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-G050431-00-Z.

Slides:



Advertisements
Similar presentations
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,
Advertisements

1 Explaining extended emission Gamma-Ray Bursts using accretion onto a magnetar Paul O’Brien & Ben Gompertz University of Leicester (with thanks to Graham.
SOFT GAMMA REPEATERS Kevin Hurley UC Berkeley Space Sciences Laboratory THE SGR-SHORT BURST CONNECTION Kevin Hurley UC Berkeley Space Sciences Laboratory.
Bruce Gendre Osservatorio di Roma / ASI Science Data Center Recent activities from the TAROT/Zadko network.
Gamma-Ray bursts from binary neutron star mergers Roland Oechslin MPA Garching, SFB/TR 7 SFB/TR7 Albert Einstein‘s Century, Paris,
1 Gamma-Ray Bursts: Early afterglows, X-ray flares, and GRB cosmology Zigao Dai Nanjing University.
Yizhong Fan (Niels Bohr International Academy, Denmark Purple Mountain Observatory, China) Fan (2009, MNRAS) and Fan & Piran (2008, Phys. Fron. China)
Low-luminosity GRBs and Relativistic shock breakouts Ehud Nakar Tel Aviv University Omer Bromberg Tsvi Piran Re’em Sari 2nd EUL Workshop on Gamma-Ray Bursts.
What’s New with Gamma-Ray Bursts Jay Norris * University of Denver, Visiting Stanford/SLAC GRB Bimodal Duration Distribution Redshifts, Look-back times,
GRB afterglows as background sources for WHIM absorption studies A. Corsi, L. Colasanti, A. De Rosa, L. Piro IASF/INAF - Rome WHIM and Mission Opportunities.
Global Properties of X-ray Afterglows Observed with XRT ENWEI LIANG (梁恩维) University of Guangxi, Nanning astro.gxu.edu.cn Nanjing
1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
Constraining the Properties of Dark Energy Using GRBs D. Q. Lamb (U. Chicago) High-Energy Transient ExplorerSwift Department of Astronomy, Nanjing University.
1 Nanjing June 2008 A universal GRB photon energy – luminosity relationship * Dick Willingale, Paul O’Brien, Mike Goad, Julian Osborne, Kim Page, Nial.
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,
X-ray/Optical flares in Gamma-Ray Bursts Daming Wei ( Purple Mountain Observatory, China)
Ehud Nakar California Institute of Technology Gamma-Ray Bursts and GLAST GLAST at UCLA May 22.
A burst of new ideas Nature Vol /28 December 2006 徐佩君 HEAR group meeting 12/
Short Bursts Daniel Perley Astro November 2005.
Gamma-Ray Burst Early Afterglows Bing Zhang Physics Department University of Nevada, Las Vegas Dec. 11, 2005, Chicago, IL.
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.
The Transient Universe: AY 250 Spring 2007 Existing Transient Surveys: High Energy I: Gamma-Ray Bursts Geoff Bower.
Solution to the Short GRB Mystery D. Q. Lamb (U. Chicago) “New Views of the Universe” Kavli Institute Symposium in Honor of David Schramm Chicago, IL,
R. Margutti Harvard University LOS ALAMOS Where do we stand Log(Time) Log(Flux) Gamma-ray Prompt X-ray Flares Swift Steep Decay Shallow Decay Normal.
Natalia Tyurina Behalf of the MASTER-team MOSCOW STATE UNIVERSITY Sternberg Astronomical Institute MASTER prompt and follow-up.
Francisco J Virgili Prompt GRB Conference, 2011 March 5, 2011; Raleigh, NC.
Gamma-ray Bursts in the E-ELT era Rhaana Starling University of Leicester.
Gamma-Ray Bursts and Supernovae Tsinghua Transient Workshop 8 Nov 2012 Elena Pian INAF-Trieste Astronomical Observatory, Italy & Scuola Normale Superiore.
Swift Kyoto GRB Conference BAT2 GRB Catalog Prompt Emission Properties of Swift GRBs T. Sakamoto (CRESST/UMBC/GSFC) on behalf of Swift/BAT.
GRB s CENTRAL -ENGINE & FLARes WARSAW Guido Chincarini & Raffaella margutti 1WARSAW 2009.
Monte-Carlo Simulation of Thermal Radiation from GRB Jets Sanshiro Shibata (Konan Univ.) Collaborator: Nozomu Tominaga (Konan Univ., IPMU)
The soft X-ray landscape of GRBs: thermal components Rhaana Starling University of Leicester Royal Society Dorothy Hodgkin Fellow With special thanks to.
Gamma Ray Bursts: open issues  Brief history  Power  Short history of the paradigm: internal vs external shocks  Afterglows: external shocks  The.
Gamma Ray Bursts Poonam Chandra National Centre for Radio Astrophysics Tata Institute of Fundamental Research.
