investigation of Stars In the Milky way with Bayesian statistics and Asteroseismology
A. R. G. Santos, T. L. Campante, W. J. Chaplin, M. S. Cunha, M. N. Lund, R. Kiefer, D. Salabert, R. A. Garcia, G. R. Davies, Y Elsworth, R. Howe
Signatures of magnetic activity in the seismic data of solar-type stars observed by Kepler
See arXiv version
Accepted for publication in ApJS, 19(+86) pages, 11(+89) figures, 2(+87) tables
Jakob Rørsted Mosumgaard, Warrick H. Ball, Víctor Silva Aguirre, Achim Weiss, Jørgen Christensen-Dalsgaard
Stellar models with calibrated convection and temperature stratification from 3D hydrodynamics simulations
See arXiv version
10 pages, 9 figures. Accepted for publication in MNRAS
C. De Masi, F. Vincenzo, F. Matteucci, G. Rosani, La Barbera, A. Pasquali, E. Spitoni
Is the IMF in ellipticals bottom-heavy? Clues from their chemical abundances
See arXiv version
24 pages, 25 figures, accepted for publication on MNRAS
Continue reading “Is the IMF in ellipticals bottom-heavy? Clues from their chemical abundances”
Melissa K. Ness, Victor Silva Aguirre, Mikkel N. Lund, Matteo Cantiello, Daniel Foreman-Mackey, David W. Hogg, Ruth Angus
Inference of stellar parameters from brightness variations
See arXiv version
10 pages, 7 Figures, submitted to ApJ
Continue reading “Inference of stellar parameters from brightness variations”
V. Van Eylen, F. Dai, S. Mathur, D. Gandolfi, S. Albrecht, M. Fridlund, R. A. García, E. Guenther, M. Hjorth, A. B. Justesen, J. Livingston, M. N. Lund, F. Pérez Hernández, J. Prieto-Arranz, C. Regulo, L. Bugnet, M. E. Everett, T. Hirano, D. Nespral, G. Nowak, E. Palle, V. Silva Aguirre, T. Trifonov, J. N. Winn, O. Barragán, P. G. Beck, W. J. Chaplin, W. D. Cochran, S. Csizmadia, H. Deeg, M. Endl, P. Heeren, S. Grziwa, A. P. Hatzes, D. Hidalgo, J. Korth, S. Mathis, P. Montañes Rodriguez, N. Narita, M. Patzold, C. M. Persson, F. Rodler, A. M. S. Smith
HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2
See arXiv version
Submitted to MNRAS on 23 February 2018, accepted for publication, 4 May 2018
Emanuele Spitoni joins SAC and the iSIMBA group on 1 May 2018.
Emanuele is an expert in chemical evolution models of the Galaxy, and will perform comparisons between the predictions of these models and the properties of stellar populations as determined from asteroseismology.
Read more about Emanuele: People
