Or “Lifetime Subscription” This Class Action Settlement May Affect Your Rights
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Sirius Satellite Radio Inc
SIRIUS SATELLITE RADIO INC FORM 10-K (Annual Report) Filed 02/29/08 for the Period Ending 12/31/07 Address 1221 AVENUE OF THE AMERICAS 36TH FLOOR NEW YORK, NY 10020 Telephone 2128995000 CIK 0000908937 Symbol SIRI SIC Code 4832 - Radio Broadcasting Stations Industry Broadcasting & Cable TV Sector Technology Fiscal Year 12/31 http://www.edgar-online.com © Copyright 2008, EDGAR Online, Inc. All Rights Reserved. Distribution and use of this document restricted under EDGAR Online, Inc. Terms of Use. Table of Contents Table of Contents UNITED STATES SECURITIES AND EXCHANGE COMMISSION WASHINGTON, D.C. 20549 F ORM 10-K ANNUAL REPORT PURSUANT TO SECTION 13 OR 15(d) OF THE SECURITIES EXCHANGE ACT OF 1934 FOR FISCAL YEAR ENDED DECEMBER 31, 2007 OR TRANSITION REPORT PURSUANT TO SECTION 13 OR 15(d) OF THE SECURITIES EXCHANGE ACT OF 1934 FOR THE TRANSITION PERIOD FROM TO COMMISSION FILE NUMBER 0-24710 SIRIUS SATELLITE RADIO INC. (Exact name of registrant as specified in its charter) Delaware 52 -1700207 (State or other jurisdiction of (I.R.S. Employer Identification Number) incorporation of organization) 1221 Avenue of the Americas, 36th Floor New York, New York 10020 (Address of principal executive offices) (Zip Code) Registrant’s telephone number, including area code: (212) 584-5100 Securities registered pursuant to Section 12(b) of the Act: Name of each exchange Title of each class: on which registered: Common Stock, par value $0.001 per share Nasdaq Global Select Market Securities registered pursuant to Section 12(g) of the Act: None (Title of class) Indicate by check mark if the registrant is a well-known seasoned issuer, as defined in Rule 405 of the Securities Act. -
The Nearest Stars: a Guided Tour by Sherwood Harrington, Astronomical Society of the Pacific
www.astrosociety.org/uitc No. 5 - Spring 1986 © 1986, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. The Nearest Stars: A Guided Tour by Sherwood Harrington, Astronomical Society of the Pacific A tour through our stellar neighborhood As evening twilight fades during April and early May, a brilliant, blue-white star can be seen low in the sky toward the southwest. That star is called Sirius, and it is the brightest star in Earth's nighttime sky. Sirius looks so bright in part because it is a relatively powerful light producer; if our Sun were suddenly replaced by Sirius, our daylight on Earth would be more than 20 times as bright as it is now! But the other reason Sirius is so brilliant in our nighttime sky is that it is so close; Sirius is the nearest neighbor star to the Sun that can be seen with the unaided eye from the Northern Hemisphere. "Close'' in the interstellar realm, though, is a very relative term. If you were to model the Sun as a basketball, then our planet Earth would be about the size of an apple seed 30 yards away from it — and even the nearest other star (alpha Centauri, visible from the Southern Hemisphere) would be 6,000 miles away. Distances among the stars are so large that it is helpful to express them using the light-year — the distance light travels in one year — as a measuring unit. In this way of expressing distances, alpha Centauri is about four light-years away, and Sirius is about eight and a half light- years distant. -
XIII Publications, Presentations
XIII Publications, Presentations 1. Refereed Publications E., Kawamura, A., Nguyen Luong, Q., Sanhueza, P., Kurono, Y.: 2015, The 2014 ALMA Long Baseline Campaign: First Results from Aasi, J., et al. including Fujimoto, M.-K., Hayama, K., Kawamura, High Angular Resolution Observations toward the HL Tau Region, S., Mori, T., Nishida, E., Nishizawa, A.: 2015, Characterization of ApJ, 808, L3. the LIGO detectors during their sixth science run, Classical Quantum ALMA Partnership, et al. including Asaki, Y., Hirota, A., Nakanishi, Gravity, 32, 115012. K., Espada, D., Kameno, S., Sawada, T., Takahashi, S., Ao, Y., Abbott, B. P., et al. including Flaminio, R., LIGO Scientific Hatsukade, B., Matsuda, Y., Iono, D., Kurono, Y.: 2015, The 2014 Collaboration, Virgo Collaboration: 2016, Astrophysical Implications ALMA Long Baseline Campaign: Observations of the Strongly of the Binary Black Hole Merger GW150914, ApJ, 818, L22. Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z = Abbott, B. P., et al. including Flaminio, R., LIGO Scientific 3.042, ApJ, 808, L4. Collaboration, Virgo Collaboration: 2016, Observation of ALMA Partnership, et al. including Asaki, Y., Hirota, A., Nakanishi, Gravitational Waves from a Binary Black Hole Merger, Phys. Rev. K., Espada, D., Kameno, S., Sawada, T., Takahashi, S., Kurono, Lett., 116, 061102. Y., Tatematsu, K.: 2015, The 2014 ALMA Long Baseline Campaign: Abbott, B. P., et al. including Flaminio, R., LIGO Scientific Observations of Asteroid 3 Juno at 60 Kilometer Resolution, ApJ, Collaboration, Virgo Collaboration: 2016, GW150914: Implications 808, L2. for the Stochastic Gravitational-Wave Background from Binary Black Alonso-Herrero, A., et al. including Imanishi, M.: 2016, A mid-infrared Holes, Phys. -
Digital Audio Broadcasting : Principles and Applications of Digital Radio
Digital Audio Broadcasting Principles and Applications of Digital Radio Second Edition Edited by WOLFGANG HOEG Berlin, Germany and THOMAS LAUTERBACH University of Applied Sciences, Nuernberg, Germany Digital Audio Broadcasting Digital Audio Broadcasting Principles and Applications of Digital Radio Second Edition Edited by WOLFGANG HOEG Berlin, Germany and THOMAS LAUTERBACH University of Applied Sciences, Nuernberg, Germany Copyright ß 2003 John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England Telephone (þ44) 1243 779777 Email (for orders and customer service enquiries): [email protected] Visit our Home Page on www.wileyeurope.com or www.wiley.com All Rights Reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning or otherwise, except under the terms of the Copyright, Designs and Patents Act 1988 or under the terms of a licence issued by the Copyright Licensing Agency Ltd, 90 Tottenham Court Road, London W1T 4LP, UK, without the permission in writing of the Publisher. Requests to the Publisher should be addressed to the Permissions Department, John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England, or emailed to [email protected], or faxed to (þ44) 1243 770571. This publication is designed to provide accurate and authoritative information in regard to the subject matter covered. It is sold on the understanding that the Publisher is not engaged in rendering professional services. If professional advice or other expert assistance is required, the services of a competent professional should be sought. -
Chapter 16 the Sun and Stars
Chapter 16 The Sun and Stars Stargazing is an awe-inspiring way to enjoy the night sky, but humans can learn only so much about stars from our position on Earth. The Hubble Space Telescope is a school-bus-size telescope that orbits Earth every 97 minutes at an altitude of 353 miles and a speed of about 17,500 miles per hour. The Hubble Space Telescope (HST) transmits images and data from space to computers on Earth. In fact, HST sends enough data back to Earth each week to fill 3,600 feet of books on a shelf. Scientists store the data on special disks. In January 2006, HST captured images of the Orion Nebula, a huge area where stars are being formed. HST’s detailed images revealed over 3,000 stars that were never seen before. Information from the Hubble will help scientists understand more about how stars form. In this chapter, you will learn all about the star of our solar system, the sun, and about the characteristics of other stars. 1. Why do stars shine? 2. What kinds of stars are there? 3. How are stars formed, and do any other stars have planets? 16.1 The Sun and the Stars What are stars? Where did they come from? How long do they last? During most of the star - an enormous hot ball of gas day, we see only one star, the sun, which is 150 million kilometers away. On a clear held together by gravity which night, about 6,000 stars can be seen without a telescope. -
