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Canutillo Independent School District El Paso, Texas
CANUTILLO INDEPENDENT SCHOOL DISTRICT EL PASO, TEXAS COMPREHENSIVE ANNUAL FINANCIAL REPORT FOR THE YEAR ENDED JUNE 30, 2018 PREPARED BY FINANCIAL SERVICES DEPARTMENT CANUTILLO INDEPENDENT SCHOOL DISTRICT Comprehensive Annual Financial Report For the Fiscal Year Ended June 30, 2018 Table of Contents Page Exhibit Introductory Section (Unaudited) .................................................... 1 Letter of Transmittal . .............................................................. 3 GFOA Certificate of Achievement for Excellence in Financial Reporting ....................... 19 ASBO Certificate of Excellence in Financial Reporting ..................................... 20 Canutillo ISD Organizational Chart ..................................................... 21 List of Elected and Appointed Officials (Directory) ........................................ 22 Certificate of Board . .............................................................. 23 Financial Section . ............................................................. 25 Independent Auditor's Report ......................................................... 27 Management’s Discussion and Analysis ................................................. 31 Basic Financial Statements .......................................................... 43 Government-Wide Financial Statements Statement of Net Position ....................................................... 44 A-1 Statement of Activities ......................................................... 45 B-1 Governmental Fund Financial Statements -
UNITED STATES DISTRICT COURT NORTHERN DISTRICT of INDIANA SOUTH BEND DIVISION in Re FEDEX GROUND PACKAGE SYSTEM, INC., EMPLOYMEN
USDC IN/ND case 3:05-md-00527-RLM-MGG document 3279 filed 03/22/19 page 1 of 354 UNITED STATES DISTRICT COURT NORTHERN DISTRICT OF INDIANA SOUTH BEND DIVISION ) Case No. 3:05-MD-527 RLM In re FEDEX GROUND PACKAGE ) (MDL 1700) SYSTEM, INC., EMPLOYMENT ) PRACTICES LITIGATION ) ) ) THIS DOCUMENT RELATES TO: ) ) Carlene Craig, et. al. v. FedEx Case No. 3:05-cv-530 RLM ) Ground Package Systems, Inc., ) ) PROPOSED FINAL APPROVAL ORDER This matter came before the Court for hearing on March 11, 2019, to consider final approval of the proposed ERISA Class Action Settlement reached by and between Plaintiffs Leo Rittenhouse, Jeff Bramlage, Lawrence Liable, Kent Whistler, Mike Moore, Keith Berry, Matthew Cook, Heidi Law, Sylvia O’Brien, Neal Bergkamp, and Dominic Lupo1 (collectively, “the Named Plaintiffs”), on behalf of themselves and the Certified Class, and Defendant FedEx Ground Package System, Inc. (“FXG”) (collectively, “the Parties”), the terms of which Settlement are set forth in the Class Action Settlement Agreement (the “Settlement Agreement”) attached as Exhibit A to the Joint Declaration of Co-Lead Counsel in support of Preliminary Approval of the Kansas Class Action 1 Carlene Craig withdrew as a Named Plaintiff on November 29, 2006. See MDL Doc. No. 409. Named Plaintiffs Ronald Perry and Alan Pacheco are not movants for final approval and filed an objection [MDL Doc. Nos. 3251/3261]. USDC IN/ND case 3:05-md-00527-RLM-MGG document 3279 filed 03/22/19 page 2 of 354 Settlement [MDL Doc. No. 3154-1]. Also before the Court is ERISA Plaintiffs’ Unopposed Motion for Attorney’s Fees and for Payment of Service Awards to the Named Plaintiffs, filed with the Court on October 19, 2018 [MDL Doc. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
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. -
A La Torre Aaker Aalbers Aaldert Aarmour Aaron
