PPT-Working Party on Noise (GRB)

General information and WP29 highlights ParticipantsAddress list A provisional address list has been prepared please check your contact data especially the emailaddress and correct them if . Vanessa Griffin, Satya Kalluri, Chris Wheeler. , Kathleen Fontaine, Joe . Zajic. , and Raj Khanna. 20 October 2011. Remote Backup (RBU) Facility. – Fairmont, WV. Wallops Command and Data Acquisition Station (WCDAS). Bethany Elisa Cobb. The George Washington University. IAU. Symposium 279. March 13, 2012. (. Fynbo. et al. 2000). GRB-SNe Connection. Energy considerations. Long-duration GRBs associated with star-forming host galaxies . R. egulation. GRB 62. Transmitted by IWG QRTV for UN Regulation . . Informal document. . GRB-. 62. -22. (. 62nd . GRB, . . 1-3 September . 2015,. agenda item . 11). . QRTV . concerns. by GRB. QRTV basic aspect : 10 meetings . t. he. . Parkes. 12 . m. Keith Bannister. k.bannister@physics.usyd.edu.au. Sydney Institute for Astronomy (SIfA) University of Sydney. CSIRO Astronomy and Space Science. CAASTRO. Supervised By:. Tara Murphy (USyd). Andrew Levan. University of Warwick. Parameter space. Kouveliotou. et al. 1993. Parameter space. Kulkarni. & . Kasliwal. 2010. Parameter space. LGRBs. SGRBs. SGRs. ?. TDEs?. Galactic sources (SGR, LMXB, HMXB, . in GRB Host Galaxies. Patricia Schady. (MPE). T.Dwelly. , . M.J.Page. , . J.Greiner. ,. T.Krühler. , . S.Savaglio. , . S.R.Oates. , . A.Rau. , . M.Still. + GROND and UVOT team. z. Number of . GRBs. GeV. Photon Delay. Kunihito. . Ioka. (KEK). Contents. Very High Lorentz Factor (VHLF). G. max. can be up to ~10. 6. (> . G. max,. conv. ~10. 3. ). Internal Shock Synchrotron. ⇒ Power-law component over >7 decades. 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. (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). Judy Racusin. Penn State University. 2008 Nanjing GRB Workshop, Nanjing, China, June 23-27. Broadband Observations of the Extraordinary . Naked-Eye GRB 080319B. . J. L. . Racusin. , S.V. . Karpov. , M. . Remembering Neil . Gehrels. The Swift Legacy. . FOE2017 – Corvallis OR – 5 June 2017. What Are Gamma Ray Bursts?. Very bright -ray flashes. Occur ~ daily. Millisecond to minute durations. Isotropic on Sky. Don Warren. RIKEN – ABBL. 6 Jun 2017. With:. Don Ellison (NCSU). Maxim Barkov (. RIKEN/Purdue). Shigehiro. . Nagataki. (RIKEN. ), and more?. Preview slide!. Radio/optical/X-ray for afterglow models with/. User Readiness for GRB and HRIT/EMWIN Paul Seymour and Matthew Seybold NOAA/NESDIS/OSPO/Satellite Products and Services Division NCWCP College Park, MD and NSOF Suitland, MD Paul.Seymour@noaa.gov Matthew.Seybold@noaa.gov Technical Comments by ISO. Doug Moore. Convener, ISO TC22&TC43 WG42. Transmitted by the expert from . ISO. . . Informal document. . GRB-. 63. -11. (. 63rd . GRB, . 16-18 February 2016,. agenda .