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Université De Montréal Relevé Polarimétrique D'étoiles Candidates
Université de Montréal Relevé polarimétrique d’étoiles candidates pour des disques de débris par Amélie Simon Département de physique Faculté des arts et des sciences Mémoire présenté à la Faculté des études supérieures en vue de l’obtention du grade de Maître ès sciences (M.Sc.) en physique Août, 2010 c Amélie Simon, 2010 Université de Montréal Faculté des études supérieures Ce mémoire intitulé: Relevé polarimétrique d’étoiles candidates pour des disques de débris présenté par: Amélie Simon a été évalué par un jury composé des personnes suivantes: Serge Demers, président-rapporteur Pierre Bastien, directeur de recherche Gilles Fontaine, membre du jury Mémoire accepté le: Sommaire Le relevé DEBRIS est effectué par le télescope spatial Herschel. Il permet d’échantillonner les disques de débris autour d’étoiles de l’environnement solaire. Dans la première partie de ce mémoire, un relevé polarimétrique de 108 étoiles des candidates de DEBRIS est présenté. Utilisant le polarimètre de l’Observatoire du Mont-Mégantic, des observations ont été effec- tuées afin de détecter la polarisation due à la présence de disques de débris. En raison d’un faible taux de détection d’étoiles polarisées, une analyse statistique a été réalisée dans le but de comparer la polarisation d’étoiles possédant un excès dans l’infrarouge et la polarisation de celles n’en possédant pas. Utilisant la théorie de diffusion de Mie, un modèle a été construit afin de prédire la polarisation due à un disque de débris. Les résultats du modèle sont cohérents avec les observations. La deuxième partie de ce mémoire présente des tests optiques du polarimètre POL-2, construit à l’Université de Montréal. -
United States Securities and Exchange Commission Form
Table of Contents 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 March 31, 2020 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: 0-29174 LOGITECH INTERNATIONAL S.A. (Exact name of registrant as specified in its charter) Canton of Vaud, Switzerland None (State or other jurisdiction of (I.R.S. Employer incorporation or organization) Identification No.) Logitech International S.A. EPFL - Quartier de l'Innovation Daniel Borel Innovation Center 1015 Lausanne, Switzerland c/o Logitech Inc. 7700 Gateway Boulevard Newark, California 94560 (Address of principal executive offices and zip code) (510) 795-8500 (Registrant's telephone number, including area code) Securities registered pursuant to Section 12(b) of the Act: Title of each class Name of each exchange on which registered Registered Shares par value CHF 0.25 per share The Nasdaq Global Select Market; SIX Swiss Exchange Securities registered or to be registered pursuant to Section 12(g) of the Act: None Indicate by check mark if the registrant is a well-known seasoned issuer, as defined in Rule 405 of the Securities Act. Yes ý No o Indicate by check mark if the registrant is not required to file reports pursuant to Section 13 or Section 15(d) of the Act. Yes o No ý Indicate by check mark whether the registrant (1) has filed all reports required to be filed by Section 13 or 15(d) of the Securities Exchange Act of 1934 during the preceding 12 months (or for such shorter period that the registrant was required to file such reports), and (2) has been subject to such filing requirements for the past 90 days. -
United States Securities and Exchange Commission Form
