Dissecting the Power Sources of Low-Luminosity Emission-Line Galaxy Nuclei via Comparison of HST-STIS and Ground-Based Spectra
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
NGC 4435: a bulge-dominated galaxy with an unforeseen low-mass central black hole
Stringent limits on the masses of the supermassive black holes in seven nearby galaxies
Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
Upper Limits on the Mass of Supermassive Black Holes from Archival Data of the Space Telescope Imaging Spectrograph
Upper limits on the mass of supermassive black holes from HST/STIS archival data.
Instrument
STIS, STIS/CCD
Temporal Coverage
2002-01-28T07:50:09Z/2003-03-09T14:20:55Z
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, Bertola comma Francesco, 2006, 'Accurate determination of the BH mass in early-type disk galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-fabht8o