2020 Nationals Results Packet
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Eat and Die: the Last Meal of Sacrificed Chimú Camelids At
Eat and Die: The Last Meal of Sacrificed Chimú Camelids at Huanchaquito-Las Llamas, Peru, as Revealed by Starch Grain Analysis Clarissa Cagnato , Nicolas Goepfert, Michelle Elliott, Gabriel Prieto, John Verano, and Elise Dufour This article reconstructs the final diet of sacrificed domestic camelids from Huanchaquito-Las Llamas to understand whether feeding was part of the ritual practice. The site is situated on the northern coast of Peru and is dated to the fifteenth century AD (Late Intermediate period; LIP). It was used by the Chimús to kill and bury a large number of camelids, mostly juveniles. We reconstructed the final meal of 11 of the sacrificed individuals by analyzing starch grains derived from the associated gut con- tents and feces. The starch grains were well preserved and allowed for the determination of five plant taxa. The comparison with previously published and new stable isotope analyses, which provide insights into long-term diet, indicates that the Chi- mús managed their herds by providing maize as fodder and allowing them to graze on natural pasture; yet they reserved special treatment for sacrificial animals, probably bringing them together a few hours or days before the sacrificial act. We show for the first time the consumption of unusual food products, which included manioc, chili peppers, and beans, as well as cooked foods. Our study provides unique information on Chimú camelid ritual and herding practices. Keywords: ritual diet, archaeobotany, stable isotope analysis, Late Intermediate period El presente artículo aborda la reconstrucción de la dieta ingerida por camélidos domesticados antes de ser sacrificados y enterrados en el sitio arqueológico Huanchaquito-Las Llamas, situado en la costa norte de Perú y data del siglo XV de nuestra era (periodo Intermedio Tardío). -
Railway Employee Records for Colorado Volume Iii
RAILWAY EMPLOYEE RECORDS FOR COLORADO VOLUME III By Gerald E. Sherard (2005) When Denver’s Union Station opened in 1881, it saw 88 trains a day during its gold-rush peak. When passenger trains were a popular way to travel, Union Station regularly saw sixty to eighty daily arrivals and departures and as many as a million passengers a year. Many freight trains also passed through the area. In the early 1900s, there were 2.25 million railroad workers in America. After World War II the popularity and frequency of train travel began to wane. The first railroad line to be completed in Colorado was in 1871 and was the Denver and Rio Grande Railroad line between Denver and Colorado Springs. A question we often hear is: “My father used to work for the railroad. How can I get information on Him?” Most railroad historical societies have no records on employees. Most employment records are owned today by the surviving railroad companies and the Railroad Retirement Board. For example, most such records for the Union Pacific Railroad are in storage in Hutchinson, Kansas salt mines, off limits to all but the lawyers. The Union Pacific currently declines to help with former employee genealogy requests. However, if you are looking for railroad employee records for early Colorado railroads, you may have some success. The Colorado Railroad Museum Library currently has 11,368 employee personnel records. These Colorado employee records are primarily for the following railroads which are not longer operating. Atchison, Topeka & Santa Fe Railroad (AT&SF) Atchison, Topeka and Santa Fe Railroad employee records of employment are recorded in a bound ledger book (record number 736) and box numbers 766 and 1287 for the years 1883 through 1939 for the joint line from Denver to Pueblo. -
The Futurist Moment : Avant-Garde, Avant Guerre, and the Language of Rupture
