Scientific Forms of Sight
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Sabbatical Leave Report 2019 – 2020
Sabbatical Leave Report 2019 – 2020 James MacDevitt, M.A. Associate Professor of Art History and Visual & Cultural Studies Director, Cerritos College Art Gallery Department of Art and Design Fine Arts and Communications Division Cerritos College January 2021 Table of Contents Title Page i Table of Contents ii Sabbatical Leave Application iii Statement of Purpose 35 Objectives and Outcomes 36 OER Textbook: Disciplinary Entanglements 36 Getty PST Art x Science x LA Research Grant Application 37 Conference Presentation: Just Futures 38 Academic Publication: Algorithmic Culture 38 Service and Practical Application 39 Concluding Statement 40 Appendix List (A-E) 41 A. Disciplinary Entanglements | Table of Contents 42 B. Disciplinary Entanglements | Screenshots 70 C. Getty PST Art x Science x LA | Research Grant Application 78 D. Algorithmic Culture | Book and Chapter Details 101 E. Just Futures | Conference and Presentation Details 103 2 SABBATICAL LEAVE APPLICATION TO: Dr. Rick Miranda, Jr., Vice President of Academic Affairs FROM: James MacDevitt, Associate Professor of Visual & Cultural Studies DATE: October 30, 2018 SUBJECT: Request for Sabbatical Leave for the 2019-20 School Year I. REQUEST FOR SABBATICAL LEAVE. I am requesting a 100% sabbatical leave for the 2019-2020 academic year. Employed as a fulltime faculty member at Cerritos College since August 2005, I have never requested sabbatical leave during the past thirteen years of service. II. PURPOSE OF LEAVE Scientific advancements and technological capabilities, most notably within the last few decades, have evolved at ever-accelerating rates. Artists, like everyone else, now live in a contemporary world completely restructured by recent phenomena such as satellite imagery, augmented reality, digital surveillance, mass extinctions, artificial intelligence, prosthetic limbs, climate change, big data, genetic modification, drone warfare, biometrics, computer viruses, and social media (and that’s by no means meant to be an all-inclusive list). -
Year XIX, Supplement Ethnographic Study And/Or a Theoretical Survey of a Their Position in the Article Should Be Clearly Indicated
III. TITLES OF ARTICLES DRU[TVO ANTROPOLOGOV SLOVENIJE The journal of the Slovene Anthropological Society Titles (in English and Slovene) must be short, informa- SLOVENE ANTHROPOLOGICAL SOCIETY Anthropological Notebooks welcomes the submis- tive, and understandable. The title should be followed sion of papers from the field of anthropology and by the name of the author(s), their position, institutional related disciplines. Submissions are considered for affiliation, and if possible, by e-mail address. publication on the understanding that the paper is not currently under consideration for publication IV. ABSTRACT AND KEYWORDS elsewhere. It is the responsibility of the author to The abstract must give concise information about the obtain permission for using any previously published objective, the method used, the results obtained, and material. Please submit your manuscript as an e-mail the conclusions. Authors are asked to enclose in English attachment on [email protected] and enclose your contact information: name, position, and Slovene an abstract of 100 – 200 words followed institutional affiliation, address, phone number, and by three to five keywords. They must reflect the field of e-mail address. research covered in the article. English abstract should be placed at the beginning of an article and the Slovene one after the references at the end. V. NOTES A N T H R O P O L O G I C A L INSTRUCTIONS Notes should also be double-spaced and used sparingly. They must be numbered consecutively throughout the text and assembled at the end of the article just before references. VI. QUOTATIONS Short quotations (less than 30 words) should be placed in single quotation marks with double marks for quotations within quotations. -
10Great Features for Moon Watchers
