Samsung Galaxy S7 Edge G935V User Manual
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Your Voice Assistant Is Mine: How to Abuse Speakers to Steal Information and Control Your Phone ∗ †
Your Voice Assistant is Mine: How to Abuse Speakers to Steal Information and Control Your Phone ∗ y Wenrui Diao, Xiangyu Liu, Zhe Zhou, and Kehuan Zhang Department of Information Engineering The Chinese University of Hong Kong {dw013, lx012, zz113, khzhang}@ie.cuhk.edu.hk ABSTRACT General Terms Previous research about sensor based attacks on Android platform Security focused mainly on accessing or controlling over sensitive compo- nents, such as camera, microphone and GPS. These approaches Keywords obtain data from sensors directly and need corresponding sensor invoking permissions. Android Security; Speaker; Voice Assistant; Permission Bypass- This paper presents a novel approach (GVS-Attack) to launch ing; Zero Permission Attack permission bypassing attacks from a zero-permission Android application (VoicEmployer) through the phone speaker. The idea of 1. INTRODUCTION GVS-Attack is to utilize an Android system built-in voice assistant In recent years, smartphones are becoming more and more popu- module – Google Voice Search. With Android Intent mechanism, lar, among which Android OS pushed past 80% market share [32]. VoicEmployer can bring Google Voice Search to foreground, and One attraction of smartphones is that users can install applications then plays prepared audio files (like “call number 1234 5678”) in (apps for short) as their wishes conveniently. But this convenience the background. Google Voice Search can recognize this voice also brings serious problems of malicious application, which have command and perform corresponding operations. With ingenious been noticed by both academic and industry fields. According to design, our GVS-Attack can forge SMS/Email, access privacy Kaspersky’s annual security report [34], Android platform attracted information, transmit sensitive data and achieve remote control a whopping 98.05% of known malware in 2013. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at Z = 7.730 Using Keck/Mosfire
Draft version May 5, 2015 Preprint typeset using LATEX style emulateapj v. 5/2/11 A SPECTROSCOPIC REDSHIFT MEASUREMENT FOR A LUMINOUS LYMAN BREAK GALAXY AT Z = 7:730 USING KECK/MOSFIRE P. A. Oesch1,2, P. G. van Dokkum2, G. D. Illingworth3, R. J. Bouwens4, I. Momcheva2, B. Holden3, G. W. Roberts-Borsani4,5, R. Smit6, M. Franx4, I. Labbe´4, V. Gonzalez´ 7, D. Magee3 Draft version May 5, 2015 ABSTRACT We present a spectroscopic redshift measurement of a very bright Lyman break galaxy at z = 7:7302 ± 0:0006 using Keck/MOSFIRE. The source was pre-selected photometrically in the EGS field as a robust z ∼ 8 candidate with H = 25:0 mag based on optical non-detections and a very red Spitzer/IRAC [3.6]−[4.5] broad-band color driven by high equivalent width [O III]+Hβ line emission. The Lyα line is reliably detected at 6:1σ and shows an asymmetric profile as expected for a galaxy embedded in a relatively neutral inter-galactic medium near the Planck peak of cosmic reionization. ˚ +90 The line has a rest-frame equivalent width of EW0 = 21 ± 4 A and is extended with VFWHM = 360−70 km s−1. The source is perhaps the brightest and most massive z ∼ 8 Lyman break galaxy in the 9:9±0:2 full CANDELS and BoRG/HIPPIES surveys, having assembled already 10 M of stars at only 650 Myr after the Big Bang. The spectroscopic redshift measurement sets a new redshift record for galaxies. This enables reliable constraints on the stellar mass, star-formation rate, formation epoch, as well as combined [O III]+Hβ line equivalent widths. -
