Highlighting Entanglement of Cultures Via Ranking of Multilingual Wikipedia Articles
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23 Minor Planet Bulletin 41
23 observation interval. The overall form of the lightcurve did not of the other observatories. To make the large number of data points change perceptibly with phase angle or viewing aspect. in the segments of the lightcurve included by Organ Mesa observations more legible, those data have been binned in sets of Further evidence against the double period near 72.6 hours is five points with a maximum of ten minutes between points. provided by Schober et al. (1993). They draw a composite bimodal lightcurve phased to 36.0 hours based on data from 6 consecutive References nights with about 60% phase coverage. Overlapping sessions on this lightcurve centered near 1989 Nov 30.3 and Dec 3.3 each Behrend, R. (2005). Observatoire de Geneve web site. show a small rise followed by a fall greater than 0.4 magnitudes in http://obswww.unige.ch/~behrend/page_cou.html about 6 hours. This sets a lower limit in their data for the amplitude. An amplitude as large as 0.4 magnitudes is possible Higgins, D.J., Menke, J., Pozzoli, V., Sheridan, E., and Dymock, only for a bimodal lightcurve. R. (2004). “Lightcurve and Period Determination for 582 Olympia.” Minor Planet Bull. 31, 12. Independently, Franco drew an H-G plot based only on sparse data from the U.S. Naval Observatory (USNO), i.e., not including any JPL (2013). http://ssd.jpl.nasa.gov/sbdb.cgi of the new photometry. These data contain no correction for rotational variation and in include the inherent scatter in the USNO Menke, J. (2011). Menke Scientific, Ltd. -
The Warped Ways of Cosmic Light
BIOLOGIE & MEDIZIN_Infektionsbiologie “Around that area there are indeed numerous small nebulous patches so close together that, upon seeing the region, one is positively startled by the strange appearance of this ‘nebula cluster’.” This was the sentiment expressed by Heidelberg-based astronomer Max Wolf in 1901 about the galaxy cluster in the constellation Coma Berenices. The cluster Abell 2218 presents a similar appearance to the viewer today on this image from the Hubble Space Telescope. The “strange appearance” – the many blue and orange arcs – owes, in this case, to the effect of a gravitational lens. PHYSICS & ASTRONOMY_Gravitational Lenses The Warped Ways of Cosmic Light Albert Einstein predicted them, modern giant telescopes detected them – and Klaus Dolag simulates them on a computer: gravitational lenses. The academic staff member at the Max Planck Institute for Astrophysics in Garching and at the University Observatory Munich uses this physical phenomenon to such ends as weighing galaxy clusters and probing that ominous substance known as dark matter. TEXT HELMUT HORNUNG he sky over Principe was a total eclipse of the Sun. The test was More recent analyses of Eddington’s cloudy and the mood in the simple: if a massive object bends space, findings show that the values measured camp on the coconut plan- then the Sun must also cause the pass- at that time did, indeed, correspond to tation had hit rock bottom. ing light from stars to deviate from its the prediction, but that they are appar- Having set out from Eng- straight course. In other words, the ently the result of an instrument error T land, the men had been traveling for points of light in the immediate vicin- of, as it so happens, the very same mag- weeks to reach the volcanic island in ity of the black Sun should be shifted nitude. -
Trojan Search at ESO E
Lf) provide an effective method (a) to dis Kron and A Renzini, (Dordrecht: Reidel), o criminate galaxy morphology, (b) to p.61. evaluate their intrinsic evolution and (c) Buzzoni, A: 1988, in preparation. Butcher, H. and Oemler, A.: 1984, Ap. J., 285, to estimate redshift with an accuracy of 426. 0.05. We emphasize that two main ± Coleman, G.D., Wu, C. C. and Weedman, ...--...0 requirements have to be fulfilled in order Q() D. W.: 1980, Ap. J. Supp., 43, 393. <\l to reach such a fair resolution in explor Couch, W.J. and Newell, E. B.: 1984, Ap. J., E ing the universe at large distances: 56,143. '-' <J Lf) (i) we need to observe clusters instead Couch, W.J., Ellis, R.S., Godwin, J. and Car o o of field galaxies to be able to recognize ter, 0.: 1983, MN.R.A.S., 205,1287. them with high statistical confidence; Ellis, R. S., Couch, W. J., Maclaren, I. and (ii) we need a combined comparison Koo, D.C.: 1985, MN.R.A.S., 217, 239. 2158+0351 Gunn, J. E., Hoessel, I. G. and Oke, J. B.: with evolutionary models, in order to 1986, Ap. J., 306, 30. properly account for the intrinsic photo Koo, D. C.: 1981, Ap. J. (Lett), 251, L 75. 0.4 0.5 metric properties as we use galaxies as Loh, E.D. and Spillar, E.J.: 1986, Ap. J., 303, REDSHI8 T standard candles in the cosmological 154. Figure 8: The photometrie determination of framework. Maclaren, 1., Ellis, R.S. and Couch, W.J.: the redshift of the cluster 2158 + 0351. -
The Internal Structure of the Asteroids
