GRB 100816A: Observations and Analysis
Implications for the origin of GRB 070201 from LIGO observations
... The remainder of the paper is organized as follows. In x 2 we discuss the LIGO detectors and the data taken around the time of GRB 070201. In x 3 we report on the inspiral gravitational-wave search, briefly ...
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Implications for the origin of GRB 051103 from LIGO observations
... with GRB 051103, and the resulting implications for the origin of this ...independent analysis packages, designed for different purposes, were ...an analysis designed to search for GW bursts from ...
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Infrared/optical-X-ray simultaneous observations of X-ray flares in GRB 071112C and GRB 080506
... our analysis. The host galaxy of GRB 080506 was not ...of GRB 071112C can be described with a broken power-law form; f ∝ t α 1 (t ≤ t break ) and, f ∝ t α 2 (t > t break ) with a weak X-ray flare ...
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Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A
... Acknowledgments: The Fermi LAT Collaboration acknowledges support from a number of agencies and institutes for both development and the operation of the LAT as well as scientific data analysis. These include NASA ...
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Broadband Observations of the Afterglow of GRB : Observing the Effect of Inverse Compton Scattering
... X-ray observations, as well as extensive multi-frequency optical and radio ...an analysis of Chandra X-ray Observatory observations of this event, along with Hubble Space Telescope and radio ...IR ...
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GRB 130427A Afterglow: A Test for GRB Models
... 2. Observations and Results Our dataset is constituted by X-ray observations carried out by Swift X-ray Telescope (XRT; Burrows et ...observed GRB 130427A until October 2013. XMM-Newton carried out ...
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GRB 071003: Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo
... long-duration GRB 071003 is among the brightest yet to be detected from any GRB, with R 12 mag in KAIT observations starting 42 s after the GRB trigger, including filtered detections during ...
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A Reverse Shock in GRB 181201A
... the observations as well as the RS model (Figure 13 ...detailed analysis requires a complete parameter search over f NT and h e that also includes the FS ...
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The host of GRB 060206 : kinematics of a distant galaxy
... of GRB 060206, focusing on the metallicity that we compared to a large sample of QSO ab- sorber metallicities and the sample of known GRB afterglow ...detailed analysis of the properties of the host ...
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A multiband study of the optically dark GRB 051028
... of GRB 051028 with the Lulin observatory ...for GRB Early Timing (WIDGET) robotic telescope ...of GRB 051028 resembles optically bright afterglows (e.g., GRB 041006, GRB 050319, ...
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An unusual transient following the short GRB 071227
... spectroscopic observations and analysis thereof of the ...South observations and processing as well as the available data from the Neil Gehrels Swift Observatory, hereafter Swift, satellite and the ...
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Implications for the origin of GRB 070201 from LIGO observations
... 3.2. Background and Results Gravitational-wave detectors are susceptible to many sources of environmental and intrinsic noise. These sources often result in non-Gaussian and non-stationary noise back- grounds. In the ...
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Stirring the Embers: High-Sensitivity VLBI Observations of GRB 030329
... The nearby (0.8 ) source J1048+2115 was used as the phase- reference calibrator and was observed regularly in a cycle of 2 minutes on the target and 1 minute on the calibrator. Since J1048+2115 is not tied to the ...
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Early time optical polarization of GRB Afterglows: GRB 060418 and GRB 090102
... Figure 2: Monte Carlo simulation demonstrating the significance of the GRB 090102 result. See [10] for details. as P = 10.2 ± 1.3%[10] (Figure 2). In interpreting this measurement first we consider whether such a ...
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The field galaxies clustering in GRB lines of sight based on observations with BTA and other telescopes
... Spitzer GRB 021004 deep field and on the clustering of galaxies around the GRB sight-line and on the excess density of field galaxies near z ~ ...the GRB 021004 ...the GRB were tested. The ...
GRB Rules & Regulations
... A schedule of the number and postings of first aid personnel shall be submitted in writing to the Convention Services Manager at least thirty (30) calendar days prior to the first day o[r] ...
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A Reverse Shock in GRB 130427A
... of GRB 130427A spanning radio to ...millimeter observations present a spectrum and temporal evolution that cannot be explained by emission from the forward shock ...
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Early GRB Afterglows Revisited
... EARLY GRB AFTERGLOWS REVISITED ...the GRB prompt radiation ahead of the blast ...the GRB ejecta moves freely in a cavity behind its own radiation ...prompt GRB duration and then the emission ...
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A REVERSE SHOCK in GRB 160509A
... tion, NSF grant AST-1211916, and NASA/Swift grant NNX12AD73G. This work was supported in part by the NSF under grant No. PHYS-1066293; A.V.F. thanks the Aspen Center for Physics for its hospitality during the black holes ...
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The Late-time Afterglow Evolution of Long Gamma-Ray Bursts GRB 160625B and GRB 160509A
... of GRB 160625B (and GRB 160509A; see below) is incompatible with the higher frequencies, the source of the radio emission that we do see may not be the same as that of the optical and X-ray synchrotron ...
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