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Table B.1

Ep evolutionary trends. Column (1) lists the GRB names.

GRB name N ρph(90%) ρen(90%) ρt(90%) trend(90%) ρph(95%) ρen(95%) ρt(95%) trend(95%) ρph(99%) ρen(99%) ρt(99%) trend(99%) trend(by eyes)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)

080817161 15 undeter. undeter. h.t.s. h.t.s.+in.track.
080825593 12 undeter. h.t.s. h.t.s. h.t.s.
080916009 21 undeter. undeter. undeter. undeter.
081009140 0
081124060 0
081125496 4

Notes. Column (2) lists the numbers of spectra with Ep. Columns (3), (7), and (11) list the Spearman’s Rank Correlation Coefficients between Ep and the photon flux and the 90%, 95%, and 99% confidence intervals, respectively. Columns (4), (8), and (12) list the Spearman’s Rank Correlation Coefficients between Ep and the energy flux and the 90%, 95%, and 99% confidence intervals, respectively. Columns (5), (9), and (13) list the Spearman’s Rank Correlation Coefficients between Ep and the time and the 90%, 95%, and 99% confidence intervals, respectively. Columns (6), (10), and (14) list the trends as determined by the computer for the 90%, 95%, and 99% confidence intervals, respectively. Column (15) lists the trends as determined by human eyes. The full Table is available at the CDS.

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