A LA TORRE ABDIE ABLEMAN ABRAMOWITCH AAKER ABE ABLES ABRAMOWITZ AALBERS ABEE ABLETSON ABRAMOWSKY AALDERT ABEEL ABLETT ABRAMS AARMOUR ABEELS ABLEY ABRAMSEN AARON ABEKE ABLI ABRAMSKI AARONS ABEKEN ABLITT ABRAMSON AARONSON ABEKING ABLOTT ABRAMZON AASEN ABEL ABNER ABRASHKIN ABAD ABELA ABNETT ABRELL ABADAM ABELE ABNEY ABREU ABADIE ABELER ABORDEAN ABREY ABALOS ABELES ABORDENE ABRIANI ABARCA ABELI ABOT ABRIL ABATE ABELIN ABOTS ABRLI ABB ABELL ABOTSON ABRUZZO ABBA ABELLA ABOTT ABSALOM ABBARCROMBIE ABELLE ABOTTS ABSALON ABBAS ABELLS ABOTTSON ABSHALON ABBAT ABELMAN ABRAHAM ABSHER ABBATE ABELS ABRAHAMER ABSHIRE ABBATIELLO ABELSON ABRAHAMI ABSOLEM ABBATT ABEMA ABRAHAMIAN ABSOLOM ABBAY ABEN ABRAHAMOF ABSOLON ABBAYE ABENDROTH ABRAHAMOFF ABSON ABBAYS ABER ABRAHAMOV ABSTON ABBDIE ABERCROMBIE ABRAHAMOVITZ ABT ABBE ABERCROMBY ABRAHAMOWICZ ABTS ABBEKE ABERCRUMBIE ABRAHAMS ABURN ABBEL ABERCRUMBY ABRAHAMS ABY ABBELD ABERCRUMMY ABRAHAMSEN ABYRCRUMBIE ABBELL ABERDEAN ABRAHAMSOHN ABYRCRUMBY ABBELLS ABERDEEN ABRAHAMSON AC ABBELS ABERDEIN ABRAHAMSSON ACASTER ABBEMA ABERDENE ABRAHAMY ACCA ABBEN ABERG ABRAHM ACCARDI ABBERCROMBIE ABERLE ABRAHMOV ACCARDO ABBERCROMMIE ABERLI ABRAHMOVICI ACE ABBERCRUMBIE ABERLIN ABRAHMS ACERO ABBERDENE ABERNATHY ABRAHMSON ACESTER ABBERDINE ABERNETHY ABRAM ACETO ABBERLEY ABERT ABRAMCHIK ACEVEDO ABBETT ABEYTA ABRAMCIK ACEVES ABBEY ABHERCROMBIE ABRAMI ACHARD ABBIE ABHIRCROMBIE ABRAMIN ACHENBACH ABBING ABIRCOMBIE ABRAMINO ACHENSON ABBIRCROMBIE ABIRCROMBIE ABRAMO ACHERSON ABBIRCROMBY ABIRCROMBY ABRAMOF ACHESON ABBIRCRUMMY ABIRCROMMBIE ABRAMOFF -
Thickness of the Martian Crust: Improved Constraints from Geoid-To-Topography Ratios Mark A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 109, E01009, doi:10.1029/2003JE002153, 2004 Thickness of the Martian crust: Improved constraints from geoid-to-topography ratios Mark A. Wieczorek De´partement de Ge´ophysique Spatiale et Plane´taire, Institut de Physique du Globe de Paris, Saint-Maur, France Maria T. Zuber Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA Received 10 July 2003; revised 1 September 2003; accepted 24 November 2003; published 24 January 2004. [1] The average crustal thickness of the southern highlands of Mars was investigated by calculating geoid-to-topography ratios (GTRs) and interpreting these in terms of an Airy compensation model appropriate for a spherical planet. We show that (1) if GTRs were interpreted in terms of a Cartesian model, the recovered crustal thickness would be underestimated by a few tens of kilometers, and (2) the global geoid and topography signals associated with the loading and flexure of the Tharsis province must be removed before undertaking such a spatial analysis. Assuming a conservative range of crustal densities (2700–3100 kg mÀ3), we constrain the average thickness of the Martian crust to lie between 33 and 81 km (or 57 ± 24 km). When combined with complementary estimates based on crustal thickness modeling, gravity/topography admittance modeling, viscous relaxation considerations, and geochemical mass balance modeling, we find that a crustal thickness between 38 and 62 km (or 50 ± 12 km) is consistent with all studies. Isotopic investigations based on Hf-W and Sm-Nd systematics suggest that Mars underwent a major silicate differentiation event early in its evolution (within the first 30 Ma) that gave rise to an ‘‘enriched’’ crust that has since remained isotopically isolated from the ‘‘depleted’’ mantle. -
2018 Annual Report
MONEY SMART WEEK® helps consumers better manage their personal finances. MONEY Programs are offered to people of all demographics and income levels and cover all facets of personal finance. SMART® WEEK Facebook.com/MoneySmartWeekNational Twitter.com/MoneySmartWeek Instagram: @chicagofed #msw2018 Pinterest: @chicagofed Money Smart Week 2018 ANNUAL REPORT MISSION MAIN DRIVER COMMUNITIES COLLABORATION CATALYST FOR CHANGE ENGAGEMENT CREATIVITY MEDIA GROWTH 2018 PARTNERS MISSION MONEY SMART WEEK® is a public education campaign that helps con- sumers better manage their personal finances through thousands WHERE DID MSW 2018 TAKE PLACE? of free programs and events. These sessions are provided by Money What began in 2002 as a Chicago-based effort with 40 events and Smart Week® partners including nonprofits, financial institutions, 30 partners has expanded to multiple states. government agencies, schools and libraries. Classes and events (offered April 21st – 28th) connected community members with resources that strengthened public-private partnerships and engaged the media. The Federal Reserve Bank of Chicago convenes the program to help consumers locate and use