A remarkable oxygen-rich asymptotic giant branch variable in the Sagittarius Dwarf Irregular Galaxy
Chemistry and Kinematics of the Late-forming Dwarf Irregular Galaxies Leo A, Aquarius, and Sagittarius DIG
Envelope overshooting in low-metallicity intermediate- and high-mass stars: a test with the Sagittarius dwarf irregular galaxy
HST/ACS observations of the old and metal-poor Sagittarius dwarf irregular galaxy
Massive stars in the Sagittarius Dwarf Irregular Galaxy
Near-infrared photometry of carbon stars in the Sagittarius dwarf irregular galaxy and DDO 210
Proper Motions and Orbits of Distant Local Group Dwarf Galaxies from a Combination of Gaia and Hubble Data
Solo dwarfs I: survey introduction and first results for the Sagittarius dwarf irregular galaxy
The extended structure of the dwarf irregular galaxy Sagittarius
The H i hole and AGB stellar population of the Sagittarius dwarf irregular galaxy . HST proper-motion decontamination
The impact of satellite trails on Hubble Space Telescope observations
The star formation history of the BCD I Zw 18
Instrument
ACS, ACS/WFC
Temporal Coverage
2003-08-18T07:50:33Z/2003-08-18T11:46:15Z
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, Momany comma Yazan, 2004, 'SagDIG: a benchmark for understanding star formation in extreme low-metallicity galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-bjb8lbd