COVID-19 Bibliography First Edition 31 March 2020 by Dr Yahia Bakelli Taibah University
Total Page：16
File Type：pdf, Size：1020Kb
Load more
Recommended publications
-
The History of Photography: the Research Library of the Mack Lee
THE HISTORY OF PHOTOGRAPHY The Research Library of the Mack Lee Gallery 2,633 titles in circa 3,140 volumes Lee Gallery Photography Research Library Comprising over 3,100 volumes of monographs, exhibition catalogues and periodicals, the Lee Gallery Photography Research Library provides an overview of the history of photography, with a focus on the nineteenth century, in particular on the first three decades after the invention photography. Strengths of the Lee Library include American, British, and French photography and photographers. The publications on French 19th- century material (numbering well over 100), include many uncommon specialized catalogues from French regional museums and galleries, on the major photographers of the time, such as Eugène Atget, Daguerre, Gustave Le Gray, Charles Marville, Félix Nadar, Charles Nègre, and others. In addition, it is noteworthy that the library includes many small exhibition catalogues, which are often the only publication on specific photographers’ work, providing invaluable research material. The major developments and evolutions in the history of photography are covered, including numerous titles on the pioneers of photography and photographic processes such as daguerreotypes, calotypes, and the invention of negative-positive photography. The Lee Gallery Library has great depth in the Pictorialist Photography aesthetic movement, the Photo- Secession and the circle of Alfred Stieglitz, as evidenced by the numerous titles on American photography of the early 20th-century. This is supplemented by concentrations of books on the photography of the American Civil War and the exploration of the American West. Photojournalism is also well represented, from war documentary to Farm Security Administration and LIFE photography. -
Dan Tassel Photography Collection11.Mwalb02702
Dan Tassel photography collection11.MWalB02702 This finding aid was produced using ArchivesSpace on September 27, 2021. eng Describing Archives: A Content Standard Brandeis University 415 South St. Waltham, MA URL: https://findingaids.brandeis.edu/ Dan Tassel photography collection11.MWalB02702 Table of Contents Summary Information .................................................................................................................................... 3 Scope and Contents ........................................................................................................................................ 3 Administrative Information ............................................................................................................................ 4 Controlled Access Headings .......................................................................................................................... 4 Collection Inventory ....................................................................................................................................... 5 Photographs by Dan Tassel: "Jerusalem Then and Now" .......................................................................... 5 Other Photographs ....................................................................................................................................... 5 Stereoscope and Slides ................................................................................................................................ 8 Printed Books ............................................................................................................................................. -
ΦYAST ΦLYER the Homer L
