Searches for continuous-wave gravitational radiation
K Riles - Living Reviews in Relativity, 2023 - Springer
Now that detection of gravitational-wave signals from the coalescence of extra-galactic
compact binary star mergers has become nearly routine, it is intriguing to consider other …
compact binary star mergers has become nearly routine, it is intriguing to consider other …
Exoplanetary atmospheres: key insights, challenges, and prospects
N Madhusudhan - Annual Review of Astronomy and …, 2019 - annualreviews.org
Exoplanetary science is on the verge of an unprecedented revolution. The thousands of
exoplanets discovered over the past decade have most recently been supplemented by …
exoplanets discovered over the past decade have most recently been supplemented by …
Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
B Macintosh, JR Graham, T Barman, RJ De Rosa… - Science, 2015 - science.org
Directly detecting thermal emission from young extrasolar planets allows measurement of
their atmospheric compositions and luminosities, which are influenced by their formation …
their atmospheric compositions and luminosities, which are influenced by their formation …
Imaging extrasolar giant planets
BP Bowler - Publications of the Astronomical Society of the …, 2016 - iopscience.iop.org
High-contrast adaptive optics (AO) imaging is a powerful technique to probe the
architectures of planetary systems from the outside-in and survey the atmospheres of self …
architectures of planetary systems from the outside-in and survey the atmospheres of self …
First light of the gemini planet imager
B Macintosh, JR Graham, P Ingraham… - proceedings of the …, 2014 - National Acad Sciences
The Gemini Planet Imager is a dedicated facility for directly imaging and spectroscopically
characterizing extrasolar planets. It combines a very high-order adaptive optics system, a …
characterizing extrasolar planets. It combines a very high-order adaptive optics system, a …
Efficient, uninformative sampling of limb darkening coefficients for two-parameter laws
DM Kipping - Monthly Notices of the Royal Astronomical Society, 2013 - academic.oup.com
Stellar limb darkening affects a wide range of astronomical measurements and is frequently
modelled with a parametric model using polynomials in the cosine of the angle between the …
modelled with a parametric model using polynomials in the cosine of the angle between the …
Rapid growth of gas-giant cores by pebble accretion
M Lambrechts, A Johansen - Astronomy & Astrophysics, 2012 - aanda.org
The observed lifetimes of gaseous protoplanetary discs place strong constraints on gas and
ice giant formation in the core accretion scenario. The approximately 10-Earth-mass solid …
ice giant formation in the core accretion scenario. The approximately 10-Earth-mass solid …
Detection and characterization of exoplanets and disks using projections on Karhunen–Loève eigenimages
We describe a new method to achieve point-spread function (PSF) subtractions for high-
contrast imaging using principal component analysis that is applicable to both point sources …
contrast imaging using principal component analysis that is applicable to both point sources …
Stellar multiplicity
Stellar multiplicity is a ubiquitous outcome of the star-formation process. The frequency and
main characteristics of multiple systems, and their dependence on primary mass and …
main characteristics of multiple systems, and their dependence on primary mass and …
Planet-disk interaction and orbital evolution
W Kley, RP Nelson - Annual Review of Astronomy and …, 2012 - annualreviews.org
As planets form and grow within gaseous protoplanetary disks, the mutual gravitational
interaction between the disk and planet leads to the exchange of angular momentum and …
interaction between the disk and planet leads to the exchange of angular momentum and …