Rev 06/2018 ASTRONOMY EXAM CONTENT OUTLINE the Following
ASTRONOMY EXAM INFORMATION CREDIT RECOMMENDATIONS This exam was developed to enable schools to award The American Council on Education’s College credit to students for knowledge equivalent to that learned Credit Recommendation Service (ACE CREDIT) by students taking the course. This examination includes has evaluated the DSST test development history of the Science of Astronomy, Astrophysics, process and content of this exam. It has made the Celestial Systems, the Science of Light, Planetary following recommendations: Systems, Nature and Evolution of the Sun and Stars, Galaxies and the Universe. Area or Course Equivalent: Astronomy Level: 3 Lower Level Baccalaureate The exam contains 100 questions to be answered in 2 Amount of Credit: 3 Semester Hours hours. Some of these are pretest questions that will not Minimum Score: 400 be scored. Source: www.acenet.edu Form Codes: SQ500, SR500 EXAM CONTENT OUTLINE The following is an outline of the content areas covered in the examination. The approximate percentage of the examination devoted to each content area is also noted. I. Introduction to the Science of Astronomy – 5% a. Nature and methods of science b. Applications of scientific thinking c. History of early astronomy II. Astrophysics - 15% a. Kepler’s laws and orbits b. Newtonian physics and gravity c. Relativity III. Celestial Systems – 10% a. Celestial motions b. Earth and the Moon c. Seasons, calendar and time keeping IV. The Science of Light – 15% a. The electromagnetic spectrum b. Telescopes and the measurement of light c. Spectroscopy d. Blackbody radiation V. Planetary Systems: Our Solar System and Others– 20% a. Contents of our solar system b. -
User Guide Guía Del Usuario Del Guía GH68-43542A Printed in USA SMARTPHONE
User Guide User Guide GH68-43542A Printed in USA Guía del Usuario del Guía SMARTPHONE User Manual Please read this manual before operating your device and keep it for future reference. Legal Notices Warning: This product contains chemicals known create source code from the software. No title to or to the State of California to cause cancer and ownership in the Intellectual Property is transferred to reproductive toxicity. For more information, please call you. All applicable rights of the Intellectual Property 1-800-SAMSUNG (726-7864). shall remain with SAMSUNG and its suppliers. Intellectual Property Open Source Software Some software components of this product All Intellectual Property, as defined below, owned by incorporate source code covered under GNU General or which is otherwise the property of Samsung or its Public License (GPL), GNU Lesser General Public respective suppliers relating to the SAMSUNG Phone, License (LGPL), OpenSSL License, BSD License and including but not limited to, accessories, parts, or other open source licenses. To obtain the source code software relating there to (the “Phone System”), is covered under the open source licenses, please visit: proprietary to Samsung and protected under federal http://opensource.samsung.com. laws, state laws, and international treaty provisions. Intellectual Property includes, but is not limited to, inventions (patentable or unpatentable), patents, trade secrets, copyrights, software, computer programs, and Disclaimer of Warranties; related documentation and other works of authorship. -
SAMSUNG GALAXY S6 USER GUIDE Table of Contents
