PPT-Bursts Kazuhiro Hayama

on behalf of the KAGRA burst working group Plans for the LVK collaboration papers Plans which will be integrated into existing LV burst plans Plans which are different from existing LV burst plans. By fo cusing on empathy and antipathy especially the process by which they are perceived by external observers this paper aims to elucidate the tendency of their perception and from it develop a computational model that realizes the automatic estima Alexander . Kotov. , . ChengXiang. . Zhai. , Richard . Sproat. University of Illinois at Urbana-Champaign. Roadmap. Problem definition. Previous work. Approach. Experiments. Summary. Motivation. Web data is generated by a large number of textual streams (news, blogs, tweets, etc. fast radio bursts . Vikram. Ravi. University of Melbourne and CASS. With Ryan Shannon and Paul . Lasky. And . with particular . thanks to the Swinburne CAS staff and students. 1. Fast radio bursts (. Ilir. . Capuni. and Peter . Gacs. Boston University. Introduction. ‘Regular’ transition. A faulty transition. A fault. : a violation of the transition function. Change the state, the tape symbol and move the head arbitrarily. 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. National Institute of Informatics. , Japan. 4. th. DIKU-IST Workshop, 2011. Modal-. μ Definable. Graph Transduction. What We Want to Do. Verification of . Graph-to-Graph Transformations. e.g., Queries on Graph-Structured Database. 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. G.F. Wieczorek reg015-082of 26 Figure 1. Map of California showing location of Sierra Nevada in California (along its eastern boundary,range extendsslightly into Nevada),physiographic regions of Calif Andrew Levan. University of Warwick. Burst durations. Swift 1644+57. Very long bursts are often image triggers (1000+s). Correction from Swift observed rates to astrophysical rates (at Swift limits) could be a factor 10. w. eb . Ryan Shannon, . ICRAR-Curtin/. ATNF (. Vikram. Ravi, Swinburne . Pulsar . Group). Outline. Fast radio bursts (. FRBs) . Exciting times!. FRB 131104 . The . (improbable/real-time) . discovery of an FRB to the Carina dwarf spheroidal. S. R. Kulkarni. References. This is a tutorial . Primary reference: E. Berger (2013) Annual Review. GW perspective: . Kalsiwal. & . Nissanke. (2013) . Properties. Defined primary by duration (T<2 . Edwin Kite (U. Chicago), John Armstrong (Weber State), . Robin Wordsworth (Harvard), Francois Forget (LMD) . c. an climate . models. h. elp distinguish. these scenarios?. h. abitable surface. s. terile surface. catch a burst and notify other observatoriesboth in space and on the ground of its approx-imate locationWithin minutes HETE-2 mayobtain a precise locationCurrent telescopestake much longer to notify o National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) .