cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Orbit-averaged Guiding-center Fokker-Planck Operator
Creators: name: Brizard, A. J.
name: Decker, J.
name: Peysson, Y.
name: Duthoit, F. -X.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A general orbit-averaged guiding-center Fokker-Planck operator suitable for the numerical analysis of transport processes in axisymmetric magnetized plasmas is presented. The orbit-averaged guiding-center operator describes transport processes in a three-dimensional guiding-center invariant space: the orbit-averaged magnetic-flux invariant $\ovψ$, the minimum-B pitch-angle coordinate $ξ_{0}$, and the momentum magnitude $p$.
description: 12 pages, accepted for publication in Physics of Plasmas
Additional file 1 of Genetic diversity of Plasmodium vivax populations from the China–Myanmar border identified by genotyping merozoite surface protein markers
Creators: name: Wang, Xun
name: Bai, Yao
name: Xiang, Zheng
name: Zeng, Weilin
name: Wu, Yanrui
name: Zhao, Hui
name: Zhao, Wei
name: Chen, Xi
name: Duan, Mengxi
name: Li, Xiaosong
name: Zhu, Wenya
name: Sun, Kemin
name: Wu, Yiman
name: Zhang, Yanmei
name: Li, Xiaomei
name: Rosenthal, Benjamin M.
name: Cui, Liwang
name: Yang, Zhaoqing
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Supplementary Tables.
A young white dwarf orbiting PSR J1835-3259B in the bulge globular cluster NGC 6652
Creators: name: Chen, J.
name: Cadelano, M.
name: Pallanca, C.
name: Ferraro, F.
name: Lanzoni, B.
name: Istrate, A.
name: Burgay, M.
name: Freire, P.
name: Gautam, T.
name: Possenti, A.
name: Ridolfi, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report on the discovery of the companion star to the millisecond pulsar PSR J1835-3259B in the Galactic globular cluster NGC 6652. Taking advantage of deep photometric archival observations acquired through the Hubble Space Telescope in near-ultraviolet and optical bands, we identified a bright and blue object at a position compatible with that of the radio pulsar. The companion is located along the helium-core white dwarf cooling sequence and the comparison with binary evolution models provides a mass of $0.17 \pm 0.02~M_\odot$, a surface temperature of $11500\pm1900$ K and a very young cooling age of only $200\pm100$ Myr. The mass and the age of the companion are compatible with a progenitor star of about $0.87~M_{\odot}$, which started transferring mass to the primary during its evolution along the sub-giant branch and stopped during the early red giant branch phase. Combining together the pulsar mass function and the companion mass, we found that this system is observed at an almost edge-on orbit and hosts a neutron star with a mass of $1.44 \pm 0.06~M_\odot$, thus suggesting a highly non-conservative mass accretion phase. The young age of the WD companion is consistent with the scenario of a powerful, relatively young MSP indicated by the earlier detection of gamma-rays from this system.
description: 11 pages, 7 figures, accepted for publication in ApJ
title: Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° ÐºÐ»Ð¸ÐµÐ½ÑÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«AAGÂ»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ
Ð±ÑÐµÐ½Ð´
Ð¸Ð¼Ð¸Ð´Ð¶ÐµÐ¾Ð»Ð¾Ð³Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° ÐÐÐ Â«AAGÂ». ÐÑÐ´ÐµÐ»ÑÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð°, ÑÑÐ½ÐºÑÐ¸Ð¸, ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸Ð¼Ð¸Ð´Ð¶Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾Ð»Ñ, Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸ ÑÑÐ°Ð¿Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð°. ÐÐ·ÑÑÐµÐ½ Ð¿Ð¾ÑÑÑÐµÑ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»Ñ ÐÐÐ Â«AAGÂ» Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿Ð¾ÐºÑÐ¿Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ²Ð°ÑÑÐ¸Ñ Ð² ÐÐ Â«Ð ÐµÐ½ÐµÑÑÐ°Ð½ÑÂ». Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ñ ÑÐµÐ»ÑÑ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° ÐÐÐ Â«AAGÂ» Ð¸ ÐµÐµ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð´Ð»Ñ ÐÐ Â«Ð ÐµÐ½ÐµÑÑÐ°Ð½ÑÂ».
Onthophagus eulophus Bates 1887
Creators: name: Kohlmann, Bert
name: Solís, Ángel
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Onthophagus
Onthophagus eulophus

description: Onthophagus eulophus species group*.
This group is diagnosed by a slightly emarginate clypeus; apical and internal male protibial margins projected (Figs. 1.23 –25); male protibial apex with some short setae (Figs. 1.23 –25); male protibial spur strongly bent inwards (Figs. 1.23 –25); male pronotum with a horn or a plate-like horn, which is level or turned upwards, never bent downwards.
