GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY

By E. Fenimore, M. Galassi, S. Astro. 2004

178 citations recorded by the source corpus.

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Citations in the corpus

• Physical Processes Shaping Gamma-Ray Burst X-Ray Afterglow Light Curves: Theoretical Implications from the Swift X-Ray Telescope Observations (2005, background): “Derishev et al. (1999), Beloborodov (2003), and Rossi et al. (2004) suggested that a baryonic fireball contains free neutrons, the decay of whichwould leave important imprints on the light curve.”
• Multi-messenger observations of a binary neutron star merger (2017, methodology): “The first pointed X-ray observations of GW170817 were obtained by the X-Ray Telescope (Burrows et al. 2005) on the Swift satellite (Gehrels 2004) and the NUclear Spectroscopic Telescope ARray (NuSTAR; Harrison et al. 2013), beginning at T0 0.62+ days and T0 0.70+ days, respectively.”
• THE FIRST POSITIVE DETECTION OF MOLECULAR GAS IN A GRB HOST GALAXY (2009, background): “The absence of wind-blown density profiles in the circumburst environment (Chevalier 2004) is thought to be due to the pre-burst interactions of the wind with the interstellar medium (ISM; Ramirez-Ruiz et al. 2005).”
• Long-Lag, Wide-Pulse Gamma-Ray Bursts (2005, background): “However, it has also been shown that in at least two BATSE bursts, the predominant emission consists of pulses with short spectral lag accompanied by a significantly delayed episode characterized by temporally smooth, low-intensity, longlag emission (Hakkila & Giblin 2004; Hakkila et al. 2004).”
• THE SECOND FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST FOUR YEARS (2014, background): “From this an improvement in the trigger sensitivity (Band 2002; Band et al. 2004) is expected.”
• THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST SIX YEARS (2016, background): “This also improves the GBM trigger sensitivity (Band 2002; Band et al. 2004).”
• Multi-messenger Observations of a Binary Neutron Star Merger (2019, methodology): “At tc+15.3 hr, the Swift satellite (Gehrels 2004) 8 detected bright, ultraviolet emission, further constraining the effective temperature (Evans et al. 2017; Evans et al. 2017).”