THE UNIVERSITY OF OKLAHOMA!SPRING 2010 ΦYAST ΦLYER The Homer L. Dodge Department of Physics and Astronomy Volume 18, Number 1 Homer L. Dodge Department associate professor and immediately became a of Physics and Astronomy highly valued member of our Department—for his internationally known experimental and Celebrates a Century! computational research in chemical physics; for his teaching (while here he won three awards for In 1909, William P. Haseman was appointed the excellence in teaching, and to date he remains the first chair of the university’s Department of only physicist the astronomers have allowed to Physics and Astronomy. Now, 100 years later, we celebrate the start of the department with a celebration this fall for alumni and friends of the department as well as faculty and students, with two main events planned. The first is a production of Michael Frayn’s play Copenhagen by the OU School of Drama. The second is a public lecture by the well-known cosmologist Andrei Linde of Stanford University. The play, presented in OU’s Weizenhoffer L to R: Greg Parker, Tom Mi!er, Xifan Liu. Theater, concerns the famous 1941 meeting Photo credit: John Cowan between Niels Bohr, played by New York actor teach their introductory course for non-majors); Paul Austin, and Werner Heisenberg, played by and for his service to the department—notably Tom Orr, director of OU’s School of Drama. The spending many weekends with Michael Morrison part of Bohr’s wife, Margrethe, has yet to be cast. and Stu Ryan cleaning out the attic, which Performances of Copenhagen will run the contained detritus that apparently pre-dated Isaac evenings of Thursday through Saturday, Sept. -
![Arxiv:1802.01539V3 [Astro-Ph.IM] 24 Jan 2019](https://docslib.b-cdn.net/cover/8631/arxiv-1802-01539v3-astro-ph-im-24-jan-2019-2858631.webp)
Arxiv:1802.01539V3 [Astro-Ph.IM] 24 Jan 2019
DRAFT VERSION JANUARY 25, 2019 A 1Typeset using LTEX default style in AASTeX61 ATLAS PROBE: BREAKTHROUGH SCIENCE OF GALAXY EVOLUTION, COSMOLOGY, MILKY WAY, AND THE SOLAR SYSTEM ∗ YUN WANG ,1 MASSIMO ROBBERTO,2, 3 MARK DICKINSON,4 LYNNE A. HILLENBRAND,5 WESLEY FRASER,6 PETER BEHROOZI,7 JARLE BRINCHMANN,8, 9 CHIA-HSUN CHUANG,10 ANDREA CIMATTI,11, 12 ROBERT CONTENT,13 EMANUELE DADDI,14 HENRY C. FERGUSON,2 CHRISTOPHER HIRATA,15 MICHAEL J. HUDSON,16 J. DAVY KIRKPATRICK,1 ALVARO ORSI,17 RUSSELL RYAN,2 ALICE SHAPLEY,18 MARIO BALLARDINI,19, 20 ROBERT BARKHOUSER,3 JAMES BARTLETT,21 ROBERT BENJAMIN,22 RANGA CHARY,1 CHARLIE CONROY,23 MEGAN DONAHUE,24 OLIVIER DORÉ,21 PETER EISENHARDT,21 KARL GLAZEBROOK,25 GEORGE HELOU,1 SANGEETA MALHOTRA,26 LAURO MOSCARDINI,11, 20, 27 JEFFREY A. NEWMAN,28 ZORAN NINKOV,29 MICHAEL RESSLER,21 JAMES RHOADS,26 JASON RHODES,21 DANIEL SCOLNIC,30 STEPHEN SMEE,3 FRANCESCO VALENTINO,31 AND RISA H. WECHSLER10, 32 1IPAC, California Institute of Technology, Mail Code 314-6, 1200 E. California Blvd., Pasadena, CA 91125 2Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 3Dept. of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218 4NOAO, 950 North Cherry Ave., Tucson, AZ 85719 5Dept. of Astronomy, California Institute of Technology, MC 249-17, 1200 East California Blvd, Pasadena CA 91125 6School of Mathematics and Physics, Queen’s University Belfast, University Road, BT7 1NN, Belfast, United Kingdom 7Steward Observatory, University of Arizona, 933 N Cherry Ave, Tucson, AZ 85719 8Leiden Observatory, Leiden Univ., P.O. -
Pos(DSU 2012)016 Ce
Probing the Nature of Cosmic Acceleration PoS(DSU 2012)016 Yun Wang∗ Homer L. Dodge Department of Physics & Astronomy, Univ. of Oklahoma, 440 W Brooks St., Norman, OK 73019 E-mail: [email protected] The cause for the observed acceleration in the expansion of the universe is unknown, and referred to as “dark energy” for convenience. Dark energy could be an unknown energy component, or a modification of Einstein’s general relativity. This dictates the measurements that are optimal in unveiling the nature of dark energy: the cosmic expansion history, and the growth history of cosmic large scale structure. Type Ia supernovae, galaxy clustering, and weak lensing are generally considered the most powerful observational probes of dark energy. Due to page limit, I will only examine Type Ia supernovae and galaxy clustering as dark energy probes, and discuss the recent results and future prospects. VIII International Workshop on the Dark Side of the Universe, June 10-15, 2012 Rio de Janeiro, Brazil ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Probing the Nature of Cosmic Acceleration Yun Wang (a) PoS(DSU 2012)016 (b) Figure 1: Left panel: Expansion history of the universe measured from current data [7]. Data used: Cosmic microwave background anisotropy (CMB) data from WMAP 7 year observations [8]; 472 Type Ia supernovae (SNe Ia) (compiled by [9], including data from the Supernova Legacy Survey (SNLS) [9], the Hubble Space Telescope (HST) [10], as well as nearby SNe Ia [36]); galaxy clustering measurements from Sloan Digital Sky Survey (SDSS) Luminous Red Galaxies (LRGs) [11], 69 Gamma Ray Bursts [14], and the latest Hubble constant (H0) measurement using the Hubble Space Telescope (HST) [16]. -
