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The initial mass function based on the full-sky 20 pc census of∼ 3600 stars and brown Dwarfs
JD Kirkpatrick, F Marocco, CR Gelino… - The Astrophysical …, 2024 - iopscience.iop.org
A complete accounting of nearby objects—from the highest-mass white dwarf progenitors
down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of …
down to low-mass brown dwarfs—is now possible, thanks to an almost complete set of …
Friends not Foes: Strong Correlation between Inner Super-Earths and Outer Gas Giants
ML Bryan, EJ Lee - The Astrophysical Journal Letters, 2024 - iopscience.iop.org
The connection between outer gas giants and inner super-Earths reflects their formation and
evolutionary histories. Past work exploring this link has suggested a tentative positive …
evolutionary histories. Past work exploring this link has suggested a tentative positive …
A review of planetary systems around HD 99492, HD 147379, and HD 190007 with HARPS-N
Context. The Rocky Planet Search (RPS) program is dedicated to a blind radial velocity (RV)
search of planets around bright stars in the northern hemisphere, using the high-resolution …
search of planets around bright stars in the northern hemisphere, using the high-resolution …
The compact multi-planet system GJ 9827 revisited with ESPRESSO
VM Passegger, AS Mascareño, R Allart… - Astronomy & …, 2024 - aanda.org
GJ 9827 is a bright, nearby K7V star orbited by two super-Earths and one mini-Neptune on
close-in orbits. The system was first discovered using K2 data and then further characterized …
close-in orbits. The system was first discovered using K2 data and then further characterized …
Efficient modeling of correlated noise-III. Scalable methods for jointly modeling several observables' time series with Gaussian processes
The radial velocity method is a very productive technique used to detect and confirm
extrasolar planets. The most recent spectrographs, such as ESPRESSO or EXPRES, have …
extrasolar planets. The most recent spectrographs, such as ESPRESSO or EXPRES, have …
Viewing the PLATO LOPS2 field through the lenses of TESS
YNE Eschen, D Bayliss, TG Wilson… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT PLATO will begin observing stars in its Southern Field (LOPS2) after its launch
in late 2026. By this time, TESS will have observed the stars in LOPS2 for at least four years …
in late 2026. By this time, TESS will have observed the stars in LOPS2 for at least four years …
Atmospheric characterization and tighter constraints on the orbital misalignment of WASP-94 A b with HARPS
We present high spectral resolution observations of the hot Jupiter WASP-94 A b using the
HARPS instrument on ESO's 3.6-m telescope in La Silla, Chile. We probed for Na absorption …
HARPS instrument on ESO's 3.6-m telescope in La Silla, Chile. We probed for Na absorption …
Dynamical Viability Assessment for Habitable Worlds Observatory Targets
Exoplanetary science is increasingly prioritizing efforts toward direct imaging of planetary
systems, with emphasis on those that may enable the detection and characterization of …
systems, with emphasis on those that may enable the detection and characterization of …
Planetary system architectures with low-mass inner planets-Direct imaging exploration of mature systems beyond 1 au
Context. The discovery of planets orbiting at less than 1 au from their host star and less
massive than Saturn in various exoplanetary systems revolutionized our theories of …
massive than Saturn in various exoplanetary systems revolutionized our theories of …
A continuous multiple hypothesis testing framework for optimal exoplanet detection
NC Hara, T De Poyferre, JB Delisle… - The Annals of Applied …, 2024 - projecteuclid.org
A continuous multiple hypothesis testing framework for optimal exoplanet detection Page 1
The Annals of Applied Statistics 2024, Vol. 18, No. 1, 749–769 https://doi.org/10.1214/23-AOAS1810 …
The Annals of Applied Statistics 2024, Vol. 18, No. 1, 749–769 https://doi.org/10.1214/23-AOAS1810 …