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arXiv 2022年

作者： Fernández-Valenzuela, Estela Morales, N. Vara-Lubiano, M. Ortiz, J.L. Benedetti-Rossi, G. Sicardy, B. Kretlow, M. Santos-Sanz, P. Morgado, B. Souami, D. Organero, F. Ana, L. Fonseca, F. Román, A. Alonso, S. Gonçalves, R. Ferreira, M. Iglesias-Marzoa, R. Lamadrid, J.L. Alvarez-Candal, A. Assafin, M. Braga-Ribas, F. Camargo, J.I.B. Colas, F. Desmars, J. Duffard, R. Lecacheux, J. Gomes-Júnior, A.R. Rommel, F.L. Vieira-Martins, R. Pereira, C.L. Casanova, V. Selva, A. Perelló, C. Mottola, S. Hellmich, S. Maestre, J.L. Castro-Tirado, A.J. Pal, A. Trigo-Rodriguez, J.M. Beisker, W. Laporta, A. Garcés, M. Escaned, L. Bretton, M. Florida Space Institute UCF 12354 Research Parkway Partnership 1 building Room 211 Orlando United States Instituto de astrofísica de Andalucía CSIC Glorieta de la Astronomía s/n Granada18008 Spain UNESP - São Paulo State University Grupo de Dinâmica Orbital e Planetologia SP Guaratinguetá12516-410 Brazil Laboratório Interinstitucional de e-Astronomia - LIneA INCT do e-Universo Rua Gal. José Cristino 77 RJ Rio de Janeiro20921-400 Brazil LESIA Observatoire de Paris Université PSL Sorbonne Université Université de Paris CNRS Meudon92190 France naXys University of Namur 8 Rempart de la Vierge NamurB-5000 Belgium Rua Gal. José Cristino 77—Bairro Imperial de São Cristóvão Rio de Janeiro20921-400 Brazil Complejo Astronómico de La Hita Camino de Doña Sol s/n LaVilla de Don fadrique45850 Spain Sociedad Astronómica Granadina Apartado de Correos 195 Granada18080 Spain Software Engineering Department Andalusian Research Institute in Data Science and Computational Intelligence University of Granada Spain Instituto Politécnico de Tomar CI2 e U.D. Matemática e Física Tomar2300-313 Portugal Centro Ciência Viva Alto de Santa Bárbara Via Galileu Galilei 817 Constância2250-100 Portugal Centro de Estudios de Física del Cosmos de Aragón Plaza San Juan 1 Teruel44001 Spain Instituto de Física Aplicada a las Ciencias y las Tecnologías Universidad de Alicante San Vicent del Raspeig AlicanteE03080 Spain Observatório do Valongo/UFRJ Ladeira Pedro Antonio 43 RJ Rio de Janeiro20.080-090 Brazil Av. Sete de Setembro 3165 CEP Curitiba80230-901 Brazil Institut Polytechnique des Sciences Avancées IPSA 63 boulevard de Brandebourg Ivry-sur-SeineF-94200 France Institut de Mécanique Céleste et de Calcul des Éphémérides IMCCE Observatoire de Paris PSL Research University CNRS Sorbonne Universités UPMC Univ Paris 06 Univ. Lille 77 Av. Denfert-Rochereau ParisF-75014 France Agrupación Astronómica de Sabadell Carrer Prat de la Riba 116 Sabadell08206 Spai

Within our program of physical characterization of trans-Neptunian objects and centaurs, we predicted a stellar occultation by the centaur (54598) Bienor to occur on January 11, 2019, with good observability potential. We obtained high accuracy astrometric data to refine the prediction, resulting in a shadow path favorable for the Iberian Peninsula. This encouraged us to carry out an occultation observation campaign that resulted in five positive detections from four observing sites. This is the fourth centaur for which a multichord (more than two chords) stellar occultation has been observed so far, the other three being (2060) Chiron, (10199) Chariklo, and (95626) 2002 GZ32. From the analysis of the occultation chords, combined with the rotational light curve obtained shortly after the occultation, we determined that Bienor has an area-equivalent diameter of 150 ± 20 km. This diameter is ∼ 30 km smaller than the one obtained from thermal measurements. The position angle of the short axis of the best fitting ellipse obtained through the analysis of the stellar occultation does not match that of the spin axis derived from long-term photometric models. We also detected a strong irregularity in one of the minima of the rotational light curve that is present no matter the aspect angle at which the observations were done. We present different scenarios to reconcile the results from the different techniques. We did not detect secondary drops related to potential rings or satellites. Nonetheless, similar rings in size to that of Chariklo’s cannot be discarded due to low data accuracy. © 2022, CC BY.

