cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Spin-Correlation Coefficients and Phase-Shift Analysis for p+$^3$He Elastic Scattering
Creators: name: Daniels, T. V.
name: Arnold, C. W.
name: Cesaratto, J. M.
name: Clegg, T. B.
name: Couture, A. H.
name: Karwowski, H. J.
name: Katabuchi, T.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Angular Distributions for the target spin-dependent observables A$_{0y}$, A$_{xx}$, and A$_{yy}$ have been measured using polarized proton beams at several energies between 2 and 6 MeV and a spin-exchange optical pumping polarized $^3$He target. These measurements have been included in a global phase-shift analysis following that of George and Knutson, who reported two best-fit phase-shift solutions to the previous global p+$^3$He elastic scattering database below 12 MeV. These new measurements, along with measurements of cross-section and beam-analyzing power made over a similar energy range by Fisher \textit{et al.}, allowed a single, unique solution to be obtained. The new measurements and phase-shifts are compared with theoretical calculations using realistic nucleon-nucleon potential models.
description: Submitted to Phys. Rev. C
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° Ðº ÐÐ­Ð¡ Ñ ÐÐÐ­Ð -600
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Ð»ÑÐ³Ð¸Ð½, Ð Ð¾Ð¼Ð°Ð½
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: Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ
ÐÐÐ­Ð -600
ÐÐÐ-1000ÐÐÐ
Ð¿Ð»Ð¾ÑÐ°Ð´Ñ ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½Ð°

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°ÑÑÐµÑÑ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÐºÐ¾Ð½-ÑÑÑÐ°, ÑÐµÐ¿Ð»Ð¾Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ ÑÐ°ÑÑÐµÑÑ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° ÐÐÐ-1000ÐÐÐ Ð¿ÑÐ¸ ÑÐ°Ð·-Ð»Ð¸ÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ°Ñ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÑÐ°.
ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ ÐÐÐ-1000ÐÐÐ Ðº ÐÐ­Ð¡ Ñ ÐÐÐ­Ð -600.
ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº, ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ»Ð¾Ð²Ð¸Ðµ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸, Ð½Ð°Ð´ÐµÐ¶Ð½Ð°Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ ÑÑÑÐ±Ð¸Ð½Ñ Ð-600-6,8/3000-1.
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Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð².
ÐÐ°ÑÑÐ½Ð°Ñ Ð½Ð¾Ð²Ð¸Ð·Ð½Ð°. Ð¡Ð¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÐºÐ¾Ð½-ÑÑÑÐ° Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ð¾ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐµÐµ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ðµ. ÐÑÐ±Ð¾Ñ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð½Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ñ ÑÐµÐ¿Ð»Ð¾Ð³Ð¾ Ð¸ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÑÑÐµÑÐ°, ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÐµÑ Ð½Ð¾ÑÐ¼Ð°Ð¼ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÑÑÐ±Ð¸Ð½Ñ.
ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÐ¾Ð²Ð°ÑÑ ÑÐµÑÐ¸Ð¹Ð½ÑÐ¹ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ ÐÐÐ-1000ÐÐÐ Ð² ÑÐµÐ°ÐºÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐµ Ñ ÐÐÐ­Ð -600 Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð´Ð¾ÑÑÐ¸ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð²ÑÐ³Ð¾Ð´Ñ, ÑÐ°Ðº ÐºÐ°Ðº Ð½ÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð½Ð°Ð»Ð°Ð¶Ð¸Ð²Ð°ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° Ð´Ð»Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÐÐÐ­Ð -600.
Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
Creators: name: Liu, Anna
name: Wong, Isaac C. F.
name: Leong, Samson H. W.
name: More, Anupreeta
name: Hannuksela, Otto A.
name: Li, Tjonnie G. F.
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Since the first detection of gravitational waves in 2015, gravitational-wave astronomy has emerged as a rapidly advancing field that holds great potential for studying the cosmos, from probing the properties of black holes to testing the limits of our current understanding of gravity. One important aspect of gravitational-wave astronomy is the phenomenon of gravitational lensing, where massive intervening objects can bend and magnify gravitational waves, providing a unique way to probe the distribution of matter in the universe, as well as finding applications to fundamental physics, astrophysics, and cosmology. However, current models for gravitational-wave millilensing - a specific form of lensing where small-scale astrophysical objects can split a gravitational wave signal into multiple copies - are often limited to simple isolated lenses, which is not realistic for complex lensing scenarios. In this paper, we present a novel phenomenological approach to incorporate millilensing in data analysis in a model-independent fashion. Our approach enables the recovery of arbitrary lens configurations without the need for extensive computational lens modeling, making it a more accurate and computationally efficient tool for studying the distribution of matter in the universe using gravitational-wave signals. When gravitational-wave lensing observations become possible, our method can provide a powerful tool for studying complex lens configurations, including dark matter subhalos and MACHOs.
description: 12 pages, 8 figures
Saari's Conjecture for the Collinear $n$-Body Problem
Creators: name: Diacu, Florin
name: Perez-Chavela, Ernesto
name: Santoprete, Manuele
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: In 1970 Don Saari conjectured that the only solutions of the Newtonian $n$-body problem that have constant moment of inertia are the relative equilibria. We prove this conjecture in the collinear case for any potential that involves only the mutual distances. Furthermore, in the case of homogeneous potentials, we show that the only collinear and non-zero angular momentum solutions are homographic motions with central configurations.