Sinus Aestuum is a lava pond hemming the Imbrium debris. Mare Orientale is another of the Moon’s large impact basins, Beginning observing On its eastern edge, dark volcanic material erupted explosively and possibly the youngest. Lunar scientists think it formed 170 along a rille. Although this region at first appears featureless, million years after Mare Imbrium. And although “Mare Orien- observe it at several different lunar phases and you’ll see the tale” translates to “Eastern Sea,” in 1961, the International dark area grow more apparent as the Sun climbs higher. Astronomical Union changed the way astronomers denote great features for Occupying a region below and a bit left of the Moon’s dead lunar directions. The result is that Mare Orientale now sits on center, Mare Nubium lies far from many lunar showpiece sites. the Moon’s western limb. From Earth we never see most of it. Look for it as the dark region above magnificent Tycho Crater. When you observe the Cauchy Domes, you’ll be looking at Yet this small region, where lava plains meet highlands, con- shield volcanoes that erupted from lunar vents. The lava cooled Moon watchers tains a variety of interesting geologic features — impact craters, slowly, so it had a chance to spread and form gentle slopes. 10Our natural satellite offers plenty of targets you can spot through any size telescope. lava-flooded plains, tectonic faulting, and debris from distant In a geologic sense, our Moon is now quiet. The only events by Michael E. Bakich impacts — that are great for telescopic exploring. -
2019 Annual Report
Alfred P. Sloan Foundation $ 2019 Annual Report 2019 Annual Report 1 Alfred P. Sloan Foundation $ 2019 Annual Report Driven by the promise of great ideas. Alfred P. Sloan Foundation $ 2019 Annual Report Contents Preface 2 Mission 3 From the President 4 On Racism and Our Responsibilities 6 The Year in Discovery 8 Deep Carbon Observatory 18 Microbiology of the Built Environment 21 About the Grants Listing 24 2019 Grants by Program 25 2019 Financial Review 123 Audited Financial Statements and Schedules 125 Board of Trustees 156 Officers and Staff 157 Index of 2019 Grant Recipients 158 Cover: A student participant in the Environmentor program holds a turtle. An initiative of RISE (the Rockaway Institute for Sustainability), the Environmentor program is a Sloan-supported science research mentorship that offers NYC high school students the opportunity to conduct authentic, hands-on environmental research on Jamaica Bay and the Rockaway shoreline. (PHOTO: RISE ROCKAWAY) 1 Alfred P. Sloan Foundation $ 2019 Annual Report Preface The Alfred P. Sloan Foundation administers a private fund for the benefit of the public. It accordingly recognizes the responsibility of making periodic reports to the public on the management of this fund. The Foundation therefore submits this public report for the year 2019. 2 Alfred P. Sloan Foundation $ 2019 Annual Report Mission The Alfred P. Sloan Foundation makes grants primarily to support original research and education related to science, technology, engineering, mathematics, and economics. The Foundation believes that these fields— and the scholars and practitioners who work in them— are chief drivers of the nation’s health and prosperity. -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Deterministic Quantum Teleportation Received 18 February; Accepted 26 April 2004; Doi:10.1038/Nature02600
letters to nature Mars concretion systems. Although the analogue is not a perfect 24. Hoffman, N. White Mars: A new model for Mars’ surface and atmosphere based on CO2. Icarus 146, match in every geologic parameter, the mere presence of these 326–342 (2000). 25. Ferna´ndez-Remolar, D. et al. The Tinto River, an extreme acidic environment under control of iron, as spherical haematite concretions implies significant pore volumes of an analog of the Terra Meridiani hematite site of Mars. Planet. Space Sci. 53, 239–248 (2004). moving subsurface fluids through porous rock. Haematite is one of the few minerals found on Mars that can be Acknowledgements We thank the donors of the American Chemical Society Petroleum Research linked directly to water-related processes. Utah haematite concre- Fund, and the Bureau of Land Management-Grand Staircase Escalante National Monument for partial support of this research (to M.A.C. and W.T.P.). The work by J.O. was supported by the tions are similar to the Mars concretions with spherical mor- Spanish Ministry for Science and Technology and the Ramon y Cajal Program. The work by G.K. phology, haematite composition, and loose, weathered was supported by funding from the Italian Space Agency. accumulations. The abundance of quartz in the Utah example could pose challenges for finding spectral matches to the concre- Competing interests statement The authors declare that they have no competing financial tions. However, the similarities and differences of the Utah and interests. Mars haematite concretions should stimulate further investigations. Correspondence and requests for materials should be addressed to M.A.C. -
