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
Hubble Asteroid Hunter. I. Identifying asteroid trails in Hubble Space Telescope images
Hubble Asteroid Hunter. III. Physical properties of newly found asteroids
Investigation of dust attenuation and star formation activity in galaxies hosting GRBs
The case for a high-redshift origin of GRB 100205A
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
The Optically Unbiased GRB Host (TOUGH) Survey. V. VLT/X-shooter Emission-line Redshifts for Swift GRBs at z ~ 2
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-09-15T00:37:13Z/2010-09-15T00:51:41Z
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 ANDREW J., 2011, 'Identifying the host galaxies for optically dark gamma-ray bursts', 1.0, European Space Agency, https://doi.org/10.5270/esa-fhvtm6b