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A population of faint, old, and massive quiescent galaxies at 3<z<4 revealed by JWST NIRSpec Spectroscopy.
- Published in:
- Scientific Reports, 2024, v. 14, n. 1, p. 1, doi. 10.1038/s41598-024-52585-4
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- Article
Revelation of Massive Quiescent Galaxies at z >3 from Deep JWST Spectroscopy.
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- Proceedings of the International Astronomical Union, 2022, v. 18, n. S377, p. 3, doi. 10.1017/S1743921323001552
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- Article
A VLT/MUSE analysis of HeIIλ1640 emitters at z = 2 – 4.
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- Proceedings of the International Astronomical Union, 2020, v. 15, n. S352, p. 78, doi. 10.1017/S1743921320001143
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- Article
Probing the ISM of Heiiλ1640 emitters at z = 2–4 via MUSE.
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- Proceedings of the International Astronomical Union, 2019, v. 15, p. 235, doi. 10.1017/S1743921319002552
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- Article
Probing the ISM of Heiiλ1640 emitters at z = 2–4 via MUSE.
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- Proceedings of the International Astronomical Union, 2019, v. 15, n. S341, p. 235, doi. 10.1017/S1743921319002552
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- Article
The mean Hα EW and Lyman-continuum photon production efficiency for faint z ≈ 4−5 galaxies.
- Published in:
- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201935227
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- Article
Exploring He II λ1640 emission line properties at z ∼2−4.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 624, p. N.PAG, doi. 10.1051/0004-6361/201834565
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- Article
The MUSE Hubble Ultra Deep Field Survey.
- Published in:
- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 619, p. N.PAG, doi. 10.1051/0004-6361/201833136
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- Article
Probing the ISM of Heiiλ1640 emitters at z = 2–4 via MUSE.
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- Proceedings of the International Astronomical Union, 2018, v. 13, n. 1S341, p. 235, doi. 10.1017/S1743921319002552
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- Article
Can we infer the Initial Mass Function of galaxies at z ~ 2?
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- Proceedings of the International Astronomical Union, 2015, v. 11, n. S319, p. 35, doi. 10.1017/S174392131500993X
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- Article