzlоv), end оf June 1895].
description: Published as part of Sorokina, Vеra S., 2018, Eleven new species of Spilogona Schnabl, 1911 (Diptera, Muscidae) from the Altai Mountains of Russia, with key to species, pp. 201-250 in Zootaxa 4410 (2) on page 236, DOI: 10.11646/zootaxa.4410.2.1, http://zenodo.org/record/1221458
Schraderiellus hughesae
Creators: name: Castro-Huertas, Valentina
name: Grazia, Jocelia
name: Forero, Dimitri
name: Fernández, Fernando
name: Schwertner, Cristiano F.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Schraderiellus
Schraderiellus hughesae

description: Schraderiellus hughesae (Ruckes, 1959)
Distribution. Costa Rica, Panama, and Colombia.
Distribution in Colombia. Valle del Cauca.
Remarks. Schraderiellus hughesae is dark brown with small yellow spots adjacent to the cicatrices on the pronotum, on the scutellum and hemelytra, and the anterolateral margin of the pronotum and hemelytra are dark brown or yellowish.
References. Roell & Campos 2018.
description: Published as part of Castro-Huertas, Valentina, Grazia, Jocelia, Forero, Dimitri, Fernández, Fernando & Schwertner, Cristiano F., 2022, Stink bugs (Hemiptera: Heteroptera: Pentatomidae) of Colombia: An annotated checklist of species, pp. 1-88 in Zootaxa 5097 (1) on page 30, DOI: 10.11646/zootaxa.5097.1.1, http://zenodo.org/record/6036639
Lecithocera melliflua Gozmany 1978
Creators: name: Yu, Shuai
name: Wang, Shuxia
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Lecithoceridae
Lecithocera
Lecithocera melliflua

description: Lecithocera melliflua Gozmány, 1978
Lecithocera melliflua Gozmány, 1978: 106. TL: China (Hunan). TD: NHMUK.
Distribution
China (Hubei, Hunan).
description: Published as part of Yu, Shuai & Wang, Shuxia, 2024, The genus Lecithocera (Lepidoptera: Lecithoceridae) from China, with descriptions of twenty-one new species, pp. 1-74 in European Journal of Taxonomy 924 on page 63, DOI: 10.5852/ejt.2024.924.2447, http://zenodo.org/record/10803382
Effective approaches to the dynamical properties of two distinguishable Bose polarons
Creators: name: Theel, F.
name: Mistakidis, S. I.
name: Schmelcher, P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We explore effective approaches for describing the dynamics of induced interactions amongst two non-interacting distinguishable impurities - Bose polarons - when their couplings to the host species are switched on. First, we evaluate the time-dependent characteristics of each polaron through reduced single-particle models. Their validity is ultimately judged by comparing to observables obtained within a many-body variational approach. We argue that utilizing a time-dependent optimization process with the effective mass and frequency being fitting parameters leads to an accurate matching on the level of one-body observables with the prediction of the many-body method. Next, we construct two-body effective models, which besides the effective parameters of the single polaron, include a contact interaction potential modelling the induced interactions. It is shown that the instantaneous coupling strength obtained with a time-dependent optimization process allows for an accurate description of the impurities two-body correlation dynamics when compared to the many-body calculations. In this sense, it is possible to describe the dynamical crossover from correlated to anti-correlated impurity patterns related to the transition from attractive to repulsive induced interactions. Our results should facilitate the description of strongly particle-imbalanced mixtures via reduced models and hence their experimental understanding.
description: 17 pages, 9 figures