Evidence for Spectropolarimetric Diversity in Type Ia Supernovae
Investigating the break in the Cepheid period-luminosity relation and its implications
The Cepheid Distance to NGC 1637: A Direct Test of the Expanding Photosphere Method Distance to SN 1999em
The Connection between Bar Strength and Circumnuclear Dust Structure
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
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-09-02T02:55:15Z/2001-10-31T15:28:35Z
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, Leonard et al., 2002, 'The Cepheid Distance to NGC 1637: A Direct Comparison with the EPM Distance to SN 1999em', 1.0, European Space Agency, https://doi.org/10.5270/esa-7tnodx4