A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive
A Chandra View of NGC 3621: A Bulgeless Galaxy Hosting an AGN in Its Early Phase?
A Study of Optical Observing Techniques for Extra-Galactic Supernova Remnants: Case of NGC300
AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary
Detailed photometric analysis of young star groups in the galaxy NGC 300
Discovery of a deep Seyfert-2 galaxy at z = 0.222 behind NGC 300
Do Nuclear Star Clusters and Supermassive Black Holes Follow the Same Host-Galaxy Correlations?
Dynamical Constraints on the Masses of the Nuclear Star Cluster and Black Hole in the Late-Type Spiral Galaxy NGC 3621
Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
Globular cluster systems in spiral galaxies
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Nearby Spiral Galaxy Globular Cluster Systems. II. Globular Cluster Metallicities in NGC 300
Physical Structure and Nature of Supernova Remnants in M101
Quantitative Spectroscopy of 24 A Supergiants in the Sculptor Galaxy NGC 300: Flux-weighted Gravity-Luminosity Relationship, Metallicity, and Metallicity Gradient
Star formation histories from resolved stellar populations in nearby galaxies
Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621
The 2008 Luminous Optical Transient in the Nearby Galaxy NGC 300
The ACS Nearby Galaxy Survey Treasury
The Advanced Camera for Surveys Nearby Galaxy Survey Treasury. V. Radial Star Formation History of NGC 300
The Ages of High-mass X-Ray Binaries in NGC 2403 and NGC 300
The Araucaria Project: An Improved Distance to the Sculptor Spiral Galaxy NGC 300 from Its Cepheid Variables
The Araucaria Project: First Cepheid Distance to the Sculptor Group Galaxy NGC 7793 from Variables Discovered in a Wide-field Imaging Survey
The Araucaria Project: The Distance to NGC 300 from the Red Giant Branch Tip Using HST ACS Imaging
The Araucaria Project: The Effect of Blending on the Cepheid Distance to NGC 300 from Advanced Camera for Surveys Images
The Chandra Local Volume Survey: The X-Ray Point-source Catalog of NGC 300
The Chandra M101 Megasecond: Diffuse Emission
The Distance to M101 Hosting Type Ia Supernova 2011fe Based on the Tip of the Red Giant Branch
The impact of satellite trails on Hubble Space Telescope observations
The Massive Star Population in M101. III. Spectra and Photometry of the Luminous and Variable Stars
The Massive Star Population in M101. II. Spatial Variations in the Recent Star Formation History
The Massive Star Population in M101. I. The Identification and Spatial Distribution of the Visually Luminous Stars
The NGC 300 Transient: An Alternative Method for Measuring Progenitor Masses
The Photometric and Spectral Evolution of the 2008 Luminous Optical Transient in NGC 300
The Red Supergiant Progenitor of Type II Supernova 2024ggi
The Slow Heartbeats of an Ultraluminous X-Ray Source in NGC 3621
The Spitzer Local Volume Legacy: Survey Description and Infrared Photometry
Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
Uncloaking globular clusters in the inner galaxy
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-07-17T19:14:23Z/2003-02-16T13:42:17Z
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, Bresolin comma Fabio, 2004, 'Extragalactic Distances: the Need for Accurate Photometry of Blue Supergiants and Cepheids', 1.0, European Space Agency, https://doi.org/10.5270/esa-airpl7g
