A Low Metallicity Massive Contact Binary Star System Candidate in WLM Identified by Hubble and James Webb Space Telescope Imaging
Far-ultraviolet Spectra of Main-sequence O Stars at Extremely Low Metallicity
The impact of satellite trails on Hubble Space Telescope observations
The JWST Resolved Stellar Populations Early Release Science Program. VIII. The Spatially Resolved Star Formation History of WLM
The Local Ultraviolet to Infrared Treasury. II. Refining Star Formation Histories of 10 Metal-poor Dwarf Galaxies with Simultaneous UV-optical Two-CMD Fitting
The Local Ultraviolet to Infrared Treasury. I. Survey Overview of the Broadband Imaging
Instrument
ACS/WFC, WFC3/UVIS
Temporal Coverage
2018-01-29T01:50:10Z/2020-01-10T08:30:02Z
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, Gilbert et al., 2020, 'Securing HST's UV Legacy in the Local Volume: Probing Star Formation and the Interstellar Medium in Low Mass Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-u207nra
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.