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Disambiguation of "Contini, Thierry"

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Discovery of a 100 kpc-wide ionised gas structure in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7

, , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1710.11225Comment: 21 pages, 12 figures, 3 tables, accepted for publication in A&A (27 October 2017).

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Elisio Contini

Luisa Contini Nemmert

Thierry Somville

Thierry Allain

Thierry Djenizian

 

Other publications of authors with the same name

Semi-blind separation of galaxy spectra from a mixture obtained by slitless spectroscopy., , , and . EUSIPCO, page 1641-1645. IEEE, (2015)Galactic Winds with MUSE: A Direct Detection of FeII* Emission from a z = 1.29 Galaxy, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1701.07843Comment: 13 pages, 6 figures, 4 tables, submitted to A&A - comments welcome.Discovery of a 100 kpc-wide ionised gas structure in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1710.11225Comment: 21 pages, 12 figures, 3 tables, accepted for publication in A&A (27 October 2017).Dark Galaxy Candidates at Redshift ~3.5 Detected with MUSE, , , , , , , , , and 11 other author(s). (2017)cite arxiv:1709.03522Comment: 28 pages, 13 figures, 5 tables, submitted to ApJ.A New Separation Method for Galaxy Spectra Based on Data Fusion between Two Grism Orders in Slitless Spectroscopy., , , , and . ICASSP, page 4245-4249. IEEE, (2019)Mixing model in slitless spectroscopy and resulting blind methods for separating galaxy spectra., , , and . MLSP, page 1-6. IEEE, (2016)The MUSE Hubble Ultra Deep Field Survey VIII : Extended Lyman-alpha haloes around high-redshift star-forming galaxies, , , , , , , , , and 10 other author(s). (2017)cite arxiv:1710.10271Comment: 24 pages, 18 figures, 1 table, accepted for publication in A&A.The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds, , , , , and . (2015)cite arxiv:1502.07895Comment: 19 pages, 12 figures.MUSE Deep-Fields: The Lya Luminosity Function in the Hubble Deep Field South at 2.91 < z < 6.64, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1609.02920Comment: 13 pages, 8 figures, submitted to MNRAS.Inferring gas-phase metallicity gradients of galaxies at the seeing limit: A forward modelling approach, , , , , , , , , and . (2017)cite arxiv:1703.01090Comment: Accepted for publication in MNRAS.