Gamma Ray Burst Discoveries with the Swift Mission

Slides:



Advertisements
Similar presentations
Jerry Fishman NASA - Marshall Space Flight Center National Space Science and Technology Center (NSSTC) Huntsville, AL AAVSO – HEA3 - Las Cruces, NM - March.
Advertisements

GRB : a canonical fake short burst L. Caito, M.G. Bernardini, C.L. Bianco, M.G. Dainotti, R. Guida, R. Ruffini. 3 rd Stueckelberg Workshop July 8–18,
Ten Years of Swift John Nousek,
Yun-Wei YU 俞云伟 June 22, 2010, Hong Kong. Outline  Background  Implications from the shallow decay afterglows of GRBs  A qualitative discussion on magnetar.
Wen-fai Fong Harvard University Advisor: Edo Berger LIGO Open Data Workshop, Livingston, LA GRB ACS/F606W.
1 Extreme Astronomy and Supernovae Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University.
Constraining the Properties of Dark Energy Using GRBs D. Q. Lamb (U. Chicago) High-Energy Transient ExplorerSwift Department of Astronomy, Nanjing University.
Swift 1 Swift Spacecraft and Instruments. Swift 2 Spacecraft Design 1 of 6 Reaction wheels Gyros Star Trackers.
Gamma-Ray Bursts: The Most Brilliant Events in the Universe D. Q. Lamb (U. Chicago) PHYSICS for the THIRD MILLENNIUM: II Huntsville, AL 5–7 April 2005.
Swift Identification of the host galaxy of Swift short GRBs by the Chandra sub-arcsecond position T. Sakamoto, N. Gehrels, E. Troja, J. Norris, S. Barthelmy,
NASA's Chandra Sees Brightest Supernova Ever N. Smith et al. 2007, astro-ph/ v2.
A burst of new ideas Nature Vol /28 December 2006 徐佩君 HEAR group meeting 12/
Short Bursts Daniel Perley Astro November 2005.
Discovery and Identification of the Very High Redshift Afterglow of GRB J. Hailsip, M. Nysewander, D. Reichart, A. Levan, N. Tavir, S. B. Cenko,
GRBs as a Probe of the Elemental Abundance History of the Universe D. Q. Lamb (U. Chicago) Workshop on Chemical Enrichment of the Early Universe Santa.
Gamma Ray Bursts and LIGO Emelie Harstad University of Oregon HEP Group Meeting Aug 6, 2007.
Swift Observations of GRBs David Burrows The Pennsylvania State University.
3rd Potsdam Thinkshop Robotic Astronomy Gamma-ray burst optical follow-ups with robotic telescopes M.I. Andersen Gamma-ray burst optical follow-ups with.
Gamma-Ray Bursts: The Biggest Explosions Since the Big Bang Edo Berger.
Gamma-Ray Bursts and Supernovae Tsinghua Transient Workshop 8 Nov 2012 Elena Pian INAF-Trieste Astronomical Observatory, Italy & Scuola Normale Superiore.
An Overview of the Swift Observatory Liz Puchnarewicz Mullard Space Science Laboratory University College London.
What are Gamma Waves?. ? Gamma-rays can kill living cells, a fact which medicine uses to its advantage, using gamma-rays to kill cancerous cells. Gamma-rays.
1 Short GRBs - and other recent developments in GRBs Tsvi Piran ( HU, Jerusalem) Dafne Guetta (Rome Obs.)
Gamma-Ray Bursts Mano-a-Mano. Short bursts T
Gamma-Ray Bursts observed by XMM-Newton Paul O’Brien X-ray and Observational Astronomy Group, University of Leicester Collaborators:- James Reeves, Darach.
1 John Nousek (Penn State University) ly Searching the Sky: The First Three Years of the Swift Gamma-Ray Burst Explorer III Cosmic Ray & Astrophysics School.
Dark Gamma-Ray Bursts and their Host Galaxies Volnova Alina (IKI RAS), Pozanenko Alexei (IKI RAS)
BH Astrophys. Ch3.6. Outline 1. Some basic knowledge about GRBs 2. Long Gamma Ray Bursts (LGRBs) - Why so luminous? - What’s the geometry? - The life.
Gamma-Ray Bursts Energy problem and beaming * Mergers versus collapsars GRB host galaxies and locations within galaxy Supernova connection Fireball model.
Gamma-Ray Bursts as a prototype of multi- messenger/time-domain astronomy, and the lessons we learned from unexpected discovery Nobuyuki Kawai (Tokyo Tech)
Mssl astrophysics group start Terribly hot stars. Liz Puchnarewicz Mullard Space Science Laboratory, UCL  -ray sources, missions.
The Progenitors of Short-Hard GRBs from an Extended Sample of Events Avishay Gal-Yam Hubble Fellow CALTECH.
Observational techniques meeting #15
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 11. Gamma-ray bursts.
G O D D A R D S P A C E F L I G H T C E N T E R 1 Recent GRB Results from Swift John Cannizzo/UMBC/Goddard LSC Meeting, Hanford, WA August 16, 2005 LIGO-G Z.
Moriond – 1 st -8 th Feb 2009 – La Thuile, Italy. Page 1 GRB results from the Swift mission Phil Evans, Paul O'Brien and the Swift team.
The nature of the longest gamma-ray bursts Andrew Levan University of Warwick.
Cosmic Explosions: Seeds of Life Poonam Chandra Royal Military College of Canada.
06/02/2009Diego Götz - The SVOM Mission1 La Thuile Italy 06/ th Rencontres de Moriond SVOM A new mission for Gamma-Ray Bursts Studies Diego Götz.
1 John Nousek & David Burrows (Penn State University) Alberto Moretti (Osservatorio Astronomico di Brera) X-Ray Telescope (XRT): Performance after Five.
The GRB Luminosity Function in the light of Swift 2-year data by Ruben Salvaterra Università di Milano-Bicocca.
Remembering Jack Tueller
1 John Nousek (Penn State University) Neil Gehrels (Goddard Space Flight Center) Five Years of Science: GRBs and More! International Workshop on Astronomical.
STScI Science Writers Workshop
The Exceptional GRB/XRF and its Associated SN 2006aj Jinsong Deng National Astronomical Observatories of China.
Gamma-Ray Bursts. Short (sub-second to minutes) flashes of gamma- rays, for ~ 30 years not associated with any counterparts in other wavelength bands.
(Review) K. Ioka (Osaka U.) 1.Short review of GRBs 2.HE  from GRB 3.HE  from Afterglow 4.Summary.
LIGO-G W Death Star Redux: 35-year mystery solved Fred Raab October 28, 2005.
Gamma Ray Bursts IV : Observational Techniques and some results Andrea Melandri INAF – Astronomical Observatory of Brera.
1 Gravitational waves from short Gamma-Ray Bursts Dafne Guetta (Rome Obs.) In collaboration with Luigi Stella.
Gamma-ray bursts Tomasz Bulik CAM K, Warsaw. Outline ● Observations: prompt gamma emission, afterglows ● Theoretical modeling ● Current challenges in.
Gamma-Ray Bursts Please press “1” to test your transmitter.
The Swift GRB Observatory
The Host Galaxies of Dust-Obscured Gamma-Ray Bursts
Gravitational waves from short Gamma-Ray Bursts
Remembering Neil Gehrels The Swift Legacy
Update on the triggered search for GRBs
What made GRBs & ? Palli Jakobsson
CEA-Saclay, IRFU-Service d’Astrophysique
Extreme Astronomy and Supernovae
Supernovae.
Einstein’s Universe and Beyond…
Short Gamma Ray Bursts Curtis DeWitt.
GRB-Supernova observations: State of the art
MAXI Mission M. Serino (RIKEN).
Soft gamma repeaters outside the Local group
Discovery of peculiar X-ray characteristics of AT2018cow with Swift
Observational techniques meeting #11
Swift observations of X-Ray naked GRBs
Chandra Science Highlight
Presentation transcript:

