Asteroid Trails in Hubble Space TelescopeWFPC2 Images: First Results
Cepheid Calibration of the Peak Brightness of SNe Ia. V. SN 1981B in NGC 4536
Cepheid Calibration of the Peak Brightness of Type IA Supernovae. VI. SN 1960F in NGC 4496A
Cepheid Calibrations of Modern Type Ia Supernovae: Implications for the Hubble Constant
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
Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks
Gone without a bang: an archival HST survey for disappearing massive stars
Nuclear star clusters in 228 spiral galaxies in the HST/WFPC2 archive: catalogue and comparison to other stellar systems
Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
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
Stellar Populations in the Large Magellanic Cloud:Evidence for a Significant Number of Older Stars or a Steeper IMF?
The dispersion in the Cepheid period-luminosity relation and the consequences for the extragalactic distance scale
The Environments of Supernovae in Post-Refurbishment Hubble Space Telescope Images
The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations
The Hubble Constant: A Summary of the Hubble Space Telescope Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXV. A Recalibration of Cepheid Distances to Type IA Supernovae and the Value of the Hubble Constant
The Opacity of Nearby Galaxies from Colors and Counts of Background Galaxies. I. The Synthetic Field Method and Its Application to NGC 4536 and NGC 3664
The Opacity of Spiral Galaxy Disks. III. Automating the Synthetic Field Method
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 Tolman Surface Brightness Test for the Reality of the Expansion. I. Calibration of the Necessary Local Parameters
The Virgo Cluster Distance from 21 Centimeter Line Widths
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-05-27T08:30:17Z/1994-08-09T05:53:36Z
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, 1995, 'CALIBRATION OF NEARBY GALAXY TYPE IA SUPERNOVAE AS STANDARD CANDLES: NGC4496 AND NGC4356 - CYCLE4MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-665a0lj
