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BOSELLI , A.

Last name: BOSELLI

First name: A.

September 11, 2024 (v1)

Journal article

Metadata-only

Physical properties of strong 1 < z < 3 Balmer and Paschen line emitters observed with JWST

Seillé, L.-M. Buat, V. Fernández, V.

Context. The ultraviolet continuum traces young stars while the near-infrared unveils older stellar populations and dust-obscured regions. Balmer emission lines provide insights into gas properties and young stellar objects but are highly affected by dust attenuation. The near-infrared Paschen lines suffer less dust attenuation and can be used...

Uploaded on: October 15, 2024
September 2024 (v1)

Journal article

Metadata-only

Physical properties of strong 1 < z < 3 Balmer and Paschen line emitters observed with JWST

Seillé, L.-M. Buat, V. Fernández, V.

Context. The ultraviolet continuum traces young stars while the near-infrared unveils older stellar populations and dust-obscured regions. Balmer emission lines provide insights into gas properties and young stellar objects but are highly affected by dust attenuation. The near-infrared Paschen lines suffer less dust attenuation and can be used...

Uploaded on: October 17, 2024
September 2014 (v1)

Journal article

Metadata-only

CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey

Walcher, C. Wisotzki, L. Bekeraité, S.

International audience

Uploaded on: December 4, 2022