Published May 22, 2008 | Version v1
Journal article

Investigating the Lag-Luminosity Relation in the Swift Era with the Burst Alert Telescope (BAT)

  • 1. NASA Goddard Space Flight Center, Code 661, Greenbelt, MD 20771 (United States)
  • 2. George Washington University, Washington, DC 20052 (United States)
  • 3. CRESST, University of Maryland, Baltimore County, Baltimore, MD 21250 (United States)
  • 4. Space Science Division, NASA/Ames Research Center, Moffett Field, CA 94035-1000 (United States)

Description

We report on an investigation that confronts the lag-luminosity relation (LLR), i.e. a surrogate redshift parameterization based upon an empirically determined anti-correlation between the observed isotropic luminosity and the temporal lag between the arrivals of photon pulses in low (25-50 keV) and high (100-300 keV) energy bands, with observations of gamma-ray bursts (GRBs) with Swift's Burst Alert Telescope (BAT). Our initial methodology is based upon a cross-correlation function (CCF) analysis of 64 ms BAT light curves (temporal spectra), for a small subset of GRBs with observed spectroscopic redshift (zobs). Our preliminary results span 4 temporal decades and indicate an agreement with LLR, within the margins of error (excluding GRBs 980425 and 060218)

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1000
Journal Issue
1
Journal Page Range
p. 137-141
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Santa Fe conference on gamma-ray bursts 2007
Dates
5-9 Nov 2007
Place
Santa Fe, NM (United States)

Optional Information

Notes
(c) 2008 American Institute of Physics