Almost gone: SN 2008S and NGC 300 2008OT-1 are fainter than their progenitors
A Robust Tip of the Red Giant Branch Distance to the Fireworks Galaxy (NGC 6946)
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
Morphological and kinematical analysis of the double-barred galaxy NGC 3504 using ALMA CO (2-1) data
SN 2002bu--Another SN 2008S-like Transient
Stellar content and distances to the isolated spiral galaxies NGC 6503 and NGC 6946
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
The impact of satellite trails on Hubble Space Telescope observations
The Intermediate Luminosity Optical Transient SN 2010da: The Progenitor, Eruption, and Aftermath of a Peculiar Supergiant High-mass X-Ray Binary
The Masses of Supernova Remnant Progenitors in NGC 6946
The MBHBM Project. I. Measurement of the Central Black Hole Mass in Spiral Galaxy NGC 3504 Using Molecular Gas Kinematics
Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2012-02-15T00:38:35Z/2012-08-30T03:08:45Z
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, Kochanek comma Chris S., 2013, 'Understanding A New Class of Mid?IR Transients', 1.0, European Space Agency, https://doi.org/10.5270/esa-uq8f6ub