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Harvard
Desidera, S, Chauvin, G, Bonavita, M, Messina, S, Lecoroller, H, Schmidt, T, Gratton, R, Lazzoni, C, Meyer, M, Schlieder, J, Cheetham, A, Hagelberg, J, Bonnefoy, M, Feldt, M, Lagrange, AM, Langlois, M, Vigan, A, Tan, TG, Hambsch, FJ, Millward, M, Alcalá, J, Benatti, S, Brandner, W, Carson, J, Covino, E, Delorme, P, D'Orazi, V, Janson, M, Rigliaco, E, Beuzit, JL, Biller, B, Boccaletti, A, Dominik, C, Cantalloube, F, Fontanive, C, Galicher, R, Henning, T, Lagadec, E, Ligi, R, Maire, AL, Menard, F, Mesa, D, Müller, A, Samland, M, Schmid, HM, Sissa, E, Turatto, M, Udry, S, Zurlo, A, Asensio-Torres, R
, Kopytova, T, Rickman, E, Abe, L, Antichi, J, Baruffolo, A, Baudoz, P, Baudrand, J, Blanchard, P, Bazzon, A, Buey, T, Carbillet, M, Carle, M, Charton, J, Cascone, E, Claudi, R, Costille, A, Deboulbé, A, De Caprio, V, Dohlen, K, Fantinel, D, Feautrier, P, Fusco, T, Gigan, P, Giro, E, Gisler, D, Gluck, L, Hubin, N, Hugot, E, Jaquet, M, Kasper, M, Madec, F, Magnard, Y, Martinez, P, Maurel, D, Le Mignant, D, Möller-Nilsson, O, Llored, M, Moulin, T, Origné, A, Pavlov, A, Perret, D, Petit, C, Pragt, J, Puget, P, Rabou, P, Ramos, J, Rigal, F, Rochat, S, Roelfsema, R, Rousset, G, Roux, A, Salasnich, B, Sauvage, JF, Sevin, A, Soenke, C, Stadler, E, Suarez, M, Weber, L & Wildi, F 2021, '
The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization',
Astronomy and Astrophysics, Том. 651, 70.
https://doi.org/10.1051/0004-6361/202038806APA
Desidera, S., Chauvin, G., Bonavita, M., Messina, S., Lecoroller, H., Schmidt, T., Gratton, R., Lazzoni, C., Meyer, M., Schlieder, J., Cheetham, A., Hagelberg, J., Bonnefoy, M., Feldt, M., Lagrange, A. M., Langlois, M., Vigan, A., Tan, T. G., Hambsch, F. J., ... Wildi, F. (2021).
The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization.
Astronomy and Astrophysics,
651, [70].
https://doi.org/10.1051/0004-6361/202038806Vancouver
Author
BibTeX
@article{5a5e29b65763450e8d81d6147ea23e60,
title = "The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization",
keywords = "Planets and satellites: general, Stars: activity, Stars: fundamental parameters, Stars: kinematics and dynamics, Stars: pre-main sequence, Stars: rotation, 51 ERIDANI B, TIME-SERIES ANALYSIS, LOW-MASS STARS, YOUNG MOVING GROUPS, PRE-MAIN-SEQUENCE, STELLAR KINEMATIC GROUPS, stars: pre-main sequence, BROWN DWARF COMPANION, planets and satellites: general, stars: fundamental parameters, stars: kinematics and dynamics, PLANET-FINDING CAMPAIGN, stars: activity, stars: rotation, BETA-PICTORIS B, DEBRIS DISK",
author = "S. Desidera and G. Chauvin and M. Bonavita and S. Messina and H. Lecoroller and T. Schmidt and R. Gratton and C. Lazzoni and M. Meyer and J. Schlieder and A. Cheetham and J. Hagelberg and M. Bonnefoy and M. Feldt and Lagrange, {A. M.} and M. Langlois and A. Vigan and Tan, {T. G.} and Hambsch, {F. J.} and M. Millward and J. Alcal{\'a} and S. Benatti and W. Brandner and J. Carson and E. Covino and P. Delorme and V. D'Orazi and M. Janson and E. Rigliaco and Beuzit, {J. L.} and B. Biller and A. Boccaletti and C. Dominik and F. Cantalloube and C. Fontanive and R. Galicher and Th Henning and E. Lagadec and R. Ligi and Maire, {A. L.} and F. Menard and D. Mesa and A. M{\"u}ller and M. Samland and Schmid, {H. M.} and E. Sissa and M. Turatto and S. Udry and A. Zurlo and R. Asensio-Torres and T. Kopytova and E. Rickman and L. Abe and J. Antichi and A. Baruffolo and P. Baudoz and J. Baudrand and P. Blanchard and A. Bazzon and T. Buey and M. Carbillet and M. Carle and J. Charton and E. Cascone and R. Claudi and A. Costille and A. Deboulb{\'e} and {De Caprio}, V. and K. Dohlen and D. Fantinel and P. Feautrier and T. Fusco and P. Gigan and E. Giro and D. Gisler and L. Gluck and N. Hubin and E. Hugot and M. Jaquet and M. Kasper and F. Madec and Y. Magnard and P. Martinez and D. Maurel and {Le Mignant}, D. and O. M{\"o}ller-Nilsson and M. Llored and T. Moulin and A. Orign{\'e} and A. Pavlov and D. Perret and C. Petit and J. Pragt and P. Puget and P. Rabou and J. Ramos and F. Rigal and S. Rochat and R. Roelfsema and G. Rousset and A. Roux and B. Salasnich and Sauvage, {J. F.} and A. Sevin and C. Soenke and E. Stadler and M. Suarez and L. Weber and F. Wildi",
