Imaging low-mass planets within the habitable zone of α Centauri
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars.
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Nature Publishing Group
2021-02-01
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| Series: | Nature Communications |
| Online Access: | https://doi.org/10.1038/s41467-021-21176-6 |
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doaj-34b7ac7a6b0c49a6be4c1b54f64995932021-02-14T12:12:06ZengNature Publishing GroupNature Communications2041-17232021-02-011211710.1038/s41467-021-21176-6Imaging low-mass planets within the habitable zone of α CentauriK. Wagner0A. Boehle1P. Pathak2M. Kasper3R. Arsenault4G. Jakob5U. Käufl6S. Leveratto7A.-L. Maire8E. Pantin9R. Siebenmorgen10G. Zins11O. Absil12N. Ageorges13D. Apai14A. Carlotti15É. Choquet16C. Delacroix17K. Dohlen18P. Duhoux19P. Forsberg20E. Fuenteseca21S. Gutruf22O. Guyon23E. Huby24D. Kampf25M. Karlsson26P. Kervella27J.-P. Kirchbauer28P. Klupar29J. Kolb30D. Mawet31M. N’Diaye32G. Orban de Xivry33S. P. Quanz34A. Reutlinger35G. Ruane36M. Riquelme37C. Soenke38M. Sterzik39A. Vigan40T. de Zeeuw41Dept. of Astronomy and Steward Observatory, University of ArizonaInstitute for Particle Physics and Astrophysics, ETH ZurichEuropean Southern ObservatoryEuropean Southern ObservatoryEuropean Southern ObservatoryEuropean Southern ObservatoryEuropean Southern ObservatoryEuropean Southern ObservatorySTAR Institute, Université de LiègeAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéEuropean Southern ObservatoryEuropean Southern ObservatorySTAR Institute, Université de LiègeKampf Telescope OpticsDept. of Astronomy and Steward Observatory, University of ArizonaUniv. Grenoble Alpes, CNRS, IPAGAix Marseille Univ, CNRS, CNES, LAMSTAR Institute, Université de LiègeAix Marseille Univ, CNRS, CNES, LAMEuropean Southern ObservatoryDepartment of Materials Science and Engineering, Ångström Laboratory, Uppsala UniversityEuropean Southern ObservatoryKampf Telescope OpticsDept. of Astronomy and Steward Observatory, University of ArizonaLESIA, Observatoire de ParisKampf Telescope OpticsDepartment of Materials Science and Engineering, Ångström Laboratory, Uppsala UniversityLESIA, Observatoire de ParisEuropean Southern ObservatoryThe Breakthrough Initiatives, NASA Research ParkEuropean Southern ObservatoryCalifornia Institute of TechnologyUniversité Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire LagrangeSTAR Institute, Université de LiègeInstitute for Particle Physics and Astrophysics, ETH ZurichKampf Telescope OpticsCalifornia Institute of TechnologyEuropean Southern ObservatoryEuropean Southern ObservatoryEuropean Southern ObservatoryAix Marseille Univ, CNRS, CNES, LAMEuropean Southern ObservatoryImaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars.https://doi.org/10.1038/s41467-021-21176-6 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw |
| spellingShingle |
K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw Imaging low-mass planets within the habitable zone of α Centauri Nature Communications |
| author_facet |
K. Wagner A. Boehle P. Pathak M. Kasper R. Arsenault G. Jakob U. Käufl S. Leveratto A.-L. Maire E. Pantin R. Siebenmorgen G. Zins O. Absil N. Ageorges D. Apai A. Carlotti É. Choquet C. Delacroix K. Dohlen P. Duhoux P. Forsberg E. Fuenteseca S. Gutruf O. Guyon E. Huby D. Kampf M. Karlsson P. Kervella J.-P. Kirchbauer P. Klupar J. Kolb D. Mawet M. N’Diaye G. Orban de Xivry S. P. Quanz A. Reutlinger G. Ruane M. Riquelme C. Soenke M. Sterzik A. Vigan T. de Zeeuw |
| author_sort |
K. Wagner |
| title |
Imaging low-mass planets within the habitable zone of α Centauri |
| title_short |
Imaging low-mass planets within the habitable zone of α Centauri |
| title_full |
Imaging low-mass planets within the habitable zone of α Centauri |
| title_fullStr |
Imaging low-mass planets within the habitable zone of α Centauri |
| title_full_unstemmed |
Imaging low-mass planets within the habitable zone of α Centauri |
| title_sort |
imaging low-mass planets within the habitable zone of α centauri |
| publisher |
Nature Publishing Group |
| series |
Nature Communications |
| issn |
2041-1723 |
| publishDate |
2021-02-01 |
| description |
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around nearby stars. |
| url |
https://doi.org/10.1038/s41467-021-21176-6 |
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