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On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits

Published onMay 31, 2019
On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
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Abstract

We discuss if Pop III stars and accretion disks around stellar-mass black holes at z > 7 may be directly observable to JWST and the next generation 25-39 meter ground-based telescopes through cluster caustic transits. About 3-30 of the best lensing clusters need to be monitored several times a years for several years to directly detect this.

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