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Disambiguation of "Matthee, Jorryt"

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The clustering of H$\beta$+OIII and OII emitters since $z 5$: dependencies with line luminosity and stellar mass

, , , , , , , , , and . (2017)cite arxiv:1705.01101Comment: 19 pages, 11 figures, 4 tables, submitted to MNRAS.

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Heinrich Matthee

Hans Matthee

Thorsten Matthée

Ulrich Matthée

Eva Matthée

 

Other publications of authors with the same name

On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictions, , , , , , , , and . (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , and 14 other author(s). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.MUSEQuBES: Calibrating the redshifts of Lyman-\alpha emitters using stacked circumgalactic medium absorption profiles, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1910.03593Comment: 9 Pages, Submitted to MNRAS, Comments Welcome!.A relationship between specific star formation rate and metallicity gradient within z=1 galaxies from KMOS-HiZELS, , , , , , , , and . (2014)cite arxiv:1407.1047Comment: Accepted for publication in MNRAS.Identification of the brightest Ly\alpha\ emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era, , , , , and . (2015)cite arxiv:1502.07355Comment: 20 pages, main results shown in Fig. 6 and Fig. 7, submitted to MNRAS.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at $z=0.4-4.7$, , , , , , , and . (2017)cite arxiv:1702.04721Comment: Submitted to MNRAS. Main text 16 pages, 7 Figures.The clustering of H$\beta$+OIII and OII emitters since $z 5$: dependencies with line luminosity and stellar mass, , , , , , , , , and . (2017)cite arxiv:1705.01101Comment: 19 pages, 11 figures, 4 tables, submitted to MNRAS.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.