An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-redshift AGB Analogs
An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). V. The Period-Luminosity Relation for Dusty Metal-poor AGB Stars
Discovery of SiC and Iron Dust around AGB Stars in the Very Metal-poor Sextans a Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift
Far-ultraviolet Spectra of Main-sequence O Stars at Extremely Low Metallicity
Ongoing star formation at the outskirts of Sextans A: spectroscopic detection of early O-type stars
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-10-02T05:24:37Z/2016-08-07T15:34:14Z
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, Boyer et al., 2017, 'Assessing the Impact of Metallicity on Stellar Dust Production', 1.0, European Space Agency, https://doi.org/10.5270/esa-qty9r0f
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.