Segue Virtual Journal
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, University of Notre Dame
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Results 1 - 2 of 2
Evidence of Pop~III stars' chemical signature in neutral gas at $zsim6$. A study based on the E-XQR-30 spectroscopic sample
Volume 19, Issue 16 - article #3
Alessio Sodini
,
Valentina D'Odorico
,
Stefania Salvadori
,
Irene Vanni
,
Manuela Bischetti
,
Guido Cupani
,
Rebecca Davies
,
George D. Becker
,
Eduardo Ba~nados
,
Sarah Bosman
,
Frederick Davies
,
Emanuele Paolo Farina
,
Andrea Ferrara
,
Laura Keating
,
Girish Kulkarni
,
Samuel Lai
,
Emma Ryan-Weber
,
Alma Maria Sebastian
,
Fabian Walter
https://arxiv.org/abs/2404.10722
PypeIt: The Python Spectroscopic Data Reduction Pipeline. (arXiv:2005.06505v1 [astro-ph.IM])
Volume 15, Issue 20 - article #5
J. Xavier Prochaska
(1, 2),
Joseph F. Hennawi
(3),
Kyle B. Westfall
(4),
Ryan J. Cooke
(5),
Feige Wang
(6),
Tiffany Hsyu
(1),
Emanuele Paolo Farina
(7)
((1) University of California, Santa Cruz,
(2) Kavli Institute for the Physics, Mathematics of the Universe,
(3) University of California, Santa Barbara,
(4) University of California Observatories,
(5) Durham University, UK,
(6) Steward Observatory, University of Arizona,
(7) Max Planck Institut fur Astrophysik)
http://arxiv.org/abs/2005.06505
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