May 23, 1969 into high earth ... The Vela 5 satellites functioned from July, 1969 to April, 1979 ... bright flash of gamma-rays lasting typically about 20 ...
The Vela 5 satellites functioned from July, 1969 to April, 1979 ... March 3, 1997 (fainter by 20) Groot, Galama, von Paradijs, et al IAUC 6584, March 12, 1997 ...
An utopia of a Geant4 user. Summary and some acknowledgements ... Airworthiness above all. Vibration attenuation. Temperature control. Modularity. Easy installation ...
Mikael Hult (S), Group leader low-level measurements, co-ordinator of CELLAR, ... CELLAR-actions. Setting up of a programme (in close. contact with ICRM LLWG) ...
University of the West of Scotland. Paisley Campus. Contents. Physics motivation ... of Engineering and Science, University of the West Scotland, Paisley PA1 2BE, UK ...
... GRB models. Lecture 5: Black Hole Accretion Disk Models. Black Hole ... Future models and future observational missions. GRBs The Historical Perspective ...
Energy index of ultra-relativistic electrons is also a free variable. p=2.2 is favored by theory ... ROTSE, TAROT, BOOTES, REM, NGAT... Rapid Response by ...
Several arrays of ground-based detectors achieve a sensitivity 1/100 of the flux ... view ~ 1 steradian) MILAGRO (LosAlamos, USA), Tibet ARGO (Yang Ba Jing, Tibet) ...
The Auto Correlation Function. Wavelet analysis. Power Density Spectra. Interpreting ... Quantify intrinsic delay, the 'pulse paradigm' can hide the QG effect ! ...
Introduction to Prompt Gamma-Ray Imaging. Introduction to Geant4. PGI Simulation by Geant4 ... 370kev prompt gamma-ray from Hg. 6Mev prompt gamma rays from Hg ...
Harvard CfA Meeting on GRBs, May 21, 2002. Requirements on the Central Engine ... The Jet-Star. Interaction. Relativistic Jet Propagation Through the Star ...
as seen by FGST. Nicola Omodei, INFN Pisa. for the Fermi Collaboration ... Isotropy, Uniformity, and Bimodality. Some hint at high energy (EGRET) COUNTERPARTS! ...
Enrico Fermi (1901-1954) was an Italian physicist who immigrated to ... starburst galaxies. galaxy clusters. measure EBL. unIDs. Dark Matter. neutralino lines ...
How did astronomers discover that they are extraordinarily distant and luminous? ... be very luminous, typically about 1000 times brighter than an ordinary galaxy ...
Probability for Compton or photoelectric interaction and for travelling a given ... Does the interaction point satisfy the photoelectric conditions ? ...
Prompt Gamma-Ray Imaging Using the GEANT4 Code. Libai Xu and Robin Gardner ... yields are 1.4 X 1010 (B) and 5.9 X 1010 (Gd) compared to 2.2 X 1010 for SPECT ...
HIGH ENERGY GAMMA-RAY SPECTROMETER NATALYA-2?. FOR ... Roentgen and gamma - radiation. R (Roentgen) 0,3-2. 920. 10% (662 ?eV) measured. 1 s. L (Low gamma) ...
Main observational properties. spatial distribution. temporal. spectral ... Observations: some correlations between temporal and specral properties ...
Milagro is a water Cherenkov extensive air shower (EAS) detector located near ... the iron nucleus and beyond (transuranic elements have been observed in cosmic rays) ...
Absorbed dose for mice. Comparison with MicroPET. 100 uCi 18F is injected into the mouse body ... dose to a 30-gram mouse by PGI (Neutron flux: 108 /cm2 ...
Efficiency Proper summing of scattered gamma rays, no solid angle lost to ... questions in nuclear structure, nuclear astrophysics, and weak interactions. ...
History and basic observational facts. BATSE observations, the 'Great Debate', and the determination of the distance scale ... Gpc-3 yr-1 (SNeIc ~ 4.8x104 Gpc ...
Subsequent ignition of nuclear reactions involving heavier elements ... Cassiopeia A. Optical. X-rays. Synchrotron Emission and Cosmic-Ray Acceleration ...
Angular reconstruction of shower done with top layer ... Will help determine shower core location -Better angular resolution -Improved g/h separation ...
High energy (20MeV-TeV) photon emission from Gamma-ray Bursts ... (Hurley et al. 1994) GRB 930131 ... GRB 940217 (Hurley et al. 1994) Afterglow emission ...
Need more than 5 hits to obtain at least one degree of freedom ... Weight limit: 500 kg, max. power: 3 kW, size: 0.8 m x 1.0 m x 1.85 m per standard port ...
J. Garrett Jernigan. MIT. George R. Ricker (PI) Geoffrey Crew ... Gilbert Vedrenne. Jean-Francois Olive. Michel Boer. UChicago. Donald Q. Lamb. Carlo Graziani ...
Provide adequate energy at high Lorentz factor. Collimate the emergent beam to approximately 0.1 radians ... energy and collimation to the jet - provided the necessary ...
Comparison with observations: spectra, light curves and spectral evolution ... The energy range for COMTEL was 1-30 Mev; EGRET energy range was 20 Mev to 30 Gev. ...
As with blazars and normal galaxies, some contribution from unIDs to the diffuse ... Can isotropy help? The Kavli Foundation. The National Science Foundation. GLAST! ...
The SED of the EC and SSC emission, as well as the seed photon SED, are computed. ... IC emission is dominated by SSC scattering, reaching EGRET energies. ...
In-spiral: last few minutes in the band accessible to LIGO and Virgo ... O(1050 ergs) would produce a GW signal that could be detected by the adv Virgo ...
Radio beam geometry and velocity kick distribution Arzoumanian, Chernoff & Cordes (2002) ... to 978 radio pulsars (Galactic plane) to 120 supernovae in the Gould Belt ...
What is dark energy? Dark energy was measured by WMAP, SDSS and SN Ia: ... 'standard candle' Cosmologically originated. April 15th, 2004. Cosmology Date @ LANL ...
Fully developed turbulence in a fluid flow (Frisch 1996) ... t N, which is the same as a boxcar-smoothing forward in time from point t to any point t t. ...
A Cosmology Independent Calibration of Gamma-Ray Burst Luminosity Relations and ... Isotropy: first sign of. cosmological origin. Bimodality of GRB duration ...
Deciphering the Gamma-Ray Sky: GeV Astronomy in the Era of GLAST. Vasiliki ... EGRET observed the sky for almost 10 years, and made many important discoveries. ...
Delayed X- and Gamma-Ray Line Emission. from Solar Flare Radioactivity ... The Gamma-Ray Imager ... an artist's Cosmic Vision. From J. Kn dlseder, ESLAB Symposium 2005 ...