Table of Contents UNITED STATES SECURITIES AND EXCHANGE COMMISSION Washington, D.C. 20549 FORM 10-K ý ANNUAL REPORT PURSUANT TO SECTION 13 OR 15(d) OF THE SECURITIES EXCHANGE ACT OF 1934 For the fiscal year ended March 31, 2019 or o 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: 0-29174 LOGITECH INTERNATIONAL S.A. (Exact name of registrant as specified in its charter) Canton of Vaud, Switzerland None (State or other jurisdiction of (I.R.S. Employer incorporation or organization) Identification No.) Logitech International S.A. EPFL - Quartier de l'Innovation Daniel Borel Innovation Center 1015 Lausanne, Switzerland c/o Logitech Inc. 7700 Gateway Boulevard Newark, California 94560 (Address of principal executive offices and zip code) (510) 795-8500 (Registrant's telephone number, including area code) Securities registered pursuant to Section 12(b) of the Act: Title of each class Name of each exchange on which registered Registered Shares par value CHF 0.25 per share The Nasdaq Global Select Market; SIX Swiss Exchange Securities registered or to be registered pursuant to Section 12(g) of the Act: None Indicate by check mark if the registrant is a well-known seasoned issuer, as defined in Rule 405 of the Securities Act. Yes ý No o Indicate by check mark if the registrant is not required to file reports pursuant to Section 13 or Section 15(d) of the Act. Yes o No ý Indicate by check mark whether the registrant (1) has filed all reports required to be filed by Section 13 or 15(d) of the Securities Exchange Act of 1934 during the preceding 12 months (or for such shorter period that the registrant was required to file such reports), and (2) has been subject to such filing requirements for the past 90 days. -
Reasnow S1 User Manual
User Manual of ReaSnow S1 ReaSnow S1 User Manual V1.4 Jan, 2021 This manual is the intellectual property of ReaSnow. It must only be published in its original form. Using parts or republishing altered parts of this document is prohibited without permission from ReaSnow. http//www.reasnow.com PAGE 1 / 30 User Manual of ReaSnow S1 Table of Contents Chapter 1：Introduction to ReaSnow S1 1.1 Major Features of ReaSnow S1 1.2 Technical Specifications 1.3 Diagram Chapter 2：Quick Guide 2.1 Upgrade Firmware 2.2 Mouse Settings 2.3 Console and game settings 2.4 Wiring 2.5 ReaSnow Manager APP Chapter 3：ReaSnow Manager APP 3.1 Home 3.2 Manager 3.3 Settings 3.4 Add Config 3.5 Edit Config 3.7 Global Settings Chapter 4：Macro 4.1 Macro Manager 4.2 Macro Glossary 4.3 Examples and Explanations Chapter 5：Steering Wheel 5.1 Introduction 5.2 Usage 5.3 Notes Chapter 6：Flight Stick, Arcade Stick, and Other Controllers 6.1 Wiring 6.2 Add a Config Chapter 7：Bluetooth Controllers 7.1 Wiring 7.2 Add a Config 7.3 Pairing Chapter 8：Restoration 8.1 Restore factory defaults http//www.reasnow.com PAGE 2 / 30 User Manual of ReaSnow S1 Chapter 1：Introduction to ReaSnow S1 ReaSnow S1 is a high-end gaming converter created by ReaSnow Team, Professional mouse optimization for FPS games is embedded in it. Accurate and stable aiming can be got easily with your preferred mouse and keyboard. And it's also an all-around converter, most of the consoles in the market are compatible, such as: PS5 S&D/PS4 Pro&Slim/PS4/PS3/ Xbox Series X&S/ Xbox One X&S/Xbox One/XBox 360/ Nintendo Switch. -
The Con Psp Iso
The con psp iso click here to download Fight for the win or throw the fight to make some extra cash in this PSP fighting game. Download page for Con, The (USA). Fight for the win or throw the fight to make some extra cash in this PSP fighting game. Con, The (Europe). FILESIZE. VOTES. RATING. DownloadRATE. MBRATE. / Direct Download. ALTERNATIVE DOWNLOAD LINK: Con, The (Europe). PlayStation One (PSX) · PlayStation Portable (PSP) · Raine · Sega CD · Sega Dreamcast · Sega Master System · Sega Genesis 32X · Super Nintendo (SNES) · Turbo Grafx 16 · Wonderswan · Links · # A B C D E F G H I J K L M N O P Q R S T U V W X Y Z · Most Votes · Highest Rated · Most Popular. Con, The. FILESIZE. The Con (USA) PSP ISO Download for the Sony PlayStation Portable/PSP. Game description, information and PSP/PPSSPP download www.doorway.rued Size: MB. ISO download page for the game: The Con (PSP) - File: www.doorway.rut - www.doorway.ru Download Con, The (I)(BAHAMUT) ROM / ISO for PSP from Rom Hustler. % Fast Download. Game Title: The Con Publisher: Sony Computer Entertainment, Ertain Developer: Think and Feel Inc., SCEA Genre: Fighting Image Format: File Size: MB How to play? Download and Install PPSSPP emulator on your device and download The Con ISO rom, run the emulator and select your ISO. Play and enjoy the. Related Games. Forgotten Worlds (CPS1) · Patapon 2 PSP ISO · Shrek The Third PSP ISO · Petz My Baby Hamsterz PSP ISO · Petz Hamsterz Bunch PSP ISO · Petz PSP ISO · Strikers Plus PSP ISO · Up (PSP) · Tokobot PSP ISO. -
