The afterglow and host galaxy of GRB 090205: evidence of a Ly-α emitter at z = 4.65

P. D’Avanzo,Matteo Perri,Dino Fugazza,R. Salvaterra,Guido Chincarini,Raffaella Margutti,Xue-Feng Wu,C. C. Thöne,Alberto Fernandez-Soto,Tilan N. Ukwatta,D. N. Burrows,N. Gehrels,P. Meszaros,K. Toma,Bing Zhang,S. Covino,Sergio Campana,V. D’Elia,M. Della Valle,S. Piranomonte

The afterglow and host galaxy of GRB 090205: evidence of a Ly-α emitter at z = 4.65

2010

Context. Gamma-ray bursts (GRBs) have proven to be detectable to distances much larger than any other astrophysical object, providing the most effective way, complementing ordinary surveys of studying the high redshift universe.

Keywords:

Astronomy
Gamma-ray burst
Universe
Astrophysics
Physics
Radial velocity
Stellar population
Galaxy
Redshift
Metallicity
Star formation
Afterglow
α emitter

Correction
Source
Cite
Save
Machine Reading By IdeaReader

References

Citations