The Sky Tonight
MARCH POUTŪ-TE-RANGI HIGHLIGHTS Conjunction of Saturn and the Moon A conjunction is when two astronomical objects appear close in the sky as seen THE- SKY TONIGHT- - from Earth. The planets, along with the TE AHUA O TE RAKI I TENEI PO Sun and the Moon, appear to travel across Brightest Stars our sky roughly following a path called the At this time of the year, we can see the ecliptic. Each body travels at its own speed, three brightest stars in the night sky. sometimes entering ‘retrograde’ where they The brightness of a star, as seen from seem to move backwards for a period of time Earth, is measured as its apparent (though the backwards motion is only from magnitude. Pictured on the cover is our vantage point, and in fact the planets Sirius, the brightest star in our night sky, are still orbiting the Sun normally). which is 8.6 light-years away. Sometimes these celestial bodies will cross With an apparent magnitude of −1.46, paths along the ecliptic line and occupy the this star can be found in the constellation same space in our sky, though they are still Canis Major, high in the northern sky. millions of kilometres away from each other. Sirius is actually a binary star system, consisting of Sirius A which is twice the On March 19, the Moon and Saturn will be size of the Sun, and a faint white dwarf in conjunction. While the unaided eye will companion named Sirius B. only see Saturn as a bright star-like object (Saturn is the eighth brightest object in our Sirius is almost twice as bright as the night sky), a telescope can offer a spectacular second brightest star in the night sky, view of the ringed planet close to our Moon. -
KMD 550/850 Multi-Function Display Flight Information Services (FIS) Pilot’S Guide Addendum
N B KMD 550/850 Multi-Function Display Flight Information Services (FIS) Pilot’s Guide Addendum For Software Version 02/02 and later Revision 6 Feb/2009 006-18237-0000 The information contained in this manual is for reference use only. If any information contained herein conflicts with similar information contained in the Airplane Flight Manual Supplement, the information in the Airplane Flight Manual Supplement shall take precedence. WARNING The enclosed technical data is eligible for export under License Designation NLR and is to be used solely by the individual/organization to whom it is addressed. Diversion contrary to U.S. law is prohibited. COPYRIGHT NOTICE Copyright © 2001, 2002, 2004, 2007, 2009 Honeywell International Inc. All rights reserved. Reproduction of this publication or any portion thereof by any means without the express written permission of Honeywell International Inc. is prohibited. For further information contact the Manager, Technical Publications; Honeywell, One Technology Center, 23500 West 105th Street, Olathe, Kansas 66061. Telephone: (913) 782-0400. Revision History Manual KMD 550/850 Flight Information Services (FIS) Pilot’s Guide Addendum Revision 6, February 2009 Part Number 006-18237-0000 Summary Added XM products: Precipitation Type (at Surface) Freezing Levels Winds Aloft Translated Metars Temporary Flight Restrictions (TFR’s) R-1 Revision History Manual KMD 550/850 Flight Information Services (FIS) Pilot’s Guide Addendum Revision 5, March 2007 Part Number 006-18237-0000 Summary Added XM Receiver functionality. R-2 Revision History Manual KMD 550/850 Flight Information Services (FIS) Pilot’s Guide Addendum Revision 4, November 2004 Part Number 006-18237-0000 Summary Add FIS Area Products (AIRMETs, SIGMETs, Convective SIGMETs and Alert Weather Watches). -
Ghost Imaging of Space Objects
