Title: Prompt optical observations of GRB 080330 and GRB 080413A
1Prompt optical observations of GRB 080330 and GRB
080413A
2Background Motivation
- Growing number of early optical afterglow
observations - Collective study of temporal behavior
- Panaitescu Vestrand 2008 peak time and peak
flux correlation - Growing number of prompt optical observations
- Some show complicated behavior, GRB 08330 and GRB
080413a - Multiple components from both internal and
external shock? - Start from the better-understood afterglow part
-
32008 Mar. 30, 034139.2 22.4 s after the burst
(7.2 s after the GCN notice time) Schaefer
Guver, GCN 7538
2008 Apr. 13, 025439.7 20.4 s after the burst
(6.7 s after the GCN notice time) Rykoff
Rujopakarn, GCN 7593
42008 Mar. 30, 034139.2 22.4 s after the burst
(7.2 s after the GCN notice time) Schaefer
Guver, GCN 7538
2008 Apr. 13, 025439.7 20.4 s after the burst
(6.7 s after the GCN notice time) Rykoff
Rujopakarn, GCN 7593
52008 Mar. 30, 034139.2 22.4 s after the burst
(7.2 s after the GCN notice time) Schaefer
Guver, GCN 7538
2008 Apr. 13, 025439.7 20.4 s after the burst
(6.7 s after the GCN notice time) Rykoff
Rujopakarn, GCN 7593
6GRB 080330
7GRB 080330
8GRB 080413a
9GRB 080413a
10Slowly decaying afterglow
- Structured flow viewed off-axis?
- Drowned by prompt emission in X-ray?
Panaitescu Vestrand 2008
11Rising of afterglow
- E?,iso 5.0 x 1051 erg
- ? 2.5 /-0.5
- tpeak 150 s
- G0 200
- (Sari Piran 1999, Molinari et al. 2007)
- Can be classified as XRF
- (Sakamoto et al. 2008, Mao et al. 2008)
- E?,iso 1.7 x 1053 erg
- ? 1.5 /-0.1
- tpeak 30 s
- G0 600
12Prompt optical flash
13Other ROTSE-III events
- E?,iso 3.1 x 1051 erg
- ? 1.9 /-0.1
- tpeak 200 s
- G0 150
- E?,iso 4.2 x 1053 erg
- ? 1.1 /-0.0
- tpeak 40 s
- G0 600
Rykoff 2008 in preparation
14Summary
- Prompt optical component
- Need better sampling
- Complicated by early afterglow
- Better understanding of the afterglow phase will
help - Low Lorentz factor events
- Delayed afterglow peak
- Easier to observe the peak and shape of the early
lightcurve
15Next with ROTSE-III
- More interesting events from Swift (sub-threshold
triggers) - GLAST launched
- ROTSE supernova verification project
- Follow-up of IceCube neutrino doublet triggers
16Thank you!
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