Future of Hubble Data NASA Award for ST-ECF Staff Finding Solar
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STS-103 Table of Contents Mission Overview
Refining the Hubble Space Telescope's View of the Universe SPACESPACESPACE SHUTTLESHUTTLESHUTTLE PRESSKITPRESSKITPRESSKIT WWW.SHUTTLEPRESSKIT.COM Updated November 24, 1999 STS-103 Table of Contents Mission Overview ......................................................................................................... 1 Mission Profile .............................................................................................................. 8 Crew.............................................................................................................................. 10 Flight Day Summary Timeline ...................................................................................................14 Rendezvous Rendezvous, Retrieval and Deploy ......................................................................................................18 EVA Hubble Space Telescope Extravehicular Activity ..................................................................................21 EVA Timeline ........................................................................................................................................24 Payloads Fine Guidance Sensor .........................................................................................................................27 Gyroscopes .........................................................................................................................................28 New Advanced Computer .....................................................................................................................30 -
Hubble Space Telescope
HUBBLE SPACE TELESCOPE Pioneering optics made by Ball Aerospace are ® GO BEYOND WITH BALL. responsible for the Hubble Space Telescope’s iconic images and revolutionary discoveries. In total, Ball has built seven instruments for Hubble, including the five currently aboard the telescope. Beginning with the first servicing mission in 1993 through the fourth in 2009, Ball’s advanced optical technologies have extended Hubble’s operational life and enabled the telescope to help us understand our universe as never before. OUR ROLE QUICK FACTS Since scientists began formulating the idea for Hubble, • Ball-built seven science instruments for the first major optical telescope in space, Ball played a Hubble, two star trackers, five major leave- part, providing a total of seven science instruments flown behind equipment subsystems. on Hubble. Today, Ball supports COS, WFC3, ACS, STIS and NICMOS and provides on-orbit mission operations • Each of the five science instruments now support. After the last servicing mission in 2009, Hubble’s operating on the telescope were Ball-designed unprecedented science capabilities made it the premier and built. space-based telescope for ultraviolet, optical and near- • Ball-built COSTAR was installed during infrared astronomy. Servicing Mission 1 in 1993 along with JPL’s Cosmic Origins Spectrograph (COS) WFPC-2 to correct Hubble’s hazy vision. COS is the most sensitive ultraviolet spectrograph ever • Ball developed more than eight custom tools built for space and replaced the Ball-built COSTAR in 2009. to support astronauts during COS improved Hubble’s ultraviolet sensitivity at least 10 servicing missions. times and up to 70 times when observing very faint objects, like distant quasars, massive celestial objects, too faint for previous spectrographs. -
Space Reporter's Handbook Mission Supplement
CBS News Space Reporter's Handbook - Mission Supplement Page 1 The CBS News Space Reporter's Handbook Mission Supplement Shuttle Mission STS-125: Hubble Space Telescope Servicing Mission 4 Written and Produced By William G. Harwood CBS News Space Analyst [email protected] CBS News 5/10/09 Page 2 CBS News Space Reporter's Handbook - Mission Supplement Revision History Editor's Note Mission-specific sections of the Space Reporter's Handbook are posted as flight data becomes available. Readers should check the CBS News "Space Place" web site in the weeks before a launch to download the latest edition: http://www.cbsnews.com/network/news/space/current.html DATE RELEASE NOTES 08/03/08 Initial STS-125 release 04/11/09 Updating to reflect may 12 launch; revised flight plan 04/15/09 Adding EVA breakdown; walkthrough 04/23/09 Updating for 5/11 launch target date 04/30/09 Adding STS-400 details from FRR briefing 05/04/09 Adding trajectory data; abort boundaries; STS-400 launch windows Introduction This document is an outgrowth of my original UPI Space Reporter's Handbook, prepared prior to STS-26 for United Press International and updated for several flights thereafter due to popular demand. The current version is prepared for CBS News. As with the original, the goal here is to provide useful information on U.S. and Russian space flights so reporters and producers will not be forced to rely on government or industry public affairs officers at times when it might be difficult to get timely responses. All of these data are available elsewhere, of course, but not necessarily in one place. -
