Electro-optic frequency combs
Frequency combs are optical spectra composed of a set of discrete equally spaced lines.
Such spectra can be generated by diverse sources such as mode-locked lasers, resonators …
Such spectra can be generated by diverse sources such as mode-locked lasers, resonators …
The occurrence and architecture of exoplanetary systems
JN Winn, DC Fabrycky - Annual Review of Astronomy and …, 2015 - annualreviews.org
The basic geometry of the Solar System—the shapes, spacings, and orientations of the
planetary orbits—has long been a subject of fascination as well as inspiration for planet …
planetary orbits—has long been a subject of fascination as well as inspiration for planet …
[HTML][HTML] Gaia Data Release 3-Stellar multiplicity, a teaser for the hidden treasure
F Arenou, C Babusiaux, MA Barstow, S Faigler… - Astronomy & …, 2023 - aanda.org
Context. The Gaia DR3 catalogue contains, for the first time, about 800 000 solutions with
either orbital elements or trend parameters for astrometric, spectroscopic, and eclipsing …
either orbital elements or trend parameters for astrometric, spectroscopic, and eclipsing …
California legacy survey. II. Occurrence of giant planets beyond the ice line
BJ Fulton, LJ Rosenthal, LA Hirsch… - The Astrophysical …, 2021 - iopscience.iop.org
We used high-precision radial velocity measurements of FGKM stars to determine the
occurrence of giant planets as a function of orbital separation spanning 0.03–30 au. Giant …
occurrence of giant planets as a function of orbital separation spanning 0.03–30 au. Giant …
The Gemini Planet Imager Exoplanet Survey: giant planet and brown dwarf demographics from 10 to 100 au
EL Nielsen, RJ De Rosa, B Macintosh… - The Astronomical …, 2019 - iopscience.iop.org
We present a statistical analysis of the first 300 stars observed by the Gemini Planet Imager
Exoplanet Survey. This subsample includes six detected planets and three brown dwarfs; …
Exoplanet Survey. This subsample includes six detected planets and three brown dwarfs; …
A terrestrial planet candidate in a temperate orbit around Proxima Centauri
G Anglada-Escudé, PJ Amado, J Barnes, ZM Berdiñas… - nature, 2016 - nature.com
At a distance of 1.295 parsecs, the red dwarf Proxima Centauri (α Centauri C, GL 551, HIP
70890 or simply Proxima) is the Sun's closest stellar neighbour and one of the best-studied …
70890 or simply Proxima) is the Sun's closest stellar neighbour and one of the best-studied …
[HTML][HTML] The CARMENES search for exoplanets around M dwarfs-Planet occurrence rates from a subsample of 71 stars
Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000
spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time …
spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time …
ALMA survey of lupus protoplanetary disks. I. Dust and gas masses
We present the first high-resolution sub-millimeter survey of both dust and gas for a large
population of protoplanetary disks. Characterizing fundamental properties of protoplanetary …
population of protoplanetary disks. Characterizing fundamental properties of protoplanetary …
The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity
CD Dressing, D Charbonneau - The Astrophysical Journal, 2015 - iopscience.iop.org
We present an improved estimate of the occurrence rate of small planets orbiting small stars
by searching the full four-year Kepler data set for transiting planets using our own planet …
by searching the full four-year Kepler data set for transiting planets using our own planet …
A revised exoplanet yield from the transiting exoplanet survey satellite (TESS)
Abstract The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small
planets orbiting stars bright enough for mass determination via ground-based radial velocity …
planets orbiting stars bright enough for mass determination via ground-based radial velocity …