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Prompt optical observations of GRB 080330 and GRB 080413A

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Title: Prompt optical observations of GRB 080330 and GRB 080413A


1
Prompt optical observations of GRB 080330 and GRB
080413A
2
Background 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

3
2008 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
4
2008 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
5
2008 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
6
GRB 080330
7
GRB 080330
8
GRB 080413a
9
GRB 080413a
10
Slowly decaying afterglow
  • Structured flow viewed off-axis?
  • Drowned by prompt emission in X-ray?

Panaitescu Vestrand 2008
11
Rising 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

12
Prompt optical flash
13
Other 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
14
Summary
  • 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

15
Next with ROTSE-III
  • More interesting events from Swift (sub-threshold
    triggers)
  • GLAST launched
  • ROTSE supernova verification project
  • Follow-up of IceCube neutrino doublet triggers

16
Thank you!
17
1.9
2.5
2.1
1.5
2.0
2.1
3.1
1.5
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