Although no species of this group could be included in the mtDNA analysis, this aggregation is established based on a characteristic set of morphological characters, like having apical and internal male protibial margins projected and a male protibial spur strongly bent inwards (Figs. 1.23 –25). Moreover, contrary to the O. mexicanus species group that have long and slender male protibiae (Figs. 1.26 –28), this group has short and stout male protibiae (Figs. 1.23 –25). All species of this group seem to be associated with rodent nests; this behavior is supported by the shortened male protibiae and bent male protibial spurs (Moctezuma & Halffter 2021; Moctezuma et al. 2023). We consider that this group includes eight species (Table 7). Zunino & Halffter (1997) and Moctezuma & Halffter (2021) consider these species part of the O. mexicanus species group. The O. eulophus species group is primarily distributed in the mountains of the southwestern United States of America and along the Mexican Pacific mountain slopes, except for O. totonacus Moctezuma & Halffter, which lives along the Mexican Gulf piedmont.
description: Published as part of Kohlmann, Bert & Solís, Ángel, 2025, A review of the species groups of the Western Hemisphere Onthophagus Latreille (Coleoptera: Scarabaeidae: Scarabaeinae) using COI barcoding and gene trees, pp. 401-447 in Zootaxa 5604 (4) on page 426, DOI: 10.11646/zootaxa.5604.4.1, http://zenodo.org/record/15213967
On the Reionization-Era Globular Cluster in Low-Mass Galaxy Eridanus II
Creators: name: Weisz, Daniel R.
name: Savino, Alessandro
name: Dolphin, Andrew E.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using color-magnitude diagrams from deep archival Hubble Space Telescope imaging, we self-consistently measure the star formation history of Eridanus II (Eri II), the lowest-mass galaxy ($M_{\star}(z=0) \sim 10^5 M_{\odot}$) known to host a globular cluster (GC), and the age, mass, and metallicity of its GC. The GC ($\sim13.2\pm0.4$ Gyr, $\langle$[Fe/H]$\rangle = -2.75\pm0.2$ dex) and field (mean age $\sim13.5\pm0.3$ Gyr, $\langle$[Fe/H]$\rangle = -2.6\pm0.15$ dex) have similar ages and metallicities. Both are reionization-era relics that formed before the peak of cosmic star and GC formation ($z\sim2-4$). The ancient star formation properties of Eri II are not extreme and appear similar to $z=0$ dwarf galaxies. We find that the GC was $\lesssim4$ times more massive at birth than today and was $\sim$10% of the galaxy's stellar mass at birth. At formation, we estimate that the progenitor of Eri II and its GC had $M_{\rm UV} \sim -7$ to $-12$, making it one of the most common type of galaxy in the early Universe, though it is fainter than direct detection limits, absent gravitational lensing. Archaeological studies of GCs in nearby low-mass galaxies may be the only way to constrain GC formation in such low-mass systems. We discuss the strengths and limitations in comparing archaeological and high redshift studies of cluster formation, including challenges stemming from the Hubble Tension, which introduces uncertainties into the mapping between age and redshift.
description: 11 pages, 3 Figures, 1 Table. Accepted for publication in ApJ
IceCube: Construction Status and First Results
Creators: name: Karle, Albrecht
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: IceCube is a 1 km3 neutrino telescope currently under construction at the South Pole. The detector will consist of 4800 optical sensors deployed at depths between 1450 m and 2450 m in clear Antarctic ice evenly distributed over 80 strings. An air shower array covering a surface area of 1 km^2 above the in-ice detector will measure cosmic ray air showers in the energy range from 300 TeV to above 1 EeV. The detector is designed to detect neutrinos of all flavors. With 40 strings currently in operation, construction is 50% complete. Based on data taken to date, the observatory meets its design goals and currently exceeds the sensitivity of AMANDA and previous neutrino telescopes. The construction outlook and possible future extensions are also discussed.
description: 8 pages, 10 figures, to appear in the proceedings of the Acoustic and Radio EeV Neutrino detection Activities (ARENA) 2008 conference
title: Gaming myth: an exploration of video gaming, heritage, and identity creation in contemporary Cuba
Creators: name: Lickert, Miranda R.
Publisher: name: University of Reading
Year: 2019

description: This thesis examines the relationship between video games and the creation and sustainment of local, national, and personal myths in contemporary Cuba. This thesis examines traditional notions of myth, particularly those which relate to culture and heritage. At the same time, it will analyse the evolving role which video games, and technology more generally, play in our lives, and how new technologies affect the creation and propagation of myth in personal and national narratives. This thesis will then go on to give an overview of the historical context of Cuba, a nation in which myth continues to play a fundamental role in the national narrative, and explore how video games are an increasingly central element of these narratives. This thesis asks whether video games and computing can tell us anything of note about Cuban culture, and whether the games which are being played and developed in Cuba are part of a broader cultural and historical tradition which shapes Cuba as it is today. This thesis answers both of these questions in the affirmative, and demonstrates the significant impact which video games have had upon Cuba (particularly the more rural and remote parts of the country). This thesis also examines the question of whether gaming in Cuba might provide us with any practical or theoretical approaches to gaming which might be missing from the existing literature, and brings to the fore the lessons which Cuba’s unique circumstances hold for the furthering of the study of video games as an academic discipline. In order to support these assertions, the final chapter of this thesis is dedicated to a case study of the rural province of Granma. Using original interviews and fieldwork, this chapter combines the extensive historical and theoretical considerations which have been laid out in the preceding chapters, and applies them to the contemporary Cuban context. This thesis makes an original contribution to both the fields of Cuban studies and video game theory. Video game studies have traditionally been Western-centric, and have all but ignored countries such as Cuba. Whilst previous works have explored the role of myth within Cuba and gaming separately, this is the first work to study the manner in which myth underpins both video gaming and Cuban culture as a symbiotic whole.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð° ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÐºÑÐ¿Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ¾Ð½Ð¾Ð²Ð°, ÐÐºÑÐ°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°
ÑÑÑÐ°Ñ Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
Ð°Ð²ÑÐ¾ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
insurance
transport vehicles
insurance companies
car insurance

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð² ÑÑÐµÑÐµ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ², Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð²ÑÐ¾ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð² ÐÐ "Ð¡ÑÑÐ°ÑÐ¾Ð²Ð°Ñ Ð³ÑÑÐ¿Ð¿Ð° "Ð£ÑÐ°Ð»Ð¡Ð¸Ð±". Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ°Ñ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ° Ð¿Ð¾ Ð°Ð²ÑÐ¾ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐÐ "Ð¡ÑÑÐ°ÑÐ¾Ð²Ð°Ñ Ð³ÑÑÐ¿Ð¿Ð° "Ð£ÑÐ°Ð»Ð¡Ð¸Ð±" Ð¸ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°ÑÐ¸ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¿Ð¾ Ð°Ð²ÑÐ¾ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ², Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ ÑÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÑÐ°ÑÐ¾Ð²ÑÑ ÑÐ¾Ð±ÑÑÐ¸Ð¹.