**FULL TITLE** ASP Conference Series, Vol. **VOLUME**, **YEAR OF PUBLICATION** **NAMES OF EDITORS** The internal structure of the asteroids V.Celebonovi´cˇ Inst.of Physics,Pregrevica 118,11080 Zemun-Beograd,Serbia Abstract. Knowledge of the internal structure of the asteroids is rather poorly developed,mainly due to lack of reliable data (masses or densities and radii). This contribution has two aims: to review the basics of existing knowledge and explore the possibility of advancing the field by introducing and using in it some well known ideas from solid state physics. 1. Introduction The largest part of astronomical research directly relies on data taken at various kinds of telescopes of variable size - from those having mirrors of 8 or 10 meters in diameter to backyard amateur telescopes. However,serious comlications arise when one attempts to gain information on the internal structure of any kind of celestial bodies. The reason for these complications is simple: the interiors of any kind of objects are unobservable. For example, nobody has ever gone (and nobody ever will) into the center of Jupiter to measure the temperature there. Surfaces of many kinds of objects are observable. However, the ”state” of a surface of any given object is a consequence of at least two factors: processes occuring in the interior of the object but also of any possible external influences. The aim of this lecture is to discuss to some extent one particular ”subfield” within the field of modelling of the internal structure of celestial objects - the internal structure of the asteroids. Apart from the introduction,this contribution has three more parts. -
Frank Schlesinger 1871-1943
NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XXIV THIRD MEMOIR BIOGRAPHICAL MEMOIR OF FRANK SCHLESINGER 1871-1943 BY DIRK BROUWER PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1945 FRANK SCHLESINGER 1871-1943 BY DIRK BROUWER Frank Schlesinger was born in New York City on May n, 1871. His father, William Joseph Schlesinger (1836-1880), and his mother, Mary Wagner Schlesinger (1832-1892), both natives of the German province of Silesia, had emigrated to the United States. In Silesia they had lived in neighboring vil- lages, but they did not know each other until they met in New York, in 1855, at the home of Mary's cousin. They were mar- ried in 1857 and had seven children, all of whom grew to maturity. Frank was the youngest and, after 1939, the last survivor. His father's death, in 1880, although it brought hardships to the family, was not permitted to interfere with Frank's educa- tion. He attended public school in New York City, and eventually entered the College of the City of New York, receiv- ing the degree of Bachelor of Science in 1890. His aptitude for mathematical science, already evident in grammar school, be- came more marked in the higher stages of his education when he began to show a preference for applied mathematics. Upon completing his undergraduate work it was not possible for him to continue with graduate studies. He had to support himself, and his health at that time made it desirable for him to engage in outdoor activities. -
Harold Knox-Shaw and the Helwan Observatory
1 Harold Knox-Shaw and the Helwan Observatory Jeremy Shears & Ashraf Ahmed Shaker Abstract Harold Knox-Shaw (1885-1970) worked at the Helwan Observatory in Egypt from 1907 to 1924. The Observatory was equipped with a 30-inch (76 cm) reflector that was financed and constructed by the Birmingham industrialist, John Reynolds (1874- 1949), to benefit from the clearer skies and more southerly latitude compared with Britain. Knox-Shaw obtained the first photograph of Halley’s Comet on its 1910 perihelion passage. He also carried out morphological studies on nebulae and may have been the first to identify what later became to be known as elliptical galaxies as a distinct class of object. Photographic analysis of the variable nebula NGC 6729 in Corona Australis enabled him to conclude that the changes in brightness and shape were correlated with the light travel time from the illuminating star, R CrA. Introduction By the beginning of the twentieth century fundamental changes in astronomy were well-advanced, with a move from a traditional positional and descriptive approach to the new science of astrophysics. This was driven by the development of two new tools: spectroscopy and photography. In Great Britain the chief practitioners of the science were no longer the self-taught individuals of independent wealth, the Grand Amateurs of the Victorian age, but increasingly they were University-trained scientists employed by professional research institutions (1). Across the Atlantic, the United States was making great strides in the development of the new astronomy. Here, in the first two decades of the twentieth century increasingly large telescopes were being built to generate astrophysical data, such as the giant reflectors on Mount Wilson which benefitted from the clear skies and southerly latitudes of California. -
Dictionary of Slovenian Exonyms Explanatory Notes
