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On the Spectra of Gamma-Ray Bursts at High Energies
University of New Hampshire University of New Hampshire Scholars' Repository Doctoral Dissertations Student Scholarship Spring 1986 ON THE SPECTRA OF GAMMA-RAY BURSTS AT HIGH ENERGIES STEVEN MICHAEL MATZ University of New Hampshire, Durham Follow this and additional works at: https://scholars.unh.edu/dissertation Recommended Citation MATZ, STEVEN MICHAEL, "ON THE SPECTRA OF GAMMA-RAY BURSTS AT HIGH ENERGIES" (1986). Doctoral Dissertations. 1483. https://scholars.unh.edu/dissertation/1483 This Dissertation is brought to you for free and open access by the Student Scholarship at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. INFORMATION TO USERS This reproduction was made from a copy of a manuscript sent to us for publication and microfilming. While the most advanced technology has been used to pho tograph and reproduce this manuscript, the quality of the reproduction is heavily dependent upon the quality of the material submitted. Pages in any manuscript may have indistinct print. In all cases the best available copy has been filmed. The following explanation of techniques is provided to help clarify notations which may appear on this reproduction. 1. Manuscripts may not always be complete. When it is not possible to obtain missing pages, a note appears to indicate this. 2. When copyrighted materials are removed from the manuscript, a note ap pears to indicate this. 3. Oversize materials (maps, drawings, and charts) are photographed by sec tioning the original, beginning at the upper left hand comer and continu ing from left to right in equal sections with small overlaps. -
A Search for Anomalous Tails of Short-Period Comets
Probable Optical Identification of LMC X-4 Claude Chevalier and Sergio A. I/ovaisky, Observatoire de Meudon Among the five X-ray sources known to exist in the Large of the sky by the UHURU satellite; it was also detected by Magellanic Cloud, none has up to now been positively the Ariel 5 and SAS-3 satellites and there is now definite idenlified with an optical object. However, this situation evidence for variability, including flares. The rotating mo may change in the near future as X-ray satellites point to dulation collimator system aboard SAS-3 determined the the source known as LMC X-4. The existence of this source position of LMC X-4 to one are minute. Inside the error box was announced in 1972 as a result of the first X-ray survey a large number of stars are visible on the ESO ass plate (field 86). Very deep objective-prism Schmidt plates taken at Cerro Tololo by N. Sanduleak and A. G. D. Philip showed an OS star near the centre of the error box. A spectrum of DELTA 13 l Me x- 'I pr; 1 ,llt1U D this star was taken by E. Maurice in January 1977 with the l' 3i'1~.(Jb Echelec spectrograph of the 1.5-m telescope at La Si lIa; it showed the star to be indeed an early-type luminous ob 3.3 ject. Du ri ng our runs at La Silla in February and March 1977 ......,', ......,', we started a systematic study of this object. One of us (C.C.) ,..... -
The Atmospheric Remote-Sensing Infrared Exoplanet Large-Survey
ariel The Atmospheric Remote-Sensing Infrared Exoplanet Large-survey Towards an H-R Diagram for Planets A Candidate for the ESA M4 Mission TABLE OF CONTENTS 1 Executive Summary ....................................................................................................... 1 2 Science Case ................................................................................................................ 3 2.1 The ARIEL Mission as Part of Cosmic Vision .................................................................... 3 2.1.1 Background: highlights & limits of current knowledge of planets ....................................... 3 2.1.2 The way forward: the chemical composition of a large sample of planets .............................. 4 2.1.3 Current observations of exo-atmospheres: strengths & pitfalls .......................................... 4 2.1.4 The way forward: ARIEL ....................................................................................... 5 2.2 Key Science Questions Addressed by Ariel ....................................................................... 6 2.3 Key Q&A about Ariel ................................................................................................. 6 2.4 Assumptions Needed to Achieve the Science Objectives ..................................................... 10 2.4.1 How do we observe exo-atmospheres? ..................................................................... 10 2.4.2 Targets available for ARIEL .................................................................................. -
Desind Finding
NATIONAL AIR AND SPACE ARCHIVES Herbert Stephen Desind Collection Accession No. 1997-0014 NASM 9A00657 National Air and Space Museum Smithsonian Institution Washington, DC Brian D. Nicklas © Smithsonian Institution, 2003 NASM Archives Desind Collection 1997-0014 Herbert Stephen Desind Collection 109 Cubic Feet, 305 Boxes Biographical Note Herbert Stephen Desind was a Washington, DC area native born on January 15, 1945, raised in Silver Spring, Maryland and educated at the University of Maryland. He obtained his BA degree in Communications at Maryland in 1967, and began working in the local public schools as a science teacher. At the time of his death, in October 1992, he was a high school teacher and a freelance writer/lecturer on spaceflight. Desind also was an avid model rocketeer, specializing in using the Estes Cineroc, a model rocket with an 8mm movie camera mounted in the nose. To many members of the National Association of Rocketry (NAR), he was known as “Mr. Cineroc.” His extensive requests worldwide for information and photographs of rocketry programs even led to a visit from FBI agents who asked him about the nature of his activities. Mr. Desind used the collection to support his writings in NAR publications, and his building scale model rockets for NAR competitions. Desind also used the material in the classroom, and in promoting model rocket clubs to foster an interest in spaceflight among his students. Desind entered the NASA Teacher in Space program in 1985, but it is not clear how far along his submission rose in the selection process. He was not a semi-finalist, although he had a strong application. -
Table of Artificial Satellites Launched in 1979
This electronic version (PDF) was scanned by the International Telecommunication Union (ITU) Library & Archives Service from an original paper document in the ITU Library & Archives collections. La présente version électronique (PDF) a été numérisée par le Service de la bibliothèque et des archives de l'Union internationale des télécommunications (UIT) à partir d'un document papier original des collections de ce service. Esta versión electrónica (PDF) ha sido escaneada por el Servicio de Biblioteca y Archivos de la Unión Internacional de Telecomunicaciones (UIT) a partir de un documento impreso original de las colecciones del Servicio de Biblioteca y Archivos de la UIT. (ITU) ﻟﻼﺗﺼﺎﻻﺕ ﺍﻟﺪﻭﻟﻲ ﺍﻻﺗﺤﺎﺩ ﻓﻲ ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﺃﺟﺮﺍﻩ ﺍﻟﻀﻮﺋﻲ ﺑﺎﻟﻤﺴﺢ ﺗﺼﻮﻳﺮ ﻧﺘﺎﺝ (PDF) ﺍﻹﻟﻜﺘﺮﻭﻧﻴﺔ ﺍﻟﻨﺴﺨﺔ ﻫﺬﻩ .ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﻓﻲ ﺍﻟﻤﺘﻮﻓﺮﺓ ﺍﻟﻮﺛﺎﺋﻖ ﺿﻤﻦ ﺃﺻﻠﻴﺔ ﻭﺭﻗﻴﺔ ﻭﺛﻴﻘﺔ ﻣﻦ ﻧﻘﻼ ً◌ 此电子版(PDF版本)由国际电信联盟(ITU)图书馆和档案室利用存于该处的纸质文件扫描提供。 Настоящий электронный вариант (PDF) был подготовлен в библиотечно-архивной службе Международного союза электросвязи путем сканирования исходного документа в бумажной форме из библиотечно-архивной службы МСЭ. © International Telecommunication Union TELECOMMUNICATION JOURNAL - VOL. 47 - IV/1980 C0SM0S-1101 1979 42B MOLNYA-3 (11) 1979 4 A COSMOS-1102 1979 43 A MOLNYA-3 (12) 1979 48 A A COSMOS-1103 1979 45A D COSMOS-1104 1979 46 A ARIANE-6 1979 104A C0SM0S-1105 1979 52A DMSP-4 1979 50A N ARIEL-6 1979 47A COSMOS-1106 1979 54A DSCS-II 13 1979 98A AYAME 1979 9 A COSMOS-1107 1979 55A DSCS-II 14 1979 98B NOAA-6 1979 57A COSMOS-11 08 1979 56A D C0SM0S-1109 1979 58A F D COSM0S-1110 1979 60 A L. -
Extension of Upper Limit Servers and Spectral Analysis of the X-Ray Binary GRO J1744−28
