A Population of Compact Elliptical Galaxies Detected with the Virtual Observatory
Cepheid Calibration of the Peak Brightness of Type IA Supernovae. X. SN 1991T in NGC 4527
Cepheid Distances to SNe Ia Host Galaxies Based on a Revised Photometric Zero Point of the HST WFPC2 and New PL Relations and Metallicity Corrections
Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae Leading to a Fully Corrected Hubble Diagram to v < 30,000 km s-1
Supernova 1991T and the Value of the Hubble Constant
The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations
The globular cluster system of NGC 1316. II. The extraordinary object SH2
The globular cluster system of NGC 1316. IV. Nature of the star cluster complex SH2
The Hubble Constant: A Summary of the Hubble Space Telescope Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
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, WFPC2/WFC
Temporal Coverage
1999-04-11T07:03:13Z/1999-08-21T22:18:53Z
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, Sandage comma Allan, 2000, 'Calibration of Nearby Type Ia Supernovae as Standard Candles: The Next Three-Year Step', 1.0, European Space Agency, https://doi.org/10.5270/esa-orl2yv4