On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
- Author(s):
- Windhorst, R.; Alpaslan, M.; Andrews, S.; Ashcraft, T.; Broadhurst, T.; Coe, D.; Conselice, C.; Cohen, S.; Diego, J.; Dijkstra, M.; Driver, S.; Duncan, K.; Finkelstein, S.; Frye, B.; Griffiths, A.; Grogin, N.; Hathi, N.; Hopkins, A.; Jansen, R.; Joshi, B.; Kashlinsky, A.; Keel, W.; Kelly, P.; Kim, D.; Koekemoer, A.; Larson, R.; Livermore, R.; Marshall, M.; Mechtley, M.; Pirzkal, N.; Rieke, M.; Riess, A.; Robotham, A.; Rodney, S.; Röttgering, H.; Rutkowski, M.; Ryan, R.; Smith, B.; Straughn, A.; Strolger, L.; Tilvi, V.; Timmes, F.; Wilkins, S.; Willmer, C.; Wyithe, S.; Yan, H.; Zitrin, A.
- Published
- 2019
- Publication type
- Article / Letter to editor
- Date issued
- 2019
- Language
- English
- Is part of
- Bulletin of the American Astronomical Society (2019), Vol. 51, no. 3, p. 449
- hdl
- 1887/84981
- URL
- https://ui.adsabs.harvard.edu/abs/2019BAAS...51c.449W
