Free Access
MJD | ObsID | Times | Active | ![]() |
covered wrt | PCUs | (![]() |
||
burst start | ||||
time (s)b | ||||
50 971.23019 | 30054-04-02-01 | -2600/+1200 | 0, 1, 2, 3, 4 | 0.0 |
50 971.70032 | 30054-04-02-000 | -2700/+900 | 0, 1, 2, 3, 4 | 0.0 |
50 988.82503 | 30060-03-01-01 | -1700/+1800 | 0, 1, 2, 3 | 0.0 |
51 725.87648 | 50035-01-02-00 | -3000/+200 | 0, 2, 3, 4 | 0.5 |
51 726.71988c,p,t | 50035-01-02-02 | -1200/+2100 | 0, 1, 2, 3 | 0.5 |
51 728.77338c,p,t | 50035-01-02-04 | -4000/+2600 | 0, 1, 2, 3 | 0.5 |
51 814.34546c,p,t | 50035-01-03-10 | -2200/+1500 | 0, 2 | 0.5 |
52 484.41775c,p,t | 70044-01-01-000 | -4000/+2200 | 0, 2, 3 | 0.0 |
52 484.56684c | 70044-01-01-00 | -2400/+700 | 0, 2, 3 | 0.0 |
52 485.00672c,p,t | 70044-01-01-02 | -4000/+2600 | 0, 2, 3 | 0.0 |
52 537.22347 | 70025-01-01-00 | -4000/+2400 | 0, 1, 2, 3 | 0.0 |
52 738.47686c,p,t | 80048-01-01-04 | -4000/+3200 | 0, 2, 3 | 0.0 |
52 738.74636c,p,t | 80048-01-01-07 | -4000/+2700 | 0, 1, 2, 3 | 0.0 |
52 820.56256c,p,t | 80049-01-01-00 | -1100/+2000 | 0, 2, 3, 4 | 0.0 |
52 893.05439 | 80105-11-01-00 | -4000/+3000 | 0, 2, 3 | 0.0 |
53 205.19659c,p,t | 70044-01-02-00 | -1900/+1500 | 0, 2, 3 | 0.0 |
53 207.07579 | 90043-01-01-01 | -4000/+3600 | 0, 2 | 2.5 |
53 207.21911c | 90043-01-01-01 | -4000/+1400 | 0, 2, 3 | 2.5 |
53 206.49150c,p,t | 90043-01-01-020 | -4000/+2800 | 0, 2, 3 | 2.5 |
53 206.63615c,p,t | 90043-01-01-02 | -4000/+1900 | 0, 2, 3 | 2.5 |
53 956.08413p,t | 92031-01-01-000 | -4000/+2200 | 0, 2, 4 | 13.8 |
53 956.22695p,t | 92031-01-01-000 | -2100/+1100 | 0, 1, 2 | 13.8 |
53 957.06785p,t | 92031-01-01-010 | -4000/+2000 | 0, 2, 3 | 13.8 |
53 957.20458p,t | 92031-01-01-010 | -1800/+1600 | 0, 2, 3 | 13.8 |
53 959.15478p,t | 92031-01-02-000 | -4000/+2900 | 1, 2 | 13.8 |
54 167.72354c,p,t | 91017-01-01-000 | -1900/+1100 | 1, 2 | 0.0 |
54 168.31443c,p,t | 91017-01-02-03 | -2000/+1600 | 2 | 0.0 |
54 168.75518c,p,t | 91017-01-02-010 | -4000/+2500 | 0, 2, 3 | 0.0 |
54 168.90229c,p,t | 91017-01-02-010 | -1900/+1600 | 0, 2 | 0.0 |
a Off-axis angle; b these values are rounded off to an integer times 100 s and may include gaps. c The spectra for these ObsIDs were used to generate average time-resolved spectra (cf., Fig. 4); p data were used to calculate average pre-burst power density spectrum (Fig. 6); t data were used to calculate average tail power density spectrum. |
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