SAMSUNG GALAXY S6 USER GUIDE Table of Contents Basics 55 Camera 71 Gallery 4 Read me first 73 Smart Manager 5 Package contents 75 S Planner 6 Device layout 76 S Health 8 SIM or USIM card 79 S Voice 10 Battery 81 Music 14 Turning the device on and off 82 Video 15 Touchscreen 83 Voice Recorder 18 Home screen 85 My Files 24 Lock screen 86 Memo 25 Notification panel 86 Clock 28 Entering text 88 Calculator 31 Screen capture 89 Google apps 31 Opening apps 32 Multi window 37 Device and data management 41 Connecting to a TV Settings 43 Sharing files with contacts 91 Introduction 44 Emergency mode 91 Wi-Fi 93 Bluetooth 95 Flight mode Applications 95 Mobile hotspot and tethering 96 Data usage 45 Installing or uninstalling apps 97 Mobile networks 46 Phone 97 NFC and payment 49 Contacts 100 More connection settings 51 Messages 102 Sounds and notifications 53 Internet 103 Display 54 Email 103 Motions and gestures 2 Table of Contents 104 Applications 104 Wallpaper 105 Themes 105 Lock screen and security 110 Privacy and safety 113 Easy mode 113 Accessibility 114 Accounts 115 Backup and reset 115 Language and input 116 Battery 116 Storage 117 Date and time 117 User manual 117 About device Appendix 118 Accessibility 133 Troubleshooting 3 Basics Read me first Please read this manual before using the device to ensure safe and proper use. • Descriptions are based on the device’s default settings. • Some content may differ from your device depending on the region, service provider, model specifications, or device’s software. -
Elements of Astronomy and Cosmology Outline 1
ELEMENTS OF ASTRONOMY AND COSMOLOGY OUTLINE 1. The Solar System The Four Inner Planets The Asteroid Belt The Giant Planets The Kuiper Belt 2. The Milky Way Galaxy Neighborhood of the Solar System Exoplanets Star Terminology 3. The Early Universe Twentieth Century Progress Recent Progress 4. Observation Telescopes Ground-Based Telescopes Space-Based Telescopes Exploration of Space 1 – The Solar System The Solar System - 4.6 billion years old - Planet formation lasted 100s millions years - Four rocky planets (Mercury Venus, Earth and Mars) - Four gas giants (Jupiter, Saturn, Uranus and Neptune) Figure 2-2: Schematics of the Solar System The Solar System - Asteroid belt (meteorites) - Kuiper belt (comets) Figure 2-3: Circular orbits of the planets in the solar system The Sun - Contains mostly hydrogen and helium plasma - Sustained nuclear fusion - Temperatures ~ 15 million K - Elements up to Fe form - Is some 5 billion years old - Will last another 5 billion years Figure 2-4: Photo of the sun showing highly textured plasma, dark sunspots, bright active regions, coronal mass ejections at the surface and the sun’s atmosphere. The Sun - Dynamo effect - Magnetic storms - 11-year cycle - Solar wind (energetic protons) Figure 2-5: Close up of dark spots on the sun surface Probe Sent to Observe the Sun - Distance Sun-Earth = 1 AU - 1 AU = 150 million km - Light from the Sun takes 8 minutes to reach Earth - The solar wind takes 4 days to reach Earth Figure 5-11: Space probe used to monitor the sun Venus - Brightest planet at night - 0.7 AU from the -
Galaxy Note 3 LTE(N900R4) Application List
Galaxy Note 3 LTE(N900R4) Application List Application Version ringtonebackup 4.4.2-N900R4TYECNG5 Kids Mode 1.0.02 Share video 1.1 Package Access Helper 4.4.2-N900R4TYECNG5 City ID 1.25.15 Samsung Cloud Quota 1.5.03 Google Search 1 Gallery 4.4.2-N900R4TYECNG5 Phone 4.4.2-N900R4TYECNG5 Software update 2.131231 Sensitivity test 1 BluetoothTest 4.4.2-N900R4TYECNG5 Bluetooth share 4.4.2-N900R4TYECNG5 Calendar storage 4.4.2-N900R4TYECNG5 S Voice 11.2.2.0 S Health 2.5.4.170 Communication Notifications 1 DeviceTest 1 Samsung Syncadapters 5.2.4 Drama 1.0.0.107_201400429 AllShare FileShare Service 1.4r476 PEN.UP 1.4.1 Enterprise SysScope Service 4.4.2-N900R4TYECNG5 Camera test 1 PickupTutorial 4.4.2-N900R4TYECNG5 Bloomberg+ 2.0.152 Eraser 1.6.0.214 Downloads 4.4.2-N900R4TYECNG5 RootPA 2.0025 (37085) Documents 