Feedback in nearby dwarf starburst galaxies and giant extragalactic H II regions
How extreme are the Wolf-Rayet clusters in NGC3125?*
HST/ACS Lyman a imaging of the nearby starburst ESO 338-IG04
Kinematics of Interstellar Gas in Nearby UV-selected Galaxies Measured with HST STIS Spectroscopy
Multiwavelength analysis of the Lyman-a emitting galaxy Haro 2: relation between the diffuse Lyman-a and soft X-ray emissions
NGC 3125-1: The Most Extreme Wolf-Rayet Star Cluster Known in the Local Universe
On the reliability of CIVl1549 as an abundance indicator for high-redshift star-forming galaxies
Supernova-driven outflows in NGC 7552: a comparison of H a and UV tracers
Testing He II Emission from Wolf-Rayet Stars as a Dust Attenuation Measure in Eight Nearby Star-forming Galaxies
The Stellar Content of Henize 2-10 from Space Telescope Imaging Spectrograph Ultraviolet Spectroscopy
The Stellar Content of Nearby Star-forming Galaxies. III. Unravelling the Nature of the Diffuse Ultraviolet Light
Using Lyman-a to detect galaxies that leak Lyman continuum
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2001-08-17T08:06:34Z/2003-03-08T20:36:21Z
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, Leitherer et al., 2003, 'An Ultraviolet Spectroscopic Survey of Star-Forming Galaxies in the Local Universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-m3dcje8