Wide Field Camera 3 Instrument Mini-Handbook for Cycle 16
Version 3.0 October 2006 Wide Field Camera 3 Instrument Mini-Handbook for Cycle 16 For long-term planning only Do not propose for WFC3 in Cycle 16 Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 [email protected] Operated by the Association of Universities for Research in Astronomy, Inc., for the National Aeronautics and Space Administration User Support For prompt answers to any question, please contact the STScI Help Desk. • E-mail: [email protected] • Phone: (410) 338-1082 (800) 544-8125 (U.S., toll free) World Wide Web Information and other resources are available on the WFC3 World Wide Web sites at STScI and GSFC: • URL: http://www.stsci.edu/hst/wfc3 • URL: http://wfc3.gsfc.nasa.gov WFC3 Mini-Handbook Revision History Version Date Editor 3.0 October 2006 Howard E. Bond 2.0 October 2003 Massimo Stiavelli 1.0 October 2002 Mauro Giavalisco Contributors: Sylvia Baggett, Tom Brown, Howard Bushouse, Mauro Giavalisco, George Hartig, Bryan Hilbert, Randy Kimble, Matt Lallo, Olivia Lupie, John MacKenty, Larry Petro, Neill Reid, Massimo Robberto, Massimo Stiavelli. Citation: In publications, refer to this document as: Bond, H. E., et al. 2006, “Wide Field Camera 3 Instrument Mini-Handbook, Version 3.0” (Baltimore: STScI) Send comments or corrections to: Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 E-mail:[email protected] Acknowledgments The WFC3 Science Integrated Product Team (2006) Sylvia Baggett Howard Bond Tom Brown Howard Bushouse George Hartig Bryan Hilbert Robert Hill (GSFC) -
Probing Star Formation and Radio Activity Using Faint Galaxy Redshift Surveys
Durham E-Theses Probing star formation and radio activity using faint galaxy redshift surveys Davies, Gregory Tudor How to cite: Davies, Gregory Tudor (2008) Probing star formation and radio activity using faint galaxy redshift surveys, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/2224/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk Probing Star Formation and Radio Activity using Faint Galaxy Redshift Survey by Gregory Tudor Davies A thesis submitted to the University of Durham in accordance with the regulations for admittance to the Degree of Doctor of Philosophy. Department of Physics University of Durham October 2008 The copyright of this thesis rests with the author or the university to which it was submitted. No quotation from it, or information derived from it may be published without the prior written consent of the author or university, and any information derived from it should be acknowledged. -
A Catalog of Mid-Infrared Sources in the Extended Groth Strip
A catalog of mid-infrared sources in the Extended Groth Strip P. Barmby,1,2 J.-S. Huang,1 M.L.N. Ashby,1 P.R.M. Eisenhardt,3 G.G. Fazio,1 S.P. Willner,1 E.L. Wright4 ABSTRACT The Extended Groth Strip (EGS) is one of the premier fields for extragalactic deep surveys. Deep observations of the EGS with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope cover an area of 0.38 deg2 to a 50% completeness limit of 1.5 µJy at 3.6 µm. The catalog comprises 57434 objects detected at 3.6 µm, with 84%, 28%, and 24% also detected at 4.5, 5.8, and 8.0 µm. Number counts are consistent with results from other Spitzer surveys. Color distributions show that the EGS IRAC sources comprise a mixture of populations: low-redshift star-forming galaxies, quiescent galaxies dominated by stellar emission at a range of redshifts, and high redshift galaxies and AGN. Subject headings: infrared: galaxies — galaxies: high-redshift — surveys — catalogs 1. Introduction Observations of unbiased, flux-limited galaxy samples via ‘blank-field’ extragalactic sur- veys have been a mainstay in the field of galaxy formation and evolution for several decades, with the well-known Hubble Deep Field (Williams et al. 1996) and Sloan Digital Sky Survey (York et al. 2000) exemplifying two very different types of galaxy survey. Extending the wavelength coverage as broadly as possible has led to numerous changes in the understand- ing of how galaxies form, evolve, and interact over cosmic time. New technologies and larger telescopes continually increase the volume of discovery space, making some ‘state-of-the-art’ observations obsolete in just a few years. -
Stsci Newsletter: 2011 Volume 028 Issue 02