note = "Funding Information: sortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF – Osservatorio di Padova (Italy), Observatoire de Gen{\`e}ve (Switzerland), ETH Z{\"u}rich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Frame-work Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 Funding Information: (2004–2008), grant number 226 604 for FP7 (2009–2012) and grant number 312430 for FP7 (2013–2016). This research has made use of the SIMBAD database and Vizier services, operated at CDS, Strasbourg, France and of the Washington Double Star Catalog maintained at the US Naval Observatory. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/ gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. This paper has made use of data products available in ESO archive. Program ID: 60.A-9036(A); 072.C-0488(E) (PI Mayor), 074.C-0364(A) (PI Robichon), 074.C-0037(A) (PI Gunther), 075.C-0202(A) (PI Gunther), 075.C-0689(A) (PI Galland), 076.C-0010(A) (PI Gunther), 077.C-0012(A) (PI Gunther), 077.C-0295(D) (PI Galland), 078.D-0245(C) (PI Dall), 079.C-0046(A) (PI Gunther), 080.D-0151(A) (PI Hatzes), 080.C-0712(A) (PI Desort), 180.C-0886(A) (PI Bonfils), 082.C-0718(B) (PI Bonfils), 082.C-0427(A) (PI Doellinger), 082.C-0390(A) (PI Weise), 183.C-0437(A) (PI Bonfils), 083.C-0794(A) (PI Chauvin), 084.C-1039(A) (PI Chauvin), 184.C-0815(B) (PI Desort), 089.C-0732(A) (PI Lo Curto), 191.C-0873(D) (PI Bonfils), 192.C-0224(A) (PI Lagrange), 097.C-0864(B) (PI Lannier), 098.C-0739(A) (PI Lagrange), 099.C-0205(A) (PI Lagrange), 099.C-0458(A) (PI Lo Curto), 1101.C-0557(A) (PI Lagrange). We have used data from the WASP public archive in this research. The WASP consortium comprises of the University of Cambridge, Keele University, University of Leicester, The Open University, The Queen{\textquoteright}s University Belfast, St. Andrews University and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UK{\textquoteright}s Science and Technology Facilities Council. Based on data retrieved from the SOPHIE archive at Observatoire de Haute-Provence (OHP), available at http://atlas.obs-hp.fr/sophie/. We thank the anonymous referee for useful comments. S.D., V.D., D.M. and R.G. acknowledge the support by INAF/Frontiera through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research, the PRIN-INAF 2019 “Planetary systems at young ages” (PLATEA) and the ASI-INAF agreement n.2018-16-HH.0. AV acknowledges funding from the European Research Council (ERC) under the European Union{\textquoteright}s Horizon 2020 research and innovation programme (grant agreement No. 757561). A.M.L. acknowledges funding from Agence Nationale de la Recherche (France) under contract number ANR-14-CE33-0018. J.C. was supported by SC Space Grant and Fulbright Colombia. M.B. acknowledges funding by the UK Science and Technology Facilities Council (STFC) grant no. ST/M001229/1. Publisher Copyright: {\textcopyright} ESO 2021. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.",
year = "2021",
month = jul,
day = "1",
doi = "10.1051/0004-6361/202038806",
language = "English",
volume = "651",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",
}
RIS
TY - JOUR
T1 - The SPHERE infrared survey for exoplanets (SHINE): I. Sample definition and target characterization
AU - Desidera, S.