New Views of Compact Object Mergers Via Short Gamma-Ray Bursts Derek B. Fox Astronomy & Astrophysics Penn State University New Views of the Universe –
The Long and the Short of Gamma-Ray Bursts Kevin Hurley UC Berkeley Space Sciences Laboratory.
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
Short Gamma-Ray Bursts and Compact Binary Mergers – Predictions for LIGO Ehud Nakar The California Institute of Technology LIGO seminar, 2005 Dec. 9.
Dark Gamma-Ray Bursts and their Host Galaxies Volnova Alina (IKI RAS), Pozanenko Alexei (IKI RAS)
A Tidal Disruption model for gamma-ray burst of GRB YE LU National Astronomical Observatories, Chinese Academy of Sciences June 22-27, 2008 Nanjing.
Gamma-Ray Bursts Energy problem and beaming * Mergers versus collapsars GRB host galaxies and locations within galaxy Supernova connection Fireball model.
Photospheric emission from Structured Jet Hirotaka Ito Collaborators Shigehiro Nagataki YITP @ YITP Lunch Seminar /30 Shoichi Yamada Waseda University.
Gamma-Ray Bursts: Open Questions and Looking Forward Ehud Nakar Tel-Aviv University 2009 Fermi Symposium Nov. 3, 2009.
Is GRB050509b a genuine short? Gustavo de Barros, Maria Grazia Bernardini, Carlo Luciano bianco, Roberto Guida, Remo Ruffini.
The Progenitors of Short-Hard GRBs from an Extended Sample of Events Avishay Gal-Yam Hubble Fellow CALTECH.
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.
Chandra Searches for Late-Time Jet Breaks in GRB Afterglows David Burrows, Judith Racusin, Gordon Garmire, George Ricker, Mark Bautz, John Nousek, & Dirk.
The nature of the longest gamma-ray bursts Andrew Levan University of Warwick.
Edo Berger − Harvard University Toward the Progenitors of Short-Duration Gamma-Ray Bursts The Prompt Activity of Gamma-Ray Bursts: their Progenitors, Engines,
The Lag-Luminosity Relation in the GRB Source Frame T. N. Ukwatta 1,2, K. S. Dhuga 1, M. Stamatikos 3, W. C. Parke 1, T. Sakamoto 2, S. D. Barthelmy 2,
STScI Science Writers Workshop
The Exceptional GRB/XRF and its Associated SN 2006aj Jinsong Deng National Astronomical Observatories of China.
(Review) K. Ioka (Osaka U.) 1.Short review of GRBs 2.HE  from GRB 3.HE  from Afterglow 4.Summary.
A relation to estimate the redshift from the X-ray afterglow light curve Bruce Gendre (IASF-Roma/INAF) & Michel Boër (OHP/CNRS)
Masnori Ohno (ISAS/JAXA). Long/Short GRBs are different ? There are two GRB classes, Long/Short GRBs in T90 distribution Different origin ? Hardness ratio;
Alessandra Corsi (1,2) Dafne Guetta (3) & Luigi Piro (2) (1)Università di Roma Sapienza (2)INAF/IASF-Roma (3)INAF/OAR-Roma Fermi Symposium 2009, Washington.
Eric Charles Two recent developments with Gamma Ray Burst Classification And their implications for GLAST Glast Science Lunch Nov. 2, 2006.
LIGO-G Z Compact object merger rates Predictions Constraints (including short GRBs) Richard O’Shaughnessy Vicky Kalogera Northwestern University.
Radio afterglows of Gamma Ray Bursts Poonam Chandra National Centre for Radio Astrophysics - Tata Institute of Fundamental Research Collaborator: Dale.
A complete sample of long bright Swift GRBs: correlation studies Paolo D’Avanzo INAF-Osservatorio Astronomico di Brera S. Campana (OAB) S. Covino (OAB)
The prompt optical emission in the Naked Eye Burst R. Hascoet with F. Daigne & R. Mochkovitch (Institut d’Astrophysique de Paris) Kyoto − Deciphering then.
Classification of Gamma-Ray Bursts: an observational review Paolo D’Avanzo INAF – Osservatorio Astronomico di Brera.
Gamma-ray bursts Tomasz Bulik CAM K, Warsaw. Outline ● Observations: prompt gamma emission, afterglows ● Theoretical modeling ● Current challenges in.
The Mysterious Burst After the Short Burst Jay Norris Brief History, Overview, Central Questions Spectral lag distributions (long & short GRBs) Pulse width.
Update on the triggered search for GRBs
Gamma Ray Burst Discoveries with the Swift Mission
Summary Talk: AGN and Gamma Rays Martin Pohl Iowa State University
Swift observations of X-Ray naked GRBs
Presentation transcript:

