Dependence of Galaxy Structure on Rest-Frame Wavelength and Galaxy Type
Galaxy Structure in the Ultraviolet: The Dependence of Morphological Parameters on Rest-frame Wavelength
Star Clusters in the Nearby Late-Type Galaxy NGC 1311
The connection between radio loudness and central surface brightness profiles in optically selected low-luminosity active galaxies
The host galaxy/AGN connection in nearby early-type galaxies. A new view of the origin of the radio-quiet/radio-loud dichotomy?
The Young Stellar Population of the Nearby Late-type Galaxy NGC 1311
UBVR and Hubble Space Telescope Mid-Ultraviolet and Near-Infrared Surface Photometry and Radial Color Gradients of Late-Type, Irregular, and Peculiar Galaxies
Instrument
NICMOS, NICMOS/NIC3
Temporal Coverage
2003-07-13T22:46:07Z/2004-11-17T04:03:47Z
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, Windhorst et al., 2004, 'NIC3 SNAPs of nearby galaxies imaged in the mid-UV: the remarkable cool stellar population in late-type galaxies.', 1.0, European Space Agency, https://doi.org/10.5270/esa-qmvhb8j