Strongly lensed [O III] emitters at Cosmic Noon with Roman: Characterizing extreme emission line galaxies on star cluster complex scales (100 pc)

Kim, Keunho J.; Bayliss, Matthew B.; Dahle, Håkon; Hutchison, Taylor; Sharon, Keren; Mahler, Guillaume; Owens, M. Riley; Rhoads, James E.

doi:10.48550/arXiv.2307.01247

Article (Scientific journals)

Strongly lensed [O III] emitters at Cosmic Noon with Roman: Characterizing extreme emission line galaxies on star cluster complex scales (100 pc)

Kim, Keunho J.; Bayliss, Matthew B.; Dahle, Håkon et al.

2023 • In arXiv e-prints, p. 2307.01247

Peer reviewed

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https://hdl.handle.net/2268/333086

DOI
10.48550/arXiv.2307.01247

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Keywords :

Astrophysics - Astrophysics of Galaxies

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Kim, Keunho J.

Bayliss, Matthew B.

Dahle, Håkon

Hutchison, Taylor

Sharon, Keren

Mahler, Guillaume ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Multi-wavelength Extragalactic and Galactic Astrophysics (MEGA)

Owens, M. Riley

Rhoads, James E.

Language :

English

Title :

Strongly lensed [O III] emitters at Cosmic Noon with Roman: Characterizing extreme emission line galaxies on star cluster complex scales (100 pc)

Publication date :

July 2023

Journal title :

arXiv e-prints

Pages :

arXiv:2307.01247

Peer reviewed :

Peer reviewed

Additional URL :

https://ui.adsabs.harvard.edu/abs/2023arXiv230701247K

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