Gamma Ray Burst Discoveries with the Swift Mission Neil Gehrels NASA/GSFC N2PS2 - GWU June 16, 2008

Swift Mission NASA MIDEX . T<10 sec T<90 sec T<2 min BAT XRT UVOT 3 instruments - BAT, -rays 15-350 keV - XRT, X-rays, 0.2-10 keV - UVOT, opt, 170-650 nm Rapid slewing spacecraft Launch November 20, 2004 UVOT Position - < 1 arcsec BAT Position - 2 arcmin XRT Position - 5 arcsec XRT BAT . T<10 sec T<90 sec T<2 min

Massive Star Core Collapse Accompanied by supernae Short GRBs: NS-NS Mergers Long GRBs: Massive Star Core Collapse GRB 050724 elliptical host GRB 080319B "naked eye: burst First afterglow and identification from Swift Brightest objects in universe: - 5.5 magnitude @ 7.5 billion lt yrs Chandra XRT In star forming galaxies Accompanied by supernae Collapsar model In non-star forming galaxies No supernovae Merger model

SN 2008D Shock Breakout - XRT monitoring of NGC 2770 (27 Mpc) SN 2007uy - XRT monitoring of NGC 2770 (27 Mpc) revealed extremely luminous X-ray outburst - No BAT detection (i.e., not a GRB) - UVOT detection of SN rising 90 min later - Supernova 2008D - Shock breakout. May occur for all SN 9 Jan 2008 Soderberg et al. 2008