MARJORIE PERLOFF Avant-Garde, Avant Guerre, and the Language of Rupture THE UNIVERSITY OF CHICAGO PRESS CHICAGO AND LONDON FUTURIST Marjorie Perloff is professor of English and comparative literature at Stanford University. She is the author of many articles and books, including The Dance of the Intellect: Studies in the Poetry of the Pound Tradition and The Poetics of Indeterminacy: Rimbaud to Cage. Published with the assistance of the J. Paul Getty Trust Permission to quote from the following sources is gratefully acknowledged: Ezra Pound, Personae. Copyright 1926 by Ezra Pound. Used by permission of New Directions Publishing Corp. Ezra Pound, Collected Early Poems. Copyright 1976 by the Trustees of the Ezra Pound Literary Property Trust. All rights reserved. Used by permission of New Directions Publishing Corp. Ezra Pound, The Cantos of Ezra Pound. Copyright 1934, 1948, 1956 by Ezra Pound. Used by permission of New Directions Publishing Corp. Blaise Cendrars, Selected Writings. Copyright 1962, 1966 by Walter Albert. Used by permission of New Directions Publishing Corp. The University of Chicago Press, Chicago 60637 The University of Chicago Press, Ltd., London © 1986 by The University of Chicago All rights reserved. Published 1986 Printed in the United States of America 95 94 93 92 91 90 89 88 87 86 54321 Library of Congress Cataloging-in-Publication Data Perloff, Marjorie. The futurist moment. Bibliography: p. Includes index. 1. Futurism. 2. Arts, Modern—20th century. I. Title. NX600.F8P46 1986 700'. 94 86-3147 ISBN 0-226-65731-0 For DAVID ANTIN CONTENTS List of Illustrations ix Abbreviations xiii Preface xvii 1. -
Kevin Gill ‘11G
InSight: RIVIER ACADEMIC JOURNAL, VOLUME 14, NUMBER 1, FALL 2018 EXPLORING THE UNIVERSE: Meet Kevin Gill ‘11G Michelle Marrone (From Rivier Today, Fall 2018) From the comfort of his lab chair in sunny, southern California, Kevin Gill ’11G has a view into outer space. As a Science Data Software Engineer at NASA’s Jet Propulsion Laboratory (JPL), he spends his time planning and designing technology in support of environmental science and space exploration, as well as data visualization and planetary imaging. His recent work not only produced the first-ever close views of Saturn, but also contributed to NASA’s team winning an Emmy Award. Kevin earned his M.S. in Computer Science at Rivier and has been designing software to render the unique images he gathers ever since. He used an algorithm he developed during his program at Rivier to generate hypothetical images portraying Mars as a vibrant planet with oceans, an oxygen-rich atmosphere, and a green biosphere. The images went viral and within a week his work was featured on major media networks—Discovery News, Fox News, Universe Today, and the Huffington Post. His work captured NASA’s attention and paved the way for his career move. “Rivier taught me many of the algorithms and development practices I still use today at NASA,” says Kevin. “In fact, I can trace the lineage of code currently running on NASA systems directly to my final master’s project at the University.” The systems and tools he develops support a range of scientists specializing in the areas of climate, oceanography, asteroids, planetary science, and others. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
2018 Teacher Impact Survey