On the Water Waves Equations with Surface Tension
Creators: name: Alazard, Thomas
name: Burq, Nicolas
name: Zuily, Claude
Publisher: name: arXiv
Year: 2009
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: The purpose of this article is to clarify the Cauchy theory of the water waves equations as well in terms of regularity indexes for the initial conditions as for the smoothness of the bottom of the domain (namely no regularity assumption is assumed on the bottom). Our main result is that, following the approach developped by T. Alazard and G. Métivier in [1], after suitable paralinearizations, the system can be arranged into an explicit symmetric system of Schrödinger type. We then show that the smoothing effect for the (one dimensional) surface tension water waves proved by H. Christianson, V. M. Hur, and G. Staffilani in [9], is in fact a rather direct consequence of this reduction, which allows also to lower the regularity indexes of the initial data, and to obtain the natural weights in the estimates.
COVID-19 Cardiotoxicity and Cardioprotection
Creators: name: Camacho, Mariam Bonyadi
name: Kocheril, Philip
name: Kocheril, Abraham
Publisher: name: figshare
Year: 2022
Subjects: Cardiology

description: We review the pathophysiology of COVID-19-induced cardiac injury through both direct and indirect mechanisms and highlight the therapeutic role of existing cardioprotective interventions.
CONTENT OF CHARACTER EDUCATION INDRAJID ON BABOON LAKON RAMAYANA EAST JAVA VERSION
Creators: name: Pudjastawa, Astrid Wangsagirindra
Publisher: name: Zenodo
Year: 2015
Subjects: character education value
Indrajit
baboon lakon

description: Content of character education in play baboon of Ramayana East Java version, can serve as character education media for student. Indrajit figure which is positioned as an antagonist, it turns out in his death, his corpse got a special treatment of Rukti. Moreover, one part of his lifestory often used as a suluk by Javanese puppeters called Dalang. The publishing of the content of character education into Indrajit figure in play baboon of Ramayana, can determine about special treatment to him and the possibility of education content emergence as positive behavior example suit to character education pursuant to UU Nomor 20 Tahun 2003. Research conducted aims to find descriptions and character education contents of Indrajit figure in play baboon of Ramayana East Java version. The research subject was a book titled “Layang Kandha Kelir” which was play baboon purwa East Java version. This research type is a Descriptive-Qualitative Research with Hermeneutic method or known also as “tafsir sastra”. Based on research problems and discussions, can be concluded as follows: Indrajit figure description in play balungan divided into three (A) general description; (B) Indrajit’s wayang genealogy; and (C) Indrajit’s life story descriptions. Value contents of character education Indrajit figure play baboon suit to UU Nomor 23 Tahun 2003 about character education mentioned in 20 value points of character education. Indrajit as a figure inclined as a nationalist, responsible, religious and creative. Indrajit figure can be created as a role models in attitude suit to UU Nomor 23 Tahun 2003 expectations.
description: Artikel ini merupakan ringkasan dari skripsi sebagai syarat kelulusan pada jenjang S1 di Universitas Negeri Malang
Additional file 1 of Generation of multilineage liver organoids with luminal vasculature and bile ducts from human pluripotent stem cells via modulation of Notch signaling
Creators: name: Kim, Hyo Jin
name: Kim, Gyeongmin
name: Chi, Kyun Yoo
name: Kim, Hyemin
name: Jang, Yu Jin
name: Jo, Seongyea
name: Lee, Jihun
name: Lee, Youngseok
name: Woo, Dong-Hun
name: Han, Choongseong
name: Kim, Sang Kyum
name: Park, Han-Jin
name: Kim, Jong-Hoon
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Virology
subject: Computational Biology

description: Additional file 1. Supplementary tables and figures.
The MeerKAT Absorption Line Survey: Homogeneous continuum catalogues towards a measurement of the cosmic radio dipole
Creators: name: Wagenveld, J. D.
name: Klöckner, H. -R.
name: Gupta, N.
name: Deka, P. P.
name: Jagannathan, P.
name: Sekhar, S.
name: Balashev, S. A.
name: Boettcher, E.
name: Combes, F.
name: Emig, K. L.
name: Hilton, M.
name: Józsa, G. I. G.
name: Kamphuis, P.
name: Klutse, D. Y.
name: Knowles, K.
name: Krogager, J. -K.
name: Mohapatra, A.
name: Momjian, E.
name: Moodley, K.
name: Muller, S.
name: Petitjean, P.
name: Salas, P.
name: Sikhosana, S.