description: The paper deals with the basic concepts and principles in the field of vehicle insurance, legal and regulatory framework of insurance of vehicles in Russia, organization of motor vehicle insurance in JSC "Insurance group "UralSib". We consider the current practice for motor insurance in the JSC "Insurance group "UralSib" and the basis of the tariff on motor insurance policy. The recommendations on the development of the transport mechanism of insurance funds, and proposed a series of measures to reduce the loss ratio in the settlement of insurance events.
The Distributed Oceanographic Data System: Requirements for Data Analysis Applications
Creators: name: Gallagher, James
name: Cornillon, Peter
Publisher: name: Zenodo
Year: 1996

description: This slide deck was presented at the Twenty-sixth International Symposium on Remote sensing of Environment on 25 March 1996.

Abstract: 

Access to distributed remote data alters both the scientist's use of data and expectations of analysis software. Access to remote data is fundamentally different from access to local data because the potential pool of resources is vastly larger. When confronted with this largesse, users requirements for data analysis software changes. Because users do not control remote data resources, they need ways to search among all available data sets for a particular type of information. These searches are different than the traditional database search because users, not knowing precisely what data exists, conduct their search in an iterative manner, asking repeatedly more specific questions. Users also want to select data from a data set in ways that suite their own work; this often means that remotely accessible data sets must support a more general query mechanism than those accessible only locally. Finally, users expect to be able to operate on several remote data sets at once, combining these different data in a single display. Within The Distributed Oceanographic Data System, we have had unique experience with the new requirements scientists place on data analysis applications because DODS provides a pathway for existing analysis programs to be extended so that they can access remote data resources.
Symmetry analysis of charmonium two-body decay
Creators: name: Mo, X. H.
name: Wang, P.
name: Zhang, J. Y.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the light of SU(3) flavor symmetry, the effective interaction Hamiltonian in tensor form is obtained by virtue of group representation theory. The strong and electromagnetic breaking effects are treated as a spurion octet so that the flavor singlet principle can be utilized as the criterion to determine the form of effective Hamiltonian. Two body decays of both baryonic and mesonic final states are parameterized in the uniform scheme, based on which the relative phase between the strong and electromagnetic amplitudes is studied for various charmonium decay modes, including psi' and/or J/jpsi decay to octet baryon pair, decuplet baryon pair, decuplet-octet baryon final state, and pseudoscalar-pseudoscalar meson final state. In data analysis of samples taken in $e^+e^-$ collider, the details of experimental effects, such as energy spread and initial state radiative correction are taken into consideration in order to make full use of experimental information and acquire the accurate and delicate results.
description: 16 pages. arXiv admin note: text overlap with arXiv:2111.15045
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¸ Ð¼Ð°ÑÐ¸Ð½. Ð¡ÑÐ°ÑÐ¸ÐºÐ° Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÐµÐ¼ÐµÐ½Ð¾Ð², Ð®ÑÐ¸Ð¹
name: Ð¡ÐµÐ¼ÐµÐ½Ð¾Ð²Ð°, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1999
Subjects: Ð¡ÑÐ°ÑÐ¸ÐºÐ°

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ âÐ¢ÐµÐ¾ÑÐ¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¸ Ð¼Ð°ÑÐ¸Ð½â Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 551800 âÐ¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµâ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ñ Ð¸Ð´ÐµÐ°Ð»ÑÐ½ÑÐ¼Ð¸ ÑÐ²ÑÐ·ÑÐ¼Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¸ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¸Ð±ÐµÑÐ½ÐµÑÐ¸ÐºÐ¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements
Creators: name: Xiao, Guang-Yao
name: Liu, Yu-Juan
name: Teng, Huan-Yu
name: Wang, Wei
name: Brandt, Timothy D.
