Cepheid Calibration of the Peak Brightness of Type Ia Supernovae. XI. SN 1998aq in NGC 3982
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
Gone without a bang: an archival HST survey for disappearing massive stars
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
The distance to Supernova 1998aq in NGC 3982
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
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2000-03-20T11:19:14Z/2000-05-12T17:45:54Z
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, Saha comma Abhijit, 2001, 'Calibration of Nearby Type Ia Supernovae as Standard Candles: The Next Step', 1.0, European Space Agency, https://doi.org/10.5270/esa-1p197yb