![Arxiv:2105.11583V2 [Astro-Ph.EP] 2 Jul 2021 Keck-HIRES, APF-Levy, and Lick-Hamilton Spectrographs](https://docslib.b-cdn.net/cover/4203/arxiv-2105-11583v2-astro-ph-ep-2-jul-2021-keck-hires-apf-levy-and-lick-hamilton-spectrographs-364203.webp)
Arxiv:2105.11583V2 [Astro-Ph.EP] 2 Jul 2021 Keck-HIRES, APF-Levy, and Lick-Hamilton Spectrographs
Draft version July 6, 2021 Typeset using LATEX twocolumn style in AASTeX63 The California Legacy Survey I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades Lee J. Rosenthal,1 Benjamin J. Fulton,1, 2 Lea A. Hirsch,3 Howard T. Isaacson,4 Andrew W. Howard,1 Cayla M. Dedrick,5, 6 Ilya A. Sherstyuk,1 Sarah C. Blunt,1, 7 Erik A. Petigura,8 Heather A. Knutson,9 Aida Behmard,9, 7 Ashley Chontos,10, 7 Justin R. Crepp,11 Ian J. M. Crossfield,12 Paul A. Dalba,13, 14 Debra A. Fischer,15 Gregory W. Henry,16 Stephen R. Kane,13 Molly Kosiarek,17, 7 Geoffrey W. Marcy,1, 7 Ryan A. Rubenzahl,1, 7 Lauren M. Weiss,10 and Jason T. Wright18, 19, 20 1Cahill Center for Astronomy & Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA 2IPAC-NASA Exoplanet Science Institute, Pasadena, CA 91125, USA 3Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA 4Department of Astronomy, University of California Berkeley, Berkeley, CA 94720, USA 5Cahill Center for Astronomy & Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA 6Department of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA 7NSF Graduate Research Fellow 8Department of Physics & Astronomy, University of California Los Angeles, Los Angeles, CA 90095, USA 9Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA 10Institute for Astronomy, University of Hawai`i, -
Two Rings but No Fellowship: Lotr 1 and Its Relation to Planetary Nebulae
Mon. Not. R. Astron. Soc. 000, 1–16 (2013) Printed 17 October 2018 (MN LATEX style file v2.2) Two rings but no fellowship: LoTr 1 and its relation to planetary nebulae possessing barium central stars. A.A. Tyndall1,2⋆, D. Jones2, H.M.J. Boffin2, B. Miszalski3,4, F. Faedi5, M. Lloyd1, J.A. L´opez6, S. Martell7, D. Pollacco5, and M. Santander-Garc´ıa8 1Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, M13 9PL, UK 2European Southern Observatory, Alonso de C´ordova 3107, Casilla 19001, Santiago, Chile 3South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa 4Southern African Large Telescope. PO Box 9, Observatory 7935, South Africa 5Department of Physics, University of Warwick, CV4 7AL, UK 6Instituto de Astronom´ıa, Universidad Nacional Aut´onoma de M´exico, Ensenada, Baja California, C.P. 22800, Mexico 7Australian Astronomical Observatory, North Ryde, 2109 NSW, Australia 8Observatorio Astron´omico National, Madrid, and Centro de Astrobiolog´ıa, CSIC-INTA, Spain Accepted xxxx xxxxxxxx xx. Received xxxx xxxxxxxx xx; in original form xxxx xxxxxxxx xx ABSTRACT LoTr 1 is a planetary nebula thought to contain an intermediate-period binary central star system ( that is, a system with an orbital period, P, between 100 and, say, 1500 days). The system shows the signature of a K-type, rapidly rotating giant, and most likely constitutes an accretion-induced post-mass transfer system similar to other PNe such as LoTr 5, WeBo 1 and A70. Such systems represent rare opportunities to further the investigation into the formation of barium stars and intermediate period post-AGB systems – a formation process still far from being understood. -
Creepy Jar S.A
