Detecting Exoplanets Closer to Stars with Moderate Spectral Resolution Integral-field Spectroscopy
While radial velocity surveys have demonstrated that the population of gas giants peaks around 3 au, the most recent high-contrast imaging surveys have only been sensitive to planets beyond ∼10 au. Sensitivity at small angular separations from stars is currently limited by the variability of the poi...
Main Authors: | Shubh Agrawal, Jean-Baptiste Ruffio, Quinn M. Konopacky, Bruce Macintosh, Dimitri Mawet, Eric L. Nielsen, Kielan K. W. Hoch, Michael C. Liu, Travis S. Barman, William Thompson, Alexandra Z. Greenbaum, Christian Marois, Jenny Patience |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astronomical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-3881/acd6a3 |
Similar Items
-
Assessing the C/O Ratio Formation Diagnostic: A Potential Trend with Companion Mass
by: Kielan K. W. Hoch, et al.
Published: (2023-01-01) -
Deep Orbital Search for Additional Planets in the HR 8799 System
by: William Thompson, et al.
Published: (2022-01-01) -
Statistical and Radio Analysis of Exoplanets and Their Host Stars
by: Baoda Li, et al.
Published: (2023-11-01) -
Correlation between exoplanet and star metallicity
by: Laith M. Karim
Published: (2011-12-01) -
Variability of Known Exoplanet Host Stars Observed by TESS
by: Emilie R. Simpson, et al.
Published: (2023-01-01)