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[HTML][HTML] The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ1909 emitters at z= 2–4

K Nakajima, D Schaerer, O Le Fèvre, R Amorín… - Astronomy & …, 2018 - aanda.org
Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically confirm high-z
galaxies and increasingly also to determine their physical properties. Aims. We construct …
被引用次数：150 相关文章

The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ1909 emitters at z= 2-4

K Nakajima, D Schaerer, O Le Fèvre… - Astronomy and …, 2018 - ui.adsabs.harvard.edu
Abstract Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically
confirm high-z galaxies and increasingly also to determine their physical properties. Aims …

The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of C III] λ 1909 emitters at z= 2-4

K Nakajima, D Schaerer, O Le Fevre… - ASTRONOMY & …, 2018 - cris.unibo.it
Abstract Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically
confirm high-z galaxies and increasingly also to determine their physical properties. Aims …
[PDF] core.ac.uk

[PDF][PDF] The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ1909 emitters at z= 2–4

K Nakajima, D Schaerer, O Le Fèvre, R Amorín, M Talia… - A&A, 2018 - core.ac.uk
ABSTRACT Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically
confirm high-z galaxies and increasingly also to determine their physical properties. Aims …
[PDF] researchgate.net

[PDF][PDF] The VIMOS Ultra Deep Survey: On the nature, ISM properties, and ionizing spectra of Ciii] λ1909 emitters at z= 2− 4

K Nakajima, D Schaerer, O Le Fèvre… - arXiv preprint arXiv …, 2017 - researchgate.net
Context. Ultraviolet (UV) emission lines spectra are used to spectroscopically-confirm high-z
galaxies and increasingly also to determine their physical properties. Aims. We construct …

The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII]λ1909 emitters at z = 2–4

K Nakajima, D Schaerer, O Le Fèvre, R Amorín… - Astronomy & …, 2018 - cir.nii.ac.jp
抄録< jats: p>< jats: italic> Context.</jats: italic> Ultraviolet (UV) emission-line spectra are
used to spectroscopically confirm high-< jats: italic> z</jats: italic> galaxies and increasingly …

[引用][C] The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ 1909 emitters at z= 2–4

K Nakajima, D Schaerer, O Le Fèvre… - … and Astrophysics-A&A, 2018 - hal.science
The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ 1909
emitters at z = 2–4 - Archive ouverte HAL Accéder directement au contenu Documentation FR …

The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ1909 emitters at z= 2-4

K Nakajima, D Schaerer, O Le Fèvre, R Amorín, M Talia… - 2018 - openaccess.inaf.it
Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically confirm high-z
galaxies and increasingly also to determine their physical properties. Aims: We construct …

The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII] λ1909 emitters at z= 2-4

K Nakajima, D Schaerer, O Le Fèvre… - Astronomy and …, 2018 - ui.adsabs.harvard.edu
Abstract Context. Ultraviolet (UV) emission-line spectra are used to spectroscopically
confirm high-z galaxies and increasingly also to determine their physical properties. Aims …

[引用][C] The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of C III] λ 1909 emitters at z= 2-4

K Nakajima, D Schaerer, O Le Fèvre… - Astronomy and …, 2018 - EDP Sciences