4.4.2-N900R4TYECNG5 VpnDialogs 4.4.2-N900R4TYECNG5 Messages 4.4.2-N900R4TYECNG5 Media Storage 4.4.2-N900R4TYECNG5 Nearby devices 2.0.0 Settings 3 MobilePrintSvc_CUPS 1 CloudAgent 1.2.2 SetDefaultLauncher 1 Manage accessibility 1 Setup Wizard 1.3 POLARIS Office 5 5.0.3406.14 Idea Sketch 3 Voice Recorder 2.0.0 SamsungSans 1 Settings 4.4.2-N900R4TYECNG5 SapaMonitor S professional audio monitor 1.0.0 CapabilityManagerService 2.4.0 S Note 3.1.0 Samsung Link 1.8.1904 Samsung WatchON Video 14062601.1.21.78 Street View 1.8.1.2 Alarm 1 PageBuddyNotiSvc 1 Favorite Contacts 4.4.2-N900R4TYECNG5 Google Search 3.4.16.1149292.arm KNOX 2.0.0 Exchange services 4.2 GestureService 1 Weather 140211.01 Samsung Print Service Plugin 1.4.140410 Tasks provider 4.4.2-N900R4TYECNG5 -
Samsung Galaxy A8
SM-A530F SM-A530F/DS SM-A730F SM-A730F/DS User Manual English (LTN). 12/2017. Rev.1.0 www.samsung.com Table of Contents Basics Apps and features 4 Read me first 52 Installing or uninstalling apps 6 Device overheating situations and 54 Bixby solutions 70 Phone 10 Device layout and functions 75 Contacts 14 Battery 79 Messages 17 SIM or USIM card (nano-SIM card) 82 Internet 23 Memory card (microSD card) 84 Email 27 Turning the device on and off 85 Camera 28 Initial setup 100 Gallery 30 Samsung account 106 Always On Display 31 Transferring data from your previous 108 Multi window device 113 Samsung Pay 35 Understanding the screen 117 Samsung Members 47 Notification panel 118 Samsung Notes 49 Entering text 119 Calendar 120 Samsung Health 124 S Voice 126 Voice Recorder 127 My Files 128 Clock 129 Calculator 130 Radio 131 Game Launcher 134 Dual Messenger 135 Samsung Connect 139 Sharing content 140 Google apps 2 Table of Contents Settings 182 Google 182 Accessibility 142 Introduction 183 General management 142 Connections 184 Software update 143 Wi-Fi 185 User manual 146 Bluetooth 185 About phone 148 Data saver 148 NFC and payment 151 Mobile Hotspot and Tethering 152 SIM card manager (dual SIM Appendix models) 186 Troubleshooting 152 More connection settings 155 Sounds and vibration 156 Notifications 157 Display 158 Blue light filter 158 Changing the screen mode or adjusting the display color 160 Screensaver 160 Wallpapers and themes 161 Advanced features 163 Device maintenance 165 Apps 166 Lock screen and security 167 Face recognition 169 Fingerprint recognition 173 Smart Lock 173 Samsung Pass 176 Secure Folder 180 Cloud and accounts 181 Backup and restore 3 Basics Read me first Please read this manual before using the device to ensure safe and proper use. -
The Milky Way Almost Every Star We Can See in the Night Sky Belongs to Our Galaxy, the Milky Way
The Milky Way Almost every star we can see in the night sky belongs to our galaxy, the Milky Way. The Galaxy acquired this unusual name from the Romans who referred to the hazy band that stretches across the sky as the via lactia, or “milky road”. This name has stuck across many languages, such as French (voie lactee) and spanish (via lactea). Note that we use a capital G for Galaxy if we are talking about the Milky Way The Structure of the Milky Way The Milky Way appears as a light fuzzy band across the night sky, but we also see individual stars scattered in all directions. This gives us a clue to the shape of the galaxy. The Milky Way is a typical spiral or disk galaxy. It consists of a flattened disk, a central bulge and a diffuse halo. The disk consists of spiral arms in which most of the stars are located. Our sun is located in one of the spiral arms approximately two-thirds from the centre of the galaxy (8kpc). There are also globular clusters distributed around the Galaxy. In addition to the stars, the spiral arms contain dust, so that certain directions that we looked are blocked due to high interstellar extinction. This dust means we can only see about 1kpc in the visible. Components in the Milky Way The disk: contains most of the stars (in open clusters and associations) and is formed into spiral arms. The stars in the disk are mostly young. Whilst the majority of these stars are a few solar masses, the hot, young O and B type stars contribute most of the light. -
