Completing the census of Lyα emitters at the reionization epoch
N Kashikawa, K Shimasaku, Y Matsuda… - The Astrophysical …, 2011 - iopscience.iop.org
We carried out extended spectroscopic confirmations of Lyα emitters (LAEs) at z= 6.5 and
5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs is
45 and 54 at z= 6.5 and 5.7, respectively, and at least 81%(70%) of our photometric
candidates at z= 6.5 (5.7) have been spectroscopically identified as real LAEs. We made
careful measurements of the Lyα luminosity, both photometrically and spectroscopically, to
accurately determine the Lyα and rest-UV luminosity functions (LFs). The substantially …
5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs is
45 and 54 at z= 6.5 and 5.7, respectively, and at least 81%(70%) of our photometric
candidates at z= 6.5 (5.7) have been spectroscopically identified as real LAEs. We made
careful measurements of the Lyα luminosity, both photometrically and spectroscopically, to
accurately determine the Lyα and rest-UV luminosity functions (LFs). The substantially …
[引用][C] Completing the Census of Lyα Emitters at the Reionization Epoch
谷口義明 - Astrophysical Journal, 2011 - cir.nii.ac.jp
Completing the Census of Lyα Emitters at the Reionization Epoch | CiNii Research …
Completing the Census of Lyα Emitters at the Reionization Epoch … タイトル Completing the
Census of Lyα Emitters at the Reionization Epoch …
Completing the Census of Lyα Emitters at the Reionization Epoch … タイトル Completing the
Census of Lyα Emitters at the Reionization Epoch …