Extending the cosmic distance ladder two orders of magnitude with strongly lensed Cepheids, carbon AGB, and RGB stars

Extreme magnification of stars near the caustics of clusters allow to detect individual luminous stars at high redshift. We show how deep exposures of caustic crossing galaxies at \(z\lesssim1\) with IR telescopes such as JWST, can detect non-explosive distance calibrators, such as Cepheids, carbon...

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Bibliographic Details
Published in:arXiv.org 2024-10
Main Authors: Diego, J M, Willner, S P, Palencia, J M
Format: Article
Language:English
Subjects:
Asymptotic giant branch stars
Asymptotic methods
Carbon stars
Cepheid variables
Dark matter
Explosives detection
Galactic clusters
Galaxies
Microlenses
Red shift
Telescopes
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Summary:Extreme magnification of stars near the caustics of clusters allow to detect individual luminous stars at high redshift. We show how deep exposures of caustic crossing galaxies at \(z\lesssim1\) with IR telescopes such as JWST, can detect non-explosive distance calibrators, such as Cepheids, carbon stars in the asymptotic giant branch or stars in the tip of the red giant branch. A large number of such detections, combined with careful modelling of the magnification affecting these stars (including microlensing), opens the door to using them as alternative standard candles to SNe in a redshift range that would extend the cosmic distance ladder two orders of magnitude for these distance calibrators. As a bonus, strongly lensed stars detected in deep exposures provide also a robust method of mapping small dark matter substructures since they cluster around the critical curves of small scale dark matter halos.
ISSN:2331-8422