Published January 1, 2009
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A multiwavelength study of Swift GRB 060111B constraining the origin of its prompt optical emission
Creators
- 1. ASI Sci Data Ctr, ASDC, I-00044 Frascati, Italy
- 2. Space Res Inst IKI, Moscow 117910, Russia
- 3. Univ Toulouse, LATT, CNRS, F-31400 Toulouse, France
- 4. Univ Toulouse, CESR, CNRS, F-31028 Toulouse 04, France
- 5. Observ Astron Marseille, LAM, F-13388 Marseille 13, France
- 6. Observ Haute Provence, F-04870 St Michel lObservatoire, France
- 7. Thueringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
- 8. NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
- 9. Ulugh Beg Astron Inst, Tashkent 700052, Uzbekistan
- 10. Akdeniz Univ, TUBITAK Natl Observ, TR-07058 Antalya, Turkey
- 11. SRI Crimean Astrophys Observ, UA-98409 Nauchnyi, Crimea, Ukraine
- 12. Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Crimean Lab, UA-98409 Nauchnyi, Crimea, Ukraine
- 13. Observ Paris, IMCCE, F-75014 Paris, France
Description
Context. The detection of bright optical emission measured with good temporal resolution during the prompt phase of GRB 060111B makes this GRB a rare event that is especially useful for constraining theories of the prompt emission.
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