name: Zhao, Gang
name: Zhao, Fei
name: Zhai, Meng
name: Gao, Qi
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Being one of the most fundamental physical parameter of astronomical objects, mass plays a vital role in the study of exoplanets, including their temperature structure, chemical composition, formation, and evolution. However, nearly a quarter of the known confirmed exoplanets lack measurements of their masses. This is particularly severe for those discovered via the radial-velocity (RV) technique, which alone could only yield the minimum mass of planets. In this study, we use published RV data combined with astrometric data from a cross-calibrated Hipparcos-Gaia Catalog of Accelerations (HGCA) to jointly constrain the masses of 115 RV-detected substellar companions, by conducting full orbital fits using the public tool \texttt{orvara}. Among them, 9 exoplanets with $M_{\rm p}\,{\rm sin}\,i<13.5\ M_{\rm Jup}$ are reclassified to the brown dwarf (BD) regime, and 16 BD candidates ($13.5\leqslant M_{\rm p}\,{\rm sin}\,i<80\,M_{\rm Jup}$) turn out to be low-mass M dwarfs. We point out the presence of a transition in the BD regime as seen in the distributions of host star metallicity and orbital eccentricity with respect to planet masses. We confirm the previous findings that companions with masses below $42.5\ M_{\rm Jup}$ might primarily form in the protoplanetary disc through core accretion or disc gravitational instability, while those with masses above $42.5\ M_{\rm Jup}$ formed through the gravitational instability of molecular cloud like stars. Selection effects and detection biases which may affect our analysis to some extent, are discussed.
description: 37 pages, 14 figures, accepted by Research in Astronomy and Astrophysics
The effect of metallicity on Cepheid magnitudes and the distance to M33
Creators: name: Scowcroft, V.
name: Bersier, D.
name: Mould, J. R.
name: Wood, P. R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the results from a multi-epoch survey of two regions of M33 using the 3.5m WIYN telescope. The inner field is located close to the centre of the galaxy, with the outer region situated about 5.1 kpc away in the southern spiral arm, allowing us to sample a large metallicity range. We have data for 167 fundamental mode Cepheids in the two regions. The reddening-free Wesenheit magnitude Wvi period-luminosity relations were used to establish the distance modulus of each region, with mu_{inner} = 24.37 +- 0.02 mag and mu_{outer} = 24.54 +- 0.03 mag. The apparent discrepancy between these two results can be explained by the significant metallicity gradient of the galaxy. We determine a value for the metallicity parameter of the Period--Luminosity relation gamma = d(m-M)/d log(Z) = -0.29 +- 0.11 mag/dex, consistent with previous measurements. This leads to a metallicity corrected distance modulus to M33 of 24.53 +- 0.11 mag.
description: MNRAS, in press. Paper with full resolution figures available at http://www.astro.ljmu.ac.uk/~vs/m33-cepheids-final.pdf
Additional file 2 of Male and female mice display consistent lifelong ability to address potential life-threatening cues using different post-threat coping strategies
Creators: name: Liu, Xue
name: Feng, Xiaolong
name: Huang, Hongren
name: Huang, Kang
name: Xu, Yang
name: Ye, Shuwei
name: Tseng, Yu-Ting
name: Wei, Pengfei
name: Wang, Liping
name: Wang, Feng
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Mental Health

description: Additional file 2: Figure S1. Elimination of estrous cycle in female mice did not affect defensive behavior following exposure to looming stimuli.
Code- Forecasting the risk of COVID-19 symptom onset
Creators: name: Wenzhong Shi
name: Chengzhuo Tong
name: Zhang, Anshu
name: Wang, Bin
name: Zhicheng Shi
name: Yepeng Yao
name: Jia, Peng
Publisher: name: Zenodo
Year: 2020

description: These are codes for predicting the onset risk.
title: Reinforcement learning control of a biomechanical model of the upper extremity
Creators: name: Fischer, Florian
name: Bachynskyi, Myroslav
name: Klar, Markus
name: Fleig, Arthur
name: Müller, Jörg
Publisher: name: University of Bayreuth
Year: 2021
Subjects: subject: Reinforcement Learning
subject: Aimed Movements
subject: Human Motor Control
subject: Arm Dynamics
subject: Upper Extremity
subject: Modeling
subject: Analysis
subject: Fitts’ Law
subject: Two-Thirds Power Law
subject: 2/3 Power Law
subject: Torque-driven
subject: Minimum Time
subject: SAC
subject: Optimal Control
subject: Optimization
subject: 000

description: Among the infinite number of possible movements that can be produced, humans are commonly assumed to choose those that optimize criteria such as minimizing movement time, subject to certain movement constraints like signal-dependent and constant motor noise. While so far these assumptions have only been evaluated for simplified point-mass or planar models, we address the question of whether they can predict reaching movements in a full skeletal model of the human upper extremity. We learn a control policy using a motor babbling approach as implemented in reinforcement learning, using aimed movements of the tip of the right index finger towards randomly placed 3D targets of varying size. We use a state-of-the-art biomechanical model, which includes seven actuated degrees of freedom. To deal with the curse of dimensionality, we use a simplified second-order muscle model, acting at each degree of freedom instead of individual muscles. The results confirm that the assumptions of signal-dependent and constant motor noise, together with the objective of movement time minimization, are sufficient for a state-of-the-art skeletal model of the human upper extremity to reproduce complex phenomena of human movement, in particular Fitts’ Law and the 2/3 Power Law. This result supports the notion that control of the complex human biomechanical system can plausibly be determined by a set of simple assumptions and can easily be learned.
Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
Creators: name: Brauner, Maren
name: Masseron, Thomas
name: García-Hernández, D. A.
name: Pignatari, Marco
name: Womack, Kate A.
name: Lugaro, Maria
name: Hayes, Christian R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The origin of phosphorus, one of the essential elements for life on Earth, is currently unknown. Prevalent models of Galactic chemical evolution (GCE) underestimate the amount of P compared to observations. The recently discovered P-rich ([P/Fe] > 1 dex) and metal-poor giants further challenge current theories on stellar nucleosynthesis. Since the observed stars are low-mass giants, our primary goal is to find clues on their progenitor. By increasing the number of known P-rich stars, we aim to narrow down a reliable chemical abundance pattern and to place robust constraints on the responsible nucleosynthetic mechanism. In the long term, identifying the progenitor of the P-rich stars may contribute to the search for the source of P in our Galaxy. We performed a detailed chemical abundance analysis based on the H-band spectra from APOGEE-2 (DR17). Employing the BACCHUS code, we measured the abundances of 13 elements in the sample, which is mainly composed of a recent collection of Si-enhanced giants. We also analyzed the orbital motions and compared the abundance results to possible nucleosynthetic formation scenarios, and also to detailed GCE models. We enlarged the sample of confirmed P-rich stars from 16 to 78 giants, which represents the largest sample of P-rich stars to date. Significant enhancements in O, Al, Si and Ce, as well as systematic correlations among the elements, unveil the chemical fingerprint of the P-rich stars. The high Mg and C+N found in some of the P-rich stars with respect to P-normal stars is not confirmed over the full sample. Strikingly, the strong over-abundance in the $α$-element Si is accompanied by normal Ca and S abundances. Our analysis of the orbital motion showed that the P-rich stars do not belong to a specific sub-population. In addition, we confirm that the majority of the sample stars are not part of binary systems.
description: 29 pages, 18 figures, 8 tables, accepted for publication in Astronomy & Astrophysics
title: Mass and Heat Transfer Evolutions of Ethanol Pool Fires under External Heat Flux
Creators: name: Yue, H.
name: Lizhong, Y.
name: Xiaodong, Z.
name: Yang, P.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019

description: This paper focuses on quantifying experimentally the evolution of conduction, convection and radiation
heat feedback mechanisms and corresponding mass burning rates of ethanol pool fires (8, 10, 12, and 15
cm diameter) under external heat fluxes ranging from 0 to 4.0 kW/m2. The results show that the
conduction heat feedback fraction is nearly independent of external heat flux, but decreases with pool
diameter. Meanwhile, the contribution fractions of convection and radiation heat feedback mechanisms
display a competitive relationship where the radiation heat feedback fraction increases with external heat
flux while the convection heat feedback fraction changes in the opposite direction. The transitional
external heat fluxes of the control regime are 3.3, 3.3, 2.8, and 1.3 kW/m2 for 8, 10, 12, and 15 cm pool
fires, respectively. The increment of the corresponding mass burning rate gradually declines in the
convection-controlled regime, while is nearly constant in the radiation-controlled regime. The flame heat
transfer blockage fraction b is introduced to express the variation of mass burning rate in the radiationcontrolled
regime based on a simple linear correlation. The heat blockage effect appears to be more
significant for larger pool diameters given that the values of b are 0.008, 0.021, 0.056, and 0.128 for
incremental pool diameters. Calculated mass burning rates based on the stagnant layer theory are in good
agreement with the measured ones.
Parameter estimation on gravitational waves from multiple coalescing binaries
Creators: name: Mandel, Ilya
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: Future ground-based and space-borne interferometric gravitational-wave detectors may capture between tens and thousands of binary coalescence events per year. There is a significant and growing body of work on the estimation of astrophysically relevant parameters, such as masses and spins, from the gravitational-wave signature of a single event. This paper introduces a robust Bayesian framework for combining the parameter estimates for multiple events into a parameter distribution of the underlying event population. The framework can be readily deployed as a rapid post-processing tool.
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð²Ð¾ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÑÐµÐ¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ð± Ð¾Ð±ÑÐµÐºÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§Ð¸Ð¶Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÑÐ·ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð·Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¿ÑÑÐºÐ¾Ð² Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð¾ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÑÐµÐ¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ð± Ð¾Ð±ÑÐµÐºÑÐµ, ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÐµÐ¹ Ð·Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð»ÑÐ±ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð´Ð°Ð½Ð½ÑÑ, Ð½Ð¾ ÑÐ¾Ð»ÑÐºÐ¾ Ð¿Ð¾ÑÐ»Ðµ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐ¾ÑÐ¼Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð¡Ð¸ÑÑÐµÐ¼Ð° ÑÐ°Ð±Ð¾ÑÐ°ÐµÑ Ñ ÑÐ°Ð¹Ð»Ð°Ð¼Ð¸ ÑÐ¾ÑÐ¼Ð°ÑÐ° CSV, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑ Ñ ÑÐ²Ð¾ÐµÐ¹ Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð±Ð¸Ð½Ð°ÑÐ½ÑÑ Ð´ÐµÑÐµÐ²ÑÐµÐ² CART. ÐÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ ÑÐ·ÑÐº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Java, Ð° ÑÐ°ÐºÐ¶Ðµ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ° Swing Ð´Ð»Ñ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»Ñ. ÐÐ»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ IntelliJ IDEA Community Edition.