name: Srianand, R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The number counts of homogeneous samples of radio sources are a tried and true method of probing the large scale structure of the Universe, as most radio sources outside the galactic plane are at cosmological distances. As such they are expected to trace the cosmic radio dipole, an anisotropy analogous to the dipole seen in the cosmic microwave background (CMB). Results have shown that although the cosmic radio dipole matches the direction of the CMB dipole, it has a significantly larger amplitude. This result challenges our assumption of the Universe being isotropic, which can have large repercussions for the current cosmological paradigm. Though significant measurements have been made, sensitivity to the radio dipole is generally hampered by systematic effects that can cause large biases in the measurement. Here we assess these systematics with data from the MeerKAT Absorption Line Survey (MALS). We present the analysis of ten MALS pointings, focusing on systematic effects that could lead to an inhomogeneous catalogue. We describe the calibration and creation of full band continuum images and catalogues, producing a combined catalogue containing 16,313 sources and covering 37.5 square degrees of sky down to a sensitivity of 10 $μ$Jy/beam. We measure the completeness, purity, and flux recovery statistics for these catalogues using simulated data. We investigate different source populations in the catalogues by looking at flux densities and spectral indices, and how they might influence source counts. Using the noise characteristics of the pointings, we find global measures that can be used to correct for the incompleteness of the catalogue, producing corrected number counts down to 100 - 200 $μ$Jy. We show that we can homogenise the catalogues and properly account for systematic effects. We determine that we can measure the dipole to $3σ$ significance with 100 MALS pointings.
description: 30 pages, 25 figures. Accepted for publication in Astronomy & Astrophysics
title: ÐÐ¿ÑÑ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ Ð¶ÑÑÐ½Ð°Ð»Ð¾Ð² Ð¿Ð¾ Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð Ð¾ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð Ð°Ð·Ð¼ÑÑÐ»Ð¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
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: Ð¶ÑÑÐ½Ð°Ð»Ñ
Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð Ð¾ÑÑÐ¸Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð³Ð¾Ð²Ð¾ÑÐ¸ÑÑÑ Ð¾ ÐºÐ¾Ð½ÑÐµÐ¿ÑÑÐ°Ð»ÑÐ½ÑÑ Ð°ÑÐ¿ÐµÐºÑÐ°Ñ ÑÐ¸Ð¿Ð¾Ð»Ð¾Ð³Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¶ÑÑÐ½Ð°Ð»Ð¾Ð² Ð² Ð Ð¾ÑÑÐ¸Ð¸, ÑÐ¸Ð¿Ð°Ñ Ð¸ Ð²Ð¸Ð´Ð°Ñ Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾Ð± Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¶ÑÑÐ½Ð°Ð»Ð¾Ð² Ð¿Ð¾ Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸. ÐÐ°ÐµÑÑÑ Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹ Â«ÐÐ°ÑÐ° Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¸ Â«PsychÐ¾lÐ¾giesÂ», ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÐºÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÐ¼ÑÑ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹.
Believe It or Not: Adding Belief Annotations to Databases
Creators: name: Gatterbauer, Wolfgang
name: Balazinska, Magdalena
name: Khoussainova, Nodira
name: Suciu, Dan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Databases (cs.DB)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences
subject: H.2.1

description: We propose a database model that allows users to annotate data with belief statements. Our motivation comes from scientific database applications where a community of users is working together to assemble, revise, and curate a shared data repository. As the community accumulates knowledge and the database content evolves over time, it may contain conflicting information and members can disagree on the information it should store. For example, Alice may believe that a tuple should be in the database, whereas Bob disagrees. He may also insert the reason why he thinks Alice believes the tuple should be in the database, and explain what he thinks the correct tuple should be instead. We propose a formal model for Belief Databases that interprets users' annotations as belief statements. These annotations can refer both to the base data and to other annotations. We give a formal semantics based on a fragment of multi-agent epistemic logic and define a query language over belief databases. We then prove a key technical result, stating that every belief database can be encoded as a canonical Kripke structure. We use this structure to describe a relational representation of belief databases, and give an algorithm for translating queries over the belief database into standard relational queries. Finally, we report early experimental results with our prototype implementation on synthetic data.
description: 17 pages, 10 figures
Measuring the vortex-nucleus pinning force from pulsar glitch rates
Creators: name: Melatos, A.
name: Millhouse, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Superfluid vortex avalanches are one plausible cause of pulsar glitch activity. If they occur according to a state-dependent Poisson process, the measured long-term glitch rate is determined by the spin-down rate of the stellar crust, $\dotΩ_{\rm c}$, and two phenomenological parameters quantifying the vortex-nucleus pinning force: a crust-superfluid angular velocity lag threshold, $X_{\rm cr}$, and a reference unpinning rate, $λ_0$. A Bayesian analysis of 541 glitches in 177 pulsars, with $N_{\rm g} \geq 1$ events per pulsar, yields $X_{\rm cr} = 0.15^{+0.09}_{-0.04} \, {\rm rad \, s^{-1}}$, $λ_{\rm ref} = 7.6^{+3.7}_{-2.6} \times 10^{-8} \, {\rm s^{-1}}$, and $a = -0.27^{+0.04}_{-0.03}$ assuming the phenomenological rate law $λ_0 = λ_{\rm ref} [τ/(1 \, {\rm yr})]^a$, where $τ$ denotes the characteristic spin-down age. The results are broadly similar, whether one includes or excludes quasiperiodic glitch activity, giant glitches, or pulsars with $N_{\rm g}=0$, up to uncertainties about the completeness of the sample and the total observation time per pulsar. The $X_{\rm cr}$ and $λ_0$ estimates are consistent with first-principles calculations based on nuclear theory, e.g. in the semiclassical local density approximation.