College in the Schools University of Minnesota, Twin Cities 5/11/2018 Teachers Impact Survey 2018 Methodology Survey links were sent to 490 teachers at CIS partner high schools on 4/13/2018. A reminder email was sent on 4/23/2018. 269 teachers responded, for a response rate of 55%. Many of the questions on the survey were developed by NACEP, the National Alliance of Concurrent Enrollment Partnerships, the accrediting body for concurrent enrollment programs across the country. CIS also included questions that were of particular interest to our program this year. Q1 - My school is located in a: # Answer % Count 1 City 23.79% 64 2 Suburb 48.33% 130 3 Town 13.75% 37 4 Rural Location 14.13% 38 Total 100% 269 Q2- My school is a: # Answer % Count 1 Public School 87.41% 236 2 Public Charter School 6.67% 18 3 Public Magnet School 1.48% 4 4 Private School 4.44% 12 5 Area Career/Technical Center 0.00% 0 Total 100% 270 Q3- The number of students enrolled at my high school is: ? 3000+ 1700+ 2000+ 1950-2000 6 8 8 11 13 13 15 17 19 23 27 40 51 56 60 60 80 80 80 81 85 100 115 122 150 150 150 155 170 190 190 196 200 200 200 200 225 235 240 240 250 250 251 265 275 286 287 300 300 315 320 325 330 345 350 350 350 350 370 375 400 400 400 400 400 400 425 438 441 450 450 450 450 450 500 500 500 500 500 500 500 500 500 500 500 525 550 550 550 550 550 550 560 560 600 600 ~600 600 600 600 600 600 610 690 700 743 750 750 780 800 800 800 821 844 850 900 900 950 950 972 1000 1000 1000 1000 1000 1000 1100 1100 1100 1100 1100 1100 1100 1145 1200 1200 1200 1200 1218 -
PUTTING LIFE on MARS: Using Computer Graphics to Render a Living Mars
InSight: RIVIER ACADEMIC JOURNAL, VOLUME 9, NUMBER 1, SPRING 2013 PUTTING LIFE ON MARS: Using Computer Graphics to Render a Living Mars Kevin M. Gill ‘11G* Senior Software Engineer, Thunderhead.com, Manchester, NH Keywords: Computer Graphics, Mars, Life, Planetary Science, OpenGL Abstract This article describes the software, algorithms & decisions that went into the development of the Living Mars image project. This includes topics related to computer graphics, software development, astronomy, & planetary science. The purpose of the project was to create a visualization of the planet Mars as could look with a living biosphere. This makes no distinction as to whether this biosphere would represent an ancient or future, possibly terraformed planet. 1 Background Mars, named for the Roman god of war. Ancient civilizations have forever associated the planet with fear, war, and destruction. It is the color of blood, and “one of a handful of planets visible to the naked eye, and the only one of marked color, so the planet demanded attention (Pyle, 2012).” Ever since man has noticed it, there have been dreams and visions of life on Mars, from Giovanni Schiaparelli and Percival Lowell describing channels and canals to Robert A. Heinlein’s science fiction. Lowell, in particular famous for fantastic writings of Mars, asked “are physical forces alone at work there, or has evolution begotten something more complex, something not unakin to what we know on Earth as life?” (Lowell, 1895) Even more recent discoveries by NASA’s Curiosity rover have found proof that liquid water once flowed billions of years ago positing an environment that could have served host to life (Brown, 2013). -
224641234.Pdf
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Helsingin yliopiston digitaalinen arkisto ASTROBIOLOGY Volume 19, Number 3, 2019 Mary Ann Liebert, Inc. DOI: 10.1089/ast.2018.1870 A Low-Diversity Microbiota Inhabits Extreme Terrestrial Basaltic Terrains and Their Fumaroles: Implications for the Exploration of Mars Charles S. Cockell,1 Jesse P. Harrison,2,3 Adam H. Stevens,1 Samuel J. Payler,1 Scott S. Hughes,4 Shannon E. Kobs Nawotniak,4 Allyson L. Brady,5 R.C. Elphic,6 Christopher W. Haberle,7 Alexander Sehlke,6 Kara H. Beaton,8 Andrew F.J. Abercromby,9 Petra Schwendner,1 Jennifer Wadsworth,1 Hanna Landenmark,1 Rosie Cane,1 Andrew W. Dickinson,1 Natasha Nicholson,1 Liam Perera,1 and Darlene S.S. Lim6,10 Abstract A major objective in the exploration of Mars is to test the hypothesis that the planet hosted life. Even in the absence of life, the mapping of habitable and uninhabitable environments is an essential task in developing a complete understanding of the geological and aqueous history of Mars and, as a consequence, understanding what factors caused Earth