The miniJPAS survey quasar selection III: Classification with artificial neural networks and hybridisation
Creators: name: Martínez-Solaeche, G.
name: Queiroz, Carolina
name: Delgado, R. M. González
name: Rodrigues, Natália V. N.
name: García-Benito, R.
name: Pérez-Ràfols, Ignasi
name: Abramo, L. Raul
name: Díaz-García, Luis
name: Pieri, Matthew M.
name: Chaves-Montero, Jonás
name: Hernán-Caballero, A.
name: Rodríguez-Martín, J. E.
name: Bonoli, Silvia
name: Morrison, Sean S.
name: Márquez, Isabel
name: Vílchez, J. M.
name: López-Sanjuan, C.
name: Cenarro, A. J.
name: Dupke, R. A.
name: Martín-Franch, A.
name: Varel, J.
name: Ramió, H. Vázquez
name: Cristóbal-Hornillos, D.
name: Moles, M.
name: Alcaniz, J.
name: Benitez, N.
name: Fernández-Ontiveros, J. A.
name: Ederoclite, A.
name: Marra, V.
name: de Oliveira, C. Mendes
name: Taylor, K.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: This paper is part of large effort within the J-PAS collaboration that aims to classify point-like sources in miniJPAS, which were observed in 60 optical bands over $\sim$ 1 deg$^2$ in the AEGIS field. We developed two algorithms based on artificial neural networks (ANN) to classify objects into four categories: stars, galaxies, quasars at low redshift ($z < 2.1)$, and quasars at high redshift ($z \geq 2.1$). As inputs, we used miniJPAS fluxes for one of the classifiers (ANN$_1$) and colours for the other (ANN$_2$). The ANNs were trained and tested using mock data in the first place. We studied the effect of augmenting the training set by creating hybrid objects, which combines fluxes from stars, galaxies, and quasars. Nevertheless, the augmentation processing did not improve the score of the ANN. We also evaluated the performance of the classifiers in a small subset of the SDSS DR12Q superset observed by miniJPAS. In the mock test set, the f1-score for quasars at high redshift with the ANN$_1$ (ANN$_2$) are $0.99$ ($0.99$), $0.93$ ($0.92$), and $0.63$ ($0.57$) for $17 < r \leq 20$, $20 < r \leq 22.5$, and $22.5 < r \leq 23.6$, respectively, where $r$ is the J-PAS rSDSS band. In the case of low-redshift quasars, galaxies, and stars, we reached $0.97$ ($0.97$), $0.82$ ($0.79$), and $0.61$ ($0.58$); $0.94$ ($0.94$), $0.90$ ($0.89$), and $0.81$ ($0.80$); and $1.0$ ($1.0$), $0.96$ ($0.94$), and $0.70$ ($0.52$) in the same r bins. In the SDSS DR12Q superset miniJPAS sample, the weighted f1-score reaches 0.87 (0.88) for objects that are mostly within $20 < r \leq 22.5$. Finally, we estimate the number of point-like sources that are quasars, galaxies, and stars in miniJPAS.
CO Spectral Line Energy Distributions of IR-luminous galaxies and AGN
Creators: name: Papadopoulos, Padeli P.
name: van der Werf, Paul
name: Isaak, Kate
name: Xilouris, Emmanuel M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report on new sensitive CO J=6-5 line observations of several luminous infrared Galaxies (LIRGs: L$_{\rm IR}$(8-1000$μ$m$)\ga 10^{11}$ L$_{\odot}$), 36% (8/22) of them ULIRGs (L$_{\rm IR}$$>10^{12}$ L$_{\odot}$), and two powerful local AGN: the optically luminous QSO PG 1119+120, and the powerful radio galaxy 3C 293 using the James Clerk Maxwell Telescope (JCMT) on Mauna Kea in Hawaii. We combine these observations with existing low-J CO data and dust emission Spectral Energy Distributions (SEDs) in the far-infrared - submillimetre from the literature to constrain the properties of the star-forming ISM in these systems. We then build the first {\it local} CO Spectral Line Energy Distributions (SLEDs) for the {\it global} molecular gas reservoirs that reach up to high J-levels. These CO SLEDs are neither biased by strong lensing (which affects many of those constructed for high-redshift galaxies), nor suffer from undersampling of CO-bright regions (as most current high-J CO observations of nearby extended systems do). We find: ...
description: 45 pages, 12 figures, accepted for publication at The Astrophysical Journal
On Evolution Equations of Quantum-Classical Systems
Creators: name: Gerasimenko, V. I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We consider the links between consistent and approximate descriptions of the quantum-classical systems, i.e. systems are composed of two interacting subsystems, one of which behaves almost classically while the other requires a quantum description.