Milky Way Haze
CURIOSITY AT HOME MILKY WAY HAZE A galaxy is a group of stars, gas and dust. Our solar system is part of the Milky Way Galaxy. This galaxy appears as a milky haze in the night sky. Have you ever wondered why the Milky Way resembles a hazy, cloud-like strip in the sky? MATERIALS • Paper hole punch • Glue • Black construction paper • White paper • Masking or painter’s tape • Pen • Paper or science notebook PROCEDURE • Use the hole punch to cut out 50 circles from the white paper. • Glue the circles very close together in the center of the black sheet of paper. • Tape the black construction paper to a pole, tree, wall or other outside object you will be able to see from a distance. • Stand so your nose is almost touching the black construction paper. • Draw or write about your observations on a piece of paper or in your science notebook. • Slowly back away until the separate circles can no longer be seen. • Estimate or measure how far away you were when you could no longer see the separate circles. • What do you notice about the circles seen from a distance as compared to close up? DID YOU KNOW Our eyes are unable to distinguish small points of light that are very close together. Rather, the separate points of light blend together. In our galaxy, the light from distant stars blends together to form the Milky Way haze. The Milky Way galaxy is home to all of the stars that are visible to the naked eye as well as billions of stars that are so far away our eyes are unable to distinguish each individual point of star light. -
Active Galactic Nuclei - Suzy Collin, Bożena Czerny
ASTRONOMY AND ASTROPHYSICS - Active Galactic Nuclei - Suzy Collin, Bożena Czerny ACTIVE GALACTIC NUCLEI Suzy Collin LUTH, Observatoire de Paris, CNRS, Université Paris Diderot; 5 Place Jules Janssen, 92190 Meudon, France Bożena Czerny N. Copernicus Astronomical Centre, Bartycka 18, 00-716 Warsaw, Poland Keywords: quasars, Active Galactic Nuclei, Black holes, galaxies, evolution Content 1. Historical aspects 1.1. Prehistory 1.2. After the Discovery of Quasars 1.3. Accretion Onto Supermassive Black Holes: Why It Works So Well? 2. The emission properties of radio-quiet quasars and AGN 2.1. The Broad Band Spectrum: The “Accretion Emission" 2.2. Optical, Ultraviolet, and X-Ray Emission Lines 2.3. Ultraviolet and X-Ray Absorption Lines: The Wind 2.4. Variability 3. Related objects and Unification Scheme 3.1. The “zoo" of AGN 3.2. The “Line of View" Unification: Radio Galaxies and Radio-Loud Quasars, Blazars, Seyfert 1 and 2 3.2.1. Radio Loud Quasars and AGN: The Jet and the Gamma Ray Emission 3.3. Towards Unification of Radio-Loud and Radio-Quiet Objects? 3.4. The “Accretion Rate" Unification: Low and High Luminosity AGN 4. Evolution of black holes 4.1. Supermassive Black Holes in Quasars and AGN 4.2. Supermassive Black Holes in Quiescent Galaxies 5. Linking the growth of black holes to galaxy evolution 6. Conclusions Acknowledgements GlossaryUNESCO – EOLSS Bibliography Biographical Sketches SAMPLE CHAPTERS Summary We recall the discovery of quasars and the long time it took (about 15 years) to build a theoretical framework for these objects, as well as for their local less luminous counterparts, Active Galactic Nuclei (AGN).