关键词： Photometry

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OzDES multi-object fibre spectroscopy for the Dark Energy Survey: Results and second data release

arXiv

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arXiv 2020年

作者： Lidman, C. Tucker, B.E. Davis, T.M. Uddin, S.A. Asorey, J. Bolejko, K. Brout, D. Calcino, J. Carollo, D. Carr, A. Childress, M. Hoormann, J.K. Foley, R.J. Galbany, L. Glazebrook, K. Hinton, S.R. Kessler, R. Kim, A.G. King, A. Kremin, A. Kuehn, K. Lagattuta, D. Lewis, G.F. Macaulay, E. Malik, U. March, M. Martini, P. Möller, A. Mudd, D. Nichol, R.C. Panther, F. Parkinson, D. Pursiainen, M. Sako, M. Swann, E. Scalzo, R. Scolnic, D. Sharp, R. Smith, M. Sommer, N.E. Sullivan, M. Webb, S. Wiseman, P. Yu, Z. Yuan, F. Zhang, B. Abbott, T.M.C. Aguena, M. Allam, S. Annis, J. Avila, S. Bertin, E. Bhargava, S. Brooks, D. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Costanzi, M. da Costa, L.N. de Vicente, J. Doel, P. Eifler, T.F. Everett, S. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gruen, D. Gruendl, R.A. Gschwend, J. Gutierrez, G. Hartley, W.G. Hollowood, D.L. Honscheid, K. James, D.J. Kuropatkin, N. Li, T.S. Lima, M. Lin, H. Maia, M.A.G. Marshall, J.L. Melchior, P. Menanteau, F. Miquel, R. Palmese, A. Paz-Chinchón, F. Plazas, A.A. Roodman, A. Rykoff, E.S. Sanchez, E. Santiago, B. Scarpine, V. Schubnell, M. Serrano, S. Sevilla-Noarbe, I. Suchyta, E. Swanson, M.E.C. Tarle, G. Tucker, D.L. Varga, T.N. Walker, A.R. Wester, W. Wilkinson, R.D. Research School of Astronomy and Astrophysics Australian National University ACT2601 Australia School of Mathematics and Physics University of Queensland BrisbaneQLD4072 Australia Observatories of the Carnegie Institution for Science 813 Santa Barbara St. PasadenaCA91101 United States Madrid Spain School of Natural Sciences College of Sciences and Engineering University of Tasmania Private Bag 37 Hobart TAS7001 Australia NASA Einstein Department of Physics and Astronomy University of Pennsylvania PhiladelphiaPA19104 United States INAF Astrophysical Observatory of Turin Pino TorineseI-10025 Italy School of Physics and Astronomy University of Southampton SouthamptonSO17 1BJ United Kingdom Santa Cruz Institute for Particle Physics Santa CruzCA95064 United States PITT PACC Department of Physics and Astronomy University of Pittsburgh PittsburghPA15260 United States Centre for Astrophysics & Supercomputing Swinburne University of Technology Victoria3122 Australia Department of Astronomy and Astrophysics University of Chicago ChicagoIL60637 United States Kavli Institute for Cosmological Physics University of Chicago ChicagoIL60637 United States Lawrence Berkeley National Laboratory 1 Cyclotron Road BerkeleyCA94720 United States School of Physics University of Melbourne ParkvilleVIC3010 Australia Department of Physics University of Michigan Ann ArborMI48109 United States Australian Astronomical Optics Macquarie University North RydeNSW2113 Australia Lowell Observatory 1400 Mars Hill Rd FlagstaffAZ86001 United States Centre for Extragalactic Astronomy Department of Physics Durham University DurhamDH1 3LE United Kingdom Institute for Computational Cosmology Durham University South Road DurhamDH1 3LE United Kingdom Sydney Institute for Astronomy School of Physics University of Sydney A28 NSW2006 Australia Institute of Cosmology and Gravitation University of Portsmouth PortsmouthPO1 3FX United Kingdom Center for Cosmology