National Aeronautics and Space Administration Interacting Galaxies UGC 1810 and UGC 1813 Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) 2011 VOL 28 ISSUE 02 NEWSLETTER Space Telescope Science Institute We received a total of 1,007 proposals, after accounting for duplications Hubble Cycle 19 and withdrawals. Review process Proposal Selection Members of the international astronomical community review Hubble propos- als. Grouped in panels organized by science category, each panel has one or more “mirror” panels to enable transfer of proposals in order to avoid conflicts. In Cycle 19, the panels were divided into the categories of Planets, Stars, Stellar Rachel Somerville, [email protected], Claus Leitherer, [email protected], & Brett Populations and Interstellar Medium (ISM), Galaxies, Active Galactic Nuclei and Blacker, [email protected] the Inter-Galactic Medium (AGN/IGM), and Cosmology, for a total of 14 panels. One of these panels reviewed Regular Guest Observer, Archival, Theory, and Chronology SNAP proposals. The panel chairs also serve as members of the Time Allocation Committee hen the Cycle 19 Call for Proposals was released in December 2010, (TAC), which reviews Large and Archival Legacy proposals. In addition, there Hubble had already seen a full cycle of operation with the newly are three at-large TAC members, whose broad expertise allows them to review installed and repaired instruments calibrated and characterized. W proposals as needed, and to advise panels if the panelists feel they do not have The Advanced Camera for Surveys (ACS), Cosmic Origins Spectrograph (COS), the expertise to review a certain proposal. Fine Guidance Sensor (FGS), Space Telescope Imaging Spectrograph (STIS), and The process of selecting the panelists begins with the selection of the TAC Chair, Wide Field Camera 3 (WFC3) were all close to nominal operation and were avail- about six months prior to the proposal deadline. -
16Th HEAD Meeting Session Table of Contents
16th HEAD Meeting Sun Valley, Idaho – August, 2017 Meeting Abstracts Session Table of Contents 99 – Public Talk - Revealing the Hidden, High Energy Sun, 204 – Mid-Career Prize Talk - X-ray Winds from Black Rachel Osten Holes, Jon Miller 100 – Solar/Stellar Compact I 205 – ISM & Galaxies 101 – AGN in Dwarf Galaxies 206 – First Results from NICER: X-ray Astrophysics from 102 – High-Energy and Multiwavelength Polarimetry: the International Space Station Current Status and New Frontiers 300 – Black Holes Across the Mass Spectrum 103 – Missions & Instruments Poster Session 301 – The Future of Spectral-Timing of Compact Objects 104 – First Results from NICER: X-ray Astrophysics from 302 – Synergies with the Millihertz Gravitational Wave the International Space Station Poster Session Universe 105 – Galaxy Clusters and Cosmology Poster Session 303 – Dissertation Prize Talk - Stellar Death by Black 106 – AGN Poster Session Hole: How Tidal Disruption Events Unveil the High 107 – ISM & Galaxies Poster Session Energy Universe, Eric Coughlin 108 – Stellar Compact Poster Session 304 – Missions & Instruments 109 – Black Holes, Neutron Stars and ULX Sources Poster 305 – SNR/GRB/Gravitational Waves Session 306 – Cosmic Ray Feedback: From Supernova Remnants 110 – Supernovae and Particle Acceleration Poster Session to Galaxy Clusters 111 – Electromagnetic & Gravitational Transients Poster 307 – Diagnosing Astrophysics of Collisional Plasmas - A Session Joint HEAD/LAD Session 112 – Physics of Hot Plasmas Poster Session 400 – Solar/Stellar Compact II 113 -
Important Events in Chile
No. 87 – March 1997 Important Events in Chile R. GIACCONI, Director General of ESO The political events foreseen in the December 1996 issue of The Messenger did take place in Chile in the early part of December 1996. On December 2, the Minister of Foreign Affairs of the Republic of Chile, Mr. Miguel Insulza, and the Director General of ESO, Professor Riccardo Giacconi, exchanged in Santiago Instruments of Ratification of the new “Interpretative, Supplementary and Amending Agreement” to the 1963 Convention between the Government of Chile and the European Southern Observatory. This agreement opens a new era of co-operation between Chilean and European Astronomers. On December 4, 1996, the “Foundation Ceremony” for the Paranal Observatory took place on Cerro Paranal, in the presence of the President of Chile, Mr. Eduardo Frei Ruiz-Tagle, the Royal couple of Sweden, King Carl XVI Gustaf and Queen Silvia, the Foreign Minister of the Republic of Chile, Mr. José Miguel Insulza, the Ambassadors of the Member States, members of the of the ESO Executive, ESO staff and the Paranal contractors’ workers. The approximately 250 guests heard addresses by Dr. Peter Creo- la, President of the ESO Council, Professor Riccardo Giacconi, Direc- tor General of ESO, Foreign Minis- ter José Miguel Insulza and Presi- dent Eduardo Frei Ruiz-Tagle. The original language version of the four addresses follows this introduction. (A translation in English of the Span- ish text is given on pages 58 and 59 in this issue of The Messenger.) A time capsule whose contents are described in Dr. Richard West's article was then deposited by Presi- dent Frei with the works being bless- ed by the Archbishop of Antofagas- ta, Monsignor Patricio Infante. -
Hubble Space Telescope's
