A Population of Massive, Luminous Galaxies Hosting Heavily Dust-obscured Gamma-Ray Bursts: Implications for the Use of GRBs as Tracers of Cosmic Star Formation
Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies
Host Galaxy Properties and Black Hole Mass of Swift J164449.3+573451 from Multi-wavelength Long-term Monitoring and HST Data
Illuminating the Darkest Gamma-Ray Bursts with Radio Observations
Late Time Multi-wavelength Observations of Swift J1644+5734: A Luminous Optical/IR Bump and Quiescent X-Ray Emission
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The Offset and Host Light Distributions of Long Gamma-Ray Bursts: A New View From HST Observations of Swift Bursts
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-08-04T06:10:17Z/2011-12-02T17:13:24Z
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, Levan et al., 2012, 'The differing environments of dark gamma-ray bursts', 1.0, European Space Agency, https://doi.org/10.5270/esa-hj0rgum