description: 34 pages, 6 figures, accepted for publication in the Astrophysical Journal
title: Co-authorship networks analysis
title: Ανάλυση δικτύων συν-συγγραφέων
titleType: AlternativeTitle
Creators: name: Αδαμόπουλος, Εμμανουήλ
name: Adanopoulos, Emmanouil
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2021
Subjects: subject: Social networks analysis
subject: Ανάλυση κοινωνικών δικτύων
subject: Co-authorship network
subject: Δίκτυα συ-συγγραφέων

description: Η Κοινωνιολογία είναι ο θεμέλιος λίθος του σύγχρονου ερευνητικού πεδίου της Ανάλυσης Κοινωνικών Δικτύων. Τη δεκαετία του 1830 έγινε η πρώτη σχετική εισήγηση (Linton, 2004), γεγονός που αποτέλεσε και την απαρχή του συγκεκριμένου επιστημονικού πεδίου. Έκτοτε, η Ανάλυση Κοινωνικών Δικτύων βρίσκεται στο επίκεντρο του επιστημονικού ενδιαφέροντος και μέχρι σήμερα συνεχίζεται να παράγεται με εντατικούς ρυθμούς γνώση επί του θέματος. Στόχος του πεδίου αποτελεί η αναγνώριση της δομής μιας κοινότητας, η οποία μπορεί να αναπαρασταθεί με τη μορφή ενός γράφου, στον οποίο υπάρχουν κορυφές συνδεδεμένες με δεσμούς. Υπάρχουν διάφορα μαθηματικά μοντέλα που εκφράζουν τη δομή ενός δικτύου, τα οποία περιγράφονται εκτενώς στη παρούσα εργασία. Οι επιστήμονες χρησιμοποιούν αυτά τα μοντέλα με σκοπό να εξάγουν πολύτιμη πληροφορία σχετικά με τα δίκτυα, όπως για παράδειγμα η εύρεση του πιο κεντρικού κόμβου ή η εύρεση του συντομότερου μονοπατιού, μέσα από το οποίο μπορεί μια πληροφορία του δικτύου να περάσει από τον ένα κόμβο σε έναν άλλο. Με την εξέλιξη της υπολογιστικής δύναμης και των μεθόδων ανάλυσης δεδομένων, είναι δυνατή πλέον η ανάλυση εκτενών κοινωνικών δικτύων με μεγάλο αριθμό συμμετεχόντων. Στην παρούσα εργασία παρουσιάζεται μια ιστορική διαδρομή στο επιστημονικό πεδίο της Ανάλυσης Κοινωνικών Δικτύων. Σημειώνονται τα βασικά χαρακτηριστικά ενός δικτύου και αναφέρονται τα διαθέσιμα εργαλεία ανάλυσης δικτύων. Κάνοντας χρήση των μαθηματικών μοντέλων, πραγματοποιήθηκε ανάλυση πάνω σε τρία δίκτυα που εξήχθησαν από τη βιβλιογραφία άρθρων-κειμένων όπως αυτή διαμορφώθηκε στο διάστημα σαράντα χρόνων μεταξύ του 1978 και 2016 γύρω από την Ανάλυση Δεδομένων Περιβάλλοντος (Data Envelopment Analysis) (Emrouznejad & Yang, 2018). Τα αποτελέσματα και συμπεράσματα αυτής της ανάλυσης αναφέρονται στο τέλος της παρούσας εργασίας και στη συνέχεια προτείνεται μελλοντική έρευνα που μπορεί να πραγματοποιηθεί.
Additional file 1 of Egfr signaling promotes juvenile hormone biosynthesis in the German cockroach
Creators: name: Li, Zhaoxin
name: Zhou, Caisheng
name: Chen, Yumei
name: Ma, Wentao
name: Cheng, Yunlong
name: Chen, Jinxin
name: Bai, Yu
name: Luo, Wei
name: Li, Na
name: Du, Erxia
name: Li, Sheng
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Effect of RNAi each Egf ligand gene on Jhamt and Cyp15A1 expression. Figure S2. Effect of RNAi pairwise combinations of the three Egf ligand genes Jhamt and Cyp15A1 expression. Figure S3. Expression patterns of Egfr, spi, vn, Jhamt and Cyp15A1 of adult females, during the first vitellogenic cycle. Figure S4. Compare Egfr RNAi with InR RNAi. Figure S5. RNAi Egfr at the nymph stage. Figure S6. Egf ligands and Pnt RNAi at the nymph stage. Figure S7. Specificity verification of anti-JHAMT. Table S1. Primers used for qPCR, RNAi and 5′-RACE.
