activity
19982002
most citedTemporal properties of gamma-ray bursts as signatures of jets from the central engine

83 citations · 179 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2002★ 23 cited

Cumulative light curves of gamma-ray bursts and relaxation systems

S. McBreen, B. McBreen, L. Hanlon +1

The cumulative light curves of a large sample of gamma-ray bursts (GRBs) were obtained by summing the BATSE counts. The smoothed profiles are much simpler than the complex and erra…

astro-ph2002★ 7 cited

Temporal properties of short and long gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis was performed on a sample of 100 bright short GRBs with T90 < 2s from the BATSE Current Catalog along with a similar analysis on 319 long bright GRBs with T90 >…

astro-ph2002★ 9 cited

Timing diagrams and correlations in gamma-ray bursts signal jets from accretion into black holes

S. McBreen, B. McBreen, F. Quilligan +1

The temporal properties of a sample of 498 bright gamma-ray bursts (GRBs) with durations between 0.05 s and 674 s were analysed. The large range in duration (T90) is accompanied by…

astro-ph2001★ 48 cited

Temporal properties of the short gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis has been performed on a sample of 100 bright gamma-ray bursts (GRBs) with T90<2s from the BATSE current catalog. The GRBs were denoised using a median filter an…

astro-ph2001★ 83 cited

Temporal properties of gamma-ray bursts as signatures of jets from the central engine

F. Quilligan, B. McBreen, L. Hanlon +3

A comprehensive temporal analysis has been performed on the 319 brightest GRBs with T90>2s from the BATSE current catalog. The rise times, fall times, full-widths at half maximum (…

astro-ph2000

ASCA and other contemporaneous observations of the blazar B2 1308+326

D. Watson, N. Smith, L. Hanlon +8

The high redshift (z=0.997) blazar B2 1308+326 was observed contemporaneously at x-ray, optical and radio wavelengths in June 1996. The x-ray observations were performed with ASCA.…