The Boundaries of Knowledge in Buddhism, Christianity and Science
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Using Concrete Scales: a Practical Framework for Effective Visual Depiction of Complex Measures Fanny Chevalier, Romain Vuillemot, Guia Gali
Using Concrete Scales: A Practical Framework for Effective Visual Depiction of Complex Measures Fanny Chevalier, Romain Vuillemot, Guia Gali To cite this version: Fanny Chevalier, Romain Vuillemot, Guia Gali. Using Concrete Scales: A Practical Framework for Effective Visual Depiction of Complex Measures. IEEE Transactions on Visualization and Computer Graphics, Institute of Electrical and Electronics Engineers, 2013, 19 (12), pp.2426-2435. 10.1109/TVCG.2013.210. hal-00851733v1 HAL Id: hal-00851733 https://hal.inria.fr/hal-00851733v1 Submitted on 8 Jan 2014 (v1), last revised 8 Jan 2014 (v2) HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Using Concrete Scales: A Practical Framework for Effective Visual Depiction of Complex Measures Fanny Chevalier, Romain Vuillemot, and Guia Gali a b c Fig. 1. Illustrates popular representations of complex measures: (a) US Debt (Oto Godfrey, Demonocracy.info, 2011) explains the gravity of a 115 trillion dollar debt by progressively stacking 100 dollar bills next to familiar objects like an average-sized human, sports fields, or iconic New York city buildings [15] (b) Sugar stacks (adapted from SugarStacks.com) compares caloric counts contained in various foods and drinks using sugar cubes [32] and (c) How much water is on Earth? (Jack Cook, Woods Hole Oceanographic Institution and Howard Perlman, USGS, 2010) shows the volume of oceans and rivers as spheres whose sizes can be compared to that of Earth [38]. -
Detection of PAH and Far-Infrared Emission from the Cosmic Eye
Accepted for publication in ApJ A Preprint typeset using LTEX style emulateapj v. 08/22/09 DETECTION OF PAH AND FAR-INFRARED EMISSION FROM THE COSMIC EYE: PROBING THE DUST AND STAR FORMATION OF LYMAN BREAK GALAXIES B. Siana1, Ian Smail2, A. M. Swinbank2, J. Richard2, H. I. Teplitz3, K. E. K. Coppin2, R. S. Ellis1, D. P. Stark4, J.-P. Kneib5, A. C. Edge2 Accepted for publication in ApJ ABSTRACT ∗ We report the results of a Spitzer infrared study of the Cosmic Eye, a strongly lensed, LUV Lyman Break Galaxy (LBG) at z =3.074. We obtained Spitzer IRS spectroscopy as well as MIPS 24 and 70 µm photometry. The Eye is detected with high significance at both 24 and 70 µm and, when including +4.7 11 a flux limit at 3.5 mm, we estimate an infrared luminosity of LIR = 8.3−4.4 × 10 L⊙ assuming a magnification of 28±3. This LIR is eight times lower than that predicted from the rest-frame UV properties assuming a Calzetti reddening law. This has also been observed in other young LBGs, and indicates that the dust reddening law may be steeper in these galaxies. The mid-IR spectrum shows strong PAH emission at 6.2 and 7.7 µm, with equivalent widths near the maximum values observed in star-forming galaxies at any redshift. The LP AH -to-LIR ratio lies close to the relation measured in local starbursts. Therefore, LP AH or LMIR may be used to estimate LIR and thus, star formation rate, of LBGs, whose fluxes at longer wavelengths are typically below current confusion limits. -
Close-Up View of a Luminous Star-Forming Galaxy at Z = 2.95 S
Close-up view of a luminous star-forming galaxy at z = 2.95 S. Berta, A. J. Young, P. Cox, R. Neri, B. M. Jones, A. J. Baker, A. Omont, L. Dunne, A. Carnero Rosell, L. Marchetti, et al. To cite this version: S. Berta, A. J. Young, P. Cox, R. Neri, B. M. Jones, et al.. Close-up view of a luminous star- forming galaxy at z = 2.95. Astronomy and Astrophysics - A&A, EDP Sciences, 2021, 646, pp.A122. 10.1051/0004-6361/202039743. hal-03147428 HAL Id: hal-03147428 https://hal.archives-ouvertes.fr/hal-03147428 Submitted on 19 Feb 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A&A 646, A122 (2021) Astronomy https://doi.org/10.1051/0004-6361/202039743 & c S. Berta et al. 2021 Astrophysics Close-up view of a luminous star-forming galaxy at z = 2.95? S. Berta1, A. J. Young2, P. Cox3, R. Neri1, B. M. Jones4, A. J. Baker2, A. Omont3, L. Dunne5, A. Carnero Rosell6,7, L. Marchetti8,9,10 , M. Negrello5, C. Yang11, D. A. Riechers12,13, H. Dannerbauer6,7, I. -
Shwe U Daung and the Burmese Sherlock Holmes: to Be a Modern Burmese Citizen Living in a Nation‐State, 1889 – 1962
