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
Understanding the Nuclear Gas Dispersion in Early-Type Galaxies in the Context of Black Hole Demographics
Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
Instrument
STIS, STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
2001-05-05T11:32:14Z/2001-05-27T05:04:14Z
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, VERDOES KLEIJN GIJS, 2002, 'Kinematics of emission-line gas disks in radio-quiet galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-6i6p9i7