VENUS: an ultra-faint galaxy hosting the metal-poor type II supernova at z=5.13 Witnessing the initial metal enrichment with extremely frequent core-collapse supernovae?
Yoshihisa Asada, Seiji Fujimoto, Joseph F. V. Allingham, David A. Coulter, Conor Larison, Matthew R. Siebert, Gabriel Brammer, Dan Coe, Pratika Dayal, Qinyue Fei, Lukas J. Furtak, Vasily Kokorev, Keiichi Maeda, Richard Pan, Johan Richard, Fengwu Sun, Abdurro'uf, Jacqueline Antwi-Danso, Franz E. Bauer, Marusa Bradac, Larry D. Bradley, Volker Bromm, John Chisholm, Christopher J. Conselice, Christa DeCoursey, Anderas L. Faisst, Brenda Frye, Mauro Gonzalez-Otero, Yuichi Harikane, Tiger Y. Y. Hsiao, Kohei Inayoshi, Yolanda Jimenez-Teja, Anton M. Koekemoer, Kotaro Kohno, Paulo A. A. Lopes, Ray A. Lucas, Georgios E. Magdis, Vladan Markov, Nicholas Martis, Jorryt Matthee, Minami Nakane, Rohan P. Naidu, Gael Noirot, Masami Ouchi, Armin Rest, Massimo Ricotti, Louis-Gregory Strolger, Raffaella Schneider, Francesco Valentino, Eros Vanzella, Hayley Williams, Rogier A. Windhorst, Adi Zitrin
astro-ph.GA, astro-ph.HE
Submitted: 2026-07-15
Comments: Submitted to ApJ. Comments are welcome!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova
- GLIMPSE-DDT spectroscopic properties of faint-end galaxies at $z\sim6$: Towards first metal enrichment, dust production, and ionizing photon production
- A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy
- SpectRes: A Fast Spectral Resampling Tool in Python
- A first GLIMPSE into star clusters populations across cosmic time
- A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
- SAPPHIRES: Extremely Metal-Poor Galaxy Candidates with $12+{\rm log(O/H)}<7.0$ at $z\sim5-7$ from Deep JWST/NIRCam Grism Observations
- A Glimpse of the Low-Mass End of the Direct Mass-Metallicity Relation at $z\sim6-8$
- Pristine Massive Star Formation Caught at the Break of Cosmic Dawn
- An Ultra-Faint, Chemically Primitive Galaxy Forming in the Reionization Era
- Constraints on the Metallicity-dependent Explodability of Massive Stars from Galactic Chemical Evolution: Toward Alleviating the Red Supergiant Problem
- The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10
- A Pristine Star-Forming Complex at z=4.19
- Strong Gravitational Lensing with the James Webb Space Telescope
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