A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys Observations
Compact Optical Counterparts of Ultraluminous X-Ray Sources
Multi-Epoch Multi-Wavelength Study of an Ultraluminous X-ray Source in M101: The Nature of the Secondary
Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
Physical Structure and Nature of Supernova Remnants in M101
The Distance to M101 Hosting Type Ia Supernova 2011fe Based on the Tip of the Red Giant Branch
The impact of satellite trails on Hubble Space Telescope observations
The Metallicity Dependence of the Cepheid P - L Relation in M101
The Vast Population of Wolf-Rayet and Red Supergiant Stars in M101. I. Motivation and First Results
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2006-12-23T00:40:49Z/2007-03-13T13:18:36Z
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, Freedman comma Wendy L., 2008, 'Reducing Systematic Errors on the Hubble Constant: Metallicity Calibration of the Cepheid PL Relation', 1.0, European Space Agency, https://doi.org/10.5270/esa-b1o4h8q