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Disambiguation of "Tacchella, Sandro"

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Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.

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Paolo Tacchella

Sandro Valle

(_1hn1_1hn2_1hn3I)-ADAM und (_1hn9_1hn9_1hnmTc)-TRODAT-1: szintigraphische In-vivo-Darstellung der serotonergen und dopaminergen Transportersysteme anhand von Micro-SPECT im ZNS von Ratten. Uni München, (2009)

Sandro Wefel

Sandro Casagrande

Sandro Limbach

 

Other publications of authors with the same name

JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty, , , , , , , , , and 18 other author(s). (2023)cite arxiv:2308.01230Comment: Submitted to A&A, 25 pages, 13 figures, 4 tables; replaced with updated M_BH-Mstar panel in Fig.7.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.Carbonaceous dust grains within galaxies seen in the first billion years of cosmic time, , , , , , , , , and 32 other author(s). (2023)cite arxiv:2302.05468Comment: 27 pages, 7 figures. Submitted.On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2111.05351Comment: 27 pages + Appendix; Submitted to ApJ; Comments welcome.High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies, , , , , , , and . (2021)cite arxiv:2104.12788Comment: 15 pages, 12 figures. To be submitted to MNRAS.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , and 57 other author(s). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.Atomic and molecular gas in IllustrisTNG galaxies at low redshift, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1902.10714Comment: 22 pages, 11 figures. Comments welcome. Additional figures and link to data at http://www.benediktdiemer.com/data/hi-h2-in-illustris/.Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence, and . (2019)cite arxiv:1901.07556Comment: 24 pages, 15 figures, submitted to MNRAS, comments welcome.