Shwe U Daung and the Burmese Sherlock Holmes: To be a modern Burmese citizen living in a nation‐state, 1889 – 1962 Yuri Takahashi Southeast Asian Studies School of Languages and Cultures Faculty of Arts and Social Sciences The University of Sydney April 2017 A thesis submitted in fulfilment of requirements for the degree of Doctor of Philosophy Statement of originality This is to certify that to the best of my knowledge, the content of this thesis is my own work. This thesis has not been submitted for any degree or other purposes. I certify that the intellectual content of this thesis is the product of my own work and that all the assistance received in preparing this thesis and sources has been acknowledged. Yuri Takahashi 2 April 2017 CONTENTS page Acknowledgements i Notes vi Abstract vii Figures ix Introduction 1 Chapter 1 Biography Writing as History and Shwe U Daung 20 Chapter 2 A Family after the Fall of Mandalay: Shwe U Daung’s Childhood and School Life 44 Chapter 3 Education, Occupation and Marriage 67 Chapter ‘San Shar the Detective’ and Burmese Society between 1917 and 1930 88 Chapter 5 ‘San Shar the Detective’ and Burmese Society between 1930 and 1945 114 Chapter 6 ‘San Shar the Detective’ and Burmese Society between 1945 and 1962 140 Conclusion 166 Appendix 1 A biography of Shwe U Daung 172 Appendix 2 Translation of Pyone Cho’s Buddhist songs 175 Bibliography 193 i ACKNOWLEGEMENTS I came across Shwe U Daung’s name quite a long time ago in a class on the history of Burmese literature at Tokyo University of Foreign Studies. -
The Fundamentals of Meditation Practice
TheThe FundamentalsFundamentals ofof MeditationMeditation PracticePractice by Ting Chen Translated by Dharma Master Lok To HAN DD ET U 'S B B O RY eOK LIBRA E-mail: [email protected] Web site: www.buddhanet.net Buddha Dharma Education Association Inc. The Fundamentals of Meditation Practice by Ting Chen Translated by Dharma Master Lok To Edited by Sam Landberg & Dr. Frank G. French 2 Transfer-of-Merit Vow (Parinamana) For All Donors May all the merit and grace gained from adorning Buddha’s Pure Land, from loving our parents, from serving our country and from respecting all sen- tient beings be transformed and transferred for the benefit and salvation of all suffering sentient be- ings on the three evil paths. Furthermore, may we who read and hear this Buddhadharma and, there- after, generate our Bodhi Minds be reborn, at the end of our lives, in the Pure Land. Sutra Translation Committee of the United States and Canada, 1999 — website: http://www.ymba.org/freebooks_main.html Acknowledgments We respectfully acknowledge the assistance, support and cooperation of the following advisors, without whom this book could not have been produced: Dayi Shi; Chuanbai Shi; Dr. John Chen; Amado Li; Cherry Li; Hoi-Sang Yu; Tsai Ping Chiang; Vera Man; Way Zen; Jack Lin; Tony Aromando; and Ling Wang. They are all to be thanked for editing and clarifying the text, sharpening the translation and preparing the manuscript for publication. Their devotion to and concentration on the completion of this project, on a voluntary basis, are highly appreciated. 3 Contents • Translator’s Introduction...................... 5 • The Foundation of Meditation Practice. -
Ast110fall2015-Labmanual.Pdf
2015/2016 (http://astronomy.nmsu.edu/astro/Ast110Fall2015.pdf) 1 2 Contents 1IntroductiontotheAstronomy110Labs 5 2TheOriginoftheSeasons 21 3TheSurfaceoftheMoon 41 4ShapingSurfacesintheSolarSystem:TheImpactsofCometsand Asteroids 55 5IntroductiontotheGeologyoftheTerrestrialPlanets 69 6Kepler’sLawsandGravitation 87 7TheOrbitofMercury 107 8MeasuringDistancesUsingParallax 121 9Optics 135 10 The Power of Light: Understanding Spectroscopy 151 11 Our Sun 169 12 The Hertzsprung-Russell Diagram 187 3 13 Mapping the Galaxy 203 14 Galaxy Morphology 219 15 How Many Galaxies Are There in the Universe? 241 16 Hubble’s Law: Finding the Age of the Universe 255 17 World-Wide Web (Extra-credit/Make-up) Exercise 269 AFundamentalQuantities 271 BAccuracyandSignificantDigits 273 CUnitConversions 274 DUncertaintiesandErrors 276 4 Name: Lab 1 Introduction to the Astronomy 110 Labs 1.1 Introduction Astronomy is a physical science. Just like biology, chemistry, geology, and physics, as- tronomers collect data, analyze that data, attempt to understand the object/subject they are looking at, and submit their results for publication. Along thewayas- tronomers use all of the mathematical techniques and physics necessary to understand the objects they examine. Thus, just like any other science, a largenumberofmath- ematical tools and concepts are needed to perform astronomical research. In today’s introductory lab, you will review and learn some of the most basic concepts neces- sary to enable you to successfully complete the various laboratory exercises you will encounter later this semester. When needed, the weekly laboratory exercise you are performing will refer back to the examples in this introduction—so keep the worked examples you will do today with you at all times during the semester to use as a refer- ence when you run into these exercises later this semester (in fact, on some occasions your TA might have you redo one of the sections of this lab for review purposes). -
12 Strong Gravitational Lenses
