Autor der Publikation

On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6

, , , , , , , , , , und . (2017)cite arxiv:1709.04470Comment: 17 pages, 12 figures. Submitted to MNRAS on July 25, 2017. Comments are welcome.

Bitte wählen Sie eine Person um die Publikation zuzuordnen

Um zwischen Personen mit demselben Namen zu unterscheiden, wird der akademische Grad und der Titel einer wichtigen Publikation angezeigt. Zudem lassen sich über den Button neben dem Namen einige der Person bereits zugeordnete Publikationen anzeigen.

 

Weitere Publikationen von Autoren mit dem selben Namen

The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6, , , , , , , , , und . (2021)cite arxiv:2105.00007Comment: Accepted for publication in MNRAS. 20 pages, 13 figures, 4 tables.The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23, , , , , , , , und . (2016)cite arxiv:1609.05897Comment: 18 pages, 10 figures. Submitted to MNRAS in July. Comments welcome.The CALYMHA survey: Ly$\alpha$ escape fraction and its dependence on galaxy properties at $z=2.23$, , , , , , und . (2016)cite arxiv:1602.02756Comment: Accepted for publication by MNRAS.The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$, , , , , , , , , und 7 andere Autor(en). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.(Re)Solving Reionization with Ly\alpha: How Bright Ly\alpha Emitters account for the $z\approx2-8$ Cosmic Ionizing Background, , , , , , , , , und 5 andere Autor(en). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6, , , , , , , , , und 1 andere Autor(en). (2017)cite arxiv:1709.04470Comment: 17 pages, 12 figures. Submitted to MNRAS on July 25, 2017. Comments are welcome.