We present a description of the Australian Dark Energy Survey (OzDES) and summarise the results from its six years of operations. Using the 2dF fibre positioner and AAOmega spectrograph on the 3.9-m Anglo-Australian Telescope, OzDES has monitored 771 AGN, classified hundreds of supernovae, and obtained redshifts for thousands of galaxies that hosted a transient within the 10 deep fields of the Dark Energy Survey. We also present the second OzDES data release, containing the redshifts of almost 30,000 sources, some as faint as rAB = 24 mag, and 375,000 individual spectra. These data, in combination with the time-series photometry from the Dark Energy Survey, will be used to measure the expansion history of the Universe out to z ~ 1.2 and the masses of hundreds of black holes out to z ~ 4. OzDES is a template for future surveys that combine simultaneous monitoring of targets with wide-field imaging cameras and wide-field multi-object spectrographs. Copyright © 2020, The Authors. All rights reserved.

关键词： Surveys

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SciPy 1.0—Fundamental algorithms for scientific computing in python

arXiv

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arXiv 2019年

作者： Virtanen, Pauli Gommers, Ralf Oliphant, Travis E. Haberland, Matt Reddy, Tyler Cournapeau, David Burovski, Evgeni Peterson, Pearu Weckesser, Warren Bright, Jonathan van der Walt, Stéfan J. Brett, Matthew Wilson, Joshua Millman, K. Jarrod Mayorov, Nikolay Nelson, Andrew R.J. Jones, Eric Kern, Robert Larson, Eric Carey, C.J. Polat, Ilhan Feng, Yu Moore, Eric W. VanderPlas, Jake Laxalde, Denis Perktold, Josef Cimrman, Robert Henriksen, Ian Quintero, E.A. Harris, Charles R. Archibald, Anne M. Ribeiro, Antônio H. Pedregosa, Fabian van Mulbregt, Paul University of Jyväskylä University of Jyväskylä FI-40014 Finland Quansight LLC AustinTX United States Ultrasound Imaging Mayo Clinic RochesterMN55902 United States Electrical Engineering Brigham Young University ProvoUT84604 United States Enthought Inc. AustinTX78701 United States Anaconda Inc AustinTX78701 United States BioResource and Agricultural Engineering Department California Polytechnic State University San Luis ObispoCA93407 United States Department of Mathematics University of California Los AngelesCA90025 United States Los Alamos National Laboratory Los AlamosNM87544 United States Independent Researcher Higher School of Economics Myasnitskaya 20 Moscow101000 Russia Independent Researcher Saue Estonia Department of Mechanics and Applied Mathematics Institute of Cybernetics Tallinn Technical University Akadeemia Rd 21 Tallinn Estonia Independent Researcher NY United States Berkeley Institute for Data Science University of California BerkeleyCA94720 United States School of Psychology University of Birmingham Edgbaston BirmighamB15 2TT United Kingdom Division of Biostatistics University of California BerkeleyCA94720 United States WayRay LLC Skolkovo Innovation Center Moscow143026 Russia Australian Nuclear Science and Technology Organisation Locked Bag 2001 Kirrawee DCNSW2232 Australia Institute for Learning and Brain Sciences University of Washington SeattleWA98195 United States College of Information and Computing Sciences University of Massachusetts Amherst AmherstMA01002 United States Berkeley Center for Cosmological Physics University of California BerkeleyCA94720 United States Bruker Biospin Corp. 15 Fortune Drive BillericaMA01821 United States University of Washington SeattleWA98195 United States New Technologies - Research Centre University of West Bohemia Univerzitní 8 Plzeň306 14 Czech Republic Oden Institute for Computational Engineering and Sciences University of Texas at Austin AustinTX7

SciPy is an open source scientific computing library for the Python programming language. SciPy 1.0 was released in late 2017, about 16 years after the original version 0.1 release. SciPy has become a de facto standard for leveraging scientific algorithms in the Python programming language, with more than 600 unique code contributors, thousands of dependent packages, over 100,000 dependent repositories, and millions of downloads per year. This includes usage of SciPy in almost half of all machine learning projects on GitHub, and usage by high profile projects including LIGO gravitational wave analysis and creation of the first-ever image of a black hole (M87). The library includes functionality spanning clustering, Fourier transforms, integration, interpolation, file I/O, linear algebra, image processing, orthogonal distance regression, minimization algorithms, signal processing, sparse matrix handling, computational geometry, and statistics. In this work, we provide an overview of the capabilities and development practices of the SciPy library and highlight some recent technical developments. Copyright © 2019, The Authors. All rights reserved.

