GRB spectral lags

We present a new technique to calculate the spectral lags of {gamma}-ray bursts (GRBs). Unlike previous processing methods, we first smooth the light curves of {gamma}-ray bursts in high- and low-energy bands using the "Loess" filter, then we directly define the spectral lags as such to maximize the cross-correlation function (CCF) between two smoothed light curves.

Cone search capability for table J/PASP/124/297/Glags (Spectral lags of GRBs)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/PASP/124/297
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/124/297
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/124/297
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/PASP/124/297
Provenance
Creator Li Z.; Chen L.; Wang D.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics