X-ray afterglow light curves: Toward a standard candle?

AIP Conference Proceedings

Volumn 1000, Issue , 2008, Pages 72-75

  Gendre, B ^a   Galli, A ^a   Boer M ^b  

^a INAF IASF ROMA   (Italy)

^b CNRS   (France)

Author keywords

bursts luminosity function galaxy.; gamma rays

Indexed keywords

EID: 69549088883     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.2943553     Document Type: Conference Paper

References (10)

1. J. Hjorth, et al., Nature 423, 847-850 (2003).
2. M. Boer and B. Gendre, A&A 361, L21-L24 (2000).
3. B. Gendre and M. BOST:, A&A 430, 465-470 (2005).
4. M. Nardini, G. Ghisellini, G. Ghirlanda, F. Tavecchio, C. Firmani, andD. Lazzad, A&A 451, 821-833 (2006).
5. E. Liang, and B. Zhang,-/J J 638, L67-L70 (2006).
6. B. Gendre, A. Galli, ndM. Boer,-/J J submited.
7. J. A. Nousek, et al., ApJ 642, 389-400 (2006).
8. R. Willingale, P. T. O'Brien, J. P. Osborne, O. Godet, K. L. Page, M. R. Goad, D. N. Burrows, B.
9. Zhang, E. Rol, N. Gehrels, and G. Chincarini, ApJ 662, 1093-1110 (2007).
10. A. Panaitescu, andP Kumar, ApJ543, 66-76 (2000).