to take a different trajectory of biological potential. We carried out the aseptic collection of samples and comparison of the bacterial and archaeal communities associated with basaltic fumaroles and rocks of varying weathering states in Hawai‘i to test four hypotheses concerning the diversity of life in these environments. Using high-throughput sequencing, we found that all these materials are inhabited by a low-diversity biota. Multivariate analyses of bacterial community data showed a clear separation between sites that have active fumaroles and other sites that comprised relict fumaroles, unaltered, and syn-emplacement basalts. -
For-Hire Motor Carriers-Unrestricted Property
For-Hire - Unrestricted Property September 23, 2021 PIN USDOT MC Name DBA Name Phone Street Suite City State Zip 172318 2382342 1ST CALL HOTSHOT SERVICE LLC 1ST CALL HOTSHOT SERVICE LLC (405) 205-1738 Mail: 2410 W MEMORIAL RD STE C533 OKLAHOMA CITY OK 73134 Physical: 406 6TH ST CHEYENNE OK 73628 106139 1129401 2 B TRUCKING LLC 2 B TRUCKING LLC (936) 635-1288 Mail: 1430 N TEMPLE DIBOLL TX 75941 Physical: 214671 3131628 2 K SERVICES LLC 2 K SERVICES LLC (405) 754-0351 Mail: 2305 COUNTY ROAD 1232 BLANCHARD OK 73010 Physical: 142776 587437 2 R TRUCKING LLC 2 R TRUCKING LLC (402) 257-4105 Mail: 1918 ROAD ""P"" GUIDE ROCK NE 68942 Physical: 152966 2089295 2 RIVERS CONVERSIONS LLC 2 RIVERS CONVERSIONS LLC (405) 380-6771 Mail: 3888 N 3726 RD HOLDENVILLE OK 74848 Physical: 227192 3273977 2 VETS TRUCKING LLC 2 VETS TRUCKING LLC (405) 343-3468 Mail: 9516 TATUM LANE OKLAHOMA CITY OK 73165 Physical: 250374 3627024 2A TRANSPORT LLC 2A TRANSPORT LLC (918) 557-4000 Mail: PO BOX 52612 TULSA OK 74152 Physical: 10055 E 590 RD CATOOSA OK 74015 144063 1885218 3 C CATTLE FEEDERS INC 3 C CATTLE FEEDERS INC (405) 947-4990 Mail: PO BOX 14620 OKLAHOMA CITY OK 73113 Physical: PO BOX 144 MILL CREEK OK 74856 193972 2881702 3 CASAS TRUCKING LLC 3 CASAS TRUCKING LLC (405) 850-0223 Mail: 3701 KEITH COURT OKLAHOMA CITY OK 73135 Physical: 3701 KEITH COURT OKLAHOMA CITY OK 73135 251354 3678453 3 FEATHERS LOGISTICS LLC 3 FEATHERS LOGISTICS LLC (918) 991-4528 Mail: 411 N HODGE ST SAPULPA OK 74066 Physical: 134041 1728299 3 LANE TRUCKING LLC 3 LANE TRUCKING LLC Mail: RR1 -
Reminder List of Productions Eligible for the 90Th Academy Awards Alien
REMINDER LIST OF PRODUCTIONS ELIGIBLE FOR THE 90TH ACADEMY AWARDS ALIEN: COVENANT Actors: Michael Fassbender. Billy Crudup. Danny McBride. Demian Bichir. Jussie Smollett. Nathaniel Dean. Alexander England. Benjamin Rigby. Uli Latukefu. Goran D. Kleut. Actresses: Katherine Waterston. Carmen Ejogo. Callie Hernandez. Amy Seimetz. Tess Haubrich. Lorelei King. ALL I SEE IS YOU Actors: Jason Clarke. Wes Chatham. Danny Huston. Actresses: Blake Lively. Ahna O'Reilly. Yvonne Strahovski. ALL THE MONEY IN THE WORLD Actors: Christopher Plummer. Mark Wahlberg. Romain Duris. Timothy Hutton. Charlie Plummer. Charlie Shotwell. Andrew Buchan. Marco Leonardi. Giuseppe Bonifati. Nicolas Vaporidis. Actresses: Michelle Williams. ALL THESE SLEEPLESS NIGHTS AMERICAN ASSASSIN Actors: Dylan O'Brien. Michael Keaton. David Suchet. Navid Negahban. Scott Adkins. Taylor Kitsch. Actresses: Sanaa Lathan. Shiva Negar. AMERICAN MADE Actors: Tom Cruise. Domhnall Gleeson. Actresses: Sarah Wright. AND THE WINNER ISN'T ANNABELLE: CREATION Actors: Anthony LaPaglia. Brad Greenquist. Mark Bramhall. Joseph Bishara. Adam Bartley. Brian Howe. Ward Horton. Fred Tatasciore. Actresses: Stephanie Sigman. Talitha Bateman. Lulu Wilson. Miranda Otto. Grace Fulton. Philippa Coulthard. Samara Lee. Tayler Buck. Lou Lou Safran. Alicia Vela-Bailey. ARCHITECTS OF DENIAL ATOMIC BLONDE Actors: James McAvoy. John Goodman. Til Schweiger. Eddie Marsan. Toby Jones. Actresses: Charlize Theron. Sofia Boutella. 90th Academy Awards Page 1 of 34 AZIMUTH Actors: Sammy Sheik. Yiftach Klein. Actresses: Naama Preis. Samar Qupty. BPM (BEATS PER MINUTE) Actors: 1DKXHO 3«UH] %LVFD\DUW $UQDXG 9DORLV $QWRLQH 5HLQDUW] )«OL[ 0DULWDXG 0«GKL 7RXU« Actresses: $GªOH +DHQHO THE B-SIDE: ELSA DORFMAN'S PORTRAIT PHOTOGRAPHY BABY DRIVER Actors: Ansel Elgort. Kevin Spacey. Jon Bernthal. Jon Hamm. Jamie Foxx. -