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

G O D D A R D S P A C E F L I G H T C E N T E R 2 GRBs Trace Comoving Volume dV/dz = 4πD 2 (z) dD(z)/dz 36 pre-Swift: =1.4, σ(z)=1.0 7 Swift + 2 other: =2.3, σ(z)=1.3

G O D D A R D S P A C E F L I G H T C E N T E R 3 Frail et al. (2001) [1] V(z<10) = 4x10 3 Gpc 3 GRB Rate: [2] Luminosity Density (V band) = 2x10 17 L ° Gpc -3 => about galaxies [3] Rate(BATSE) ~10 3 yr -1 So, rate per galaxy is about 1 in 10 7 yr.

G O D D A R D S P A C E F L I G H T C E N T E R 4 Long GRBs: Jet from a Collapsar (Weiqun Zhang - Stanford)

G O D D A R D S P A C E F L I G H T C E N T E R 5 Short GRBs: NS-NS Merger (Max Ruffert - University of Edinburgh)

G O D D A R D S P A C E F L I G H T C E N T E R 6 BAT+XRT 2-10 keV Decay; f=f 0 t - α Barthelmy et al. (2005)

G O D D A R D S P A C E F L I G H T C E N T E R 7 Interpretation: “Curvature Effect” Kumar & Panaitescu (2000):

G O D D A R D S P A C E F L I G H T C E N T E R 8 First Localization of a Short GRB GRB050509b: 40 ms duration (BAT), soft part of the short/hard population XRT: 11 photons (10 σ sig.) z=0.225 elliptical galaxy chance probability ~10 -4 E iso =1.1x10 48 erg ( keV) ~10 2 E(2004 Dec 27 SGR flare) --> supports NS-NS merger Gehrels et al. (2005)

G O D D A R D S P A C E F L I G H T C E N T E R 9 Summary GRBs trace comoving volume of the Universe, which exhibits a maximum at z~1-2. In two cases, the prompt emission seen in BAT+XRT forms a continuous decay with t - α, where α ~3, consistent with “curvature radiation” effect. Localization of one short GRB appears to be in a luminous, non-star forming elliptical galaxy, consistent with NS-NS merger theory.