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Disambiguation of "Calhau, Joao"

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

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

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Gil dos Santos Guerreiro João

Joao Alves

João Barros

João Fonseca

João Carreira

 

Other publications of authors with the same name

The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$, , , , , , , , , and 7 other author(s). (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, , , , , , , , , and 5 other author(s). (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.The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2, , , , , , , and . (2016)cite arxiv:1609.03571Comment: 10 pages, 8 figures, accepted to MNRAS.CF-HiZELS, a 10 deg$^2$ emission-line survey with spectroscopic follow-up: H\alpha, OIII+H\beta\ and OII luminosity functions at z=0.8, 1.4 and 2.2, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1502.06602Comment: 22 pages, 15 figures, submitted to MNRAS.On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1709.04470Comment: 17 pages, 12 figures. Submitted to MNRAS on July 25, 2017. Comments are welcome.A $1.4$ deg$^2$ blind survey for CII, CIII and CIV at $z\sim0.7-1.5$. I: nature, morphologies and equivalent widths, , , , and . (2017)cite arxiv:1703.10169Comment: Submitted to MNRAS. Comments welcome! 17 pages, 12 figures, 8 tables.A $1.4$ deg$^2$ blind survey for CII, CIII and CIV at $z\sim0.7-1.5$. II: luminosity functions and cosmic average line ratios, , , , and . (2017)cite arxiv:1704.01124Comment: Submitted to MNRAS. Comments welcome! 11 pages, 7 figures, 5 tables. Paper I can be found here: https://arxiv.org/abs/1703.10169.The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6, , , , , , , , , and . (2021)cite arxiv:2105.00007Comment: Accepted for publication in MNRAS. 20 pages, 13 figures, 4 tables.