关键词： Open source software

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Author Correction: The SEQC2 epigenomics quality control (EpiQC) study

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Genome biology 2021年第1期22卷 350页

作者： Jonathan Foox Jessica Nordlund Claudia Lalancette Ting Gong Michelle Lacey Samantha Lent Bradley W Langhorst V K Chaithanya Ponnaluri Louise Williams Karthik Ramaswamy Padmanabhan Raymond Cavalcante Anders Lundmark Daniel Butler Christopher Mozsary Justin Gurvitch John M Greally Masako Suzuki Mark Menor Masaki Nasu Alicia Alonso Caroline Sheridan Andreas Scherer Stephen Bruinsma Gosia Golda Agata Muszynska Paweł P Łabaj Matthew A Campbell Frank Wos Amanda Raine Ulrika Liljedahl Tomas Axelsson Charles Wang Zhong Chen Zhaowei Yang Jing Li Xiaopeng Yang Hongwei Wang Ari Melnick Shang Guo Alexander Blume Vedran Franke Inmaculada Ibanez de Caceres Carlos Rodriguez-Antolin Rocio Rosas Justin Wade Davis Jennifer Ishii Dalila B Megherbi Wenming Xiao Will Liao Joshua Xu Huixiao Hong Baitang Ning Weida Tong Altuna Akalin Yunliang Wang Youping Deng Christopher E Mason Department of Physiology and Biophysics Weill Cornell Medicine New York NY USA. The HRH Prince Alwaleed Bin Talal Bin Abdulaziz Alsaud Institute for Computational Biomedicine Weill Cornell Medicine New York NY USA. Department of Medical Sciences and Science for Life Laboratory Uppsala University Uppsala Sweden. EATRIS ERIC- European Infrastructure for Translational Medicine De Boelelaan 1118 1081 HZ Amsterdam The Netherlands. BRCF Epigenomics Core University of Michigan Medicine Ann Arbor MI 48109 USA. Department of Quantitative Health Sciences University of Hawaii John A. Burns School of Medicine Honolulu HI 96813 USA. Tulane University New Orleans LA 70118 USA. AbbVie Genomics Research Center 1 N. Waukegan Rd North Chicago IL 60036 USA. New England Biolabs Ipswich MA 01938 USA. Albert Einstein College of Medicine Bronx NY 10461 USA. Division of Hematology/Oncology Department of Medicine Epigenomics Core Facility Weill Cornell Medicine New York NY USA. Institute for Molecular Medicine Finland (FIMM) University of Helsinki Helsinki Finland. Illumina Inc Madison WI 53705 USA. Faculty of Biochemistry Biophysics and Biotechnology Jagiellonian University Krakow Poland. Małopolska Centre of Biotechnology Jagiellonian University Krakow Poland. New York Genome Center New York NY 10013 USA. Center for Genomics School of Medicine Loma Linda University Loma Linda CA 92350 USA. Department of Allergy and Clinical Immunology State Key Laboratory of Respiratory Disease Guangzhou Institute of Respiratory Health the First Affiliated Hospital of Guangzhou Medical University Guangzhou Guangdong China. Department of Neurology The Second Affiliated Hospital of Zhengzhou University Zhengzhou 450014 China. Development of Medicine the University of Chicago Chicago IL 60637 USA. Department of Neurology the Second Affiliated Hospital of Zhengzhou University Zhengzhou 450014 China. Bioinformatics and Omics Data Science Platform Berlin Institute f

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Stability of Inverse Transport Equation in Diffusion Scaling And Fokker-Planck Limit

arXiv

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arXiv 2017年

作者： Chen, Ke LI, Qin Wang, Li Mathematics Department University of Wisconsin-Madison 480 Lincoln Dr. MadisonWI53705 United States Mathematics Department and Wisconsin Institute of Discovery University of Wisconsin-Madison 480 Lincoln Dr. MadisonWI53705 United States Department of Mathematics Computational and Data-Enabled Science and Engineering Program State University of New York at Buffalo 244 Mathematics Building BuffaloNY14206 United States

We consider the inverse problem of reconstructing the scattering and absorption coefficients using boundary measurements for a time dependent radiative transfer equation (RTE). As the measurement is mostly polluted by errors, both experimental and computational, an important question is to quantify how the error is amplified in the process of reconstruction. In the forward setting, the solution to the RTE behaves differently in different regimes, and the stability of the inverse problem vary accordingly. In particular, we consider two scalings in this paper. The first one concerns with a diffusive scaling whose macroscopic limit is a diffusion equation. In this case, we showed, following the similar approach as in [Chen, Li and Wang, arXiv:1703.00097], that the stability degrades when the limit is taken. The second one considers a highly forward peaked scattering, wherein the scattering operator is approximated by a Fokker-Planck operator as a limit. In this case, we showed that a fully recover of the scattering coefficient is less possible in the limit, whereas obtaining a rescaled version of the scattering coefficient becomes more practice friendly. Copyright © 2017, The Authors. All rights reserved.