CREEPY JAR S.A. (spółka akcyjna z siedzibą w Blizne Łaszczyńskiego przy ul. Gościnnej 11 lok. 28, 05-082 Stare Babice, zarejestrowana w rejestrze przedsiębiorców Krajowego Rejestru Sądowego pod numerem 0000666293) DOKUMENT INFORMACYJNY __________________________________________________________________________________ sporządzony w związku z ubieganiem się o wprowadzenie do obrotu w alternatywnym systemie obrotu na rynku NewConnect 204.588 akcji serii A oraz 64.848 akcji serii B o wartości nominalnej 1,00 PLN każda akcja Niniejszy dokument informacyjny został sporządzony w związku z ubieganiem się o wprowadzenie instrumentów finansowych objętych tym dokumentem do obrotu w alternatywnym systemie obrotu prowadzonym przez Giełdę Papierów Wartościowych w Warszawie S.A. Wprowadzenie instrumentów finansowych do obrotu w alternatywnym systemie obrotu nie stanowi dopuszczenia ani wprowadzenia tych instrumentów do obrotu na rynku regulowanym prowadzonym przez Giełdę Papierów Wartościowych w Warszawie S.A. (rynku podstawowym lub równoległym). Inwestorzy powinni być świadomi ryzyka jakie niesie ze sobą inwestowanie w instrumenty finansowe notowane w alternatywnym systemie obrotu, a ich decyzje inwestycyjne powinny być poprzedzone właściwą analizą, a także, jeżeli wymaga tego sytuacja, konsultacją z doradcą inwestycyjnym. Treść niniejszego dokumentu informacyjnego nie była zatwierdzana przez Giełdę Papierów Wartościowych w Warszawie S.A. pod względem zgodności informacji w nim zawartych ze stanem faktycznym lub przepisami prawa. Dokument Informacyjny został sporządzony w Warszawie, w dniu 7 stycznia 2019 r. Autoryzowany Doradca Navigator Capital S.A. CREEPY JAR S.A. Dokument Informacyjny 1. Oświadczenie osób odpowiedzialnych za informacje zawarte w dokumencie informacyjnym 1.1. Emitent 2 CREEPY JAR S.A. Dokument Informacyjny 1.2. Autoryzowany Doradca 3 CREEPY JAR S.A. Dokument Informacyjny Spis treści 1. Oświadczenie osób odpowiedzialnych za informacje zawarte w dokumencie informacyjnym ........................................................ -
Creepy Jar WYCENA 1 175 PLN RAPORT ANALITYCZNY 26 MAJA 2021, 07:40 CEST
KUPUJ (RAPORT INICJUJĄCY) Creepy Jar WYCENA 1 175 PLN RAPORT ANALITYCZNY 26 MAJA 2021, 07:40 CEST Rozpoczynamy wydawanie rekomendacji dla spółki Creepy Jar od zalecenia KUPUJ z ceną docelową 1 175 PLN, czyli 43% powyżej obecnej ceny rynkowej. Spółka od momentu powstania koncentruje się na tworzeniu tytułów w popularnej niszy gier survivalowych. Swoją pierwszą produkcją udowodniła, że czuje się w niej bardzo dobrze, mimo relatywnie niskiego budżetu (5,2 mln PLN), „Green Hell” cechuje się wysoką jakością wykonania zbliżoną do gier AAA, co prawdopodobnie byłoby niemożliwe do osiągnięcia gdyby nie umiejętności i doświadczenie Wycena DCF [PLN] 1 175 deweloperów. Tytuł ten istnieje na rynku od blisko 3 lat, a jego sprzedaż lada dzień przekroczy 2 Wycena końcowa [PLN] 1 175 mln kopii. Wydając w 1Q’21 pierwszą z trzech części dodatków z serii „Spirits of Amazonia” i osiągając wynikowo drugi najlepszy kwartał w historii udowodniła jaki dalej duży potencjał Potencjał do wzrostu 43% drzemie w tej produkcji. To naszym zdaniem jednak przedsmak tego co nas czeka w tym roku, gdyż Koszt kapitału 9% już w czerwcu zadebiutuje jej konsolowa wersja, a na 2/3Q’21 zapowiedziane są dwa kolejne dodatki. Spodziewamy się, że w 2021 roku sprzeda blisko 0,9 mln kopii gry „Green Hell”, z czego za 32% czyli ok. 0,3 mln będą odpowiadały konsole, co przełoży się 39,4 mln PLN przychodów, 23,8 Cena rynkowa [PLN] 823 mln PLN EBIT oraz 22,3 mln PLN zysku netto. Spodziewamy się, że spółka już w tym roku ujawni Kapitalizacja [mln PLN] 559,2 więcej informacji na temat „Chimery”. -
Abstract Sporting Mega-Events Generate Substantial Carbon
Abstract Sporting mega-events generate substantial carbon footprint where return transportation of event participants and visitors between the source and host countries makes the largest contribution. To enhance environmental sustainability of sporting mega-events, it is paramount to select a host country with the lowest carbon footprint from international transportation without compromising the magnitude of major visitor flows. The Facility Location Problem (FLP) model represents an established tool employed in the business environment to determine the best location for the installation of facilities to provide for existing or envisaged consumer demand. The model has proven its feasibility in a number of economic sectors, but rarely been applied in tourism, and never with sustainability management and planning