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Cited by 947 publications
(628 citation statements)
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References 14 publications
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“…In many such cases afterglow emission was detected, the host galaxies were discovered, and the associated measurement of spectral line redshifts confirmed the cosmological distances to the burst sources (e.g., Costa et al 1997;Piro et al 1998;van Paradijs et al 1997;Bremer et al 1998;Frail et al 1997). Observational evidence also indicates that the bursts originate from star formation regions, suggesting a possible link to massive star explosions.…”
Section: Introductionmentioning
confidence: 71%
“…In many such cases afterglow emission was detected, the host galaxies were discovered, and the associated measurement of spectral line redshifts confirmed the cosmological distances to the burst sources (e.g., Costa et al 1997;Piro et al 1998;van Paradijs et al 1997;Bremer et al 1998;Frail et al 1997). Observational evidence also indicates that the bursts originate from star formation regions, suggesting a possible link to massive star explosions.…”
Section: Introductionmentioning
confidence: 71%
“…Among the most important results obtained with the WFCs is the discovery of the X-ray afterglow phenomenon of Gamma Ray Bursts in 1997 (Costa et al 1997). Moreover, the 12 monitoring campaigns of the Galactic Bulge allowed the spectral and timing monitoring of known persistent and transient X-ray sources and the discovery of many new galactic X-ray transients and phenomena (see for example Ubertini et al 1999;Cornelisse et al 2000;in 't Zand 2001in 't Zand , 2004aCornelisse et al 2003).…”
Section: Introductionmentioning
confidence: 99%
“…They were discovered in 1967 (see Bonnell & Klebesadel 1996 for a discussion of the first GRB detections), but due to the lack of rapid and precise localisations, their emission at other wavelengths was not detected until 1997 (van Paradijs et al 1997;Frail et al 1997;Costa et al 1997). Thus, for 30 years they were not localised at longer wavelengths (X-ray, UV, optical, IR, radio) and their distances could not be measured.…”
Section: Introductionmentioning
confidence: 99%