D
Daniel Angerhausen
Researcher at University of Bern
Publications - 91
Citations - 2827
Daniel Angerhausen is an academic researcher from University of Bern. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 25, co-authored 84 publications receiving 2380 citations. Previous affiliations of Daniel Angerhausen include University of Stuttgart & Max Planck Society.
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WATER, METHANE, AND CARBON DIOXIDE PRESENT IN THE DAYSIDE SPECTRUM OF THE EXOPLANET HD 209458b
Mark R. Swain,Giovanna Tinetti,Gautam Vasisht,Pieter Deroo,Caitlin A. Griffith,Jeroen Bouwman,Pin Chen,Yuk L. Yung,Adam Burrows,Linda R. Brown,Jaymie M. Matthews,Jason F. Rowe,Rainer Kuschnig,Daniel Angerhausen +13 more
TL;DR: In this paper, the dayside spectrum of HD 209458b between 1.5 and 2.5 μm was measured using the NICMOS instrument on the Hubble Space Telescope.
Journal ArticleDOI
Water, Methane, and Carbon Dioxide Present in the Dayside Spectrum of the Exoplanet HD 209458b
Mark G. Swain,Giovanna Tinetti,G. Vasisht,Pieter Deroo,Caitlin A. Griffith,Jeroen Bouwman,Pin Chen,Yuk L. Yung,Adam Burrows,Linda R. Brown,Jaymie M. Matthews,J. F. Roe,Rainer Kuschnig,Daniel Angerhausen +13 more
TL;DR: In this paper, the dayside spectrum of HD 209458b between 1.5 and 2.5 microns was measured using the NICMOS instrument on the Hubble Space Telescope.
Journal ArticleDOI
A ground-based near-infrared emission spectrum of the exoplanet HD 189733b
Mark R. Swain,Pieter Deroo,Caitlin A. Griffith,Giovanna Tinetti,Azam Mihir Thatte,Gautam Vasisht,Pin Chen,Jeroen Bouwman,Ian J. M. Crossfield,Daniel Angerhausen,Cristina Afonso,Thomas Henning +11 more
TL;DR: Ground-based observations of the dayside emission spectrum for HD’s 189733b suggest that non-LTE effects may need to be considered when interpreting measurements of strongly irradiated exoplanets.
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Characterizing Transiting Planet Atmospheres through 2025
Nicolas B. Cowan,Thomas P. Greene,Daniel Angerhausen,Natasha E. Batalha,Mark Clampin,Knicole D. Colón,Ian J. M. Crossfield,J. J. Fortney,B. S. Gaudi,Joseph Harrington,Nicolas Iro,Charles F. Lillie,Jeffrey L. Linsky,Mercedes Lopez-Morales,Avi Mandell,Kevin B. Stevenson +15 more
TL;DR: The Transiting Exoplanet Survey Satellite (TESS) as discussed by the authors will discover transiting planets orbiting the brightest stars, enabling, in principle, an atmospheric survey of 102-103 bright hot Jupiters and warm sub-Neptunes.
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A Comprehensive Study of Kepler Phase Curves and Secondary Eclipses: Temperatures and Albedos of Confirmed Kepler Giant Planets
TL;DR: In this article, a comprehensive study of phase curves and secondary eclipses in the Kepler data set using all data from 16 quarters that were available in 2013-2014 was presented, consisting of 20 confirmed planets with Rp > 4 Re, P 0.1.