description: 8 pages
Data-Driven Uncertainty Quantification of the Wave-Telescope Technique: General Equations and Application to HelioSwarm
Creators: name: Broeren, Theodore
name: Klein, Kristopher
Publisher: name: arXiv
Year: 2023
Subjects: subject: Space Physics (physics.space-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Plasma Physics (physics.plasm-ph)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The upcoming NASA mission HelioSwarm will use nine spacecraft to make the first simultaneous multi-point measurements of space plasmas spanning multiple scales. Using the wave-telescope technique, HelioSwarm's measurements will allow for both the calculation of the power in wavevector-and-frequency space and the characterization of the associated dispersion relations of waves present in the plasma at MHD and ion-kinetic scales. This technique has been applied to the four-spacecraft missions of CLUSTER and MMS and its effectiveness has previously been characterized in a handful of case studies. We expand this uncertainty quantification analysis to arbitrary configurations of four through nine spacecraft for three-dimensional plane waves. We use Bayesian inference to learn equations that approximate the error in reconstructing the wavevector as a function of relative wavevector magnitude, spacecraft configuration shape, and number of spacecraft. We demonstrate the application of these equations to data drawn from a nine-spacecraft configuration to both improve the accuracy of the technique, as well as expand the magnitudes of wavevectors that can be characterized.
description: 20 pages, 13 figures, 3 tables
A noncommutative Davis' decomposition for martingales
Creators: name: Perrin, Mathilde
Publisher: name: arXiv
Year: 2009
Subjects: subject: Operator Algebras (math.OA)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 46L53, 46L52 (Primary) 46L51, 60G42 (Secondary)

description: We prove an analogue of the classical Davis' decomposition for martingales in noncommutative L_p-spaces, involving the square functions. We also determine the dual space of the noncommutative conditioned Hardy space \h_1. We further extend this latter result to the case 1
description: To be published in Journal of London Math. Soc
Evolution of rotating massive stars with new hydrodynamic wind models
Creators: name: Gormaz-Matamala, Alex Camilo
name: Cuadra, Jorge
name: Meynet, Georges
name: Curé, Michel
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Mass loss due to line-driven winds is central to our understanding of the evolution of massive stars. We extend the evolution models introduced in Paper I, where the mass loss recipe is based on the simultaneous calculation of the wind hydrodynamics and the line-acceleration, by incorporating the effects of stellar rotation. We introduce a grid of self-consistent line-force parameters for a set of standard evolutionary tracks. With that, we generate a new set of evolutionary tracks with rotation for $M_\text{ZAMS}=25,40,70,$ and $120\,M_\odot$, and metallicities $Z=0.014$ and $0.006$. The self-consistent approach gives lower mass loss rates than the standard values adopted in previous evolution models. This decrease impacts strongly on the tracks of the most massive models. Weaker winds allow the star to retain more mass, but also more angular momentum. As a consequence, weaker wind models rotate faster and show a less efficient mixing in their inner stellar structure. The new tracks predict an evolution of the rotational velocities through the MS in close agreement with the range of $\varv\sin i$ values found by recent surveys of Galactic O-type stars. As subsequent implications, the weaker winds from self-consistent models suggest a reduction of the contribution of the isotope $^{26}$Al to the ISM due to stellar winds of massive stars during the MS phase. Moreover, the higher luminosities found for the self-consistent evolutionary models suggest that some populations of massive stars might be less massive than previously thought, as in the case of Ofpe stars at the Galactic Centre. Therefore, this study opens a wide range of consequences for further research based on the evolution of massive stars.
description: Accepted for publication in Astronomy & Astrophysics journal
Tunneling studies in a homogeneously disordered s-wave superconductor: NbN
Creators: name: Chockalingam, S. P.
name: Chand, Madhavi
name: Kamlapure, Anand
name: Jesudasan, John
name: Mishra, Archana
name: Tripathi, Vikram
name: Raychaudhuri, Pratap
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We report the evolution of superconducting properties as a function of disorder in homogeneously disordered epitaxial NbN thin films grown on (100) MgO substrates, studied through a combination of electrical transport, Hall Effect and tunneling measurements. The thickness of all our films are >50nm much larger than the coherence length ~5nm. The effective disorder in different films encompasses a large range, with the Ioffe-Regel parameter varying in the range kFl~1.38-8.77. Tunneling measurements on films with different disorder reveals that for films with large disorder the bulk superconducting transition temperature (Tc) is not associated with a vanishing of the superconducting energy gap, but rather a large broadening of the superconducting density of states. Our results provide strong evidence of the loss of superconductivity via phase-fluctuations in a disordered s-wave superconductor.
