Reversal of Fortune: Increased Star Formation Efficiencies in the Early Histories of Dwarf Galaxies?
The ACS LCID Project. IX. Imprints of the Early Universe in the Radial Variation of the Star Formation History of Dwarf Galaxies
The ACS LCID Project: On the Origin of Dwarf Galaxy Types--A Manifestation of the Halo Assembly Bias?
The Aptly Named Phoenix Dwarf Galaxy
The extended structure of the Phoenix dwarf galaxy
The RR Lyrae Variable Population in the Phoenix Dwarf Galaxy
The Star Formation Histories of Local Group Dwarf Galaxies. I. Hubble Space Telescope/Wide Field Planetary Camera 2 Observations
The Star Formation Histories of Local Group Dwarf Galaxies. II. Searching For Signatures of Reionization
The star formation history from resolved stellar populations. State of the art and future perspectives
The Very Faint End of the UV Luminosity Function over Cosmic Time: Constraints from the Local Group Fossil Record
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-01-10T11:25:13Z/2001-01-17T12:27:13Z
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, Aparicio comma Antonio, 2002, 'Phoenix: ``halo/disk'' structures in dwarf galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-hcx8woj