Ghost Imaging of Space Objects Dmitry V. Strekalov, Baris I. Erkmen, Igor Kulikov, and Nan Yu Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109-8099 USA NIAC Final Report September 2014 Contents I. The proposed research 1 A. Origins and motivation of this research 1 B. Proposed approach in a nutshell 3 C. Proposed approach in the context of modern astronomy 7 D. Perceived benefits and perspectives 12 II. Phase I goals and accomplishments 18 A. Introducing the theoretical model 19 B. A Gaussian absorber 28 C. Unbalanced arms configuration 32 D. Phase I summary 34 III. Phase II goals and accomplishments 37 A. Advanced theoretical analysis 38 B. On observability of a shadow gradient 47 C. Signal-to-noise ratio 49 D. From detection to imaging 59 E. Experimental demonstration 72 F. On observation of phase objects 86 IV. Dissemination and outreach 90 V. Conclusion 92 References 95 1 I. THE PROPOSED RESEARCH The NIAC Ghost Imaging of Space Objects research program has been carried out at the Jet Propulsion Laboratory, Caltech. The program consisted of Phase I (October 2011 to September 2012) and Phase II (October 2012 to September 2014). The research team consisted of Drs. Dmitry Strekalov (PI), Baris Erkmen, Igor Kulikov and Nan Yu. The team members acknowledge stimulating discussions with Drs. Leonidas Moustakas, Andrew Shapiro-Scharlotta, Victor Vilnrotter, Michael Werner and Paul Goldsmith of JPL; Maria Chekhova and Timur Iskhakov of Max Plank Institute for Physics of Light, Erlangen; Paul Nu˜nez of Coll`ege de France & Observatoire de la Cˆote d’Azur; and technical support from Victor White and Pierre Echternach of JPL. -
Sirius Xm Radio Inc
SIRIUS XM RADIO INC. FORM 10-K (Annual Report) Filed 02/06/13 for the Period Ending 12/31/12 Address 1221 AVENUE OF THE AMERICAS 36TH FLOOR NEW YORK, NY 10020 Telephone 212-584-5100 CIK 0000908937 Symbol SIRI SIC Code 4832 - Radio Broadcasting Stations Industry Broadcasting & Cable TV Sector Services Fiscal Year 12/31 http://www.edgar-online.com © Copyright 2013, EDGAR Online, Inc. All Rights Reserved. Distribution and use of this document restricted under EDGAR Online, Inc. Terms of Use. UNITED STATES SECURITIES AND EXCHANGE COMMISSION WASHINGTON, D.C. 20549 FORM 10-K ANNUAL REPORT PURSUANT TO SECTION 13 OR 15(d) OF THE SECURITIES EXCHANGE ACT OF 1934 FOR THE FISCAL YEAR ENDED DECEMBER 31, 2012 OR TRANSITION REPORT PURSUANT TO SECTION 13 OR 15(d) OF THE SECURITIES EXCHANGE ACT OF 1934 FOR THE TRANSITION PERIOD FROM __________ TO ________ COMMISSION FILE NUMBER 001-34295 SIRIUS XM RADIO INC. (Exact name of registrant as specified in its charter) Delaware 52-1700207 (State or other jurisdiction of (I.R.S. Employer Identification Number) incorporation or organization) 1221 Avenue of the Americas, 36th Floor New York, New York 10020 (Address of principal executive offices) (Zip Code) Registrant’s telephone number, including area code: (212) 584-5100 Securities registered pursuant to Section 12(b) of the Act: Title of Each Class: Name of Each Exchange on Which Registered: Common Stock, par value $0.001 per share The Nasdaq Global Select Market Securities registered pursuant to Section 12(g) of the Act: None (Title of class) Indicate by check mark if the registrant is a well-known seasoned issuer, as defined in Rule 405 of the Securities Act. -
Request for Proposal for Satellite Radio Programming Services Pursuant to FCC Qualified Entity Set-Aside
Request for Proposal for Satellite Radio Programming Services Pursuant to FCC Qualified Entity Set-Aside Issued March 25, 2021 - Deadline to Respond - April 25, 2021, 11:59 pm Eastern Time Sirius XM Radio Inc. Qualified Entity RFP, March 25, 2021 I. INTRODUCTION Sirius XM Radio Inc. (“Sirius XM,” “we,” or “us”) invites interested and qualified parties (the “Proposer” or “you”) to participate in this Request for Proposal (“RFP”) process for providing satellite radio programming that we will carry on satellite radio channels pursuant to the Qualified Entity set-aside required by the Federal Communications Commission (“FCC”). Company Background Sirius XM is America’s satellite radio company. We deliver over 130 channels of audio entertainment, including commercial-free music, premier sports, news, talk, entertainment, traffic and weather, to more than 34 million customers. SiriusXM’s satellite and streaming audio platform is the home of Howard Stern's two exclusive channels. Its ad-free, curated music channels represent many