description: pdf file including figures
title: Ð¡Ð¸Ð³Ð½Ð°Ð»ÑÐ½Ð¾-ÐºÐ¾Ð´Ð¾Ð²ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð½ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ñ ÑÐ¿ÑÐ°Ð²Ð»ÑÐµÐ¼Ð¾Ð¹ Ð¼ÐµÐ¶ÑÐ¸Ð¼Ð²Ð¾Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐµÑÑÐµÑÐµÐ½ÑÐ¸ÐµÐ¹
title: Ð°Ð²ÑÐ¾ÑÐµÑ. Ð´Ð¸Ñ. â¦ ÐºÐ°Ð½Ð´. ÑÐµÑ Ð½. Ð½Ð°ÑÐº: 05.12.04
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ»Ð¾Ð², ÐÐ½ÑÐ¾Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸Ð³Ð½Ð°Ð»Ñ
ÐÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð¼ÐµÑ Ð¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ðµ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¸Ð½ÑÐµÐ·Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð´Ð»Ñ ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑÐ¸Ñ ÑÐ¸Ð»ÑÑÑÐ¾Ð², Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½Ð¾Ðµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»Ð¾ÑÑ ÑÐ°ÑÑÐ¾Ñ, Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾ ÐºÑÐ¸ÑÐµÑÐ¸Ñ 99%-Ð¹ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸ ÑÐ¸Ð³Ð½Ð°Ð»Ð°. ÐÐ° Ð¸ÑÐºÐ¾Ð¼ÑÐµ Ð½Ð°ÐºÐ»Ð°Ð´ÑÐ²Ð°ÑÑÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð½Ð° Ð¿Ð¸Ðº-ÑÐ°ÐºÑÐ¾Ñ ÑÐ¸Ð³Ð½Ð°Ð»Ð° Ð¸ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¼ÐµÐ¶ÑÐ¸Ð¼Ð²Ð¾Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐµÑÑÐµÑÐµÐ½ÑÐ¸Ð¸, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÐ¼ÑÐ¹ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½ÑÐ¼ ÐµÐ²ÐºÐ»Ð¸Ð´Ð¾Ð²ÑÐ¼ ÑÐ°ÑÑÑÐ¾ÑÐ½Ð¸ÐµÐ¼ Ð»Ð¸Ð±Ð¾ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¼ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ¾Ð¼ Ð³ÑÑÐ¿Ð¿Ð¾Ð²Ð¾Ð¹ ÐºÐ¾ÑÑÐµÐ»ÑÑÐ¸Ð¸. ÐÐ»Ñ ÑÐ¸Ð³Ð½Ð°Ð»ÑÐ½Ð¾-ÐºÐ¾Ð´Ð¾Ð²ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð½ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐºÑÑÑÐ¸Ð²Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²ÑÑÑÐ¾ÑÐ½ÑÑ ÐºÐ¾Ð´Ð¾Ð², ÑÐ¸Ð³Ð½Ð°Ð»ÑÐ½ÑÑ ÑÐ¾Ð·Ð²ÐµÐ·Ð´Ð¸Ð¹ ÐÐÐ Ð¸ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ¾Ð², Ð¿Ð¾Ð»ÑÑÐµÐ½ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð²ÑÐ¸Ð³ÑÑÑ Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð¸Ð·Ð²ÐµÑÑÐ½ÑÐ¼Ð¸ ÑÑÐµÐ¼Ð°Ð¼Ð¸ ÑÐµÑÑÑÑÐ°ÑÐ¾Ð¹ ÐºÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÑÐ»ÑÑÐ¸Ð¸.
Constraints from muon g-2 and LFV processes in the Higgs Triplet Model
Creators: name: Fukuyama, Takeshi
name: Sugiyama, Hiroaki
name: Tsumura, Koji
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Constraints from the muon anomalous magnetic dipole moment and lepton flavor violating processes are translated into lower bounds on v_Delta*m_H++ in the Higgs Triplet Model by considering correlations through the neutrino mass matrix. The discrepancy of the sign of the contribution to the muon anomalous magnetic dipole moment between the measurement and the prediction in the model is clarified. It is shown that mu to e gamma, tau decays (especially, tau to mu e e), and the muonium conversion can give a more stringent bound on v_Delta*m_H++ than the bound from mu to eee which is expected naively to give the most stringent one.
description: 18 pages, 16 figures
Onthophagus gazellinus Bates 1887
Creators: name: Kohlmann, Bert
name: Solís, Ángel
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Onthophagus
Onthophagus gazellinus

description: Onthophagus gazellinus species group.
This group is diagnosed by the male having no head horns (Figs. 5.7–8); male protibial apex with a tuft of long setae resembling a fine-pointed paintbrush (Figs. 1.57 –58); pronotum with four transversely aligned tubercles along a straight carina (Figs. 5.7–8), base unrimmed; metafemur light brown with fine punctures (Figs. 2.57 –58); at the excavated posterior pronotal margin a line of 5–6 large, ocellate punctures with one short, stiff, upward pointing seta, punctures disappearing towards middle of the pronotal margin; apex of elytra and pygidium with long, erect setae.
Boucomont (1932) initially established this species group as his “10 e Groupe” and was supported by Kohlmann & Solís (2001) under the name of O. gazellinus species group. This group contains, at present, only two species, O. gazellinus Bates and O. onthochromus Arrow (Table 7). Boucomont (1932) defined the group as having large species with long erect setae at the end of the elytra and on the pygidium; male head unarmed and female with two carinae; thorax base not rimmed; coloration light, elytral points brown. This species group is distributed from Nicaragua to Brazil.
description: Published as part of Kohlmann, Bert & Solís, Ángel, 2025, A review of the species groups of the Western Hemisphere Onthophagus Latreille (Coleoptera: Scarabaeidae: Scarabaeinae) using COI barcoding and gene trees, pp. 401-447 in Zootaxa 5604 (4) on page 426, DOI: 10.11646/zootaxa.5604.4.1, http://zenodo.org/record/15213967