THE COLLECTIONS and ACTIVITIES of Museumsnews of CITIES 2015 Ivers N Ar N Y a H
INTERNATIONAL COUNCIL OF MUSEUMS 02 http://network.icom.muse- CONSEIL INTERNATIONAL DES MUSEES um/camoc/CONSEJO INTERNATCIONAL DE MUSEOS THE COLLECTIONS AND ACTIVITIES OF MUSEUMSnews OF CITIES 2015 www.camoc.icom.museum iversa nn r A y h t 1 0 THE MAS - a city museum 0 1 t h A y n r n with a global mission a s i v r LEEN BEYERS* e Display of World Portís Power. Photo: © Filip Dujardin “It is with justification that the wealthy and bounds, come here to trade their wares… The city lies populous city of Antwerp should be called the capital on the banks of the Scheldt, which ferries the ships of of the world. All the things that God has fashioned all the nations of the world bearing vast cargos …” are united in and flow towards this place. All the (Juan Cristóbal ete de Estrella, writer at the courts of the peoples of Christendom, and even those without its Spanish kings Charles V and Philip II of Spain, 1549) ▸ CONTENTS IN THIS ISSUE 01 THE MAS, a city museum with a global mission 16 CAMOC Workshop Berlin: “Defining Museums of 04 The Chair’s note Cities in the 21st Century” 05 Digital Mediain Cultural Participation And 18 Museum 2015 - The Agile Museum Cultural Democracy 20 Sarajevolution: Documenting Sarajevo’s 08 The Industrial Gas Museum Reconstruction 10 Phonambient: when cities speak 22 CAMOC Conference 2015: Memory and Migration 12 Museums, Cities and Difficult Heritage 25 Conference Alert 14 ‘Liège in torment’ exhibition 28 Exhibition Alert * Leen Beyers, Coördinator Onderzoek / Head of Research Museum aan de Stroom. -
Three Photographers from the Bronx: Jules Aarons, Morton Broffman, Joe Conzo
Resource Guide Three Photographers from the Bronx: Jules Aarons, Morton Broffman, Joe Conzo he exhibition Three Photographers from the Bronx: Jules Aarons, Morton Broffman, and Joe Conzo surveys the work of three artists for whom the idea of Tcommunity played a central role. Collectively, their work narrates the dynamic changes in the borough spanning the sixties to the eighties. By presenting a series of artworks ranging from the very personal to the historically significant, the exhibition encourages viewers to consider the role of photography as an effective form of social activism that expands traditional notions of community. Learning Objectives • Participants will be introduced to the unique history of the Bronx through documentary images that show the borough’s evolution from the late 1940s through the early 1980s. • Participants will be introduced to the national Civil Rights Movement during the second half of the twentieth century. • Participants will understand the term documentary photography and discuss it as an artistic practice. • Participants will closely observe, interpret, and draw meaning from the photographs in relation to their own lives. This guide focuses on one work by each of the three photographers. Each section includes a brief biography of the artist, questions and topics for discussion. Three Photographers from the Bronx 1 Civil rights activism in the National events United States and the Bronx Bronx events 1900 1940 1950 1960 1965 1896 1920-1940 1953-54 1963 In Plessy vs. Ferguson the Urban neighborhoods develop In Brown vs. Board of Education Martin Luther King Jr. gives his Supreme Court rules facilities can in the Bronx, supplemented by the Supreme Court rules that “I Have a Dream” speech on the be “separate but equal,” allowing major institutions like the New “separate” facilities cannot steps of the Lincoln Memorial in segregation. -
Arxiv:Astro-Ph/0601163V2 25 Apr 2006 Rpittpstuigl Using Typeset Preprint 2018 25, August Version Draft 1 2 M Aafo MP(Ent Ta.20;Seglet Spergel 2003; Al