Global quantization of pseudo-differential operators on compact Lie groups, SU(2) and 3-sphere
Creators: name: Ruzhansky, Michael
name: Turunen, Ville
Publisher: name: arXiv
Year: 2008
Subjects: subject: Functional Analysis (math.FA)
subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35S05, 22E30

description: Global quantization of pseudo-differential operators on compact Lie groups is introduced relying on the representation theory of the group rather than on expressions in local coordinates. Operators on the 3-dimensional sphere and on group SU(2) are analysed in detail. A new class of globally defined symbols is introduced giving rise to the usual Hormander's classes of operators $Ψ^m(G)$, $Ψ^m(S^3)$ and $Ψ^m(SU(2))$. Properties of the new class and symbolic calculus are analysed. Properties of symbols as well as $L^2$-boundedness and Sobolev $L^2$--boundedness of operators in this global quantization are established on general compact Lie groups.
description: 42 pages
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ³Ð¸Ð¾Ð½Ð¾Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¾Ð³Ð¾ ÐºÑÐ°Ñ)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ·Ð¸Ð½Ð°, ÐÐ»Ð¸Ð·Ð°Ð²ÐµÑÐ°
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Ð°Ð½ÑÐ¿Ð¾ÑÑ
Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ°
ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¸Ð¹ ÐºÑÐ°Ð¹ Ð¸ ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¾Ð³Ð¾ ÐºÑÐ°Ñ Â«Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¾Ð¼ ÐºÑÐ°Ðµ Ð½Ð° 2014 -2025 Ð³Ð¾Ð´ÑÂ». Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ (Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸) - Ð²ÑÑÐ²Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¾Ð¼ ÐºÑÐ°Ðµ Ð½Ð° 2014 -2025 Ð³Ð¾Ð´ÑÂ» Ð¿Ð¾ ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸ÑÐ¼ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ. ÐÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ ÑÑÐµÐ´ÑÑÐ² Ð¸Ð· ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÐ´Ð¶ÐµÑÐ°, ÐºÐ¾Ð½ÑÐ¾Ð»Ð¸Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð±ÑÐ´Ð¶ÐµÑÐ° Ð¸ ÐºÑÐ°ÐµÐ²Ð¾Ð³Ð¾ Ð±ÑÐ´Ð¶ÐµÑÐ° Ð½Ðµ ÑÐ²Ð°ÑÐ°ÐµÑ, ÑÑÐ¾ ÑÑÐµÐ±ÑÐµÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ³Ð¸Ð¾Ð½Ð° - ÐÐ°Ð¼ÑÐ°ÑÑÐºÐ¾Ð³Ð¾ ÐºÑÐ°Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÐ¸ Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼.
Two Massive, Low-Luminosity Cores Toward Infrared Dark Clouds
Creators: name: Swift, Jonathan J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This article presents high-resolution interferometric mosaics in the 850 micron waveband of two massive, quiescent infrared dark clouds. The two clouds were chosen based on their likelihood to represent environments preceding the formation of massive stars. The brightest compact sources detected in each cloud have masses of approximately 110 and 60 solar masses with radii < 0.1 pc, implying mean volume densities of approximately 1 million particles per cubic centimeter and mean column densities of about 1 gram per square centimeter. Supplementary data show these cores to be cold and inactive. Low upper limits to their bolometric luminosities and temperatures place them at a very early stage of evolution while current models of massive star formation suggest they have the potential to form massive stars.
description: 6 pages, 5 figures. Accepted for publication by the Astrophysical Journal
Vacuum misalignment in presence of four-Fermi operators
Creators: name: Banerjee, Avik
name: Ferretti, Gabriele
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the issue of vacuum misalignment induced by four-Fermi couplings in a generic strongly coupled four-dimensional gauge theory. After briefly reviewing the general formalism, we focus on the case of partial compositness-like operators at leading order, which is relevant in applications to phenomenology. We show that the interactions between an elementary fermion and composite spin-1/2 operators in various representations contribute to the effective potential with relative sign differences. Thus the correct sign required to misalign the vacuum is guaranteed to occur for some representations but not all of them. The overall sign dictating the specific representations responsible for misalignment can in principle be determined on the lattice. We also comment on the likely sign for some simple cases.
description: 15 pages, 1 captioned figure. Comments are welcome
title: Συμπεριληπτική εκπαίδευση μαθητών με ειδικές ανάγκες, στάσεις και αντιλήψεις εκπαιδευτικών
title: Inclusive education for students with special needs, teachers’ attitudes and perceptions
titleType: AlternativeTitle
Creators: name: Ανδρεαδάκη, Γεωργία
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2021
Subjects: subject: Συμπεριληπτική εκπαίδευση
subject: Ισότιμη εκπαίδευση
subject: Στάσεις εκπαιδευτικών
subject: Ειδικές ανάγκες

