A comparison between the soft X-ray and O III morphologies of active galactic nuclei
Improved Dynamical Constraints on the Mass of the Central Black Hole in NGC 404
Revealing the intermediate-mass black hole at the heart of the dwarf galaxy NGC 404 with sub-parsec resolution ALMA observations
Instrument
STIS, STIS/CCD, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-11-18T05:10:12Z/2012-11-18T15:32:36Z
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, Seth et al., 2013, 'Weighing the Low Mass Central Black Hole in NGC404', 1.0, European Space Agency, https://doi.org/10.5270/esa-mbnjkm3