An Ultraviolet Spectroscopic Atlas of Local Starbursts and Star-forming Galaxies: The Legacy of FOS and GHRS
Carbon in Spiral Galaxies from Hubble Space Telescope Spectroscopy
Near-ultraviolet Spectroscopy of Star-forming Galaxies from eBOSS: Signatures of Ubiquitous Galactic-scale Outflows
Physical Structure and Nature of Supernova Remnants in M101
The impact of resolution on observed Hii region properties from WFPC2 observations of M 101
The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra
Instrument
FOS/RD, WFPC2, WFPC2/PC
Temporal Coverage
1995-11-13T13:27:20Z/1997-01-29T08:36:22Z
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, Garnett et al., 1998, 'THE EVOLUTION OF CARBON ABUNDANCES IN THE ISM OF SPIRAL GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-z00kjsb