Extension of Upper Limit Servers and spectral analysis of the X-ray binary GRO J1744−28 Master's Thesis in Physics Presented by Ole K¨onig Wednesday 31st July, 2019 Dr. Karl Remeis-Sternwarte & ECAP Friedrich-Alexander-Universit¨atErlangen-N¨urnberg Supervisor: Prof. Dr. J¨ornWilms Abstract This thesis is about applications in the field of X-ray astronomy. It is divided into a software development and data analysis part. The Upper Limit Servers allow the user to generate long-term lightcurves of X-ray sources. They combine historical data and calculate upper limits in real-time. A web-based front- end provides facile querying, plotting and downloading of the data. They utilize data from 12 satellites including current observatories such as XMM-Newton, back to ROSAT, Einstein, Ariel V and Uhuru. This enables the user to query 50 years of X-ray data and, for instance, study outburst behavior of transient sources. Part I of this thesis describes the software layout, database format, as well as nine X-ray missions, which I implemented. In particular, the implementation of catalog calls, image footprints, point spread functions, and vignetting is described. The count rate is converted to a flux by approximating the spectral shape with an absorbed power-law or black body. In order to outline possible applications of this software, I interpret four lightcurves. In the second part, the spectral analysis of the low-mass X-ray binary GRO J1744−28 is presented. The ∼29 ks data was taken with the Nuclear Spectroscopic Telescope Array (NuSTAR) in 2017 February, during the source's fourth reactivation phase after three years of quiescence. -
<> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA
1 SATELITES ARTIFICIALES. Capítulo 5º Subcap. 10 <> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA TIERRA. Esta es una relación cronológica de todos los lanzamientos de satélites artificiales de nuestro planeta, con independencia de su éxito o fracaso, tanto en el disparo como en órbita. Significa pues que muchos de ellos no han alcanzado el espacio y fueron destruidos. Se señala en primer lugar (a la izquierda) su nombre, seguido de la fecha del lanzamiento, el país al que pertenece el satélite (que puede ser otro distinto al que lo lanza) y el tipo de satélite; este último aspecto podría no corresponderse en exactitud dado que algunos son de finalidad múltiple. En los lanzamientos múltiples, cada satélite figura separado (salvo en los casos de fracaso, en que no llegan a separarse) pero naturalmente en la misma fecha y juntos. NO ESTÁN incluidos los llevados en vuelos tripulados, si bien se citan en el programa de satélites correspondiente y en el capítulo de “Cronología general de lanzamientos”. .SATÉLITE Fecha País Tipo SPUTNIK F1 15.05.1957 URSS Experimental o tecnológico SPUTNIK F2 21.08.1957 URSS Experimental o tecnológico SPUTNIK 01 04.10.1957 URSS Experimental o tecnológico SPUTNIK 02 03.11.1957 URSS Científico VANGUARD-1A 06.12.1957 USA Experimental o tecnológico EXPLORER 01 31.01.1958 USA Científico VANGUARD-1B 05.02.1958 USA Experimental o tecnológico EXPLORER 02 05.03.1958 USA Científico VANGUARD-1 17.03.1958 USA Experimental o tecnológico EXPLORER 03 26.03.1958 USA Científico SPUTNIK D1 27.04.1958 URSS Geodésico VANGUARD-2A -
A Study of Background for IXPE
A Study of background for IXPE F. Xiea,∗, R. Ferrazzolia, P. Soffittaa, S. Fabiania, E. Costaa, F. Muleria, A. Di Marcoa aINAF-IAPS, via del Fosso del Cavaliere 100, I-00133 Roma, Italy Abstract Focal plane X-ray polarimetry is intended for relatively bright sources with a negligible impact of background. However this might not be always possible for IXPE (Imaging X-ray Polarimetry Explorer) when observing faint extended sources like supernova remnants. We present for the first time the expected background of IXPE by Monte Carlo simulation and its impact on real observations of point and extended X-ray sources. The simulation of background has been performed by Monte Carlo based on GEANT4 framework. The spacecraft and the detector units have been modeled, and the