resources that will help them analyze spending, manage debt, build savings and plan for the future. “Money Smart Week helps people from all backgrounds build financial capability. When consumers learn how to best save, spend, plan, and invest, they can take steps toward securing their financial futures. A community of Events: 4,350 Attendance: 141,740 Attendees 1 34,000 well-informed consumers helps support a healthy economy.” Events 1 900 States: 41 — Charles L. Evans, President & CEO, Federal Reserve Bank of Chicago Partners: 2,500+ MONEY SMART® MISSION MAIN DRIVER COMMUNITIES COLLABORATION CHANGE ENGAGEMENT CREATIVITY MEDIA GROWTH 2018 PARTNERS WEEK 2018 THE MAIN DRIVER During Money Smart Week 2018, groups across the country worked together to reach consumers with information and ideas to encourage financial well-being. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Quicksilver Deposits of Steens Mountain and Pueblo Mountains Southeast Oregon
Quicksilver Deposits of Steens Mountain and Pueblo Mountains Southeast Oregon GEOLOGICAL SURVEY BULLETIN 995-B A CONTRIBUTION TO ECONOMIC GEOLOGY QUICKSILVER DEPOSITS OF STEENS MOUNTAIN AND PUEBLO MOUNTAINS, SOUTHEAST OREGON By HOWEL WILLIAMS and ROBERT R. The object of this survey was to examine the quicksilver deposits with the hope of locating large tonnages of low-grade ore. The deposits occur in the south-central part of Harney County and are more than 100 miles from either Burns, Oreg., or Winuemucca, Nev., the nearest towns. The region is sparsely settled by stockmen; Fields, Denio, and Andrews are the only settlements. The range consisting of Steens Mountain and Pueblo Mountains is a dissected fault block, 90 miles long in a north-south direction and as much as 25 miles wide, tilted gently to the west. Pre-Tertiary rnetarnorphic and plutonic rocks occur at the southern end, but most of the block consists of Pliocene volcanic rocks. The major boundary faults on the east side of the range are concealed by alluvium. Minor northwestward-trending faults branch from them, their throws diminish ing toward the crest of the range; other minor fractures occur near, and parallel to, the mountain front. The quicksilver lodes were formed in and along these subsidiary fractures. The lodes occur in a more or less continuous belt just west of the eastern front of the range. They are steeply dipping and arranged in subparallel clusters, commonly standing out as resistant siliceous ribs against the softer kaolinized rocks that flank them. The lodes were formed in two hydrothermal stages, the first producing the reeflike masses of chalcedony and quartz with their halos of limonitic and calcitic clays and the second introducing silica and barite along with sulfides of iron, copper, and mercury. -
Trans-Baykal (Rusya) Bölgesi'nin Coğrafyasi
International Journal of Geography and Geography Education (IGGE) To Cite This Article: Can, R. R. (2021). Geography of the Trans-Baykal (Russia) region. International Journal of Geography and Geography Education (IGGE), 43, 365-385. Submitted: October 07, 2020 Revised: November 01, 2020 Accepted: November 16, 2020 GEOGRAPHY OF THE TRANS-BAYKAL (RUSSIA) REGION Trans-Baykal (Rusya) Bölgesi’nin Coğrafyası Reyhan Rafet CAN1 Öz Zabaykalskiy Kray (Bölge) olarak isimlendirilen saha adını Rus kâşiflerin ilk kez 1640’ta karşılaştıkları Daur halkından alır. Rusçada Zabaykalye, Balkal Gölü’nün doğusu anlamına gelir. Trans-Baykal Bölgesi, Sibirya'nın en güneydoğusunda, doğu Trans-Baykal'ın neredeyse tüm bölgesini işgal eder. Bölge şiddetli iklim koşulları; birçok mineral ve hammadde kaynağı; ormanların ve tarım arazilerinin varlığı ile karakterize edilir. Rusya Federasyonu'nun Uzakdoğu Federal Bölgesi’nin bir parçası olan on bir kurucu kuruluşu arasında bölge, alan açısından altıncı, nüfus açısından dördüncü, bölgesel ürün üretimi açısından (GRP) altıncı sıradadır. Bölge topraklarından geçen Trans-Sibirya Demiryolu yalnızca Uzak Doğu ile Rusya'nın batı bölgeleri arasında bir ulaşım bağlantısı değil, aynı zamanda Avrasya geçişini sağlayan küresel altyapının da bir parçasıdır. Bölgenin üretim yapısında sanayi, tarım ve ulaşım yüksek