description: Τα παιδιά με ειδικές ανάγκες και αναπηρίες αναμφισβήτητα έρχονται αντιμέτωπα με πολλά εμπόδια κατά την εκπαιδευτική διαδικασία. Η συμπεριληπτική εκπαίδευση συμβάλει στην προώθηση της ισότιμης και ποιοτικής εκπαίδευσης για όλους. Πρόκειται για μια διαδικασία που εστιάζει στα μοναδικά και ιδιαίτερα χαρακτηριστικά κάθε παιδιού. Καθοριστικό ρόλο στην προώθηση της συμπεριληπτικής εκπαίδευσης έχουν οι εκπαιδευτικοί και τα στελέχη εκπαίδευσης. Σκοπός της παρούσας εργασίας ήταν να διερευνήσει τις στάσεις και αντιλήψεις των εκπαιδευτικών για τη συμπερίληψη στις γενικές τάξεις παιδιών με αυτισμό, με διάσπαση προσοχής και υπερκινητικότητα, με νοητική καθυστέρηση και με ειδικές μαθησιακές δυσκολίες. Ακόμη, η εργασία είχε ως στόχο να εντοπιστούν παράγοντες που συμβάλουν ή δυσχαιρένουν την συμπεριληπτική διαδικασία. Το δείγμα της έρευνας αποτελείται από 206 εκπαιδευτικούς και στελέχη εκπαίδευσης των περιφεριακών ενοτήτων των Αθηνών, της Θεσσαλονίκης και της Κρήτης. Προκειμένου να καταγραφούν οι στάσεις χορηγήθηκε ερωτηματολόγιο το οποίο βασίστηκε στο ερευνητικό εργαλείο Teacher Attitude Inclusion Scale (TAIS) των Monsen, Ewing & Boyle (2014), και τη σχετική βιβλιογραφία το οποίο αποτελεί μη σταθμισμένο εργαλείο με κλειστού τύπου ερωτήσεις. Τα αποτελέσματα της παρούσας έρευνας έδειξαν ότι οι εκπαιδευτικοί εμφανίζουν θετικές στάσεις για τη συμπερίληψη μαθητών με Ε.Α. και αναπηρίες αλλά οι στάσεις τους αυτές εξαρτώνται από το είδος της αναπηρίας το οποίο καλούνται να αντιμετωπίσουν. Συγκεκριμένα, οι εκπαιδευτικοί τείνουν να είναι περισσότερο αρνητικοί στη συμπερίληψη παιδιών στο φάσμα του αυτισμού καθώς και παιδιών με νοητική καθυστέρηση. Ακόμη αναδείχθηκε η συμβολή της ενασχόλησης με την ειδική αγωγή, είτε ως απόκτηση εμπειρίας είτε ως άντληση εξειδικευμένων γνώσεων στη διαμόρφωση θετικών στάσεων προς τη συμπερίληψη. Τέλος οι ερωτώμενοι υπέδειξαν ότι μόνο δύο παράγοντες έτσι όπως υφίστανται σήμερα στα σχολεία λειτουργούν υποστηρικτικά στη συμπεριληπτική διαδικασία, οι οποίοι είναι η στάση της διοίκησης και το επίπεδο συνεργασίας των εκπαιδευτικών.
title: ÐÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÐÐ¡Ð¤Ð Ð² Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð Ð¾ÑÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ»Ð°Ñ, ÐÐ½Ð°ÑÑÐ°ÑÐ¸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: Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ
Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
ÐºÑÐµÐ´Ð¸ÑÐ½Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÑÑÐ¿Ð°ÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ðµ Ð±Ð°Ð½ÐºÐ¸ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¸Ñ Ð¿ÐµÑÐµÑÐ¾Ð´Ð° Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð¸ÑÐº Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÑÐµÐ¹ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÐÐ¡Ð¤Ð Ð² Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐ¶Ðµ Ð¸Ð¼ÐµÑÑÐµÐ³Ð¾ÑÑ Ð¾Ð¿ÑÑÐ° Ð¸ Ð¾ÑÐ¸Ð±Ð¾Ðº. ÐÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¿ÑÐµÐ´Ð¿Ð¾ÑÑÐ»ÐºÐ¸ Ð¸ ÑÑÐ°Ð¿Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÐÐ¡Ð¤Ð, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÑÑ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ.
Migrating Carrollian particles on magnetized black hole horizons
Creators: name: Bicak, Jiri
name: Kubiznak, David
name: Perche, T. Rick
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: By considering a misaligned (asymptotically uniform) magnetic field in the background of a rotating black hole, we uncover a possibility for a highly non-trivial motion of Carrollian particles on the black hole horizon that is characterized by a time-dependent velocity field and reminds us (because of its latitudinal oscillations) of a 'monarch butterfly migration'.
description: 6 pages, 3 figures
Characteristics of EUV coronal jets observed with STEREO/SECCHI
Creators: name: Nistico, G.
name: Bothmer, V.
name: Patsourakos, S.
name: Zimbardo, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper we present the first comprehensive statistical study of EUV coronal jets observed with the SECCHI imaging suites of the two STEREO spacecraft. A catalogue of 79 polar jets is presented, identified from simultaneous EUV and white-light coronagraph observations, taken during the time period March 2007 to April 2008. The appearances of the coronal jets were always correlated with underlying small-scale chromospheric bright points. A basic characterisation of the morphology and identification of the presence of helical structure were established with respect to recently proposed models for their origin and temporal evolution. A classification of the events with respect to previous jet studies shows that amongst the 79 events there were 37 Eiffel tower-type jet events commonly interpreted as a small-scale (about 35 arcsec) magnetic bipole reconnecting with the ambient unipolar open coronal magnetic fields at its looptops, and 12 lambda-type jet events commonly interpreted as reconnection with the ambient field happening at the bipoles footpoints. Five events were termed micro-CME type jet events because they resembled the classical coronal mass ejections (CMEs) but on much smaller scales. A few jets are also found in equatorial coronal holes. The typical lifetimes in the SECCHI/EUVI (Extreme UltraViolet Imager) field of view between 1.0 to 1.7 solar radius and in SECCHI/COR1 field of view between 1.4 to 4 solar radius are obtained, and the derived speed are roughly estimated. In summary, the observations support the assumption of continuous small-scale reconnection as an intrinsic feature of the solar corona, with its role for the heating of the corona, particle acceleration, structuring and acceleration of the solar wind remaining to be explored in more details in further studies.