AU - Chauvin, G.
AU - Bonavita, M.
AU - Messina, S.
AU - Lecoroller, H.
AU - Schmidt, T.
AU - Gratton, R.
AU - Lazzoni, C.
AU - Meyer, M.
AU - Schlieder, J.
AU - Cheetham, A.
AU - Hagelberg, J.
AU - Bonnefoy, M.
AU - Feldt, M.
AU - Lagrange, A. M.
AU - Langlois, M.
AU - Vigan, A.
AU - Tan, T. G.
AU - Hambsch, F. J.
AU - Millward, M.
AU - Alcalá, J.
AU - Benatti, S.
AU - Brandner, W.
AU - Carson, J.
AU - Covino, E.
AU - Delorme, P.
AU - D'Orazi, V.
AU - Janson, M.
AU - Rigliaco, E.
AU - Beuzit, J. L.
AU - Biller, B.
AU - Boccaletti, A.
AU - Dominik, C.
AU - Cantalloube, F.
AU - Fontanive, C.
AU - Galicher, R.
AU - Henning, Th
AU - Lagadec, E.
AU - Ligi, R.
AU - Maire, A. L.
AU - Menard, F.
AU - Mesa, D.
AU - Müller, A.
AU - Samland, M.
AU - Schmid, H. M.
AU - Sissa, E.
AU - Turatto, M.
AU - Udry, S.
AU - Zurlo, A.
AU - Asensio-Torres, R.
AU - Kopytova, T.
AU - Rickman, E.
AU - Abe, L.
AU - Antichi, J.
AU - Baruffolo, A.
AU - Baudoz, P.
AU - Baudrand, J.
AU - Blanchard, P.
AU - Bazzon, A.
AU - Buey, T.
AU - Carbillet, M.
AU - Carle, M.
AU - Charton, J.
AU - Cascone, E.
AU - Claudi, R.
AU - Costille, A.
AU - Deboulbé, A.
AU - De Caprio, V.
AU - Dohlen, K.
AU - Fantinel, D.
AU - Feautrier, P.
AU - Fusco, T.
AU - Gigan, P.
AU - Giro, E.
AU - Gisler, D.
AU - Gluck, L.
AU - Hubin, N.
AU - Hugot, E.
AU - Jaquet, M.
AU - Kasper, M.
AU - Madec, F.
AU - Magnard, Y.
AU - Martinez, P.
AU - Maurel, D.
AU - Le Mignant, D.
AU - Möller-Nilsson, O.
AU - Llored, M.
AU - Moulin, T.
AU - Origné, A.
AU - Pavlov, A.
AU - Perret, D.
AU - Petit, C.
AU - Pragt, J.
AU - Puget, P.
AU - Rabou, P.
AU - Ramos, J.
AU - Rigal, F.
AU - Rochat, S.
AU - Roelfsema, R.
AU - Rousset, G.
AU - Roux, A.
AU - Salasnich, B.
AU - Sauvage, J. F.
AU - Sevin, A.
AU - Soenke, C.
AU - Stadler, E.
AU - Suarez, M.
AU - Weber, L.
AU - Wildi, F.
