Roland Ottensamer
University of Vienna
137 Papers
550 Citations
Roland Ottensamer is an academic researcher from University of Vienna. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 19, co-authored 81 publications. Previous affiliations of Roland Ottensamer include Graz University of Technology.
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Papers
•Posted Content
The changing face of AU Mic b: stellar spots, spin-orbit commensurability, and Transit Timing Variations as seen by CHEOPS and TESS
Gy. M. Szabó,Davide Gandolfi,Alexis Brandeker,Sz. Csizmadia,Z. Garai,Nicolas Billot,C. Broeg,David Ehrenreich,Andrea Fortier,Luca Fossati,Sergio Hoyer,László L. Kiss,A. Lecavelier des Etangs,Pierre F. L. Maxted,Ignasi Ribas,Yann Alibert,Roi Alonso,G. Anglada Escudé,T. Bárczy,S. C. C. Barros,David Barrado,Wolfgang Baumjohann,M. Beck,Thomas Beck,A. Bekkelien,X. Bonfils,Willy Benz,L. Borsato,M.-D. Busch,J. Cabrera,S. Charnoz,A. Collier Cameron,C. Corral Van Damme,Melvyn B. Davies,L. Delrez,M. Deleuil,O. D. S. Demangeon,B. O. Demory,Anders Erikson,M. Fridlund,D. Futyan,A. García Muñoz,M. Gillon,Manuel Guedel,P. Guterman,Kevin Heng,K. G. Isaak,G. Lacedelli,Jacques Laskar,M. Lend,C. Lovis,A. Luntzer,Demetrio Magrin,V. Nascimbeni,G. Olofsson,Hugh P. Osborn,Roland Ottensamer,I. Pagano,Enric Palle,Gisbert Peter,Daniele Piazza,G. Piotto,D. L. Pollacco,Didier Queloz,Roberto Ragazzoni,Nicola Rando,Heike Rauer,N. C. Santos,G. Scandariato,D. Segransan,L. M. Serrano,D. Sicilia,A. E. Simon,A. M. Smith,S. G. Sousa,M. Steller,N. Thomas,Stéphane Udry,Valérie Van Grootel,N. A. Walton,T. G. Wilson +80 more
TL;DR: In this article, the authors analyzed three transits of AU Mic b observed with the CHaracterising ExOPlanet Satellite (CHEOPS), supplemented with sector 1 and 27 Transiting Exoplanet Survey Satellite (TESS) photometry, and the All-Sky Automated Survey (ASAS) from the ground.
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The tidal deformation and atmosphere of WASP-12\,b from its phase curve
B. Akinsanmi,S. C. C. Barros,Monika Lendl,L. Carone,P. E. Cubillos,A. Bekkelien,Andrea Fortier,H. G. Floren,A. Collier Cameron,G. Boué,G. Bruno,Brice-Olivier Demory,Alexis Brandeker,S. Sousa,T. G. Wilson,A. Deline,A. Bonfanti,Gaetano Scandariato,Matthew J. Hooton,A. Correia,Olivier Demangeon,A.M.S. Smith,Vikash Singh,Y. Alibert,R Alonso,J. Asquier,T. Bárczy,D. Barrado Navascues,W. Baumjohann,M. Beck,Thomas Boeck,W. Benz,N. Billot,Xavier Bonfils,Luca Borsato,C. Broeg,Maximilian Buder,Sebatien Charnoz,Sz. Csizmadia,M. B. Davies,Magali Deleuil,Laetitia Delrez,David Ehrenreich,Alex Erikson,J. Farinato,Luciano Fossati,M. Fridlund,D. Gandolfi,M. Gillon,M. Güdel,M. N. Günther,A. Heitzmann,Ch. Helling,Sergio Hoyer,Kate Gudrun Isaak,L. Kiss,K. W. F. Lam,J. Laskar,A. Lecavelier des Etangs,D. Magrin,P. Maxted,M. Mecina,Christoph Mordasini,Valerio Nascimbeni,G. Olofsson,Roland Ottensamer,Isabella Pagano,Elfriede Palle,Gao Peter,D. Piazza,G. Piotto,D. Pollacco,D. Queloz,Roberto Ragazzoni,Nicola Rando,Heike Rauer,I. Ribas,N. C. Santos,Damien Ségransan,A. E. Simon,M. Stalport,M. G. Szabó,Nicolas Thomas,S. Udry,Valérie Van Grootel,J. Venturini,E. Villaver,N. A. Walton +87 more
- 16 Feb 2024
TL;DR: The tidal deformation and atmosphere of WASP-12b from its phase curve measures the planet's tidal deformation, atmospheric properties, and orbital decay rate. The Love number is measured to be 0.012 ± 0.004, which provides insight into the planet's interior structure. The atmospheric properties are measured to be similar to those of the dayside atmosphere of the planet at a temperature of 2900 K.
The instrument control unit of the ARIEL payload: design evolution following the unit and payload subsystems SRR (system requirements review)
Vladimiro Noce,Mauro Focardi,A. M. di Giorgio,Emanuele Galli,M. Farina,G. Giusi,M. Vela Nuñez,Luca Naponiello,Andrea Lorenzani,Luca Serafini,C. Del Vecchio Blanco,Marco Verna,Cristophe Cara,Michel Berthé,J. Martignac,Roland Ottensamer,Giuseppina Micela,Giuseppe Malaguti,Emanuele Pace,Giampaolo Preti,Federico Antonio Gutiérrez Miceli,Enzo Pascale,Giovanna Tinetti,Paul Eccleston,E. Tommasi,F. De Persio,Pietro Bolli,Renzo Nesti,M. Iuzzolino,Luca Carbonaro,Ciro Del Vecchio,D. Ferruzzi,Anna Brucalassi,G. Falcini,Angelo Tozzi,Daniele Gottini +35 more
- 27 Aug 2022
TL;DR: ARIEL (Atmospheric remote-sensing InfraRed Large-survey) is a medium-class mission of the European Space Agency, part of the Cosmic Vision program, whose launch is foreseen by early 2029 as mentioned in this paper .
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