bir paya sahiptir. Bu çalışmada Trans-Baykal Bölgesi’nin fiziki, beşeri ve ekonomik coğrafya özellikleri ele alınmıştır. Trans-Baykal Bölgesinin coğrafi özelliklerinin yanı sıra, ekonomik ve kültürel yapısını incelenmiştir. Bu kapsamda konu ile ilgili kurumsal raporlardan ve alan araştırmalarından yararlanılmıştır. Bu çalışma sonucunda 350 yıldan beri Rus gelenek, kültür ve yaşam tarzının devam ettiği, farklı etnik grupların toplumsal birliği sağladığı, yer altı kaynaklarının bölge ekonomisi için yüzyıllardır olduğu gibi günümüzde de önem arz ettiği, coğrafyasının halkın yaşam şeklini belirdiği sonucuna varılmıştır. -
Crater Ice Deposits Near the South Pole of Mars Owen William Westbrook
Crater Ice Deposits Near the South Pole of Mars by Owen William Westbrook Submitted to the Department of Earth, Atmospheric, and Planetary Sciences in partial fulfillment of the requirements for the degree of Master of Science in Earth and Planetary Sciences at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2009 © Massachusetts Institute of Technology 2009. All rights reserved. A uth or ........................................ Department of Earth, Atmospheric, and Planetary Sciences May 22, 2009 Certified by . Maria T. Zuber E. A. Griswold Professor of Geophysics Thesis Supervisor 6- Accepted by.... ...... ..... ........................................... Daniel Rothman Professor of Geophysics Department of Earth, Atmospheric and Planetary Sciences MASSACHUSETTS INSTWITE OF TECHNOLOGY JUL 2 0 2009 ARCHIES LIBRARIES Crater Ice Deposits Near the South Pole of Mars by Owen William Westbrook Submitted to the Department of Earth, Atmospheric, and Planetary Sciences on May 22, 2009, in partial fulfillment of the requirements for the degree of Master of Science in Earth and Planetary Sciences Abstract Layered deposits atop both Martian poles are thought to preserve a record of past climatic conditions in up to three km of water ice and dust. Just beyond the extent of these south polar layered deposits (SPLD), dozens of impact craters contain large mounds of fill material with distinct similarities to the main layered deposits. Previously identified as outliers of the main SPLD, these deposits could offer clues to the climatic history of the Martian south polar region. We extend previous studies of these features by cataloging all crater deposits found near the south pole and quantifying the physical parameters of both the deposits and their host craters. -
RED Versión Impresa
Año 30 • Número 345 • Diciembre 2017 2,10 € ESPAÑOLA DE REVISTA DEFENSDE ESTRATEGIASEGURIDADA NACIONAL 2017 En marcha la Cooperación Estructurada Permanente (PESCO) AVANZAR en una Europa más segura CARLOS III Y LAS ORDENANZAS DE 1768 Exposición estrella del semestre en el Museo del Ejército [ nacional ] Don Juan Carlos expresa su reconocimiento a las Fuerzas Armadas y a la Guardia Civil “por su ejemplar entrega a España y a los españoles” L Palacio Real en la madri- actual crisis económica, “que ha exigi- to de Ley de Derechos y Deberes de los leña Plaza de Oriente fue, do priorizar las capacidades militares a Miembros de las Fuerzas Armadas y la el pasado 6 de enero, el es- alcanzar”. Destacó además la “extraor- adaptación del nuevo modelo de ense- cenario de la tradicional ce- dinaria labor” de los cien mil militares ñanza a los suboficiales. En relación con lebración de la Pascua Mi- españoles que han intervenido en nume- las cuatro operaciones internacionales litarE presidida por el rey Don Juan Car- rosas misiones en el extranjero a lo largo los. Acompañado en el Salón del Trono en curso, Chacón apuntó que tres de PASCUA de más de dos décadas. “Su presencia en ellas están actualmente dirigidas por mi- por la reina Doña Sofía y los príncipes muchas zonas del mundo ha sido un fac- litares españoles (en Líbano, en el Océa- [ cultura ] de Asturias, Don Felipe y Doña Letizia, tor clave –señaló- para afianzar el peso Su Majestad expresó los mejores deseos no Índico y en Uganda), “un dato –su- de España y su compromiso con la paz y brayó- que ilustra el grado de confianza para el nuevo año a todos los miembros la seguridad internacionales”.