Results 91 to 100 of about 14,838,227 (209)
HARPS-N @ TNG, two year harvesting data : performances and results [PDF]
The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a
Latham, D.W. +40 more
core +1 more source
Modeling Exoplanet Demographics Across Detection Methods
Exoplanet demographics leverages large-scale survey data to give us population-level in- sight to questions of planet formation, evolution, and habitability.
Bergsten, Galen Justice
core +5 more sources
The NEID Earth Twin Survey. III. Survey Performance after Three Years on Sky
The NEID Earth Twin Survey (NETS) has been delivering a rich set of precise radial velocity (RV) measurements for 41 bright, nearby main-sequence stars.
Arvind F. Gupta +24 more
doaj +1 more source
It has been suggested that giant planet occurrence peaks for stars with M _* ≈ 3 M _⊙ at a value a factor of 4 higher than observed for solar-mass stars.
Sihao Cheng +2 more
doaj +1 more source
We report the discovery of a new massive giant planet, HD 164604 c ( ${a}_{c}=5.55{6}_{-0.10}^{+0.093}$ au, ${e}_{c}=0.19{6}_{-0.078}^{+0.078}$ , and ${m}_{c}=9.{5}_{-1.25}^{+1.2}$ , or $7.{6}_{-1.0}^{+1.0}\,{M}_{{\rm{Jup}}}$ ), orbiting a K3.5 dwarf ...
Guang-Yao Xiao +6 more
doaj +1 more source
The Interpolation Constraint in the RV Analysis of M Dwarfs Using Empirical Templates
Precise radial velocity (pRV) measurements of M dwarfs in the near-infrared rely on empirical templates due to the lack of accurate stellar spectral models in this regime.
Dhvani Doshi +6 more
doaj +1 more source
We present new VLTI/GRAVITY astrometry and updated orbit fits for the directly imaged companions YSES 1 b and HR 2562 B, substellar objects straddling the planet–brown-dwarf boundary.
Jonathan Roberts +22 more
doaj +1 more source
The Transiting Exoplanet Survey Satellite (TESS) has transformed the study of nearby exoplanetary systems; however, its nominal observing strategy limits sensitivity to planets with orbital periods shorter than ∼10 days for most parts of the sky. The two
Andrew Hotnisky +11 more
doaj +1 more source
A Pair of Dynamically Interacting Sub-Neptunes around TOI-6054
We confirm the planetary nature of a pair of transiting sub-Neptune exoplanets orbiting the bright F-type subgiant star TOI-6054 ( V = 8.02, K = 6.673) as a part of the OrCAS radial velocity survey using WIYN/NEID observations. We find that TOI-6054b and
Maxwell A. Kroft +33 more
doaj +1 more source
Revised Masses for Low-density Planets Orbiting the Disordered M-dwarf System TOI-1266
We present an analysis of 126 new radial velocity measurements from the MAROON-X spectrograph to investigate the TOI-1266 system, which hosts two known transiting sub-Neptunes at 10.8 and 18.8 days.
Dakotah Tyler +7 more
doaj +1 more source

