Distances to dwarf galaxies of the Canes Venatici I cloud
Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks
Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
Globular cluster systems in spiral galaxies
M 101 group galaxies
Nearby Spiral Galaxy Globular Cluster Systems. II. Globular Cluster Metallicities in NGC 300
The Distance to M101 Hosting Type Ia Supernova 2011fe Based on the Tip of the Red Giant Branch
The Effect of Metallicity on Cepheid-based Distances
The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks
The opacity of spiral galaxy disks. V. Dust opacity, HI distributions and sub-mm emission
The opacity of spiral galaxy disks. VI. Extinction, stellar light and color
The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
The opacity of spiral galaxy disks. VII. The accuracy of galaxy counts as an extinction probe
The Red Supergiant Progenitor of Type II Supernova 2024ggi
The Stellar Content and Star Formation History of the Late-Type Spiral Galaxy NGC 300 from Hubble Space Telescope Observations
The structure and environment of young stellar clusters in spiral galaxies
Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
Uncloaking globular clusters in the inner galaxy
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2000-10-22T00:20:13Z/2001-12-17T16:34:35Z
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, Kennicutt comma Robert C., 2002, 'Calibrating the Metallicity Dependence of the Cepheid PL Relation', 1.0, European Space Agency, https://doi.org/10.5270/esa-8zc8vus