关键词： Inverse problems

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A Bluetooth low energy based beacon system for smart short range surveillance

A Bluetooth low energy based beacon system for smart short r...

引用

IEEE International Conference on Recent Trends in Electronics, Information & Communication Technology (RTEICT)

作者： B G Anil Kumar K C Bhagyalakshmi K Lavanya K H Gowranga Department of Computer Science and Engineering Vijaya Vittala Institute of Technology Bangalore India Department of Computational and Data Sciences Indian Institute of Science Bangalore India

ISBN: (纸本)9781509007752

The aim of this paper is to propose a fault-tolerant smart system which can render, track and monitor the process of attendance of students. A smart attendance system is refined in a systematic manner where the students enter the lecture hall with an android device which possesses a beacon compatible mobile app. The main purpose of this system is to minimize the power consumption of Bluetooth using Bluetooth Low Energy (BLE) technology, which prevents fraud and favors in an attendance system by using a Bluetooth smart beacon.

关键词： Bluetooth Radiofrequency identification Smart phones Internet of Things Smart cities databases Fingers

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Development of a fast reactor for minor actinides transmutation - Improvement of prediction accuracy for ma-related integral parameters based on cross-section adjustment technique

Development of a fast reactor for minor actinides transmutat...

引用

Physics of Reactors 2016: Unifying Theory and Experiments in the 21st Century, PHYSOR 2016

作者： Yokoyama, Kenji Maruyama, Shuhei Numata, Kazuyuki Ishikawa, Makoto Takeda, Toshikazu Nuclear Data and Reactor Engineering Division Nuclear Science and Engineering Center Japan Atomic Energy Agency Ibaraki Japan Research Institute of Nuclear Engineering University of Fukui Fukui Japan Fast Reactor Computational Engineering Department Advanced Fast Reactor Cycle System Research and Development Center Japan Atomic Energy Agency Ibaraki Japan

ISBN: (纸本)9781510825734

In order to improve the prediction accuracy of the minor actinide transmutation in fast reactors, the cross-section adjustment technique was applied. In the present study, we utilized the MA-related integral experimental data that were extensively collected and evaluated in detail as a part of the ongoing project "Study on Minor Actinides Transmutation Using Monju data." This is one of the national projects entitled "technology development for the environmental burden reduction," which has been launched by MEXT (Ministry of Education, Culture, Sports, science and Technology) in Japan. Those data include neutronics parameters, such as the criticality and the sodium void reactivity measured in massively Np-loaded cores, MA fission reaction rate ratios measured in fast critical assemblies, MA samples irradiated in fast reactors, and neutronics parameters measured in an 241Am-accumulated fast breeder reactor. These MA-related integral experimental data were applied to the cross-section adjustment with the existing general, i.e., non-MA-related experimental data. For the criticality and sodium void reactivity, significant improvement of prediction accuracy is seen both for the cores with MA and without MA. As for the fission rate ratios, the cross-section adjustment result suggests the large reduction of 244Cm fission cross section.

关键词： Fast reactors

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Breast Cancer Risk Genes-Association Analysis in More than 113,000 Women

