Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
AGAdam G. RiessSCStefano CasertanoWYWenlong YuanLMLucas M. MacriDSDan Scolnic
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Abstract
Abstract We present an improved determination of the Hubble constant from Hubble Space Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud (LMC). These were obtained with the same WFC3 photometric system used to measure extragalactic Cepheids in the hosts of SNe Ia. Gyroscopic control of HST was employed to reduce overheads while collecting a large sample of widely separated Cepheids. The Cepheid period–luminosity relation provides a zero-point-independent link with 0.4% precision between the new 1.2% geometric distance to the LMC from detached eclipsing binaries (DEBs) measured by Pietrzyński et al. and the luminosity of SNe Ia. Measurements and analysis of the LMC Cepheids…
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Authors
5- AGAdam G. RiessCorresponding
- SCStefano Casertano
- WYWenlong Yuan
- LMLucas M. Macri
- DSDan Scolnic
Topics & keywords
Topics
Keywords
- Cepheid variable
- Large Magellanic Cloud
- Hubble's law
- Cosmic microwave background
- Milky Way
- Luminosity
- Cosmic distance ladder
- Stars
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