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GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$

Fuente: arXiv

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Bibliographic Details
Main Authors:	Fujimoto, Seiji, Naidu, Rohan P., Chisholm, John, Atek, Hakim, Endsley, Ryan, Kokorev, Vasily, Furtak, Lukas J., Pan, Richard, Liu, Boyuan, Bromm, Volker, Venditti, Alessandra, Visbal, Eli, Sarmento, Richard, Weibel, Andrea, Oesch, Pascal A., Brammer, Gabriel, Schaerer, Daniel, Adamo, Angela, Berg, Danielle A., Bezanson, Rachel, Chemerynska, Iryna, Claeyssens, Adélaïde, Dessauges-Zavadsky, Miroslava, Frebel, Anna, Korber, Damien, Labbe, Ivo, Marques-Chaves, Rui, Matthee, Jorryt, McQuinn, Kristen B. W., Muñoz, Julian B., Natarajan, Priyamvada, Saldana-Lopez, Alberto, Suess, Katherine A., Volonteri, Marta, Zitrin, Adi
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2501.11678