A new calibration of Galactic Cepheid period-luminosity relations from B to K bands, and a comparison to LMC relations
Astrometry with Hubble Space Telescope Fine Guidance Sensors--A Review
Cepheid parallaxes and the Hubble constant
Gaia Cepheid parallaxes and Local Hole relieve H0 tension
Gaia Data Release 2. Catalogue validation
Hubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations
The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 mm in the Milky Way
The Distances to Open Clusters from Main-Sequence Fitting. IV. Galactic Cepheids, the LMC, and the Local Distance Scale
The mid-infrared Leavitt law for classical Cepheids in the Magellanic Clouds
The e Aquilae System: Radial Velocities and Astrometry in Search of e Aql B
Instrument
FGS
Temporal Coverage
2003-06-26T13:14:43Z/2004-06-14T02:13:11Z
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, Benedict comma George Fritz, 2005, 'An Astrometric Calibration of the Cepheid Period-Luminosity Relation', 1.0, European Space Agency, https://doi.org/10.57780/esa-z2mx7b6