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Its Game Rating Board (GRB), with the legal power to ban any game, now risks obstructing the development of an entire industry, one of the country's most vibrant.Graphic games such as Grand Theft Auto III are already off-limits to Korean gamers.
This supernovae may thus be a GRB, with its jets pointed away from Earth when it exploded.
Working via the internet, Reichart's team checked the site of the GRB with the 4.1-meter Southern Observatory for Astrophysical Research telescope atop Cerro Pachon, Chile.
Related sites HETE-2 mission Swift mission, with background on gamma ray bursts RAPTOR home page KAIT home page Abstract of KAIT paper on 11 December GRB, with link to full text.
We have analysed the 4B revised BATSE catalog: temporal profiles of GRB with t90 < 3 s (287 short and 100 intermediate) were studied on TTE data, a sample of 278 intermediate GRB with t90 ⩾ 3 s were studied on DISCSC data.
Because typically an X-ray observatory can only observe a GRB several kiloseconds after the detection of a GRB with a typical observation time of kiloseconds, we can only study the dust in the nearby several kilo parsecs from the Earth in the direction of the GRB.
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In particular, we discuss the constraints in several dark energy models by combining GRBs with supernovae Ia (SNe Ia).
We analyze several recently detected gamma-ray bursts (GRBs) with late X-ray flares in the context of late internal shock and late external shock models.
The distribution of low energy index α associated with the CPL term shows clear discordance with synchrotron models for 31.4% of the analysed GRBs with values exceeding that for the line of death, α = −2/3.
We analysed the rest frame de-absorbed and K-corrected optical and X-ray light curves of a sample of 33 GRBs with known redshift and optical extinction at the host frame.
Comparing this burst with other GRBs with evidence of optical peaks, we find that the optical peak epoch (tp) is anti-correlated with the high energy burst energetic assuming an isotropic energy release (Eiso) in agreement with Liang et al. (2009), and that the steeper is the post-peak afterglow decay, the less is the agreement with the correlation.
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