Roberto Philip Saglia
Affiliations: | Max-Planck Institute for extraterrestrial Physics |
Website:
http://www.mpe.mpg.de/~saglia/saglia.htmlGoogle:
"Roberto Saglia"Children
Sign in to add trainee| Maurilio Pannella | grad student | 2007 | Ludwig Maximilian University Munich |
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Publications
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| Mendel JT, Beifiori A, Saglia RP, et al. (2020) The Kinematics of Massive Quiescent Galaxies at 1.4 < z <2.1: Dark Matter Fractions, IMF Variation, and the Relation to Local Early-type Galaxies The Astrophysical Journal. 899: 87 |
| Wilman DJ, Fossati M, Mendel JT, et al. (2020) The Regulation of Galaxy Growth along the Size–Mass Relation by Star Formation, as Traced by Hα in KMOS3D Galaxies at 0.7 ≲ z ≲ 2.7 The Astrophysical Journal. 892: 1 |
| Bisigello L, Kuchner U, Conselice CJ, et al. (2020) Euclid: The selection of quiescent and star-forming galaxies using observed colours Monthly Notices of the Royal Astronomical Society. 494: 2337-2354 |
| Nicola Sd, Saglia RP, Thomas J, et al. (2020) Non-parametric triaxial deprojection of elliptical galaxies Monthly Notices of the Royal Astronomical Society. 496: 3076-3100 |
| Blanchard A, Camera S, Carbone C, et al. (2020) Euclid preparation: VII. Forecast validation for Euclid cosmological probes Astronomy and Astrophysics |
| Paykari P, Kitching TD, Hoekstra H, et al. (2020) Euclid preparation VI. Verifying the performance of cosmic shear experiments Astronomy and Astrophysics. 635 |
| Pires S, Vandenbussche V, Kansal V, et al. (2020) Euclid : reconstruction of weak-lensing mass maps for non-Gaussianity studies. Astronomy and Astrophysics. 638 |
| Mehrgan K, Thomas J, Saglia R, et al. (2019) A 40-billion solar mass black hole in the extreme core of Holm 15A, the central galaxy of Abell 85 The Astrophysical Journal. 887: 195 |
| Wisnioski E, Schreiber NMF, Fossati M, et al. (2019) The KMOS3D Survey: Data Release and Final Survey Paper The Astrophysical Journal. 886: 124 |
| Übler H, Genzel R, Wisnioski E, et al. (2019) The Evolution and Origin of Ionized Gas Velocity Dispersion fromz∼ 2.6 toz∼ 0.6 with KMOS3D The Astrophysical Journal. 880: 48 |