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四川生理科学杂志 2021年第1期43卷 7-7页

作者： Leila Dorling The authors' affiliations are as follows: the Centre for Cancer Genetic Epidemiology Departments of Public Health and Primary Care (L.D. S. Carvalho J.A. K.A.P. Q.W. M.K.B. J.D. B.D. N. Mavaddat K. Michailidou A.C.A. P.D.P.P. D.F.E.) and Oncology (C.L. P.A.H. C. Baynes D.M.C. L.F. V.R. M. Shah P.D.P.P. A.M.D. D.F.E.) University of Cambridge Cambridge the Centre for Genomic and Experimental Medicine MRC Institute of Genetics and Molecular Medicine (A. Campbell D.J.P.) and the Centre for Cognitive Ageing and Cognitive Epidemiology Department of Psychology (D.J.P.) University of Edinburgh the Cancer Research UK Edinburgh Centre (D.A.C. J.F.) and the Usher Institute of Population Health Sciences and Informatics University of Edinburgh Medical School (A. Campbell J.F.) Edinburgh the Divisions of Informatics Imaging and Data Sciences (E.F.H.) Cancer Sciences (A. Howell) Population Health Health Services Research and Primary Care (A. Lophatananon K. Muir) and Evolution and Genomic Sciences School of Biological Sciences (W.G.N. E.M.V. D.G.E.) University of Manchester the NIHR Manchester Biomedical Research Unit (E.F.H.) and the Nightingale Breast Screening Centre Wythenshawe Hospital (E.F.H. H.I.) Academic Health Science Centre and North West Genomics Laboratory Hub and the Manchester Centre for Genomic Medicine St. Mary's Hospital Manchester University NHS Foundation Trust (W.G.N. E.M.V. D.G.E.) Manchester the School of Cancer and Pharmaceutical Sciences Comprehensive Cancer Centre Guy's Campus King's College London London (E.J.S.) the Institute of Cancer and Genomic Sciences University of Birmingham Birmingham (I.T.) and the Wellcome Trust Centre for Human Genetics and Oxford NIHR Biomedical Research Centre University of Oxford Oxford (I.T.) - all in the United Kingdom the Human Genotyping-CEGEN Unit Human Cancer Genetic Program (A.G.-N. M.R.A. N.Á. B.H. R.N.-T.) and the Human Genetics Group (V.F. A.O. J.B.) Spanish National Cancer Research

Background:Genetic testing for breast cancer susceptibility is widely used,but for many genes,evidence of an association with breast cancer is weak,underlying risk estimates are imprecise,and reliable subtype-specific risk estimates are ***:We used a panel of 34 putative susceptibility genes to perform sequencing on samples from 60,466 women with breast cancer and 53,461 *** separate analyses for protein-truncating variants and rare missense variants in these genes,we estimated odds ratios for breast cancer overall and tumor *** evaluated missense-variant associations according to domain and classification of pathogenicity.

关键词： cancer Breast Cancer

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Correction to: A CCR5+ memory subset within HIV-1-infected primary resting CD4+ T cells is permissive for replication-competent, latently infected viruses in vitro

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BMC research notes 2019年第1期12卷 322页

作者： Kazutaka Terahara Ryutaro Iwabuchi Masahito Hosokawa Yohei Nishikawa Haruko Takeyama Yoshimasa Takahashi Yasuko Tsunetsugu-Yokota Department of Immunology National Institute of Infectious Diseases 1-23-1 Toyama Shinjuku-ku Tokyo 162-8640 Japan. tera@nih.go.jp. Department of Immunology National Institute of Infectious Diseases 1-23-1 Toyama Shinjuku-ku Tokyo 162-8640 Japan. Department of Life Science and Medical Bioscience Waseda University 2-2 Wakamatsu-cho Shinjuku-ku Tokyo 162-8480 Japan. Computational Bio Big-Data Open Innovation Laboratory National Institute of Advanced Industrial Science and Technology 3-4-1 Okubo Shinjuku-ku Tokyo 169-8555 Japan. Research Organization for Nano & Life Innovation Waseda University 513 Wasedatsurumaki-cho Shinjuku-ku Tokyo 162-0041 Japan. Institute for Advanced Research of Biosystem Dynamics Waseda Research Institute for Science and Engineering Waseda University 2-2 Wakamatsu-cho Shinjuku-ku Tokyo 162-8480 Japan. Department of Medical Technology School of Human Sciences Tokyo University of Technology 5-23-22 Nishikamata Ota-ku Tokyo 144-8535 Japan.

After publication of the original article [1], the authors became aware of a miscalculation in the original Fig. 2d.

