A progenitor candidate for the type II-P supernova SN 2018aoq in NGC 4151
The Black Hole Mass of NGC 4151 from Stellar Dynamical Modeling
The Cepheid Distance to the Narrow-line Seyfert 1 Galaxy NGC 4051
The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
The Dusty Heart of NGC 4151 Revealed by l ~ 1-40 mm Reverberation Mapping and Variability: A Challenge to Current Clumpy Torus Models
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2015-12-07T01:29:57Z/2016-02-18T22:48:06Z
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, Peterson comma Bradley M, 2016, 'A Cepheid-Based Distance to the Benchmark AGN NGC 4151', 1.0, European Space Agency, https://doi.org/10.5270/esa-ln5uo9v