Base Year 2010 School Enrollment Data
Base Year 2010 School Enrollment Data September 2013 Unified Planning Work Program FY 2013 Task 1.01, Subtask 8 Association of Central Oklahoma Governments 21 East Main Street, Suite 100 Oklahoma City, OK 73104-2405 Telephone: (405) 234-ACOG (2264) Fax: (405) 234-2200 www.acogok.org PRELIMINARY Not For Publication This report is the product of a project (study) financed in part by the Federal Transit Administration and the Federal Highway Administration of the U.S. Department of Transportation. The contents of this report reflect the views of the Association of Central Oklahoma Governments (ACOG), the Metropolitan Planning Organization for the Oklahoma City Area Regional Transportation Study (OCARTS) Transportation Management Area. ACOG is responsible for the facts and the accuracy of the data presented herein. The contents do not necessarily reflect official views or policy of the U.S. Department of Transportation. This report does not constitute a standard, specification, or regulation. Technical Report Documentation Page 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. UMTRIS/FTA/FHWA/SECTION Task 1.01 Subtask 8 5. Report Date: September 2013 FY 2013 UPWP 6. Performing Organization Code 4. Title and Subtitle Base Year 2010 School Enrollment Data 8. Performing Organization Report No. 10. Work Unit No. (TRAIS) 7. Author(s): John Sharp 11. Contract or Grant No. FTA-FHWA 9. Performing Organization Name and Address MPO Planning Funds Association of Central Oklahoma Governments 21 E. Main St., Ste 100 Oklahoma City, OK 73104-2405 12. Sponsoring Agency Name and Address 13. Type of Report and Period Covered Federal Transit Administration UPWP - 7/1/2012 - 6/30/2013 Federal Highway Administration 14. -
RSL), Described in the 5 August 2011 Science Report “Seasonal Flows on Warm Martian Slopes”
Animated GIFs to illustrate activity of Recurring Slope Lineae (RSL), described in the 5 August 2011 Science report “Seasonal Flows on Warm Martian Slopes”. All of these animated GIF files consist of a series of orthorectified HiRISE images over locations with RSL activity. Orthorectification corrects oblique images to show how the scene would appear from directly overhead. We perform this using HiRISE Digital Terrain Models (DTMs) at a scale of 1 m/posting. The orthorectified images are all at 0.25 m/pixel scale (or 0.5 m/pixel in cases noted below), so features smaller than 1-2 m diameter cannot be correctly rectified; the result is that small-scale features like boulders appear to wag back and forth. Each GIF is timed to dwell 2 seconds on the first and last frames and 1 second on intermediate frames, but network or computer performance may cause this to vary. The legend on each image gives the exact HiRISE image identifier; see http://uahirise.org/{image identified} for more information about each image. The legend also marks the year and seasonal identifier (Ls) for each image. The Mars years begin with the first years of Mars exploration by robot spacecraft. Ls stands for areocentric longitude of the sun, dividing the year into 360 degrees to mark the seasons. Ls = 180 is the beginning of southern spring, Ls = 270 is the beginning of southern summer, and Ls = 360 (or 0) is the beginning of southern autumn. Well-preserved crater on floor of Newton Crater Each of the gifs below are enhanced color sequences from different section of this crater slope, starting with faded RSL in MY29 (except one in which the color data was largely missing), then showing a sequence of RSL forming and fading in MY30.