N1 - Funding Information:
sortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF – Osservatorio di Padova (Italy), Observatoire de Genève (Switzerland), ETH Zürich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Frame-work Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6
Funding Information:
(2004–2008), grant number 226 604 for FP7 (2009–2012) and grant number 312430 for FP7 (2013–2016). This research has made use of the SIMBAD database and Vizier services, operated at CDS, Strasbourg, France and of the Washington Double Star Catalog maintained at the US Naval Observatory. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/ gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. This paper has made use of data products available in ESO archive. Program ID: 60.A-9036(A); 072.C-0488(E) (PI Mayor), 074.C-0364(A) (PI Robichon), 074.C-0037(A) (PI Gunther), 075.C-0202(A) (PI Gunther), 075.C-0689(A) (PI Galland), 076.C-0010(A) (PI Gunther), 077.C-0012(A) (PI Gunther), 077.C-0295(D) (PI Galland), 078.D-0245(C) (PI Dall), 079.C-0046(A) (PI Gunther), 080.D-0151(A) (PI Hatzes), 080.C-0712(A) (PI Desort), 180.C-0886(A) (PI Bonfils), 082.C-0718(B) (PI Bonfils), 082.C-0427(A) (PI Doellinger), 082.C-0390(A) (PI Weise), 183.C-0437(A) (PI Bonfils), 083.C-0794(A) (PI Chauvin), 084.C-1039(A) (PI Chauvin), 184.C-0815(B) (PI Desort), 089.C-0732(A) (PI Lo Curto), 191.C-0873(D) (PI Bonfils), 192.C-0224(A) (PI Lagrange), 097.C-0864(B) (PI Lannier), 098.C-0739(A) (PI Lagrange), 099.C-0205(A) (PI Lagrange), 099.C-0458(A) (PI Lo Curto), 1101.C-0557(A) (PI Lagrange). We have used data from the WASP public archive in this research. The WASP consortium comprises of the University of Cambridge, Keele University, University of Leicester, The Open University, The Queen’s University Belfast, St. Andrews University and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UK’s Science and Technology Facilities Council. Based on data retrieved from the SOPHIE archive at Observatoire de Haute-Provence (OHP), available at http://atlas.obs-hp.fr/sophie/. We thank the anonymous referee for useful comments. S.D., V.D., D.M. and R.G. acknowledge the support by INAF/Frontiera through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research, the PRIN-INAF 2019 “Planetary systems at young ages” (PLATEA) and the ASI-INAF agreement n.2018-16-HH.0. AV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 757561). A.M.L. acknowledges funding from Agence Nationale de la Recherche (France) under contract number ANR-14-CE33-0018. J.C. was supported by SC Space Grant and Fulbright Colombia. M.B. acknowledges funding by the UK Science and Technology Facilities Council (STFC) grant no. ST/M001229/1.
Publisher Copyright:
© ESO 2021.
Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.
PY - 2021/7/1
Y1 - 2021/7/1
KW - Planets and satellites: general
KW - Stars: activity
KW - Stars: fundamental parameters
KW - Stars: kinematics and dynamics
KW - Stars: pre-main sequence
KW - Stars: rotation
KW - 51 ERIDANI B
KW - TIME-SERIES ANALYSIS
KW - LOW-MASS STARS
KW - YOUNG MOVING GROUPS
KW - PRE-MAIN-SEQUENCE
KW - STELLAR KINEMATIC GROUPS
KW - stars: pre-main sequence
KW - BROWN DWARF COMPANION
KW - planets and satellites: general
KW - stars: fundamental parameters
KW - stars: kinematics and dynamics
KW - PLANET-FINDING CAMPAIGN
KW - stars: activity
KW - stars: rotation
KW - BETA-PICTORIS B
KW - DEBRIS DISK
UR - http://www.scopus.com/inward/record.url?scp=85110441170&partnerID=8YFLogxK
UR - https://elibrary.ru/item.asp?id=46910314
U2 - 10.1051/0004-6361/202038806
DO - 10.1051/0004-6361/202038806
M3 - Article
AN - SCOPUS:85110441170
VL - 651
JO - Astronomy and Astrophysics
JF - Astronomy and Astrophysics
SN - 0004-6361
M1 - 70
ER -
