The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their otherwise smooth Keplerian motions. Twenty-one of those systems were observed 10 or more times and show no evidence of additional companions. A new algorithm is presented for identifying astrometric companions and establishing the (companion mass)-(orbital period) combinations that can be excluded from existence with high confidence based on the PHASES observations, and the regions of mass-period phase space being excluded are presented for 21 PHASES binaries. Subject headings: astrometry – binar...
We conducted multi-epoch VLBI observations to search for astrometric reflex motion caused by a sub-s...
Observations with the planned astrometry satellite GAIA are modeled in order to determine the detec...
We have surveyed a sample of 165 solar-type spectroscopic binaries (SB) with periods from 1 to 30 da...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 sub-ar...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 subarc...
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
International audienceWe started a survey with CHARA/MIRC-X and VLTI/GRAVITY to search for low-mass ...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
We conducted multi-epoch VLBI observations to search for astrometric reflex motion caused by a sub-s...
Observations with the planned astrometry satellite GAIA are modeled in order to determine the detec...
We have surveyed a sample of 165 solar-type spectroscopic binaries (SB) with periods from 1 to 30 da...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 sub-ar...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 subarc...
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcseco...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplane...
International audienceWe started a survey with CHARA/MIRC-X and VLTI/GRAVITY to search for low-mass ...
Abstract. Apparent acceleration of proper motion is one of the observable manifestations of orbital ...
We conducted multi-epoch VLBI observations to search for astrometric reflex motion caused by a sub-s...
Observations with the planned astrometry satellite GAIA are modeled in order to determine the detec...
We have surveyed a sample of 165 solar-type spectroscopic binaries (SB) with periods from 1 to 30 da...