PPT-Gamma-ray Burst Afterglow Spectroscopy

J P U Fynbo Niels Bohr Institute Dark Cosmology Centre What is a gammaray burst Brief ms min and intense 10 7 erg cm 2 s 1 burst of soft . A Keyser R M Twomey T R ORTEC PerkinElmer Instruments Inc 801 South I llinois Avenue Oak Ridge TN 37831 Abstract The loss of valid counts from the spectrum due to the system being busy is referred to as counting loss The traditional method of correc 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 . for the 1. st. Advanced LIGO Science Run. Jordan Camp. NASA Goddard Space Flight Center. Moriond. Gravitation Meeting. March 25, 2015. Search Team. Lindy Blackburn (. CfA. ). Nelson Christensen (Carleton College). extreme physics at play. Bruce Gendre. ARTEMIS. Description of a GRB. Gamma-ray Burst : . burst of high energy photons. Isotropic distribution on the sky. extragalactic events. . quite common (~2/day. Spectroscopy. Scott Powers. Molecular Spectroscopy Presentation. 1. Adolf . Mossbauer. Born on January 31, 1929. Born in Munich, Germany. Discovered ". Mossbauer. Effect". Won Nobel Prize in 1961 in physics. Osservatorio. di Roma / ASI Science Data Center. Recent activities from the TAROT/Zadko network. The TAROT/Zadko Network. Set of 3 robotic telescopes. France (20 cm diameter). Chile (20 cm diameter). 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. 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. H. . Herrmann (LANL. ). e. -. Next . Steps. Cherenkov detectors . Energy . thresholded. Gas limited to >2.5 . MeV. Solid limited to <~0.2 . MeV. Aerogel. might span the gap. Real . g. -ray spectroscopy (Energy resolved) . 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 InterSpec. Will Johnson. 1. UUR SAND2021-2864 TR. wcjohns@sandia.gov. , . InterSpec@sandia.gov. . Outline. What to expect. Physics review. Basics of using . InterSpec. to look at data. Nuclide ID. Fitting for activity and shielding. Marie-Laure Mauborgne. SLB. CSG17 – July 17. th. 2023. 1. Founded by a physicist and an engineer in 1926 to conduct the first geophysical measurements of rock formations . What is SLB?. (former Schlumberger). A novel gamma-ray detector configuration. Roi . Rahin*. Department of Physics, Technion. For . the. GALI collaboration. . *Ramon fellow by the Israeli Ministry of Science and Technology.. Background - Gamma ray bursts. Marie-Laure Mauborgne. , R. J. Radtke, Fabien . Haranger. Schlumberger. MMauborgne@slb.com. Founded in 1927 by a physicist and an engineer to conduct geophysical measurements of rock formations. Now:.