Large Interferometer for Exoplanets: VIII. Where Is the Phosphine? Observing Exoplanetary PH<sub>3</sub> with a Space-Based Mid-Infrared Nulling Interferometer-Reference-Cited by-同舟云学术

Large Interferometer for Exoplanets: VIII. Where Is the Phosphine? Observing Exoplanetary PH₃ with a Space-Based Mid-Infrared Nulling Interferometer

Published:2023-02-01 Issue:2 Volume:23 Page:183-194
ISSN:1531-1074
Container-title:Astrobiology
language:en
Short-container-title:Astrobiology

Author:

Angerhausen Daniel¹²³^ORCID,Ottiger Maurice¹,Dannert Felix¹,Miguel Yamila⁴⁵,Sousa-Silva Clara⁶⁷^ORCID,Kammerer Jens⁸,Menti Franziska¹,Alei Eleonora¹²,Konrad Björn S.¹²,Wang Haiyang S.¹²,Quanz Sascha P.¹²,

Affiliation:

1. Department of Physics, Institute for Particle Physics and Astrophysics, ETH Zurich, Zurich, Switzerland.

2. National Center of Competence in Research PlanetS, Bern, Switzerland.

3. Blue Marble Space Institute of Science, Seattle, Washington, USA.

4. SRON Netherlands Institute for Space Research, Utrecht, The Netherlands.

5. Leiden Observatory, University of Leiden, Leiden, The Netherlands.

6. Center for Astrophysics, Harvard-Smithsonian, Cambridge, Massachusetts, USA.

7. Division of Science, Mathematics, and Computing, Bard College, Annandale-on-Hudson, New York, USA.

8. Space Telescope Science Institute, Baltimore, Maryland, USA.

Publisher

Mary Ann Liebert Inc

Subject

Space and Planetary Science,Agricultural and Biological Sciences (miscellaneous)

Link

https://www.liebertpub.com/doi/pdf/10.1089/ast.2022.0010

Reference48 articles.

1. Complications in the ALMA Detection of Phosphine at Venus

2. Large Interferometer For Exoplanets (LIFE)

3. The Chemical Composition of the Sun

4. Phosphine on Venus Cannot Be Explained by Conventional Processes

5. New technique to measure the cavity defects of Fabry–Perot interferometers

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