( en | de | ru )

 

Disambiguation of "Buat, Véronique"

Author of the publication

copydeleteadd this publication to your clipboard
Fitting AGN/galaxy X-ray-to-radio SEDs with CIGALE and improvement of the code

, , , , , , , , , , , , , and . (2022)cite arxiv:2201.03718Comment: ApJ accepted. The code is available at https://cigale.lam.fr/news/.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

Véronique Trappe

Véronique Buschmann

Véronique Porra

Véronique Mersseman

Véronique Henn

 

Other publications of authors with the same name

Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation, , , , , , , , , and 10 other author(s). (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.Fitting AGN/galaxy X-ray-to-radio SEDs with CIGALE and improvement of the code, , , , , , , , , and 4 other author(s). (2022)cite arxiv:2201.03718Comment: ApJ accepted. The code is available at https://cigale.lam.fr/news/.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , and 54 other author(s). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.The Herschel view of the dominant mode of galaxy growth from z=4 to the present day, , , , , , , , , and 13 other author(s). (2014)cite arxiv:1409.5433Comment: 28 pages, 25 figures, submitted to A&A.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.Impact of star formation history on the measurement of star formation rates, , and . (2014)cite arxiv:1409.5792Comment: 10 pages, 10 figures, 1 table. Accepted for publication in A&A.A hyperluminous obscured quasar at a redshift of z ~ 4.3, , , , , , , , , and 2 other author(s). (2021)cite arxiv:2103.08032Comment: Accepted for publication in Monthly Notices of the Royal Astronomical Society Letters. Models used in this work are available at http://ahpc.euc.ac.cy/.Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2106.12573Comment: Accepted to A&A.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.