12 Strong Gravitational Lenses Phil Marshall, MaruˇsaBradaˇc,George Chartas, Gregory Dobler, Ard´ısEl´ıasd´ottir,´ Emilio Falco, Chris Fassnacht, James Jee, Charles Keeton, Masamune Oguri, Anthony Tyson LSST will contain more strong gravitational lensing events than any other survey preceding it, and will monitor them all at a cadence of a few days to a few weeks. Concurrent space-based optical or perhaps ground-based surveys may provide higher resolution imaging: the biggest advances in strong lensing science made with LSST will be in those areas that benefit most from the large volume and the high accuracy, multi-filter time series. In this chapter we propose an array of science projects that fit this bill. We first provide a brief introduction to the basic physics of gravitational lensing, focusing on the formation of multiple images: the strong lensing regime. Further description of lensing phenomena will be provided as they arise throughout the chapter. We then make some predictions for the properties of samples of lenses of various kinds we can expect to discover with LSST: their numbers and distributions in redshift, image separation, and so on. This is important, since the principal step forward provided by LSST will be one of lens sample size, and the extent to which new lensing science projects will be enabled depends very much on the samples generated. From § 12.3 onwards we introduce the proposed LSST science projects. This is by no means an exhaustive list, but should serve as a good starting point for investigators looking to exploit the strong lensing phenomenon with LSST. -
12.748 Lecture 2 Cosmic Abundances, Nucleosynthesis and Element Origins
12.748 Lecture 2 Cosmic Abundances, Nucleosynthesis and Element Origins Our intent is to shed further light on the reasons for the abundance of the elements. We made progress in this regard when we discussed nuclear stability and nuclear binding energy explaining the zigzag structure, along with the broad maxima around Iron and Lead. The overall decrease with mass, however, arises from the creation of the universe, and the fact that the universe started out with only the most primitive building blocks of matter, namely electrons, protons and neutrons. The initial explosion that created the universe created a rather bland mixture of just hydrogen, a little helium, and an even smaller amount of lithium. The other elements were built from successive generations of star formation and death. The Origin of the Universe It is generally accepted that the universe began with a bang, not a whimper, some 15 billion years ago. The two most convincing lines of evidence that this is the case are observation of • the Hubble expansion: objects are receding at a rate proportional to their distance • the cosmic microwave background (CMB): an almost perfectly isotropic black-body spectrum Isotopes 12.748 Lecture 2: Cosmic Abundances, Nucleosynthesis and Element Origins 1 In the initial fraction of a second, the temperature is so hot that even subatomic particles like neutrons, electrons and protons fall apart into their constituent pieces (quarks and gluons). These temperatures are well beyond anything achievable in the universe since. As the fireball expands, the temperature drops, and progressively higher-level particles are manufactured. By the end of the first second, the temperature has dropped to a mere billion degrees or so, and things are starting to get a little more normal: electrons, neutrons and protons can now exist. -
Buddhist-Christian Dialogue As Theological Exchange an Orthodox Contribution to Comparative Eology
199 West 8th Avenue, Suite 3, Eugene, OR 97401 PICKWICK Publications Tel. (541) 344-1528 • Fax (541) 344-1506 An imprint of WIPF and STOCK Publishers Visit our Web site at www.wipfandstock.com Buddhist-Christian Dialogue as Theological Exchange An Orthodox Contribution to Comparative eology Ernest M. Valea is book is intended to encourage the use of comparative theology in contemporary Buddhist-Christian dialogue as a new approach that would truly respect each religious tradition’s uniqueness and make dialogue beneficial for all participants interested in a real theological exchange. As a result of the impasse reached by the current theologies of religions (exclusivism, inclusivism, and pluralism) in formulating a constructive approach in dialogue, this volume assesses the thought of the founding fathers of an academic Buddhist-Christian dialogue in search of clues that would encourage a comparativist approach. ese founding fathers are considered to be three important representatives of the Kyoto School—Kitaro Nishida, Keiji Nishitani, and Masao Abe—and John Cobb, an American process theologian. e guiding line for assessing their views of dialogue is the concept of human perfection, as it is expressed by the original traditions in Mahayana Buddhism and Orthodox Christianity. Following Abe’s methodology in dialogue, an Orthodox contribu- tion to comparative theology proposes a reciprocal enrichment of traditions, not by syncretistic means, but by providing a better understanding and even correction of one’s own tradition when considering it in the light of the other, while using internal resources for making the necessary corrections. ISBN: 978-1-4982-2119-1 | 262 pp. -
