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Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO

Authors :
Sulis, S.
Lendl, M.
Cegla, H. M.
Rodriguez Diaz, L. F.
Bigot, L.
Van Grootel, V.
Bekkelien, A.
Collier Cameron, A.
Maxted, P. F. L.
Simon, A. E.
Lovis, C.
Scandariato, G.
Bruno, G.
Nardiello, D.
Bonfanti, A.
Fridlund, M.
Persson, C. M.
Salmon, S.
Sousa, S. G.
Wilson, T. G.
Krenn, A.
Hoyer, S.
Santerne, A.
Ehrenreich, D.
Alibert, Y.
Alonso, R.
Anglada Escudé, G.
Bàrczy, T.
Barrado y Navascués, D.
Barros, S. C. C.
Baumjohann, W.
Beck, M.
Beck, T.
Benz, W.
Billot, N.
Bonfils, X.
Borsato, L.
Brandeker, A.
Broeg, C.
Cabrera, J.
Charnoz, S.
Corral Van Damme, C.
Csizmadia, Sz.
Davies, M. B.
Deleuil, M.
Deline, A.
Delrez, L.
Demangeon, O. D. S.
Demory, B. -O.
Erikson, A.
Fortier, A.
Fossati, L.
Gandolfi, D.
Gillon, M.
Güdel, M.
Heng, K.
Isaak, K. G.
Kiss, L. L.
Laskar, J.
Lecavelier des Etangs, A.
Magrin, D.
Munari, M.
Nascimbeni, V.
Olofsson, G.
Ottensamer, R.
Pagano, I.
Palle, E.
Peter, G.
Piotto, G.
Pollacco, D.
Queloz, D.
Ragazzoni, R.
Rando, N.
Rauer, H.
Ribas, I.
Rieder, M.
Santos, N. C.
Segransan, D.
Smith, A. M. S.
Steinberger, M.
Steller, M.
Szabó, Gy. M.
Thomas, N.
Udry, S.
Walton, N. A.
Wolter, D.
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Institut de Planétologie et d'Astrophysique de Grenoble (IPAG)
Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG )
Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France
Institut de Physique du Globe de Paris (IPGP (UMR_7154))
Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Institut d'Astrophysique de Paris (IAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Science & Technology Facilities Council
University of St Andrews. School of Physics and Astronomy
University of St Andrews. St Andrews Centre for Exoplanet Science
University of St Andrews. School of Economics and Finance
University of St Andrews. University of St Andrews
Source :
Astronomy & Astrophysics, 670, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2023, 670, ⟨10.1051/0004-6361/202244223⟩, Sulis, S, Lendl, M, Cegla, H M, Rodríguez Díaz, L F, Bigot, L, Van Grootel, V, Bekkelien, A, Cameron, A C, Maxted, P F L, Simon, A E, Lovis, C, Scandariato, G, Bruno, G, Nardiello, D, Bonfanti, A, Fridlund, M, Persson, C M, Salmon, S, Sousa, S G, Wilson, T G, Krenn, A, Hoyer, S, Santerne, A, Ehrenreich, D, Alibert, Y, Alonso, R, Anglada, G, Bárczy, T, Barrado Y Navascues, D, Barros, S C C, Baumjohann, W, Beck, M, Beck, T, Benz, W, Billot, N, Bonfils, X, Borsato, L, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Corral Van Damme, C, Csizmadia, S, Davies, M B, Deleuil, M, Deline, A, Delrez, L, Demangeon, O D S, Demory, B O, Erikson, A, Fortier, A, Fossati, L, Gandolfi, D, Gillon, M, Güdel, M, Heng, K, Isaak, K G, Kiss, L L, Laskar, J, Lecavelier Des Etangs, A, Magrin, D, Munari, M, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Rieder, M, Santos, N C, Ségransan, D, Smith, A M S, Steinberger, M, Steller, M, Szabó, G M, Thomas, N, Udry, S, Walton, N A & Wolter, D 2023, ' Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO ', Astronomy and Astrophysics, vol. 670, A24 . https://doi.org/10.1051/0004-6361/202244223
Publication Year :
2023
Publisher :
EDP Sciences, 2023.