Draft version August 25, 2018 A Preprint typeset using L TEX style emulateapj v. 11/12/01 DARK ENERGY CONSTRAINTS FROM BARYON ACOUSTIC OSCILLATIONS Yun Wang1 Draft version August 25, 2018 ABSTRACT Baryon acoustic oscillations (BAO) in the galaxy power spectrum allows us to extract the scale of the comoving sound horizon at recombination, a cosmological standard ruler accurately determined by the cosmic microwave background anisotropy data. We examine various issues important in the use of 2 2 BAO to probe dark energy. We find that assuming a flat universe, and priors on Ωm, Ωmh , and Ωbh ′ as expected from the Planck mission, the constraints on dark energy parameters (w0, w ) scale much less steeply with survey area than (area)−1/2 for a given redshift range. The constraints on the dark −1/2 energy density ρX (z), however, do scale roughly with (area) due to the strong correlation between H(z) and Ωm (which reduces the effect of priors on Ωm). Dark energy constraints from BAO are very sensitive to the assumed linear scale of matter clustering and the redshift accuracy of the survey. For −1 a BAO survey with 0.5 z 2, σ(R)=0.4 (corresponding to kmax(z =0)= 0.086 h Mpc ), and ≤ ′≤ 2 σz/(1 + z)=0.001, (σw0 , σw ) =(0.115, 0.183) and (0.069, 0.104) for survey areas of 1000 (deg) and 10000 (deg)2 respectively. We find that it is critical to minimize the bias in the scale estimates in order to derive reliable dark energy constraints. For a 1000 (10000) square degree BAO survey, a 1σ bias in ′ ′ ln H(z) leads to a 2σ (3σ) bias in w . -
Baryon Acoustic Oscillations and Beyond
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 7 August 2012 (MN LATEX style file v2.2) Galaxy clustering as dark energy probe: baryon acoustic oscillations and beyond Yun Wang⋆ Homer L. Dodge Department of Physics & Astronomy, Univ. of Oklahoma, 440 W Brooks St., Norman, OK 73019, U.S.A. 7 August 2012 ABSTRACT Galaxy clustering is one of the most powerful probes of the true nature of the observed cosmic acceleration. It contains baryon acoustic oscillations (BAO) that are cosmological standard rulers calibrated by the cosmic microwave background anisotropy data. The BAO allows us to measure the cosmic expansion history directly. Beyond the BAO, the full shape of galaxy clustering (either in the measured galaxy power spectrum or the galaxy correlation function) provides significantly more cosmological information, and in particular, allows us to test deviations from general relativity via the redshift space distortions. Here we introduce the basic ideas and analysis techniques for using galaxy clustering data to constrain dark energy and test gravity. We examine the critical issues, current status, as well as future prospects. s Since the 1980s, galaxy redshift surveys have been used to sk sH(z), s⊥ , (1) map the large scale structure in the universe, and constrain cosmo- ∝ ∝ DA(z) logical parameters. Galaxy redshift surveys are powerful as dark where s is the sound horizon scale at the drag epoch, and the angu- energy probe, since they can allow us to measure the cosmic ex- lar diameter distance DA(z) = r(z)/(1 + z), with r(z) denoting pansion history H(z) through the measurement of baryon acous- the comoving distance given by tic oscillations (BAO) in the galaxy distribution, and the growth −1 −1/2 1/2 history of cosmic large scale structure f (z) through independent r(z)= cH Ωk sinn[ Ωk Γ(z)], (2) g 0 | | | | measurements of redshift-space distortions and the bias factor be- z dz′ tween the distribution of galaxies and that of matter (Wang 2008). -
The History of the Universe in 60 Minutes