description: 20 pages, 7 tables of figures, 2 tables of plots, an appendix with list events
The Siegel modular forms of genus 2 with the simplest divisor
Creators: name: Gritsenko, Valery
name: Clery, Fabien
Publisher: name: arXiv
Year: 2008
Subjects: subject: Number Theory (math.NT)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 11F46

description: We prove that there exist exactly eight Siegel modular forms with respect to the congruence subgroups of Hecke type of the paramodular groups of genus two vanishing precisely along the diagonal of the Siegel upper half-plane. This is a solution of a question formulated during the conference "Black holes, Black Rings and Modular Forms" (ENS, Paris, August 2007). These modular forms generalize the classical Igusa form and the forms constructed by Gritsenko and Nikulin in 1998.
title: ÐÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½ÑÐµ Ð´Ð°ÑÑÐ¸ÐºÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾ÐºÐ°
Creators: name: Ð¡Ð°Ð¿Ð¾Ð¶Ð½Ð¸ÐºÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ¸ÑÑÐºÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¸ÑÑÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2003
Subjects: ÐÐ°ÑÑÐ¸ÐºÐ¸ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ
Ð¢ÐµÑÐ¼Ð¾Ð¼ÐµÑÑÐ¸Ñ

description: ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½ÑÐµ Ð´Ð°ÑÑÐ¸ÐºÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾ÐºÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð¸Ð·Ð¾ÑÑÐ¾Ð¿Ð½ÑÑ Ð¼Ð¾Ð½Ð¾ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² Ð²Ð¸ÑÐ¼ÑÑÐ°. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð²; ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð°Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ðµ Ð·Ð°Ð²Ð¸ÑÐ¸Ñ Ð¾Ñ ÑÐ¾Ð»ÑÐ¸Ð½Ñ Ð´Ð°ÑÑÐ¸ÐºÐ° Ð¸ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÐµÑ Ð¾ÐºÐ¾Ð»Ð¾ 50 Ð¼ÐºÑ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½ÑÑ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð² ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐµ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½ÑÑ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð´Ð»Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑ, ÐºÐ°ÑÐ°ÑÐµÐ»ÑÐ½ÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹ ÑÑÐµÐ½Ð¸Ñ, ÑÐ°ÑÑÐ¾Ð´Ð° Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÐ¿Ð»Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¸ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° Ð² ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ¿ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÐ¸ÑÐ¾ÐºÐ¾Ð³Ð¾ ÐºÑÑÐ³Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð·Ð°Ð½ÑÑÑÑ ÑÐµÐ¿Ð»Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² ÑÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹.
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 Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Additional file 2 of Associations between urinary concentrations of bisphenols and serum concentrations of sex hormones among US. Males
Creators: name: Zhang, Chichen
name: Luo, Yuehong
name: Qiu, Shi
name: Huang, Xinyi
name: Jin, Kun
name: Li, Jiakun
name: Yang, Mi
name: Hu, Dan
name: Zheng, Xiaonan
name: Jiang, Zhongyuan
name: Wang, Mingda
name: Zou, Xiaoli
name: Wei, Qiang
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 2: Supplementary Table 1. Population Characteristics of participants stratified by BPA in the 2011–2016 continuous NHANES.
The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey -- I. Survey design and processing pipeline
Creators: name: Bhat, N. D. R.
name: Swainston, N. A.
name: McSweeney, S. J.
name: Xue, M.
name: Meyers, B. W.
name: Kudale, S.
name: Dai, S.
name: Tremblay, S. E.
name: van Straten, W.
name: Shannon, R. M.
name: Smith, K. R.
name: Sokolowski, M.
name: Ord, S. M.
name: Sleap, G.
name: Williams, A.
name: Hancock, P. J.
name: Lange, R.
name: Tocknell, J.
name: Johnston-Hollitt, M.
name: Kaplan, D. L.
name: Tingay, S. J.
name: Walker, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present an overview of the Southern-sky MWA Rapid Two-metre (SMART) pulsar survey that exploits the MWA's large field of view and voltage capture system to survey the sky south of 30 degree in declination for pulsars and fast transients in the 140-170 MHz band. The survey is enabled by the advent of the Phase II MWA's compact configuration, which offers an enormous efficiency in beam-forming and processing costs, thereby making an all-sky survey of this magnitude tractable with the MWA. Even with the long dwell times of the survey (4800 s), data collection can be completed in < 100 hours of telescope time, while still retaining the ability to reach a limiting sensitivity of ~2-3 mJy. Each observation is processed to generate ~5000-8000 tied-array beams that tessellate the full ~610 square degree field of view, which are then processed to search for pulsars. The voltage-capture recording allows a multitude of post hoc processing options including the reprocessing of data for higher time resolution. Due to the substantial computational cost in pulsar searches at low frequencies, processing is undertaken in multiple passes: in the first pass, a shallow survey is performed, where 10 minutes of each observation is processed, reaching about one-third of the full search sensitivity. Here we present the system overview and initial results. Further details including first pulsar discoveries and a census of low-frequency detections are presented in a companion paper. Future plans include deeper searches to reach the full sensitivity and acceleration searches to target binary and millisecond pulsars. Simulation analysis forecasts ~300 new pulsars upon the completion of full processing. The SMART survey will also generate a complete digital record of the low-frequency sky, which will serve as a valuable reference for future pulsar searches planned with the low-frequency Square Kilometre Array.