purposes. This study contributes to knowledge by demonstrating the applicability of the FLP model when planning for sporting mega-events. The model enables selection of a host country with better climate credentials by quantifying the magnitude of international transportation of the event participants alongside the associated carbon footprint. Application of the FLP model to the FIFA World Cups shows that, to facilitate the progress of these mega-events towards sustainability, a decision on a host country should be made after the team qualification round, rather than before, as it currently stands. The model can then identify prospective hosts with the lowest carbon footprint from international transportation. Keywords: Facility -
TOKYO GAME SHOW 2011 Visitors Survey Report November 2011
TOKYO GAME SHOW 2011 Visitors Survey Report November 2011 Computer Entertainment Supplier's Association ■ Contents ■ Outline of Survey 3 Ⅰ．Visitors' Characteristics 4 １．Gender -------------------------------------------------------------------------- 4 ２．Age ---------------------------------------------------------------------------- 4 ３．Residential area --------------------------------------------------------------- 5 ４．Occupation --------------------------------------------------------------------- 5 ５．Hobbies and interests --------------------------------------------------------------- 6 Ⅱ．Household Videogames 9 １．Hardware ownership・Hardware most frequently used -------------------------------------- 9 ２．Hardware the respondents wish to purchase --------------------------------------------- 12 ３．Favorite game genres ---------------------------------------------------------------- 15 ４．Frequency of game playing ----------------------------------------------------------- 19 ５．Duration of game playing ------------------------------------------------------------- 21 ６．Tendency of software purchases ------------------------------------------------------ 24 ７．Tendency of software purchases by downloading ----------------------------------------- 27 Ⅲ．Social Games 28 １．Familiarity with SNS and social games -------------------------------------------------- 28 ２．Hardware used for SNS 【All SNS users】 ------------------------------------------------ 31 ３．Frequency of game playing 【All social game players】 ------------------------------------- -
Transition from Spot to Faculae Domination--An Alternate
Astronomy & Astrophysics manuscript no. AC2_arxiv c ESO 2018 October 30, 2018 Transition from spot to faculae domination An alternate explanation for the dearth of intermediate Kepler rotation periods Timo Reinhold1; 2, Keaton J. Bell1; 2, James Kuszlewicz1; 2, Saskia Hekker1; 2, Alexander I. Shapiro1 1 Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany 2 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, 120 Ny Munkegade, Building 1520, DK- 8000 Aarhus C, Denmark Received day month year / Accepted day month year ABSTRACT Context. The study of stellar activity cycles is crucial to understand the underlying dynamo and how it causes magnetic activity signatures such as dark spots and bright faculae. Having knowledge about the dominant source of surface activity might allow us to draw conclusions about the star’s age and magnetic field topology, and to put the solar cycle in context. Aims. We investigate the underlying process that causes magnetic activity by studying the appearance of activity signatures in con- temporaneous photometric and chromospheric time series. Methods. Lomb-Scargle periodograms are used to search for cycle periods present in the photometric and chromospheric time series. To emphasize the signature of the activity cycle we account for rotation-induced scatter in both data sets by fitting a quasi-periodic Gaussian process model to each observing season. After subtracting the rotational variability, cycle amplitudes and the phase differ- ence between the two time series are obtained by fitting both time series simultaneously using the same cycle period. Results. We find cycle periods in 27 of the 30 stars in our sample.