expected background components in IXPE orbital environment have been evaluated. We studied different background rejection techniques based on the analysis of the tracks collected by the Gas Pixel Detectors on board IXPE. The estimated background is about 2.9 times larger than the requirement, yet it is still negligible when observing point like sources. Albeit small, the impact on supernova remnants indicates the need for a background subtraction for the observation of the extended sources. Keywords: X-Ray, polarimeter, background 1. Introduction 16.1% ± 1.4% at 160:2° ± 2:6°, with a 10 standard deviation significance in six days observation. Furthermore, [6] reported The Imaging X-ray Polarimetry Explorer (IXPE) is a NASA with the same polarimeter the polarization measurement of the Astrophysics Small Explorer (SMEX) mission, selected in Jan- Crab nebula without pulsar contamination, resulting on a po- uary 2017. -
NASA Astronauts
PUBLISHED BY Public Affairs Divisio~l Washington. D.C. 20546 1983 IColor4-by-5 inch transpar- available free to information lead and sent to: Non-informstionmedia may obtain identical material for a fee through a photographic contractor by using the order forms in the rear of this book. These photqraphs are government publications-not subject to copyright They may not be used to state oiimply the endorsement by NASA or by any NASA employee of a commercial product piocess or service, or used in any other manner that might mislead. Accordingly, it is requested that if any photograph is used in advertising and other commercial promotion. layout and copy be submitted to NASA prior to release. Front cover: "Lift-off of the Columbia-STS-2 by artist Paul Salmon 82-HC-292 82-ti-304 r 8arnr;w u vowzn u)rorr ~ nsrvnv~~nrnno................................................ .-- Seasat .......................................................................... 197 Skylab 1 Selected Pictures .......................................................150 Skylab 2 Selected Pictures ........................................................ 151 Skylab 3 Selected Pictures ........................................................152 Skylab 4 Selected Pictures ........................................................ 153 SpacoColony ...................................................................183 Space Shuttle ...................................................................171 Space Stations ..................................................................198 \libinn 1 1f.d Apoiio 17/Earth 72-HC-928 72-H-1578 Apolb B/Earth Rise 68-HC-870 68-H-1401 Voyager ;//Saturn 81-HC-520 81-H-582 Voyager I/Ssturian System 80-HC-647 80-H-866 Voyager IN~lpiterSystem 79-HC-256 79-H-356 Viking 2 on Mars 76-HC-855 76-H-870 Apollo 11 /Aldrin 69-HC-1253 69-H-682 Apollo !I /Aldrin 69-HC-684 69-H-1255 STS-I /Young and Crippen 79-HC-206 79-H-275 STS-1- ! QTPLaunch of the Columbia" 82-HC-23 82-H-22 Major Launches NAME UUNCH VEHICLE MISSIONIREMARKS 1956 VANGUARD Dec. -
Riccardo Giacconi - a Hard Act to Follow
Riccardo Giacconi - a hard act to follow Ken Pounds University of Leicester in 1956 Riccardo was studying cosmic radiation with Beppo Occhialini in Milan …. as I graduated in Physics at UCL and accepted an Admiralty grant to join the new Rocket Group ant to join the new Rocket Group …….. initially with no rocket .… and no project …. but 3 more years of student life in London was attractive 1957 Skylark duly arrived • first flight at Woomera in February • payloads of 150 kg to 300 km (10 mins for x-ray observation) • Sun-pointing version from 1964 • PhD project : ‘Observing the Sun’s X-ray emission’ • data from flights in 1959 and 1960 1959 RG joined American Science and Engineering, a small military- space company in Cambridge 1960 I was ‘transferred’ to a Lectureship at Leicester to set up a Research Group to study‘solar and stellar X-ray sources’ with the Sun as the first (only realistic ?) target April 1962 Ariel 1 – exploring the ionosphere taking my solar spectrometer into orbit • Delta launch from Canaveral on 26 April All worked fine for 2.5 months, then … 9 July 1962 ‘The sky glowed red over Honolulu as X-rays from the Starfish nuclear test excited atomic oxygen in the atmosphere’ 2004 report to US Congress USAF 100Mt hydrogen bomb detonated 400 km above Johnstone Island in the Pacific swamping PCS detectors with radioactive debris! - also seriously damaging the spacecraft solar arrays DOD denials but then other satellites failed…. Riccardo was there! meanwhile – a few weeks earlier (12 June) – Herb Gursky led the ASE team at White Sands where…. -
