SMEAL WIKI

Multi-band high resolution spectroscopy rules out the hot Jupiter BD+20 1790b

I. Carleo, S. Benatti, A. F. Lanza, R. Gratton, R. Claudi, S. Desidera, Gregory N. Mace, S. Messina, N. Sanna, E. Sissa, A. Ghedina, F. Ghinassi, J. Guerra, A. Harutyunyan, G. Micela, E. Molinari, E. Oliva, Andrea Tozzi, C. Baffa, Andrea Baruffolo, A. Bignamini, N. Buchschacher, M. Cecconi, R. Cosentino, Michael Endl, G. Falcini, D. Fantinel, Luca Fini, D. Fugazza, A. Galli, E. Giani, Carlos Gómez González, E. González-Álvarez, M. Pantaleoni González, N. Hernandez, Marcos Hernandez Díaz, M. Iuzzolino, Kyle Kaplan, Benjamin L. Kidder, Marcello Lodi, L. Malavolta, J. Maldonado, L. Origlia, Héctor Pérez Ventura, Alfio Puglisi, M. Rainer, Luis Riverol, C. Riverol, J. San Juan, Salvatore Scuderi, U. Seemann, Kimberly R. Sokal, A. Sozzetti, M. Sozzi
Year2018
VenueAstronomy and Astrophysics
Typearticle
Citations35
DOI10.1051/0004-6361/201732350
OpenAlexW2798398299

Topics

Stellar, planetary, and galactic studiesPhysicsPlanetAstrophysicsPhotometry (optics)Amplitude