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Advances in understanding high-mass X-ray binaries with INTEGRAL and Future Directions

arXiv

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arXiv 2020年

作者： Kretschmar, Peter Fürst, Felix Sidoli, Lara Bozzo, Enrico Alfonso-Garzón, Julia Bodaghee, Arash Chaty, Sylvain Chernyakova, Masha Ferrigno, Carlo Manousakis, Antonios Negueruela, Ignacio Postnov, Konstantin Paizis, Adamantia Reig, Pablo Rodes-Roca, José Joaquín Tsygankov, Sergey Bird, Antony J. né Kühnel, Matthias Bissinger Blay, Pere Caballero, Isabel Coe, Malcolm J. Domingo, Albert Doroshenko, Victor Ducci, Lorenzo Falanga, Maurizio Grebenev, Sergei A. Grinberg, Victoria Hemphill, Paul Kreykenbohm, Ingo née Fritz, Sonja Kreykenbohm Li, Jian Lutovinov, Alexander A. Martínez-Núñez, Silvia Mas-Hesse, J. Miguel Masetti, Nicola McBride, Vanessa A. Neronov, Andrii Pottschmidt, Katja Rodriguez, Jérôme Romano, Patrizia Rothschild, Richard E. Santangelo, Andrea Sguera, Vito Staubert, Rüdiger Tomsick, John A. Torrejón, José Miguel Torres, Diego F. Walter, Roland Wilms, Jörn Wilson-Hodge, Colleen A. Zhang, Shu E-28692 Spain E-28692 Spain INAF - IASF Istituto di Astrofisica Spaziale e Fisica Cosmica Via A. Corti 12 MilanoI-20133 Italy Department of Astronomy ISDC University of Geneva Chemin d'Ecogia 16 VersoixCH-1290 Switzerland E-28692 Spain Department of Chemistry Physics and Astronomy Georgia College and State University MilledgevilleGA31061 United States AIM CEA CNRS Université Paris-Saclay Université de Paris Gif-sur-YvetteF-91191 France Université de Paris CNRS Astroparticule et Cosmologie ParisF-75006 France School of Physical Sciences and CfAR Dublin City University Dublin 9 Ireland Dublin Institute for Advanced Studies 31 Fitzwilliam Place Dublin 2 Ireland Department of Applied Physics & Astronomy University of Sharjah Sharjah United Arab Emirates Sharjah United Arab Emirates Department of Applied Physics University of Alicante AlicanteE-03080 Spain Sternberg Astronomical Institute Moscow State University Moscow119234 Russia Kazan Federal University Kazan Russia Institute of Astrophysics Foundation for Research and Technology-Hellas Heraklion Crete71110 Greece University of Crete Physics Department Institute of Theoretical & Computational Physics Heraklion Crete70013 Greece Department of Physics Systems Engineering and Signal Theory University of Alicante AlicanteE-03690 Spain University Institute of Physics Applied to Sciences and Technologies University of Alicante AlicanteE-03690 Spain Department of Physics and Astronomy University of Turku FI-20014 Finland Space Research Institute The Russian Academy of Sciences Profsoyuznaya Str. 84/32 Moscow117997 Russia School of Physics and Astronomy Faculty of Physical Sciences and Engineering University of Southampton SouthamptonSO17 1BJ United Kingdom Erwin-Rommel-Strae 1 Erlangen91058 Germany Universidad Internacional de Valencia - VIU C/Pintor Sorolla 21 Valencia46002 Spain E-28692 Spain Institut für Astronomie und Astrophysik Universität Tübingen Sand 1 Tübingen

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology, they have attracted the interest of the high energy astrophysical community since the dawn of X-ray Astronomy. In more recent years, they have challenged our comprehension of physical processes in many more energy bands, ranging from the infrared to very high energies. In this review, we provide a broad but concise summary of the physical processes dominating the emission from high mass X-ray binaries across virtually the whole electromagnetic spectrum. These comprise the interaction of stellar winds with the high gravitational and magnetic fields of compact objects, the behaviour of matter under extreme magnetic and gravity conditions, and the perturbation of the massive star evolutionary processes by presence in a binary system. We highlight the role of the INTEGRAL mission in the discovery of many of the most interesting objects in the high mass X-ray binary class and its contribution in reviving the interest for these sources over the past two decades. We show how the INTEGRAL discoveries have not only contributed to significantly increase the number of high mass X-ray binaries known, thus advancing our understanding of the population as a whole, but also have opened new windows of investigation that stimulated the multi-wavelength approach nowadays common in most astrophysical research fields. We conclude the review by providing an overview of future facilities being planned from the X-ray to the very high energy domain that will hopefully help us in finding an answer to the many questions left open after more than 18 years of INTEGRAL scientific observations. Copyright © 2020, The Authors. All rights reserved.

关键词： Galaxies

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