( en | de | ru )

 

Disambiguation of "Saglia, R."

Author of the publication

copydeleteadd this publication to your clipboard
The angular momentum distribution and baryon content of star forming galaxies at z~1-3

, , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2015)cite arxiv:1510.03262Comment: Submitted to Astrophysical Journal.

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.

Roberto Saglia

Roberto Philip Saglia

R Chaudhury

R Bässler

R Giese

 

Other publications of authors with the same name

Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey, , , , , , , , , and 80 other author(s). (2020)cite arxiv:2005.00055Comment: 15 pages, 8 figures.MOONS: a multi-object optical and near-infrared spectrograph for the VLT, , , , , , , , , and 70 other author(s). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, volume 8446 of Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, (September 2012)$Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis, , , , , , , , , and 199 other author(s). (2021)cite arxiv:2106.08346Comment: 19 pages, 8 figures, 4 tables, 1 appendix.Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data, , , , , , , , , and 85 other author(s). (2021)cite arxiv:2105.09746Comment: 14 pages, 7 figures. Submitted to Astronomy & Astrophysics.Euclid preparation: V. Predicted yield of redshift 7<z<9 quasars from the wide survey, , , , , , , , , and 119 other author(s). (2019)cite arxiv:1908.04310Comment: Submitted to A&A. This paper has been internally reviewed by the Euclid Consortium.Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies, , , , , , , , , and 28 other author(s). (2014)cite arxiv:1406.0183Comment: Submitted to Astrophysical Journal.The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7, , , , , , , , , and 17 other author(s). (2014)cite arxiv:1409.6791Comment: 20 pages, 11 figures, submitted to ApJ.The angular momentum distribution and baryon content of star forming galaxies at z~1-3, , , , , , , , , and 18 other author(s). (2015)cite arxiv:1510.03262Comment: Submitted to Astrophysical Journal.Euclid: Modelling massive neutrinos in cosmology -- a code comparison, , , , , , , , , and 126 other author(s). (2022)cite arxiv:2211.12457Comment: 43 pages, 17 figures, 2 tables; published on behalf of the Euclid Consortium; data available at https://doi.org/10.5281/zenodo.7297976.KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks, , , , , , , , , and 19 other author(s). (2016)cite arxiv:1603.03432Comment: Submitted to ApJ. Fig. 4 compares stellar and baryonic masses to dynamical masses. Fig. 6 and 7 show the dependence of stellar and baryonic mass fractions on redshift and surface density.