Hubble Space Telescope’s Top Science Findings When Galileo used his homemade telescope 400 years ago to view mountains on the Moon, satellites cir- cling Jupiter, and a myriad of stars in our Milky Way Galaxy, he launched a revolution that changed our view of an Earth-cen- tered universe. The launch of NASA’s Hubble Space Telescope aboard the space shuttle Discovery 17 years ago initiated another revolution in astronomy. For the first time, a large telescope that sees in visible light be- gan orbiting above Earth’s distorting atmosphere, which blurs starlight and makes images appear fuzzy. Astronomers anticipated great discoveries from Hubble. The telescope has delivered as promised and continues serving up new discoveries. Astronomers and astrophysicists using Hubble data have published more than 4,000 scientific papers, on top- ics from the solar system to the very distant universe. The following list highlights some of Hubble’s greatest achievements. 2 Hubble Space Telescope’s Top Science Findings Shining a Light on Dark Matter Astronomers used Hubble to make the first three-dimensional map of dark matter, which is considered the construction scaffolding of the universe. Dark matter’s invisible gravity allows normal matter in the form of gas and dust to collect and build up into stars and galaxies. The Hubble telescope played a starring role in helping to shed light on dark matter, which is much more abundant than normal matter. Although astronomers cannot see dark matter, they can detect it in galaxy clusters by observ- ing how its gravity bends the light of more distant background galaxies, a phenomenon called gravitational lensing. -
Number 28 Space Telescope European Coordinating Facility
January 2001 Number 28 Page 1 Number 28 January 2001 This 140 nm ultraviolet image of Jupiter was taken with the Hubble Space Telescope Imaging Spectrograph (STIS) on 26 November 1998 (Credit: NASA; ESA & John T. Clarke, Univ. of Michigan) when Jupiter was at a distance of 700 million km from Earth. In addition to the main auroral oval, centred on the magnetic north pole, and a pattern of more diffuse emission inside the polar cap, unique features are the ‘magnetic footprints’ of three of Jupiter’s satellites, Io, Ganymede and Europa. Space Telescope ST-ECF Newsletter ST-ECF European Coordinating Facility Page 2 ST–ECF Newsletter European news As the ESA contribution to HST moves away Group and, in September, by the Space Science Advisory from hardware provision, support for another Committee that NGST be selected as the next ‘Flexi-mission’ project has been agreed for the ST-ECF. in ESA’s future plan for implementation between 2008 and Following the successful provision of a 2013. This selection was endorsed by the Science Programme software package for extraction of NICMOS Committee at its meeting in October. grism spectra (NICMOSLook, see ST-ECF Newsletter 24, p. 7, This approval has allowed ESA to follow up the industry 1997), support for the spectroscopic modes of the ACS will studies it funded during 1999 with new investigations also be provided. ACS has both grisms and prisms: the Wide focussed on the specific European contributions to the Field Camera, with a coverage of 3.4' × 3.4', is fitted with a mission. In November, a study of the 1–5µm near-IR multi- grism offering 40Å/pixel resolution (5500–11000Å) over the object spectrograph to be provided by ESA was awarded to a full WFC field; the High resolution Camera (26'' × 29'') consortium headed by Astrium (Munich) and Laboratoire provides 30Å/pix grism spectra and prism spectra with a d’Astronomie Spatiale (Marseille). -
NASA-ATP09-Submitted
Cover Page for Proposal NASA Proposal Number Submitted to the National Aeronautics and 09-ATP09-0189 Space Administration NASA PROCEDURE FOR HANDLING PROPOSALS This proposal shall be used and disclosed for evaluation purposes only, and a copy of this Government notice shall be applied to any reproduction or abstract thereof. Any authorized restrictive notices that the submitter places on this proposal shall also be strictly complied with. Disclosure of this proposal for any reason outside the Government evaluation purposes shall be made only to the extent authorized by the Government. SECTION I - Proposal Information Principal Investigator E-mail Address Phone Number Joel Primack [email protected] 831-459-2580 Street Address (1) Street Address (2) 1156 High St Physics Department City State / Province Postal Code Country Code Santa Cruz CA 95064-1077 US Proposal Title : Evolution of Structure and of the Cosmic Population of Galactic Spheroids Proposed Start Date Proposed End Date Total Budget Year 1 Budget Year 2 Budget Year 3 Budget Year 4 Budget 01 / 01 / 2010 12 / 31 / 2012 577090.00 168877.00 200832.00 207381.00 0.00 SECTION II - Application Information NASA Program Announcement Number NASA Program Announcement Title NNH09ZDA001N-ATP Astrophysics Theory For Consideration By NASA Organization (the soliciting organization, or the organization to which an unsolicited proposal is submitted) Astrophysics Date Submitted Submission Method Grants.gov Application Identifier Applicant Proposal Identifier 05 / 29 / 2009 Electronic Submission