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Disambiguation of "Matthee, Jorryt"

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MUSEQuBES: Calibrating the redshifts of Lyman-\alpha emitters using stacked circumgalactic medium absorption profiles

, , , , , , , , , , , , , , , , , , , and . (2019)cite arxiv:1910.03593Comment: 9 Pages, Submitted to MNRAS, Comments Welcome!.

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Thorsten Matthée

Heinrich Matthee

Hans Matthee

Eva Matthée

Ulrich Matthée

 

Other publications of authors with the same name

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.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.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!.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.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.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.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.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.A 10 deg$^2$ Lyman-$\alpha$ survey at z=8.8 with spectroscopic follow-up: strong constraints on the LF and implications for other surveys, , , , , , , , and . (2014)cite arxiv:1402.6697Comment: 15 pages, 9 figures, accepted for publication in 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!.