GEOGRAFSKI INŠTITUT ANTONA MELIKA ZNANSTVENORAZISKOVALNI CENTER SLOVENSKE AKADEMIJE ZNANOSTI IN UMETNOSTI ANTON MELIK GEOGRAPHICAL INSTITUTE OF ZRC SAZU DICTIONARY OF SLOVENIAN EXONYMS EXPLANATORY NOTES Drago Kladnik Drago Perko AMGI ZRC SAZU Ljubljana 2013 1 Preface The geocoded collection of Slovenia exonyms Zbirka slovenskih eksonimov and the dictionary of Slovenina exonyms Slovar slovenskih eksonimov have been set up as part of the research project Slovenski eksonimi: metodologija, standardizacija, GIS (Slovenian Exonyms: Methodology, Standardization, GIS). They include more than 5,000 of the most frequently used exonyms that were collected from more than 50,000 documented various forms of these types of geographical names. The dictionary contains thirty-four categories and has been designed as a contribution to further standardization of Slovenian exonyms, which can be added to on an ongoing basis and used to find information on Slovenian exonym usage. Currently, their use is not standardized, even though analysis of the collected material showed that the differences are gradually becoming smaller. The standardization of public, professional, and scholarly use will allow completely unambiguous identification of individual features and items named. By determining the etymology of the exonyms included, we have prepared the material for their final standardization, and by systematically documenting them we have ensured that this important aspect of the Slovenian language will not sink into oblivion. The results of this research will not only help preserve linguistic heritage as an important aspect of Slovenian cultural heritage, but also help preserve national identity. Slovenian exonyms also enrich the international treasury of such names and are undoubtedly important part of the world’s linguistic heritage. -
Europe and Media: the History on the Web France, Great Britain, Hungary, Italy, Slovenia, Spain
Europe and media: the History on the Web France, Great Britain, Hungary, Italy, Slovenia, Spain 1 11 In this volume of “Il Filo d’Europa” we bring out the first research re- port made by Istituto storico Parri Emilia-Romagna with Europe Di- rect Emilia-Romagna and Videoteca of Legislative Assembly of the Emilia-Romagna Region, for the project “Europe and media: the hi- story in the web”. We continue in this way our engagement, after the conclusion of the project that has investigated the European history on the na- tional televisions, in order to understand how history is described through the new media and to imagine together a possible Euro- pean history. Stefania Fenati Istituto Storico Parri Emilia-Romagna The Istituto Storico Parri Emilia-Romagna was established in 1963. Its mission is to promote retrieval and knowledge of contemporary history’s sources. The main objective of the Institute is the study and research of the history of the 20th century. Videoteca Regionale The Regional Video Library was established in 1996 by the Legisla- tive Assembly of the Region Emilia-Romagna in collaboration with Istituto Beni Culturali, Artistici e Naturali. It is part of the Library of the Legislative Assembly of the Region Emilia-Romagna. Europe Direct of Emilia-Romagna The Europe Direct network is the main instrument used by the Eu- ropean institutions to encourage contacts with regional territories and citizens. It acts as intermediary between the EU and citizens at local level and allows citizens to have information, advice, assistan- ce and answers on EU policies and funding, and an opportunity to communicate with European institutions as well. -
Cultural Identities in Wikipedias
Cultural Identities in Wikipedias Marc Miquel-Ribé David Laniado Universitat Pompeu Fabra Eurecat Roc Boronat, 138, 08018, Barcelona, Av. Diagonal, 177, 080018, Barcelona, Catalonia, Spain Catalonia, Spain [email protected] [email protected] ABSTRACT 1. INTRODUCTION Wikipedia is self-defined as "a free-access, free-content Internet In this paper we study identity-based motivation in Wikipedia as encyclopedia”1. When Jimmy Wales and Larry Sanger started a drive for editors to act congruently with their cultural identity Wikipedia in 2001, they were already developing a free values by contributing with content related to them. To assess its encyclopedia called Nupedia with this same purpose. It was the influence, we developed a computational method to identify implementation of the wiki technology that completely changed articles related to the cultural identities associated to a language their approach by allowing collaborative modifications directly and applied it to 40 Wikipedia language editions. The results from the browser. This grew into the current site we know. The show that about a quarter of each Wikipedia language edition is result is a dual object: a social network that also serves the dedicated to represent the corresponding cultural identities. The purpose of creating a knowledge repository. However, , topical coverage of these articles reflects that geography, Wikipedia does not encourage editors to build their identities biographies, and culture are the most common themes, although based on personal traits, biography and social affinities2, which each language shows its idiosyncrasy and other topics are also is different from other online communities. Instead, Wikipedians present. The majority of these articles remain exclusive to each are valued according to their activity, their writing skills, the language, which is consistent with the idea that a Cultural languages they speak or acknowledgements they have received Identity is defined in relation to others; as entangled and from other peers, such as barnstars3 and praising comments. -
VNIR Spectral Properties of Five G-Class Asteroids: Implications for Mineralogy and Geologic Evolution