Carnegie Institution Carnegie
C68099_CVR.qxd:CVR 3/29/11 7:58 Page 1 2009-2010 CARNEGIE INSTITUTION FOR 2009-2010 SCIENCE YEAR BOOK 1530 P Street, N.W. Washington DC 20005 Phone: 202.387.6400 Carnegie Institution Fax: 202.387.8092 www.CarnegieScience.edu FOR SCIENCE CARNEGIE INSTITUTION FOR SCIENCE INSTITUTION FOR CARNEGIE YEAR BOOK The paper used in the manufacturing this year book contains 30% post-consumer recycled fiber. By using recycled fiber in place of virgin fiber, the Carnegie Institution preserved 41 trees, saved 126 pounds of waterborne waste, saved 18,504 gallons of water and prevented 4031 pounds of greenhouse gasses. The energy used to print the report was produced by wind power. Designed by Tina Taylor, T2 Design Printed by Monroe Litho ISSN 0069-066X C68099_CVR.qxd:CVR 3/29/11 7:58 Page 2 Department of Embryology 3520 San Martin Dr. / Baltimore, MD 21218 410.246.3001 Geophysical Laboratory 5251 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8900 Department of Global Ecology 260 Panama St. / Stanford, CA 94305-4101 650.462.1047 The Carnegie Observatories 813 Santa Barbara St. / Pasadena, CA 91101-1292 626.577.1122 Las Campanas Observatory Casilla 601 / La Serena, Chile Department of Plant Biology 260 Panama St. / Stanford, CA 94305-4101 650.325.1521 Department of Terrestrial Magnetism 5241 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8820 Office of Administration 1530 P St., N.W. / Washington, DC 20005-1910 202.387.6400 www.CarnegieScience.edu 2 009-2010 YEAR BOOK The President’s Report July 1, 2009 - June 30, 2010 CARNEGIE INSTITUTION FOR SCIENCE Former Presidents Former Trustees Daniel C. -
J. Paul Getty Trust Report 2018 Art and Science J
J. Paul Getty Trust Report 2018 Art and Science J. Paul Getty Trust Report 2018 On the cover: Macro-XRF scanning of mummy portrait Isidora, AD 100–110. Encaustic on linden wood; gilt; linen. The J. Paul Getty Museum Table of Contents 3 Chair Message Maria Hummer-Tuttle, Chair, Board of Trustees 7 Foreword James Cuno, President and CEO, J. Paul Getty Trust 10 Art and Science 11 Thoughts on Art and Science David Baltimore, President Emeritus and Robert Andrews Millikan Professor of Biology at the California Institute of Technology 15 Getty Conservation Institute Timothy P. Whalen, John E. and Louise Bryson Director 27 Getty Foundation Deborah Marrow, Director 39 J. Paul Getty Museum Timothy Potts, Director 49 Getty Research Institute Andrew Perchuk, Acting Director 59 Trust Report Lists 60 Getty Conservation Institute Projects 72 Getty Foundation Grants 82 Exhibitions and Acquisitions 110 Getty Guest Scholars 114 Getty Publications 122 Getty Councils 131 Honor Roll of Donors 139 Board of Trustees, Officers, and Directors 141 Financial Information Chair Message MARIA HUMMER-TUTTLE, CHAIR, BOARD OF TRUSTEES J. Paul Getty Trust ART AND SCIENCE—the theme of this year’s Trust Time: Art in L.A. 1945–1980, which ran from October Report—merge seamlessly in the Getty’s work of 2011 to April 2012. preserving, protecting, and interpreting the world’s While the majority of PST: LA/LA exhibitions artistic legacy. In the following essays by our four showcased modern and contemporary art, exhibitions program directors, you will learn how these disciplines about the ancient world and the pre-modern era were inform the work of the Getty Conservation Institute, also included. -
Geological and Geochemical Data from the Proposed Sirente Crater Field: New Age Dating and Evidence for Heating of Target
Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target Item Type Article; text Authors Ormö, Jens; Koeberl, Christian; Rossi, Angelo Pio; Komatsu, Goro Citation Ormö, J., Koeberl, C., Rossi, A. P., & Komatsu, G. (2006). Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target. Meteoritics & Planetary Science, 41(9), 1331-1345. DOI 10.1111/j.1945-5100.2006.tb00525.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 27/09/2021 20:14:45 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656183 Meteoritics & Planetary Science 41, Nr 9, 1331–1345 (2006) Abstract available online at http://meteoritics.org Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target Jens ORMÖ1*, Christian KOEBERL2, Angelo Pio ROSSI3, 4, and Goro KOMATSU3 1Centro de Astrobiología (CSIC/INTA), Instituto Nacional de Técnica Aeroespacial, Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain 2Department of Geological Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria 3International Research School of Planetary Sciences, Universita d’Annunzio, Viale Pindaro 42, 65127 Pescara, Italy 4ESA Research and Scientific Support Department, Keplerlaan 1, Postbus 299, ESTEC/SCI-SB, 2200 AG Noordwijk, The Netherlands *Corresponding author. E-mail: [email protected] (Received 23 February 2006; revision accepted 05 July 2006) Abstract–The proposed Sirente crater field consists of a slightly oblong main structure (main crater) 120 m in width and about 30 smaller structures (satellite craters), all in unconsolidated but stiff carbonate mud. -
User Guide To
USER GUIDE TO 1 2 5 0 , 000 S CA L E L U NA R MA P S DANNY C. KINSLER Lunar Science Institute 3303 NASA Road #1 Houston, TX 77058 Telephone: 713/488-5200 Cable Address: LUNSI The Lunar Science Institute is operated by the Universities Space Research Association under Contract No. NSR 09-051-001 with the National Aeronautics and Space Administration. This document constitutes LSI Contribution No. 206 March 1975 USER GUIDE TO 1 : 250 , 000 SCALE LUNAR MAPS GENERAL In 1 972 the NASA Lunar Programs Office initiated the Apoll o Photographic Data Analysis Program. The principal point of this program was a detail ed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17 . One of the requirements of this program was the production of detailed photo base maps at a useabl e scale . NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas . This paper is desi gned to present in outline form the neces- sary background information for users to become familiar with the program. MAP FORMAT The scale chosen for the project was 1:250,000* . The re- search being done required a scale that Principal Investigators (PI's) using orbital photography could use, but would also serve PI's doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west. The base is compiled from vertical Metric photography from Apollo missions 15, 16, and 17. -
8705K CIW 2002 YB Text
THE PRESIDENT’ S REPORT Year Book 01/02 July 1, — June 30, CARNEGIE INSTITUTION OF WASHINGTON Department of Embryology ABOUT CARNEGIE 115 West University Parkway Baltimore, MD 21210-3301 410.554.1200 . TO ENCOURAGE, IN THE BROADEST AND Department of Plant Biology MOST LIBERAL MANNER, INVESTIGATION, 260 Panama St. RESEARCH, AND DISCOVERY, AND THE Stanford, CA 94305-4101 650.325.1521 APPLICATION OF KNOWLEDGE TO THE Geophysical Laboratory IMPROVEMENT OF MANKIND . 5251 Broad Branch Rd., N.W. Washington, DC 20015-1305 202.478.8900 The Carnegie Institution of Washington Department of Terrestrial Magnetism was incorporated with these words in 1902 5241 Broad Branch Rd., N.W. Washington, DC 20015-1305 by its founder, Andrew Carnegie. Since 202.478.8820 then, the institution has remained true to The Carnegie Observatories 813 Santa Barbara St. its mission. At six research departments Pasadena, CA 91101-1292 across the country, the scientific staff and 626.577.1122 a constantly changing roster of students, Las Campanas Observatory Casilla 601 postdoctoral fellows, and visiting investiga- La Serena, Chile tors tackle fundamental questions on the Department of Global Ecology 260 Panama St. frontiers of biology, earth sciences, and Stanford, CA 94305-4101 astronomy. 650.325.1521 Office of Administration 1530 P St., N.W. Washington, DC 20005-1910 202.387.6400 http://www.CarnegieInstitution.org ISSN 0069-066X Design by Hasten Design, Washington, DC Printing by Mount Vernon Printing, Landover, MD March 2003 CONTENTS The President’s Commentary Losses, Gains, Honors Contributions, Grants, and Private Gifts First Light and CASE Geophysical Laboratory Department of Plant Biology Department of Embryology The Observatories Department of Terrestrial Magnetism Department of Global Ecology Extradepartmental and Administrative Financial Statements An electronic version of the Year Book is accessible via the Internet at www.CarnegieInstitution.org/yearbook.html.