description: 22 pages, 12 figures, 2 tables, Accepted for publication in PASA
New Agegraphic Dark Energy in Brans-Dicke Theory
Creators: name: Liu, Xiang-Lai
name: Zhang, Xin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this paper, we investigate the new agegraphic dark energy model in the framework of Brans-Dicke theory which is a natural extension of the Einstein's general relativity. In this framework the form of the new agegraphic dark energy density takes as $ρ_{q} =3n^2 Φ(t)η^{-2}$, where $η$ is the conformal age of the universe and $Φ(t)$ is the Brans-Dicke scalar field representing the inverse of the time-variable Newton's constant. We derive the equation of state of the new agegraphic dark energy and the deceleration parameter of the universe in the Brans-Dicke theory. It is very interesting to find that in the Brans-Dicke theory the agegraphic dark energy realizes quintom-like behavior, i.e., its equation of state crosses the phantom divide $w=-1$ during the evolution. We also compare the situation of the agegraphic dark energy model in the Brans-Dicke theory with that in the Einstein's theory. In addition, we discuss the new agegraphic dark energy model with interaction in the framework of the Brans-Dicke theory.
description: 15 pages, 4 figures
Self-paced learning for VII grades Junior Highschool using canvas.
Creators: name: M.A.A, Muhammad Amzah
name: Slamet Muhanif
Publisher: name: Zenodo
Year: 2021
Subjects: Self-faced learning

description: It's materials for self-paced learning, including its description, adventages of canvas, and materials for Junior Highschool especially for VII grades.
description: Canvas
title: ÐÐ¾Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¿ÑÑÐµÐ¼ ÑÐ¼Ð¸ÑÑÐ¸Ð¸ ÑÐµÐ½Ð½ÑÑ Ð±ÑÐ¼Ð°Ð³
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¡ÐµÑÐ¿ÑÐºÐ¾Ð², ÐÐ¾Ð³Ð´Ð°Ð½
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Ð¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°
ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÑ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸
ÑÐ¼Ð¸ÑÑÐ¸Ñ ÑÐµÐ½Ð½ÑÑ Ð±ÑÐ¼Ð°Ð³

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¡Ð±ÐµÑÐ±Ð°Ð½Ðº Ð Ð¾ÑÑÐ¸Ð¸Â».
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ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÑÐ¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¼Ð¾Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¿ÑÑÐµÐ¼ ÑÐ¼Ð¸ÑÑÐ¸Ð¸ ÑÐµÐ½Ð½ÑÑ Ð±ÑÐ¼Ð°Ð³ Ð² ÐÐÐ Â«Ð¡Ð±ÐµÑÐ±Ð°Ð½Ðº Ð Ð¾ÑÑÐ¸Ð¸Â».
title: ÐÐ°Ð¿ÑÑÐ¶ÑÐ½Ð½Ð¾-Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, ÑÑÐ¸Ð»ÐµÐ½Ð½ÑÑ ÑÐ³Ð»ÐµÐ¿Ð»Ð°ÑÑÐ¸ÐºÐ¾Ð¼
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¾Ð»ÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
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: ÐÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸
ÐÐ°Ð»ÐºÐ¸ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ
ÑÐ³Ð»ÐµÐ¿Ð»Ð°ÑÑÐ¸ÐºÐ¸
ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ

description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾-Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, ÑÑÐ¸Ð»ÐµÐ½Ð½ÑÑ ÑÐ³Ð»ÐµÐ¿Ð»Ð°ÑÑÐ¸ÐºÐ¾Ð¼. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð±Ð°Ð»Ð¾Ðº Ð¿Ð¾ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½ÑÑ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹, ÑÐ¾Ð³Ð»Ð°ÑÐ½Ð¾ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°ÑÑÐµÑÑ, Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ»Ð°Ð³Ð°ÐµÐ¼ÑÐ¼Ð¸, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐ¸Ð¼Ð¸ Ð²ÐºÐ»Ð°Ð´ Ð² Ð½ÐµÑÑÑÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¸ Ð¾Ð±ÑÑÑ Ð¶ÐµÑÑÐºÐ¾ÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð½Ð¾Ð²ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÑÐ¸Ð»ÐµÐ½Ð¸Ñ.
Additional file 2 of Genomic features and its potential implication in bone oligometastatic NSCLC
Creators: name: Liao, Rongxin
name: Yi, Guangming
name: Shen, Lu
name: Zhang, Xiaoyue
name: Xu, Zaicheng
name: Peng, Yuan
name: Yang, Zhenzhou
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 2: Fig. S1. A Mutational fraction of the six-base substitution for each sample. B Comparison of the high-frequency mutations identified in bone oligometastatic LUAD with that in the MSKCC cohort of LUAD. C Frequency distributions of EGFR. D Frequency of concurrent EGFR/TP53 mutations in bone oligometastasis. *p < 0.05, and **p < 0.01. Fig. S2. The mutated sites of genes with high mutation frequency, including EGFR (A), TP53 (B), KRAS (C), CDKN2A (D), MET (E), ARID2 (F), ATM (G), CTNNB1 (H), SMARCA4 (I).