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2021 VNIR Spectral Properties Of Five G-Class Asteroids: Implications For Mineralogy And Geologic Evolution Justin Todd Germann Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Germann, Justin Todd, "VNIR Spectral Properties Of Five G-Class Asteroids: Implications For Mineralogy And Geologic Evolution" (2021). Theses and Dissertations. 3927. https://commons.und.edu/theses/3927 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. VNIR SPECTRAL PROPERTIES OF FIVE G-CLASS ASTEROIDS: IMPLICATIONS FOR MINERALOGY AND GEOLOGIC EVOLUTION by Justin Todd Germann Bachelor of Science, University of North Dakota, 2017 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota May 2021 ii DocuSign Envelope ID: FACAE050-8099-49F3-B21B-B535F8B6B93E Justin Germann Name: Degree: Master of Science This document, submitted in partial fulfillment of the requirements for the degree from the University of North Dakota, has been read by the Faculty Advisory Committee under whom the work has been done and is hereby approved. ____________________________________ Dr. Sherry Fieber-Beyer ____________________________________ Dr. Michael Gaffey ____________________________________ Dr. Wayne Barkhouse ____________________________________ ____________________________________ ____________________________________ This document is being submitted by the appointed advisory committee as having met all the requirements of the School of Graduate Studies at the University of North Dakota and is hereby approved. -
Is Wikipedia Really Neutral? a Sentiment Perspective Study of War-Related Wikipedia Articles Since 1945
PACLIC 29 Is Wikipedia Really Neutral? A Sentiment Perspective Study of War-related Wikipedia Articles since 1945 Yiwei Zhou, Alexandra I. Cristea and Zachary Roberts Department of Computer Science University of Warwick Coventry, United Kingdom fYiwei.Zhou, A.I.Cristea, [email protected] Abstract include books, journal articles, newspapers, web- pages, sound recordings2, etc. Although a “Neutral Wikipedia is supposed to be supporting the 3 “Neutral Point of View”. Instead of accept- point of view” (NPOV) is Wikipedia’s core content ing this statement as a fact, the current paper policy, we believe sentiment expression is inevitable analyses its veracity by specifically analysing in this user-generated content. Already in (Green- a typically controversial (negative) topic, such stein and Zhu, 2012), researchers have raised doubt as war, and answering questions such as “Are about Wikipedia’s neutrality, as they pointed out there sentiment differences in how Wikipedia that “Wikipedia achieves something akin to a NPOV articles in different languages describe the across articles, but not necessarily within them”. same war?”. This paper tackles this chal- Moreover, people of different language backgrounds lenge by proposing an automatic methodology based on article level and concept level senti- share different cultures and sources of information. ment analysis on multilingual Wikipedia arti- These differences have reflected on the style of con- cles. The results obtained so far show that rea- tributions (Pfeil et al., 2006) and the type of informa- sons such as people’s feelings of involvement tion covered (Callahan and Herring, 2011). Further- and empathy can lead to sentiment expression more, Wikipedia webpages actually allow to con- differences across multilingual Wikipedia on tain opinions, as long as they come from reliable au- war-related topics; the more people contribute thors4. -
Papers from the 2015 ICWSM Workshop
I CWSM Wikipedia, a Social Pedia: Research Challenges and Opportunities Papers from the 2015 ICWSM Workshop Technical Report WS-15-19 AAAI Press Association for the Advancement of Artificial Intelligence Wikipedia, a Social Pedia: Research Challenges and Opportunities Papers from the 2015 ICWSM Workshop Technical Report WS-15-19 AAAI Press Palo Alto, California Copyright © 2015, AAAI Press The Association for the Advancement of Artificial Intelligence 2275 East Bayshore Road, Suite 160 Palo Alto, California 94303 USA AAAI maintains compilation copyright for this technical report and retains the right of first refusal to any publication (including electronic distribution) arising from this AAAI event. Please do not make any inquiries or arrangements for hardcopy or electronic publication of all or part of the papers contained in these working notes without first explor- ing the options available through AAAI Press and AI Magazine (concur- rent submission to AAAI and an another publisher is not acceptable). A signed release of this right by AAAI is required before publication by a third party. Distribution of this technical report by any means including electronic (including, but not limited to the posting of the papers on any website) without permission is prohibited. ISBN 978-1-57735-737-7 WS-15-19 Manufactured in the United States of America Organizers Chairs Robert West (Stanford University) Leila Zia (Wikimedia Foundation) Jure Leskovec (Stanford University) iii This AAAI-sponsored workshop was collocated with ICWSM-15 and held Tuesday, May 26, 2015 in Oxford, UK iv Contents Preface / vii Robert West, Leila Zia, Jure Leskovec Wikipedia, Academia, and Science / 2 Eduard Aibar On the Evolution of Wikipedia: Dynamics of Categories and Articles / 6 Ramakrishna B.