A New Age and Distance for I Zw 18, the Most Metal-Poor Galaxy in the Nearby Universe
Chemical and stellar properties of star-forming dwarf galaxies
Extremely Metal-Poor Star-Forming Dwarf Galaxies
I Zw 18 as morphological paradigm for rapidly assembling high-z galaxies
IZw18, or The Picture of Dorian Gray: The More You Watch it, The Older it Gets
I Zw 18 Revisited with HST ACS and Cepheids: New Distance and Age
Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
Multi-Epoch Hubble Space Telescope Observations of IZw18: Characterization of Variable Stars at Ultra-Low Metallicities
Spatial Distribution and Evolution of the Stellar Populations and Candidate Star Clusters in the Blue Compact Dwarf I Zwicky 18
The Blue Compact Dwarf Galaxy IZw18
The impact of satellite trails on Hubble Space Telescope observations
The size-density relation of extragalactic H II regions
The star formation history of the BCD I Zw 18
The Star Formation History of the Very Metal-poor Blue Compact Dwarf I Zw 18 from HST/ACS Data
Variable Stars in Nearby Galaxies with HST
Variable Stars in (Not Only) Dwarf Galaxies: Key Tools to Constrain Distances and Stellar Content
Very metal poor classical cepheids: the distance of IZw18
Instrument
ACS, ACS/WFC
Temporal Coverage
2005-10-02T11:33:45Z/2006-01-06T13:57:13Z
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, Aloisi comma Alessandra, 2007, 'The Rosetta Stone without a Distance: Hunting for Cepheids in the "Primordial" Galaxy I Zw 18', 1.0, European Space Agency, https://doi.org/10.5270/esa-753tbds