PPT-The soft X-ray landscape of GRBs:

thermal components Rhaana Starling University of Leicester Royal Society Dorothy Hodgkin Fellow With special thanks to Martin Sparre DARKLeicester and Kim Page Leicester Outline GRB Xray spectra the basic shape. (in the era of pre-Gravitational Waves). Wen-fai. Fong. Harvard University. Advisor: Edo Berger. LIGO Open Data Workshop, Livingston, LA 10.27.2011. 1. GRB 070809. ACS/F606W. Outline. 1. Introduction to GRBs and our program. HSTs continuing contribution to gamma-ray bursts. Andrew Levan. University of Warwick. Javier . Gorosabel. . Urkia. . 27 Oct 1969- 21 Apr 2015. A major contributor to the field of gamma-ray bursts from the first afterglows to today. Requirements 22 cm (9 in) square of lightweight cotton fabric to use as backing. 22 cm (9 in) square of silk fabric. An assortment of small quantities of thread including cotton perle, cotton a broder Raffaella Margutti. Harvard – Institute for Theory and Computation. On behalf of the Harvard SN forensic team . Kyoto2013. What happens when jets barely break out of a star?. Type . Ic. SN. core. Thomas Krühler (DARK). Thanks to J. . Fynbo. , D. . Malesani. , J. . Hjorth. ,. J. Greiner, D. A. . Kann. , D. . Perley. , N. . Tanvir. , . S. . Klose. and many others. Very High Energy Phenomena in the . GRBs. in the era of . ELTs. Nial . Tanvir. University of Leicester. GRB types. Short duration bursts are suspected of being. (mostly) due . to compact binary mergers. Classical long bursts are associated with core collapse of. Gemma Anderson. ICRAR-Curtin University. 7 July 2016. gemma.anderson. @curtin.edu.au. ESO. Gamma-ray Bursts (GRBs). ICRAR-Curtin – science & engineering. Gemma Anderson, Transient triggering with AMI (ASA 2016) . (aka Swift J164449.3+573451). Prof. David Burrows,. Penn State. We now . know that . most galaxies have a supermassive black hole (SMBH) at their center. Most of these black holes are inactive (very weak emission). Swift short GRBs by the Chandra . sub-. arcsecond. position. T. Sakamoto, N. . Gehrels. , E. . Troja. , . J. Norris, S. . Barthelmy. , J. . Racusin. , . N. Kawai, A. . Fruchter. Mystery solved for short GRBs?. from keV to . GeV. energies and . beyond. . Elisabetta Bissaldi. Member of the Fermi-GBM and . Fermi-LAT Collaborations, . and of the CTA Consortium. Politecnico. . & INFN . Bari. elisabetta.bissaldi@ba.infn.it. Theories*. Arnon . Dar**. . Scientific theories must be . falsifiable (K. M. Popper 1959). . . Only confrontations of their main predictions, which do . not . depend . on free adjustable . parameters, with observational . Arnon. Dar* . Technion. , Haifa, Israel . *a. Based on :. - The . Smoking Guns Of Short Hard Gamma Ray . Bursts, . . Dado . and . Dar, arXiv:1708.04603. - Cannonball . model diagnosis of the short gamma ray burst . Arnon. Dar* . Technion. , Haifa, Israel . *a. * Based on:. - The . Smoking Guns Of Short Hard Gamma Ray . Bursts, . . Dado . and . Dar, arXiv:1708.04603 . - Cannonball . model diagnosis of the short gamma ray burst . . Luigi Piro. C. . Kouveliotou. , . J.W.. den . Herder. , T. Ohashi, D. . Hartmann. , D. . Burrows. and the . Xenia. team:. consortium. . of. . Institutes. . from. US, . Eu. , . Japan. Xenia. .