The History of the Universe in 60 Minutes Max Tegmark, MIT 100dpi Cosmology timeline: 500 BC 2000 AD Overduin & Priester 2001, astro-ph/0101484 1900 Cosmology timeline: 1910 s e Einstein’s theory of gravity i 1920 p o Expanding Universe theoretically possible (Friedmann) r t o s Universe is expanding (Hubble) i y 1930 n g a o l d o s u 1940 y m o e s r v o g r c Big Bang Nucleosynthesis (Gamow) k g u y c n s 1950 n Cosmic Microwave Background predicted (Alpher & Herman) g a i o t i s o y f b l s i n g i o e h r e o l v l s e 1960 m a l o y d s D 1st quasar discovered (Schmidt) a e g o w m r n o c o s l Cosmic Microwave Background detected (Penzias & Wilson) o r t y o i o s c t c x 1970 i e a m a a r t l s m i v o a o v f c o c y i a G n g a r 1980 r r m o Inflation invented (Guth, Linde, Albrecht & Steinhardt) e g l e n s t o s a o p CfA Galaxy Redshift Survey k u u a C m l m e S 1990 s y C CMB anisotropies detected (COBE) o L W c m y Dark energy discovered with supernovae (2 teams), CMB peaks detected c g 2000 Weak lensing detected (4 teams) o 1 l WMAP CMB, SDSS galaxy clustering 2dF galaxy clustering 2 o Planck CMB satellite CMB polarization detected (DASI) m 2010 s o c CMBPOL satellite? JDEM? JWST? LSST? SKA? n o 2020 i s i c e r P Flyabout + SDSS movie Max Tegmark Dept. -
Complete PAAM Collection Click Here for a PDF of Our Entire Permanent
First Middle Last Birth Death Sex Accession Acc ext Media code Title Date Medium H W D Finished size Credit Jules Aarons 1921 2008 m 1828 Ph06 Jules Aarons Portfolio: In the Jewish Neighborhoods 1946-76 box, 100 silver gelatin prints, signed verso 15.5 12 3 Gift of David Murphy, 2006 Jules Aarons 1921 2008 m 1928 001 Ph08 untitled (Weldon Kees speaking to assembly of artists) c.1949-50 silver gelatin photograph 8 10 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 002 Ph08 Sunday (The fishermen's children playing on the loading wharf.) c.1949-50 silver gelatin photograph 8 9.5 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 003 Ph08 untitled (Sunday II, fishermen's children playing on loading wharf.) c.1949-50 silver gelatin photograph 8 10 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 004 Ph08 untitled (the flag bearers) c.1949-50 silver gelatin photograph 8 10 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 005 Ph08 Parting c.1949-50 silver gelatin photograph 9 7 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 006 Ph08 untitled (2 ladies at an exhibition) c.1949-50 silver gelatin photograph 7.5 9.5 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 007 Ph08 Dante (I, Giglio Raphael Dante sitting on floor, ptg. behind) c.1949-50 silver gelatin photograph 10 8 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 008 Ph08 Lawrence Kupferman, a Prominent Modern American Artist (etc.) c.1949-50 silver gelatin photograph 7.5 9.5 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 009 Ph08 Kahlil (Gibran, playing music on bed) c.1949-50 silver gelatin photograph 7 7.5 Gift of David Murphy, 2008 Jules Aarons 1921 2008 m 1928 010 Ph08 Kahlil & Ellie G. -
Newsletter Fall 2002
"All The ν's That's Fit To Print" ΦYAST ΦLYER The Department of Physics & Astronomy The University of Oklahoma Volume 11, Number 1 Fall, 2002 Dick Henry, Editor; Sonya Brindle, Production Website: http://www.nhn.ou.edu D0 WORKSHOP REVIEW About 230 experimental particle physicists gathered at OU from July 812 for the annual D0 (DeeZero) Workshop. The participants in the workshop are all members of the D0 collaboration at the Fermi National Accelerator Laboratory near Chicago. The D0 experiment observes the collisions of protons and antiprotons at the Tevatron Collider. Debris from the highenergy collisions reveal clues about the basic particles and forces in the universe. The collaboration consists of more than 400 physicists from over 20 countries. Many of the participants at the workshop had never been to Oklahoma before. Three OU physicists who are active researchers on the D0 experiment hosted this year's workshop: Mike Strauss, Phil Gutierrez, and Brad Abbott. The workshop is a time when the collaboration can assess the current status of the experiment and plan for the future. Such reflection was crucial this year in the wake of a major upgrade to the D0 detector and to the Tevatron collider. Plenary sessions, parallel sessions, and working groups were located throughout Nielsen Hall and Dale Hall as the participants developed strategies for analyzing and understanding the data being collected in their detector. In addition to time spent working on physics, the workshop participants got a good look at many of OU's treasures, including the Sam Noble Oklahoma Museum of Natural History, and the university's history of science collection.