Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
Blending of Cepheids in M33
Compact Star Clusters in M81. I. Data from Hubble Space Telescope Wide Field Planetary Camera 2 Imaging
Compact Star Clusters in M81. II. Two Populations
Compact Star Clusters in Nearby Dwarf Irregular Galaxies
Confirmation of New Planetary Nebulae in the Large Magellanic Cloud
Far-Ultraviolet Spectroscopy of Star-forming Regions in Nearby Galaxies: Stellar Populations and Abundance Indicators
HST Astrometry in the 30 Doradus Region: Measuring Proper Motions of Individual Stars in the Large Magellanic Cloud
Hubble Space Telescope Images of Magellanic Cloud Planetary Nebulae
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. V. The Rapid Rotation of 47 Tuc Traced and Modeled in Three Dimensions
Hubble Space Telescope study of resolved red giant stars in the outer halos of nearby dwarf starburst galaxies
Kinematics of Star Clusters in M33: Distinct Populations
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
On the Distance to Nearby Dwarf Galaxy NGC 1569
Photometric determination of the mass accretion rates of pre-mainsequence stars - III. Results in the Large Magellanic Cloud
Probing interstellar extinction near the 30 Doradus nebula with red giant stars
Star Cluster Candidates in M81
Star clusters in M 33. IV. A new survey from deep HST images
The DIRECT Project: Influence of Blending on the Cepheid Distance Scale. I. Cepheids in M31
The Globular Cluster Systems of the Early-Type Galaxies NGC 3379, NGC 4406, and NGC 4594 and Implications for Galaxy Formation
The Initial Mass Function toward the Low-Mass End in the Large Magellanic Cloud with Hubble Space Telescope WFPC2 Observations
The Low-Mass Pre-Main-Sequence Population of the Stellar Association LH 52 in the Large Magellanic Cloud Discovered with Hubble Space Telescope WFPC2 Observations
The progenitors of the Milky Way stellar halo: big bricks favoured over little bricks.
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
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
1998-07-12T02:16:14Z/2002-05-25T05:35:16Z
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, Casertano et al., 2002, 'POMS Test Proposal: WFII targeted parallel archive proposal', 1.0, European Space Agency, https://doi.org/10.5270/esa-ufgggl2