Lanzamientos De Satelites Notificados En 1974
This electronic version (PDF) was scanned by the International Telecommunication Union (ITU) Library & Archives Service from an original paper document in the ITU Library & Archives collections. La présente version électronique (PDF) a été numérisée par le Service de la bibliothèque et des archives de l'Union internationale des télécommunications (UIT) à partir d'un document papier original des collections de ce service. Esta versión electrónica (PDF) ha sido escaneada por el Servicio de Biblioteca y Archivos de la Unión Internacional de Telecomunicaciones (UIT) a partir de un documento impreso original de las colecciones del Servicio de Biblioteca y Archivos de la UIT. (ITU) ﻟﻼﺗﺼﺎﻻﺕ ﺍﻟﺪﻭﻟﻲ ﺍﻻﺗﺤﺎﺩ ﻓﻲ ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﺃﺟﺮﺍﻩ ﺍﻟﻀﻮﺋﻲ ﺑﺎﻟﻤﺴﺢ ﺗﺼﻮﻳﺮ ﻧﺘﺎﺝ (PDF) ﺍﻹﻟﻜﺘﺮﻭﻧﻴﺔ ﺍﻟﻨﺴﺨﺔ ﻫﺬﻩ .ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﻓﻲ ﺍﻟﻤﺘﻮﻓﺮﺓ ﺍﻟﻮﺛﺎﺋﻖ ﺿﻤﻦ ﺃﺻﻠﻴﺔ ﻭﺭﻗﻴﺔ ﻭﺛﻴﻘﺔ ﻣﻦ ﻧﻘﻼ ً◌ 此电子版(PDF版本)由国际电信联盟(ITU)图书馆和档案室利用存于该处的纸质文件扫描提供。 Настоящий электронный вариант (PDF) был подготовлен в библиотечно-архивной службе Международного союза электросвязи путем сканирования исходного документа в бумажной форме из библиотечно-архивной службы МСЭ. © International Telecommunication Union lanzamientos de satélites notificados en 1974 Esta lista integra los satélites artificiales lanzados en 1974; está basada en los datos proporcionados por las administraciones de telecomunicaciones, el Comité de Investigaciones Espaciales (COSPAR), el Goddard Space Flight Center (GSFC — Centro de Vuelos Espaciales Goddard) de la Administración Nacional de la Aeronáutica y del Espacio (NASA), de Estados Unidos, el Ministerio de Comunicaciones de la URSS, el Centre national d'études spatiales (CNES), de Francia, la Junta Internacional de Registro de Frecuencias (IFRB), uno de los cuatro organismos permanentes de la UIT, y en las informaciones publicadas por la prensa especializada. -
Aeronautics and Space Report of the President 1981 Activities
Aeronautics and Space Report of the President 1981 Activities NOTE TO READERS: ALL PRINTED PAGES ARE INCLUDED, UNNUMBERED BLANK PAGES DURING SCANNING AND QUALITY CONTROL CHECK HAVE BEEN DELETED Aeronautics and Space Report of the President 1981 Activities National Aeronautics and Space Administration Washington, D.C. 20546 Con tents Page Page Summary ................................ 1 Department of Agriculture ................. 57 Communications ...................... 1 Federal Communications Commission ........ 58 Earth’s Resources and Environment ...... 2 CommunicationsSatellites .............. 58 Space Science ........................ 3 Experiments and Studies ............... 59 Space Transportation .................. 4 Department of Transportation .............. 61 International Activities ................ 5 Aviation Safety ....................... 61 Aeronautics .......................... 6 Environmental Research ............... 63 National Aeronautics and Space Air Navigation and Air Traffic Control ... 64 Administration ..................... 8 Environmental Protection Agency ........... 66 Applications to the Earth ............... 8 National Science Foundation ................ 67 Science .............................. 13 Smithsonian Institution .................... 68 Space Transportation .................. 19 Spacesciences ........................ 68 Space Research and Technology ......... 23 Lunar Research ...................... 69 Space Tracking and Data Services ........ 25 Planetary Research .................... 70 Aeronautical