Disentangling the Physical Origin of Emission Line Ratio Offsets at High Redshift with Spatially Resolved Spectroscopy

Jessie Hirtenstein; Tucker Jones; Ryan L. Sanders; Crystal L. Martin; M. C. Cooper; Gabriel Brammer; Tommaso Treu; Kasper Schmidt; Alice Shapley

doi:10.3847/1538-4357/ac1d52

Disentangling the Physical Origin of Emission Line Ratio Offsets at High Redshift with Spatially Resolved Spectroscopy

Jessie Hirtenstein, Tucker Jones, Ryan L. Sanders, Crystal L. Martin, M. C. Cooper, Gabriel Brammer, Tommaso Treu, Kasper Schmidt, Alice Shapley

The Cosmic Dawn Center

Research output: Contribution to journal › Journal article › Research › peer-review

Original language	English
Article number	12
Journal	Astrophysical Journal
Volume	922
Issue number	1
Number of pages	16
ISSN	0004-637X
DOIs	https://doi.org/10.3847/1538-4357/ac1d52
Publication status	Published - 15 Nov 2021

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10.3847/1538-4357/ac1d52

https://arxiv.org/pdf/2106.13810.pdf

Cite this

Disentangling the Physical Origin of Emission Line Ratio Offsets at High Redshift with Spatially Resolved Spectroscopy. / Hirtenstein, Jessie; Jones, Tucker; Sanders, Ryan L.; Martin, Crystal L.; Cooper, M. C.; Brammer, Gabriel; Treu, Tommaso; Schmidt, Kasper; Shapley, Alice.

In: Astrophysical Journal, Vol. 922, No. 1, 12, 15.11.2021.

Research output: Contribution to journal › Journal article › Research › peer-review

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