A Photometric Investigation of the GRB 970228 Afterglow and the Associated Nebulosity
HST Data suggest proper motion for the optical counterpart of GRB 970228.
Observations and Theoretical Implications of GRB 970228
Observations of GRB 970228 and GRB 970508 and the Neutron Star Merger Model
The Fading Optical Counterpart of GRB 970228, 6 Months and 1 Year Later
The optical counterparts of g-ray bursts
The optical counterpart to g-ray burst GRB970228 observed using the Hubble Space Telescope
UV star-formation rates of GRB host galaxies
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-03-26T07:51:14Z/1997-04-07T07:41:34Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Sahu et al., 1997, 'FOLLOW-UP OBSERVATIONS OF A POSSIBLE OPTICAL COUNTERPART OF GRB 970228', 1.0, European Space Agency, https://doi.org/10.5270/esa-t0d8ivh