( en | de | ru )

 

Disambiguation of "Schaller, Matthieu"

Author of the publication

copydeleteadd this publication to your clipboard
Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7

, , , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an additional 32 pages of supplementary figures and data tables are available from http://astro.dur.ac.uk/~ams/MUSEcubes/.

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.

Matthieu Felsinger

Matthieu Saubanère

Matthieu Hammer

Friedrich Matthieu

Matthieu Barukinamwo

 

Other publications of authors with the same name

The effect of baryons on the inner density profiles of rich clusters, , , , , , , , , and . (2014)cite arxiv:1409.8297Comment: 13 pages, 7 figures, submitted to MNRAS.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations, , , , , , , , , and . (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.SWIFT: task-based hydrodynamics and gravity for cosmological simulations, , , and . (2015)cite arxiv:1508.00115Comment: Proceedings of the EASC 2015 conference, Edinburgh, UK, April 21-23, 2015.It's not easy being green: The evolution of galaxy colour in the EAGLE simulation, , , , , , and . (2016)cite arxiv:1601.07907Comment: 15 pages, 10 figures. Submitted to MNRAS. All comments welcome. Larger version of Fig. 1 included in source. For the animated evolution of the EAGLE intrinsic u-r CMD (with central and satellite galaxies coloured red and blue respectively) see http://community.dur.ac.uk/j.w.trayford/media/CMD_evolution_EAGLE.mp4.The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end, , , , , , and . (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.A machine learning approach to mapping baryons onto dark matter halos using the EAGLE and C-EAGLE simulations, , , , , , and . (2021)cite arxiv:2106.04980Comment: 15 pages, 13 figures, submitted to MNRAS. Comments welcome!.EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, , , , , , , and . (2022)cite arxiv:2210.09978.A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find., , , and . PARCO, volume 36 of Advances in Parallel Computing, page 263-274. IOS Press, (2019)The Hydrangea simulations: galaxy formation in and around massive clusters, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.The properties of "dark" ŁambdaCDM halos in the Local Group, , , , , , , , , and . (2016)cite arxiv:1609.01301Comment: Submitted to MNRAS. Comments are welcome.