ASTR110G Astronomy Laboratory Exercises C the GEAS Project 2020
ASTR110G Astronomy Laboratory Exercises c The GEAS Project 2020 ASTR110G Laboratory Exercises Lab 1: Fundamentals of Measurement and Error Analysis ...... ....................... 1 Lab 2: Observing the Sky ............................... ............................. 35 Lab 3: Cratering and the Lunar Surface ................... ........................... 73 Lab 4: Cratering and the Martian Surface ................. ........................... 97 Lab 5: Parallax Measurements and Determining Distances ... ....................... 129 Lab 6: The Hertzsprung-Russell Diagram and Stellar Evolution ..................... 157 Lab 7: Hubble’s Law and the Cosmic Distance Scale ........... ..................... 185 Lab 8: Properties of Galaxies .......................... ............................. 213 Appendix I: Definitions for Keywords ..................... .......................... 249 Appendix II: Supplies ................................. .............................. 263 Lab 1 Fundamentals of Measurement and Error Analysis 1.1 Introduction This laboratory exercise will serve as an introduction to all of the laboratory exercises for this course. We will explore proper techniques for obtaining and analyzing data, and practice plotting and analyzing data. We will discuss a scientific methodology for conducting exper- iments in which we formulate a question, predict the behavior of the system based on likely solutions, acquire relevant data, and then compare our predictions with the observations. You will have a chance to plan a short experiment, -
A Buddhist Inspiration for a Contemporary Psychotherapy
1 A BUDDHIST INSPIRATION FOR A CONTEMPORARY PSYCHOTHERAPY Gay Watson Thesis presented for the degree of Doctor of Philosophy at the School of Oriental & African Studies, University of London. 1996 ProQuest Number: 10731695 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a com plete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest ProQuest 10731695 Published by ProQuest LLC(2017). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States C ode Microform Edition © ProQuest LLC. ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 48106- 1346 ABSTRACT It is almost exactly one hundred years since the popular and not merely academic dissemination of Buddhism in the West began. During this time a dialogue has grown up between Buddhism and the Western discipline of psychotherapy. It is the contention of this work that Buddhist philosophy and praxis have much to offer a contemporary psychotherapy. Firstly, in general, for its long history of the experiential exploration of mind and for the practices of cultivation based thereon, and secondly, more specifically, for the relevance and resonance of specific Buddhist doctrines to contemporary problematics. Thus, this work attempts, on the basis of a three-way conversation between Buddhism, psychotherapy and various themes from contemporary discourse, to suggest a psychotherapy that may be helpful and relevant to the current horizons of thought and contemporary psychopathologies which are substantially different from those prevalent at the time of psychotherapy's early years. -
Aspects of the Study of the (Earlier) Indian Mahāyāna
JIABS Journal of the International Association of Buddhist Studies Volume 27 Number 1 2004 David SEYFORT RUEGG Aspects of the Investigation of the (earlier) Indian Mahayana....... 3 Giulio AGOSTINI Buddhist Sources on Feticide as Distinct from Homicide ............... 63 Alexander WYNNE The Oral Transmission of the Early Buddhist Literature ................ 97 Robert MAYER Pelliot tibétain 349: A Dunhuang Tibetan Text on rDo rje Phur pa 129 Sam VAN SCHAIK The Early Days of the Great Perfection........................................... 165 Charles MÜLLER The Yogacara Two Hindrances and their Reinterpretations in East Asia.................................................................................................... 207 Book Review Kurt A. BEHRENDT, The Buddhist Architecture of Gandhara. Handbuch der Orientalistik, section II, India, volume seventeen, Brill, Leiden-Boston, 2004 by Gérard FUSSMAN............................................................................. 237 Notes on the Contributors............................................................................ 251 ASPECTS OF THE STUDY OF THE (EARLIER) INDIAN MAHAYANA* D. SEYFORT RUEGG Il est aussi facile dans l’Inde de constater des prolongements que malaisé d’assister à des ruptures. (L. Renou, Études védiques et pa∞inéennes, tome VI [Paris, 1960], p. 11) Proem As a continuation of his monumental Histoire du bouddhisme indien, published in 1958, Étienne Lamotte once envisaged writing a second volume to be devoted to the Indian Mahayana. This second part was, however,