Abstract

Context. Stellar granulation generates fluctuations in photometric and spectroscopic data whose properties depend on the stellar type, composition, and evolutionary state. Characterizing granulation is key for understanding stellar atmospheres and detecting planets. Aims. We aim to detect the signatures of stellar granulation, link spectroscopic and photometric signatures of convection for mainsequence stars, and test predictions from 3D hydrodynamic models. Methods. For the first time, we observed two bright stars (Teff = 5833 and 6205 K) with high-precision observations taken simultaneously with CHEOPS and ESPRESSO. We analyzed the properties of the stellar granulation signal in each individual dataset. We compared them to Kepler observations and 3D hydrodynamic models. While isolating the granulation-induced changes by attenuating and filtering the p-mode oscillation signals, we studied the relationship between photometric and spectroscopic observables. Results. The signature of stellar granulation is detected and precisely characterized for the hotter F star in the CHEOPS and ESPRESSO observations. For the cooler G star, we obtain a clear detection in the CHEOPS dataset only. The TESS observations are blind to this stellar signal. Based on CHEOPS observations, we show that the inferred properties of stellar granulation are in agreement with both Kepler observations and hydrodynamic models. Comparing their periodograms, we observe a strong link between spectroscopic and photometric observables. Correlations of this stellar signal in the time domain (flux versus radial velocities, RV) and with specific spectroscopic observables (shape of the cross-correlation functions) are however difficult to isolate due to S/N dependent variations. Conclusions. In the context of the upcoming PLATO mission and the extreme precision RV surveys, a thorough understanding of the properties of the stellar granulation signal is needed. The CHEOPS and ESPRESSO observations pave the way for detailed analyses of this stellar process.<br />Astronomy & Astrophysics, 670<br />ISSN:0004-6361<br />ISSN:1432-0746

Details

Language :
English
ISSN :
00046361 and 14320746
Database :
OpenAIRE
Journal :
Astronomy & Astrophysics, 670, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2023, 670, ⟨10.1051/0004-6361/202244223⟩, Sulis, S, Lendl, M, Cegla, H M, Rodríguez Díaz, L F, Bigot, L, Van Grootel, V, Bekkelien, A, Cameron, A C, Maxted, P F L, Simon, A E, Lovis, C, Scandariato, G, Bruno, G, Nardiello, D, Bonfanti, A, Fridlund, M, Persson, C M, Salmon, S, Sousa, S G, Wilson, T G, Krenn, A, Hoyer, S, Santerne, A, Ehrenreich, D, Alibert, Y, Alonso, R, Anglada, G, Bárczy, T, Barrado Y Navascues, D, Barros, S C C, Baumjohann, W, Beck, M, Beck, T, Benz, W, Billot, N, Bonfils, X, Borsato, L, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Corral Van Damme, C, Csizmadia, S, Davies, M B, Deleuil, M, Deline, A, Delrez, L, Demangeon, O D S, Demory, B O, Erikson, A, Fortier, A, Fossati, L, Gandolfi, D, Gillon, M, Güdel, M, Heng, K, Isaak, K G, Kiss, L L, Laskar, J, Lecavelier Des Etangs, A, Magrin, D, Munari, M, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Rieder, M, Santos, N C, Ségransan, D, Smith, A M S, Steinberger, M, Steller, M, Szabó, G M, Thomas, N, Udry, S, Walton, N A & Wolter, D 2023, ' Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO ', Astronomy and Astrophysics, vol. 670, A24 . https://doi.org/10.1051/0004-6361/202244223
Accession number :
edsair.doi.dedup.....fa06384592b4140ef9abb698917ea0e6
Full Text :
https://doi.org/10.1051/0004-6361/202244223⟩