decades and genres, from rock, to pop, country, hip hop, classical, Latin, electronic dance, jazz, heavy metal and more. SiriusXM's programming includes news from respected national outlets, and a broad range of in- depth talk, comedy and entertainment. For sports fans, SiriusXM also offers live games, events, news, analysis and opinion for all major professional sports, fulltime channels for top college sports conferences, and programming that covers other sports such as auto sports, golf, soccer, and more. SiriusXM is also the home of exclusive and popular podcasts including many original SiriusXM series and a highly-curated selection of podcasts from leading creators and providers. -
ANNUAL REPORT June 30, 2021
JOB TITLE SA FUNDS AR REVISION 8 SERIAL <12345678> TIME Friday, August 27, 2021 JOB NUMBER 393837-1 TYPE PAGE NO. I ANNUAL REPORT June 30, 2021 PORTFOLIOS OF INVESTMENTS SA U.S. Fixed Income Fund SA Global Fixed Income Fund SA U.S. Core Market Fund SA U.S. Value Fund SA U.S. Small Company Fund SA International Value Fund SA International Small Company Fund SA Emerging Markets Value Fund SA Real Estate Securities Fund SA Worldwide Moderate Growth Fund Beginning on January 1, 2022, as permitted by regulations adopted by the Securities and Exchange Commission, we intend to no longer mail paper copies of each Fund’s shareholder reports, unless you specifically request paper copies of the reports from the SA Funds - Investment Trust (the “Trust”) or from your financial intermediary, such as a broker-dealer or bank. Instead, the reports will be made available on the Trust’s website (http://www.sa-funds.com), and you will be notified by mail each time a report is posted and provided with a website link to access the report. If you already elected to receive shareholder reports electronically, you will not be affected by this change and you need not take any action. You may elect to continue to receive paper copies of all future reports free of charge. If you invest through a financial intermediary, you may contact your financial intermediary to request that you continue to receive paper copies of your shareholder reports. If you invest directly with the Trust, you may inform the Trust that you wish to continue receiving paper copies of your shareholder reports by contacting us at (844) 366-0905. -
Part 2 – Brightness of the Stars
5th Grade Curriculum Space Systems: Stars and the Solar System An electronic copy of this lesson in color that can be edited is available at the website below, if you click on Soonertarium Curriculum Materials and login in as a guest. The password is “soonertarium”. http://moodle.norman.k12.ok.us/course/index.php?categoryid=16 PART 2 – BRIGHTNESS OF THE STARS -PRELIMINARY MATH BACKGROUND: Students may need to review place values since this lesson uses numbers in the hundred thousands. There are two website links to online education games to review place values in the section. -ACTIVITY - HOW MUCH BIGGER IS ONE NUMBER THAN ANOTHER NUMBER? This activity involves having students listen to the sound that different powers of 10 of BBs makes in a pan, and dividing large groups into smaller groups so that students get a sense for what it means to say that 1,000 is 10 times bigger than 100. Astronomy deals with many big numbers, and so it is important for students to have a sense of what these numbers mean so that they can compare large distances and big luminosities. -ACTIVITY – WHICH STARS ARE THE BRIGHTEST IN THE SKY? This activity involves introducing the concepts of luminosity and apparent magnitude of stars. The constellation Canis Major was chosen as an example because Sirius has a much smaller luminosity but a much bigger apparent magnitude than the other stars in the constellation, which leads to the question what else effects the brightness of a star in the sky. -ACTIVITY – HOW DOES LOCATION AFFECT THE BRIGHTNESS OF STARS? This activity involves having the students test how distance effects apparent magnitude by having them shine flashlights at styrene balls at different distances.