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Physical Properties of Strong 1 < Z < 3 Balmer and Paschen Line Emitters Observed with JWST

L. -M. Seille,V. Buat,V. Fernandez,M. Boquien,Y. Roehlly,A. Boselli,A. Calabro,R. O. Amorin,P. Arrabal Haro, B. E. Backhaus,M. B. Bagley,D. Burgarella,N. J. Cleri,M. Dickinson,S. L. Finkelstein,N. P. Hathi,B. W. Holwerda,J. S. Kartaltepe,A. M. Koekemoer,L. Napolitano,F. Pacucci,C. Papovich,N. Pirzkal, C. Robertson,L. Y. A. Yung

ASTRONOMY & ASTROPHYSICS（2024）

Cited 2|Views24
Key words
HII regions,galaxies: high-redshift,galaxies: ISM,galaxies: star formation
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